31 Cygni

31 Cygni
Location of 31 Cygni (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
31 Cygni A
Right ascension 20h 13m 37.908s
Declination +46° 44′ 28.76″
Apparent magnitude (V) 3.73 - 3.89
HD 192579
Right ascension 20h 13m 39.199s
Declination +46° 42′ 42.70″
Apparent magnitude (V) 6.99
Characteristics
31 Cygni A
Spectral type K3Ib + B2IV-V
Variable type Algol
HD 192579
Evolutionary stage main sequence
Spectral type B5V
Astrometry
31 Cygni A
Radial velocity (Rv)−7.41±0.08 km/s
Proper motion (μ) RA: 1.744 mas/yr
Dec.: 3.390 mas/yr
Parallax (π)2.9167±0.1327 mas
Distance1,120 ± 50 ly
(340 ± 20 pc)
HD 192579
Proper motion (μ) RA: 3.906 mas/yr
Dec.: 1.978 mas/yr
Parallax (π)2.9160±0.0336 mas
Distance1,120 ± 10 ly
(343 ± 4 pc)
Orbit
Primary31 Cygni Aa
Name31 Cygni Ab
Period (P)10.301+0.030
−0.037
years
Eccentricity (e)0.203+0.007
−0.008
Inclination (i)101.007+28.772
−18.623
°
Longitude of the node (Ω)307.271+9.802
−11.253
°
Periastron epoch (T)1950.508+0.171
−0.129
Argument of periastron (ω)
(secondary)
198.619+2.771
−1.963
°
Semi-amplitude (K1)
(primary)
13.94±0.04 km/s
Semi-amplitude (K2)
(secondary)
18.0 km/s
Details
K supergiant
Mass9.44+1.51
−1.39
 M
Radius127 R
Luminosity2,512 - 2,559 L
Temperature4,043±170 K
B dwarf
Mass6.475 M
Radius5.2±0.5 R
Temperature16,500+1,000
−2,000
 K
Age39.8 Myr
HD 192579
Mass4.1 M
Radius3.3 R
Luminosity373 L
Surface gravity (log g)4.04 cgs
Temperature13,949 K
Metallicity [Fe/H]+0.68 dex
Other designations
ο1 Cyg, ο2 Cyg, 31 Cyg, ADS 13554, WDS J20136+4644
31 Cygni A (HD 192577): V695 Cyg, HD 192577, BD+46°2882, HIP 99675, HR 7735, SAO 49337
HD 192579: HD 192579, BD+46°2883, HIP 99676, SAO 49338
Database references
SIMBADdata
HD 192579

31 Cygni, also known as ο1 Cygni, Omicron1 Cygni, ο2 Cygni or V695 Cygni, is a ternary star system about 750 light years away in the constellation Cygnus.

The Bayer designation ο (omicron) has been variously applied to two or three of the stars 30, 31, and 32 Cygni. 31 Cygni has been designated, variously, as ο1 or ο2 Cygni — therefore for clarity, it is preferred to use the Flamsteed designation 31 Cygni.

31 Cygni consists of a visible pair of stars 109 apart as of 2016, and the brighter of the two is also a spectroscopic binary. 31 Cygni A is also designated HD 192577 and HR 7735, while its 7th-magnitude visual companion is designated HD 192579. Some multiple star catalogues designate a 13th-magnitude star 36″ from 31 Cygni A as 31 Cygni B, and HD 192579 as 31 Cygni C. The 13th-magnitude star is likely to be an unrelated background object.

The spectroscopic pair are an orange supergiant of spectral type K3Ib and a blue-white star likely to be evolving off the main sequence with a spectral type of B2IV-V. The visible companion is a 7th-magnitude B5 main sequence star.

31 Cygni A is an Algol-type eclipsing binary and ranges between magnitudes 3.73 and 3.89 over a period of ten years. The eclipsing system has been studied in attempts to determine an accurate direct mass for a red supergiant. The value 6.73 M is believed to be accurate to about 2%, but there are some discrepancies in the orbital fit.

30 Cygni is another naked eye star a tenth of a degree away, forming a bright triple.

32 Cygni is about a degree away to the north, also a detached eclipsing binary system. It comprises a large cool evolved star and a small hot main sequence or subgiant companion.