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57 Cygni
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]
Distance530 ± 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
Mass5.54±0.55 [5]  M
Radius3.3±0.4 [4]  R
Temperature17,190 [7]  K
Rotational velocity (v sin i)40 [8] km/s
57 Cyg B
Mass4.92±0.49 [5]  M
Radius2.9±0.4 [4]  R
Rotational velocity (v sin i)30 [8] km/s
Other designations
57 Cyg, BD+43°3755, HD 199081, HIP 103089, HR 8001, SAO 50180 [9]
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]

References

  1. ^ a b c d e van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv: 0708.1752, Bibcode: 2007A&A...474..653V, doi: 10.1051/0004-6361:20078357, S2CID  18759600.
  2. ^ a b c d e f Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID  119257644.
  3. ^ Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement, 17: 371, Bibcode: 1968ApJS...17..371L, doi: 10.1086/190179.
  4. ^ a b c d e f g Hilditch, R. W. (1973), "The binary system 57 Cygni - apsidal motion and effects of spectral line blending", Monthly Notices of the Royal Astronomical Society, 164 (2): 101–110, Bibcode: 1973MNRAS.164..101H, doi: 10.1093/mnras/164.2.101.
  5. ^ a b c De Laurentis, M.; et al. (August 2012), "Testing gravitational theories using eccentric eclipsing detached binaries", Monthly Notices of the Royal Astronomical Society, 424 (3): 2371–2379, arXiv: 1207.5410, Bibcode: 2012MNRAS.424.2371D, doi: 10.1111/j.1365-2966.2012.21410.x, S2CID  119109320.
  6. ^ a b Jetsu, L.; et al. (November 1999), "Photometry of V 1794 Cygni between 1975 and 1995", Astronomy and Astrophysics Supplement, 139 (3): 513–523, Bibcode: 1999A&AS..139..513J, doi: 10.1051/aas:1999397.
  7. ^ Zorec, J.; et al. (July 2009), "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ1, D) parameters into Teff", Astronomy and Astrophysics, 501 (1): 297–320, arXiv: 0903.5134, Bibcode: 2009A&A...501..297Z, doi: 10.1051/0004-6361/200811147, S2CID  14969137.
  8. ^ a b Abt, Helmut A.; et al. (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode: 2002ApJ...573..359A, doi: 10.1086/340590
  9. ^ "57 Cyg". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 January 2019.
  10. ^ Tapia, M.; Smith, R. C. (November 1979), "On the spectroscopic binary 57 Cygni", Monthly Notices of the Royal Astronomical Society, 189 (3): 551–561, Bibcode: 1979MNRAS.189..551T, doi: 10.1093/mnras/189.3.551.