Zeta Leonis

Zeta Leonis
Diagram showing star positions and boundaries of the Leo constellation and its surroundings


Adhafera is the ζ star in the lion's mane (circled)

Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 10h 16m 41.41597s[1]
Declination +23° 25′ 02.3221″[1]
Apparent magnitude (V) 3.33[2]
Characteristics
Spectral type F0 III[3][4]
U−B color index +0.07[2]
B−V color index +0.30[2]
Variable type Suspected
Astrometry
Radial velocity (Rv)-15.6[5] km/s
Proper motion (μ) RA: +18.39[1] mas/yr
Dec.: -6.84[1] mas/yr
Parallax (π)11.90 ± 0.18[1] mas
Distance274 ± 4 ly
(84 ± 1 pc)
Details
Mass3[6] M☉
Radius6[7] R☉
Luminosity85[7] L☉
Surface gravity (log g)3.0[7] cgs
Temperature6,792[7] K
Metallicity [Fe/H]–0.03[8] dex
Rotational velocity (v sin i)72.4[7] km/s
Other designations
Adhafera, Aldhafera, Adhafara, ζ Leo, 36 Leo, HR 4031, BD +24°2209, HD 89025, FK5 384, HIP 50335, SAO 81265, GC 14107, NSV 04804, WDS 10167+2325A.[9]
Database references
SIMBADdata

Zeta Leonis (ζ Leonis, abbreviated Zeta Leo, ζ Leo), also named Adhafera,[10] is a third-magnitude star in the constellation of Leo, the lion. It forms the second star (after Gamma Leonis) in the blade of 'the Sickle', which is an asterism formed from the head of Leo.[11]

Nomenclature

ζ Leonis (Latinised to Zeta Leonis) is the star's Bayer designation. It has the traditional name Adhafera (Aldhafera, Adhafara), which comes from the Arabic الضفيرة al-ðafīrah 'the braid/curl', a reference to its position in the lion's mane. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[12] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[13] included a table of the first two batches of names approved by the WGSN; which included Adhafera for this star.

Properties

Adhafera is a giant star with a stellar classification of F0 III. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.[4] Its apparent magnitude is +3.44, making it relatively faint for a star that is visible to the naked eye. Nevertheless, it shines with 85 times the luminosity of the Sun.[7] Adhafera has about three times the Sun's mass[6] and six times the radius of the Sun.[7] Parallax measurements from the Hipparcos satellite yield an estimated distance to Adhafera of 274 light-years (84 parsecs)[1] from the Sun.

Adhafera forms a double star with an optical companion that has an apparent magnitude of 5.90. Known as 35 Leo, this star is separated from Adhafera by 325.9 arcseconds along a position angle of 340°.[14][15] The two stars do not form a binary star system as 35 Leo is only 100 light years from Earth, thus separating the two stars by approximately 174 light-years (53 parsecs).

See also

References

  1. 1 2 3 4 5 6 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, Bibcode:2007A&A...474..653V, arXiv:0708.1752 Freely accessible, doi:10.1051/0004-6361:20078357
  2. 1 2 3 Fernie, J. D. (May 1983), "New UBVRI photometry for 900 supergiants", Astrophysical Journal Supplement Series, 52: 7–22, Bibcode:1983ApJS...52....7F, doi:10.1086/190856
  3. ↑ Montes, D.; et al. (November 2001), "Late-type members of young stellar kinematic groups - I. Single stars", Monthly Notices of the Royal Astronomical Society, 328 (1): 45–63, Bibcode:2001MNRAS.328...45M, arXiv:astro-ph/0106537 Freely accessible, doi:10.1046/j.1365-8711.2001.04781.x
  4. 1 2 Garrison, R. F. (December 1993), "Anchor Points for the MK System of Spectral Classification", Bulletin of the American Astronomical Society, 25: 1319, Bibcode:1993AAS...183.1710G, retrieved 2012-02-04
  5. ↑ Wielen, R.; et al. (1999), Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions (35), Astronomisches Rechen-Institut Heidelberg, Bibcode:1999VeARI..35....1W
  6. 1 2 Kaler, James B., "ADHAFERA (Zeta Leonis)", Stars, University of Illinois, retrieved 2010-05-12
  7. 1 2 3 4 5 6 7 Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209
  8. ↑ Gray, R. O.; Graham, P. W.; Hoyt, S. R. (April 2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. II. Basic Parameters of Program Stars and the Role of Microturbulence", The Astronomical Journal, 121 (4): 2159–2172, Bibcode:2001AJ....121.2159G, doi:10.1086/319957
  9. ↑ "zet Leo -- Variable Star", SIMBAD, Centre de Données astronomiques de Strasbourg, retrieved 2010-05-12
  10. ↑ "IAU Catalog of Star Names". Retrieved 28 July 2016.
  11. ↑ Proctor, Mary (July 1896), "Evenings with the Stars", Popular Astronomy, 4: 565
  12. ↑ "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
  13. ↑ "Bulletin of the IAU Working Group on Star Names, No. 1" (PDF). Retrieved 28 July 2016.
  14. ↑ "CCDM (Catalog of Components of Double & Multiple stars (Dommanget+ 2002)", VizieR, Centre de Données astronomiques de Strasbourg, retrieved 2010-05-12
  15. ↑ Adhafera, Alcyone Bright Star Catalogue, retrieved 2010-05-12
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.