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Letters to Nature
Nature 418, 403-405 (25 July 2002) | doi:10.1038/nature00923; Received 26 March 2002; Accepted 18 June 2002
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Tungsten isotope evidence from
3.8-Gyr metamorphosed sediments for early meteorite bombardment of the Earth
Ronny Schoenberg1, Balz S. Kamber1, Kenneth D. Collerson1 & Stephen Moorbath2
- Advanced Centre for Queensland University Research Excellence (ACQUIRE), The University of Queensland, St Lucia, Queensland 4072, Australia
- Department of Earth Sciences, University of Oxford, Parks Road, Oxford OX1 3PR, UK
Correspondence to: Ronny Schoenberg1 Correspondence and requests for materials should be addressed to R.S. (e-mail: Email: ronny@earth.uq.edu.au).
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.
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