1 0:00:02 --> 00:00:08 Today we're going to continue with playing with liquids. 2 00:00:08 --> 00:00:14 If I have an object that floats, 3 00:00:12 --> 00:00:18 a simple cylinder that floats in some liquid, 4 00:00:19 --> 00:00:25 the area is A here, the mass of the cylinder is M. 5 00:00:23 --> 00:00:29 The density of the cylinder is rho and its length is l 6 00:00:29 --> 00:00:35 and the surface area is A. 7 00:00:31 --> 00:00:37 So this is l. 8 00:00:34 --> 00:00:40 And let the liquid line be here, 9 00:00:38 --> 00:00:44 and the fluid has a density rho fluid. 10 00:00:43 --> 00:00:49 I call this level y1, this level y2. 11 00:00:49 --> 00:00:55 The separation is h, 12 00:00:51 --> 00:00:57 and right on top here, there is the atmospheric pressure P2, 13 00:00:55 --> 00:01:01 which is the same as it is here on the liquid. 14 00:00:59 --> 00:01:05 And here we have a pressure P1 in the liquid. 15 00:01:06 --> 00:01:12 For this object to float 16 00:01:11 --> 00:01:17 we need equilibrium between, on the one hand, the force Mg 17 00:01:18 --> 00:01:24 and the buoyant force. 18 00:01:22 --> 00:01:28 There is a force up here which I call F1, 19 00:01:28 --> 00:01:34 and there is a force down here which I call F2-- 20 00:01:32 --> 00:01:38 barometric pressure. 21 00:01:34 --> 00:01:40 The force is always perpendicular to the surface. 22 00:01:37 --> 00:01:43 There couldn't be any tangential component 23 00:01:39 --> 00:01:45 because then the air starts to flow, and it's static. 24 00:01:42 --> 00:01:48 And here we have F1, 25 00:01:44 --> 00:01:50 which contains the hydrostatic pressure. 26 00:01:48 --> 00:01:54 So P1 minus P2-- as we learned last time from Pascal-- 27 00:01:54 --> 00:02:00 equals rho of the fluid 28 00:02:00 --> 00:02:06 g to the minus y2 minus y1, which is h. 29 00:02:05 --> 00:02:11 So that's the difference between the pressure P1 and P2. 30 00:02:09 --> 00:02:15 For this to be in equilibrium, 31 00:02:12 --> 00:02:18 F1 minus F2 minus Mg has to be zero, 32 00:02:21 --> 00:02:27 and this we call the buoyant force. 33 00:02:26 --> 00:02:32 And "buoyant" is spelt in a very strange way: b-u-o-y-a-n-t. 34 00:02:33 --> 00:02:39 I always have to think about that. 35 00:02:34 --> 00:02:40 It's the buoyant force. 36 00:02:36 --> 00:02:42 F1 equals the area times P1 and F2 is the area times P2, 37 00:02:47 --> 00:02:53 so it is the area times P1 minus P2, 38 00:02:52 --> 00:02:58 and that is rho fluids times g times h. 39 00:02:58 --> 00:03:04 And when you look at this, 40 00:03:00 --> 00:03:06 this is exactly the weight of the displaced fluid. 41 00:03:05 --> 00:03:11 The area times h 42 00:03:07 --> 00:03:13 is the volume of the fluid which is displaced by this cylinder, 43 00:03:13 --> 00:03:19 and you multiply it by its density, that gives it mass. 44 00:03:17 --> 00:03:23 Multiply it by g, that gives it weight. 45 00:03:20 --> 00:03:26 So this is the weight of the displaced fluids. 46 00:03:25 --> 00:03:31 47 00:03:29 --> 00:03:35 And this is a very special case of a general principle 48 00:03:34 --> 00:03:40 which is called Archimedes' principle. 49 00:03:37 --> 00:03:43 Archimedes' principle is as follows: 50 00:03:39 --> 00:03:45 The buoyant force on an immersed body has the same magnitude 51 00:03:44 --> 00:03:50 as the weight of the fluid which is displaced by the body. 52 00:03:49 --> 00:03:55 According to legend 53 00:03:51 --> 00:03:57 Archimedes thought about this while he was taking a bath, 54 00:03:55 --> 00:04:01 and I have a picture of that here-- 55 00:03:58 --> 00:04:04 I don't know from when that dates-- 56 00:04:00 --> 00:04:06 but you see him there in his bath, 57 00:04:03 --> 00:04:09 but what you also see are there are two crowns. 58 00:04:06 --> 00:04:12 And there is a reason why those crowns are there. 59 00:04:09 --> 00:04:15 Archimedes lived in the third century B.C. 60 00:04:12 --> 00:04:18 Archimedes had been given the task 61 00:04:15 --> 00:04:21 to determine whether a crown that was made for King Hieron II 62 00:04:20 --> 00:04:26 was pure gold. 63 00:04:25 --> 00:04:31 The problem for him was 64 00:04:26 --> 00:04:32 to determine the density of this crown-- 65 00:04:28 --> 00:04:34 which is a very irregular-shaped object-- 66 00:04:31 --> 00:04:37 without destroying it. 67 00:04:32 --> 00:04:38 And the legend has it 68 00:04:34 --> 00:04:40 that as Archimedes was taking a bath, he found the solution. 69 00:04:38 --> 00:04:44 He rushed naked through the streets of Syracuse 70 00:04:41 --> 00:04:47 and he shouted, "Eureka! Eureka! Eureka!" 71 00:04:45 --> 00:04:51 which means, "I found it! I found it!" 72 00:04:48 --> 00:04:54 What did he find? 73 00:04:49 --> 00:04:55 What did he think of? 74 00:04:51 --> 00:04:57 He had the great vision to do the following: 75 00:04:54 --> 00:05:00 You take the crown and you weigh it in a normal way. 76 00:04:58 --> 00:05:04 So the weight of the crown-- I call it W1-- 77 00:05:01 --> 00:05:07 is the volume of the crown times the density of which it is made. 78 00:05:06 --> 00:05:12 If it is gold, it should be 19.3, I believe, 79 00:05:10 --> 00:05:16 and so this is the mass of the crown 80 00:05:13 --> 00:05:19 and this is the weight of the crown. 81 00:05:16 --> 00:05:22 Now he takes the crown and he immerses it in water. 82 00:05:21 --> 00:05:27 And he has a spring balance, and he weighs it again. 83 00:05:25 --> 00:05:31 And he finds that the weight is less 84 00:05:29 --> 00:05:35 and so now we have the weight immersed in water. 85 00:05:36 --> 00:05:42 So what you get is 86 00:05:39 --> 00:05:45 the weight of the crown minus the buoyant force, 87 00:05:44 --> 00:05:50 which is the weight of the displaced fluid. 88 00:05:48 --> 00:05:54 And the weight of the displaced fluid 89 00:05:50 --> 00:05:56 is the volume of the crown-- because the crown is where... 90 00:05:54 --> 00:06:00 the water has been removed where the crown is-- 91 00:05:57 --> 00:06:03 times the density of the fluid-- 92 00:06:00 --> 00:06:06 which is water, which he knew very well-- times g. 93 00:06:04 --> 00:06:10 And so this part here is weight loss. 94 00:06:10 --> 00:06:16 That's the loss of weight. 95 00:06:11 --> 00:06:17 You can see that, you can measure that with a spring. 96 00:06:13 --> 00:06:19 It's lost weight, because of the buoyant force. 97 00:06:16 --> 00:06:22 And so now what he does, 98 00:06:17 --> 00:06:23 he takes W1 and divides that by the weight loss 99 00:06:24 --> 00:06:30 and that gives you this term divided by this term, 100 00:06:27 --> 00:06:33 which immediately gives you 101 00:06:28 --> 00:06:34 rho of the crown divided by rho of the water. 102 00:06:31 --> 00:06:37 And he knows rho of the water, so he can find rho of the crown. 103 00:06:35 --> 00:06:41 It's an amazing idea; he was a genius. 104 00:06:39 --> 00:06:45 I don't know how the story ended, 105 00:06:41 --> 00:06:47 whether it was gold or not. 106 00:06:43 --> 00:06:49 It probably was, because chances are that if it hadn't been gold 107 00:06:49 --> 00:06:55 that the king would have killed him-- for no good reason, 108 00:06:52 --> 00:06:58 but that's the way these things worked in those days. 109 00:06:55 --> 00:07:01 This method is also used 110 00:06:56 --> 00:07:02 to measure the percentage of fat in persons' bodies, 111 00:07:00 --> 00:07:06 so they immerse them in water and then they weigh them 112 00:07:02 --> 00:07:08 and they compare that with their regular weight. 