Nuclear Fusion
Nuclear fusion is a nuclear reaction in which two light atomic nuclei combine to form a single heavier nucleus. This process is significant as it releases a substantial amount of energy, which is why it powers stars and is harnessed in hydrogen bombs. Fusion is the opposite of nuclear fission, where a heavy nucleus splits into lighter nuclei. Fusion reactions require extreme temperatures and pressures for the nuclei to overcome their electrostatic repulsion. This section delves into the nature and implications of nuclear fusion, highlighting its role in both natural and artificial contexts.