Observations of Exoplanets Transits in the Far Infrared with SPICA-SAFARI

Details Observations of Exoplanets Transits in the Far Infrared with SPICA-SAFARI Observations of Exoplanets Transits in the Far Infrared with SPICA-SAFARI

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sitc.conf.2007p&link_type=abstract

SPICA joint European/Japanese Workshop, held 6-8 July, 2009 at Oxford, United Kingdom. Edited by A.M. Heras, B.M. Swinyard, K.G

Physics

Stars: Planetary Systems, Missions: Spica, Techniques: Photometric

Scientific paper

When the disks of a star and of a planet overlap as a consequence of the orbital motion, the total light coming from the system dims. If an instrument is sensitive enough to detect this flux variation, important parameters of the planetary system can be derived from the observed light curve. In this paper I show under which conditions the transits can be detected given the sensitivity of SAFARI.

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