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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 0 00:00:00,500 --> 00:00:01,750 ERIC S. LANDER: Section three. 1 00:00:04,920 --> 00:00:07,890 The breaking of sugar. 2 00:00:07,890 --> 00:00:14,110 The breaking of sugar is called glyco-- 3 00:00:14,110 --> 00:00:16,530 sugar, like glucose-- 4 00:00:16,530 --> 00:00:18,630 breaking, lysis. 5 00:00:18,630 --> 00:00:21,180 To lyse something is to break something. 6 00:00:21,180 --> 00:00:22,800 Glycolysis. 7 00:00:22,800 --> 00:00:24,725 Glycolysis, the breaking of sugars. 8 00:00:32,229 --> 00:00:33,520 So we have our hexose. 9 00:00:38,080 --> 00:00:42,350 C6H12O6. 10 00:00:42,350 --> 00:00:46,360 It's going to go into this box, this-- 11 00:00:46,360 --> 00:00:49,520 I call it a white box, but it's sort of a black box or it's whatever. 12 00:00:49,520 --> 00:00:50,560 So it's a black-white box. 13 00:00:50,560 --> 00:00:52,870 It goes into this box called glycolysis that we'll talk about. 14 00:00:56,470 --> 00:01:05,660 And what's going to come out is pyruvate, an intermediate molecule. 15 00:01:05,660 --> 00:01:07,280 Pyruvate. 16 00:01:07,280 --> 00:01:12,490 And pyruvate is going to go down here. 17 00:01:12,490 --> 00:01:16,760 And it's going to take one more step and get us ethanol plus CO2. 18 00:01:20,820 --> 00:01:22,430 If you're yeast. 19 00:01:22,430 --> 00:01:23,680 That's what yeast does. 20 00:01:27,270 --> 00:01:31,010 It turns out you also break down sugars. 21 00:01:31,010 --> 00:01:35,650 Glycolysis is a fundamental pathway in you as well. 22 00:01:35,650 --> 00:01:39,590 When you break down sugars to pyruvate, you don't turn them into 23 00:01:39,590 --> 00:01:42,460 ethanol, it turns out. 24 00:01:42,460 --> 00:01:44,760 Which is probably a good thing, right? 25 00:01:44,760 --> 00:01:48,490 Because then you'd all be going off to the bakery and getting drunk, right? 26 00:01:48,490 --> 00:01:50,110 You don't want to do that. 27 00:01:50,110 --> 00:01:50,730 OK. 28 00:01:50,730 --> 00:01:53,540 I mean, there really would be problems with that, right? 29 00:01:53,540 --> 00:01:54,230 OK. 30 00:01:54,230 --> 00:02:01,840 In fact, instead what happens in you, it goes to lactic acid. 31 00:02:04,700 --> 00:02:09,009 Or the ion of lactic acid, really, lactate. 32 00:02:09,008 --> 00:02:09,780 All right? 33 00:02:09,780 --> 00:02:12,050 That's what happens there. 34 00:02:12,050 --> 00:02:14,730 Now, why do you bother doing this? 35 00:02:14,730 --> 00:02:17,220 You bother doing this because-- 36 00:02:17,220 --> 00:02:18,250 actually, why do you bother doing this? 37 00:02:18,250 --> 00:02:19,320 What's the point? 38 00:02:19,320 --> 00:02:20,610 Was the point to make-- 39 00:02:20,610 --> 00:02:21,700 and why does yeast do this? 40 00:02:21,700 --> 00:02:28,150 Does yeast make carbon dioxide and ethanol for the enjoyment of humans? 41 00:02:28,150 --> 00:02:29,210 Why is it doing this? 42 00:02:29,210 --> 00:02:30,060 Energy. 43 00:02:30,060 --> 00:02:31,120 It's getting energy. 