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  2. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    This is what Betelgeuse may have looked like up until about 1 million years ago, when it was a main-sequence star. The surface of Betelgeuse shows enhancement of nitrogen, relatively low levels of carbon, and a high proportion of 13 C relative to 12 C , all indicative of a star that has experienced the first dredge-up .

  3. Betelgeuse aftermath: Still recovering from blowing its stack

    www.aol.com/news/betelgeuse-aftermath-still...

    In late 2019 and early 2020, Betelgeuse blew its top. Literally. Around that time the famous bright star marking the right shoulder of Orion suddenly started dimming, dropping to about half its ...

  4. Betelgeuse Is Being Weird Again - AOL

    www.aol.com/lifestyle/betelgeuse-being-weird...

    Betelgeuse has entered an uncommon period of brightening again, this time rising in brightness by around 50 percent. Is the star about to go supernova?

  5. Orion (constellation) - Wikipedia

    en.wikipedia.org/wiki/Orion_(constellation)

    Betelgeuse, also designated Alpha Orionis, is a massive M-type red supergiant star nearing the end of its life. It is the second brightest star in Orion, and is a semiregular variable star. [7] It serves as the "right shoulder" of the hunter (assuming that he is facing the observer).

  6. The red giant star Betelgeuse is closer than we thought ... - AOL

    www.aol.com/red-giant-star-betelgeuse-closer...

    By studying movements (like sound waves) on the surface of the star suggest Betelgeuse is still fusing helium. That would mean that the star is not close (on a human timescale) to erupting as a ...

  7. Red supergiant - Wikipedia

    en.wikipedia.org/wiki/Red_supergiant

    Betelgeuse; Epsilon Pegasi; Zeta Cephei; Lambda Velorum; Eta Persei; 31 and 32 Cygni; Psi 1 Aurigae; 119 Tauri; Mira was historically thought to be a red supergiant star, but is now widely accepted to be an asymptotic giant branch star. [32] Some red supergiants are larger and more luminous, with radii exceeding over a thousand times that of ...

  8. Variable star - Wikipedia

    en.wikipedia.org/wiki/Variable_star

    Comparison of VLT-SPHERE images of Betelgeuse taken in January 2019 and December 2019, showing the changes in brightness and shape. Betelgeuse is an intrinsically variable star. A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes systematically with time.

  9. Orion Arm - Wikipedia

    en.wikipedia.org/wiki/Orion_Arm

    The arm is named after the Orion Constellation, one of the most prominent constellations of the Northern Hemisphere in winter (or the Southern Hemisphere in summer).Some of the brightest stars in the sky as well as other well-known celestial objects of the constellation (e.g. Betelgeuse, Rigel, the three stars of Orion's Belt, and the Orion Nebula) are found within it, as shown on Orion Arm's ...