Nuclear fission is the splitting of a large, unstable nucleus, typically Uranium-235 or Plutonium-239, into smaller daughter nuclei following the absorption of a slow-moving neutron. This process releases two or three high-speed neutrons and significant thermal energy, potentially sustaining a chain reaction if not regulated by control rods and moderators. Conversely, nuclear fusion requires the forcing together of light nuclei against strong electrostatic repulsion to form heavier nuclei, the primary energy mechanism in stars. Both processes demonstrate mass-energy equivalence, where a small decrease in mass results in a large release of energy according to E=mc².
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