Comparisons of Mineralogy of Lunar Meteorites Possibly from the Farside and the Kaguya Remote Sensing Data to Reconstruct the Earliest Anorthositic Crust of the Moon

Details Comparisons of Mineralogy of Lunar Meteorites Possibly from the Farside and the Kaguya Remote Sensing Data to Reconstruct the Earliest Anorthositic Crust of the Moon Comparisons of Mineralogy of Lunar Meteorites Possibly from the Farside and the Kaguya Remote Sensing Data to Reconstruct the Earliest Anorthositic Crust of the Moon

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1379t&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1379

Computer Science

Scientific paper

Comparisons of mineralogy of lunar meteorites (Dhofar 911, etc.) from
the farside and the Kaguya Th concentrations a to reconstruct the
earliest, asymmetric anorthositic crust of the Moon. We propose that
these meteorites might have come from the Dirichlet-Jackson basin.

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