Lunar Mantle Temperature Structure from Seismic and Geodetic Observations and Laboratory Dissipation Experiments

Details Lunar Mantle Temperature Structure from Seismic and Geodetic Observations and Laboratory Dissipation Experiments Lunar Mantle Temperature Structure from Seismic and Geodetic Observations and Laboratory Dissipation Experiments

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1564n&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1564

Physics

Scientific paper

The observed dissipation and k_2 Love number of the Moon can be
reconciled with laboratory measurements by invoking a relatively cold
Moon, in which two-thirds of the radiogenic elements are in the crust. A
deep zone of partial melt is not needed.

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