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 --> 00:00:19 Today is a very big day for all of you. 6 00:00:19 --> 00:00:24 Your first semester at MIT is half over. 7 00:00:24 --> 00:00:30 8 00:00:30 --> 00:00:35 And, in addition to that, you have a lot of challenges 9 00:00:35 --> 00:00:41 remaining ahead of you for the rest of this semester. 10 00:00:41 --> 00:00:47 I am going to help make the chemical challenges fun for you. 11 00:00:47 --> 00:00:52 That is what I am here to do. I love chemistry. 12 00:00:52 --> 00:00:57 I love teaching 5.112. This is the best part of my 13 00:00:57 --> 00:01:01 week. So, here we are. 14 00:01:01 --> 00:01:07 Do you guys know that chemistry can be incredibly fun? 15 00:01:07 --> 00:01:15 16 00:01:15 --> 00:01:19 Let me just show you how fun chemistry can be. 17 00:01:19 --> 00:01:26 18 00:01:26 --> 00:01:29 And that is just the gravy. The fun part is actually making 19 00:01:29 --> 00:01:34 the molecules. Any of you see this picture in 20 00:01:34 --> 00:01:37 U.S.A. Today recently? 21 00:01:37 --> 00:01:42 22 00:01:42 --> 00:01:44 Not reading that important journal, I see. 23 00:01:44 --> 00:01:48 Well, this picture did appear very recently in U.S.A. 24 00:01:48 --> 00:01:52 Today in a story that talked about the recent Nobel Prize in 25 00:01:52 --> 00:01:56 chemistry that was awarded to Professor Richard R. 26 00:01:56 --> 00:01:59 Schrock, of our department. And, in fact, 27 00:01:59 --> 00:02:03 I don't know if you realize this, but Professor Schrock was 28 00:02:03 --> 00:02:07 the first person ever awarded the Nobel Prize in Chemistry at 29 00:02:07 --> 00:02:10 MIT for work conducted while at MIT. 30 00:02:10 --> 00:02:13 That is a pretty amazing accomplishment because we have 31 00:02:13 --> 00:02:17 so many tremendous chemists on the faculty here, 32 00:02:17 --> 00:02:20 and he is the first one to break through in that manner. 33 00:02:20 --> 00:02:23 And maybe you are here at a very special time, 34 00:02:23 --> 00:02:29 and we will see a number more of these in the next few years. 35 00:02:29 --> 00:02:33 May with you contributing, so much the better because you 36 00:02:33 --> 00:02:35 are here. And let me just explain 37 00:02:35 --> 00:02:37 something, too. Chemistry is fun. 38 00:02:37 --> 00:02:41 And only on very rare occasions like this would Professor 39 00:02:41 --> 00:02:45 Schrock be drinking champagne at 8:30 in the morning, 40 00:02:45 --> 00:02:49 when this picture was taken. The Reuters reporter, 41 00:02:49 --> 00:02:53 Brian, who took this photo, is actually a pretty good 42 00:02:53 --> 00:02:57 friend of Professor Nocera here. And so he rode over from the 43 00:02:57 --> 00:03:01 Schrock household. And Dick and Dan came in 44 00:03:01 --> 00:03:04 together in the same car, as they often do, 45 00:03:04 --> 00:03:07 from Winchester on that morning, which was a very 46 00:03:07 --> 00:03:10 exciting day. If you come to see me for 47 00:03:10 --> 00:03:14 office hours maybe I will tell you more about it in detail, 48 00:03:14 --> 00:03:17 but it was an exciting day. And I am in here, 49 00:03:17 --> 00:03:19 too. My name is Kit Cummins. 50 00:03:19 --> 00:03:21 Kit is my nickname. My name is Christopher. 51 00:03:21 --> 00:03:25 You can call me Christopher or Kit, or you can call me 52 00:03:25 --> 00:03:28 Professor Cummins, or you can just say hey, 53 00:03:28 --> 00:03:32 chemistry guy. That will be fine. 54 00:03:32 --> 00:03:36 I am in this picture primarily because it is part of being in 55 00:03:36 --> 00:03:40 the right place at the right time, just like I am here now in 56 00:03:40 --> 00:03:43 front of you. But also I am in it because we 57 00:03:43 --> 00:03:47 three are three in one of the areas in our department that 58 00:03:47 --> 00:03:51 really focus our research on inorganic chemistry. 59 00:03:51 --> 00:03:53 And what is inorganic chemistry? 60 00:03:53 --> 00:03:58 I will say more about this during the semester. 61 00:03:58 --> 00:04:02 But inorganic chemistry is really the chemistry of the 62 00:04:02 --> 00:04:05 elements of the Periodic Table inclusively. 63 00:04:05 --> 00:04:09 So, a pretty broad topic. And I like doing chemistry with 64 00:04:09 --> 00:04:12 lots of elements. And so that is why these guys 65 00:04:12 --> 00:04:16 and I share an association with each other. 66 00:04:16 --> 00:04:19 And, in fact, I was a graduate student with 67 00:04:19 --> 00:04:21 Professor Schrock. And I am very, 68 00:04:21 --> 00:04:24 very proud to be able to say that. 69 00:04:24 --> 00:04:29 Hopefully, my computer will be staying on, here. 70 00:04:29 --> 00:04:32 And I want to point out, too, that people who love 71 00:04:32 --> 00:04:36 science want to know something about its history. 72 00:04:36 --> 00:04:40 And part of all of that is knowing the academic family from 73 00:04:40 --> 00:04:43 which you derive, depending on the person you've 74 00:04:43 --> 00:04:46 studied with in learning about chemistry. 75 00:04:46 --> 00:04:50 And I studied with Schrock. And Schrock studied with 76 00:04:50 --> 00:04:53 Osborn, a fantastic chemist in his own right, 77 00:04:53 --> 00:04:56 no longer alive, sadly, to see his progeny, 78 00:04:56 --> 00:05:01 Professor Schrock, win the Nobel Prize. 79 00:05:01 --> 00:05:04 And Osborn studied with Wilkinson, and Wilkinson was 80 00:05:04 --> 00:05:08 also a Nobel Prize winner. So, you do not have to go very 81 00:05:08 --> 00:05:11 far back in that lineage to encounter that recognition, 82 00:05:11 --> 00:05:14 the Nobel Prize, Schrock, and then it skipped 83 00:05:14 --> 00:05:18 Osborne, and if you go back to Wilkinson, there is another one. 84 00:05:18 --> 00:05:22 And you can keep going back. And I am not going to go 85 00:05:22 --> 00:05:26 through that whole history today because I have another history 86 00:05:26 --> 00:05:31 that I am going to need to go through with you today. 