Evaluating Models of Crustal Cooling Using CRISM Observations of Impact Craters in Terra Tyrrhena and Noachis Terra

Details Evaluating Models of Crustal Cooling Using CRISM Observations of Impact Craters in Terra Tyrrhena and Noachis Terra Evaluating Models of Crustal Cooling Using CRISM Observations of Impact Craters in Terra Tyrrhena and Noachis Terra

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2320f&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Other

Scientific paper

Occurrence of CRISM-detected hydrated silicates around Southern
Highlands impact craters are used to assess models of crustal cooling.
Preliminarily, lack of mineralogy-depth correlation favors cooling
mediated by hydrothermal processes.

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