A Chronology of Mars Hydrological Evolution from Impact Degradation

Details A Chronology of Mars Hydrological Evolution from Impact Degradation A Chronology of Mars Hydrological Evolution from Impact Degradation

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1210m&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1210

Physics

Scientific paper

Degradation of impact craters >20 km is studied in two Noachian
regions. Results show a shift in degradation at 3.7 Gy. Craters with
alluvial fans are distinct from the most degraded by being better
preserved, and being formed during the Hesperian.

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