Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Taygeta

Coordinates:Sky map03h 45m 12.49578s, +24° 28′ 02.2097″
From Wikipedia, the free encyclopedia
Triple star system in the constellation Taurus
Taygeta
Image of the Pleiades star cluster
Taygeta in the Pleiades cluster (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationTaurus
Right ascension03h 45m 12.49578s[1]
Declination+24° 28′ 02.2097″[1]
Apparent magnitude (V)4.30[2]
Characteristics
Evolutionary stagesubgiant[3]
Spectral typeB6IV[4] + ?[5]
U−Bcolor index−0.48[6]
B−Vcolor index−0.12[6]
Astrometry
Radial velocity (Rv)10.1[7] km/s
Proper motion (μ)RA: +21.24±0.38[1]mas/yr
Dec.: −40.56±0.35[1]mas/yr
Parallax (π)7.97±0.33 mas[1]
Distance410 ± 20 ly
(125 ± 5 pc)
Details
Taygeta
Mass4.41±0.09[8] M
Radius4.36±0.14[8] R
Luminosity600[9] L
Surface gravity (log g)3.772±0.113[8] cgs
Temperature13,696±222[8] K
Rotational velocity (v sin i)105±16[8] km/s
19 Tauri Ab
Mass3.2[9] M
Luminosity150[9] L
Surface gravity (log g)4.2[8] cgs
Temperature8,306[8] K
Other designations
q Tauri,19 Tauri,HR 1145,HD 23338,BD+24°547,HIP 17531,SAO 76140, GC 4486, BDS 1848, CCDM 03452+2429[10]
Database references
SIMBADdata

Taygeta is adouble star in theconstellation ofTaurus and a member of thePleiadesopen star cluster (M45).

It consists of abinary pair designated 19 Tauri A together with a single star visual companion, 19 Tauri B. 'A's' two components are themselves designated 19 Tauri Aa (officially namedTaygeta/tˈɪətə/,[11] the traditional name for the entire system)[12] and Ab.

Based onparallax measurements obtained during theHipparcos mission, Taygeta is approximately 410light-years from theSun.

Nomenclature

[edit]

19 Tauri is the system'sFlamsteed designation. It also bears the little-usedBayer designationq Tauri. The designations of the two constituents as19 Tauri A andB, and those ofA's components -19 Tauri Aa andAb - derive from the convention used by the Washington Multiplicity Catalog (WMC) formultiple star systems, and adopted by theInternational Astronomical Union (IAU).[13]

The system bore the traditional nameTaygeta (orTaygete).[14]Taygete was one of thePleiades sisters inGreek mythology. In 2016, the IAU organized aWorking Group on Star Names (WGSN)[15] to catalogue and standardize proper names for stars. The WGSN approved the nameTaygeta for the component 19 Tauri Aa on 21 August 2016 and it is now so included in the List of IAU-approved Star Names.[12]

Properties

[edit]

Taygeta has anapparent magnitude of +4.30 and presents as a blue-whiteB-typesubgiant. It has been used as a standard star for that spectral type.[4] It is aspectroscopic binary, whose component stars have magnitudes of +4.6 and +6.1. They are separated by 0.012arcseconds and complete oneorbit every 1313 days. The subgiant primary is one of just a handful of stars in the young Pleiades cluster that haveevolved away from themain sequence.[3]

The 8th magnitudevisual companion, 19 Tauri B, is 69 arcseconds away. It is thought to be a yellow star somewhat more massive and larger than the Sun, and further away than the Pleiades cluster.[16]

Taygeta was once reported to be variable,[17] but has since been measured to be very nearly constant.[18][19]

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.Vizier catalog entry
  2. ^Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".Vizier Online Data Catalog.2237.Bibcode:2002yCat.2237....0D.
  3. ^abMazzei, P.; Pigatto, L. (1989). "The Pleiades'age and the sequential star formation".Astronomy and Astrophysics.213.Bibcode:1989A&A...213L...1M.
  4. ^abMorgan, W. W.; Keenan, P. C. (1973). "Spectral Classification".Annual Review of Astronomy and Astrophysics.11: 29.Bibcode:1973ARA&A..11...29M.doi:10.1146/annurev.aa.11.090173.000333.
  5. ^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.
  6. ^abPenston M.J. (1973)."Photoelectric UBV observations made on the Palomar 20-inch telescope".Mon. Not. R. Astron. Soc.164 (2):133–154.Bibcode:1973MNRAS.164..133P.doi:10.1093/mnras/164.2.133.
  7. ^Torres, Guillermo (2020)."Spectroscopic Monitoring of Rapidly Rotating Early-type Stars in the Pleiades Cluster".The Astrophysical Journal.901 (2): 91.arXiv:2008.08590.Bibcode:2020ApJ...901...91T.doi:10.3847/1538-4357/abb136.
  8. ^abcdefgWhite, T. R.; et al. (2017)."Beyond the Kepler/K2 bright limit: Variability in the seven brightest members of the Pleiades".Monthly Notices of the Royal Astronomical Society.471 (3):2882–2901.arXiv:1708.07462.Bibcode:2017MNRAS.471.2882W.doi:10.1093/mnras/stx1050.S2CID 119221178.
  9. ^abcProfessor James B. (Jim) Kaler."TAYGETA (19 Tauri)". University of Illinois. Retrieved2014-08-18.
  10. ^"* q Tau".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2014-08-18.
  11. ^Davis, George A. (1944). "The pronunciations, derivations, and meanings of a selected list of star names".Popular Astronomy.52:8–30.
  12. ^ab"Naming Stars". IAU.org. Retrieved5 March 2018.
  13. ^Hessman, F. V.; Dhillon, V. S.; Winget, D. E.; Schreiber, M. R.; Horne, K.; Marsh, T. R.; Guenther, E.; Schwope, A.; Heber, U. (2010). "On the naming convention used for multiple star systems and extrasolar planets".arXiv:1012.0707 [astro-ph.SR].
  14. ^Allen, Richard Hinckley (1899).Star-names and their meanings. G. E. Stechert. p. 407. Retrieved2009-10-10.
  15. ^"IAU Working Group on Star Names (WGSN)".International Astronomical Union. Retrieved22 May 2016.
  16. ^Huber, Daniel; Bryson, Stephen T; Haas, Michael R; Barclay, Thomas; Barentsen, Geert; Howell, Steve B; Sharma, Sanjib; Stello, Dennis; Thompson, Susan E (2016)."The K2 Ecliptic Plane Input Catalog (EPIC) and Stellar Classifications of 138,600 Targets in Campaigns 1-8".The Astrophysical Journal Supplement Series.224 (1): 2.arXiv:1512.02643.Bibcode:2016ApJS..224....2H.doi:10.3847/0067-0049/224/1/2.S2CID 118621218.
  17. ^Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S.1.Bibcode:2009yCat....102025S.
  18. ^Percy, John R.; Wilson, Joseph B. (2000)."Another Search for Maia Variable Stars".The Publications of the Astronomical Society of the Pacific.112 (772): 846.Bibcode:2000PASP..112..846P.doi:10.1086/316577.
  19. ^Adelman, S. J. (2001)."Research Note Hipparcos photometry: The least variable stars".Astronomy and Astrophysics.367:297–298.Bibcode:2001A&A...367..297A.doi:10.1051/0004-6361:20000567.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Astronomical events
Retrieved from "https://en.wikipedia.org/w/index.php?title=Taygeta&oldid=1284759926"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp