Quantifying the Amount of Impact Ejecta at the MER Landing Sites and Potential Paleolakes in the Southern Martian Highlands

Details Quantifying the Amount of Impact Ejecta at the MER Landing Sites and Potential Paleolakes in the Southern Martian Highlands Quantifying the Amount of Impact Ejecta at the MER Landing Sites and Potential Paleolakes in the Southern Martian Highlands

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1043c&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1043

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Scientific paper

Applying previous equations for impact ejecta thickness to Mars, tens of
meters of ejecta are expected over the southern hemisphere. This is not
enough to explain observed depth discrepancies in Gusev Crater or in
other potential Martian paleolakes.

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