1 00:00:03,660 --> 00:00:06,660 Let's determine the moment of inertia of a big wheel. 2 00:00:09,330 --> 00:00:14,040 Here we have a big wheel and on the side it's attached here 3 00:00:14,040 --> 00:00:15,270 at the center . 4 00:00:15,270 --> 00:00:20,160 And there's a string going around here, and on that string 5 00:00:20,160 --> 00:00:24,030 is a little mass hanging. 6 00:00:24,030 --> 00:00:29,370 And our disk here has a radius R. 7 00:00:29,370 --> 00:00:35,550 And we now want to in a little experiment 8 00:00:35,550 --> 00:00:37,580 what the moment of inertia is of this disk. 9 00:00:37,580 --> 00:00:39,090 And what we have to do is we have 10 00:00:39,090 --> 00:00:45,240 to drop this mass to the ground, and we 11 00:00:45,240 --> 00:00:48,400 need to measure what height is here, 12 00:00:48,400 --> 00:00:51,220 and we need to measure how long it takes to drop. 13 00:00:51,220 --> 00:00:52,840 So we need to measure t. 14 00:00:56,200 --> 00:00:58,520 So how are we going to go about that? 15 00:00:58,520 --> 00:01:01,230 Well the moment of inertia, that probably 16 00:01:01,230 --> 00:01:03,870 has something to do with the torque of this wheel. 17 00:01:03,870 --> 00:01:07,830 So we have to start doing a torque analysis. 18 00:01:07,830 --> 00:01:13,660 So torque about the center of mass equals moment of inertia 19 00:01:13,660 --> 00:01:18,820 about the center of mass times the angular acceleration. 20 00:01:18,820 --> 00:01:22,350 And we need to recall that the torque is 21 00:01:22,350 --> 00:01:26,610 the product of the radius times the perpendicular force, 22 00:01:26,610 --> 00:01:29,760 so we're going to have R here, and then 23 00:01:29,760 --> 00:01:32,789 the force that's acting on this wheel 24 00:01:32,789 --> 00:01:37,320 here is actually this tension force here. 25 00:01:37,320 --> 00:01:41,670 So we are going to have our RT here. 26 00:01:41,670 --> 00:01:47,289 And now we need to look at how things actually moving 27 00:01:47,289 --> 00:01:49,509 with respect to coordinate system. 28 00:01:49,509 --> 00:01:53,270 So if I let this mass drop, to the disk 29 00:01:53,270 --> 00:01:55,890 it's going to spin clockwise. 30 00:01:55,890 --> 00:02:01,620 So we're going to have theta hat going this way. 31 00:02:01,620 --> 00:02:04,230 And if theta hat is going clockwise, 32 00:02:04,230 --> 00:02:09,690 my k hat vector is going to go into the board. 33 00:02:09,690 --> 00:02:12,570 And if k hat is going to go there, 34 00:02:12,570 --> 00:02:16,820 and it's rotating clockwise, the angular acceleration 35 00:02:16,820 --> 00:02:22,600 is going to go in the k hat direction. 36 00:02:22,600 --> 00:02:24,650 And if that is the case, then the torque 37 00:02:24,650 --> 00:02:26,530 is going to follow suit. 38 00:02:26,530 --> 00:02:31,410 So torque also goes into the board. 39 00:02:31,410 --> 00:02:33,150 And so that means here we're going 40 00:02:33,150 --> 00:02:35,410 to deal with k hat direction. 41 00:02:35,410 --> 00:02:38,690 And we're going to have Icm and then 42 00:02:38,690 --> 00:02:42,420 alpha Z in the k hat direction. 43 00:02:42,420 --> 00:02:51,390 OK, so we can solve this I RT over alpha Z. OK, 44 00:02:51,390 --> 00:02:56,760 well that's pretty good, but we have two unknowns-- the T 45 00:02:56,760 --> 00:03:01,140 and the alpha Z. And we can use some other concepts to actually 46 00:03:01,140 --> 00:03:03,920 get information on those. 47 00:03:03,920 --> 00:03:08,700 The T, as you can guess already, plays a role here 48 00:03:08,700 --> 00:03:13,440 in this massless string, so we can do a quick free body 49 00:03:13,440 --> 00:03:22,530 diagram, an F equals ma analysis to get to that tension force. 