Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites

P(論文) The abundances of Mg, Ca, Fe, K, Rb, Sr, Ba, and REE in five Antarctic "unique" meteorites, acapulcoite-lodranite type, Yamato (Y)-74063,Y-74357,Y-8002,and Allan Hills (ALH)-78230,and winonaite type, Y-75300 were determined by isotope dilution mass spectrometry. The Sr isotopic compo...

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Main Authors: Torigoye,Noriko, Ymamoto,Koshi, Misawa,Keiji, Nakamura,Noboru
Language:English
Published: National Institute of Polar Research 1993
Subjects:
Online Access:https://nipr.repo.nii.ac.jp/record/4604/files/KJ00000036410.pdf
https://doi.org/10.15094/00004604
https://nipr.repo.nii.ac.jp/records/4604
_version_ 1829302376307097600
author Torigoye,Noriko
Ymamoto,Koshi
Misawa,Keiji
Nakamura,Noboru
author_facet Torigoye,Noriko
Ymamoto,Koshi
Misawa,Keiji
Nakamura,Noboru
author_sort Torigoye,Noriko
collection National Institute of Polar Research Repository, Japan
description P(論文) The abundances of Mg, Ca, Fe, K, Rb, Sr, Ba, and REE in five Antarctic "unique" meteorites, acapulcoite-lodranite type, Yamato (Y)-74063,Y-74357,Y-8002,and Allan Hills (ALH)-78230,and winonaite type, Y-75300 were determined by isotope dilution mass spectrometry. The Sr isotopic compositions of Y-74063,Y-75300,Y-8002,and ALH-78230 were also measured to investigate the whole-rock Rb-Sr isotopic systematics. In terms of the REE abundance pattern, these meteorites are grouped as follows; (1) Y-74063 and ALH-78230 with chondritic REE patterns, (2) Y-74357 with light REE depletion plus alkali and alkaline earth element depletion, and (3) Y-75300 and Y-8002 with middle REE depletion (V-shaped REE pattern) plus a positive Eu anomaly). The mineralogy of these meteorites is closely related to the above REE classification. The ^<87>Rb-^<87>Sr age determined from 'whole-rock samples' for Y-74063,Y-75300,Y-8002,and ALH-78230 is consistent with their formation of 4.5Ga, albeit with a large uncertainty due to the blank correction. Using the mineral/liquid partition coefficients of trace elements, the petrogenetic model calculations were performed. The results give indication on the origin of these "unique" meteorites. Y-74063 and ALH-78230 could be formed through a small degree of partial melting (less than a few%) from a chondritic starting material. Y-74357 could be formed by a larger degree (12%) of partial melting. On the other hand, the V-shaped REE pattern of the third group (Y-75300 and Y-8002) could not be explained by a simple partial melting process. The V-shaped REE pattern may be explained only by assuming the solid state equilibration within a reservoir with chondritic composition. It is suggested that Y-75300 and Y-8002 might be derived from parental materials depleted in phosphate and clinopyroxene. departmental bulletin paper
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
geographic Antarctic
Yamato
Allan Hills
geographic_facet Antarctic
Yamato
Allan Hills
id ftnipr:oai:nipr.repo.nii.ac.jp:00004604
institution Open Polar
language English
long_lat ENVELOPE(35.583,35.583,-71.417,-71.417)
ENVELOPE(159.667,159.667,-76.717,-76.717)
op_collection_id ftnipr
op_doi https://doi.org/10.15094/00004604
op_relation Proceedings of the NIPR Symposium on Antarctic Meteorites
6
100
119
AA10784627
https://nipr.repo.nii.ac.jp/record/4604/files/KJ00000036410.pdf
https://doi.org/10.15094/00004604
https://nipr.repo.nii.ac.jp/records/4604
publishDate 1993
publisher National Institute of Polar Research
record_format openpolar
spelling ftnipr:oai:nipr.repo.nii.ac.jp:00004604 2025-04-13T14:10:33+00:00 Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites Torigoye,Noriko Ymamoto,Koshi Misawa,Keiji Nakamura,Noboru 1993-05 application/pdf https://nipr.repo.nii.ac.jp/record/4604/files/KJ00000036410.pdf https://doi.org/10.15094/00004604 https://nipr.repo.nii.ac.jp/records/4604 eng eng National Institute of Polar Research Proceedings of the NIPR Symposium on Antarctic Meteorites 6 100 119 AA10784627 https://nipr.repo.nii.ac.jp/record/4604/files/KJ00000036410.pdf https://doi.org/10.15094/00004604 https://nipr.repo.nii.ac.jp/records/4604 1993 ftnipr https://doi.org/10.15094/00004604 2025-03-19T10:19:57Z P(論文) The abundances of Mg, Ca, Fe, K, Rb, Sr, Ba, and REE in five Antarctic "unique" meteorites, acapulcoite-lodranite type, Yamato (Y)-74063,Y-74357,Y-8002,and Allan Hills (ALH)-78230,and winonaite type, Y-75300 were determined by isotope dilution mass spectrometry. The Sr isotopic compositions of Y-74063,Y-75300,Y-8002,and ALH-78230 were also measured to investigate the whole-rock Rb-Sr isotopic systematics. In terms of the REE abundance pattern, these meteorites are grouped as follows; (1) Y-74063 and ALH-78230 with chondritic REE patterns, (2) Y-74357 with light REE depletion plus alkali and alkaline earth element depletion, and (3) Y-75300 and Y-8002 with middle REE depletion (V-shaped REE pattern) plus a positive Eu anomaly). The mineralogy of these meteorites is closely related to the above REE classification. The ^<87>Rb-^<87>Sr age determined from 'whole-rock samples' for Y-74063,Y-75300,Y-8002,and ALH-78230 is consistent with their formation of 4.5Ga, albeit with a large uncertainty due to the blank correction. Using the mineral/liquid partition coefficients of trace elements, the petrogenetic model calculations were performed. The results give indication on the origin of these "unique" meteorites. Y-74063 and ALH-78230 could be formed through a small degree of partial melting (less than a few%) from a chondritic starting material. Y-74357 could be formed by a larger degree (12%) of partial melting. On the other hand, the V-shaped REE pattern of the third group (Y-75300 and Y-8002) could not be explained by a simple partial melting process. The V-shaped REE pattern may be explained only by assuming the solid state equilibration within a reservoir with chondritic composition. It is suggested that Y-75300 and Y-8002 might be derived from parental materials depleted in phosphate and clinopyroxene. departmental bulletin paper Other/Unknown Material Antarc* Antarctic National Institute of Polar Research Repository, Japan Antarctic Yamato ENVELOPE(35.583,35.583,-71.417,-71.417) Allan Hills ENVELOPE(159.667,159.667,-76.717,-76.717)
spellingShingle Torigoye,Noriko
Ymamoto,Koshi
Misawa,Keiji
Nakamura,Noboru
Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites
title Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites
title_full Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites
title_fullStr Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites
title_full_unstemmed Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites
title_short Compositions of REE, K, Rb, Sr, Ba, Mg, Ca, Fe, and Sr isotopes in Antarctic"unique" meteorites
title_sort compositions of ree, k, rb, sr, ba, mg, ca, fe, and sr isotopes in antarctic"unique" meteorites
url https://nipr.repo.nii.ac.jp/record/4604/files/KJ00000036410.pdf
https://doi.org/10.15094/00004604
https://nipr.repo.nii.ac.jp/records/4604