小行星
芯(光纤)
天体生物学
土(古典元素)
集合(抽象数据类型)
地质学
天文
物理
太阳系
计算机科学
光学
程序设计语言
作者
Antoine S. G. Roth,Christian Liebske,C. Maden,Kevin W. Burton,Maria Schönbächler,H. Busemann
标识
DOI:10.7185/geochemlet.1901
摘要
The primordial He budget of the Earth's interior is commonly thought to have been set by full liquid metal-silicate equilibration in a terrestrial magma ocean.However, incomplete metal-silicate equilibration during accretion will have a substantial effect on this budget.Here we present liquid-solid partitioning experiments indicating that He behaves as a moderately siderophile element during percolative core formation in planetesimals.Mass balance considerations show that even minor disequilibrium will allow the Earth's early core to incorporate sufficient primordial He-and possibly other noble gases-to supply the lower mantle throughout Earth's history.We conclude that the high 3 He/ 4 He ratios in basalts may well represent primarily the last vestiges of metal-silicate disequilibrium in a terrestrial magma ocean preserved from the time of Earth's formation.
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