Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Perseus |
Right ascension | 04h 08m 15.38813s [1] |
Declination | +37° 43′ 38.9875″ [1] |
Apparent magnitude (V) | 6.07 [2] |
Characteristics | |
Spectral type | K1 III [3] |
B−V color index | 0.943±0.003 [2] |
Astrometry | |
Radial velocity (Rv) | −44.35±0.20 [2] km/s |
Proper motion (μ) |
RA: −98.909
[1]
mas/
yr Dec.: −195.772 [1] mas/ yr |
Parallax (π) | 22.0897 ± 0.0483 mas [1] |
Distance | 147.7 ± 0.3
ly (45.27 ± 0.10 pc) |
Absolute magnitude (MV) | 2.85 [2] |
Details | |
Mass | 1.38 [4] M☉ |
Radius | 3.72+0.10 −0.09 [1] R☉ |
Luminosity | 7.95±0.03 [1] L☉ |
Surface gravity (log g) | 3.45 [4] cgs |
Temperature | 5,028+61 −70 [1] K |
Metallicity [Fe/H] | 0.02±0.04 [2] dex |
Age | 3.93 [4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
49 Persei is a star in the northern constellation of Perseus. It is just visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 6.09. [2] Based upon parallax measurements, this star is located around 147.7 light-years (45.27 parsecs) away from the Sun, but is drifting closer with a radial velocity of −44 km/s. [2] It has a relatively large proper motion, traversing the celestial sphere at a rate of 0.220 ″·yr−1. [6]
This is an aging red giant star with a stellar classification of K1III, a star that has used up its core hydrogen and is expanding. It is a candidate horizontal branch star, which would indicate it is past the red giant branch stage and is fusing helium at its core. [7] The star is nearly four [4] billion years old with 1.4 [4] times the mass of the Sun and 3.7 [1] times the Sun's radius. It is radiating eight [1] times the luminosity of the Sun from its photosphere at an effective temperature of 5,028 K. [1]