1 00:00:00,000 --> 00:00:00,660 2 00:00:00,660 --> 00:00:03,220 Let's say I have a balloon. 3 00:00:03,220 --> 00:00:05,250 And in that balloon I have a bunch of 4 00:00:05,250 --> 00:00:07,439 particles bouncing around. 5 00:00:07,440 --> 00:00:10,710 They're gas particles, so they're floating freely. 6 00:00:10,710 --> 00:00:17,660 And they each have some velocity, some kinetic energy. 7 00:00:17,660 --> 00:00:23,910 And what I care about, let me just draw a few more, what I 8 00:00:23,910 --> 00:00:27,559 care about is the pressure that is exerted on the surface 9 00:00:27,559 --> 00:00:28,139 of the balloon. 10 00:00:28,140 --> 00:00:29,960 So I care about the pressure. 11 00:00:29,960 --> 00:00:30,839 And what's pressure? 12 00:00:30,839 --> 00:00:32,365 It's force per area. 13 00:00:32,365 --> 00:00:36,219 14 00:00:36,219 --> 00:00:39,149 So the area here, you can think of it as the inside 15 00:00:39,149 --> 00:00:40,070 surface of the balloon. 16 00:00:40,070 --> 00:00:42,960 And what's going to apply force to that? 17 00:00:42,960 --> 00:00:46,329 Well any given moment-- I only drew six particles here, but 18 00:00:46,329 --> 00:00:50,849 in a real balloon you would have gazillions of particles, 19 00:00:50,850 --> 00:00:54,070 and we could talk about how large, but more particles than 20 00:00:54,070 --> 00:00:57,439 you can really probably imagine-- but at any given 21 00:00:57,439 --> 00:00:59,759 moment, some of those particles are bouncing off the 22 00:00:59,759 --> 00:01:01,929 wall of the container. 23 00:01:01,929 --> 00:01:03,820 That particle is bouncing there, this particle is 24 00:01:03,820 --> 00:01:06,909 bouncing there, this guy's bouncing like that. 25 00:01:06,909 --> 00:01:10,899 And when they bounce, they apply force to the container. 26 00:01:10,900 --> 00:01:14,850 An outward force, that's what keeps the balloon blown up. 27 00:01:14,849 --> 00:01:16,969 So think about what the pressure is going to be 28 00:01:16,969 --> 00:01:18,679 dependent on. 29 00:01:18,680 --> 00:01:22,470 So first of all, the faster these particles move, the 30 00:01:22,469 --> 00:01:23,719 higher the pressure. 31 00:01:23,719 --> 00:01:31,750 32 00:01:31,750 --> 00:01:34,319 Slower particles, you're going to be bouncing into the 33 00:01:34,319 --> 00:01:37,479 container less, and when you do bounce into the container, 34 00:01:37,480 --> 00:01:40,070 it's going to be less of a ricochet, or less of a change 35 00:01:40,069 --> 00:01:41,109 in momentum. 36 00:01:41,109 --> 00:01:45,840 So slower particles, you're going to 37 00:01:45,840 --> 00:01:47,549 have pressure go down. 38 00:01:47,549 --> 00:01:50,689 Now, it's practically impossible to measure the 39 00:01:50,689 --> 00:01:53,799 kinetic energy, or the velocity, or the direction of 40 00:01:53,799 --> 00:01:55,060 each individual particle. 41 00:01:55,060 --> 00:01:56,490 Especially when you have gazillions 42 00:01:56,489 --> 00:01:57,629 of them in a balloon. 43 00:01:57,629 --> 00:02:00,079 So we do is we think of the average 44 00:02:00,079 --> 00:02:01,609 energy of the particles. 45 00:02:01,609 --> 00:02:04,599 And the average energy of the particles, you might say oh, 46 00:02:04,599 --> 00:02:08,299 Sal is about to introduce us to a new concept. 47 00:02:08,300 --> 00:02:11,050 It's a new way of looking at probably a very familiar 48 00:02:11,050 --> 00:02:12,070 concept to you. 49 00:02:12,069 --> 00:02:14,409 And that's temperature. 50 00:02:14,409 --> 00:02:18,639 Temperature can and should be viewed as the average energy 51 00:02:18,639 --> 00:02:20,639 of the particles in the system. 