1 00:00:01 --> 00:00:04 The following content is provided by MIT OpenCourseWare 2 00:00:04 --> 00:00:06 under a Creative Commons license. 3 00:00:06 --> 00:00:10 Additional information about our license and MIT 4 00:00:10 --> 00:00:15 OpenCourseWare in general is available at ocw.mit.edu. 5 00:00:15 --> 00:00:20 I am going to continue our blitz through a review of 6 00:00:20 --> 00:00:24 thermodynamics. And we are going to start, 7 00:00:24 --> 00:00:30 right now, talking about spontaneous change. 8 00:00:30 --> 00:00:34 And you all know what spontaneous change means. 9 00:00:34 --> 00:00:38 It means some change that occurs without intervention. 10 00:00:38 --> 00:00:42 Spontaneous change has a directionality to it. 11 00:00:42 --> 00:00:46 For example, if you put a rock at the top of 12 00:00:46 --> 00:00:49 a hill and you let go, it rolls down, 13 00:00:49 --> 00:00:54 it doesn't roll up. If you put a warm body next to 14 00:00:54 --> 00:00:59 a hot body, the heat flows from the hot body to the cold body, 15 00:00:59 --> 00:01:04 and not the other way. If you, for example, 16 00:01:04 --> 00:01:08 have a bulb of gas here and a stop-cock and an empty bulb, 17 00:01:08 --> 00:01:12 you open the stop-cock, that gas flows from the high 18 00:01:12 --> 00:01:15 pressure region to the low pressure region, 19 00:01:15 --> 00:01:18 and it does not go the other way. 20 00:01:18 --> 00:01:22 However, spontaneous change does not have to be fast. 21 00:01:22 --> 00:01:25 You know that if you take a bottle of ketchup, 22 00:01:25 --> 00:01:29 when it used to be a glass bottle that you couldn't 23 00:01:29 --> 00:01:34 squeeze, and you turn it over, that ketchup has a spontaneous 24 00:01:34 --> 00:01:39 tendency to flow out. But it does not have to be 25 00:01:39 --> 00:01:42 fast. What is, in chemical reactions, 26 00:01:42 --> 00:01:46 the key to spontaneity? Is it the exothermicity? 27 00:01:46 --> 00:01:51 Well, certainly iron rusts. You don't have to do anything 28 00:01:51 --> 00:01:55 to make it rust. A very exothermic reaction. 29 00:01:55 --> 00:02:00 Delta H is about 824 kilojoules per mole. 30 00:02:00 --> 00:02:05 If you have an acidic stomach and you then ingest something 31 00:02:05 --> 00:02:10 that is a little bit more basic, well, this reaction goes. 32 00:02:10 --> 00:02:15 It neutralizes that acid, also an exothermic reaction. 33 00:02:15 --> 00:02:21 You did not have to do anything other than drink the more basic 34 00:02:21 --> 00:02:23 solution. This reaction, 35 00:02:23 --> 00:02:28 here, this hydrolysis of ATP to ADP, adenosine diphosphate, 36 00:02:28 --> 00:02:32 -- -- proceeds in every cell of 37 00:02:32 --> 00:02:37 your body, and you don't have to do anything to make that go. 38 00:02:37 --> 00:02:42 That is an exothermic reaction. But what about an endothermic 39 00:02:42 --> 00:02:45 reaction? How about this reaction? 40 00:02:45 --> 00:02:50 This is ammonium nitrate dissolving in water to make 41 00:02:50 --> 00:02:55 ammonium ions and nitrate ions. The delta H for this reaction 42 00:02:55 --> 00:03:00 is positive, plus 25.7 kilojoules per mole. 43 00:03:00 --> 00:03:05 It is an endothermic reaction. Is this reaction spontaneous? 44 00:03:05 --> 00:03:07 Well, yes. We are going to do an 45 00:03:07 --> 00:03:11 experiment anyway. And the experiment we are going 46 00:03:11 --> 00:03:17 to do is, you are going to be given one of these cold packs. 47 00:03:17 --> 00:03:20 And the TAs can start distributing them. 48 00:03:20 --> 00:03:25 What you have to do is find the little pouch inside the cold 49 00:03:25 --> 00:03:31 pack that contains the water. You have to press on that, 50 00:03:31 --> 00:03:35 allowing the water to disperse in the material, 51 00:03:35 --> 00:03:38 and you will see if the reaction goes. 52 00:03:38 --> 00:03:43 If it goes, that cold pack better get cold because this is 53 00:03:43 --> 00:03:47 an endothermic reaction. It is going to remove some heat 54 00:03:47 --> 00:03:52 from the environment. Some of you will get hot packs, 55 00:03:52 --> 00:03:55 and we will see if that is spontaneous. 56 00:03:55 --> 00:04:00 Is an endothermic reaction spontaneous? 57 00:04:00 --> 00:04:03 Yes. Is an exothermic reaction 58 00:04:03 --> 00:04:06 spontaneous? Yes, right. 59 00:04:06 --> 00:04:10 Is delta H the key to spontaneity? 60 00:04:10 --> 00:04:12 No. What is? 61 00:04:12 --> 00:04:17 Delta G, right. So, delta G is the key to 62 00:04:17 --> 00:04:21 spontaneity. You already know that when 63 00:04:21 --> 00:04:27 delta G is negative, you have a spontaneous 64 00:04:27 --> 00:04:32 reaction. When delta G is positive, 65 00:04:32 --> 00:04:35 you have a non-spontaneous reaction. 66 00:04:35 --> 00:04:38 And very importantly, when delta G is zero, 67 00:04:38 --> 00:04:41 that is when you are at equilibrium. 68 00:04:41 --> 00:04:47 That is what we are going to be talking about in just a few 69 00:04:47 --> 00:04:50 minutes, when delta G is equal to zero. 70 00:04:50 --> 00:04:54 These are the conditions, of course, for constant 71 00:04:54 --> 00:04:59 temperature and pressure. Delta S, in this expression for 72 00:04:59 --> 00:05:04 delta G, is the change in the entropy. 73 00:05:04 --> 00:05:08 It is a measure of disorder. When delta S is positive, 74 00:05:08 --> 00:05:12 we have an increase in the disorder. 