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Studies of Expolanets and Solar Systems with SPICA

Authors :
Takami, Michihiro
Tamura, Motohide
Enya, Keigo
Ootsubo, Takafumi
Fukagawa, Misato
Honda, Mitsuhiko
Okamoto, Yoshiko
Sako, Shigehisa
Yamashita, Takuya
Hasegawa, Sunao
Kataza, Hirokazu
Matsuhara, Hideo
Nakagawa, Takao
Goicoechea, Javier R.
Isaak, Kate
Swinyard, Bruce
Publication Year :
2009

Abstract

The SPace Infrared telescope for Cosmology and Astrophysics (SPICA) is a proposed mid-to-far infrared (4-200 um) astronomy mission, scheduled for launch in 2017. A single, 3.5m aperture telescope would provide superior image quality at 5-200 um, and its very cold (~5 K) instrumentation would provide superior sensitivity in the 25-200 um wavelength regimes. This would provide a breakthrough opportunity for studies of exoplanets, protoplanetary and debris disk, and small solar system bodies. This paper summarizes the potential scientific impacts for the proposed instrumentation.<br />Comment: 17 pages, 4 figures, 1 table, accepted for Advances in Space Research (conference proceeding of 37th COSPAR Scientific Assembly)

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.0911.3974
Document Type :
Working Paper
Full Text :
https://doi.org/10.1016/j.asr.2009.11.006