OCR · A-Level · Physics
Course version: H556 · Version from Sept 2015
(b) gravitational potential V g r GM =- at a distance r from a point mass…
Full specification wording
Gravitational potential and energy: (b) gravitational potential V g r GM =- at a distance r from a point mass M ; changes in gravitational potential
Gravitational potential at a point is the work done per unit mass in bringing a small test mass from infinity to that point, giving V = −GM/r for a point mass M at distance r.
Checked against the OCR H556 specification (opens in a new tab) on .
- Point 2 of 5
Study notes
From the checked teaching notes for this specification point.
The idea
Gravitational potential at a point is the work done per unit mass in bringing a small test mass from infinity to that point, giving V = −GM/r for a point mass M at distance r. The negative sign shows that potential is zero at infinity and decreases as you approach the mass, so a test mass falls spontaneously towards M. For a spherical mass of uniform density, the same expression applies outside the sphere, with r measured from the centre. A change in potential ΔV = V_final − V_initial equals the work done per unit mass moving between two points without change in kinetic energy.
For example: Moving from r = 2R to r = R near a planet changes V from −GM/2R to −GM/R, a change of −GM/2R, meaning potential decreases and gravitational potential energy is released.
What earns the marks
- States V = −GM/r for a point mass M at distance r, with r measured from the centre of the mass.
- Explains that gravitational potential is defined as work done per unit mass in bringing a test mass from infinity to the point.
- Interprets the negative sign: V is zero at infinity and becomes more negative closer to M.
- Calculates a change in potential as ΔV = V_final − V_initial, e.g. −GM/R − (−GM/2R) = −GM/2R.
- Applies the expression outside a spherical mass, treating it as a point mass at its centre.
Common mistakes and how to put them right
Omitting the negative sign and writing V = GM/r.
Put it right: Potential is negative because work is done by the field as the test mass moves in from infinity.
Measuring r from the surface rather than the centre of the spherical mass.
Put it right: r is the distance from the centre when the point lies outside the sphere.
Treating a change in potential as a simple subtraction of magnitudes.
Put it right: Subtract signed values, V_final − V_initial, so the sign of ΔV is meaningful.
Exam tips
- Write the defining equation with its negative sign before substituting numbers, so the sign is not lost in rearrangement.
- When asked for a change in potential, show both potential values with their signs and subtract them explicitly.
- Check that r is larger than the radius of any spherical mass before using the point-mass expression.
Try the lesson
The start of the Gravitational potential and energy: (b) gravitational potential V g r GM =- at a distance r from a point mass M ; changes in gravitational potential lesson, made from checked teaching notes for this specification point.
Listen
Gravitational potential at a point is the work done per unit mass in bringing a small test mass from infinity to that point, giving V = −GM/r for a point mass M at distance r. The negative sign shows that potential is zero at infinity and decreases as you approach the mass, so a test mass falls spontaneously towards M. For a spherical mass of uniform density, the same expression applies outside the sphere, with r measured from the centre. A change in potential ΔV = V_final − V_initial equals the work done per unit mass moving between two points without change in kinetic energy. For example, moving from r = 2R to r = R near a planet changes V from −GM/2R to −GM/R, a change of −GM/2R, meaning potential decreases and gravitational potential energy is released. A strong answer earns marks for these points. States V = −GM/r for a point mass M at distance r, with r measured from the centre of the mass. Explains that gravitational potential is defined as work done per unit mass in bringing a test mass from infinity to the point. Interprets the negative sign: V is zero at infinity and becomes more negative closer to M. Calculates a change in potential as ΔV = V_final − V_initial, e.g. −GM/R − (−GM/2R) = −GM/2R. A common slip: Omitting the negative sign and writing V = GM/r. Instead, potential is negative because work is done by the field as the test mass moves in from infinity. Exam tip: Write the defining equation with its negative sign before substituting numbers, so the sign is not lost in rearrangement.
There is more to this lesson
The full lesson goes on to check your understanding and help you earn the marks. Create a free account to carry on, with your progress saved.
A week of Premium from your first lesson · Then the free plan continues · No card, no charge
Test your understanding of Gravitational potential and energy: (b) gravitational potential V g r GM =- at a distance r from a point mass M ; changes in gravitational potential
Active recall beats re-reading. Take an instant quiz now to test what you’ve learned and lock it into long-term memory.
A week of Premium from your first lesson · Then the free plan continues · No card, no charge