Environmental Conditions of Origin of Surface Morphologies of Martian Glacier-like Flows

Details Environmental Conditions of Origin of Surface Morphologies of Martian Glacier-like Flows Environmental Conditions of Origin of Surface Morphologies of Martian Glacier-like Flows

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.2092k&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.2092

Physics

1

Scientific paper

Martian lineated valley fill and lobate debris aprons share many of
characteristics, and some different ones, of terrestrial debris-covered
glaciers. Features indicate surface or shallow subsurface melting in
some cases, but mostly sublimation.

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