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How fusion—which releases energy when two lighter atoms combine to form a heavier atom—differs from fission
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Fusion is one of two primary nuclear processes that produce energy, the other being fission. Fusion occurs when two lighter atoms (typically hydrogen) combine to form a heavier atom (usually helium). Fission occurs when a heavy atom (e.g., uranium or plutonium) split into smaller atoms.
In the fusion process, the new atom has slightly less mass than the two original atoms, and the difference is released as energy (a consequence of Einstein's famous E=mc^2 formulation).
Stars are fueled by fusion, with such extreme pressures and temperatures so high that the process is self-sustaining (until the fuel, the star's hydrogen, depletes)
Researchers, notably the National Ignition Facility at Livermore National Laboratory, are working to create fusion systems on Earth. In principle, such systems could provide more energy than they consume (the extra energy coming from the conversion of mass), offering unlimited power
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