1 00:00:00 --> 00:00:01 2 00:00:01 --> 00:00:02 The following content is provided under a Creative 3 00:00:02 --> 00:00:03 Commons license. 4 00:00:03 --> 00:00:06 Your support will help MIT OpenCourseWare continue to 5 00:00:06 --> 00:00:10 offer high-quality educational resources for free. 6 00:00:10 --> 00:00:13 To make a donation or view additional materials from 7 00:00:13 --> 00:00:15 hundreds of MIT courses, visit MIT OpenCourseWare 8 00:00:15 --> 00:00:17 at ocw.mit.edu. 9 00:00:17 --> 00:00:23 PROFESSOR: OK, everyone, pay attention to the 10 00:00:23 --> 00:00:24 clicker question. 11 00:00:24 --> 00:00:27 If you haven't responded, now's a good time to 12 00:00:27 --> 00:00:46 click in your response. 13 00:00:46 --> 00:01:04 All right, let's just take 10 more seconds. 14 00:01:04 --> 00:01:13 OK, we can do better than this. 15 00:01:13 --> 00:01:17 So, tetrahedral complexes. 16 00:01:17 --> 00:01:21 Do you recall tetrahedral complexes with angles of 17 00:01:21 --> 00:01:24 what between the ligands? 18 00:01:24 --> 00:01:25 109 . 19 00:01:25 --> 00:01:28 5. 20 00:01:28 --> 00:01:33 The ligands' negative point charges aren't facing any of 21 00:01:33 --> 00:01:36 the d orbitals perfectly. 22 00:01:36 --> 00:01:40 They're a little bit closer to the orbitals that are 45 23 00:01:40 --> 00:01:44 degrees off-axis, so those three are the most repelled. 24 00:01:44 --> 00:01:48 But they're not really directly hitting any of them. 25 00:01:48 --> 00:01:51 So that's in contrast with the octahedral system or square 26 00:01:51 --> 00:01:54 planar where the ligands negative point charges are 27 00:01:54 --> 00:01:56 headed directly toward some of the d orbitals. 28 00:01:56 --> 00:02:01 So because the ligands in a tetrahedral case are not headed 29 00:02:01 --> 00:02:05 directly toward any of the d orbitals, there is not a huge 30 00:02:05 --> 00:02:09 amount of crystal fields splitting, so that's small. 31 00:02:09 --> 00:02:13 And so, when the splitting is small, then you tend to 32 00:02:13 --> 00:02:16 have high spin systems. 33 00:02:16 --> 00:02:19 So you put in all of the electrons singly to the fullest 34 00:02:19 --> 00:02:23 extent of the orbital as possible before you pair. 35 00:02:23 --> 00:02:26 And so, since you put them in singly for the fullest extent 36 00:02:26 --> 00:02:30 possible before you pair them up, that will lead to a high 37 00:02:30 --> 00:02:33 spin system, which is the maximum number of 38 00:02:33 --> 00:02:34 unpaired electrons. 39 00:02:34 --> 00:02:41 So today is then the last lecture on transition metals, 40 00:02:41 --> 00:02:44 and we've been talking about crystal field theory, and today 41 00:02:44 --> 00:02:48 we're going to talk about colors and crystal 42 00:02:48 --> 00:02:50 field theory. 43 00:02:50 --> 00:02:58 So, colors, there are a lot of beautiful colors in nature, and 44 00:02:58 --> 00:03:01 some of the beautiful colors you find in nature have to do 45 00:03:01 --> 00:03:08 with transition metals or other liganded states. 46 00:03:08 --> 00:03:12 So, we're going to start with an example of how colors can 47 00:03:12 --> 00:03:15 change, how a molecule's color can depend on its oxidation 48 00:03:15 --> 00:03:19 state, how a molecule's color can depend on its 49 00:03:19 --> 00:03:20 liganded state. 50 00:03:20 --> 00:03:27 So, Dr. Taylor is going to be doing this for you -- should we 51 00:03:27 --> 00:03:30 do it the demo and then look at the questions or do 52 00:03:30 --> 00:03:31 the questions first? 53 00:03:31 --> 00:03:32 Demo first? 54 00:03:32 --> 00:03:36 PROFESSOR: OK. 55 00:03:36 --> 00:03:39 PROFESSOR: So, here are some of the reactions up on the 56 00:03:39 --> 00:03:43 Powerpoint that you're going to be looking at, and as the 57 00:03:43 --> 00:03:46 reaction proceeds, there's going to be changes in 58 00:03:46 --> 00:03:50 oxidation state, and also changes in ligand in state, and 59 00:03:50 --> 00:03:52 that will lead to changes in color. 60 00:03:52 --> 00:04:49 [DEMONSTRATION] 61 00:04:49 --> 00:04:58 PROFESSOR: So, how would you describe that first color? 62 00:04:58 --> 00:04:59 Any predictions? 63 00:04:59 --> 00:05:01 Have any of you seen this before, what's going 64 00:05:01 --> 00:05:19 to happen next? 65 00:05:19 --> 00:05:19 [DEMONSTRATION] 66 00:05:19 --> 00:05:36 PROFESSOR: So this is called an oscillating clock reaction, so 67 00:05:36 --> 00:05:56 as it runs through, it cycles between the different colors. 68 00:05:56 --> 00:06:01 So, that should happily keep going, and we can consider 69 00:06:01 --> 00:06:02 what's happening. 70 00:06:02 --> 00:06:05 So here's the overall reaction here and it can be divided 71 00:06:05 --> 00:06:07 into two components. 72 00:06:07 --> 00:06:13 So, why don't you tell me, what is happening to iodide in that 73 00:06:13 --> 00:07:08 first reaction, and there it is again. 74 00:07:08 --> 00:07:23 All right, so let's take 10 more seconds. 75 00:07:23 --> 00:07:25 Very good. 76 00:07:25 --> 00:07:29 So, if you looked up here, you see that you have minus 2 for 77 00:07:29 --> 00:07:33 the oxygen, three of them, minus 6, and it needs to equal 78 00:07:33 --> 00:07:36 minus 1, so you have plus 5. 