{"id":292191,"date":"2026-01-19T13:10:09","date_gmt":"2026-01-19T13:10:09","guid":{"rendered":"https:\/\/www.europesays.com\/ie\/292191\/"},"modified":"2026-01-19T13:10:09","modified_gmt":"2026-01-19T13:10:09","slug":"deltas-and-canyons-on-mars-hint-at-ocean-that-covered-half-the-planet","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/ie\/292191\/","title":{"rendered":"Deltas and Canyons on Mars Hint at Ocean That Covered Half the Planet"},"content":{"rendered":"<p><a href=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/01\/44453_2025_15_Fig1_HTML_20260113_171840.webp.webp\"><img src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/01\/44453_2025_15_Fig1_HTML_20260113_171840.webp.webp\" height=\"455\" width=\"1000\"   class=\"wp-image-297406 sp-no-webp no-lazy\" alt=\"- Terrain elevation and topography maps of Mars with color-coded altitude legend.\" fetchpriority=\"high\" decoding=\"async\"\/> <\/a>The location of the research area in Southeast Coprates Chasma. Credit: Argadestya et al. 2026<\/p>\n<p><a href=\"https:\/\/www.zmescience.com\/science\/news-science\/new-mineral-mars\/\" rel=\"nofollow noopener\" target=\"_blank\">Mars <\/a>today is a frozen, dusty desert. But if you look deep inside Valles Marineris, the largest canyon system on Mars and in the Solar System, you find familiar landforms. They resemble river deltas, those fan-shaped deposits that form on Earth where rushing <a href=\"https:\/\/www.zmescience.com\/ecology\/new-global-river-map-is-the-first-to-include-river-bifurcations-and-canals\/\" data-wpil-monitor-id=\"3500\" rel=\"nofollow noopener\" target=\"_blank\">rivers crash into still waters<\/a>.<\/p>\n<p>On our planet, these structures mark a shoreline. Scientists now believe they serve the exact same purpose on Mars.<\/p>\n<p>In a new study published in <a href=\"https:\/\/www.nature.com\/articles\/s44453-025-00015-8\" rel=\"nofollow noopener\" target=\"_blank\">npj Space Exploration<\/a>, researchers report three delta-like features along the southeastern edge of Coprates Chasma, a massive sub-canyon near the Martian equator. The team argues that these deposits record the highest proposed levels of an <a href=\"https:\/\/www.zmescience.com\/science\/geology\/leeches-silurian-not-bloodsucking\/\" data-wpil-monitor-id=\"3499\" rel=\"nofollow noopener\" target=\"_blank\">ancient ocean<\/a>, dating to about three billion years ago.<\/p>\n<p>An Old Shoreline<\/p>\n<p><a href=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/01\/44453_2025_15_Fig2_HTML_20260113_172652.webp.webp\"><img loading=\"lazy\" height=\"1000\" width=\"983\" class=\"wp-image-297408 sp-no-webp perfmatters-lazy\" alt=\"Valley topography map showing elevation and landforms, with detailed analysis of terrain features and geological structures.\" decoding=\"async\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/01\/44453_2025_15_Fig2_HTML_20260113_172652.webp.webp\"  data-\/> <\/a>The SFDs are located along the northern margin of the promontory in Southeast Coprates Chasma. The dashed black line indicates the boundary of the deposits. Credit: Argadestya et al. 2026<\/p>\n<p>The formations in question are technically called \u201cscarp-fronted deposits\u201d (SFDs). They sit at the foot of a rocky rise in Southeast Coprates Chasma, a huge <a href=\"https:\/\/www.zmescience.com\/science\/news-science\/mars-grand-canyon-harbors-copious-amounts-of-water-beneath-its-surface\/\" data-wpil-monitor-id=\"3496\" rel=\"nofollow noopener\" target=\"_blank\">canyon on Mars<\/a>. From that high ground, networks of <a href=\"https:\/\/www.zmescience.com\/science\/physics\/hotspot-magma-plume-seismic-tomography-10092013\/\" data-wpil-monitor-id=\"3497\" rel=\"nofollow noopener\" target=\"_blank\">channels flow<\/a> downhill and fan out, leaving behind broad, wedge-shaped piles of sediment.<\/p>\n<p>On Earth, you see this combination of upstream channels and downstream fans where rivers empty into lakes or seas. The research team, led by the University of Bern, analyzed the geometry and concluded the same process was at work here.<\/p>\n<p>To prove it, the researchers combined images from several orbiting spacecraft. They used NASA\u2019s CTX and HiRISE cameras aboard <a href=\"https:\/\/science.nasa.gov\/mission\/mars-reconnaissance-orbiter\/\" rel=\"nofollow noopener\" target=\"_blank\">Mars Reconnaissance Orbiter<\/a>, along with the color imaging system CaSSIS on ESA\u2019s <a href=\"https:\/\/esoc.esa.int\/content\/exomarstgo\" rel=\"nofollow noopener\" target=\"_blank\">ExoMars Trace Gas Orbiter<\/a>. They also relied on precise elevation data from multiple digital terrain models.<\/p>\n<p>\u201cThe unique high-resolution satellite images of Mars have enabled us to study the Martian landscape in great detail by surveying and mapping,\u201d said Ignatius Argadestya, the study\u2019s lead author and a PhD student at the University of Bern.<\/p>\n<p>But the smoking gun wasn\u2019t just the shape\u2014it was the elevation. All three deltas sit at nearly the same height above the Martian datum (between -3,750 and -3,650 meters). That consistency is key. On Earth, when you find <a href=\"https:\/\/www.zmescience.com\/science\/tectonic-model-beatiful-new\/\" data-wpil-monitor-id=\"3498\" rel=\"nofollow noopener\" target=\"_blank\">geological features<\/a> at the same height across a wide area, it usually signals a former water level.<\/p>\n<p>\u00d7<\/p>\n<p>                        Thank you! One more thing&#8230;<\/p>\n<p>Please check your inbox and confirm your subscription.