BI 253

BI 253

NW portion of the Tarantula Nebula, with BI 253 towards the top right
Credit: Hubble Legacy Archive
Observation data
Epoch J2000      Equinox J2000
Constellation Dorado
Right ascension 05h 37m 34.461s
Declination −69° 01 10.20
Apparent magnitude (V) 13.76
Characteristics
Evolutionary stage Main sequence
Spectral type O2V-III(n)((f*))
U−B color index 1.02
B−V color index 0.13
Astrometry
Proper motion (μ) RA: 2.3 mas/yr
Dec.: 3.1 mas/yr
Distance164,000 ly
(50,000 pc)
Absolute magnitude (MV)5.7
Details
Mass97.6 M
Radius10.9+1.7
−1.6
 R
Luminosity1,200,000+210,000
−370,000
 L
Surface gravity (log g)4.36+0.12
−0.33
 cgs
Temperature58,000+1,600
−5,500
 K
Rotational velocity (v sin i)153±24 km/s
Age0.4+0.8
−0.4
 Myr
Other designations
BI 253, VFTS 72, 2MASS J05373446-6901102, IRSF J05373446-6901102
Database references
SIMBADdata

BI 253 is an O2V star in the Large Magellanic Cloud and is a primary standard of the O2 type. It is one of the hottest main-sequence stars known and one of the most-massive and most-luminous stars known.