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HR 8799

(star with four exoplanets)

HR 8799 is a young main sequence star with a debris disk and four giant extra-solar planets. It is one of the first systems where the Exoplanets were confirmed by direct imaging.

Characteristics:


(star,disk,exoplanets)
http://en.wikipedia.org/wiki/HR_8799
RedshiftParsecs
/Distance
Lightyears
/Lookback Years
  
~040pc129lyHR 8799
Coordinates:HR 8799
J230728.7150+210803.302

Referenced by:
direct imaging

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