{"id":55385,"date":"2025-07-10T23:49:09","date_gmt":"2025-07-10T23:49:09","guid":{"rendered":"https:\/\/www.europesays.com\/us\/55385\/"},"modified":"2025-07-10T23:49:09","modified_gmt":"2025-07-10T23:49:09","slug":"ancient-river-systems-reveal-mars-was-wetter-than-we-thought","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/us\/55385\/","title":{"rendered":"Ancient river systems reveal Mars was wetter than we thought"},"content":{"rendered":"<p>            <img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.europesays.com\/us\/wp-content\/uploads\/2025\/07\/ancient-river-systems-1.jpg\" alt=\"Ancient river systems reveal Mars was wetter than we thought\" title=\"Color image of a flat top, heavily eroded FSR. Sand dunes can be seen migrating over the top of the FSR. Credit: HiRISE Image: ESP_085386_1505 NASA\/JPL\/University of Arizona\" width=\"800\" height=\"530\"\/><\/p>\n<p>                Color image of a flat top, heavily eroded FSR. Sand dunes can be seen migrating over the top of the FSR. Credit: HiRISE Image: ESP_085386_1505 NASA\/JPL\/University of Arizona<\/p>\n<p>The discovery of more than 15,000 kilometers of ancient riverbeds on Mars suggests that the Red Planet may once have been much wetter than previously thought.<\/p>\n<p>Researchers looked at fluvial sinuous ridges, also known as inverted channels, across Noachis Terra\u2014a region in Mars&#8217; southern highlands. These are believed to have formed when sediment deposited by rivers hardened and was later exposed as the surrounding material eroded.<\/p>\n<p>Similar ridges have been found across a range of terrains on Mars. Their presence suggests that flowing water was once widespread in this region of Mars, with precipitation being the most likely source of this water.<\/p>\n<p>The new <a href=\"https:\/\/conference.astro.dur.ac.uk\/event\/7\/contributions\/607\/\" target=\"_blank\" rel=\"noopener\">research<\/a>, led by Adam Losekoot\u2014a Ph.D. student at the Open University, is being presented today at the <a href=\"https:\/\/conference.astro.dur.ac.uk\/event\/7\/\" target=\"_blank\" rel=\"noopener\">Royal Astronomical Society&#8217;s National Astronomy Meeting 2025<\/a> in Durham.<\/p>\n<p>The findings indicate that <a href=\"https:\/\/phys.org\/tags\/surface+water\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">surface water<\/a> may have been stable in Noachis Terra during the Noachian-Hesperian transition, a period of geologic and climatic change around 3.7 billion years ago.<\/p>\n<p>Noachis Terra has not been studied as extensively as other regions of Mars, in part because it contains few <a href=\"https:\/\/phys.org\/tags\/valley+networks\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">valley networks<\/a>, which are branching erosional features that have traditionally been used to infer historical rainfall and runoff.<\/p>\n<p>The study instead focuses on fluvial sinuous ridges as an alternate form of evidence for ancient surface water.<\/p>\n<p>&#8220;Studying Mars, particularly an underexplored region like Noachis Terra, is really exciting because it&#8217;s an environment which has been largely unchanged for billions of years. It&#8217;s a <a href=\"https:\/\/phys.org\/tags\/time+capsule\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">time capsule<\/a> that records fundamental geological processes in a way that just isn&#8217;t possible here on Earth,&#8221; said Losekoot.<\/p>\n<p>            <img decoding=\"async\" src=\"https:\/\/www.europesays.com\/us\/wp-content\/uploads\/2025\/07\/ancient-river-systems.jpg\" alt=\"Ancient river systems reveal Mars was wetter than we thought\" title=\"A moderately eroded fluvial sinuous ridge (FSR), with lots of small craters in it, that stands out clearly above the surrounding material. To the north east it emerges from a small valley and becomes progressively clearer to the west, until it disappears. There is a clear curve in the FSR, likely a meander. North of the FSR is a round, flat feature that was likely an impact crater which was filled with water or sediment. CTX image: MurrayLab_V01_E020_N-20_Mosaic. Credit: NASA\/JPL\/MSSS\/The Murray Lab\"\/><\/p>\n<p>                A moderately eroded fluvial sinuous ridge (FSR), with lots of small craters in it, that stands out clearly above the surrounding material. To the north east it emerges from a small valley and becomes progressively clearer to the west, until it disappears. There is a clear curve in the FSR, likely a meander. North of the FSR is a round, flat feature that was likely an impact crater which was filled with water or sediment. CTX image: MurrayLab_V01_E020_N-20_Mosaic. Credit: NASA\/JPL\/MSSS\/The Murray Lab<\/p>\n<p>He and his team used data from three orbital instruments: the Context Camera (CTX), the Mars Orbiter Laser Altimeter (MOLA) and the High Resolution Imaging Science Experiment (HiRISE).