113 00:07:06 --> 00:07:12 114 00:07:08 --> 00:07:14 Let's look at an iceberg. 115 00:07:12 --> 00:07:18 116 00:07:14 --> 00:07:20 Here is an iceberg. 117 00:07:18 --> 00:07:24 Here is the water-- it's floating in water. 118 00:07:20 --> 00:07:26 It has mass M, it has a total volume V total, 119 00:07:24 --> 00:07:30 and the density of the ice is rho ice, 120 00:07:27 --> 00:07:33 which is 0.92 in grams per cubic centimeter. 121 00:07:34 --> 00:07:40 It's less than water. 122 00:07:36 --> 00:07:42 123 00:07:40 --> 00:07:46 This is floating, and so there's equilibrium 124 00:07:44 --> 00:07:50 between Mg and the buoyant force. 125 00:07:49 --> 00:07:55 So Mg must be equal to the buoyant force. 126 00:07:52 --> 00:07:58 Now, Mg is the total volume times rho ice times g, 127 00:08:01 --> 00:08:07 just like the crown. 128 00:08:03 --> 00:08:09 The buoyant force is the volume underwater, which is this part, 129 00:08:11 --> 00:08:17 times the density of water, rho water, times g. 130 00:08:19 --> 00:08:25 You lose your g, and so you find 131 00:08:23 --> 00:08:29 that the volume underwater divided by the total volume 132 00:08:28 --> 00:08:34 equals rho ice divided by rho of water, which is 0.92. 133 00:08:34 --> 00:08:40 That means 92% of the iceberg is underwater, 134 00:08:39 --> 00:08:45 and this explains something about the tragedy 135 00:08:43 --> 00:08:49 on April 15, 1912, when theTitanic hit an iceberg. 136 00:08:48 --> 00:08:54 When you encounter an iceberg, 137 00:08:49 --> 00:08:55 you literally only see the tip of the iceberg. 138 00:08:51 --> 00:08:57 That's where the expression comes from. 139 00:08:53 --> 00:08:59 92% is underwater. 140 00:08:56 --> 00:09:02 141 00:09:00 --> 00:09:06 I want to return now to my cylinder, 142 00:09:03 --> 00:09:09 and I want to ask myself the question, 143 00:09:06 --> 00:09:12 when does that cylinder float? 144 00:09:09 --> 00:09:15 What is the condition for floating? 145 00:09:12 --> 00:09:18 Well, clearly, for that cylinder to float 146 00:09:15 --> 00:09:21 the buoyant force must be Mg, and the buoyant force 147 00:09:23 --> 00:09:29 is the area times h-- that's the volume underwater-- 148 00:09:31 --> 00:09:37 multiplied by the density of the fluid times g 149 00:09:36 --> 00:09:42 must be the total volume of the cylinder, 150 00:09:40 --> 00:09:46 which is the area times l, 151 00:09:42 --> 00:09:48 because that was the length of the cylinder, 152 00:09:45 --> 00:09:51 times the density of the object itself times g. 153 00:09:49 --> 00:09:55 I lose my A, I lose my g, 154 00:09:54 --> 00:10:00 but I know that h must be less than l; 155 00:09:58 --> 00:10:04 otherwise it wouldn't be floating, right? 156 00:10:00 --> 00:10:06 The part below the water has to be smaller 157 00:10:02 --> 00:10:08 than the length of the cylinder. 158 00:10:05 --> 00:10:11 And if h is less than l, 159 00:10:07 --> 00:10:13 that means that the density of the fluid 160 00:10:11 --> 00:10:17 must be larger than the density of the object, 161 00:10:14 --> 00:10:20 and this is a necessary condition for floating. 162 00:10:18 --> 00:10:24 163 00:10:21 --> 00:10:27 And therefore, if an object sinks 164 00:10:23 --> 00:10:29 then the density of the object is larger 165 00:10:27 --> 00:10:33 than the density of the fluid. 166 00:10:31 --> 00:10:37 And the amazing thing is that this is completely independent 167 00:10:33 --> 00:10:39 of the dimensions of the object. 168 00:10:35 --> 00:10:41 The only thing that matters is the density. 169 00:10:39 --> 00:10:45 170 00:10:42 --> 00:10:48 If you take a pebble and you throw it in the water, 171 00:10:45 --> 00:10:51 it sinks, because the density of a pebble is higher than water. 172 00:10:48 --> 00:10:54 If you take a piece of wood, 173 00:10:49 --> 00:10:55 which has a density lower than water, 174 00:10:51 --> 00:10:57 and you throw it on water, it floats 175 00:10:53 --> 00:10:59 independent of its shape. 176 00:10:55 --> 00:11:01 Whether it sinks or whether it floats, 177 00:10:58 --> 00:11:04 the buoyant force is always identical 178 00:11:00 --> 00:11:06 to the weight of the displaced fluid. 179 00:11:04 --> 00:11:10 And this brings up one of my favorite questions 180 00:11:07 --> 00:11:13 that I have for you that I want you to think about. 181 00:11:10 --> 00:11:16 And if you have 182 00:11:11 --> 00:11:17 a full understanding now of Archimedes' principle, 183 00:11:14 --> 00:11:20 you will be able to answer it, 184 00:11:16 --> 00:11:22 so concentrate on what I am going to present you with. 185 00:11:19 --> 00:11:25 I am in a swimming pool, and I'm in a boat. 186 00:11:25 --> 00:11:31 Here is the swimming pool and here is the boat, 187 00:11:29 --> 00:11:35 and I am sitting in the boat 188 00:11:31 --> 00:11:37 and I have a rock here in my boat. 189 00:11:34 --> 00:11:40 I'm sitting in the swimming pool, nice rock in my boat. 190 00:11:38 --> 00:11:44 I mark the waterline of the swimming pool very carefully. 191 00:11:46 --> 00:11:52 I take the rock and I throw it overboard. 192 00:11:50 --> 00:11:56 Will the waterline go up, or will the waterline go down, 193 00:11:55 --> 00:12:01 or maybe the waterline will stay the same? 194 00:11:59 --> 00:12:05 Now, use your intuition-- don't mind being wrong. 195 00:12:02 --> 00:12:08 At home you have some time to think about it, 196 00:12:04 --> 00:12:10 and I am sure you will come up with the right answer. 197 00:12:06 --> 00:12:12 Who thinks that the waterline will go up the swimming pool? 198 00:12:10 --> 00:12:16 Who thinks that the waterline will go down? 199 00:12:14 --> 00:12:20 Who thinks that it will make no difference, 200 00:12:15 --> 00:12:21 that the waterline stays the same? 201 00:12:17 --> 00:12:23 202 00:12:19 --> 00:12:25 Amazing-- okay. 203 00:12:21 --> 00:12:27 Well, the waterline will change, but you figure it out. 204 00:12:25 --> 00:12:31 Okay, you apply Archimedes' principle 205 00:12:28 --> 00:12:34 and you'll get the answer. 206 00:12:31 --> 00:12:37 I want to talk about stability, particularly stability of ships, 207 00:12:35 --> 00:12:41 which is a very important thing-- they float. 208 00:12:39 --> 00:12:45 Suppose I have an object here which is floating in water. 209 00:12:44 --> 00:12:50 Here is the waterline, 210 00:12:46 --> 00:12:52 and let here be the center of mass of that object. 211 00:12:50 --> 00:12:56 Could be way off center. 212 00:12:51 --> 00:12:57 It could be an iceberg, 213 00:12:53 --> 00:12:59 it could be boulders, it could be rocks in there, right? 214 00:12:55 --> 00:13:01 It doesn't have to be uniform density. 215 00:12:57 --> 00:13:03 The center of mass could be off the center... 216 00:13:00 --> 00:13:06 of the geometric center. 217 00:13:02 --> 00:13:08 So if this object has a certain mass, 218 00:13:04 --> 00:13:10 then this is the gravitational force. 