Transiting exoplanets from the CoRoT space mission. XXII. CoRoT-16b: a hot Jupiter with a hint of eccentricity around a faint solar-like star

M. OLLIVIER; M. GILLON; A. SANTERNE; G. WUCHTERL; M. HAVEL; H. BRUNNTT; P. BORDÉ; T. PASTERNACKI; M. ENDL; D. GANDOLFI; S. AIGRAIN; J. M. ALMENARA; R. ALONSO; M. AUVERGNE; A. BAGLIN; P. BARGE; A. S. BONOMO; F. BOUCHY; J. CABRERA; L. CARONE; S. CARPANO; C. CAVARROC; W. D. COCHRAN; SZ. CSIZMADIA; H. J. DEEG; M. DELEUIL; R. F. DÍAZ; AND 29 COAUTHORS

ASTRONOMY AND ASTROPHYSICS

EDP SCIENCES S A

Lugar: Paris; Año: 2012 vol. 541 p. 1 - 10

0004-6361

Aims: We report the discovery of CoRoT-16b, a low density hot jupiter that orbits a faint G5V star (mV = 15.63) in 5.3523 ± 0.0002 days with slight eccentricity. A fit of the data with no a priori assumptions on the orbit leads to an eccentricity of 0.33 ± 0.1. We discuss this value and also derive the mass and radius of the planet. Methods: We analyse the photometric transit curve of CoRoT-16 given by the CoRoT satellite, and radial velocity data from the HARPS and HIRES spectrometers. A combined analysis using a Markov chain Monte Carlo algorithm is used to get the system parameters. Results: CoRoT-16b is a 0.535 -0.083/+0.085 MJ, 1.17 -0.14/+0.16 RJ hot Jupiter with a density of 0.44 -0.14/+0.21 g cm-3. Despite its short orbital distance (0.0618 ± 0.0015 AU) and the age of the parent star (6.73 ± 2.8 Gyr), the planet orbit exhibits significantly non-zero eccentricity. This is very uncommon for this type of objects as tidal effects tend to circularise the orbit. This value is discussed taking into account the characteristics of the star and the observation accuracy.