Early Martian Surface Conditions from Thermodynamics of Phyllosilicates

Details Early Martian Surface Conditions from Thermodynamics of Phyllosilicates Early Martian Surface Conditions from Thermodynamics of Phyllosilicates

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2515c&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

Thermodynamic equilibria are used to determine the geochemical
conditions during the Noachian era. Results show that CO2 pressure and
temperature can explain observations of various phyllosilicates and
carbonates.

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