{"Type":"Events","Count":4238,"Next":"https://supernova.eso.org/astrocal/d2d/?page=2","Collections":[{"ID":"5669","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-12-30T18:59:00Z","EndDate":"2026-12-30T18:59:00Z","PeakDate":"2026-12-30T18:59:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T22:20:23Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5668","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-12-24T01:28:00Z","EndDate":"2026-12-24T01:28:00Z","PeakDate":"2026-12-24T01:28:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T22:16:31Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5664","Title":"December Solstice","Categories":["Sky"],"Headline":"December Solstice","Description":"<p>The December solstice is the day with the shortest daylight hours in the Earth's northern hemisphere, where it marks the start of the winter and so it is referred to as the \"winter solstice\". Conversely, in the southern hemisphere it is the day with the longest daylight hours. There it marks the start of the summer, and is referred to as the \"summer solstice\". The date of the solstice varies between December 20 and 22, because it is delayed by about 6 hours each year, to be set back again at every leap year. In 2026, the December solstice falls on 21 December.</p>","Event":{"StartDate":"2026-12-21T20:50:00Z","EndDate":"2026-12-21T20:50:00Z","PeakDate":"2026-12-21T20:50:00Z","DisplayDuration":1,"Phenomenon":"Solstice"},"PublicationDate":"2026-04-23T22:00:26Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Earth","Sun"]},"Assets":[{"ID":"2017-december-solstice","MediaType":"Image","Title":"December solstice GEN","Description":"<p>Artist's impression of a December solstice.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org).</p>","Resources":[{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/2017-december-solstice.tif","MediaType":"Image","ResourceType":"Original","FileSize":6553868,"ProjectionType":"Tan"},{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/2017-december-solstice.jpg","MediaType":"Image","ResourceType":"Large","FileSize":660363,"ProjectionType":"Tan"},{"Dimensions":[1280.0,699.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/2017-december-solstice.jpg","MediaType":"Image","ResourceType":"Small","FileSize":93729,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/2017-december-solstice.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7357,"ProjectionType":"Tan"},{"Dimensions":[60.0,33.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/2017-december-solstice.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4211,"ProjectionType":"Tan"}]}]},{"ID":"5667","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-12-17T05:43:00Z","EndDate":"2026-12-17T05:43:00Z","PeakDate":"2026-12-17T05:43:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T22:13:20Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5666","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-12-09T00:52:00Z","EndDate":"2026-12-09T00:52:00Z","PeakDate":"2026-12-09T00:52:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T22:09:32Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5670","Title":"Geminids Meteor Shower","Categories":["Sky"],"Headline":"Geminids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Geminids meteor shower are thought to be dust left behind by the comet 3200 Phaethon. The meteors appear to radiate from a point on the sky in the constellation of Gemini, close to the star Castor. Up to 60 shooting stars an hour can be seen at the peak, for approximately three days around 14 December 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2026-12-07T00:00:00Z","EndDate":"2026-12-17T00:00:00Z","PeakDate":"2026-12-14T00:00:00Z","DisplayDuration":1,"Phenomenon":"Meteor shower"},"PublicationDate":"2026-04-23T22:25:09Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Geminids","Comet 3200 Phaethon"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]},{"ID":"esocast52a","MediaType":"Video","Title":"ESOcast 52/Chile Chill 2: It's Raining Stars — Geminid meteor shower","Description":"<p>A video podcast by Gianluca Lombardi celebrating the Geminid meteor shower.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\"></div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/esocast52a.m4v","Checksum":"d9d562b65a58f8e864792102b128a682d3b5b03584a74a54dc38aa4c71084c05","MediaType":"Video","ResourceType":"Preview","FileSize":144643614,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/esocast52a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6078,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/esocast52a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":769,"ProjectionType":"Tan"}]}]},{"ID":"5665","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-12-01T06:09:00Z","EndDate":"2026-12-01T06:09:00Z","PeakDate":"2026-12-01T06:09:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T22:05:45Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5662","Title":"Jupiter Occultation by the Moon","Categories":["Sky"],"Headline":"Jupiter Occultation by the Moon","Description":"<p>The Moon passes in front of Jupiter in the sky. This is called a lunar occultation and Jupiter is in this case hidden for about 2 hours. The occultation is visible from the South America and Antarctica.</p>","Event":{"StartDate":"2026-11-30T07:15:00Z","EndDate":"2026-11-30T09:32:00Z","PeakDate":"2026-11-30T08:24:00Z","DisplayDuration":1,"Phenomenon":"Occultation"},"PublicationDate":"2026-04-23T21:52:12Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Jupiter","Moon"]},"Assets":[{"ID":"heic1410a","MediaType":"Image","Title":"Jupiter and its Great Red Spot","Description":"<p>This full-disc image of Jupiter was taken on 21 April 2014 by the Hubble Space Telescope.</p>","Credit":"<p>NASA, ESA, and A. Simon (Goddard Space Flight Center)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/heic1410a.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":736946,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/heic1410a.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":159256,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/heic1410a.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":174584,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/heic1410a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":12011,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/heic1410a.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5104,"MediaType":"Image"}]},{"ID":"occu-2019-11-28","MediaType":"Image","Title":"Occultation of a Planet by the Moon","Description":"<p>Artist's impression of the Jupiter occultation by the Moon on 28 November 2019, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/occu-2019-11-28.tif","MediaType":"Image","ResourceType":"Original","FileSize":7397784,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Large","FileSize":365242,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Small","FileSize":59174,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5139,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3805,"ProjectionType":"Tan"}]}]},{"ID":"5657","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-11-24T14:53:00Z","EndDate":"2026-11-24T14:53:00Z","PeakDate":"2026-11-24T14:53:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T21:32:45Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5656","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-11-17T11:48:00Z","EndDate":"2026-11-17T11:48:00Z","PeakDate":"2026-11-17T11:48:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T21:29:18Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5658","Title":"Planet conjunction (Jupiter and Mars)","Categories":["Sky"],"Headline":"Planet conjunction (Jupiter and Mars)","Description":"<p>A planetary conjunction happens when two planets appear close together in the sky as seen from Earth. It is a projection effect, as the planets are not really close to each other in space. Over several days, Jupiter and Mars can be seen close together, with Jupiter reaching a minimum angular distance of 1°14' south of Mars on 15 November 2026.</p>","Event":{"StartDate":"2026-11-15T02:42:00Z","EndDate":"2026-11-15T02:42:00Z","PeakDate":"2026-11-15T02:42:00Z","DisplayDuration":1,"Phenomenon":"Conjunction"},"PublicationDate":"2026-04-23T21:38:32Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Jupiter","Mars"]},"Assets":[{"ID":"yb_vlt_moon_cnn_cc","MediaType":"Image","Title":"Celestial conjunction at Paranal","Description":"<p>In the night sky over ESO’s Very Large Telescope (VLT) observatory at Paranal, the Moon shines along with two bright companions : already aloft in the heavens and glowing in the centre of the image is Venus, Earth’s closest planetary neighbour, and, to its right, the giant, though more distant planet, Jupiter. Such apparent celestial near misses — although the heavenly bodies are actually tens to hundreds of millions of kilometres apart — are called conjunctions.</p>\r\n<p>Still other sights delight this night view at Paranal : the radiant, reddish plane of the Milky Way, smouldering on the horizon, and an 8.2-metre VLT Unit Telescope, along with a 1.8-metre Auxiliary Telescope, standing firmly on the ground.</p>","Credit":"<p>ESO/<a href=\"https://www.facebook.com/yuribeletskyphoto\">Y. Beletsky</a></p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/yb_vlt_moon_cnn_cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":63459778,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/yb_vlt_moon_cnn_cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1861464,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/yb_vlt_moon_cnn_cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":255904,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/yb_vlt_moon_cnn_cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9257,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/yb_vlt_moon_cnn_cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":4442,"MediaType":"Image"}]}]},{"ID":"5655","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-11-09T07:02:00Z","EndDate":"2026-11-09T07:02:00Z","PeakDate":"2026-11-09T07:02:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T21:26:10Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5661","Title":"Venus Occultation by the Moon","Categories":["Sky"],"Headline":"Venus Occultation by the Moon","Description":"<p>The Moon passes in front of Venus in the sky. This is called a lunar occultation and Venus is in this case hidden for about 3 hours. The occultation is visible from the South America and Antarctica.