1 00:00:01,000 --> 00:00:04,000 The following content is provided by MIT OpenCourseWare 2 00:00:04,000 --> 00:00:06,000 under a Creative Commons license. 3 00:00:06,000 --> 00:00:10,000 Additional information about our license and MIT 4 00:00:10,000 --> 00:00:15,000 OpenCourseWare in general is available at ocw.mit.edu. 5 00:00:15,000 --> 00:00:19,000 Today is a very big day for all of you. 6 00:00:19,000 --> 00:00:24,000 Your first semester at MIT is half over. 7 00:00:30,000 --> 00:00:35,000 And, in addition to that, you have a lot of challenges 8 00:00:35,000 --> 00:00:41,000 remaining ahead of you for the rest of this semester. 9 00:00:41,000 --> 00:00:47,000 I am going to help make the chemical challenges fun for you. 10 00:00:47,000 --> 00:00:52,000 That is what I am here to do. I love chemistry. 11 00:00:52,000 --> 00:00:57,000 I love teaching 5.112. This is the best part of my 12 00:00:57,000 --> 00:01:01,000 week. So, here we are. 13 00:01:01,000 --> 00:01:07,000 Do you guys know that chemistry can be incredibly fun? 14 00:01:15,000 --> 00:01:19,000 Let me just show you how fun chemistry can be. 15 00:01:26,000 --> 00:01:29,000 And that is just the gravy. The fun part is actually making 16 00:01:29,000 --> 00:01:34,000 the molecules. Any of you see this picture in 17 00:01:34,000 --> 00:01:37,000 U.S.A. Today recently? 18 00:01:42,000 --> 00:01:44,000 Not reading that important journal, I see. 19 00:01:44,000 --> 00:01:48,000 Well, this picture did appear very recently in U.S.A. 20 00:01:48,000 --> 00:01:52,000 Today in a story that talked about the recent Nobel Prize in 21 00:01:52,000 --> 00:01:56,000 chemistry that was awarded to Professor Richard R. 22 00:01:56,000 --> 00:01:59,000 Schrock, of our department. And, in fact, 23 00:01:59,000 --> 00:02:03,000 I don't know if you realize this, but Professor Schrock was 24 00:02:03,000 --> 00:02:07,000 the first person ever awarded the Nobel Prize in Chemistry at 25 00:02:07,000 --> 00:02:10,000 MIT for work conducted while at MIT. 26 00:02:10,000 --> 00:02:13,000 That is a pretty amazing accomplishment because we have 27 00:02:13,000 --> 00:02:17,000 so many tremendous chemists on the faculty here, 28 00:02:17,000 --> 00:02:20,000 and he is the first one to break through in that manner. 29 00:02:20,000 --> 00:02:23,000 And maybe you are here at a very special time, 30 00:02:23,000 --> 00:02:29,000 and we will see a number more of these in the next few years. 31 00:02:29,000 --> 00:02:33,000 May with you contributing, so much the better because you 32 00:02:33,000 --> 00:02:35,000 are here. And let me just explain 33 00:02:35,000 --> 00:02:37,000 something, too. Chemistry is fun. 34 00:02:37,000 --> 00:02:41,000 And only on very rare occasions like this would Professor 35 00:02:41,000 --> 00:02:45,000 Schrock be drinking champagne at 8:30 in the morning, 36 00:02:45,000 --> 00:02:49,000 when this picture was taken. The Reuters reporter, 37 00:02:49,000 --> 00:02:53,000 Brian, who took this photo, is actually a pretty good 38 00:02:53,000 --> 00:02:57,000 friend of Professor Nocera here. And so he rode over from the 39 00:02:57,000 --> 00:03:01,000 Schrock household. And Dick and Dan came in 40 00:03:01,000 --> 00:03:04,000 together in the same car, as they often do, 41 00:03:04,000 --> 00:03:07,000 from Winchester on that morning, which was a very 42 00:03:07,000 --> 00:03:10,000 exciting day. If you come to see me for 43 00:03:10,000 --> 00:03:14,000 office hours maybe I will tell you more about it in detail, 44 00:03:14,000 --> 00:03:17,000 but it was an exciting day. And I am in here, 45 00:03:17,000 --> 00:03:19,000 too. My name is Kit Cummins. 46 00:03:19,000 --> 00:03:21,000 Kit is my nickname. My name is Christopher. 47 00:03:21,000 --> 00:03:25,000 You can call me Christopher or Kit, or you can call me 48 00:03:25,000 --> 00:03:28,000 Professor Cummins, or you can just say hey, 49 00:03:28,000 --> 00:03:32,000 chemistry guy. That will be fine. 50 00:03:32,000 --> 00:03:36,000 I am in this picture primarily because it is part of being in 51 00:03:36,000 --> 00:03:40,000 the right place at the right time, just like I am here now in 52 00:03:40,000 --> 00:03:43,000 front of you. But also I am in it because we 53 00:03:43,000 --> 00:03:47,000 three are three in one of the areas in our department that 54 00:03:47,000 --> 00:03:51,000 really focus our research on inorganic chemistry. 55 00:03:51,000 --> 00:03:53,000 And what is inorganic chemistry? 56 00:03:53,000 --> 00:03:58,000 I will say more about this during the semester. 57 00:03:58,000 --> 00:04:02,000 But inorganic chemistry is really the chemistry of the 58 00:04:02,000 --> 00:04:05,000 elements of the Periodic Table inclusively. 59 00:04:05,000 --> 00:04:09,000 So, a pretty broad topic. And I like doing chemistry with 60 00:04:09,000 --> 00:04:12,000 lots of elements. And so that is why these guys 61 00:04:12,000 --> 00:04:16,000 and I share an association with each other. 62 00:04:16,000 --> 00:04:19,000 And, in fact, I was a graduate student with 63 00:04:19,000 --> 00:04:21,000 Professor Schrock. And I am very, 64 00:04:21,000 --> 00:04:24,000 very proud to be able to say that. 65 00:04:24,000 --> 00:04:29,000 Hopefully, my computer will be staying on, here. 66 00:04:29,000 --> 00:04:32,000 And I want to point out, too, that people who love 67 00:04:32,000 --> 00:04:36,000 science want to know something about its history. 68 00:04:36,000 --> 00:04:40,000 And part of all of that is knowing the academic family from 69 00:04:40,000 --> 00:04:43,000 which you derive, depending on the person you've 70 00:04:43,000 --> 00:04:46,000 studied with in learning about chemistry. 71 00:04:46,000 --> 00:04:50,000 And I studied with Schrock. And Schrock studied with 72 00:04:50,000 --> 00:04:53,000 Osborn, a fantastic chemist in his own right, 73 00:04:53,000 --> 00:04:56,000 no longer alive, sadly, to see his progeny, 74 00:04:56,000 --> 00:05:01,000 Professor Schrock, win the Nobel Prize. 75 00:05:01,000 --> 00:05:04,000 And Osborn studied with Wilkinson, and Wilkinson was 76 00:05:04,000 --> 00:05:08,000 also a Nobel Prize winner. So, you do not have to go very 77 00:05:08,000 --> 00:05:11,000 far back in that lineage to encounter that recognition, 78 00:05:11,000 --> 00:05:14,000 the Nobel Prize, Schrock, and then it skipped 79 00:05:14,000 --> 00:05:18,000 Osborne, and if you go back to Wilkinson, there is another one. 80 00:05:18,000 --> 00:05:22,000 And you can keep going back. And I am not going to go 81 00:05:22,000 --> 00:05:26,000 through that whole history today because I have another history 82 00:05:26,000 --> 00:05:31,000 that I am going to need to go through with you today. 