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HandWiki. Zeta Ursae Majoris. Encyclopedia. Available online: https://encyclopedia.pub/entry/27953 (accessed on 15 November 2024).
HandWiki. Zeta Ursae Majoris. Encyclopedia. Available at: https://encyclopedia.pub/entry/27953. Accessed November 15, 2024.
HandWiki. "Zeta Ursae Majoris" Encyclopedia, https://encyclopedia.pub/entry/27953 (accessed November 15, 2024).
HandWiki. (2022, September 29). Zeta Ursae Majoris. In Encyclopedia. https://encyclopedia.pub/entry/27953
HandWiki. "Zeta Ursae Majoris." Encyclopedia. Web. 29 September, 2022.
Zeta Ursae Majoris
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The content is sourced from: https://handwiki.org/wiki/Astronomy:Zeta_Ursae_Majoris

Mizar is a 2nd magnitude star in the handle of the Big Dipper asterism in the constellation of Ursa Major. It has the Bayer designation ζ Ursae Majoris (Latinised as Zeta Ursae Majoris). It forms a well-known naked eye double star with the fainter star Alcor, and is itself a quadruple star system. The whole system lies about 83 light-years away from the Sun, as measured by the Hipparcos astrometry satellite, and is part of the Ursa Major Moving Group.

mizar alcor double star

1. Nomenclature

ζ Ursae Majoris (Latinised to Zeta Ursae Majoris and abbreviated to ζ UMa or Zeta UMa) is Mizar's Bayer designation. It also has the Flamsteed designation 79 Ursae Majoris.

The traditional name Mizar derives from the Arabic المئزر miʼzar meaning 'apron; wrapper, covering, cover'.[1] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[2] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[3] included a table of the first two batches of names approved by the WGSN; which included Mizar for ζ UMa. According to IAU rules, the name Mizar strictly only applies to component Aa,[4] although it is traditionally and popularly used for all four stars making up the single naked-eye star.[5][6]

2. Stellar System

Figure 1. The Big Dipper's bowl and part of the handle photographed from the International Space Station. Mizar and Alcor are at the upper right. By NASA - http://spaceflight.nasa.gov/gallery/images/station/crew-6/html/iss006e40545.htmlTransferred from en.wikipedia to Commons. Transfer was stated to be made by User:Blast., Public Domain, https://commons.wikimedia.org/w/index.php?curid=3185602

Mizar is a visual double with a separation of 14.4 arcseconds, each of which is a spectroscopic binary. Its combined apparent magnitude is 2.04. The two visible stars are referred to as ζ1 and ζ2 Ursae Majoris, or Mizar A and B. The spectroscopic components are generally referred to as Mizar Aa, Ab, Ba, and Bb. The stars all share a single Hipparcos designation of HIP 65378, but separate Bright Star Catalogue and Henry Draper Catalogue entries. Mizar, together with Alcor and many of the other bright stars in Ursa Major, is a member of the Ursa Major Moving Group.[7]

An easily split visual target, Mizar was the first telescopic binary discovered, most probably by Benedetto Castelli who in 1617 asked Galileo Galilei to observe it. Galileo then produced a detailed record of the double star.[8] Later, around 1650, Riccioli wrote of Mizar appearing as a double.[9] The secondary star (Mizar B) comes within 380 AU of the primary (Mizar A) and the two take thousands of years to revolve around each other.[10]

Mizar A was the first spectroscopic binary to be discovered, as part of Antonia Maury's spectral classification work, and an orbit was published in 1890. Some spectroscopic binaries cannot be visually resolved and are discovered by studying the spectral lines of the suspect system over a long period of time. The two components of Mizar A are both about 35 times as bright as the Sun, and revolve around each other in about 20 days 12 hours and 55 minutes. In 1908, Mizar B was also found to be a spectroscopic binary, its components completing an orbital period every six months.[11] In 1996, 107 years after their discovery, the components of the Mizar A binary system were imaged in extremely high resolution using the Navy Prototype Optical Interferometer.[12]

2.1. ζ1 Ursae Majoris

Figure 2. Radial velocity curves for the two almost identical components. By No machine-readable author provided. FredA assumed (based on copyright claims). - No machine-readable source provided. Own work assumed (based on copyright claims)., CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=407398

The two components of ζ1 Ursae Majoris (Mizar Aa and Ab) are observed to be identical, with the exception of slightly different radial velocity variations which indicate very slightly different masses.