<\/p>\n<p>These <a href=\"https:\/\/phys.org\/tags\/datasets\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">datasets<\/a> allowed the team to map the locations, lengths and morphologies of ridge systems across a wide area.<\/p>\n<p>Many of the features appear as isolated ridge segments, while others form systems extending for hundreds of kilometers and rising tens of meters above the surrounding terrain.<\/p>\n<p>The broad distribution and form of these ridges suggest that they likely formed over a geologically significant period under relatively stable surface conditions.<\/p>\n<p>The <a href=\"https:\/\/phys.org\/tags\/spatial+distribution\/\" rel=\"tag noopener\" class=\"textTag\" target=\"_blank\">spatial distribution<\/a> and extent of the features indicate that the water source was precipitation.<\/p>\n<p>&#8220;Our work is a new piece of evidence that suggests that Mars was once a much more complex and active planet than it is now, which is such an exciting thing to be involved in,&#8221; said Losekoot.<\/p>\n<p>The fact that the ridges form extensive interconnected systems suggests that the watery conditions must have been relatively long-lived, meaning Noachis Terra experienced warm and wet conditions for a geologically relevant period.<\/p>\n<p>These findings challenge existing theories that Mars was generally cold and dry, with a few valleys formed by ice-sheet meltwater in sporadic, short periods of warming.<\/p>\n<p><strong>More information:<\/strong><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tThe Fluvial History of Noachis Terra, Mars, <a href=\"https:\/\/conference.astro.dur.ac.uk\/event\/7\/contributions\/607\/\" target=\"_blank\" rel=\"noopener\">conference.astro.dur.ac.uk\/eve \u2026 7\/contributions\/607\/<\/a><\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t\tProvided by<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a href=\"https:\/\/phys.org\/partners\/royal-astronomical-society\/\" target=\"_blank\" rel=\"noopener\">Royal Astronomical Society<\/a><br \/>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<a class=\"icon_open\" href=\"http:\/\/www.ras.org.uk\/\" target=\"_blank\" rel=\"nofollow noopener\"><\/p>\n<p>\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t\t<strong>Citation<\/strong>:<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tAncient river systems reveal Mars was wetter than we thought (2025, July 9)<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tretrieved 10 July 2025<br \/>\n\t\t\t\t\t\t\t\t\t\t\t\tfrom https:\/\/phys.org\/news\/2025-07-ancient-river-reveal-mars-wetter.html\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n<p>\n\t\t\t\t\t\t\t\t\t\t\t This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no<br \/>\n\t\t\t\t\t\t\t\t\t\t\t part may be reproduced without the written permission. The content is provided for information purposes only.\n\t\t\t\t\t\t\t\t\t\t\t <\/p>\n","protected":false},"excerpt":{"rendered":"Color image of a flat top, heavily eroded FSR. Sand dunes can be seen migrating over the top&hellip;\n","protected":false},"author":3,"featured_media":55386,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[493,494,492,489,159,490,158,491,67,132,68],"class_list":{"0":"post-55385","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-science","8":"tag-materials","9":"tag-nanotech","10":"tag-physics","11":"tag-physics-news","12":"tag-science","13":"tag-science-news","14":"tag-technology","15":"tag-technology-news","16":"tag-united-states","17":"tag-unitedstates","18":"tag-us"},"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@us\/114831619822880102","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts\/55385","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/comments?post=55385"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts\/55385\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/media\/55386"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/media?parent=55385"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/categories?post=55385"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/tags?post=55385"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}