HD 268835

HD 268835
Observation data
Epoch J2000      Equinox J2000
Constellation Mensa
Right ascension 04h 56m 47.0791s
Declination −69° 50′ 24.792″
Apparent magnitude (V) 10.6[1]
Characteristics
Spectral type B8Iae[2]
U−B color index -0.66[1]
B−V color index 0.14[1]
Variable type LBV?[1]
Astrometry
Radial velocity (Rv)278 km/s
Proper motion (μ) RA: 1.63 mas/yr
Dec.: -2.38 mas/yr
Absolute magnitude (MV)-8.5[1]
Details
Mass<30[3] M☉
Radius131[3] R☉
Luminosity320,000[3] L☉
Temperature12,000[3] K
Other designations
HD 268835, HIP 22989, CD-70°273
Database references
SIMBADdata

HD 268835 (or R66) (30 SM) is one of two stars that were identified by NASA's Spitzer Space Telescope in the Milky Way's nearest neighbor galaxy, the Large Magellanic Cloud (the other being R 126 or HD 37974), as being circled by monstrous dust disks that are theorised to be the origin of planets.

  1. ^ a b c d e Stahl, O.; Wolf, B.; Zickgraf, F.-J.; Leitherer, C.; Bastian, U.; de Groot, M. J. H. (April 1983). "R 66(Aeq) - an LMC B supergiant with a massive cool and dusty wind". Astronomy and Astrophysics. 120 (2): 287–296. Bibcode:1983A&A...120..287S.
  2. ^ Kastner, J. H.; Thorndike, S. L.; Romanczyk, P. A.; Buchanan, C. L.; Hrivnak, B. J.; Sahai, R.; Egan, M. (2008). "The Large Magellanic Cloud's Top 250: Classification of the Most Luminous Compact 8 μm Sources in the Large Magellanic Cloud". The Astronomical Journal. 136 (3): 1221–1241. arXiv:astro-ph/0703584. Bibcode:2008AJ....136.1221K. doi:10.1088/0004-6256/136/3/1221. S2CID 117820349.
  3. ^ a b c d Kastner, J. H.; Buchanan, C. L.; Sargent, B.; Forrest, W. J. (2006). "SpitzerSpectroscopy of Dusty Disks around B[e] Hypergiants in the Large Magellanic Cloud". The Astrophysical Journal. 638 (1): L29–L32. Bibcode:2006ApJ...638L..29K. doi:10.1086/500804.