Omicron Cephei

ο Cephei
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cepheus
ο Cep A
Right ascension 23h 18m 37.493s
Declination +68° 06 41.20
Apparent magnitude (V) 4.86
ο Cep B
Right ascension 23h 18m 37.115s
Declination +68° 06 38.65
Apparent magnitude (V) 7.13
Characteristics
U−B color index +0.49
B−V color index +0.84
R−I color index +0.45
ο Cep A
Spectral type G8III
ο Cep B
Spectral type F6V
Astrometry
ο Cep A
Proper motion (μ) RA: 54.88 mas/yr
Dec.: 10.91 mas/yr
Parallax (π)15.48±0.55 mas
Distance211 ± 7 ly
(65 ± 2 pc)
Absolute magnitude (MV)0.78
ο Cep B
Proper motion (μ) RA: 45.70 mas/yr
Dec.: 13.19 mas/yr
Orbit
Period (P)1505±40 y
Semi-major axis (a)3.13±0.12 
Eccentricity (e)0.439±0.020
Inclination (i)16.0±4.0°
Longitude of the node (Ω)4.5±4.5°
Periastron epoch (T)B1692 ± 20
Argument of periastron (ω)
(secondary)
93.0±20.0°
Details
ο Cep A
Mass2.35 ± 0.15 M
Luminosity51 L
Metallicity [Fe/H]0.05±0.02 dex
ο Cep B
Mass1.29 M
Other designations
ο Cep, Omicron Cephei, Omicron Cep, 34 Cephei, 34 Cep, STF 3001AB, ADS 16666 AB, BD+67°1514, CCDM J23186+6807AB, GC 32463, GSC 04478-01361, HD 219916, HIP 115088, HR 8872, IDS 23145+6734 AB, PPM 24360, SAO 20554, WDS 23186+6807AB.
Database references
SIMBADdata

Omicron Cephei, Latinized from ο Cephei, is a binary star in the constellation of Cepheus. It consists of a less massive F-type main sequence star in orbit with a more massive G-type giant star. The overall apparent visual magnitude of the system is 4.75.

The pair was first determined to be binary by F. G. W. Struve in 1832. Since then, the secondary has been seen to revolve approximately 45 degrees around the primary. A number of orbits have been computed, the most recent giving a period of approximately 1500 years.