Alpha Sculptoris

Alpha Sculptoris is the brightest star in the generally faint constellation Sculptor, it is the brightest star in the constellation because it has an apparent visual magnitude of +4.30.[1] Parallax measurements collected during the Hipparcos mission give an estimated distance for this star at about 780 light-years (240 parsecs), with a 4% margin of error.[2]

α Sculptoris
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Location of α Sculptoris (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sculptor
Right ascension 00h 58m 36.35930s[2]
Declination -29° 21′ 26.8247″[2]
Apparent magnitude (V) +4.30[1]
Characteristics
Spectral type B7 IIIp[3]
U−B color index −0.515[4]
B−V color index −0.155[4]
Variable type SX Ari[5]
Astrometry
Radial velocity (Rv)+10.2[1] km/s
Proper motion (μ) RA: +20.13[2] mas/yr
Dec.: +5.31[2] mas/yr
Parallax (π)4.20 ± 0.18[2] mas
Distance780 ± 30 ly
(240 ± 10 pc)
Absolute magnitude (MV)−2.58[6]
Details
Mass5.01[7] M
Radius7.52[8] R
Luminosity1,549[7] L
Surface gravity (log g)3.20[9] cgs
Temperature13,600[9] K
Metallicity [Fe/H]0.90[10] dex
Rotational velocity (v sin i)17[9] km/s
Age93[7] Myr
Other designations
α Scl, CD−30°297, FK5 35, HD 5737, HIP 4577, HR 280, SAO 166716[11]
Database references
SIMBADdata

Alpha Sculptoris is a B-type giant star. It is classified as an SX Arietis type variable star. It's magnitude changes by less than a tenth of a magnitude.[5]

The luminosity of Alpha Sculptoris is about 1,500 times brighter than that of the Sun and is very hot with a surface temperature of 13,600 K. It is 7 times larger than the Sun in radius and is 5 times massive than the Sun.

References

  1. 1.0 1.1 1.2 Wielen, R.; et al. (1999). "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions". Veröff. Astron. Rechen-Inst. Heidelb. Astronomisches Rechen-Institut Heidelberg. 35 (35): 1. Bibcode:1999VeARI..35....1W.
  2. 2.0 2.1 2.2 2.3 2.4 2.5 van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
  3. Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 3. Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan. Bibcode:1982mcts.book.....H.
  4. 4.0 4.1 Gutierrez-Moreno, Adelina; et al. (1966). "A System of photometric standards". Publ. Dept. Astron. Univ. Chile. Publicaciones Universidad de Chile, Department de Astronomy. 1: 1–17. Bibcode:1966PDAUC...1....1G.
  5. 5.0 5.1 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.
  6. Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644.
  7. 7.0 7.1 7.2 Kochukhov, O.; Bagnulo, S. (2006). "Evolutionary state of magnetic chemically peculiar stars". Astronomy and Astrophysics. 450 (2): 763. arXiv:astro-ph/0601461. Bibcode:2006A&A...450..763K. doi:10.1051/0004-6361:20054596. S2CID 18596834.
  8. Shulyak, D.; Paladini, C.; Causi, G. Li; Perraut, K.; Kochukhov, O. (2014). "Interferometry of chemically peculiar stars: Theoretical predictions versus modern observing facilities". Monthly Notices of the Royal Astronomical Society. 443 (2): 1629. arXiv:1406.6093. Bibcode:2014MNRAS.443.1629S. doi:10.1093/mnras/stu1259.
  9. 9.0 9.1 9.2 Saffe, C.; Levato, H. (2014). "On the nature of sn stars. I. A detailed abundance study". Astronomy & Astrophysics. 562: A128. arXiv:1401.5764. Bibcode:2014A&A...562A.128S. doi:10.1051/0004-6361/201322091. S2CID 119261402.
  10. Schmitt, A. (March 1973). "The weak-helium-line star α Sculptoris. I. The line-spectrum". Astronomy and Astrophysics Supplement. 9: 427. Bibcode:1973A&AS....9..427S.
  11. Template:Cite simbad