Origin and Evolution of Sediments in Gale Crater Through Ice-Hosted Processes

Details Origin and Evolution of Sediments in Gale Crater Through Ice-Hosted Processes Origin and Evolution of Sediments in Gale Crater Through Ice-Hosted Processes

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2575n&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2575

Computer Science

Scientific paper

The Gale Crater sediments on Mars were formed by ice-dust deposition,
weathering, and diagenesis. This is supported by modeling, geomorphic
relationships, and comparisons to similar martian sedimentary deposits
and will be tested by MSL.

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