Remote Sensing Studies of Copernicus Rays: Implications for the Copernican-Eratosthenian Boundary

Details Remote Sensing Studies of Copernicus Rays: Implications for the Copernican-Eratosthenian Boundary Remote Sensing Studies of Copernicus Rays: Implications for the Copernican-Eratosthenian Boundary

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1133h&link_type=abstract

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

Computer Science

Scientific paper

The mere presence of bright rays is not a reliable indicator that a
crater was formed during the Copernican Period because compositional
rays can persist for 3 Ga or more. The optical maturity parameter should
be used to define the C-E boundary.

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