Clathrate and Ice Stability in a Porous Martian Regolith

Details Clathrate and Ice Stability in a Porous Martian Regolith Clathrate and Ice Stability in a Porous Martian Regolith

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1955l&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1955

Physics

Scientific paper

CO2-clathrate becomes stable with respect to combinations of CO2-rich
gas and water ice at depths >=7 m on Mars. However, if the gas in a
porous regolith is in hydraulic contact with the atmosphere, both
clathrate and ice will be unstable.

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