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41 Cygni

From Wikipedia, the free encyclopedia
Star in the constellation Cygnus
41 Cygni
Location of 41 Cyg (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus
Right ascension20h 29m 23.73561s[1]
Declination+30° 22′ 06.7968″[1]
Apparent magnitude (V)4.02[2]
Characteristics
Evolutionary stagesupergiant[3]
Spectral typeF5Ib-II[3]
B−Vcolor index+0.38[2]
Variable typeconstant[3]
Astrometry
Radial velocity (Rv)−18.20[4] km/s
Proper motion (μ)RA: 6.89[1]mas/yr
Dec.: −0.87[1]mas/yr
Parallax (π)4.24±0.16 mas[1]
Distance770 ± 30 ly
(236 ± 9 pc)
Absolute magnitude (MV)−3.32[5]
Details
Mass5.3±0.4[6] M
Radius27.01+2.51
−1.01
[7] R
Luminosity1,197±90[7] L
Surface gravity (log g)2.32±0.08[6] cgs
Temperature6533+126
−283
[7] K
Metallicity[Fe/H]0.00±0.07[6] dex
Rotational velocity (v sin i)9.5±2.0[3] km/s
Age85[6] Myr
Other designations
41 Cyg,BD+29°4057,HD 195295,HIP 101076,HR 7834,SAO 70095[8]
Database references
SIMBADdata

41 Cygni is a single[9]star in the northernconstellation ofCygnus, located near the southern border withVulpecula. It is visible to the naked eye as a faint, yellow-white hued star with anapparent visual magnitude of 4.02.[2] The star lies at a distance of around 770 light years from the Sun, based onparallax, and is drifting closer with aradial velocity of −18 km/s.[4]

This is a sharp-linedsupergiant star[10] with astellar classification of F5Ib-II.[3] It is 85[6] million years old with 5.3[6] times themass of the Sun and is spinning with aprojected rotational velocity of 9.5 km/s.[3] Having exhausted the supply of hydrogen at itscore, the star has expanded to 27[7] times theSun's radius. It is radiating about 1,200[7] times theSun's luminosity from its swollenphotosphere at aneffective temperature of 6,533 K.[7]

It is the brightest star in Cygnus without aBayer designation. It was once designatedi Cygni byJohn Flamsteed and was included in his Atlas Coelestis, but the designation is now dropped.[11]

References

[edit]
  1. ^abcdeVan 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. ^abcLuck, R. Earle (2014)."Parameters and Abundances in Luminous Stars".The Astronomical Journal.147 (6): 137.Bibcode:2014AJ....147..137L.doi:10.1088/0004-6256/147/6/137.
  3. ^abcdefGray, R. O.; et al. (April 2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars",The Astronomical Journal,121 (4):2148–2158,Bibcode:2001AJ....121.2148G,doi:10.1086/319956
  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. ^Kovtyukh, V. V.; et al. (2012)."Accurate luminosities from the oxygen λ7771-4 Å triplet and the fundamental parameters of F-G supergiants".Monthly Notices of the Royal Astronomical Society.423 (4): 3268.arXiv:1204.4115.Bibcode:2012MNRAS.423.3268K.doi:10.1111/j.1365-2966.2012.21117.x.S2CID 118683158.
  6. ^abcdefLyubimkov, Leonid S.; et al. (2010)."Accurate fundamental parameters for A-, F- and G-type Supergiants in the solar neighbourhood".Monthly Notices of the Royal Astronomical Society.402 (2): 1369.arXiv:0911.1335.Bibcode:2010MNRAS.402.1369L.doi:10.1111/j.1365-2966.2009.15979.x.S2CID 119096173.
  7. ^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.
  8. ^"41 Cyg".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-07-22.
  9. ^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.
  10. ^Adelman, S. J.; et al. (January 2008)."Elemental abundance analyses with DAO spectrograms: XXXI. The early F supergiants ν Her (F2 II) and 41 Cyg (F5 Ib-II)".Astronomische Nachrichten.329 (1):26–38.Bibcode:2008AN....329....4A.doi:10.1002/asna.200710863.
  11. ^Wagman, M. (August 1987), "Flamsteed's Missing Stars",Journal for the History of Astronomy,18 (3):209–223,Bibcode:1987JHA....18..209W,doi:10.1177/002182868701800305,S2CID 118445625.
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