1 00:00:00,940 --> 00:00:08,320 So up until this point, we were busy mostly with kinematics, that is things that involve the position, 2 00:00:08,320 --> 00:00:10,590 the speed and acceleration of a particle. 3 00:00:11,530 --> 00:00:14,700 But we considered this particle to be massless. 4 00:00:15,070 --> 00:00:21,030 We did not consider the forces that might work in on this particle and that is called kinematics. 5 00:00:21,610 --> 00:00:29,050 What are we going to look at going forward is kinetics and kinetics looks at the causes of motion that 6 00:00:29,050 --> 00:00:37,420 will say that the particle that undergoes position, speed and acceleration has a certain mass which 7 00:00:37,420 --> 00:00:38,610 we are going to consider. 8 00:00:39,010 --> 00:00:46,860 We are going to consider certain forces that works on this mass and that is called also dynamics. 9 00:00:47,800 --> 00:00:56,440 And an example of kinematics that we have looked at in the previous videos is the study of celestial 10 00:00:56,440 --> 00:01:02,440 bodies, how planets move around the sun, for instance, how a moon moves around the planet. 11 00:01:02,740 --> 00:01:10,450 You can describe the motion of that body using kinematics without considering the fact that the body 12 00:01:10,450 --> 00:01:11,580 has a certain mass. 13 00:01:11,800 --> 00:01:16,680 So Chromatics is just describing the position mostly as a function of time. 14 00:01:17,350 --> 00:01:23,010 When you look at kinetics, you are going to incorporate the mass in the forces. 15 00:01:23,020 --> 00:01:31,570 So that is mostly employed where you design things like airplanes and motor vehicles, trains, etc. 16 00:01:31,870 --> 00:01:38,680 So they we need to consider how different forces work in on this body and for that we will use a free 17 00:01:38,680 --> 00:01:39,900 body diagram. 18 00:01:41,770 --> 00:01:46,930 So there are three methods of solving kinetics problems that we are going to look at. 19 00:01:46,930 --> 00:01:53,740 The first one is Newton's second law, which says that F is equal to M times A, the force is equal 20 00:01:53,740 --> 00:01:58,270 to the mass of the body multiplied by its acceleration. 21 00:02:12,650 --> 00:02:21,250 And that force you will see is the sum of forces working on the body broken down into different directions, 22 00:02:21,260 --> 00:02:21,650 you'll see. 23 00:02:21,650 --> 00:02:22,950 We'll do an example of that. 24 00:02:23,090 --> 00:02:28,780 So if is equal to M times a mass multiplied by acceleration, that's Newton's second law. 25 00:02:29,300 --> 00:02:32,380 That is a starting point for solving some kinetics problems. 26 00:02:32,930 --> 00:02:37,510 Another starting point for solving some kinetic problems is the principle of work and energy. 27 00:02:38,240 --> 00:02:39,590 We will look at that as well. 28 00:02:39,920 --> 00:02:44,540 And then we will also look at the principle of impulse and momentum. 29 00:02:46,130 --> 00:02:52,190 So without further ado, let us look at Newton's second law and how we can use that to solve a kinetic 30 00:02:52,250 --> 00:02:52,700 problem.