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24 April 2024
 
  » arxiv » 1001.1426

 Article overview


Transiting exoplanets from the CoRoT space mission IX. CoRoT-6b: a transiting 'hot Jupiter' planet in an 8.9d orbit around a low-metallicity star
M. Fridlund ; G. Hebrard ; R. Alonso ; M. Deleuil ; D. Gandolfi ; M. Gillon ; H. Bruntt ; A. Alapini ; Sz. Csizmadia ; T. Guillot ; H. Lammer ; S. Aigrain ; J.M. Almenara ; M. Auvergne ; A. Baglin ; P. Barge ; P. Borde ; F. Bouchy ; J. Cabrera ; L. Carone ; S. Carpano ; H. J. Deeg ; R. De la Reza ; R. Dvorak ; A. Erikson ; S. Ferraz-Mello ; E. Guenther ; P. Gondoin ; R. den Hartog ; A. Hatzes ; L. Jorda ; A. Leger ; A. Llebaria ; P. Magain ; T. Mazeh ; C. Moutou ; M. Ollivier ; M. Patzold ; D. Queloz ; H. Rauer ; D. Rouan ; B. Samuel ; J. Schneider ; A. Shporer ; B. Stecklum ; B. Tingley ; J. Weingrill ; G. Wuchterl ;
Date 9 Jan 2010
AbstractThe CoRoT satellite exoplanetary team announces its sixth transiting planet in this paper. We describe and discuss the satellite observations as well as the complementary ground-based observations - photometric and spectroscopic - carried out to assess the planetary nature of the object and determine its specific physical parameters. The discovery reported here is a ’hot Jupiter’ planet in an 8.9d orbit, 18 stellar radii, or 0.08 AU, away from its primary star, which is a solar-type star (F9V) with an estimated age of 3.0 Gyr. The planet mass is close to 3 times that of Jupiter. The star has a metallicity of 0.2 dex lower than the Sun, and a relatively high $^7$Li abundance. While thelightcurveindicatesamuchhigherlevelof activity than, e.g., the Sun, there is no sign of activity spectroscopically in e.g., the [Ca ] H&K lines.
Source arXiv, 1001.1426
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