WEKO3
アイテム
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微小重力小惑星における金属鉄・ケイ酸塩溶融液の分離機構解明
https://jaxa.repo.nii.ac.jp/records/13723
https://jaxa.repo.nii.ac.jp/records/1372342958004-5526-440a-82f7-133ecce3888c
名前 / ファイル | ライセンス | アクション |
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64113106.pdf (470.8 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | 微小重力小惑星における金属鉄・ケイ酸塩溶融液の分離機構解明 | |||||
言語 | ||||||
言語 | jpn | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Microgravity, Asteroids, Planetismals, Origin of terrestrial planets, Core formation | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
その他のタイトル(英) | ||||||
その他のタイトル | Segregation mechanism of metal and silicate liquids on the microgravity asteroids | |||||
著者 |
荒井, 朋子
× 荒井, 朋子× 武田, 弘× 村上, 敬司× Arai, Tomoko× Takeda, Hiroshi× Murakami, Keiji |
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著者所属 | ||||||
国立極地研究所 | ||||||
著者所属 | ||||||
千葉工業大学 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙環境利用センター | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
著者所属(英) | ||||||
en | ||||||
Chiba Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Space Environment Utilization Center, Japan Aerospace Exploration Agency (JAXA) | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙利用シンポジウム en : Space Utilization Research: Proceedings of Space Utilization Symposium 巻 22, 発行日 2006-03 |
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会議概要(会議名, 開催地, 会期, 主催者等) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第22回宇宙利用シンポジウム(2006年1月17日-19日, 日本学術会議6階会議室 六本木、東京) | |||||
会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The Twenty-second Space Utilization Symposium (January 17-19, 2006: Science Council of Japan, Roppongi, Tokyo, Japan) | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | IAB irons are one of a few types of iron meteorites that contain silicate inclusions. Caddo County IAB iron meteorite includes silicate inclusions rich in Na-rich plagioclase and diopside, which is classified as andesite. The andestic material can be an early partial melt product of chondritic materials. This indicates inhomogeneous segregation of partial melt of andesitic silicate and Fe-Ni-S metal from chondritic source occured even in a small planetesimal. This further implies that building block of terrestrial planets are not only chondritic materials, but also such inhomogeneously segregated partial melts from chondritic sources. Thus, the physical mechanism of metal segregation under microgravity, low pressure, and low oxygen fugacity needs to be understood, in order to decipher the abundances and partitioning behaviors of chemical compositions of the terrestrial planets. We plan to experimentally verify our model for the segregation mechanism of metal and silicate liquids on the microgravity planetismal. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 共催: 日本学術会議 | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Meeting sponsors: The Science Council of Japan, The Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN10324210 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064113106 |