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The
Supernova 1987A
Photo: The Anglo-Australian
Observatory
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What is a supernova?
When the fusion reactions in a massive star end, it
collapses and throws off its outer layers in a giant
explosion. In just a few seconds, huge amounts of
energy – about 100 times the energy generated
by our sun during its lifetime – are released.
Gravitation compresses the stellar core, producing a
neutron star or – if the star is sufficiently
massive – a black hole. Protons in the stellar
core are transformed into neutrons, a process which
also generates neutrinos. Some of these were detected
by Kamiokande.
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