75 00:05:12 --> 00:05:16 When delta S is negative, we have a decrease in the 76 00:05:16 --> 00:05:20 disorder. Where do these conditions come 77 00:05:20 --> 00:05:23 from? You are going to talk about 78 00:05:23 --> 00:05:28 that in exquisite detail in 5.60, but I want to give you a 79 00:05:28 --> 00:05:34 physical understanding for what delta G is. 80 00:05:34 --> 00:05:38 And that is this. Suppose you have an exothermic 81 00:05:38 --> 00:05:41 reaction. It turns out that not all of 82 00:05:41 --> 00:05:44 that exothermicity, not all of that enthalpy, 83 00:05:44 --> 00:05:49 can be released to the outside world to do useful work. 84 00:05:49 --> 00:05:53 Some of that enthalpy is actually caught up in the 85 00:05:53 --> 00:05:57 product molecules, or can be caught up in the 86 00:05:57 --> 00:06:02 product molecules. Some of that enthalpy gets 87 00:06:02 --> 00:06:07 stuck in the product molecules. It gets stuck in the vibrations 88 00:06:07 --> 00:06:12 and rotations of the product molecules in the internal 89 00:06:12 --> 00:06:16 degrees of freedom. It is that energy that is not 90 00:06:16 --> 00:06:21 available to do useful work. For some exothermic reactions, 91 00:06:21 --> 00:06:27 here, the amount of energy that is available to do useful work 92 00:06:27 --> 00:06:31 is something smaller than delta H. 93 00:06:31 --> 00:06:35 It is delta H minus T delta S, where T delta S, 94 00:06:35 --> 00:06:40 then, is a measure of how much of that enthalpy is stuck in the 95 00:06:40 --> 00:06:44 internal degrees of freedom of the molecule. 96 00:06:44 --> 00:06:50 And so, this delta G is called the free energy because this is 97 00:06:50 --> 00:06:54 the amount of energy that is free to do useful work. 98 00:06:54 --> 00:06:59 That is what delta G is. For example, 99 00:06:59 --> 00:07:04 if you go home and turn on your gas stove, oxidize some methane, 100 00:07:04 --> 00:07:10 burn some natural gas to heat up the water for your pasta, 101 00:07:10 --> 00:07:15 that delta H is very negative. But let's now calculate delta 102 00:07:15 --> 00:07:17 G. Well, to do that, 103 00:07:17 --> 00:07:20 we need to know what delta S is. 104 00:07:20 --> 00:07:24 Delta S, I will show you in just a moment, 105 00:07:24 --> 00:07:30 is the change in the entropy. We can calculate that. 106 00:07:30 --> 00:07:35 But knowing delta S then, we can plug in the delta H and 107 00:07:35 --> 00:07:39 the temperature. What we find is that delta G 108 00:07:39 --> 00:07:43 here is less negative than delta H. 109 00:07:43 --> 00:07:48 Not all of this enthalpy, not all of that energy is 110 00:07:48 --> 00:07:52 available to the outside world to do useful work. 111 00:07:52 --> 00:07:58 Some of it, in this reaction, gets trapped or caught in the 112 00:07:58 --> 00:08:04 internal degrees of freedom of a molecule. 113 00:08:04 --> 00:08:08 And it is not available to do that useful work. 114 00:08:08 --> 00:08:12 Delta G, in this case, is less negative than delta H. 115 00:08:12 --> 00:08:15 But let's take the eat, breathe, exhale, 116 00:08:15 --> 00:08:19 pee reaction. The oxidation of glucose, 117 00:08:19 --> 00:08:24 going on in every cell of your body, this reaction also very 118 00:08:24 --> 00:08:27 exothermic. Let's calculate delta G for 119 00:08:27 --> 00:08:31 this reaction. Well, first of all, 120 00:08:31 --> 00:08:35 we need delta S. From that, we can calculate 121 00:08:35 --> 00:08:38 delta G. And, in this case, 122 00:08:38 --> 00:08:40 what do you see? In this case, 123 00:08:40 --> 00:08:45 you see that delta G is more negative than delta H. 124 00:08:45 --> 00:08:51 In this exothermic reaction, we are getting back all of the 125 00:08:51 --> 00:08:55 enthalpy and then some. We are getting back even more. 126 00:08:55 --> 00:09:01 And that extra energy is coming from the energy that is tied up 127 00:09:01 --> 00:09:08 in the internal degrees of freedom of the reactants. 128 00:09:08 --> 00:09:11 In this reaction, here, delta S is positive. 129 00:09:11 --> 00:09:17 We are increasing the disorder. If we increase the disorder, 130 00:09:17 --> 00:09:22 there are fewer ways to tie up energy in the internal degrees 131 00:09:22 --> 00:09:27 of freedom of the molecule. When we increase the disorder, 132 00:09:27 --> 00:09:33 that is what happens. And so, your body has figured 133 00:09:33 --> 00:09:39 out how to get back all of that delta H, and then some. 134 00:09:39 --> 00:09:45 We are getting that energy out that is locked up in the 135 00:09:45 --> 00:09:51 reactants, in the internal degrees of freedom of the 136 00:09:51 --> 00:09:55 reactants. That is a physical feeling, 137 00:09:55 --> 00:10:02 there, for what delta G is. Entropy for a reaction. 138 00:10:02 --> 00:10:06 The entropy is calculated from the absolute entropies of the 139 00:10:06 --> 00:10:10 products and the reactants. And so, what you need are the 140 00:10:10 --> 00:10:15 absolute entropies for each one of the products multiplied by 141 00:10:15 --> 00:10:18 the appropriate stoichiometric number. 142 00:10:18 --> 00:10:22 You sum them all up. And you do the same then for 143 00:10:22 --> 00:10:25 the reactants, the absolute entropy of each 144 00:10:25 --> 00:10:29 one of the reactants multiplied by that stoichiometric number. 145 00:10:29 --> 00:10:32 Sum them up. Subtract it. 146 00:10:32 --> 00:10:36 That is the entropy change for the reaction. 147 00:10:36 --> 00:10:40 Now, one thing I do want to point out is that in the case of 148 00:10:40 --> 00:10:43 entropies, here, these are absolute entropies. 149 00:10:43 --> 00:10:46 That is rather unusual in thermodynamics. 150 00:10:46 --> 00:10:51 In thermodynamics usually we look at changes in energies, 151 00:10:51 --> 00:10:54 but here we are talking about absolute entropies. 152 00:10:54 --> 00:11:00 That is a consequence of the third law of thermodynamics. 