1 00:00:01 --> 00:00:04 The following content is provided by MIT OpenCourseWare 2 00:00:04 --> 00:00:06 under a Creative Commons license. 3 00:00:06 --> 00:00:10 Additional information about our license and MIT 4 00:00:10 --> 00:00:15 OpenCourseWare in general is available at ocw.mit.edu. 5 00:00:15 --> 00:00:21 Last time we were talking about the general interactions that 6 00:00:21 --> 00:00:25 are present in a chemical bond. And we were, 7 00:00:25 --> 00:00:29 in particular, looking at the energy of 8 00:00:29 --> 00:00:34 interaction, here, as we brought two hydrogen 9 00:00:34 --> 00:00:40 atoms together. We were looking at that energy 10 00:00:40 --> 00:00:48 of interaction as a function of the distance r between these two 11 00:00:48 --> 00:00:51 nuclei. And we saw, of course, 12 00:00:51 --> 00:00:56 way out here, that the energy of interaction 13 00:00:56 --> 00:01:02 was minus 2,624 kilojoules per mole. 14 00:01:02 --> 00:01:06 As we brought the two hydrogen atoms in closer together, 15 00:01:06 --> 00:01:08 that interaction energy went down. 16 00:01:08 --> 00:01:12 It became a maximum negative value at some r. 17 00:01:12 --> 00:01:15 That r is the equilibrium bond length. 18 00:01:15 --> 00:01:19 And then, as you try to push the two nuclei closer together, 19 00:01:19 --> 00:01:24 the energy of interaction goes up again, so far up that when 20 00:01:24 --> 00:01:28 you get them really close, the energy of interaction is 21 00:01:28 --> 00:01:34 greater than that of the two separated hydrogen atoms. 22 00:01:34 --> 00:01:37 And so, in this region, the hydrogen atoms are no 23 00:01:37 --> 00:01:41 longer bound. Wherever this energy is lower 24 00:01:41 --> 00:01:45 than that of the separated hydrogen atom limit you have a 25 00:01:45 --> 00:01:49 bound molecule. This was the attractive part of 26 00:01:49 --> 00:01:52 the potential. This was the well depth or the 27 00:01:52 --> 00:01:56 bond association energy, measured from here to here. 28 00:01:56 --> 00:02:01 That is how much energy you would have to put in to pull the 29 00:02:01 --> 00:02:08 two hydrogens apart. This is the repulsive region of 30 00:02:08 --> 00:02:15 that interaction potential. We were talking about how that 31 00:02:15 --> 00:02:22 curve, that energy, was really the sum of three 32 00:02:22 --> 00:02:27 components. That energy of interaction was 33 00:02:27 --> 00:02:34 the sum of the nuclear-nuclear repulsion. 34 00:02:34 --> 00:02:40 That is, the repulsion between the nucleus of this hydrogen and 35 00:02:40 --> 00:02:45 the nucleus of that hydrogen. In addition to that 36 00:02:45 --> 00:02:50 nuclear-nuclear repulsion, there is the electron-nuclear 37 00:02:50 --> 00:02:53 attraction. The electron-nuclear 38 00:02:53 --> 00:02:59 attraction, between the electron on the original nucleus and, 39 00:02:59 --> 00:03:03 when the two hydrogens get close enough, 40 00:03:03 --> 00:03:10 the electron attraction between the other nucleus. 41 00:03:10 --> 00:03:14 And then, finally, there is the electron-electron 42 00:03:14 --> 00:03:17 repulsion. When these two hydrogen atoms 43 00:03:17 --> 00:03:21 come so close, the electrons now are going to 44 00:03:21 --> 00:03:24 repel. And so, this curve is actually 45 00:03:24 --> 00:03:29 the sum of those three contributions. 46 00:03:29 --> 00:03:34 And what we were trying to do last time is to look at the 47 00:03:34 --> 00:03:37 dependence of these interactions, 48 00:03:37 --> 00:03:39 individually, on r. 49 00:03:39 --> 00:03:45 And then we wanted to sum them up to see why we actually have 50 00:03:45 --> 00:03:51 the shape of this interaction potential that we do. 51 00:03:51 --> 00:03:54 We are trying to decompose this. 52 00:03:54 --> 00:03:59 We are trying to understand over what regions of r, 53 00:03:59 --> 00:04:06 which one of these interaction energies is dominant. 54 00:04:06 --> 00:04:10 That is what we are doing. And I think last time we 55 00:04:10 --> 00:04:16 started in the sense that we recognized what the r dependence 56 00:04:16 --> 00:04:19 was for the nuclear-nuclear repulsion. 57 00:04:19 --> 00:04:25 The nuclear-nuclear repulsion is just the Coulomb interaction 58 00:04:25 --> 00:04:30 energy between two like positive charges. 59 00:04:30 --> 00:04:35 That nuclear-nuclear repulsion was e squared over 4 pi epsilon 60 00:04:35 --> 00:04:40 nought times r. 61 00:04:40 --> 00:04:44 And so that component I could easily draw. 62 00:04:44 --> 00:04:47 And I did draw it last time, I think. 63 00:04:47 --> 00:04:51 This is one over r dependence. 64 00:04:51 --> 00:04:57 This is the e squared over 4 pi epsilon nought r. 65 00:04:57 --> 00:05:00 66 00:05:00 --> 00:05:05 67 00:05:05 --> 00:05:11 That was one of them. Now, next, these two terms are 68 00:05:11 --> 00:05:17 what I am going to call the electron interactions because 69 00:05:17 --> 00:05:21 both of them involve the electron. 70 00:05:21 --> 00:05:28 This one did not. This was just the nucleus. 71 00:05:28 --> 00:05:33 It turns out that I don't have a nice simple way to tell you 72 00:05:33 --> 00:05:37 what the r dependence between the nuclei will be for the 73 00:05:37 --> 00:05:42 electron-nuclear attraction, nor do I have a nice simple way 74 00:05:42 --> 00:05:47 to figure out what the r dependence will be for the 75 00:05:47 --> 00:05:51 electron-electron repulsion. I cannot do that without 76 00:05:51 --> 00:05:55 actually solving the Schrödinger equation. 