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  2. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    The last supernova directly observed in the Milky Way was Kepler's Supernova in 1604, appearing not long after Tycho's Supernova in 1572, both of which were visible to the naked eye. The remnants of more recent supernovae have been found, and observations of supernovae in other galaxies suggest they occur in the Milky Way on average about three ...

  3. Type II supernova - Wikipedia

    en.wikipedia.org/wiki/Type_II_supernova

    The expanding remnant of SN 1987A, a peculiar Type II supernova in the Large Magellanic Cloud. NASA image. A Type II supernova or SNII [1] (plural: supernovae) results from the rapid collapse and violent explosion of a massive star.

  4. 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 ...

  5. List of supernovae - Wikipedia

    en.wikipedia.org/wiki/List_of_supernovae

    SN 1054 remnant (Crab Nebula)A supernova is an event in which a star destroys itself in an explosion which can briefly become as luminous as an entire galaxy.This list of supernovae of historical significance includes events that were observed prior to the development of photography, and individual events that have been the subject of a scientific paper that contributed to supernova theory.

  6. History of supernova observation - Wikipedia

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

    Although supernovae thought to occur on average about once every 50 years in the Milky Way, [33] observations of distant galaxies allowed supernovae to be discovered and examined more frequently. The first supernova detection patrol was begun by Zwicky in 1933. He was joined by Josef J. Johnson from Caltech in 1936.

  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. Six hostages, including Israeli American Hersh Goldberg-Polin ...

    www.aol.com/news/israeli-military-says-located...

    One day after the Israeli army recovered the bodies of six hostages held by Hamas in Gaza, hundreds of thousands of protesters took to the streets in Tel Aviv on Sunday to demand the Israeli ...

  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 ...