219 00:13:07 --> 00:13:13 But now look at the center of mass fluid that is displaced. 220 00:13:13 --> 00:13:19 That's clearly more here, 221 00:13:16 --> 00:13:22 somewhere here, the displaced fluid. 222 00:13:19 --> 00:13:25 That is where the buoyant force acts. 223 00:13:24 --> 00:13:30 And so now what you have... 224 00:13:25 --> 00:13:31 You have a torque on this object 225 00:13:27 --> 00:13:33 relative to any point that you choose. 226 00:13:29 --> 00:13:35 It doesn't matter where you pick a point, you have a torque. 227 00:13:32 --> 00:13:38 And so what's going to happen, 228 00:13:34 --> 00:13:40 this object is clearly going to rotate in this direction. 229 00:13:37 --> 00:13:43 And the torque will only be zero when the buoyant force 230 00:13:41 --> 00:13:47 and the gravitational force are on one line. 231 00:13:44 --> 00:13:50 Then the torque becomes zero, and then it is completely happy. 232 00:13:48 --> 00:13:54 Now, there are two ways that you can get them on one line. 233 00:13:52 --> 00:13:58 We discussed that earlier in a different context. 234 00:13:56 --> 00:14:02 You can either have the center of mass of the object 235 00:14:00 --> 00:14:06 below the center of mass of the displaced fluid or above. 236 00:14:04 --> 00:14:10 In both cases would they be on one line. 237 00:14:07 --> 00:14:13 However, in one case, there would be stable equilibrium. 238 00:14:11 --> 00:14:17 In the other, there would not be a stable equilibrium. 239 00:14:15 --> 00:14:21 I have here an object which has its center of mass very low. 240 00:14:19 --> 00:14:25 You can't tell that-- no way of knowing. 241 00:14:22 --> 00:14:28 All you know is that the weight of the displaced fluid 242 00:14:26 --> 00:14:32 that you see here is the same as the weight of the object. 243 00:14:31 --> 00:14:37 That's all you know. 244 00:14:33 --> 00:14:39 If I took this object and I tilt it a little 245 00:14:37 --> 00:14:43 with the center of mass very low-- 246 00:14:40 --> 00:14:46 so here is Mg and here is somewhere the waterline-- 247 00:14:45 --> 00:14:51 so the center of mass of the displaced fluid 248 00:14:49 --> 00:14:55 is somewhere here, so Fb is here, the buoyant force, 249 00:14:52 --> 00:14:58 you can see what's going to happen. 250 00:14:54 --> 00:15:00 It's going to rotate towards the right-- it's a restoring torque, 251 00:14:59 --> 00:15:05 and so it's completely stable. 252 00:15:01 --> 00:15:07 I can wobble it back and forth and it is stable. 253 00:15:05 --> 00:15:11 If I would turn it over, then it's not stable, 254 00:15:10 --> 00:15:16 because now I would have the center of mass 255 00:15:12 --> 00:15:18 somewhere here, high up, so now I have Mg. 256 00:15:19 --> 00:15:25 And the center of the buoyant force, the displaced water, 257 00:15:22 --> 00:15:28 is about here, so now I have the buoyant force up, 258 00:15:26 --> 00:15:32 and now you see what's going to happen. 259 00:15:28 --> 00:15:34 I tilt it to the side, and it will rotate even further. 260 00:15:32 --> 00:15:38 This torque will drive it away from the vertical. 261 00:15:34 --> 00:15:40 And that's very important, therefore, with ships, 262 00:15:37 --> 00:15:43 that you always build the ship 263 00:15:38 --> 00:15:44 such that the center of mass of the ship is 264 00:15:41 --> 00:15:47 as low as you can get it. 265 00:15:42 --> 00:15:48 That gives you the most stable configuration. 266 00:15:45 --> 00:15:51 If you bring the center of mass of ships very high-- 267 00:15:47 --> 00:15:53 in the 17th century, they had these very massive cannons 268 00:15:50 --> 00:15:56 which were very high on the deck-- 269 00:15:52 --> 00:15:58 then the ship can capsize, and it has happened many times 270 00:15:55 --> 00:16:01 because the center of mass was just too high. 271 00:15:58 --> 00:16:04 So here... the center of mass is somewhere here. 272 00:16:02 --> 00:16:08 Very heavy, this part. 273 00:16:04 --> 00:16:10 And so now, if I lower it in the water 274 00:16:06 --> 00:16:12 notice it goes into the water to the same depth, 275 00:16:09 --> 00:16:15 because the buoyant force is, of course, the same, 276 00:16:13 --> 00:16:19 so the amount of displaced water is the same in both cases. 277 00:16:17 --> 00:16:23 But now the center of mass is high and this is very unstable. 278 00:16:21 --> 00:16:27 When I let it go, it flips over. 279 00:16:23 --> 00:16:29 So the center of mass of the object was higher 280 00:16:27 --> 00:16:33 than the center of mass of the displaced fluid. 281 00:16:30 --> 00:16:36 And so with ships, you have to be very careful about that. 282 00:16:34 --> 00:16:40 283 00:16:38 --> 00:16:44 Let's talk a little bit about balloons. 284 00:16:41 --> 00:16:47 285 00:16:45 --> 00:16:51 If I have a balloon, the situation is not too dissimilar 286 00:16:52 --> 00:16:58 from having an object floating in a liquid. 287 00:16:56 --> 00:17:02 Let the balloon have a mass M. 288 00:16:59 --> 00:17:05 That is the mass of the gas in the balloon 289 00:17:04 --> 00:17:10 plus all the rest, and what I mean by "all the rest"... 290 00:17:08 --> 00:17:14 That is the material of the balloon and the string-- 291 00:17:11 --> 00:17:17 everything else that makes up the mass. 292 00:17:13 --> 00:17:19 It has a certain volume v, 293 00:17:16 --> 00:17:22 and so there is a certain rho of the gas inside 294 00:17:20 --> 00:17:26 and there is rho of air outside. 295 00:17:23 --> 00:17:29 And I want to evaluate 296 00:17:25 --> 00:17:31 what the criterion is for this balloon to rise. 297 00:17:29 --> 00:17:35 Well, for it to rise, 298 00:17:30 --> 00:17:36 the buoyant force will have to be larger than Mg. 299 00:17:34 --> 00:17:40 What is the buoyant force? 300 00:17:36 --> 00:17:42 That is the weight of the displaced fluid. 301 00:17:39 --> 00:17:45 The fluid, in this case, is air. 302 00:17:41 --> 00:17:47 So the weight of the displaced fluid 303 00:17:43 --> 00:17:49 is the volume times the density of the air-- 304 00:17:47 --> 00:17:53 that's the fluid in which it is now-- 305 00:17:50 --> 00:17:56 times g, that is the buoyant force. 306 00:17:53 --> 00:17:59 That's... the weight of the displaced fluid 307 00:17:56 --> 00:18:02 has to be larger than Mg. 308 00:17:59 --> 00:18:05 Now, Mg is the mass of the gas, 309 00:18:02 --> 00:18:08 which is the volume of the gas times the density of the gas. 310 00:18:09 --> 00:18:15 That's the mass times g-- 311 00:18:12 --> 00:18:18 because we have to convert it to a force-- 312 00:18:14 --> 00:18:20 plus all the rest, times g. 313 00:18:19 --> 00:18:25 I lose my g, and what you see... 314 00:18:24 --> 00:18:30 that this, of course, is always larger than zero. 315 00:18:28 --> 00:18:34 There's always some mass associated with the skin 316 00:18:32 --> 00:18:38 and in this case with the string. 