Nuclear fusion is a process in which two light atomic nuclei combine to form a heavier nucleus. This process releases a large amount of energy and is the same process that powers the sun and other stars. Unlike nuclear fission, which involves the splitting of heavy atomic nuclei, nuclear fusion involves the merging of light atomic nuclei.
In order for nuclear fusion to occur, the nuclei of two atoms must overcome the strong electrostatic repulsion between them. This usually happens at extremely high temperatures and pressures. When the nuclei fuse, they release a tremendous amount of energy in the form of light and heat.