Delta Cephei
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cepheus | 
| δ Cep A | |
| Right ascension | 22h 29m 10.26502s | 
| Declination | +58° 24′ 54.7139″ | 
| Apparent magnitude (V) | 4.07 (3.48–4.37) / 7.5 | 
| δ Cep C | |
| Right ascension | 22h 29m 09.248s | 
| Declination | +58° 24′ 14.76″ | 
| Apparent magnitude (V) | 6.3 | 
| Characteristics | |
| Spectral type | F5Ib-G1Ib + B7-8 | 
| U−B color index | 0.36 | 
| B−V color index | 0.60 | 
| Variable type | Cepheid | 
| Astrometry | |
| Radial velocity (Rv) | −16.8 km/s | 
| Proper motion (μ) | RA: +15.35 mas/yr Dec.: +3.52 mas/yr | 
| Parallax (π) | 3.66+0.09 −0.10 mas | 
| Distance | 887±26 ly (272±8 pc) | 
| Absolute magnitude (MV) | −3.47±0.10 (−3.94 - −3.05) | 
| Orbit | |
| Primary | δ Cep A | 
| Companion | δ Cep B | 
| Period (P) | 9.32+0.03 −0.04 years | 
| Semi-major axis (a) | 0.029+0.002 −0.003″ | 
| Eccentricity (e) | 0.71±0.02 | 
| Inclination (i) | 124+17 −12° | 
| Longitude of the node (Ω) | 78+56 −50° | 
| Periastron epoch (T) | 1982.294+0.111 −0.101 | 
| Argument of periastron (ω) (secondary) | 230+4 −3° | 
| Semi-amplitude (K1) (primary) | 1.509±0.2 km/s | 
| Details | |
| δ Cep A | |
| Mass | 5.26+1.26 −1.4 M☉ | 
| Radius | 46.1+1.9 −2.1 R☉ | 
| Luminosity | 1,949±107 L☉ | 
| Surface gravity (log g) | 1.65 cgs | 
| Temperature | 5,905±29 K | 
| Metallicity [Fe/H] | +0.08 dex | 
| Rotational velocity (v sin i) | 9 km/s | 
| δ Cep B | |
| Mass | 0.72±0.11 M☉ | 
| δ Cep C | |
| Temperature | 8,800 K | 
| Other designations | |
| 27 Cephei, BD+57 2548, FK5 847, HD 213306, HIP 110991, HR 8571, SAO 34508. | |
| Database references | |
| SIMBAD | data | 
Delta Cephei (δ Cep, δ Cephei) is a quadruple star system located approximately 887 light-years away in the northern constellation of Cepheus, the King. At this distance, the visual magnitude of the star is diminished by 0.23 as a result of extinction caused by gas and dust along the line of sight. It is the prototype of the Cepheid variable stars that undergo periodic changes in luminosity.