Chasmata of Planum Australe, Mars: Are Their Formation and Location Structurally Controlled?

Details Chasmata of Planum Australe, Mars: Are Their Formation and Location Structurally Controlled? Chasmata of Planum Australe, Mars: Are Their Formation and Location Structurally Controlled?

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2298k&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2298

Mathematics

Logic

3

Scientific paper

This abstract details results of our 1:1.5M-scale geologic mapping of
Mars' polar ice caps. We show that the location and formation of the
south pole chasma of Planum Australe are structurally controlled by
substrate and SPLD paleosurface topography.

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