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Tungsten isotope evidence from ∼3.8-Gyr metamorphosed sediments for early meteorite bombardment of the Earth

Author

Listed:
  • Ronny Schoenberg

    (Advanced Centre for Queensland University Research Excellence (ACQUIRE), The University of Queensland)

  • Balz S. Kamber

    (Advanced Centre for Queensland University Research Excellence (ACQUIRE), The University of Queensland)

  • Kenneth D. Collerson

    (Advanced Centre for Queensland University Research Excellence (ACQUIRE), The University of Queensland)

  • Stephen Moorbath

    (University of Oxford)

Abstract

The ‘Late Heavy Bombardment’ was a phase in the impact history of the Moon that occurred 3.8–4.0 Gyr ago, when the lunar basins with known dates were formed1,2. But no record of this event has yet been reported from the few surviving rocks of this age on the Earth. Here we report tungsten isotope anomalies, based on the 182Hf–182W system (half-life of 9 Myr), in metamorphosed sedimentary rocks from the 3.7–3.8-Gyr-old Isua greenstone belt of West Greenland and closely related rocks from northern Labrador, Canada. As it is difficult to conceive of a mechanism by which tungsten isotope heterogeneities could have been preserved in the Earth's dynamic crust–mantle environment from a time when short-lived 182Hf was still present, we conclude that the metamorphosed sediments contain a component derived from meteorites.

Suggested Citation

  • Ronny Schoenberg & Balz S. Kamber & Kenneth D. Collerson & Stephen Moorbath, 2002. "Tungsten isotope evidence from ∼3.8-Gyr metamorphosed sediments for early meteorite bombardment of the Earth," Nature, Nature, vol. 418(6896), pages 403-405, July.
    • Handle: RePEc:nat:nature:v:418:y:2002:i:6896:d:10.1038_nature00923
    DOI: 10.1038/nature00923
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