77 00:05:55 --> 00:06:00 I don't have a simple way to break that down. 78 00:06:00 --> 00:06:08 However, what I can do is I can estimate what the sum of these 79 00:06:08 --> 00:06:14 electron interactions are at two extremes. 80 00:06:14 --> 00:06:19 Is this noisy? Can you hear me? 81 00:06:19 --> 00:06:24 I can see why it is noisy. 82 00:06:24 --> 00:06:43 83 00:06:43 --> 00:06:46 I do know what it is at two extremes. 84 00:06:46 --> 00:06:51 I know what those sums of those interactions are for very large 85 00:06:51 --> 00:06:55 r, and I know what it is for r equals 0. 86 00:06:55 --> 00:07:00 What I am going to do is calculate it for r equals 87 00:07:00 --> 00:07:05 infinity and r equals 0. And I am going to then put it 88 00:07:05 --> 00:07:09 on this plot. And then to just estimate what 89 00:07:09 --> 00:07:13 the r dependence is, I am going to draw a line from 90 00:07:13 --> 00:07:18 that point to that point. That is the best I can do. 91 00:07:18 --> 00:07:20 Let's do that. 92 00:07:20 --> 00:07:27 93 00:07:27 --> 00:07:33 Let me start with this energy of interaction at r equals 94 00:07:33 --> 00:07:37 infinity. I want to evaluate what the 95 00:07:37 --> 00:07:42 repulsive interaction is between the electrons at r equals 96 00:07:42 --> 00:07:45 infinity. What is that interaction 97 00:07:45 --> 00:07:47 energy? It is zero because the 98 00:07:47 --> 00:07:53 electrons are so far apart at r equals infinity that there is no 99 00:07:53 --> 00:07:56 interaction energy. It is the repulsive 100 00:07:56 --> 00:08:00 interaction. It is this kind of interaction, 101 00:08:00 --> 00:08:05 r equals infinity. That is going to be zero. 102 00:08:05 --> 00:08:10 But now this term, this electron-nuclear 103 00:08:10 --> 00:08:14 attraction. When the two hydrogen atoms 104 00:08:14 --> 00:08:20 here are very far apart, what is the energy of the 105 00:08:20 --> 00:08:24 electron-nuclear attraction there? 106 00:08:24 --> 00:08:30 I cannot hear you, so I will tell you. 107 00:08:30 --> 00:08:34 It is the binding energy of a 1s electron. 108 00:08:34 --> 00:08:38 I mean that is the energy of interaction. 109 00:08:38 --> 00:08:42 When r is very large, when r is infinity, 110 00:08:42 --> 00:08:47 the energy of interaction is just the 1s binding energy of 111 00:08:47 --> 00:08:51 the electron to each of its nuclei. 112 00:08:51 --> 00:08:56 The energy of interaction, the electron-nuclear attraction 113 00:08:56 --> 00:09:02 is just E sub 1s for this one. 114 00:09:02 --> 00:09:05 And e sub 1s for that one. 115 00:09:05 --> 00:09:09 In a hydrogen atom that is what it is. 116 00:09:09 --> 00:09:12 It is the electron-nuclear attraction. 117 00:09:12 --> 00:09:17 And so, right here, this is equal to 2 times E sub 118 00:09:17 --> 00:09:20 1s. 119 00:09:20 --> 00:09:30 120 00:09:30 --> 00:09:36 Now, you know that E sub 1s is equal to minus 121 00:09:36 --> 00:09:41 2.18x10^-18 joules, but in kilojoules per mole, 122 00:09:41 --> 00:09:47 that is equal to minus 1 kilojoules per mole. 123 00:09:47 --> 00:09:54 And, if we have two of them, as we do, 2 times E sub 1s 124 00:09:54 --> 00:09:59 is minus 2 kilojoules per mole. 125 00:09:59 --> 00:10:08 I calculated what the electron 126 00:10:08 --> 00:10:14 interaction energy is at r is equal to infinity. 127 00:10:14 --> 00:10:21 That is way out here. This is hydrogen plus hydrogen. 128 00:10:21 --> 00:10:28 This is minus 2,624, the same number I got over 129 00:10:28 --> 00:10:33 there. Now, what we have to do -- 130 00:10:33 --> 00:10:42 131 00:10:42 --> 00:10:47 -- is calculate what that energy of interaction is at r is 132 00:10:47 --> 00:10:50 equal to 0. When r is equal to 0, 133 00:10:50 --> 00:10:55 we have two hydrogen atoms right on top of each other. 134 00:10:55 --> 00:11:02 We have two hydrogen nuclei right on top of each other. 135 00:11:02 --> 00:11:06 That means, in our kind of thought experiment here, 136 00:11:06 --> 00:11:10 that the charge on the nucleus is Z equals 2. 137 00:11:10 --> 00:11:15 That means when the two hydrogen atoms are right on top 138 00:11:15 --> 00:11:18 of each other, it looks like we have a helium 139 00:11:18 --> 00:11:22 nucleus. And there is electron number 140 00:11:22 --> 00:11:26 one around it and electron number two around it. 141 00:11:26 --> 00:11:32 That looks like a helium atom. What is the total electron 142 00:11:32 --> 00:11:36 interaction in the case of a helium atom? 143 00:11:36 --> 00:11:41 What is the total energy of interaction there? 144 00:11:41 --> 00:11:47 Well, the total energy of interaction is going to be minus 145 00:11:47 --> 00:11:53 the first ionization energy, this is going to be the energy 146 00:11:53 --> 00:12:00 of interaction of the helium, for a helium atom. 147 00:12:00 --> 00:12:05 Because minus the first ionization energy of the helium 148 00:12:05 --> 00:12:12 atom is the binding energy of the first electron to the helium 149 00:12:12 --> 00:12:18 plus minus the second ionization energy of the helium atom. 150 00:12:18 --> 00:12:22 In other words, if I hid this one away, 151 00:12:22 --> 00:12:27 then the electron-nuclear attraction between the helium 152 00:12:27 --> 00:12:33 nucleus in electron two is just minus the second ionization 153 00:12:33 --> 00:12:39 energy of helium. Does that make sense? 