Distant Secondary Craters and Age Constraints on Young Martian Terrains

Details Distant Secondary Craters and Age Constraints on Young Martian Terrains Distant Secondary Craters and Age Constraints on Young Martian Terrains

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2111m&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2111

Physics

Scientific paper

Small martian craters (<300 m) are mostly distant secondaries, not
useful for age dating, and the primary production function is "flatter"
than previously assumed, which is why much of the Martian surface has
well-preserved meter-scale morphologies.

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