Variable star in the constellation Sculptor
Sigma Sculptoris , Latinized from σ Sculptoris, is a binary star in the southern constellation of Sculptor . It is faintly visible to the naked eye with an apparent visual magnitude of +5.54.[ 3] Based upon an annual parallax shift of 14.04 mas as seen from Earth,[ 2] it is located about 232 light years from the Sun .
The main component is an main sequence A-type star with a stellar classification of A1/A2 IV.[ 11] It was suspected to be an Ap star and an Alpha2 Canum Venaticorum variable ,[ 12] but no chemical peculiarity or variability was found in 2018.[ 4] The star has an estimated 1.95 the mass of the Sun and around two times the Sun's radius .[ 4] It is spinning with a projected rotational velocity of 82 km/s[ 9] and is about 560 million years old.[ 4] Sigma Sculptoris radiates 25.7[ 7] times the solar luminosity from its photosphere at an effective temperature of 8,470 K.[ 4]
The secondary is a small star with 72% the mass of the Sun, 5.7 times fainter than the primary.[ 4]
References
^ Manfroid, J.; Renson, P. (January 1994). "Photometric variations of AP stars" . Astronomy and Astrophysics . 281 : 73– 89. Bibcode :1994A&A...281...73M . Retrieved 20 September 2024 .
^ a b c d e f van Leeuwen, F. (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 .
^ a b c d Westerlund, B. E. (1963), "Three-colour photometry of early-type stars near the galactic poles", Monthly Notices of the Royal Astronomical Society , 127 (1): 83, Bibcode :1963MNRAS.127...83W , doi :10.1093/mnras/127.1.83 .
^ a b c d e f g Waisberg, Idel; Klein, Ygal; Katz, Boaz (April 2024). "Hidden Companions to Intermediate-mass Stars. XVII. Uncovering a 0.72 M⊙, 0.35 au Companion in the Spectroscopic Binary Sigma Sculptoris*" . Research Notes of the AAS . 8 (4): 101. doi :10.3847/2515-5172/ad3de9 . ISSN 2515-5172 .
^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics , 546 : 14, arXiv :1208.3048 , Bibcode :2012A&A...546A..61D , doi :10.1051/0004-6361/201219219 , S2CID 59451347 , A61.
^ 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 .
^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society , 427 (1): 343– 57, arXiv :1208.2037 , Bibcode :2012MNRAS.427..343M , doi :10.1111/j.1365-2966.2012.21873.x , S2CID 118665352 .
^ David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal , 804 (2): 146, arXiv :1501.03154 , Bibcode :2015ApJ...804..146D , doi :10.1088/0004-637X/804/2/146 , S2CID 33401607 .
^ a b Díaz, C. G.; et al. (July 2011), "Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum", Astronomy & Astrophysics , 531 : A143, arXiv :1012.4858 , Bibcode :2011A&A...531A.143D , doi :10.1051/0004-6361/201016386 , S2CID 119286673 .
^ "sig Scl -- Variable Star of alpha2 CVn type" , SIMBAD Astronomical Database , Centre de Données astronomiques de Strasbourg, retrieved 2017-04-13 .
^ 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 .
^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs . 1 . Bibcode :2009yCat....102025S .