83 00:05:31,000 --> 00:05:40,000 And I am going to bring this back over so it does not 84 00:05:40,000 --> 00:05:48,000 distract you. And this other history that I 85 00:05:48,000 --> 00:05:57,000 need to impart to you today has to do with some of the 86 00:05:57,000 --> 00:06:06,000 contributions of Gilbert Newton Lewis. 87 00:06:06,000 --> 00:06:09,000 This is one of the most famous of all chemists ever. 88 00:06:09,000 --> 00:06:14,000 And if you like chemistry, I encourage you to think of the 89 00:06:14,000 --> 00:06:18,000 word Newton, as it is found engraved in one of the pillars 90 00:06:18,000 --> 00:06:23,000 in Killian Court at MIT as the middle name of Gilbert Newton 91 00:06:23,000 --> 00:06:26,000 Lewis. It is conceivable that having 92 00:06:26,000 --> 00:06:30,000 that middle name weighed heavily upon Gilbert during his 93 00:06:30,000 --> 00:06:34,000 lifetime. But it remains a good moniker. 94 00:06:34,000 --> 00:06:37,000 And in the future, when you have kids, 95 00:06:37,000 --> 00:06:41,000 I encourage you to consider using it as a middle name. 96 00:06:41,000 --> 00:06:43,000 It worked well in this particular case. 97 00:06:43,000 --> 00:06:48,000 When you get the notes for today, which incidentally will 98 00:06:48,000 --> 00:06:51,000 be available on the website after class today, 99 00:06:51,000 --> 00:06:56,000 so you don't need to write down everything I am writing down. 100 00:06:56,000 --> 00:07:00,000 You are actually going to get a little bit more in the online 101 00:07:00,000 --> 00:07:05,000 version than what I am writing down here. 102 00:07:05,000 --> 00:07:08,000 And if you find that you forgot something that I said during 103 00:07:08,000 --> 00:07:11,000 class, just email me. I will tell you what I said. 104 00:07:11,000 --> 00:07:14,000 It is not a problem. But if you want to write down 105 00:07:14,000 --> 00:07:17,000 notes while I am speaking just to make notes that you can refer 106 00:07:17,000 --> 00:07:20,000 to later to refresh your memory, that is fine. 107 00:07:20,000 --> 00:07:23,000 I think your taking in information in lots of different 108 00:07:23,000 --> 00:07:25,000 ways. We are going to use the 109 00:07:25,000 --> 00:07:29,000 computer and we are going to use the blackboard today. 110 00:07:29,000 --> 00:07:32,000 And you are going to have available stuff from the 111 00:07:32,000 --> 00:07:34,000 Internet a little bit later, too. 112 00:07:34,000 --> 00:07:37,000 And all of that is good. I think you should try to 113 00:07:37,000 --> 00:07:42,000 reinforce and not worry if some of the information is a little 114 00:07:42,000 --> 00:07:44,000 redundant. And never be afraid to ask 115 00:07:44,000 --> 00:07:48,000 questions, especially, I like to take questions by 116 00:07:48,000 --> 00:07:52,000 email or if you come knock on my office door. 117 00:07:52,000 --> 00:07:58,000 In 1916, Gilbert Lewis published a landmark paper in 118 00:07:58,000 --> 00:08:06,000 chemistry in the journal of the American Chemical Society which 119 00:08:06,000 --> 00:08:14,000 remains the flagship journal of the American Chemical Society. 120 00:08:14,000 --> 00:08:23,000 And this paper was entitled "The Atom and the Molecule." 121 00:08:37,000 --> 00:08:41,000 Besides being an incredibly important and influential paper 122 00:08:41,000 --> 00:08:45,000 in the history of chemistry, "The Atom and the Molecule" was 123 00:08:45,000 --> 00:08:47,000 also the basis for -- 124 00:09:08,000 --> 00:09:10,000 Like I said, besides being a hugely 125 00:09:10,000 --> 00:09:13,000 influential manuscript, "The Atom and the Molecule" 126 00:09:13,000 --> 00:09:17,000 also laid the foundations for Lewis's thinking about 127 00:09:17,000 --> 00:09:21,000 electronic structure theory that shaped the way we still today 128 00:09:21,000 --> 00:09:24,000 talk about valence and chemical bonding. 129 00:09:24,000 --> 00:09:28,000 So, an incredibly important paper from 1916. 130 00:09:28,000 --> 00:09:31,000 In the lecture notes today, you will find the specific 131 00:09:31,000 --> 00:09:35,000 volume and page number for that reference in the journal of the 132 00:09:35,000 --> 00:09:39,000 American Chemical Society. And I encourage you in your 133 00:09:39,000 --> 00:09:42,000 copious free time to download that paper. 134 00:09:42,000 --> 00:09:45,000 It is really great. All the American Chemical 135 00:09:45,000 --> 00:09:48,000 Society journal articles are available, from the very 136 00:09:48,000 --> 00:09:51,000 beginning. And you can download it and 137 00:09:51,000 --> 00:09:52,000 read it. And, having had this 138 00:09:52,000 --> 00:09:56,000 introduction today, I think it will probably prove 139 00:09:56,000 --> 00:09:59,000 to be a very fascinating exercise for you, 140 00:09:59,000 --> 00:10:04,000 if you choose to do so. It also was the basis of a book 141 00:10:04,000 --> 00:10:09,000 that Gilbert Newton Lewis later wrote on valance and on atoms 142 00:10:09,000 --> 00:10:13,000 and molecules. That is also a classic in 143 00:10:13,000 --> 00:10:16,000 chemistry. And, should you be shopping for 144 00:10:16,000 --> 00:10:21,000 chemistry books on e-bay or something, you might find a rare 145 00:10:21,000 --> 00:10:25,000 copy of it. And if you do and choose not to 146 00:10:25,000 --> 00:10:30,000 buy it, please alert me and I will buy it. 147 00:10:30,000 --> 00:10:36,000 But Gilbert Newton Lewis, "The Atom and the Molecule." 148 00:10:36,000 --> 00:10:43,000 In this paper you are going to see, if you do choose to 149 00:10:43,000 --> 00:10:49,000 download it, that he was thinking about polarity. 150 00:10:49,000 --> 00:10:56,000 And he was also thinking about the relationship between the 151 00:10:56,000 --> 00:11:05,000 polarity of a molecule relates to the polarity of a substance. 152 00:11:05,000 --> 00:11:09,000 And I mean, when I say a polarity of a substance, 153 00:11:09,000 --> 00:11:14,000 that that would be a sample, you could say a water molecule 154 00:11:14,000 --> 00:11:18,000 down here and liquid water up here. 155 00:11:23,000 --> 00:11:28,000 And you will see this kind of sigmoidal graph that Lewis made 156 00:11:28,000 --> 00:11:33,000 in thinking about how polar condensed phase substances were 157 00:11:33,000 --> 00:11:38,000 as compared with the structure of the molecules that comprise 158 00:11:38,000 --> 00:11:42,000 the substance. Down here, in this region, 159 00:11:42,000 --> 00:11:47,000 you will find that there are substances that are not terribly 160 00:11:47,000 --> 00:11:50,000 polar. And what I have written here is 161 00:11:50,000 --> 00:11:54,000 the organic shorthand for the hexane molecule. 