nuclear fusion

Nuclear fusion is a type of reaction in which two or more atomic nuclei join together to form a single, heavier nucleus. It is the opposite of nuclear fission, in which one nucleus splits into two or more smaller nuclei. When this happens, a large amount of energy is released. The process is the same that powers stars like our Sun. In nuclear fusion, energy is released when two nuclei of light elements, such as hydrogen, combine to form a single, heavier nucleus. This is the same process that powers stars like the Sun. The amount of energy released is much greater than in nuclear fission, which is why fusion is seen as a possible source of clean, safe energy. The process of nuclear fusion is very complex and requires extremely high temperatures and pressures. A common example of a nuclear fusion reaction is the combination of two hydrogen nuclei to form a single helium nucleus. This releases a large amount of energy, which is why it is seen as a possible source of clean, safe energy. Nuclear fusion is the same process that powers stars like our Sun. Every second, the Sun produces energy through the fusion of hydrogen into helium. This energy is then released in the form of light, heat, and other forms of radiation. A fun fact about nuclear fusion is that it is the same process that powers the hydrogen bomb. Although it produces a huge amount of energy, it is not used as a source of energy due to the risks involved.