Cygnus OB2-12

Cygnus OB2 #12 is an extremely luminous blue hypergiant with an absolute bolometric magnitude (all electromagnetic radiation) of −10.9, among the most luminous stars known in the galaxy. This makes the star nearly two million times more luminous than the Sun, although estimates were even higher when the star was first discovered. It is now known to be a binary, with the companion approximately a tenth as bright. A very approximate initial estimate of the orbit gives the total system mass as 120 M and the period as 30 years.

Cygnus OB2 #12
Location of Cygnus OB2 #12 (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 20h 32m 40.9572s
Declination 41° 14 29.279
Apparent magnitude (V) 11.702
Characteristics
Spectral type B3–4 Ia+
Apparent magnitude (B) 14.41
Apparent magnitude (V) 11.40
Apparent magnitude (J) 4.667±0.324
Apparent magnitude (H) 3.512±0.260
Apparent magnitude (K) 2.704±0.364
U−B color index 1.69
B−V color index 3.01
Variable type cLBV
Astrometry
Radial velocity (Rv)−11.00 km/s
Proper motion (μ) RA: −1.703 mas/yr
Dec.: −3.412 mas/yr
Parallax (π)0.5895 ± 0.0518 mas
Distance5,500 ± 500 ly
(1,700 ± 100 pc)
Absolute magnitude (MV)−9.82
Details
Mass110 M
Radius246 R
Luminosity1,660,000 L
Temperature13,700 K
Age3.0 Myr
Other designations
Cyg OB2 #12, Schulte 12, 2MASS J20324096+4114291, NSV 13138, HIP 101364, Gaia DR2 2067782734461462912
Database references
SIMBADdata
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