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BAT99-116
Melnick 34 - Hubble - WFPC2.jpg
Melnick 34
Credit: Wide Field and Planetary Camera of the Hubble Space Telescope
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Dorado
Right ascension 5h 38m 44.26s
Declination −69° 06′ 05.88″
Apparent magnitude (V) 13.09
Characteristics
Evolutionary stage Wolf–Rayet star
Spectral type WN5h + WN5h
B−V color index +0.25
Astrometry
Radial velocity (Rv) 287±5 km/s
Distance 163,000 ly
(49,970 pc)
Absolute magnitude (MV) -7.42
Orbit
Period (P) 154.55±0.05 d
Eccentricity (e) 0.68±0.02
Inclination (i) ~50°
Periastron epoch (T) 57671.2±0.9 JD
Argument of periastron (ω)
(secondary)
20.9±3.8°
Semi-amplitude (K1)
(primary)
130±7 km/s
Semi-amplitude (K2)
(secondary)
141±6 km/s
Details
A
Mass 148 M
Radius 19.3±2.8 R
Luminosity 2,042,000 L
Temperature 53,000±1,200 K
Age 0.5±0.3 Myr
B
Mass 135 M
Radius 18.2±2.7 R
Luminosity 1,585,000 L
Temperature 53,000±1,200 K
Age 0.6±0.3 Myr
Other designations
BAT99 116, [HSH95] 8, Melnick 34, 2MASS J05384424-6906058, Brey 84
Database references
SIMBAD data

BAT99-116 (commonly called Melnick 34 or Mk34) is a binary Wolf–Rayet star near R136 in the 30 Doradus complex (also known as the Tarantula Nebula) in the Large Magellanic Cloud. Both parts are amongst the most massive and luminous stars known. It has a spectral type of WN5h and the most massive binary system with x-ray luminosity.

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