00:01
So this is a question involving an object orbiting the earth, this was the skylab.
00:08
So if you have an object orbiting the earth, we can derive a formula for the speed at which it is orbiting as a function of the radius of its orbit.
00:21
So we're gonna, by saying radius, i'm assuming a circular orbit, but it turns out that the formula applies for an elliptical orbit as well, as long as you use for that distance, the radius of the orbit, use the average distance that the satellite is from the planet.
00:36
We'll proceed as follows.
00:38
The force that is causing the satellite to orbit, say the planet earth, is the force of gravity.
00:47
And we know the force of gravity is given to us by this formula.
00:52
We have gravitational constant, universal gravitational constant, times the mass of the planet, in this case, it would be the earth, times the mass of the satellite, divided by the radius of the orbit squared.
01:12
So as we derive it here, we're gonna call it the radius, because we're thinking of it being the radius of the orbit.
01:20
But as i said, you can use the same formula that we're gonna derive, just replace r with the average distance of the satellite from the center of the earth.
01:33
Okay, that's the force.
01:35
And because it's going in a circular orbit, we know that the force must equal the mass times the centripetal acceleration formula.
01:45
In other words, this formula here, this force, must equal the mass of the satellite times the speed of the satellite squared divided by the radius, because that is the acceleration.
01:58
V squared divided by r is the acceleration of something that is going at a uniform speed in a circular path...