52 00:02:20,639 --> 00:02:23,219 So I'll put a little squiggly line, because there's a lot of 53 00:02:23,219 --> 00:02:24,109 ways to think about it. 54 00:02:24,110 --> 00:02:25,615 Average energy. 55 00:02:25,615 --> 00:02:28,430 56 00:02:28,430 --> 00:02:31,020 And mostly kinetic energy, because these particles are 57 00:02:31,020 --> 00:02:32,140 moving and bouncing. 58 00:02:32,139 --> 00:02:35,689 The higher the temperature, the faster that these 59 00:02:35,689 --> 00:02:36,819 particles move. 60 00:02:36,819 --> 00:02:40,849 And the more that they're going to bounce into the side 61 00:02:40,849 --> 00:02:41,609 of the container. 62 00:02:41,610 --> 00:02:44,540 But temperature is average energy. 63 00:02:44,539 --> 00:02:49,644 It tells us energy per particle. 64 00:02:49,645 --> 00:02:52,909 65 00:02:52,909 --> 00:02:57,449 So obviously, if we only had one particle in there with 66 00:02:57,449 --> 00:03:00,169 super high temperature, that's going to have less pressure 67 00:03:00,169 --> 00:03:02,619 than if we have a million particles in there. 68 00:03:02,620 --> 00:03:05,430 Let me draw that. 69 00:03:05,430 --> 00:03:12,110 If I have, let's take two cases right here. 70 00:03:12,110 --> 00:03:16,990 One is, I have a bunch of particles with a certain 71 00:03:16,990 --> 00:03:22,020 temperature, moving in their different directions. 72 00:03:22,020 --> 00:03:25,120 And the other example, I have one particle. 73 00:03:25,120 --> 00:03:27,319 And maybe they have the same temperature. 74 00:03:27,319 --> 00:03:29,689 That on average, they have the same kinetic energy. 75 00:03:29,689 --> 00:03:32,449 The kinetic energy per particle is the same. 76 00:03:32,449 --> 00:03:35,939 Clearly, this one is going to be applying more pressure to 77 00:03:35,939 --> 00:03:38,129 its container, because at any given moment more of these 78 00:03:38,129 --> 00:03:40,750 particles are going to be bouncing off the side than in 79 00:03:40,750 --> 00:03:41,310 this example. 80 00:03:41,310 --> 00:03:43,199 This guy's going to bounce, bam, then going to go and 81 00:03:43,199 --> 00:03:44,119 move, bounce, bam. 82 00:03:44,120 --> 00:03:46,450 So he's going to be applying less pressure, even though his 83 00:03:46,449 --> 00:03:47,839 temperature might be the same. 84 00:03:47,840 --> 00:03:51,069 Because temperature is kinetic energy, or you can view it as 85 00:03:51,069 --> 00:03:53,019 kinetic energy per particles. 86 00:03:53,020 --> 00:03:55,780 Or it's a way of looking at kinetic energy per particle. 87 00:03:55,780 --> 00:03:59,250 So if we wanted to look at the total energy in the system, we 88 00:03:59,250 --> 00:04:04,259 would want to multiply the temperature times the number 89 00:04:04,259 --> 00:04:05,019 of particles. 90 00:04:05,020 --> 00:04:08,469 And just since we're dealing on the molecular scale, the 91 00:04:08,469 --> 00:04:11,090 number of particles can often be represented as moles. 92 00:04:11,090 --> 00:04:13,539 Remember, moles is just a number of particles. 93 00:04:13,539 --> 00:04:19,959 So we're saying that that pressure-- well, I'll say it's 94 00:04:19,959 --> 00:04:26,160 proportional, so it's equal to some constant, 95 00:04:26,160 --> 00:04:29,200 let's call that R. 96 00:04:29,199 --> 00:04:31,019 Because we've got to make all the units work out in the end. 97 00:04:31,019 --> 00:04:33,099 I mean temperature is in Kelvin but we eventually want 98 00:04:33,100 --> 00:04:34,470 to get back to joules. 99 00:04:34,470 --> 00:04:36,470 So let's just say it's equal to some constant, or it's 100 00:04:36,470 --> 00:04:41,790 proportional to temperature times the number of particles. 101 00:04:41,790 --> 00:04:43,270 And we can do that a bunch of ways. 102 00:04:43,269 --> 00:04:44,649 But let's think of that in moles. 