Permanent CO2 Deposits on Mars at Low Obliquity: The Role of Surface Topography

Details Permanent CO2 Deposits on Mars at Low Obliquity: The Role of Surface Topography Permanent CO2 Deposits on Mars at Low Obliquity: The Role of Surface Topography

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1234k&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1234

Physics

Scientific paper

During long low obliquity epochs, massive solid CO2 deposits would form
on steep pole-facing topographic slopes at moderately high latitudes
rather than at the poles. Such deposits could survive short obliquity
peaks and leave observable traces.

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