V381 Cephei

V381 Cephei
Location of V381 Cephei (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cepheus
Right ascension 21h 19m 15.682s
Declination +58° 37 24.550
Apparent magnitude (V) 5.51 - 5.71
Characteristics
Spectral type M1epIb + B
U−B color index 0.00
B−V color index +1.34
Variable type Lc
Astrometry
Radial velocity (Rv)−14.10 km/s
Proper motion (μ) RA: −1.435 mas/yr
Dec.: −5.427 mas/yr
Parallax (π)1.59±0.23 mas
Distanceapprox. 2,100 ly
(approx. 630 pc)
Absolute magnitude (MV)−5.2
Details
Aa
Mass7.2 - 16 M
Radius977 R
Luminosity178,000 L
Temperature3,745±170 K
Ab
Mass13 M
B
Mass7.1 M
Radius3.4 R
Luminosity1,487 L
Surface gravity (log g)4.18 cgs
Temperature19,965 K
Metallicity [Fe/H]−0.30 dex
Rotational velocity (v sin i)42.8 km/s
Age49.1 Myr
Other designations
V381 Cephei, HR 8164, HIP 105259, BD+58°2249, ADS 14864, 2MASS J21191567+5837246, WDS J21193+5837
A: HD 203338
B: HD 203339
Database references
A
B

V381 Cephei (HR 8164) is a triple star system in the northern constellation of Cepheus. Its apparent magnitude is slightly variable between 5.5 and 5.7. It is faintly visible to the naked eye under good observing conditions.

The star was discovered to be a variable star in 1991, by Elaine M. Halbedel. It was given its variable star designation, V381 Cephei, in 1995.