162 00:11:54,000 --> 00:11:58,000 Liquid hexane is an alkane, akin to methane, 163 00:11:58,000 --> 00:12:03,000 which is natural gas. And so, if you are not familiar 164 00:12:03,000 --> 00:12:07,000 with this way of writing organic molecules, I will just tell you 165 00:12:07,000 --> 00:12:11,000 briefly that this terminus is CH three or a methyl group, 166 00:12:11,000 --> 00:12:13,000 and then it is CH two, CH two, CH two, 167 00:12:13,000 --> 00:12:16,000 CH two, and then CH three, another methyl group. 168 00:12:16,000 --> 00:12:20,000 So, that is some organic shorthand. 169 00:12:20,000 --> 00:12:23,000 And I will go through that kind of shorthand occasionally so 170 00:12:23,000 --> 00:12:25,000 that you become familiar with it. 171 00:12:25,000 --> 00:12:28,000 And that is the hexane molecule, a very non-polar 172 00:12:28,000 --> 00:12:31,000 molecule composed of elements, carbon and hydrogen, 173 00:12:31,000 --> 00:12:35,000 that have very similar electronegativity. 174 00:12:35,000 --> 00:12:40,000 And then he goes on up the curve here, and you find this 175 00:12:40,000 --> 00:12:44,000 familiar molecule, benzene, considered next, 176 00:12:44,000 --> 00:12:49,000 as being somehow more polar than hexane, and liquid benzene 177 00:12:49,000 --> 00:12:54,000 accordingly in its solvating properties in the condensed 178 00:12:54,000 --> 00:13:00,000 phase, being a more polar medium, as it were. 179 00:13:00,000 --> 00:13:04,000 And then, as we continue progress up this scale, 180 00:13:04,000 --> 00:13:09,000 he writes next molecules like the diethyl ether molecule. 181 00:13:09,000 --> 00:13:14,000 No doubt you are familiar with ether and its applications as an 182 00:13:14,000 --> 00:13:18,000 anesthetic. The first use of ether as an 183 00:13:18,000 --> 00:13:23,000 anesthesia in an operation in medicine was carried out just 184 00:13:23,000 --> 00:13:28,000 across the river in Boston. There is this historical Ether 185 00:13:28,000 --> 00:13:33,000 Dome there that you can go and look at. 186 00:13:33,000 --> 00:13:37,000 But, nonetheless, we are just getting up a little 187 00:13:37,000 --> 00:13:41,000 bit more polar than benzene. And then next you find 188 00:13:41,000 --> 00:13:45,000 molecules like this one. That contains an organic 189 00:13:45,000 --> 00:13:48,000 functional group called an ester. 190 00:13:48,000 --> 00:13:52,000 That is ethyl acetate, which is a substance that you 191 00:13:52,000 --> 00:13:56,000 might have smelled if you ever built models, 192 00:13:56,000 --> 00:14:01,000 because some of the glues that you may have used would contain 193 00:14:01,000 --> 00:14:06,000 it, or the paints. And so, it is a system that, 194 00:14:06,000 --> 00:14:11,000 in terms of its molecular structure, is more polar. 195 00:14:11,000 --> 00:14:15,000 And, when you use it in the condensed phase, 196 00:14:15,000 --> 00:14:21,000 it behaves in a manner that you would describe as more polar. 197 00:14:21,000 --> 00:14:25,000 And then, finally, you get up to some very polar 198 00:14:25,000 --> 00:14:30,000 systems, like the water molecule. 199 00:14:30,000 --> 00:14:33,000 Like the ammonia molecule. And, finally, 200 00:14:33,000 --> 00:14:38,000 Lewis talks about a species like this, which is sodium twice 201 00:14:38,000 --> 00:14:43,000 sulfur. That is actually called sodium 202 00:14:43,000 --> 00:14:46,000 sulfide. And it is a salt analogous to 203 00:14:46,000 --> 00:14:49,000 table salt, sodium chloride. 204 00:14:49,000 --> 00:14:53,000 And being a salt, it is obviously very polar 205 00:14:53,000 --> 00:14:58,000 because there is quite a large degree of charge separation 206 00:14:58,000 --> 00:15:03,000 between the atoms in the molecule. 207 00:15:03,000 --> 00:15:05,000 And, accordingly, if you take that salt and heat 208 00:15:05,000 --> 00:15:09,000 it up until you have got it as hot as its melting point and 209 00:15:09,000 --> 00:15:11,000 make it liquid, that molten salt has 210 00:15:11,000 --> 00:15:14,000 individually charged ions moving around in solution. 211 00:15:14,000 --> 00:15:18,000 And that provides a very polar medium, which would be excellent 212 00:15:18,000 --> 00:15:22,000 at dissolving polar things. You will notice here that on 213 00:15:22,000 --> 00:15:25,000 the non-polar side we have elements, carbon and hydrogen, 214 00:15:25,000 --> 00:15:30,000 that are very close to each other in electronegativity. 215 00:15:30,000 --> 00:15:33,000 And then, as we examine this relationship, 216 00:15:33,000 --> 00:15:37,000 we start putting in elements like oxygen or nitrogen, 217 00:15:37,000 --> 00:15:41,000 which are very electronegative close to the upper right-hand 218 00:15:41,000 --> 00:15:45,000 side of the Periodic Table. That introduces polarity both 219 00:15:45,000 --> 00:15:49,000 in the molecule and in substances comprised of the 220 00:15:49,000 --> 00:15:52,000 molecule. And then all the way over to 221 00:15:52,000 --> 00:15:55,000 the involved atoms, sodium and sulfur are very 222 00:15:55,000 --> 00:15:58,000 different in electronegativity and, therefore, 223 00:15:58,000 --> 00:16:03,000 have very strongly separated charges. 224 00:16:03,000 --> 00:16:08,000 And, in thinking about this, Lewis proposed the notion of a 225 00:16:08,000 --> 00:16:12,000 continuum. And his musing on this are 226 00:16:12,000 --> 00:16:18,000 really quite lucid in that paper, but the idea was that a 227 00:16:18,000 --> 00:16:22,000 molecule, or a part of a molecule even, 228 00:16:22,000 --> 00:16:28,000 you can analyze molecules in terms of smaller pieces of them 229 00:16:28,000 --> 00:16:33,000 that can be identified within the larger molecule, 230 00:16:33,000 --> 00:16:38,000 can lie on either side of a continuum in reference to a 231 00:16:38,000 --> 00:16:46,000 number of different properties. And the section of class that 232 00:16:46,000 --> 00:16:53,000 we are launching into today deals with acid-base properties. 233 00:16:53,000 --> 00:16:57,000 Let's mention that first, acid and base. 234 00:16:57,000 --> 00:17:02,000 These are two ends of a continuum. 