00:01
Okay, so you're given a graph of kinetic energy versus the distance to the earth, so to the center of the earth, of an asteroid.
00:10
So at any given distance, there is a certain amount of kinetic energy in the asteroid.
00:17
And so in the first part of the problem, they want us to find the mass based on this information.
00:25
And so you can look at conservation of energy where the kinetic energy at one point plus the gravitational potential energy at one point.
00:41
It's going to be equal to the kinetic energy at another point plus the gravitational energy at that point.
00:53
And so gravitational energy is given by negative g mass of the earth times the mass of the asteroid over the distance.
01:05
So from this graph, we can get two different values of kinetic energy and the corresponding distances.
01:16
So normally kinetic energy is going to be 1 .5 mv squared, but we just have the actual value of the kinetic energy here.
01:25
So first let's choose two different points.
01:30
So we'll say r1 at 1 .85 times 10 of the 7 meters.
01:41
So we'll use that one in the corresponding kinetic energy at that point is going to be 2 .21 approximately times 10 to the 9 joules.
02:01
So for this graph you have some number, right? and so we've got 1 .85 here.
02:17
And we're saying this corresponds to about 2 .21 times, then you have to multiply by times 10 to the 9.
02:24
And the jules is the units.
02:26
Okay.
02:27
And so that's our first point.
02:30
And then the second point we'll say r2.
02:35
And you can do this at any 2.
02:36
Points, it doesn't actually matter, as long as you have the correct corresponding kinetic energies and distances.
02:44
So we'll say at 1 .75 times 10 to the 7 meters, corresponding kinetic energy at that point, this was supposed to be 75.
03:02
So at that point, just going straight up, and we get, on the actual graph, we get something like 3 .41 times 10 to the 9 joules.
03:25
So this graph i have drawn is not exactly to scale, but looking at the actual graph, that's the, about the number that you get.
03:34
Okay, and so we can plug in what we have here.
03:36
And first let's get our kinetic energies on one side and our potential energies on one side.
03:46
So just plugging in the actual equations here.
03:57
So this is g mass of earth times mass of the asteroid over r1 minus.
04:07
This goes we added this one to this side.
04:10
And then minus g m -e -m -a over r2.
04:17
Okay, so now we can plug in the actual values here...