12 Vulpeculae

Star in the constellation Vulpecula From Wikipedia, the free encyclopedia

12 Vulpeculae is a star in the northern constellation of Vulpecula, located approximately 630 light years away based on parallax. It has the variable star designation V395 Vul; 12 Vulpeculae is the Flamsteed designation. This object is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of about 4.9. It is moving closer to the Earth with a heliocentric radial velocity of -25 km/s.

Right ascension19h 51m 04.1083s[2]
Declination+22° 36 36.173[2]
Apparentmagnitude(V)4.78 - 4.97[3]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
12 Vulpeculae
Location of 12 Vulpeculae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Vulpecula[1]
Right ascension 19h 51m 04.1083s[2]
Declination +22° 36 36.173[2]
Apparent magnitude (V) 4.78 - 4.97[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type B2.5V[1]
Apparent magnitude (U) 4.104±0.020[4]
Apparent magnitude (B) 4.759±0.017[4]
Variable type Be star[3]
Astrometry
Radial velocity (Rv)−24.90[5] km/s
Proper motion (μ) RA: 23.404±0.068[2] mas/yr
Dec.: −15.797±0.099[2] mas/yr
Parallax (π)5.1710±0.1070 mas[2]
Distance630 ± 10 ly
(193 ± 4 pc)
Absolute magnitude (MV)−1.52[1]
Details
Mass6.8[6] M
Luminosity963[1] L
Surface gravity (log g)3.36[7] cgs
Temperature18,859[7] K
Metallicity [Fe/H]−0.01[7] dex
Rotational velocity (v sin i)195[8] km/s
Other designations
12 Vul, V395 Vul, BD+22°3833, FK5 3585, GC 27493, HD 187811, HIP 97679, HR 7565, SAO 87813[9]
Database references
SIMBADdata
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This is a variable Be star with a stellar classification of B2.5V;[1] its brightness ranges from magnitude 4.78 down to 4.97.[3] As is true with other Be stars, it has a high rate of rotation with a projected rotational velocity of 195 km/s.[8] The star has 6.8[6] times the mass of the Sun and is radiating 963[1] times the Sun's luminosity from its photosphere at an effective temperature of 18,859 K.[7]

References

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