A View of Meridiani from Above: Evidence for Deposition in Standing Water from THEMIS, TES, and MOLA

Details A View of Meridiani from Above: Evidence for Deposition in Standing Water from THEMIS, TES, and MOLA A View of Meridiani from Above: Evidence for Deposition in Standing Water from THEMIS, TES, and MOLA

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1961c&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1961

Computer Science

Scientific paper

The preferred model for Meridiani is deposition of precursor Fe-
oxyhydroxides in water-filled basins. This model accounts for the sharp
upper boundary of the hematite unit, goethite as a precursor, embayment
relationships, remnants in isolated craters, and basalt as the major
component.

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