153 00:11:00 --> 00:11:04 You will see how that arises again in 5.60, 154 00:11:04 --> 00:11:09 but right now we are going to use it to calculate the entropy 155 00:11:09 --> 00:11:14 for a reaction. And some reactions here are 156 00:11:14 --> 00:11:17 completely entropy-driven. For example, 157 00:11:17 --> 00:11:21 if you melt ice, this is an endothermic 158 00:11:21 --> 00:11:24 reaction, 6.95 kilojoules per mole. 159 00:11:24 --> 00:11:28 In going from solid water to liquid water, 160 00:11:28 --> 00:11:35 you have to put energy into the system to do that. 161 00:11:35 --> 00:11:39 But you know that this reaction occurs spontaneously. 162 00:11:39 --> 00:11:43 If I had a cube of ice here, it would melt. 163 00:11:43 --> 00:11:45 This reaction is entropy-driven. 164 00:11:45 --> 00:11:47 Why? Let's look at it. 165 00:11:47 --> 00:11:51 Let's calculate delta S for that reaction. 166 00:11:51 --> 00:11:56 You need the absolutely entropy for water in the liquid phase, 167 00:11:56 --> 00:12:00 that is the product, minus the absolute entropy for 168 00:12:00 --> 00:12:07 water in the solid phase. The difference between the two 169 00:12:07 --> 00:12:11 is positive. We have increased the disorder. 170 00:12:11 --> 00:12:17 There are less ways to tie up energy in liquid water than 171 00:12:17 --> 00:12:21 there are in solid water, in ice. 172 00:12:21 --> 00:12:27 And that fact is going to make this reaction then spontaneous, 173 00:12:27 --> 00:12:33 6.95 positive for delta H minus T delta S. 174 00:12:33 --> 00:12:37 This term, T delta S, now is larger in absolute 175 00:12:37 --> 00:12:42 magnitude. Therefore, delta G is negative. 176 00:12:42 --> 00:12:48 This reaction is spontaneous. It is certainly entropy-driven. 177 00:12:48 --> 00:12:55 The other concept I want to talk about is the free energy of 178 00:12:55 --> 00:13:02 formation, which is analogous to what we talked about last time, 179 00:13:02 --> 00:13:09 the enthalpy of formation. The free energy of formation is 180 00:13:09 --> 00:13:14 the free energy for a reaction that forms one mole of a 181 00:13:14 --> 00:13:19 compound from the elements in their most stable form in the 182 00:13:19 --> 00:13:24 standard state. And our standard state is one 183 00:13:24 --> 00:13:27 bar. The free energy of formation, 184 00:13:27 --> 00:13:33 here, is tabulated like the heats of formation. 185 00:13:33 --> 00:13:38 You can find tables of free energy and enthalpy of formation 186 00:13:38 --> 00:13:43 for all molecules. However, unlike the enthalpy of 187 00:13:43 --> 00:13:49 formation, the free energy of formation can also be calculated 188 00:13:49 --> 00:13:53 easily by you, which is the following, 189 00:13:53 --> 00:14:00 if you know the enthalpy of formation for some reaction. 190 00:14:00 --> 00:14:04 Or, for the reaction that defines the enthalpy of 191 00:14:04 --> 00:14:07 formation. And if you know what the 192 00:14:07 --> 00:14:12 entropy change is for that reaction that defines the 193 00:14:12 --> 00:14:17 enthalpy of formation, then you can calculate the free 194 00:14:17 --> 00:14:21 energy here of formation. You have two choices in the 195 00:14:21 --> 00:14:25 case of the free energy of formation. 196 00:14:25 --> 00:14:30 You can look it up. Or, if you know what delta H 197 00:14:30 --> 00:14:35 sub f and delta S are for the reaction, 198 00:14:35 --> 00:14:41 that defines the free energy of formation or the enthalpy of 199 00:14:41 --> 00:14:45 formation. You can calculate the free 200 00:14:45 --> 00:14:47 energy of formation, here. 201 00:14:47 --> 00:14:53 Here is a reaction that forms one mole of CO two. 202 00:14:53 --> 00:14:58 And the delta G for this reaction is minus 394 kilojoules 203 00:14:58 --> 00:15:03 per mole. The delta G for this reaction 204 00:15:03 --> 00:15:09 is defined as the free energy of formation for CO two. 205 00:15:09 --> 00:15:14 It is so because we are forming one mole of this molecule from 206 00:15:14 --> 00:15:19 the elements in their most stable form in the standard 207 00:15:19 --> 00:15:22 state. The most stable form of the 208 00:15:22 --> 00:15:26 element carbon is graphite. The most stable form of the 209 00:15:26 --> 00:15:31 element oxygen is molecular oxygen. 210 00:15:31 --> 00:15:36 But what is important about the free energy of formation, 211 00:15:36 --> 00:15:42 here, is that it is a measure of a compound stability relative 212 00:15:42 --> 00:15:46 to decomposition to its elements. 213 00:15:46 --> 00:15:50 For example, the free energy of formation of 214 00:15:50 --> 00:15:55 carbon dioxide is negative. What that means is CO two 215 00:15:55 --> 00:16:01 is thermodynamically stable relative to decomposition 216 00:16:01 --> 00:16:07 into its elements. Because delta G for this 217 00:16:07 --> 00:16:13 reaction is written as negative. The reaction is spontaneous in 218 00:16:13 --> 00:16:18 this direction. It is not spontaneous in the 219 00:16:18 --> 00:16:22 reverse direction. That is, the decomposition of 220 00:16:22 --> 00:16:28 CO two to its elements is not a spontaneous process. 221 00:16:28 --> 00:16:34 Therefore, we say that CO two is thermodynamically stable 222 00:16:34 --> 00:16:40 relative to decomposition into its elements. 223 00:16:40 --> 00:16:44 If you have a free energy of formation for a molecule that is 224 00:16:44 --> 00:16:47 negative, it is thermodynamically stable, 225 00:16:47 --> 00:16:52 but if you have a free energy of formation that is positive, 226 00:16:52 --> 00:16:56 then that compound is not thermodynamically stable 227 00:16:56 --> 00:17:00 relative to decomposition to its elements. 228 00:17:00 --> 00:17:03 For example, let's look at benzene. 229 00:17:03 --> 00:17:09 Here is a reaction that forms one mole of liquid benzene from 230 00:17:09 --> 00:17:14 the elements in their most stable form in the standard 231 00:17:14 --> 00:17:18 state, graphite and molecular hydrogen. 232 00:17:18 --> 00:17:24 The free energy of formation for this benzene is positive 233 00:17:24 --> 00:17:31 kilojoules per mole. That means that this forward 234 00:17:31 --> 00:17:36 reaction, as written, is not spontaneous. 