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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. History of supernova observation - Wikipedia

    en.wikipedia.org/wiki/History_of_supernova...

    It was the first supernova to be detected through its neutrino emission and the first to be observed across every band of the electromagnetic spectrum. The relative proximity of this supernova has allowed detailed observation, and it provided the first opportunity for modern theories of supernova formation to be tested against observations. [49 ...

  4. Photodisintegration - Wikipedia

    en.wikipedia.org/wiki/Photodisintegration

    In explosions of very large stars (250 or more solar masses), photodisintegration is a major factor in the supernova event. As the star reaches the end of its life, it reaches temperatures and pressures where photodisintegration's energy-absorbing effects temporarily reduce pressure and temperature within the star's core.

  5. A huge star just exploded, and you can actually see it - AOL

    www.aol.com/huge-star-just-exploded-actually...

    Boom.In the colossal Pinwheel galaxy, 25 million light-years away, a star has just exploded and is even visible through small telescopes. The supernova-hunting astronomer Koichi Itagaki discovered ...

  6. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    A supernova (pl.: supernovae or supernovas) is a powerful and luminous explosion of a star. A supernova occurs during the last evolutionary stages of a massive star, or when a white dwarf is triggered into runaway nuclear fusion.

  7. Stellar collision - Wikipedia

    en.wikipedia.org/wiki/Stellar_collision

    where N is the number of encounters per million years that come within a radius D of the Sun in parsecs. [15] For comparison, the mean radius of the Earth's orbit, 1 AU, is 4.82 × 10 −6 parsecs. Our star will likely not be directly affected by such an event because there are no stellar clusters close enough to cause such interactions. [14]

  8. Supernova nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Supernova_nucleosynthesis

    Supernova nucleosynthesis is the nucleosynthesis of chemical elements in supernova explosions.. In sufficiently massive stars, the nucleosynthesis by fusion of lighter elements into heavier ones occurs during sequential hydrostatic burning processes called helium burning, carbon burning, oxygen burning, and silicon burning, in which the byproducts of one nuclear fuel become, after ...

  9. SN 1987A - Wikipedia

    en.wikipedia.org/wiki/SN_1987A

    After the supernova faded, that identification was definitively confirmed, as Sk -69 202 had disappeared. The possibility of a blue supergiant producing a supernova was considered surprising, [8] and the confirmation led to further research which identified an earlier supernova with a blue supergiant progenitor. [9]