317 00:18:35 --> 00:18:41 But you see, the only way that this balloon can rise 318 00:18:39 --> 00:18:45 is that the density of the gas must be smaller 319 00:18:43 --> 00:18:49 than the density of air. 320 00:18:44 --> 00:18:50 Density of the gas must be less than the density of the air. 321 00:18:49 --> 00:18:55 This is a necessary condition for this to hold. 322 00:18:52 --> 00:18:58 It is not a sufficient condition, 323 00:18:55 --> 00:19:01 because I can take a balloon, 324 00:18:57 --> 00:19:03 put a little bit of helium in there-- 325 00:18:59 --> 00:19:05 so the density of the gas is lower than the density of air-- 326 00:19:04 --> 00:19:10 but it may not rise, and that's because of this term. 327 00:19:08 --> 00:19:14 But it is a necessary condition but not a sufficient condition. 328 00:19:13 --> 00:19:19 Now I'm going to make you see 329 00:19:15 --> 00:19:21 a demonstration which is extremely nonintuitive, 330 00:19:19 --> 00:19:25 and I will try, step by step, to explain to you 331 00:19:23 --> 00:19:29 why you see what you see. 332 00:19:25 --> 00:19:31 What you're going to see, very nonintuitive, 333 00:19:28 --> 00:19:34 so try to follow closely why you see what you will see. 334 00:19:34 --> 00:19:40 I have here a pendulum with an apple, 335 00:19:38 --> 00:19:44 and here I have a balloon filled with helium. 336 00:19:42 --> 00:19:48 I cut this string and I cut this string. 337 00:19:44 --> 00:19:50 Gravity is in this direction. 338 00:19:46 --> 00:19:52 The apple will fall, the balloon will rise. 339 00:19:49 --> 00:19:55 The balloon goes in the opposite direction 340 00:19:52 --> 00:19:58 than the gravitational acceleration. 341 00:19:55 --> 00:20:01 If there were no gravity, this balloon would not rise 342 00:20:00 --> 00:20:06 and the apple would not fall. 343 00:20:03 --> 00:20:09 Do we agree so far? 344 00:20:04 --> 00:20:10 Without gravity, apple would not fall, balloon would not rise. 345 00:20:09 --> 00:20:15 Now we go in outer space. 346 00:20:11 --> 00:20:17 347 00:20:16 --> 00:20:22 Here is a compartment and here is an apple. 348 00:20:21 --> 00:20:27 349 00:20:24 --> 00:20:30 I'm here as well. 350 00:20:28 --> 00:20:34 None of us have weight, there's no gravity, 351 00:20:31 --> 00:20:37 and here is a helium-filled object, a balloon, 352 00:20:35 --> 00:20:41 and there's air inside. 353 00:20:36 --> 00:20:42 We're in outer space, there's no gravity. 354 00:20:39 --> 00:20:45 Nothing has any weight. 355 00:20:42 --> 00:20:48 We're all floating. 356 00:20:44 --> 00:20:50 357 00:20:46 --> 00:20:52 Now I'm going to accelerate. 358 00:20:48 --> 00:20:54 I have a rocket-- I'm going to accelerate it in this direction 359 00:20:53 --> 00:20:59 with acceleration a. 360 00:20:55 --> 00:21:01 We all perceive, now, a perceived gravity 361 00:21:00 --> 00:21:06 in this direction. 362 00:21:02 --> 00:21:08 I call it g. 363 00:21:04 --> 00:21:10 So the apple will fall. 364 00:21:07 --> 00:21:13 I'm standing there, I see this apple fall. 365 00:21:09 --> 00:21:15 I'm in this compartment, closed compartment. 366 00:21:11 --> 00:21:17 I see the apple go down. 367 00:21:12 --> 00:21:18 A little later, the apple will be here. 368 00:21:14 --> 00:21:20 I myself fall; a little later, I'm there. 369 00:21:17 --> 00:21:23 I can put a bathroom scale here 370 00:21:19 --> 00:21:25 and weigh myself on the bathroom scale. 371 00:21:22 --> 00:21:28 My weight will be M times this a, 372 00:21:24 --> 00:21:30 M being my mass, a being this acceleration. 373 00:21:26 --> 00:21:32 I really think that it is gravity in this direction. 374 00:21:30 --> 00:21:36 The air wants to fall, 375 00:21:34 --> 00:21:40 but the balloon wants to go against gravity. 376 00:21:38 --> 00:21:44 The balloon will rise. 377 00:21:41 --> 00:21:47 378 00:21:45 --> 00:21:51 The air wants to fall, so inside here 379 00:21:49 --> 00:21:55 you create a differential pressure between the bottom, P1, 380 00:21:55 --> 00:22:01 and the top of the air, P2, inside here. 381 00:21:59 --> 00:22:05 Just like the atmosphere on earth-- 382 00:22:01 --> 00:22:07 the atmosphere is pushing down on us-- 383 00:22:04 --> 00:22:10 the pressure is here higher than there. 384 00:22:06 --> 00:22:12 So you get P1 is higher than P2. 385 00:22:11 --> 00:22:17 386 00:22:13 --> 00:22:19 So you create yourself an atmosphere, 387 00:22:16 --> 00:22:22 and the balloon will rise. 388 00:22:18 --> 00:22:24 The balloon goes in the opposite direction of gravity. 389 00:22:22 --> 00:22:28 If there were no air in there, 390 00:22:25 --> 00:22:31 then clearly all of us would fall: 391 00:22:27 --> 00:22:33 The apple would fall, I would fall, 392 00:22:29 --> 00:22:35 and the helium balloon would fall. 393 00:22:31 --> 00:22:37 The only reason why the helium balloon rises 394 00:22:34 --> 00:22:40 is because the air is there 395 00:22:36 --> 00:22:42 and because you build up this differential pressure. 396 00:22:40 --> 00:22:46 Now comes my question to you: 397 00:22:42 --> 00:22:48 Instead of accelerating it upwards 398 00:22:46 --> 00:22:52 and creating perceived gravity down, 399 00:22:49 --> 00:22:55 I'm now going to accelerate it in this direction, 400 00:22:53 --> 00:22:59 something that I'm going to do shortly in the classroom. 401 00:22:58 --> 00:23:04 I'm going to accelerate all of us in this direction a. 402 00:23:03 --> 00:23:09 In which direction will the apple go? 403 00:23:05 --> 00:23:11 In which direction will the balloon go? 404 00:23:08 --> 00:23:14 What do you think? 405 00:23:11 --> 00:23:17 The apple will go 406 00:23:13 --> 00:23:19 in the direction that it perceives gravity. 407 00:23:16 --> 00:23:22 The apple will go like this. 408 00:23:18 --> 00:23:24 I will go like this. 409 00:23:20 --> 00:23:26 The air wants to go like this. 410 00:23:22 --> 00:23:28 But helium-- balloon-- goes 411 00:23:24 --> 00:23:30 in the opposite direction of gravity, 412 00:23:27 --> 00:23:33 so helium goes in this direction. 413 00:23:29 --> 00:23:35 In fact, what you're doing, 414 00:23:30 --> 00:23:36 you're building here an atmosphere 415 00:23:32 --> 00:23:38 where pressure P1 here will be higher 416 00:23:34 --> 00:23:40 than the pressure P2 there. 417 00:23:36 --> 00:23:42 The air wants to go in this direction. 418 00:23:39 --> 00:23:45 The pressure here is higher than the pressure there-- 419 00:23:43 --> 00:23:49 larger than zero. 420 00:23:45 --> 00:23:51 421 00:23:47 --> 00:23:53 If there's no air in there, we would all fall. 422 00:23:50 --> 00:23:56 Helium would fall... helium balloon would fall, 423 00:23:54 --> 00:24:00 apple would fall, and I would fall. 424 00:23:56 --> 00:24:02 425 00:23:59 --> 00:24:05 I have here an apple on a string 426 00:24:06 --> 00:24:12 in a closed compartment, not unlike what we have there 427 00:24:12 --> 00:24:18 except I can't take you out 428 00:24:14 --> 00:24:20 to an area where we have no gravity. 429 00:24:17 --> 00:24:23 So here is that closed compartment, 430 00:24:20 --> 00:24:26 and here is the apple. 431 00:24:22 --> 00:24:28 There is gravity in this direction. 432 00:24:25 --> 00:24:31 It wants to fall 433 00:24:27 --> 00:24:33 in that direction of gravity if I cut the wire. 434 00:24:30 --> 00:24:36 Now I'm going to accelerate it in this direction, 435 00:24:33 --> 00:24:39 and when I do that, I add a perceived component of gravity 436 00:24:37 --> 00:24:43 in the opposite direction. 437 00:24:39 --> 00:24:45 So I add a perceived component of gravity in this direction. 