00:01
Okay, so this problem is about a gravitational force as a function of m and r, where m is mass and r is the distance from the center.
00:09
We're talking about the earth, and here's a formula for the function of gravitational force on earth, where r is, where big r is the radius of the earth.
00:23
G is a gravitational constant, which is 32 p .3 p.
00:28
Per second squared.
00:30
M and r values are the mass and radius of a body.
00:40
So this problem has two parts, a and b.
00:43
Part a wants you to find the partial derivatives with respect to m and with respect to r.
00:49
So if we took the partial derivative with respect to m, if we do the partial derivative with respect to m, this is essentially just taken the derivative of m, which is one, and everything else is constant.
01:01
So our equation becomes g times big r squared over small r squared.
01:09
All right, so this is formula.
01:12
Now they also want us to interpret what this is, what means.
01:16
So we're going to go ahead and type it in this text box.
01:20
And this is the rate of change, rate of change, of in the force, in the force per unit, the force per unit, the force per unit change in mass while keeping the distance from the center.
01:57
All right, so this is our interpretation for the partial derivative with respect to m.
02:03
Now they also want us to take the partial derivative with respect to r.
02:07
If we do that, well, there is an r squared in the denominator, so using the power rule, we'd have to bring down a negative 2.
02:15
So in the numerator, we would have negative 2mg, big r squared, divided by r cubed, since we have to subtract the exponent by 1.
02:28
Because of power rule, now to interpret this, we're going to say this is the rate of change in the force.
02:41
Per unit, per unit change in distance while keeping the mass of the body constant.
02:59
So this is our interpretation for the partial derivative with respect to r...