79 00:07:36 --> 00:07:40 And then over here, we again have plus 1 minus 2, and 80 00:07:40 --> 00:07:42 so that has to be plus 1. 81 00:07:42 --> 00:07:47 So that was actually a quiz question, but you score three 82 00:07:47 --> 00:07:51 points if you answered, even if you got it wrong, but we could 83 00:07:51 --> 00:07:54 have had that four points, most people got that right anyway. 84 00:07:54 --> 00:07:58 But if you answered, you get an extra few points on that one. 85 00:07:58 --> 00:08:01 All right, so very good. 86 00:08:01 --> 00:08:03 That's what's happening to iodide. 87 00:08:03 --> 00:08:07 Now you notice that in this reaction h o i is being 88 00:08:07 --> 00:08:09 produced, and then in the second step it's 89 00:08:09 --> 00:08:12 being consumed. 90 00:08:12 --> 00:08:16 This later reaction can be divided, then, into two 91 00:08:16 --> 00:08:20 additional reactions. 92 00:08:20 --> 00:08:24 And one of the reactions, you can tell me again what is 93 00:08:24 --> 00:08:26 happening, what is being oxidized and what is being 94 00:08:26 --> 00:09:09 reduced in this part of the reaction. 95 00:09:09 --> 00:09:22 OK, let's take 10 more seconds. 96 00:09:22 --> 00:09:23 Excellent. 97 00:09:23 --> 00:09:26 Even a little higher than before. 98 00:09:26 --> 00:09:29 All right, so you figured out that this was the plus 1, this 99 00:09:29 --> 00:09:31 is minus 1, and they're both going to 0. 100 00:09:31 --> 00:09:35 So you have oxidation and reduction going on 101 00:09:35 --> 00:09:41 all involving iodide in that reaction. 102 00:09:41 --> 00:09:45 OK, so as the reaction was proceeding, you could see that 103 00:09:45 --> 00:09:49 it started out with clear and then it went to sort of amber 104 00:09:49 --> 00:09:53 color, and that was the i 2, the clear was i minus, and the 105 00:09:53 --> 00:09:56 sort of darker blue color that you saw is the complex with 106 00:09:56 --> 00:09:58 starch in the reaction. 107 00:09:58 --> 00:10:02 So that both of these guys have colors independent, but then 108 00:10:02 --> 00:10:04 when they're liganded to something else, the 109 00:10:04 --> 00:10:05 color is different. 110 00:10:05 --> 00:10:09 And that's very true with coordination complexes that 111 00:10:09 --> 00:10:13 the metal by itself will be strongly influenced 112 00:10:13 --> 00:10:14 by what the ligands are. 113 00:10:14 --> 00:10:17 And depending on what type of ligands it has, it can have a 114 00:10:17 --> 00:10:21 really entirely different color than it had before. 115 00:10:21 --> 00:10:24 So, today we're going to talk about why that's true, and how 116 00:10:24 --> 00:10:27 you can predict colors based on what type of ligand is bound 117 00:10:27 --> 00:10:30 to a transition metal. 118 00:10:30 --> 00:10:34 So, a lot of transition metals have really beautiful colors, 119 00:10:34 --> 00:10:38 and my laboratory studies metals bound to proteins, and 120 00:10:38 --> 00:10:41 often the proteins will have really beautiful colors because 121 00:10:41 --> 00:10:45 of the metal cofactor involved, and that's one of the things 122 00:10:45 --> 00:10:48 that I liked about that particular area of study 123 00:10:48 --> 00:10:52 is just how beautiful these proteins can be. 124 00:10:52 --> 00:10:56 So, the color given off depends on the nature of the metal, and 125 00:10:56 --> 00:10:57 depends on the nature of the ligand. 126 00:10:57 --> 00:11:01 And so we can use crystal field theory, which again, is a very 127 00:11:01 --> 00:11:06 simplified theory, to try to predict or explain 128 00:11:06 --> 00:11:08 the observed colors. 129 00:11:08 --> 00:11:14 And so again, this is not always very precise, but given, 130 00:11:14 --> 00:11:17 if you're told information out of color, you can rationalize 131 00:11:17 --> 00:11:20 why that would be true, and you can also predict at least a 132 00:11:20 --> 00:11:22 range of color that you would have under certain 133 00:11:22 --> 00:11:23 circumstances. 134 00:11:23 --> 00:11:28 So, let's take a look at this more. 135 00:11:28 --> 00:11:30 So the ligands again, have the ability to split 136 00:11:30 --> 00:11:31 those d orbitals. 137 00:11:31 --> 00:11:33 And when we're talking about for metals, it's 138 00:11:33 --> 00:11:35 all about the d orbitals. 139 00:11:35 --> 00:11:38 And we talked already about strong field ligands and weak 140 00:11:38 --> 00:11:41 field ligands, and we're going to talk more about that today, 141 00:11:41 --> 00:11:43 but this time in terms of color. 142 00:11:43 --> 00:11:47 So a strong field ligand, as we discussed, creates a big 143 00:11:47 --> 00:11:51 splitting in the d orbital energy, whereas weak field 144 00:11:51 --> 00:11:55 ligand, like the first question you had today with tetrahedral 145 00:11:55 --> 00:11:59 complexes, there's usually a weak field there, so we have a 146 00:11:59 --> 00:12:05 small energy separation between the d orbitals. 