</p>","Event":{"StartDate":"2026-11-07T09:26:00Z","EndDate":"2026-11-07T11:59:00Z","PeakDate":"2026-11-07T10:43:00Z","DisplayDuration":1,"Phenomenon":"Occultation"},"PublicationDate":"2026-04-23T21:48:46Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Venus","Moon"]},"Assets":[{"ID":"occult-2019-01-31","MediaType":"Image","Title":"Venus occultation by the Moon GEN","Description":"<p>Artist's impression of a Venus occultation by the Moon, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/occult-2019-01-31.tif","MediaType":"Image","ResourceType":"Original","FileSize":6889204,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546680,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Small","FileSize":99196,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7519,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4220,"ProjectionType":"Tan"}]}]},{"ID":"5663","Title":"Leonids Meteor Shower","Categories":["Sky"],"Headline":"Leonids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Leonids meteor shower are thought to be dust left behind by the comet 55P/Tempel-Tuttle. The meteors appear to radiate from a point on the sky in the constellation of Leo, close to the “Sickle stars” that are above Regulus. Up to 10 shooting stars an hour can be seen at the peak, for approximately three days around 18 November 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2026-11-06T00:00:00","EndDate":"2026-11-30T00:00:00","PeakDate":"2026-11-18T00:00:00","DisplayDuration":3,"Phenomenon":"Meteor shower"},"PublicationDate":"2026-04-23T21:56:24Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Leonids","Comet 55P/Tempel-Tuttle"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5660","Title":"Jupiter Occultation by the Moon","Categories":["Sky"],"Headline":"Jupiter Occultation by the Moon","Description":"<p>The Moon passes in front of Jupiter in the sky. This is called a lunar occultation and Jupiter is in this case hidden for about 4 hours. The occultation is visible from the Oceania and South Asia.</p>","Event":{"StartDate":"2026-11-02T20:45:00Z","EndDate":"2026-11-03T00:45:00Z","PeakDate":"2026-11-02T22:45:00Z","DisplayDuration":1,"Phenomenon":"Occultation"},"PublicationDate":"2026-04-23T21:45:23Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Jupiter","Moon"]},"Assets":[{"ID":"heic1410a","MediaType":"Image","Title":"Jupiter and its Great Red Spot","Description":"<p>This full-disc image of Jupiter was taken on 21 April 2014 by the Hubble Space Telescope.</p>","Credit":"<p>NASA, ESA, and A. Simon (Goddard Space Flight Center)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/heic1410a.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":736946,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/heic1410a.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":159256,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/heic1410a.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":174584,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/heic1410a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":12011,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/heic1410a.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5104,"MediaType":"Image"}]},{"ID":"occu-2019-11-28","MediaType":"Image","Title":"Occultation of a Planet by the Moon","Description":"<p>Artist's impression of the Jupiter occultation by the Moon on 28 November 2019, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/occu-2019-11-28.tif","MediaType":"Image","ResourceType":"Original","FileSize":7397784,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Large","FileSize":365242,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Small","FileSize":59174,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5139,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3805,"ProjectionType":"Tan"}]}]},{"ID":"5659","Title":"Mars Occultation by the Moon","Categories":["Sky"],"Headline":"Mars Occultation by the Moon","Description":"<p>The Moon passes in front of Mars in the sky. This is called a lunar occultation and Mars is in this case hidden for about 3 hours. The occultation is visible from the French Polynesia, Cook Islands, and Pitcairn Islands.</p>","Event":{"StartDate":"2026-11-02T12:15:00Z","EndDate":"2026-11-02T15:02:00Z","PeakDate":"2026-11-02T13:39:00Z","DisplayDuration":1,"Phenomenon":"Occultation"},"PublicationDate":"2026-04-23T21:42:01Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Mars","Moon"]},"Assets":[{"ID":"20181116-mars-from-earth","MediaType":"Image","Title":"Mars occultation by the Moon GEN","Description":"<p>Artist's impression of a Mars occultation by the Moon, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/<a href=\"http://www.spaceengine.org/\">spaceengine.org</a></p>","Resources":[{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/20181116-mars-from-earth.tif","MediaType":"Image","ResourceType":"Original","FileSize":8737836,"ProjectionType":"Tan"},{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Large","FileSize":725213,"ProjectionType":"Tan"},{"Dimensions":[1280.0,699.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Small","FileSize":94946,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7693,"ProjectionType":"Tan"},{"Dimensions":[60.0,33.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4300,"ProjectionType":"Tan"}]}]},{"ID":"5654","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-11-01T20:28:00Z","EndDate":"2026-11-01T20:28:00Z","PeakDate":"2026-11-01T20:28:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-23T21:23:16Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5649","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. 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It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-10-10T15:50:00Z","EndDate":"2026-10-10T15:50:00Z","PeakDate":"2026-10-10T15:50:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-22T21:38:34Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5652","Title":"Jupiter Occultation by the Moon","Categories":["Sky"],"Headline":"Jupiter Occultation by the Moon","Description":"<p>The Moon passes in front of Jupiter in the sky. This is called a lunar occultation and Jupiter is in this case hidden for about 4 hours. The occultation is visible from the East coast of the USA and Africa.</p>","Event":{"StartDate":"2026-10-06T08:14:00Z","EndDate":"2026-10-06T12:32:00Z","PeakDate":"2026-10-06T10:23:00Z","DisplayDuration":1,"Phenomenon":"Occultation"},"PublicationDate":"2026-04-22T21:54:42Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Jupiter","Moon"]},"Assets":[{"ID":"heic1410a","MediaType":"Image","Title":"Jupiter and its Great Red Spot","Description":"<p>This full-disc image of Jupiter was taken on 21 April 2014 by the Hubble Space Telescope.</p>","Credit":"<p>NASA, ESA, and A. Simon (Goddard Space Flight Center)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/heic1410a.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":736946,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/heic1410a.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":159256,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/heic1410a.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":174584,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/heic1410a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":12011,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/heic1410a.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5104,"MediaType":"Image"}]},{"ID":"occu-2019-11-28","MediaType":"Image","Title":"Occultation of a Planet by the Moon","Description":"<p>Artist's impression of the Jupiter occultation by the Moon on 28 November 2019, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/occu-2019-11-28.tif","MediaType":"Image","ResourceType":"Original","FileSize":7397784,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Large","FileSize":365242,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Small","FileSize":59174,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5139,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/occu-2019-11-28.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3805,"ProjectionType":"Tan"}]}]},{"ID":"5651","Title":"Mars Occultation by the Moon","Categories":["Sky"],"Headline":"Mars Occultation by the Moon","Description":"<p>The Moon passes in front of Mars in the sky. This is called a lunar occultation and Mars is in this case hidden for about 2 hours. The occultation is visible from the north part of Canada.</p>","Event":{"StartDate":"2026-10-05T05:07:00Z","EndDate":"2026-10-05T07:15:00Z","PeakDate":"2026-10-05T06:11:00Z","DisplayDuration":1,"Phenomenon":"Occultation"},"PublicationDate":"2026-04-22T21:51:29Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Mars","Moon"]},"Assets":[{"ID":"20181116-mars-from-earth","MediaType":"Image","Title":"Mars occultation by the Moon GEN","Description":"<p>Artist's impression of a Mars occultation by the Moon, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/<a href=\"http://www.spaceengine.org/\">spaceengine.org</a></p>","Resources":[{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/20181116-mars-from-earth.tif","MediaType":"Image","ResourceType":"Original","FileSize":8737836,"ProjectionType":"Tan"},{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Large","FileSize":725213,"ProjectionType":"Tan"},{"Dimensions":[1280.0,699.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Small","FileSize":94946,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7693,"ProjectionType":"Tan"},{"Dimensions":[60.0,33.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/20181116-mars-from-earth.