Gravitational Field Strength in a Radial Field (AQA A Level Physics): Revision Note

Gravitational Field Strength in a Radial Field

• The gravitational field strength at a point describes how strong or weak a gravitational field is at that point

• The equation for gravitational field strength due to a point mass is:

• Where:

  • g = gravitational field strength (N kg^-1)

  • G = Newton’s gravitational constant

  • M = mass of the body producing the gravitational field (kg)

  • r = distance between point source (mass, m) and position in field (m)

• Gravitational field strength, g, is a vector quantity

• The direction of g is always towards the centre of the body creating the gravitational field

  • This is the same direction as the gravitational field lines

  • On the Earth’s surface, g has a constant value of 9.81 N kg^-1

• However, outside the Earth’s surface, g is not constant

  • g decreases as r increases by a factor of 1/r²

  • This is an inverse square law relationship with distance

• When g is plotted against the distance from the centre of a planet, r has two parts:

  • When r < R, the radius of the planet, g is directly proportional to r

  • When r > R, g is inversely proportional to r² (this is an ‘L’ shaped curve and shows that g decreases rapidly with increasing distance r)

Graph showing how gravitational field strength varies at greater distance from the Earth’s surface

• Sometimes, g is referred to as the ‘acceleration due to gravity’ with units of m s^-2

  • Any object that falls freely in a uniform gravitational field on Earth has an acceleration of 9.81 m s^-2