Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites

P(論文) Yamato (Y) 000593 is a new nakhlite recovered from Antarctica and is composed of roughly 80% augite, 10% olivine and 10% mesostasis. Augite is chemically homogeneous except for Fe-rich rims adjacent to the mesostasis. Olivine has more extensive chemical zoning, but the most Fe-rich part is als...

Full description

Bibliographic Details
Main Authors: Mikouchi,Takashi, Koizumi,Eisuke, Monkawa,Akira, Ueda,Yuji, Miyamoto,Masamichi
Language:English
Published: National Institute of Polar Research 2003
Subjects:
Online Access:https://nipr.repo.nii.ac.jp/record/6025/files/KJ00000040861.pdf
https://doi.org/10.15094/00006025
https://nipr.repo.nii.ac.jp/records/6025
_version_ 1829302730016948224
author Mikouchi,Takashi
Koizumi,Eisuke
Monkawa,Akira
Ueda,Yuji
Miyamoto,Masamichi
author_facet Mikouchi,Takashi
Koizumi,Eisuke
Monkawa,Akira
Ueda,Yuji
Miyamoto,Masamichi
author_sort Mikouchi,Takashi
collection National Institute of Polar Research Repository, Japan
description P(論文) Yamato (Y) 000593 is a new nakhlite recovered from Antarctica and is composed of roughly 80% augite, 10% olivine and 10% mesostasis. Augite is chemically homogeneous except for Fe-rich rims adjacent to the mesostasis. Olivine has more extensive chemical zoning, but the most Fe-rich part is also near the mesostasis. These observations suggest that chemical zoning of both augite and olivine was produced by interaction with the mesostasis. The crystallization history of Y000593 as deduced from this study is as follows. (1) Crystallization of cumulus augite and olivine and formation of symplectites in olivine. (2) Accumulation of augite and olivine. (3) Mesostasis crystallization and interaction of the augite and olivine rims with the intercumulus melt. (4) Aqueous alteration. The petrography and mineralogy of Y000593 is generally similar to other nakhlites, but minor mineralogical differences are observed. These differences resulted from different thermal histories due to different locations (burial depths) in the same cooling cumulate pile. Y000593 is most similar to Nakhla and both samples experienced similar formation histories. However, later mesostasis crystallization of Y000593 was more rapid than Nakhla due to its faster cooling rate. The burial depth of Y000593 would be shallower than 3 m from the surface, and is intermediate between NWA817 and Nakhla. The abundance and mineralogy of the mesostasis as well as augite and olivine rim compositions are related to the burial depths of nakhlites. departmental bulletin paper
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
geographic Yamato
geographic_facet Yamato
id ftnipr:oai:nipr.repo.nii.ac.jp:00006025
institution Open Polar
language English
long_lat ENVELOPE(35.583,35.583,-71.417,-71.417)
op_collection_id ftnipr
op_doi https://doi.org/10.15094/00006025
op_relation Antarctic meteorite research
16
34
57
AA11182426
https://nipr.repo.nii.ac.jp/record/6025/files/KJ00000040861.pdf
https://doi.org/10.15094/00006025
https://nipr.repo.nii.ac.jp/records/6025
publishDate 2003
publisher National Institute of Polar Research
record_format openpolar
spelling ftnipr:oai:nipr.repo.nii.ac.jp:00006025 2025-04-13T14:10:52+00:00 Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites Mikouchi,Takashi Koizumi,Eisuke Monkawa,Akira Ueda,Yuji Miyamoto,Masamichi 2003-03 application/pdf https://nipr.repo.nii.ac.jp/record/6025/files/KJ00000040861.pdf https://doi.org/10.15094/00006025 https://nipr.repo.nii.ac.jp/records/6025 eng eng National Institute of Polar Research Antarctic meteorite research 16 34 57 AA11182426 https://nipr.repo.nii.ac.jp/record/6025/files/KJ00000040861.pdf https://doi.org/10.15094/00006025 https://nipr.repo.nii.ac.jp/records/6025 nakhlite augite olivine crystallization cooling rate 2003 ftnipr https://doi.org/10.15094/00006025 2025-03-19T10:19:57Z P(論文) Yamato (Y) 000593 is a new nakhlite recovered from Antarctica and is composed of roughly 80% augite, 10% olivine and 10% mesostasis. Augite is chemically homogeneous except for Fe-rich rims adjacent to the mesostasis. Olivine has more extensive chemical zoning, but the most Fe-rich part is also near the mesostasis. These observations suggest that chemical zoning of both augite and olivine was produced by interaction with the mesostasis. The crystallization history of Y000593 as deduced from this study is as follows. (1) Crystallization of cumulus augite and olivine and formation of symplectites in olivine. (2) Accumulation of augite and olivine. (3) Mesostasis crystallization and interaction of the augite and olivine rims with the intercumulus melt. (4) Aqueous alteration. The petrography and mineralogy of Y000593 is generally similar to other nakhlites, but minor mineralogical differences are observed. These differences resulted from different thermal histories due to different locations (burial depths) in the same cooling cumulate pile. Y000593 is most similar to Nakhla and both samples experienced similar formation histories. However, later mesostasis crystallization of Y000593 was more rapid than Nakhla due to its faster cooling rate. The burial depth of Y000593 would be shallower than 3 m from the surface, and is intermediate between NWA817 and Nakhla. The abundance and mineralogy of the mesostasis as well as augite and olivine rim compositions are related to the burial depths of nakhlites. departmental bulletin paper Other/Unknown Material Antarc* Antarctica National Institute of Polar Research Repository, Japan Yamato ENVELOPE(35.583,35.583,-71.417,-71.417)
spellingShingle nakhlite
augite
olivine
crystallization
cooling rate
Mikouchi,Takashi
Koizumi,Eisuke
Monkawa,Akira
Ueda,Yuji
Miyamoto,Masamichi
Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites
title Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites
title_full Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites
title_fullStr Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites
title_full_unstemmed Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites
title_short Mineralogy and petrology of Yamato 000593: Comparison with other Martian nakhlite meteorites
title_sort mineralogy and petrology of yamato 000593: comparison with other martian nakhlite meteorites
topic nakhlite
augite
olivine
crystallization
cooling rate
topic_facet nakhlite
augite
olivine
crystallization
cooling rate
url https://nipr.repo.nii.ac.jp/record/6025/files/KJ00000040861.pdf
https://doi.org/10.15094/00006025
https://nipr.repo.nii.ac.jp/records/6025