The 176Lu to 176Hf decay series has been widely used to understand the nature of Earth's early crust–mantle system1,2,3,4,5,6. The interpretation, however, of Lu–Hf isotope data requires accurate knowledge of the radioactive decay constant of 176Lu (), as well as bulk-Earth reference parameters. A recent calibration of the value calls for the presence of highly unradiogenic hafnium in terrestrial zircons with ages greater than 3.9 Gyr, implying widespread continental crust extraction from an isotopically enriched mantle source more than 4.3 Gyr ago7, but does not provide evidence for a complementary depleted mantle reservoir. Here we report Lu–Hf isotope measurements of different Solar System objects including chondrites and basaltic eucrites. The chondrites define a Lu–Hf isochron with an initial 176Hf/177Hf ratio of 0.279628 ± 0.000047, corresponding to = 1.983 ± 0.033 × 10-11 yr-1 using an age of 4.56 Gyr for the chondrite-forming event. This value indicates that Earth's oldest minerals were derived from melts of a mantle source with a time-integrated history of depletion rather than enrichment7. The depletion event must have occurred no later than 320 Myr after planetary accretion, consistent with timing inferred from extinct radionuclides8,9,10.
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We thank F. Albarède and H. C. Larsen for comments on an earlier version of the manuscript, J. Blichert-Toft for access to unpublished data, Y. Amelin for discussion, and T. Waight for help in the Danish Lithosphere Centre MC-ICP-MS laboratory. This project was supported by the Danish Lithosphere Centre (funded by the Danish National Science Foundation). M.B. was supported by an NSERC postdoctoral fellowship.
The authors declare that they have no competing financial interests.
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Bizzarro, M., Baker, J., Haack, H. et al. Early history of Earth's crust–mantle system inferred from hafnium isotopes in chondrites. Nature 421, 931–933 (2003). https://doi.org/10.1038/nature01421
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