Q.A given coin has a mass of 3.0g. 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 62.92960u).
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?
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.
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.
Note
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.
Important
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 massm=1−v2/c2m0, or equivalently:
Separating every nucleon in the coin means supplying the coin's total nuclear binding energy: the mass defect per 2963Cu atom (0.5919u→551.4MeV) times the 2.87×1022 atoms in 3.0g, giving ≈2.5×1012J.
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 62.92960u 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=0.591935u
2. Binding energy per atom
Using 1u=931.5MeV/c2:
Eatom=0.591935×931.5=551.4MeV
In SI units (1MeV=1.602×10−13J):
Eatom=551.4×1.602×10−13=8.833×10−11J
3. Number of atoms in the coin
An atomic mass of 62.92960u means a molar mass of 62.92960g/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 = 3.0g=3.0×10−3kg
Molar mass of 63Cu = 62.92960g/mol (since 1 u ≈ 1 g/mol for this purpose)
Number of moles:
n=62.929603.0≈0.04767mol
Number of atoms:
N=n×NA=0.04767×6.022×1023≈2.87×1022atoms
Step 2 — Find the mass defect for one atom
For 2963Cu:
Protons = 29, neutrons = 63−29=34
The given mass (62.92960u) is an atomic mass, so pair it with the hydrogen ATOM mass (not the bare proton mass — that would silently drop 29 electron masses):
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 3.0g, 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 62.92960u. Convert this to grams using 1u=1.660539×10−27kg, or better, use the fact that 1u=1.660539×10−24g.
Number of atoms N=mass of one atommass of coin=62.92960×1.660539×10−243.0
Watch out
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 62.92960u 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 = 29×1.007276u
Mass of 34 neutrons = 34×1.008665u
Mass of 29 electrons = 29×0.000548u (if using atomic masses)
Important
Always check whether you're given atomic masses (include electrons) or nuclear masses. Here, 62.92960u 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 1u⋅c2=931.5MeV. They might try to convert to joules incorrectly.