Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988

Noble gases and K concentrations have been determined for aliquot samples prepared from the five Antarctic R-chondrites Yamato (Y)-75302,Y-791827,Y-793575,Y-82002,and Asuka (A)-881988. K-Ar ages of about 4.2Ga were obtained for Y-75302,Y-791827,Y-793575 and A-881988,while Y-82002 showed a slightly y...

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Main Authors: Nagao,Keisuke, Okazaki,Ryuji, Sawada,Shinobu, Nakamura,Noboru
Format: Report
Language:English
Published: Laboratory for Earthquake Chemistry, Graduate School of Science, University of Tokyo/Laboratory for Earthquake Chemistry, Graduate School of Science, University of Tokyo/Graduate School of Science and Technology, Kobe University/Graduate School of Science and Technology, Kobe University 1999
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spelling ftnipr:oai:nipr.repo.nii.ac.jp:00005946 2023-05-15T13:46:39+02:00 Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988 Nagao,Keisuke Okazaki,Ryuji Sawada,Shinobu Nakamura,Noboru 1999-03 https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=5946 http://id.nii.ac.jp/1291/00005946/ https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=5946&item_no=1&attribute_id=18&file_no=1 en eng Laboratory for Earthquake Chemistry, Graduate School of Science, University of Tokyo/Laboratory for Earthquake Chemistry, Graduate School of Science, University of Tokyo/Graduate School of Science and Technology, Kobe University/Graduate School of Science and Technology, Kobe University National Institute of Polar Research https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=5946 http://id.nii.ac.jp/1291/00005946/ AA11182426 Antarctic meteorite research, 12, 81-93(1999-03) https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=5946&item_no=1&attribute_id=18&file_no=1 Departmental Bulletin Paper P(論文) 1999 ftnipr 2023-02-25T20:13:36Z Noble gases and K concentrations have been determined for aliquot samples prepared from the five Antarctic R-chondrites Yamato (Y)-75302,Y-791827,Y-793575,Y-82002,and Asuka (A)-881988. K-Ar ages of about 4.2Ga were obtained for Y-75302,Y-791827,Y-793575 and A-881988,while Y-82002 showed a slightly younger age of 3.9Ga. The Y-75302,Y-791827 and Y-82002 are enriched in solar light noble gases. Four meteorites Y-75302,Y-791827,Y-82002 and A-881988 have cosmic-ray exposure ages of about 20Ma, while the age of Y-793575 is about 7Ma. Based on the noble gas compositions and K-Ar ages, Y-75302 and Y-791827 are probably paired and Y-82002 may belong to this pair. Relatively high and variable ^<129>Xe/^<132>Xe ratios between 2-3.7 as well as enrichments of heavier Xe isotopes were observed in all R-chondrites. Report Antarc* Antarctic National Institute of Polar Research Repository, Japan Antarctic The ''Y'' ENVELOPE(-112.453,-112.453,57.591,57.591) 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 Noble gases and K concentrations have been determined for aliquot samples prepared from the five Antarctic R-chondrites Yamato (Y)-75302,Y-791827,Y-793575,Y-82002,and Asuka (A)-881988. K-Ar ages of about 4.2Ga were obtained for Y-75302,Y-791827,Y-793575 and A-881988,while Y-82002 showed a slightly younger age of 3.9Ga. The Y-75302,Y-791827 and Y-82002 are enriched in solar light noble gases. Four meteorites Y-75302,Y-791827,Y-82002 and A-881988 have cosmic-ray exposure ages of about 20Ma, while the age of Y-793575 is about 7Ma. Based on the noble gas compositions and K-Ar ages, Y-75302 and Y-791827 are probably paired and Y-82002 may belong to this pair. Relatively high and variable ^<129>Xe/^<132>Xe ratios between 2-3.7 as well as enrichments of heavier Xe isotopes were observed in all R-chondrites.
format Report
author Nagao,Keisuke
Okazaki,Ryuji
Sawada,Shinobu
Nakamura,Noboru
spellingShingle Nagao,Keisuke
Okazaki,Ryuji
Sawada,Shinobu
Nakamura,Noboru
Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988
author_facet Nagao,Keisuke
Okazaki,Ryuji
Sawada,Shinobu
Nakamura,Noboru
author_sort Nagao,Keisuke
title Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988
title_short Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988
title_full Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988
title_fullStr Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988
title_full_unstemmed Noble gases and K-Ar ages of five Rumuruti chondrites Yamato(Y)-75302, Y-791827, Y-793575, Y-82002, and Asuka-881988
title_sort noble gases and k-ar ages of five rumuruti chondrites yamato(y)-75302, y-791827, y-793575, y-82002, and asuka-881988
publisher Laboratory for Earthquake Chemistry, Graduate School of Science, University of Tokyo/Laboratory for Earthquake Chemistry, Graduate School of Science, University of Tokyo/Graduate School of Science and Technology, Kobe University/Graduate School of Science and Technology, Kobe University
publishDate 1999
url https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=5946
http://id.nii.ac.jp/1291/00005946/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=5946&item_no=1&attribute_id=18&file_no=1
long_lat ENVELOPE(-112.453,-112.453,57.591,57.591)
ENVELOPE(35.583,35.583,-71.417,-71.417)
geographic Antarctic
The ''Y''
Yamato
geographic_facet Antarctic
The ''Y''
Yamato
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_relation https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=5946
http://id.nii.ac.jp/1291/00005946/
AA11182426
Antarctic meteorite research, 12, 81-93(1999-03)
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=5946&item_no=1&attribute_id=18&file_no=1
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