Omicron Tauri

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ο Tauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Taurus
Right ascension 03h 24m 48.79796s[1]
Declination +09° 01′ 43.9489″[1]
Apparent magnitude (V) +4.875 ± 0.012[2]
Characteristics
Spectral type B2 V[2]
U−B color index −0.768 ± 0.005[2]
B−V color index −0.145 ± 0.006[2]
Astrometry
Radial velocity (Rv) –21.0 km/s
Proper motion (μ) RA: –67.04 ± 1.03[1] mas/yr
Dec.: –78.04 ± 1.02[1] mas/yr
Parallax (π) 11.21 ± 0.87[1] mas
Distance 290 ± 20 ly
(89 ± 7 pc)
Details
Surface gravity (log g) 4.15 ± 0.07[2] cgs
Temperature 20,700 ± 200[2] K
Rotational velocity (v sin i) 25 ± 2[2] km/s
Other designations
1 Tauri, BD+08 511, FK5 121, HD 21120, HIP 15900, HR 1030, SAO 111172

Omicron Tauri (ο Tau, ο Tauri) is a star in the constellation Taurus. Omicron Tauri is a yellow G-type giant with an apparent magnitude of +3.61. This star has three times the mass of the Sun and fifteen[3] to eighteen times the Sun's radius. Based on the latter, interferometry-measured radius, it is rotating once every 533 days.[4] It is approximately 212 light years from Earth and is radiating 155 times the luminosity of the Sun.[5]

This is a binary star system with the two components orbiting each other over a period of 1,655 days at an eccentricity of 0.263.[6]

References

  1. 1.0 1.1 1.2 1.3 1.4 Lua error in package.lua at line 80: module 'strict' not found. Vizier catalog entry
  2. 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Lua error in package.lua at line 80: module 'strict' not found.
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External links

  • Lua error in package.lua at line 80: module 'strict' not found.


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