147 00:12:05 --> 00:12:07 So here is something that you actually have to memorize -- 148 00:12:07 --> 00:12:11 there's not much memorization in this course, but you do need 149 00:12:11 --> 00:12:15 to memorize these six ligands in terms of their ability 150 00:12:15 --> 00:12:18 to split d orbitals. 151 00:12:18 --> 00:12:21 So, on the side, we have three that are strong field ligands, 152 00:12:21 --> 00:12:28 cyanide, c o, and ammonia, and so those are going to be strong 153 00:12:28 --> 00:12:30 field, so they're going to have big splitting energy, and so 154 00:12:30 --> 00:12:32 they'll tend to be low spin. 155 00:12:32 --> 00:12:36 Then we have three that are sort of in between that are 156 00:12:36 --> 00:12:40 intermediate field -- water, hydroxide and f minus. 157 00:12:40 --> 00:12:45 And so, in comparing, those are intermediate, so you're going 158 00:12:45 --> 00:12:48 to be asked questions such as how does that compare to a 159 00:12:48 --> 00:12:51 weak field, how does that compare to a strong field. 160 00:12:51 --> 00:12:55 And then our weak field ligands or a lot of our halides down 161 00:12:55 --> 00:12:59 here, i minus, b r minus, c l minus. 162 00:12:59 --> 00:13:03 And so those are weak field ligands, so you'll have a small 163 00:13:03 --> 00:13:09 splitting, so they'll tend to be in high spin complexes. 164 00:13:09 --> 00:13:16 So let's take a look at some examples. 165 00:13:16 --> 00:13:21 So we talked about iron before in complexes, and now we can 166 00:13:21 --> 00:13:26 consider two cases where we have iron plus 3, so the same 167 00:13:26 --> 00:13:30 metal in the same oxidation state, but it has 168 00:13:30 --> 00:13:30 different ligands. 169 00:13:30 --> 00:13:35 It So in one case you have a high spin system with six water 170 00:13:35 --> 00:13:38 ligands, and then the other in a low spin system with 171 00:13:38 --> 00:13:40 six cyanide ligands. 172 00:13:40 --> 00:13:43 So first, before you do anything else with this, you 173 00:13:43 --> 00:13:46 always have to think about what the d count is. 174 00:13:46 --> 00:13:50 So, to do the d count, we're going to look at where iron is 175 00:13:50 --> 00:13:53 in the periodic table, and we're going to see 176 00:13:53 --> 00:13:56 it's in group 8. 177 00:13:56 --> 00:14:01 And then, we'll have 8 minus 3, the oxidation 178 00:14:01 --> 00:14:08 number is d 5 system. 179 00:14:08 --> 00:14:12 So now we have two diagrams here, one has a big splitting, 180 00:14:12 --> 00:14:15 one has a small splitting, and why don't you fill in for me in 181 00:14:15 --> 00:14:18 a clicker question, what the high spin system 182 00:14:18 --> 00:14:19 would look like. 183 00:14:19 --> 00:15:15 OK, let's just take 10 more seconds. 184 00:15:15 --> 00:15:17 Very good. 185 00:15:17 --> 00:15:20 I think that's one of our highest numbers in a while. 186 00:15:20 --> 00:15:23 That's right, so we're going to fill to the fullest extent 187 00:15:23 --> 00:15:30 possible before we pair any of the electrons. 188 00:15:30 --> 00:15:34 So again, here we put in electrons down here, and then 189 00:15:34 --> 00:15:37 go up here, because the splitting is small, so it 190 00:15:37 --> 00:15:41 doesn't take that much energy to put an electron in the upper 191 00:15:41 --> 00:15:43 orbitals, it takes more energy to pair the electrons for 192 00:15:43 --> 00:15:45 this weak field system. 193 00:15:45 --> 00:15:49 And so, this is a high spin case, we have a maximum number 194 00:15:49 --> 00:15:51 of unpaired electrons. 195 00:15:51 --> 00:15:55 So, over here when we have a much bigger splitting energy, 196 00:15:55 --> 00:15:58 it's going to take a lot more energy to put electrons up 197 00:15:58 --> 00:16:01 there, and so we're going to fill up all of these orbitals 198 00:16:01 --> 00:16:05 down here until we have to put an electron up there. 199 00:16:05 --> 00:16:09 So, if we do that, put in the three, and now we're going to 200 00:16:09 --> 00:16:12 pair, because it takes less energy to pair than it does to 201 00:16:12 --> 00:16:16 put an electron up there, so we do four and five. 202 00:16:16 --> 00:16:22 And so then here is our system where we have a strong field, 203 00:16:22 --> 00:16:26 and so here's a weak field and it's going to be high spin, 204 00:16:26 --> 00:16:28 maximum number of unpaired electrons, here we have the 205 00:16:28 --> 00:16:32 strong field and it'll be low spin, the minimum number 206 00:16:32 --> 00:16:35 of unpaired electrons. 207 00:16:35 --> 00:16:40 And we're doing this, again, because we know that cyanide is 208 00:16:40 --> 00:16:44 a strong field ligand, whereas water is an intermediate 209 00:16:44 --> 00:16:49 field ligand, it's a lot weaker than cyanide. 210 00:16:49 --> 00:16:51 OK, now we can continue doing some of the things that 211 00:16:51 --> 00:16:52 we've done before. 212 00:16:52 --> 00:16:56 So just to review this material, we can write the d 213 00:16:56 --> 00:16:58 n electron configurations. 214 00:16:58 --> 00:17:02 What are the orbitals called that are down here? 215 00:17:02 --> 00:17:04 Yup, t 2 g. 216 00:17:04 --> 00:17:08 And how many electrons do we have there? three. 217 00:17:08 --> 00:17:14 And then the e g system up here with two electrons. 