A nucleon has more mass when it is not bound to the nucleus of an atom.
When the nucleon is bound to other nucleons the binding energy that keeps them together comes from the mass of the nucleon. Therefore the mass of a single nucleon will be smaller in an atom than on it's own.
The binding energy per nucleon peaks at a mass number of around 56.
The binding energy per nucleon varies with mass number because it represents the average energy required to separate a nucleus into its individual nucleons. For lighter nuclei, the binding energy per nucleon increases as the nucleus becomes more stable. As nuclei become larger (higher mass number), the binding energy per nucleon decreases due to the diminishing strength of the nuclear force relative to the electrostatic repulsion between protons.
The order of binding energy per nucleon for nuclei generally follows the trend that larger nuclei have higher binding energy per nucleon. This means that as you move to heavier nuclei (with more protons and neutrons), their binding energy per nucleon tends to increase. This trend is due to the strong nuclear force that holds the nucleus together becoming more efficient as the nucleus grows in size.
The binding energy per nucleon graph shows that the higher the binding energy per nucleon, the more stable the nucleus is. In nuclear reactions, energy is released when the reactants form products with higher binding energy per nucleon, indicating a more stable configuration.
The nucleon number, also known as the mass number, can be found by adding the number of protons and neutrons in an atomic nucleus. It is represented by the letter A in the notation of an element's isotopes.
The binding energy per nucleon peaks at a mass number of around 56.
This is not something I really know anything about, but I do know that energy is liberated in the process, so you could expect it to be less in the fission fragments. It also depends on the nucleus. Proton and neutron masses differ somewhat, so it depends on what the ratio of protons and neutrons is as well.
The uranium nucleus has over 200 MeV more mass than the sum of the masses of the fission product nuclei plus the free neutrons emitted. Most of this energy appears as the kinetic energy of those particles and manifests as heat energy. Enough heat energy to cause the air around a bomb to radiate x-rays.
The binding energy per nucleon varies with mass number because it represents the average energy required to separate a nucleus into its individual nucleons. For lighter nuclei, the binding energy per nucleon increases as the nucleus becomes more stable. As nuclei become larger (higher mass number), the binding energy per nucleon decreases due to the diminishing strength of the nuclear force relative to the electrostatic repulsion between protons.
The mass per nucleon decreases when uranium is split into smaller nuclei through fission. This is because energy is released during the fission process, leading to a conversion of mass to energy based on Einstein's equation (E=mc^2).
The nucleon number (or mass number).
Nucleon Number (total number of protons and neutrons)
For helium the binding energy per nucleon is 28.3/4 = 7.1 MeV. The helium nucleus has a high binding energy per nucleon and is more stable than some of the other nuclei close to it in the periodic table.
The mass of an atomic nucleon is approximately 1 atomic mass unit (u) or 1.66 x 10^-27 kg. This value is commonly used as a reference unit for expressing the masses of atomic particles such as protons and neutrons.
The order of binding energy per nucleon for nuclei generally follows the trend that larger nuclei have higher binding energy per nucleon. This means that as you move to heavier nuclei (with more protons and neutrons), their binding energy per nucleon tends to increase. This trend is due to the strong nuclear force that holds the nucleus together becoming more efficient as the nucleus grows in size.
The mass number also refers to the nucleon number. Usually the larger number among the two present in the periodic table, the nucleon number refers to the number of protons and neutrons present within an atomic nucleus of an element.
The binding energy per nucleon graph shows that the higher the binding energy per nucleon, the more stable the nucleus is. In nuclear reactions, energy is released when the reactants form products with higher binding energy per nucleon, indicating a more stable configuration.