44 00:02:31,120 --> 00:02:32,330 STUDENT: It makes ATP. 45 00:02:32,330 --> 00:02:35,370 ERIC S. LANDER: It makes ATP. 46 00:02:35,370 --> 00:02:38,330 The whole point of breaking down sugars is when you break bonds, you 47 00:02:38,330 --> 00:02:39,610 liberate energy from the bonds. 48 00:02:39,610 --> 00:02:43,870 You use the energy from the bonds to put them into ATP, which you use for 49 00:02:43,870 --> 00:02:44,730 other reactions. 50 00:02:44,730 --> 00:02:47,930 The entire point of this whole fermentation thing that Buchner and 51 00:02:47,930 --> 00:02:51,390 everybody studied is to make ATP. 52 00:02:51,390 --> 00:02:56,405 So in fact, this reaction produces four ATPs. 53 00:03:00,340 --> 00:03:02,830 But you don't get something for nothing. 54 00:03:02,830 --> 00:03:05,820 You had to drive some of those reactions forward, right? 55 00:03:05,820 --> 00:03:07,660 So you probably use some ATPs-- 56 00:03:07,660 --> 00:03:10,410 you do use some ATPs in the process, don't you? 57 00:03:10,410 --> 00:03:17,860 You use two ATPs, but you get four ATPs. 58 00:03:17,860 --> 00:03:21,940 Some ATPs are driving the reaction, but you manage to break enough energy 59 00:03:21,940 --> 00:03:26,360 out of the bonds there and do it in a clever enough way to get ATPs. 60 00:03:26,360 --> 00:03:29,060 And you do a little bit of other things. 61 00:03:29,060 --> 00:03:30,970 There is an electron carrier. 62 00:03:30,970 --> 00:03:37,570 And I'm not going to talk a lot about it, but NAD+ goes to NADH. 63 00:03:40,260 --> 00:03:50,790 And in this step over here, the NADH gets recycled back to NAD+. 64 00:03:50,790 --> 00:03:52,040 Same thing here. 65 00:03:56,200 --> 00:03:58,540 So that all washes out. 66 00:03:58,540 --> 00:04:00,220 The electron carrier NADH. 67 00:04:00,220 --> 00:04:02,030 We're not going to fuss a lot over it. 68 00:04:02,030 --> 00:04:03,580 That's what goes on. 69 00:04:03,580 --> 00:04:08,960 That is the fundamental way bodies get energy, get ATP. 70 00:04:08,960 --> 00:04:13,830 Well, it was the fundamental way for the first billion 71 00:04:13,830 --> 00:04:15,860 years of life on Earth. 72 00:04:15,860 --> 00:04:20,079 This is the primitive way of breaking things down. 73 00:04:20,079 --> 00:04:26,180 It so happens that there's another solution too. 74 00:04:29,090 --> 00:04:32,560 And we'll talk about it later in this lecture. 75 00:04:32,560 --> 00:04:36,230 It turns out you can do better than this glycolysis and the measly two 76 00:04:36,230 --> 00:04:40,650 ATPs, but it took about a billion years to work that out. 77 00:04:40,650 --> 00:04:43,680 And the reason it took a billion years to work that out, we'll come to see, 78 00:04:43,680 --> 00:04:45,820 is it uses oxygen. 79 00:04:45,820 --> 00:04:49,580 And for about the first billion years of life on Earth there wasn't oxygen 80 00:04:49,580 --> 00:04:50,720 in the atmosphere. 81 00:04:50,720 --> 00:04:52,110 So this was worked out before. 82 00:04:52,110 --> 00:04:55,740 You can actually see the remnants of this ancient reaction in 83 00:04:55,740 --> 00:04:57,970 every living organism. 84 00:04:57,970 --> 00:05:00,220 And we'll talk a little bit more about that in the next part there. 