Stars with at least eight times the mass of our sun end their lives in spectacular supernova explosions, where core temperatures briefly reach 100 billion degrees Celsius, fusing elements heavier than iron; the subsequent shockwave expands at speeds exceeding 30,000 km per second, ejecting most of the star's mass into space, and if the remaining core is between 1.4 and 2.8 solar masses, it collapses into an incredibly dense neutron star where a single teaspoon of material would weigh approximately 4 billion tons.
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A single supernova explosion can [music] outshine an entire galaxy of 100 billion stars for several weeks. Only stars at least eight times [music] the mass of our sun will end their lives in such a spectacular fashion. During this final [music] collapse, the core temperature can briefly reach 100 billion degrees Celsius, fusing elements heavier than iron.
>> [music] >> The subsequent shockwave expands outwards at speeds exceeding 30,000 km per second, [music] ejecting most of the star's mass into space. The Crab Nebula, a famous supernova remnant, [music] was observed by Chinese astronomers in 1054 AD. This event released more energy in 10 seconds than [music] the sun will produce in its entire 10-billion-year lifespan. After such a cataclysm, [music] if the remaining core is between 1.4 and 2.8 solar masses, it collapses [music] into a neutron star, an object so dense that a single teaspoon of its material would weigh approximately 4 billion tons.
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