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Table 2 The assumed average content of heat-producing elements (HPEs) in today’s bulk silicate Moon

From: Effects of magma-generation and migration on the expansion and contraction history of the Moon

HPEs

heating rate (pW kg−1)

Concentration (kg kg−1)

Decay constant (Gyr−1)

\({ }{}_{ }^{238} {\text{U}}\)

\(9.46 \times 10^{7}\)

\(21.3 \times 10^{ - 9}\)

0.16

\({ }{}_{ }^{235} {\text{U}}\)

\(5.69 \times 10^{8}\)

\(0.15 \times 10^{ - 9}\)

0.98

\({ }{}_{ }^{232} {\text{Th}}\)

\(2.64 \times 10^{7}\)

\(79.5 \times 10^{ - 9}\)

0.05

\({ }{}_{ }^{40} {\text{K}}\)

\(2.92 \times 10^{7}\)

\(4.39 \times 10^{ - 9}\)

0.55

  1. Heating rates and decay constants are after Turcotte and Schubert (2014). We assumed that the lunar bulk Th is the same as a value of the Earth (McDonough and Sun 1995; Tayor and Wieczorek 2014; Laneuville et al. 2018) and then, we estimated the K and U concentrations using the Th/U ratio (Lodders 2003) and K/Th ratio (Tayor and Wieczorek 2014)