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The trans-Neptunian Objects after Herschel: What Could SPICA Add to the Understanding of the Kuiper Belt?
https://jaxa.repo.nii.ac.jp/records/3063
https://jaxa.repo.nii.ac.jp/records/306381f8405e-035c-4a8c-b449-2f7b7e984d42
名前 / ファイル | ライセンス | アクション |
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AA1730027086.pdf (274.1 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 | The trans-Neptunian Objects after Herschel: What Could SPICA Add to the Understanding of the Kuiper Belt? | |||||
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 |
Kiss, Cs.
× Kiss, Cs.× Muller, Th. G.× Vilenius, E.× Pal, A.× SantosSanz, P.× Lellouch, E.× Stansberry, J.× Mommert, M.× Muller, M. |
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著者所属(英) | ||||||
en | ||||||
Konkoly Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Max Planck Institute for Extraterrestrial Physics | ||||||
著者所属(英) | ||||||
en | ||||||
Max Planck Institute for Extraterrestrial Physics | ||||||
著者所属(英) | ||||||
en | ||||||
Konkoly Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
Instituto de Astrofisica de Andalucia | ||||||
著者所属(英) | ||||||
en | ||||||
Observatorie de Paris | ||||||
著者所属(英) | ||||||
en | ||||||
Steward Observatory | ||||||
著者所属(英) | ||||||
en | ||||||
German Aerospace Center (DLR) | ||||||
著者所属(英) | ||||||
en | ||||||
Netherlands Institute for Space Research (SRON) | ||||||
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. 389-391, 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 | About 400 hours of the Herschel Space Observatory’s time has been used by the Open Time Key Programme “TNOs are Cool: A survey of the trans-Neptunian region” to obtain PACS (70, 100 and 160 μm) and SPIRE (250, 350 and 500 μm) photometry of 132 objects representing different dynamical classes (resonant, classical, scattered disk and detached TNOs as well as Centaurs), including 25 binary systems. As leftovers of the formation of the Solar System TNOs and their physical properties provide constraints to the models of formation and evolution of the various dynamical classes. SPICA is going to be a main leap forward on the way that Herschel started in the characterization of TNOs by determining size, albedo and other surface properties. SPICA is going to cover the mid- to far-IR wavelengths where TNO SEDs peaks (currently covered with Herschel/PACS and Spitzer/MIPS together). While Herschel could observe about 10% of the known TNOs, with its increased sensitivity SPICA would be able to detect most (probably all) currently known TNOs. The observing strategy we used in our key program will also be relevant for SPICA observations to beat the confusion noise. | |||||
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: AA1730027086 | |||||
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 |