The Composition and Origin of Lunar Crater Rays: Implications for the Copernican-Eratosthenian Boundary

Details The Composition and Origin of Lunar Crater Rays: Implications for the Copernican-Eratosthenian Boundary The Composition and Origin of Lunar Crater Rays: Implications for the Copernican-Eratosthenian Boundary

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1133h&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1133

Computer Science

2

Scientific paper

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

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