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  2. Nova - Wikipedia

    en.wikipedia.org/wiki/Nova

    Artist's conception of a white dwarf, right, accreting hydrogen from the Roche lobe of its larger companion star A nova (pl. novae or novas) is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star (hence the name "nova", Latin for "new") that slowly fades over weeks or months.

  3. List of stellar explosion types - Wikipedia

    en.wikipedia.org/wiki/List_of_stellar_explosion...

    Luminous red nova, an explosion thought to be caused by stellar collision Solar flares are a minor type of stellar explosion [ 1 ] Tidal disruption event , the pulling apart of a star by tidal forces

  4. 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 (roughly less than 10 to 300 parsecs [30 to 1000 light-years] away [2]) to have noticeable effects on Earth's biosphere.

  5. Largest artificial non-nuclear explosions - Wikipedia

    en.wikipedia.org/wiki/Largest_artificial_non...

    The 6 October 1854 great fire of Newcastle and Gateshead, UK, caused the explosion of combustibles in a bond warehouse on the quayside, which rained masonry and flaming timbers across wide areas of both cities, and left a crater with a depth of 40 feet (12 m) and 50 feet (15 m) in diameter. The explosion was heard at locations as far as 40 ...

  6. Bosenova - Wikipedia

    en.wikipedia.org/wiki/Bosenova

    A bosenova or bose supernova is a very small, supernova-like explosion, which can be induced in a Bose–Einstein condensate (BEC) by changing the external magnetic field, so that the "self-scattering" interaction transitions from repulsive to attractive due to the Feshbach resonance, causing the BEC to "collapse and bounce" or "rebound."

  7. Micronova - Wikipedia

    en.wikipedia.org/wiki/Micronova

    A micronova is a putative type of thermonuclear explosion on the surface of a white dwarf much smaller than the strength of a nova; being about 1 × 10 39 ergs (1.0 × 10 −12 foe; 1.0 × 10 32 J) in strength, about a millionth that of a typical nova. The phenomenon was first described in April 2022.

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  9. Quark-nova - Wikipedia

    en.wikipedia.org/wiki/Quark-nova

    A quark-nova is the hypothetical violent explosion resulting from the conversion of a neutron star to a quark star.Analogous to a supernova heralding the birth of a neutron star, a quark nova signals the creation of a quark star.