438 00:24:43 --> 00:24:49 So this apple wants to fall down 439 00:24:45 --> 00:24:51 because of the gravity that I cannot avoid, 440 00:24:48 --> 00:24:54 and it wants to fall in this direction. 441 00:24:50 --> 00:24:56 So what will the string do? 442 00:24:52 --> 00:24:58 It's very clear, very intuitive, 443 00:24:54 --> 00:25:00 no one has any problem with that-- the string will do this. 444 00:24:59 --> 00:25:05 Now I have a balloon here. 445 00:25:01 --> 00:25:07 446 00:25:06 --> 00:25:12 Helium. 447 00:25:07 --> 00:25:13 There is gravity in this direction. 448 00:25:09 --> 00:25:15 That's why the balloon wants to go up. 449 00:25:11 --> 00:25:17 It opposes gravity. 450 00:25:13 --> 00:25:19 I'm going to accelerate the car in this direction. 451 00:25:16 --> 00:25:22 I introduce perceived gravity in this direction. 452 00:25:18 --> 00:25:24 What does the balloon want to do? 453 00:25:20 --> 00:25:26 It wants to go against gravity. 454 00:25:21 --> 00:25:27 I build up in here, and it must be a closed compartment... 455 00:25:24 --> 00:25:30 I must build up there a pressure differential. 456 00:25:27 --> 00:25:33 The air wants to fall in this direction. 457 00:25:29 --> 00:25:35 I build up a pressure here 458 00:25:31 --> 00:25:37 which is larger than the pressure there. 459 00:25:33 --> 00:25:39 That's why it has to be a closed compartment. 460 00:25:36 --> 00:25:42 What will the helium balloon do? 461 00:25:39 --> 00:25:45 It will go like that. 462 00:25:40 --> 00:25:46 That is very nonintuitive. 463 00:25:42 --> 00:25:48 So I accelerate this car. 464 00:25:44 --> 00:25:50 As I will do, the apple will go back, 465 00:25:46 --> 00:25:52 which is completely consistent with all our intuition, 466 00:25:49 --> 00:25:55 but the helium balloon will go forward. 467 00:25:52 --> 00:25:58 468 00:25:54 --> 00:26:00 Let's first do it with the apple, 469 00:25:56 --> 00:26:02 which is totally consistent with anyone's intuition. 470 00:26:00 --> 00:26:06 I'm going to make sure that the apple is not swinging too much. 471 00:26:07 --> 00:26:13 Now, it only happens during the acceleration, 472 00:26:10 --> 00:26:16 so it's only during the very short portion that I accelerate 473 00:26:14 --> 00:26:20 that you see the apple go back, 474 00:26:16 --> 00:26:22 and then of course it starts to swing-- forget that part. 475 00:26:19 --> 00:26:25 So watch closely-- only the moment that I accelerate 476 00:26:22 --> 00:26:28 the apple will come this way. 477 00:26:23 --> 00:26:29 It goes in the direction 478 00:26:24 --> 00:26:30 of the extra component of perceived gravity. 479 00:26:26 --> 00:26:32 Ready? 480 00:26:27 --> 00:26:33 481 00:26:29 --> 00:26:35 Boy, it almost hit this glass here. 482 00:26:31 --> 00:26:37 Everyone could see that, right? 483 00:26:32 --> 00:26:38 Okay. 484 00:26:34 --> 00:26:40 Now we're going to do it with the balloon. 485 00:26:37 --> 00:26:43 We're going to take this one off. 486 00:26:39 --> 00:26:45 487 00:26:42 --> 00:26:48 And now let's take one of our beautiful balloons. 488 00:26:45 --> 00:26:51 489 00:26:54 --> 00:27:00 We're going to put a balloon in here. 490 00:26:57 --> 00:27:03 Has to be a closed compartment 491 00:26:58 --> 00:27:04 so that the air can build up the pressure differential. 492 00:27:05 --> 00:27:11 493 00:27:13 --> 00:27:19 There's always problems 494 00:27:14 --> 00:27:20 with static charges on these systems. 495 00:27:18 --> 00:27:24 Okay. 496 00:27:20 --> 00:27:26 Only as long as I accelerate 497 00:27:22 --> 00:27:28 will the balloon go in a forward direction, 498 00:27:24 --> 00:27:30 so I accelerate in this direction, 499 00:27:26 --> 00:27:32 and what you're going to see is really very nonintuitive. 500 00:27:29 --> 00:27:35 Every time I see it, I say to myself, 501 00:27:31 --> 00:27:37 "I can reason it, but do I understand it?" 502 00:27:34 --> 00:27:40 I don't know, what is the difference 503 00:27:35 --> 00:27:41 between reasoning and understanding? 504 00:27:36 --> 00:27:42 There we go. 505 00:27:37 --> 00:27:43 506 00:27:39 --> 00:27:45 The balloon went this way. 507 00:27:41 --> 00:27:47 You can do this in your car with your parents. 508 00:27:44 --> 00:27:50 It's really fun to do it. 509 00:27:46 --> 00:27:52 Have a string with an apple or something else 510 00:27:48 --> 00:27:54 and have a helium balloon. 511 00:27:50 --> 00:27:56 Close the windows. 512 00:27:52 --> 00:27:58 They don't have to be totally closed, but more or less, 513 00:27:56 --> 00:28:02 and ask your dad or your mom to slam the brakes. 514 00:27:59 --> 00:28:05 If you slam the brakes, what will happen? 515 00:28:02 --> 00:28:08 The apple will go... what do you think? 516 00:28:05 --> 00:28:11 If you slam the brakes, 517 00:28:07 --> 00:28:13 the apple will go forwards, balloon will go backward. 518 00:28:09 --> 00:28:15 If you accelerate the car all of a sudden, 519 00:28:11 --> 00:28:17 the apple will go backwards and the balloon will go forward. 520 00:28:14 --> 00:28:20 You can do that at home. 521 00:28:16 --> 00:28:22 You can enjoy... entertain your parents at Thanksgiving. 522 00:28:20 --> 00:28:26 They'll get some of their $25,000 tuition back. 523 00:28:24 --> 00:28:30 (class laughs ) 524 00:28:25 --> 00:28:31 525 00:28:29 --> 00:28:35 When fluids are moving, 526 00:28:32 --> 00:28:38 situations are way more complicated 527 00:28:36 --> 00:28:42 than when they are static. 528 00:28:39 --> 00:28:45 And this leads 529 00:28:40 --> 00:28:46 to, again, very nonintuitive behavior of fluids. 530 00:28:49 --> 00:28:55 I will derive in a short-cut way 531 00:28:55 --> 00:29:01 a very famous equation which is called Bernoulli's equation, 532 00:29:00 --> 00:29:06 which relates kinetic energy 533 00:29:04 --> 00:29:10 with potential energy and pressure. 534 00:29:09 --> 00:29:15 Suppose I have a fluid, noncompressible, like so. 535 00:29:17 --> 00:29:23 This cross-sectional area is A2 and the pressure here is P2. 536 00:29:26 --> 00:29:32 And I have a velocity of that liquid which is v2 537 00:29:34 --> 00:29:40 and this level is y2. 538 00:29:36 --> 00:29:42 Here I have a cross-sectional area A1. 539 00:29:41 --> 00:29:47 I have a pressure P1. 540 00:29:43 --> 00:29:49 My level is y1; this is increasing y. 541 00:29:48 --> 00:29:54 And I have a much larger velocity 542 00:29:50 --> 00:29:56 because the cross-section is substantially smaller there. 543 00:29:54 --> 00:30:00 Now, if this fluid were completely static, 544 00:29:57 --> 00:30:03 if it were not moving-- 545 00:29:59 --> 00:30:05 so forget about the v1 and forget about the v2; 546 00:30:02 --> 00:30:08 it's just sitting still-- 547 00:30:04 --> 00:30:10 then P1 minus P2 would be rho g times y2 minus y1 548 00:30:13 --> 00:30:19 if rho is the density of the fluid. 549 00:30:16 --> 00:30:22 That's Pascal's Law. 550 00:30:18 --> 00:30:24 So it would just be sitting still, 551 00:30:20 --> 00:30:26 and we know that the pressure here 552 00:30:23 --> 00:30:29 would be lower than the pressure there. 