Observed Degradation Stages of Ring-Mold Craters (RMC): Geomorphic Evidence for Modification of Ice-rich Deposits in the Transition Zone Between Elysium and Utopia Basin, Mars

Details Observed Degradation Stages of Ring-Mold Craters (RMC): Geomorphic Evidence for Modification of Ice-rich Deposits in the Transition Zone Between Elysium and Utopia Basin, Mars Observed Degradation Stages of Ring-Mold Craters (RMC): Geomorphic Evidence for Modification of Ice-rich Deposits in the Transition Zone Between Elysium and Utopia Basin, Mars

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1790p&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1790

Physics

Scientific paper

Deposits with pits, depressions and RMCs observed north of Elysium rise
are interpreted as degraded mixtures of ice and clastic material (CCF,
LVF and LDA). Degradation stages of RMCs are an important tool for
mapping dusty, deflated ice-rich units.

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