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4300,"ProjectionType":"Tan"}]}]},{"ID":"5646","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-10-03T13:25:00Z","EndDate":"2026-10-03T13:25:00Z","PeakDate":"2026-10-03T13:25:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-22T21:35:59Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5653","Title":"Orionids Meteor Shower","Categories":["Sky"],"Headline":"Orionids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Orionids meteor shower are thought to be dust left behind by the comet 1P/Halley (Halley’s comet). The meteors appear to radiate from a point on the sky in the constellation of Orion, close to the star Betelgeuse. Up to 30 shooting stars an hour can be seen at the peak, for approximately three days around 22 October 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2026-10-02T00:00:00Z","EndDate":"2026-11-07T00:00:00Z","PeakDate":"2026-10-22T00:00:00Z","DisplayDuration":3,"Phenomenon":"Meteor shower"},"PublicationDate":"2026-04-22T21:59:05Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Orionids","Halley's comet"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5643","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-09-26T16:49:00Z","EndDate":"2026-09-26T16:49:00Z","PeakDate":"2026-09-26T16:49:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-15T21:45:41Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5639","Title":"September Equinox","Categories":["Sky"],"Headline":"September Equinox","Description":"<p>At the equinox everybody on Earth experiences a day and night of equal lengths, 12 hours of daylight and 12 hours of night time. In astronomical terms it is the exact moment the Sun crosses the celestial equator — the imaginary line in the sky above the Earth’s Equator — from north to south. In 2026, the September equinox falls on 23 September. In the northern hemisphere, after the September equinox, daylight hours start to be shorter, and it's thus considered as the beginning of the season of Autumn. The opposite happens in the southern hemisphere, with the beginning of Spring.</p>","Event":{"StartDate":"2026-09-23T00:05:00Z","EndDate":"2026-09-23T00:05:00Z","PeakDate":"2026-09-23T00:05:00Z","DisplayDuration":1,"Phenomenon":"Equinox"},"PublicationDate":"2026-04-15T21:32:29Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Earth","Sun"]},"Assets":[{"ID":"2019-september-equinox","MediaType":"Image","Title":"September equinox GEN","Description":"<p>Artist's impression of a September equinox.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org).</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/2019-september-equinox.tif","MediaType":"Image","ResourceType":"Original","FileSize":9592740,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/2019-september-equinox.jpg","MediaType":"Image","ResourceType":"Large","FileSize":691639,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/2019-september-equinox.jpg","MediaType":"Image","ResourceType":"Small","FileSize":89223,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/2019-september-equinox.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7246,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/2019-september-equinox.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4116,"ProjectionType":"Tan"}]}]},{"ID":"5642","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-09-18T20:44:00Z","EndDate":"2026-09-18T20:44:00Z","PeakDate":"2026-09-18T20:44:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-15T21:42:12Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5645","Title":"Venus Occultation by the Moon","Categories":["Sky"],"Headline":"Venus Occultation by the Moon","Description":"<p>The Moon passes in front of Venus in the sky. This is called a lunar occultation and Venus is in this case hidden for about 4 hours. 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It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-09-11T03:27:00Z","EndDate":"2026-09-11T03:27:00Z","PeakDate":"2026-09-11T03:27:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-15T21:39:14Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. 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The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-09-04T07:51:00Z","EndDate":"2026-09-04T07:51:00Z","PeakDate":"2026-09-04T07:51:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-15T21:36:27Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. 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It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. 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As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5632","Title":"Partial Lunar Eclipse","Categories":["Sky"],"Headline":"Partial Lunar Eclipse","Description":"<p>A partial lunar eclipse happens when the Sun, the Earth and the Moon are approximately, but not exactly, aligned in space, and the Moon is full. The Earth prevents the Sun's light from reaching the Moon's surface directly. Part of the Moon is obscured within the darkest, central part of the Earth's shadow, called the umbra. The rest of the Moon falls within the outer part of the Earth's shadow, called the penumbra. The Moon will appear a bit dimmer than usual. This eclipse will be visible in Europe, the western part of Asia, Africa, North America, South America, the Pacific, the Atlantic, the Indian Ocean, and Antarctica.</p>","Event":{"StartDate":"2026-08-28T01:23:58Z","EndDate":"2026-08-28T07:01:47Z","PeakDate":"2026-08-28T04:12:53Z","DisplayDuration":1,"Phenomenon":"Lunar eclipse"},"PublicationDate":"2026-04-09T22:00:24Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso-p-sunset-lv","MediaType":"Image","Title":"Partial lunar eclipse from the VLT platform","Description":"<p>A partially eclipsed moon rises on the shadow of Cerro Paranal on 16 August, 2008. On the left side, the VLT´s Auxiliary Telescope AT4.</p>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[2560,1572],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso-p-sunset-lv.tif","MediaType":"Image","ResourceType":"Original","FileSize":5331488,"ProjectionType":"Tan"},{"Dimensions":[2560,1572],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso-p-sunset-lv.jpg","MediaType":"Image","ResourceType":"Large","FileSize":664894,"ProjectionType":"Tan"},{"Dimensions":[1280.0,786.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso-p-sunset-lv.jpg","MediaType":"Image","ResourceType":"Small","FileSize":165497,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso-p-sunset-lv.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9216,"ProjectionType":"Tan"},{"Dimensions":[60.0,37.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso-p-sunset-lv.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4487,"ProjectionType":"Tan"}]},{"ID":"moon-eclipse-lasilla","MediaType":"Image","Title":"Moon eclipse seen from La Silla","Description":"<p>View from a lunar eclipse taken from La Silla, Chile.</p>","Credit":"<p>ESO/F. Char</p>","Resources":[{"Dimensions":[4272,2848],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/moon-eclipse-lasilla.tif","MediaType":"Image","ResourceType":"Original","FileSize":8393266,"ProjectionType":"Tan"},{"Dimensions":[4272,2848],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/moon-eclipse-lasilla.jpg","MediaType":"Image","ResourceType":"Large","FileSize":763402,"ProjectionType":"Tan"},{"Dimensions":[1280.0,854.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/moon-eclipse-lasilla.jpg","MediaType":"Image","ResourceType":"Small","FileSize":81961,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/moon-eclipse-lasilla.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7601,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/moon-eclipse-lasilla.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4313,"ProjectionType":"Tan"}]}]},{"ID":"5635","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-08-20T02:46:00Z","EndDate":"2026-08-20T02:46:00Z","PeakDate":"2026-08-20T02:46:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-09T22:08:56Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5637","Title":"Planet conjunction (Jupiter and Mercury)","Categories":["Sky"],"Headline":"Planet conjunction (Jupiter and Mercury)","Description":"<p>A planetary conjunction happens when two planets appear close together in the sky as seen from Earth. It is a projection effect, as the planets are not really close to each other in space. Over several days, Jupiter and Mercury can be seen close together, with Jupiter reaching a minimum angular distance of 33' south of Mercury on 15 August 2026.</p>","Event":{"StartDate":"2026-08-15T09:13:00Z","EndDate":"2026-08-15T09:13:00Z","PeakDate":"2026-08-15T09:13:00Z","DisplayDuration":1,"Phenomenon":"Planet conjunction"},"PublicationDate":"2026-04-09T22:17:18Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Jupiter","Mercury"]},"Assets":[{"ID":"2021-01-11","MediaType":"Image","Title":"Planet conjunction Jupiter and Mercury GEN","Description":"<p>Artist's impression of a Jupiter and Mercury conjunction, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/2021-01-11.tif","MediaType":"Image","ResourceType":"Original","FileSize":5489268,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/2021-01-11.jpg","MediaType":"Image","ResourceType":"Large","FileSize":368774,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/2021-01-11.jpg","MediaType":"Image","ResourceType":"Small","FileSize":85874,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/2021-01-11.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8828,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/2021-01-11.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4458,"ProjectionType":"Tan"}]}]},{"ID":"5634","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-08-12T17:37:00Z","EndDate":"2026-08-12T17:37:00Z","PeakDate":"2026-08-12T17:37:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-09T22:06:17Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5631","Title":"Total Solar Eclipse","Categories":["Sky"],"Headline":"Total Solar Eclipse","Description":"<p>A total solar eclipse happens when the Sun, the Moon and the Earth are perfectly aligned and the Moon is new. During totality, the Moon completely covers the disc of the Sun as seen from Earth, with only the Sun's corona visible. During a total solar eclipse the sky goes dark and temperatures fall drastically. This eclipse will be visible from Europe, the nothern part of Asia, North and West Africa, a great part of North America, the Pacific, the Atlantic, and the Arctic.</p>","Event":{"StartDate":"2026-08-12T15:34:15Z","EndDate":"2026-08-12T19:57:57Z","PeakDate":"2026-08-12T17:46:06Z","DisplayDuration":1,"Phenomenon":"Solar eclipse"},"PublicationDate":"2026-04-09T21:56:22Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Sun"]},"Assets":[{"ID":"0206-eclipse-english-only-3k","MediaType":"Image","Title":"Solar eclipses diagram","Description":"<p>This graphic demonstrates the juxtaposition of the Moon with the Sun necessary to produce a partial or complete solar eclipse. Note: the objects and distances are not to scale.