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23 Cygni

From Wikipedia, the free encyclopedia
Star in the constellation Cygnus
23 Cygni
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus
Right ascension19h 53m 17.37873s[1]
Declination+57° 31′ 24.4810″[1]
Apparent magnitude (V)5.14[2]
Characteristics
Spectral typeB5 V[3]
U−Bcolor index+0.76[2]
B−Vcolor index−0.13[2]
Astrometry
Radial velocity (Rv)−31.6±1.6[4] km/s
Proper motion (μ)RA: +5.768[1]mas/yr
Dec.: +11.483[1]mas/yr
Parallax (π)5.9155±0.1728 mas[1]
Distance550 ± 20 ly
(169 ± 5 pc)
Absolute magnitude (MV)−1.30[5]
Details[2]
Mass4.7+0.64
−0.53
[6] M
Radius4.30±0.45 R
Luminosity611.53[5] L
Surface gravity (log g)3.82±0.08 cgs
Temperature14,893±214 K
Metallicity[Fe/H]−0.17±0.16 dex
Rotational velocity (v sin i)145 km/s
Age26+32
−19
[6] Myr
Other designations
23 Cyg,BD+57°2084,HD 188665,HIP 97870,HR 7608,SAO 32085,WDS J19533+5731[7]
Database references
SIMBADdata

23 Cygni is a single,[2] blue-white huedstar in the northernconstellationCygnus. It is a faint star, visible to the naked eye, with anapparent visual magnitude of 5.14.[2] The distance to this star, as estimated from its annualparallax shift of5.9 mas,[1] is about 550 light years. It is moving closer to the Earth with a heliocentricradial velocity of −32 km/s,[4] and is expected to come as near as 166 light-years in around 5.6 million years.[2] At that distance, the current star would be of magnitude 2.24.[8]

This is an ordinaryB-type main-sequence star of spectral type B5V, a star that is generating energy throughhydrogen fusion at itscore. It is roughly 26[2] million years old with 4.7[6] times themass of the Sun and 4.3 times theSun's radius.[2] The star has a high rate of spin, having aprojected rotational velocity of 145 km/s.[2] It is radiating 612[5] times theSun's luminosity from itsphotosphere at aneffective temperature of 14,893 K.[2]

References

[edit]
  1. ^abcdefBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  2. ^abcdefghijkFitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry",The Astronomical Journal,129 (3):1642–1662,arXiv:astro-ph/0412542,Bibcode:2005AJ....129.1642F,doi:10.1086/427855,S2CID 119512018.
  3. ^Hill, P. W.; Lynas-Gray, A. E. (September 1977), "UBV photometry and MK spectral classification of northern early-type stars at intermediate galactic latitudes.",Monthly Notices of the Royal Astronomical Society,180 (4):691–702,Bibcode:1977MNRAS.180..691H,doi:10.1093/mnras/180.4.691.
  4. ^abGontcharov, G. A. (2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system",Astronomy Letters,32 (11):759–771,arXiv:1606.08053,Bibcode:2006AstL...32..759G,doi:10.1134/S1063773706110065,S2CID 119231169.
  5. ^abcAnderson, 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.
  6. ^abcGullikson, Kevin; et al. (August 2016), "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars",The Astronomical Journal,152 (2): 13,arXiv:1604.06456,Bibcode:2016AJ....152...40G,doi:10.3847/0004-6256/152/2/40,S2CID 119179065, 40.
  7. ^"23 Cyg".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-01-09.
  8. ^At a distance (D) of 50.99 and an absolute magnitude (M) of −1.30, ignoringextinction (A), the apparent magnitude (m) would be:
    m = M + A + 5·log D + 5 ≈ −1.30 + 5·log 50.99 − 5 = 2.24
    Ref.:Dopita, Michael A.; Sutherland, Ralph S. (2004),Astrophysics of the Diffuse Universe, Astronomy and Astrophysics Library, Springer Science & Business Media, p. 296,ISBN 3540433627
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