218 00:17:14 --> 00:17:17 And over here what do we have? 219 00:17:17 --> 00:17:21 Yup, t 2 g to the 5. 220 00:17:21 --> 00:17:24 So, a review, electron configurations, these are just 221 00:17:24 --> 00:17:28 shorthand notations, which tell people what these 222 00:17:28 --> 00:17:32 diagrams look like. 223 00:17:32 --> 00:17:36 Then, we also talked about this before. 224 00:17:36 --> 00:17:42 So, what does this term stand for? 225 00:17:42 --> 00:17:47 Crystal field stabilization energy, right. 226 00:17:47 --> 00:17:49 So now why don't you tell me what it is for the 227 00:17:49 --> 00:18:15 high spin system. 228 00:18:15 --> 00:18:29 OK, let's just take 10 more seconds. 229 00:18:29 --> 00:18:34 Yup, zero. 230 00:18:34 --> 00:18:40 So if we look at that, we have three electrons down here, so 231 00:18:40 --> 00:18:46 that's minus 2/5, two electrons up here, which is plus 3/5, so 232 00:18:46 --> 00:18:53 3 times minus 2/5 is minus 6/5, plus 6/5 gives you 0. 233 00:18:53 --> 00:18:56 So here is a case where you really don't have 234 00:18:56 --> 00:18:58 much stabilization. 235 00:18:58 --> 00:19:02 It would be equivalent then, so there's zero stabilization 236 00:19:02 --> 00:19:06 because you have three electrons down and two up. 237 00:19:06 --> 00:19:11 All right, so what about the low spin system now? 238 00:19:11 --> 00:19:13 So if we can look at that, what are we going to 239 00:19:13 --> 00:19:18 have for this system? 240 00:19:18 --> 00:19:24 So, we have 5 times minus 2/5 or minus 10/5, and we also have 241 00:19:24 --> 00:19:30 two pairing energy terms there, which we can write in, because 242 00:19:30 --> 00:19:33 there are two sets that are paired. 243 00:19:33 --> 00:19:38 So this is mostly review on what we've had before, and we 244 00:19:38 --> 00:19:40 haven't talked about some of these things in a little while, 245 00:19:40 --> 00:19:43 so we go over it again, and now we're going to take it a next 246 00:19:43 --> 00:19:48 step and think about what sort of wavelength would be absorbed 247 00:19:48 --> 00:19:51 if you're going to promote some of these electrons to 248 00:19:51 --> 00:19:54 unfilled orbitals. 249 00:19:54 --> 00:19:57 So what about the light absorbed by these octahedral 250 00:19:57 --> 00:20:00 coordination complexes? 251 00:20:00 --> 00:20:02 So, if you remember back to the beginning of the course, a 252 00:20:02 --> 00:20:07 physics course or high school, a substance absorbs photons of 253 00:20:07 --> 00:20:11 light if the energy of the photons match the energy 254 00:20:11 --> 00:20:14 required to excite those electrons to a higher 255 00:20:14 --> 00:20:16 energy level. 256 00:20:16 --> 00:20:20 And so now we are doing some review from the first part of 257 00:20:20 --> 00:20:21 the course, which is always good. 258 00:20:21 --> 00:20:25 As I mentioned, everything kind of comes together and we need 259 00:20:25 --> 00:20:28 to go over everything for the final, but there's also 260 00:20:28 --> 00:20:30 connections between all the different parts 261 00:20:30 --> 00:20:32 of the semester. 262 00:20:32 --> 00:20:34 So this should look familiar to you. 263 00:20:34 --> 00:20:37 So, the energy of the absorbed light equals Planck's constant 264 00:20:37 --> 00:20:40 times the frequency of that light. 265 00:20:40 --> 00:20:44 But now we can make that equal to another term, a term we've 266 00:20:44 --> 00:20:47 been talking about in this unit, and that is our 267 00:20:47 --> 00:20:50 octahedral crystal field splitting energy. 268 00:20:50 --> 00:20:53 Because the energy that's going to be required to bump an 269 00:20:53 --> 00:20:57 electron from here to here is that energy, that 270 00:20:57 --> 00:20:58 splitting energy. 271 00:20:58 --> 00:21:04 So that's going to be equal to this term here. 272 00:21:04 --> 00:21:08 OK, so what does this mean in terms of the wavelengths of 273 00:21:08 --> 00:21:14 lights absorbed by different coordination complexes. 274 00:21:14 --> 00:21:16 So we can think about that. 275 00:21:16 --> 00:21:20 So if you have high frequency of light is absorbed, the 276 00:21:20 --> 00:21:25 wavelength of the absorbed light is going to be short. 277 00:21:25 --> 00:21:28 And we know that relationship -- again, think back to the 278 00:21:28 --> 00:21:30 beginning of the course and also probably to physics and to 279 00:21:30 --> 00:21:34 high school, we know a very handy equation for telling us 280 00:21:34 --> 00:21:38 about the relationship of frequency and wavelength of 281 00:21:38 --> 00:21:41 light, so we have the speed of light equals the wavelength 282 00:21:41 --> 00:21:43 times the frequency. 283 00:21:43 --> 00:21:46 So if you have a high frequency of light absorbed, the absorbed 284 00:21:46 --> 00:21:51 wavelength is going to be short. 285 00:21:51 --> 00:21:54 So, let's look at a couple of examples, the example here, 286 00:21:54 --> 00:21:56 going back to our example. 