From Wikipedia, the free encyclopedia
(Redirected from Cha 110913)
Cha 110913−773444

WISE image centered on the brown dwarf Cha 110913−773444
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Chamaeleon
Right ascension 11h 09m 13.63s [1]
Declination −77° 34′ 44.6″ [1]
Astrometry
Distance529 [1] [note 1]  ly
(162 [1]  pc)
Details
Mass8+7
−3
[1]  MJup
Radius1.8 [1]  RJup
Luminosity (bolometric)0.000603 [1] [note 2]  L
Temperature1300–1400 [1]  K
Age0.5–10 [1]  Myr
Database references
SIMBAD data

Cha 110913−773444 (sometimes abbreviated Cha 110913) is an astronomical object surrounded by what appears to be a protoplanetary disk. It lies at a distance of 529 light-years from Earth. There is no consensus yet among astronomers whether to classify the object as a sub-brown dwarf (with planets) or a rogue planet (with moons). [2]

Cha 110913−773444 was discovered in 2004 by Kevin Luhman and others at Pennsylvania State University using the Spitzer Space Telescope and the Hubble Space Telescope, as well as two Earth-bound telescopes in Chile.

See also

References

  1. ^ a b c d e f g h i Luhman, K. L; Adame, Lucía; d'Alessio, Paola; Calvet, Nuria; Hartmann, Lee; Megeath, S. T; Fazio, G. G (2005). "Discovery of a Planetary-Mass Brown Dwarf with a Circumstellar Disk". The Astrophysical Journal. 635 (1): L93–L96. arXiv: astro-ph/0511807. Bibcode: 2005ApJ...635L..93L. doi: 10.1086/498868. S2CID  11685964.
  2. ^ Whitney Clavin (2005-11-29). "A Planet With Planets? Spitzer Finds Cosmic Oddball". NASA. Archived from the original on 2012-10-11. Retrieved 2006-03-26.

Notes

  1. ^ From a distance modulus (μ) of 6.05
  2. ^ From the logarithm (log Lbol) of −3.22