63 Cygni

K-type bright giant/supergiant star in the constellation Cygnus From Wikipedia, the free encyclopedia

63 Cygni is a single[9] star in the northern constellation of Cygnus, located around 1,030 light years away from Sun. It is visible to the naked eye as an orange-hued star with an apparent visual magnitude of 4.56.[2] 63 Cyg is moving closer to the Earth with a heliocentric radial velocity of −26 km/s.[2]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
63 Cygni
Location of 63 Cygni (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 21h 06m 36.103s[1]
Declination +47° 38 54.22[1]
Apparent magnitude (V) 4.56[2]
Characteristics
Spectral type K4 Ib–IIa[3]
B−V color index 1.569±0.012[2]
Astrometry
Radial velocity (Rv)−26.32±0.23[2] km/s
Proper motion (μ) RA: +5.992[4] mas/yr
Dec.: −1.067[4] mas/yr
Parallax (π)2.66±0.29 mas[4]
Distanceapprox. 1,200 ly
(approx. 380 pc)
Absolute magnitude (MV)−2.93[5]
Details
Radius138[1] R
Luminosity3,981 - 4,130[1] L
Surface gravity (log g)1.27[6] cgs
Temperature3,927[1] K
Metallicity [Fe/H]0.12[6] dex
Rotational velocity (v sin i)6.3[7] km/s
Other designations
f2 Cyg, 63 Cyg, BD+47°3292, FK5 3688, HD 201251, HIP 104194, HR 8089, SAO 50456, WDS J21066+4739[8]
Database references
SIMBADdata
Close

This is an evolved star showing a stellar spectrum with mixed traits between a bright giant and supergiant. It has been chosen as a spectral standard for the class of K4 Ib–IIa.[3]

For reasons that are not yet clear, 63 Cygni is displaying very long period (982 days) and low-amplitude (742 m/s) variations in radial velocity.[2] The star has expanded to 35[2] times the Sun's radius and is radiating 4,397[5] times the Sun's luminosity from its photosphere at an effective temperature of 4,204 K.[6]

References

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