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Auvergne, M. Deleuil, M. Endl, M. Fridlund, M. Gillon, M. Havel, M. Ollivier, M. Paetzold, P. Barge, P. Borde, P. J. MacQueen, R. Alonso, R. Dvorak, R. F. Diaz, R. Titz-Weider, S. Aigrain, S. Carpano, S. Ferraz-Mello, Sz. Csizmadia, T. Guillot, Th. Fruth, T. Mazeh, W. Cochran","submitted_at":"2011-06-22T08:44:05Z","abstract_excerpt":"We report on the discovery of a hot Jupiter-type exoplanet, CoRoT-17b, detected by the CoRoT satellite. It has a mass of $2.43\\pm0.30$\\Mjup and a radius of $1.02\\pm0.07$\\Rjup, while its mean density is $2.82\\pm0.38$ g/cm$^3$. CoRoT-17b is in a circular orbit with a period of $3.7681\\pm0.0003$ days. The host star is an old ($10.7\\pm1.0$ Gyr) main-sequence star, which makes it an intriguing object for planetary evolution studies. 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