Equal-Area Radial Crater Counts at Large Copernican Impact Craters: Implications for Late-Stage Ejecta Emplacement

Details Equal-Area Radial Crater Counts at Large Copernican Impact Craters: Implications for Late-Stage Ejecta Emplacement Equal-Area Radial Crater Counts at Large Copernican Impact Craters: Implications for Late-Stage Ejecta Emplacement

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2131z&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2131

Physics

1

Scientific paper

The distribution of small impact craters in the continuous ejecta of
Copernican craters using equal-area counts oriented radially to the rim
show a trend of decreasing age with increasing distance, suggesting an
influence of self-secondary cratering.

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