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  2. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    This is among the earliest supernovae caught after detonation, and it is the earliest for which spectra have been obtained, beginning six hours after the actual explosion. The star is located in a spiral galaxy named NGC 7610, 160 million light-years away in the constellation of Pegasus. [37] [38]

  3. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    At what is called the star's death (when a star has burned out its fuel supply), it will undergo a contraction that can be halted only if it reaches a new state of equilibrium. Depending on the mass during its lifetime, these stellar remnants can take one of three forms: White dwarfs, in which gravity is opposed by electron degeneracy pressure [4]

  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 (less than roughly 10 to 300 parsecs [33 to 978 light-years] away [2]) to have noticeable effects on Earth's biosphere.

  5. Powerful Webb Telescope captures photos of one of the ... - AOL

    www.aol.com/powerful-webb-telescope-captures...

    The James Webb Space Telescope captured photos of one of the earliest supernovas ever seen using infrared technology, and creating a time lapse of the phenomena.

  6. Stellar collision - Wikipedia

    en.wikipedia.org/wiki/Stellar_collision

    Simulated collision of two neutron stars. A stellar collision is the coming together of two stars [1] caused by stellar dynamics within a star cluster, or by the orbital decay of a binary star due to stellar mass loss or gravitational radiation, or by other mechanisms not yet well understood.

  7. This is what happens when a star devours a planet - AOL

    www.aol.com/article/2016/06/07/this-is-what...

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  8. Type II supernova - Wikipedia

    en.wikipedia.org/wiki/Type_II_supernova

    The major unsolved problem with Type II supernovae is that it is not understood how the burst of neutrinos transfers its energy to the rest of the star producing the shock wave which causes the star to explode. From the above discussion, only one percent of the energy needs to be transferred to produce an explosion, but explaining how that one ...

  9. Supernova remnant - Wikipedia

    en.wikipedia.org/wiki/Supernova_remnant

    SN 1054 remnant (Crab Nebula).. A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova.The supernova remnant is bounded by an expanding shock wave, and consists of ejected material expanding from the explosion, and the interstellar material it sweeps up and shocks along the way.

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