31 Pegasi

Star in the constellation Pegasus From Wikipedia, the free encyclopedia

31 Pegasi is a single[11] star in the northern constellation of Pegasus. It is visible to the naked eye as a dim, blue-white hued point of light with an apparent visual magnitude of about 5. It is located approximately 1,600 light years away from the Sun based on parallax,[1] but is drifting closer with a radial velocity of −5.3 km/s.[6]

A light curve for IN Pegasi, plotted from Hipparcos data[12]
Right ascension22h 21m 31.07511s[1]
Declination12° 12 18.6628[1]
Apparentmagnitude(V)4.85 - 5.05[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
31 Pegasi
Location of 31 Pegasi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Pegasus
Right ascension 22h 21m 31.07511s[1]
Declination 12° 12 18.6628[1]
Apparent magnitude (V) 4.85 - 5.05[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type B2IV-Ve[4]
U−B color index -0.81[5]
B−V color index -0.10[5]
Variable type γ Cas[2]
Astrometry
Radial velocity (Rv)−5.30[6] km/s
Proper motion (μ) RA: +6.32[1] mas/yr
Dec.: +4.80[1] mas/yr
Parallax (π)2.01±0.28 mas[1]
Distanceapprox. 1,600 ly
(approx. 500 pc)
Absolute magnitude (MV)−3.61[7]
Details
Mass12.5±0.7[3] M
Radius11.6[8] R
Luminosity (bolometric)27,925+4,360
−3,770
[3] L
Surface gravity (log g)3.71±0.15[3] cgs
Temperature23,890±740[3] K
Rotational velocity (v sin i)98±8[3] km/s
Age15.4±1.3[9] Myr
Other designations
31 Peg, IN Peg, BD+11°4784, FK5 843, GC 31255, HD 212076, HIP 110386, HR 8520, SAO 107854[10]
Database references
SIMBADdata
Close

This is a massive Be star with a stellar classification of B2IV-V.[13] It is a γ Cas variable; a type of shell star with a circumstellar disc of gas surrounding the star at the equator, and ranges from 5.05 up to 4.85 in visual magnitude.[2] It is spinning with a projected rotational velocity of 98 km/s, with the pole being inclined by an estimated angle of 26°± to the line of sight from the Earth.[3] The star is 15.4[9] million years old with 12.5[3] times the mass of the Sun. It is radiating around 28,000 times the luminosity of the Sun from its photosphere at an effective temperature of 23,890 K.[3]

References

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