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Lunar tungsten isotopic evidence for the late veneer

Author

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  • Thomas S. Kruijer

    (Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Strasse 10, D-48149 Münster, Germany)

  • Thorsten Kleine

    (Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Strasse 10, D-48149 Münster, Germany)

  • Mario Fischer-Gödde

    (Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Strasse 10, D-48149 Münster, Germany)

  • Peter Sprung

    (Institut für Planetologie, Westfälische Wilhelms-Universität Münster, Wilhelm-Klemm-Strasse 10, D-48149 Münster, Germany
    †Present address: Universität zu Köln, Institut für Geologie und Mineralogie, Zülpicher Strasse 49b, D-50674 Köln, Germany.)

Abstract

Precise measurements of the tungsten isotopic composition of lunar rocks show that the Moon exhibits a well-resolved excess of 182W of about 27 parts per million over the present-day Earth’s mantle: this excess is consistent with the expected 182W difference resulting from a late veneer with a total mass and composition inferred from previously measured highly siderophile elements.

Suggested Citation

  • Thomas S. Kruijer & Thorsten Kleine & Mario Fischer-Gödde & Peter Sprung, 2015. "Lunar tungsten isotopic evidence for the late veneer," Nature, Nature, vol. 520(7548), pages 534-537, April.
    • Handle: RePEc:nat:nature:v:520:y:2015:i:7548:d:10.1038_nature14360
    DOI: 10.1038/nature14360
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