Q.Obtain the binding energy of the nuclei 2656Fe and 83209Bi in units of MeV from the following data:
m(2656Fe)=55.934939 u,
m(83209Bi)=208.980388 u.
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Mass Energy Equivalence: From Intuition to the Formula
Imagine you have a lump of coal. You know you can burn it to get heat, and that heat can run a steam engine. The energy you get out seems to come from the chemical bonds in the coal. But what if I told you that the coal itself — just sitting there, not burning — already contains a staggering amount of energy locked inside its very mass? That is the core idea of mass-energy equivalence.
The Intuition: Mass is Frozen Energy
Think of mass as a kind of "frozen" or "stored" energy. When you burn coal, you are only releasing a tiny fraction of this stored energy — the energy in the chemical bonds. The rest of the mass remains as matter. But if you could somehow completely convert that lump of coal into pure energy, you would get an unimaginable amount — enough to power a city for years.
This is not a metaphor. Mass and energy are not two separate things that can be converted into each other like dollars and rupees. They are the same fundamental thing, just in different forms. Mass is a highly concentrated form of energy. Energy, when concentrated enough, behaves like mass.
The Precise Statement
The relationship is given by the most famous equation in physics:
E=mc2
Where:
- E is the energy equivalent of the mass (in joules, J)
- m is the mass (in kilograms, kg)
- c is the speed of light in vacuum (3×108 m/s)
The speed of light is a huge number. Squaring it makes it enormous. This is why a tiny amount of mass corresponds to a colossal amount of energy.
What This Equation Actually Means
The equation tells you exactly how much energy is "stored" inside any object with mass m. If you could annihilate that mass completely, you would get E joules of energy.
Example: A 1 kg mass (like a litre of water) contains:
E=1×(3×108)2=9×1016 J
That is 90 quadrillion joules — roughly the energy released by a 20-megaton nuclear bomb. This is not energy you can normally access; it is locked inside the nucleus of atoms.
Where Does This Show Up in Real Life?
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Nuclear Reactions: In nuclear fission (splitting atoms) or fusion (joining atoms), a tiny fraction of the mass of the nucleus is converted into energy. The mass of the products is slightly less than the mass of the reactants. The "missing" mass has become energy — exactly as E=mc2 predicts. This is how the Sun works and how nuclear power plants generate electricity.
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Particle Physics: When a particle and its antiparticle meet, they annihilate completely into pure energy (usually gamma rays). The energy produced equals mc2 for the two particles. …
Why this formula?
Why E=mc2 — The Reasoning Behind Mass-Energy Equivalence
The formula E=mc2 is not a random guess. Einstein arrived at it by thinking deeply about what happens to energy when you move an object. The core insight: if an object gains energy, it must behave as if it has gained mass.
The Starting Point: Relativistic Momentum
In special relativity, the momentum of a particle is not simply p=mv. Instead, it is:
p=1−v2/c2m0v
where m0 is the rest mass (mass measured when the object is at rest). This formula already tells us something strange: as speed approaches c, momentum shoots toward infinity — no object with mass can reach the speed of light.
The Energy-Momentum Relation
Einstein then asked: what is the correct expression for kinetic energy that matches this new momentum? In classical physics, kinetic energy is K=21mv2. But that formula fails at high speeds.
The relativistic kinetic energy turns out to be:
K=1−v2/c2m0c2−m0c2
This looks odd — why subtract m0c2? Because when v=0, the first term becomes m0c2, and we want K=0 at rest. So the subtraction gives zero kinetic energy when the object is stationary.
The term m0c2 appears naturally as a rest energy — energy that an object has simply because it has mass, even when completely at rest.
The Crucial Step: What Happens When You Add Energy?
Now consider a box that emits light (photons) in opposite directions. The light carries away energy. Classical physics says the box loses energy but its mass stays the same. Einstein showed this cannot be true.
The argument (simplified): if the box emits a pulse of light with energy E, the light carries momentum p=E/c. By conservation of momentum, the box recoils. But after the light is absorbed by the opposite wall, the box stops. The net effect: the box has moved slightly. Its center of mass has shifted — unless the energy carried by the light also carried mass.
For the center of mass of the entire system (box + light) to remain stationary, the light must behave as if it has an effective mass m=E/c2. Therefore, energy itself has inertia.
The Full Formula
The total energy of any object — moving or at rest — is:
E=1−v2/c2m0c2
For an object at rest (v=0), this reduces to:
E=m0c2
For a moving object, the total energy is the sum of rest energy and kinetic energy:
E=m0c2+K
E=mc2
where m is the relativistic mass m=1−v2/c2m0, or equivalently:
E2=(pc)2+(m0c2)2
Why It's Not Just a "Conversion" …
The binding energy is the energy equivalent of the mass defect, B=[ZmH+(A−Z)mn−M]c2, using atomic masses with 1 u=931.5 MeV/c2, mH=1.007825 u, mn=1.008665 u.
