Studies of Expolanets and Solar Systems with SPICA

(10) Rutherford Appleton Laboratory); (2) National Astronomical Observatory of Japan; (3) Japan Aerospace Exploration Agency; (4) Osaka University; (5) Kanagawa University; (6) Ibaraki University; (7) University of Tokyo; (8) Centro de Astrobiologia (CSIC-INTA); (9) Cardiff University; Academia Sinica

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Studies of Expolanets and Solar Systems with SPICA

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arxiv 0911.3974 v1 pith:JOCO4GEL submitted 2009-11-20 astro-ph.IM astro-ph.EP

Studies of Expolanets and Solar Systems with SPICA

Michihiro Takami (1) , Motohide Tamura (2) , Keigo Enya (3) , Takafumi Ootsubo (3) , Misato Fukagawa (4) , Mitsuhiko Honda (5) , Yoshiko Okamoto (6) , Shigehisa Sako (7)

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Takuya Yamashita (2) Sunao Hasegawa (3) Hirokazu Kataza (3) Hideo Matsuhara (3) Takao Nakagawa (3) Javier R. Goicoechea (8) Kate Isaak (9) Bruce Swinyard (10) ((1) Institute of Astronomy Astrophysics Academia Sinica (2) National Astronomical Observatory of Japan (3) Japan Aerospace Exploration Agency (4) Osaka University (5) Kanagawa University (6) Ibaraki University (7) University of Tokyo (8) Centro de Astrobiologia (CSIC-INTA) (9) Cardiff University (10) Rutherford Appleton Laboratory)

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keywords infraredinstrumentationproposedsolarspicastudiessuperiortelescope

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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.

Studies of Expolanets and Solar Systems with SPICA

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