Astrophysics (Index)About

Betelgeuse

(Alpha Orionis)
(second brightest star in constellation Orion)

Betelgeuse is the bright star representing the constellation Orion's right shoulder, assuming Orion pictures a man who is facing us. Betelgeuse is a red supergiant with spectral type M2Iab and is among the larger and more luminous stars known. Characteristics:

Betelgeuse is near the end of the short lifetime of a massive star and has been thought likely to supernova within the next 100,000 years. Astronomers occasionally casually/humorously refer to the possibility that it will supernova any time now, but its state of evolution is not so precisely known as to make that likely (though a 2023 claim is that modelling suggests it is in a very late stage of stellar evolution, i.e., carbon burning, suggesting it could happen this century). It generally shows somewhat periodic variation (on the order of a magnitude) but a longer and deeper reduction in brightness from November 2019 to March 2020 (the Great Dimming) produced speculation regarding its current state.


(star,bright star,variable star,giant star)
Further reading:
https://en.wikipedia.org/wiki/Betelgeuse
http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Betelgeuse
https://www.aavso.org/vsots_alphaori
http://spider.seds.org/spider/Vars/alphaOri.html
https://ui.adsabs.harvard.edu/abs/2022ApJ...936...18D/abstract
https://ui.adsabs.harvard.edu/abs/2023MNRAS.526.2765S/abstract
RedshiftParsecs
/Distance
Lightyears
/Lookback Years
  
~0168pc548lyBetelgeuse
Coordinates:Betelgeuse
J055510.30536+072425.4304

Referenced by pages:
Bayer designation
M-type star (M)
near-Earth supernova
Orion
red giant
right ascension (RA)
solar luminosity (LSun)
stellar designation
supergiant

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