Editing Nuclear fusion
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− | [[Category: Physics]] | + | [[Category: more Physics]] |
== Explanation == | == Explanation == | ||
Nuclear fusion is the process in which lighter nuclei fuse together at a very high [[temperature]] to form a stable heavier [[atomic nucleus|nucleus]]. In the process, a massive amount of [[energy]] is released along with [[proton]]s and [[neutron]]s. A good example of the nuclear fusion reaction is the stars. The [[hydrogen]] atoms in the core of the [[sun]], fuses due to the high [[kinetic energy]] from the temperature to form [[helium]], thus powering it up with the energy. | Nuclear fusion is the process in which lighter nuclei fuse together at a very high [[temperature]] to form a stable heavier [[atomic nucleus|nucleus]]. In the process, a massive amount of [[energy]] is released along with [[proton]]s and [[neutron]]s. A good example of the nuclear fusion reaction is the stars. The [[hydrogen]] atoms in the core of the [[sun]], fuses due to the high [[kinetic energy]] from the temperature to form [[helium]], thus powering it up with the energy. |