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The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling
The Earth and Moon have identical or very similar isotopic compositions for many elements, including tungsten. However, canonical models of the Moon-forming impact predict that the Moon should be made mostly of material from the impactor, Theia. Here we evaluate the probability of the Moon inheritin...
Autores principales: | , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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Nature Publishing Group UK
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7782809/ https://www.ncbi.nlm.nih.gov/pubmed/33397911 http://dx.doi.org/10.1038/s41467-020-20266-1 |
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author | Fischer, Rebecca A. Zube, Nicholas G. Nimmo, Francis |
author_facet | Fischer, Rebecca A. Zube, Nicholas G. Nimmo, Francis |
author_sort | Fischer, Rebecca A. |
collection | PubMed |
description | The Earth and Moon have identical or very similar isotopic compositions for many elements, including tungsten. However, canonical models of the Moon-forming impact predict that the Moon should be made mostly of material from the impactor, Theia. Here we evaluate the probability of the Moon inheriting its Earth-like tungsten isotopes from Theia in the canonical giant impact scenario, using 242 N-body models of planetary accretion and tracking tungsten isotopic evolution, and find that this probability is <1.6–4.7%. Mixing in up to 30% terrestrial materials increases this probability, but it remains <10%. Achieving similarity in stable isotopes is also a low-probability outcome, and is controlled by different mechanisms than tungsten. The Moon’s stable isotopes and tungsten isotopic composition are anticorrelated due to redox effects, lowering the joint probability to significantly less than 0.08–0.4%. We therefore conclude that alternate explanations for the Moon’s isotopic composition are likely more plausible. |
format | Online Article Text |
id | pubmed-7782809 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-77828092021-01-14 The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling Fischer, Rebecca A. Zube, Nicholas G. Nimmo, Francis Nat Commun Article The Earth and Moon have identical or very similar isotopic compositions for many elements, including tungsten. However, canonical models of the Moon-forming impact predict that the Moon should be made mostly of material from the impactor, Theia. Here we evaluate the probability of the Moon inheriting its Earth-like tungsten isotopes from Theia in the canonical giant impact scenario, using 242 N-body models of planetary accretion and tracking tungsten isotopic evolution, and find that this probability is <1.6–4.7%. Mixing in up to 30% terrestrial materials increases this probability, but it remains <10%. Achieving similarity in stable isotopes is also a low-probability outcome, and is controlled by different mechanisms than tungsten. The Moon’s stable isotopes and tungsten isotopic composition are anticorrelated due to redox effects, lowering the joint probability to significantly less than 0.08–0.4%. We therefore conclude that alternate explanations for the Moon’s isotopic composition are likely more plausible. Nature Publishing Group UK 2021-01-04 /pmc/articles/PMC7782809/ /pubmed/33397911 http://dx.doi.org/10.1038/s41467-020-20266-1 Text en © The Author(s) 2021 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/. |
spellingShingle | Article Fischer, Rebecca A. Zube, Nicholas G. Nimmo, Francis The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling |
title | The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling |
title_full | The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling |
title_fullStr | The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling |
title_full_unstemmed | The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling |
title_short | The origin of the Moon’s Earth-like tungsten isotopic composition from dynamical and geochemical modeling |
title_sort | origin of the moon’s earth-like tungsten isotopic composition from dynamical and geochemical modeling |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7782809/ https://www.ncbi.nlm.nih.gov/pubmed/33397911 http://dx.doi.org/10.1038/s41467-020-20266-1 |
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