CoRoT-5

Last updated
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]
Distance 2,830 ± 50  ly
(870 ± 10  pc)
Details
Mass 1.12 [2]   M☉
Radius 1.1 [2]   R☉
Luminosity 1.7 [2]   L☉
Surface gravity (log g)4.33 [2]   cgs
Temperature 6,190 [2]   K
Metallicity [Fe/H]0.04 [4]   dex
Rotation 4.03 days [5]
Rotational velocity (v sin i)3.82 [4]  km/s
Age 1.7 [2]   Gyr
Other designations
CoRoT-Exo-5, 2MASS J06450653+0048548
Database references
SIMBAD data

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

Contents

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 0.04954.03840.09—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. 1 2 3 4 5 6 7 8 9 10 11 12 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. 1 2 3 4 5 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. 1 2 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.


This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.