71 Cygni

Star in the constellation Cygnus From Wikipedia, the free encyclopedia

71 Cygni is a star in the northern constellation of Cygnus, located 212 light years from the Sun.[1] 71 Cygni is the Flamsteed designation; it has the Bayer designation g Cygni.[7] It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.22.[2] The star is moving closer to the Earth with a heliocentric radial velocity of −21.5 km/s.[6]

Right ascension21h 29m 26.94995s[1]
Declination+46° 32 26.1024[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
71 Cygni
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 21h 29m 26.94995s[1]
Declination +46° 32 26.1024[1]
Apparent magnitude (V) 5.22[2]
Characteristics
Evolutionary stage red clump[3][4]
Spectral type K0− III[5]
B−V color index 0.965±0.004[2]
Astrometry
Radial velocity (Rv)−21.54±0.10[6] km/s
Proper motion (μ) RA: +43.048[1] mas/yr
Dec.: +104.683[1] mas/yr
Parallax (π)15.4057±0.1077 mas[1]
Distance212 ± 1 ly
(64.9 ± 0.5 pc)
Absolute magnitude (MV)1.11[2]
Details[6]
Mass2.05±0.09 M
Radius8.31±0.32 R
Luminosity44.7+7.8
−6.7
 L
Surface gravity (log g)3.03±0.05 cgs
Temperature4,983±18 K
Metallicity [Fe/H]0.05±0.06 dex
Rotational velocity (v sin i)2.03±0.85 km/s
Age1.07±0.15 Gyr
Other designations
g Cyg, 71 Cyg, BD+45°3558, FK5 807, HD 204771, HIP 106093, HR 8228, SAO 50934[7]
Database references
SIMBADdata
Close

At the age of one billion years,[6] this is an evolved giant star with a stellar classification of K0− III,[5] which means it has used up its core hydrogen and expanded. It is a red clump giant, indicating that it is on the horizontal branch of the Hertzsprung–Russell diagram and is generating energy by helium fusion at its center.[3][4] The star has double the mass of the Sun and eight times the Sun's radius. It is radiating 45 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,983 K.[6]

References

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