87 00:05:31 --> 00:05:40 And I am going to bring this back over so it does not 88 00:05:40 --> 00:05:48 distract you. And this other history that I 89 00:05:48 --> 00:05:57 need to impart to you today has to do with some of the 90 00:05:57 --> 00:06:06 contributions of Gilbert Newton Lewis. 91 00:06:06 --> 00:06:09 This is one of the most famous of all chemists ever. 92 00:06:09 --> 00:06:14 And if you like chemistry, I encourage you to think of the 93 00:06:14 --> 00:06:18 word Newton, as it is found engraved in one of the pillars 94 00:06:18 --> 00:06:23 in Killian Court at MIT as the middle name of Gilbert Newton 95 00:06:23 --> 00:06:26 Lewis. It is conceivable that having 96 00:06:26 --> 00:06:30 that middle name weighed heavily upon Gilbert during his 97 00:06:30 --> 00:06:34 lifetime. But it remains a good moniker. 98 00:06:34 --> 00:06:37 And in the future, when you have kids, 99 00:06:37 --> 00:06:41 I encourage you to consider using it as a middle name. 100 00:06:41 --> 00:06:43 It worked well in this particular case. 101 00:06:43 --> 00:06:48 When you get the notes for today, which incidentally will 102 00:06:48 --> 00:06:51 be available on the website after class today, 103 00:06:51 --> 00:06:56 so you don't need to write down everything I am writing down. 104 00:06:56 --> 00:07:00 You are actually going to get a little bit more in the online 105 00:07:00 --> 00:07:05 version than what I am writing down here. 106 00:07:05 --> 00:07:08 And if you find that you forgot something that I said during 107 00:07:08 --> 00:07:11 class, just email me. I will tell you what I said. 108 00:07:11 --> 00:07:14 It is not a problem. But if you want to write down 109 00:07:14 --> 00:07:17 notes while I am speaking just to make notes that you can refer 110 00:07:17 --> 00:07:20 to later to refresh your memory, that is fine. 111 00:07:20 --> 00:07:23 I think your taking in information in lots of different 112 00:07:23 --> 00:07:25 ways. We are going to use the 113 00:07:25 --> 00:07:29 computer and we are going to use the blackboard today. 114 00:07:29 --> 00:07:32 And you are going to have available stuff from the 115 00:07:32 --> 00:07:34 Internet a little bit later, too. 116 00:07:34 --> 00:07:37 And all of that is good. I think you should try to 117 00:07:37 --> 00:07:42 reinforce and not worry if some of the information is a little 118 00:07:42 --> 00:07:44 redundant. And never be afraid to ask 119 00:07:44 --> 00:07:48 questions, especially, I like to take questions by 120 00:07:48 --> 00:07:52 email or if you come knock on my office door. 121 00:07:52 --> 00:07:58 In 1916, Gilbert Lewis published a landmark paper in 122 00:07:58 --> 00:08:06 chemistry in the journal of the American Chemical Society which 123 00:08:06 --> 00:08:14 remains the flagship journal of the American Chemical Society. 124 00:08:14 --> 00:08:23 And this paper was entitled "The Atom and the Molecule." 125 00:08:23 --> 00:08:37 126 00:08:37 --> 00:08:41 Besides being an incredibly important and influential paper 127 00:08:41 --> 00:08:45 in the history of chemistry, "The Atom and the Molecule" was 128 00:08:45 --> 00:08:47 also the basis for -- 129 00:08:47 --> 00:09:08 130 00:09:08 --> 00:09:10 Like I said, besides being a hugely 131 00:09:10 --> 00:09:13 influential manuscript, "The Atom and the Molecule" 132 00:09:13 --> 00:09:17 also laid the foundations for Lewis's thinking about 133 00:09:17 --> 00:09:21 electronic structure theory that shaped the way we still today 134 00:09:21 --> 00:09:24 talk about valence and chemical bonding. 135 00:09:24 --> 00:09:28 So, an incredibly important paper from 1916. 136 00:09:28 --> 00:09:31 In the lecture notes today, you will find the specific 137 00:09:31 --> 00:09:35 volume and page number for that reference in the journal of the 138 00:09:35 --> 00:09:39 American Chemical Society. And I encourage you in your 139 00:09:39 --> 00:09:42 copious free time to download that paper. 140 00:09:42 --> 00:09:45 It is really great. All the American Chemical 141 00:09:45 --> 00:09:48 Society journal articles are available, from the very 142 00:09:48 --> 00:09:51 beginning. And you can download it and 143 00:09:51 --> 00:09:52 read it. And, having had this 144 00:09:52 --> 00:09:56 introduction today, I think it will probably prove 145 00:09:56 --> 00:09:59 to be a very fascinating exercise for you, 146 00:09:59 --> 00:10:04 if you choose to do so. It also was the basis of a book 147 00:10:04 --> 00:10:09 that Gilbert Newton Lewis later wrote on valance and on atoms 148 00:10:09 --> 00:10:13 and molecules. That is also a classic in 149 00:10:13 --> 00:10:16 chemistry. And, should you be shopping for 150 00:10:16 --> 00:10:21 chemistry books on e-bay or something, you might find a rare 151 00:10:21 --> 00:10:25 copy of it. And if you do and choose not to 152 00:10:25 --> 00:10:30 buy it, please alert me and I will buy it. 153 00:10:30 --> 00:10:36 But Gilbert Newton Lewis, "The Atom and the Molecule." 154 00:10:36 --> 00:10:43 In this paper you are going to see, if you do choose to 155 00:10:43 --> 00:10:49 download it, that he was thinking about polarity. 156 00:10:49 --> 00:10:56 And he was also thinking about the relationship between the 157 00:10:56 --> 00:11:05 polarity of a molecule relates to the polarity of a substance. 158 00:11:05 --> 00:11:09 And I mean, when I say a polarity of a substance, 159 00:11:09 --> 00:11:14 that that would be a sample, you could say a water molecule 160 00:11:14 --> 00:11:18 down here and liquid water up here. 161 00:11:18 --> 00:11:23 162 00:11:23 --> 00:11:28 And you will see this kind of sigmoidal graph that Lewis made 163 00:11:28 --> 00:11:33 in thinking about how polar condensed phase substances were 164 00:11:33 --> 00:11:38 as compared with the structure of the molecules that comprise 165 00:11:38 --> 00:11:42 the substance. Down here, in this region, 166 00:11:42 --> 00:11:47 you will find that there are substances that are not terribly 167 00:11:47 --> 00:11:50 polar. And what I have written here is 168 00:11:50 --> 00:11:54 the organic shorthand for the hexane molecule. 