New maps of the subsurface of Mars show for the first time buried channels below the surface of the red planet. Mars is considered to have been cold and dry over the past 2.5 billion years, but these channels suggest evidence of flooding. Understanding the source and scale of the young channels present in Elysium Planitia -- an expanse of plains along the equator, and the youngest volcanic region on the planet -- is essential to comprehend recent Martian hydrologic activity and determine if such floods could have induced climate change.
The findings are reported by a team from NASA's Goddard Space Flight Center, the Jet Propulsion Laboratory, the Planetary Science Directorate in the Southwest Research Institute and the Smithsonian Institution, led by Smithsonian scientist Gareth A. Morgan, in a paper in the March 7 issue of the journal Science.
As a consequence of extensive volcanism throughout the past several hundred million years, young lava covers most of the surface of Elysium Planitia, burying evidence of its recent geologic history, including the source and most of the length of the 1,000 kilometer-long Marte Vallis channel system. Marte Vallis has a similar morphology to more ancient channel systems on Mars that likely formed by the catastrophic release of ground water; however, little is known about Marte Vallis due to its burial by lava.
The team used data from the Shallow Radar on board the NASA Mars Reconnaissance Orbiter spacecraft to probe the subsurface of Elysium Planitia. They were able to map the buried channels and establish that the floods originated from a now buried portion of the Cerberus Fossae fracture system.
"Our findings show that the scale of erosion was previously underestimated and that channel depth was at least twice that of previous approximations," said Morgan, geologist at the National Air and Space Museum's Center for Earth and Planetary Studies and lead author on the paper. "The source of the floodwaters suggests they originated from a deep groundwater reservoir and may have been released by local tectonic or volcanic activity. This work demonstrates the importance of orbital sounding radar in understanding how water has shaped the surface of Mars."
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