The spectral lines of the two stars can be observed separately and both are given a spectral type of A2Vp. They are Ap stars, chemically peculiar due to stratification of some heavy elements in the photosphere of slowly-rotating hot stars. In this case, they show elevated abundances of strontium and silicon.[13]

With the assumption of identical physical properties for the two stars, they both have temperatures of 9,000 K, radii of 2.4 R☉, and bolometric luminosities of 33.3 L☉.[14] They are thought to be around 370 million years old.[15]

2.2. ζ2 Ursae Majoris

ζ2 Ursae Majoris is a single-lined spectroscopic binary, and the visible spectrum is of an Am star, named for their unusually strong lines of some metals. The spectral type of kA1h(eA)mA7IV-V is in a form used for metallic-lined stars: the type is A1 based on the calcium K lines, early A based on the hydrogen lines, and A7 based on lines of other metals. The luminosity class is ranked between main sequence and subgiant.

3. Other Names

Mizar is known as Vashistha one of the Saptarishi, in traditional Indian astronomy.[16]

Al-Sahja was the rhythmical form of the usual Suha. It appears as الخوّار al-Khawwar, 'the Faint One'.[5]

Chinese Taoism personifies ζ Ursae Majoris as the Lu star.

In Chinese, 北斗 (Běi Dǒu), meaning Northern Dipper, refers to an asterism consisting of ζ Ursae Majoris, α Ursae Majoris, β Ursae Majoris, γ Ursae Majoris, δ Ursae Majoris, ε Ursae Majoris and η Ursae Majoris. Consequently, ζ Ursae Majoris itself is known as 北斗六 Běi Dǒu liù, (English: the Sixth Star of Northern Dipper) and 開陽 Kāi Yáng, (English: Star of The Opener of Heat).[17]

Mizar is Chickadee and Alcor is his cooking pot in the Mi'kmaq myth of the great bear and the seven hunters.[18]

3.1. Military namesakes

  • USS Mizar is a cargo and passenger liner converted to a United States Navy ship
  • USNS Mizar, a United States Navy ship

