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Highly Siderophile Element Constraints on Accretion and Differentiation of the Earth-Moon System
Open accessAbstract
A new combined rhenium-osmium– and platinum-group element data set for basalts from the Moon establishes that the basalts have uniformly low abundances of highly siderophile elements. The data set indicates a lunar mantle with long-term, chondritic, highly siderophile element ratios, but with absolute abundances that are over 20 times lower than those in Earth's mantle. The results are consistent with silicate-metal equilibrium during a giant impact and core formation in both bodies, followed by post–core-formation late accretion that replenished their mantles with highly siderophile elements. The lunar mantle experienced late accretion that was similar in composition to that of Earth but volumetrically less than (∼0.02% lunar mass) and terminated earlier than for Earth.
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Origin of the Moon in a giant impact near the end of the Earth's formation
Canup, R. M., & Asphaug, E. (2001) · Nature · doi:10.1038/35089010 · Cited by 1,094
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Metadata
- Authors
- Day, J. M. D., Pearson, D. G., & Taylor, L. A.
- Venue
- Science
- Published
- 2007-01-12
- Volume
- 315
- Issue
- 5809
- Pages
- 217-219
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W2092917902
- Cited by
- 210
- References
- 1
- FWCI
- 4.03
- Type
- journal article
- Language
- en
- Open access
- green
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- Day, J. M. D., Pearson, D. G., & Taylor, L. A. (2007). Highly Siderophile Element Constraints on Accretion and Differentiation of the Earth-Moon System. Science. https://doi.org/10.1126/science.1133355
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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