Chemically and Mineralogically Distinct Regions on Mars Derived from GRS and TES Data

Details Chemically and Mineralogically Distinct Regions on Mars Derived from GRS and TES Data Chemically and Mineralogically Distinct Regions on Mars Derived from GRS and TES Data

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1757t&link_type=abstract

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

Computer Science

Scientific paper

Mars Odyssey GRS and TES data show that the martian surface contains
compositionally distinct regions. TES and GRS regions do not correspond
exactly, suggesting that mineral abundance is not always correlated with
chemical composition.

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