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Table A.1

Estimates of radiogenic heat output in the Earth upon its formation and at the present day.

Concentration (ppb) Heat (TW)(a)


Nuclide (X) Present-day(b) Upon formation(c) X/Mg(d) Present-day Upon formation
232Th 74.6 ± 6.8 93.5 ± 8.5 4.19 ± 0.38 × 10−7 7.9 ± 0.7 9.9 ± 0.9
235U 0.143 ± 0.014 12.7 ± 1.3 5.70 ± 0.58 × 10−8 0.33 ± 0.03 29.1 ± 2.9
238U 19.7 ± 2.0 39.9 ± 4.0 1.79 ± 0.18 × 10−7 7.5 ± 0.8 15.3 ± 1.5
40K 28.2 ± 3.0 353.6 ± 37.3 1.59 ± 0.17 × 10−6 3.2 ± 0.3 40.6 ± 4.3
Th+U+K 122.6 ± 7.6 499.6 ± 38.5 ... 19.0 ± 1.1 94.9 ± 5.5

Notes. (a) Calculated by multiplying the corresponding concentrations (upon planet formation and at the present day) with the heat generation rates, h, of individual radionuclides (see Table 3). (b)We refer to the mantle concentrations of Wang et al. (2018) (Col. 3 of their Table 1), based on which the radioactive elemental concentrations are converted into the radionuclide concentrations by adopting 232Th/Th = 1, 235U/U = 0.0072, 238U/U = 0.9928, and 40K/K = 1.19 × 10−4 (Turcotte & Schubert 2002) for the present-day bulk silicate Earth. (c) C0 = Ct × et ln 2∕T1∕2, where C0 and Ct represent the abundances of a radionuclide upon the Earth formation (t = 4.56 Ga) and at the present day, respectively; T1∕2 is given in Table 3. (d) X/Mg = C0(X)/C0(Mg), which refers to the early stage of Hadean Earth (i.e. upon the planet formation); C0 (Mg) = C(Mg) = 22.3 ± 0.2% (Wang et al. 2018), i.e. the concentration of Mg is kept unchanged over gelogical time.

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