Origin of Aristarchus Olivine Based on M^3 and Diviner Analyses

Details Origin of Aristarchus Olivine Based on M^3 and Diviner Analyses Origin of Aristarchus Olivine Based on M^3 and Diviner Analyses

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2515w&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2515

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Scientific paper

Olivine-bearing material is exposed in ejecta deposits on the SE portion
of the Aristarchus crater wall. We investigate the nature of these
deposits with M^3 and Diviner and compare them to other olivine-bearing
deposits in the vicinity of Imbrium.

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