Astrophysics (Index)About

Beta Centauri

(Hadar, Agena)
(second brightest star in Centaurus)

Beta Centauri (Hadar or Agena) is a variable star in the southern sky with magnitude +0.6. It is a triple star and a double-line spectroscopic binary, including two nearly-equal stars orbiting in 357 days, roughly 4 AU apart, with a third star considerably further from them. The pair are giant stars and all three are B-type stars. Characteristics:


(star,bright star,binary star,variable star,giant star)
Further reading:
https://en.wikipedia.org/wiki/Beta_Centauri
http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=beta+centauri
RedshiftParsecs
/Distance
Lightyears
/Lookback Years
  
~0120pc390lyBeta Centauri
Coordinates:Beta Centauri
J140349.40535-602222.9266

Referenced by page:
B-type star (B)

Index