How do you prove Kepler's Third Law?

For starters, what exactly is Kepler's Third Law?

Kepler's Third Law states that the square of the time period of orbit is directly proportional to the cuber of the semi-major axis of that respective orbit. (the semi-major axis for a circular orbit is of course the radius) Mathematically this can be represented as: T2 / r3 = k where k is a constant. The value k is related to physical constants such that k = 4pi2/GM where G is the gravitational constant and M the mass of the object at the centre of the orbit (NOT the object doing the orbiting!)

 

How did Kepler arrive at this result? Unfortunately, through experiment, which is not particularly convenient for us, but, thankfully we have knowledge Kepler had not! 

 

The result can be obtained surprisingly easily, assuming we have the necessary tools. 

We will need the following four equations:

Circular Motion: a = v2/r; v = wr = 2pi/T

Gravitational attraction: F = GMm/r2 

Newton's Second Law: F = ma

 

Substituting circular motion and gravitational attraction into the above formula yields:

mv2/r = Gmm/r2 

Cancelling the m's multiplying by r and by GM gives:

v2/GM = 1/r

This is very close to the result we want, one more substitution should give us the desired equation. Notice that v = wr = 2rpi/T from circular motion equations.

And so we have:

4pi2/GMT2 = 1/r3

Multiplying by T2:

T2/r3 = 4pi2/GM as required!

DB

Related Physics A Level answers

All answers ▸

How does a capacitor work and how do I treat it in a circuit?


A mass, m, is resting on a slope being slowly tilted upwards from horizontal. The static friction co-efficient is 0.3 and the dynamic friction co-efficient is 0.2: at what angle will the mass begin to slip?


Name the four fundamental forces.


A small ball is projected with speed 15 m/s at an angle of 60 degrees above the horizontal. Find the distance from the point of projection of the ball at the instant when it is travelling horizontally.