CoRoT-2

CoRoT-2

CoRoT-2 is a G7V class star somewhat less massive than the Sun (G2V)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Aquila
Right ascension 19h 27m 06.4944s
Declination +01° 23 01.360
Apparent magnitude (V) 12.57
Characteristics
Evolutionary stage main sequence
Spectral type G7V
Apparent magnitude (V) ~12.577
Apparent magnitude (I) 11.49 ±0.03
Apparent magnitude (J) 10.5783 ±0.028
Apparent magnitude (H) 10.44 ±0.04
Apparent magnitude (K) 10.31 ±0.03
Astrometry
Proper motion (μ) RA: −3.360(16) mas/yr
Dec.: −11.101(12) mas/yr
Parallax (π)4.6895±0.0143 mas
Distance696 ± 2 ly
(213.2 ± 0.7 pc)
Details
Mass0.97 M
Radius0.94 R
Surface gravity (log g)4.48 cgs
Temperature5,529 K
Metallicity−0.04
Rotation4.542 d
Rotational velocity (v sin i)10.2 km/s
Age5.2 Gyr
Other designations
GSC 00465-01282, CoRoT-Exo-2, GSC2 N023200075, UCAC2 32263596, CoRoT 101206560, DENIS-P J192706.4+012301, 2MASS J19270649+0123013, USNO-B1.0 0913-00447544
Database references
SIMBADdata

CoRoT-2 is a yellow dwarf main sequence star a little cooler than the Sun. This star is located approximately 700 light-years away in the constellation of Aquila. The apparent magnitude of this star is 12, which means it is not visible to the naked eye but can be seen with a medium-sized amateur telescope on a clear dark night.

It has a true physical companion, 2MASS J19270636+0122577, with a spectral type of K9, as earlier hypothesized by Alonso et al. (2008), making CoRoT-2 a wide binary system with at least one planet.