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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. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    The heavy elements are produced by: nuclear fusion for nuclei up to 34 S; silicon photodisintegration rearrangement and quasiequilibrium during silicon burning for nuclei between 36 Ar and 56 Ni; and rapid capture of neutrons during the supernova's collapse for elements heavier than iron.

  4. Type Ia supernova - Wikipedia

    en.wikipedia.org/wiki/Type_Ia_supernova

    In the case of a nova, the infalling matter causes a hydrogen fusion surface explosion that does not disrupt the star. [ 13 ] Type Ia supernovae differ from Type II supernovae , which are caused by the cataclysmic explosion of the outer layers of a massive star as its core collapses, powered by release of gravitational potential energy via ...

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

  6. Type II supernova - Wikipedia

    en.wikipedia.org/wiki/Type_II_supernova

    The difference in the shape of the light curves is believed to be caused, in the case of Type II-L supernovae, by the expulsion of most of the hydrogen envelope of the progenitor star. [29] The plateau phase in Type II-P supernovae is due to a change in the opacity of the exterior layer.

  7. 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 ...

  8. My house didn't burn but ash from the L.A. fires fell in my ...

    www.aol.com/news/house-didnt-burn-ash-l...

    Ash from urban wildfires is potentially full of heavy metals and other toxins. Here's a guide for what to do if ash is covering your soil, plants and veggies. My house didn't burn but ash from the ...

  9. Hypernova - Wikipedia

    en.wikipedia.org/wiki/Hypernova

    From analyzing the spectroscopic data for both the GRB 970508 and its host galaxy, Bloom et al. concluded in 1998 that a hypernova was the likely cause. [6] That same year, hypernovae were hypothesized in greater detail by Polish astronomer Bohdan PaczyƄski as supernovae from rapidly spinning stars.