</p>","Credit":"<p>ESO/M. Kornmesser</p>","Resources":[{"Dimensions":[4000,2442],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/0206-eclipse-english-only-3k.tif","MediaType":"Image","ResourceType":"Original","FileSize":4927324,"ProjectionType":"Tan"},{"Dimensions":[4000,2442],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/0206-eclipse-english-only-3k.jpg","MediaType":"Image","ResourceType":"Large","FileSize":600133,"ProjectionType":"Tan"},{"Dimensions":[1280.0,782.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/0206-eclipse-english-only-3k.jpg","MediaType":"Image","ResourceType":"Small","FileSize":90335,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/0206-eclipse-english-only-3k.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7805,"ProjectionType":"Tan"},{"Dimensions":[60.0,37.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/0206-eclipse-english-only-3k.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4504,"ProjectionType":"Tan"}]},{"ID":"0206e-solar-eclipse-cc","MediaType":"Image","Title":"Total solar eclipse","Description":"<p>Picture of the total solar eclipse on 9 March 2016 over the cloudy sky of Maba, a town in North Maluku, Indonesia.</p>","Credit":"<p><a href=\"http://www.facebook.com/PetrHoralekPhotography\">Petr Horálek</a> and <a href=\"http://www.zam.fme.vutbr.cz/~druck/\">Miloslav Druckmüller</a></p>","Resources":[{"Dimensions":[3582,2388],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/0206e-solar-eclipse-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":9769088,"ProjectionType":"Tan"},{"Dimensions":[3582,2388],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/0206e-solar-eclipse-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1020134,"ProjectionType":"Tan"},{"Dimensions":[1280.0,854.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/0206e-solar-eclipse-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":124946,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/0206e-solar-eclipse-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6005,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/0206e-solar-eclipse-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4179,"ProjectionType":"Tan"}]},{"ID":"solareclipse_mos","MediaType":"Video","Title":"Solar Eclipse (fulldome artist's impression)","Description":"<p><span>This is a fulldome rendition of the whole sky during a total solar eclipse (not a specific eclipse or location). Timings are exaggerated to emphasize phenomena near and during totality. The Sun is also enlarged for clarity and Mercury, Venus, and Jupiter are visible.</span></p>","Credit":"<p><span>Charles Hayden Planetarium, Museum of Science, Boston</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/solareclipse_mos.zip","MediaType":"Video","ResourceType":"Original","FileSize":49501172538,"ProjectionType":"Fulldome"},{"Dimensions":[1536.0,1536.0],"URL":"https://cdn.eso.org/videos/dome_mov/solareclipse_mos.mov","MediaType":"Video","ResourceType":"Large","FileSize":160177448,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/solareclipse_mos.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":240681938,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/solareclipse_mos.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5126,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/solareclipse_mos.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4413,"ProjectionType":"Fulldome"}]}]},{"ID":"5633","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-08-06T02:21:00Z","EndDate":"2026-08-06T02:21:00Z","PeakDate":"2026-08-06T02:21:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-09T22:03:31Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5629","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-07-29T14:36:00Z","EndDate":"2026-07-29T14:36:00Z","PeakDate":"2026-07-29T14:36:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-01T21:32:48Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5628","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-07-21T11:06:00Z","EndDate":"2026-07-21T11:06:00Z","PeakDate":"2026-07-21T11:06:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-01T21:28:49Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5638","Title":"Perseids Meteor Shower","Categories":["Sky"],"Headline":"Perseids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Perseids meteor shower are thought to be dust left behind by the comet 109P/Swift–Tuttle. The meteors appear to radiate from a point on the sky in the constellation of Perseus. Up to 60 shooting stars an hour can be seen at the peak, for approximately three days around 13 August 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2026-07-17T00:00:00Z","EndDate":"2026-08-24T00:00:00Z","PeakDate":"2026-08-13T00:00:00Z","DisplayDuration":3,"Phenomenon":"Meteor shower"},"PublicationDate":"2026-04-09T22:20:56Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Perseids","Comet 109P/Swift–Tuttle"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5627","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-07-14T09:43:00Z","EndDate":"2026-07-14T09:43:00Z","PeakDate":"2026-07-14T09:43:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-01T21:24:28Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5630","Title":"Delta Aquarids Meteor Shower","Categories":["Sky"],"Headline":"Delta Aquarids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Delta Aquarids meteor shower appear to radiate from a point on the sky in the constellation of Aquarius. Up to 30 shooting stars an hour can be seen at the peak, for approximately seven days around 31 July 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2026-07-12T00:00:00","EndDate":"2026-08-23T00:00:00","PeakDate":"2026-07-31T00:00:00","DisplayDuration":7,"Phenomenon":"Meteor shower"},"PublicationDate":"2026-04-01T21:37:20Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Delta Aquarids"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5626","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-07-07T19:29:00Z","EndDate":"2026-07-07T19:29:00Z","PeakDate":"2026-07-07T19:29:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-04-01T21:21:30Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5623","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-06-29T23:56:00Z","EndDate":"2026-06-29T23:56:00Z","PeakDate":"2026-06-29T23:56:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-03-26T22:59:04Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5622","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-06-21T21:55:00Z","EndDate":"2026-06-21T21:55:00Z","PeakDate":"2026-06-21T21:55:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-03-26T22:54:37Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5619","Title":"June Solstice","Categories":["Sky"],"Headline":"June Solstice","Description":"<p>The June solstice is the day with the longest daylight hours in the Earth's northern hemisphere, where it marks the start of the summer and so it is referred to as the \"summer solstice\". Conversely, in the southern hemisphere it is the day with the shortest daylight hours. There it marks the start of the winter, and is referred to as the \"winter solstice\". The date of the solstice varies between June 20 and 22, because it is delayed by about 6 hours each year, to be set back again at every leap year. In 2026, the June solstice falls on 21 June.</p>","Event":{"StartDate":"2026-06-21T08:24:00Z","EndDate":"2026-06-21T08:24:00Z","PeakDate":"2026-06-21T08:24:00Z","DisplayDuration":1,"Phenomenon":"Solstice"},"PublicationDate":"2026-03-26T22:42:59Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Earth","Sun"]},"Assets":[{"ID":"2019-june-solstice","MediaType":"Image","Title":"June solstice GEN","Description":"<p>Artist's impression of a June solstice.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org).</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/2019-june-solstice.tif","MediaType":"Image","ResourceType":"Original","FileSize":9625728,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/2019-june-solstice.jpg","MediaType":"Image","ResourceType":"Large","FileSize":768561,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/2019-june-solstice.jpg","MediaType":"Image","ResourceType":"Small","FileSize":97919,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/2019-june-solstice.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7710,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/2019-june-solstice.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4145,"ProjectionType":"Tan"}]}]},{"ID":"5625","Title":"Venus Occultation by the Moon","Categories":["Sky"],"Headline":"Venus Occultation by the Moon","Description":"<p>The Moon passes in front of Venus in the sky. This is called a lunar occultation and Venus is in this case hidden for about 5 hours. The occultation is visible from the northern part of Brazil, Venezuela, Caribean Islands, the USA, and Canada.</p>","Event":{"StartDate":"2026-06-17T18:17:00Z","EndDate":"2026-06-17T22:43:00Z","PeakDate":"2026-06-17T20:30:00Z","DisplayDuration":1,"Phenomenon":"Occultation"},"PublicationDate":"2026-03-26T23:08:00Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Venus","Moon"]},"Assets":[{"ID":"occult-2019-01-31","MediaType":"Image","Title":"Venus occultation by the Moon GEN","Description":"<p>Artist's impression of a Venus occultation by the Moon, as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/occult-2019-01-31.tif","MediaType":"Image","ResourceType":"Original","FileSize":6889204,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546680,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Small","FileSize":99196,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7519,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/occult-2019-01-31.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4220,"ProjectionType":"Tan"}]}]},{"ID":"5621","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-06-15T02:54:00Z","EndDate":"2026-06-15T02:54:00Z","PeakDate":"2026-06-15T02:54:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-03-26T22:50:41Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. 