00:01
We're told of a satellite that is rotating about the earth, and we have a question in three parts.
00:06
The first is to derive an equation for the speed of that satellite as a function of g, the gravitational constant, h, the height of the satellite above the earth, m, the mass of the satellite, m sub e, the mass of the earth, and r sub e, the radius of the earth.
00:25
And to do that, we begin with the force equation.
00:29
F equals g times m times the mass of the earth.
00:35
And you might know this is r squared.
00:38
With you look at the top right of the screen, we know that the r in this problem, the radius is actually the sum of the radius of the earth and the height of the satellite.
00:49
That's squared.
00:51
And we also know by newton's second law, that's equal times the mass.
00:55
That's equal to the mass times the acceleration...