Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Hercules |
Right ascension | 18h 08m 45.49142s[1] |
Declination | +20° 48′ 52.4079″[1] |
Apparent magnitude (V) | 4.37[2] |
Characteristics | |
Spectral type | B2 IV[3][4] or B2 V[5][6] |
B−V color index | −0.164±0.013[2] |
Astrometry | |
Radial velocity (Rv) | −14.9±0.6[2] km/s |
Proper motion (μ) | RA: −1.92[1] mas/yr Dec.: −5.89[1] mas/yr |
Parallax (π) | 3.56 ± 0.19 mas[1] |
Distance | 920 ± 50 ly (280 ± 10 pc) |
Absolute magnitude (MV) | −2.87[2] |
Details | |
Mass | 9.7±0.2[4] M☉ |
Luminosity | 3,631.92[2] L☉ |
Surface gravity (log g) | 3.54[7] cgs |
Temperature | 22,420±1,440[8] K |
Rotational velocity (v sin i) | 41[9] km/s |
Age | 20.0±1.4[4] Myr |
Other designations | |
Database references | |
SIMBAD | data |
102 Herculis is a single[11] star in the northern constellation of Hercules. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.37.[2] Based upon parallax measurements, it is located around 920 light years away from the Sun.[1] The star is moving closer to the Earth with a heliocentric radial velocity of −15 km/s.[2]
The stellar classification of this object matches a massive, early B-type star with a luminosity class of IV[3] or V,[5] corresponding to a subgiant or main sequence star, respectively. It is 20[4] million years old with nearly ten[4] times the mass of the Sun and is spinning with a projected rotational velocity of 41 km/s.[9] The strength of the stellar magnetic field has been measured at (209.5±135.4)×10−4 T.[6] The star is radiating 3,632[2] times the Sun's luminosity from its photosphere at an effective temperature of 22,420 K.[8]
vanLeeuwen2007
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