9 Cygni

Star in the constellation Cygnus From Wikipedia, the free encyclopedia

9 Cygni is a binary star system in the northern constellation of Cygnus. 9 Cygni is its Flamsteed designation. The two stars have a combined magnitude of 5.39,[2] so it can be seen with the naked eye under good viewing conditions. Parallax measurements made by Gaia put the star at a distance of around 590 light-years (182 parsecs) away.[1]

Right ascension19h 34m 50.9285s[1]
Declination+29° 27 46.697[1]
Apparentmagnitude(V)5.39[2] (5.9 + 6.4)[3]
Quick facts Constellation, Right ascension ...
9 Cygni
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 34m 50.9285s[1]
Declination +29° 27 46.697[1]
Apparent magnitude (V) 5.39[2] (5.9 + 6.4)[3]
Characteristics
Evolutionary stage Red clump + main sequence[4]
Spectral type G8 IIIa + A2 V[4]
B−V color index 0.581[2]
Astrometry
Radial velocity (Rv)20.09±1.98[1] km/s
Proper motion (μ) RA: +14.822[1] mas/yr
Dec.: +13.554[1] mas/yr
Parallax (π)5.4904±0.0892 mas[1]
Distance594 ± 10 ly
(182 ± 3 pc)
Absolute magnitude (MV)0.70[2]
Orbit[3]
Period (P)4.56 yr
Semi-major axis (a)0.030″
Eccentricity (e)0.82
Inclination (i)114.6°
Longitude of the node (Ω)29.3°
Periastron epoch (T)1985.56
Argument of periastron (ω)
(secondary)
45.5°
Details
9 Cyg A
Mass2.9±0.4[2] M
Radius18.2[4] R
Surface gravity (log g)3.040±0.370[5] cgs
Temperature5,047[4] K
Metallicity [Fe/H]−0.260±0.090[5] dex
9 Cyg B
Mass2.7±0.4[2] M
Radius3.5[4] R
Temperature9,247[4] K
Age437.1[4] Myr
Other designations
BD+29 3651, HIP 96302, HR 7441, SAO 87385[6]
9 Cyg A: HD 184759
9 Cyg B: HD 184760
Database references
SIMBADdata
Close

The two stars of 9 Cygni are a G-type giant and an A-type star. Both stars are over twice as massive as the Sun.[2] They orbit once every 4.56 years, separated with a semi-major axis of 0.030 arcseconds. However, the eccentricity is high, at 0.82.[3] The primary is a red clump giant, a star on the cool end of the horizontal branch fusing helium in its core. The secondary star has begun to evolve off the main sequence; it is sometimes classified as a giant star[2] and sometimes as a main-sequence star.[4]

References

See also

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