Tau Herculis
Tau Herculis, a name Latinized from τ Herculis, is a variable star in the northern constellation of Hercules. It has a blue-white hue and is visible to the naked eye at night with an apparent visual magnitude that fluctuates around 3.91. The star is located at a distance of approximately 307 light years from the Sun based on parallax, but it is drifting closer with a radial velocity of −16 km/s.
Historical depiction of the constellation Hercules with τ, bottom left, as the "northern knee" | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hercules |
| Right ascension | 16h 19m 44.43666s |
| Declination | 46° 18′ 48.1123″ |
| Apparent magnitude (V) | 3.91 3.83 to 3.86 |
| Characteristics | |
| Evolutionary stage | Main sequence |
| Spectral type | B5 IV |
| U−B color index | −0.569 |
| B−V color index | −0.151±0.009 |
| Variable type | SPB |
| Astrometry | |
| Radial velocity (Rv) | −15.5±0.5 km/s |
| Proper motion (μ) | RA: −13.33 mas/yr Dec.: 38.48 mas/yr |
| Parallax (π) | 10.61 ± 0.11 mas |
| Distance | 307 ± 3 ly (94.3 ± 1.0 pc) |
| Absolute magnitude (MV) | −0.96 |
| Details | |
| Mass | 4.01 M☉ |
| Radius | 3.55±0.19 R☉ 3.80±0.25 R☉ |
| Luminosity | 574 L☉ |
| Surface gravity (log g) | 4.02±0.05 cgs |
| Temperature | 15,615±301 K |
| Metallicity [Fe/H] | 0.15 dex |
| Rotational velocity (v sin i) | 32 km/s |
| Age | 26 Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
The stellar classification of Tau Hercules is B5 IV, and it serves as a standard spectrum in the modern Morgan–Keenan (MK) classification. It is estimated to be just 26 million years old with a relatively low projected rotational velocity of 32 km/s. Slowly rotating B-type stars are often chemically peculiar, so the mostly normal spectra of this star suggests we may be viewing it from near pole-on. The abundance of most heavier elements in this star are about 85% of those in the Sun. The star has four times the mass of the Sun and around 3.8 times the Sun's radius. On average, it is radiating 574 times the luminosity of the Sun from its photosphere at an effective temperature of 15,615 K.
During the Hipparcos mission, Tau Hercules was discovered to be a variable star of the slowly pulsating B-type. These are mid-B main sequence stars that vary with a period of about a day; the brightness of Tau Hercules varies by 0.03 magnitude over a period of 1.24970±0.00008 days. The radial velocity of the star varies at a different rate than the photometric period, with the object showing both radial and non-radial pulsation modes.