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Zeta Draconis

From Wikipedia, the free encyclopedia
Binary star in the constellation Draco
ζ Draconis
Location of ζ Draconis (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationDraco
Right ascension17h 08m 47.19596s[1]
Declination+65° 42′ 52.8634″[1]
Apparent magnitude (V)+3.17[2]
Characteristics
Spectral typeB6 III[3]
U−Bcolor index−0.43[2]
B−Vcolor index−0.11[2]
Astrometry
Radial velocity (Rv)−17[4] km/s
Proper motion (μ)RA: –20.43[1]mas/yr
Dec.: +19.61[1]mas/yr
Parallax (π)9.93±0.35 mas[1]
Distance330 ± 10 ly
(101 ± 4 pc)
Absolute magnitude (MV)−1.88[5]
Details
A
Mass5.940±1.134[6] M
Radius6.19±0.49[7] R
Luminosity883[8] L
Surface gravity (log g)4.24[3] cgs
Temperature15,000±800[7] K
Metallicity [Fe/H]−0.95[3] dex
Rotational velocity (v sin i)55[9] km/s
B
Mass3.645±0.770[6] M
Other designations
22 Draconis,BD+65 1170,FK5 639,HD 155763,HIP 83895,HR 6396,SAO 17365,WDS 17088+6543[10]
Database references
SIMBADdata

Zeta Draconis (ζ Draconis, abbreviatedZet Dra,ζ Dra) is abinary star in the northerncircumpolar constellation ofDraco. With anapparent visual magnitude of +3.17,[2] it is thefifth-brightest member of this generally faint constellation. Its distance from theSun has been measured using theparallax technique, yielding an estimate of roughly 330light-years (100parsecs).[1]

The two components are designated Zeta Draconis A (formally namedAldhibah/ælˈdbə/, after the traditional name of the system)[11] and B.

Nomenclature

[edit]

ζ Draconis (Latinised toZeta Draconis) is the system'sBayer designation. The designations of the two components asZeta Draconis A andB derives from the convention used by the Washington Multiplicity Catalog (WMC) formultiple star systems, and adopted by theInternational Astronomical Union (IAU).[12]

Zeta Draconis has the oldArabic name الذئبal-dhiʼb "the wolf" or "the hyena", given in its feminine form "Al Dhiʼbah" (ذئبة) in Allen (1899) (though he mistranslated it as plural "hyenas", which would be الضباعal-ḍibāʽ).[13] It shares the dual form of the name, الذئبينal-dhiʼbayn, withEta Draconis.[14] It is also known asNodus III (Third Knot, the knot being a loop in the tail of Draco).[15]

In 2016, the IAU organized aWorking Group on Star Names (WGSN)[16] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entiremultiple systems.[17] It approved the nameAldhibah for the component Zeta Draconis A on 5 September 2017. It also approved the nameAthebyne for Eta Draconis A on the same date. Both are now so included in the List of IAU-approved Star Names.[11]

Zeta Draconis is mentioned inHindu texts asTara who was a celestialgoddess married to LordBrhaspati. A divine epic was played out in the night sky when LordChandra, the moon, lusted after and abducted Tara, the blue pole star of Brhaspati, the planetJupiter. By the completion of the epic Tara gives birth to LordBudha, orMercury.[18]

InChinese,紫微左垣 (Zǐ Wēi Zuǒ Yuán), meaningLeft Wall of Purple Forbidden Enclosure, refers to an asterism consisting of Zeta Draconis,Iota Draconis, Eta Draconis,Theta Draconis,Upsilon Draconis,73 Draconis,Gamma Cephei and23 Cassiopeiae.[19] Consequently, theChinese name for Zeta Draconis itself is紫微左垣四 (Zǐ Wēi Zuǒ Yuán sì, English:the Fourth Star of Left Wall of Purple Forbidden Enclosure),[20] representing上弼 (Shǎngbì), meaningThe First Minister.[21] 上弼 (Shǎngbì) is westernized intoShang Pih by R.H. Allen with meaning "the Higher Minister".[22]

Properties

[edit]

Zeta Draconis A is agiant star with astellar classification of B6 III.[3] Compared to the Sun, this star is about six timeslarger[7] and moremassive,[6] and is radiating 880 times as muchluminosity.[8] This energy is being emitted from the star'souter envelope at aneffective temperature of nearly 13,400K.[3] Theazimuthalrotation velocity along the equator is at least 55 km/s.[9]

