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These are the user uploaded subtitles that are being translated: 0 00:00:00,000 --> 00:00:01,812 PROFESSOR: Welcome back. 1 00:00:01,812 --> 00:00:02,720 You're still here. 2 00:00:02,720 --> 00:00:04,850 That's good, everybody is still here. 3 00:00:04,850 --> 00:00:11,430 And what I want to do today is pick up on our themes from biochemistry. 4 00:00:11,430 --> 00:00:18,090 We last time, you will recall, looked at our code of arms. 5 00:00:18,090 --> 00:00:23,950 Biological function, two ways of understanding it-- 6 00:00:23,950 --> 00:00:29,185 biochemistry, genetics. 7 00:00:35,490 --> 00:00:41,010 Proteins are what I said are the molecules of major interest in 8 00:00:41,010 --> 00:00:42,040 biochemistry. 9 00:00:42,040 --> 00:00:45,422 Because proteins are amazingly diverse. 10 00:00:45,422 --> 00:00:51,370 Now lipids, they're good, carbohydrates are OK, but proteins 11 00:00:51,370 --> 00:00:54,100 have stunning, stunning diversity. 12 00:00:54,100 --> 00:00:59,040 And when we talked about Buchner and the discovery of enzymes, these 13 00:00:59,040 --> 00:01:02,420 amazing things that could carry out chemical transformations, what was 14 00:01:02,420 --> 00:01:05,200 really going on was proteins. 15 00:01:05,200 --> 00:01:07,810 So that's what we're planning to do today is understand the 16 00:01:07,810 --> 00:01:09,700 structure of proteins. 17 00:01:09,700 --> 00:01:13,620 So what have we understood so far? 18 00:01:13,620 --> 00:01:17,480 Well, we've understood atoms-- 19 00:01:17,480 --> 00:01:18,220 well, barely. 20 00:01:18,220 --> 00:01:21,420 We've given brief cursory mention to the existence of atoms. 21 00:01:21,420 --> 00:01:24,340 You'll have to take a chemistry course to really understand atoms. 22 00:01:24,340 --> 00:01:27,950 We've mentioned molecules, we've mentioned bonds, and we've done some 23 00:01:27,950 --> 00:01:34,620 just enough to have a handle on the different kinds of bonds that get made 24 00:01:34,620 --> 00:01:36,960 that help us understand biological molecules. 25 00:01:36,960 --> 00:01:41,055 And we've done injustice to all of the wonderful things that bonds really do 26 00:01:41,055 --> 00:01:42,060 in all of the details. 27 00:01:42,060 --> 00:01:45,830 But you know enough with covalent bonds, with hydrogen bonds, with ionic 28 00:01:45,830 --> 00:01:48,930 bonds, with van der Waals interactions, and with this thing that 29 00:01:48,930 --> 00:01:50,230 isn't the bond. 30 00:01:50,230 --> 00:01:53,710 It's hydrophobic forces, it's entropy-- 31 00:01:53,710 --> 00:01:57,890 folding something in to avoid breaking up other good bonds. 32 00:01:57,890 --> 00:01:59,170 So we've done that. 33 00:01:59,170 --> 00:02:00,790 We then looked at examples. 34 00:02:00,790 --> 00:02:05,520 We looked at the examples of lipids and showed how a molecule that was 35 00:02:05,520 --> 00:02:10,240 amphipathic had a partly hydrophobic tail-- 36 00:02:10,240 --> 00:02:13,420 that was part hydrophobic, had a very hydrophobic tail and a very 37 00:02:13,420 --> 00:02:15,000 hydrophilic head-- 38 00:02:15,000 --> 00:02:19,860 would spontaneously organize into a shape like a lipid bilayer that could 39 00:02:19,860 --> 00:02:23,940 wrap a cell, and you didn't need any magic to make the membrane of a cell. 40 00:02:23,940 --> 00:02:29,050 You could simply invoke the laws here of chemistry and make a membrane. 41 00:02:29,050 --> 00:02:30,300 So we did lipids. 42 00:02:33,750 --> 00:02:40,280 We talked about ATP, a high energy molecule that has three very 43 00:02:40,280 --> 00:02:43,050 negatively-charged groups right next to each other. 44 00:02:43,050 --> 00:02:48,420 And we anticipated, and we're going to see in the class, that that is a great 45 00:02:48,420 --> 00:02:49,100 source of energy. 46 00:02:49,100 --> 00:02:51,500 When you need to get energy for reaction, you're going to break those 47 00:02:51,500 --> 00:02:52,870 bonds and use it. 48 00:02:52,870 --> 00:03:00,230 And then, we talked about sugars and carbohydrates. 