169 00:11:54 --> 00:11:58 Liquid hexane is an alkane, akin to methane, 170 00:11:58 --> 00:12:03 which is natural gas. And so, if you are not familiar 171 00:12:03 --> 00:12:07 with this way of writing organic molecules, I will just tell you 172 00:12:07 --> 00:12:11 briefly that this terminus is CH three or a methyl group, 173 00:12:11 --> 00:12:13 and then it is CH two, CH two, CH two, 174 00:12:13 --> 00:12:16 CH two, and then CH three, another methyl group. 175 00:12:16 --> 00:12:20 So, that is some organic shorthand. 176 00:12:20 --> 00:12:23 And I will go through that kind of shorthand occasionally so 177 00:12:23 --> 00:12:25 that you become familiar with it. 178 00:12:25 --> 00:12:28 And that is the hexane molecule, a very non-polar 179 00:12:28 --> 00:12:31 molecule composed of elements, carbon and hydrogen, 180 00:12:31 --> 00:12:35 that have very similar electronegativity. 181 00:12:35 --> 00:12:40 And then he goes on up the curve here, and you find this 182 00:12:40 --> 00:12:44 familiar molecule, benzene, considered next, 183 00:12:44 --> 00:12:49 as being somehow more polar than hexane, and liquid benzene 184 00:12:49 --> 00:12:54 accordingly in its solvating properties in the condensed 185 00:12:54 --> 00:13:00 phase, being a more polar medium, as it were. 186 00:13:00 --> 00:13:04 And then, as we continue progress up this scale, 187 00:13:04 --> 00:13:09 he writes next molecules like the diethyl ether molecule. 188 00:13:09 --> 00:13:14 No doubt you are familiar with ether and its applications as an 189 00:13:14 --> 00:13:18 anesthetic. The first use of ether as an 190 00:13:18 --> 00:13:23 anesthesia in an operation in medicine was carried out just 191 00:13:23 --> 00:13:28 across the river in Boston. There is this historical Ether 192 00:13:28 --> 00:13:33 Dome there that you can go and look at. 193 00:13:33 --> 00:13:37 But, nonetheless, we are just getting up a little 194 00:13:37 --> 00:13:41 bit more polar than benzene. And then next you find 195 00:13:41 --> 00:13:45 molecules like this one. That contains an organic 196 00:13:45 --> 00:13:48 functional group called an ester. 197 00:13:48 --> 00:13:52 That is ethyl acetate, which is a substance that you 198 00:13:52 --> 00:13:56 might have smelled if you ever built models, 199 00:13:56 --> 00:14:01 because some of the glues that you may have used would contain 200 00:14:01 --> 00:14:06 it, or the paints. And so, it is a system that, 201 00:14:06 --> 00:14:11 in terms of its molecular structure, is more polar. 202 00:14:11 --> 00:14:15 And, when you use it in the condensed phase, 203 00:14:15 --> 00:14:21 it behaves in a manner that you would describe as more polar. 204 00:14:21 --> 00:14:25 And then, finally, you get up to some very polar 205 00:14:25 --> 00:14:30 systems, like the water molecule. 206 00:14:30 --> 00:14:33 Like the ammonia molecule. And, finally, 207 00:14:33 --> 00:14:38 Lewis talks about a species like this, which is sodium twice 208 00:14:38 --> 00:14:43 sulfur. That is actually called sodium 209 00:14:43 --> 00:14:46 sulfide. And it is a salt analogous to 210 00:14:46 --> 00:14:49 table salt, sodium chloride. 211 00:14:49 --> 00:14:53 And being a salt, it is obviously very polar 212 00:14:53 --> 00:14:58 because there is quite a large degree of charge separation 213 00:14:58 --> 00:15:03 between the atoms in the molecule. 214 00:15:03 --> 00:15:05 And, accordingly, if you take that salt and heat 215 00:15:05 --> 00:15:09 it up until you have got it as hot as its melting point and 216 00:15:09 --> 00:15:11 make it liquid, that molten salt has 217 00:15:11 --> 00:15:14 individually charged ions moving around in solution. 218 00:15:14 --> 00:15:18 And that provides a very polar medium, which would be excellent 219 00:15:18 --> 00:15:22 at dissolving polar things. You will notice here that on 220 00:15:22 --> 00:15:25 the non-polar side we have elements, carbon and hydrogen, 221 00:15:25 --> 00:15:30 that are very close to each other in electronegativity. 222 00:15:30 --> 00:15:33 And then, as we examine this relationship, 223 00:15:33 --> 00:15:37 we start putting in elements like oxygen or nitrogen, 224 00:15:37 --> 00:15:41 which are very electronegative close to the upper right-hand 225 00:15:41 --> 00:15:45 side of the Periodic Table. That introduces polarity both 226 00:15:45 --> 00:15:49 in the molecule and in substances comprised of the 227 00:15:49 --> 00:15:52 molecule. And then all the way over to 228 00:15:52 --> 00:15:55 the involved atoms, sodium and sulfur are very 229 00:15:55 --> 00:15:58 different in electronegativity and, therefore, 230 00:15:58 --> 00:16:03 have very strongly separated charges. 231 00:16:03 --> 00:16:08 And, in thinking about this, Lewis proposed the notion of a 232 00:16:08 --> 00:16:12 continuum. And his musing on this are 233 00:16:12 --> 00:16:18 really quite lucid in that paper, but the idea was that a 234 00:16:18 --> 00:16:22 molecule, or a part of a molecule even, 235 00:16:22 --> 00:16:28 you can analyze molecules in terms of smaller pieces of them 236 00:16:28 --> 00:16:33 that can be identified within the larger molecule, 237 00:16:33 --> 00:16:38 can lie on either side of a continuum in reference to a 238 00:16:38 --> 00:16:46 number of different properties. And the section of class that 239 00:16:46 --> 00:16:53 we are launching into today deals with acid-base properties. 240 00:16:53 --> 00:16:57 Let's mention that first, acid and base. 241 00:16:57 --> 00:17:02 These are two ends of a continuum. 242 00:17:02 --> 00:17:09 But he also recognized that you could have a molecule that would 243 00:17:09 --> 00:17:15 be an oxidant. And the counterpart to that is 244 00:17:15 --> 00:17:20 a reductant. And then, here is a term that 245 00:17:20 --> 00:17:27 maybe those of you who have studied organic chemistry in 246 00:17:27 --> 00:17:33 more detail than most would recognize. 247 00:17:33 --> 00:17:36 This is electrophile. 