Active Processes on Mars: Dry Ice and Dunes

Details Active Processes on Mars: Dry Ice and Dunes Active Processes on Mars: Dry Ice and Dunes

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1150h&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1150

Physics

Scientific paper

Icy volatiles on Mars are responsible for geomorphic changes on dunes, taking place in today's climate. Both north and south polar regions show sediment transport in the spring, associated with sublimation of seasonal ice. Using HiRISE, the High Resolution Imaging Science Experiment, on the Mars Reconnaissance Orbiter (MRO), we explore possible mechanisms.

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