553 00:30:25 --> 00:30:31 This is also, if you want to, rho gh 554 00:30:29 --> 00:30:35 if you call this distance h. 555 00:30:34 --> 00:30:40 556 00:30:36 --> 00:30:42 Rho gh-- that reminds me of mgh, 557 00:30:39 --> 00:30:45 and mgh is gravitational potential energy. 558 00:30:43 --> 00:30:49 When I divide m by volume, I get density. 559 00:30:47 --> 00:30:53 So this is really a term 560 00:30:50 --> 00:30:56 which is gravitational potential energy 561 00:30:54 --> 00:31:00 per unit volume. 562 00:30:56 --> 00:31:02 That makes the m divided by volume become density. 563 00:31:01 --> 00:31:07 Therefore, pressure itself must also have 564 00:31:05 --> 00:31:11 the dimension of energy per unit volume. 565 00:31:10 --> 00:31:16 And if we now set this whole machine in motion, 566 00:31:13 --> 00:31:19 then there are three players: 567 00:31:16 --> 00:31:22 There is, on the one hand, kinetic energy-- of motion-- 568 00:31:20 --> 00:31:26 kinetic energy... I take it, per unit volume. 569 00:31:24 --> 00:31:30 There is gravitational potential energy... 570 00:31:28 --> 00:31:34 I will take it, per unit volume. 571 00:31:30 --> 00:31:36 And then there is pressure. 572 00:31:32 --> 00:31:38 They're equal partners. 573 00:31:34 --> 00:31:40 574 00:31:36 --> 00:31:42 And if I apply the conservation of energy, 575 00:31:39 --> 00:31:45 the sum of these three should remain constant. 576 00:31:42 --> 00:31:48 That's the idea behind Bernoulli's law, 577 00:31:45 --> 00:31:51 Bernoulli's equation. 578 00:31:47 --> 00:31:53 When I take a fluid element 579 00:31:49 --> 00:31:55 and I move it from one position in the tube to another position, 580 00:31:54 --> 00:32:00 it trades speed for either height or for pressure. 581 00:31:58 --> 00:32:04 What is the kinetic energy per unit volume? 582 00:32:01 --> 00:32:07 Well, the kinetic energy is one-half mv squared. 583 00:32:05 --> 00:32:11 I divide by volume, I get one-half rho v squared. 584 00:32:08 --> 00:32:14 What is gravitational potential energy? 585 00:32:10 --> 00:32:16 That is mgy. 586 00:32:12 --> 00:32:18 I divide by volume, and so I get rho gy 587 00:32:16 --> 00:32:22 plus the pressure at that location y, 588 00:32:20 --> 00:32:26 and that must be a constant. 589 00:32:23 --> 00:32:29 And this, now, is Bernoulli's equation. 590 00:32:30 --> 00:32:36 It is a conservation of energy equation. 591 00:32:37 --> 00:32:43 And as I will show you, 592 00:32:39 --> 00:32:45 it has very remarkable consequences. 593 00:32:42 --> 00:32:48 594 00:32:46 --> 00:32:52 First I will show you an example whereby I keep y constant. 595 00:32:52 --> 00:32:58 So I have a tube which changes diameter, 596 00:32:57 --> 00:33:03 but the tube is not changing with level y, as I do there. 597 00:33:05 --> 00:33:11 So I come in here, cross-sectional area A1. 598 00:33:12 --> 00:33:18 I widen it, cross-sectional area A2. 599 00:33:17 --> 00:33:23 600 00:33:20 --> 00:33:26 This is y-- it's the same for both. 601 00:33:23 --> 00:33:29 I have here inside pressure P1 602 00:33:26 --> 00:33:32 and here inside I have pressure P2 603 00:33:29 --> 00:33:35 and this is the density of the fluid. 604 00:33:33 --> 00:33:39 There is here a velocity v2, and there is here a velocity v1. 605 00:33:39 --> 00:33:45 And clearly v1 is way larger than v2 606 00:33:42 --> 00:33:48 because A1 times v1 must be A2 times v2 607 00:33:46 --> 00:33:52 because the fluid is incompressible. 608 00:33:50 --> 00:33:56 So the same amount of matter 609 00:33:52 --> 00:33:58 that flows through here in one second 610 00:33:54 --> 00:34:00 must flow through here in one second. 611 00:33:56 --> 00:34:02 And so these have to be the same, 612 00:33:58 --> 00:34:04 and since A1 is much smaller than A2, 613 00:34:01 --> 00:34:07 this velocity is much larger than v2. 614 00:34:05 --> 00:34:11 615 00:34:08 --> 00:34:14 Now I'm going to apply Bernoulli's equation. 616 00:34:12 --> 00:34:18 So the first term tells me that one-half rho v1 squared... 617 00:34:17 --> 00:34:23 I can forget the second term 618 00:34:19 --> 00:34:25 because I get the same term here as I get there 619 00:34:21 --> 00:34:27 because I measure the pressure here 620 00:34:23 --> 00:34:29 and I measure the pressure there. 621 00:34:24 --> 00:34:30 They have the same level of y. 622 00:34:25 --> 00:34:31 So I can ignore the second term. 623 00:34:29 --> 00:34:35 Plus P1 must be one-half rho v2 squared plus P2. 624 00:34:36 --> 00:34:42 That's what Bernoulli's equation tells me. 625 00:34:41 --> 00:34:47 Now, v1 is larger than v2. 626 00:34:47 --> 00:34:53 The only way that this can be correct, then, 627 00:34:49 --> 00:34:55 is that P1 must be less than P2. 628 00:34:51 --> 00:34:57 So you will say, "Big deal." 629 00:34:53 --> 00:34:59 Well, it's a big deal, because I would have guessed 630 00:34:56 --> 00:35:02 exactly the other way around, and so would you, 631 00:34:58 --> 00:35:04 because here is where the highest velocity is, 632 00:35:00 --> 00:35:06 and all our instincts would say, 633 00:35:02 --> 00:35:08 "Oh, if the velocity is high, there's a lot of pressure." 634 00:35:05 --> 00:35:11 It's exactly the other way around. 635 00:35:07 --> 00:35:13 Here is the low pressure, and here is the high pressure, 636 00:35:10 --> 00:35:16 which is one quite bizarre consequence 637 00:35:12 --> 00:35:18 of Bernoulli's equation. 638 00:35:16 --> 00:35:22 639 00:35:20 --> 00:35:26 You must all have encountered in your life 640 00:35:24 --> 00:35:30 what we call a siphon. 641 00:35:26 --> 00:35:32 They were used in the medieval and they're still used today. 642 00:35:31 --> 00:35:37 You have here... 643 00:35:34 --> 00:35:40 A bucket in general is used with water-- lakes. 644 00:35:38 --> 00:35:44 We have water here, but it could be any liquid. 645 00:35:42 --> 00:35:48 And I stick in here a tube which is small in diameter, 646 00:35:49 --> 00:35:55 substantially smaller than this area here. 647 00:35:52 --> 00:35:58 And there will be water in here up to this level-- 648 00:35:58 --> 00:36:04 this level P2, y2. 649 00:36:04 --> 00:36:10 This is y1, increasing value of y. 650 00:36:09 --> 00:36:15 This height difference is h. 651 00:36:11 --> 00:36:17 P2 is one atmosphere. 652 00:36:13 --> 00:36:19 I put a one there-- it's atmosphere. 653 00:36:16 --> 00:36:22 And here, if it's open, then P1 is also one atmosphere. 654 00:36:21 --> 00:36:27 So there's air in here and there's liquid in here. 655 00:36:26 --> 00:36:32 I take this open end in my mouth and I suck the water in 656 00:36:31 --> 00:36:37 so that it's filled with this water, full with this water. 657 00:36:37 --> 00:36:43 And strange as it may be, it's like making a hole in this tank. 658 00:36:43 --> 00:36:49 If I take my finger off here, the water will start to run out, 659 00:36:47 --> 00:36:53 and I will show you that. 660 00:36:48 --> 00:36:54 And you have here a velocity v1. 661 00:36:52 --> 00:36:58 The water will stream down into this here 662 00:36:55 --> 00:37:01 and the velocity here is approximately zero, 663 00:36:59 --> 00:37:05 because this area is so much larger 664 00:37:01 --> 00:37:07 than this cross-sectional area that to a good approximation 665 00:37:06 --> 00:37:12 this water is going down extremely slowly. 