CoRoT-6

CoRoT-6
Observation data; Epoch J2000 Equinox J2000
Constellation	Ophiuchus
Right ascension	18h 44m 17.4079s
Declination	+6° 39′ 47.513″
Apparent magnitude (V)	13.9
Characteristics
Spectral type	F5V
Astrometry
Proper motion (μ)	RA: 5.438±0.017 mas/yr ; Dec.: 1.889±0.016 mas/yr
Parallax (π)	1.5641 ± 0.0163 mas
Distance	2,090 ± 20 ly ; (639 ± 7 pc)
Details
Mass	1.1 M☉
Radius	1.02 R☉
Luminosity	1.4 L☉
Surface gravity (log g)	428 cgs
Temperature	5,922 K
Metallicity	−0.20 dex
Rotational velocity (v sin i)	7.5 km/s
Age	4.9 Gyr
Other designations
	CoRoT-Exo-6
Database references
SIMBAD	data
Exoplanet Archive	data

CoRoT-6 is a magnitude 13.9 star located in the Ophiuchus constellation.^[6]

Location and properties

The star has a radius of about 102% of the Sun and a mass of about 110% of the Sun.^[2] It is a main sequence F type star a little larger and hotter than the Sun.

Planetary system

The star is orbited by one known extrasolar planet identified as CoRoT-6b. The discovery was made by the CoRoT program using the transit method.^[2]

The CoRoT-6 planetary system^[6]
Companion (in order from star)	Mass	Semimajor axis (AU)	Orbital period (days)	Eccentricity	Inclination	Radius
b	2.96 $M$ _J	0.0855	8.887	< 0.1	—	1.166 $R$ _J

References

^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
^ ^a ^b ^c ^d ^e ^f H. Rauer, M. Fridlund (2009). "CoRoT's exoplanet harvest" (PDF). First CoRoT International Symposium. Archived from the original (PDF) on 2011-07-20. Retrieved 2009-04-19.
^ Ehrenreich, D.; Désert, J.-M. (2011). "Mass-loss rates for transiting exoplanets". Astronomy & Astrophysics. 529: A136. arXiv:1103.0011. Bibcode:2011A&A...529A.136E. doi:10.1051/0004-6361/201016356. S2CID 119302960.
^ Chen, Di-Chang; Xie, Ji-Wei; Zhou, Ji-Lin; Dong, Subo; Liu, Chao; Wang, Hai-Feng; Xiang, Mao-Sheng; Huang, Yang; Luo, Ali; Zheng, Zheng (2021). "Planets Across Space and Time (PAST). I. Characterizing the Memberships of Galactic Components and Stellar Ages: Revisiting the Kinematic Methods and Applying to Planet Host Stars". The Astrophysical Journal. 909 (2): 115. arXiv:2102.09424. Bibcode:2021ApJ...909..115C. doi:10.3847/1538-4357/abd5be. S2CID 231951508.
^ Damiani, C.; Lanza, A. F. (2015). "Evolution of angular-momentum-losing exoplanetary systems. Revisiting Darwin stability". Astronomy and Astrophysics. 574. arXiv:1411.3802. Bibcode:2015A&A...574A..39D. doi:10.1051/0004-6361/201424318. S2CID 54727372.
^ ^a ^b Fridlund, M.; et al. (2010). "Transiting exoplanets from the CoRoT space mission. IX. CoRoT-6b: a transiting 'hot Jupiter' planet in an 8.9d orbit around a low-metallicity star". Astronomy and Astrophysics. 512. A14. arXiv:1001.1426v1. Bibcode:2010A&A...512A..14F. doi:10.1051/0004-6361/200913767. S2CID 54014374.

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[dr3-1] ^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.

[harvest-2] ^ ^a ^b ^c ^d ^e ^f H. Rauer, M. Fridlund (2009). "CoRoT's exoplanet harvest" (PDF). First CoRoT International Symposium. Archived from the original (PDF) on 2011-07-20. Retrieved 2009-04-19.

[ehrenreich2011-3] Ehrenreich, D.; Désert, J.-M. (2011). "Mass-loss rates for transiting exoplanets". Astronomy & Astrophysics. 529: A136. arXiv:1103.0011. Bibcode:2011A&A...529A.136E. doi:10.1051/0004-6361/201016356. S2CID 119302960.

[chen2021-4] Chen, Di-Chang; Xie, Ji-Wei; Zhou, Ji-Lin; Dong, Subo; Liu, Chao; Wang, Hai-Feng; Xiang, Mao-Sheng; Huang, Yang; Luo, Ali; Zheng, Zheng (2021). "Planets Across Space and Time (PAST). I. Characterizing the Memberships of Galactic Components and Stellar Ages: Revisiting the Kinematic Methods and Applying to Planet Host Stars". The Astrophysical Journal. 909 (2): 115. arXiv:2102.09424. Bibcode:2021ApJ...909..115C. doi:10.3847/1538-4357/abd5be. S2CID 231951508.

[damiani2015-5] Damiani, C.; Lanza, A. F. (2015). "Evolution of angular-momentum-losing exoplanetary systems. Revisiting Darwin stability". Astronomy and Astrophysics. 574. arXiv:1411.3802. Bibcode:2015A&A...574A..39D. doi:10.1051/0004-6361/201424318. S2CID 54727372.

[Fridlund2010-6] Fridlund, M.; et al. (2010). "Transiting exoplanets from the CoRoT space mission. IX. CoRoT-6b: a transiting 'hot Jupiter' planet in an 8.9d orbit around a low-metallicity star". Astronomy and Astrophysics. 512. A14. arXiv:1001.1426v1. Bibcode:2010A&A...512A..14F. doi:10.1051/0004-6361/200913767. S2CID 54014374.

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Observation data Epoch J2000 Equinox J2000
Constellation	Ophiuchus
Right ascension	18^h 44^m 17.4079^s^[1]
Declination	+6° 39′ 47.513″^[1]
Apparent magnitude (V)	13.9^[2]
Characteristics
Spectral type	F5V^[3]
Astrometry

Proper motion (μ)	RA: 5.438±0.017^[1] mas/yr Dec.: 1.889±0.016^[1] mas/yr
Parallax (π)	1.5641 ± 0.0163 mas^[1]
Distance	2,090 ± 20 ly (639 ± 7 pc)

Details

Mass	1.1^[2] `M`_☉
Radius	1.02^[2] `R`_☉
Luminosity	1.4^[1] `L`_☉
Surface gravity (log g)	428^[1] cgs
Temperature	5,922^[1] K
Metallicity	−0.20^[4] dex
Rotational velocity (v sin i)	7.5^[5] km/s
Age	4.9^[1] Gyr

Other designations
CoRoT-Exo-6^[2]
Database references
SIMBAD	data
Exoplanet Archive	data