154 00:12:39 --> 00:12:44 155 00:12:44 --> 00:12:47 You are too hot to think. Okay. 156 00:12:47 --> 00:12:52 That is what that is. And if you look them up, 157 00:12:52 --> 00:12:59 the total energy of interaction is minus 7,622 kilojoules per 158 00:12:59 --> 00:13:01 mole. 159 00:13:01 --> 00:13:06 160 00:13:06 --> 00:13:10 I can plot that on this graph at r equals 0. 161 00:13:10 --> 00:13:15 I have minus 7,622 kilojoules. Now, I have two points. 162 00:13:15 --> 00:13:20 I have a point over here and a point over there. 163 00:13:20 --> 00:13:25 I am going to draw a straight line between the two. 164 00:13:25 --> 00:13:31 To get my total energy of interaction, I am going to add 165 00:13:31 --> 00:13:37 this curve to that curve. And when I do that, 166 00:13:37 --> 00:13:44 we are going to get something that looks like that. 167 00:13:44 --> 00:13:52 The bottom line is that this shape here is determined by the 168 00:13:52 --> 00:13:58 competition between the electron interactions, 169 00:13:58 --> 00:14:05 which are always attractive. They are always negative. 170 00:14:05 --> 00:14:09 The electron interactions are actually the sum of an 171 00:14:09 --> 00:14:14 attractive term and a repulsive term, but the repulsive term is 172 00:14:14 --> 00:14:18 not so repulsive as to overcome the attractive term. 173 00:14:18 --> 00:14:22 It is always negative. Overall, the sum is still 174 00:14:22 --> 00:14:25 attractive. The electron interactions are 175 00:14:25 --> 00:14:28 attractive. This particular curve is the 176 00:14:28 --> 00:14:32 competition between the electron interactions, 177 00:14:32 --> 00:14:36 those attractive interactions and the nuclear interactions, 178 00:14:36 --> 00:14:41 which are repulsive. In other words, 179 00:14:41 --> 00:14:45 you have to get the two hydrogen atoms close enough in 180 00:14:45 --> 00:14:50 order for the attractive interactions to take hold. 181 00:14:50 --> 00:14:55 But you cannot get them so close because if you get them 182 00:14:55 --> 00:15:00 too close, the nuclear-nuclear repulsions set in. 183 00:15:00 --> 00:15:05 Where your chemical bond length is, is determined by that 184 00:15:05 --> 00:15:11 competition between the electron attractive interactions and 185 00:15:11 --> 00:15:14 those nuclear-nuclear repulsions. 186 00:15:14 --> 00:15:18 That is what determines the bond length. 187 00:15:18 --> 00:15:23 That is fundamentally, here, what determines the bond 188 00:15:23 --> 00:15:29 strength, the competition between these overall attractive 189 00:15:29 --> 00:15:33 interactions due to the electrons and the 190 00:15:33 --> 00:15:39 nuclear-nuclear repulsion. That was the concept, 191 00:15:39 --> 00:15:44 really, that I wanted to get across here, those fundamental 192 00:15:44 --> 00:15:49 interactions that make up this kind of curve. 193 00:15:49 --> 00:15:53 You are going to see this curve a lot. 194 00:15:53 --> 00:15:58 All chemical bonds have this kind of dependence on r, 195 00:15:58 --> 00:16:05 energy of interaction on r. There is one other point I want 196 00:16:05 --> 00:16:09 to make. That is that what we often and 197 00:16:09 --> 00:16:14 usually do is we reset our zero of energy. 198 00:16:14 --> 00:16:19 Another words, we are going to reset our zero 199 00:16:19 --> 00:16:24 of energy, here, so that the zero of energy 200 00:16:24 --> 00:16:30 corresponds to the separated atom limit. 201 00:16:30 --> 00:16:35 Why do we do that? Well, because this energy 202 00:16:35 --> 00:16:41 difference, the minus 2,624, was really the attractive 203 00:16:41 --> 00:16:47 interaction between the electron and its nucleus. 204 00:16:47 --> 00:16:54 It did not have anything to do with the attraction or repulsion 205 00:16:54 --> 00:17:00 between the two atoms. And so, when we want to talk 206 00:17:00 --> 00:17:05 only about the chemical bond and the energy changes when we make 207 00:17:05 --> 00:17:09 a chemical bond, it is often useful to shift our 208 00:17:09 --> 00:17:13 zero of energy down, so that the separated atom 209 00:17:13 --> 00:17:18 limit is our zero of energy. And now, everything that is 210 00:17:18 --> 00:17:22 negative relative to that is a bound interaction. 211 00:17:22 --> 00:17:26 When it gets too close, it will be a positive 212 00:17:26 --> 00:17:31 interaction and the atoms are no longer bound. 213 00:17:31 --> 00:17:36 I mean, we are not forgetting about this energy here. 214 00:17:36 --> 00:17:40 We know if you are calculating the total energy, 215 00:17:40 --> 00:17:45 it has to be there, but oftentimes we just want to 216 00:17:45 --> 00:17:51 talk about the relative changes of the energy of interaction as 217 00:17:51 --> 00:17:56 a function of r when we are concerned only with forming a 218 00:17:56 --> 00:17:58 bond. Make sense? 219 00:17:58 --> 00:18:03 Okay. That is the general phenomenon. 220 00:18:03 --> 00:18:22 221 00:18:22 --> 00:18:31 Now, what I want to talk about is one very simple model for an 222 00:18:31 --> 00:18:36 ionic bond. This is a classical model. 