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  2. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    Another possible explanation is that accretion of gas onto the central neutron star can create a disk that drives highly directional jets, propelling matter at a high velocity out of the star, and driving transverse shocks that completely disrupt the star. These jets might play a crucial role in the resulting supernova.

  3. 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 ...

  4. Jack-in-the-box effect - Wikipedia

    en.wikipedia.org/wiki/Jack-in-the-box_effect

    The jack-in-the-box effect, [1] also known as a turret toss, is a specific effect of a catastrophic kill on a tank or other turreted armored vehicle in which an ammunition explosion causes the tank's turret to be violently blown off the chassis and into the air.

  5. Unique white dwarf will help clarify what happens to dying stars

    www.aol.com/news/2016-04-01-zombie-white-dwarf...

    Researchers have discovered a white dwarf (a dead star), with an oxygen atmosphere surrounding it -- the first of its kind. Astronomers managed to pick up the star from spectral lines: colored ...

  6. 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 ...

  7. Earth hit by blast of energy from dead star so powerful that ...

    www.aol.com/earth-hit-blast-energy-dead...

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  8. Silicon-burning process - Wikipedia

    en.wikipedia.org/wiki/Silicon-burning_process

    Silicon burning begins when gravitational contraction raises the star's core temperature to 2.7–3.5 billion kelvins . The exact temperature depends on mass. When a star has completed the silicon-burning phase, no further fusion is possible. The star catastrophically collapses and may explode in what is known as a Type II supernova.

  9. Earth hit by blast of energy from dead star so powerful that ...

    www.aol.com/news/earth-hit-blast-energy-dead...

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