85 00:05:00,220 --> 00:05:00,850 So that's it. 86 00:05:00,850 --> 00:05:01,790 It's glycolysis. 87 00:05:01,790 --> 00:05:03,850 Now it's time to open up the black box. 88 00:05:03,850 --> 00:05:07,080 What is in the black box? 89 00:05:07,080 --> 00:05:08,950 So let's go take a look. 90 00:05:16,960 --> 00:05:18,040 This is glycolysis. 91 00:05:18,040 --> 00:05:22,020 You have this all on your sheets, so you shouldn't be copying it down 92 00:05:22,020 --> 00:05:24,760 because it's a waste of your time to copy it down. 93 00:05:24,760 --> 00:05:26,880 But what you do want to do is think about it. 94 00:05:26,880 --> 00:05:30,730 So let's take a look at the reactions that are going on here. 95 00:05:30,730 --> 00:05:35,050 We start off with glucose. 96 00:05:38,510 --> 00:05:39,990 We are going to do what to glucose? 97 00:05:39,990 --> 00:05:43,900 We're going to add, in the very first reaction, a phosphate group. 98 00:05:43,900 --> 00:05:46,980 We've written a blue P with a circle around it because I don't want to keep 99 00:05:46,980 --> 00:05:50,680 writing the four oxygens and the phosphorus in the middle. 100 00:05:50,680 --> 00:05:54,855 So I'm just writing that there as my phosphate group. 101 00:05:54,855 --> 00:05:56,090 OK? 102 00:05:56,090 --> 00:05:59,180 Circled blue Ps will be a phosphate group that's added. 103 00:05:59,180 --> 00:05:59,920 All right? 104 00:05:59,920 --> 00:06:05,090 So I go from glucose to a glucose in which there is a phosphate on carbon 105 00:06:05,090 --> 00:06:08,610 number six, and that we call that-- very sensibly-- 106 00:06:08,610 --> 00:06:11,220 glucose-6-phosphate. 107 00:06:11,220 --> 00:06:15,310 So from glucose to glucose-6-phosphate we put on a phosphate, where are we 108 00:06:15,310 --> 00:06:17,252 going to get a phosphate? 109 00:06:17,252 --> 00:06:19,120 STUDENT: [INAUDIBLE]. 110 00:06:19,120 --> 00:06:23,360 ERIC S. LANDER: Oh, we're going to take off the last phosphate of ATP? 111 00:06:23,360 --> 00:06:26,180 And guess what, you get a lot of energy by taking 112 00:06:26,180 --> 00:06:27,740 off that last phosphate. 113 00:06:27,740 --> 00:06:33,300 So we can drive this reaction forward by breaking an ATP. 114 00:06:33,300 --> 00:06:36,535 We get an ATP, and ATP's going to turn into what? 115 00:06:36,535 --> 00:06:36,930 STUDENT: ADP. 116 00:06:36,930 --> 00:06:40,570 ERIC S. LANDER: ADP, and that phosphate is going to 117 00:06:40,570 --> 00:06:42,150 get used over there. 118 00:06:42,150 --> 00:06:42,690 Excellent. 119 00:06:42,690 --> 00:06:46,030 That's going to be a reaction that's going to be very happy going forward. 120 00:06:46,030 --> 00:06:47,000 Now what happens? 121 00:06:47,000 --> 00:06:48,430 Let's see what the difference is. 122 00:06:48,430 --> 00:06:53,060 We changed this sugar from glucose 6-phosphate to fructose-6-phosphate. 123 00:06:56,210 --> 00:06:58,950 And what that involved was just a little bit of rearrangement. 124 00:06:58,950 --> 00:07:01,760 You see this double bond here on this bottom carbon? 125 00:07:01,760 --> 00:07:05,500 Now the double bond is over here, one carbon up. 126 00:07:05,500 --> 00:07:10,130 It's just what they call an isomerization reaction. 