103 00:04:44,649 --> 00:04:47,589 If I say there are 5 mole particles there, you know 104 00:04:47,589 --> 00:04:50,869 that's 5 times 6 times 10 to the 23 particles. 105 00:04:50,870 --> 00:04:52,639 So, this is the number of particles. 106 00:04:52,639 --> 00:04:55,370 107 00:04:55,370 --> 00:04:57,430 This is the temperature. 108 00:04:57,430 --> 00:04:58,680 And this is just some constant. 109 00:04:58,680 --> 00:05:02,829 110 00:05:02,829 --> 00:05:04,769 Now, what else is the pressure dependent on? 111 00:05:04,769 --> 00:05:06,319 We gave these two examples. 112 00:05:06,319 --> 00:05:08,290 Obviously, it is dependent on the temperature; the faster 113 00:05:08,290 --> 00:05:10,900 each of these particles move, the higher pressure we'll 114 00:05:10,899 --> 00:05:13,839 have. It's also dependent on the number of particles, the 115 00:05:13,839 --> 00:05:16,769 more particles we have, the more pressure we'll have. What 116 00:05:16,769 --> 00:05:18,689 about the size of the container? 117 00:05:18,689 --> 00:05:20,120 The volume of the container. 118 00:05:20,120 --> 00:05:23,540 If we took this example, but we shrunk the container 119 00:05:23,540 --> 00:05:26,040 somehow, maybe by pressing on the outside. 120 00:05:26,040 --> 00:05:29,870 So if this container looked like this, but we still had 121 00:05:29,870 --> 00:05:37,600 the same four particles in it, with the same average kinetic 122 00:05:37,600 --> 00:05:39,550 energy, or the same temperature. 123 00:05:39,550 --> 00:05:41,439 So the number of particles stays the same, the 124 00:05:41,439 --> 00:05:44,329 temperature is the same, but the volume has gone down. 125 00:05:44,329 --> 00:05:47,199 Now, these guys are going to bump into the sides of the 126 00:05:47,199 --> 00:05:50,680 container more frequently and there's less area. 127 00:05:50,680 --> 00:05:54,384 So at any given moment, you have more force and less area. 128 00:05:54,384 --> 00:05:56,180 So when you have more force and less area, your pressure 129 00:05:56,180 --> 00:05:57,720 is going to go up. 130 00:05:57,720 --> 00:06:03,910 So when the volume went down, your pressure went up. 131 00:06:03,910 --> 00:06:08,030 132 00:06:08,029 --> 00:06:10,559 So we could say that pressure is inversely 133 00:06:10,560 --> 00:06:12,939 proportional to volume. 134 00:06:12,939 --> 00:06:13,959 So let's think about that. 135 00:06:13,959 --> 00:06:15,189 Let's put that into our equation. 136 00:06:15,189 --> 00:06:22,879 We said that pressure is proportional-- and I'm just 137 00:06:22,879 --> 00:06:26,620 saying some proportionality constant, let's call that R, 138 00:06:26,620 --> 00:06:31,610 to the number of particles times the temperature, this 139 00:06:31,610 --> 00:06:32,660 gives us the total energy. 140 00:06:32,660 --> 00:06:36,750 And it's inversely proportional to the volume. 141 00:06:36,750 --> 00:06:39,920 And if we multiply both sides of this times the volume, we 142 00:06:39,920 --> 00:06:46,230 get the pressure times the volume is proportional to the 143 00:06:46,230 --> 00:06:49,040 number of particles times the temperature. 144 00:06:49,040 --> 00:06:51,350 So PV is equal to RnT. 145 00:06:51,350 --> 00:06:53,920 And just to switch this around a little bit, so it's in a 146 00:06:53,920 --> 00:06:56,395 form that you're more likely to see in your chemistry book, 147 00:06:56,394 --> 00:06:58,659 if we just switch the n and the R term. 148 00:06:58,660 --> 00:07:03,750 You get pressure times volume is equal to n, the number of 149 00:07:03,750 --> 00:07:08,470 particles you have, times some constant times temperature. 