223 00:18:36 --> 00:18:42 And the amazing thing about it is that this simple classical 224 00:18:42 --> 00:18:50 model does give us insight into the mechanism by which this bond 225 00:18:50 --> 00:18:54 is formed. It is a mechanism that is only 226 00:18:54 --> 00:19:01 going to work when you form a very ionic bond. 227 00:19:01 --> 00:19:05 This is particular for a very ionic bond. 228 00:19:05 --> 00:19:12 We want to take a look at this mechanism because it is going to 229 00:19:12 --> 00:19:19 give us some insight into how the bond is actually formed. 230 00:19:19 --> 00:19:25 We are going to look at the formation of sodium chloride, 231 00:19:25 --> 00:19:30 here. We have a sodium atom and a 232 00:19:30 --> 00:19:35 chlorine atom, and they are coming together, 233 00:19:35 --> 00:19:42 moving toward each other. What happens is that at a 234 00:19:42 --> 00:19:47 certain distance from each other, the sodium atom, 235 00:19:47 --> 00:19:51 believe it or not, actually ejects an electron. 236 00:19:51 --> 00:19:55 And that electron hooks onto the chlorine. 237 00:19:55 --> 00:20:00 When it does that, of course the chlorine now 238 00:20:00 --> 00:20:05 becomes bigger than the sodium, but now we have two charges 239 00:20:05 --> 00:20:10 separated. A positive and a negative ion. 240 00:20:10 --> 00:20:17 And there is a large attractive interaction between those two. 241 00:20:17 --> 00:20:23 What happens is these two ions are attracted in to each other. 242 00:20:23 --> 00:20:28 They are just roped right in. It is called the Harpoon 243 00:20:28 --> 00:20:32 Mechanism. Why does the sodium and the 244 00:20:32 --> 00:20:36 chlorine just pull right into each other? 245 00:20:36 --> 00:20:41 Well, because of that rope. That rope is that Coulomb 246 00:20:41 --> 00:20:44 interaction. This really happens. 247 00:20:44 --> 00:20:49 At some distance the sodium atom ejects that electron, 248 00:20:49 --> 00:20:54 and then that sodium just pulls that chlorine right into it 249 00:20:54 --> 00:20:59 until it gets close enough to form a chemical bond, 250 00:20:59 --> 00:21:03 -- and you have sodium chloride. 251 00:21:03 --> 00:21:08 This is a reaction mechanism that was elucidated many years 252 00:21:08 --> 00:21:11 ago, called the harpoon mechanicism. 253 00:21:11 --> 00:21:15 It is a mechanics elucidated by Dudley Herschbach, 254 00:21:15 --> 00:21:19 who is here at Harvard in the Chemistry Department, 255 00:21:19 --> 00:21:22 who has since retired. John Polanyi, 256 00:21:22 --> 00:21:25 who is at Toronto, and Yuan Lee, 257 00:21:25 --> 00:21:30 who was at Berkeley, for most of his career. 258 00:21:30 --> 00:21:34 They received the Nobel Prize for this discovery of this 259 00:21:34 --> 00:21:40 mechanism, and many other kinds of mechanism and dynamics of 260 00:21:40 --> 00:21:43 chemical reactions. Yuan Lee right here, 261 00:21:43 --> 00:21:46 this gentleman was actually my Ph.D. 262 00:21:46 --> 00:21:50 thesis supervisor at Berkeley. 263 00:21:50 --> 00:22:00 264 00:22:00 --> 00:22:04 This is a simple picture, and this is exactly what is 265 00:22:04 --> 00:22:08 going on. This seems a little strange to 266 00:22:08 --> 00:22:14 you, so let's try to understand exactly how this is working. 267 00:22:14 --> 00:22:19 To understand this, what we are going to have to do 268 00:22:19 --> 00:22:22 is look at the energetics of the system. 269 00:22:22 --> 00:22:27 And now I am going to raise this screen here, 270 00:22:27 --> 00:22:31 I think. No, I don't want to. 271 00:22:31 --> 00:22:32 I am going to raise it a little bit. 272 00:22:32 --> 00:22:33 How is that? 273 00:22:33 --> 00:23:00 274 00:23:00 --> 00:23:04 All right. What we are seeing is this gas 275 00:23:04 --> 00:23:10 phase sodium atom ejecting an electron to form this gas phase 276 00:23:10 --> 00:23:15 sodium ion, plus this electron. And of course, 277 00:23:15 --> 00:23:21 that is going to cost energy. The energy change is the 278 00:23:21 --> 00:23:25 ionization energy, which for sodium is 279 00:23:25 --> 00:23:31 kilojoules per mole. But, at the same time, 280 00:23:31 --> 00:23:35 that electron is being caught by the chlorine. 281 00:23:35 --> 00:23:40 And when a chlorine and an electron recombine to form the 282 00:23:40 --> 00:23:45 Cl minus gas phase, there is an energy 283 00:23:45 --> 00:23:49 release, as we saw. That energy release is minus 284 00:23:49 --> 00:23:52 the electron affinity of chlorine. 285 00:23:52 --> 00:23:56 That is equal to minus kilojoules per mole. 286 00:23:56 --> 00:24:02 Overall, going from a gas phase 287 00:24:02 --> 00:24:08 sodium atom plus a gas phase chlorine atom 288 00:24:08 --> 00:24:13 to a gas phase sodium ion and a gas phase 289 00:24:13 --> 00:24:19 chlorine ion, the overall energy change here, 290 00:24:19 --> 00:24:24 which is now the ionization energy minus the electron 291 00:24:24 --> 00:24:29 affinity, that overal energy change is 147 kilojoules per 292 00:24:29 --> 00:24:33 mole. Although we get some energy 293 00:24:33 --> 00:24:38 back when that electron attaches to the chlorine, 294 00:24:38 --> 00:24:44 we don't get enough energy back to compensate for having to pull 295 00:24:44 --> 00:24:49 the electron off of the sodium. Right now, this still looks 296 00:24:49 --> 00:24:53 like an overall endothermic reaction. 