127 00:07:10,130 --> 00:07:13,970 We simply change that double bond. 128 00:07:13,970 --> 00:07:16,130 There's some rearranging to be done there. 129 00:07:16,130 --> 00:07:18,870 But it's just from glucose to fructose. 130 00:07:18,870 --> 00:07:22,250 Another hexose. 131 00:07:22,250 --> 00:07:25,770 Another six-carbon sugar. 132 00:07:25,770 --> 00:07:28,290 There's some enzyme there that does that, and it's a different enzyme. 133 00:07:28,290 --> 00:07:31,590 It's called phosphoglucomutase, and you don't have to remember all the 134 00:07:31,590 --> 00:07:33,230 names of each of the enzymes. 135 00:07:33,230 --> 00:07:34,180 Now what happens? 136 00:07:34,180 --> 00:07:35,900 We get this guy. 137 00:07:35,900 --> 00:07:36,810 What's the next thing we're doing? 138 00:07:36,810 --> 00:07:39,642 Taking a look at the picture, what happened to it? 139 00:07:39,642 --> 00:07:40,750 STUDENT: [INAUDIBLE]. 140 00:07:40,750 --> 00:07:41,720 ERIC S. LANDER: Another phosphate. 141 00:07:41,720 --> 00:07:43,040 How are we going to do that phosphate? 142 00:07:43,040 --> 00:07:43,970 STUDENT: ATP. 143 00:07:43,970 --> 00:07:48,820 ERIC S. LANDER: Same deal, ATP to ADP. 144 00:07:48,820 --> 00:07:49,950 Excellent. 145 00:07:49,950 --> 00:07:55,378 Now what happens, taking a look at this pathway? 146 00:07:55,378 --> 00:07:57,286 STUDENT: [INAUDIBLE] 147 00:07:57,286 --> 00:07:58,240 pop it apart. 148 00:07:58,240 --> 00:07:59,260 ERIC S. LANDER: Pop it apart. 149 00:07:59,260 --> 00:08:02,060 I have a six-carbon sugar. 150 00:08:02,060 --> 00:08:03,030 Right? 151 00:08:03,030 --> 00:08:04,910 Six-carbon sugar. 152 00:08:04,910 --> 00:08:06,610 And I make two three-carbon sugars. 153 00:08:06,610 --> 00:08:08,950 Well, two three-carbon sugar like molecules. 154 00:08:08,950 --> 00:08:10,840 So I've got this one-- 155 00:08:10,840 --> 00:08:12,055 oh, actually, huh. 156 00:08:12,055 --> 00:08:12,960 That's G3P. 157 00:08:12,960 --> 00:08:14,320 Look at that. 158 00:08:14,320 --> 00:08:14,940 That's interesting. 159 00:08:14,940 --> 00:08:16,160 That's G3P. 160 00:08:16,160 --> 00:08:17,150 Our friend. 161 00:08:17,150 --> 00:08:20,230 So we have G3P there, and we have another molecule here. 162 00:08:20,230 --> 00:08:22,150 Let's not worry about that other molecule for now. 163 00:08:22,150 --> 00:08:25,110 But we have three-carbon structure here. 164 00:08:25,110 --> 00:08:29,490 And now what's going to happen? 165 00:08:29,490 --> 00:08:32,309 Well, you have your sheets. 166 00:08:32,308 --> 00:08:36,360 We're going to go over to the next board there. 167 00:08:36,360 --> 00:08:39,690 And this is where-- 168 00:08:39,690 --> 00:08:41,360 let's see, what do we have to do to it? 169 00:08:41,360 --> 00:08:43,460 Can you jump across from here to there? 170 00:08:43,460 --> 00:08:44,730 Who sees what happens here? 171 00:08:47,290 --> 00:08:50,180 NAD+ to NADH. 172 00:08:50,180 --> 00:08:51,630 Good. 173 00:08:51,630 --> 00:08:59,080 So then here we've now got a molecule that's got two phosphates here, right? 