{"id":793460,"date":"2025-02-09T06:47:05","date_gmt":"2025-02-09T11:47:05","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=793460"},"modified":"2025-02-09T06:47:05","modified_gmt":"2025-02-09T11:47:05","slug":"are-grooves-on-uranus-moon-ariel-evidence-for-an-ocean","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=793460","title":{"rendered":"Are grooves on Uranus\u2019 moon Ariel evidence for an ocean?"},"content":{"rendered":"<p> <br \/>\n<\/p>\n<div>\n<figure id=\"attachment_501333\" aria-describedby=\"caption-attachment-501333\" style=\"width: 800px\" class=\"wp-caption aligncenter\"><figcaption id=\"caption-attachment-501333\" class=\"wp-caption-text\">View larger. | NASA\u2019s Voyager 2 spacecraft captured this view of Uranus\u2019 moon Ariel on January 24, 1986. We can clearly see various canyons and grooves. Image via NASA\/ Jet Propulsion Laboratory.<\/figcaption><\/figure>\n<ul>\n<li><strong>Uranus\u2019 moon Ariel might have a subsurface ocean<\/strong>, a study found last year. The ocean could be ancient or it could still exist today.<\/li>\n<li><strong>A new study of unusual grooves on Ariel<\/strong> suggests that carbon materials on the moon\u2019s surface originate from deep below.<\/li>\n<li><strong>The carbon could come from the subsurface ocean,<\/strong> although scientists haven\u2019t proven a link yet.<\/li>\n<\/ul>\n<h3>Uranus\u2019 moon Ariel is groovy<\/h3>\n<p>The hidden oceans on some moons of Jupiter and Saturn \u2013 such as Europa, Enceladus and others \u2013 are well-known. Then last year, scientists using NASA\u2019s Webb Space Telescope found evidence for a possible subsurface ocean on Uranus\u2019 moon Ariel as well. Now, a new study from researchers at Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, adds to the earlier findings. The researchers said on February 3, 2025, that carbon molecules on the surface, including carbon dioxide ice, might be coming up through trench-like grooves in Ariel\u2019s canyons. The carbon might have originated from a subsurface ocean.<\/p>\n<p>The research team published their peer-reviewed findings in <em>The Planetary Science Journal<\/em> on February 3, 2025.<\/p>\n<p>2025 EarthSky lunar calendar is available now. A unique and beautiful poster-sized calendar with phases of the moon for every night of the year. Get yours today!<\/p>\n<h3>Carbon from deep grooves on Uranus\u2019 moon Ariel?<\/h3>\n<p>Ariel has carbon dioxide ice and other carbon deposits on its surface. How did they get there? The study last year suggested they originated from within the moon itself instead of external sources. They might even be from a subsurface ocean, similar to ones on other icy moons in the outer solar system.<\/p>\n<p>Now, the new study from Johns Hopkins shows <em>how<\/em> those materials might reach the surface. The answer might be what scientists call <em>medial grooves<\/em>. Those are trenches within Ariel\u2019s larger canyons. Chloe Beddingfield, lead author of the new study at Johns Hopkins, said:<\/p>\n<blockquote>\n<p>If we\u2019re right, these medial grooves are probably the best candidates for sourcing those carbon oxide deposits and uncovering more details about the moon\u2019s interior. No other surface features show evidence of facilitating the movement of materials from inside Ariel, making this finding particularly exciting.<\/p>\n<\/blockquote>\n<blockquote class=\"bluesky-embed\" data-bluesky-uri=\"at:\/\/did:plc:len5cwjgxo4n444c4hqglj2l\/app.bsky.feed.post\/3lhcf6gvbmk2h\" data-bluesky-cid=\"bafyreiaay3t7wpkuisty6mrhqcvqr65x3sxw3np4rduneqfn5bfkkx6m6u\">\n<p lang=\"en\">New research from Johns Hopkins APL suggests grooves on Uranus&#8217; moon Ariel may act as spreading centers, transporting materials between its interior and surface, similar to tectonic and volcanic activity on Earth. jhuapl.link\/505<\/p>\n<p>\u2014 Johns Hopkins APL (@jhuapl.bsky.social) 2025-02-03T20:32:00.274Z<\/p>\n<\/blockquote>\n<h3>Earth-like spreading centers<\/h3>\n<p>The researchers said the grooves are likely what scientists call spreading centers. On Earth, they are the linear boundary between two diverging lithospheric plates \u2013 regions of Earth\u2019s crust and upper mantle that are fractured into plates \u2013 on the ocean floor. As they move apart, molten rock wells up to fill the gap. It solidifies, creating new oceanic crust.