31 Cygni
From Infogalactic: the planetary knowledge core
Observation data Epoch J2000.0 Equinox J2000.0 |
|
---|---|
Constellation | Cygnus |
Right ascension | 20h 13m 37.907s[1] |
Declination | +46° 44′ 28.78″[1] |
Characteristics | |
Spectral type | K4Iab+B4IV-V [2] |
Astrometry | |
Radial velocity (Rv) | –7.41 ± 0.08[3] km/s |
Proper motion (μ) | RA: 4.78 ± 0.38[1] mas/yr Dec.: 1.21 ± 0.35[1] mas/yr |
Parallax (π) | 3.69 ± 0.41[1] mas |
Distance | approx. 880 ly (approx. 270 pc) |
Orbit[3] | |
Primary | Omicron1 Cygni A |
Companion | Omicron1 Cygni B |
Period (P) | 3786.1 ± 0.7 days |
Eccentricity (e) | 0.224 ± 0.006 |
Periastron epoch (T) | 2,452,372.8 ± 2.2 |
Argument of periastron (ω) (secondary) |
206.4 ± 1.4° |
Semi-amplitude (K1) (primary) |
13.78 ± 0.13 km/s |
Other designations | |
31 Cygni, also known as Omicron1 Cygni or V695 Cygni, is a star in the constellation Cygnus. An Algol-type eclipsing binary, it ranges between magnitudes 3.73 and 3.89 over a period of ten years; the component stars are an orange supergiant of spectrial type K4Iab and a blue-white star likely to be evolving off the main sequence with a spectral type of B4IV-V.[2]
References
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