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arXiv · 0911.3974

Studies of Expolanets and Solar Systems with SPICA

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

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Michihiro Takami, Motohide Tamura, Keigo Enya, Takafumi Ootsubo, Misato Fukagawa, Mitsuhiko Honda, Yoshiko Okamoto, Shigehisa Sako, Takuya Yamashita, Sunao Hasegawa, Hirokazu Kataza, Hideo Matsuhara, Takao Nakagawa, Javier R. Goicoechea, Kate Isaak, Bruce Swinyard. 2009-11-20. Studies of Expolanets and Solar Systems with SPICA. https://doi.org/10.1016/j.asr.2009.11.006

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