View source for CoRoT-11b

{{Infobox planet
| name                     = COROT-11b
| symbol                   = 
| image                    = 
| image_size               = 
| image_alt                = 
| caption                  = 
| background               = 
| bgcolour                 = 
| label_width              = 
<!-- DISCOVERY           -->
| discoverer               = [[CoRoT]] space telescope
| discovery_site           = 
| discovered               = 
| discovery_method         = Transit
| discovery_ref            =
<!-- DESIGNATIONS        -->
| exosolar planets         = 
| minorplanet              = 
| extrasolarplanet         =  
| mpc_name                 =
| pronounced               =  
| named_after              = 
| alt_names                = 
| mp_category              = 
| adjectives               = 
<!-- ORBITAL             --> 
| orbit_ref                = 
| orbit_diagram            = 
| epoch                    = 
| uncertainty              = 
| observation_arc          = 
| earliest_precovery_date  = 
| apsis                    = astron
| aphelion                 = 
| perihelion               = 
| semimajor                = {{convert|0.04351|AU|km|abbr=on}}<ref name=EU>{{cite web
 |url=https://exoplanet.eu/catalog/corot_11_b--645/
 |work=[[Extrasolar Planets Encyclopaedia]]
 |title=Notes on CoRoT-11 b
 |access-date=February 25, 2019}}</ref>
| mean_orbit_radius        = 
| eccentricity             = 0
| period                   = {{val|2.99427803|(49)|ul=days}}<ref name="Kokori2023"/>
| synodic_period           = 
| avg_speed                = 
| mean_anomaly             = 
| mean_motion              = 
| inclination              = 81.41
| angular_dist             = 
| asc_node                 = 
| long_periastron          = 
| time_periastron          = 
| arg_peri                 = 
| semi-amplitude           = 
| satellite_of             = 
| satellites               = 
| star                     = CoRoT-11
| allsatellites            = 
| tisserand                = 
<!-- PHYS CHARS          --> 
| physical_ref             =
| dimensions               = 
| mean_diameter            = 
| mean_radius              = 1.43 {{Jupiter radius|link=y}}
| equatorial_radius        = 
| polar_radius             = 
| flattening               = 
| circumference            = 
| surface_area             = 
| volume                   = 
| mass                     = 2.33 {{Jupiter mass|link=y}}
| density                  = 
| surface_grav             = 
| moment_of_inertia_factor = 
| escape_velocity          = 
| rotation                 = 
| sidereal_day             = 
| rot_velocity             = 
| axial_tilt               = 
| right_asc_north_pole     = 
| declination              = 
| pole_ecliptic_lat        = 
| pole_ecliptic_lon        = 
| albedo                   = 
| single_temperature       = 1593 K<ref>{{cite web
 |url=http://www.openexoplanetcatalogue.com/planet/CoRoT-11%20b/
 |title=COROT-11 Planets in the system
 |accessdate=February 25, 2019}}</ref>
| spectral_type            = 
| magnitude                = 
| abs_magnitude            = 
| angular_size             = 
| family                   =
<!-- ATMOSPHERE          --> 
| atmosphere_ref           =  
| atmosphere               = 
| scale_height             = 
| surface_pressure         = 
| atmosphere_composition   = 
<!-- NOTES               --> 
| note                     =
}}
[[File:Exoplanet_Comparison_CoRoT-11_b.png|thumb|right|alt=Comparison of best-fit size of the exoplanet CoRoT-11 b with the Solar System planet Jupiter|CoRoT-11 b beside Jupiter]]
'''CoRoT-11b''' is a transiting [[Hot Jupiter]]-sized [[exoplanet]] found by the [[CoRoT]] [[space telescope]] in 2010.<ref name="Gandolfi2010"/> From obtained light curves and [[Bayesian inference]] on the data, it is highly likely that CoRoT-11b has been observed in a secondary eclipse around its host star ([[Astronomical transit|transiting behind]] it). <ref>https://www.aanda.org/articles/aa/full_html/2013/02/aa20081-12/aa20081-12.html</ref>

==Host star==
CoRoT-11b orbits the star CoRoT-11 in the constellation of [[Serpens (constellation)|Serpens]]. It is a [[F-type main sequence star|F6V star]] with an [[effective temperature]] of {{val|6440|120}} [[Kelvin (unit)|K]], a mass of {{val|1.270|0.050}} {{Solar mass|link=y}}, a radius of {{val|1.370|0.030}} {{Solar radius|link=y}}, and a near-solar [[metallicity]] of {{val|−0.03| 0.08}} dex.{{efn|name=n1}} It has an estimated age of {{val|2.0|1.0}} [[billion years|Gyr]].<ref name="Bonomo2017"/>

