Pi2 Pegasi
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Pegasus |
| Right ascension | 22h 09m 59.24371s |
| Declination | +33° 10′ 41.5976″ |
| Apparent magnitude (V) | +4.28 |
| Characteristics | |
| Spectral type | F5 III |
| B−V color index | 0.471±0.012 |
| Astrometry | |
| Radial velocity (Rv) | +5.1±0.9 km/s |
| Proper motion (μ) | RA: −12.87±0.12 mas/yr Dec.: −18.95±0.16 mas/yr |
| Parallax (π) | 12.40±0.17 mas |
| Distance | 263 ± 4 ly (81 ± 1 pc) |
| Absolute magnitude (MV) | 0.21 |
| Details | |
| Mass | 2.48 M☉ |
| Radius | 8.5±0.8 R☉ |
| Luminosity | 102.9±2.6 L☉ |
| Temperature | 6,300+298 −263 K |
| Rotational velocity (v sin i) | 139.7 km/s |
| Age | 530 Myr |
| Other designations | |
| π2 Peg, 29 Pegasi, BD+32°4352, FK5 835, HD 210459, HIP 109410, HR 8454, SAO 72077 | |
| Database references | |
| SIMBAD | data |
π2 Pegasi, Latinized as Pi2 Pegasi, is a single star in the northern constellation Pegasus. It is yellow-white in hue and visible to the naked eye as a faint point of light with an apparent visual magnitude of +4.28. The distance to this object is approximately 263 light years based on parallax, and it is drifting further away with a radial velocity of +5 km/s. This star is an outlying member of the Ursa Major Moving Group.
This object has a stellar classification of F5 III, matching an aging giant star that has exhausted the supply of hydrogen at its core then cooled and expanded off the main sequence. At present it has 8.5 times the radius of the Sun. The star is 530 million years old with 2.48 times the Sun's mass. It shows a high rotation rate considering its evolutionary status, with a projected rotational velocity of 140 km/s. The star has been noted as a possible variable shell star. Pi2 Pegasi is radiating 103 times the Sun's luminosity from its swollen photosphere at an effective temperature of 6,300 K.