Sigma Aurigae
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 05h 24m 39.14142s[1] |
Declination | +37° 23′ 07.2589″[1] |
Apparent magnitude (V) | 4.99[2] |
Characteristics | |
Spectral type | K4 III[3] |
U−B color index | +1.75[2] |
B−V color index | +1.42[2] |
Absolute magnitude (MV) | −0.75[6] |
Details | |
Rotational velocity (v sin i) | 10[8] km/s |
Database references | |
SIMBAD | data |
Sigma Aurigae,
mas,[5] it is approximately 530 light-years (160 parsecs) distant from the Earth. This is an evolved giant star with a stellar classification of K4 III.[3]
Sigma Aurigae has a 12th magnitude companion at an
arcseconds, as well as two fainter companions at 28 and 35" respectively.[10]
All are background objects, stars much further away than Sigma itself.
Sigma Aurigae, along with λ Aur and μ Aur, were Kazwini's Al Ḣibāʽ (ألحباع), the Tent.[11] According to the catalogue of stars in the Technical Memorandum 33-507 – A Reduced Star Catalog Containing 537 Named Stars, Al Ḣibāʽ were the title for three stars: λ Aur as Al Ḣibāʽ I, μ Aur as Al Ḣibāʽ II and σ Aur as Al Ḣibāʽ III.[12]
References
- ^ .
- ^ .
- ^ doi:10.1086/145598.
- S2CID 17804304.
- ^ .
- S2CID 119257644.
- ^ doi:10.1086/191527.
- Bibcode:1970CoAsi.239....1B.
- ^ "sig Aur -- Star in double system", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2012-08-22.
- doi:10.1086/323920.
- ISBN 0-486-21079-0. Retrieved 2010-12-12.
- ^ Rhoads, Jack W. (November 15, 1971), Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars (PDF), California Institute of Technology: Jet Propulsion Laboratory, retrieved 2012-08-19.