Newton's Law of Gravity

What you should know

The Earth, other planets and stars produce gravitational fields, which exert a force on other massive objects

A gravitational field exerts a 'non-contact' force, which acts over very long distances

Gravitational field strength, g, is defined as the force that acts on a mass of 1kg. On Earth, g = 9.81 Nkg-1

A planet's or stars gravitational field strength, at its surface, depends on its mass and radius

The gravitational potential energy, Ep (in J), gained by a mass, m (in kg), lifted through a height, h (in m), in a uniform gravitational field, g (in NKg), is given by E = mgh

The kinetic energy of an object is given by 1/2 m v2

Summary

Newton's law of gravitation states that the gravitational force of attraction between two point masses, m1 and m2 (measured in kg), separated by a distance, r (in metres), is given by:

Newton's law of gravity

This constant can only be accurately measured by careful laboratory experiment

Although Newton's law only applies to point masses, it can also be used to calculate the force of attraction between two large spherical objects (like planets and stars) because a sphere behaves as if all the mass were concentrated at the centre

Newton's law of gravity

So Newton's law can be correctly used to calculate the force of attraction in each of the cases above:

  • In (a), the force between two point masses
  • In (b), the force between a planet and a small mass
  • In (c), the force between two planets or stars

Newton's law cannot be used to calculate the force between two irregularly shaped objects, unless a complicated summation of the forces is made

Example

Newton's law of gravity

Newton's law of gravity

The Inverse Square Law

When Newton formulated his law of gravity, he imagined that the law of gravity spreads out in the same way as light spreads out from a candle

Newton's law of gravity

This image shows his idea

When you hold a card at a distance of 1m from the candle, you see a particular intensity of light, l

When you move a distance of 2m from the candle, the same amount of light now spreads out over four cards of the same area

  • So the light intensity is now a quarter of its original value, 1/4 l

Light intensity obeys an inverse square law:

Newton's law of gravity

Here I is the intensity of light in W m-2, L is the luminosity of the light source (the amount of energy emitted per second) in W, and r is the distance away from the light source in m

The factor 4π comes into the equation because the light spreads out into a sphere, and the surface area of a sphere of radius r is 4πr2