666 00:37:09 --> 00:37:15 667 00:37:11 --> 00:37:17 Let's call this height difference d. 668 00:37:16 --> 00:37:22 I apply Bernoulli's law. 669 00:37:17 --> 00:37:23 So now we have a situation where the y's are different 670 00:37:21 --> 00:37:27 but the pressure is the same, 671 00:37:23 --> 00:37:29 because right here at this point of the liquid 672 00:37:26 --> 00:37:32 I have one atmosphere, which is barometric pressure, 673 00:37:29 --> 00:37:35 and since this is open with the outside world, 674 00:37:32 --> 00:37:38 P1 is also one atmosphere. 675 00:37:33 --> 00:37:39 So now I lose my P term. 676 00:37:35 --> 00:37:41 There I lost my y term; now I lose my P term. 677 00:37:39 --> 00:37:45 So now I have that one-half rho... rho-- 678 00:37:43 --> 00:37:49 this is rho of the liquid-- 679 00:37:47 --> 00:37:53 v1 squared plus rho g times y1 must be one-half rho v2 squared, 680 00:37:57 --> 00:38:03 but we agreed that that was zero, so I don't have that term. 681 00:38:01 --> 00:38:07 So I only have rho gy2. 682 00:38:07 --> 00:38:13 I lose my g's... no, I don't lose my g's. 683 00:38:10 --> 00:38:16 One-half rho v squared-- no, that's fine. 684 00:38:13 --> 00:38:19 And so... I lose my rho. 685 00:38:15 --> 00:38:21 This is one-half. 686 00:38:17 --> 00:38:23 I lose my rho. 687 00:38:18 --> 00:38:24 And so you get 688 00:38:20 --> 00:38:26 that one-half v1 squared equals g times y2 minus y1, which is h. 689 00:38:27 --> 00:38:33 And so what do you find? 690 00:38:29 --> 00:38:35 That the speed with which this water is running out here, v1, 691 00:38:33 --> 00:38:39 is the square root of 2gh. 692 00:38:36 --> 00:38:42 And you've seen that before. 693 00:38:39 --> 00:38:45 If you take a pebble and you release a pebble from this level 694 00:38:43 --> 00:38:49 and you let it fall, 695 00:38:44 --> 00:38:50 it will reach this point here, this level 696 00:38:47 --> 00:38:53 with the speed the square root of 2gh. 697 00:38:50 --> 00:38:56 We've seen that many times. 698 00:38:52 --> 00:38:58 So what is happening here-- 699 00:38:54 --> 00:39:00 since the pressure terms are the same here and there, 700 00:38:57 --> 00:39:03 now there's only a conversion. 701 00:38:59 --> 00:39:05 Gravitational potential energy-- 702 00:39:01 --> 00:39:07 which is higher here than there-- 703 00:39:02 --> 00:39:08 is now converted to kinetic energy. 704 00:39:07 --> 00:39:13 This siphon would only work if d is less than ten meters. 705 00:39:12 --> 00:39:18 Because of the barometric pressure 706 00:39:14 --> 00:39:20 you can never suck up this water-- 707 00:39:16 --> 00:39:22 no one can; a vacuum pump can't either-- 708 00:39:18 --> 00:39:24 to a level that is higher than ten meters. 709 00:39:21 --> 00:39:27 When I did the experiment there with the cranberry juice, 710 00:39:24 --> 00:39:30 I was able to get it up to five meters, 711 00:39:26 --> 00:39:32 but ten meters would have been the theoretical maximum. 712 00:39:30 --> 00:39:36 So this has to be less than ten meters that you go up. 713 00:39:33 --> 00:39:39 If I would have made a hole in this tank here, 714 00:39:37 --> 00:39:43 just like this, down to exactly this level, 715 00:39:40 --> 00:39:46 and I would have asked you to calculate 716 00:39:42 --> 00:39:48 with what speed the water is running out, 717 00:39:45 --> 00:39:51 you would have found exactly the same 718 00:39:47 --> 00:39:53 if you had applied Bernoulli's equation. 719 00:39:49 --> 00:39:55 This is a way that people... 720 00:39:51 --> 00:39:57 I've seen people steal other people's gasoline 721 00:39:53 --> 00:39:59 in the time that gasoline was very scarce 722 00:39:56 --> 00:40:02 and that there were no locks yet on the gasoline caps. 723 00:39:59 --> 00:40:05 You would put a hose in the gasoline tank 724 00:40:01 --> 00:40:07 and you would have to suck on it a little-- 725 00:40:03 --> 00:40:09 you have to sacrifice a little bit-- 726 00:40:04 --> 00:40:10 you get a little bit of gasoline in your mouth, 727 00:40:07 --> 00:40:13 and then you can just empty someone's gasoline tank 728 00:40:10 --> 00:40:16 by having a canister or by having a jerrican 729 00:40:13 --> 00:40:19 and fill it with gasoline. 730 00:40:15 --> 00:40:21 And I'm going to show that now to you by emptying... 731 00:40:19 --> 00:40:25 That's still cranberry juice, by the way, from our last lecture. 732 00:40:26 --> 00:40:32 So let's put this up on a stool. 733 00:40:30 --> 00:40:36 734 00:40:32 --> 00:40:38 So there is the hose-- it's that thing-- 735 00:40:39 --> 00:40:45 and I'm going to transfer this liquid from here to here. 736 00:40:43 --> 00:40:49 So first I have to fill it with cranberry juice. 737 00:40:46 --> 00:40:52 738 00:40:50 --> 00:40:56 And there it goes. 739 00:40:52 --> 00:40:58 And as long as this level is below that level, 740 00:40:56 --> 00:41:02 it keeps running. 741 00:40:59 --> 00:41:05 Not so intuitive. 742 00:41:00 --> 00:41:06 I remember, I was at a summer camp 743 00:41:03 --> 00:41:09 when I was maybe six or seven years old. 744 00:41:05 --> 00:41:11 I couldn't believe it when I saw this for the first time. 745 00:41:10 --> 00:41:16 We had these outdoor sinks 746 00:41:11 --> 00:41:17 where we washed ourselves and brushed our teeth, 747 00:41:14 --> 00:41:20 and the sink was clogged, it was full with water. 748 00:41:17 --> 00:41:23 And one of the camp leaders took a hose, sucked up 749 00:41:21 --> 00:41:27 and it emptied itself. 750 00:41:22 --> 00:41:28 And I really thought, you know, 751 00:41:24 --> 00:41:30 you'd have to take spoonfuls of water or maybe buckets 752 00:41:27 --> 00:41:33 and scoop it out. 753 00:41:28 --> 00:41:34 This is the way you do it. 754 00:41:30 --> 00:41:36 Very nonintuitive. 755 00:41:31 --> 00:41:37 The nonintuitive part is 756 00:41:33 --> 00:41:39 that it runs up against gravity there. 757 00:41:36 --> 00:41:42 So we can let it sit there 758 00:41:37 --> 00:41:43 and we have a transfer, mass transfer of cranberry juice. 759 00:41:42 --> 00:41:48 760 00:41:57 --> 00:42:03 Last time I was testing my lungs to see how strong I was. 761 00:42:01 --> 00:42:07 I wasn't very good, right? 762 00:42:03 --> 00:42:09 I could only blow up one meter of water 763 00:42:05 --> 00:42:11 and only suck one meter water. 764 00:42:08 --> 00:42:14 Differential pressure only one-tenth of an atmosphere. 765 00:42:11 --> 00:42:17 Today I would like to test one of the students 766 00:42:15 --> 00:42:21 who, no doubt, is more powerful than I am. 767 00:42:19 --> 00:42:25 And I have here a funnel... 768 00:42:25 --> 00:42:31 with a Ping-Pong ball here, very lightweight, 769 00:42:28 --> 00:42:34 and we're going to have a contest 770 00:42:30 --> 00:42:36 to see who can blow it the highest. 771 00:42:32 --> 00:42:38 I have two funnels, so it's very hygienic. 772 00:42:35 --> 00:42:41 I will try it with this one. 773 00:42:37 --> 00:42:43 They're clean, they just... 774 00:42:38 --> 00:42:44 We just got them from the chemistry department. 775 00:42:41 --> 00:42:47 And so I would like to see a volunteer-- 776 00:42:43 --> 00:42:49 woman or man, it doesn't matter. 