174 00:08:59,080 --> 00:09:01,750 These two phosphates make this molecule very 175 00:09:01,750 --> 00:09:03,000 negative at its two ends. 176 00:09:06,890 --> 00:09:08,740 It wants to break it off. 177 00:09:08,740 --> 00:09:12,140 And we're going to get energy back for breaking it off. 178 00:09:12,140 --> 00:09:15,944 And what are we going to do with that energy when we break off a phosphate? 179 00:09:15,944 --> 00:09:16,750 STUDENT: Pop it back on. 180 00:09:16,750 --> 00:09:24,580 ERIC S. LANDER: We're going to pop it back onto an ADP to an ATP. 181 00:09:24,580 --> 00:09:26,720 That's pretty good. 182 00:09:26,720 --> 00:09:29,700 See, we now got this molecule here that's got those two. 183 00:09:29,700 --> 00:09:32,160 Now what are we going to do? 184 00:09:32,160 --> 00:09:40,340 We move the phosphate to the middle, and then we rearrange some bonds here. 185 00:09:40,340 --> 00:09:41,500 I don't care about the details. 186 00:09:41,500 --> 00:09:43,170 We're moving the phosphate to the middle. 187 00:09:43,170 --> 00:09:44,780 We're rearranging some bonds. 188 00:09:44,780 --> 00:09:49,310 And it turns out, now, that this is a very unhappy molecule which would like 189 00:09:49,310 --> 00:09:50,245 to get rid of that phosphate. 190 00:09:50,245 --> 00:09:52,330 It would be very energetically favorable to 191 00:09:52,330 --> 00:09:53,280 get rid of that phosphate. 192 00:09:53,280 --> 00:09:55,150 So what do we do? 193 00:09:55,150 --> 00:10:01,920 We take an ADP to an ATP. 194 00:10:01,920 --> 00:10:04,220 And we end up with pyruvate. 195 00:10:04,220 --> 00:10:10,690 So the logic here was we spent ATP to add phosphate groups. 196 00:10:10,690 --> 00:10:15,020 We then have unfavorable molecules. 197 00:10:15,020 --> 00:10:19,680 And we release that energy to make ATP. 198 00:10:19,680 --> 00:10:21,500 And let's look at the energy over here. 199 00:10:21,500 --> 00:10:26,520 See, some of these steps the delta G zero primes, 200 00:10:26,520 --> 00:10:27,880 some of them are negative. 201 00:10:27,880 --> 00:10:31,670 They'll go forward on their own easily at equal concentrations. 202 00:10:31,670 --> 00:10:36,290 Some of them are positive and wouldn't go forward at equal concentrations. 203 00:10:36,290 --> 00:10:40,950 But notice that the delta Gs are negative. 204 00:10:40,950 --> 00:10:41,670 They do go forward. 205 00:10:41,670 --> 00:10:44,900 Why do they go forward even though the delta G0 primes were positive? 206 00:10:47,530 --> 00:10:49,600 The concentrations. 207 00:10:49,600 --> 00:10:55,390 So the concentrations of all of these molecules along this pathway ensure 208 00:10:55,390 --> 00:11:02,270 that every single one of these is negative or zero, which is 209 00:11:02,270 --> 00:11:04,370 equilibrium, it's still flowing slightly through. 210 00:11:04,370 --> 00:11:08,340 Negative, zero, zero, negative, negative. 211 00:11:08,340 --> 00:11:12,080 Every one of these will allow it to flow in that direction because of the 212 00:11:12,080 --> 00:11:14,180 concentrations and because-- 213 00:11:14,180 --> 00:11:15,760 so our two tricks-- 214 00:11:15,760 --> 00:11:21,300 direct coupling of some of these ATPs and indirect coupling by sucking 215 00:11:21,300 --> 00:11:23,370 reactions down. 216 00:11:23,370 --> 00:11:24,850 The whole thing works. 