235 00:17:02,000 --> 00:17:09,000 But he also recognized that you could have a molecule that would 236 00:17:09,000 --> 00:17:15,000 be an oxidant. And the counterpart to that is 237 00:17:15,000 --> 00:17:20,000 a reductant. And then, here is a term that 238 00:17:20,000 --> 00:17:27,000 maybe those of you who have studied organic chemistry in 239 00:17:27,000 --> 00:17:33,000 more detail than most would recognize. 240 00:17:33,000 --> 00:17:36,000 This is electrophile. 241 00:17:44,000 --> 00:17:50,000 Electrophile has a counterpart called a nucleophile. 242 00:18:00,000 --> 00:18:06,000 And then, the fourth one that I would like to mention is 243 00:18:06,000 --> 00:18:08,000 acceptor. 244 00:18:13,000 --> 00:18:15,000 And, of course, the counterpart to that is 245 00:18:15,000 --> 00:18:16,000 donor. 246 00:18:21,000 --> 00:18:25,000 Please remember those four pairs because when you can 247 00:18:25,000 --> 00:18:31,000 understand and make predictions about those four properties as a 248 00:18:31,000 --> 00:18:38,000 function of molecular structure, then you will be a chemist. 249 00:18:38,000 --> 00:18:41,000 I mean that is a large part of what it is all about, 250 00:18:41,000 --> 00:18:46,000 understanding all the different chemical properties that will 251 00:18:46,000 --> 00:18:50,000 make it interested in terms of acid-base, oxidant-reductant, 252 00:18:50,000 --> 00:18:55,000 electrophile-nucleophile, and acceptor and donor. 253 00:18:55,000 --> 00:19:00,000 And the currency of chemistry can be seen, with reference to 254 00:19:00,000 --> 00:19:05,000 this, to be the electron. That is what chemistry is all 255 00:19:05,000 --> 00:19:08,000 about. And so, we will be talking a 256 00:19:08,000 --> 00:19:13,000 lot about atoms and molecules with reference to their 257 00:19:13,000 --> 00:19:17,000 properties and how the properties stem from knowing 258 00:19:17,000 --> 00:19:21,000 something about the electrons in the molecule. 259 00:19:21,000 --> 00:19:28,000 And I think you are going to find this to be quite fun. 260 00:19:35,000 --> 00:19:38,000 With respect to the properties of the medium, 261 00:19:38,000 --> 00:19:43,000 let's talk about a substance like hydrogen chloride. 262 00:19:48,000 --> 00:19:53,000 This is just to illustrate what I was saying over there. 263 00:19:53,000 --> 00:19:57,000 If you take a molecule like hydrogen chloride, 264 00:19:57,000 --> 00:20:00,000 and it is a gas, of course. 265 00:20:00,000 --> 00:20:04,000 And if you make a solution of it in hexane, 266 00:20:04,000 --> 00:20:10,000 hexane is going to be our solvent, and then what you find 267 00:20:10,000 --> 00:20:16,000 is that in this low polarity medium hexane solution, 268 00:20:16,000 --> 00:20:21,000 liquid hexane, the HCl molecule remains intact 269 00:20:21,000 --> 00:20:27,000 and floats around in solution, interacting weakly with hexane 270 00:20:27,000 --> 00:20:34,000 molecules that surround it. But if you take this HCl 271 00:20:34,000 --> 00:20:40,000 molecule and put it into a solvent like water, 272 00:20:40,000 --> 00:20:47,000 then something on the other end of the continuum transpires 273 00:20:47,000 --> 00:20:53,000 because we get ionization to produce hydrogen ions. 274 00:20:53,000 --> 00:20:59,000 And they go off and are separated in solution from 275 00:20:59,000 --> 00:21:04,000 chloride ions. And we will talk more about 276 00:21:04,000 --> 00:21:09,000 just what is going on when you separate H plus from Cl 277 00:21:09,000 --> 00:21:13,000 minus and let them diffuse apart in aqueous 278 00:21:13,000 --> 00:21:15,000 solution. But you can see, 279 00:21:15,000 --> 00:21:19,000 I think, the dichotomy. Either the proton shares in the 280 00:21:19,000 --> 00:21:24,000 electrons of the chloride, or it just pops off and ionizes 281 00:21:24,000 --> 00:21:28,000 and goes out into solution. And Lewis wanted to understand 282 00:21:28,000 --> 00:21:32,000 this. And, to understand it, 283 00:21:32,000 --> 00:21:37,000 he developed a theory. And his theory was the "cube 284 00:21:37,000 --> 00:21:42,000 theory." In this part we get to draw some cubes. 285 00:21:42,000 --> 00:21:47,000 And he decided that if you thought of the nucleus, 286 00:21:47,000 --> 00:21:53,000 which he calls the kernel, of an atom as being located at 287 00:21:53,000 --> 00:21:59,000 the center of the system, then if you had an atom like 288 00:21:59,000 --> 00:22:05,000 neon, which is a noble gas with eight valance electrons, 289 00:22:05,000 --> 00:22:11,000 that these valance electrons would want to get away from each 290 00:22:11,000 --> 00:22:19,000 other as far as possible because they repel each other. 291 00:22:19,000 --> 00:22:21,000 They are all negatively charged. 292 00:22:21,000 --> 00:22:24,000 This could be, here, the neon atom. 293 00:22:24,000 --> 00:22:28,000 Here, on that cube, is how he would represent the 294 00:22:28,000 --> 00:22:33,000 electronic structure of the neon atom, with the eight electrons 295 00:22:33,000 --> 00:22:37,000 here represented by peach-colored circles, 296 00:22:37,000 --> 00:22:42,000 each the vertex of a cube. So, they got far away from each 297 00:22:42,000 --> 00:22:44,000 other. And you can see that in the 298 00:22:44,000 --> 00:22:48,000 historical archives, some of his original sketch 299 00:22:48,000 --> 00:22:52,000 books containing these ideas are there, and now you will know 300 00:22:52,000 --> 00:22:55,000 what they mean. You will see that he progressed 301 00:22:55,000 --> 00:23:01,000 beyond understanding the atom to understanding the molecule. 302 00:23:01,000 --> 00:23:07,000 And here is one of the molecules that he talks about. 303 00:23:22,000 --> 00:23:28,000 Here we have a molecule containing 14 valance electrons, 304 00:23:28,000 --> 00:23:34,000 all arranged in that manner. And this could be, 305 00:23:34,000 --> 00:23:39,000 for example, the I two molecule. 306 00:23:39,000 --> 00:23:45,000 And let me draw it in terms of a dot structure, 307 00:23:45,000 --> 00:23:46,000 -- 308 00:23:52,000 --> 00:23:55,000 -- like that. And there was known at the 309 00:23:55,000 --> 00:24:01,000 time, partly because of the contributions of Lewis himself, 310 00:24:01,000 --> 00:24:05,000 something called the Rule of Eight. 311 00:24:05,000 --> 00:24:10,000 And that was a reference to this notion that most atoms want 312 00:24:10,000 --> 00:24:14,000 to have eight electrons in their valance shell, 313 00:24:14,000 --> 00:24:20,000 and it is also something that we call today the Octet Rule. 314 00:24:20,000 --> 00:24:25,000 So, when you see the Rule of Eight mentioned in his paper, 315 00:24:25,000 --> 00:24:31,000 it is the familiar Octet Rule. And you can see here that one 316 00:24:31,000 --> 00:24:37,000 of the key features is two electrons shared equally. 