Jump to content

Luhman 16

From Simple English Wikipedia, the free encyclopedia
Revision as of 22:07, 2 January 2014 by Osiris (talk | changes) (Reverted to revision 4673809 by Auntof6. (TW))
The Luhman 16 binary brown dwarf is the yellow disc at the center of this WISE image. The two individual stars are seen as one here.

Luhman 16 is a binary brown dwarf in the southern constellation Vela at 6.6 light-years from the Sun. It is also known as WISE 1049-5319.

These are the nearest known brown dwarfs to the Solar System, and the closest system discovered since Barnard's Star in 1916.[1][2]

The primary has a stellar classification of L8 ± 1, and the secondary is probably near the L/T transition. The pair orbit each other at a distance of about 3 AU with an orbital period of about 25 years.[1]

References

  1. 1.0 1.1 Luhman K.L. 2013. Discovery of a binary brown dwarf at 2 parsecs from the Sun. Astrophysical Journal Letters, in press. [1]
  2. Kennedy, Barbara K. 2013. The closest star system found in a century. Penn State. [2]