# Transiting exoplanets from the CoRoT space mission - X. CoRoT-10b: a giant planet in a 13.24 day eccentric orbit

@article{Bonomo2010TransitingEF,
title={Transiting exoplanets from the CoRoT space mission - X. CoRoT-10b: a giant planet in a 13.24 day eccentric orbit},
author={Aldo Stefano Bonomo and Alexandre Santerne and Roi Alonso and J. C. Gazzano and Mathieu Havel and Suzanne Aigrain and Michel Auvergne and Annie Baglin and Mauro Barbieri and Pierre Barge and W. Benz and P. Bord'e and François Bouchy and Hans Bruntt and Juan Cabrera and Andrew Collier Cameron and Ludmila Carone and Stefania Carpano and Sz. Csizmadia and Magali Deleuil and Hans J. Deeg and Rudolf Dvorak and Anders Erikson and Sylvio Ferraz-Mello and Malcolm Fridlund and Davide Gandolfi and Micha{\"e}l Gillon and E. W. Guenther and Tristan Guillot and A. P. Hatzes and Guillaume H'ebrard and Laurent Jorda and Helmut Lammer and Antonino Francesco Lanza and Alain L'eger and Antoine Llebaria and Michel Mayor and Tsevi Mazeh and Claire Moutou and Marc Ollivier and Martin Patzold and Francesco A. Pepe and Didier Queloz and Heike Rauer and Daniel Rouan and Benjamin Samuel and Jodi Schneider and Brandon Tingley and St{\'e}phane Udry and G{\"u}nther Wuchterl},
journal={Astronomy and Astrophysics},
year={2010},
volume={520},
pages={65}
}
• Published 15 June 2010
• Physics, Geology
• Astronomy and Astrophysics
Context. The space telescope CoRoT searches for transiting extrasolar planets by continuously monitoring the optical flux of thousands of stars in several fields of view. Aims. We report the discovery of CoRoT-10b, a giant planet on a highly eccentric orbit (e = 0.53 ± 0.04) revolving in 13.24 days around a faint (V = 15.22) metal-rich K1V star. Methods. We used CoRoT photometry, radial velocity observations taken with the HARPS spectrograph, and UVES spectra of the parent star to derive the…

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