D.1.6 (HL)—Gravitational potential energy

Syllabus
First assessment 2025
Objective
Level
HL

Model Gravitational Potential Energy

HL only

Define the reference

Gravitational potential energy is defined as the work done to assemble the masses of a system from infinite separation. Set the potential energy at infinite separation to zero. Because gravity is attractive, bringing masses together releases energy, so the gravitational potential energy of a bound system is negative.

Interpret the sign

Moving a mass farther from an attracting body increases gravitational potential energy toward zero and requires positive external work if done slowly. Moving it inward makes the potential energy more negative; the gravitational field can do positive work and transfer potential energy into kinetic energy.

Use the field model

Gravitational force is conservative, so the work between two fixed positions depends only on the endpoints, not the path. Near Earth’s surface, where gg is approximately constant, changes can be approximated by ΔEp=mgΔh\Delta E_p=mg\Delta h; for large distances use the field-based potential model rather than a constant-g approximation.

Common trap

Do not make gravitational potential energy positive simply because the mass is high above a planet. With zero at infinity, every finite point in the isolated attractive field has negative potential energy.

D.1.6 (HL) Exam Analysis

HL only

Assessment in practice

2 marks
How it is assessed

Questions explain why an isolated mass has negative potential or relate gravitational potential energy to kinetic energy in an orbit.

Command terms

Explain / Show that

What earns marks

Use infinity as the zero reference, explain the negative sign from attraction, and distinguish positive work moving outward from field work moving inward.

Watch for

Forgetting the infinity reference, or claiming that inward motion requires positive work by the external agent when the gravitational field is doing the work.

Representative question

Question 1

[Maximum number: 1]

A moon of mass M orbits a planet of mass 100 M. The radius of the planet is R and the distance between the centres of the planet and moon is 22 R.

What is the distance from the centre of the planet at which the total gravitational potential has a maximum value?

A

2 R

B

11 R

C

20 R

D

2 R and 20 R

Retrieve the HL D.1 Gravitational Fields Model

HL only

The HL gravitational-fields model is secure when you can move between energy, potential, gradients and orbital consequences.

  • Ep=−Gm1m2/r and Vg=−GM/r, zero at infinity
  • g=−ΔVg/Δr and W=mΔVg
  • Equipotentials are perpendicular to field lines
  • vesc=√(2GM/r) and vorbital=√(GM/r)
  • Atmospheric drag lowers orbital energy and radius while increasing the speed of the new lower orbit