CoRoT-20b: Difference between revisions
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{{Short description|Exoplanet}} |
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{{Infobox planet |
{{Infobox planet |
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| name = |
| name = CoRoT-20b |
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| symbol = |
| symbol = |
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| image = |
| image = |
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| perihelion = |
| perihelion = |
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| semimajor = {{convert|0.0902|AU|km|abbr=on}}<ref name=EU>{{cite web |
| semimajor = {{convert|0.0902|AU|km|abbr=on}}<ref name=EU>{{cite web |
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|url= |
|url=https://exoplanet.eu/catalog/corot_20_b--826/ |
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|work=[[Extrasolar Planets Encyclopaedia]] |
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|title=Notes on CoRoT-20 b |
|title=Notes on CoRoT-20 b |
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| |
|access-date=February 25, 2019}}</ref> |
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| mean_orbit_radius = |
| mean_orbit_radius = |
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| eccentricity = 0.562 |
| eccentricity = 0.562 |
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| satellite_of = |
| satellite_of = |
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| satellites = |
| satellites = |
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| star = {{ill| |
| star = {{ill|CoRoT-20|ru}} |
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| allsatellites = |
| allsatellites = |
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| tisserand = |
| tisserand = |
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| note = |
| note = |
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}} |
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'''CoRoT-20b''' is a transiting [[Extrasolar planet|exoplanet]] found by the [[CoRoT]] space telescope |
'''CoRoT-20b''' is a transiting [[Extrasolar planet|exoplanet]] found by the [[CoRoT]] [[space telescope]] in 2011. |
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It is a hot [[Jupiter]]-sized planet orbiting |
It is a hot [[Jupiter]]-sized planet orbiting CoRoT-20. It is a young planet, with an estimated age between 0.06 and 0.14 Gyr. Its density (8.87 g/cm<sup>3</sup>) is remarkably high for its mass, making CoRoT-20b one of the most compact gas giants.<ref>{{cite journal |
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|url=https://arxiv.org/pdf/1109.3203.pdf |
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|title=Transiting exoplanets from the CoRoT space mission⋆ XX. CoRoT-20b: A very high density, high eccentricity transiting giant planet |
|title=Transiting exoplanets from the CoRoT space mission⋆ XX. CoRoT-20b: A very high density, high eccentricity transiting giant planet |
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|doi=10.1051/0004-6361/201117681 |
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|accessdate=February 25, 2019}}</ref> |
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|arxiv=1109.3203 |
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|last1=Deleuil |
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|first1=M. |
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|last2=Bonomo |
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|first2=A. S. |
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|last3=Ferraz-Mello |
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|first3=S. |
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|last4=Erikson |
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|first4=A. |
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|last5=Bouchy |
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|first5=F. |
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|last6=Havel |
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|first6=M. |
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|last7=Aigrain |
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|first7=S. |
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|last8=Almenara |
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|first8=J. -M. |
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|last9=Alonso |
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|first9=R. |
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|last10=Auvergne |
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|first10=M. |
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|last11=Baglin |
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|first11=A. |
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|last12=Barge |
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|first12=P. |
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|last13=Bordé |
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|first13=P. |
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|last14=Bruntt |
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|first14=H. |
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|last15=Cabrera |
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|first15=J. |
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|last16=Carpano |
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|first16=S. |
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|last17=Cavarroc |
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|first17=C. |
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|last18=Csizmadia |
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|first18=Sz. |
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|last19=Damiani |
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|first19=C. |
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|last20=Deeg |
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|first20=H. J. |
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|last21=Dvorak |
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|first21=R. |
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|last22=Fridlund |
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|first22=M. |
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|last23=Hébrard |
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|first23=G. |
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|last24=Gandolfi |
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|first24=D. |
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|last25=Gillon |
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|first25=M. |
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|last26=Guenther |
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|first26=E. |
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|last27=Guillot |
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|first27=T. |
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|last28=Hatzes |
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|first28=A. |
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|last29=Jorda |
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|first29=L. |
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|last30=Léger |
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|first30=A. |
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|year=2011 |
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|s2cid=118339296 |
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|display-authors=29 |
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}}</ref> |
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==Host star== |
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The host star, CoRoT-20 is a G2V star with T<sub>e</sub> = 5880K, M = 1.14[[Solar mass|M<sub>☉</sub>]], R = 0.92[[Solar radius|R<sub>☉</sub>]], and it is above-solar metallicity. It also hosts another exoplanet, [[CoRoT-20c]]. |
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==See also== |
==See also== |
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*[[ |
*[[CoRoT-14b]] |
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*[[COROT-14b]] |
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*[[WASP-18b]] |
*[[WASP-18b]] |
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==References== |
==References== |
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{{Reflist}} |
{{Reflist}}{{Stars of Monoceros}}{{Exoplanet-stub}} |
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[[Category:Hot Jupiters]] |
[[Category:Hot Jupiters]] |
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[[Category:Transiting exoplanets]] |
[[Category:Transiting exoplanets]] |
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[[Category:Exoplanets discovered in 2011]] |
[[Category:Exoplanets discovered in 2011]] |
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[[Category:Exoplanets discovered by |
[[Category:Exoplanets discovered by CoRoT|20b]] |
Revision as of 20:07, 20 January 2024
Discovery | |
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Discovered by | CoRoT space telescope |
Transit | |
Orbital characteristics | |
0.0902 AU (13,490,000 km)[1] | |
Eccentricity | 0.562 |
9.24285 d | |
Inclination | 88.21 |
Star | CoRoT-20 |
Physical characteristics | |
Mean radius | 0.84 RJ |
Mass | 4.24MJ |
Temperature | 1002 K[2] |
CoRoT-20b is a transiting exoplanet found by the CoRoT space telescope in 2011.
It is a hot Jupiter-sized planet orbiting CoRoT-20. It is a young planet, with an estimated age between 0.06 and 0.14 Gyr. Its density (8.87 g/cm3) is remarkably high for its mass, making CoRoT-20b one of the most compact gas giants.[3]
Host star
The host star, CoRoT-20 is a G2V star with Te = 5880K, M = 1.14M☉, R = 0.92R☉, and it is above-solar metallicity. It also hosts another exoplanet, CoRoT-20c.
See also
References
- ^ "Notes on CoRoT-20 b". Extrasolar Planets Encyclopaedia. Retrieved February 25, 2019.
- ^ "COROT-20 Planets in the system". Retrieved February 25, 2019.
- ^ Deleuil, M.; Bonomo, A. S.; Ferraz-Mello, S.; Erikson, A.; Bouchy, F.; Havel, M.; Aigrain, S.; Almenara, J. -M.; Alonso, R.; Auvergne, M.; Baglin, A.; Barge, P.; Bordé, P.; Bruntt, H.; Cabrera, J.; Carpano, S.; Cavarroc, C.; Csizmadia, Sz.; Damiani, C.; Deeg, H. J.; Dvorak, R.; Fridlund, M.; Hébrard, G.; Gandolfi, D.; Gillon, M.; Guenther, E.; Guillot, T.; Hatzes, A.; Jorda, L.; et al. (2011). "Transiting exoplanets from the CoRoT space mission⋆ XX. CoRoT-20b: A very high density, high eccentricity transiting giant planet". arXiv:1109.3203. doi:10.1051/0004-6361/201117681. S2CID 118339296.
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