VW Cephei

VW Cephei

A visual band light curve for VW Cephei, adapted from Kreiner and Winiarski (1981)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cepheus
Right ascension 20h 37m 21.5439s
Declination +75° 36 01.467
Apparent magnitude (V) 7.30  7.84
Characteristics
A
Spectral type G8V
B
Spectral type K0V
Astrometry
Proper motion (μ) RA: +308.71 mas/yr
Dec.: +540.86 mas/yr
Parallax (π)36.25±0.58 mas
Distance91.00 ± 0.95 ly
(27.90±0.29 pc)
Details
A
Mass1.13 M
Radius0.99 R
Temperature5,050 K
Age9.029 Gyr
B
Mass0.34 M
Radius0.57 R
Temperature5,342±15 K
Age9.029 Gyr
Orbit
PrimaryA
CompanionB
Period (P)0.2783146 days
Semi-major axis (a)(1.412±0.010)×106 km
(2.030±0.014 R)
Inclination (i)62.86±0.04°
Other designations
VW Cep, LHS 3565, SAO 9828, LTT 16039, BD+75 752, GJ 1255, GJ 9703, HD 197433, HIP 101750
Database references
SIMBADdata

VW Cephei (VW Cep) is an eclipsing contact binary of W Ursae Majoris-type located roughly at 90.6 light years from the Sun, whose two component stars share a common outer layer. Because the two components share their outer layers, as the components of W Ursae Majoris do, they have the same stellar classification, and are classified as yellow G-type main sequence dwarfs. The components take 0.2783 days (roughly 6.7 hours) to revolve around a common barycentre.


Jan Schilt discovered that the star is an eclipsing variable, in 1926.