297 00:24:53 --> 00:25:00 We have to put 147 kilojoules into the system to make it go. 298 00:25:00 --> 00:25:05 It is beginning to seem a little peculiar. 299 00:25:05 --> 00:25:11 How does this work? Well, we have to remember that 300 00:25:11 --> 00:25:17 once we make that sodium plus and the chlorine minus, 301 00:25:17 --> 00:25:23 that there is that Coulomb interaction. 302 00:25:23 --> 00:25:28 The Coulomb interaction, bringing the sodium ion plus 303 00:25:28 --> 00:25:33 the chlorine ion together to make the sodium chloride, 304 00:25:33 --> 00:25:37 that delta E, 305 00:25:37 --> 00:25:41 if I take two ions, sodium and chlorine, 306 00:25:41 --> 00:25:46 in from infinity and bring them together at the bond length, 307 00:25:46 --> 00:25:51 that energy change is minus kilojoules per mole. 308 00:25:51 --> 00:25:57 If I add up all three reactions to get sodium gas plus chlorine 309 00:25:57 --> 00:26:03 gas to make sodium chloride in the gas phase, 310 00:26:03 --> 00:26:08 the overall energy change there 311 00:26:08 --> 00:26:13 is minus 445 kilojoules per mole. 312 00:26:13 --> 00:26:17 And, of course, the reaction is downhill. 313 00:26:17 --> 00:26:23 But that still doesn't give you a really good feeling for what 314 00:26:23 --> 00:26:28 is really going on here. To do that, let's look at an 315 00:26:28 --> 00:26:33 energy level diagram. You want to kill the front 316 00:26:33 --> 00:26:36 lights. This is going to be back and 317 00:26:36 --> 00:26:38 forth here. All right. 318 00:26:38 --> 00:26:42 What have I draw here? I have drawn the energy of 319 00:26:42 --> 00:26:47 interaction between a sodium atom and a chlorine atom, 320 00:26:47 --> 00:26:53 just like I did for hydrogen. I said all chemical bonds have 321 00:26:53 --> 00:26:56 this same shape of energy of interaction. 322 00:26:56 --> 00:27:01 Here is the bond length. 2.36 angstroms. 323 00:27:01 --> 00:27:06 Here is the well depth or the dissociation energy. 324 00:27:06 --> 00:27:11 In this case, I show it measured from here to 325 00:27:11 --> 00:27:14 there. It is minus delta E sub d, 326 00:27:14 --> 00:27:16 minus 445. 327 00:27:16 --> 00:27:22 Here I set the zero of energy at the separated atom limit, 328 00:27:22 --> 00:27:28 sodium plus chlorine. When sodium and chlorine are 329 00:27:28 --> 00:27:31 way out here, when r is really large, 330 00:27:31 --> 00:27:37 we saw that it is going to take 147 kilojoules to make a sodium 331 00:27:37 --> 00:27:41 ion from sodium and a chlorine ion from chlorine. 332 00:27:41 --> 00:27:45 That is what I calculated, right here. 333 00:27:45 --> 00:27:50 If the two are far apart, if you pull an electron off a 334 00:27:50 --> 00:27:55 sodium and put it onto chlorine, it is still going to require 335 00:27:55 --> 00:28:03 energy, 147 kilojoules per mole. However, I also said that when 336 00:28:03 --> 00:28:08 the sodium and the chlorine come close enough, 337 00:28:08 --> 00:28:15 the ions are pulled in close enough such that they can form a 338 00:28:15 --> 00:28:20 chemical bond, the energy you get back is 339 00:28:20 --> 00:28:24 kilojoules per mole. On this diagram, 340 00:28:24 --> 00:28:30 where is that? Well, that is this energy. 341 00:28:30 --> 00:28:36 From up here to down there is 592 kilojoules per mole. 342 00:28:36 --> 00:28:42 Where did I get that number, 592 kilojoules per mole? 343 00:28:42 --> 00:28:50 Well, I calculated it using the Coulomb potential energy of 344 00:28:50 --> 00:28:57 interaction, which I am calling, here, U of r sub E 345 00:28:57 --> 00:29:03 at this value of r. The Coulomb potential energy of 346 00:29:03 --> 00:29:07 interaction is right here for a point charge. 347 00:29:07 --> 00:29:12 If you treat the sodium as a plus one charge and you treat 348 00:29:12 --> 00:29:15 the chlorine as a minus one charge. 349 00:29:15 --> 00:29:19 All of a sudden, we are forgetting everything 350 00:29:19 --> 00:29:24 about the other electrons. We are just treating sodium ion 351 00:29:24 --> 00:29:29 and chlorine ion as two point charges. 352 00:29:29 --> 00:29:34 If you forget completely about the other electrons and just 353 00:29:34 --> 00:29:40 treat them as point charges, that is the interaction energy 354 00:29:40 --> 00:29:44 right here. That 592 comes from taking that 355 00:29:44 --> 00:29:48 expression and plugging in 2.36 angstroms. 356 00:29:48 --> 00:29:51 That is how much energy you get back. 357 00:29:51 --> 00:29:55 Now we understand the energies a little bit, 358 00:29:55 --> 00:30:01 but we still don't understand exactly how this electron jump 359 00:30:01 --> 00:30:07 process is happening. Because the way I have it 360 00:30:07 --> 00:30:13 drawn, here, it still looks like we have an electron jumping from 361 00:30:13 --> 00:30:19 sodium to chlorine way out here. And we have to put in 362 00:30:19 --> 00:30:23 kilojoules before we get any energy back. 363 00:30:23 --> 00:30:28 Well, that is not the case. And that is not the case 364 00:30:28 --> 00:30:32 because of this. This blue curve, 365 00:30:32 --> 00:30:36 here, is just the Coulomb energy of interaction. 366 00:30:36 --> 00:30:40 We evaluated that point, that number, 367 00:30:40 --> 00:30:43 from here to here using this expression. 