Deep-mantle krypton reveals Earth’s early accretion of carbonaceous matter
Deep-mantle krypton reveals Earth’s early accretion of carbonaceous matter
复制标题
深地幔氪揭示了地球早期碳质物质的吸积
DOI:
10.1038/s41586-021-04092-z
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发表时间:
2021
期刊:
影响因子:
64.8
通讯作者:
Graham, David W.
中科院分区:
文献类型:
--
作者:
Péron, Sandrine;Mukhopadhyay, Sujoy;Kurz, Mark D.;Graham, David W.
Establishing when, and from where, carbon, nitrogen and water were delivered to Earth is a fundamental objective in understanding the origin of habitable planets such as Earth. Yet, volatile delivery to Earth remains controversial, , , –. Krypton isotopes provide insights on volatile delivery owing to their substantial isotopic variations among sources, , , –, although pervasive atmospheric contamination has hampered analytical efforts. Here we present the full suite of krypton isotopes from the deep mantle of the Galápagos and Iceland plumes, which have the most primitive helium, neon and tungsten isotopic compositions, , , , –. Except for86Kr, the krypton isotopic compositions are similar to a mixture of chondritic and atmospheric krypton. These results suggest early accretion of carbonaceous material by proto-Earth and rule out any combination of hydrodynamic loss with outgassing of the deep or shallow mantle to explain atmospheric noble gases. Unexpectedly, the deep-mantle sources have a deficit in the neutron-rich86Kr relative to the average composition of carbonaceous meteorites, which suggests a nucleosynthetic anomaly. Although the relative depletion of neutron-rich isotopes on Earth compared with carbonaceous meteorites has been documented for a range of refractory elements,,, our observations suggest such a depletion for a volatile element. This finding indicates that accretion of volatile and refractory elements occurred simultaneously, with krypton recording concomitant accretion of non-solar volatiles from more than one type of material, possibly including outer Solar System planetesimals.
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