235 00:17:36 --> 00:17:43 However, the reverse reaction is spontaneous because delta G 236 00:17:43 --> 00:17:47 is minus 124 kilojoules per mole. 237 00:17:47 --> 00:17:52 And so we say benzene, here, is thermodynamically 238 00:17:52 --> 00:17:58 unstable relative to its elements. 239 00:17:58 --> 00:18:02 But, even though you might have a reaction, here, 240 00:18:02 --> 00:18:08 that is spontaneous, that is the reverse reaction. 241 00:18:08 --> 00:18:12 You have a delta G formation that is positive, 242 00:18:12 --> 00:18:17 meaning the reverse reaction is spontaneous. 243 00:18:17 --> 00:18:22 Even though that reverse reaction may be spontaneous, 244 00:18:22 --> 00:18:27 it also could be very, very slow. 245 00:18:27 --> 00:18:32 When was the last time you saw a pint of benzene decompose into 246 00:18:32 --> 00:18:37 graphite and hydrogen? You haven't seen that. 247 00:18:37 --> 00:18:40 I haven't seen that and I am a lot older. 248 00:18:40 --> 00:18:45 What this means is that even though you might have a 249 00:18:45 --> 00:18:50 thermodynamic tendency to compose, it does not mean that 250 00:18:50 --> 00:18:56 it is going to happen because there is a question of the rate 251 00:18:56 --> 00:19:02 of the chemical reaction. We have two different terms to 252 00:19:02 --> 00:19:08 describe the thermodynamic tendency and then the kinetic 253 00:19:08 --> 00:19:12 tendency, and these terms are the following. 254 00:19:12 --> 00:19:18 We call the molecules stable or unstable when we are referring 255 00:19:18 --> 00:19:23 to the thermodynamic tendency. That is when we are referring 256 00:19:23 --> 00:19:29 to delta G or the free energy of formation. 257 00:19:29 --> 00:19:32 If it is negative, the molecule is stable. 258 00:19:32 --> 00:19:36 If it is positive, the molecule is unstable 259 00:19:36 --> 00:19:41 relative to decomposition. However, we also have to 260 00:19:41 --> 00:19:45 consider the rates. And we have another term to 261 00:19:45 --> 00:19:49 describe the rates. And that is labile and 262 00:19:49 --> 00:19:52 non-labile. If a molecule is non-labile, 263 00:19:52 --> 00:19:57 what that means is that the rate, at which the thermodynamic 264 00:19:57 --> 00:20:03 tendency is realized, is very, very slow. 265 00:20:03 --> 00:20:07 Benzene, for example, is thermodynamically unstable 266 00:20:07 --> 00:20:11 relative to decomposition into its elements, 267 00:20:11 --> 00:20:15 carbon and hydrogen, but it is non-labile. 268 00:20:15 --> 00:20:21 The rate at which that reaction happens is just too slow to be 269 00:20:21 --> 00:20:24 of any practical interest to you. 270 00:20:24 --> 00:20:30 However, if this decomposition reaction occurred very readily, 271 00:20:30 --> 00:20:35 then we would call that molecule labile. 272 00:20:35 --> 00:20:41 That is, the rate of the decomposition is something that 273 00:20:41 --> 00:20:48 is going to affect your ability to handle that particular 274 00:20:48 --> 00:20:55 compound or that molecule. Like the enthalpy of formation, 275 00:20:55 --> 00:21:02 the free energy of formation can also be zero. 276 00:21:02 --> 00:21:07 Last time, we talked about how the enthalpy of formation for 277 00:21:07 --> 00:21:10 hydrogen, oxygen, chlorine, xenon, 278 00:21:10 --> 00:21:14 all of that, had zero enthalpy of formation. 279 00:21:14 --> 00:21:18 Well, all of these molecules have zero free energy of 280 00:21:18 --> 00:21:24 formation because they are all in the most stable form already, 281 00:21:24 --> 00:21:29 in the standard state. The free energy of formation of 282 00:21:29 --> 00:21:34 bromine liquid and mercury liquid is 283 00:21:34 --> 00:21:38 zero. Because they are in the most 284 00:21:38 --> 00:21:41 stable form at the standard state. 285 00:21:41 --> 00:21:46 The free energy of formation of carbon in the form of graphite, 286 00:21:46 --> 00:21:49 sodium solid, 287 00:21:49 --> 00:21:53 iron solid, iodine solid. 288 00:21:53 --> 00:21:57 Those free energies of formation are all equal to zero, 289 00:21:57 --> 00:22:02 but the free energy of formation here of bromine in the 290 00:22:02 --> 00:22:09 gas phase is not equal to zero. Because bromine gas is not the 291 00:22:09 --> 00:22:12 most stable form in our standard state. 292 00:22:12 --> 00:22:17 Liquid bromine is, so it is going to take energy 293 00:22:17 --> 00:22:23 to produce bromine gas. So Delta G of formation is not 294 00:22:23 --> 00:22:27 going to be zero. Likewise, the free energy of 295 00:22:27 --> 00:22:33 formation of diamond is not equal to zero. 296 00:22:33 --> 00:22:36 Because carbon, in the form of diamond, 297 00:22:36 --> 00:22:40 is not the most stable form of carbon. 298 00:22:40 --> 00:22:44 Graphite is. This is going to take energy to 299 00:22:44 --> 00:22:47 form that configuration of carbon. 300 00:22:47 --> 00:22:53 So free energies of formation are very important in terms of 301 00:22:53 --> 00:23:00 understanding the thermodynamic stability of molecules. 302 00:23:00 --> 00:23:01 Just a review, here. 303 00:23:01 --> 00:23:05 If you want to calculate delta G for a reaction, 304 00:23:05 --> 00:23:08 what can you do? You can take the free energy of 305 00:23:08 --> 00:23:13 formation for each one of the products, multiply it by the 306 00:23:13 --> 00:23:17 appropriate stoichiometric number, since those free 307 00:23:17 --> 00:23:21 energies of formation are given per mole, add them all up, 308 00:23:21 --> 00:23:24 and then do the same thing for the reactants. 309 00:23:24 --> 00:23:30 Free energies of formation for each of the reactants. 