Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pegasus |
Right ascension | 22h 10m 11.98528s[1] |
Declination | +06° 11′ 52.3078″[1] |
Apparent magnitude (V) | +3.52[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | A2V[4] + M4-5.5[5] |
B−V color index | 0.086±0.002[2] |
Astrometry | |
Radial velocity (Rv) | −7.9±2.4[2] km/s |
Proper motion (μ) | RA: +282.18[1] mas/yr Dec.: +30.46[1] mas/yr |
Parallax (π) | 35.34 ± 0.85 mas[1] |
Distance | 92 ± 2 ly (28.3 ± 0.7 pc) |
Absolute magnitude (MV) | 1.24[2] |
Orbit[5] | |
Semi-major axis (a) | 6.55+3.0 −0.48 au |
Eccentricity (e) | 0.54+0.28 −0.15 |
Inclination (i) | 66.7+8.5 −14° |
Details | |
θ Peg A | |
Mass | 2.09 ± 0.16[6] M☉ |
Radius | 2.623±0.083[5] R☉ |
Luminosity | 23.7±1.1[4] L☉ |
Surface gravity (log g) | 3.95[6] cgs |
Temperature | 7872±82[4] K |
Metallicity [Fe/H] | −0.38[4] dex |
Rotational velocity (v sin i) | 136[6] km/s |
Age | 448[6] Myr |
θ Peg B | |
Mass | 0.280+0.18 −0.059[5] M☉ |
Surface gravity (log g) | 5.5[5] cgs |
Temperature | 3200[5] K |
Other designations | |
Database references | |
SIMBAD | data |
θ Pegasi, Latinized as Theta Pegasi, is a single[8] star in the equatorial constellation of Pegasus, lying about 7.5 degrees southwest of Enif.[9] It has the traditional name Biham /ˈbaɪ.æm/,[10][11] and the Flamsteed designation 26 Pegasi. This object is visible to the naked eye as a white-hued point of light with an apparent visual magnitude of +3.52.[2] The system is located 92 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −8 km/s.[2]
This object an A-type main-sequence star with a stellar classification of A2V.[4] It is 448[6] million years old with a high rate of spin, showing a projected rotational velocity of 136 km/s.[6] This star has 2.09[5] times the mass of the Sun and 2.6[12] times the Sun's radius. It is radiating 25 times the luminosity of the Sun from its outer envelope at an effective temperature of 7,951 K.[12] The star appears to display a slight infrared excess.[13]
θ Pegasi was suspected of being a binary star due to an acceleration detected by Hipparcos. In 2021, a low-mass companion star was discovered, associated with θ Pegasi.[5] It is a red dwarf with a spectral type of M4 to M5.5, and a luminosity of 0.5% that of the Sun.[5] The orbit around the primary is estimated to be moderately eccentric, at 0.54, and has a semimajor axis of 6.55 au.[5]
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