Rigel (β Orionis/Orionis Beta) is the the most brilliant star of the Constellation of Orion.
Rigel is located at a distance from 650 to 950 light-years of the Ground, to be known too far with precision by the measurement of its Parallaxe, even if the best estimate of the satellite Hipparcos gives 773 light-years. It is possible to deduce from it that the absolute Magnitude of Rigel is about -6,7, which in fact an extremely luminous star.
It is of spectral Type B8Ia, a blue Supergéante, 55 000 times more luminous than the Sun. With a diameter of almost 116 000 000 km, 84 times that of the Sun, Rigel would extend until the Orbite from Venus in our Solar system.
As much of supergéantes, Rigel is slightly variable, in an irregular way, 3 to 30% over one 25 days period on average. This variability would come from pulsations of surface from star.
With 21 solar masses, Rigel is dedicated to finish in Supernova and will probably finish its life in the form of a " neutron star " , of mass comparable with the Sun.
Rigel evolves/moves in an area rich in Nébuleuse S and lights several clouds of dust, like the Nebula of the Head of Witch (IC 2118).
Rigel is probably a remote member of a vast star association bound by the age, association OB1 of Orion, including the belt of Orion, stars illuminating the Nébuleuse of Orion and other blue-white stars of the constellation. One however more often classifies it in association R1 de Taureau/Orion, holding association OB1 of Orion to stars young people and closer to the nebula of Orion.
Rigel was also named Algebar or Elgebar, of Arab origin there still.
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