248 00:17:36 --> 00:17:44 249 00:17:44 --> 00:17:50 Electrophile has a counterpart called a nucleophile. 250 00:17:50 --> 00:18:00 251 00:18:00 --> 00:18:06 And then, the fourth one that I would like to mention is 252 00:18:06 --> 00:18:08 acceptor. 253 00:18:08 --> 00:18:13 254 00:18:13 --> 00:18:15 And, of course, the counterpart to that is 255 00:18:15 --> 00:18:16 donor. 256 00:18:16 --> 00:18:21 257 00:18:21 --> 00:18:25 Please remember those four pairs because when you can 258 00:18:25 --> 00:18:31 understand and make predictions about those four properties as a 259 00:18:31 --> 00:18:38 function of molecular structure, then you will be a chemist. 260 00:18:38 --> 00:18:41 I mean that is a large part of what it is all about, 261 00:18:41 --> 00:18:46 understanding all the different chemical properties that will 262 00:18:46 --> 00:18:50 make it interested in terms of acid-base, oxidant-reductant, 263 00:18:50 --> 00:18:55 electrophile-nucleophile, and acceptor and donor. 264 00:18:55 --> 00:19:00 And the currency of chemistry can be seen, with reference to 265 00:19:00 --> 00:19:05 this, to be the electron. That is what chemistry is all 266 00:19:05 --> 00:19:08 about. And so, we will be talking a 267 00:19:08 --> 00:19:13 lot about atoms and molecules with reference to their 268 00:19:13 --> 00:19:17 properties and how the properties stem from knowing 269 00:19:17 --> 00:19:21 something about the electrons in the molecule. 270 00:19:21 --> 00:19:28 And I think you are going to find this to be quite fun. 271 00:19:28 --> 00:19:35 272 00:19:35 --> 00:19:38 With respect to the properties of the medium, 273 00:19:38 --> 00:19:43 let's talk about a substance like hydrogen chloride. 274 00:19:43 --> 00:19:48 275 00:19:48 --> 00:19:53 This is just to illustrate what I was saying over there. 276 00:19:53 --> 00:19:57 If you take a molecule like hydrogen chloride, 277 00:19:57 --> 00:20:00 and it is a gas, of course. 278 00:20:00 --> 00:20:04 And if you make a solution of it in hexane, 279 00:20:04 --> 00:20:10 hexane is going to be our solvent, and then what you find 280 00:20:10 --> 00:20:16 is that in this low polarity medium hexane solution, 281 00:20:16 --> 00:20:21 liquid hexane, the HCl molecule remains intact 282 00:20:21 --> 00:20:27 and floats around in solution, interacting weakly with hexane 283 00:20:27 --> 00:20:34 molecules that surround it. But if you take this HCl 284 00:20:34 --> 00:20:40 molecule and put it into a solvent like water, 285 00:20:40 --> 00:20:47 then something on the other end of the continuum transpires 286 00:20:47 --> 00:20:53 because we get ionization to produce hydrogen ions. 287 00:20:53 --> 00:20:59 And they go off and are separated in solution from 288 00:20:59 --> 00:21:04 chloride ions. And we will talk more about 289 00:21:04 --> 00:21:09 just what is going on when you separate H plus from Cl 290 00:21:09 --> 00:21:13 minus and let them diffuse apart in aqueous 291 00:21:13 --> 00:21:15 solution. But you can see, 292 00:21:15 --> 00:21:19 I think, the dichotomy. Either the proton shares in the 293 00:21:19 --> 00:21:24 electrons of the chloride, or it just pops off and ionizes 294 00:21:24 --> 00:21:28 and goes out into solution. And Lewis wanted to understand 295 00:21:28 --> 00:21:32 this. And, to understand it, 296 00:21:32 --> 00:21:37 he developed a theory. And his theory was the "cube 297 00:21:37 --> 00:21:42 theory." In this part we get to draw some cubes. 298 00:21:42 --> 00:21:47 And he decided that if you thought of the nucleus, 299 00:21:47 --> 00:21:53 which he calls the kernel, of an atom as being located at 300 00:21:53 --> 00:21:59 the center of the system, then if you had an atom like 301 00:21:59 --> 00:22:05 neon, which is a noble gas with eight valance electrons, 302 00:22:05 --> 00:22:11 that these valance electrons would want to get away from each 303 00:22:11 --> 00:22:19 other as far as possible because they repel each other. 304 00:22:19 --> 00:22:21 They are all negatively charged. 305 00:22:21 --> 00:22:24 This could be, here, the neon atom. 306 00:22:24 --> 00:22:28 Here, on that cube, is how he would represent the 307 00:22:28 --> 00:22:33 electronic structure of the neon atom, with the eight electrons 308 00:22:33 --> 00:22:37 here represented by peach-colored circles, 309 00:22:37 --> 00:22:42 each the vertex of a cube. So, they got far away from each 310 00:22:42 --> 00:22:44 other. And you can see that in the 311 00:22:44 --> 00:22:48 historical archives, some of his original sketch 312 00:22:48 --> 00:22:52 books containing these ideas are there, and now you will know 313 00:22:52 --> 00:22:55 what they mean. You will see that he progressed 314 00:22:55 --> 00:23:01 beyond understanding the atom to understanding the molecule. 315 00:23:01 --> 00:23:07 And here is one of the molecules that he talks about. 316 00:23:07 --> 00:23:22 317 00:23:22 --> 00:23:28 Here we have a molecule containing 14 valance electrons, 318 00:23:28 --> 00:23:34 all arranged in that manner. And this could be, 319 00:23:34 --> 00:23:39 for example, the I two molecule. 320 00:23:39 --> 00:23:45 And let me draw it in terms of a dot structure, 321 00:23:45 --> 00:23:46 -- 322 00:23:46 --> 00:23:52 323 00:23:52 --> 00:23:55 -- like that. And there was known at the 324 00:23:55 --> 00:24:01 time, partly because of the contributions of Lewis himself, 325 00:24:01 --> 00:24:05 something called the Rule of Eight. 326 00:24:05 --> 00:24:10 And that was a reference to this notion that most atoms want 327 00:24:10 --> 00:24:14 to have eight electrons in their valance shell, 328 00:24:14 --> 00:24:20 and it is also something that we call today the Octet Rule. 329 00:24:20 --> 00:24:25 So, when you see the Rule of Eight mentioned in his paper, 330 00:24:25 --> 00:24:31 it is the familiar Octet Rule. And you can see here that one 331 00:24:31 --> 00:24:37 of the key features is two electrons shared equally. 