Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cepheus |
Right ascension | 23h 07m 53.854s[1] |
Declination | +75° 23′ 15.00″[1] |
Apparent magnitude (V) | 4.419[2] 4.61[3] + 6.75[4]) |
Characteristics | |
Spectral type | G7III[5] / F5V[5] / A7V-A9V[6] |
U−B color index | -0.46 |
B−V color index | 0.8 |
Astrometry | |
Radial velocity (Rv) | -18.6 ± 0.9 km/s |
Proper motion (μ) | RA: 6.81 ± 1.05[1] mas/yr Dec.: -34.06 ± 0.88[1] mas/yr |
Parallax (π) | 13.8 ± 0.41 mas[6] |
Distance | 236 ± 7 ly (72 ± 2 pc) |
Absolute magnitude (MV) | 0.24 |
Orbit[5] | |
Primary | π Cep Aa |
Companion | π Cep Ab |
Period (P) | 556.72 ± 0.05 d |
Semi-major axis (a) | 39.0 ± 3.9 mas[6] |
Eccentricity (e) | 0.297 ± 0.006 |
Inclination (i) | 99.0 ± 2.5[6]° |
Longitude of the node (Ω) | 109.2 ± 3.5[6]° |
Periastron epoch (T) | 2,439,172.9 ± 1.6 |
Argument of periastron (ω) (secondary) | 7.6 ± 1.2° |
Semi-amplitude (K1) (primary) | 24.18 ± 0.15 km/s |
Orbit[7] | |
Primary | π Cephei A (Aa + Ab) |
Companion | π Cephei B |
Period (P) | 162.8 ± 2.8 yr |
Semi-major axis (a) | 0.810 ± 0.050″ |
Eccentricity (e) | 0.5968 ± 0.0067 |
Inclination (i) | 30.0 ± 3.0° |
Longitude of the node (Ω) | 90.3 ± 4.9° |
Periastron epoch (T) | B 1934.573 ± 0.35 |
Argument of periastron (ω) (secondary) | 90.0 ± 4.4° |
Details[6] | |
π Cep Aa | |
Mass | 3.63 ± 0.53 M☉ |
Surface gravity (log g) | 3.05±0.11[8] cgs |
Temperature | 5,226±92[8] K |
Metallicity [Fe/H] | 0.29±0.05[8] dex |
Age | 100[8] Myr |
π Cep Ab | |
Mass | 3.27 ± 0.48 M☉ |
π Cep B | |
Mass | 1.93 ± 0.23 M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Pi Cephei (π Cephei) is a trinary star located in the constellation Cepheus.[6] With a combined apparent magnitude of about 4.4,[2] the system is faintly visible to the naked eye. The inner pair of stars orbits in 1.5 years while the outer companion completes one orbit in about 160 years.[6]
Pi Cephei was found to have a visual companion star by Otto Wilhelm von Struve in 1843.[6] That the primary is itself a spectroscopic binary was first noticed by William Wallace Campbell in 1901 using photographic plates taken at Lick Observatory.[10]
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