1 00:00:00,000 --> 00:00:00,660 2 00:00:00,660 --> 00:00:01,960 This is just a quick review of what we were 3 00:00:01,960 --> 00:00:03,050 doing in the last video. 4 00:00:03,050 --> 00:00:08,320 We had this oddly shaped pipe and the fluid coming in had 5 00:00:08,320 --> 00:00:09,780 input velocity V1. 6 00:00:09,780 --> 00:00:13,010 The pressure on the left-hand side pushing to the right is 7 00:00:13,010 --> 00:00:19,530 P1, and the area of this hole is A1. 8 00:00:19,530 --> 00:00:22,090 Everything that the same variables with the 2 on it is 9 00:00:22,090 --> 00:00:23,800 coming out of the pipe. 10 00:00:23,800 --> 00:00:27,500 What we just set up in that last video is we said by the 11 00:00:27,500 --> 00:00:33,280 law of conservation of energy, essentially the joules, the 12 00:00:33,280 --> 00:00:37,080 energy at this point in the system, or that we're putting 13 00:00:37,080 --> 00:00:39,570 into the system, has to be equal to the energy coming out 14 00:00:39,570 --> 00:00:41,650 of the system. 15 00:00:41,650 --> 00:00:44,360 We used that information to set up this big equation, but 16 00:00:44,360 --> 00:00:45,320 it's not too complicated. 17 00:00:45,320 --> 00:00:48,560 We figured out that the work going into the system was the 18 00:00:48,560 --> 00:00:52,730 input pressure times the mass of volume over some period of 19 00:00:52,730 --> 00:00:58,590 time divided by the density of whatever type of liquid we 20 00:00:58,590 --> 00:00:59,580 had, which was the potential energy. 21 00:00:59,580 --> 00:01:03,350 This is just typically mgh, where the mass is the mass of 22 00:01:03,350 --> 00:01:05,040 this column of fluid. 23 00:01:05,040 --> 00:01:08,530 We're saying, how much work was done over some 24 00:01:08,530 --> 00:01:10,550 period of time T? 25 00:01:10,550 --> 00:01:11,710 That's the way I would think about it. 26 00:01:11,710 --> 00:01:15,510 How much energy was there over some period of time T? 27 00:01:15,510 --> 00:01:17,920 The kinetic energy over that period of time would have been 28 00:01:17,920 --> 00:01:23,300 the mass of this volume of fluid times its velocity 29 00:01:23,300 --> 00:01:24,370 squared divided by 2. 30 00:01:24,370 --> 00:01:26,870 That's typical kinetic energy. 31 00:01:26,870 --> 00:01:29,510 Of course, that has to be equal to essentially the 32 00:01:29,510 --> 00:01:35,250 output energy, and so this is the output work, or how much 33 00:01:35,250 --> 00:01:40,060 work a column of water could do on the output side. 34 00:01:40,060 --> 00:01:43,110 It's an equivalent volume of water, remember that. 35 00:01:43,110 --> 00:01:45,840 In some period of time T, whatever volume of water this 36 00:01:45,840 --> 00:01:50,240 was, an equivalent volume of water-- maybe it'll be a 37 00:01:50,240 --> 00:01:53,505 longer cylinder now, because it's going to be going faster. 38 00:01:53,505 --> 00:01:56,040 39 00:01:56,040 --> 00:01:59,040 So on the output side, it's this longer cylinder that 40 00:01:59,040 --> 00:02:00,700 we're talking about, but it's going to be the same volume 41 00:02:00,700 --> 00:02:01,655 and the same mass. 42 00:02:01,655 --> 00:02:06,640 So what we say is that the work that this column can do 43 00:02:06,640 --> 00:02:10,650 in that same amount of time would be the output pressure 44 00:02:10,650 --> 00:02:13,556 times the mass of this column divided by the density of the 45 00:02:13,556 --> 00:02:15,690 column-- which is the same because the density of the 46 00:02:15,690 --> 00:02:19,230 liquid is the same throughout-- times the mass of 47 00:02:19,230 --> 00:02:22,820 this column, which is the same as the mass of this column 48 00:02:22,820 --> 00:02:26,890 because the volume and the density hasn't changed, so 49 00:02:26,890 --> 00:02:28,510 they're the same mass. 50 00:02:28,510 --> 00:02:30,960 Now, this column has more potential energy. 