Thermal and Volatile Evolution of Mars from Dichotomy Relaxation Models

Details Thermal and Volatile Evolution of Mars from Dichotomy Relaxation Models Thermal and Volatile Evolution of Mars from Dichotomy Relaxation Models

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3342s&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3342

Physics

Scientific paper

We show that loss of crustal volatiles, at least locally, at the
Hesperian/Amazonian boundary is needed along with cooling predicted by
thermal evolution models to preserve the dichotomy topography and
crustal thickness variations to the present day.

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