317 00:24:37,000 --> 00:24:40,000 And when electrons are shared equally like that, 318 00:24:40,000 --> 00:24:45,000 you have a molecule with symmetrical charge distribution, 319 00:24:45,000 --> 00:24:48,000 charge referring to the electrons where they are in 320 00:24:48,000 --> 00:24:51,000 space. And then, he showed that you 321 00:24:51,000 --> 00:24:55,000 could think about this another way. 322 00:25:05,000 --> 00:25:10,000 You could consider some kind of a geometric distortion of the I 323 00:25:10,000 --> 00:25:12,000 two molecule, like this. 324 00:25:12,000 --> 00:25:17,000 Distorted, not only because of my drawing, but because of the 325 00:25:17,000 --> 00:25:22,000 way the atoms themselves are thought to be rearranging in 326 00:25:22,000 --> 00:25:24,000 this process. 327 00:25:34,000 --> 00:25:39,000 Notice that what has happened here is that the I two 328 00:25:39,000 --> 00:25:44,000 molecule is doing something electronically such that one 329 00:25:44,000 --> 00:25:49,000 iodine is starting to pull away from the other. 330 00:25:49,000 --> 00:25:55,000 This one over here is carrying with it the electron that came 331 00:25:55,000 --> 00:25:58,000 from over here. And, in that case, 332 00:25:58,000 --> 00:26:04,000 what we have is a molecule in which we are developing partial 333 00:26:04,000 --> 00:26:08,000 negative charge on the right-hand side and partial 334 00:26:08,000 --> 00:26:14,000 positive charge on the left-hand side. 335 00:26:14,000 --> 00:26:18,000 As I was talking up here, I was thinking about what I was 336 00:26:18,000 --> 00:26:21,000 going to say here, because the ideal is that 337 00:26:21,000 --> 00:26:25,000 molecules, even if they are inherently non-polar like the I 338 00:26:25,000 --> 00:26:29,000 two molecule, in their equilibrium structure 339 00:26:29,000 --> 00:26:33,000 they can have electron fluctuations that lead to 340 00:26:33,000 --> 00:26:37,000 partial charges in the manner shown here. 341 00:26:37,000 --> 00:26:39,000 And Lewis was working beautifully toward the 342 00:26:39,000 --> 00:26:42,000 development of a theory like this that would allow the 343 00:26:42,000 --> 00:26:45,000 description of electronic structure to be made graphically 344 00:26:45,000 --> 00:26:48,000 apparent. And this is something that 345 00:26:48,000 --> 00:26:51,000 chemists really like to do, is we like to be able to see 346 00:26:51,000 --> 00:26:53,000 stuff. I hope I am going to be able to 347 00:26:53,000 --> 00:26:56,000 show you some really cool stuff this semester. 348 00:26:56,000 --> 00:26:58,000 And, in fact, even some really cool stuff 349 00:26:58,000 --> 00:27:03,000 before we finish here today. So, that is the development of 350 00:27:03,000 --> 00:27:08,000 charge as represented using the Lewis cube theory in an I two 351 00:27:08,000 --> 00:27:12,000 molecule. Next, one thing you could do is 352 00:27:12,000 --> 00:27:17,000 say, let's just continue this process, and the right-hand 353 00:27:17,000 --> 00:27:20,000 iodine with its eight electrons pops off. 354 00:27:20,000 --> 00:27:25,000 That would give you an ionized situation in which you had an I 355 00:27:25,000 --> 00:27:32,000 minus floating away from an I plus molecule. 356 00:27:32,000 --> 00:27:35,000 And that situation is drawn in the notes, and because I am 357 00:27:35,000 --> 00:27:39,000 running out of space on this board I am not going to draw 358 00:27:39,000 --> 00:27:42,000 that one up. Instead I am going to go onto 359 00:27:42,000 --> 00:27:46,000 another triumph of the Lewis cube theory, which was its 360 00:27:46,000 --> 00:27:50,000 ability to explain different chemical bond orders. 361 00:28:02,000 --> 00:28:05,000 By the way, Lewis never got the Nobel Prize. 362 00:28:05,000 --> 00:28:08,000 He certainly should have. A dramatic oversight. 363 00:28:08,000 --> 00:28:13,000 He was born in Massachusetts. He was a Harvard professor for 364 00:28:13,000 --> 00:28:16,000 a while and did not like it, and came to MIT to be a 365 00:28:16,000 --> 00:28:20,000 professor for a while. And, although he liked that, 366 00:28:20,000 --> 00:28:23,000 that was not far enough away from Harvard, 367 00:28:23,000 --> 00:28:27,000 so he went to Berkeley, where he became the department 368 00:28:27,000 --> 00:28:31,000 head and was very successful over a long period of time in 369 00:28:31,000 --> 00:28:37,000 learning about chemistry and in teaching chemistry. 370 00:28:37,000 --> 00:28:40,000 I will invite you, and you will see this in the 371 00:28:40,000 --> 00:28:45,000 notes, too, to go ahead and see if you can find a good biography 372 00:28:45,000 --> 00:28:49,000 of Lewis because it is very instructive. 373 00:28:49,000 --> 00:28:53,000 Anyway, here is another molecule considered by Lewis's 374 00:28:53,000 --> 00:28:55,000 cube theory. 375 00:29:00,000 --> 00:29:05,000 How many electrons are being shared by the two nuclei or 376 00:29:05,000 --> 00:29:09,000 atoms involved? Four electrons shared. 377 00:29:09,000 --> 00:29:15,000 We can circle them here. That is four electrons shared. 378 00:29:15,000 --> 00:29:18,000 Therefore, that is not a single bond. 379 00:29:18,000 --> 00:29:23,000 We call that a double bond. And so, that might be a 380 00:29:23,000 --> 00:29:27,000 representation of, for example, 381 00:29:27,000 --> 00:29:32,000 the O two molecule. Here we have I two, 382 00:29:32,000 --> 00:29:37,000 here we have distorted I two with charges developing, 383 00:29:37,000 --> 00:29:41,000 and here we have O two. O two is a very 384 00:29:41,000 --> 00:29:45,000 interesting diatomic molecule. We are going to talk about that 385 00:29:45,000 --> 00:29:49,000 later in the semester, but for now let's just leave it 386 00:29:49,000 --> 00:29:53,000 at that. But then, even though this was 387 00:29:53,000 --> 00:29:57,000 quite a successful theory, the cube theory, 388 00:29:57,000 --> 00:30:00,000 it has certain problems, certain shortcomings, 389 00:30:00,000 --> 00:30:04,000 such as, we can do single bonds with it quite well, 390 00:30:04,000 --> 00:30:09,000 and now we can do double bonds with the cube theory, 391 00:30:09,000 --> 00:30:13,000 but what do you do if you have to make a triple bond? 392 00:30:13,000 --> 00:30:18,000 That was a problem for Lewis. That should be a problem for 393 00:30:18,000 --> 00:30:21,000 you, too. Cubes just don't fit together 394 00:30:21,000 --> 00:30:24,000 that way. They have edges and faces, 395 00:30:24,000 --> 00:30:29,000 and that is it. And they have vertices. 