332 00:24:37 --> 00:24:40 And when electrons are shared equally like that, 333 00:24:40 --> 00:24:45 you have a molecule with symmetrical charge distribution, 334 00:24:45 --> 00:24:48 charge referring to the electrons where they are in 335 00:24:48 --> 00:24:51 space. And then, he showed that you 336 00:24:51 --> 00:24:55 could think about this another way. 337 00:24:55 --> 00:25:05 338 00:25:05 --> 00:25:10 You could consider some kind of a geometric distortion of the I 339 00:25:10 --> 00:25:12 two molecule, like this. 340 00:25:12 --> 00:25:17 Distorted, not only because of my drawing, but because of the 341 00:25:17 --> 00:25:22 way the atoms themselves are thought to be rearranging in 342 00:25:22 --> 00:25:24 this process. 343 00:25:24 --> 00:25:34 344 00:25:34 --> 00:25:39 Notice that what has happened here is that the I two 345 00:25:39 --> 00:25:44 molecule is doing something electronically such that one 346 00:25:44 --> 00:25:49 iodine is starting to pull away from the other. 347 00:25:49 --> 00:25:55 This one over here is carrying with it the electron that came 348 00:25:55 --> 00:25:58 from over here. And, in that case, 349 00:25:58 --> 00:26:04 what we have is a molecule in which we are developing partial 350 00:26:04 --> 00:26:08 negative charge on the right-hand side and partial 351 00:26:08 --> 00:26:14 positive charge on the left-hand side. 352 00:26:14 --> 00:26:18 As I was talking up here, I was thinking about what I was 353 00:26:18 --> 00:26:21 going to say here, because the ideal is that 354 00:26:21 --> 00:26:25 molecules, even if they are inherently non-polar like the I 355 00:26:25 --> 00:26:29 two molecule, in their equilibrium structure 356 00:26:29 --> 00:26:33 they can have electron fluctuations that lead to 357 00:26:33 --> 00:26:37 partial charges in the manner shown here. 358 00:26:37 --> 00:26:39 And Lewis was working beautifully toward the 359 00:26:39 --> 00:26:42 development of a theory like this that would allow the 360 00:26:42 --> 00:26:45 description of electronic structure to be made graphically 361 00:26:45 --> 00:26:48 apparent. And this is something that 362 00:26:48 --> 00:26:51 chemists really like to do, is we like to be able to see 363 00:26:51 --> 00:26:53 stuff. I hope I am going to be able to 364 00:26:53 --> 00:26:56 show you some really cool stuff this semester. 365 00:26:56 --> 00:26:58 And, in fact, even some really cool stuff 366 00:26:58 --> 00:27:03 before we finish here today. So, that is the development of 367 00:27:03 --> 00:27:08 charge as represented using the Lewis cube theory in an I two 368 00:27:08 --> 00:27:12 molecule. Next, one thing you could do is 369 00:27:12 --> 00:27:17 say, let's just continue this process, and the right-hand 370 00:27:17 --> 00:27:20 iodine with its eight electrons pops off. 371 00:27:20 --> 00:27:25 That would give you an ionized situation in which you had an I 372 00:27:25 --> 00:27:32 minus floating away from an I plus molecule. 373 00:27:32 --> 00:27:35 And that situation is drawn in the notes, and because I am 374 00:27:35 --> 00:27:39 running out of space on this board I am not going to draw 375 00:27:39 --> 00:27:42 that one up. Instead I am going to go onto 376 00:27:42 --> 00:27:46 another triumph of the Lewis cube theory, which was its 377 00:27:46 --> 00:27:50 ability to explain different chemical bond orders. 378 00:27:50 --> 00:28:02 379 00:28:02 --> 00:28:05 By the way, Lewis never got the Nobel Prize. 380 00:28:05 --> 00:28:08 He certainly should have. A dramatic oversight. 381 00:28:08 --> 00:28:13 He was born in Massachusetts. He was a Harvard professor for 382 00:28:13 --> 00:28:16 a while and did not like it, and came to MIT to be a 383 00:28:16 --> 00:28:20 professor for a while. And, although he liked that, 384 00:28:20 --> 00:28:23 that was not far enough away from Harvard, 385 00:28:23 --> 00:28:27 so he went to Berkeley, where he became the department 386 00:28:27 --> 00:28:31 head and was very successful over a long period of time in 387 00:28:31 --> 00:28:37 learning about chemistry and in teaching chemistry. 388 00:28:37 --> 00:28:40 I will invite you, and you will see this in the 389 00:28:40 --> 00:28:45 notes, too, to go ahead and see if you can find a good biography 390 00:28:45 --> 00:28:49 of Lewis because it is very instructive. 391 00:28:49 --> 00:28:53 Anyway, here is another molecule considered by Lewis's 392 00:28:53 --> 00:28:55 cube theory. 393 00:28:55 --> 00:29:00 394 00:29:00 --> 00:29:05 How many electrons are being shared by the two nuclei or 395 00:29:05 --> 00:29:09 atoms involved? Four electrons shared. 396 00:29:09 --> 00:29:15 We can circle them here. That is four electrons shared. 397 00:29:15 --> 00:29:18 Therefore, that is not a single bond. 398 00:29:18 --> 00:29:23 We call that a double bond. And so, that might be a 399 00:29:23 --> 00:29:27 representation of, for example, 400 00:29:27 --> 00:29:32 the O two molecule. Here we have I two, 401 00:29:32 --> 00:29:37 here we have distorted I two with charges developing, 402 00:29:37 --> 00:29:41 and here we have O two. O two is a very 403 00:29:41 --> 00:29:45 interesting diatomic molecule. We are going to talk about that 404 00:29:45 --> 00:29:49 later in the semester, but for now let's just leave it 405 00:29:49 --> 00:29:53 at that. But then, even though this was 406 00:29:53 --> 00:29:57 quite a successful theory, the cube theory, 407 00:29:57 --> 00:30:00 it has certain problems, certain shortcomings, 408 00:30:00 --> 00:30:04 such as, we can do single bonds with it quite well, 409 00:30:04 --> 00:30:09 and now we can do double bonds with the cube theory, 410 00:30:09 --> 00:30:13 but what do you do if you have to make a triple bond? 411 00:30:13 --> 00:30:18 That was a problem for Lewis. That should be a problem for 412 00:30:18 --> 00:30:21 you, too. Cubes just don't fit together 413 00:30:21 --> 00:30:24 that way. They have edges and faces, 414 00:30:24 --> 00:30:29 and that is it. And they have vertices. 415 00:30:29 --> 00:30:33 You can do one vertex. So, triple bond is a problem. 