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Q.Explain the terms mass defect and binding energy. How are they related ?

Yanam CbseCBSE Class XII Board 2026Subjective· 2mImportance★★★★★
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Mass defect is the difference between the actual mass of a nucleus and the sum of the masses of its individual nucleons; binding energy is the energy equivalent of this mass defect, given by E=Δmc2E = \Delta m c^2, and it represents the energy required to break the nucleus apart.

The Core Idea

When you add up the masses of the protons and neutrons that make up a nucleus, you get a number that is larger than the mass of the actual nucleus itself. That missing mass is the mass defect. It isn't really "lost" — it has been converted into the energy that holds the nucleus together, called the binding energy. This is a direct consequence of Einstein's famous equation E=mc2E = mc^2, which tells us that mass and energy are two sides of the same coin.

Think of it this way: to assemble a nucleus from its individual nucleons, you would need to supply energy to overcome the electrostatic repulsion between protons. But nature does the opposite — when nucleons come together, they release energy (the binding energy), and that released energy carries away some mass. So the assembled nucleus is lighter than its parts.

Step-by-Step Explanation

  1. Define mass defect (Δm\Delta m) For a nucleus with ZZ protons, NN neutrons, and mass MnucleusM_{\text{nucleus}}, the mass defect is:

Δm=[Zmp+Nmn]−Mnucleus\Delta m = [Z m_p + N m_n] - M_{\text{nucleus}}

where mpm_p is the mass of a proton and mnm_n is the mass of a neutron.

Watch out

A common mistake is to use atomic masses instead of nuclear masses. Atomic masses include electrons, so if you use them, you must subtract the electron masses correctly. For most exam problems, you'll be given nuclear masses directly or told to use atomic masses with the electron mass accounted for.

  1. Define binding energy (EbE_b) The binding energy is the energy released when a nucleus forms from its constituent nucleons. It is also the energy you would need to supply to break the nucleus apart. Using Einstein's mass-energy equivalence:

Eb=Δm⋅c2E_b = \Delta m \cdot c^2

where c=3×108 m/sc = 3 \times 10^8 \text{ m/s} is the speed of light.

  1. Understand the relationship

    The mass defect and binding energy are directly proportional. A larger mass defect means more mass has been converted into energy, so the nucleus is more tightly bound and has a larger binding energy. Conversely, a smaller mass defect means a less stable nucleus.

    Eb=Δm c2E_b = \Delta m \, c^2

  2. Why this matters for stability

    A more useful quantity for comparing nuclei is the binding energy per nucleon:

Binding energy per nucleon=EbA\text{Binding energy per nucleon} = \frac{E_b}{A}

where A=Z+NA = Z + N is the total number of nucleons.

  • Higher binding energy per nucleon → more stable nucleus.
  • Iron-56 has the highest binding energy per nucleon (~8.8 MeV), making it the most stable nucleus. …

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