368 00:30:43 --> 00:30:48 But you know that this is a minus one over r 369 00:30:48 --> 00:30:52 dependence. If you are way up here and you 370 00:30:52 --> 00:30:57 treat this as a zero of energy for a plus charge and a minus 371 00:30:57 --> 00:31:03 charge, one over r kind of looks like this. 372 00:31:03 --> 00:31:09 That is the blue curve. But you also notice that right 373 00:31:09 --> 00:31:17 here, you see that that Coulomb interaction is intersecting with 374 00:31:17 --> 00:31:24 this interaction potential between a neutral sodium atom 375 00:31:24 --> 00:31:31 and a neutral chlorine atom, right in there. 376 00:31:31 --> 00:31:37 Right at this value of r, which we are going to call r 377 00:31:37 --> 00:31:44 star, the potential energy of interaction from here to here is 378 00:31:44 --> 00:31:50 equal to the sum of this ionization energy minus the 379 00:31:50 --> 00:31:55 electron affinity. Right here, the electron can 380 00:31:55 --> 00:32:03 jump without having to put any energy into the system. 381 00:32:03 --> 00:32:09 You are close enough for the electron to jump because that 382 00:32:09 --> 00:32:15 Coulomb interaction has gotten lower, and it is right at that 383 00:32:15 --> 00:32:21 point when you can have that electron transfer and not have 384 00:32:21 --> 00:32:26 to put any energy into the system to get it to go. 385 00:32:26 --> 00:32:31 In other words, right here, the energy from 386 00:32:31 --> 00:32:37 right there to this point is minus e squared 4 pi epsilon 387 00:32:37 --> 00:32:44 nought r star. 388 00:32:44 --> 00:32:49 That energy right at that point is equal to, if I am measuring 389 00:32:49 --> 00:32:53 here from the top minus the quantity ionization energy of 390 00:32:53 --> 00:32:58 sodium minus the electron affinity of chlorine. 391 00:32:58 --> 00:33:02 In order to solve for this 392 00:33:02 --> 00:33:07 distance r at which the electron jumps, for which that electron 393 00:33:07 --> 00:33:13 jump is energetically allowed, I am going to set this equal to 394 00:33:13 --> 00:33:16 this. I know what the ionization 395 00:33:16 --> 00:33:21 energy and the electron affinity of sodium and chlorine are. 396 00:33:21 --> 00:33:27 I know everything except r star, so I am going to solve 397 00:33:27 --> 00:33:30 for r star. Let's do that. 398 00:33:30 --> 00:33:33 I am going to need the lights, here. 399 00:33:33 --> 00:33:40 400 00:33:40 --> 00:33:45 If I rearrange that equation, r star is equal to e squared 401 00:33:45 --> 00:33:50 over 4 pi epsilon nought times the ionization energy of sodium 402 00:33:50 --> 00:33:53 minus the electron affinity of chlorine. 403 00:33:53 --> 00:33:58 I know 404 00:33:58 --> 00:34:04 what e star is. It is 1.602x10^-19 Coulomb's 405 00:34:04 --> 00:34:08 squared. I have a 4 pi epsilon nought. 406 00:34:08 --> 00:34:14 I know what epsilon nought is. And then, the difference 407 00:34:14 --> 00:34:21 between the ionization energy and the electron affinity I 408 00:34:21 --> 00:34:27 calculated over there. That is 147 kilojoules per mole 409 00:34:27 --> 00:34:35 or 1.47x10^5 joules per mole. But now, and this is what 410 00:34:35 --> 00:34:42 everybody forgets on an exam, I have to calculate r star per 411 00:34:42 --> 00:34:49 molecule, not per mole because per mole does not make sense. 412 00:34:49 --> 00:34:54 And I have this energy written here per mole, 413 00:34:54 --> 00:35:03 so I need an Avogadro's number up here, 6.022x10^23 per mole. 414 00:35:03 --> 00:35:11 Don't forget Avogadro's number when you calculate r. 415 00:35:11 --> 00:35:18 What is r star? Well, it comes out to be 416 00:35:18 --> 00:35:26 9.45x10^-10 meters. Let's get a perspective on 417 00:35:26 --> 00:35:34 these distances. The sodium atom diameter is 3.8 418 00:35:34 --> 00:35:39 angstroms. Chlorine atom diameter, 419 00:35:39 --> 00:35:45 2 angstroms. What I am saying is that this 420 00:35:45 --> 00:35:51 electron can jump, or does jump from sodium to 421 00:35:51 --> 00:35:59 chlorine at this distance r star, which is equal to 9.45 422 00:35:59 --> 00:36:04 angstroms. So, the sodium and the chlorine 423 00:36:04 --> 00:36:09 really are a considerable distance apart when that 424 00:36:09 --> 00:36:12 electron jumps. But that electron can jump 425 00:36:12 --> 00:36:18 because it is at that point that the Coulomb interaction is large 426 00:36:18 --> 00:36:24 enough here to compensate for the difference in the ionization 427 00:36:24 --> 00:36:27 energy and the electron affinity. 428 00:36:27 --> 00:36:31 And this actual number, here, was verified in these 429 00:36:31 --> 00:36:36 experiments by Herschbach and Lee. 430 00:36:36 --> 00:36:41 It actually does happen. And this very simple classical 431 00:36:41 --> 00:36:46 model, where we are actually treating the sodium and the 432 00:36:46 --> 00:36:51 chlorine as point charges, we have forgotten everything 433 00:36:51 --> 00:36:55 else about the electrons, that works remarkably well. 434 00:36:55 --> 00:37:01 Now, what this model does not give you very well is the bond 435 00:37:01 --> 00:37:06 energy. Because, if you look at this 436 00:37:06 --> 00:37:12 diagram again right in here, let me go back on here, 437 00:37:12 --> 00:37:17 this 147 kilojoules here, that I can look up. 438 00:37:17 --> 00:37:22 This 592 kilojoules, that is just the Coulomb 439 00:37:22 --> 00:37:29 interaction between a positive and a negative charge at 2.36 440 00:37:29 --> 00:37:32 eV. That is all that is. 441 00:37:32 --> 00:37:36 You can calculate that. And so, therefore, 442 00:37:36 --> 00:37:41 if I want to calculate the bond energy of sodium chloride, 443 00:37:41 --> 00:37:46 the bond energy is just the difference between this energy 444 00:37:46 --> 00:37:50 and that energy, and that is 435 kilojoules per 445 00:37:50 --> 00:37:53 mole. Well, that does not come out so 446 00:37:53 --> 00:37:57 well in terms of the actual bond energy. 