00:01
In this example, i'm going to be looking at two types of collisions, an elastic and inelastic.
00:08
And we're also going to be looking at some conservation of energy and momentum rules.
00:13
All right.
00:14
So let's get started.
00:16
What we have is an experimental setup shown below.
00:22
So we have two masses on a track.
00:25
Right.
00:25
We have mass 1 equals 2 .00 kilograms.
00:32
We have mass 2 equals 4 .00 kilograms.
00:38
All right, we're going to release these masses from rest.
00:42
They're going to obtain some velocity and collide at some point.
00:47
First, we're going to look at elastic collision, and we want to find the blocks velocities before and after the collision.
00:54
We'll do the same for an inelastic collision.
00:56
All right, and we're also given the height, which is the same for each block.
01:00
H equals 5 meters, 0, 0 meters.
01:06
And obviously this track is not drawn to scale, but disregard that.
01:11
All right.
01:11
So the first thing we're asked to do is find the coordinate of the center of mass in the x direction for this system.
01:18
So we're just looking at the blocks.
01:20
We're not including the track here.
01:22
All right.
01:23
So how do we do that? we know x center of mass times mass 1, 4.
01:31
Plus mass 2 equals m1x1 plus m2 x2.
01:44
Plus m2 x2.
01:45
All right, and for this example, i have x1.
01:50
Here it is negative 5, x2 is positive 5.
01:54
I know my two masses.
01:56
So i get x and mass equals 2 kilograms times negative 5.
02:04
And i'm leaving out the units for my calculations.
02:07
Make sure you always include your units.
02:09
Plus mass 2 is 4 kilograms times positive 5.
02:14
That's all divided by 6 kilograms.
02:16
That gives me a center of mass of 1 .67 meters.
02:22
All right.
02:23
This makes sense.
02:24
Since the second object here is more massive, we'd expect the center of mass to be closer to that.
02:30
Next, we want to find the velocities of each block, each block after they're released and just before the collision.
02:36
All right.
02:38
So when they meet somewhere around here, and they're both on flat ground, they'll have constant velocity at that point.
02:45
How do we find velocity? we want to use conservation of energy.
02:48
We know that mgh equals 1�mv square.
02:54
That's just saying total mechanical energy is conserved.
03:00
All right.
03:01
You'll see the mass drops out.
03:03
Each of these blocks is going to have the same velocity of v equals root 2, g .h, where h is my 5 meter height.
03:16
G is the acceleration due to gravity...