310 00:23:30 --> 00:23:32 Stoichiometric number. Add them all up. 311 00:23:32 --> 00:23:36 Subtract the two. That is the delta G for your 312 00:23:36 --> 00:23:40 chemical reaction. Like delta H for the chemical 313 00:23:40 --> 00:23:44 reaction, which you calculated from the differences in the 314 00:23:44 --> 00:23:48 heats of formation, the products and reactants, 315 00:23:48 --> 00:23:51 note that this is products minus reactants. 316 00:23:51 --> 00:23:55 This is different from when you calculate delta H, 317 00:23:55 --> 00:23:59 for example, from bond enthalpies. 318 00:23:59 --> 00:24:01 That was reactants minus products. 319 00:24:01 --> 00:24:06 Something to remember. But again, in the case of delta 320 00:24:06 --> 00:24:11 G, we can calculate it from knowing the free energies of 321 00:24:11 --> 00:24:14 formation of the reactants and the products. 322 00:24:14 --> 00:24:19 But we can also calculate it from this expression. 323 00:24:19 --> 00:24:22 If, for example, you know the enthalpy change 324 00:24:22 --> 00:24:28 for a reaction and you know the entropy change for a reaction, 325 00:24:28 --> 00:24:32 you can calculate the free energy change from these two 326 00:24:32 --> 00:24:37 quantities. You have two choices to 327 00:24:37 --> 00:24:43 calculate the free energy change of some chemical reaction, 328 00:24:43 --> 00:24:49 depending on what information is known or is given to you. 329 00:24:49 --> 00:24:55 Now, I want to talk kind of briefly about controlling the 330 00:24:55 --> 00:25:00 spontaneity of a chemical reaction. 331 00:25:00 --> 00:25:04 And, to do so, I am going to talk about this 332 00:25:04 --> 00:25:07 molecule, which is sodium bicarbonate. 333 00:25:07 --> 00:25:12 Sodium bicarbonate is better known as baking soda. 334 00:25:12 --> 00:25:17 It is what you put into some batter of soft baked goods that 335 00:25:17 --> 00:25:22 you want to make. What happens is that the sodium 336 00:25:22 --> 00:25:27 bicarbonate decomposes and two of the products are gases, 337 00:25:27 --> 00:25:32 CO two and water. And so, in your batter, 338 00:25:32 --> 00:25:37 what you get are these bubbles of CO two and water. 339 00:25:37 --> 00:25:42 And what happens is that the dough starts to harden around 340 00:25:42 --> 00:25:45 these bubbles. And then, of course, 341 00:25:45 --> 00:25:49 eventually, the CO2 and water leave, are completely driven 342 00:25:49 --> 00:25:54 off, but what that leaves behind in the batter is a very porous 343 00:25:54 --> 00:25:59 structure, so porous that after you remove it from the oven you 344 00:25:59 --> 00:26:04 can actually put your teeth into it. 345 00:26:04 --> 00:26:08 Have you ever left out the baking soda in some soft baked 346 00:26:08 --> 00:26:12 goods? You cannot get your teeth into 347 00:26:12 --> 00:26:15 it, right? So, this is an important 348 00:26:15 --> 00:26:18 reaction. But this is a reaction, 349 00:26:18 --> 00:26:22 here, that is very endothermic. It does increase in the 350 00:26:22 --> 00:26:27 entropy, but at room temperature, this reaction has a 351 00:26:27 --> 00:26:33 positive delta G. This reaction does not proceed. 352 00:26:33 --> 00:26:37 It is non-spontaneous in the forward direction, 353 00:26:37 --> 00:26:41 as written. And that is good because you do 354 00:26:41 --> 00:26:47 not want this reaction to start when your batter is still on 355 00:26:47 --> 00:26:53 your kitchen counter. You want it to start when it is 356 00:26:53 --> 00:26:57 in the oven. What happens as we raise the 357 00:26:57 --> 00:27:02 temperature, here? For the purposes of what we are 358 00:27:02 --> 00:27:07 going to do, we have the same delta H and delta S. 359 00:27:07 --> 00:27:11 But now, when we calculate delta G, the temperature, 360 00:27:11 --> 00:27:16 here, is going to be our baking temperature of 350 degrees 361 00:27:16 --> 00:27:20 Fahrenheit. And now, what you see is delta 362 00:27:20 --> 00:27:24 G is negative, minus 14 kilojoules per mole. 363 00:27:24 --> 00:27:27 All of a sudden, this reaction became 364 00:27:27 --> 00:27:33 spontaneous. And we made it spontaneous 365 00:27:33 --> 00:27:39 simply by increasing the absolute magnitude of T delta S. 366 00:27:39 --> 00:27:44 We increased it by increasing the temperature, 367 00:27:44 --> 00:27:49 in this case. We made it spontaneous by 368 00:27:49 --> 00:27:54 raising the temperature. For some reactions, 369 00:27:54 --> 00:27:59 we can do that. We can find a temperature at 370 00:27:59 --> 00:28:05 which the reaction will be spontaneous. 371 00:28:05 --> 00:28:09 Let's look at the particular conditions. 372 00:28:09 --> 00:28:14 Delta G is a linear function of the temperature, 373 00:28:14 --> 00:28:19 so let me draw that for this particular case, 374 00:28:19 --> 00:28:24 for the sodium bicarbonate decomposition. 375 00:28:24 --> 00:28:30 The slope of this line for this reaction is, of course, 376 00:28:30 --> 00:28:35 minus delta S. The intercept is delta H. 377 00:28:35 --> 00:28:39 And now, let me just draw a zero here. 378 00:28:39 --> 00:28:45 What I want you to notice is that there is some temperature 379 00:28:45 --> 00:28:49 that I am going to call T star. 380 00:28:49 --> 00:28:55 There is some temperature at which the sign of delta G 381 00:28:55 --> 00:28:58 changes. You see that below T star, 382 00:28:58 --> 00:29:04 delta G is positive. Below those temperatures, 383 00:29:04 --> 00:29:08 such as room temperature for the sodium bicarbonate 384 00:29:08 --> 00:29:11 decomposition, delta G is positive. 385 00:29:11 --> 00:29:14 We have a non-spontaneous reaction. 386 00:29:14 --> 00:29:18 Above some temperature delta G has become negative. 