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  2. Near-Earth supernova - Wikipedia

    en.wikipedia.org/wiki/Near-Earth_supernova

    The Crab Nebula is a pulsar wind nebula associated with the 1054 supernova.It is located about 6,500 light-years from the Earth. [1]A near-Earth supernova is an explosion resulting from the death of a star that occurs close enough to the Earth (less than roughly 10 to 300 parsecs [33 to 978 light-years] away [2]) to have noticeable effects on Earth's biosphere.

  3. Unprecedented image may reveal impending supernova that could ...

    www.aol.com/first-close-image-behemoth-beyond...

    In it, the “behemoth” star appears to puff out gas and dust, a critical final step before exploding in a supernova. The star, known as WOH G64, is 160,000 light-years from Earth in the Large ...

  4. How the Universe Works - Wikipedia

    en.wikipedia.org/wiki/How_the_Universe_Works

    The universe is home to real-life Death Stars that could destroy Earth. The latest science reveals the terrifying secrets of NASA's six deadliest: Cataclysmic variable stars, supernovas that can vaporize a planet, and unpredictable intergalactic stars.

  5. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    A near-Earth supernova is a supernova close enough to the Earth to have noticeable effects on its biosphere. Depending upon the type and energy of the supernova, it could be as far as 3,000 light-years away. In 1996 it was theorised that traces of past supernovae might be detectable on Earth in the form of metal isotope signatures in rock strata.

  6. Type Ia supernova - Wikipedia

    en.wikipedia.org/wiki/Type_Ia_supernova

    A Type Ia supernova (read: "type one-A") is a type of supernova that occurs in binary systems (two stars orbiting one another) in which one of the stars is a white dwarf. The other star can be anything from a giant star to an even smaller white dwarf.

  7. Hypernova - Wikipedia

    en.wikipedia.org/wiki/Hypernova

    When core collapse occurs in a star with a core at least around fifteen times the Sun's mass (M ☉) — though chemical composition and rotational rate are also significant — the explosion energy is insufficient to expel the outer layers of the star, and it will collapse into a black hole without producing a visible supernova outburst. A ...

  8. Supernova neutrinos - Wikipedia

    en.wikipedia.org/wiki/Supernova_Neutrinos

    Supernova neutrinos are weakly interactive elementary particles produced during a core-collapse supernova explosion. [1] A massive star collapses at the end of its life, emitting on the order of 10 58 neutrinos and antineutrinos in all lepton flavors. [2] The luminosity of different neutrino and antineutrino species are roughly the same. [3]

  9. SN 1572 - Wikipedia

    en.wikipedia.org/wiki/SN_1572

    The supernova has been confirmed as Type Ia, [1] in which a white dwarf star has accreted matter from a companion until it approaches the Chandrasekhar limit and explodes. This type of supernova does not typically create the spectacular nebula more typical of Type II supernovas, such as SN 1054 which created the Crab Nebula. A shell of gas is ...