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Hf-W chronometry of lunar metals and the age and early differentiation of the Moon.

Abstract:
The use of hafnium-tungsten chronometry to date the Moon is hampered by cosmogenic tungsten-182 production mainly by neutron capture of tantalum-181 at the lunar surface. We report tungsten isotope data for lunar metals, which contain no 181Ta-derived cosmogenic 182W. The data reveal differences in indigenous 182W/184W of lunar mantle reservoirs, indicating crystallization of the lunar magma ocean 4.527 +/- 0.010 billion years ago. This age is consistent with the giant impact hypothesis and defines the completion of the major stage of Earth's accretion.
Publication status:
Published

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Publisher copy:
10.1126/science.1118842

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Role:
Author


Journal:
Science (New York, N.Y.) More from this journal
Volume:
310
Issue:
5754
Pages:
1671-1674
Publication date:
2005-12-01
DOI:
EISSN:
1095-9203
ISSN:
0036-8075


Language:
English
Pubs id:
pubs:82618
UUID:
uuid:0e3b5b8c-8638-4e97-9f79-3a30b63882df
Local pid:
pubs:82618
Source identifiers:
82618
Deposit date:
2012-12-19
ARK identifier:

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