Radiogenic Heat Production in the Moon: Constraints from Plagioclase-Melt Trace Element Partitioning Experiments

Details Radiogenic Heat Production in the Moon: Constraints from Plagioclase-Melt Trace Element Partitioning Experiments Radiogenic Heat Production in the Moon: Constraints from Plagioclase-Melt Trace Element Partitioning Experiments

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1737d&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1737

Physics

Scientific paper

We estimate radiogenic heat production in the Moon, and its depth
distribution, by combining highland surface concentrations of U, Th, and
K with experimental constraints on the distribution of these elements
between anorthositic plagioclase and melt.

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