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It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-06-08T10:00:00Z","EndDate":"2026-06-08T10:00:00Z","PeakDate":"2026-06-08T10:00:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-03-26T22:46:41Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5617","Title":"Full Moon (Blue Moon)","Categories":["Sky"],"Headline":"Full Moon (Blue Moon)","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual. The second Full Moon in a month is called \"Blue Moon\". The name has nothing to do with the moon's color. It is solely a calendrical event.</p>","Event":{"StartDate":"2026-05-31T08:45:00Z","EndDate":"2026-05-31T08:45:00Z","PeakDate":"2026-05-31T08:45:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-03-24T22:45:33Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5616","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-05-23T11:11:00Z","EndDate":"2026-05-23T11:11:00Z","PeakDate":"2026-05-23T11:11:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-03-24T22:39:39Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. 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It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-05-01T17:23:00Z","EndDate":"2026-05-01T17:23:00Z","PeakDate":"2026-05-01T17:23:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-03-24T22:30:42Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. 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Over several days, Venus and Uranus can be seen close together, with Venus reaching a minimum angular distance of 46' north of Uranus on 24 April 2026.</p>","Event":{"StartDate":"2026-04-24T05:24:00Z","EndDate":"2026-04-24T05:24:00Z","PeakDate":"2026-04-24T05:24:00Z","DisplayDuration":1,"Phenomenon":"Conjunction"},"PublicationDate":"2026-02-10T22:10:56Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Venus","Uranus"]},"Assets":[{"ID":"2020-03-09","MediaType":"Image","Title":"Planet Conjunction (Venus and Uranus) GEN","Description":"<p>Artist's impression of the Venus and Uranus conjunction as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/2020-03-09.tif","MediaType":"Image","ResourceType":"Original","FileSize":7176172,"ProjectionType":"Tan"},{"Dimensions":[3840,2160],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/2020-03-09.jpg","MediaType":"Image","ResourceType":"Large","FileSize":348947,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/2020-03-09.jpg","MediaType":"Image","ResourceType":"Small","FileSize":59640,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/2020-03-09.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6970,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/2020-03-09.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4153,"ProjectionType":"Tan"}]}]},{"ID":"5606","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-04-24T02:32:00Z","EndDate":"2026-04-24T02:32:00Z","PeakDate":"2026-04-24T02:32:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-02-10T21:55:00Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5610","Title":"Planet conjunction (Saturn and Mars)","Categories":["Sky"],"Headline":"Planet conjunction (Saturn and Mars)","Description":"<p>A planetary conjunction happens when two planets appear close together in the sky as seen from Earth. It is a projection effect, as the planets are not really close to each other in space. Over several days, Saturn and Mars can be seen close together, with Saturn reaching a minimum angular distance of 1°18' south of Mars on 20 April 2026.</p>","Event":{"StartDate":"2026-04-20T17:36:00Z","EndDate":"2026-04-20T17:36:00Z","PeakDate":"2026-04-20T17:36:00Z","DisplayDuration":1,"Phenomenon":"Conjunction"},"PublicationDate":"2026-02-10T22:07:55Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Saturn","Mars"]},"Assets":[{"ID":"conj-iss-2018-04-02","MediaType":"Image","Title":"Planet Conjunction (Saturn and Mars) GEN","Description":"<p>Visualization of Saturn and Mars conjunction as seen from the ISS's orbit.</p>","Credit":"<p>ESO/Nico Bartmann/<a href=\"http://www.spaceengine.org/\">spaceengine.org</a></p>","Resources":[{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/conj-iss-2018-04-02.tif","MediaType":"Image","ResourceType":"Original","FileSize":6273348,"ProjectionType":"Tan"},{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/conj-iss-2018-04-02.jpg","MediaType":"Image","ResourceType":"Large","FileSize":475372,"ProjectionType":"Tan"},{"Dimensions":[1280.0,699.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/conj-iss-2018-04-02.jpg","MediaType":"Image","ResourceType":"Small","FileSize":92707,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/conj-iss-2018-04-02.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7169,"ProjectionType":"Tan"},{"Dimensions":[60.0,33.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/conj-iss-2018-04-02.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4179,"ProjectionType":"Tan"}]}]},{"ID":"5609","Title":"Planet Conjunction (Mercury and Saturn)","Categories":["Sky"],"Headline":"Planet Conjunction (Mercury and Saturn)","Description":"<p>A planetary conjunction happens when two planets appear close together in the sky as seen from Earth. It is a projection effect, as the planets are not really close to each other in space. Over several days, Mercury and Saturn can be seen close together, with Mercury reaching a minimum angular distance of 30' south of Saturn on 20 April 2026.</p>","Event":{"StartDate":"2026-04-20T08:03:00Z","EndDate":"2026-04-20T08:03:00Z","PeakDate":"2026-04-20T08:03:00Z","DisplayDuration":1,"Phenomenon":"Conjunction"},"PublicationDate":"2026-02-10T22:04:40Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Mercury","Saturn"]},"Assets":[{"ID":"yb_vlt_moon_cnn_cc","MediaType":"Image","Title":"Celestial conjunction at Paranal","Description":"<p>In the night sky over ESO’s Very Large Telescope (VLT) observatory at Paranal, the Moon shines along with two bright companions : already aloft in the heavens and glowing in the centre of the image is Venus, Earth’s closest planetary neighbour, and, to its right, the giant, though more distant planet, Jupiter. Such apparent celestial near misses — although the heavenly bodies are actually tens to hundreds of millions of kilometres apart — are called conjunctions.</p>\r\n<p>Still other sights delight this night view at Paranal : the radiant, reddish plane of the Milky Way, smouldering on the horizon, and an 8.2-metre VLT Unit Telescope, along with a 1.8-metre Auxiliary Telescope, standing firmly on the ground.</p>","Credit":"<p>ESO/<a href=\"https://www.facebook.com/yuribeletskyphoto\">Y. Beletsky</a></p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/yb_vlt_moon_cnn_cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":63459778,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/yb_vlt_moon_cnn_cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1861464,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/yb_vlt_moon_cnn_cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":255904,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/yb_vlt_moon_cnn_cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9257,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/yb_vlt_moon_cnn_cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":4442,"MediaType":"Image"}]}]},{"ID":"5608","Title":"Planet Conjunction (Mercury and Mars)","Categories":["Sky"],"Headline":"Planet Conjunction (Mercury and Mars)","Description":"<p>A planetary conjunction happens when two planets appear close together in the sky as seen from Earth. It is a projection effect, as the planets are not really close to each other in space. Over several days, Mercury and Mars can be seen close together, with Mercury reaching a minimum angular distance of 1°48' south of Mars on 20 April 2026.</p>","Event":{"StartDate":"2026-04-20T00:00:00Z","EndDate":"2026-04-20T00:00:00Z","PeakDate":"2026-04-20T00:00:00Z","DisplayDuration":1,"Phenomenon":"Conjunction"},"PublicationDate":"2026-02-10T22:01:25Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Mercury","Mars"]},"Assets":[{"ID":"conj-ground-2017-09-16","MediaType":"Image","Title":"Planet conjunction Mercury and Mars GEN","Description":"<p>Artist's impression of a Mercury and Mars conjunction, as seen from the Earth's surface.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/Nico Bartmann/<a href=\"http://www.spaceengine.org/\">spaceengine.org</a></p>","Resources":[{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/conj-ground-2017-09-16.tif","MediaType":"Image","ResourceType":"Original","FileSize":7335748,"ProjectionType":"Tan"},{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Large","FileSize":349357,"ProjectionType":"Tan"},{"Dimensions":[1280.0,699.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Small","FileSize":54504,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5560,"ProjectionType":"Tan"},{"Dimensions":[60.0,33.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4010,"ProjectionType":"Tan"}]}]},{"ID":"5618","Title":"Eta Aquarids Meteor Shower","Categories":["Sky"],"Headline":"Eta Aquarids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Eta Aquarids meteor shower are thought to be dust left behind by the comet 1P/Halley (Halley’s comet). The meteors appear to radiate from a point on the sky in the constellation of Aquarius, very close to the star Eta Aquarii. Up to 20 shooting stars an hour can be seen at the peak, for approximately three days around 6 May 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2026-04-19T00:00:00","EndDate":"2026-05-28T00:00:00","PeakDate":"2026-05-06T00:00:00","DisplayDuration":3,"Phenomenon":"Meteor showe"},"PublicationDate":"2026-03-24T22:50:27Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Eta Aquarids","Halley's comet"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5605","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-04-17T11:52:00Z","EndDate":"2026-04-17T11:52:00Z","PeakDate":"2026-04-17T11:52:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-02-10T21:51:51Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5612","Title":"Lyrids Meteor Shower","Categories":["Sky"],"Headline":"Lyrids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Lyrids meteor shower are thought to be dust left behind by the comet C/1861 GI (Thatcher). The meteors appear to radiate from a point on the sky in the constellation of Lyra, very close to Vega, the brightest star in this constellation. Up to 20 shooting stars an hour can be seen at the peak, for approximately three days around 22 April 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2026-04-14T00:00:00Z","EndDate":"2026-04-30T00:00:00Z","PeakDate":"2026-04-22T00:00:00Z","DisplayDuration":1,"Phenomenon":"Meteor shower"},"PublicationDate":"2026-02-10T22:16:41Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Lyrids","Comet C/1861 GI"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5650","Title":"Saturn at Opposition","Categories":["Sky"],"Headline":"Saturn at Opposition","Description":"<p>A planetary opposition happens when the Sun, the Earth and one of the outer planets of the Solar System (Mars, Jupiter, Saturn, Uranus or Neptune) are all in a straight line. As seen from the Earth, on 4 October 2026 Saturn is fully illuminated by the Sun and can be observed throughout the night.