Radiogenic Heat Source Concentration in the Lunar Farside Crust Estimated from Viscoelastic Deformation of Impact Basins

Details Radiogenic Heat Source Concentration in the Lunar Farside Crust Estimated from Viscoelastic Deformation of Impact Basins Radiogenic Heat Source Concentration in the Lunar Farside Crust Estimated from Viscoelastic Deformation of Impact Basins

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1648k&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1648

Physics

Scientific paper

Viscoelastic modeling of impact basins and Kaguya's selenodetic data
yield an estimate for the mean Th concentration in the lunar farside
crust (<0.5 ppm), much lower than SPA, suggesting great horizontal
heterogeneity of lower farside crust.

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