CoRoT-5

CoRoT-5
Observation data
Epoch J2000      Equinox J2000
Constellation Monoceros[1]
Right ascension 06h 45m 06.5407s[2]
Declination +00° 48′ 54.906″[2]
Apparent magnitude (V) 14.0[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type F9V[3]
Astrometry
Proper motion (μ) RA: −3.040[2] mas/yr
Dec.: −8.205[2] mas/yr
Parallax (π)1.1535±0.0188 mas[2]
Distance2,830 ± 50 ly
(870 ± 10 pc)
Details
Mass1.12[2] M☉
Radius1.1[2] R☉
Luminosity1.7[2] L☉
Surface gravity (log g)4.33[2] cgs
Temperature6,190[2] K
Metallicity [Fe/H]0.04[4] dex
Rotation4.03 days[5]
Rotational velocity (v sin i)3.82[4] km/s
Age1.7[2] Gyr
Other designations
CoRoT-Exo-5, 2MASS J06450653+0048548
Database references
SIMBADdata

CoRoT-5 is a magnitude 14 star located in the Monoceros constellation.[6]

Location and properties

CoRoT-5 is located within the LRa01 field of view of the CoRoT spacecraft, in the Monoceros constellation.[3] It is an F-type main-sequence star with a radius of about 116% of the Sun's and a mass of about 101% of the Sun.[3]

Planetary system

A single planet, CoRoT-5b, has been detected using the astronomical transit method by the CoRoT program.[3]

The CoRoT-5 planetary system
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 0.459 MJ 0.0495 4.0384 0.09 — 1.28 RJ

References

  1. ^ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
  2. ^ a b c d e f g h i j k l 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.
  3. ^ a b c d e Moutou, Claire; Deleuil, Magali; Guillot, Tristan; Baglin, Annie; Bordé, Pascal; Bouchy, Francois; Cabrera, Juan; Csizmadia, Szilárd; Deeg, Hans J.; the CoRoT Exoplanet Science Team (2013). "CoRoT: Harvest of the exoplanet program". Icarus. 226 (2): 1625. arXiv:1306.0578. Bibcode:2013Icar..226.1625M. doi:10.1016/j.icarus.2013.03.022.
  4. ^ a b Delgado Mena, E.; Bertrán De Lis, S.; Adibekyan, V. Zh.; Sousa, S. G.; Figueira, P.; Mortier, A.; González Hernández, J. I.; Tsantaki, M.; Israelian, G.; Santos, N. C. (2015). "Li abundances in F stars: Planets, rotation, and Galactic evolution". Astronomy and Astrophysics. 576: A69. arXiv:1412.4618. Bibcode:2015A&A...576A..69D. doi:10.1051/0004-6361/201425433.
  5. ^ Bohigas, J. (2020). "On the Evolution of Angular Momentum, Magnetic Activity and Mass Loss Rate of Late Type Main Sequence Stars". Revista Mexicana de Astronomía y Astrofísica. 56: 139. Bibcode:2020RMxAA..56..139B. doi:10.22201/ia.01851101p.2020.56.01.14.
  6. ^ Rauer, H; et al. (2009). "Transiting exoplanets from the CoRoT space mission. VII. The hot-Jupiter-type planet CoRoT-5b". Astronomy and Astrophysics. 506 (1): 281–286. arXiv:0909.3397. Bibcode:2009A&A...506..281R. doi:10.1051/0004-6361/200911902. S2CID 13117298.



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