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A Level · Cambridge (CIE) · 9702

Use gravitational potential energy for point masses

Connect potential to the energy of a test mass, use Ep = −GMm/r and interpret energy changes between orbital radii.

Gravitational fields · Cambridge International AS & A Level Physics 9702 · 13.4

A Level; Cambridge International Physics 9702, 2025–2027 syllabus, Topic 13. These original explanations and calculations are study aids; full timed assessment and human subject-teacher review remain outstanding.

Before you begin

  • Use Newton's laws, circular motion, vectors, scientific notation and SI units.

Work on paper. Try each question before revealing help, and explain why your method works.

Quick readiness check

How do you obtain a test mass's gravitational potential energy from potential?

What you will learn

  • Relate gravitational potential to potential energy per unit mass
  • Use Ep = −GMm/r for two point masses
  • Calculate energy changes relative to infinity

Potential energy is mass multiplied by potential

A test mass m at potential φ has gravitational potential energy Ep = mφ. Substituting φ = −GM/r gives Ep = −GMm/r for two point masses with zero potential energy at infinite separation.

The energy is negative for a bound pair because work must be supplied to separate the masses to infinity. The equation uses centre-to-centre distance and masses in kilograms.

Compare positions by taking an energy difference

When a mass moves from r₁ to r₂, its energy change is ΔEp = Ep₂ − Ep₁. Moving outward makes the value less negative, so ΔEp is positive and energy must be supplied against gravity.

Near Earth's surface, mgΔh is a useful approximation for small height changes. The point-mass formula describes larger changes in distance and uses the zero at infinity; do not mix the two reference conventions without calculating a difference.

Ep = −GMm/r · ΔEp = Ep₂ − Ep₁

Pause and explain

What is Ep for two positive point masses at a finite separation using zero at infinity?

Put the idea to work

Worked example

Find the gravitational potential energy of a 2.0 kg mass at radius 2.0 × 10⁷ m from a point mass 6.0 × 10²⁴ kg.

Show the worked solution
  1. Use Ep = −GMm/r.
  2. Substitute −6.67 × 10⁻¹¹ × 6.0 × 10²⁴ × 2.0 / 2.0 × 10⁷.
  3. Give joules and preserve the sign.

Answer Ep ≈ −4.0 × 10⁷ J.

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From guided practice to a new situation

Write your answer and reasoning first. Use a hint only if you are stuck. The model solution is for self-checking; your written work is not automatically marked.

1 · Guided

Calculate Ep for masses 3.0 kg and 4.0 kg separated by 0.50 m.

Give me a hint

Use −Gm₁m₂/r, distinguish this energy in joules from potential in J kg⁻¹.

Compare my reasoning
  1. Ep = −Gm₁m₂/r.
  2. Ep = −(6.67 × 10⁻¹¹)(3.0)(4.0)/0.50.
  3. Evaluate in joules.

Ep ≈ −1.6 × 10⁻⁹ J.

Look for these in your work

  • Both masses included
  • Separation not squared
  • Negative energy and unit stated
2 · Independent

A satellite moves from r₁ = 2.0 × 10⁷ m to r₂ = 4.0 × 10⁷ m around a mass 6.0 × 10²⁴ kg. Find the change in Ep for a 2.0 kg satellite.

Give me a hint

Calculate each negative energy, then subtract initial energy from final energy.

Compare my reasoning
  1. Ep₁ = −GMm/r₁ ≈ −4.00 × 10⁷ J.
  2. Ep₂ = −GMm/r₂ ≈ −2.00 × 10⁷ J.
  3. ΔEp = Ep₂ − Ep₁ ≈ +2.00 × 10⁷ J.

The potential energy increases by about 2.0 × 10⁷ J as the satellite moves outward.

Look for these in your work

  • Both endpoint energies calculated
  • Final minus initial used
  • Positive outward change interpreted
3 · Transfer

A student says negative gravitational potential energy means the satellite has negative mass. Correct the interpretation.

Give me a hint

Separate the sign of a chosen energy reference from the sign of the physical mass.

Compare my reasoning
  1. The masses are positive.
  2. Zero potential energy is defined at infinite separation.
  3. At finite separation the bound pair has lower energy, so Ep is negative; separating it requires positive work.

Negative Ep describes energy below the zero-at-infinity reference, not negative mass.

Look for these in your work

  • Mass sign distinguished
  • Reference explained
  • Energy meaning corrected

Common mistakes

  • Confusing potential with potential energy
  • Dropping the negative sign on a bound pair's energy
  • Using mgΔh for a change comparable with the planet's radius
Recall without your notes

What can you explain now?

How do you obtain a test mass's gravitational potential energy from potential?

Compare with the explanation

Multiply potential by the mass

Ep = mφ, with joules as the resulting unit.

After trying it yourself, choose your next review. This is your self-assessment.

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Make it stick

Why does moving a satellite outward from a planet increase its gravitational potential energy?

If you needed the solution, close it and solve the problem again from a blank page. A correct answer is stronger when you can explain the reason for each step.

Keep learning Physics

Course scope and assessment

One hundred and sixty-two original lessons cover all 12 published subject-content outcomes in Topic 1 (sections 1.1–1.4), all nine outcomes in Topic 2 (section 2.1), all 13 outcomes in Topic 3 (sections 3.1–3.3), all 13 outcomes in Topic 4 (sections 4.1–4.3), all 11 outcomes in Topic 5 (sections 5.1–5.2), all 10 outcomes in Topic 6 (sections 6.1–6.2), all 16 outcomes in Topic 7 (sections 7.1–7.5), all 12 outcomes in Topic 8 (sections 8.1–8.4), all 15 outcomes in Topic 9 (sections 9.1–9.3), all 16 outcomes in Topic 10 (sections 10.1–10.3), all 18 outcomes in Topic 11 (sections 11.1–11.2), all seven outcomes in Topic 12 (sections 12.1–12.2), all 12 outcomes in Topic 13 (sections 13.1–13.4), all eight outcomes in Topic 14 (sections 14.1–14.3), and all nine outcomes in Topic 15 (sections 15.1–15.3), plus all four outcomes in Topic 16 (sections 16.1–16.2), and all ten outcomes in Topic 17 (sections 17.1–17.3), plus all 12 outcomes in Topic 18 (sections 18.1–18.5), all nine outcomes in Topic 19 (sections 19.1–19.3), all 19 outcomes in Topic 20 (sections 20.1–20.5), and all eight outcomes in Topic 21 (sections 21.1–21.2), and all 17 outcomes in Topic 22 (sections 22.1–22.4), and all 13 outcomes in Topic 23 (sections 23.1–23.2), and all 16 outcomes in Topic 24 (sections 24.1–24.3), and all 11 outcomes in Topic 25 (sections 25.1–25.3), of the 2025–2027 syllabus. Each lesson has guided, independent and application practice with explained answers. All 25 syllabus topics now have mapped teaching and practice; the 2028–2030 changes outside Topics 23–25 still need reconciliation. Online study cannot demonstrate supervised Paper 3 laboratory competence. Paper 5 planning and analysis, full timed cumulative assessment and human subject-teacher review remain outstanding.

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