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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)
https://doi.org/10.15094/00007720
https://doi.org/10.15094/0000772007684316-44f5-4b1f-b807-40e459591ba4
名前 / ファイル | ライセンス | アクション |
---|---|---|
KJ00002476720 (3.5 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1973-09-01 | |||||
タイトル | ||||||
タイトル | 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) | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Study of the Extraterrestrial Materials at Antarctica, III : On the Yamato Meteorites | |||||
言語 | ||||||
言語 | jpn | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00007720 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
論文名よみ | ||||||
その他のタイトル | 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 | |||||
著者名(日) |
島, 正子
× 島, 正子× 岡田, 昭彦× 島, 誠 |
|||||
著者名(英) |
SHIMA, Masako
× SHIMA, Masako× OKADA, Akihiko× SHIMA, Makoto |
|||||
著者所属(日) | ||||||
理化学研究所 | ||||||
著者所属(日) | ||||||
理化学研究所 | ||||||
著者所属(英) | ||||||
en | ||||||
Max-Planck Institut fur Chemie | ||||||
著者所属(英) | ||||||
en | ||||||
The Institute of Physical and Chemical Research | ||||||
著者所属(英) | ||||||
en | ||||||
The Institute of Physical and Chemical Research | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 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. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00181831 | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00857289 | |||||
書誌情報 |
南極資料 巻 47, p. 86-97, 発行日 1973-09 |
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国際十進分類法 | ||||||
主題Scheme | UDC | |||||
主題 | 552.6 | |||||
出版者 | ||||||
出版者 | 国立極地研究所 |