Binding Energy
Key idea: Define nuclear binding energy, relate it to mass defect using E_b = Δm c^2, and use it to compare nuclear stability (A Level Physics).
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The core idea
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Learning objectives
- Use mass-energy equivalence, mass defect and binding energy.
1. Definitions (Must Know)
A. Nuclear binding energy, E_b
The nuclear binding energy, E_b, is the energy required to separate a nucleus completely into its individual nucleons (protons and neutrons).
B. Relationship with mass defect
If a nucleus has mass defect Δ m, then: E_b = Δ m c²
Equivalently (energy conservation form): m_nucleusc² + E_b = (sum of nucleon rest energies)
2. Key Ideas (What Earns Marks)
- Binding energy is a measure of how strongly nucleons are bound in the nucleus.
- Mass defect exists because energy is released when the nucleus forms: E_b = Δ m c²
- Larger binding energy per nucleon usually means greater stability (handled in the next lesson).
“Binding energy is the energy needed to separate the nucleus into its nucleons.”
3. Detailed Explanations
A. Why bound nuclei have smaller mass
When nucleons bind, energy is released. The system’s mass decreases by Δ m so that mass–energy is conserved: E_b = Δ m c²
B. What binding energy tells you physically
A larger binding energy means you must do more work against the strong nuclear force to pull the nucleus apart.
4. Common Mistakes
- Defining binding energy as “energy released in decay” (it is the energy to separate the nucleus).
- Mixing up binding energy (total) with binding energy per nucleon (average).
- Using Δ m with the wrong sign (use Δ m = m_separated-m_bound).
5. Exam Tips
- In calculations: find Δ m first, then multiply by c².
- Keep units consistent: u → kg before using c in SI, or use 1u c² ≈ 931 MeV (if allowed/given).
- If asked about stability: mention “binding energy per nucleon”, not total binding energy.
6. Worked Examples
Modelled example 1
Binding energy from a mass defect (in u)
Problem
Study the worked solution
Convert mass to SI
Method
Δ m = 2.49 × 10⁻²⁹ kg.Reason
The SI form E = mc² returns joules only when mass is in kilograms.Working
Δ m = 0.0150(1.66 × 10⁻²⁷) = 2.49 × 10⁻²⁹ kgApply mass–energy equivalence
Method
E_b = 2.24 × 10⁻¹² J.Reason
The mass defect is the energy equivalent of nuclear binding.Working
E_b = (2.49 × 10⁻²⁹)(3.00 × 10⁸)² = 2.24 × 10⁻¹² J
Guided practice 2
Meaning question
Problem
Try this before viewing the solution
Hints
Hint 1: return to the definition
View solution step by step
State the interpretation
Method
The nucleons are more strongly bound: more energy is required to separate the nucleus completely.Reason
Binding energy is defined as separation energy for that nucleus.Working
larger E_b → more separation workLimit the comparison
Method
For nuclei with different nucleon numbers, stability comparisons should use binding energy per nucleon.Reason
A larger nucleus can have greater total binding energy simply because it contains more nucleons.Working
stability comparison: E_b/A
Common misconception 3
Binding energy using the u to MeV shortcut
Learner claim
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View solution step by step
Read the conversion factor
Method
Multiply mass in u by 931 MeV per u.Reason
The factor states the energy equivalent of one atomic mass unit.Working
E_b = (0.025 u)(931 MeV/u)Evaluate
Method
E_b = 23.3 MeV.Reason
The atomic-mass unit cancels, leaving energy.Working
E_b = 0.025(931) = 23.3 MeV
Examiner practice 4
Mass defect from binding energy
Examination question
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View solution step by step
Reverse the conversion
1 markMethod
Δ m = E_b/(931 MeV/u).Reason
Energy is being converted back to its mass equivalent.Working
Δ m = 28.0/931 uEvaluate
1 markMethod
Δ m = 3.01 × 10⁻² u ≈ 0.030 u.Reason
The result is a mass expressed in atomic mass units.Working
Δ m = 3.01 × 10⁻² u
Self-mark with the mark scheme
Compare your response with each mark point. Select a point only when your response contains that evidence.
Self-mark the inverse conversion and mass defect.
Challenge 5
Comparing stability (binding energy per nucleon)
Independent transfer
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Hints
Hint 1: normalise each total
View solution step by step
Calculate X average
Method
For X, E_b/A = 7.67 MeV per nucleon.Reason
Divide the whole-nucleus energy by its 12 nucleons.Working
(E_b/A)_X = 92/12 = 7.67 MeVCalculate Y average
Method
For Y, E_b/A = 7.50 MeV per nucleon.Reason
Use the same average for a fair comparison.Working
(E_b/A)_Y = 120/16 = 7.50 MeVCompare stability
Method
X is slightly more tightly bound by this measure.Reason
Its binding energy per nucleon is larger even though its total binding energy is smaller.Working
7.67 > 7.50
7. Mind Stretchers
Mind stretcher 1: Why can a nucleus release energy if it forms from nucleons?Extension
Show Answer
Because the bound nucleus has lower total energy (and lower mass) than the separated nucleons. The difference is released (often as kinetic energy and gamma radiation) when the nucleus forms.
Mind stretcher 2: Why is binding energy not “stored chemical energy”?Extension
Explain why nuclear binding energy is much larger than chemical bond energies, even though both involve “binding”.
Show Answer
Chemical bonds involve electromagnetic interactions between electrons and nuclei, with energy scales typically eV per bond.
Nuclear binding energy comes from the strong nuclear force acting at femtometre distances between nucleons, giving MeV-scale energy changes per nucleon, which is much larger.
Continue with the next resource in this course.
Course and syllabus information
- Course
- GCE A-Level H2 Physics
- Edition
- GCE A-Level H2 Physics 2027