Observation data Epoch J2000 Equinox J2000 | |
---|---|
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 mas [1] |
Distance | approx. 600 ly (approx. 190 pc) |
Orbit [7] [3] | |
Primary | A |
Companion | B |
Period (P) | 118±7 yr |
Semi-major axis (a) | 0.185±0.007″ |
Eccentricity (e) | 0.78±0.01 |
Inclination (i) | 68.9±0.7° |
Longitude of the node (Ω) | 63.5±0.8° |
Periastron epoch (T) | 61118±35 |
Argument of periastron (ω) (secondary) | 338±4° |
Orbit [7] | |
Primary | Ba |
Companion | Bb |
Period (P) | 4.77095±0.00023 d |
Semi-major axis (a) | 0.055±0.013 mas |
Eccentricity (e) | 0.0 |
Inclination (i) | 30±19° |
Longitude of the node (Ω) | 310±14° |
Periastron epoch (T) | 59529.10±0.01 |
Argument of periastron (ω) (secondary) | 0.0° |
Semi-amplitude (K1) (primary) | 72.9±0.3 km/s |
Details | |
128 Tau A | |
Mass | 6.14 [8] M☉ |
Luminosity | 2,061 [4] L☉ |
Temperature | 17,900 [4] K |
Ba | |
Mass | 3.19 [8] M☉ |
B | |
Mass | 1.65 [8] M☉ |
Other designations | |
BD+16°841, HD 37711, HIP 26777, HR 1946, SAO 94759 | |
Database references | |
SIMBAD | data |
126 Tauri (126 Tau) is a triple star system in the constellation Taurus, approximately 600 light years away. Its apparent magnitude is 4.83, making it visible to the naked eye with dark skies.
126 Tauri is a well-known binary star with the two components in an eccentric orbit of over a hundred years. The secondary, component B, has also shown radial velocity variations that indicate an unseen companion in a 4.77-day orbit. [7]
The combined spectral class is typically quoted as B3IV, occasionally B3V. [9] The primary alone has been classed as B3V, [10] although the two components have been individually measured at B8V and B7V. [7]