777 00:42:45 --> 00:42:51 You want to try it, see whether you can reach the ceiling? 778 00:42:50 --> 00:42:56 You don't want to try it? 779 00:42:52 --> 00:42:58 Come on! You want to try it? 780 00:42:54 --> 00:43:00 You're shy? You don't want to? 781 00:42:57 --> 00:43:03 Can I persuade you? I can. 782 00:43:00 --> 00:43:06 Okay, come along. 783 00:43:01 --> 00:43:07 Come right here. 784 00:43:03 --> 00:43:09 You think you can make it to the ceiling? 785 00:43:06 --> 00:43:12 It's only a very light Ping-Pong ball. 786 00:43:08 --> 00:43:14 So, you go like this, blow as hard as you can. 787 00:43:12 --> 00:43:18 STUDENT: Okay. 788 00:43:13 --> 00:43:19 LEWIN: Try it, don't be nervous. 789 00:43:15 --> 00:43:21 STUDENT: All right. 790 00:43:16 --> 00:43:22 LEWIN: Straight up. 791 00:43:18 --> 00:43:24 STUDENT: No... 792 00:43:19 --> 00:43:25 LEWIN: Blow as hard as you can-- get it out. 793 00:43:21 --> 00:43:27 Amazing! Do it again. 794 00:43:23 --> 00:43:29 Come on, there must have been something wrong. 795 00:43:25 --> 00:43:31 (class laughs ) 796 00:43:26 --> 00:43:32 LEWIN: You're not sick today, are you? 797 00:43:29 --> 00:43:35 Blow. 798 00:43:30 --> 00:43:36 Harder! 799 00:43:32 --> 00:43:38 STUDENT: Is this a trick? 800 00:43:33 --> 00:43:39 LEWIN: No, there's nothing, there's no trick in here. 801 00:43:35 --> 00:43:41 I mean, my goodness-- 802 00:43:36 --> 00:43:42 this is a Ping-Pong ball, I'm not a magician. 803 00:43:38 --> 00:43:44 (class laughs ) 804 00:43:39 --> 00:43:45 LEWIN: Come on, blow it up! 805 00:43:42 --> 00:43:48 Hey, it doesn't work. 806 00:43:44 --> 00:43:50 It's amazing. 807 00:43:45 --> 00:43:51 Why don't you sit down? 808 00:43:47 --> 00:43:53 (class laughs ) 809 00:43:50 --> 00:43:56 LEWIN: Why doesn't it work? 810 00:43:52 --> 00:43:58 Why doesn't it work? 811 00:43:53 --> 00:43:59 The harder you blow, the least it will work. 812 00:43:57 --> 00:44:03 Air is flowing here... 813 00:44:02 --> 00:44:08 and right here, where there is very little room, 814 00:44:05 --> 00:44:11 the air will have very high speed, 815 00:44:08 --> 00:44:14 way higher than it has where it has lots of room. 816 00:44:11 --> 00:44:17 And so at the highest speed, you get the lowest pressure. 817 00:44:16 --> 00:44:22 And so the Ping-Pong ball is sucked in 818 00:44:19 --> 00:44:25 while you're blowing it. 819 00:44:21 --> 00:44:27 And to give you the conclusive proof of that 820 00:44:24 --> 00:44:30 I will do it this way. 821 00:44:26 --> 00:44:32 822 00:44:29 --> 00:44:35 I will put the Ping-Pong ball like so, 823 00:44:33 --> 00:44:39 and I'm going to blow like this, and if I blow hard enough, 824 00:44:36 --> 00:44:42 the Ping-Pong ball will stay in there 825 00:44:39 --> 00:44:45 because I generate a lower pressure right here 826 00:44:43 --> 00:44:49 where the passage is the smallest, 827 00:44:45 --> 00:44:51 but I have to blow quite hard. 828 00:44:47 --> 00:44:53 (inhales deeply, blowing hard ) 829 00:44:51 --> 00:44:57 You see that? Isn't that amazing? 830 00:44:53 --> 00:44:59 That's the reason why she couldn't get it up. 831 00:44:56 --> 00:45:02 (inhales deeply, blowing hard ) 832 00:45:01 --> 00:45:07 That's what Bernoulli does for you. 833 00:45:03 --> 00:45:09 Not so intuitive, is it? 834 00:45:04 --> 00:45:10 835 00:45:07 --> 00:45:13 I have here an air flow, a hose with air coming out, 836 00:45:13 --> 00:45:19 and I can show you there 837 00:45:14 --> 00:45:20 something that is equally nonintuitive. 838 00:45:17 --> 00:45:23 839 00:45:21 --> 00:45:27 Let's start the air flow. 840 00:45:24 --> 00:45:30 (air hissing ) 841 00:45:25 --> 00:45:31 It's coming out. 842 00:45:26 --> 00:45:32 843 00:45:29 --> 00:45:35 I take a Ping-Pong ball. 844 00:45:31 --> 00:45:37 845 00:45:34 --> 00:45:40 It stays there. 846 00:45:38 --> 00:45:44 Is that due to Mr. Bernoulli? No. 847 00:45:41 --> 00:45:47 No, that's more complicated physics, 848 00:45:44 --> 00:45:50 because it has to do with turbulence. 849 00:45:46 --> 00:45:52 It has to do with vortices, which is very difficult. 850 00:45:49 --> 00:45:55 What is happening here 851 00:45:51 --> 00:45:57 is that as the air flows, you get turbulence above here 852 00:45:54 --> 00:46:00 and the turbulence creates a lower pressure. 853 00:45:59 --> 00:46:05 So the vortices, which are the turbulence, are keeping this up, 854 00:46:02 --> 00:46:08 because there's a lower pressure here and there. 855 00:46:05 --> 00:46:11 But why is it so stable? 856 00:46:08 --> 00:46:14 I can see that I have... 857 00:46:10 --> 00:46:16 because of this turbulence, that it's held up. 858 00:46:13 --> 00:46:19 Why is it so stable? 859 00:46:14 --> 00:46:20 If I give it a little push 860 00:46:15 --> 00:46:21 it doesn't... it's sucked back in again. 861 00:46:20 --> 00:46:26 It's very stable-- that is Bernoulli. 862 00:46:22 --> 00:46:28 Because if I blow air, like so... 863 00:46:28 --> 00:46:34 864 00:46:32 --> 00:46:38 then the velocity here is the highest, 865 00:46:35 --> 00:46:41 because it's diverging the air as it's coming out, 866 00:46:38 --> 00:46:44 but in the center, it is the highest, 867 00:46:40 --> 00:46:46 and so when this Ping-Pong ball goes to this side, 868 00:46:43 --> 00:46:49 it clearly has a lower pressure here than there 869 00:46:46 --> 00:46:52 and so it's being sucked back in again. 870 00:46:48 --> 00:46:54 So the stability is due to Bernoulli, 871 00:46:50 --> 00:46:56 but the fact that it is held up is more difficult physics. 872 00:46:54 --> 00:47:00 It is so stable that I can even tilt this... 873 00:46:57 --> 00:47:03 874 00:47:01 --> 00:47:07 and it will still stay there. 875 00:47:04 --> 00:47:10 876 00:47:06 --> 00:47:12 Now I have something 877 00:47:07 --> 00:47:13 that I want you to show your parents on Thanksgiving. 878 00:47:11 --> 00:47:17 It's a little present for them, 879 00:47:14 --> 00:47:20 and that is something that you can very easily do at home. 880 00:47:19 --> 00:47:25 You take a glass and you fill it with cranberry juice-- 881 00:47:24 --> 00:47:30 not all the way, up to here. 882 00:47:30 --> 00:47:36 Take a thin piece of cardboard, 883 00:47:33 --> 00:47:39 the kind of stuff that you have on the back of pads. 884 00:47:36 --> 00:47:42 You put it on top. 885 00:47:37 --> 00:47:43 The table is beautifully set-- turkey, everything is there-- 886 00:47:41 --> 00:47:47 and you suggest to your parents that you turn this over. 887 00:47:45 --> 00:47:51 Your mother will scream bloody murder, 888 00:47:47 --> 00:47:53 because she would think 889 00:47:49 --> 00:47:55 that the cranberry juice will fall out. 890 00:47:51 --> 00:47:57 In fact, itmay actually fall out. 891 00:47:53 --> 00:47:59 I can't guarantee you that it won't. 892 00:47:56 --> 00:48:02 (class laughs ) 893 00:47:57 --> 00:48:03 894 00:47:59 --> 00:48:05 LEWIN: But it may not, in which case 895 00:48:02 --> 00:48:08 you now have all the tools to explain that. 896 00:48:06 --> 00:48:12 897 00:48:11 --> 00:48:17 Please do invite me to your Thanksgiving dinner 898 00:48:14 --> 00:48:20 and I'll show it to your parents. 899 00:48:15 --> 00:48:21 900 00:48:17 --> 00:48:23