The Curve Of Binding Energy Access

Light nuclei move "up" the curve to become more stable by fusing together. This process powers stars like our Sun.

Heavy, less stable nuclei like Uranium-235 split into smaller fragments. These fragments are closer to the iron peak, meaning they have higher binding energy and release the "missing" energy during the split. Stellar Nucleosynthesis The curve of binding energy

The curve of binding energy is a graph that plots against the atomic mass number ( Light nuclei move "up" the curve to become

) . It illustrates the stability of atomic nuclei and explains why certain nuclear reactions—like fusion and fission—release energy. Peak Stability: The curve peaks around a mass number of to The curve of binding energy