Sigma Arietis
  | |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Aries[1] |
| Right ascension | 02h 51m 29.586s[2] |
| Declination | +15° 04′ 55.44″[2] |
| Apparent magnitude (V) | +5.52[3] |
| Characteristics | |
| Evolutionary stage | main sequence[4] |
| Spectral type | B7 V[5] |
| U−B color index | −0.43[3] |
| B−V color index | −0.09[3] |
| Astrometry | |
| Radial velocity (Rv) | +17±2[6] km/s |
| Proper motion (μ) | RA: +29.636 mas/yr[2] Dec.: −24.650 mas/yr[2] |
| Parallax (π) | 7.0519±0.134 mas[2] |
| Distance | 463 ± 9 ly (142 ± 3 pc) |
| Absolute magnitude (MV) | −0.38[1] |
| Details | |
| A | |
| Mass | 3.84±0.08[4] M☉ |
| Radius | 3[7] R☉ |
| Luminosity | 301[4] L☉ |
| Surface gravity (log g) | 4.0±0.25[8] cgs |
| Temperature | 13,121[4] K |
| Rotational velocity (v sin i) | 165[4] km/s |
| Age | 36+57 −27[8] Myr |
| B | |
| Mass | 1.0–1.2[8] M☉ |
| Temperature | 5,524±150[8] K |
| Metallicity [Fe/H] | −0.5[8] dex |
| Rotational velocity (v sin i) | 5 km/s |
| Other designations | |
| σ Ari, 43 Arietis, BD+14 480, FK5 1079, GC 3427, HD 17769, HIP 13327, HR 847, SAO 93144, PPM 118608[9] | |
| Database references | |
| SIMBAD | data |
Sigma Arietis is a star in the northern constellation of Aries. Its name is a Bayer designation that is Latinized from σ Arietis, and abbreviated Sigma Ari or σ Ari. This star has an apparent visual magnitude of +5.52,[3] which is bright enough for the star to be seen with the naked eye from dark suburban skies. The star is located at a distance of approximately 463 light-years (142 parsecs) from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +17 km/s.[6] On November 20, 1952, it was observed being occulted by the planet Jupiter.[10]
Sigma Arietis is a B-type main sequence star with a stellar classification of B7 V.[5] This is a large star with three[7] times the radius of the Sun and 3.8[4] times the Sun's mass. It shines around 301[4] times as brightly as the Sun, with this energy being radiated into space from its outer atmosphere at an effective temperature of 13,121 K.[4] It is this heat that gives the star the blue-white hue of a B-type star. Sigma Arietis is spinning at a rapid clip, with a projected rotational velocity of 165 km/s.[4] It is about 36[8] million years old and is a probable member of the Cas-Tau OB association of stars that share a common motion through space.[11]
In 2016, a stellar companion was reported based on observations using adaptive optics with the Gemini North Telescope. This object has a mass equal to or slightly greater than the Sun. It has an effective temperature of 5,524 K.[8]
References
[edit]- 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. XHIP record for this object at VizieR.
- 1 2 3 4 5 Vallenari, A.; et al. (Gaia collaboration) (2023), "Gaia Data Release 3. Summary of the content and survey properties", Astronomy and Astrophysics, 674: A1, arXiv:2208.00211, Bibcode:2023A&A...674A...1G, doi:10.1051/0004-6361/202243940, S2CID 244398875. Gaia DR3 record for this source at VizieR.
- 1 2 3 4 Crawford, D. L.; Barnes, J. V.; Golson, J. C. (1971), "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere", The Astronomical Journal, 76: 1058, Bibcode:1971AJ.....76.1058C, doi:10.1086/111220.
- 1 2 3 4 5 6 7 8 9 Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789.
- 1 2 Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement, 17: 371, Bibcode:1968ApJS...17..371L, doi:10.1086/190179.
- 1 2 Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg, 35 (35), Astronomisches Rechen-Institut Heidelberg: 1, Bibcode:1999VeARI..35....1W.
- 1 2 Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367 (2): 5211–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
- 1 2 3 4 5 6 7 Gullikson, Kevin; et al. (August 2016), "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars", The Astronomical Journal, 152 (2): 13, arXiv:1604.06456, Bibcode:2016AJ....152...40G, doi:10.3847/0004-6256/152/2/40, S2CID 119179065, 40.
- ↑ "sig Ari". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2012-07-18.
{{cite web}}: CS1 maint: postscript (link) - ↑ de Zeeuw, P. T.; et al. (January 1999), "A HIPPARCOS Census of the Nearby OB Associations", The Astronomical Journal, 117 (1): 354–399, arXiv:astro-ph/9809227, Bibcode:1999AJ....117..354D, doi:10.1086/300682, S2CID 16098861.