287 00:21:56 --> 00:22:00 So we had this high spin system with water, and now I'm telling 288 00:22:00 --> 00:22:06 you that the splitting energy is 171 kilojoules per mole, and 289 00:22:06 --> 00:22:10 when you have cyanide as your ligand, your splitting energy 290 00:22:10 --> 00:22:13 is 392 kilojoules per mole. 291 00:22:13 --> 00:22:15 Again, this was a stronger field ligand, so we have a 292 00:22:15 --> 00:22:17 bigger splitting energy. 293 00:22:17 --> 00:22:21 And this was an intermediate field ligand, certainly weaker 294 00:22:21 --> 00:22:25 than cyanide, so this has a smaller splitting energy. 295 00:22:25 --> 00:22:29 So, from these values now, we can calculate the wavelength 296 00:22:29 --> 00:22:32 of absorbed light. 297 00:22:32 --> 00:22:36 So for the high spin system first, we can rearrange these 298 00:22:36 --> 00:22:40 equations, which you know well, to come up with the rearranged 299 00:22:40 --> 00:22:44 equation, the wavelength equals Planck's constant times the 300 00:22:44 --> 00:22:48 speed of light, and divided by e, and this time our e is that 301 00:22:48 --> 00:22:51 crystal field splitting energy. 302 00:22:51 --> 00:22:54 So we can put in these terms. 303 00:22:54 --> 00:22:59 So we have Planck's constant times the speed of light over 304 00:22:59 --> 00:23:03 our octahedral field splitting energy, oh, but then we 305 00:23:03 --> 00:23:04 have some other terms here. 306 00:23:04 --> 00:23:07 Now one thing that you have to pay attention to in 307 00:23:07 --> 00:23:09 this unit is your units. 308 00:23:09 --> 00:23:14 So, splitting energies are often given in kilojoules per 309 00:23:14 --> 00:23:18 mole, whereas you often see Planck's constant in joules, so 310 00:23:18 --> 00:23:21 we want to make sure that we convert one or the other, and 311 00:23:21 --> 00:23:25 here it's set up to convert the kilojoules to joules. 312 00:23:25 --> 00:23:28 And also, we want our final unit, we're talking about 313 00:23:28 --> 00:23:32 wavelengths, in meters or nanometers, so we need to 314 00:23:32 --> 00:23:35 get rid of this mole term, and we use Avagadro's 315 00:23:35 --> 00:23:38 number to do that. 316 00:23:38 --> 00:23:40 So now we should be able to cancel our units and 317 00:23:40 --> 00:23:42 get the correct units. 318 00:23:42 --> 00:23:47 So we should be able to cancel the seconds over here, and we 319 00:23:47 --> 00:23:50 should also be able to go in and cancel our moles. 320 00:23:50 --> 00:23:55 We should be able to cancel the joules and the kilojoules out, 321 00:23:55 --> 00:23:59 and that should leave us just with this over here, 322 00:23:59 --> 00:24:01 which is meters. 323 00:24:01 --> 00:24:02 So this is 7 . 324 00:24:02 --> 00:24:06 0 0 times 10 to the minus 7 meters. 325 00:24:06 --> 00:24:11 Does that make sense in terms of a wavelength of light? 326 00:24:11 --> 00:24:16 Because that would convert to what nanometers? 327 00:24:16 --> 00:24:18 700 nanometers. 328 00:24:18 --> 00:24:22 So if you do something strange and you forget Avagadro's 329 00:24:22 --> 00:24:24 number, you're going to come up with a very interesting 330 00:24:24 --> 00:24:25 wavelength. 331 00:24:25 --> 00:24:28 So that's a good way to check to make sure that you've 332 00:24:28 --> 00:24:31 done the problem correctly. 333 00:24:31 --> 00:24:35 So, 700 nanometers, anyone remember what light that is, 334 00:24:35 --> 00:24:38 what color that corresponds to? 335 00:24:38 --> 00:24:41 Red, so it's absorbing red light. 336 00:24:41 --> 00:24:44 All right, so now let's just do the same thing for the low spin 337 00:24:44 --> 00:24:48 system with the cyanide ligand, and we're going to plug in 338 00:24:48 --> 00:24:55 our 392 here, and we get 305 over here. 339 00:24:55 --> 00:25:03 And so, that is a much shorter wavelength of light. 340 00:25:03 --> 00:25:07 So again, light absorbed for the compound with water, 700 341 00:25:07 --> 00:25:13 nanometers, and the compound of iron with cyanide, 305, and so 342 00:25:13 --> 00:25:18 we're absorbing a red light over with the water compound, 343 00:25:18 --> 00:25:24 and sort of purple or violet light is being absorbed 344 00:25:24 --> 00:25:26 in the cyanide complex. 345 00:25:26 --> 00:25:29 And we're talk in a minute about the light that is being 346 00:25:29 --> 00:25:32 transmitted, which is complementary to the color 347 00:25:32 --> 00:25:35 of the light absorbed. 348 00:25:35 --> 00:25:38 So by knowing something about splitting energies, by knowing 349 00:25:38 --> 00:25:42 something about the types of ligands, then you can know 350 00:25:42 --> 00:25:45 something about colors. 351 00:25:45 --> 00:25:49 So now, for another example, we're going to look at the 352 00:25:49 --> 00:25:55 different colors of two chromium complexes. 353 00:25:55 --> 00:26:01 So first, what is the oxidation number of chromium in 354 00:26:01 --> 00:26:06 the water complex here? 355 00:26:06 --> 00:26:08 What is it? 356 00:26:08 --> 00:26:12 And what about over here with n h 3 ligands. 357 00:26:12 --> 00:26:14 Plus 3. 358 00:26:14 --> 00:26:18 So, plus 3 and plus 3. 359 00:26:18 --> 00:26:19 And what is our d count? 360 00:26:19 --> 00:26:23 You know where chromium is, in what group? 361 00:26:23 --> 00:26:24 Six. 362 00:26:24 --> 00:26:29 6 minus 3 is 3, so we have a d 3 system. 