Journal
ASTRONOMY & ASTROPHYSICS
Volume 528, Issue -, Pages -Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201015480
Keywords
planetary systems; techniques: photometric; techniques: radial velocities; techniques: spectroscopic
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Funding
- Spanish Ministerio de Ciencia e Inovacion [ESP2007-65480-C02-02]
- Belgian Science Policy Office
- W. M. Keck Foundation
- NASA
- UK Space Agency [ST/G002266/2] Funding Source: researchfish
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In this paper, the CoRoT Exoplanet Science Team announces its 14th discovery. Herein, we discuss the observations and analyses that allowed us to derive the parameters of this system: a hot Jupiter with a mass of 7.6 +/- 0.6 Jupiter masses orbiting a solar-type star (F9V) with a period of only 1.5 d, less than 5 stellar radii from its parent star. It is unusual for such a massive planet to have such a small orbit: only one other known higher mass exoplanet orbits with a shorter period.
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