1 00:00:03,760 --> 00:00:08,400 Let's try to find the center of mass of a uniform object 2 00:00:08,400 --> 00:00:10,790 like a uniform rod. 3 00:00:10,790 --> 00:00:13,560 And let's assume this rod is length L, 4 00:00:13,560 --> 00:00:17,730 and we want to find the center of mass. 5 00:00:17,730 --> 00:00:21,130 Now, before I begin this calculation, 6 00:00:21,130 --> 00:00:23,020 you can probably already guess that it's 7 00:00:23,020 --> 00:00:25,990 going to be exactly in the middle, and we'll verify that, 8 00:00:25,990 --> 00:00:30,390 but let's first define what we mean by our center of mass 9 00:00:30,390 --> 00:00:34,140 for discrete particles. 10 00:00:34,140 --> 00:00:37,190 Recall that this was a sum over all 11 00:00:37,190 --> 00:00:38,930 the particles in the system. 12 00:00:38,930 --> 00:00:41,560 So we'll take a label J goes from 1 to N, 13 00:00:41,560 --> 00:00:45,980 and it was the mass of that jth particle times the position 14 00:00:45,980 --> 00:00:49,660 vector that jth particle with respect to some origin, 15 00:00:49,660 --> 00:00:51,680 and we're dividing that by j equals 16 00:00:51,680 --> 00:00:58,050 from 1 to N of the total mass in the system. 17 00:00:58,050 --> 00:00:59,920 Now, how do we translate this equation 18 00:00:59,920 --> 00:01:01,400 for a continuous system? 19 00:01:01,400 --> 00:01:04,870 And let me just again show that we had chosen an origin. 20 00:01:04,870 --> 00:01:11,860 Here was our jth particle of mass mj and rj. 21 00:01:11,860 --> 00:01:13,610 So what we want to do is draw the analogy, 22 00:01:13,610 --> 00:01:18,600 and here's how it works-- that for each discrete particle, 23 00:01:18,600 --> 00:01:23,910 we're going to look at that as some mass element delta mj. 24 00:01:23,910 --> 00:01:29,100 Our vector rj will go to a vector for this mass element. 25 00:01:29,100 --> 00:01:31,580 I'll just write it delta m. 26 00:01:31,580 --> 00:01:35,979 And our sum from j goes from 1 to N 27 00:01:35,979 --> 00:01:41,120 is actually going to go to an integral over the body. 28 00:01:41,120 --> 00:01:43,670 So let's see how that looks. 29 00:01:43,670 --> 00:01:47,530 So first, we'll do it with the total mass, 30 00:01:47,530 --> 00:01:58,660 m-- here we're summing over j-- from 1 to N of mj. 31 00:01:58,660 --> 00:02:02,330 That goes to the integral over the body. 32 00:02:02,330 --> 00:02:06,570 Now, the delta m, when we take limits, 33 00:02:06,570 --> 00:02:10,805 because that's when an integral goes, we'll write that as dm. 34 00:02:10,805 --> 00:02:13,930 So that becomes a limit over the body. 35 00:02:13,930 --> 00:02:16,960 And likewise, our sum j goes from 1 36 00:02:16,960 --> 00:02:25,765 to N of mj rj goes to an integral over the body of dm 37 00:02:25,765 --> 00:02:28,360 vector r going to that element. 38 00:02:28,360 --> 00:02:31,110 So we can say in the limit that this becomes 39 00:02:31,110 --> 00:02:34,770 r going to that element. 40 00:02:34,770 --> 00:02:38,820 Now, that means that our continuous expression 41 00:02:38,820 --> 00:02:40,880 for the continuous object is an integral 42 00:02:40,880 --> 00:02:46,460 over the body of dm r to that element dm divided 43 00:02:46,460 --> 00:02:50,402 by an integral over the body of dm.