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  2. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    The word supernova has the plural form supernovae (/-v iː /) or supernovas and is often abbreviated as SN or SNe. It is derived from the Latin word nova, meaning ' new ', which refers to what appears to be a temporary new bright star. Adding the prefix "super-" distinguishes supernovae from ordinary novae, which are far less luminous.

  3. Type Ia supernova - Wikipedia

    en.wikipedia.org/wiki/Type_Ia_supernova

    The Type Ia supernova leaves no compact remnant, but the whole mass of the former white dwarf dissipates through space. The theory of this type of supernova is similar to that of novae, in which a white dwarf accretes matter more slowly and does not approach the Chandrasekhar limit. In the case of a nova, the infalling matter causes a hydrogen ...

  4. Type II supernova - Wikipedia

    en.wikipedia.org/wiki/Type_II_supernova

    A Type II supernova or SNII [1] (plural: supernovae) results from the rapid collapse and violent explosion of a massive star. A star must have at least eight times, but no more than 40 to 50 times, the mass of the Sun ( M ☉ ) to undergo this type of explosion. [ 2 ]

  5. 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.

  6. 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 ...

  7. Rare nova could be visible on Earth 'any day now,' NASA ... - AOL

    www.aol.com/rare-nova-could-visible-earth...

    That's because a white dwarf star has about the same mass as Earth's sun, Hounsell said. ... But while supernovas occur only once, a nova can happen again and again.

  8. Stellar collision - Wikipedia

    en.wikipedia.org/wiki/Stellar_collision

    The normal route by which this happens involves a white dwarf drawing material off a main sequence or red giant star to form an accretion disc. Much more rarely, a type Ia supernova occurs when two white dwarfs orbit each other closely. [4] Emission of gravitational waves causes the pair to spiral inward.

  9. Ever see a star explode? You're about to get a chance very soon

    www.aol.com/news/ever-see-star-explode-youre...

    Once the nova happens, Gattini-IR will go from observing the Blaze Star every couple nights to every couple hours. ... novas like the Blaze Star could be precursors to supernovas. These explosions ...