49 00:03:00,230 --> 00:03:05,820 Sugars are important because, of course, that is what Buchner's yeast-- 50 00:03:05,820 --> 00:03:07,070 carbohydrates-- 51 00:03:11,850 --> 00:03:13,100 was digesting. 52 00:03:13,100 --> 00:03:19,910 It was digesting sugars to make alcohol and carbon dioxide. 53 00:03:19,910 --> 00:03:25,260 Well, it turns out the digestion of sugars is not a trivial matter at all. 54 00:03:25,260 --> 00:03:29,480 Sugars are the fundamental energy source for most cells. 55 00:03:29,480 --> 00:03:33,410 And we're going to look a lot more deeply into understanding how sugars 56 00:03:33,410 --> 00:03:34,270 are digested. 57 00:03:34,270 --> 00:03:38,800 In fact, lecture number five is going to be all about the 58 00:03:38,800 --> 00:03:40,710 digestion of sugars. 59 00:03:40,710 --> 00:03:45,320 But to get to any of that, we have to go to one of the most interesting 60 00:03:45,320 --> 00:03:46,420 molecule types-- 61 00:03:46,420 --> 00:03:47,050 proteins. 62 00:03:47,050 --> 00:03:49,270 And that's the subject of today's lecture. 63 00:03:49,270 --> 00:03:53,260 So proteins-- 64 00:03:56,580 --> 00:03:59,623 and particularly today, protein structure-- 65 00:04:02,150 --> 00:04:04,730 all right, so that's where we were. 66 00:04:04,730 --> 00:04:05,980 Section one-- 67 00:04:09,430 --> 00:04:15,065 proteins, primary structure. 68 00:04:22,670 --> 00:04:24,680 Proteins have four levels of structure. 69 00:04:24,680 --> 00:04:27,020 They have primary structure, secondary structure, tertiary structure, 70 00:04:27,020 --> 00:04:29,820 quaternary structure as you might imagine if you have four levels. 71 00:04:29,820 --> 00:04:34,010 And we're going to start with the primary structure of proteins. 72 00:04:34,010 --> 00:04:38,640 It's actually ridiculously simple, the primary structure of proteins. 73 00:04:38,640 --> 00:04:41,400 You need to know what the building block is, and then you need to know 74 00:04:41,400 --> 00:04:43,610 how the building blocks are joined together. 75 00:04:43,610 --> 00:04:46,680 And then, you can join together as many building blocks as you want to. 76 00:04:46,680 --> 00:04:50,060 The building block is called an amino acid. 77 00:04:53,090 --> 00:04:57,410 And amino acids have a very simple structure. 78 00:04:57,410 --> 00:05:02,970 In the middle is a carbon, and it's like the big dog carbon here. 79 00:05:02,970 --> 00:05:04,990 It's called the alpha carbon. 80 00:05:04,990 --> 00:05:10,320 We write C alpha to indicate how important that carbon is there. 81 00:05:10,320 --> 00:05:13,470 And it has four bonds it's going to make. 82 00:05:13,470 --> 00:05:17,330 One of those bonds is always just plain hydrogen. 83 00:05:17,330 --> 00:05:23,550 One of those bonds is an amino group. 84 00:05:26,900 --> 00:05:28,480 One of these bonds here-- 85 00:05:32,060 --> 00:05:33,310 a carboxyl group. 86 00:05:36,110 --> 00:05:41,680 And one of these bonds here connects to something else. 87 00:05:41,680 --> 00:05:43,660 And I'm writing an R there. 88 00:05:43,660 --> 00:05:46,000 R means something else. 89 00:05:46,000 --> 00:05:55,040 That something else is referred to as the side chain of the amino acid here. 90 00:05:55,040 --> 00:05:56,980 So we have a side chain, and I'm not going to say what the 91 00:05:56,980 --> 00:05:57,970 side chains are yet. 92 00:05:57,970 --> 00:05:59,900 We're going to come to them in just a moment. 93 00:05:59,900 --> 00:06:01,560 So we've got four bonds. 94 00:06:01,560 --> 00:06:07,380 It's always an amino, always a carboxyl, always a hydrogen, and some 95 00:06:07,380 --> 00:06:08,480 side chain-- 96 00:06:08,480 --> 00:06:10,850 incredibly simple. 97 00:06:10,850 --> 00:06:13,270 Now, we're going to stick two of these guys together. 98 00:06:13,270 --> 00:06:14,640 So we're going to stick them together. 99 00:06:14,640 --> 00:06:28,730 I'm going to make another amino acid here, another alpha carbon, and 100 00:06:28,730 --> 00:06:29,900 another side chain. 