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v0.1.1065
NotesPhysics HLTopic 4.1Gravitational potential energy and potential (HL)
Back to Physics HL Topics
4.1.52 min read

Gravitational potential energy and potential (HL)

IB Physics • Unit 4

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Contents

  • Potential beyond the surface
  • Gravitational potential V_g
  • Gravitational potential energy E_p
  • Equipotentials and work done
  • In the exam
Why SL's mgh is not enough: Near the ground the field is roughly constant, so SL uses E_p = mgh. But over astronomical distances g changes with height (g = GM/r²), so that shortcut breaks down. HL replaces it with two exact field quantities:

- gravitational potential Vg — the PE per kilogram at a point - gravitational potential energy Ep — the PE of an actual mass m at that point
Where is 'zero'?: We set the zero of potential at infinity — infinitely far from every mass. Bring a mass in from infinity and it loses PE, so everywhere closer the value is negative.

The gravitational potential Vg at a point is the work done per unit mass to bring a small test mass from infinity to that point. Because gravity does the work for you on the way in, that work is negative — so Vg is negative and tends to zero at infinity.

Given in the data booklet. The minus sign and the zero-at-infinity convention come as a pair.
gravitational potential (J kg⁻¹)
gravitational constant, 6.67×10⁻¹¹ N m² kg⁻²
mass producing the field (kg)
distance from the centre of M (m)

Worked example — potential at Earth's surface

Earth has mass M = 6.0×10²⁴ kg and radius r = 6.4×10⁶ m. Find the gravitational potential at its surface. (G = 6.67×10⁻¹¹ N m² kg⁻²)

Solution

  1. Write the given formula first:
  2. Substitute the values:
  3. Work it out — keep the unit:

Final answer

Vg = −6.3×10⁷ J kg⁻¹. The minus sign shows you sit in a potential well.

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From potential to energy: Potential is per kilogram; multiply by the actual mass m to get the energy. So Ep = m × Vg, which gives the full-field expression below. Like Vg it is negative and zero at infinity.
Given in the data booklet. This replaces E_p = mgh once g can no longer be treated as constant.
gravitational potential energy (J)
mass placed in the field (kg)
mass producing the field (kg)
separation of the centres (m)

Worked example — PE of a satellite at the surface

Find the gravitational potential energy of a 500 kg satellite sitting at Earth's surface, where Vg = −6.3×10⁷ J kg⁻¹.

Solution

  1. Use the given relation between energy and potential:
  2. Substitute m = 500 kg and Vg = −6.3×10⁷ J kg⁻¹:
  3. Work it out — keep the unit:

Final answer

Ep = −3.1×10¹⁰ J (the same as −GMm/r). It is negative: energy must be added to lift the satellite away.

Surfaces of equal potential: An equipotential surface links all points at the same Vg. Around a point mass these are concentric spheres. They are always perpendicular to the field lines, and no work is done moving a mass along one (ΔVg = 0).

Field lines

  • Point radially inward toward the mass
  • Closer together where the field is stronger
  • Show the direction of the gravitational force

Equipotentials

  • Spheres of constant potential (rings in 2D)
  • Always perpendicular to the field lines
  • Moving along one does no work (ΔVg = 0)

To move a mass between equipotentials you do work equal to the mass times the change in potential. This is the HL way to find energy changes when g is not constant.

Given in the data booklet. Climbing to a higher (less negative) potential ⇒ positive work.
work done on the mass (J)
mass moved (kg)
change in gravitational potential, V_final − V_initial (J kg⁻¹)

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Where it shows up: Gravitational potential is HL only (D.1):

- Paper 1A — 'why is the potential negative?', 'which point has the larger V_g?', or 'how do equipotentials relate to field lines?'. - Paper 2 — determine Vg or Ep at a distance, or find the work (= mΔVg) to move a probe between two points.
Three easy marks: (1) Keep the minus sign — Vg and Ep are negative below infinity. (2) Use the separation of centres for r, not the height above the surface. (3) Work between points = m × (Vfinal − Vinitial), so a rise in potential gives positive work.

IB-style question — work to lift a probe

At a planet's surface the gravitational potential is −4.0×10⁷ J kg⁻¹; at the orbit of a probe it is −1.5×10⁷ J kg⁻¹. Determine the work needed to raise a 200 kg probe from the surface to that orbit.

Solution

  1. Use the given work formula:
  2. Find ΔVg = Vfinal − Vinitial:
  3. Multiply by the mass — keep the unit:

Final answer

W = 5.0×10⁹ J. Positive, because the probe climbs to a higher (less negative) potential.

IB Exam Questions on Gravitational potential energy and potential (HL)

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Define

Give the precise meaning of key terms related to Gravitational potential energy and potential (HL).

AO1
Describe

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AO2
Explain

Give reasons WHY — cause and effect within Gravitational potential energy and potential (HL).

AO3
Evaluate

Weigh strengths AND limitations of approaches in Gravitational potential energy and potential (HL).

AO3
Discuss

Present arguments FOR and AGAINST with a balanced conclusion.

AO3

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Related Physics HL Topics

Continue learning with these related topics from the same unit:

4.1.1Newton's law of gravitation and field strength
4.1.2Kepler's laws and orbital motion
4.1.3Circular orbits and satellites
4.1.4Gravitational potential energy and escape speed
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