Age Constraints on Martian Valley Networks from Buffered Crater Counting

Details Age Constraints on Martian Valley Networks from Buffered Crater Counting Age Constraints on Martian Valley Networks from Buffered Crater Counting

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1030f&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

Scientific paper

Buffered crater counting on Mars' 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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