Retention time of crater ray materials on the lunar highland

Details Retention time of crater ray materials on the lunar highland Retention time of crater ray materials on the lunar highland

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1146h&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1146

Physics

Scientific paper

We investigate the retention time of crater ray materials around smaller lunar craters with multiband images and high-resolution images acquired by Kaguya / MI and TC, respectively. In our research, we surveyed rayed craters using OMAT (Optical Maturity) parameter developed by [1]. We surveyed craters from 300 m to 10 km in diameter in lunar highland. The craters larger than 1 km in diameter are plotted above the 750 Ma isochron which was estimated by [2]. However, the distribution cannot be fitted by a single isochron, this might suggest that the retention time of crater ray materials is longer than 750 Myr.

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