A historic breakthrough in nuclear fusion has been achieved
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Nuclear fusion is a reaction in which two or more atomic nuclei are combined to form one or more different atomic nuclei and subatomic particles (neutrons or protons).

The difference in mass between reactants and products manifests itself either in the release or absorption of energy.

This difference in mass is due to the difference in nuclear binding energy between the atomic nuclei before and after the reaction.

Nuclear fusion is the process that powers active or main sequence stars and other large magnitude stars, where large amounts of energy are released.

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