Delta Cephei

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.

Delta Cephei
Location of δ Cep (circled)
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)3.77 ± 0.16 mas
Distance887 ± 26 ly
(272 ± 8 pc)
Absolute magnitude (MV)–3.47 ± 0.10 (–3.94 - –3.05)
Details
δ Cep A
Mass4.5 ± 0.3 M
Radius44.5 R
Luminosity~2000 L
Temperature5,500–6,800 K
Metallicity [Fe/H]+0.08 dex
Rotational velocity (v sin i)9 km/s
Age~100 Myr
δ Cep B
Mass0.2 - 1.2 M
Orbit
Primaryδ Cep A
Companionδ Cep B
Period (P)6.03 yr
Eccentricity (e)0.647
Semi-amplitude (K1)
(primary)
1.509 ± 0.2 km/s
Other designations
27 Cephei, BD+57 2548, FK5 847, HD 213306, HIP 110991, HR 8571, SAO 34508.
Database references
SIMBADdata
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