==References==
{{Reflist|refs=

<ref name="Gandolfi2010">{{cite journal | title=Transiting exoplanets from the CoRoT space mission. XIV. CoRoT-11b: a transiting massive "hot-Jupiter" in a prograde orbit around a rapidly rotating F-type star | last1=Gandolfi | first1=D. | last2=Hébrard | first2=G. | last3=Alonso | first3=R. | last4=Deleuil | first4= M. | last5=Guenther | first5=E. W. | last6=Fridlund | first6=M. | last7=Endl | first7=M. | last8=Eigmüller | first8=P. | last9=Csizmadia | first9=Sz. | last10=Havel | first10=M. | last11=Aigrain | first11=S. | last12=Auvergne | first12=M. | last13=Baglin | first13=A. | last14=Barge | first14=P. | last15=Bonomo | first15=A. S. | last16=Bordé | first16=P. | last17=Bouchy | first17=F. | last18=Bruntt | first18=H. | last19=Cabrera | first19=J. | last20=Carpano | first20=S. | last21=Carone | first21=L. | last22=Cochran | first22=W. D. | last23=Deeg | first23=H. J. | last24=Dvorak | first24=R. | last25=Eislöffel | first25=J. | last26=Erikson | first26=A. | last27=Ferraz-Mello | first27=S. | last28=Gazzano | first28=J.-C. | last29=Gibson | first29=N. B. | last30=Gillon | first30=M. | display-authors=1 | journal=Astronomy and Astrophysics | date=23 November 2010 | volume=524 | page=<!-- to prevent citation bot adding nonexistent page number--> | article-number=A55 | bibcode=2010A&A...524A..55G | bibcode-access=free | doi=10.1051/0004-6361/201015132 | arxiv=1009.2597 | doi-access=free }}</ref>

<ref name="Kokori2023">{{cite journal | title=ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations | last1=Kokori | first1=A. | last2=Tsiaras | first2=A. | last3=Edwards | first3=B. | last4=Jones | first4=A. | last5=Pantelidou | first5=G. | last6=Tinetti | first6=G. | last7=Bewersdorff | first7=L. | last8=Iliadou | first8=A. | last9=Jongen | first9=Y. | last10=Lekkas | first10=G. | last11=Nastasi | first11=A. | last12=Poultourtzidis | first12=E. | last13=Sidiropoulos | first13=C. | last14=Walter | first14=F. | last15=Wünsche | first15=A. | last16=Abraham | first16=R. | last17=Agnihotri | first17=V. K. | last18=Albanesi | first18=R. | last19=Arce-Mansego | first19=E. | last20=Arnot | first20=D. | last21=Audejean | first21=M. | last22=Aumasson | first22=C. | last23=Bachschmidt | first23=M. | last24=Baj | first24=G. | last25=Barroy | first25=P. R. | last26=Belinski | first26=A. A. | last27=Bennett | first27=D. | last28=Benni | first28=P. | last29=Bernacki | first29=K. | last30=Betti | first30=L. | display-authors=1 | journal=The Astrophysical Journal Supplement Series | date=14 February 2023 | volume=265 | issue=1 | page=<!-- to prevent citation bot adding nonexistent page number--> | article-number=4 | bibcode=2023ApJS..265....4K | bibcode-access=free | doi=10.3847/1538-4365/ac9da4 | arxiv=2209.09673 | doi-access=free }} [https://vizier.cds.unistra.fr/viz-bin/VizieR-5?-out.add=.&-source=J/ApJS/265/4/table7&recno=2 Vizier catalog entry ]</ref>

<ref name="Bonomo2017">{{cite journal | display-authors=1 | last=Bonomo | first=A. S. | last2=Desidera | first2=S. | last3=Benatti | first3=S. | last4=Borsa | first4=F. | last5=Crespi | first5=S. | last6=Damasso | first6=M. | last7=Lanza | first7=A. F. | last8=Sozzetti | first8=A. | last9=Lodato | first9=G. | last10=Marzari | first10=F. | last11=Boccato | first11=C. | last12=Claudi | first12=R. U. | last13=Cosentino | first13=R. | last14=Covino | first14=E. | last15=Gratton | first15=R. | last16=Maggio | first16=A. | last17=Micela | first17=G. | last18=Molinari | first18=E. | last19=Pagano | first19=I. | last20=Piotto | first20=G. | last21=Poretti | first21=E. | last22=Smareglia | first22=R. | last23=Affer | first23=L. | last24=Biazzo | first24=K. | last25=Bignamini | first25=A. | last26=Esposito | first26=M. | last27=Giacobbe | first27=P. | last28=Hébrard | first28=G. | last29=Malavolta | first29=L. | last30=Maldonado | first30=J. | last31=Mancini | first31=L. | last32=Martinez Fiorenzano | first32=A. | last33=Masiero | first33=S. | last34=Nascimbeni | first34=V. | last35=Pedani | first35=M. | last36=Rainer | first36=M. | last37=Scandariato | first37=G. | title=The GAPS Programme with HARPS-N at TNG: XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets⋆ | journal=Astronomy & Astrophysics | volume=602 | date=2017 | issn=0004-6361 | doi=10.1051/0004-6361/201629882 | page=A107| arxiv=1704.00373 }}</ref>
}}

===Footnotes===
{{noteslist|notes=
{{efn|name=n1|This means that the star has an [[iron]] content {{val|1.07|0.22|0.18}} times that of the [[Sun]].}}
}}

{{Stars of Serpens}}
[[Category:Hot Jupiters]]
[[Category:Transiting exoplanets]]
[[Category:Exoplanets discovered in 2010]]
[[Category:Exoplanets discovered by CoRoT|11b]]


{{exoplanet-stub}}