Ice Content of Martian Permafrost Deduced from Rheology of Ice-Rock Mixtures

Details Ice Content of Martian Permafrost Deduced from Rheology of Ice-Rock Mixtures Ice Content of Martian Permafrost Deduced from Rheology of Ice-Rock Mixtures

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1016m&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1016

Physics

2

Scientific paper

Experimental results on ice-rock mixtures show that a minimal ice
content of 28% is needed to produce a viscous deformation like that
observed in martian softened terrains. A global inventory of water of
about 200 m is deduced from this high proportion of ice.

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