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Ruthenium isotopic evidence for an inner Solar System origin of the late veneer

Author

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  • Mario Fischer-Gödde

    (Institut für Planetologie, University of Münster)

  • Thorsten Kleine

    (Institut für Planetologie, University of Münster)

Abstract

All chondrites are shown to have Ru isotopic compositions that are more different from that of the Earth’s mantle the further from the Sun they formed; this means the Earth’s late veneer cannot derive from volatile-rich material formed in the outer Solar System.

Suggested Citation

  • Mario Fischer-Gödde & Thorsten Kleine, 2017. "Ruthenium isotopic evidence for an inner Solar System origin of the late veneer," Nature, Nature, vol. 541(7638), pages 525-527, January.
    • Handle: RePEc:nat:nature:v:541:y:2017:i:7638:d:10.1038_nature21045
    DOI: 10.1038/nature21045
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    Cited by:

    1. Lanlan Shi & Wenhua Lu & Takanori Kagoshima & Yuji Sano & Zenghao Gao & Zhixue Du & Yun Liu & Yingwei Fei & Yuan Li, 2022. "Nitrogen isotope evidence for Earth’s heterogeneous accretion of volatiles," Nature Communications, Nature, vol. 13(1), pages 1-15, December.
    2. Joshua Krissansen-Totton & Nicholas Wogan & Maggie Thompson & Jonathan J. Fortney, 2024. "The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets," Nature Communications, Nature, vol. 15(1), pages 1-16, December.

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