00:01
The force due to gravity is f equals g, which is the gravitational constant, times the mass of one of the objects, in this case, m of the mass of the earth, times the mass of the other object that's being attracted by the gravitational force, divided by the distance between them squared, which is r squared.
00:31
And when i say the distance between them, i mean the distance between their centers of mass.
00:37
So, for example, if you have the earth with its center of mass here, and you're looking at some object here with center of mass, then r would be this distance here.
00:56
The acceleration due to gravity is given by newton's second law, f equals m .a, where m is the mass of m.
01:08
This object here.
01:10
So if we set the forces equal to each other, we have m .a is equal to g times m times m divided by r squared.
01:22
I can divide by little m on those sides to get that the acceleration due to gravity is equal to g times m over r squared.
01:37
We want to find the altitude above earth's surface where acceleration is equal to g over 2.
01:45
So the altitude above earth's surface is only a section of r.
01:53
It's only this part.
01:54
So this i'll call h for height.
01:59
And then we still have this section here, which is the radius of earth.
02:06
So we see that a little r is equal to 8.
02:14
Plus the radius of earth so i can plug that in to the equation so we have a equals g times m e divided by h plus r e and this is squared okay so we're trying to find the altitude h where a equals g over two so when i plug that in we have g over two is equal to big g times m e divided by h plus r .e all squared.
02:53
And we're solving for h.
02:55
So i'll multiply by h plus r e squared on both sides.
02:59
So i have g over two times h plus re squared is equal to g m .e...