Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 20h 53m 14.75503s [1] |
Declination | +44° 23′ 14.1408″ [1] |
Apparent magnitude (V) | 4.80 [2] |
Characteristics | |
Spectral type | B5 V [3] |
B−V color index | −0.134±0.006 [2] |
Astrometry | |
Radial velocity (Rv) | −21.1±2.8 [2] km/s |
Proper motion (μ) |
RA: +11.94
[1]
mas/
yr Dec.: −2.08 [1] mas/ yr |
Parallax (π) | 6.21 ± 0.22 mas [1] |
Distance | 530 ± 20
ly (161 ± 6 pc) |
Absolute magnitude (MV) | −1.23 [2] |
Orbit [4] | |
Period (P) | 2.8548 days |
Eccentricity (e) | 0.139±0.014 [5] |
Inclination (i) | ≈ 48 [6]° |
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 | |
Mass | 5.54±0.55 [5] M☉ |
Radius | 3.3±0.4 [4] R☉ |
Temperature | 17,190 [7] K |
Rotational velocity (v sin i) | 40 [8] km/s |
57 Cyg B | |
Mass | 4.92±0.49 [5] M☉ |
Radius | 2.9±0.4 [4] R☉ |
Rotational velocity (v sin i) | 30 [8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
57 Cygni is a close binary star [4] 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. [2] The pair have a magnitude difference of 0.34. [4] This system is moving closer to the Earth with a heliocentric radial velocity of −21 km/s. [2]
This is a double-lined spectroscopic binary with an orbital period of 2.85 days and an eccentricity of 0.15. [4] They show a steady change in their longitude of periastron, showing an apsidal period of 203±4 years. [10] The system does not form an eclipsing binary, having the orbital inclination of around 48°. [6] Both components are B-type main-sequence stars with a stellar classification of B5 V. [4]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 20h 53m 14.75503s [1] |
Declination | +44° 23′ 14.1408″ [1] |
Apparent magnitude (V) | 4.80 [2] |
Characteristics | |
Spectral type | B5 V [3] |
B−V color index | −0.134±0.006 [2] |
Astrometry | |
Radial velocity (Rv) | −21.1±2.8 [2] km/s |
Proper motion (μ) |
RA: +11.94
[1]
mas/
yr Dec.: −2.08 [1] mas/ yr |
Parallax (π) | 6.21 ± 0.22 mas [1] |
Distance | 530 ± 20
ly (161 ± 6 pc) |
Absolute magnitude (MV) | −1.23 [2] |
Orbit [4] | |
Period (P) | 2.8548 days |
Eccentricity (e) | 0.139±0.014 [5] |
Inclination (i) | ≈ 48 [6]° |
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 | |
Mass | 5.54±0.55 [5] M☉ |
Radius | 3.3±0.4 [4] R☉ |
Temperature | 17,190 [7] K |
Rotational velocity (v sin i) | 40 [8] km/s |
57 Cyg B | |
Mass | 4.92±0.49 [5] M☉ |
Radius | 2.9±0.4 [4] R☉ |
Rotational velocity (v sin i) | 30 [8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
57 Cygni is a close binary star [4] 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. [2] The pair have a magnitude difference of 0.34. [4] This system is moving closer to the Earth with a heliocentric radial velocity of −21 km/s. [2]
This is a double-lined spectroscopic binary with an orbital period of 2.85 days and an eccentricity of 0.15. [4] They show a steady change in their longitude of periastron, showing an apsidal period of 203±4 years. [10] The system does not form an eclipsing binary, having the orbital inclination of around 48°. [6] Both components are B-type main-sequence stars with a stellar classification of B5 V. [4]