Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cepheus |
Right ascension | 21h 28m 39.59685s[1] |
Declination | +70° 33′ 38.5747″[1] |
Apparent magnitude (V) | 3.16 – 3.27[2] |
Characteristics | |
Spectral type | B1 IV[3] |
U−B color index | –0.95[4] |
B−V color index | –0.22[4] |
Variable type | β Cep[2] |
Astrometry | |
Radial velocity (Rv) | –8.2[5] km/s |
Proper motion (μ) | RA: +12.54[1] mas/yr Dec.: +8.39[1] mas/yr |
Parallax (π) | 4.76 ± 0.30 mas[1] |
Distance | 690 ± 40 ly (210 ± 10 pc) |
Absolute magnitude (MV) | –3.03[3] |
Orbit[6] | |
Primary | β Cep Aa |
Companion | β Cep Ab |
Period (P) | 29616.54 ± 1.36 d |
Semi-major axis (a) | 206.96 ± 0.53 mas |
Eccentricity (e) | 0.7478 ± 0.0005 |
Inclination (i) | 88.80 ± 0.07° |
Longitude of the node (Ω) | 227.83 ± 0.14° |
Periastron epoch (T) | 2450944.5 ± 24.2 |
Argument of periastron (ω) (secondary) | 202.43 ± 0.31° |
Semi-amplitude (K1) (primary) | 9.63 ± 0.26 km/s |
Details | |
β Cep Aa | |
Mass | 7.4[6] M☉ |
Radius | 7.22±0.42[7] R☉ |
Luminosity | 20,000+5,200 −4,100[8] L☉ |
Surface gravity (log g) | 4.12±0.07[7] cgs |
Temperature | 23,600±1,000[7] K |
Metallicity [Fe/H] | –0.23[9] dex |
Rotational velocity (v sin i) | 28[10] km/s |
Age | 8.7[3] Myr |
β Cep Ab | |
Mass | 5.0[6] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Beta Cephei (β Cephei, abbreviated Beta Cep, β Cep) is a triple star system of the third magnitude in the constellation of Cepheus. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 690 light-years distant from the Sun. It is the prototype of the Beta Cephei variable stars.
It consists of a binary pair (designated Beta Cephei A) together with a third companion (B). The binary's two components are themselves designated Beta Cephei Aa (officially named Alfirk /ˈælfərk/, the traditional name for the system)[11][12] and Ab.
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