Geochemical and geophysical constraints for thermal state of the Moon

Details Geochemical and geophysical constraints for thermal state of the Moon Geochemical and geophysical constraints for thermal state of the Moon

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..175k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.175

Physics

Scientific paper

temperature distribution and its influence on the internal structure of the Moon. The problem of thermal state of the Moon was provisionally divided into two parts: 1. The probable temperature distributions in the mantle were found from seismic and geochemical data for various geochemical models of the Moon. 2. Using these data and mass and moment of inertia of the Moon as well as seismic velocities we determine temperature distributions and major oxide concentrations in the lunar mantle.

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