The mass defect of a nucleus represents the disparity between the combined mass of its individual protons and neutrons and the nucleus's actual measured mass. It is calculated as:
\[ \Delta m = \text{Total nucleon mass} - \text{Nucleus mass} \]
Binding energy is the energy required to disassemble a nucleus into its constituent protons and neutrons. This energy is directly proportional to the mass defect, as described by Einstein's equation:
\[ E = \Delta m c^2 \]
Here, \( \Delta m \) signifies the mass defect, \( c \) is the speed of light, and \( E \) represents the binding energy.
Nuclear fission describes the fragmentation of a heavy nucleus, such as uranium-235, into two or more lighter nuclei, accompanied by a significant energy release. This process is initiated when a nucleus captures a neutron, rendering it unstable. During fission: