Earth's chondritic Th/U: Negligible fractionation during accretion, core formation, and crust–mantle differentiation
Earth's chondritic Th/U: Negligible fractionation during accretion, core formation, and crust–mantle differentiation
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DOI:
10.1016/j.epsl.2018.06.029
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发表时间:
2018-01
影响因子:
5.3
通讯作者:
S. Wipperfurth;Meng Guo;O. Šrámek;W. McDonough
中科院分区:
文献类型:
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作者:
S. Wipperfurth;Meng Guo;O. Šrámek;W. McDonough
Radioactive decay of potassium (K), thorium (Th), and uranium (U) power the Earth's engine, with variations in 232 Th/238 U recording planetary differentiation, atmospheric oxidation, and biologically mediated processes. We report several thousand 232 Th/238 U (κ) and time-integrated Pb isotopic (κ P b) values and assess their ratios for the Earth, core, and silicate Earth. Complementary bulk silicate Earth domains (ie, continental crust κ P b C C= 3.95− 0.13+ 0.19 and modern mantle κ P b M M= 3.87− 0.07+ 0.15) tightly bracket the solar system initial κ P b S S= 3.890±0.015. These findings reveal the bulk silicate Earth's κ P b B S E is 3.90− 0.08+ 0.13 (or Th/U= 3.77 for the mass ratio), which resolves a long-standing debate regarding the Earth's Th/U value. We performed a Monte Carlo simulation to calculate the κ P b of the BSE and bulk Earth for a range of U concentrations in the core (from 0 to 10 ng/g). Comparison of our results with κ P b S S constrains the available U and Th budget in the core. Negligible Th/U fractionation accompanied accretion, core formation, and crust–mantle differentiation, and trivial amounts of these elements (< 0.2 ng/g U) were added to the core and do not significantly power (∼ 0.03 TW) the geodynamo.