AbstractThe SPace Infrared telescope for Cosmology and Astrophysics (SPICA) is a proposed mid-to-far infrared ( 4 200 μ m ) astronomy mission, scheduled for launch in 2017. A single, 3.5m aperture telescope would provide superior image quality at 5 200 μ m , and its very cold ( 5 K ) instrumentation would provide superior sensitivity in the 25–200 μ m 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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    Titel :

    Studies of expolanets and solar systems with SPICA


    Beteiligte:
    Takami, Michihiro (Autor:in) / Tamura, Motohide (Autor:in) / Enya, Keigo (Autor:in) / Ootsubo, Takafumi (Autor:in) / Fukagawa, Misato (Autor:in) / Honda, Mitsuhiko (Autor:in) / Okamoto, Yoshiko (Autor:in) / Sako, Shigehisa (Autor:in) / Yamashita, Takuya (Autor:in) / Hasegawa, Sunao (Autor:in)

    Erschienen in:

    Advances in Space Research ; 45 , 8 ; 1000-1006


    Erscheinungsdatum :

    2009-11-06


    Format / Umfang :

    7 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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    ESI: a proposed european instrument for SPICA

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