Cygnus OB2-12

From the Science Archives, the open-project database of science information
Jump to navigation Jump to search

Cygnus OB2 #12
Cygnus OB2-12 with planet.jpg
Artist Impression of Cygnus OB2-12 with a planet
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 20h 32m 40.9589s[1]
Declination 41° 14′ 29.286″[1]
Spectral type B5 Ia-0[2]
Apparent magnitude (B) 14.41[3]
Apparent magnitude (V) 11.40[3]
Apparent magnitude (J) 4.667±0.324[4]
Apparent magnitude (H) 3.512±0.260[4]
Apparent magnitude (K) 2.704±0.364[4]
U−B color index 1.69[3]
B−V color index 3.01[3]
Variable type cLBV
Radial velocity (Rv)−11.00[5] km/s
Proper motion (μ) RA: 2.62[1] mas/yr
Dec.: −2.94[1] mas/yr
Parallax (π)0.40 ± 2.30[1] mas
Distance1,600[2] pc
Absolute magnitude (MV)−9.5[2]
Mass110[6] M
Radius246[6] R
Diameter246[6] D
Luminosity1,900,000[6][7] L
Temperature13,700[6] K
Age3.0x106[6] years
Other designations
Cyg OB2 #12, Schulte 12, 2MASS J20324096+4114291, NSV 13138, HIP 101364.
Database references

Cygnus OB2 #12 is an extremely bright 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 less than half the estimates 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.[8]

It is a member of the Cyg OB2 Association, a cluster of young massive stars about 5,000 light years away in Cygnus, and resides in a region of the Milky Way from which visible light is heavily absorbed by interstellar dust when viewed from Earth. The dust causes the star to be strongly reddened despite being an intrinsically hot and blue star, hence it has been extensively studied in the infra-red. 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.[8]

There are several fainter stars around Cygnus OB2 #12, thought to comprise a small cluster. Two stars are only resolved by speckle interferometry. One is thought to be a main sequence B star in a 100-200 year orbit. It is 2.3 magnitudes fainter than the primary star and 0.063" away. The other is 4.8 magnitudes fainter and about an arc-second distant.[9]

Cygnus OB2 #12 is a candidate luminous blue variable (LBV). Its position in the HR diagram, luminosity, and spectrum all classify it as an LBV. It shows brightness variations of a few tenths of a magnitude, but these do not seem to be associated with colour changes that would be expected from an LBV.[2] The spectral type has varied slightly since its discovery, but not to the extent that would be normal for an LBV.[6]


  1. 1.0 1.1 1.2 1.3 1.4 Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. arXiv:0708.1752. Bibcode 2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
  2. 2.0 2.1 2.2 2.3 Chentsov, E. L.; Klochkova, V. G.; Panchuk, V. E.; Yushkin, M. V.; Nasonov, D. S. (2013). "Spectroscopy of 13 high-mass stars in the Cyg OB2 association". Astronomy Reports 57 (7): 527–547. arXiv:1306.1087. Bibcode 2013ARep...57..527C. doi:10.1134/S1063772913070019.
  3. 3.0 3.1 3.2 3.3 Reed, B. Cameron (2003). "Catalog of Galactic OB Stars". The Astronomical Journal 125 (5): 2531–2533. Bibcode 2003AJ....125.2531R. doi:10.1086/374771.
  4. 4.0 4.1 4.2 Cutri, R. M.; Skrutskie, M. F.; Van Dyk, S.; Beichman, C. A.; Carpenter, J. M.; Chester, T.; Cambresy, L.; Evans, T. et al. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". VizieR On-line Data Catalog: II/246. Originally published in: 2003yCat.2246....0C 2246: 0. Bibcode 2003yCat.2246....0C.
  5. Klochkova, V. G.; Chentsov, E. L. (2004). "The Optical Spectrum of an LBV Candidate in the Cyg OB2 Association". Astronomy Reports 48 (12): 1005–1018. arXiv:astro-ph/0605483. Bibcode 2004ARep...48.1005K. doi:10.1134/1.1836024.
  6. 6.0 6.1 6.2 6.3 6.4 6.5 Clark, J. S.; Najarro, F.; Negueruela, I.; Ritchie, B. W.; Urbaneja, M. A.; Howarth, I. D. (2012). "On the nature of the galactic early-B hypergiants". Astronomy & Astrophysics 541: A145. arXiv:1202.3991. Bibcode 2012A&A...541A.145C. doi:10.1051/0004-6361/201117472.
  7. De Jager, C. (1998). "The yellow hypergiants". Astronomy and Astrophysics Review 8 (3): 145–180. Bibcode 1998A&ARv...8..145D. doi:10.1007/s001590050009.
  8. 8.0 8.1 Caballero-Nieves, S. M.; Nelan, E. P.; Gies, D. R.; Wallace, D. J.; Degioia-Eastwood, K.; Herrero, A.; Jao, W.-C.; Mason, B. D. et al. (2014). "A High Angular Resolution Survey of Massive Stars in Cygnus OB2: Results from the Hubble Space Telescope Fine Guidance Sensors". The Astronomical Journal 147 (2): 40. arXiv:1311.5087. Bibcode 2014AJ....147...40C. doi:10.1088/0004-6256/147/2/40.
  9. Maryeva, O. V.; Chentsov, E. L.; Goranskij, V. P.; Dyachenko, V. V.; Karpov, S. V.; Malogolovets, E. V.; Rastegaev, D. A. (2016). "On the nature of high reddening of Cygnus OB2 #12 hypergiant". Monthly Notices of the Royal Astronomical Society 1602. arXiv:1602.05042. Bibcode 2016MNRAS.458..491M. doi:10.1093/mnras/stw385.

Add your comment
The Science Archives welcomes all comments. If you do not want to be anonymous, register or log in. It is free.

As a reminder, article comments are only for discussions on how to improve the article. Please direct other comments to a user's talk page. Please be formal and do not use excessive uppercase. Please be advised you may receive an automatic block if you break the article comments policy. For information regarding what is acceptable/not acceptable in article comments, please message Joey (talk), ynoss (talk), or Nussun (talk).

External links[edit]