CoRoT-14b: Difference between revisions

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| perihelion =
| perihelion =
| semimajor = {{convert|0.027|AU|km|abbr=on}}<ref name=EU>{{cite web
| semimajor = {{convert|0.027|AU|km|abbr=on}}<ref name=EU>{{cite web
|url=http://exoplanet.eu/catalog/corot-14_b/
|url=https://exoplanet.eu/catalog/corot_14_b--652/
|work=[[Extrasolar Planets Encyclopaedia]]
|title=Notes on CoRoT-14 b
|title=Notes on CoRoT-14 b
|accessdate=February 25, 2019}}</ref>
|access-date=February 25, 2019}}</ref>
| mean_orbit_radius =
| mean_orbit_radius =
| eccentricity = 0
| eccentricity = 0
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CoRoT-14b orbits CoRoT-14 in the constellation of [[Monoceros]]. It is a F9V star with T<sub>e</sub> = 6035K, M = 1.13[[Solar mass|M<sub>☉</sub>]], R = 1.21[[Solar radius|R<sub>☉</sub>]], and near-solar metallicity. It has an estimated age between 0.4 and 8.0 Gyr.{{cn|date=May 2021}}
CoRoT-14b orbits CoRoT-14 in the constellation of [[Monoceros]]. It is a F9V star with T<sub>e</sub> = 6035K, M = 1.13[[Solar mass|M<sub>☉</sub>]], R = 1.21[[Solar radius|R<sub>☉</sub>]], and near-solar metallicity. It has an estimated age between 0.4 and 8.0 Gyr.{{cn|date=May 2021}}
==Characteristics==
==Characteristics==
The planet is unusually dense (7.3 g/cm<sup>3</sup>) for its mass and distance from host star, making CoRoT-14b one of the most dense gas giants known.<ref>{{cite journal
The planet is unusually dense (7.3 g/cm<sup>3</sup>) for its mass and distance from host star, making CoRoT-14b one of the densest gas giants known.<ref>{{cite journal
|title=Transiting exoplanets from the CoRoT space mission⋆ XIII. CoRoT-14b: an unusually dense very hot Jupiter
|title=Transiting exoplanets from the CoRoT space mission: XIII. CoRoT-14b: an unusually dense very hot Jupiter
|journal=[[Astronomy & Astrophysics]]
|volume=528
|number=A97
|doi=10.1051/0004-6361/201015480
|doi=10.1051/0004-6361/201015480
|arxiv=1101.1899
|arxiv=1101.1899
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|last30=Guillot
|last30=Guillot
|first30=T.
|first30=T.
|year=2011
|date=April 2011
|s2cid=56139010
|s2cid=56139010
|display-authors=29
|display-authors=29

Latest revision as of 08:35, 12 May 2024

CoRoT-14b
Discovery
Discovered byCoRoT space telescope
Transit
Orbital characteristics
0.027 AU (4,000,000 km)[1]
Eccentricity0
1.51214 d
Inclination79.6
StarCoRoT-14 [ru]
Physical characteristics
Mean radius
1.09 RJ
Mass7.6MJ
Temperature1781 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
Exoplanet CoRoT-14 b size comparison to Jupiter

CoRoT-14b is a transiting Hot Jupiter exoplanet found by the CoRoT space telescope in 2010.[citation needed]

Host star[edit]

CoRoT-14b orbits CoRoT-14 in the constellation of Monoceros. It is a F9V star with Te = 6035K, M = 1.13M, R = 1.21R, and near-solar metallicity. It has an estimated age between 0.4 and 8.0 Gyr.[citation needed]

Characteristics[edit]

The 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]

  1. ^ "Notes on CoRoT-14 b". Extrasolar Planets Encyclopaedia. Retrieved February 25, 2019.
  2. ^ "COROT-14 Planets in the system". Retrieved February 25, 2019.
  3. ^ 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[edit]