363 00:26:29 --> 00:26:32 What does c n mean again? 364 00:26:32 --> 00:26:37 Coordination number, so what is that for both of these? 365 00:26:37 --> 00:26:39 Six. 366 00:26:39 --> 00:26:42 So there's Six things coordinated to the chromium, 367 00:26:42 --> 00:26:48 and so we have, again, an octahedral system. 368 00:26:48 --> 00:26:55 And what type of ligand is water? 369 00:26:55 --> 00:26:56 Intermediate. 370 00:26:56 --> 00:27:00 And what about n h 3? 371 00:27:00 --> 00:27:01 Strong. 372 00:27:01 --> 00:27:06 So this is strong, and water is and intermediate ligand, 373 00:27:06 --> 00:27:10 and certainly, it is weaker than n h 3. 374 00:27:10 --> 00:27:14 So, we expect one system over here for a strong ligand, and 375 00:27:14 --> 00:27:17 then something that's weaker than that strong ligand. 376 00:27:17 --> 00:27:26 All right, so here are two diagrams, one with a big 377 00:27:26 --> 00:27:30 splitting energy, and one with a smaller splitting energy. 378 00:27:30 --> 00:27:34 Are the diagrams going to look same or different? 379 00:27:34 --> 00:27:35 The same. 380 00:27:35 --> 00:27:39 Because we only have three electrons, so they're 381 00:27:39 --> 00:27:40 going to be the same. 382 00:27:40 --> 00:27:43 In both cases, we put in the three electrons in the lowest 383 00:27:43 --> 00:27:46 orbitals, and then there's no decision to be made, because 384 00:27:46 --> 00:27:50 there isn't that fourth electron, so we don't have to 385 00:27:50 --> 00:27:53 decide which place to put this. 386 00:27:53 --> 00:27:56 So these diagrams are going to look the same, and before when 387 00:27:56 --> 00:27:59 we were doing this in this unit, we said OK, we're 388 00:27:59 --> 00:28:00 done, they look the same. 389 00:28:00 --> 00:28:04 But now, we realize that these are really not the same 390 00:28:04 --> 00:28:06 compounds and that they're going to have different 391 00:28:06 --> 00:28:09 properties, even though their diagrams are going 392 00:28:09 --> 00:28:10 to look the same. 393 00:28:10 --> 00:28:13 Because the energy that it's going to take to excite an 394 00:28:13 --> 00:28:17 electron here is much smaller than over here, and that's 395 00:28:17 --> 00:28:20 going to result in a different wavelength of light being 396 00:28:20 --> 00:28:23 absorbed in these two different cases, which will mean a 397 00:28:23 --> 00:28:28 different wavelength of light being transmitted. 398 00:28:28 --> 00:28:31 So, again, here we have a weaker field and here we 399 00:28:31 --> 00:28:35 have a stronger field. 400 00:28:35 --> 00:28:40 So again, we can go through and think about these two cases. 401 00:28:40 --> 00:28:45 So when we have a smaller term here, that means a lower energy 402 00:28:45 --> 00:28:47 -- this is a splitting energy, and so we'll have a 403 00:28:47 --> 00:28:49 lower frequency. 404 00:28:49 --> 00:28:53 When we have a larger case or higher energy, we 405 00:28:53 --> 00:28:57 have a higher frequency. 406 00:28:57 --> 00:29:02 Again, if you have a lower frequency absorbed, we have a 407 00:29:02 --> 00:29:06 longer wavelength absorbed, and in this case, the higher 408 00:29:06 --> 00:29:12 frequency translates into a shorter wavelength absorbed. 409 00:29:12 --> 00:29:15 The color of the transmitted light is complementary to the 410 00:29:15 --> 00:29:18 color of the absorbed light. 411 00:29:18 --> 00:29:24 So now we can think about -- I always want to ask, when 412 00:29:24 --> 00:29:26 do people learn about complementary colors? 413 00:29:26 --> 00:29:33 Is that 6th grade, earlier? 414 00:29:33 --> 00:29:38 I don't really remember, but I think it's pretty early on. 415 00:29:38 --> 00:29:42 And people always ask me, are you going to have that on the 416 00:29:42 --> 00:29:45 equation sheet, or do I have to actually remember my 417 00:29:45 --> 00:29:46 complementary colors? 418 00:29:46 --> 00:29:52 And I tell people that I will put some version of this on, so 419 00:29:52 --> 00:29:58 you don't have to review your kindergarten notes for this 420 00:29:58 --> 00:30:00 class, if that's when you learned it. 421 00:30:00 --> 00:30:05 It's pretty early, I don't know when it is exactly. 422 00:30:05 --> 00:30:09 So, the color of the light is going to be complementary about 423 00:30:09 --> 00:30:14 -- this is very approximate. 424 00:30:14 --> 00:30:19 So here, if the transmitted light is shorter because we 425 00:30:19 --> 00:30:24 have this weaker splitting, then we are expecting we're 426 00:30:24 --> 00:30:26 going to have this shorter wavelength, the transmitted 427 00:30:26 --> 00:30:29 light, and experimentally, if you make this compound 428 00:30:29 --> 00:30:31 you'll see it's violet. 429 00:30:31 --> 00:30:35 In this other case, we have a stronger field ligand, and so 430 00:30:35 --> 00:30:38 you have a larger energy, higher frequency absorbed, 431 00:30:38 --> 00:30:41 shorter wavelength absorbed, then you're going to have 432 00:30:41 --> 00:30:44 a longer wavelength from your transmitted light. 433 00:30:44 --> 00:30:48 And that this compound, if you make it, is actually yellow. 