Direct Constraints on the Timing of Martian Valley Network Formation Derived Using Buffered Crater Counting

Details Direct Constraints on the Timing of Martian Valley Network Formation Derived Using Buffered Crater Counting Direct Constraints on the Timing of Martian Valley Network Formation Derived Using Buffered Crater Counting

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3050f&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3050

Physics

Scientific paper

Buffered crater counting on martian valley networks reveal they are
Early Hesperian or older, with only a few interesting local exceptions.
This is consistent with a global shift in the surface environment having
occurred from early Mars to today.

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