CoRoT-14b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2010.[3]
Discovery | |
---|---|
Discovered by | CoRoT space telescope |
Transit | |
Orbital characteristics | |
0.027 AU (4,000,000 km)[1] | |
Eccentricity | 0 |
1.51214 d | |
Inclination | 79.6 |
Star | CoRoT-14 |
Physical characteristics | |
1.09 RJ | |
Mass | 7.6 MJ |
Temperature | 1781 K[2] |
![Exoplanet CoRoT-14 b size comparison to Jupiter. Jupiter is on the left and is around 7.6 times less massive than CoRoT-14 b, which is white in colour](http://up.wiki.x.io/wikipedia/commons/thumb/2/2a/Exoplanet_Comparison_CoRoT-14_b.png/220px-Exoplanet_Comparison_CoRoT-14_b.png)
Host star
editCoRoT-14b orbits CoRoT-14 in the constellation of Monoceros. It is an F9V star with an effective temperature of 6,035 K (5,762 °C; 10,403 °F), a mass of 1.13 M☉, a radius of 1.21 R☉, and a near-solar metallicity. It has an estimated age between 0.4 and 8.0 Gyr.[3]
Characteristics
editThe planet is unusually dense (7.3 g/cm3) for its mass and distance from host star, making CoRoT-14b one of the densest gas giants known.[3]
References
edit- ^ "Notes on CoRoT-14 b". Extrasolar Planets Encyclopaedia. Retrieved February 25, 2019.
- ^ "COROT-14 Planets in the system". Retrieved February 25, 2019.
- ^ a b c Tingley, B.; Endl, M.; Gazzano, J. -C.; Alonso, R.; Mazeh, T.; Jorda, L.; Aigrain, S.; Almenara, J. -M.; Auvergne, M.; Baglin, A.; Barge, P.; Bonomo, A. S.; Bordé, P.; Bouchy, F.; Bruntt, H.; Cabrera, J.; Carpano, S.; Carone, L.; Cochran, W. D.; Csizmadia, Sz.; Deleuil, M.; Deeg, H. J.; Dvorak, R.; Erikson, A.; Ferraz-Mello, S.; Fridlund, M.; Gandolfi, D.; Gillon, M.; Guenther, E. W.; et al. (April 2011). "Transiting exoplanets from the CoRoT space mission: XIII. CoRoT-14b: an unusually dense very hot Jupiter". Astronomy & Astrophysics. 528 (A97). arXiv:1101.1899. doi:10.1051/0004-6361/201015480. S2CID 56139010.
See also
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