Sigma1 Gruis

Sigma1 Gruis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Grus
Right ascension 22h 36m 29.30757s[1]
Declination −40° 34 57.6836[1]
Apparent magnitude (V) 6.26[2]
Characteristics
Spectral type A3 Vn[2]
B−V color index +0.12[2]
Astrometry
Proper motion (μ) RA: +46.00[1] mas/yr
Dec.: −72.64[1] mas/yr
Parallax (π)14.64 ± 0.42[1] mas
Distance223 ± 6 ly
(68 ± 2 pc)
Absolute magnitude (MV)+2.11[3]
Details[4]
Mass2.00 M
Radius2.0[5] R
Luminosity12[3] L
Surface gravity (log g)4.24±0.14 cgs
Temperature9,230±314 K
Rotational velocity (v sin i)163.4±2.0[6] km/s
Age194 Myr
Other designations
σ1 Gru, CD−41° 14959, FK5 3811, HD 214085, HIP 111594, HR 8600, SAO 231211[7]
Database references
SIMBADdata

Sigma1 Gruis is a white-hued star in the constellation Grus. Its apparent magnitude is 6.28. Located around 68.31 parsecs (222.8 ly) distant, it is an A-type main-sequence star with a stellar classification of A3 Vn; a star that is currently fusing its core hydrogen. It is a source of X-ray emission, which may indicate it has a stellar companion.[8]

References

  1. 1 2 3 4 5 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.
  2. 1 2 3 Evans, D. S. (1966), "Fundamental data for Southern stars (6th list)", Royal Observatory Bulletin, 110, Bibcode:1966RGOB..110..185E.
  3. 1 2 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.
  4. 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.
  5. Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy & Astrophysics (3rd ed.), 367: 521–24, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451.
  6. 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.
  7. "sig01 Gru". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-06-24.
  8. Schröder, C.; Schmitt, J. H. M. M. (November 2007), "X-ray emission from A-type stars", Astronomy and Astrophysics, 475 (2): 677–684, Bibcode:2007A&A...475..677S, doi:10.1051/0004-6361:20077429.
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