3 Persei
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Perseus |
| Right ascension | 01h 58m 33.50596s |
| Declination | +49° 12′ 15.6705″ |
| Apparent magnitude (V) | 5.70 |
| Characteristics | |
| Spectral type | K0 IV |
| Astrometry | |
| Radial velocity (Rv) | −0.67±0.17 km/s |
| Proper motion (μ) | RA: +7.051 mas/yr Dec.: +41.686 mas/yr |
| Parallax (π) | 12.6940±0.0671 mas |
| Distance | 257 ± 1 ly (78.8 ± 0.4 pc) |
| Absolute magnitude (MV) | 1.33 |
| Details | |
| Mass | 1.41±0.17 M☉ |
| Radius | 8.27±0.55 R☉ |
| Luminosity | 37.2+7.5 −6.3 L☉ |
| Surface gravity (log g) | 2.72±0.09 cgs |
| Temperature | 4,757±25 K |
| Metallicity [Fe/H] | −0.15±0.05 dex |
| Rotational velocity (v sin i) | 1.85±0.45 km/s |
| Age | 2.91±0.98 Gyr |
| Other designations | |
| 3 Per, BD+48°576, HD 11949, HIP 9222, HR 568, SAO 37665 | |
| Database references | |
| SIMBAD | data |
3 Persei is a single, orange-hued star in the northern constellation of Perseus. It is dimly visible to the naked eye under good viewing conditions, having an apparent visual magnitude of 5.70 The star is located around 79 parsecs (257 ly) distant, based upon an annual parallax shift of 12.7 mas.
This star has a stellar classification of K0 IV, suggesting it is a K-type subgiant – an evolved star that has used up its core hydrogen and is evolving to become a red giant. However, da Silva et al. (2015) categorized it as a giant star proper. At the age of around three billion years, it has an estimated 1.4 times the mass of the Sun and has expanded to move than 8 times the Sun's radius. It is radiating roughly 37 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,757 K.