The origin of volatile elements in the Earth–Moon system
Abstract
The origin of volatile species such as water in the Earth–Moon system is a subject of intense debate but is obfuscated by the potential for volatile loss during the Giant Impact that resulted in the formation of these bodies. One way to address these topics and place constraints on the temporal evolution of volatile components in planetary bodies is by using the observed decay of 87Rb to 87Sr because Rb is a moderately volatile element, whereas Sr is much more refractory. Here, we show that lunar highland rocks that crystallized ~4.35 billion years ago exhibit very limited ingrowth of 87Sr, indicating that prior to the Moon-forming impact, the impactor commonly referred to as “Theia” and the proto-Earth both must have already been strongly depleted in volatile elements relative to primitive meteorites. These results imply that 1) the volatile element depletion of the Moon did not arise from the Giant Impact, 2) volatile element distributions on the Moon and Earth were principally inherited from their precursors, 3) both Theia and the proto-Earth probably formed in the inner solar system, and 4) the Giant Impact occurred relatively late in solar system history.
- Authors:
-
- Nuclear and Chemical Science Division, Lawrence Livermore National Laboratory, Livermore, CA 94550
- Nuclear and Chemical Science Division, Lawrence Livermore National Laboratory, Livermore, CA 94550, Department of Solar System, Impacts &, Meteorites, Museum fur Naturkunde, Berlin 10115, Germany
- Publication Date:
- Research Org.:
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA); National Aeronautics and Space Administration (NASA)
- OSTI Identifier:
- 1845032
- Alternate Identifier(s):
- OSTI ID: 1862734
- Report Number(s):
- LLNL-JRNL-827054
Journal ID: ISSN 0027-8424; e2115726119
- Grant/Contract Number:
- 20-ERD-001; AC52-07NA27344; NNH19ZDA001N
- Resource Type:
- Published Article
- Journal Name:
- Proceedings of the National Academy of Sciences of the United States of America
- Additional Journal Information:
- Journal Name: Proceedings of the National Academy of Sciences of the United States of America Journal Volume: 119 Journal Issue: 8; Journal ID: ISSN 0027-8424
- Publisher:
- Proceedings of the National Academy of Sciences
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 58 GEOSCIENCES
Citation Formats
Borg, Lars E., Brennecka, Gregory A., and Kruijer, Thomas S. The origin of volatile elements in the Earth–Moon system. United States: N. p., 2022.
Web. doi:10.1073/pnas.2115726119.
Borg, Lars E., Brennecka, Gregory A., & Kruijer, Thomas S. The origin of volatile elements in the Earth–Moon system. United States. https://doi.org/10.1073/pnas.2115726119
Borg, Lars E., Brennecka, Gregory A., and Kruijer, Thomas S. Mon .
"The origin of volatile elements in the Earth–Moon system". United States. https://doi.org/10.1073/pnas.2115726119.
@article{osti_1845032,
title = {The origin of volatile elements in the Earth–Moon system},
author = {Borg, Lars E. and Brennecka, Gregory A. and Kruijer, Thomas S.},
abstractNote = {The origin of volatile species such as water in the Earth–Moon system is a subject of intense debate but is obfuscated by the potential for volatile loss during the Giant Impact that resulted in the formation of these bodies. One way to address these topics and place constraints on the temporal evolution of volatile components in planetary bodies is by using the observed decay of 87Rb to 87Sr because Rb is a moderately volatile element, whereas Sr is much more refractory. Here, we show that lunar highland rocks that crystallized ~4.35 billion years ago exhibit very limited ingrowth of 87Sr, indicating that prior to the Moon-forming impact, the impactor commonly referred to as “Theia” and the proto-Earth both must have already been strongly depleted in volatile elements relative to primitive meteorites. These results imply that 1) the volatile element depletion of the Moon did not arise from the Giant Impact, 2) volatile element distributions on the Moon and Earth were principally inherited from their precursors, 3) both Theia and the proto-Earth probably formed in the inner solar system, and 4) the Giant Impact occurred relatively late in solar system history.},
doi = {10.1073/pnas.2115726119},
journal = {Proceedings of the National Academy of Sciences of the United States of America},
number = 8,
volume = 119,
place = {United States},
year = {Mon Feb 14 00:00:00 EST 2022},
month = {Mon Feb 14 00:00:00 EST 2022}
}
https://doi.org/10.1073/pnas.2115726119
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