396 00:30:29,000 --> 00:30:33,000 You can do one vertex. So, triple bond is a problem. 397 00:30:33,000 --> 00:30:37,000 And we know that there are molecules that have triple 398 00:30:37,000 --> 00:30:39,000 bonds. And we cannot handle them with 399 00:30:39,000 --> 00:30:43,000 the cube theory, so we are going to have to 400 00:30:43,000 --> 00:30:46,000 something a little different, for that reason. 401 00:30:46,000 --> 00:30:51,000 But there is also another reason that had to do with just 402 00:30:51,000 --> 00:30:55,000 considering the chemistry of light elements like hydrogen and 403 00:30:55,000 --> 00:30:58,000 helium. Those elements tend to 404 00:30:58,000 --> 00:31:03,000 associate themselves with only two electrons. 405 00:31:03,000 --> 00:31:08,000 And so, Lewis decided, well, maybe the rule of two is 406 00:31:08,000 --> 00:31:14,000 more fundamental than the rule of eight, and that we should be 407 00:31:14,000 --> 00:31:18,000 thinking about pairs of electrons somehow. 408 00:31:18,000 --> 00:31:24,000 Because he looked at what was known about chemistry and 409 00:31:24,000 --> 00:31:29,000 realized that in most molecules, the number of electrons is 410 00:31:29,000 --> 00:31:35,000 always even, is always divisible by two. 411 00:31:35,000 --> 00:31:39,000 That is something interesting about two electrons at a time 412 00:31:39,000 --> 00:31:43,000 being important. You take that together with the 413 00:31:43,000 --> 00:31:47,000 triple bond problem, and Lewis started thinking in 414 00:31:47,000 --> 00:31:51,000 terms of electron pairs, and this is where this 415 00:31:51,000 --> 00:31:55,000 "electron pair theory" comes from. 416 00:32:00,000 --> 00:32:04,000 Although he spent a lot of time on the cube theory, 417 00:32:04,000 --> 00:32:09,000 he was perfectly willing to cast that theory aside in favor 418 00:32:09,000 --> 00:32:14,000 of something that maybe was going to work a little better, 419 00:32:14,000 --> 00:32:18,000 the electron pair theory. And how does that look? 420 00:32:18,000 --> 00:32:23,000 Well, of course, his initial pictures still had 421 00:32:23,000 --> 00:32:28,000 the cube, which just shows that once the human mind fixes on 422 00:32:28,000 --> 00:32:33,000 something, it fixes on it with great tenacity and it can be 423 00:32:33,000 --> 00:32:39,000 hard to shake your way of thinking about things. 424 00:32:39,000 --> 00:32:42,000 But hopefully you will be able to do that. 425 00:32:42,000 --> 00:32:45,000 He still decided, let's arrange these electron 426 00:32:45,000 --> 00:32:50,000 pairs on a cube with the nucleus of the atom supposed to be at 427 00:32:50,000 --> 00:32:54,000 the center, and let's keep these electrons, now, 428 00:32:54,000 --> 00:32:58,000 nicely collected in pairs. And let's get these pairs as 429 00:32:58,000 --> 00:33:03,000 far away from each other as possible, for the same reasons 430 00:33:03,000 --> 00:33:08,000 we used to be putting eight electrons as far away from each 431 00:33:08,000 --> 00:33:13,000 other as possible, namely, electron repulsion. 432 00:33:13,000 --> 00:33:17,000 Now, the problem of electron repulsion between the pairs was 433 00:33:17,000 --> 00:33:20,000 not really solved. And Lewis decided that the pair 434 00:33:20,000 --> 00:33:25,000 theory worked so well that he was not going to worry about 435 00:33:25,000 --> 00:33:27,000 that, and so we won't worry about it yet, 436 00:33:27,000 --> 00:33:31,000 either. You have your four pairs of 437 00:33:31,000 --> 00:33:37,000 electrons arranged at the center of four of the edges of the 438 00:33:37,000 --> 00:33:43,000 cube, and that geometry is what we call a tetrahedron, 439 00:33:43,000 --> 00:33:47,000 which I am drawing the edges of here in pink. 440 00:33:47,000 --> 00:33:52,000 You have a tetrahedral disposition of four pairs of 441 00:33:52,000 --> 00:33:55,000 electrons, now, for an atom. 442 00:33:55,000 --> 00:34:00,000 This might again be the neon atom. 443 00:34:00,000 --> 00:34:11,000 But the nice thing about this choice is that if you want to 444 00:34:11,000 --> 00:34:24,000 you can make single bonds with this theory, and you can make 445 00:34:24,000 --> 00:34:28,000 double bonds -- 446 00:34:33,000 --> 00:34:39,000 -- with this theory, like that. 447 00:34:39,000 --> 00:34:49,000 And then, due to the properties of the tetrahedron, 448 00:34:49,000 --> 00:35:00,000 you can also make triple bonds. This is marvelous. 449 00:35:00,000 --> 00:35:05,000 You can see that the famous chemist Gilbert Newton Lewis was 450 00:35:05,000 --> 00:35:09,000 talking about electronic structure in terms of 451 00:35:09,000 --> 00:35:12,000 symmetrical things, like tetrahedra and cubes, 452 00:35:12,000 --> 00:35:17,000 as a way of arranging electrons reasonably in space. 453 00:35:17,000 --> 00:35:20,000 This could, again, be our iodine molecule. 454 00:35:20,000 --> 00:35:24,000 This could be, now, our O two molecule. 455 00:35:24,000 --> 00:35:29,000 And, if we continue that progression in the Periodic 456 00:35:29,000 --> 00:35:35,000 Table, what is this molecule? Dinitrogen, N two, 457 00:35:35,000 --> 00:35:41,000 the major component of our atmosphere, another interesting 458 00:35:41,000 --> 00:35:47,000 molecule that we will be talking about as the semester progresses 459 00:35:47,000 --> 00:35:51,000 forward. But chemical language and 460 00:35:51,000 --> 00:35:57,000 electronic structure theory are very much still permeated with 461 00:35:57,000 --> 00:36:03,000 this affection for symmetry and the problems that you can solve 462 00:36:03,000 --> 00:36:10,000 using symmetry to analyze electronic structure theory. 463 00:36:10,000 --> 00:36:15,000 Let's talk next about another molecule because we want to talk 464 00:36:15,000 --> 00:36:20,000 about Lewis's development of the electron pair theory, 465 00:36:20,000 --> 00:36:26,000 but also we want to understand how that relates to acid-base 466 00:36:26,000 --> 00:36:29,000 properties. And so, let me draw here 467 00:36:29,000 --> 00:36:32,000 another molecule. 468 00:36:37,000 --> 00:36:41,000 And when you look at this molecule, which is the aluminum 469 00:36:41,000 --> 00:36:45,000 trichloride molecule, in which I am drawing out 470 00:36:45,000 --> 00:36:50,000 explicitly all of the electrons, not forgetting these two. 471 00:36:50,000 --> 00:36:54,000 And having drawn the aluminum trichloride molecule 472 00:36:54,000 --> 00:36:59,000 and looked at it like that, you can ask yourself is the 473 00:36:59,000 --> 00:37:03,000 number of electrons divisible by eight? 