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Mu Cygni
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Mu Cygni
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 21h 44m 08.57767s[1]
Declination +28° 44′ 33.4567″[1]
Apparent magnitude (V) 4.49[2]
Characteristics
Spectral type F6V + G2V[3]
B−V color index +0.512±0.007[2]
Astrometry
Radial velocity (Rv)+16.95[4] km/s
Proper motion (μ) RA: +257.012[1] mas/yr
Dec.: −239.009[1] mas/yr
Parallax (π)45.2207±0.2383 mas[1]
Distance72.1 ± 0.4 ly
(22.1 ± 0.1 pc)
Absolute magnitude (MV)2.75[2]
μ1 Cyg
Absolute magnitude (MV)2.77[5]
Absolute bolometric
magnitude
 (Mbol)
2.91±0.06[6]
μ2 Cyg
Absolute magnitude (MV)4.38[5]
Absolute bolometric
magnitude
 (Mbol)
4.32±0.06[6]
Orbit[7]
Period (P)789 yr
Semi-major axis (a)5.32″
Eccentricity (e)0.66
Inclination (i)75.5°
Longitude of the node (Ω)110.1°
Periastron epoch (T)1958.0
Argument of periastron (ω)
(secondary)
145.7°
Details[5]
μ1 Cyg
Mass1.31 M
Radius1.88±0.07[6] R
Luminosity6.0 L
Surface gravity (log g)3.93 cgs
Temperature6,354 K
Metallicity [Fe/H]−0.16 dex
Rotational velocity (v sin i)11.6 km/s
Age3.46 Gyr
μ2 Cyg
Mass0.99 M
Radius1.08±0.05 R
Luminosity1.4 L
Surface gravity (log g)4.33 cgs
Temperature5,998 K
Metallicity [Fe/H]−0.24 dex
Rotational velocity (v sin i)6.4 km/s
Age7.11[5] Gyr
Other designations
78 Cyg, BD+28°4169, HIP 107310, CCDM J21442+2845AB, WDS J21441+2845AB[8]
μ1 Cyg: HD 206826, HR 8309, SAO 89940[9]
μ2 Cyg: HD 206827, HR 8310, SAO 89939[10]
Database references
SIMBADμ Cyg
μ1 Cyg
μ2 Cyg

Mu Cygni is a binary star[11] in the northern constellation of Cygnus. Its name is a Bayer designation that is Latinized from μ Cygni, and abbreviated Mu Cyg or μ Cyg. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.49.[2] The system is located 72 light years distant from the Sun, based on parallax,[1] and is drifting further away with a radial velocity of +17 km/s.[4]

The pair have an orbital period of around 800 years, with a semimajor axis of 5 and an eccentricity around 0.6.[12] The primary,[9] with an apparent magnitude of 4.69, is an F-type main-sequence star with a stellar classification of F6V.[3] It has 35% more mass than the Sun and 188% of the Sun's radius.[6] The star is spinning with a projected rotational velocity of 9.6 km/s. The secondary companion,[10] with an apparent magnitude of 6.12, is a G-type main-sequence star with a class of G2V.[3] It has a similar radius as the Sun and slightly more mass.[6]

Two reported additional components, C (apparent magnitude 12.93) and D (apparent magnitude 6.94), are believed to be optical doubles rather than part of the Mu Cygni system.[3] Component D is the more distant spectroscopic binary HD 206874 (HIP 107326), consisting of two early F-type subgiants.[13]

References

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