Melting a Martian Viscous Flow Feature: A Modern-Climate, Dust-Blanketed Glacier Model

Details Melting a Martian Viscous Flow Feature: A Modern-Climate, Dust-Blanketed Glacier Model Melting a Martian Viscous Flow Feature: A Modern-Climate, Dust-Blanketed Glacier Model

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2266k&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2266

Physics

Scientific paper

Evidence points to glacial flow and melting of a landform in a crater
east of Hellas, Mars. A thick blanket of insulating dust might allow
melting under the present climate, thus offering an alternative to a
modified, warmer recent climate.

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