{"id":554753,"date":"2018-12-10T04:00:00","date_gmt":"2018-12-10T08:00:00","guid":{"rendered":"https:\/\/spaceweekly.com\/?guid=7ce0cf98f352fddf47433f38afe64080"},"modified":"2018-12-10T04:00:00","modified_gmt":"2018-12-10T08:00:00","slug":"dione-and-rhea-appear-as-one","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=554753","title":{"rendered":"Dione and Rhea appear as one"},"content":{"rendered":"

\t\t\t\t\t<\/p>\n

\nSometimes it\u2019s all about perspective. This very convincing image of a conjoined moon masquerading as a snowman is actually two separate Saturnian moons \u2013 Dione and Rhea \u2013 taken from such an angle by the international Cassini spacecraft that they appear as one.\n<\/p>\n

\nDione (top) was actually closer to the spacecraft at the time the image was taken, at  around 1.1 million kilometres, compared to Rhea (bottom) which was around 1.6 million kilometres from Cassini. Dione has a diameter of 1123 kilometres and Rhea is larger with a diameter of 1528 kilometres, but they appear to have a similar size in this image due to the difference in distance.\n<\/p>\n

\nThe moons also orbit Saturn at different distances: Dione lies at roughly the same distance as the Moon from the Earth and orbits around the ringed planet in just 2.7 days, while Rhea sits slightly further away and has a 4.5 day orbit.\n<\/p>\n

\nDione has a large crater called Evander, centred at the south polar region, which allows the two moons to blend seamlessly together in this view. They also have a similar reflectivity, contributing to the snowman-like appearance, while also pointing to a comparable surface composition.\n<\/p>\n

\nDione is made of around one third rock, comprising the core, and two thirds ice with a suspected subsurface ocean.\n<\/p>\n

\nInterestingly, the moon is more heavily cratered on the hemisphere that faces away from the direction of motion compared to the hemisphere that faces the direction of motion, opposite to what is expected as the forward facing side of the moon should be bombarded with more material. This unusual cratering pattern suggests that it suffered an impact which spun the moon around 180 degrees.\n<\/p>\n

\nRhea is Saturn\u2019s second largest moon, after Titan, and is similar to Dione in density, but is around one quarter rock mixed with three quarters ice \u2013 a giant frozen dirty snowball.\n<\/p>\n

\nThe image was taken on 27 July 2010 by Cassini in visible light using the narrow-angle camera. The resolution is seven kilometres per pixel on Dione and ten kilometres per pixel on Rhea. Saturn is towards the right and out of view. The Cassini mission is a cooperative project of NASA, ESA and Italy\u2019s ASI space agency. The mission concluded in September 2017<\/a>.<\/p>\n","protected":false},"excerpt":{"rendered":"

<\/p>\n

\nSometimes it’s all about perspective. This very convincing image of a conjoined moon masquerading as a snowman is actually two separate Saturnian moons – Dione and Rhea – taken from such an angle by the international Cassini spacecraft that they appear as one.\n<\/p>\n

\nDione (top) was actually closer to the spacecraft at the time the image was taken, at  around 1.1 million kilometres, compared to Rhea (bottom) which was around 1.6 million kilometres from Cassini. Dione has a diameter of 1123 kilometres and Rhea is larger with a diameter of 1528 kilometres, but they appear to have a similar size in this image due to the difference in distance.\n<\/p>\n

\nThe moons also orbit Saturn at different distances: Dione lies at roughly the same distance as the Moon from the Earth and orbits around the ringed planet in just 2.7 days, while Rhea sits slightly further away and has a 4.5 day orbit.\n<\/p>\n

\nDione has a large crater called Evander, centred at the south polar region, which allows the two moons to blend seamlessly together in this view. They also have a similar reflectivity, contributing to the snowman-like appearance, while also pointing to a comparable surface composition.\n<\/p>\n

\nDione is made of around one third rock, comprising the core, and two thirds ice with a suspected subsurface ocean.\n<\/p>\n

\nInterestingly, the moon is more heavily cratered on the hemisphere that faces away from the direction of motion compared to the hemisphere that faces the direction of motion, opposite to what is expected as the forward facing side of the moon should be bombarded with more material. This unusual cratering pattern suggests that it suffered an impact which spun the moon around 180 degrees.\n<\/p>\n

\nRhea is Saturn’s second largest moon, after Titan, and is similar to Dione in density, but is around one quarter rock mixed with three quarters ice – a giant frozen dirty snowball.\n<\/p>\n

\nThe image was taken on 27 July 2010 by Cassini in visible light using the narrow-angle camera. The resolution is seven kilometres per pixel on Dione and ten kilometres per pixel on Rhea. Saturn is towards the right and out of view. The Cassini mission is a cooperative project of NASA, ESA and Italy’s ASI space agency. The mission concluded in September 2017<\/a>.<\/p>\n","protected":false},"author":5,"featured_media":615444,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[27],"tags":[],"class_list":["post-554753","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-multimedia"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/554753","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=554753"}],"version-history":[{"count":1,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/554753\/revisions"}],"predecessor-version":[{"id":554754,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/554753\/revisions\/554754"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/615444"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=554753"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=554753"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=554753"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}