HD 268835

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

Template:Short description

HD 268835
File:HD268835LightCurve.png
A visual band light curve for HD 268835, adapted from van Genderen & Sterken (2002)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Mensa
Right ascension Template:RA
Declination Template:DEC
Apparent magnitude (V) 10.6[2]
Characteristics
Spectral type B8Iae[3]
U−B Template:Engvar -0.66[2]
B−V Template:Engvar 0.14[2]
Variable type LBV?[2]
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[2]
Details
Mass<30[4] Template:Solar mass
Radius131[4] Template:Solar radius
Luminosity320,000[4] Template:Solar luminosity
Temperature12,000[4] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
HD 268835, HIP 22989, CD-70°273
Database references
SIMBADdata

Script error: No such module "Check for unknown parameters".

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.

Significance

Both HD 268835 and HD 37974 are classified as hypergiants, very large and very bright. The dust cloud around them surprised astronomers because stars as big as these were thought to be inhospitable to planet formation as they have very strong winds making it difficult/impossible for the dust clouds to "condense" into planets. "We do not know if planets like those in our solar system are able to form in the highly energetic, dynamic environment of these massive stars, but if they could, their existence would be a short and exciting one" said Charles Beichman, an astronomer at NASA's Jet Propulsion Laboratory and the California Institute of Technology, both in Pasadena, California.[5]

File:Solar System and Star R66.jpg
Artist's impression depicting HD 268835's dust disk compared to the Solar System
File:R 66 and R 126 graph.png
The infrared spectrum of HD 268835 compared to that of a multi-component model of the disk composition

References

<templatestyles src="Reflist/styles.css" />

  1. Script error: No such module "Citation/CS1".
  2. a b c d e Script error: No such module "Citation/CS1".
  3. Script error: No such module "Citation/CS1".
  4. a b c d Script error: No such module "Citation/CS1".
  5. NASA's Spitzer Uncovers Hints of Mega Solar Systems Template:Webarchive, Nasa.gov, accessed 11 Feb 2006

Script error: No such module "Check for unknown parameters".

Template:Stars of Mensa

ko:R 66과 R 126 it:R 66 e R 126