Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pegasus |
Right ascension | 21h 46m 04.364s [1] |
Declination | +22° 56′ 55.96″ [1] |
Apparent magnitude (V) | +5.266 [2] |
Characteristics | |
Spectral type | K0IbHdel0.5 [3] |
U−B color index | +1.33 [4] |
B−V color index | +1.41 [4] |
Astrometry | |
Proper motion (μ) |
RA: 8.299
[1]
mas/
yr Dec.: −2.478 [1] mas/ yr |
Parallax (π) | 2.3673 ± 0.1279 mas [1] |
Distance | 1,380 ± 70
ly (420 ± 20 pc) |
Absolute magnitude (MV) | −4.03 [4] |
Details | |
Mass | 6.3 [5] M☉ |
Radius | 81 [6] R☉ |
Luminosity | 1,722–1,820 [6] L☉ |
Surface gravity (log g) | 1.11 [7] cgs |
Temperature | 4,185 [6] K |
Metallicity [Fe/H] | +0.03 [7] dex |
Rotational velocity (v sin i) | 19.5 [8] km/s |
Age | 19.8 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
12 Pegasi is a K-type supergiant star in the constellation of Pegasus. It has a spectral type of K0Ib Hdel0.5, [9] which indicates that it is a less luminous K-type supergiant with strong H-δ Balmer lines. The star has expanded to 81 times the radius of the Sun, and has an effective temperature of 4,185 K. [6]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pegasus |
Right ascension | 21h 46m 04.364s [1] |
Declination | +22° 56′ 55.96″ [1] |
Apparent magnitude (V) | +5.266 [2] |
Characteristics | |
Spectral type | K0IbHdel0.5 [3] |
U−B color index | +1.33 [4] |
B−V color index | +1.41 [4] |
Astrometry | |
Proper motion (μ) |
RA: 8.299
[1]
mas/
yr Dec.: −2.478 [1] mas/ yr |
Parallax (π) | 2.3673 ± 0.1279 mas [1] |
Distance | 1,380 ± 70
ly (420 ± 20 pc) |
Absolute magnitude (MV) | −4.03 [4] |
Details | |
Mass | 6.3 [5] M☉ |
Radius | 81 [6] R☉ |
Luminosity | 1,722–1,820 [6] L☉ |
Surface gravity (log g) | 1.11 [7] cgs |
Temperature | 4,185 [6] K |
Metallicity [Fe/H] | +0.03 [7] dex |
Rotational velocity (v sin i) | 19.5 [8] km/s |
Age | 19.8 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
12 Pegasi is a K-type supergiant star in the constellation of Pegasus. It has a spectral type of K0Ib Hdel0.5, [9] which indicates that it is a less luminous K-type supergiant with strong H-δ Balmer lines. The star has expanded to 81 times the radius of the Sun, and has an effective temperature of 4,185 K. [6]