50 00:03:22,530 --> 00:03:28,380 So we have a little mass, m, here gravity is acting on it. 51 00:03:28,380 --> 00:03:30,360 And we have this tension force here. 52 00:03:30,360 --> 00:03:34,140 And we're going to put j hat down. 53 00:03:34,140 --> 00:03:40,560 So we're going to get mg minus t, equals ma. 54 00:03:40,560 --> 00:03:44,079 It's only going to go in y direction, 55 00:03:44,079 --> 00:03:46,600 so we can just leave it here. 56 00:03:46,600 --> 00:03:48,960 And we can solve this for t. 57 00:03:48,960 --> 00:03:57,020 And then we have mg minus a. 58 00:03:57,020 --> 00:03:59,190 OK, good, so we have that. 59 00:03:59,190 --> 00:04:02,190 Now about the angular acceleration. 60 00:04:02,190 --> 00:04:06,900 And whenever there was a string going around a disk then, 61 00:04:06,900 --> 00:04:12,210 we of course, have a constrained condition, 62 00:04:12,210 --> 00:04:18,660 because the linear acceleration of this little mass going down 63 00:04:18,660 --> 00:04:25,050 is related to the radius of the disk, times the angular 64 00:04:25,050 --> 00:04:26,010 acceleration. 65 00:04:26,010 --> 00:04:28,740 So we can solve this for alpha. 66 00:04:28,740 --> 00:04:36,700 And then we have a over R. So let's put that in here. 67 00:04:36,700 --> 00:04:44,250 R, and then we have mg minus a over a, 68 00:04:44,250 --> 00:04:46,540 and then we get another R here. 69 00:04:46,540 --> 00:04:53,070 And we can write that a little bit more compact, mR squared g 70 00:04:53,070 --> 00:04:56,380 over a minus 1. 71 00:04:56,380 --> 00:05:04,140 Good, so now we have one last hurdle, namely that a here. 72 00:05:04,140 --> 00:05:07,290 That a we can't measure. 73 00:05:07,290 --> 00:05:11,250 I said in the beginning, we want to make an experiment. 74 00:05:11,250 --> 00:05:15,540 Actually we need experiment, because we can't otherwise 75 00:05:15,540 --> 00:05:17,610 get to this a, so what we need is 76 00:05:17,610 --> 00:05:23,640 a relation that connects what we can measure, which is the time. 77 00:05:23,640 --> 00:05:29,490 It falls down the height here to the acceleration of this block. 78 00:05:29,490 --> 00:05:35,370 And of course, that comes from one dimensional kinematics. 79 00:05:35,370 --> 00:05:48,030 And we know that h equals 1/2 at squared, so we can solve for a. 80 00:05:48,030 --> 00:05:53,320 2h over t squared. 81 00:05:53,320 --> 00:05:56,560 And now we can stick that in here. 82 00:05:56,560 --> 00:06:08,660 And we have mR squared, gt squared over 2h minus 1. 83 00:06:08,660 --> 00:06:11,530 And let's just write this here again. 84 00:06:11,530 --> 00:06:15,220 And that is our final solution. 85 00:06:15,220 --> 00:06:19,380 So now we have only measurable quantities here. 86 00:06:19,380 --> 00:06:21,390 The t we can measure. 87 00:06:21,390 --> 00:06:24,410 We just need a stopwatch. 88 00:06:24,410 --> 00:06:28,500 And the h we can measure, as well. 89 00:06:28,500 --> 00:06:32,640 And this actually already resembles, 90 00:06:32,640 --> 00:06:37,590 if you know the theoretical, this already 91 00:06:37,590 --> 00:06:40,830 resembles the theoretical solution, 92 00:06:40,830 --> 00:06:44,540 which of course is for a disk. 93 00:06:44,540 --> 00:06:52,110 1/2 mR squared, so that's what one expects for a disk. 94 00:06:52,110 --> 00:06:55,230 And you see that we're very close, so this term here 95 00:06:55,230 --> 00:06:58,500 is probably something like 1.5, or should better 96 00:06:58,500 --> 00:07:01,570 come out to be 1.5, because if we subtract 1, 97 00:07:01,570 --> 00:07:03,540 we get to that 1/2 here. 98 00:07:03,540 --> 00:07:06,720 And you can use it to in return-- in return, 99 00:07:06,720 --> 00:07:09,390 you can also use it to predict the time 100 00:07:09,390 --> 00:07:13,265 it takes to fall down if you know what the height is 101 00:07:13,265 --> 00:07:15,363 or vice versa.