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Stars of the main sequence with masses about 9 times as large as our Sun will normally form supernovas, the cataclysmic explosion of the star.

When they near the end of their hydrogen-to-helium fusion cycle, the heat and pressure inside the star can begin further fusion reactions in various layers (helium-to-carbon, carbon-to-neon, neon-to-oxygen, oxygen-to-silicon, and silicon-to-iron). Eventually, however, the outward force of these reactions can no longer support the gravitational weight of the outer layers. When they collapse, they trigger an explosive compression and rebound that blows off a large proportion of the star's mass.

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15y ago

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blackholes, neutron stars, or a white dwarf wich eventually cools and becomes a black dwarf

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16y ago
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Red of Super Giant

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15y ago
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Yesterday.

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12y ago
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