51 00:02:30,960 --> 00:02:35,060 It's up at h2, which I'm assuming is higher than h1. 52 00:02:35,060 --> 00:02:38,590 This kinetic energy is just the mass of this cylinder of 53 00:02:38,590 --> 00:02:41,780 fluid times its velocity squared, which is the output 54 00:02:41,780 --> 00:02:42,840 velocity divided by 2. 55 00:02:42,840 --> 00:02:48,770 This is potential energy out, and this is 56 00:02:48,770 --> 00:02:50,920 kinetic energy out. 57 00:02:50,920 --> 00:02:52,930 These equal each other. 58 00:02:52,930 --> 00:02:57,180 This setup is Bernoulli's equation, but let's see if we 59 00:02:57,180 --> 00:03:00,150 can clean it up so that we can get rid of variables that we 60 00:03:00,150 --> 00:03:02,020 don't have to know about. 61 00:03:02,020 --> 00:03:04,280 One thing that we see is that there's an m in every term, so 62 00:03:04,280 --> 00:03:04,990 let's get rid of them. 63 00:03:04,990 --> 00:03:06,860 Divide both sides of this equation by m. 64 00:03:06,860 --> 00:03:12,070 65 00:03:12,070 --> 00:03:13,320 We get that. 66 00:03:13,320 --> 00:03:15,940 67 00:03:15,940 --> 00:03:18,640 I don't like this density in the denominator here, so let's 68 00:03:18,640 --> 00:03:21,590 multiply both sides of this equation by density, and what 69 00:03:21,590 --> 00:03:24,800 we're left with is-- let me write this in a vibrant color. 70 00:03:24,800 --> 00:03:27,860 71 00:03:27,860 --> 00:03:32,470 P, the input pressure, plus-- and we're multiplying 72 00:03:32,470 --> 00:03:34,320 everything by this rho, this density. 73 00:03:34,320 --> 00:03:42,050 So we have input pressure plus rho g h1, the input height, 74 00:03:42,050 --> 00:03:49,760 the initial height, plus rho v squared over 2. 75 00:03:49,760 --> 00:03:54,920 76 00:03:54,920 --> 00:03:58,290 This is rho v squared over 2, and that equals-- we 77 00:03:58,290 --> 00:04:05,600 multiplied both sides by rho, so we get the input velocity, 78 00:04:05,600 --> 00:04:10,990 so that equals the pressure out plus the density times 79 00:04:10,990 --> 00:04:13,260 gravity times the output height. 80 00:04:13,260 --> 00:04:16,019 81 00:04:16,019 --> 00:04:16,935 Let's make everything consistent. 82 00:04:16,935 --> 00:04:20,144 I wrote 2's here, so let's just say this is pressure 2, 83 00:04:20,144 --> 00:04:26,880 this is height 2, plus rho times the velocity squared. 84 00:04:26,880 --> 00:04:30,100 85 00:04:30,100 --> 00:04:34,180 This is Bernoulli's equation, and it has all sorts of what I 86 00:04:34,180 --> 00:04:37,230 would say is fairly neat repercussions. 87 00:04:37,230 --> 00:04:41,790 For example, let's assume that the height stays constant, so 88 00:04:41,790 --> 00:04:44,070 we can ignore these middle terms. If the height is 89 00:04:44,070 --> 00:04:50,770 constant, if I have a higher velocity and this whole term 90 00:04:50,770 --> 00:04:54,810 is constant, then my pressure is going to be lower. 91 00:04:54,810 --> 00:04:59,490 Think about it: If height is constant, this doesn't change, 92 00:04:59,490 --> 00:05:02,520 but if this velocity increases, but this whole 93 00:05:02,520 --> 00:05:05,360 thing is constant, pressure has to decrease. 