Q.A given coin has a mass of 3.0 g. Calculate the nuclear energy that would be required to separate all the neutrons and protons from each other. For simplicity assume that the coin is entirely made of 2963Cu atoms (of mass 62.92960 u).
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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Mass Energy Equivalence
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 energy to pull every nucleon apart is the total nuclear binding energy of the coin, from the mass defect (E=Δmc2).
Mass defect per 2963Cu atom (29 protons + 34 neutrons, comparing atomic masses so electrons cancel):
Δm=29(1.007825)+34(1.008665)−62.92960=0.59193 u
Binding energy per atom:
Eatom=0.59193×931.5=551.4 MeV
Number of atoms in 3.0 g:
N=62.929603.0×6.022×1023=2.871×1022 …
Separating every nucleon in the coin means supplying the coin's total nuclear binding energy: the mass defect per 2963Cu atom (0.5919 u→551.4 MeV) times the 2.87×1022 atoms in 3.0 g, giving ≈2.5×1012 J.
To pull apart every proton and neutron in the coin, we must supply the total nuclear binding energy of every atom in it. Binding energy is what holds each nucleus together; by mass–energy equivalence it equals the mass defect converted to energy, E=Δmc2.
1. Mass defect of one 2963Cu atom
Copper-63 has Z=29 protons and N=63−29=34 neutrons. Since the quoted mass 62.92960 u is the atomic mass (it already includes the 29 electrons), we compare it against 29 hydrogen atoms plus 34 free neutrons, so the electron masses cancel exactly:
Δm=29m(1H)+34mn−m(63Cu)
Δm=29(1.007825)+34(1.008665)−62.92960
Δm=29.226925+34.294610−62.92960=0.591935 u
2. Binding energy per atom
Using 1 u=931.5 MeV/c2:
Eatom=0.591935×931.5=551.4 MeV
In SI units (1 MeV=1.602×10−13 J):
Eatom=551.4×1.602×10−13=8.833×10−11 J
3. Number of atoms in the coin
An atomic mass of 62.92960 u means a molar mass of 62.92960 g/mol, so …
Method: Mass Defect → Binding Energy (Mass-Energy Equivalence)
The idea is simple: the nucleus is held together by the strong force, and to pull it apart you must supply energy equal to the binding energy. That binding energy comes from the mass defect — the difference between the mass of the separated nucleons and the actual mass of the nucleus. Einstein’s E=mc2 converts that missing mass into energy.
Step 1 — Find the number of atoms in the coin
Mass of coin = 3.0 g=3.0×10−3 kg
Molar mass of 63Cu = 62.92960 g/mol (since 1 u ≈ 1 g/mol for this purpose)
Number of moles:
n=62.929603.0≈0.04767 mol
Number of atoms:
N=n×NA=0.04767×6.022×1023≈2.87×1022 atoms
Step 2 — Find the mass defect for one atom
For 2963Cu:
- Protons = 29, neutrons = 63−29=34
The given mass (62.92960 u) is an atomic mass, so pair it with the hydrogen ATOM mass (not the bare proton mass — that would silently drop 29 electron masses):
- Mass of a hydrogen atom = 1.007825 u
- Mass of a neutron = 1.008665 u
Total mass of 29 hydrogen atoms + 34 neutrons:
29(1.007825)+34(1.008665)=29.226925+34.29461=63.521535 u
Actual atomic mass of one 63Cu atom = 62.92960 u
Mass defect for one atom:
Δm=63.521535−62.92960=0.591935 u≈0.59193 u
Step 3 — Convert mass defect to energy per atom
Using 1 u=931.5 MeV/c2:
Eper atom=0.59193×931.5≈551.4 MeV
Step 4 — Total energy for the coin …
Common Mistakes on Mass–Energy Equivalence Problems
Mistake 1: Forgetting to convert mass from grams to atomic mass units
The coin's mass is given as 3.0 g, but the copper atom's mass is in atomic mass units (u). Many students directly use the gram value in Einstein's equation without converting.
