ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク

P(論文) Antarctica is thought to be the most suitable place for searching extraterrestrial materials. Since 1965, we have been studying microtektite and cosmic dust in Antarctica. In 1969, the Japanese Expedition Team collected stony meteorites and brought them back to Japan. Scientific study of these...

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Main Authors: 島, 正子, シマ, マサコ, 岡田, 昭彦, オカダ, アキヒコ, 島, 誠, シマ, マコト, SHIMA, Masako, OKADA, Akihiko, SHIMA, Makoto
Language:Japanese
Published: 国立極地研究所 1973
Subjects:
Online Access:https://nipr.repo.nii.ac.jp/record/7720/files/KJ00002476720.pdf
https://doi.org/10.15094/00007720
https://nipr.repo.nii.ac.jp/records/7720
_version_ 1829307400570535936
author 島, 正子
シマ, マサコ
岡田, 昭彦
オカダ, アキヒコ
島, 誠
シマ, マコト
SHIMA, Masako
OKADA, Akihiko
SHIMA, Makoto
author_facet 島, 正子
シマ, マサコ
岡田, 昭彦
オカダ, アキヒコ
島, 誠
シマ, マコト
SHIMA, Masako
OKADA, Akihiko
SHIMA, Makoto
author_sort 島, 正子
collection National Institute of Polar Research Repository, Japan
description P(論文) Antarctica is thought to be the most suitable place for searching extraterrestrial materials. Since 1965, we have been studying microtektite and cosmic dust in Antarctica. In 1969, the Japanese Expedition Team collected stony meteorites and brought them back to Japan. Scientific study of these samples has just been started. A part of the samples was examined for mineral composition, and was also analyzed for chemical composition by means of wet chemistry. At the same time, examination of rare gas was carried out with a gas mass-spectrometer. The purpose of the study is to know whether these meteorites are extraterrestrial materials or not. As a result, they were found to be chondrites, which are classified into enstatite chondrite, achondrite, carbonaceous chondrite and bronzite chondrite. For the samples we proposed the name Yamato (a), Yamato (b), Yamato (c) and Yamato (d), following Huss method. They were found on the glacier near the Yamato Mountains (70°S, 37°E) within a small area (about lOxlOkm^2). It is a quite interesting phenomena that different kinds of chondrites are found within a narrow area. This may indicate one shower of meteorites. Also, it is different kinds of chondrites fell at different times in a small area. Or the meteorites, which had fallen over a wide region, have been carried to this narrow area by the glacier movement. departmental bulletin paper
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
geographic Yamato
geographic_facet Yamato
id ftnipr:oai:nipr.repo.nii.ac.jp:00007720
institution Open Polar
language Japanese
long_lat ENVELOPE(35.583,35.583,-71.417,-71.417)
op_collection_id ftnipr
op_doi https://doi.org/10.15094/00007720
op_relation 南極資料
47
86
97
AN00181831
00857289
https://nipr.repo.nii.ac.jp/record/7720/files/KJ00002476720.pdf
https://doi.org/10.15094/00007720
https://nipr.repo.nii.ac.jp/records/7720
publishDate 1973
publisher 国立極地研究所
record_format openpolar
spelling ftnipr:oai:nipr.repo.nii.ac.jp:00007720 2025-04-13T14:07:34+00:00 ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク 南極における宇宙物質に関する研究(III) : 隕石について(日本南極地域観測隊の報告) Study of the Extraterrestrial Materials at Antarctica, III : On the Yamato Meteorites 島, 正子 シマ, マサコ 岡田, 昭彦 オカダ, アキヒコ 島, 誠 シマ, マコト SHIMA, Masako OKADA, Akihiko SHIMA, Makoto 1973-09 application/pdf https://nipr.repo.nii.ac.jp/record/7720/files/KJ00002476720.pdf https://doi.org/10.15094/00007720 https://nipr.repo.nii.ac.jp/records/7720 jpn jpn 国立極地研究所 南極資料 47 86 97 AN00181831 00857289 https://nipr.repo.nii.ac.jp/record/7720/files/KJ00002476720.pdf https://doi.org/10.15094/00007720 https://nipr.repo.nii.ac.jp/records/7720 552.6 1973 ftnipr https://doi.org/10.15094/00007720 2025-03-19T10:19:57Z P(論文) Antarctica is thought to be the most suitable place for searching extraterrestrial materials. Since 1965, we have been studying microtektite and cosmic dust in Antarctica. In 1969, the Japanese Expedition Team collected stony meteorites and brought them back to Japan. Scientific study of these samples has just been started. A part of the samples was examined for mineral composition, and was also analyzed for chemical composition by means of wet chemistry. At the same time, examination of rare gas was carried out with a gas mass-spectrometer. The purpose of the study is to know whether these meteorites are extraterrestrial materials or not. As a result, they were found to be chondrites, which are classified into enstatite chondrite, achondrite, carbonaceous chondrite and bronzite chondrite. For the samples we proposed the name Yamato (a), Yamato (b), Yamato (c) and Yamato (d), following Huss method. They were found on the glacier near the Yamato Mountains (70°S, 37°E) within a small area (about lOxlOkm^2). It is a quite interesting phenomena that different kinds of chondrites are found within a narrow area. This may indicate one shower of meteorites. Also, it is different kinds of chondrites fell at different times in a small area. Or the meteorites, which had fallen over a wide region, have been carried to this narrow area by the glacier movement. 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 552.6
島, 正子
シマ, マサコ
岡田, 昭彦
オカダ, アキヒコ
島, 誠
シマ, マコト
SHIMA, Masako
OKADA, Akihiko
SHIMA, Makoto
ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク
title ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク
title_full ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク
title_fullStr ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク
title_full_unstemmed ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク
title_short ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク
title_sort ナンキョク ニオケル ウチュウ ブッシツ ニ カンスル ケンキュウ 3 インセキ ニツイテ ニホン ナンキョク チイキ カンソクタイ ノ ホウコク
topic 552.6
topic_facet 552.6
url https://nipr.repo.nii.ac.jp/record/7720/files/KJ00002476720.pdf
https://doi.org/10.15094/00007720
https://nipr.repo.nii.ac.jp/records/7720