217 00:11:24,850 --> 00:11:26,520 So it's gorgeous. 218 00:11:26,520 --> 00:11:29,403 And how many ATPs did we make? 219 00:11:29,403 --> 00:11:31,370 STUDENT: [INAUDIBLE]. 220 00:11:31,370 --> 00:11:31,710 ERIC S. LANDER: Sorry? 221 00:11:31,710 --> 00:11:32,200 What-- no, wait a second. 222 00:11:32,200 --> 00:11:32,650 Wait a second. 223 00:11:32,650 --> 00:11:33,520 STUDENT: 2 minus 2. 224 00:11:33,520 --> 00:11:37,460 ERIC S. LANDER: We spent two ATPs, and we got two ATPs. 225 00:11:37,460 --> 00:11:38,710 STUDENT: [INAUDIBLE]. 226 00:11:40,945 --> 00:11:42,130 ERIC S. LANDER: Wait a second. 227 00:11:42,130 --> 00:11:43,660 We're supposed to get four. 228 00:11:43,660 --> 00:11:45,604 We've only got two. 229 00:11:45,604 --> 00:11:46,600 STUDENT: There's another half. 230 00:11:46,600 --> 00:11:46,950 ERIC S. LANDER: Wait, wait. 231 00:11:46,950 --> 00:11:47,365 Sorry? 232 00:11:47,365 --> 00:11:49,610 STUDENT: There's another half. 233 00:11:49,610 --> 00:11:50,740 ERIC S. LANDER: There's something over here? 234 00:11:50,740 --> 00:11:52,234 STUDENT: Yes. 235 00:11:52,234 --> 00:11:54,730 ERIC S. LANDER: Oh. 236 00:11:54,730 --> 00:11:57,230 We have another molecule we didn't use. 237 00:11:57,230 --> 00:12:01,250 But that is not G3P. 238 00:12:01,250 --> 00:12:04,180 So we can't use it, can we? 239 00:12:04,180 --> 00:12:05,770 What molecule is that? 240 00:12:05,770 --> 00:12:07,450 Does anybody recognize that molecule? 241 00:12:07,450 --> 00:12:09,620 STUDENT: [INAUDIBLE]. 242 00:12:09,620 --> 00:12:11,640 ERIC S. LANDER: That's DHAP. 243 00:12:11,640 --> 00:12:13,990 STUDENT: Ohhh. 244 00:12:13,990 --> 00:12:16,550 ERIC S. LANDER: That's DHAP. 245 00:12:16,550 --> 00:12:23,540 So if only we could convert DHAP into G3P we could send it down the pathway 246 00:12:23,540 --> 00:12:24,790 and now we'd get two more ATPs. 247 00:12:27,420 --> 00:12:29,263 Anybody got any ideas on how to do that? 248 00:12:29,263 --> 00:12:30,169 STUDENT: I don't know. 249 00:12:30,169 --> 00:12:31,075 I'm at a loss. 250 00:12:31,075 --> 00:12:31,530 ERIC S. LANDER: Pshaw. 251 00:12:31,530 --> 00:12:33,010 At a loss. 252 00:12:33,010 --> 00:12:39,820 Why don't we engage triose phosphate isomerase to save the day? 253 00:12:39,820 --> 00:12:42,450 TIM saves the day here. 254 00:12:42,450 --> 00:12:50,390 Triose phosphate isomerase now converts DHAP to G3P. 255 00:12:50,390 --> 00:12:51,870 Wait a second. 256 00:12:51,870 --> 00:12:57,218 I thought DHAP was more energetically favorable than G3P. 257 00:12:57,218 --> 00:12:59,920 STUDENT: But if you're using all the G3P-- 258 00:12:59,920 --> 00:13:01,725 ERIC S. LANDER: I'm using all the G3P. 259 00:13:01,725 --> 00:13:06,550 So even though DHAP is more energetically favorable, I'm sucking 260 00:13:06,550 --> 00:13:10,250 out all of the G3P to go down the pathway this way. 261 00:13:10,250 --> 00:13:14,720 And so it runs in that direction, which is perhaps why we discussed that 262 00:13:14,720 --> 00:13:16,410 at the beginning of the lecture. 263 00:13:16,410 --> 00:13:16,910 Exactly. 