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SPICA Spectroscopy of Cometary Refractory and Icy Dust Grains
https://jaxa.repo.nii.ac.jp/records/3062
https://jaxa.repo.nii.ac.jp/records/3062f8378509-6fce-4dd4-b7df-8db14316c911
名前 / ファイル | ライセンス | アクション |
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AA1730027085.pdf (188.2 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-07 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | SPICA Spectroscopy of Cometary Refractory and Icy Dust Grains | |||||
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 | |||||
著者 |
古荘, 玲子
× 古荘, 玲子× 大坪, 貴文× 本田, 充彦× 渡部, 潤一× 布施, 哲治× 石黒, 正晃× Furusho, Reiko× Otsubo, Takafumi× Honda, Mitsuhiko× Watanabe, Junichi× Fuse, Tetsuharu× Ishiguro, Masateru |
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著者所属 | ||||||
都留文科大学 : 国立天文台 | ||||||
著者所属 | ||||||
東北大学 | ||||||
著者所属 | ||||||
神奈川大学 | ||||||
著者所属 | ||||||
国立天文台 | ||||||
著者所属 | ||||||
情報通信研究機構 | ||||||
著者所属 | ||||||
Seoul National University | ||||||
著者所属(英) | ||||||
en | ||||||
Tsuru University : National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Tohoku University | ||||||
著者所属(英) | ||||||
en | ||||||
kanagawa University | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Information & Communications Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Seoul National University | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構(JAXA) | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe 巻 JAXA-SP-17-010E, p. 387-388, 発行日 2018-03-09 |
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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 | SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We propose mid/far-infrared spectroscopy of comets to study (1) precise astromineralogy of cometary refractory dust and, (2) environment of H2O ice formation (temperature and gas density) in the early solar nebula. The mid/far-infrared spectroscopy is a powerful diagnostic tool to investigate the size, shape, and chemical composition of cometary dust, so that it will enable us to reveal the process of refractory grain growth and radial transportation of dust grains in the early solar nebula. However, it is not easy to disentangle constituent minerals clearly only with the 10 μm-band of ground-based observations. The crystalline silicate bands at 33, 49, and 69 μm are a clue to investigate the dust size and chemical composition. Whether cometary H2O icy dust grain is amorphous or crystalline reflects its formation environment (temperature and gas density). The H2O ice bands are at 6, 12, 44 and 65 μm. Since the reason why crystalline H2O icy grains were detected in a few comets is still unclear, statistical study on the abundance of the cometary crystalline H2O ice dust is important to reveal the history of formation and evolution of the comets. | |||||
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(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
ISSNONLINE | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2433-2232 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA1730027085 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-17-010E |