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Omicron1 Cygni

31 Cygni
Cygnus constellation map.svg
Red circle.svg

Location of 31 Cygni (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cygnus
Right ascension 20h 13m 37.907s
Declination +46° 44′ 28.78″
Apparent magnitude (V) 3.73 - 3.89
Characteristics
Spectral type K4Iab + B4IV-V
Variable type Algol
Astrometry
Radial velocity (Rv) –7.41 ± 0.08 km/s
Proper motion (μ) RA: 4.78 ± 0.38 mas/yr
Dec.: 1.21 ± 0.35 mas/yr
Parallax (π) 3.69 ± 0.41mas
Distance approx. 880 ly
(approx. 270 pc)
Orbit
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
Details
K supergiant
Mass 11.7 ± 1.3 M
Radius 197 ± 20 R
Luminosity 4,300 ± 1,100 L
Temperature 3,590 ± 225 K
B dwarf
Mass 7.1 ± 0.8 M
Radius 5.2 ± 0.5 R
Temperature 16500+1000
−2000
 K
Other designations
ο1 Cyg, ο2 Cyg,31 Cyg, V695 Cyg, HD 192577, BD+46°2882, HIP 99675, HR 7735, SAO 49337
Database references
SIMBAD data

31 Cygni, also known as ο1 Cygni, Omicron1 Cygni, or V695 Cygni, is a star in the constellation Cygnus.

The Bayer letter ο has been variously applied to two or three of the stars 30, 31, and 32 Cygni. 31 Cygni has been designated as either ο1 or ο2 Cygni. For clarity, it is preferred to use the Flamsteed designation 31 Cygni rather than one of the Bayer designations.

It is an Algol-type eclipsing binary and 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.

ο2 Cygni is about a degree away to the north, also a detached eclipsing binary system containing a cool giant and a small hot star. 30 Cygni is another naked eye star a tenth of a degree away from the 31 Cygni pair, forming a bright triple.


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