474 00:37:03,000 --> 00:37:06,000 Yes it is. We have a 24 valance electron 475 00:37:06,000 --> 00:37:10,000 system here. It is divisible by eight. 476 00:37:10,000 --> 00:37:14,000 Of course, it is also divisible by two. 477 00:37:14,000 --> 00:37:18,000 You can also ask yourself is this molecule, 478 00:37:18,000 --> 00:37:23,000 as written, one that satisfies the rule of eight for all four 479 00:37:23,000 --> 00:37:25,000 of the atoms? No. 480 00:37:25,000 --> 00:37:30,000 We have a problem there because this thing is electron 481 00:37:30,000 --> 00:37:33,000 deficient. 482 00:37:42,000 --> 00:37:45,000 And if you were Lewis, you would want to know, 483 00:37:45,000 --> 00:37:50,000 well, if it is electron deficient, this molecule must be 484 00:37:50,000 --> 00:37:54,000 doing something about that to get more electrons. 485 00:37:54,000 --> 00:37:58,000 Which atom is missing electrons, here? 486 00:37:58,000 --> 00:38:02,000 The aluminum. How can we give aluminum more 487 00:38:02,000 --> 00:38:04,000 electrons, in a structure like this? 488 00:38:04,000 --> 00:38:08,000 Can we get it up to the rule of eight? 489 00:38:13,000 --> 00:38:14,000 Double bonds, awesome. 490 00:38:14,000 --> 00:38:18,000 Beautiful. We can make a double bond. 491 00:38:18,000 --> 00:38:22,000 And, if we do that, we can allow aluminum to 492 00:38:22,000 --> 00:38:27,000 satisfy the rule of eight, or allow the rule of eight to 493 00:38:27,000 --> 00:38:33,000 satisfy aluminum. Whichever way you want to look 494 00:38:33,000 --> 00:38:36,000 at it. And see what we have done, 495 00:38:36,000 --> 00:38:39,000 here? We have taken one of the 496 00:38:39,000 --> 00:38:42,000 electron pairs, say, this one, 497 00:38:42,000 --> 00:38:49,000 and we have moved it in between the aluminum and the chlorine, 498 00:38:49,000 --> 00:38:52,000 so it joins the other one in there. 499 00:38:52,000 --> 00:38:57,000 And we get a double bond. And now, everybody has an 500 00:38:57,000 --> 00:39:02,000 octet. But what is the problem with 501 00:39:02,000 --> 00:39:05,000 that? The problem with that is that 502 00:39:05,000 --> 00:39:08,000 chlorine is very electronegative, 503 00:39:08,000 --> 00:39:13,000 and it does not want its electrons stolen away by the 504 00:39:13,000 --> 00:39:16,000 very electropositive aluminum center. 505 00:39:16,000 --> 00:39:21,000 There are other ways that aluminum can ultimately satisfy 506 00:39:21,000 --> 00:39:27,000 its octet, and this is how we get into the realm of "Lewis 507 00:39:27,000 --> 00:39:32,000 acid-base theory." And I want to show you one of 508 00:39:32,000 --> 00:39:36,000 the other ways that aluminum can satisfy its octet, 509 00:39:36,000 --> 00:39:41,000 and then, we are going to move to the computer so we can 510 00:39:41,000 --> 00:39:44,000 visualize some of these properties. 511 00:39:44,000 --> 00:39:49,000 If I put my aluminum here -- and do you remember this 512 00:39:49,000 --> 00:39:52,000 molecule up here, the ammonia molecule? 513 00:39:52,000 --> 00:39:57,000 I am going to say that if I draw that ammonia molecule in 514 00:39:57,000 --> 00:40:00,000 place, here -- 515 00:40:05,000 --> 00:40:10,000 The ammonia molecule comes in, and it has its eight electrons. 516 00:40:10,000 --> 00:40:13,000 It is sharing six of them with three hydrogens. 517 00:40:13,000 --> 00:40:18,000 The idea is that it has an extra pair of electrons on that 518 00:40:18,000 --> 00:40:23,000 nitrogen in the ammonia molecule, that it can share with 519 00:40:23,000 --> 00:40:26,000 the aluminum. And now we go ahead and 520 00:40:26,000 --> 00:40:30,000 complete the picture. And we can have eight electrons 521 00:40:30,000 --> 00:40:33,000 around everybody. 522 00:40:38,000 --> 00:40:42,000 And so the rule of eight is now satisfied for the three 523 00:40:42,000 --> 00:40:46,000 chlorines, for the aluminum, and for the nitrogen of the 524 00:40:46,000 --> 00:40:50,000 ammonia molecule. The ammonia molecule is what we 525 00:40:50,000 --> 00:40:53,000 call a "Lewis base." 526 00:40:58,000 --> 00:41:03,000 And the aluminum trichloride molecule is what we 527 00:41:03,000 --> 00:41:08,000 call a "Lewis acid," for reasons that should now be 528 00:41:08,000 --> 00:41:12,000 quite clear. And I want to show you how we 529 00:41:12,000 --> 00:41:17,000 can look at these things. And if you will give me just a 530 00:41:17,000 --> 00:41:22,000 second here, I am going to load the aluminum trichloride 531 00:41:22,000 --> 00:41:26,000 molecule up onto the screen. 532 00:41:33,000 --> 00:41:38,000 What we are going to do is remember that there are lots of 533 00:41:38,000 --> 00:41:42,000 different ways in which you can visualize molecules. 534 00:41:42,000 --> 00:41:48,000 And I want to show you some of the more interesting ways. 535 00:42:26,000 --> 00:42:33,000 All that is is a picture of the aluminum trichloride 536 00:42:33,000 --> 00:42:40,000 molecule with spheres drawn at kind of arbitrary radii. 537 00:42:40,000 --> 00:42:45,000 The size of these spheres is not representative of any 538 00:42:45,000 --> 00:42:51,000 particular physical quantity, but we can change that. 539 00:42:51,000 --> 00:42:56,000 And so now, what we are going to do is draw the thing a 540 00:42:56,000 --> 00:43:02,000 slightly different way. And what you can see is that 541 00:43:02,000 --> 00:43:07,000 the positions of those nuclei are in this flat box. 542 00:43:07,000 --> 00:43:13,000 I made the box kind of flat. It is kind of a slab because 543 00:43:13,000 --> 00:43:19,000 this AlCl three molecule is conveniently kind of 544 00:43:19,000 --> 00:43:24,000 flat in its structure. And what are we going to do 545 00:43:24,000 --> 00:43:28,000 now? We are going to draw a contour 546 00:43:28,000 --> 00:43:31,000 surface. And I like this. 547 00:43:31,000 --> 00:43:34,000 We are going to use the solid surface method, 548 00:43:34,000 --> 00:43:37,000 first. And can you see that now? 549 00:43:37,000 --> 00:43:41,000 These curves that enclose the four nuclei of the aluminum 550 00:43:41,000 --> 00:43:45,000 trichloride molecule do have some physical 551 00:43:45,000 --> 00:43:49,000 significance, because what I have done here 552 00:43:49,000 --> 00:43:53,000 is taken results, in this case from the quantum 553 00:43:53,000 --> 00:43:57,000 chemistry calculation, but you could also take it from 554 00:43:57,000 --> 00:44:03,000 an X-ray crystallographic structure determination study. 