</p>","Event":{"StartDate":"2026-04-10T12:21:00Z","EndDate":"2026-04-10T12:21:00Z","PeakDate":"2026-04-10T12:21:00Z","DisplayDuration":1,"Phenomenon":"Opposition"},"PublicationDate":"2026-04-22T21:48:04Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Saturn"]},"Assets":[{"ID":"saturn-bycassini-enlarged","MediaType":"Image","Title":"Saturn by Cassini","Description":"<p>This Cassini's view shows Saturn's northern hemisphere in 2016, as that part of the planet nears its northern hemisphere summer solstice in May 2017.</p>","Credit":"<p>NASA/JPL-Caltech/Space Science Institute</p>","Resources":[{"Dimensions":[3929,2000],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/saturn-bycassini-enlarged.tif","MediaType":"Image","ResourceType":"Original","FileSize":4435348,"ProjectionType":"Tan"},{"Dimensions":[3929,2000],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/saturn-bycassini-enlarged.jpg","MediaType":"Image","ResourceType":"Large","FileSize":515652,"ProjectionType":"Tan"},{"Dimensions":[1280.0,652.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/saturn-bycassini-enlarged.jpg","MediaType":"Image","ResourceType":"Small","FileSize":69713,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/saturn-bycassini-enlarged.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8005,"ProjectionType":"Tan"},{"Dimensions":[60.0,31.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/saturn-bycassini-enlarged.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4312,"ProjectionType":"Tan"}]}]},{"ID":"5604","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. 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It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. 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Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5600","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-03-11T09:38:00Z","EndDate":"2026-03-11T09:38:00Z","PeakDate":"2026-03-11T09:38:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-02-10T21:38:20Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5607","Title":"Planet Conjunction (Venus and Saturn)","Categories":["Sky"],"Headline":"Planet Conjunction (Venus and Saturn)","Description":"<p>A planetary conjunction happens when two planets appear close together in the sky as seen from Earth. It is a projection effect, as the planets are not really close to each other in space. Over several days, Venus and Saturn can be seen close together, with Venus reaching a minimum angular distance of 1°00' north of Saturn on 8 March 2026.</p>","Event":{"StartDate":"2026-03-08T22:11:00Z","EndDate":"2026-03-08T22:11:00Z","PeakDate":"2026-03-08T22:11:00Z","DisplayDuration":1,"Phenomenon":"Planetary conjunction"},"PublicationDate":"2026-02-10T21:58:15Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Venus","Saturn"]},"Assets":[{"ID":"conj-2019-12-11","MediaType":"Image","Title":"Planet Conjunction (Venus and Saturn) GEN","Description":"<p>Artist's impression of the Venus and Saturn conjunction as seen from the Earth's surface.</p>","Credit":"<p>ESO/Nico Bartmann/Vladimir Romanyuk (spaceengine.org)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/conj-2019-12-11.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":5693364,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/conj-2019-12-11.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":261670,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/conj-2019-12-11.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":57605,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/conj-2019-12-11.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6344,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/conj-2019-12-11.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":4074,"MediaType":"Image"}]}]},{"ID":"5599","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-03-03T11:38:00Z","EndDate":"2026-03-03T11:38:00Z","PeakDate":"2026-03-03T11:38:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-02-10T21:35:42Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5592","Title":"Total Lunar Eclipse","Categories":["Sky"],"Headline":"Total Lunar Eclipse","Description":"<p>A lunar eclipse occurs when the Moon passes directly behind the Earth and into its shadow. This can occur only when the Sun, Earth and Moon are almost exactly aligned. Hence, a lunar eclipse can be seen only on the night of a full Moon. During totality the Moon turns red: this happens because some of Sun's light filters through the Earth's atmosphere, such that the blue colours are scattered away and the red colours are bent towards the Moon. This eclipse will be visible in the East of Europe, Asia, Australia, North America, South America, Pacific, Atlantic, Indian Ocean, Arctic, and Antarctica.</p>","Event":{"StartDate":"2026-03-03T08:44:25Z","EndDate":"2026-03-03T14:23:06Z","PeakDate":"2026-03-03T11:33:46Z","DisplayDuration":1,"Phenomenon":"Lunar eclipse"},"PublicationDate":"2026-01-20T21:01:48Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"img_3892","MediaType":"Image","Title":"Blood Moon","Description":"<p>A full Moon with a difference is captured in this image. Sometimes called a total lunar eclipse, or 'Blood Moon', this phenomenon occurs when the Moon passes into Earth's shadow.</p>\r\n<p>For the same reasons the sky appears red at sunset, namely that red light is scattered less than blue light, the Moon is overcome with a soft red glow.</p>","Credit":"<p>D. Schreiner and S. Degezelle/ESO</p>","Resources":[{"Dimensions":[5184,3456],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/img_3892.tif","MediaType":"Image","ResourceType":"Original","FileSize":5734136,"ProjectionType":"Tan"},{"Dimensions":[5184,3456],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/img_3892.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1307229,"ProjectionType":"Tan"},{"Dimensions":[1280.0,854.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/img_3892.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57497,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/img_3892.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4688,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/img_3892.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3819,"ProjectionType":"Tan"}]}]},{"ID":"5596","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-02-24T12:28:00Z","EndDate":"2026-02-24T12:28:00Z","PeakDate":"2026-02-24T12:28:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2026-01-20T21:20:37Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5597","Title":"Mercury Occultation by the Moon","Categories":["Sky"],"Headline":"Mercury Occultation by the Moon","Description":"<p>The Moon passes in front of Mercury in the sky. This is called a lunar occultation and Mercury is in this case hidden for about 4 hours. 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It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2026-01-26T04:47:00Z","EndDate":"2026-01-26T04:47:00Z","PeakDate":"2026-01-26T04:47:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-12-10T22:30:10Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5587","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2026-01-18T19:52:00Z","EndDate":"2026-01-18T19:52:00Z","PeakDate":"2026-01-18T19:52:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-12-10T22:25:16Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5586","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2026-01-10T15:48:00Z","EndDate":"2026-01-10T15:48:00Z","PeakDate":"2026-01-10T15:48:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-12-10T22:21:46Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5589","Title":"Jupiter at Opposition","Categories":["Sky"],"Headline":"Jupiter at Opposition","Description":"<p>A planetary opposition happens when the Sun, the Earth and one of the outer planets of the Solar System (Mars, Jupiter, Saturn, Uranus or Neptune) are all in a straight line. As seen from the Earth, on 10 January 2026 Jupiter is fully illuminated by the Sun and can be observed throughout the night.</p>","Event":{"StartDate":"2026-01-10T08:34:00Z","EndDate":"2026-01-10T08:34:00Z","PeakDate":"2026-01-10T08:34:00Z","DisplayDuration":1,"Phenomenon":"Opposition"},"PublicationDate":"2025-12-10T22:34:19Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Jupiter"]},"Assets":[{"ID":"eso0123a","MediaType":"Image","Title":"Jupiter and Io","Description":"<p>This is a thermal-infrared image of Jupiter, obtained by the ISAAC multi-mode instrument at the 8.2-m VLT ANTU telescope on Paranal on November 14, 2000. On the left, the motion of the volcanic moon Io is visible.</p>","Credit":"<p>ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso0123a.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":521590,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso0123a.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":91913,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso0123a.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":162757,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso0123a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":12243,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso0123a.