<\/p>\n<p><a href=\"https:\/\/pubmed.ncbi.nlm.nih.gov\/15232103\/\" rel=\"nofollow noopener\" target=\"_blank\">Earlier studies <\/a>had hinted at ancient water in Valles Marineris, but they lacked this level of detail. \u201cEarlier claims were based on less precise data and partly on indirect arguments,\u201d said Fritz Schlunegger, a study co-author. \u201cOur reconstruction of the sea level, on the other hand, is based on clear evidence for such a coastline.\u201d<\/p>\n<p>The Northern Ocean<\/p>\n<p><a href=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/01\/44453_2025_15_Fig7_HTML_20260113_182636.jpg\"><img loading=\"lazy\" height=\"568\" width=\"821\" class=\"wp-image-297411 sp-no-webp perfmatters-lazy\" alt=\"- Color-coded map showing geological features and paleo shoreline in Chryse Chaos, Mars.\" decoding=\"async\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/01\/44453_2025_15_Fig7_HTML_20260113_182636.jpg\"  data-\/> <\/a>The westward extension of the inferred paleoshoreline identified in the study area (red rectangle) across the Valles Marineris depression into Chryse Chaos. Credit:  Argadestya et al. 2026<\/p>\n<p>If these were isolated features, we might write them off as local anomalies. But the Coprates Chasma deltas have company. Researchers have identified similar fan-shaped deposits in Capri Chasma, Chryse Chaos, and Hydraotes Chaos. These are the regions that connect the equatorial canyon system to Mars\u2019 vast northern lowlands.<\/p>\n<p>Taken together, these features line up along a broad elevation band that stretches hundreds of kilometers. The study interprets this alignment as a paleoshoreline, tracing the edge of an ocean that once covered much of Mars\u2019 northern hemisphere.<\/p>\n<p>\u201cWith our study, we were able to provide evidence for the deepest and largest former ocean on Mars to date\u2014an ocean that stretched across the northern hemisphere of the planet,\u201d said Argadestya.<\/p>\n<p>Planetary scientists have argued about a Martian ocean for decades. Some evidence comes from minerals that only form in water; other clues are hidden in valley networks carved by flowing liquid eons ago. This new work adds specific landforms whose shapes and elevations match coastal deltas on Earth almost perfectly.<\/p>\n<p>It reflects a broader trend in Mars science: as our images get better, we can read the Red Planet the same way geologists read Earth. Layer by layer, we are finding patterns shaped by water, wind, and time.<\/p>\n<p>Just Like Earth<\/p>\n<p><a href=\"https:\/\/cdn.zmescience.com\/wp-content\/uploads\/2026\/01\/Mars_with_Oceans_27891525397-scaled.jpg\" rel=\"nofollow noopener\" target=\"_blank\"><img loading=\"lazy\" height=\"1024\" width=\"1024\" class=\"wp-image-297412 sp-no-webp perfmatters-lazy\" alt=\"depiction of Mars covered by an ocean\" decoding=\"async\" src=\"https:\/\/www.europesays.com\/ie\/wp-content\/uploads\/2026\/01\/Mars_with_Oceans_27891525397-1024x1024.jpg\"  data-\/> <\/a>Artistic depiction of Mars with an ocean. Image via Wikpiedia.<\/p>\n<p>On Earth, deltas are among the most dynamic and fertile environments, concentrating sediments and preserving chemical traces of their surroundings. For Mars, that makes them especially interesting.<\/p>\n<p>The period identified in the study\u2014the transition from the Late Hesperian to the Early Amazonian\u2014may represent the last era when surface water was widespread. \u201cWe consider this as the time with the largest availability of surface water on Mars,\u201d the authors write in the paper.<\/p>\n<p>Today, the deltas in Coprates Chasma lie partly buried beneath the dunes. Yet their outlines remain visible from orbit, frozen in place as the <a href=\"https:\/\/www.zmescience.com\/science\/water-scarcity-2025-23032016\/\" data-wpil-monitor-id=\"3495\" rel=\"nofollow noopener\" target=\"_blank\">climate changed and water<\/a> disappeared.<\/p>\n<p>The discovery does not prove that life ever existed on Mars. But it strengthens the case that the planet once offered stable bodies of water\u2014places where chemistry could unfold slowly, and where signs of past habitability might still be preserved.<\/p>\n<p>\u201cWe know Mars as a dry, red planet,\u201d Argadestya said. \u201cHowever, our results show that it was a blue planet in the past, similar to Earth.\u201d<\/p>\n","protected":false},"excerpt":{"rendered":"The location of the research area in Southeast Coprates Chasma. Credit: Argadestya et al. 2026 Mars today is&hellip;\n","protected":false},"author":2,"featured_media":292192,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[77],"tags":[145736,18,19,17,1203,2438,145737,8197,133,145738,111683],"class_list":{"0":"post-292191","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-science","8":"tag-deltas","9":"tag-eire","10":"tag-ie","11":"tag-ireland","12":"tag-mars","13":"tag-mars-geology","14":"tag-martian-ocean","15":"tag-planetary-science","16":"tag-science","17":"tag-valles-marineris","18":"tag-water-on-mars"},"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@ie\/115921933010533507","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/292191","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/comments?post=292191"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/posts\/292191\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media\/292192"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/media?parent=292191"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/categories?post=292191"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/ie\/wp-json\/wp\/v2\/tags?post=292191"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}