Geothermal Heating, Convective Flow and Ice Thickness on Mars

Details Geothermal Heating, Convective Flow and Ice Thickness on Mars Geothermal Heating, Convective Flow and Ice Thickness on Mars

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1390t&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1390

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Scientific paper

Our 3D calculations suggest that hydrothermal circulation may occur in
the Martian regolith and may significantly thin the surface ice layer on
Mars at some locations due to the upwelling of warm convecting fluids
driven solely by background geothermal heating.

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