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These are the user uploaded subtitles that are being translated: 1 00:00:09,760 --> 00:00:13,360 On scales far beyond human perception 2 00:00:13,360 --> 00:00:16,320 there are strange beasts... 3 00:00:16,320 --> 00:00:19,920 ..exquisite palaces... 4 00:00:19,920 --> 00:00:22,120 ..wondrous landscapes. 5 00:00:23,520 --> 00:00:28,360 Some just a few thousandths of a millimetre long. 6 00:00:28,360 --> 00:00:32,840 Others dominate the vast expanses of the cosmos. 7 00:00:34,440 --> 00:00:37,320 Thanks to ground-breaking new technologies, 8 00:00:37,320 --> 00:00:42,000 I'm setting out to explore these hidden worlds for the first time. 9 00:00:42,000 --> 00:00:44,800 You're looking at the craters and bumps and hills 10 00:00:44,800 --> 00:00:46,760 on the skin of bacteria. 11 00:00:48,440 --> 00:00:50,360 Mind-blowing to look at that. 12 00:00:52,800 --> 00:00:55,600 Each one of these dots is a galaxy. 13 00:00:57,240 --> 00:01:03,440 We have an instrument here that allows you to look at an atom. 14 00:01:03,440 --> 00:01:06,960 We can block the Covid-19 virus itself. Yeah. 15 00:01:06,960 --> 00:01:11,080 And at the tiniest and the largest scales, 16 00:01:11,080 --> 00:01:15,480 I'll see how physics has bizarre consequences. 17 00:01:15,480 --> 00:01:18,800 My journey will take me to the frontiers of modern science, 18 00:01:18,800 --> 00:01:23,840 revealing our latest discoveries and our biggest unanswered questions. 19 00:01:25,600 --> 00:01:28,960 This is the story of how the universe works 20 00:01:28,960 --> 00:01:31,920 at scales we can't normally see, 21 00:01:31,920 --> 00:01:36,000 from nanoparticles, to galactic superclusters. 22 00:01:47,440 --> 00:01:52,880 These are the very first images ever recorded of the microscopic world. 23 00:02:01,600 --> 00:02:04,960 They appeared in a book called Micrographia, 24 00:02:04,960 --> 00:02:08,560 written by the 17th century scientist Robert Hooke, 25 00:02:08,560 --> 00:02:11,040 using the first microscopes. 26 00:02:12,360 --> 00:02:14,360 Even at this magnification, 27 00:02:14,360 --> 00:02:17,480 they seem so unfamiliar. 28 00:02:17,480 --> 00:02:21,360 With Micrographia, three-and-a-half centuries ago, 29 00:02:21,360 --> 00:02:24,840 Hooke started us off on a voyage of discovery, 30 00:02:24,840 --> 00:02:28,520 into the universe at ever-smaller scales. 31 00:02:30,480 --> 00:02:33,680 As we began to see the microscopic world, 32 00:02:33,680 --> 00:02:37,320 we realised that it's very different from our own. 33 00:02:43,200 --> 00:02:47,320 These tiny insects have evolved extraordinary adaptations 34 00:02:47,320 --> 00:02:53,000 to navigate the world at scales we can barely imagine, 35 00:02:53,000 --> 00:02:55,000 because, when you're this small, 36 00:02:55,000 --> 00:02:59,160 the laws of physics have unexpected consequences. 37 00:03:00,880 --> 00:03:04,960 This is a type of wasp called Megaphragma, 38 00:03:04,960 --> 00:03:08,960 one of the smallest flying insects in the world. 39 00:03:08,960 --> 00:03:12,240 It's just a few tenths of a millimetre long, 40 00:03:12,240 --> 00:03:16,600 some five or ten times smaller than a flea. 41 00:03:16,600 --> 00:03:19,600 It has wings like paddles.. 42 00:03:22,520 --> 00:03:25,800 ..and flies in an unusual way. 43 00:03:25,800 --> 00:03:28,680 That's because air feels very different to it 44 00:03:28,680 --> 00:03:32,080 than it does to us. We're barely aware of the air around us 45 00:03:32,080 --> 00:03:34,160 as we move through it. 46 00:03:34,160 --> 00:03:38,720 And that's because of the science of air resistance. 47 00:03:38,720 --> 00:03:42,000 Take a golf ball and a ping-pong ball. 48 00:03:42,000 --> 00:03:46,480 It's easier to throw a golf ball than a ping-pong ball. 49 00:03:46,480 --> 00:03:49,280 They both have the same surface area 50 00:03:49,280 --> 00:03:52,880 and so feel the same air resistance. 51 00:03:52,880 --> 00:03:55,360 But the ping-pong ball is lighter, 52 00:03:55,360 --> 00:04:00,960 with less momentum and struggles to push through the air. 53 00:04:00,960 --> 00:04:04,680 Megaphragma is like a tiny ping-pong ball, 54 00:04:04,680 --> 00:04:08,360 with little momentum for its surface area, 55 00:04:08,360 --> 00:04:13,280 so, to it, the air feels more like a liquid 56 00:04:13,280 --> 00:04:19,520 and it's evolved its unusually shaped wings to swim through it. 57 00:04:19,520 --> 00:04:21,760 If you were to make this the size of a human, 58 00:04:21,760 --> 00:04:24,160 then it'd be barely able to move its wings, 59 00:04:24,160 --> 00:04:26,080 let alone use them to fly. 60 00:04:26,080 --> 00:04:31,000 Yet, it's so successively adapted to the world in which it exists that, 61 00:04:31,000 --> 00:04:34,960 in recent years, entomologists have found them all over the world, 62 00:04:34,960 --> 00:04:37,760 from Africa to the Pacific to South America, 63 00:04:37,760 --> 00:04:40,160 even in the woods outside London. 