what is nuclear fusion
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In nuclear physics, nuclear fusion is a reaction in which two or more atomic nuclei come close enough to form one or more different atomic nuclei and subatomic particles (neutrons or protons). The difference in mass between the reactants and products is manifested as the release of large amounts of energy. This difference in mass arises due to the difference in atomic "binding energy" between the atomic nuclei before and after the reaction. Fusion is the process that powers active or "main sequence" stars, or other high magnitude stars.
A fusion process that produces a nucleus lighter than iron-56 or nickel-62 will generally yield a net energy release.
A fusion process that produces a nucleus lighter than iron-56 or nickel-62 will generally yield a net energy release.
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A nuclear reaction in which atomic nuclei of low atomic number fuse to form a heavier nucleus with the release of energy is Called nuclear fusion.
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