How to avoid: First find how many copper atoms are in the coin. The mass of one 63Cu atom is 62.92960 u. Convert this to grams using 1 u=1.660539×10−27 kg, or better, use the fact that 1 u=1.660539×10−24 g.
Number of atoms N=mass of one atommass of coin=62.92960×1.660539×10−243.0
A shortcut that causes errors: some students divide 3.0 by 62.92960 directly, forgetting the conversion factor. This gives a meaningless number.
Mistake 2: Using the atomic mass instead of the mass defect
The energy required to separate all nucleons is the binding energy, which comes from the mass defect — not from the atomic mass itself.
Students often plug 62.92960 u into E=mc2 and get a huge number, not realising that this is the mass of the whole atom, not the missing mass.
How to avoid: The mass defect Δm is the difference between the mass of the separated nucleons and the actual mass of the nucleus.
For 2963Cu:
- Number of protons = 29
- Number of neutrons = 63−29=34
- Mass of 29 protons = 29×1.007276 u
- Mass of 34 neutrons = 34×1.008665 u
- Mass of 29 electrons = 29×0.000548 u (if using atomic masses)
Always check whether you're given atomic masses (include electrons) or nuclear masses. Here, 62.92960 u is the atomic mass of 63Cu, so you must account for electrons when computing the mass defect.
Mistake 3: Forgetting to multiply by the number of atoms
After finding the binding energy for one copper nucleus, students sometimes stop there. The question asks for the energy to separate all nucleons in the entire coin.
How to avoid: Once you have the binding energy per nucleus (in J or MeV), multiply by the number of atoms N found in Mistake 1.
Mistake 4: Unit confusion — mixing MeV, J, and u
Students often compute Δm in u, then use E=Δmc2 but forget that 1 u⋅c2=931.5 MeV. They might try to convert to joules incorrectly.
How to avoid: Use the conversion directly:
Eper nucleus=Δm (in u)×931.5 MeV/u …
- GUJCET 2026Set x1 markMCQQ.The energy equivalent of 1.0 kg of substance is ______. (A) 9×1013 J (B) 3×1013 J (C) 9×1016 J (D) 9×1014 J
›Reveal solutionSolution
Mass–energy equivalence: E=mc2=9×1016 J for 1 kg.
Einstein's mass–energy relation:
E=mc2
With m=1.0 kg and c=3×108 m/s: …
- GSEB Higher Secondary Certificate (HSC) Examination 2026Set ANNUAL1 markMCQQ.Equivalent energy of 2 g of substance is ___.(a) 18 x 10^13 J(b) 9 x 10^13 J(c) 6 x 10^11 J(d) 6 x 10^8 J
›Reveal solutionSolution
Mass-energy equivalence, E = m c^2, converts any mass entirely into energy; even a small mass corresponds to an enormous energy because c^2 is so large.
m = 2 g = 2 x 10^-3 kg, c = 3 x 10^8 m/s.
…
- GSEB Higher Secondary Certificate (HSC) Examination 2024Set ANNUAL1 markMCQQ.According to Einstein's mass-energy equivalent relation, the energy equivalent of 1mg of substance is ___. (Speed of light in vacuum C = 3 x 10^8 m/s)(a) 9 x 10^13 J(b) 9 x 10^10 J(c) 9 x 10^-13 J(d) 9 x 10^-10 J
›Reveal solutionSolution
Mass-energy equivalence: E = mc², where m is the rest mass and c is the speed of light in vacuum.
Given m = 1 mg = 1 × 10⁻⁶ kg, c = 3 × 10⁸ m/s.
…
- GUJCET 2023Set 091 markMCQQ.In proton-proton cycle in Sun the energy released when an electron & its antiparticle combines is ______. (A) 1.021×10−13 J (B) 0.672×10−13 J (C) 1.126×10−13 J (D) 1.632×10−13 J
›Reveal solutionSolution
[!TLDR] 2mec2=1.022 MeV =1.63×10−13 J.
