00:01
Hello.
00:03
So here the potential energy u is going to be equal to gmm over r.
00:11
Let's say m1m2.
00:17
So let's look at this substitution here.
00:23
So of course potential energy is negative.
00:27
So this is going to be so our universal gravitational constant is 6 .674 times 10 to the negative.
00:43
The m1 is mass of the earth.
00:46
This is 5 .98 times 10 to the 24.
00:56
M2 is the mass of the satellite.
00:59
It's 1 .2 times 10 to the third.
01:06
So for the r, r is a distance that we have to be very careful with.
01:12
So r is going to be the height or the radius of the earth plus the height above the okay, so the height here.
01:40
So that's just going to be, so the radius of the earth is one point, oops, one second.
01:53
So the satellite is two 30 kilometers above the air.
01:58
So we have h so we just need to find r.
02:00
So yeah, r is 6 .38 times 10 to the 6 plus 2 .30 kilometers is that is times 10 to the third.
02:18
We need to cube all of this.
02:20
Excuse me.
02:22
Oh, this is just r.
02:23
So we just have this...