The origin of volatile elements in the Earth–Moon system
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 evol...
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| Published in | Proceedings of the National Academy of Sciences - PNAS Vol. 119; no. 8; pp. 1 - 5 |
|---|---|
| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
United States
National Academy of Sciences
22.02.2022
Proceedings of the National Academy of Sciences |
| Subjects | |
| Online Access | Get full text |
| ISSN | 0027-8424 1091-6490 1091-6490 |
| DOI | 10.1073/pnas.2115726119 |
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| 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. |
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| AbstractList | 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. Understanding the history of volatile species such as water in the Earth–Moon system is a major objective of planetary science. In this work, we use the moderately volatile element Rb, which has a long-lived isotope ( 87 Rb) that decays to 87 Sr, to show that lunar volatile element depletion was not caused by the Moon-forming impact. The Rb–Sr systematics of lunar rocks mandate that the bodies involved in the impact that formed the Earth–Moon system were depleted in volatile elements relative to the bulk solar system prior to the impact. As such, Earth’s relatively small proportion of water is either primarily indigenous or was added after the Giant Impact from a source that contained essentially no moderately volatile elements. 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 87 Rb to 87 Sr 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 87 Sr, 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. 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. 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 Rb to Sr 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 Sr, 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. 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.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. |
| Author | Brennecka, Gregory A. Borg, Lars E. Kruijer, Thomas S. |
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| Cites_doi | 10.1029/2019JE005966 10.1016/j.icarus.2003.09.028 10.1038/nature12285 10.1016/j.epsl.2004.04.031 10.1016/j.epsl.2008.06.010 10.1126/science.1226073 10.1016/j.gca.2009.11.005 10.1086/375492 10.1016/j.epsl.2007.07.055 10.1038/nature10328 10.1016/j.icarus.2005.11.009 10.1038/ngeo1429 10.1038/ngeo2574 10.1016/j.icarus.2015.07.018 10.1126/sciadv.aba8949 10.1016/j.chemer.2008.10.001 10.1038/nature14333 10.1002/2017JE005333 10.1016/j.gca.2020.09.013 10.1016/j.gca.2012.01.026 10.1016/j.epsl.2017.07.021 10.1038/nature14360 10.1016/j.epsl.2016.07.010 10.1146/annurev.earth.26.1.53 10.1126/science.1168221 10.1126/science.1225542 10.1038/s41561-019-0398-3 10.1016/j.icarus.2021.114451 10.1016/j.gca.2018.07.023 10.1016/j.epsl.2020.116705 10.1126/science.aad0525 10.1111/j.1945-5100.2010.01137.x 10.1016/j.epsl.2013.05.029 10.1016/j.gca.2016.11.021 10.1016/S0012-821X(01)00479-4 10.1073/pnas.1704461114 10.3847/1538-4357/ab2537 10.1016/j.gca.2008.10.021 10.1038/nature20830 10.1016/j.icarus.2008.03.011 10.1016/0019-1035(75)90070-6 10.1088/0004-637X/787/1/81 10.1016/j.gca.2015.11.041 10.1016/S0016-7037(99)00130-1 10.1126/science.aaa0602 10.1038/s41550-019-0959-9 10.1016/j.epsl.2016.05.039 |
