赤外線宇宙望遠鏡による系外惑星スペクトルの観測
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(120) . ῎῍῏ῌ 1) Mayor M., Queloz D., 1995, Nature 378, 355 2) Tinetti G., et al., 2007, Nature 448, 169 3) Swain M. R., Vasisht G., Tinetti G., 2008, Nature 452, 329 4) Kalas P., et al., 2008, Science 322, 1345 5) Nakagawa T., SPICA working group, 2008, Proc. of SPIEῌ7010, 70100H 6) Enya K., Tanaka S., Abe L., Nakagawa T., 2007, A&A 461, 783 7) ¡¢£ 2007, ¤¥ 100, 400. , -./(01 234 56 789:; < ()*+(=>7 #$?@AB
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(125) c:d e fgh:dijklmn3! o^p:;Z qr56 < C Cs ()*+(tu S d ' L 7 v s S 7 C Z COROT, KEPLAR 3 w x K y z { v 102 ». v3¼. Spectroscopy of Exo-planets with Space Infrared Telescopes Keigo ENYA and Takao NANAGAWA Department of Infrared Astrophysics, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3῍1῍1 Yoshinodai, Sagamihara, Kanagawa 229῍8510, Japan Abstract : Observational study of exo-planetary system is going to phase of systematic study, from phase of discovery. Spectroscopy of exo-planets with space infrared telescopes will be more important. Large space infrared telescopes, e.g., Space Infrared Telescope for Cosmology and Astrophysics (SPICA), are planed to be launched and used in the 2010s. It’s expected that such large space telescopes will provide information on spectrum of exo-planetary system via direct observation with coronagraph, transit monitoring, and so on.. 205.
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