Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Sagittarius |
Right ascension | 17h 45m 47.541s[1] |
Declination | −26° 10′ 27.78″[1] |
Apparent magnitude (V) | 14.10[2] |
Characteristics | |
Evolutionary stage | Wolf–Rayet star |
Spectral type | WO2[3] |
B−V color index | +0.77[4] |
Astrometry | |
Proper motion (μ) | RA: +0.672[1] mas/yr Dec.: −0.059[1] mas/yr |
Parallax (π) | 0.3421 ± 0.0208 mas[1] |
Distance | 9,500 ± 600 ly (2,900 ± 200 pc) |
Absolute magnitude (MV) | −1.46[5] |
Details | |
Mass | 16.1+1.7 −1.4[5] M☉ |
Radius | 0.52[5] R☉ |
Luminosity | 380,000[5] L☉ |
Temperature | 200,000[5] K |
Metallicity [Fe/H] | 0.0[3] dex |
Other designations | |
V3893 Sagittarii, LS 4368, ALS 4368, Sand 4 | |
Database references | |
SIMBAD | data |
WR 102 is a Wolf–Rayet star in the constellation Sagittarius, an extremely rare star on the WO oxygen sequence. It is a luminous and very hot star, highly evolved and close to exploding as a supernova.
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