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| References | e_1_3_4_3_2 e_1_3_4_2_2 e_1_3_4_1_2 e_1_3_4_9_2 e_1_3_4_8_2 e_1_3_4_7_2 e_1_3_4_41_2 e_1_3_4_6_2 e_1_3_4_40_2 e_1_3_4_4_2 e_1_3_4_22_2 e_1_3_4_45_2 e_1_3_4_23_2 e_1_3_4_44_2 e_1_3_4_20_2 e_1_3_4_43_2 e_1_3_4_21_2 e_1_3_4_42_2 e_1_3_4_26_2 Gaffney A. (e_1_3_4_5_2) 2011; 46 e_1_3_4_27_2 e_1_3_4_24_2 e_1_3_4_47_2 e_1_3_4_25_2 e_1_3_4_46_2 e_1_3_4_28_2 e_1_3_4_29_2 e_1_3_4_30_2 e_1_3_4_11_2 e_1_3_4_34_2 e_1_3_4_12_2 e_1_3_4_33_2 e_1_3_4_32_2 e_1_3_4_10_2 e_1_3_4_31_2 e_1_3_4_15_2 e_1_3_4_38_2 e_1_3_4_16_2 e_1_3_4_37_2 e_1_3_4_13_2 e_1_3_4_36_2 e_1_3_4_14_2 e_1_3_4_35_2 e_1_3_4_19_2 e_1_3_4_17_2 e_1_3_4_18_2 e_1_3_4_39_2 |
| References_xml | – ident: e_1_3_4_46_2 doi: 10.1029/2019JE005966 – ident: e_1_3_4_15_2 doi: 10.1016/j.icarus.2003.09.028 – ident: e_1_3_4_23_2 doi: 10.1038/nature12285 – ident: e_1_3_4_6_2 doi: 10.1016/j.epsl.2004.04.031 – ident: e_1_3_4_47_2 doi: 10.1016/j.epsl.2008.06.010 – ident: e_1_3_4_17_2 doi: 10.1126/science.1226073 – ident: e_1_3_4_30_2 doi: 10.1016/j.gca.2009.11.005 – ident: e_1_3_4_2_2 doi: 10.1086/375492 – ident: e_1_3_4_35_2 doi: 10.1016/j.epsl.2007.07.055 – ident: e_1_3_4_42_2 doi: 10.1038/nature10328 – ident: e_1_3_4_27_2 doi: 10.1016/j.icarus.2005.11.009 – ident: e_1_3_4_19_2 doi: 10.1038/ngeo1429 – ident: e_1_3_4_39_2 doi: 10.1038/ngeo2574 – ident: e_1_3_4_40_2 doi: 10.1016/j.icarus.2015.07.018 – ident: e_1_3_4_13_2 doi: 10.1126/sciadv.aba8949 – ident: e_1_3_4_21_2 doi: 10.1016/j.chemer.2008.10.001 – ident: e_1_3_4_38_2 doi: 10.1038/nature14333 – ident: e_1_3_4_36_2 doi: 10.1002/2017JE005333 – ident: e_1_3_4_44_2 doi: 10.1016/j.gca.2020.09.013 – ident: e_1_3_4_22_2 doi: 10.1016/j.gca.2012.01.026 – ident: e_1_3_4_11_2 doi: 10.1016/j.epsl.2017.07.021 – ident: e_1_3_4_24_2 doi: 10.1038/nature14360 – ident: e_1_3_4_9_2 doi: 10.1016/j.epsl.2016.07.010 – ident: e_1_3_4_25_2 doi: 10.1146/annurev.earth.26.1.53 – ident: e_1_3_4_29_2 doi: 10.1126/science.1168221 – ident: e_1_3_4_18_2 doi: 10.1126/science.1225542 – ident: e_1_3_4_12_2 doi: 10.1038/s41561-019-0398-3 – ident: e_1_3_4_41_2 doi: 10.1016/j.icarus.2021.114451 – ident: e_1_3_4_3_2 doi: 10.1016/j.gca.2018.07.023 – ident: e_1_3_4_32_2 doi: 10.1016/j.epsl.2020.116705 – ident: e_1_3_4_20_2 doi: 10.1126/science.aad0525 – volume: 46 start-page: 35 year: 2011 ident: e_1_3_4_5_2 article-title: Disturbance of isotopic systematics during experimental shock and thermal metamorphism on a lunar basalt with implications for martian meteorite chronology publication-title: Meteoritics Planetary Sci. doi: 10.1111/j.1945-5100.2010.01137.x – ident: e_1_3_4_7_2 doi: 10.1016/j.epsl.2013.05.029 – ident: e_1_3_4_43_2 doi: 10.1016/j.gca.2016.11.021 – ident: e_1_3_4_14_2 doi: 10.1016/S0012-821X(01)00479-4 – ident: e_1_3_4_8_2 doi: 10.1073/pnas.1704461114 – ident: e_1_3_4_26_2 doi: 10.3847/1538-4357/ab2537 – ident: e_1_3_4_45_2 doi: 10.1016/j.gca.2008.10.021 – ident: e_1_3_4_37_2 doi: 10.1038/nature20830 – ident: e_1_3_4_16_2 doi: 10.1016/j.icarus.2008.03.011 – ident: e_1_3_4_1_2 doi: 10.1016/0019-1035(75)90070-6 – ident: e_1_3_4_28_2 doi: 10.1088/0004-637X/787/1/81 – ident: e_1_3_4_33_2 doi: 10.1016/j.gca.2015.11.041 – ident: e_1_3_4_4_2 doi: 10.1016/S0016-7037(99)00130-1 – ident: e_1_3_4_10_2 doi: 10.1126/science.aaa0602 – ident: e_1_3_4_31_2 doi: 10.1038/s41550-019-0959-9 – ident: e_1_3_4_34_2 doi: 10.1016/j.epsl.2016.05.039 |
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| SubjectTerms | Crystallization Depletion Earth GEOSCIENCES Inner solar system Lunar rocks Moon Physical Sciences Planetary evolution Solar system Strontium 87 |
| Title | The origin of volatile elements in the Earth–Moon system |
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