Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples

We report INAA compositional data for a 171mg bulk-rock sample of lunar meteorite Yamato-82192,and for two small clasts extracted from the matrix. The two clasts were also studied petrographically, but both appear to be polymict impact melt breccias, not greatly different in composition from the bul...

Full description

Bibliographic Details
Main Authors: Warren,Paul H., Kallemeyn,Gregory W.
Format: Report
Language:English
Published: Institute of Geophysics and Planetary Physics, University of California/Institute of Geophysics and Planetary Physics, University of California 1987
Subjects:
Online Access:https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=2117
http://id.nii.ac.jp/1291/00002117/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=2117&item_no=1&attribute_id=18&file_no=1
id ftnipr:oai:nipr.repo.nii.ac.jp:00002117
record_format openpolar
spelling ftnipr:oai:nipr.repo.nii.ac.jp:00002117 2023-05-15T17:10:59+02:00 Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples Warren,Paul H. Kallemeyn,Gregory W. 1987-03 https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=2117 http://id.nii.ac.jp/1291/00002117/ https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=2117&item_no=1&attribute_id=18&file_no=1 en eng Institute of Geophysics and Planetary Physics, University of California/Institute of Geophysics and Planetary Physics, University of California https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=2117 http://id.nii.ac.jp/1291/00002117/ AA00733561 Memoirs of National Institute of Polar Research. Special issue, 46, 3-20(1987-03) https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=2117&item_no=1&attribute_id=18&file_no=1 Departmental Bulletin Paper P(論文) 1987 ftnipr 2022-11-12T19:42:57Z We report INAA compositional data for a 171mg bulk-rock sample of lunar meteorite Yamato-82192,and for two small clasts extracted from the matrix. The two clasts were also studied petrographically, but both appear to be polymict impact melt breccias, not greatly different in composition from the bulk rock. Like two previously-studied lunar meteorites, Y-82192 is a regolith breccia from a highlands region with remarkably low contents of incompatible elements, by the standards of the small region of the central near side that was explored by the Apollo and Luna sample-return missions. Based on disparities in mg between Y-82192 and ALHA81005,and in Eu/Al and Na/Al between Y-82192 and-791197,we argue that these meteorites probably formed at three different locations, many km apart. Considering the low probability that a crater exists which is both sufficiently large and sufficiently young to account for all three meteorites, we conclude that more than one, and probably more than two, impacts were responsible for launching these samples off the Moon. It follows that at least one of these meteorites is almost certainly a product of the Moon's far side. The coincidence that all three are regolith breccias may be explained by postulating that these rocks were created out of incoherent soils by shocks associated with the same impacts that launched them off the Moon. Report Memoirs of National Institute of Polar Research Polar Research National Institute of Polar Research Repository, Japan Yamato ENVELOPE(35.583,35.583,-71.417,-71.417)
institution Open Polar
collection National Institute of Polar Research Repository, Japan
op_collection_id ftnipr
language English
description We report INAA compositional data for a 171mg bulk-rock sample of lunar meteorite Yamato-82192,and for two small clasts extracted from the matrix. The two clasts were also studied petrographically, but both appear to be polymict impact melt breccias, not greatly different in composition from the bulk rock. Like two previously-studied lunar meteorites, Y-82192 is a regolith breccia from a highlands region with remarkably low contents of incompatible elements, by the standards of the small region of the central near side that was explored by the Apollo and Luna sample-return missions. Based on disparities in mg between Y-82192 and ALHA81005,and in Eu/Al and Na/Al between Y-82192 and-791197,we argue that these meteorites probably formed at three different locations, many km apart. Considering the low probability that a crater exists which is both sufficiently large and sufficiently young to account for all three meteorites, we conclude that more than one, and probably more than two, impacts were responsible for launching these samples off the Moon. It follows that at least one of these meteorites is almost certainly a product of the Moon's far side. The coincidence that all three are regolith breccias may be explained by postulating that these rocks were created out of incoherent soils by shocks associated with the same impacts that launched them off the Moon.
format Report
author Warren,Paul H.
Kallemeyn,Gregory W.
spellingShingle Warren,Paul H.
Kallemeyn,Gregory W.
Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples
author_facet Warren,Paul H.
Kallemeyn,Gregory W.
author_sort Warren,Paul H.
title Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples
title_short Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples
title_full Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples
title_fullStr Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples
title_full_unstemmed Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples
title_sort geochemistry of lunar meteorite yamato-82192: comparison with yamato-791197, alha81005, and other lunar samples
publisher Institute of Geophysics and Planetary Physics, University of California/Institute of Geophysics and Planetary Physics, University of California
publishDate 1987
url https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=2117
http://id.nii.ac.jp/1291/00002117/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=2117&item_no=1&attribute_id=18&file_no=1
long_lat ENVELOPE(35.583,35.583,-71.417,-71.417)
geographic Yamato
geographic_facet Yamato
genre Memoirs of National Institute of Polar Research
Polar Research
genre_facet Memoirs of National Institute of Polar Research
Polar Research
op_relation https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=2117
http://id.nii.ac.jp/1291/00002117/
AA00733561
Memoirs of National Institute of Polar Research. Special issue, 46, 3-20(1987-03)
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=2117&item_no=1&attribute_id=18&file_no=1
_version_ 1766067793326768128