416 00:30:33 --> 00:30:37 And we know that there are molecules that have triple 417 00:30:37 --> 00:30:39 bonds. And we cannot handle them with 418 00:30:39 --> 00:30:43 the cube theory, so we are going to have to 419 00:30:43 --> 00:30:46 something a little different, for that reason. 420 00:30:46 --> 00:30:51 But there is also another reason that had to do with just 421 00:30:51 --> 00:30:55 considering the chemistry of light elements like hydrogen and 422 00:30:55 --> 00:30:58 helium. Those elements tend to 423 00:30:58 --> 00:31:03 associate themselves with only two electrons. 424 00:31:03 --> 00:31:08 And so, Lewis decided, well, maybe the rule of two is 425 00:31:08 --> 00:31:14 more fundamental than the rule of eight, and that we should be 426 00:31:14 --> 00:31:18 thinking about pairs of electrons somehow. 427 00:31:18 --> 00:31:24 Because he looked at what was known about chemistry and 428 00:31:24 --> 00:31:29 realized that in most molecules, the number of electrons is 429 00:31:29 --> 00:31:35 always even, is always divisible by two. 430 00:31:35 --> 00:31:39 That is something interesting about two electrons at a time 431 00:31:39 --> 00:31:43 being important. You take that together with the 432 00:31:43 --> 00:31:47 triple bond problem, and Lewis started thinking in 433 00:31:47 --> 00:31:51 terms of electron pairs, and this is where this 434 00:31:51 --> 00:31:55 "electron pair theory" comes from. 435 00:31:55 --> 00:32:00 436 00:32:00 --> 00:32:04 Although he spent a lot of time on the cube theory, 437 00:32:04 --> 00:32:09 he was perfectly willing to cast that theory aside in favor 438 00:32:09 --> 00:32:14 of something that maybe was going to work a little better, 439 00:32:14 --> 00:32:18 the electron pair theory. And how does that look? 440 00:32:18 --> 00:32:23 Well, of course, his initial pictures still had 441 00:32:23 --> 00:32:28 the cube, which just shows that once the human mind fixes on 442 00:32:28 --> 00:32:33 something, it fixes on it with great tenacity and it can be 443 00:32:33 --> 00:32:39 hard to shake your way of thinking about things. 444 00:32:39 --> 00:32:42 But hopefully you will be able to do that. 445 00:32:42 --> 00:32:45 He still decided, let's arrange these electron 446 00:32:45 --> 00:32:50 pairs on a cube with the nucleus of the atom supposed to be at 447 00:32:50 --> 00:32:54 the center, and let's keep these electrons, now, 448 00:32:54 --> 00:32:58 nicely collected in pairs. And let's get these pairs as 449 00:32:58 --> 00:33:03 far away from each other as possible, for the same reasons 450 00:33:03 --> 00:33:08 we used to be putting eight electrons as far away from each 451 00:33:08 --> 00:33:13 other as possible, namely, electron repulsion. 452 00:33:13 --> 00:33:17 Now, the problem of electron repulsion between the pairs was 453 00:33:17 --> 00:33:20 not really solved. And Lewis decided that the pair 454 00:33:20 --> 00:33:25 theory worked so well that he was not going to worry about 455 00:33:25 --> 00:33:27 that, and so we won't worry about it yet, 456 00:33:27 --> 00:33:31 either. You have your four pairs of 457 00:33:31 --> 00:33:37 electrons arranged at the center of four of the edges of the 458 00:33:37 --> 00:33:43 cube, and that geometry is what we call a tetrahedron, 459 00:33:43 --> 00:33:47 which I am drawing the edges of here in pink. 460 00:33:47 --> 00:33:52 You have a tetrahedral disposition of four pairs of 461 00:33:52 --> 00:33:55 electrons, now, for an atom. 462 00:33:55 --> 00:34:00 This might again be the neon atom. 463 00:34:00 --> 00:34:11 But the nice thing about this choice is that if you want to 464 00:34:11 --> 00:34:24 you can make single bonds with this theory, and you can make 465 00:34:24 --> 00:34:28 double bonds -- 466 00:34:28 --> 00:34:33 467 00:34:33 --> 00:34:39 -- with this theory, like that. 468 00:34:39 --> 00:34:49 And then, due to the properties of the tetrahedron, 469 00:34:49 --> 00:35:00 you can also make triple bonds. This is marvelous. 470 00:35:00 --> 00:35:05 You can see that the famous chemist Gilbert Newton Lewis was 471 00:35:05 --> 00:35:09 talking about electronic structure in terms of 472 00:35:09 --> 00:35:12 symmetrical things, like tetrahedra and cubes, 473 00:35:12 --> 00:35:17 as a way of arranging electrons reasonably in space. 474 00:35:17 --> 00:35:20 This could, again, be our iodine molecule. 475 00:35:20 --> 00:35:24 This could be, now, our O two molecule. 476 00:35:24 --> 00:35:29 And, if we continue that progression in the Periodic 477 00:35:29 --> 00:35:35 Table, what is this molecule? Dinitrogen, N two, 478 00:35:35 --> 00:35:41 the major component of our atmosphere, another interesting 479 00:35:41 --> 00:35:47 molecule that we will be talking about as the semester progresses 480 00:35:47 --> 00:35:51 forward. But chemical language and 481 00:35:51 --> 00:35:57 electronic structure theory are very much still permeated with 482 00:35:57 --> 00:36:03 this affection for symmetry and the problems that you can solve 483 00:36:03 --> 00:36:10 using symmetry to analyze electronic structure theory. 484 00:36:10 --> 00:36:15 Let's talk next about another molecule because we want to talk 485 00:36:15 --> 00:36:20 about Lewis's development of the electron pair theory, 486 00:36:20 --> 00:36:26 but also we want to understand how that relates to acid-base 487 00:36:26 --> 00:36:29 properties. And so, let me draw here 488 00:36:29 --> 00:36:32 another molecule. 489 00:36:32 --> 00:36:37 490 00:36:37 --> 00:36:41 And when you look at this molecule, which is the aluminum 491 00:36:41 --> 00:36:45 trichloride molecule, in which I am drawing out 492 00:36:45 --> 00:36:50 explicitly all of the electrons, not forgetting these two. 493 00:36:50 --> 00:36:54 And having drawn the aluminum trichloride molecule 494 00:36:54 --> 00:36:59 and looked at it like that, you can ask yourself is the 495 00:36:59 --> 00:37:03 number of electrons divisible by eight? 