434 00:30:48 --> 00:30:52 So if we go back to our colors for a minute, you see that 435 00:30:52 --> 00:30:55 when you have the shorter wavelength, we have a violet, 436 00:30:55 --> 00:30:58 and that is a short wavelength. 437 00:30:58 --> 00:31:03 And in this case for the strong field ligand, we are going to 438 00:31:03 --> 00:31:05 have transmitted light of a longer wavelength 439 00:31:05 --> 00:31:07 and it's yellow. 440 00:31:07 --> 00:31:11 So it's the same oxidation state of chromium, it's the 441 00:31:11 --> 00:31:15 same -- it's an octahedral complex, six ligands in both 442 00:31:15 --> 00:31:20 cases, same octahedral crystal field diagrams, but yet one 443 00:31:20 --> 00:31:23 compound has a violet color, and the other 444 00:31:23 --> 00:31:30 one has a yellow color. 445 00:31:30 --> 00:31:35 All right, so one can also be asked to calculate a crystal 446 00:31:35 --> 00:31:39 field splitting energy in kilojoules per mole, given 447 00:31:39 --> 00:31:41 the appropriate information. 448 00:31:41 --> 00:31:45 So we've looked at when a splitting energy is given, and 449 00:31:45 --> 00:31:48 we've been asked to calculate wavelength absorbed, you can 450 00:31:48 --> 00:31:52 also be asked to go in the other direction. 451 00:31:52 --> 00:31:55 And so here we have another chromium complex to work with. 452 00:31:55 --> 00:31:57 And we're told that the wavelength of the most 453 00:31:57 --> 00:32:04 intensely absorbed light is 740, and so what would you 454 00:32:04 --> 00:32:10 predict the color of this to be? 455 00:32:10 --> 00:32:12 It would be greenish. 456 00:32:12 --> 00:32:14 So that would be what you would predict. 457 00:32:14 --> 00:32:18 Again, chemistry is an experimental science, but based 458 00:32:18 --> 00:32:21 on having a complementary color to the one absorbed, 459 00:32:21 --> 00:32:22 that would be a guess. 460 00:32:22 --> 00:32:31 All right, so we can actually calculate the frequency 461 00:32:31 --> 00:32:34 of the light absorbed. 462 00:32:34 --> 00:32:38 So we were given the wavelength, and use speed of 463 00:32:38 --> 00:32:41 light, and plug in your wavelength and you can come up 464 00:32:41 --> 00:32:48 with a frequency, 4.05 times 10 to the 14 per second. 465 00:32:48 --> 00:32:51 Then we can calculate from that the crystal field splitting 466 00:32:51 --> 00:32:55 energy, and so we use Planck's constant, and we have our 467 00:32:55 --> 00:32:59 frequency, and we calculate 2 . 468 00:32:59 --> 00:33:02 6 8 times 10 to the minus 19 joules. 469 00:33:02 --> 00:33:07 Am I done with the problem? 470 00:33:07 --> 00:33:09 What does the problem ask for? 471 00:33:09 --> 00:33:15 It asks for it in kilojoules per mole, and so, we're not 472 00:33:15 --> 00:33:18 done, we need to convert to kilojoules per mole. 473 00:33:18 --> 00:33:20 And I'm making this point, because often this is where 474 00:33:20 --> 00:33:24 people lose points on the final exam, and that's not where 475 00:33:24 --> 00:33:25 you want to lose points. 476 00:33:25 --> 00:33:28 You want to lose them on a really hard problem, not 477 00:33:28 --> 00:33:29 on something like this. 478 00:33:29 --> 00:33:33 So, most of the time you're asked for kilojoules per mole, 479 00:33:33 --> 00:33:36 so make sure that if that's what asked for, that's 480 00:33:36 --> 00:33:37 what you provide. 481 00:33:37 --> 00:33:41 So here, we can just do the conversion of units, and then 482 00:33:41 --> 00:33:44 we're going to use Avagadro's number to give us 483 00:33:44 --> 00:33:45 that per mole. 484 00:33:45 --> 00:33:49 And so, this translates into a 160 kilojoules per mole, which 485 00:33:49 --> 00:33:52 you might recognize is more similar to the other numbers 486 00:33:52 --> 00:34:00 that you saw for octahedral crystal field splitting energy. 487 00:34:00 --> 00:34:01 All right. 488 00:34:01 --> 00:34:06 Sadly, there are some coordination complexes 489 00:34:06 --> 00:34:11 that do not have colors. 490 00:34:11 --> 00:34:19 Why would that be? 491 00:34:19 --> 00:34:21 Why would something not have a color? 492 00:34:21 --> 00:34:32 It has d orbitals, it's a transition metal. 493 00:34:32 --> 00:34:34 So what would be true about all of the d orbitals? 494 00:34:34 --> 00:34:43 Yeah, so one example, is if they're all full, and that is 495 00:34:43 --> 00:34:46 the most common thing that we see, so it's not possible to 496 00:34:46 --> 00:34:51 have a d to d transition in the visible range. 497 00:34:51 --> 00:34:53 So there are a number of examples of metals who 498 00:34:53 --> 00:34:56 have this situation. 499 00:34:56 --> 00:35:01 Zinc and cadmium are two of the most common that give you 500 00:35:01 --> 00:35:05 problems in biological systems. 501 00:35:05 --> 00:35:06 So why is this? 502 00:35:06 --> 00:35:11 Well, that's because they're over here in group twelve. 503 00:35:11 --> 00:35:15 But their most common oxidation states are plus 2. 504 00:35:15 --> 00:35:21 So, if you have 12 minus 2 you have a d 10 system, and that's 505 00:35:21 --> 00:35:24 the case for both of these systems here. 506 00:35:24 --> 00:35:27 And so all the d orbitals are filled. 