WEKO3
アイテム
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The cooling rate of several shergottites as inferred from Fe-Mg zoning of olivine
https://jaxa.repo.nii.ac.jp/records/20350
https://jaxa.repo.nii.ac.jp/records/20350a3fffb9a-c378-4942-897f-c56daec94bad
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 | ||||||
言語 | en | |||||
タイトル | The cooling rate of several shergottites as inferred from Fe-Mg zoning of olivine | |||||
言語 | ||||||
言語 | eng | |||||
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 | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
宮本, 正道
× 宮本, 正道× Miyamoto, Masamichi× Koizumi, E.× Kaiden, H.× Mikouchi, T |
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著者所属 | ||||||
東京大学大学院理学系研究科地球惑星科学専攻宇宙惑星科学講座 | ||||||
著者所属 | ||||||
リモート・センシング技術センター | ||||||
著者所属 | ||||||
東京大学大学院理学系研究科地球惑星科学専攻宇宙惑星科学講座 | ||||||
著者所属(英) | ||||||
en | ||||||
Space and Planetary Science, Graduate School of Science, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Remote Sensing Technology Center of Japan(RESTEC) | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
著者所属(英) | ||||||
en | ||||||
Space and Planetary Science, Graduate School of Science, University of Tokyo | ||||||
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 |
月・惑星シンポジウム en : Proceedings of the ISAS lunar and planetary symposium 巻 42, p. 26-29, 発行日 2009-08 |
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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42回 月・惑星シンポジウム(2009年8月5-7日, 宇宙航空研究開発機構宇宙科学研究本部) | |||||
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 42nd ISAS Lunar and Planetary Symposium (August 5-7, 2009. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We developed a model to calculate the cooling rate (or burial depth) by using the Fe-Mg chemical zoning profile of olivine considering diffusional modification during crystal growth, because chemical zoning provides information on thermal history of minerals. We calculated the cooling rate and burial depth of martian meteorites (olivine-phyric shergottites: Yamato980459, DaG476, and EET79001). The calculated cooling rate for an olivine in Yamato980459 is 0.20C/h and that for an olivine in DaG476 is 0.089C/h. The calculated cooling rates for olivines in EET79001 are 0.032C/h, 0.08C/h, and 0.30C/h. This result may be consistent with xenocryst origin of EET79001 olivines. These cooling rates correspond to the burial depth of 2-7 m, assuming the rock-like thermal diffusivity. This result suggests shallow intrusions or lava flows on the surface of Mars for the origin of these shergottites. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: CD-ROM1枚 | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Note: One CD-ROM | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA12268968 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064739006 |