<\/p>\n<p>A similar process might be occurring on Ariel. Heat from Ariel\u2019s interior could cause carbon-rich material to move upward, splitting the surface and creating the grooves.<\/p>\n<p>The researchers also considered volcanic conduits or fissures to explain the grooves. But after studying old images from NASA\u2019s Voyager 2 spacecraft, spreading centers became the most likely explanation. Voyager 2 passed by Uranus and its moons in January 1986. It is still the only mission to do so.<\/p>\n<p>The images provided important clues. For example, the canyon walls flanking the trenches fit together like puzzle pieces when their central floors were digitally removed. In addition, the canyon floors displayed regularly spaced ridges in some locations. This was also consistent with a series of material depositions.<\/p>\n<figure id=\"attachment_501338\" aria-describedby=\"caption-attachment-501338\" style=\"width: 650px\" class=\"wp-caption aligncenter\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/earthsky.org\/upl\/2025\/02\/Ariel-medial-groove-Voyager-2-January-24-1986.jpg\" alt=\"Overhead view of gray terrain with thin grooves and small hills. A black arrow points to 1 groove.\" width=\"650\" height=\"1224\" class=\"size-full wp-image-501338\" srcset=\"https:\/\/earthsky.org\/upl\/2025\/02\/Ariel-medial-groove-Voyager-2-January-24-1986.jpg 650w, https:\/\/earthsky.org\/upl\/2025\/02\/Ariel-medial-groove-Voyager-2-January-24-1986-159x300.jpg 159w, https:\/\/earthsky.org\/upl\/2025\/02\/Ariel-medial-groove-Voyager-2-January-24-1986-544x1024.jpg 544w\" sizes=\"auto, (max-width: 650px) 100vw, 650px\"\/><figcaption id=\"caption-attachment-501338\" class=\"wp-caption-text\">View larger. | A medial groove on Ariel (highlighted by arrow) that Voyager 2 saw in 1986. The new study suggests these grooves are spreading centers similar to ones on Earth, where 2 sections of the crust are moving apart and material upwells from below to fill in the gap. Image via NASA\/ Jet Propulsion Laboratory\/ Johns Hopkins Applied Physics Laboratory.<\/figcaption><\/figure>\n<h3>Does Ariel have an ocean?<\/h3>\n<p>The findings strongly suggest that the carbon on Ariel\u2019s surface came from below. But is it from an ocean? As the study last year demonstrated, there is evidence suggesting the existence of an ocean below the icy crust. Scientists know Ariel and some other Uranian moons have had multiple periods of strong geological activity. Tidal forces likely drove that activity. This can cause cycles of heating, melting and freezing inside those moons. So Ariel likely had some kind of ocean and it might still be liquid today.<\/p>\n<p>The grooves and a possible ocean could help explain how short-lived carbon oxides are able to remain present on Ariel\u2019s surface. As co-author Tom Nordheim at Johns Hopkins explained:<\/p>\n<blockquote>\n<p>These new results suggest a possible mechanism for emplacing fresh material and short-lived compounds, including carbon monoxide and perhaps ammonia-bearing species on the surface.<\/p>\n<\/blockquote>\n<p>Beddingfield added:<\/p>\n<blockquote>\n<p>It\u2019s a fascinating situation, how this cycle affects these moons, their evolution and their characteristics.<\/p>\n<\/blockquote>\n<h3>Still a lot of unknowns<\/h3>\n<p>Scientists haven\u2019t proven the link between the trenches and a possible ocean quite yet, however. Beddingfield said:<\/p>\n<blockquote>\n<p>The size of Ariel\u2019s possible ocean and its depth beneath the surface can only be estimated, but it may be too isolated to interact with spreading centers. There\u2019s just a lot we don\u2019t know. And while carbon oxide ices are present on Ariel\u2019s surface, it\u2019s still unclear whether they\u2019re associated with the grooves because Voyager 2 didn\u2019t have instruments that could map the distribution of ices.