94 00:05:05,360 --> 00:05:09,400 Similarly, if pressure increases, then velocity is 95 00:05:09,400 --> 00:05:10,430 going to decrease. 96 00:05:10,430 --> 00:05:12,360 That might be a little unintuitive, but the other 97 00:05:12,360 --> 00:05:13,270 way, it makes a lot of sense. 98 00:05:13,270 --> 00:05:16,840 When velocity increases, this pressure is going to decrease, 99 00:05:16,840 --> 00:05:20,050 and that's actually what makes planes fly and all sorts of 100 00:05:20,050 --> 00:05:21,330 neat things happen, but we'll get more 101 00:05:21,330 --> 00:05:22,550 into that in a second. 102 00:05:22,550 --> 00:05:25,920 Let's see if we can use Bernoulli's equation to do 103 00:05:25,920 --> 00:05:26,790 something useful. 104 00:05:26,790 --> 00:05:28,740 You should memorize this, and it shouldn't 105 00:05:28,740 --> 00:05:30,710 be too hard to memorize. 106 00:05:30,710 --> 00:05:33,140 It's pressure, and then you have this potential energy 107 00:05:33,140 --> 00:05:35,370 term, but instead of mass, you have density. 108 00:05:35,370 --> 00:05:37,160 You have this kinetic energy term. 109 00:05:37,160 --> 00:05:38,410 It's not kinetic energy anymore, because we 110 00:05:38,410 --> 00:05:40,180 manipulated it some, but instead of 111 00:05:40,180 --> 00:05:43,290 mass, you have density. 112 00:05:43,290 --> 00:05:45,070 With that said, let's do a problem. 113 00:05:45,070 --> 00:05:47,170 I'll keep this down here, since you probably haven't 114 00:05:47,170 --> 00:05:50,680 memorized it as yet. 115 00:05:50,680 --> 00:05:53,076 Let me erase everything else. 116 00:05:53,076 --> 00:05:55,930 That's not how I wanted to erase it. 117 00:05:55,930 --> 00:05:59,070 118 00:05:59,070 --> 00:06:00,900 That's how I wanted to erase it. 119 00:06:00,900 --> 00:06:04,960 I wanted to erase it like that without getting rid of 120 00:06:04,960 --> 00:06:06,155 anything useful. 121 00:06:06,155 --> 00:06:07,940 OK, that's good enough. 122 00:06:07,940 --> 00:06:10,464 And then let me clean up. 123 00:06:10,464 --> 00:06:12,568 Clean up all this stuff. 124 00:06:12,568 --> 00:06:17,580 125 00:06:17,580 --> 00:06:20,300 Let's say that I have a cup. 126 00:06:20,300 --> 00:06:26,330 127 00:06:26,330 --> 00:06:28,100 I'll just draw a cup. 128 00:06:28,100 --> 00:06:31,715 It's easier to draw sometimes then to draw straight lines 129 00:06:31,715 --> 00:06:32,680 and all of that. 130 00:06:32,680 --> 00:06:34,170 No, that's too dark. 131 00:06:34,170 --> 00:06:35,420 Do purple. 132 00:06:35,420 --> 00:06:37,280 133 00:06:37,280 --> 00:06:39,120 I'm using a super-wide tool. 134 00:06:39,120 --> 00:06:40,440 I have to switch the length. 135 00:06:40,440 --> 00:06:41,410 OK, so that's my cup. 136 00:06:41,410 --> 00:06:42,110 It has some fluid. 137 00:06:42,110 --> 00:06:47,870 Actually, let's say it has a top to it, and I have some 138 00:06:47,870 --> 00:06:50,090 fluid in it. 139 00:06:50,090 --> 00:06:51,910 Maybe it happens to be red. 140 00:06:51,910 --> 00:06:55,370 We haven't been dealing with red fluids as yet,. 141 00:06:55,370 --> 00:06:59,450 Let me-- oh, I didn't want to do that. 142 00:06:59,450 --> 00:07:01,980 So you know there's a fluid there. 143 00:07:01,980 --> 00:07:04,780 And let's say that there's no air here, so this is a vacuum. 144 00:07:04,780 --> 00:07:08,660 145 00:07:08,660 --> 00:07:12,840 Let's say that h-- we don't know what units are, but let's 146 00:07:12,840 --> 00:07:17,150 say h meters below the surface of the fluid. 