Binding Energy Calculator

Calculate nuclear binding energy, mass defect, and binding energy per nucleon from isotope mass data.

Important: Atomic masses include electrons. Nuclear masses do not. This calculator supports both methods and uses the correct mass formula for each input type.

About the Author: Created by Fotios Angelakis, MSc in Mechanical Engineering, with experience in engineering calculations, data analytics, and energy systems. Learn more about the author's qualifications and experience.

Enter isotope data or select an isotope to calculate binding energy.

What Is Nuclear Binding Energy?

Nuclear binding energy is the energy required to separate a nucleus into its individual protons and neutrons. It is also the energy released when the nucleus is formed from separated nucleons.

A higher binding energy per nucleon generally means a more tightly bound and stable nucleus. Binding energy is central to nuclear physics, fission, fusion, radioactive decay, and stellar energy production.

Bound nucleus Energy input Separated nucleons Mass of bound nucleus is lower Mass defect becomes energy

Binding Energy Formula

Binding energy is calculated from the mass defect:

BE = Δm × 931.494 MeV/u

where Δm is the mass defect in atomic mass units.

Atomic Mass Formula

Most isotope tables give the mass of the neutral atom, not the bare nucleus. When using atomic mass, use:

Δm = ZmH + Nmn - Matom

where:

  • Z = number of protons
  • N = A - Z = number of neutrons
  • mH = mass of hydrogen atom
  • mn = mass of neutron
  • Matom = neutral atomic mass

Nuclear Mass Formula

If you are using the mass of the bare nucleus only, use:

Δm = Zmp + Nmn - Mnucleus

where mp is the proton mass and Mnucleus is the nuclear mass without electrons.

Binding Energy Per Nucleon

Binding energy per nucleon is:

BE/A

This value is useful for comparing nuclear stability across different isotopes.

How to Use the Calculator

  1. Choose custom data or select an isotope from the list.
  2. If entering custom data, choose whether your mass is atomic mass or nuclear mass.
  3. Enter atomic number Z, mass number A, and mass in atomic mass units.
  4. Click calculate to get mass defect, total binding energy, and binding energy per nucleon.

Example: Iron-56

Iron-56 has Z = 26 and A = 56. Using atomic mass data, the calculator applies:

Δm = 26mH + 30mn - Matom

The total binding energy is then:

BE = Δm × 931.494 MeV/u

Dividing by 56 gives the binding energy per nucleon.

Typical Binding Energy Per Nucleon

Region Typical Behavior
Light nucleiBinding energy per nucleon generally rises as nuclei become heavier.
Iron/nickel regionAmong the highest binding energy per nucleon values.
Very heavy nucleiBinding energy per nucleon slowly decreases.

Important Assumptions

  • Masses are treated using atomic mass units.
  • The energy equivalent used is approximately 931.494 MeV/u.
  • Electron binding energies are very small compared with nuclear binding energies and are ignored in the atomic-mass method.
  • Isotope list values are neutral atomic masses.
  • For high-precision nuclear data, use official evaluated atomic mass tables.
Scientific note: Do not mix atomic mass and nuclear mass formulas. If your mass comes from an isotope table, it is usually atomic mass, so the hydrogen atom mass formula is the correct approach.

Frequently Asked Questions

What is binding energy?

Binding energy is the energy required to separate a nucleus into its protons and neutrons.

What is mass defect?

Mass defect is the difference between the mass of separated nucleons and the measured mass of the bound atom or nucleus.

Why is binding energy per nucleon important?

Binding energy per nucleon helps compare nuclear stability. Higher values generally mean the nucleus is more tightly bound.

Why does the calculator ask for atomic mass or nuclear mass?

Atomic mass includes electrons, while nuclear mass does not. The correct mass-defect formula depends on which type of mass you enter.

How is binding energy related to fission and fusion?

Fission and fusion release energy when the products have a higher total binding energy per nucleon than the reactants.