<\/p>\n<\/blockquote>\n<p>Scientists say that another moon of Uranus, Miranda, also likely had an ocean. And that ocean might still exist today as well.<\/p>\n<h3>New mission to Uranus needed<\/h3>\n<p>As of now, the Voyager 2 images are still the best we have. A new mission \u2013 such as the proposed Uranus Orbiter and Probe (UOP) mission \u2013 will be necessary to further explore Uranus and its moons. Richard Cartwright at Johns Hopkins, who led last year\u2019s study, said:<\/p>\n<blockquote>\n<p>We need an orbiter that can make close passes of Ariel, map its medial grooves in detail, and analyze their spectral signatures for components like carbon dioxide and carbon monoxide. If carbon-bearing molecules are concentrated along these grooves, then it would strongly support the idea that they\u2019re windows into Ariel\u2019s interior.<\/p>\n<\/blockquote>\n<p>And as the paper noted:<\/p>\n<blockquote>\n<p>The medial grooves are some of the youngest geologic features observed on Ariel, and close flybys of these features by a future Uranus orbiter are imperative to gain insight into recent geologic events and the geologic and geochemical properties of this candidate ocean world.<\/p>\n<\/blockquote>\n<p>Bottom line: Deep trenches are the likely source of carbon on the surface of Uranus\u2019 moon Ariel and might be connected to a subsurface ocean, a new study suggests.<\/p>\n<p>Source: Ariel\u2019s Medial Grooves: Spreading Centers on a Candidate Ocean World<\/p>\n<p>Via Johns Hopkins Applied Physics Laboratory<\/p>\n<p>Read more: Does Uranus\u2019 moon Ariel have a hidden ocean?<\/p>\n<p>Read more: Evidence for ocean on Uranus moon Miranda is a surprise<\/p>\n<p><span class=\"cp-load-after-post\"\/><\/div>\n<div>\n<div class=\"post-author\">\n<h4>Paul Scott Anderson<\/h4>\n<p>                    View Articles\n                  <\/p><\/div>\n<div class=\"post-tags\">\n<h6 data-udy-fe=\"text_7c58270d\">About the Author:<\/h6>\n<p>Paul Scott Anderson has had a passion for space exploration that began when he was a child when he watched Carl Sagan\u2019s Cosmos. He studied English, writing, art and computer\/publication design in high school and college. He later started his blog The Meridiani Journal in 2005, which was later renamed Planetaria. He also later started the blog Fermi Paradoxica, about the search for life elsewhere in the universe.&#13;<br \/>\n&#13;<br \/>\nWhile interested in all aspects of space exploration, his primary passion is planetary science and SETI. In 2011, he started writing about space on a freelance basis with Universe Today. He has also written for SpaceFlight Insider and AmericaSpace and has also been published in The Mars Quarterly. He also did some supplementary writing for the iOS app Exoplanet.&#13;<br \/>\n&#13;<br \/>\nHe has been writing for EarthSky since 2018, and also assists with proofing and social media.<\/p>\n<\/p><\/div>\n<\/p><\/div>\n<p><br \/>\n<br \/><a href=\"https:\/\/earthsky.org\/space\/uranus-moon-ariel-trenches-geology-ocean-moons\/?rand=772280\">Source link <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>View larger. | NASA\u2019s Voyager 2 spacecraft captured this view of Uranus\u2019 moon Ariel on January 24, 1986. We can clearly see various canyons and grooves. Image via NASA\/ Jet&hellip; <\/p>\n","protected":false},"author":1,"featured_media":793461,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[46],"tags":[],"class_list":["post-793460","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-earth-sky"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/793460","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\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=793460"}],"version-history":[{"count":0,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/793460\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/793461"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=793460"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=793460"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=793460"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}