496 00:37:03 --> 00:37:06 Yes it is. We have a 24 valance electron 497 00:37:06 --> 00:37:10 system here. It is divisible by eight. 498 00:37:10 --> 00:37:14 Of course, it is also divisible by two. 499 00:37:14 --> 00:37:18 You can also ask yourself is this molecule, 500 00:37:18 --> 00:37:23 as written, one that satisfies the rule of eight for all four 501 00:37:23 --> 00:37:25 of the atoms? No. 502 00:37:25 --> 00:37:30 We have a problem there because this thing is electron 503 00:37:30 --> 00:37:33 deficient. 504 00:37:33 --> 00:37:42 505 00:37:42 --> 00:37:45 And if you were Lewis, you would want to know, 506 00:37:45 --> 00:37:50 well, if it is electron deficient, this molecule must be 507 00:37:50 --> 00:37:54 doing something about that to get more electrons. 508 00:37:54 --> 00:37:58 Which atom is missing electrons, here? 509 00:37:58 --> 00:38:02 The aluminum. How can we give aluminum more 510 00:38:02 --> 00:38:04 electrons, in a structure like this? 511 00:38:04 --> 00:38:08 Can we get it up to the rule of eight? 512 00:38:08 --> 00:38:13 513 00:38:13 --> 00:38:14 Double bonds, awesome. 514 00:38:14 --> 00:38:18 Beautiful. We can make a double bond. 515 00:38:18 --> 00:38:22 And, if we do that, we can allow aluminum to 516 00:38:22 --> 00:38:27 satisfy the rule of eight, or allow the rule of eight to 517 00:38:27 --> 00:38:33 satisfy aluminum. Whichever way you want to look 518 00:38:33 --> 00:38:36 at it. And see what we have done, 519 00:38:36 --> 00:38:39 here? We have taken one of the 520 00:38:39 --> 00:38:42 electron pairs, say, this one, 521 00:38:42 --> 00:38:49 and we have moved it in between the aluminum and the chlorine, 522 00:38:49 --> 00:38:52 so it joins the other one in there. 523 00:38:52 --> 00:38:57 And we get a double bond. And now, everybody has an 524 00:38:57 --> 00:39:02 octet. But what is the problem with 525 00:39:02 --> 00:39:05 that? The problem with that is that 526 00:39:05 --> 00:39:08 chlorine is very electronegative, 527 00:39:08 --> 00:39:13 and it does not want its electrons stolen away by the 528 00:39:13 --> 00:39:16 very electropositive aluminum center. 529 00:39:16 --> 00:39:21 There are other ways that aluminum can ultimately satisfy 530 00:39:21 --> 00:39:27 its octet, and this is how we get into the realm of "Lewis 531 00:39:27 --> 00:39:32 acid-base theory." And I want to show you one of 532 00:39:32 --> 00:39:36 the other ways that aluminum can satisfy its octet, 533 00:39:36 --> 00:39:41 and then, we are going to move to the computer so we can 534 00:39:41 --> 00:39:44 visualize some of these properties. 535 00:39:44 --> 00:39:49 If I put my aluminum here -- and do you remember this 536 00:39:49 --> 00:39:52 molecule up here, the ammonia molecule? 537 00:39:52 --> 00:39:57 I am going to say that if I draw that ammonia molecule in 538 00:39:57 --> 00:40:00 place, here -- 539 00:40:00 --> 00:40:05 540 00:40:05 --> 00:40:10 The ammonia molecule comes in, and it has its eight electrons. 541 00:40:10 --> 00:40:13 It is sharing six of them with three hydrogens. 542 00:40:13 --> 00:40:18 The idea is that it has an extra pair of electrons on that 543 00:40:18 --> 00:40:23 nitrogen in the ammonia molecule, that it can share with 544 00:40:23 --> 00:40:26 the aluminum. And now we go ahead and 545 00:40:26 --> 00:40:30 complete the picture. And we can have eight electrons 546 00:40:30 --> 00:40:33 around everybody. 547 00:40:33 --> 00:40:38 548 00:40:38 --> 00:40:42 And so the rule of eight is now satisfied for the three 549 00:40:42 --> 00:40:46 chlorines, for the aluminum, and for the nitrogen of the 550 00:40:46 --> 00:40:50 ammonia molecule. The ammonia molecule is what we 551 00:40:50 --> 00:40:53 call a "Lewis base." 552 00:40:53 --> 00:40:58 553 00:40:58 --> 00:41:03 And the aluminum trichloride molecule is what we 554 00:41:03 --> 00:41:08 call a "Lewis acid," for reasons that should now be 555 00:41:08 --> 00:41:12 quite clear. And I want to show you how we 556 00:41:12 --> 00:41:17 can look at these things. And if you will give me just a 557 00:41:17 --> 00:41:22 second here, I am going to load the aluminum trichloride 558 00:41:22 --> 00:41:26 molecule up onto the screen. 559 00:41:26 --> 00:41:33 560 00:41:33 --> 00:41:38 What we are going to do is remember that there are lots of 561 00:41:38 --> 00:41:42 different ways in which you can visualize molecules. 562 00:41:42 --> 00:41:48 And I want to show you some of the more interesting ways. 563 00:41:48 --> 00:42:26 564 00:42:26 --> 00:42:33 All that is is a picture of the aluminum trichloride 565 00:42:33 --> 00:42:40 molecule with spheres drawn at kind of arbitrary radii. 566 00:42:40 --> 00:42:45 The size of these spheres is not representative of any 567 00:42:45 --> 00:42:51 particular physical quantity, but we can change that. 568 00:42:51 --> 00:42:56 And so now, what we are going to do is draw the thing a 569 00:42:56 --> 00:43:02 slightly different way. And what you can see is that 570 00:43:02 --> 00:43:07 the positions of those nuclei are in this flat box. 571 00:43:07 --> 00:43:13 I made the box kind of flat. It is kind of a slab because 572 00:43:13 --> 00:43:19 this AlCl three molecule is conveniently kind of 573 00:43:19 --> 00:43:24 flat in its structure. And what are we going to do 574 00:43:24 --> 00:43:28 now? We are going to draw a contour 575 00:43:28 --> 00:43:31 surface. And I like this. 576 00:43:31 --> 00:43:34 We are going to use the solid surface method, 577 00:43:34 --> 00:43:37 first. And can you see that now? 578 00:43:37 --> 00:43:41 These curves that enclose the four nuclei of the aluminum 579 00:43:41 --> 00:43:45 trichloride molecule do have some physical 580 00:43:45 --> 00:43:49 significance, because what I have done here 581 00:43:49 --> 00:43:53 is taken results, in this case from the quantum 582 00:43:53 --> 00:43:57 chemistry calculation, but you could also take it from 583 00:43:57 --> 00:44:03 an X-ray crystallographic structure determination study. 