Astronomy:Epsilon Centauri

From HandWiki
Short description: Star in the constellation Centaurus
ε Centauri
Location of ε Centauri (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Centaurus[1]
Right ascension  13h 39m 53.25774s[2]
Declination −53° 27′ 59.0081″[2]
Apparent magnitude (V) 2.29 - 2.31[3]
Characteristics
Spectral type B1 III[4]
U−B color index −0.92[5]
B−V color index −0.22[5]
Variable type β Cep[3]
Astrometry
Radial velocity (Rv)+3.0[6] km/s
Proper motion (μ) RA: −15.30[2] mas/yr
Dec.: −11.72[2] mas/yr
Parallax (π)7.63 ± 0.48[2] mas
Distance430 ± 30 ly
(131 ± 8 pc)
Absolute magnitude (MV)−3.29[1]
Details
Mass8.2[7] M☉
Radius5.8[8] R☉
Luminosity16,137[8] L☉
Surface gravity (log g)3.88[8] cgs
Temperature24,937[8] K
Metallicity [Fe/H]−0.14±0.10[9] dex
Rotational velocity (v sin i)140[10] km/s
Age16.3[11] Myr
Other designations
ε Cen, CPD−52°6655, FK5 504, HD 118716, HIP 66657, HR 5132, SAO 241047[12]
Database references
SIMBADdata

Epsilon Centauri is a star in the southern constellation of Centaurus. Its name is a Bayer designation that is Latinized from ε Centauri, and abbreviated Epsilon Cen or ε Cen. This is one of the brightest stars in the constellation with a slightly variable apparent visual magnitude of +2.30. Parallax measurements put it at a distance of around 430 light-years (130 parsecs) from Earth.

In Chinese, 南門 (Nán Mén), meaning Southern Gate, refers to an asterism consisting of ε Centauri and α Centauri.[13] Consequently, the Chinese name for ε Centauri itself is 南門一 (Nán Mén yī, English: the First Star of Southern Gate.)[14]

A yellow-light light curve for Epsilon Centauri, adapted from Shobbrook (1972)[15]

ε Centauri is a massive star with 8.2 times the mass of the Sun.[7] The spectrum matches a stellar classification of B1 III,[4] indicating this is an evolved giant star. It is radiating more than 16,000 times the luminosity of the Sun[8] from its outer atmosphere at an effective temperature of about 25,000 K,[8] giving it the blue-white hue of a B-type star.[16] It is classified as a Beta Cephei type variable star with a primary period of 0.16961 days (4 hours 4 minutes), completing 5.9 cycles per day.[9] During each cycle, the brightness of the star varies from apparent magnitude +2.29 to +2.31.

This star is a proper motion member of the Lower Centaurus–Crux sub-group in the Scorpius–Centaurus OB association, the nearest such association of co-moving massive stars to the Sun.[17] Epsilon Centauri is a relatively young star, with an age of around 16 million years.[18]

The IAU has not assigned a proper name to this star.[19]

References

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 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. 
  3. ↑ 3.0 3.1 Samus, N. N. 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: 02025. Bibcode: 2009yCat....102025S. 
  4. ↑ 4.0 4.1 Hohle, M. M. et al. (April 2010). "Masses and luminosities of O- and B-type stars and red supergiants". Astronomische Nachrichten 331 (4): 349. doi:10.1002/asna.200911355. Bibcode: 2010AN....331..349H. 
  5. ↑ 5.0 5.1 Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues 2237: 0. Bibcode: 2002yCat.2237....0D. 
  6. ↑ Evans, D. S. (June 20–24, 1966). "The Revision of the General Catalogue of Radial Velocities". in Batten, Alan Henry; Heard, John Frederick. Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30. 30. University of Toronto: International Astronomical Union. p. 57. Bibcode: 1967IAUS...30...57E. 
  7. ↑ 7.0 7.1 Quintana, Alexis L.; Wright, Nicholas J.; Martínez García, Juan (2025). "A census of OB stars within 1 KPC and the star formation and core collapse supernova rates of the Milky Way". Monthly Notices of the Royal Astronomical Society 538 (3): 1367. doi:10.1093/mnras/staf083. Bibcode: 2025MNRAS.538.1367Q. 
  8. ↑ 8.0 8.1 8.2 8.3 8.4 8.5 McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars". Monthly Notices of the Royal Astronomical Society 471 (1): 770. doi:10.1093/mnras/stx1433. Bibcode: 2017MNRAS.471..770M. 
  9. ↑ 9.0 9.1 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. 
  10. ↑ Van Belle, Gerard T. (2012). "Interferometric observations of rapidly rotating stars". Astronomy and Astrophysics Review 20 (1). doi:10.1007/s00159-012-0051-2. Bibcode: 2012A&ARv..20...51V. 
  11. ↑ Gratton, R.; Squicciarini, V.; Nascimbeni, V.; Janson, M.; Reffert, S.; Meyer, M.; Delorme, P.; Mamajek, E. E. et al. (2023). "Multiples among B stars in the Scorpius-Centaurus association". Astronomy and Astrophysics 678: A93. doi:10.1051/0004-6361/202346806. Bibcode: 2023A&A...678A..93G. 
  12. ↑ "Eps Cen". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Eps+Cen. 
  13. ↑ Script error: The function "in_lang" does not exist. 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.
  14. ↑ Script error: The function "in_lang" does not exist. AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 25 日
  15. ↑ Shobbrook, R. R. (1972). "Two new Beta Canis Majoris variables: epsilon Cen and delta Lup". Monthly Notices of the Royal Astronomical Society 157. doi:10.1093/mnras/157.1.5P. Bibcode: 1972MNRAS.157P...5S. 
  16. ↑ "The Colour of Stars". Australia Telescope, Outreach and Education. Commonwealth Scientific and Industrial Research Organisation. December 21, 2004. http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html. 
  17. ↑ de Geus, E. J. et al. (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. 
  18. ↑ Tetzlaff, N. et al. (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. 
  19. ↑ "Naming Stars". International Astronomical Union. https://www.iau.org/public/themes/naming_stars/. 



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:Epsilon_Centauri&oldid=4287217"