The northecliptic pole is located atright ascension 18h anddeclination +66.5°.[23] This is located roughly midway betweenDelta Draconis and Zeta Draconis.[24] The north ecliptic pole almost coincides with the south celestial pole ofVenus; Zeta Draconis is also the north pole star ofJupiter.[25]

References

[edit]
  1. ^abcdefvan Leeuwen, F. (November 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. ^abcdJohnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars",Communications of the Lunar and Planetary Laboratory,4 (99): 99,Bibcode:1966CoLPL...4...99J.
  3. ^abcdeCenarro, A. J.; et al. (2007), "Medium-resolution Isaac Newton Telescope Library of Empirical Spectra – II. The Stellar Atmospheric Parameters",Monthly Notices of the Royal Astronomical Society,374 (2):664–690,arXiv:astro-ph/0611618,Bibcode:2007MNRAS.374..664C,doi:10.1111/j.1365-2966.2006.11196.x,S2CID 119428437.
  4. ^Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.),Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto:International Astronomical Union, p. 57,Bibcode:1967IAUS...30...57E.
  5. ^Huang, W.; et al. (2012), "A catalogue of Paschen-line profiles in standard stars",Astronomy & Astrophysics,547: A62,arXiv:1210.7893,Bibcode:2012A&A...547A..62H,doi:10.1051/0004-6361/201219804,S2CID 119286159.
  6. ^abcMartin, C.; Mignard, F.; Hartkopf, W. I.; McAlister, H. A. (1998-12-01), "Mass determination of astrometric binaries with Hipparcos - III. New results for 28 systems",Astronomy and Astrophysics Supplement Series,133 (2):149–162,doi:10.1051/aas:1998459,ISSN 0365-0138.
  7. ^abcGordon, Kathryn D.; et al. (2019), "Angular Sizes, Radii, and Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array",The Astrophysical Journal,873 (1): 91,Bibcode:2019ApJ...873...91G,doi:10.3847/1538-4357/ab04b2,S2CID 125181833.
  8. ^abMcDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017-10-01)."Fundamental parameters and infrared excesses of Tycho-Gaia stars".Monthly Notices of the Royal Astronomical Society.471:770–791.arXiv:1706.02208.Bibcode:2017MNRAS.471..770M.doi:10.1093/mnras/stx1433.ISSN 0035-8711.Zeta Draconis' database entry atVizieR.
  9. ^abRoyer, F.; et al. (October 2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i",Astronomy and Astrophysics,393:897–911,arXiv:astro-ph/0205255,Bibcode:2002A&A...393..897R,doi:10.1051/0004-6361:20020943,S2CID 14070763.
  10. ^"Zet Dra",SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved2009-10-10.
  11. ^ab"Naming Stars". IAU.org. Retrieved16 December 2017.
  12. ^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].
  13. ^Allen, Richard Hinckley (1899),Star-names and their meanings, New York: G. E. Stechert, p. 210.
  14. ^Rumrill, H. B. (June 1936), "Star Name Pronunciation",Publications of the Astronomical Society of the Pacific,48 (283):139–154,Bibcode:1936PASP...48..139R,doi:10.1086/124681,S2CID 120743052.
  15. ^Kaler, Jim,"Al Dhibain ("The Posterior")",Stars, University of Illinois, retrieved2009-10-12.
  16. ^"IAU Working Group on Star Names (WGSN)". Retrieved22 May 2016.
  17. ^"WG Triennial Report (2015-2018) - Star Names"(PDF). p. 5. Retrieved2018-07-14.
  18. ^George Mason Williams (2003).Handbook of Hindu Mythology. ABC-CLIO. p. 91.ISBN 1576071065. Retrieved17 July 2015.
  19. ^(in Chinese)中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005,ISBN 978-986-7332-25-7.
  20. ^(in Chinese)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 10 日Archived 2011-05-21 at theWayback Machine
  21. ^(in Chinese)English-Chinese Glossary of Chinese Star Regions, Asterisms and Star NameArchived August 10, 2010, at theWayback Machine, Hong Kong Space Museum. Accessed on line November 23, 2010.
  22. ^Star Name - R.H. Allen p. 210
  23. ^Chartrand, Mark R.; Wimmer, Helmut K. (2001),Night Sky: A Guide To Field Identification, Macmillan, p. 12,ISBN 1-58238-126-7.
  24. ^Young, Charles Augustus (1919),Anne Sewell Young (ed.),The Elements of Astronomy: a Textbook, Ginn and company, p. 69, retrieved2009-10-12.
  25. ^Sharrah, Paul C. (1975)."Pole Stars of Other Planets"(PDF).Arkansas Academy of Sciences Proceedings.XXIX:62–63.


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