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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

    The compression caused by the collapse raises the temperature until thermonuclear fusion occurs at the center of the star, at which point the collapse gradually comes to a halt as the outward thermal pressure balances the gravitational forces. The star then exists in a state of dynamic equilibrium. During the star's evolution a star might ...

  4. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    Once a star like the Sun has exhausted its nuclear fuel, its core collapses into a dense white dwarf and the outer layers are expelled as a planetary nebula. Stars with around ten or more times the mass of the Sun can explode in a supernova as their inert iron cores collapse into an extremely dense neutron star or black hole.

  5. 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.

  6. Stellar mass loss - Wikipedia

    en.wikipedia.org/wiki/Stellar_mass_loss

    Often when a star is a member of a pair of close-orbiting binary stars, the tidal attraction of the gasses near the center of mass is sufficient to pull gas from one star onto its partner. This effect is especially prominent when the partner is a white dwarf, neutron star, or black hole. Mass loss in binary systems has particularly interesting ...

  7. 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.

  8. What happens when you crack an egg underwater? - AOL

    www.aol.com/news/2016-04-13-what-happens-when...

    Apparently, had the experiment been performed even deeper underwater, the pressure would have been too intense and the egg would have eventually exploded on its own -- much like it did when the ...

  9. Star - Wikipedia

    en.wikipedia.org/wiki/Star

    A supernova explosion blows away the star's outer layers, leaving a remnant such as the Crab Nebula. [98] The core is compressed into a neutron star, which sometimes manifests itself as a pulsar or X-ray burster. In the case of the largest stars, the remnant is a black hole greater than 4 M ☉. [99]