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":6156,"MediaType":"Image"}]}]},{"ID":"5585","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2026-01-03T10:03:00Z","EndDate":"2026-01-03T10:03:00Z","PeakDate":"2026-01-03T10:03:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-12-10T22:18:17Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5590","Title":"Quadrantids Meteor Shower","Categories":["Sky"],"Headline":"Quadrantids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by the friction against the air. The meteors in the Quadrantids meteor shower are thought to be dust left behind by the extinct Comet 2003 EH1. The meteors radiate in the sky from a point in the constellation Bootes, in a region that was once known as Quadrans Muralis. Up to 40 shooting stars an hour can be seen at its peak, for a couple of days around 3 January 2026. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2025-12-28T00:00:00Z","EndDate":"2026-01-12T00:00:00Z","PeakDate":"2026-01-03T00:00:00Z","DisplayDuration":1,"Phenomenon":"Meteor shower"},"PublicationDate":"2025-12-10T22:37:37Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Quadrantids","Comet 2003 EH1"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5582","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2025-12-27T19:10:00Z","EndDate":"2025-12-27T19:10:00Z","PeakDate":"2025-12-27T19:10:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T13:30:57Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5581","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2025-12-20T01:43:00Z","EndDate":"2025-12-20T01:43:00Z","PeakDate":"2025-12-20T01:43:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T13:28:24Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]},{"ID":"5580","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2025-12-11T20:52:00Z","EndDate":"2025-12-11T20:52:00Z","PeakDate":"2025-12-11T20:52:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T13:25:50Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5583","Title":"Geminids Meteor Shower","Categories":["Sky"],"Headline":"Geminids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Geminids meteor shower are thought to be dust left behind by the comet 3200 Phaethon. The meteors appear to radiate from a point on the sky in the constellation of Gemini, close to the star Castor. Up to 60 shooting stars an hour can be seen at the peak, for approximately three days around 13 December 2025. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2025-12-07T00:00:00Z","EndDate":"2025-12-17T00:00:00Z","PeakDate":"2025-12-13T00:00:00Z","DisplayDuration":1,"Phenomenon":"Meteor shower"},"PublicationDate":"2025-04-25T13:34:18Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Geminids","Comet 3200 Phaethon"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]},{"ID":"esocast52a","MediaType":"Video","Title":"ESOcast 52/Chile Chill 2: It's Raining Stars — Geminid meteor shower","Description":"<p>A video podcast by Gianluca Lombardi celebrating the Geminid meteor shower.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\"></div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/esocast52a.m4v","Checksum":"d9d562b65a58f8e864792102b128a682d3b5b03584a74a54dc38aa4c71084c05","MediaType":"Video","ResourceType":"Preview","FileSize":144643614,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/esocast52a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6078,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/esocast52a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":769,"ProjectionType":"Tan"}]}]},{"ID":"5579","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2025-12-04T23:14:00Z","EndDate":"2025-12-04T23:14:00Z","PeakDate":"2025-12-04T23:14:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T13:22:04Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. 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It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2025-11-28T06:59:00Z","EndDate":"2025-11-28T06:59:00Z","PeakDate":"2025-11-28T06:59:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T13:04:18Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. 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It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2025-11-20T06:47:00Z","EndDate":"2025-11-20T06:47:00Z","PeakDate":"2025-11-20T06:47:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T13:01:43Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. 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It is a projection effect, as the planets are not really close to each other in space. Over several days, Mercury and Mars can be seen close together, with Mercury reaching a minimum angular distance of 1°18' south of Mars on 12 November 2025.</p>","Event":{"StartDate":"2025-11-12T18:41:00Z","EndDate":"2025-11-12T18:41:00Z","PeakDate":"2025-11-12T18:41:00Z","DisplayDuration":1,"Phenomenon":"Conjunction"},"PublicationDate":"2025-04-25T13:12:56Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Mercury","Mars"]},"Assets":[{"ID":"conj-ground-2017-09-16","MediaType":"Image","Title":"Planet conjunction Mercury and Mars GEN","Description":"<p>Artist's impression of a Mercury and Mars conjunction, as seen from the Earth's surface.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/Nico Bartmann/<a href=\"http://www.spaceengine.org/\">spaceengine.org</a></p>","Resources":[{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/conj-ground-2017-09-16.tif","MediaType":"Image","ResourceType":"Original","FileSize":7335748,"ProjectionType":"Tan"},{"Dimensions":[3840,2097],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Large","FileSize":349357,"ProjectionType":"Tan"},{"Dimensions":[1280.0,699.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Small","FileSize":54504,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5560,"ProjectionType":"Tan"},{"Dimensions":[60.0,33.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/conj-ground-2017-09-16.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4010,"ProjectionType":"Tan"}]}]},{"ID":"5573","Title":"Third Quarter Moon","Categories":["Sky"],"Headline":"Third Quarter Moon","Description":"<p>The Third Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The First Quarter phase is also called a Half Moon. The term Third Quarter is used during the \"waning\" phase, when the lit part of the visible side of the Moon is decreasing day by day.</p>","Event":{"StartDate":"2025-11-12T05:28:00Z","EndDate":"2025-11-12T05:28:00Z","PeakDate":"2025-11-12T05:28:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T12:59:11Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"eso9903c","MediaType":"Image","Title":"The Waning Moon","Description":"<p>The waning Moon at sunrise.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/eso9903c.tif","MediaType":"Image","ResourceType":"Original","FileSize":8632368,"ProjectionType":"Tan"},{"Dimensions":[5315,7780],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/eso9903c.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2771274,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1874.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/eso9903c.jpg","MediaType":"Image","ResourceType":"Small","FileSize":285722,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/eso9903c.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7327,"ProjectionType":"Tan"},{"Dimensions":[60.0,88.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/eso9903c.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4696,"ProjectionType":"Tan"}]},{"ID":"phase-third-quarter1012-cc","MediaType":"Image","Title":"Third quarter Moon phase","Description":"<p>The Moon in its third quarter phase.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-third-quarter1012-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":10254652,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":1489109,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":206496,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":8385,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-third-quarter1012-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4575,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5576","Title":"Leonids Meteor Shower","Categories":["Sky"],"Headline":"Leonids Meteor Shower","Description":"<p>Meteors are produced when dust from space enters the Earth's atmosphere and burns up as a result of the heat generated by friction against the air. The meteors in the Leonids meteor shower are thought to be dust left behind by the comet 55P/Tempel-Tuttle. The meteors appear to radiate from a point on the sky in the constellation of Leo, close to the “Sickle stars” that are above Regulus. Up to 10 shooting stars an hour can be seen at the peak, for approximately three days around 17 November 2025. They are best viewed from a dark location after midnight.</p>","Event":{"StartDate":"2025-11-06T00:00:00","EndDate":"2025-11-30T00:00:00","PeakDate":"2025-11-17T00:00:00","DisplayDuration":3,"Phenomenon":"Meteor shower"},"PublicationDate":"2025-04-25T13:07:42Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Leonids","Comet 55P/Tempel-Tuttle"]},"Assets":[{"ID":"lasillagreenmeteor-cc","MediaType":"Image","Title":"Meteor above La Silla Observatory","Description":"<p>A colourful meteor photographed above La Silla telescope domes in the Atacama desert, Chile.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/B. Tafreshi (<a href=\"http://twanight.org/\">twanight.org</a>)</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/lasillagreenmeteor-cc.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":18020774,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/lasillagreenmeteor-cc.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":2075713,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/lasillagreenmeteor-cc.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":213370,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/lasillagreenmeteor-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9610,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/lasillagreenmeteor-cc.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5096,"MediaType":"Image"}]}]},{"ID":"5572","Title":"Full Moon","Categories":["Sky"],"Headline":"Full Moon","Description":"<p>The Full Moon is one of the four main phases of the Moon. It occurs when the Sun, the Earth and the Moon are approximately aligned, and the Moon and the Sun are on opposite sides of the Earth. In this arrangement the entire sunlit part of the Moon faces us. A Full Moon is sometimes called a “Supermoon” when the Moon is at its closest distance from Earth, as it then appears bigger and brighter than usual.