139 Tauri
139 Tauri is a single, blue-white hued star in the zodiac constellation of Taurus. It is faintly visible to the naked eye with an apparent visual magnitude of 4.81. The distance to this star, as determined from an annual parallax shift of 2.10±0.19 mas, is roughly 1,600 light years. Because this star is located near the ecliptic, it is subject to occultations by the Moon. One such event was observed April 28, 1990.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Taurus |
| Right ascension | 05h 57m 59.65632s |
| Declination | +25° 57′ 14.0799″ |
| Apparent magnitude (V) | 4.81 |
| Characteristics | |
| Spectral type | B1 Ib or B0.5 II |
| B−V color index | −0.088±0.003 |
| Astrometry | |
| Radial velocity (Rv) | +8.0±4.2 km/s |
| Proper motion (μ) | RA: −2.06 mas/yr Dec.: −1.95 mas/yr |
| Parallax (π) | 2.10 ± 0.19 mas |
| Distance | 1,600 ± 100 ly (480 ± 40 pc) |
| Absolute magnitude (MV) | −4.4 |
| Details | |
| Mass | 10.1±1.0 M☉ |
| Radius | 20.7 R☉ |
| Luminosity | 81,000 L☉ |
| Surface gravity (log g) | 3.559±0.059 cgs |
| Temperature | 24,660±1,620 K |
| Rotational velocity (v sin i) | 140 km/s |
| Age | 22.5±2.6 Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
This is a massive B-type lower-luminosity supergiant or bright giant star with a stellar classification of B1 Ib or B0.5 II, respectively. It is around 22.5 million years old with a high rate of spin, showing a projected rotational velocity of 140 km/s. J. D. Rosendhal (1973) identified weak emission features associated with an asymmetric H-alpha absorption line, providing evidence of mass loss. The star has about 10 times the mass of the Sun and around 20 times the Sun's radius. It is radiating over 80,000 times the Sun's luminosity from its photosphere at an effective temperature of around 24,660 K. Stars such as this with 10 or more solar masses are expected to end their life by exploding as a Type II supernova.