387 00:29:18 --> 00:29:23 We have a spontaneous reaction. We can calculate the value of 388 00:29:23 --> 00:29:26 this T star, where the spontaneity switches, 389 00:29:26 --> 00:29:31 by setting delta G nought equal to zero 390 00:29:31 --> 00:29:36 and then solving for T star. Let's do that. 391 00:29:36 --> 00:29:41 I rearrange this to give me T star is equal to delta H over 392 00:29:41 --> 00:29:43 delta S. For this reaction, 393 00:29:43 --> 00:29:46 I know the values of delta H and delta S. 394 00:29:46 --> 00:29:51 And for this reaction that value of T star is 406 Kelvin. 395 00:29:51 --> 00:29:56 So, your oven has to be higher in temperature than 406 Kelvin 396 00:29:56 --> 00:30:01 if you want to make some baked goods that you can put your 397 00:30:01 --> 00:30:06 teeth into. For some reaction, 398 00:30:06 --> 00:30:11 in this particular case here that is endothermic, 399 00:30:11 --> 00:30:17 delta H greater than zero, in which case we have an 400 00:30:17 --> 00:30:22 increase in entropy, that reaction is spontaneous 401 00:30:22 --> 00:30:30 whenever the temperature is above some temperature T star. 402 00:30:30 --> 00:30:35 But we also have reactions which are exothermic, 403 00:30:35 --> 00:30:40 delta H less than zero, and reactions in which the 404 00:30:40 --> 00:30:45 entropy decreases. Delta S is less than zero. 405 00:30:45 --> 00:30:51 And I have plotted that line here, delta G versus T. 406 00:30:51 --> 00:30:57 For the opposite condition, we have the opposite slope 407 00:30:57 --> 00:31:02 because delta S has changed sign. 408 00:31:02 --> 00:31:04 In this case, the reaction will be 409 00:31:04 --> 00:31:08 spontaneous whenever the temperature is below some 410 00:31:08 --> 00:31:12 temperature T star. And you can see that by looking 411 00:31:12 --> 00:31:15 at the relative signs in this expression. 412 00:31:15 --> 00:31:20 If delta H is less than zero up here, then we have a negative 413 00:31:20 --> 00:31:24 quantity right here. And, since delta S is less than 414 00:31:24 --> 00:31:30 zero, we have minus times a minus, which is a plus. 415 00:31:30 --> 00:31:35 This term here is positive, this term is negative, 416 00:31:35 --> 00:31:40 and so this positive term better not be in absolute value 417 00:31:40 --> 00:31:44 very much larger than delta H here. 418 00:31:44 --> 00:31:49 If it is, then we are going to have a positive delta G, 419 00:31:49 --> 00:31:55 but if this term is small compared to the absolute value 420 00:31:55 --> 00:32:01 of delta H, then we will have a spontaneous reaction at low 421 00:32:01 --> 00:32:06 temperatures. So, you want to keep this term 422 00:32:06 --> 00:32:09 small. That is why it is spontaneous 423 00:32:09 --> 00:32:14 when T is less than T star. But we can also have reactions 424 00:32:14 --> 00:32:18 that are exothermic and reactions in which the entropy 425 00:32:18 --> 00:32:20 increases. In this case, 426 00:32:20 --> 00:32:23 you have the best of all worlds. 427 00:32:23 --> 00:32:26 In this case, this reaction is spontaneous at 428 00:32:26 --> 00:32:30 all temperatures. You cannot adjust the 429 00:32:30 --> 00:32:35 spontaneity of this reaction by temperature. 430 00:32:35 --> 00:32:37 This is always going to be negative. 431 00:32:37 --> 00:32:41 Delta H is negative here, minus T delta S. 432 00:32:41 --> 00:32:44 This is going to be minus a positive number. 433 00:32:44 --> 00:32:48 A negative minus a positive number is always a negative 434 00:32:48 --> 00:32:52 number, always spontaneous. And then, finally, 435 00:32:52 --> 00:32:57 we can have a condition where we have an endothermic reaction, 436 00:32:57 --> 00:33:00 delta H is greater than zero, and where the entropy 437 00:33:00 --> 00:33:05 decreases, delta S is less than zero. 438 00:33:05 --> 00:33:07 In this case, the reaction is never 439 00:33:07 --> 00:33:11 spontaneous, no matter what temperature you do. 440 00:33:11 --> 00:33:14 You cannot adjust that non-spontaneity with 441 00:33:14 --> 00:33:17 temperature. Delta H, you can see that, 442 00:33:17 --> 00:33:21 is going to be positive. And since delta S is negative, 443 00:33:21 --> 00:33:25 we have a minus times a minus, that is positive, 444 00:33:25 --> 00:33:29 delta G is positive at all temperatures. 445 00:33:29 --> 00:33:34 So we have failed to adjust the spontaneity with temperature for 446 00:33:34 --> 00:33:38 some reactions that are endothermic and in which the 447 00:33:38 --> 00:33:40 entropy decreases. 448 00:33:40 --> 00:33:45 449 00:33:45 --> 00:33:56 What we have been talking about are values of delta G that are 450 00:33:56 --> 00:34:02 standard state. We have been talking about 451 00:34:02 --> 00:34:06 delta G nought, one bar pressure. 452 00:34:06 --> 00:34:10 That is what we have been talking about. 453 00:34:10 --> 00:34:17 What that means is that the delta G nought for any reaction 454 00:34:17 --> 00:34:23 means that we have one atmosphere each of the products 455 00:34:23 --> 00:34:28 and the reactants. That is what delta G nought 456 00:34:28 --> 00:34:32 means. That our famous reaction here, 457 00:34:32 --> 00:34:35 argon-boron, argon plus boron going to 458 00:34:35 --> 00:34:39 carbon plus deuterium. Let's take this reaction. 459 00:34:39 --> 00:34:44 When I give you a delta G nought for this famous reaction, 460 00:34:44 --> 00:34:48 what that means is that that is the delta G nought when the 461 00:34:48 --> 00:34:52 partial pressure of the reactant A is one bar, 462 00:34:52 --> 00:34:57 and the partial pressure of reactant B, is one bar and the 463 00:34:57 --> 00:35:02 partial pressure of product C is one bar, and the partial 464 00:35:02 --> 00:35:06 pressure of product D is one bar. 465 00:35:06 --> 00:35:11 That does not seem real useful, because say you were going to 466 00:35:11 --> 00:35:17 start a reaction and you just start it even with one bar of A 467 00:35:17 --> 00:35:21 and one bar of B, this is not the delta G under 468 00:35:21 --> 00:35:27 those particular conditions. We have to be able to calculate 469 00:35:27 --> 00:35:33 delta G under any conditions. Not just our standard state 470 00:35:33 --> 00:35:36 conditions. And that is what we are going 471 00:35:36 --> 00:35:41 to do with this expression. We are going to be able to 472 00:35:41 --> 00:35:45 calculate a delta G at any time during a reaction. 