2656Fe (Z=26, N=30):
Δm=26(1.007825)+30(1.008665)−55.934939=56.463400−55.934939=0.528461 u,
B=0.528461×931.5≈492.3 MeV.
83209Bi (Z=83, N=126): …
Converting the mass defect to energy with 1 u=931.5 MeV/c2 gives binding energies B(2656Fe)≈492.3 MeV and B(83209Bi)≈1640.2 MeV.
Principle
The measured mass of a nucleus is less than the total mass of its separate protons and neutrons. This missing mass — the mass defect Δm — is the mass equivalent of the energy that binds the nucleons together. The binding energy is
B=[ZmH+(A−Z)mn−M]c2.
Because the tabulated nuclear masses are atomic masses (they include the electrons), we use the hydrogen-atom mass mH=1.007825 u for each proton so the electron masses cancel. With mn=1.008665 u and 1 u=931.5 MeV/c2, multiplying Δm (in u) by 931.5 gives B in MeV directly.
2656Fe (Z=26, N=30)
Mass of the constituents:
26×1.007825=26.203450 u,30×1.008665=30.259950 u,
total=56.463400 u.
Mass defect:
Δm=56.463400−55.934939=0.528461 u.
Binding energy:
B=0.528461×931.5≈492.3 MeV.
83209Bi (Z=83, N=126)
Mass of the constituents: …
Method: Mass Defect → Binding Energy (Einstein’s mass-energy equivalence)
The binding energy of a nucleus is the energy required to separate it into its individual protons and neutrons. It is found by first calculating the mass defect — the difference between the mass of the separated nucleons and the actual nuclear mass — then converting that mass difference into energy using E=Δmc2, with the conversion factor 1 u=931.5 MeV/c2.
Steps for each nucleus:
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Identify the number of protons (Z) and neutrons (N).
For 2656Fe: Z=26, N=56−26=30.
For 83209Bi: Z=83, N=209−83=126.
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Write the mass of the separated constituents — atomic mass throughout.
The given nuclear masses are atomic masses (electrons included), so pair them with the hydrogen ATOM mass mH=1.007825 u (not the bare proton mass mp=1.007276 u — that would silently drop Z electron masses) and the neutron mass mn=1.008665 u.
Total mass of constituents = Z⋅mH+N⋅mn.
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Compute the mass defect Δm.
Δm=(mass of constituents)−(actual atomic mass).
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Convert Δm to energy.
Binding energy B=Δm×931.5 MeV.
B=[ZmH+Nmn−matom]×931.5 MeV
For 2656Fe:
- Constituent mass = 26×1.007825+30×1.008665 =26.203450+30.259950=56.463400 u.
- Δm=56.463400−55.934939=0.528461 u.
- B=0.528461×931.5≈492.3 MeV.
For 83209Bi:
- Constituent mass = 83×1.007825+126×1.008665 …
Common Mistakes in Nuclear Binding Energy Calculations
Students often lose marks on this exact type of problem. Here are the most frequent errors and how to avoid each.
Mistake 1: Forgetting to account for electrons in atomic masses
The given masses are atomic masses (include electrons), but the binding energy formula uses nuclear masses. The mass of Z electrons is already in the atomic mass — if you subtract only the proton mass from the atomic mass, you double-count the electrons.
How to avoid: Use the standard shortcut: treat the hydrogen atom mass m(1H)=1.007825 u as the combined mass of one proton and one electron. Then:
B=[Z⋅m(1H)+N⋅mn−m(ZAX)]×931.5 MeV/u
This automatically handles the electron mass correctly.
Mistake 2: Using wrong number of neutrons
For 2656Fe, N=56−26=30. For 83209Bi, N=209−83=126. Students sometimes confuse A and Z or subtract incorrectly.
How to avoid: Write N=A−Z clearly before plugging in. Double-check: the mass number A is the superscript, atomic number Z is the subscript.
Mistake 3: Using proton mass instead of hydrogen mass
If you use mp=1.007276 u directly, you must also add Z⋅me separately. Most students forget the electron term.
How to avoid: Stick to the hydrogen-atom shortcut above. It's the standard method in NCERT and all board exams.
Mistake 4: Arithmetic errors in the mass defect
The mass defect Δm is small — a few tenths of a u. Students often misalign decimal places when subtracting.
For Fe:
- Z⋅m(1H)=26×1.007825=26.20345 u
- N⋅mn=30×1.008665=30.25995 u
- Sum = 56.46340 u
- Subtract m(56Fe)=55.934939 u
- Δm=0.528461 u
How to avoid: Write each term to 6 decimal places and subtract carefully. Use column subtraction, not mental math.
Mistake 5: Using 931 MeV/u incorrectly …
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