1 00:00:00,499 --> 00:00:03,170 This week, we will examine some more advanced topics 2 00:00:03,170 --> 00:00:05,970 in the application of Newton's laws of motion. 3 00:00:05,970 --> 00:00:09,700 First, we will look at more examples of constrained motion, 4 00:00:09,700 --> 00:00:11,280 where the motion is forced to obey 5 00:00:11,280 --> 00:00:13,520 some particular condition in addition 6 00:00:13,520 --> 00:00:15,370 to Newton's laws of motion. 7 00:00:15,370 --> 00:00:18,980 These conditions usually specify some particular relationship 8 00:00:18,980 --> 00:00:22,380 between coordinates of objects and the system we are studying. 9 00:00:22,380 --> 00:00:24,960 Specifically, we will re-examine the case 10 00:00:24,960 --> 00:00:27,700 of objects suspended with pulleys and ropes, 11 00:00:27,700 --> 00:00:29,480 but with more complex systems than we 12 00:00:29,480 --> 00:00:31,480 have discussed previously. 13 00:00:31,480 --> 00:00:33,620 The fact that the ropes have fixed length 14 00:00:33,620 --> 00:00:35,240 will provide a constraint condition 15 00:00:35,240 --> 00:00:38,890 relating the coordinates of our various masses. 16 00:00:38,890 --> 00:00:42,140 Second, we will examine the case of forces 17 00:00:42,140 --> 00:00:46,280 acting on a continuous, extended mass distribution as opposed 18 00:00:46,280 --> 00:00:48,780 to acting on discrete point masses. 19 00:00:48,780 --> 00:00:52,240 This will allow us to introduce a powerful differential 20 00:00:52,240 --> 00:00:56,500 analysis technique from calculus where we model continuous mass 21 00:00:56,500 --> 00:01:00,480 distributions as made up of lots of small, discrete mass 22 00:01:00,480 --> 00:01:03,240 elements and then examine the limiting case 23 00:01:03,240 --> 00:01:05,620 of infinitesimally small elements 24 00:01:05,620 --> 00:01:07,835 to obtain the continuous behavior. 25 00:01:07,835 --> 00:01:09,210 This is a technique that you will 26 00:01:09,210 --> 00:01:12,390 see applied over and over again in physics and engineering. 27 00:01:12,390 --> 00:01:16,700 And in fact, we will return to it again later in this course. 28 00:01:16,700 --> 00:01:19,890 Our specific example will be to study how tension 29 00:01:19,890 --> 00:01:22,440 varies in a long, massive rope. 30 00:01:22,440 --> 00:01:24,140 This is in contrast to the light, 31 00:01:24,140 --> 00:01:28,320 effectively massless ropes that we discussed previously. 32 00:01:28,320 --> 00:01:32,250 Finally, we will discuss velocity-dependent forces-- 33 00:01:32,250 --> 00:01:35,759 that is, forces whose strength depends on the velocity 34 00:01:35,759 --> 00:01:39,890 or some function of the velocity of the mass being acted on. 35 00:01:39,890 --> 00:01:43,300 The most common example of this is resistive forces or drag 36 00:01:43,300 --> 00:01:46,570 forces, which are caused by motion of a solid object 37 00:01:46,570 --> 00:01:49,390 through a fluid, like air or water. 38 00:01:49,390 --> 00:01:51,770 That is the example we will discuss this week. 39 00:01:51,770 --> 00:01:53,820 Another example you may be aware of 40 00:01:53,820 --> 00:01:56,880 is the magnetic force that acts on a charged particle, which 41 00:01:56,880 --> 00:02:00,390 depends upon the velocity of the charged particle. 42 00:02:00,390 --> 00:02:02,860 In all three of these cases, we will simply 43 00:02:02,860 --> 00:02:06,470 be applying Newton's three laws of motion, 44 00:02:06,470 --> 00:02:09,240 but the situations will require a more sophisticated treatment 45 00:02:09,240 --> 00:02:11,283 to what has come before.