555 00:44:03,000 --> 00:44:06,000 And I have drawn a three-dimensional contour map. 556 00:44:06,000 --> 00:44:11,000 The value of the electron density at every point on the 557 00:44:11,000 --> 00:44:14,000 surface of one of those ovaloid shapes is the same. 558 00:44:14,000 --> 00:44:19,000 Just like when you have a contour map to describe in two 559 00:44:19,000 --> 00:44:22,000 dimensions an interesting complicated surface, 560 00:44:22,000 --> 00:44:27,000 we can do this in three dimensions as well. 561 00:44:27,000 --> 00:44:30,000 And one of the things you notice, when you look at a 562 00:44:30,000 --> 00:44:33,000 surface like this, is that the value of the 563 00:44:33,000 --> 00:44:37,000 electron density actually goes down to some low value in 564 00:44:37,000 --> 00:44:39,000 between the nuclei, for this. 565 00:44:39,000 --> 00:44:43,000 When you see molecules represented as balls and sticks, 566 00:44:43,000 --> 00:44:47,000 or if you represent molecules this way, just showing a pair of 567 00:44:47,000 --> 00:44:51,000 dots between the aluminum and chloride, you may not be getting 568 00:44:51,000 --> 00:44:56,000 a physically complete picture of the situation. 569 00:44:56,000 --> 00:44:59,000 You can get a much more complete picture if you have 570 00:44:59,000 --> 00:45:02,000 access to the actual electron density. 571 00:45:02,000 --> 00:45:06,000 And then, you can even go a little further, 572 00:45:06,000 --> 00:45:09,000 and I want to show you something very cool. 573 00:45:09,000 --> 00:45:14,000 First I am going to need to load in a second molecule. 574 00:45:19,000 --> 00:45:22,000 And that will be the product of the first "Lewis acid-base 575 00:45:22,000 --> 00:45:25,000 reaction" that we have discussed. 576 00:45:25,000 --> 00:45:29,000 Because, I didn't say it over there, but that was your first 577 00:45:29,000 --> 00:45:33,000 exposure to a Lewis acid-base reaction, in which the ammonia 578 00:45:33,000 --> 00:45:36,000 molecule comes in and binds to the aluminum trichloride 579 00:45:36,000 --> 00:45:40,000 molecule, in order to satisfy the valence 580 00:45:40,000 --> 00:45:44,000 requirements of the respective atom types. 581 00:45:44,000 --> 00:45:47,000 And so, here we are going to look at that molecule, 582 00:45:47,000 --> 00:45:51,000 and we are going to look at its electron density. 583 00:46:00,000 --> 00:46:04,000 And I think you are going to like this very much. 584 00:46:26,000 --> 00:46:29,000 Here it comes. And then I am going to 585 00:46:29,000 --> 00:46:33,000 represent this as a solid surface. 586 00:46:33,000 --> 00:46:38,000 The value of the electron density everywhere on this 587 00:46:38,000 --> 00:46:42,000 surface is 0.1 electron density units. 588 00:46:42,000 --> 00:46:48,000 I want you to start thinking about how that shape appears 589 00:46:48,000 --> 00:46:53,000 there because I am going to underscore that a little bit 590 00:46:53,000 --> 00:46:59,000 more in just a second. But one thing you should notice 591 00:46:59,000 --> 00:47:04,000 is that at the NH three molecule, which is pictured at 592 00:47:04,000 --> 00:47:10,000 the top of that representation, what you are seeing is that the 593 00:47:10,000 --> 00:47:15,000 value of the electron density does not get very small as you 594 00:47:15,000 --> 00:47:19,000 go between the nitrogen and hydrogen nuclei because both 595 00:47:19,000 --> 00:47:25,000 nitrogen and hydrogen are quite similar in electronegativity as 596 00:47:25,000 --> 00:47:30,000 compared with the aluminum atom in this system. 597 00:47:38,000 --> 00:47:46,000 The fascinating thing about illustrating a molecule in this 598 00:47:46,000 --> 00:47:55,000 way is that we can actually associate another property with 599 00:47:55,000 --> 00:48:02,000 the color on the surface. Now what we are doing is 600 00:48:02,000 --> 00:48:06,000 looking at the aluminum trichloride ammonia system. 601 00:48:06,000 --> 00:48:10,000 And let me see if I can make this thing gradually spin, 602 00:48:10,000 --> 00:48:15,000 so that I can talk about it without being pinned to my 603 00:48:15,000 --> 00:48:18,000 computer. What we have on the surface on 604 00:48:18,000 --> 00:48:23,000 each of these electron density isosurface enclosed regions is a 605 00:48:23,000 --> 00:48:28,000 color that corresponds with a value of a function that tells 606 00:48:28,000 --> 00:48:33,000 us about the propensity of electrons to be paired at that 607 00:48:33,000 --> 00:48:38,000 point in space. The Lewis theory is now colored 608 00:48:38,000 --> 00:48:42,000 onto the electron density isosurface of this Lewis acid, 609 00:48:42,000 --> 00:48:47,000 Lewis base complex molecule. And the values that correspond 610 00:48:47,000 --> 00:48:52,000 to those regions in space where electrons are most likely to be 611 00:48:52,000 --> 00:48:54,000 found paired up are colored blue. 612 00:48:54,000 --> 00:48:59,000 Where they are least likely to be found paired up are colored 613 00:48:59,000 --> 00:49:02,000 kind of red-orange, here. 614 00:49:02,000 --> 00:49:05,000 And then an intermediate color is this green. 615 00:49:05,000 --> 00:49:09,000 And so, you can see that you have electron pairs associated 616 00:49:09,000 --> 00:49:12,000 with each of the three NH bonds, up at the top. 617 00:49:12,000 --> 00:49:16,000 You have another electron pair here in blue, 618 00:49:16,000 --> 00:49:19,000 which is very proximate to this aluminum center, 619 00:49:19,000 --> 00:49:24,000 that is very electron deficient as we had found right over here 620 00:49:24,000 --> 00:49:27,000 because it lacks an octet. And then, each of these 621 00:49:27,000 --> 00:49:32,000 chlorines is able to attract electron pairs. 622 00:49:32,000 --> 00:49:34,000 Because chlorine is very electronegative, 623 00:49:34,000 --> 00:49:39,000 it attracts the electron pairs to itself and sort of withholds 624 00:49:39,000 --> 00:49:43,000 them from the aluminum center, but yet, that development of 625 00:49:43,000 --> 00:49:47,000 charge separation keeps everything together in what we 626 00:49:47,000 --> 00:49:51,000 can call an ionic interaction, an electrostatic interaction. 627 00:49:51,000 --> 00:49:55,000 You can see here covalent bonding, donor-acceptor complex 628 00:49:55,000 --> 00:50:00,000 formation, and electrostatic contributions to bonding. 629 00:50:00,000 --> 00:50:03,000 And all of this is just an illustration of the brilliant 630 00:50:03,942 --> 00:50:06,000 ideas of Gilbert Newton Lewis.