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A Level · Cambridge (CIE) · 9702

Define gravitational potential and calculate its value

Define gravitational potential relative to infinity and use the negative point-mass potential −GM/r.

Section 13 · Gravitational fields

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

Where is gravitational potential conventionally zero for an isolated point mass?

What you will learn

  • Define gravitational potential as work done per unit mass from infinity
  • Use φ = −GM/r for a point mass
  • Interpret negative potential and the zero at infinity

Potential is energy transferred per unit mass

Gravitational potential φ at a point is the work done per unit mass in bringing a small test mass from infinity to that point, with the usual zero of potential chosen at infinity. Potential is a scalar, measured in J kg⁻¹.

Gravity attracts, so an external agent bringing a test mass slowly from infinity does negative work: the field transfers energy to the motion unless the agent removes it. This reference choice makes the potential around an isolated mass negative.

A point mass has potential −GM/r

For a point mass M, φ = −GM/r. The potential becomes less negative as r increases and approaches zero at infinity. A stronger source mass makes the potential more negative at the same radius.

Do not confuse potential φ, which is energy per unit mass, with potential energy Ep for a particular mass. Multiplying φ by a test mass gives its gravitational potential energy.

φ = −GM/r · reference φ = 0 at infinity

Pause and explain

What is the sign of φ = −GM/r for positive M and r?

Put the idea to work

Worked example

Find the gravitational potential at radius 6.0 × 10⁶ m from a point mass of 6.0 × 10²⁴ kg.

Show the worked solution
  1. Use φ = −GM/r.
  2. Substitute 6.67 × 10⁻¹¹ × 6.0 × 10²⁴ / 6.0 × 10⁶.
  3. Retain the negative sign and give J kg⁻¹.

Answer φ ≈ −6.67 × 10⁷ J kg⁻¹.

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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 φ at radius 2.0 × 10⁷ m from a mass 6.0 × 10²⁴ kg.

Give me a hint

Substitute into −GM/r and keep the sign through the calculation.

Compare my reasoning
  1. φ = −GM/r.
  2. φ = −(6.67 × 10⁻¹¹)(6.0 × 10²⁴)/(2.0 × 10⁷).
  3. Give J kg⁻¹.

φ ≈ −2.0 × 10⁷ J kg⁻¹.

Look for these in your work

  • Potential equation used
  • Negative sign retained
  • Unit stated
2 · Independent

At a fixed distance, a source mass is tripled. How does its gravitational potential change?

Give me a hint

Use direct proportionality of φ to source mass while holding r fixed.

Compare my reasoning
  1. φ = −GM/r.
  2. With M replaced by 3M, φ₂ = −3GM/r.
  3. The potential remains negative and its magnitude triples.

The potential becomes three times as negative; its magnitude triples.

Look for these in your work

  • Distance held fixed
  • Mass proportionality applied
  • Sign and magnitude distinguished
3 · Transfer

Two points are at radii R and 2R from the same isolated mass. Compare their potentials.

Give me a hint

Apply the inverse-distance dependence, including the common negative sign.

Compare my reasoning
  1. φ(R) = −GM/R.
  2. φ(2R) = −GM/(2R) = φ(R)/2.
  3. The farther point has half the magnitude and is less negative.

At 2R the potential is half as negative as at R.

Look for these in your work

  • Equation applied twice
  • Radius ratio correct
  • Negative values interpreted

Common mistakes

  • Omitting the negative sign
  • Giving potential in joules instead of joules per kilogram
  • Setting potential to zero at the surface while using φ = −GM/r
Recall without your notes

What can you explain now?

Where is gravitational potential conventionally zero for an isolated point mass?

Compare with the explanation

At infinity

The potential approaches zero as the separation becomes very large.

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Make it stick

Why is gravitational potential negative when its zero is chosen at infinity?

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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