Gravitational Potential (DP IB Physics): Revision Note
Gravitational Potential
The gravitational potential V at a point can, therefore, be defined as:
The work done per unit mass in bringing a test mass from infinity to a defined point
Gravitational potential is measured in J kg−1
It is always has a negative value because:
It is defined as having a value of zero at infinity
Since the gravitational force is attractive, work must be done on a mass to reach infinity
On the surface of a mass (such as a planet), gravitational potential has a negative value
The value becomes less negative, i.e. it increases, with distance from that mass
Work has to be done against the gravitational pull of the planet to take a unit mass away from the planet
The gravitational potential at a point depends on:
The mass of the object
The distance from the centre of mass of the object to the point
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Gravitational potential decreases as the satellite moves closer to the Earth
Calculating Gravitational Potential
The equation for gravitational potential V is defined by the mass M and distance r:
Where:
Vg = gravitational potential (J kg−1)
G = Newton’s gravitational constant
M = mass of the body producing the gravitational field (kg)
r = distance from the centre of the mass to the point mass (m)
The gravitational potential always is negative near an isolated mass, such as a planet, because:
The potential when r is at infinity (∞) is defined as zero
Work must be done to move a mass away from a planet (V 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 r 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 0 at infinity
This means when the distance r becomes very large, the gravitational force tends rapidly towards zero the further away the point is from a planet
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Gravitational potential increases and decreases depending on whether the object is travelling towards or against the field lines from infinity
Worked Example
A planet has a diameter of 7600 km and a mass of 3.5 × 1023 kg. A meteor of mass 6000 kg accelerates towards the planet from infinity.
Calculate the gravitational potential of the rock at a distance of 400 km above the planet's surface.
Answer:
The gravitational potential at a point is
Where r is the distance from the centre of the planet to the point i.e. the radius of the planet + the height above the planet's surface
And M is the mass of the larger mass, i.e. the planet (not the meteor)
Examiner Tips and Tricks
Notice the red herring in the worked example. You do not need the mass m of the meteor, as M in the equation for gravitational potential is only the mass of the object creating the gravitational field. m will come into play with gravitational potential energy.
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