147 00:07:17,150 --> 00:07:19,350 This is all fluid here. 148 00:07:19,350 --> 00:07:26,860 I poke a hole right there, and fluid starts spurting out. 149 00:07:26,860 --> 00:07:32,870 My question to you is, what is this output velocity of the 150 00:07:32,870 --> 00:07:36,120 fluid as a function of this height? 151 00:07:36,120 --> 00:07:37,000 Let me tell you something else. 152 00:07:37,000 --> 00:07:39,930 Let's say that this hole is so small, let's call the area of 153 00:07:39,930 --> 00:07:44,840 that hole A2, and let's say that the surface area of the 154 00:07:44,840 --> 00:07:47,600 water is A1. 155 00:07:47,600 --> 00:07:51,570 Let's say that hole is so small that the surface area 156 00:07:51,570 --> 00:07:59,560 the water-- let's say that A2 if equal to 1/1,000 of A1. 157 00:07:59,560 --> 00:08:02,270 This is a small hole relative to the surface 158 00:08:02,270 --> 00:08:05,340 area of this cup. 159 00:08:05,340 --> 00:08:07,790 With that said, let's see what we can do about figuring out 160 00:08:07,790 --> 00:08:09,430 the velocity coming out. 161 00:08:09,430 --> 00:08:12,030 Bernoulli's equation tells us that the input pressure plus 162 00:08:12,030 --> 00:08:14,700 the input potential energy plus the input kinetic energy 163 00:08:14,700 --> 00:08:16,100 is equal to the output, et cetera. 164 00:08:16,100 --> 00:08:18,960 165 00:08:18,960 --> 00:08:21,190 So what is the input pressure? 166 00:08:21,190 --> 00:08:24,690 Well, the input pressure, the pressure at this point, 167 00:08:24,690 --> 00:08:27,340 there's no air or no fluid above it, so the pressure at 168 00:08:27,340 --> 00:08:30,500 that point is zero. 169 00:08:30,500 --> 00:08:34,020 What is the input height? 170 00:08:34,020 --> 00:08:38,280 Let's just assume that the hole is done at height 0, h 171 00:08:38,280 --> 00:08:45,060 equals 0, so the input height h1 is just h. 172 00:08:45,060 --> 00:08:49,930 If this is 0, then this height right here is h. 173 00:08:49,930 --> 00:08:52,440 What is the input velocity? 174 00:08:52,440 --> 00:08:54,950 We know from the continuity equation, or whatever that 175 00:08:54,950 --> 00:09:00,580 thing was called, that the input velocity times the input 176 00:09:00,580 --> 00:09:04,030 area is equal to the output velocity 177 00:09:04,030 --> 00:09:05,330 times the output area. 178 00:09:05,330 --> 00:09:09,660 179 00:09:09,660 --> 00:09:15,360 We also know that the output area is equal to 1/1,000 of 180 00:09:15,360 --> 00:09:22,810 the input area-- and this is area 2-- so we know that the 181 00:09:22,810 --> 00:09:28,510 input velocity times area 1 is equal to the output velocity 182 00:09:28,510 --> 00:09:31,230 times 1/1,000 of area 1. 183 00:09:31,230 --> 00:09:36,590 We could say area 1 over 1,000 and divide both 184 00:09:36,590 --> 00:09:38,030 sides by area 1. 185 00:09:38,030 --> 00:09:42,170 We know that the input velocity is equal to V2 over 186 00:09:42,170 --> 00:09:46,290 1,000, so that's good to know. 187 00:09:46,290 --> 00:09:51,790 These are the three inputs into the left-hand side of 188 00:09:51,790 --> 00:09:53,570 Bernoulli's equation. 189 00:09:53,570 --> 00:09:57,150 What's on the right-hand side of Bernoulli's equation? 190 00:09:57,150 --> 00:09:58,400 What's P2? 191 00:09:58,400 --> 00:10:02,280 192 00:10:02,280 --> 00:10:04,850 What's the pressure at this point? 193 00:10:04,850 --> 00:10:05,820 Oh, I just ran out of time. 194 00:10:05,820 --> 00:10:08,290 I'll continue this into the next video. 195 00:10:08,290 --> 00:00:00,000