150 00:07:08,470 --> 00:07:14,480 And this right here is the ideal gas equation. 151 00:07:14,480 --> 00:07:15,965 Hopefully, it makes some sense to you. 152 00:07:15,964 --> 00:07:21,549 153 00:07:21,550 --> 00:07:25,689 When they say ideal gas, it's based on this little mental 154 00:07:25,689 --> 00:07:27,379 exercise I did to come up with this. 155 00:07:27,379 --> 00:07:30,529 I made some implicit assumptions when I did this. 156 00:07:30,529 --> 00:07:35,439 One is I assumed that we're dealing with an ideal gas. 157 00:07:35,439 --> 00:07:38,469 And so you say what, Sal, is an ideal gas? 158 00:07:38,470 --> 00:07:43,060 An ideal gas is one where the molecules are not too 159 00:07:43,060 --> 00:07:44,329 concerned with each other. 160 00:07:44,329 --> 00:07:46,740 They're just concerned with their own kinetic energy and 161 00:07:46,740 --> 00:07:47,980 bouncing off the wall. 162 00:07:47,980 --> 00:07:50,580 So they don't attract or repel each other. 163 00:07:50,579 --> 00:07:56,779 164 00:07:56,779 --> 00:07:59,119 Let's say they attracted each other, then as you increased 165 00:07:59,120 --> 00:08:01,490 the number of particles maybe they'd want to 166 00:08:01,490 --> 00:08:02,550 not go to the side. 167 00:08:02,550 --> 00:08:04,770 Maybe they'd all gravitate towards the center a little 168 00:08:04,769 --> 00:08:06,729 bit more if they did attract each other. 169 00:08:06,730 --> 00:08:08,730 And if they did that, they would bounce into the walls 170 00:08:08,730 --> 00:08:10,740 less and the pressure would be a little bit lower. 171 00:08:10,740 --> 00:08:11,935 So we're assuming that they don't attract 172 00:08:11,935 --> 00:08:13,709 or repel each other. 173 00:08:13,709 --> 00:08:17,979 And we're also assuming that the actual volume of the 174 00:08:17,980 --> 00:08:20,629 individual particles are inconsequential. 175 00:08:20,629 --> 00:08:22,209 Which is a pretty good assumption, because they're 176 00:08:22,209 --> 00:08:22,870 pretty small. 177 00:08:22,870 --> 00:08:28,850 Although, if you start putting a ton of particles into a 178 00:08:28,850 --> 00:08:31,210 certain volume, then at some point, especially if they're 179 00:08:31,209 --> 00:08:34,250 big molecules, it'll start to matter in terms of their size. 180 00:08:34,250 --> 00:08:37,840 But we're assuming for the purposes of our little mental 181 00:08:37,840 --> 00:08:43,190 exercise that the molecules have inconsequential volumes 182 00:08:43,190 --> 00:08:45,100 and they don't attract or repel each other. 183 00:08:45,100 --> 00:08:50,190 And in that situation, we can apply the ideal gas equation 184 00:08:50,190 --> 00:08:52,310 right here. 185 00:08:52,309 --> 00:08:54,359 Now, we've established the ideal gas equation. 186 00:08:54,360 --> 00:08:56,430 But you're like, well what's R, how do I deal with it, and 187 00:08:56,429 --> 00:08:59,179 how do I do math problems, and solve chemistry 188 00:08:59,179 --> 00:08:59,889 problems with it? 189 00:08:59,889 --> 00:09:01,230 And how do the units all work out? 190 00:09:01,230 --> 00:09:03,899 We'll do all of that in the next video where we'll solve a 191 00:09:03,899 --> 00:09:06,939 ton of equations, or a ton of exercises with 192 00:09:06,940 --> 00:09:08,350 the ideal gas equation. 193 00:09:08,350 --> 00:09:12,159 The important takeaway from this video is just to have the 194 00:09:12,159 --> 00:09:15,329 intuition as to why this actually does make sense. 195 00:09:15,330 --> 00:09:17,100 And frankly, once you have this intution, you should 196 00:09:17,100 --> 00:09:17,870 never forget it. 197 00:09:17,870 --> 00:09:21,560 You should be able to maybe even derive it on your own.