Cygnus OB2-12

Cygnus OB2-12
Cygnus OB2-12
Cygnus OB2-12 with planet.jpg
Cygnus OB2-12 as seen by a hypothetical close orbiting planet.
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 20h 32m 40.9589s
Declination +41° 14' 29.286"
Characteristics
Spectral type B3-B5Iae
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
B−V color index 3.0
Astrometry
Proper motion (μ) RA: 1.91 mas/yr
Dec.: -2.47 mas/yr
Parallax (π) -0.60 ± 2.07 mas
Distance approx. -5000 ly
(approx. -2000 pc)
Absolute magnitude (MV) -10.6
Details
Mass 92 M
Radius 244 R
Luminosity 6,300,000 L
Temperature 18,500 K
Age 6.43 million years
Other designations
VI CYG 12, 2MASS J20324096+4114291, NSV 13138, HIP 101364.
Database references
SIMBAD data

Cygnus OB2-12 is an extremely bright blue hypergiant with an absolute bolometric magnitude (all electromagnetic radiation) of -12.2, which approaches the upper limit believed possible for normal single stars. This makes the star more than 6 million times brighter than the Sun, and among the most luminous stars known in the galaxy.

It is a member of the Cyg OB2 Association, a cluster of young massive stars about 5000 light years away in Cygnus, and resides in a region of the Galaxy from which visible light is heavily absorbed by interstellar dust when viewed from the Earth. Were it not for the dust extinction, the star would have a visual magnitude about 1.5, nearly as bright as Deneb (Alpha Cygni), but because of the dust, the observed visual magnitude is 11.4, so that it requires binoculars or a small telescope to be seen.

References


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