473 00:35:45 --> 00:35:50 We can stop a reaction, and we can measure the partial 474 00:35:50 --> 00:35:54 pressures of the reactants and the products present, 475 00:35:54 --> 00:35:59 and we can get from that, then, a delta G for a reaction 476 00:35:59 --> 00:36:05 at that particular point. That is what we are going to 477 00:36:05 --> 00:36:08 do, here. What have I got written here? 478 00:36:08 --> 00:36:12 I have delta G is equal to this delta G nought, 479 00:36:12 --> 00:36:16 the standard state delta G, plus RT ln of the partial 480 00:36:16 --> 00:36:22 pressure of product C over some reference pressure raised to the 481 00:36:22 --> 00:36:26 appropriate stoichiometric number, times the partial 482 00:36:26 --> 00:36:31 pressure of the other reactant, divided by some reference 483 00:36:31 --> 00:36:35 pressure raised to the appropriate stoichiometric 484 00:36:35 --> 00:36:39 number. And that is all over the 485 00:36:39 --> 00:36:44 product of the partial pressure of A over that reference 486 00:36:44 --> 00:36:49 pressure, raised to the appropriate stoichiometric 487 00:36:49 --> 00:36:53 number, times the same for reactant B. 488 00:36:53 --> 00:36:58 What this ratio here of partial pressures is, 489 00:36:58 --> 00:37:02 or what it is called, is the reaction quotient, 490 00:37:02 --> 00:37:06 Q. It is the ratio of the partial 491 00:37:06 --> 00:37:11 pressures present during any time during the reaction. 492 00:37:11 --> 00:37:15 Not necessarily at equilibrium -- at any time during the 493 00:37:15 --> 00:37:18 reaction. That is what Q is here. 494 00:37:18 --> 00:37:21 And so in this way, with this expression, 495 00:37:21 --> 00:37:26 we are going to be able to calculate what delta G is for 496 00:37:26 --> 00:37:31 the reaction at any time outside of this special standard state 497 00:37:31 --> 00:37:36 of one bar pressure for each one of the reactants, 498 00:37:36 --> 00:37:42 one bar partial pressure for each one of the products. 499 00:37:42 --> 00:37:46 Where this expression comes from is, again, 500 00:37:46 --> 00:37:50 discussed in exquisite detail in 5.60. 501 00:37:50 --> 00:37:56 You will see where it comes from later, but right now we are 502 00:37:56 --> 00:38:02 going to use it to calculate delta G at any time during the 503 00:38:02 --> 00:38:06 reaction. But now let me point out that 504 00:38:06 --> 00:38:09 our reference pressure right here is one bar. 505 00:38:09 --> 00:38:13 What I am going to do is substitute a one in here for 506 00:38:13 --> 00:38:18 each one of the reference pressures, so that my reaction 507 00:38:18 --> 00:38:20 quotient is going to look like this. 508 00:38:20 --> 00:38:25 And I did not put in the bars because what you are going to do 509 00:38:25 --> 00:38:31 is put in the pressures in bars. And then, the reaction quotient 510 00:38:31 --> 00:38:35 will be just fine. You have to use bar pressure 511 00:38:35 --> 00:38:37 here, since that is our standard state. 512 00:38:37 --> 00:38:42 That is our reference pressure. Now, keep this in mind. 513 00:38:42 --> 00:38:45 This is important. We are going to use this again 514 00:38:45 --> 00:38:49 in just a moment. Let's start talking about the 515 00:38:49 --> 00:38:53 equilibrium constant. Here is our famous A plus B 516 00:38:53 --> 00:38:58 going to C plus D reaction. 517 00:38:58 --> 00:39:03 We already said if delta G, for this reaction as written is 518 00:39:03 --> 00:39:07 negative, then that forward reaction is spontaneous. 519 00:39:07 --> 00:39:13 If delta G for that reaction is positive for the reaction as 520 00:39:13 --> 00:39:18 written, what that means is then, the reverse reaction is 521 00:39:18 --> 00:39:21 spontaneous. And now, very importantly, 522 00:39:21 --> 00:39:25 if delta G is zero, then we are at chemical 523 00:39:25 --> 00:39:29 equilibrium. Notice this is delta G equal to 524 00:39:29 --> 00:39:33 zero. This is not delta G nought 525 00:39:33 --> 00:39:37 equal to zero. A big difference here. 526 00:39:37 --> 00:39:43 This is delta G equal to zero. Then, we are at equilibrium. 527 00:39:43 --> 00:39:48 What I am going to do is I am going to bring back my 528 00:39:48 --> 00:39:53 expression that allowed me to calculate delta G at any 529 00:39:53 --> 00:40:00 arbitrary pressures of the reactants and the products. 530 00:40:00 --> 00:40:03 And I just said that equilibrium, here, 531 00:40:03 --> 00:40:07 is defined by delta G being equal to zero, 532 00:40:07 --> 00:40:11 so I am going to plug in a zero right in there. 533 00:40:11 --> 00:40:15 If that is the case, then I am going to rearrange 534 00:40:15 --> 00:40:19 this equation. I am going to bring delta G 535 00:40:19 --> 00:40:23 over to the other side, and that is what I do here on 536 00:40:23 --> 00:40:27 the next slide. I have delta G nought is equal 537 00:40:27 --> 00:40:31 to minus RT ln of this reaction quotient. 538 00:40:31 --> 00:40:37 Now, we have a special 539 00:40:37 --> 00:40:41 condition here. And that is when delta G is 540 00:40:41 --> 00:40:45 equal to zero, when we are at thermodynamic 541 00:40:45 --> 00:40:51 equilibrium this reaction quotient has a special name. 542 00:40:51 --> 00:40:56 That special name is the equilibrium constant, 543 00:40:56 --> 00:40:59 K. This reaction quotient is equal 544 00:40:59 --> 00:41:05 to the thermodynamic equilibrium constant. 