Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

22 Cygni

From Wikipedia, the free encyclopedia
Star in the constellation Cygnus
22 Cygni
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus
Right ascension19h 55m 51.75718s[1]
Declination+38° 29′ 12.154″[1]
Apparent magnitude (V)4.95[2]
Characteristics
Spectral typeB5 IV[3]
B−Vcolor index−0.086±0.009[2]
Astrometry
Radial velocity (Rv)−14.8±2.2[4] km/s
Proper motion (μ)RA: +6.559[1]mas/yr
Dec.: −0.469[1]mas/yr
Parallax (π)3.0418±0.2388 mas[1]
Distance1,070 ± 80 ly
(330 ± 30 pc)
Absolute magnitude (MV)−3.18[2]
Orbit[5]
Period (P)78.2±0.4 d
Eccentricity (e)0.17±0.13
Periastronepoch (T)2443734.5±2.1 JD
Argument of periastron (ω)
(secondary)
139±11°
Semi-amplitude (K1)
(primary)
20.7±3.1 km/s
Details
22 Cyg A
Mass7.9±0.4[6] M
Radius5.6[7] R
Luminosity7,305[8] L
Surface gravity (log g)3.35[9] cgs
Temperature15,200[8] K
Rotational velocity (v sin i)30[10] km/s
Age37.3±4.2[6] Myr
Other designations
22 Cyg,BD+38°3817,HD 188892,HIP 98068,HR 7613,SAO 69101[11]
Database references
SIMBADdata

22 Cygni is abinary star system in the northernconstellation ofCygnus. It is visible to the naked eye as a faint, blue-white hued star with anapparent visual magnitude of 4.95.[2] The annualshift of3.0 mas[1] yields a distance estimate of around 1,070 light years. It is moving closer to the Earth with a heliocentricradial velocity of −15 km/s.[4]

This is a single-linedspectroscopic binary with anorbital period of 78.2 days and aneccentricity of roughly 0.17.[5] The visible component has astellar classification of B5 IV[3] that matches aB-typesubgiant star. It is 37[6] million years old with aprojected rotational velocity of 30[10] km/s and has an essentially solarmetallicity, within the margin of error.[9] The star has eight[6] times themass of the Sun and about 5.6[7] times theSun's radius. It is radiating 7,305[8] times theSun's luminosity from itsphotosphere at aneffective temperature of 15,200 K.[8]

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. ^abcdAnderson, 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. ^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. ^abAbt, Helmut A.; et al. (October 1990), "The Frequency and Formation Mechanism of B2--B5 Main-Sequence Binaries",Astrophysical Journal Supplement,74: 551,Bibcode:1990ApJS...74..551A,doi:10.1086/191508.
  6. ^abcdTetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun",Monthly Notices of the Royal Astronomical Society,410 (1):190–200,arXiv:1007.4883,Bibcode:2011MNRAS.410..190T,doi:10.1111/j.1365-2966.2010.17434.x,S2CID 118629873.
  7. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (Third ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  8. ^abcdHohle, M. M.; et al. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants",Astronomische Nachrichten,331 (4): 349,arXiv:1003.2335,Bibcode:2010AN....331..349H,doi:10.1002/asna.200911355,S2CID 111387483.
  9. ^abAdelman, 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.
  10. ^abAbt, 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
  11. ^"22 Cyg".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-01-09.
Stars
Bayer
Flamsteed
Variable
HR
HD
Gliese
Kepler
WR
Other
Star
clusters
Association
Open
Molecular
clouds
Nebulae
Dark
H II
Planetary
WR
SNR
Galaxies
NGC
Other
Exoplanets
Kepler
Other
Exomoons
Kepler
Retrieved from "https://en.wikipedia.org/w/index.php?title=22_Cygni&oldid=1234889366"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp