Formation of Martian Silica-rich Deposits Through Rock Alteration: A Theoretical Assessment

Details Formation of Martian Silica-rich Deposits Through Rock Alteration: A Theoretical Assessment Formation of Martian Silica-rich Deposits Through Rock Alteration: A Theoretical Assessment

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2371m&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Physical-chemical models of rock alteration show that silica-rich
deposits, like those at Home Plate in Gusev crater, could form in cold
and hot spring settings. Cold settings imply low pH conditions.

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