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  2. List of supernova candidates - Wikipedia

    en.wikipedia.org/wiki/List_of_supernova_candidates

    Map showing various supernova candidates, most of which are within one kiloparsec from the Solar System. [1] This is a list of supernova candidates, or stars that are believed to soon become supernovae. Type II supernova progenitors include stars with at least 8~10 solar masses that are in the final stages

  3. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    As seen from Earth, Betelgeuse as a type II-P supernova would have a peak apparent magnitude somewhere in the range −8 to −12. [176] This would be easily visible in daylight, with a possible brightness up to a significant fraction of the full moon, though likely not exceeding it. This type of supernova would remain at roughly constant ...

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

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

    This red giant star will, one day, explode as a supernova. Betelgeuse is one of the best-known stars in the night sky, as well as the easiest to find. New examinations of this behemoth star ...

  5. Red supergiant - Wikipedia

    en.wikipedia.org/wiki/Red_supergiant

    Models indicate that even rapidly rotating main-sequence stars should be braked by their mass loss so that red supergiants hardly rotate at all. Those red supergiants such as Betelgeuse that do have modest rates of rotation may have acquired it after reaching the red supergiant stage, perhaps through binary interaction. The cores of red ...

  6. Betelgeuse, Betelgeuse... Betelbuddy? Experts Think This ...

    www.aol.com/betelgeuse-betelgeuse-betelbuddy...

    Betelgeuse—the star and not the slimy, suit-wearing demon—is one of the most celebrated celestial objects in the night sky. Found in the constellation Orion, Betelgeuse is extremely bright ...

  7. Variable star - Wikipedia

    en.wikipedia.org/wiki/Variable_star

    A supernova can briefly emit as much energy as an entire galaxy, brightening by more than 20 magnitudes (over one hundred million times brighter). The supernova explosion is caused by a white dwarf or a star core reaching a certain mass/density limit, the Chandrasekhar limit, causing the object to collapse in a fraction of a second. This ...

  8. 319 Leona - Wikipedia

    en.wikipedia.org/wiki/319_Leona

    Leona is approximately 80 by 55 kilometres, hence is projected to have a silhouette of roughly 46 by 41 milliarcseconds (mas). [5] [23] Betelgeuse has an apparent size in the sky of about 45 mas, but its diffuse atmosphere may make it appear 55 mas in size. A preliminary analysis of results showed only a slight dimming, consistent with a ...

  9. SN 2023rve - Wikipedia

    en.wikipedia.org/wiki/SN_2023rve

    SN 2023rve is a type II supernova that happened in the 10th magnitude barred spiral galaxy NGC 1097 on September 8, 2023. [1] Scientists from the McDonald Observatory in the state of Texas, United States, have observed the supernova and conducted photometric measurements, they described it to be the brightest supernova in the sky as of September 12, 2023.