Fresh Polar Channels on Mars as Evidence of Continuing CO2 Vapour-supported Density Flows

Details Fresh Polar Channels on Mars as Evidence of Continuing CO2 Vapour-supported Density Flows Fresh Polar Channels on Mars as Evidence of Continuing CO2 Vapour-supported Density Flows

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1271h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1271

Physics

Scientific paper

A set of gullies and channels is located at 71 deg. south, within the
annual CO2 polecap. Mean temperatures are ~200K which implies:- 1) At
least some of the channels flow on an annual basis 2) Dense CO2
vapour-supported flows is far more likely than liquid water.

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