545 00:41:05 --> 00:41:10 And it is so only when delta G is equal to zero. 546 00:41:10 --> 00:41:13 Not delta G nought equal to zero. 547 00:41:13 --> 00:41:18 We get the equation, delta G nought is equal to 548 00:41:18 --> 00:41:23 minus RT ln of K. 549 00:41:23 --> 00:41:30 That is where this particular expression comes from. 550 00:41:30 --> 00:41:34 So, the reaction quotient is equal to K when we are at 551 00:41:34 --> 00:41:39 thermodynamic equilibrium. Now what we are going to do is 552 00:41:39 --> 00:41:45 set up some equations here that are going to allow us to quickly 553 00:41:45 --> 00:41:48 tell when our reaction is at equilibrium. 554 00:41:48 --> 00:41:52 We are going to compare Q to K. Let's do that. 555 00:41:52 --> 00:41:57 Here is that general expression I had that allowed me to 556 00:41:57 --> 00:42:02 calculate delta G at any arbitrary pressures of the 557 00:42:02 --> 00:42:08 reactants and the products. Here is the expression delta G 558 00:42:08 --> 00:42:12 nought at equilibrium, delta G nought equal minus RT 559 00:42:12 --> 00:42:15 ln of K. 560 00:42:15 --> 00:42:19 What I am going to do is substitute this delta G nought 561 00:42:19 --> 00:42:22 into here right in there. Let me do that. 562 00:42:22 --> 00:42:25 I am just going to plug it right in. 563 00:42:25 --> 00:42:29 So, I have minus RT ln of K plus RT ln of Q. 564 00:42:29 --> 00:42:34 Now I have the difference 565 00:42:34 --> 00:42:39 between two logs. The difference between two logs 566 00:42:39 --> 00:42:45 is the log of the quotient of those arguments of the logs. 567 00:42:45 --> 00:42:50 So, delta G then is RT times ln of Q over K. 568 00:42:50 --> 00:42:55 Remember what Q is? 569 00:42:55 --> 00:43:02 It is this ratio of instantaneous partial pressures. 570 00:43:02 --> 00:43:08 If we have a reaction running and we somehow measure the 571 00:43:08 --> 00:43:15 partial pressures at some time, and we calculate the reaction 572 00:43:15 --> 00:43:21 quotient from that and then we find that Q is less than K, 573 00:43:21 --> 00:43:28 the equilibrium constant, what that means is that we have 574 00:43:28 --> 00:43:34 fewer products present than equilibrium says we should have 575 00:43:34 --> 00:43:38 -- -- because Q is less than K. 576 00:43:38 --> 00:43:43 If that is the case, then what is going to happen is 577 00:43:43 --> 00:43:49 that the reaction is going to proceed in the forward direction 578 00:43:49 --> 00:43:55 in order to make more products, so that Q can get to the point 579 00:43:55 --> 00:44:01 of being equal to K. You can also see that up here. 580 00:44:01 --> 00:44:06 When Q is less than K, we had the log of a number that 581 00:44:06 --> 00:44:11 is going to be less than one. The log of a number less than 582 00:44:11 --> 00:44:15 one is a negative number. When Q is equal to K, 583 00:44:15 --> 00:44:19 delta G is going to be negative, meaning, 584 00:44:19 --> 00:44:24 the reaction as written is spontaneous in the forward 585 00:44:24 --> 00:44:28 direction. That is what our equilibrium 586 00:44:28 --> 00:44:32 says. It wants to make more products. 587 00:44:32 --> 00:44:36 On the other hand, if we have Q greater than K, 588 00:44:36 --> 00:44:40 that says we have too many products compared to what 589 00:44:40 --> 00:44:44 equilibrium says we should have. And, of course, 590 00:44:44 --> 00:44:49 then the reaction is going to run in the reverse direction. 591 00:44:49 --> 00:44:54 It is going to try to use up those products and make more 592 00:44:54 --> 00:44:57 reactant. You can also see that by this 593 00:44:57 --> 00:45:02 expression. When Q is greater than K, 594 00:45:02 --> 00:45:07 we are going to have a log of a number that is greater than one, 595 00:45:07 --> 00:45:13 that is going to be positive. If delta G is positive in the 596 00:45:13 --> 00:45:17 forward direction for the reaction as written, 597 00:45:17 --> 00:45:22 then it is the reverse reaction that is going to be spontaneous. 598 00:45:22 --> 00:45:26 Another way to look at it is shown here. 599 00:45:26 --> 00:45:32 Suppose we are in a situation where Q is less than K. 600 00:45:32 --> 00:45:37 I am plotting here Q as a function of the time in the 601 00:45:37 --> 00:45:44 reaction, and I am starting out here at T equals zero and Q is 602 00:45:44 --> 00:45:47 less than K. If Q is less than K, 603 00:45:47 --> 00:45:53 it means that we have fewer products than what equilibrium 604 00:45:53 --> 00:45:58 tells us we should have. The reaction is going to 605 00:45:58 --> 00:46:04 proceed in the forward direction, so that Q will 606 00:46:04 --> 00:46:09 increase to the value of K, so that we can attain 607 00:46:09 --> 00:46:13 equilibrium. On the other hand, 608 00:46:13 --> 00:46:18 if we have a situation where we start a reaction, 609 00:46:18 --> 00:46:21 but Q is greater than K, in that case, 610 00:46:21 --> 00:46:26 we started the reaction by putting all the products in 611 00:46:26 --> 00:46:32 instead of the reactants. When Q is greater than K, 612 00:46:32 --> 00:46:38 it says we have more products than equilibrium says we should 613 00:46:38 --> 00:46:41 have. What is going to happen is that 614 00:46:41 --> 00:46:45 the reverse reaction is going to proceed. 615 00:46:45 --> 00:46:49 It is going to try to use up those products, 616 00:46:49 --> 00:46:54 so that we attain this ratio given by the equilibrium 617 00:46:54 --> 00:46:58 constant. That is how we are going to use 618 00:46:58 --> 00:47:04 Q, compare it to K to determine whether or not we are at 619 00:47:04 --> 00:47:08 chemical equilibrium. Professor Cummins will be here 620 00:47:08 --> 00:47:12 on Wednesday. I will see you later in the 621 00:47:12.755 --> 47:15 week.