Astronomy:Beta Lupi

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Short description: Star in the constellation of Lupus
Beta Lupi
Lupus IAU.svg
Red circle.svg
Location of β Lupus (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Lupus
Right ascension  14h 58m 31.92536s[1]
Declination −43° 08′ 02.2699″[1]
Apparent magnitude (V) 2.68[2]
Characteristics
Spectral type B2 III[3]
U−B color index −0.902[4]
B−V color index −0.226[4]
Variable type β Cep[5]
Astrometry
Radial velocity (Rv)+0.1 ± 1.0[3] km/s
Proper motion (μ) RA: −35.78[1] mas/yr
Dec.: −39.83[1] mas/yr
Parallax (π)8.52 ± 0.18[1] mas
Distance383 ± 8 ly
(117 ± 2 pc)
Absolute magnitude (MV)−3.3[6]
Details
Mass8.8±0.2[7] M☉
Radius6.6[8] R☉
Luminosity10,000[6] L☉
Surface gravity (log g)3.76[6] cgs
Temperature24,090[9] K
Metallicity [Fe/H]−0.35±0.11[5] dex
Rotational velocity (v sin i)92[3] km/s
Age24.6±2.7[7] Myr
Other designations
Kekouan, β Lup, CD−42° 9853, FK5 552, HD 132058, HIP 73273, HR 5571, SAO 225335[10]
Database references
SIMBADdata

Beta Lupi (Latinized from β Lupi) or Kekouan (/ˈkɛkwɑːn/), is a star in the southern constellation of Lupus. It has an apparent visual magnitude of 2.7,[2] making it readily visible to the naked eye. Based upon parallax measurements, this star is located at a distance of about 383 light-years (117 parsecs) from Earth.[2]

Properties

The stellar classification of B2 III indicates this is a giant star.[3] The effective temperature of the star's outer envelope is 24,090 K,[9] giving it the blue-white hue of a B-type star.[11] With an age of around 25 million years,[7] it is near the end of its hydrogen phase, where hydrogen is fused into the element helium, and transferring into a red supergiant star. At about 8.8[7] solar masses, it may have enough mass to end its life as a Type II supernova, but there is the possibility of Beta Lupi becoming a white dwarf.[12]

This is a multi-period Beta Cephei variable with a dominant oscillation period of 0.232 days.[5] It is a proper motion member of the Upper Centaurus–Lupus sub-group in the Scorpius–Centaurus OB association, the nearest such co-moving association of massive stars to the Sun.[6] Beta Lupi has a high proper motion of more than 50 mas per year, suggesting a significant transverse velocity.[13]

It is positioned about 1.3° SSW of the supernova remnant SN 1006.[14]

Name

In Chinese, 騎官 (Qí Guān), meaning Imperial Guards, refers to an asterism consisting of β Lupi, γ Lupi, δ Lupi, κ Centauri, λ Lupi, ε Lupi, μ Lup, π Lupi, ο Lupi and α Lupi.[15] Consequently, the Chinese name for β Lupi itself is 騎官四 (Qí Guān sì, English: the Fourth Star of Imperial Guards.).[16] From the French rendering of this Chinese name derives the traditional European name Kekouan (Ke Kwan).[17]

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V 
  2. ↑ 2.0 2.1 2.2 Wielen, R. et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg (Astronomisches Rechen-Institut Heidelberg) 35 (35): 1, Bibcode: 1999VeARI..35....1W 
  3. ↑ 3.0 3.1 3.2 3.3 Jilinski, E. et al. (March 2006), "Radial velocity measurements of B stars in the Scorpius–Centaurus association", Astronomy and Astrophysics 448 (3): 1001–1006, doi:10.1051/0004-6361:20041614, Bibcode: 2006A&A...448.1001J 
  4. ↑ 4.0 4.1 Gutierrez-Moreno, Adelina; Moreno, Hugo (June 1968), "A photometric investigation of the Scorpio-Centaurus association", Astrophysical Journal Supplement 15: 459, doi:10.1086/190168, Bibcode: 1968ApJS...15..459G 
  5. ↑ 5.0 5.1 5.2 Daszyńska-Daszkiewicz, J.; Niemczura, E. (April 2005), "Metallicity of mono- and multiperiodic β Cephei stars", Astronomy and Astrophysics 433 (3): 1031–1035, doi:10.1051/0004-6361:20040397, Bibcode: 2005A&A...433.1031D 
  6. ↑ 6.0 6.1 6.2 6.3 de Geus, E. J.; de Zeeuw, P. T.; Lub, J. (June 1989), "Physical parameters of stars in the Scorpio-Centaurus OB association", Astronomy and Astrophysics 216 (1–2): 44–61, Bibcode: 1989A&A...216...44D 
  7. ↑ 7.0 7.1 7.2 7.3 Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society 410 (1): 190–200, doi:10.1111/j.1365-2966.2010.17434.x, Bibcode: 2011MNRAS.410..190T 
  8. ↑ Underhill, A. B. et al. (November 1979), "Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars", Monthly Notices of the Royal Astronomical Society 189 (3): 601–605, doi:10.1093/mnras/189.3.601, Bibcode: 1979MNRAS.189..601U 
  9. ↑ 9.0 9.1 Zorec, J. et al. (July 2009), "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into Teff", Astronomy and Astrophysics 501 (1): 297–320, doi:10.1051/0004-6361/200811147, Bibcode: 2009A&A...501..297Z 
  10. ↑ "bet Lup -- Variable Star", SIMBAD (Centre de Données astronomiques de Strasbourg), http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Beta+Lupi, retrieved 2012-01-16 
  11. ↑ "The Colour of Stars", Australia Telescope, Outreach and Education (Commonwealth Scientific and Industrial Research Organisation), December 21, 2004, archived from the original on 2012-03-18, https://web.archive.org/web/20120318151427/http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html, retrieved 2012-01-16 
  12. ↑ Kaler, James B. (2007), "Beta Lupi", Stars (University of Illinois), archived from the original on 2011-07-16, https://web.archive.org/web/20110716072207/http://www.astro.illinois.edu/~jkaler/sow/betalup.html, retrieved 2009-07-03 
  13. ↑ Jiménez-Esteban, F. M.; Caballero, J. A.; Solano, E. (January 2011), "Identification of blue high proper motion objects in the Tycho-2 and 2MASS catalogues using Virtual Observatory tools", Astronomy and Astrophysics 525: A29, doi:10.1051/0004-6361/201015223, Bibcode: 2011A&A...525A..29J 
  14. ↑ Sinnott, Roger W.; Perryman, Michael A. C. (1997), Millennium Star Atlas, 2, Sky Publishing Corporation and the European Space Agency, p. 929, ISBN 0-933346-83-2. 
  15. ↑ (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.
  16. ↑ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 , Hong Kong Space Museum. Accessed on line November 23, 2010.]
  17. ↑ Richard Hinckley Allen: Star Names — Their Lore and Meaning: Lupus

External links



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