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Hafnium–tungsten chronometry and the timing of terrestrial core formation

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Abstract

THE accretion of the Earth and Moon within the solar nebula is thought1–3 to have taken 50 to 100 million years. But the timing of formation of the Earth's core has been controversial, with some4,5 proposing that it took place within the first 15 Myr of Earth's accretion history and others6,7 proposing that it occurred after 50 Myr of accretion. Meteorite chronometry based on the 182Hf–182W system has the potential to resolve this debate, as segregation of a metal core from silicates should induce strong fractionation of hafnium from tungsten. Here we report tungsten isotope compositions for two iron meteorites, two carbonaceous chondrites, and a lunar mare basalt. We see clear 182W deficits in both iron meteorites, in agreement with previous results4,5. But the data for chondrites are inconsistent with the hypothesis of early core formation, suggesting that both this event and the formation of the Moon must have occurred at least 62 ± 10 Myr after the iron meteorites formed.

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Authors and Affiliations

  1. Department of Geological Sciences, University of Michigan, Ann Arbor, Michigan, 48109-1063, USA

    Der-Chuen Lee & Alex N. Halliday

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  1. Der-Chuen Lee
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Lee, DC., Halliday, A. Hafnium–tungsten chronometry and the timing of terrestrial core formation. Nature 378, 771–774 (1995). https://doi.org/10.1038/378771a0

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