264 00:13:16,910 --> 00:13:17,770 STUDENT: Now it all makes sense. 265 00:13:17,770 --> 00:13:18,830 ERIC S. LANDER: It all makes sense. 266 00:13:18,830 --> 00:13:19,430 All right. 267 00:13:19,430 --> 00:13:21,760 So now we have the logic to this thing, right? 268 00:13:21,760 --> 00:13:23,340 We've got the logic to this thing. 269 00:13:23,340 --> 00:13:24,850 This is how glycolysis works. 270 00:13:24,850 --> 00:13:29,470 There's an investment phase, where you attach these phosphates, you build up 271 00:13:29,470 --> 00:13:32,160 these sugars, you break them apart, you send them down, you make the 272 00:13:32,160 --> 00:13:38,090 molecules more and more unfavorable, being clever at every stage to either 273 00:13:38,090 --> 00:13:43,380 couple it to a favorable reaction or suck it down the pathway by coupling 274 00:13:43,380 --> 00:13:46,120 it directly or indirectly to a favorable reaction. 275 00:13:46,120 --> 00:13:51,910 And at the end of day, in order to get two extra ATPs, we had to actually use 276 00:13:51,910 --> 00:13:55,030 both of those three-carbon structures, and that's what triose phosphate 277 00:13:55,030 --> 00:13:56,840 isomerase did for us. 278 00:13:56,840 --> 00:13:58,970 TIM saves the day. 279 00:13:58,970 --> 00:14:00,740 All right. 280 00:14:00,740 --> 00:14:06,000 So let's take a look at that over here. 281 00:14:06,000 --> 00:14:10,250 That's the way you should really think about glycolysis without all of these 282 00:14:10,250 --> 00:14:12,000 chemical structures here. 283 00:14:12,000 --> 00:14:15,050 Six-carbon sugar, phosphate, phosphate, break it 284 00:14:15,050 --> 00:14:17,560 apart, phosphate, phosphate. 285 00:14:17,560 --> 00:14:18,180 There we go. 286 00:14:18,180 --> 00:14:19,270 Break it apart. 287 00:14:19,270 --> 00:14:24,250 And you either spend ATPs or you get back ATPs, but we only use one of the 288 00:14:24,250 --> 00:14:26,290 three-carbons here. 289 00:14:26,290 --> 00:14:32,480 When TIM comes along, we've got this, and it doubles up. 290 00:14:32,480 --> 00:14:33,400 All right. 291 00:14:33,400 --> 00:14:34,630 So that's how we do it. 292 00:14:34,630 --> 00:14:36,156 That's pretty good. 293 00:14:36,156 --> 00:14:36,594 STUDENT: Professor Lander? 294 00:14:36,594 --> 00:14:37,032 ERIC S. LANDER: Yeah. 295 00:14:37,032 --> 00:14:39,970 STUDENT: Where does our extra phosphate come-- 296 00:14:39,970 --> 00:14:40,360 ERIC S. LANDER: Sorry. 297 00:14:40,360 --> 00:14:40,835 STUDENT: [INAUDIBLE] 298 00:14:40,835 --> 00:14:41,310 G3P. 299 00:14:41,310 --> 00:14:44,360 ERIC S. LANDER: An inorganic phosphate I should have drawn there too. 300 00:14:44,360 --> 00:14:45,340 STUDENT: [INAUDIBLE] 301 00:14:45,340 --> 00:14:45,670 ERIC S. LANDER: Yeah, yeah, yeah. 302 00:14:45,670 --> 00:14:46,680 Use an inorganic phosphate. 303 00:14:46,680 --> 00:14:48,550 Sorry. 304 00:14:48,550 --> 00:14:52,140 Plus an inorganic phosphate. 305 00:14:52,140 --> 00:14:54,790 All right, before you go onto the next segment, we've got a question for you 306 00:14:54,790 --> 00:14:56,360 about ATP and glycolysis. 22242

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