507 00:35:27 --> 00:35:32 Now, zinc is a really important metal in biological systems, 508 00:35:32 --> 00:35:37 and because it has all these d orbitals filled, it 509 00:35:37 --> 00:35:38 doesn't have a color. 510 00:35:38 --> 00:35:44 And so it's very hard to tell if an enzyme molecule has zinc. 511 00:35:44 --> 00:35:47 And I think one of the problems that you have on this 512 00:35:47 --> 00:35:50 problem-set talks about how zinc is important in a 513 00:35:50 --> 00:35:54 biological system by altering the p k a of a residue 514 00:35:54 --> 00:35:56 that coordinates to it. 515 00:35:56 --> 00:36:01 And that's often its job, and so biochemists are often faced 516 00:36:01 --> 00:36:04 with the problem of trying to figure out if their protein has 517 00:36:04 --> 00:36:08 zinc, but they have no color of the protein, also they might 518 00:36:08 --> 00:36:12 try to look for a paramagnetic or diamagnetic system. 519 00:36:12 --> 00:36:15 They're not -- you know if they see a paramagnetic system, they 520 00:36:15 --> 00:36:19 say oh, unpaired electrons, we know we must have metal 521 00:36:19 --> 00:36:21 involved, but there's no sort of spectroscopic 522 00:36:21 --> 00:36:23 probe for zinc. 523 00:36:23 --> 00:36:26 And so, often someone will determine a crystal structure, 524 00:36:26 --> 00:36:30 and it'll be a huge surprise that there's zinc associated 525 00:36:30 --> 00:36:32 with this protein. 526 00:36:32 --> 00:36:36 Do you think there's a lot of proteins that use cadmium as 527 00:36:36 --> 00:36:39 of part of their mechanism? 528 00:36:39 --> 00:36:42 What do you know about cadmium? 529 00:36:42 --> 00:36:44 Yeah, cadmium is poisonous. 530 00:36:44 --> 00:36:47 Old barbecue grills were sometimes, they used to 531 00:36:47 --> 00:36:50 coat things with cadmium on a barbecue grill. 532 00:36:50 --> 00:36:54 Yeah, that was not very smart. 533 00:36:54 --> 00:36:56 So, cadmium poisoning is a problem, and people have been 534 00:36:56 --> 00:36:59 trying to figure out the mechanism of that, but again, 535 00:36:59 --> 00:37:01 it's hard to study cadmium because it has no 536 00:37:01 --> 00:37:07 spectroscopic signal. 537 00:37:07 --> 00:37:13 All right, so getting back now to just kind of review over 538 00:37:13 --> 00:37:16 what we've talked about in terms of colors. 539 00:37:16 --> 00:37:19 So we have our weak field ligands, again, you need to 540 00:37:19 --> 00:37:20 memorize what they are. 541 00:37:20 --> 00:37:23 You have your intermediate field ligands, which you need 542 00:37:23 --> 00:37:27 to memorize, and also your strong field ligands. 543 00:37:27 --> 00:37:30 So these weak field ligands are going to have a small splitting 544 00:37:30 --> 00:37:34 energy, and that means that in terms of how the complex 545 00:37:34 --> 00:37:39 absorbs, low energy, low frequency, long wavelength, and 546 00:37:39 --> 00:37:41 that the color transmitted will be complementary. 547 00:37:41 --> 00:37:48 And usually what this means is that it'll be sort of in the 548 00:37:48 --> 00:37:51 end of the spectra, so it's often hard to say well, red 549 00:37:51 --> 00:37:53 will definitely be green. 550 00:37:53 --> 00:37:57 So it's not a perfect agreement, but you can usually 551 00:37:57 --> 00:37:59 say well, it's probably going to be in the blue-violet 552 00:37:59 --> 00:38:00 or green end. 553 00:38:00 --> 00:38:05 So in sort of one part of the spectra. 554 00:38:05 --> 00:38:08 Strong field ligands, again, have a huge splitting energy. 555 00:38:08 --> 00:38:11 So you're going to have big energy, high frequency, short 556 00:38:11 --> 00:38:14 wavelength, and so it's going to transmit, then, in the 557 00:38:14 --> 00:38:17 complementary, so it should be in the yellow, 558 00:38:17 --> 00:38:19 orange or red end. 559 00:38:19 --> 00:38:22 And you will be asked in some of the problems, in again, 560 00:38:22 --> 00:38:25 problem-set 9 due Wednesday, and you should be able to 561 00:38:25 --> 00:38:28 finish that up pretty quickly tonight after this lecture, 562 00:38:28 --> 00:38:30 and there are some problems on this. 563 00:38:30 --> 00:38:36 So, for cobalt complexes, you get pretty much the 564 00:38:36 --> 00:38:39 entire range of colors. 565 00:38:39 --> 00:38:44 So I'm just going to end with one more biological example. 566 00:38:44 --> 00:38:49 And here are some pictures of actual colors, and so this is 567 00:38:49 --> 00:38:53 cobalt coordinated to vitamin B12. 568 00:38:53 --> 00:38:57 So one ligand gives you this brilliant red color, another 569 00:38:57 --> 00:39:00 gives you an orange color, and a third ligand 570 00:39:00 --> 00:39:02 gives you a pink color. 571 00:39:02 --> 00:39:06 So you can tell the oxidation state of vitamin B12 by the 572 00:39:06 --> 00:39:10 colors of the molecule. 573 00:39:10 --> 00:39:12 All right. 574 00:39:12 --> 00:39:14 Now you have all the information to finish your 575 00:39:14 --> 00:39:18 problem-set, and that's the end of transition metals. 576 00:39:18 --> 00:39:21 On Wednesday we start kinetics. 577 00:39:21 --> 00:39:22