References

  1. Wehr, Hans (1994). A Dictionary of Modern Written Arabic (Arabic-English) (4 ed.). Urbana, Illinois: Spoken Language Services. p. 17. ISBN 0879500034. 
  2. "IAU Working Group on Star Names (WGSN)". https://www.iau.org/science/scientific_bodies/working_groups/280/. Retrieved 22 May 2016. 
  3. "Bulletin of the IAU Working Group on Star Names, No. 1". http://www.pas.rochester.edu/~emamajek/WGSN/WGSN_bulletin1.pdf. Retrieved 28 July 2016. 
  4. "IAU Catalog of Star Names". http://www.pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt. Retrieved 28 July 2016. 
  5. Richard H. Allen (28 February 2013). Star Names: Their Lore and Meaning. Courier Corporation. ISBN 978-0-486-13766-7. https://books.google.com/books?id=vWDsybJzz7IC. 
  6. Guy Consolmagno; Dan M. Davis (19 October 2000). Turn Left at Orion: A Hundred Night Sky Objects to See in a Small Telescope - and How to Find Them. Cambridge University Press. pp. 83–. ISBN 978-1-139-45750-7. https://books.google.com/books?id=PexKTfPy3voC&pg=PA83. 
  7. Jones, Jeremy; White, R. J; Boyajian, T; Schaefer, G; Baines, E; Ireland, M; Patience, J; Ten Brummelaar, T et al. (2015). "The Ages of A-Stars. I. Interferometric Observations and Age Estimates for Stars in the Ursa Major Moving Group". The Astrophysical Journal 813: 58. doi:10.1088/0004-637X/813/1/58. Bibcode: 2015ApJ...813...58J.  https://dx.doi.org/10.1088%2F0004-637X%2F813%2F1%2F58
  8. Michael Marett-Crosby (28 June 2013). Twenty-Five Astronomical Observations That Changed the World: And How To Make Them Yourself. Springer Science & Business Media. pp. 32–. ISBN 978-1-4614-6800-4. https://books.google.com/books?id=0KRSphlvsqgC&pg=PA32. 
  9. Steven J. Dick (9 September 2013). Discovery and Classification in Astronomy: Controversy and Consensus. Cambridge University Press. pp. 117–. ISBN 978-1-107-03361-0. https://books.google.com/books?id=IT8oAAAAQBAJ&pg=PA117. 
  10. Robert Burnham (1978). Burnham's Celestial Handbook: An Observer's Guide to the Universe Beyond the Solar System. Courier Corporation. ISBN 978-0-486-23673-5. https://books.google.com/books?id=tBQoCSRdLAAC. 
  11. Mamajek, Eric E.; Kenworthy, Matthew A.; Hinz, Philip M.; Meyer, Michael R. (2010). "Discovery of a Faint Companion to Alcor Using MMT/AO 5 μm Imaging". The Astronomical Journal 139 (3): 919–925. doi:10.1088/0004-6256/139/3/919. Bibcode: 2010AJ....139..919M.  https://dx.doi.org/10.1088%2F0004-6256%2F139%2F3%2F919
  12. Benson, J. A; Hutter, D. J; Elias, N. M; Bowers, P. F; Johnston, K. J; Hajian, A. R; Armstrong, J. T; Mozurkewich, D et al. (1997). "Multichannel optical aperture synthesis imaging of zeta1 URSAE majoris with the Navy prototype optical interferometer". Astronomical Journal 114: 1221. doi:10.1086/118554. Bibcode: 1997AJ....114.1221B.  https://dx.doi.org/10.1086%2F118554
  13. Abt, H. A; Cardona, O (1984). "The nature of the visual companions of AP and AM stars". Astrophysical Journal 276: 266. doi:10.1086/161610. Bibcode: 1984ApJ...276..266A.  https://dx.doi.org/10.1086%2F161610
  14. Hummel, C. A.; Mozurkewich, D.; Armstrong, J. T.; Hajian, Arsen R.; Elias Ii, N. M.; Hutter, D. J. (1998). "Navy Prototype Optical Interferometer Observations of the Double Stars Mizar a and Matar". The Astronomical Journal 116 (5): 2536. doi:10.1086/300602. Bibcode: 1998AJ....116.2536H.  https://dx.doi.org/10.1086%2F300602
  15. Thureau, N. D; Greaves, J. S; Matthews, B. C; Kennedy, G; Phillips, N; Booth, M; Duchêne, G; Horner, J et al. (2014). "An unbiased study of debris discs around A-type stars with Herschel". Monthly Notices of the Royal Astronomical Society 445 (3): 2558. doi:10.1093/mnras/stu1864. Bibcode: 2014MNRAS.445.2558T.  https://dx.doi.org/10.1093%2Fmnras%2Fstu1864
  16. V.Chandran (1993-01-01). Astronomy Quiz Book. Pustak Mahal, 1993. ISBN 978-81-223-0366-7. https://books.google.com/books?id=8iPU8bZQQdsC. "... the seven rishis in the constellation Saptarishi (Ursa Major) ... In Vasishta (Zeta), its tiny companion star is named after Arundhati, the wife of Vasishta ... today known by their Arabic names Dubhe (Kratu), Merak (Pulaha), Phekda (Pulastya), Megrez (Atri), Benetnash (Marichi) and Mizar (Vasishta) ..." 
  17. "天文教育資訊網" (in zh). http://aeea.nmns.edu.tw/2006/0606/ap060615.html. Retrieved 2018-01-01. 
  18. "The Celestial Bear, A Micmac Legend". http://capebretonsmagazine.com/modules/publisher/item.php?itemid=71. Retrieved 2018-01-01. 
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