CoRoT-14b: Difference between revisions

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{{Infobox planet
{{Infobox planet
| name = COROT-14b
| name = CoRoT-14b
| symbol =
| symbol =
| image =
| image =
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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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| satellite_of =
| satellite_of =
| satellites =
| satellites =
| star = {{ill|COROT-14|ru}}
| star = {{ill|CoRoT-14|ru}}
| allsatellites =
| allsatellites =
| tisserand =
| tisserand =
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| note =
| note =
}}
}}
[[File:Exoplanet_Comparison_CoRoT-14_b.png|thumb|right|alt=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 [[Extrasolar planet|exoplanet]] found by the [[CoRoT]] space telescope on 2010.
'''CoRoT-14b''' is a transiting [[Hot Jupiter]] [[exoplanet]] found by the [[CoRoT]] [[space telescope]] in 2010.{{cn|date=May 2021}}


==Host star==
It is an hot [[Jupiter]]-sized planet orbiting 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.
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==
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 web
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
|url=https://arxiv.org/pdf/1101.1899.pdf
|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]]
|accessdate=February 25, 2019}}</ref>
|volume=528
|number=A97
|doi=10.1051/0004-6361/201015480
|arxiv=1101.1899
|last1=Tingley
|first1=B.
|last2=Endl
|first2=M.
|last3=Gazzano
|first3=J. -C.
|last4=Alonso
|first4=R.
|last5=Mazeh
|first5=T.
|last6=Jorda
|first6=L.
|last7=Aigrain
|first7=S.
|last8=Almenara
|first8=J. -M.
|last9=Auvergne
|first9=M.
|last10=Baglin
|first10=A.
|last11=Barge
|first11=P.
|last12=Bonomo
|first12=A. S.
|last13=Bordé
|first13=P.
|last14=Bouchy
|first14=F.
|last15=Bruntt
|first15=H.
|last16=Cabrera
|first16=J.
|last17=Carpano
|first17=S.
|last18=Carone
|first18=L.
|last19=Cochran
|first19=W. D.
|last20=Csizmadia
|first20=Sz.
|last21=Deleuil
|first21=M.
|last22=Deeg
|first22=H. J.
|last23=Dvorak
|first23=R.
|last24=Erikson
|first24=A.
|last25=Ferraz-Mello
|first25=S.
|last26=Fridlund
|first26=M.
|last27=Gandolfi
|first27=D.
|last28=Gillon
|first28=M.
|last29=Guenther
|first29=E. W.
|last30=Guillot
|first30=T.
|date=April 2011
|s2cid=56139010
|display-authors=29
}}</ref>


==References==
==References==
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==See also==
==See also==
*[[WASP-18b]]
*[[WASP-18b]]
*[[COROT-20b]]
*[[CoRoT-20b]]
{{Stars of Monoceros}}

[[Category:Hot Jupiters]]
[[Category:Hot Jupiters]]
[[Category:Transiting exoplanets]]
[[Category:Transiting exoplanets]]
[[Category:Exoplanets discovered in 2010]]
[[Category:Exoplanets discovered in 2010]]
[[Category:Exoplanets discovered by the COROT program|14b]]
[[Category:Exoplanets discovered by CoRoT|14b]]


{{exoplanet-stub}}

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]


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