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Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977
Northwest Africa (NWA) 2977 is a lunar basaltic meteorite that was found in 2005 and has been classified as an olivine cumulate gabbro. This meteorite contains a shock melt vein (SMV) induced by an intense shock event. We report herein on an in-situ analysis of phosphates in the host gabbro and the...
Autores principales: | , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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The Mass Spectrometry Society of Japan
2023
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Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10209660/ https://www.ncbi.nlm.nih.gov/pubmed/37250597 http://dx.doi.org/10.5702/massspectrometry.A0115 |
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author | Moromoto, Narumi Kawai, Yosuke Terada, Kentaro Miyahara, Masaaki Takahata, Naoto Sano, Yuji Fujikawa, Naoko Anand, Mahesh |
author_facet | Moromoto, Narumi Kawai, Yosuke Terada, Kentaro Miyahara, Masaaki Takahata, Naoto Sano, Yuji Fujikawa, Naoko Anand, Mahesh |
author_sort | Moromoto, Narumi |
collection | PubMed |
description | Northwest Africa (NWA) 2977 is a lunar basaltic meteorite that was found in 2005 and has been classified as an olivine cumulate gabbro. This meteorite contains a shock melt vein (SMV) induced by an intense shock event. We report herein on an in-situ analysis of phosphates in the host gabbro and the shock vein for the U–Pb dating of NWA 2977 using an ion microprobe, NanoSIMS. The majority of the analyzed phosphates, in both the SMV and host-rock, lie on a linear regression in (238)U/(206)Pb–(207)Pb/(206)Pb–(204)Pb/(206)Pb three-dimensional space, indicating a total Pb/U isochron age of 3.15±0.12 Ga (95% confidence level), which is consistent ages determined in previous isotopic studies of NWA 2977 (Sm–Nd age of 3.10±0.05 Ga, Rb–Sr age of 3.29±0.11 Ga, and Pb–Pb baddeleyite age of 3.12±0.01 Ga), and identical to the age of the U–Pb phosphate in a paired meteorite NWA 773, 3.09±0.20 Ga, derived from our dataset. There was no clear difference in the formation age between the phosphates found in the SMV and host-rock, although the shape and size of the grains and the Raman spectra show the evidence of intense shock metamorphism. Based on these findings, the cooling rate of the phosphate was very rapid, constrained to be larger than 140 K/s. |
format | Online Article Text |
id | pubmed-10209660 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2023 |
publisher | The Mass Spectrometry Society of Japan |
record_format | MEDLINE/PubMed |
spelling | pubmed-102096602023-05-26 Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977 Moromoto, Narumi Kawai, Yosuke Terada, Kentaro Miyahara, Masaaki Takahata, Naoto Sano, Yuji Fujikawa, Naoko Anand, Mahesh Mass Spectrom (Tokyo) Original Article Northwest Africa (NWA) 2977 is a lunar basaltic meteorite that was found in 2005 and has been classified as an olivine cumulate gabbro. This meteorite contains a shock melt vein (SMV) induced by an intense shock event. We report herein on an in-situ analysis of phosphates in the host gabbro and the shock vein for the U–Pb dating of NWA 2977 using an ion microprobe, NanoSIMS. The majority of the analyzed phosphates, in both the SMV and host-rock, lie on a linear regression in (238)U/(206)Pb–(207)Pb/(206)Pb–(204)Pb/(206)Pb three-dimensional space, indicating a total Pb/U isochron age of 3.15±0.12 Ga (95% confidence level), which is consistent ages determined in previous isotopic studies of NWA 2977 (Sm–Nd age of 3.10±0.05 Ga, Rb–Sr age of 3.29±0.11 Ga, and Pb–Pb baddeleyite age of 3.12±0.01 Ga), and identical to the age of the U–Pb phosphate in a paired meteorite NWA 773, 3.09±0.20 Ga, derived from our dataset. There was no clear difference in the formation age between the phosphates found in the SMV and host-rock, although the shape and size of the grains and the Raman spectra show the evidence of intense shock metamorphism. Based on these findings, the cooling rate of the phosphate was very rapid, constrained to be larger than 140 K/s. The Mass Spectrometry Society of Japan 2023 2023-02-10 /pmc/articles/PMC10209660/ /pubmed/37250597 http://dx.doi.org/10.5702/massspectrometry.A0115 Text en Copyright © 2023 Narumi Moromoto, Yosuke Kawai, Kentaro Terada, Masaaki Miyahara, Naoto Takahata, Yuji Sano, Naoko Fujikawa, and Mahesh Anand. https://creativecommons.org/licenses/by/2.5/This is an open-access article distributed under the terms of Creative Commons Attribution Non-Commercial 4.0 International License, which permits use, distribution, and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes. |
spellingShingle | Original Article Moromoto, Narumi Kawai, Yosuke Terada, Kentaro Miyahara, Masaaki Takahata, Naoto Sano, Yuji Fujikawa, Naoko Anand, Mahesh Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977 |
title | Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977 |
title_full | Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977 |
title_fullStr | Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977 |
title_full_unstemmed | Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977 |
title_short | Uranium–Lead Systematics of Lunar Basaltic Meteorite Northwest Africa 2977 |
title_sort | uranium–lead systematics of lunar basaltic meteorite northwest africa 2977 |
topic | Original Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10209660/ https://www.ncbi.nlm.nih.gov/pubmed/37250597 http://dx.doi.org/10.5702/massspectrometry.A0115 |
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