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
Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.