The binding energy per nucleon remains nearly constant in medium-sized nuclei due to the short-range nature of nuclear forces. Nuclear forces act only between nearest neighboring nucleons, meaning that even as the number of nucleons increases, each nucleon primarily interacts with a limited number of nearby nucleons, leading to binding energy saturation.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of