447 00:37:57 --> 00:38:03 The actual bond energy is kilojoules per mole. 448 00:38:03 --> 00:38:07 And we know why that did not come out too well. 449 00:38:07 --> 00:38:14 That is because this depends on all of the interactions that are 450 00:38:14 --> 00:38:20 much closer into the nucleus. By the time you get down here, 451 00:38:20 --> 00:38:24 the repulsive interactions are present. 452 00:38:24 --> 00:38:30 The nuclear-nuclear repulsions are present. 453 00:38:30 --> 00:38:34 And, in our simple model, we did not take that into 454 00:38:34 --> 00:38:37 account, the nuclear-nuclear repulsions. 455 00:38:37 --> 00:38:42 This simple model worked to get r star because r star is further 456 00:38:42 --> 00:38:45 out. The nuclear-nuclear repulsions 457 00:38:45 --> 00:38:49 have not really set in yet. Therefore, the simple model 458 00:38:49 --> 00:38:54 works when you are at a far distance, when r is large. 459 00:38:54 --> 00:39:00 But to get the bond strength, here, you are much closer in. 460 00:39:00 --> 00:39:04 You are at 2.36 angstroms. That is the difference in 461 00:39:04 --> 00:39:08 energy from here to there. We forgot about the repulsive 462 00:39:08 --> 00:39:13 interactions between the two nuclei, so the model is not 463 00:39:13 --> 00:39:18 going to work so close to the nucleus, but it does a really 464 00:39:18 --> 00:39:22 good job of getting r star far away from the nucleus. 465 00:39:22 --> 00:39:27 Again, this simple model only works for very ionic compounds, 466 00:39:27 --> 00:39:32 very ionic bonds like sodium chloride. 467 00:39:32 --> 00:39:39 It won't work very well for hydrogen chloride, 468 00:39:39 --> 00:39:43 for example. Questions on that? 469 00:39:43 --> 00:39:45 Yes? 470 00:39:45 --> 00:39:55 471 00:39:55 --> 00:39:59 We are going to deal with entropy and Gibbs free energy 472 00:39:59 --> 00:40:03 changes in a week or two. Right now, what I am writing 473 00:40:03 --> 00:40:07 here are energy changes. I am actually dealing with 474 00:40:07 --> 00:40:10 single molecules. I might have, 475 00:40:10 --> 00:40:13 in my mind, here, energies per mole. 476 00:40:13 --> 00:40:18 But what I am thinking about is not an ensemble of molecules. 477 00:40:18 --> 00:40:23 I am actually thinking about what is happening in each 478 00:40:23 --> 00:40:28 individual single molecule interaction. 479 00:40:28 --> 00:40:33 That is why I have not talked about delta G here at all. 480 00:40:33 --> 00:40:38 And, in the field of chemical dynamics, that is where we want 481 00:40:38 --> 00:40:44 to look at individual events as opposed to a Boltzmann average 482 00:40:44 --> 00:40:48 of events. That is what I am talking about 483 00:40:48 --> 00:40:53 right here, but we are going to talk about collections of 484 00:40:53 --> 00:40:58 molecules and the energy changes. 485 00:40:58 --> 00:41:05 I am going to change my definition from delta E to delta 486 00:41:05 --> 00:41:11 H, the bond enthalpy, in a couple of days or so. 487 00:41:11 --> 00:41:14 Other questions? Okay. 488 00:41:14 --> 00:41:22 Well, there is one other just rather brief topic that I wanted 489 00:41:22 --> 00:41:27 to talk about. That is, measuring dipole 490 00:41:27 --> 00:41:32 moments. And then, from the dipole 491 00:41:32 --> 00:41:37 moments, getting out some ionic character to a chemical bond. 492 00:41:37 --> 00:41:41 Your book actually calls ionic bonds polar covalent bonds. 493 00:41:41 --> 00:41:46 And that is fine because even a very ionic bond like sodium 494 00:41:46 --> 00:41:51 chloride is not completely ionic, in the sense that when it 495 00:41:51 --> 00:41:56 is the molecule you know that it is not a point charge on sodium 496 00:41:56 --> 00:42:02 and a point charge on chlorine. You have an electron 497 00:42:02 --> 00:42:06 distribution when you are that close. 498 00:42:06 --> 00:42:13 And so, what you have in an ionic bond or a polar covalent 499 00:42:13 --> 00:42:18 bond, here, is an asymmetric charge distribution. 500 00:42:18 --> 00:42:23 In HCl, here, you have both electrons, 501 00:42:23 --> 00:42:28 on the average, being closer to the chlorine 502 00:42:28 --> 00:42:34 nucleus than to the hydrogen nucleus. 503 00:42:34 --> 00:42:39 And you have that because you have a bond between atoms with 504 00:42:39 --> 00:42:42 two very different electronegativities. 505 00:42:42 --> 00:42:45 So, that is a polar covalent bond. 506 00:42:45 --> 00:42:51 Now, what we are going to do is we are going to use this symbol 507 00:42:51 --> 00:42:56 delta here as a measure of the amount of electron transfer. 