584 00:44:03 --> 00:44:06 And I have drawn a three-dimensional contour map. 585 00:44:06 --> 00:44:11 The value of the electron density at every point on the 586 00:44:11 --> 00:44:14 surface of one of those ovaloid shapes is the same. 587 00:44:14 --> 00:44:19 Just like when you have a contour map to describe in two 588 00:44:19 --> 00:44:22 dimensions an interesting complicated surface, 589 00:44:22 --> 00:44:27 we can do this in three dimensions as well. 590 00:44:27 --> 00:44:30 And one of the things you notice, when you look at a 591 00:44:30 --> 00:44:33 surface like this, is that the value of the 592 00:44:33 --> 00:44:37 electron density actually goes down to some low value in 593 00:44:37 --> 00:44:39 between the nuclei, for this. 594 00:44:39 --> 00:44:43 When you see molecules represented as balls and sticks, 595 00:44:43 --> 00:44:47 or if you represent molecules this way, just showing a pair of 596 00:44:47 --> 00:44:51 dots between the aluminum and chloride, you may not be getting 597 00:44:51 --> 00:44:56 a physically complete picture of the situation. 598 00:44:56 --> 00:44:59 You can get a much more complete picture if you have 599 00:44:59 --> 00:45:02 access to the actual electron density. 600 00:45:02 --> 00:45:06 And then, you can even go a little further, 601 00:45:06 --> 00:45:09 and I want to show you something very cool. 602 00:45:09 --> 00:45:14 First I am going to need to load in a second molecule. 603 00:45:14 --> 00:45:19 604 00:45:19 --> 00:45:22 And that will be the product of the first "Lewis acid-base 605 00:45:22 --> 00:45:25 reaction" that we have discussed. 606 00:45:25 --> 00:45:29 Because, I didn't say it over there, but that was your first 607 00:45:29 --> 00:45:33 exposure to a Lewis acid-base reaction, in which the ammonia 608 00:45:33 --> 00:45:36 molecule comes in and binds to the aluminum trichloride 609 00:45:36 --> 00:45:40 molecule, in order to satisfy the valence 610 00:45:40 --> 00:45:44 requirements of the respective atom types. 611 00:45:44 --> 00:45:47 And so, here we are going to look at that molecule, 612 00:45:47 --> 00:45:51 and we are going to look at its electron density. 613 00:45:51 --> 00:46:00 614 00:46:00 --> 00:46:04 And I think you are going to like this very much. 615 00:46:04 --> 00:46:26 616 00:46:26 --> 00:46:29 Here it comes. And then I am going to 617 00:46:29 --> 00:46:33 represent this as a solid surface. 618 00:46:33 --> 00:46:38 The value of the electron density everywhere on this 619 00:46:38 --> 00:46:42 surface is 0.1 electron density units. 620 00:46:42 --> 00:46:48 I want you to start thinking about how that shape appears 621 00:46:48 --> 00:46:53 there because I am going to underscore that a little bit 622 00:46:53 --> 00:46:59 more in just a second. But one thing you should notice 623 00:46:59 --> 00:47:04 is that at the NH three molecule, which is pictured at 624 00:47:04 --> 00:47:10 the top of that representation, what you are seeing is that the 625 00:47:10 --> 00:47:15 value of the electron density does not get very small as you 626 00:47:15 --> 00:47:19 go between the nitrogen and hydrogen nuclei because both 627 00:47:19 --> 00:47:25 nitrogen and hydrogen are quite similar in electronegativity as 628 00:47:25 --> 00:47:30 compared with the aluminum atom in this system. 629 00:47:30 --> 00:47:38 630 00:47:38 --> 00:47:46 The fascinating thing about illustrating a molecule in this 631 00:47:46 --> 00:47:55 way is that we can actually associate another property with 632 00:47:55 --> 00:48:02 the color on the surface. Now what we are doing is 633 00:48:02 --> 00:48:06 looking at the aluminum trichloride ammonia system. 634 00:48:06 --> 00:48:10 And let me see if I can make this thing gradually spin, 635 00:48:10 --> 00:48:15 so that I can talk about it without being pinned to my 636 00:48:15 --> 00:48:18 computer. What we have on the surface on 637 00:48:18 --> 00:48:23 each of these electron density isosurface enclosed regions is a 638 00:48:23 --> 00:48:28 color that corresponds with a value of a function that tells 639 00:48:28 --> 00:48:33 us about the propensity of electrons to be paired at that 640 00:48:33 --> 00:48:38 point in space. The Lewis theory is now colored 641 00:48:38 --> 00:48:42 onto the electron density isosurface of this Lewis acid, 642 00:48:42 --> 00:48:47 Lewis base complex molecule. And the values that correspond 643 00:48:47 --> 00:48:52 to those regions in space where electrons are most likely to be 644 00:48:52 --> 00:48:54 found paired up are colored blue. 645 00:48:54 --> 00:48:59 Where they are least likely to be found paired up are colored 646 00:48:59 --> 00:49:02 kind of red-orange, here. 647 00:49:02 --> 00:49:05 And then an intermediate color is this green. 648 00:49:05 --> 00:49:09 And so, you can see that you have electron pairs associated 649 00:49:09 --> 00:49:12 with each of the three NH bonds, up at the top. 650 00:49:12 --> 00:49:16 You have another electron pair here in blue, 651 00:49:16 --> 00:49:19 which is very proximate to this aluminum center, 652 00:49:19 --> 00:49:24 that is very electron deficient as we had found right over here 653 00:49:24 --> 00:49:27 because it lacks an octet. And then, each of these 654 00:49:27 --> 00:49:32 chlorines is able to attract electron pairs. 655 00:49:32 --> 00:49:34 Because chlorine is very electronegative, 656 00:49:34 --> 00:49:39 it attracts the electron pairs to itself and sort of withholds 657 00:49:39 --> 00:49:43 them from the aluminum center, but yet, that development of 658 00:49:43 --> 00:49:47 charge separation keeps everything together in what we 659 00:49:47 --> 00:49:51 can call an ionic interaction, an electrostatic interaction. 660 00:49:51 --> 00:49:55 You can see here covalent bonding, donor-acceptor complex 661 00:49:55 --> 00:50:00 formation, and electrostatic contributions to bonding. 662 0:50:00 --> 00:50:03 And all of this is just an illustration of the brilliant 663 0:50:03.942 --> 50:06 ideas of Gilbert Newton Lewis.