Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan
Centro de Astrobiologia, CSIC-INTA, Spain
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)
著者所属（英）
Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan
Centro de Astrobiologia, CSIC-INTA, Spain
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
出版者
宇宙航空研究開発機構(JAXA)
出版者（英）
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料
雑誌名(英)
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
ページ
299 - 305
発行年
2018-03-09
会議概要（会議名, 開催地, 会期, 主催者等）（英）
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）
SPICA will be a powerful facility to help us understand the formation and evolution of our solar system and exoplanetary systems in 2020's. The wavelength coverage (5-210 micrometers) is optimal for observations of key targets including exoplanets, protoplanetary and debris disks, and solar system small bodies. At this coverage SPICA will offer several dramatic advantages, including extremely high sensitivity and excellent image quality with a cooled (approximately 6 K) monolithic 3-m class mirror telescope, a variety of capabilities for spectroscopy and spectro-imaging, and an unprecedented high spectral resolution for mid-infrared spectroscopy free from telluric absorption and emission. We briefly summarize our discussions for possible science impacts on the above targets and research topics.
内容記述
形態: カラー図版あり
内容記述（英）
Physical characteristics: Original contains color illustrations
Studies of Exoplanets and Solar Systems with SPICA: An Overview
AA1730027065.pdf
(4.08MB)
