Impact Melting and the Role of Sub-Surface Volatiles: Implications for the Formation of Valley Networks and Phyllosilicate-rich Lithologies on Early Mars

Details Impact Melting and the Role of Sub-Surface Volatiles: Implications for the Formation of Valley Networks and Phyllosilicate-rich Lithologies on Early Mars Impact Melting and the Role of Sub-Surface Volatiles: Implications for the Formation of Valley Networks and Phyllosilicate-rich Lithologies on Early Mars

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3288t&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3288

Mathematics

Logic

7

Scientific paper

HiRISE, CTX and other datasets have identified putative volatile-rich
impact melt bearing features in geologically young and well-preserved
impact craters. Implications for valley network and phyllosilicates will
be discussed.

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