508 00:42:56 --> 00:43:01 Delta is the fraction of a full charge that is asymmetrically 509 00:43:01 --> 00:43:05 distributed. This plus delta, 510 00:43:05 --> 00:43:09 this delta that was on the hydrogen, is now on the 511 00:43:09 --> 00:43:12 chlorine. That is the interpretation of 512 00:43:12 --> 00:43:15 that symbol. That asymmetric charge 513 00:43:15 --> 00:43:20 distribution leads to a dipole moment, which is defined as q, 514 00:43:20 --> 00:43:25 where q is the magnitude of the charge separation, 515 00:43:25 --> 00:43:28 times r, where r is that charge separation. 516 00:43:28 --> 00:43:34 It is, strictly speaking, 517 00:43:34 --> 00:43:39 a vector. Q times R is what we define as 518 00:43:39 --> 00:43:44 a dipole moment. The units of dipole moment is 519 00:43:44 --> 00:43:49 Coulombs times meters. You can see that from Q times 520 00:43:49 --> 00:43:52 R. A dipole moment is also a 521 00:43:52 --> 00:43:57 vector. I have the vector on this slide 522 00:43:57 --> 00:44:03 going from the positively charged end to the negatively 523 00:44:03 --> 00:44:07 charged end. That is the way your present 524 00:44:07 --> 00:44:09 book does it. In your notes, 525 00:44:09 --> 00:44:12 I have it reversed. I have it reversed because the 526 00:44:12 --> 00:44:16 last time I taught this, I was using a book that used a 527 00:44:16 --> 00:44:20 different notation and I sent it out for Xeroxing before I 528 00:44:20 --> 00:44:23 noticed it was different. So, change it around. 529 00:44:23 --> 00:44:26 Not that it is every going to make any difference, 530 00:44:26 --> 00:44:29 but your book has this convention from positive to 531 00:44:29 --> 00:44:31 negative. 532 00:44:31 --> 00:44:37 533 00:44:37 --> 00:44:40 This unit, though, of a Coulomb meter, 534 00:44:40 --> 00:44:44 is a very large unit, an inconvenient unit, 535 00:44:44 --> 00:44:48 so we have another unit. It is called the Debye, 536 00:44:48 --> 00:44:53 named after Peter Debye who first studied these polar 537 00:44:53 --> 00:44:56 covalent molecules. And a Debye, 538 00:44:56 --> 00:45:00 here, is defined as the following. 539 00:45:00 --> 00:45:05 It is defined as if you have a full unit charge, 540 00:45:05 --> 00:45:09 not a delta, moved from here to here, 541 00:45:09 --> 00:45:15 and the charge is separated by 0.208 angstroms, 542 00:45:15 --> 00:45:20 that defines this unit called the Debye. 543 00:45:20 --> 00:45:26 So, there are 0.208 angstroms per Debye. 544 00:45:26 --> 00:45:31 545 00:45:31 --> 00:45:36 If you knew the fraction of charge that is separated and you 546 00:45:36 --> 00:45:41 knew the bond length in angstroms, and then you have our 547 00:45:41 --> 00:45:46 definition for a Debye, which is 0.208 angstroms per 548 00:45:46 --> 00:45:51 Debye, you could calculate the dipole moment in Debye. 549 00:45:51 --> 00:45:57 Usually what we do is not to calculate the dipole moment. 550 00:45:57 --> 00:46:02 We usually measure the dipole moment and calculate the partial 551 00:46:02 --> 00:46:08 charge distribution. Because we usually don't know 552 00:46:08 --> 00:46:10 this. We can measure that. 553 00:46:10 --> 00:46:14 We can measure the dipole moments in kind of a capacitor 554 00:46:14 --> 00:46:18 arrangement, where we have some molecules that have a dipole 555 00:46:18 --> 00:46:23 moment, a positive charge on one plate, a negative charge on the 556 00:46:23 --> 00:46:25 other. And, when you do that, 557 00:46:25 --> 00:46:30 of course, these electric dipoles are going to align. 558 00:46:30 --> 00:46:32 That is going to change the capacitance. 559 00:46:32 --> 00:46:36 If this capacitor is part of a resonant circuit, 560 00:46:36 --> 00:46:39 it is going to change the resonant frequent. 561 00:46:39 --> 00:46:43 The resonant frequency is related to the dipole moment. 562 00:46:43 --> 00:46:46 And, in that way, you calculate or measure the 563 00:46:46 --> 00:46:49 dipole moment. That is how it was originally 564 00:46:49 --> 00:46:52 done. However, you can now measure 565 00:46:52 --> 00:46:56 dipole moments very accurately by rotational spectroscopy. 566 00:46:56 --> 00:47:02 And we are going to look at that in a few lectures or so. 567 00:47:02 --> 00:47:05 But take HCl right here. Here is HCl. 568 00:47:05 --> 00:47:10 Here is the measured dipole moment, and here is the bond 569 00:47:10 --> 00:47:13 length. We can use these two pieces of 570 00:47:13 --> 00:47:19 information to calculate the fraction of charge distributed. 571 00:47:19 --> 00:47:23 And, in the case of HCl, that is about 0.18. 572 00:47:23 --> 00:47:28 Sometimes, we refer to this in a percentage. 573 00:47:28 --> 00:47:32 So, this would be 18% of a charge separation. 574 00:47:32 --> 00:47:36 Sometimes we say 18% ionic character in HCl. 575 00:47:36 --> 00:47:43 That compares to something like 70% or 80% in sodium chloride or 576 00:47:43 --> 00:47:48 lithium chloride. So, HCl is not anywhere near as 577 00:47:48 --> 00:47:51 ionic. The charge distribution is not 578 00:47:51 --> 00:47:59 as asymmetric as it is in sodium chloride or lithium chloride. 579 00:47:59 --> 00:48:03 Thank you very much for hanging in here today. 580 00:48:03 --> 00:48:07 It has been hot. Have a nice cool weekend. 581 00:48:07.875 --> 48:10 See you next Wednesday.