Issue |
A&A
Volume 528, April 2011
|
|
---|---|---|
Article Number | A97 | |
Number of page(s) | 7 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201015480 | |
Published online | 08 March 2011 |
Transiting exoplanets from the CoRoT space mission⋆
XVI. CoRoT-14b: an unusually dense very hot Jupiter
1
Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain
e-mail: btingley@iac.es
2
Dpto. de Astrofísica, Universidad de La Laguna,
38206 La Laguna, Tenerife, Spain
3
McDonald Observatory, University of Texas at Austin,
Austin, 78712
TX,
USA
4
Laboratoire d’Astrophysique de Marseille,
38 rue Frédéric Joliot-Curie,
13388
Marseille Cedex 13,
France
5
Observatoire de l’Université de Genève,
51 chemin des Maillettes,
1290
Sauverny,
Switzerland
6
Wise Observatory, Tel Aviv University,
Tel Aviv
69978,
Israel
7
Department of Physics, Denys Wilkinson Building Keble Road,
Oxford, OX1 3RH, UK
8
LESIA, UMR 8109 CNRS, Observatoire de Paris, UPMC, Université
Paris-Diderot, 5 place J.
Janssen, 92195
Meudon,
France
9
Institut d’Astrophysique Spatiale, Université Paris-Sud 11
& CNRS (UMR 8617), Bât.
121, 91405
Orsay,
France
10
Observatoire de Haute Provence, 04670 Saint Michel l’Observatoire,
France
11
Institut d’Astrophysique de Paris, 98bis boulevard Arago, 75014
Paris,
France
12
University of Vienna, Institute of Astronomy,
Türkenschanzstr. 17,
1180
Vienna,
Austria
13
Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2,
12489
Berlin,
Germany
14
IAG, Universidade de Sao Paulo,
Brazil
15
Research and Scientific Support Department,
ESTEC/ESA, PO Box 299,
2200 AG
Noordwijk, The
Netherlands
16
University of Liège, Allée du 6 août 17, Sart Tilman, Liège 1, Belgium
17
Thüringer Landessternwarte, Sternwarte 5, Tautenburg
5, 07778
Tautenburg,
Germany
18
Space Research Institute, Austrian Academy of
Science, Schmiedlstr.
6, 8042
Graz,
Austria
19
School of Physics and Astronomy, Raymond and Beverly Sackler
Faculty of Exact Sciences, Tel Aviv University, Tel Aviv, Israel
20
Rheinisches Institut für Umweltforschung an der Universität zu
Köln, Aachener Strasse
209, 50931,
Germany
21
Observatoire de la Côte d’Azur, Laboratoire
Cassiopée, BP
4229, 06304
Nice Cedex 4,
France
22
LUTH, Observatoire de Paris, CNRS, Université Paris
Diderot, 5 place Jules
Janssen, 92195
Meudon,
France
23
Center for Astronomy and Astrophysics, TU Berlin, Hardenbergstr.
36, 10623
Berlin,
Germany
24
School of Physics, University of Exeter,
Stocker Road, Exeter
EX4 4QL,
UK
25
Laboratoire d’Astronomie de Lille, Université de Lille 1, 1
impasse de l’Observatoire, 59000
Lille,
France
26
Institut de Mécanique Céleste et de Calcul des Ephémérides, UMR
8028 du CNRS, 77 Ave.
Denfert-Rochereau, 75014
Paris,
France
Received:
27
July
2010
Accepted:
13
December
2010
In this paper, the CoRoT ExoplanetScience 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.
Key words: planetary systems / techniques: photometric / techniques: radial velocities / techniques: spectroscopic
© ESO, 2011
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