00:01
We start with three spherical masses arranged in an equilateral triangle orientation, and here i've drawn a diagram of this on the left that i've indicated as position 1.
00:12
We let these three balls move towards each other due to their gravitational forces, and they'll end up in position 2, where they form a smaller equilateral triangle where all of the three balls touch.
00:26
We want to find the speed at which all these three balls collide.
00:33
So here we can use the conservation of energy equation to find the ending speed given the initial gravitational potential energy and the initial kinetic energy.
00:47
So let's go ahead and write out the conservation of energy which tells us e1 is equal to e2.
00:53
E1 is composed of kinetic energy and gravitational potential energy.
00:59
Both of these will be for position one.
01:09
And on the right, we have the same two terms for position two.
01:15
So for kinetic energy, we have zero kinetic energy in the first position because we let them go from rest.
01:23
And the gravitational potential energy will actually be composed of three components...