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\n Sedimentologic and mineralogic evidence for sedimentary rocks, clay stratigraphy and open-basin deltas along and within the detected shelf. a,b, Polar stereographic projections of the detected shelf showing 14,386 mounds interpreted to have formed by dichotomy retreat, consisting of thick-layered deposits up to 500 m in southern Chryse Planitia, Mars, along with widespread clay-bearing stratigraphy and open-basin deltas. \u2014 Nature <\/p>\n
Caltech researchers have identified geological features on Mars that could point to the existence of a long-dried ocean that once covered a third of the Red Planet\u2019s surface.<\/p>\n
The research was conducted by former Caltech postdoctoral scholar Abdallah Zaki and Caltech professor of geology Michael Lamb. The study is described in a paper appearing in the journal Nature on April 15.<\/p>\n
As a key ingredient for life, water on other bodies in the solar system is a major area of study. While it is widely accepted that Mars once had some amount of liquid water on its surface, it is still unclear whether that water was limited to lakes and streams, or if there was enough to form long-lasting oceans.<\/p>\n
Past Mars missions have discovered geologic features that look like shorelines, but they are subtle and are found at varying elevations across the planet. If they were true signatures of a stable ocean, these shorelines would need to all be at the same elevation in the same way that sea levels are consistent across our own planet.<\/p>\n
\u201cIf Mars did have an ocean, it dried up a long time ago\u2014possibly several billion years ago, more than half of the age of the planet itself,\u201d Lamb says. \u201cThere is hardly anything on Earth that is that old; anything on Mars from that time has been eroded by billions of years of wind blowing, volcanoes erupting, and other disturbances removing subtle features. We wanted to find a better topographic feature than shorelines that could be evidence for an ocean.\u201d<\/p>\n
Zaki and Lamb looked first to Earth to determine which geological features are indicative of an ocean on our own planet. Using computer simulations, they first \u201cdried up\u201d the oceans to see which topographic features remained.<\/p>\n
The models showed that the most distinct feature of the oceans is a flat band of land, up to several hundreds of kilometers wide, wrapping the contours of where land meets ocean like a ring that remains around a drained bathtub. That band is called the continental shelf. Though sea levels on Earth, and thus the location of shorelines, have fluctuated over many years, the continental shelf is a large landform that is relatively stable over time.<\/p>\n
The team then looked at topographic data of Mars taken by orbiters and found an analogous band that is suggestive of an ocean in the Martian northern hemisphere covering a third of the planet\u2019s surface. A landform like this takes time to form\u2014and notably is not found around lakes\u2014which indicates that the ocean must have existed stably for possibly millions of years.<\/p>\n
The team also saw evidence that river deltas, the triangular plains of sediment created where rivers spill into the ocean, lined up with the \u201cbathtub ring\u201d shelf.<\/p>\n
\u201cThe shelf is a new observation that ties together evidence of what the coastal zone would have looked like,\u201d Zaki says. \u201cNobody had really looked for it before. It\u2019s a strong additional piece of evidence supporting a northern ocean on Mars, but there\u2019s plenty of follow-up work to be done for rovers to examine deposits and for further analysis of satellite data.\u201d<\/p>\n
The study suggests new targets for future missions. If there once was life on Mars, sedimentary deposits from the Martian coastlines could have preserved its signatures, just as coastal sediments on Earth contain a historic record of fossils from the continents.<\/p>\n