Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Aquila |
Right ascension | 19h 27m 06.4944s[1] |
Declination | +01° 23′ 01.360″[1] |
Apparent magnitude (V) | 12.57[2] |
Characteristics | |
Spectral type | G7V[3] K0V (SIMBAD)[2] |
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[1] Dec.: −11.101(12) mas/yr[1] |
Parallax (π) | 4.6895 ± 0.0143 mas[1] |
Distance | 696 ± 2 ly (213.2 ± 0.7 pc) |
Details | |
Mass | 0.97 ±0.06 M☉ |
Radius | 0.902 ±0.018 R☉ |
Temperature | 5625 ±120 K |
Metallicity | 0 ±0.1 |
Age | ? years |
Other designations | |
Database references | |
SIMBAD | data |
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.[2]
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.[4]
Gaia DR3
was invoked but never defined (see the help page).Alonso2008
was invoked but never defined (see the help page).