Calculating Gravitational Potential (AQA A Level Physics): Revision Note
Exam code: 7408
Calculating gravitational potential
The equation for gravitational potential is defined by the mass and distance :
Where:
= gravitational potential (J kg-1)
= Newton’s gravitational constant
M = mass of the body producing the gravitational field (kg)
= distance from the centre of the mass to the point mass (m)
The gravitational potential is always negative near an isolated mass, such as a planet, because:
the potential when is at infinity (∞) is defined as zero
work must be done to move a mass away from a planet ( becomes less negative)
It is also a scalar quantity, unlike the gravitational field strength which is a vector quantity
Gravitational forces are always attractive, this means as decreases, positive work is done by the mass when moving from infinity to that point
When a mass is closer to a planet, its gravitational potential becomes smaller (more negative)
As a mass moves away from a planet, its gravitational potential becomes larger (less negative) until it reaches zero at infinity
This means when the distance () becomes very large, the gravitational force tends rapidly towards zero at a point further away from a planet

Worked Example
A planet has a diameter of 7600 km and a mass of 3.5 × 1023 kg. A rock of mass 528 kg accelerates towards the planet from infinity. At a distance of 400 km above the planet's surface, calculate the gravitational potential of the rock.
[3]
Answer:
Step 1: Write the gravitational potential equation
Step 2: Determine the value of r
is the distance from the centre of the planet
[1 mark]
Step 3: Substitute in values
[1 mark]
[1 mark]
Examiner Tips and Tricks
Remember to keep the negative sign in your solution for the gravitational potential at a point. However, if you’re asked for the ‘change in’ gravitational potential, no negative sign needs to be included since you are finding a difference in values and just the magnitude is normally required. Remember to also calculate r as the distance from the centre of the planet, and not just the distance above the planet's surface
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