Formation of Mars Impact Crater Ramparts by Volatile Degassing of the Overland Ejecta Flow

Details Formation of Mars Impact Crater Ramparts by Volatile Degassing of the Overland Ejecta Flow Formation of Mars Impact Crater Ramparts by Volatile Degassing of the Overland Ejecta Flow

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1309b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1309

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We present a two component crater ejecta flow model where solids are
conserved and volatiles are released. The presence of a gaseous
component that is lost during emplacement may uniquely distinguish Mars
rampart deposits from those of impact-generated deposits on other
planetary surfaces.

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