Astronomy:136 Tauri
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Taurus |
Right ascension | 05h 53m 19.64606s[1] |
Declination | +27° 36′ 44.1378″[1] |
Apparent magnitude (V) | 4.56[2] |
Characteristics | |
Spectral type | A0 V[3] (A0 V + A0 V)[2] |
B−V color index | −0.008±0.009[2] |
Variable type | suspected[4] |
Astrometry | |
Radial velocity (Rv) | −17.2±4.2[5] km/s |
Proper motion (μ) | RA: +3.72[1] mas/yr Dec.: −10.11[1] mas/yr |
Parallax (π) | 7.71 ± 0.22[1] mas |
Distance | 420 ± 10 ly (130 ± 4 pc) |
Absolute magnitude (MV) | −1.00[2] |
Orbit[6] | |
Period (P) | 5.969 d |
Eccentricity (e) | 0.00 |
Periastron epoch (T) | 2,420,147.25±10.0 JD |
Argument of periastron (ω) (secondary) | 0.00° |
Semi-amplitude (K1) (primary) | 48.9 km/s |
Semi-amplitude (K2) (secondary) | 71.0 km/s |
Details | |
136 Tau A | |
Radius | 2.1[7] R☉ |
Luminosity | 197.19[8] L☉ |
Temperature | 8,732[8] K |
Rotational velocity (v sin i) | 10[9] km/s |
Other designations | |
Database references | |
SIMBAD | data |
136 Tauri is a white-hued binary star system in the zodiac constellation of Taurus. It has a combined apparent visual magnitude of 4.56,[2] which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 7.71±0.22 mas as seen from Earth's orbit,[1] it is located approximately 420 light years from the Sun. The system is moving nearer with a heliocentric radial velocity of −17.2 km/s,[5] and is expected to make its closest approach in 6.5 million years at a distance of 150 ly (45 pc).[2]
This is a close, double-lined spectroscopic binary with an orbital period of 5.96 days and an eccentricity of 0.00.[6] Tidal effects between the pair may have circularized their orbit and slowed their rotation rates – the primary has a projected rotational velocity of 10 km/s.[9] They have a combined stellar classification of A0 V,[3] and both are most likely A-type main-sequence stars of the same class.[2]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 3.0 3.1 Cowley, A. et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal 74: 375–406, doi:10.1086/110819, Bibcode: 1969AJ.....74..375C.
- ↑ Samus, N. N. 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.
- ↑ 5.0 5.1 De Bruijne, J. H. J.; Eilers, A.-C. (2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics 546: A61, doi:10.1051/0004-6361/201219219, Bibcode: 2012A&A...546A..61D.
- ↑ 6.0 6.1 Luyten, W. J. (July 1936), "A rediscussion of the orbits of seventy-seven spectroscopic binaries", Astrophysical Journal 84: 85, doi:10.1086/143751, Bibcode: 1936ApJ....84...85L.
- ↑ Pasinetti Fracassini, L. E. et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy & Astrophysics 367: 521–24, doi:10.1051/0004-6361:20000451, Bibcode: 2001A&A...367..521P.
- ↑ 8.0 8.1 McDonald, I. et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society 427 (1): 343–357, doi:10.1111/j.1365-2966.2012.21873.x, Bibcode: 2012MNRAS.427..343M.
- ↑ 9.0 9.1 Abt, Helmut A.; Boonyarak, Chayan (November 2004), "Tidal Effects in Binaries of Various Periods", The Astrophysical Journal 616 (1): 562–566, doi:10.1086/423795, Bibcode: 2004ApJ...616..562A.
- ↑ "136 Tau". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=136+Tau.
Original source: https://en.wikipedia.org/wiki/136 Tauri.
Read more |