Possible Sea Sediments Due to Glaciofluvial Activity in Elysium Planitia, Mars

Details Possible Sea Sediments Due to Glaciofluvial Activity in Elysium Planitia, Mars Possible Sea Sediments Due to Glaciofluvial Activity in Elysium Planitia, Mars

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3176n&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3176

Physics

Scientific paper

The observation of fluvial morphologies in southern Elysium Planitia and
zig-zag features potentially analogous to those observed near the Wadden
Sea on Earth may help show in more detail the origin of water in this
region of Mars.

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