12 Vulpeculae

12 Vulpeculae
Location of 12 Vulpeculae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Vulpecula
Right ascension 19h 51m 04.1083s
Declination +22° 36 36.173
Apparent magnitude (V) 4.928±0.015 (4.78 - 4.97)
Characteristics
Spectral type B2.5V
Apparent magnitude (U) 4.104±0.020
Apparent magnitude (B) 4.759±0.017
Variable type Be star
Astrometry
Radial velocity (Rv)−24.90 km/s
Proper motion (μ) RA: 23.404±0.068 mas/yr
Dec.: −15.797±0.099 mas/yr
Parallax (π)5.1710±0.1070 mas
Distance630 ± 10 ly
(193 ± 4 pc)
Absolute magnitude (MV)−1.52
Details
Mass6.8 M
Luminosity963 L
Surface gravity (log g)3.36 cgs
Temperature18,859 K
Metallicity [Fe/H]−0.01 dex
Rotational velocity (v sin i)195 km/s
Other designations
12 Vul, V395 Vul, BD+22°3833, FK5 3585, GC 27493, HD 187811, HIP 97679, HR 7565, SAO 87813
Database references
SIMBADdata

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 a baseline apparent visual magnitude of 4.928. It is moving closer to the Earth with a heliocentric radial velocity of -25 km/s.

This is a variable Be star with a stellar classification of B2.5V; its brightness ranges from magnitude 4.78 down to 4.97. As is true with other Be stars, it has a high rate of rotation with a projected rotational velocity of 195 km/s. The star has 6.8 times the mass of the Sun and is radiating 963 times the Sun's luminosity from its photosphere at an effective temperature of 18,859 K.