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8 Cygni

From Wikipedia, the free encyclopedia
Star in the constellation Cygnus
8 Cygni
Observation data
EpochJ2000      EquinoxJ2000
ConstellationCygnus
Right ascension19h 31m 46.32184s[1]
Declination+34° 27′ 10.6874″[1]
Apparent magnitude (V)4.75[2]
Characteristics
Spectral typeB3 IV[3]
B−Vcolor index−0.155[2]
Astrometry
Radial velocity (Rv)−21.20±0.1[4] km/s
Proper motion (μ)RA: 1.16[1]mas/yr
Dec.: −3.47[1]mas/yr
Parallax (π)3.79±0.16 mas[1]
Distance860 ± 40 ly
(260 ± 10 pc)
Absolute magnitude (MV)−2.21[5]
Details
Mass6.1[5] M
Radius6.50[6] R
Luminosity2,291[5] L
Surface gravity (log g)3.58[5] cgs
Temperature16,300[5] K
Metallicity[Fe/H]+0.25[6] dex
Rotational velocity (v sin i)55[5] km/s
Age53[5] Myr
Other designations
8 Cygni,BD+34°3590,HD 184171,HIP 96052,HR 7426,SAO 68447.
Database references
SIMBADdata

8 Cygni is a single[7]star in the northernconstellation ofCygnus. Based upon itsparallax of 3.79 mas,[1] it is approximately 860light-years (260parsecs) away fromEarth. It is visible to the naked eye as a faint, bluish-white hued star with anapparent visual magnitude of about 4.7.[2] The star is moving closer to the Earth with a heliocentricradial velocity of −21 km/s.[4]

This is an agingsubgiant star, as indicated by itsspectral type of B3IV.[3] Itseffective temperature of 16,300K fits into the normal range ofB-type stars: 11,000 to 25,000 K. 8 Cygni is about twice as hot as theSun, and it is six times larger and many times brighter in comparison. Theelemental abundances are near solar.[8]

References

[edit]
  1. ^abcdefvan Leeuwen, F.; et al. (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. ^abcMermilliod, J.-C. (1986)."Compilation of Eggen's UBV data, transformed to UBV (unpublished)".Catalogue of Eggen's UBV Data.Bibcode:1986EgUBV........0M.
  3. ^abLesh, 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. ^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. ^abcdefgJin, Harim; Langer, Norbert; Lennon, Daniel J.; Proffitt, Charles R. (2024). "Boron depletion in Galactic early B-type stars reveals two different main sequence star populations".Astronomy and Astrophysics.690: A135.arXiv:2405.18266.Bibcode:2024A&A...690A.135J.doi:10.1051/0004-6361/202450896.
  6. ^abChallouf, M.; et al. (2014), "Improving the surface brightness-color relation for early-type stars using optical interferometry⋆",Astronomy & Astrophysics,570: A104,arXiv:1409.1351,Bibcode:2014A&A...570A.104C,doi:10.1051/0004-6361/201423772,S2CID 14624307.
  7. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  8. ^Adelman, Saul J. (June 1998)."Elemental abundance analyses with DAO spectrograms - XIX. The superficially normal B stars zeta Draconis, epsilon Lyrae, 8 Cygni and 22 Cygni".Monthly Notices of the Royal Astronomical Society.296 (4):856–862.Bibcode:1998MNRAS.296..856A.doi:10.1046/j.1365-8711.1998.01426.x.
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