</p>","Event":{"StartDate":"2025-11-05T13:19:00Z","EndDate":"2025-11-05T13:19:00Z","PeakDate":"2025-11-05T13:19:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-25T12:55:12Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"gordon-gillet_1","MediaType":"Image","Title":"Dramatic Moonset over Paranal","Description":"<p>The full Moon is about to set behind the Paranal Observatory, home to ESO's Very Large Telescope.</p>","Credit":"<p>G.Gillet/ESO</p>","Resources":[{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/gordon-gillet_1.tif","ResourceType":"Original","ProjectionType":"Tan","FileSize":10288538,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/gordon-gillet_1.jpg","ResourceType":"Large","ProjectionType":"Tan","FileSize":1350187,"MediaType":"Image"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/gordon-gillet_1.jpg","ResourceType":"Small","ProjectionType":"Tan","FileSize":302672,"MediaType":"Image"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/gordon-gillet_1.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6159,"ProjectionType":"Tan"},{"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/gordon-gillet_1.jpg","ResourceType":"Icon","ProjectionType":"Tan","FileSize":5027,"MediaType":"Image"}]},{"ID":"phase-full-cc","MediaType":"Image","Title":"The Full Moon","Description":"<p>The Full Moon, with its entire sunlit part facing us.</p>","Credit":"<p>NASA's Scientific Visualization Studio</p>","Resources":[{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/phase-full-cc.tif","MediaType":"Image","ResourceType":"Original","FileSize":12702352,"ProjectionType":"Tan"},{"Dimensions":[3240,3240],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2106465,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1280.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Small","FileSize":287153,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":10822,"ProjectionType":"Tan"},{"Dimensions":[60.0,60.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/phase-full-cc.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4928,"ProjectionType":"Tan"}]},{"ID":"almatimelapse12f","MediaType":"Video","Title":"The Full Moon and the Magellanic Clouds over ALMA","Description":"<p><span>Night time-lapse video of the ALMA antennas performing observations in the Chajnantor plain. As the sky appears to rotate clockwise, the Full Moon disappears beneath the horizon and the Magellanic Clouds take the spotlight appearing in the upper left edge of the image.</span></p>","Credit":"<p><span>ESO/C. Malin (</span><a href=\"http://christophmalin.com/\">christophmalin.com</a><span>)</span></p>","Resources":[{"Dimensions":[3840.0,2160.0],"URL":"https://cdn.eso.org/videos/ultra_hd/almatimelapse12f.mp4","MediaType":"Video","ResourceType":"Original","FileSize":33358629,"ProjectionType":"Tan"},{"Dimensions":[1280.0,720.0],"URL":"https://cdn.eso.org/videos/hd_and_apple/almatimelapse12f.m4v","MediaType":"Video","ResourceType":"Preview","FileSize":12974854,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7437,"ProjectionType":"Tan"},{"Dimensions":[60.0,34.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/almatimelapse12f.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":900,"ProjectionType":"Tan"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5569","Title":"First Quarter Moon","Categories":["Sky"],"Headline":"First Quarter Moon","Description":"<p>The First Quarter Moon is one of the four main lunar phases, also called a Half Moon. It occurs when the Moon is at an angle of 90 degrees to a line between the Earth and the Sun. In this position we see half of the Moon illuminated and the other half in shadow. The Third Quarter phase is also called a Half Moon. The term First Quarter is used during the \"waxing\" phase, when the lit part of the visible side of the Moon is increasing day by day.</p>","Event":{"StartDate":"2025-10-29T16:21:00Z","EndDate":"2025-10-29T16:21:00Z","PeakDate":"2025-10-29T16:21:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-04T12:56:17Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"potw1129a","MediaType":"Image","Title":"The waxing Moon","Description":"<p>Image of the waxing Moon showing sunlight skimming across the heavily pocked surface, filling its craters with shadows.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>\r\n<p> </p>","Credit":"<p>ESO and Andy Strappazzon</p>","Resources":[{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/potw1129a.tif","MediaType":"Image","ResourceType":"Original","FileSize":2414628,"ProjectionType":"Tan"},{"Dimensions":[2377,3679],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/potw1129a.jpg","MediaType":"Image","ResourceType":"Large","FileSize":546408,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1982.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/potw1129a.jpg","MediaType":"Image","ResourceType":"Small","FileSize":185825,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/potw1129a.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":7036,"ProjectionType":"Tan"},{"Dimensions":[60.0,93.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/potw1129a.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4570,"ProjectionType":"Tan"}]},{"ID":"moon_big_fd","MediaType":"Video","Title":"Close-up of the Moon's phases","Description":"<p>This close-up fulldome video shows the shadow that creates the Moon's phases sweeping across the surface of the Moon as it orbits Earth.</p>\r\n<p> </p>\r\n<p><strong> </strong></p>","Credit":"<p><span>NASA/LROC/M. Kornmesser</span></p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_big_fd.zip","MediaType":"Video","ResourceType":"Original","FileSize":6092681398,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_big_fd.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":81328187,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":9095,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_big_fd.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1778,"ProjectionType":"Fulldome"}]},{"ID":"moon_phases-fulldome","MediaType":"Video","Title":"Fulldome of the Moon's Phases as Seen from Space","Description":"<p>This fulldome video provides an illustration of how the Moon passes through its phases — a product of its orbit, which allows different parts of its surface to be illuminated by the Sun over the course of a month. The camera is locked to the Moon as the Earth rapidly rotates in the foreground.</p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO</p>","Resources":[{"Dimensions":[4096.0,4096.0],"URL":"https://cdn2.eso.org/videos/dome_4kmaster/moon_phases-fulldome.zip","MediaType":"Video","ResourceType":"Original","FileSize":6901451177,"ProjectionType":"Fulldome"},{"Dimensions":[1024.0,1024.0],"URL":"https://cdn.eso.org/videos/dome_preview/moon_phases-fulldome.mp4","MediaType":"Video","ResourceType":"Preview","FileSize":61831196,"ProjectionType":"Fulldome"},{"Dimensions":[220.0,140.0],"URL":"https://www.eso.org/public/archives/videos/potwmedium/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":6361,"ProjectionType":"Fulldome"},{"Dimensions":[60.0,60.0],"URL":"https://www.eso.org/public/archives/videos/newsmini/moon_phases-fulldome.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":1548,"ProjectionType":"Fulldome"}]}]},{"ID":"5568","Title":"New Moon","Categories":["Sky"],"Headline":"New Moon","Description":"<p>The New Moon is one of the four main phases of the Moon. It occurs when the Sun, the Moon and the Earth are approximately aligned, with the Moon positioned between the Sun and the Earth. In this arrangement the only part of the Moon that is lit by the Sun is the far side, the one we cannot see.</p>","Event":{"StartDate":"2025-10-21T12:25:00Z","EndDate":"2025-10-21T12:25:00Z","PeakDate":"2025-10-21T12:25:00Z","DisplayDuration":1,"Phenomenon":"Lunar phase"},"PublicationDate":"2025-04-04T12:53:58Z","Credit":"ESO","Creator":"European Southern Observatory","Contact":{"Address":"Karl-Schwarzschild-Strasse 2","City":"Garching bei München","Country":"Germany","PostalCode":"D-85748"},"Subject":{"Name":["Moon"]},"Assets":[{"ID":"15976350973788b0a6142","MediaType":"Image","Title":"Venus and Mars above the crescent Moon","Description":"<p>Venus (left) and Mars above a thin peel of the crescent Moon, seen from Paranal.</p>\r\n<p> </p>\r\n<p> </p>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/15976350973788b0a6142.tif","MediaType":"Image","ResourceType":"Original","FileSize":24902344,"ProjectionType":"Tan"},{"Dimensions":[3784,5668],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Large","FileSize":2114513,"ProjectionType":"Tan"},{"Dimensions":[1280.0,1918.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Small","FileSize":95377,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":4583,"ProjectionType":"Tan"},{"Dimensions":[60.0,90.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/15976350973788b0a6142.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":4079,"ProjectionType":"Tan"}]},{"ID":"brammer_9827","MediaType":"Image","Title":"Crescent Moon at night","Description":"<p>Image of the crescent phase of the Moon at night.</p>\r\n<p> </p>\r\n<p> </p>\r\n<div class=\"credit\">\r\n<p> </p>\r\n</div>","Credit":"<p>ESO/G. Brammer</p>","Resources":[{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/original/brammer_9827.tif","MediaType":"Image","ResourceType":"Original","FileSize":5416106,"ProjectionType":"Tan"},{"Dimensions":[4599,3046],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/large/brammer_9827.jpg","MediaType":"Image","ResourceType":"Large","FileSize":654093,"ProjectionType":"Tan"},{"Dimensions":[1280.0,848.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/screen/brammer_9827.jpg","MediaType":"Image","ResourceType":"Small","FileSize":57625,"ProjectionType":"Tan"},{"Dimensions":[220.0,140.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/potwmedium/brammer_9827.jpg","MediaType":"Image","ResourceType":"Thumbnail","FileSize":5113,"ProjectionType":"Tan"},{"Dimensions":[60.0,40.0],"URL":"https://supernova.eso.org/static/archives/exhibitionimages/newsmini/brammer_9827.jpg","MediaType":"Image","ResourceType":"Icon","FileSize":3816,"ProjectionType":"Tan"}]}]}]}