Astronomy:126 Tauri

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Short description: Star in the constellation Taurus
126 Tauri
Observation data
Equinox J2000.0]] (ICRS)
Constellation Taurus
Right ascension  05h 41m 17.71768s[1]
Declination +16° 32′ 02.9253″[1]
Apparent magnitude (V) 4.836[2]
(5.04 / 6.56)[3]
Characteristics
Spectral type B3 IV[4]
U−B color index -0.64[5]
B−V color index -0.12[5]
Astrometry
Radial velocity (Rv)21.90 ± 0.9[6] km/s
Proper motion (μ) RA: 3.50[1] mas/yr
Dec.: −15.47[1] mas/yr
Parallax (π)5.13 ± 0.81[1] mas
Distanceapprox. 600 ly
(approx. 190 pc)
Orbit[3]
Period (P)111.02 ± 1.37 yr
Semi-major axis (a)0.245 ± 0.014″
Eccentricity (e)0.661 ± 0.036
Inclination (i)80.5 ± 1.1°
Longitude of the node (Ω)53.2 ± 0.8°
Periastron epoch (T)B 1938.13 ± 1.64
Argument of periastron (ω)
(secondary)
40.9 ± 5.8°
Details
128 Tau A
Mass6.31 ± 0.42[4] M
Luminosity2061[4] L
Temperature17900[4] K
Other designations
Database references
SIMBADdata

126 Tauri (126 Tau) is a blue subgiant star in the constellation Taurus. Its apparent magnitude is 4.83. It is also a binary star, with an orbital period of 111 years.[3]

References

  1. 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode2007A&A...474..653V. 
  2. Høg, E. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. Bibcode2000A&A...355L..27H. 
  3. 3.0 3.1 3.2 "Sixth Catalog of Orbits of Visual Binary Stars". United States Naval Observatory. http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6. Retrieved 20 August 2017. 
  4. 4.0 4.1 4.2 4.3 Hohle, M.M.; Neuhäuser, R.; Schutz, B.F. (2010). "Masses and luminosities of O- and B-type stars and red supergiants". Astronomische Nachrichten 331 (4): 349. doi:10.1002/asna.200911355. Bibcode2010AN....331..349H. 
  5. 5.0 5.1 Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory 4: 99. Bibcode1966CoLPL...4...99J. 
  6. Kharchenko, N. V. (2007). "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ~55000 stars and mean radial velocities of 516 Galactic open clusters and associations". Astronomische Nachrichten 328 (9): 889. doi:10.1002/asna.200710776. Bibcode2007AN....328..889K.