Astronomy:Theta Leonis

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Short description: Binary star system in the constellation Leo
θ Leonis
Leo constellation map.svg
Red circle.svg
Location of θ Leonis (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Leo
Right ascension  11h 14m 14.40446s[1]
Declination +15° 25′ 46.4541″[1]
Apparent magnitude (V) +3.324[2]
Characteristics
Spectral type A2 V[3]
U−B color index +0.07[2]
B−V color index –0.02[2]
Astrometry
Radial velocity (Rv)+7.6[4] km/s
Proper motion (μ) RA: -60.31[1] mas/yr
Dec.: -79.10[1] mas/yr
Parallax (π)19.76 ± 0.17[1] mas
Distance165 ± 1 ly
(50.6 ± 0.4 pc)
Absolute magnitude (MV)−0.19[5]
Details
Mass2.5[6] M☉
Luminosity141[6] L☉
Surface gravity (log g)3.65[7] cgs
Temperature9,350[7] K
Metallicity [Fe/H]+0.05[7] dex
Rotational velocity (v sin i)23[8] km/s
Age550[7] Myr
Other designations
Chertan, Chort, Coxa, θ Leo, Theta Leo, 70 Leo, HR 4359, BD+16 2234, HD 97633, SAO 99512, FK5 423, HIP 54879.[9]
Database references
SIMBADdata

Theta Leonis, Latinized from θ Leonis, formally named Chertan,[10] is a star in the constellation of Leo. With an apparent visual magnitude of +3.324[2] it is visible to the naked eye and forms one of the brighter stars in the constellation. The distance from the Sun can be directly determined from parallax measurements, yielding a value of about 165 light-years (51 parsecs).[1]

Description

This is a large star with 2.5 times the mass of the Sun.[6] The spectrum matches a stellar classification of A2 V,[3] making this a seemingly typical A-type main sequence star. However, the spectrum shows enhanced absorption lines of metals, marking this as a chemically peculiar Am star.[11] The abundance of elements other than hydrogen and helium, what astronomers term the star's metallicity, appears around 12% higher than in the Sun.[7] It is radiating 141[6] times the luminosity of the Sun from its outer atmosphere at an effective temperature of 9,350 K,[7] literally giving it a white-hot glow.[12]

Theta Leonis is much younger than the Sun, with an estimated age of around 550 million years.[7] It has a moderately high rate of rotation, with a projected rotational velocity of 23 km s−1.[8] Measurements in the infrared band show an excess of emission from the star and its surroundings, suggesting the presence of a circumstellar disk of dust. The temperature of this emission indicates the disk has an orbital radius of 36 AU.[7]

Nomenclature

θ Leonis (Latinised to Theta Leonis) is the star's Bayer designation.

It bore the traditional names Chertan, Chort /ˈtʃɔːrt/[13] and Coxa /ˈkɒksə/.[14] Chertan is derived from the Arabic al-kharātān 'two small ribs', originally referring to Delta Leonis and Theta Leonis; Chort from Arabic al-kharāt or al-khurt 'small rib', and Coxa is Latin for 'hip'. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[16] included a table of the first two batches of names approved by the WGSN; which included Chertan for this star.

In Chinese, 太微右垣 (Tài Wēi Yòu Yuán), meaning Right Wall of Supreme Palace Enclosure, refers to an asterism consisting of Theta Leonis, Beta Virginis, Sigma Leonis, Iota Leonis and Delta Leonis.[17] Consequently, the Chinese name for Theta Leonis itself is 太微右垣四 (Tài Wēi Zuǒ Yuán sì, English: the Fourth Star of Right Wall of Supreme Palace Enclosure.),[18] representing 西次相 (Xīcìxiāng), meaning The Second Western Minister.[19] 西次相 (Xīcìxiāng), spelled Tsze Seang by R.H. Allen, means "the Second Minister of State" [20]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 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 2.3 Johnson, 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. ↑ 3.0 3.1 Cowley, A. et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal 74: 375–406, doi:10.1086/110819, Bibcode: 1969AJ.....74..375C 
  4. ↑ 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 
  5. ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A. 
  6. ↑ 6.0 6.1 6.2 6.3 Wyatt, M. C. et al. (July 2007), "Steady State Evolution of Debris Disks around A Stars", The Astrophysical Journal 663 (1): 365–382, doi:10.1086/518404, Bibcode: 2007ApJ...663..365W 
  7. ↑ 7.0 7.1 7.2 7.3 7.4 7.5 7.6 7.7 Smith, K. C.; Dworetsky, M. M. (1993), "Elemental Abundances in Normal Late B-Stars and Hgmn-Stars from Co-Added IUE Spectra - Part One - Iron Peak Elements", Astronomy and Astrophysics 274 (2): 335, Bibcode: 1993A&A...274..335S 
  8. ↑ 8.0 8.1 Royer, F.; Zorec, J.; Gómez, A. E. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682, doi:10.1051/0004-6361:20065224, Bibcode: 2007A&A...463..671R 
  9. ↑ "tet Leo -- Variable Star", SIMBAD (Centre de Données astronomiques de Strasbourg), http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Theta+Leonis, retrieved 2012-02-11 
  10. ↑ "List of IAU-approved Star Names". https://www.iau.org/public/themes/naming_stars/#n4. Retrieved 17 January 2023. 
  11. ↑ Netopil, M. et al. (November 2008), "Chemically peculiar stars and their temperature calibration", Astronomy and Astrophysics 491 (2): 545–554, doi:10.1051/0004-6361:200810325, Bibcode: 2008A&A...491..545N 
  12. ↑ "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, retrieved 2012-01-16 
  13. ↑ Rumrill, H. B. (June 1936). "Star Name Pronunciation". Publications of the Astronomical Society of the Pacific (San Francisco, California) 48 (283): 139. doi:10.1086/124681. Bibcode: 1936PASP...48..139R. 
  14. ↑ Burnham, Robert (1978), Burnham's celestial handbook: an observer's guide to the universe beyond the Solar System, Dover Books on Astronomy, 2 (2nd ed.), Courier Dover Publications, p. 1067, ISBN 0-486-23568-8, https://books.google.com/books?id=wB9uZ9lH5bgC&pg=PA1067 
  15. ↑ "IAU Working Group on Star Names (WGSN)". https://www.iau.org/science/scientific_bodies/working_groups/280/. Retrieved 22 May 2016. 
  16. ↑ "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. 
  17. ↑ (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.
  18. ↑ (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.
  19. ↑ (in Chinese) English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name , Hong Kong Space Museum. Accessed on line November 23, 2010.
  20. ↑ "LacusCurtius • Allen's Star Names — Leo". https://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Leo*.html. 



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