101 00:06:29,900 --> 00:06:32,980 And maybe, since that was the side chain of the first amino acid, I'll 102 00:06:32,980 --> 00:06:36,110 label it, side chain number one, and I'll label this guy, side 103 00:06:36,110 --> 00:06:38,080 chain number two. 104 00:06:38,080 --> 00:06:39,640 That's it. 105 00:06:39,640 --> 00:06:43,800 Now, we are going to pull off the standard reaction, which basically 106 00:06:43,800 --> 00:06:48,430 makes everything in this course go, which is dehydration synthesis. 107 00:06:48,430 --> 00:06:51,590 We're going to take two monomers, and we're going to connect these two 108 00:06:51,590 --> 00:06:57,220 monomers by eliminating a water here. 109 00:06:57,220 --> 00:07:01,890 So the reaction kicks out this water. 110 00:07:01,890 --> 00:07:07,670 This OH and this H comes off as a water. 111 00:07:07,670 --> 00:07:10,520 And we get a bond here. 112 00:07:10,520 --> 00:07:14,020 And that bond is called the peptide bond. 113 00:07:14,020 --> 00:07:16,520 So let's take a look at it here. 114 00:07:16,520 --> 00:07:33,025 We have a peptide bond C alpha, C alpha, over here. 115 00:07:35,910 --> 00:07:45,200 And we've got another OH there that could be used to go on and on and on. 116 00:07:45,200 --> 00:07:49,570 So here is our first amino acid here. 117 00:07:49,570 --> 00:07:52,160 Here's the second amino acid here. 118 00:07:52,160 --> 00:07:53,860 And we could keep going-- 119 00:07:57,860 --> 00:08:03,940 another C alpha here, and onward. 120 00:08:03,940 --> 00:08:10,890 So this peptide bond is a very special bond. 121 00:08:10,890 --> 00:08:12,790 It's what's joining together the monomers. 122 00:08:12,790 --> 00:08:15,130 And that peptide bond-- 123 00:08:15,130 --> 00:08:20,690 single bonds can rotate freely, double bonds cannot rotate freely. 124 00:08:20,690 --> 00:08:26,300 Although I call this a single bond, it has the chemists say partial double 125 00:08:26,300 --> 00:08:28,000 bond character. 126 00:08:28,000 --> 00:08:30,910 That means, it really doesn't rotate very freely. 127 00:08:30,910 --> 00:08:38,120 And we can think about this thing here as kind of a plane, 128 00:08:38,120 --> 00:08:39,750 a planar bond there. 129 00:08:42,770 --> 00:08:48,790 It can rotate here, it can rotate here, and we've got our side chains 130 00:08:48,790 --> 00:08:51,310 coming off, and they can rotate. 131 00:08:51,310 --> 00:08:56,155 Here's side chain number two, here's side chain number three, and again. 132 00:08:59,690 --> 00:09:04,360 So we have these peptide bonds, these planar bonds, and we have these side 133 00:09:04,360 --> 00:09:05,230 chains coming off. 134 00:09:05,230 --> 00:09:07,720 And you've got three angles to play with. 135 00:09:07,720 --> 00:09:11,196 You can turn this guy, you can turn that guy, you can turn that guy. 136 00:09:11,196 --> 00:09:14,000 That's it, that's all there is to a protein. 137 00:09:14,000 --> 00:09:17,500 Any questions about protein structure, the basic 138 00:09:17,500 --> 00:09:19,040 aspects of protein structure? 139 00:09:19,040 --> 00:09:23,160 When I talk about the primary structure of a protein, I just mean 140 00:09:23,160 --> 00:09:27,520 amino acid, amino acid, amino acid, amino acid, amino acid, amino acid, 141 00:09:27,520 --> 00:09:30,780 and the identities of which ones they are. 142 00:09:30,780 --> 00:09:32,820 So it's ridiculously simple-- sounds boring. 143 00:09:36,730 --> 00:09:40,600 Turns out it's not so boring. 144 00:09:40,600 --> 00:09:46,270 Turns out that these side chains can differ spectacularly. 145 00:09:46,270 --> 00:09:50,790 And when they differ spectacularly, they can make that chain fold up in 146 00:09:50,790 --> 00:09:53,100 all different sorts of ways. 147 00:09:53,100 --> 00:10:02,340 But to understand that, we have to go look at some of those amino acids. 148 00:10:02,340 --> 00:10:04,780 Let's make sure you've understood what you've just heard. 149 00:10:04,780 --> 00:10:06,040 Try answering these questions. 12100

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