Small Crater Ejecta Retention Ages Inside Gale Crater: Recent Erosional History and Potential Sampling Locations for the Mars Science Laboratory

Details Small Crater Ejecta Retention Ages Inside Gale Crater: Recent Erosional History and Potential Sampling Locations for the Mars Science Laboratory Small Crater Ejecta Retention Ages Inside Gale Crater: Recent Erosional History and Potential Sampling Locations for the Mars Science Laboratory

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2674c&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2674

Physics

Scientific paper

We recorded all fresh craters with ejecta or blocks outside their crater
rim within or near the MSL Gale landing ellipse in a GIS. Ejecta
retention rates are <10 My for craters D < 100 m. These craters
would be ideal for sample acquisition by MSL.

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