Concept
In electron–positron annihilation the entire rest mass of both particles converts to energy (usually two gamma photons). Each has rest energy mec2=0.511 MeV, so the total released is 2×0.511=1.022 MeV.
Solution
Convert to joules: …
- GSEB Higher Secondary Certificate (HSC) Examination 2023Set ANNUAL1 markMCQQ.According to mass energy equivalence relation, 9 x 10^13 J of energy can be converted into ___ maximum mass. [Speed of light c = 3 x 10^8 m/s](a) 81 g(b) 9 g(c) 3 g(d) 1 g
›Reveal solutionSolution
Mass-energy equivalence m = E/c^2 gives 9x10^13/(9x10^16) = 10^-3 kg = 1 g.
Einstein's relation: E = m c^2, so m = E/c^2.
…
- GSEB Higher Secondary Certificate (HSC) Examination 2023Set ANNUAL1 markMCQQ.One of the fusion reaction in Sun is given by (2,1)H + (1,1)H -> (3,2)He + gamma + ___. Fill in the blank with correct option.(a) 1.02 MeV(b) 5.49 MeV(c) 12.86 MeV(d) 0.42 MeV
›Reveal solutionSolution
The deuterium-proton fusion d + p -> He-3 + gamma releases 5.49 MeV; this is a known step of the solar proton-proton cycle.
The reaction (2,1)H + (1,1)H -> (3,2)He + gamma is the second step of the proton-proton fusion chain that powers the Sun.
…
- GUJCET 2022Set 171 markMCQQ.Given the following atomic masses: 92238U=238.05079 u, 24He=4.00260 u, 90234Th=234.04363 u. Calculate the energy released during the alpha decay of 92238U. (1u=931.5 MeV/c2) (A) 4.25 MeV (B) 6.23 MeV (C) 5.75 MeV (D) 3.25 MeV
›Reveal solutionSolution
Energy released =Δm×931.5 MeV.
Steps.
- Δm=238.05079−(234.04363+4.00260)=0.00456 u. …
- GUJCET 2020Set 071 markMCQQ.Calculate the energy equivalent of 1g of substance (A) 6×1011 J (B) 9×1013 J (C) 4×1012 J (D) 7×1012 J
›Reveal solutionSolution
Mass–energy equivalence: E=mc2 with m=1 g =10−3 kg.
Concept: E=mc2 where m=1g=10−3kg and c=3×108m/s: …
- GUJCET 2015Set C1 markMCQQ.The energy released by the fission of one uranium atom is 200 MeV. The number of fission per second required to produce 6.4 W power is _____. (A) 2×1011 (B) 1011 (C) 1010 (D) 2×1010
›Reveal solutionSolution
[!TLDR] n=P/Efission=2×1011 fissions per second.
Concept
Power is energy released per unit time. If each fission releases energy E, then producing power P requires n=P/E fissions per second.
Solution …
- GUJCET 2014Set A1 markMCQQ.The binding energy per nuclean of 8O16 is 7.97 MeV and that of 8O17 is 7.75 MeV. The energy required to remove one neutron from 8O17 is __________ MeV. (A) 3.52 (B) 3.62 (C) 4.23 (D) 7.86
›Reveal solutionSolution
[!TLDR]
Energy to remove a neutron = BE(O-17) - BE(O-16) = 131.75−127.52=4.23 MeV. Answer: (C).
Concept
The binding energy of a nucleus is (BE per nucleon) x (number of nucleons). Removing one neutron from 8O17 leaves 8O16; the energy needed equals the difference between the total binding energies of the two nuclei (NCERT/CBSE nuclei chapter).
Solution
Total binding energy of 8O17 (17 nucleons):
BE17=7.75×17=131.75 MeV …
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