VFTS 682

VFTS 682

VFTS 682 is at the very centre of this image of the Tarantula Nebula
Credit: ESO/M.-R. Cioni/VISTA Magellanic Cloud survey. Acknowledgment: Cambridge Astronomical Survey Unit
Observation data
Epoch J2000      Equinox J2000
Constellation Dorado
Right ascension 05h 38m 55.51s
Declination −69° 04 26.72
Apparent magnitude (V) 16.08
Characteristics
Spectral type WN5h
U−B color index -0.349
B−V color index -0.58
Astrometry
Radial velocity (Rv)300 km/s
Distance164,000 ly
(50,000 pc)
Absolute magnitude (MV)-6.83±0.12
Absolute bolometric
magnitude
 (Mbol)
-11.5
Details
Mass137.8+27.5
−15.9
 M
Radius20.2+2.5
−2.3
 R
Luminosity3,200,000 L
Temperature54,450±1,960 K
Rotational velocity (v sin i)<200 km/s
Age1.0±0.2 Myr
Other designations
2MASS J05385552-6904267, IRSF J05385552-6904267, DENIS J053855.4-690425, DENIS J053855.5-690426, Dor IRS 153
Database references
SIMBADdata

VFTS 682 is a Wolf–Rayet star in the Large Magellanic Cloud. It is located over 29 parsecs (95 ly) north-east of the massive cluster R136 in the Tarantula Nebula. It is 138 times the mass of the Sun and 3.2 million times more luminous, which makes it one of the most massive and most luminous stars known.