57 Cygni

57 Cygni
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 20h 53m 14.75503s
Declination +44° 23 14.1408
Apparent magnitude (V) 4.80
Characteristics
Spectral type B5 V
B−V color index −0.134±0.006
Astrometry
Radial velocity (Rv)−21.1±2.8 km/s
Proper motion (μ) RA: +11.94 mas/yr
Dec.: −2.08 mas/yr
Parallax (π)6.21±0.22 mas
Distance530 ± 20 ly
(161 ± 6 pc)
Absolute magnitude (MV)−1.23
Orbit
Period (P)2.8548 days
Eccentricity (e)0.139±0.014
Inclination (i) 48°
Periastron epoch (T)2441571.275 JD
Argument of periastron (ω)
(secondary)
159.6°
Semi-amplitude (K1)
(primary)
111.9 km/s
Semi-amplitude (K2)
(secondary)
126.0 km/s
Details
57 Cyg A
Mass5.54±0.55 M
Radius3.3±0.4 R
Temperature17,190 K
Rotational velocity (v sin i)40 km/s
57 Cyg B
Mass4.92±0.49 M
Radius2.9±0.4 R
Rotational velocity (v sin i)30 km/s
Other designations
57 Cyg, BD+43°3755, HD 199081, HIP 103089, HR 8001, SAO 50180
Database references
SIMBADdata

57 Cygni is a close binary star system in the constellation Cygnus, located about 530 light years from Earth. It is visible to the naked eye as a blue-white hued star with a baseline apparent visual magnitude of 4.80. The pair have a magnitude difference of 0.34. This system is moving closer to the Earth with a heliocentric radial velocity of −21 km/s.

This is a double-lined spectroscopic binary with an orbital period of 2.85 days and an eccentricity of 0.15. They show a steady change in their longitude of periastron, showing an apsidal period of 203±4 years. The system does not form an eclipsing binary, having the orbital inclination of around 48°. Both components are B-type main-sequence stars with a stellar classification of B5 V.