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Epsilon Leonis

In today's world, Epsilon Leonis is a topic that has captured the attention of many people. With its increasing relevance in modern society, Epsilon Leonis has become an important point of discussion in various spheres. In both academia and entertainment, there has been an increase in interest and attention devoted to Epsilon Leonis. As the years go by, Epsilon Leonis has proven to be a topic that continues to generate debate and reflection, challenging common perceptions and encouraging new ideas. In this article, we will further explore the impact of Epsilon Leonis on our society and discuss its relevance today.

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Epsilon Leonis
Location of ε Leonis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 09h 45m 51.07330s[1]
Declination +23° 46′ 27.3208″[1]
Apparent magnitude (V) 2.98[2]
Characteristics
Evolutionary stage Supergiant[3]
Spectral type G1 IIIa[4]
U−B color index +0.47[2]
B−V color index +0.808[5]
Variable type suspected[6]
Astrometry
Radial velocity (Rv)4.86 ± 0.33[5] km/s
Proper motion (μ) RA: –45.61[1] mas/yr
Dec.: –9.21[1] mas/yr
Parallax (π)13.22±0.15 mas[1]
Distance247 ± 3 ly
(75.6 ± 0.9 pc)
Absolute magnitude (MV)–1.49[7]
Details
Mass3.71±0.04[8] M☉
Radius21.03+0.31
−0.32[8] R☉
Luminosity282±13[9] L☉
Surface gravity (log g)2.36±0.05[9] cgs
Temperature5,314±17[9] K
Metallicity −0.03±0.11[9] dex
Rotational velocity (v sin i)8.1[5] km/s
Age210±0[8] Myr
Other designations
Algenubi, Ras Elased Australis,[10] ε Leo, 17 Leo, BD+24°2129, FK5 367, GC 13443, HD 84441, HIP 47908, HR 3873, SAO 81004[11]
Database references
SIMBADdata

Epsilon Leonis (ε Leo, ε Leonis) is the fifth-brightest star in the constellation Leo, consistent with its Bayer designation Epsilon. It is known as Algenubi or Ras Elased Australis. Both names mean "the southern star of the lion's head". Australis is Latin for "southern" and Genubi is Arabic for "south".

Properties

Epsilon Leonis has a stellar classification of G1 III,[4] with the luminosity class of III indicating that, it has evolved into a giant star. However, Usenko (2017) classified it as a yellow supergiant.[3] It is much larger and brighter than the Sun with a luminosity 282 times[9] and a radius 21 times solar.[8] Consequently, its absolute magnitude is actually –1.49,[7] making it one of the more luminous stars in the constellation, significantly more than Regulus. Its apparent brightness, though, is only 2.98.[2] Given its distance of about 247 light-years (76 parsecs), the star is more than three times the distance from the Sun than Regulus. At this distance, the visual magnitude of Epsilon Leonis is reduced by 0.03 as a result of extinction caused by intervening gas and dust.[7]

Epsilon Leonis exhibits the characteristics of a Cepheid-like variable, changing by an amplitude of 0.3 magnitude every few days.[12][10] It has around four times the mass of the Sun and a projected rotational velocity of 8.1 km s−1.[5] Based upon its iron abundance, the metallicity of this star's outer atmosphere is only around 52% of the Sun's. That is, the abundance of elements other than hydrogen and helium is about half that in the Sun.[5]

See also

References

  1. ^ a b c d e van Leeuwen, Floor (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752v1, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600 Note: see VizieR catalogue I/311.
  2. ^ a b c 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. ^ a b Usenko, I. A. (April 2017), "Spectroscopic studies of yellow supergiants in the Cepheid instability strip", Astronomy Letters, 43 (4): 265–283, Bibcode:2017AstL...43..265U, doi:10.1134/S1063773717040090, ISSN 1063-7737
  4. ^ a b Keenan, Philip C.; McNeil, Raymond C. (1989-10-01), "The Perkins Catalog of Revised MK Types for the Cooler Stars", The Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373, ISSN 0067-0049, S2CID 123149047
  5. ^ a b c d e 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
  6. ^ Samus, N. N.; Durlevich, O. V.; 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. Bibcode:2009yCat....102025S.
  7. ^ a b c Takeda, Yoichi; Sato, Bun'ei; Murata, Daisuke (August 2008), "Stellar parameters and elemental abundances of late-G giants", Publications of the Astronomical Society of Japan, 60 (4): 781–802, arXiv:0805.2434, Bibcode:2008PASJ...60..781T, doi:10.1093/pasj/60.4.781, S2CID 16258166
  8. ^ a b c d Baines, Ellyn K.; et al. (2018), "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer", The Astronomical Journal, 155 (1), 30, arXiv:1712.08109, Bibcode:2018AJ....155...30B, doi:10.3847/1538-3881/aa9d8b, S2CID 119427037.
  9. ^ a b c d e Soubiran, C.; Creevey, O. L.; Lagarde, N.; Brouillet, N.; Jofré, P.; Casamiquela, L.; Heiter, U.; Aguilera-Gómez, C.; Vitali, S.; Worley, C.; de Brito Silva, D. (2024-02-01), "Gaia FGK benchmark stars: Fundamental Teff and log g of the third version", Astronomy and Astrophysics, 682: A145, arXiv:2310.11302, Bibcode:2024A&A...682A.145S, doi:10.1051/0004-6361/202347136, ISSN 0004-6361 Epsilon Leonis' database entry at VizieR.
  10. ^ a b Kaler, James B., "ALGENUBI (Epsilon Leonis)", Stars, University of Illinois, retrieved 2010-05-10
  11. ^ "eps Leo". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-05-10.
  12. ^ Andrievsky, S. M. (July 1998), "BA II lines as luminosity indicators: s-Cepheids and non-variable supergiants", Astronomische Nachrichten, 319 (4): 239–240, Bibcode:1998AN....319..239A, doi:10.1002/asna.2123190405
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