Here are the essential concepts you must grasp in order to answer the question correctly.
Nuclear Fusion
Nuclear fusion is a process where two light atomic nuclei combine to form a heavier nucleus, releasing energy in the process. This reaction is the source of energy for stars, including the sun, and occurs under extreme temperature and pressure conditions. In the case of hydrogen isotopes, deuterium (2H) and protium (1H), their fusion produces helium and releases significant energy.
Recommended video:
Energy Release in Reactions
In nuclear reactions, the energy released is often measured in kilojoules per mole (kJ/mol). This energy comes from the mass defect, where the mass of the resulting nucleus is less than the sum of the original masses. According to Einstein's equation E=mc², this mass difference is converted into energy, which is released during the fusion process.
Recommended video:
Gibbs Free Energy of Reactions
Binding Energy
Binding energy is the energy required to disassemble a nucleus into its constituent protons and neutrons. It is a measure of the stability of a nucleus; higher binding energy indicates a more stable nucleus. In fusion reactions, the binding energy of the resulting nucleus is greater than that of the original nuclei, leading to the release of energy as the system moves to a lower energy state.
Recommended video: