Jump to content

Beta2 Sagittarii

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Cuddlyopedia (talk | contribs) at 11:07, 5 February 2018 (Redrafting with more information as to nomenclature). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

For other stars with this Bayer designation, see β Sagittarii.
Beta² Sagittarii
Diagram showing star positions and boundaries of the Sagittarius constellation and its surroundings
Location of β Sagittarii (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Sagittarius
Right ascension 19h 23m 13.13745s[1]
Declination −44° 47′ 59.2051″[1]
Apparent magnitude (V) +4.29[2]
Characteristics
Spectral type F2/3 V[3] or F2 III[4]
U−B color index +0.07[2]
B−V color index +0.34[2]
Astrometry
Radial velocity (Rv)+19.0[5] km/s
Proper motion (μ) RA: +93.45[1] mas/yr
Dec.: −54.09[1] mas/yr
Parallax (π)24.31 ± 0.19 mas[1]
Distance134 ± 1 ly
(41.1 ± 0.3 pc)
Absolute magnitude (MV)+1.20[6]
Details
Mass1.43[7] M☉
Luminosity20[8] L☉
Surface gravity (log g)3.57[7] cgs
Temperature7,035±239[7] K
Metallicity [Fe/H]−0.54[5] dex
Rotational velocity (v sin i)155[9] km/s
Age933[7] Myr
Other designations
Arkab Posterior, β² Sgr, CD−45° 13171, HD 181623, HIP 95294, HR 7343, SAO 229654[10]
Database references
SIMBADdata

Beta² Sagittarii (β² Sagittarii, abbreviated Beta² Sgr, β² Sgr) is a star in the zodiac constellation of Sagittarius. It is visible to the naked eye, having an apparent visual magnitude of +4.29.[2] Based upon an annual parallax shift of 24.31 mas as seen from Earth,[1] it is located 134 light-years from the Sun.

Based upon variations in its proper motion, this is a probable astrometric binary system.[11] As such, its two components would be designated Beta² Sagittarii A (also named Arkab Posterior[12]) and B

Nomenclature

β² Sagittarii (Latinised to Beta² Sagittarii) is the system's Bayer designation. The designations of the two components as Beta² Sagittarii A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[13]

In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[14] to catalog and standardize proper names for stars. The WGSN approved the name Arkab Posterior for Beta² Sagittarii on 5 October 2016 and it is now so included in the List of IAU-approved Star Names.[12] For such names relating to members of multiple star systems, and where a component letter (from e.g. Washington Double Star Catalog) is not explicitly listed, the WGSN says that the name should be understood to be attributed to the brightest component by visual brightness.[15]

In Chinese, 天淵 (Tiān Yuān), meaning Celestial Spring, refers to an asterism consisting of Beta² Sagittarii, Beta¹ Sagittarii and Alpha Sagittarii. Consequently, Beta² Sagittarii itself is known as 天淵一 (Tiān Yuān yī, Template:Lang-en.)[16]

Properties

Houk (1978) categorizes the visible component (Beta² Sagittarii A) as an F-type main-sequence star with a stellar classification of F2/3 V.[3] However, Malaroda (1975) lists it as an F-type giant star.[4] It is spinning rapidly with a projected rotational velocity of 155 km/s. This is giving it an oblate shape with an equatorial bulge that is 22% larger than the polar radius.[9] Beta² Sagittarii has an estimated 1.4[7] times the mass of the Sun and is around 933[7] million years old.

References

  1. ^ a b c d e f van 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.
  2. ^ a b c d Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99), Bibcode:1966CoLPL...4...99J.
  3. ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H.
  4. ^ a b Malaroda, S. (August 1975), "Study of the F-type stars. I. MK spectral types", Astronomical Journal, 80: 637–641, Bibcode:1975AJ.....80..637M, doi:10.1086/111786.
  5. ^ a b Casagrande, L.; et al. (2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics, 530 (A138): 21, arXiv:1103.4651, Bibcode:2011A&A...530A.138C, doi:10.1051/0004-6361/201016276.
  6. ^ Anderson, 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.
  7. ^ a b c d e f David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv:1501.03154, Bibcode:2015ApJ...804..146D, doi:10.1088/0004-637X/804/2/146.
  8. ^ McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x.{{citation}}: CS1 maint: unflagged free DOI (link)
  9. ^ a b Belle, G. T. (2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review, 20: 51, arXiv:1204.2572, Bibcode:2012A&ARv..20...51V, doi:10.1007/s00159-012-0051-2.
  10. ^ "bet02 Sgr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-07-10.{{cite web}}: CS1 maint: postscript (link)
  11. ^ 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.{{citation}}: CS1 maint: unflagged free DOI (link)
  12. ^ a b "Naming Stars". IAU.org. Retrieved 16 December 2017.
  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. ^ "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
  15. ^ "Bulletin of the IAU Working Group on Star Names, No. 2" (PDF). Retrieved 16 December 2017.
  16. ^ Template:Zh icon AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 2 日
Retrieved from "https://en.wikipedia.org/w/index.php?title=Beta2_Sagittarii&oldid=824109825"