64 00:04:41,800 --> 00:04:44,600 When we look at even tinier objects, 65 00:04:44,600 --> 00:04:47,480 ten times smaller than Megaphragma, 66 00:04:47,480 --> 00:04:51,400 we come to the scale of a typical animal cell. 67 00:04:51,400 --> 00:04:53,920 As we increase magnification, 68 00:04:53,920 --> 00:04:58,000 the laws of physics become ever more strange. 69 00:05:02,440 --> 00:05:06,160 Professor Susan Anderson at the University of Nottingham 70 00:05:06,160 --> 00:05:08,720 uses powerful optical microscopes 71 00:05:08,720 --> 00:05:11,880 to study human heart cells. 72 00:05:11,880 --> 00:05:13,640 So, what is it we're seeing there? 73 00:05:13,640 --> 00:05:17,520 So, this is the sort of detail that we get in a light microscope. 74 00:05:17,520 --> 00:05:19,960 We have lots of individual cells here, 75 00:05:19,960 --> 00:05:22,480 so we can see individual cells. 76 00:05:22,480 --> 00:05:25,520 In each you can see nuclei. So these are the nuclei. 77 00:05:25,520 --> 00:05:28,840 The little bright spots are the nucleoli. 78 00:05:28,840 --> 00:05:31,920 This is the edge of the cell, and then the cytoplasm of the cell, 79 00:05:31,920 --> 00:05:34,560 you can't really see any detail inside. 80 00:05:34,560 --> 00:05:36,800 So, why is it that you're looking at these? 81 00:05:36,800 --> 00:05:40,480 The useful thing about this is that we can see dynamic cells, 82 00:05:40,480 --> 00:05:43,880 so the cells that we're looking at here are human heart muscle cells. 83 00:05:43,880 --> 00:05:46,120 So we can actually see them beating. 84 00:05:47,520 --> 00:05:49,840 Oh, wow, right, yes. Yeah. 85 00:05:49,840 --> 00:05:52,600 Seeing them beat in such detail 86 00:05:52,600 --> 00:05:56,800 means scientists can begin to understand why they go wrong. 87 00:05:56,800 --> 00:05:59,760 You can see the nucleus, you can see the outline of the cell here. 88 00:05:59,760 --> 00:06:02,440 You can see lots of them beating at about 30 beats per minute, 89 00:06:02,440 --> 00:06:05,640 which is about half the rate of a human heart. 90 00:06:05,640 --> 00:06:07,640 They're from a living heart? 91 00:06:07,640 --> 00:06:10,960 It would be difficult to do that ethically so what we do is 92 00:06:10,960 --> 00:06:13,800 we obtain stem cells from human skin. 93 00:06:13,800 --> 00:06:17,040 We reprogram the human skin cells back to stem cells 94 00:06:17,040 --> 00:06:19,560 and then we direct them down a differentiation pathway 95 00:06:19,560 --> 00:06:21,040 to being muscle cells 96 00:06:21,040 --> 00:06:23,200 and we can obviously see that they are contracting 97 00:06:23,200 --> 00:06:25,480 and beating like a heart muscle cell. 98 00:06:25,480 --> 00:06:27,120 What's actually happening here? 99 00:06:27,120 --> 00:06:30,560 The cytoplasm contains lots of contractile filaments 100 00:06:30,560 --> 00:06:34,400 and they're shortening and lengthening so that the cell beats. 101 00:06:34,400 --> 00:06:37,760 There's a whole community of cells here that are talking to each other 102 00:06:37,760 --> 00:06:40,320 and they're passing that signal from cell to cell 103 00:06:40,320 --> 00:06:43,200 and they're beating on mass. How does it make you feel 104 00:06:43,200 --> 00:06:47,200 when you're looking at these living cells? I love them. 105 00:06:47,200 --> 00:06:50,400 They've got personality. You know, they do what they want. 106 00:06:50,400 --> 00:06:53,680 If the light here is too bright they will just move, 107 00:06:53,680 --> 00:06:57,320 they will just walk away. They're very entertaining. 108 00:07:00,400 --> 00:07:04,160 Microscopes are key to understanding cells, 109 00:07:04,160 --> 00:07:06,040 because right across the living world, 110 00:07:06,040 --> 00:07:09,400 they're tiny compared to most everyday objects. 111 00:07:10,960 --> 00:07:14,040 For instance, a 200-tonne blue whale 112 00:07:14,040 --> 00:07:19,160 and a tiny Megaphragma are both made of cells that are similar in size, 113 00:07:19,160 --> 00:07:23,560 roughly between 100th and a 10th of a millimetre across. 114 00:07:23,560 --> 00:07:26,160 Why are cells this size? 115 00:07:28,040 --> 00:07:31,800 The answer lies in the fact that in certain crucial ways, 116 00:07:31,800 --> 00:07:33,840 small things are much more effective 117 00:07:33,840 --> 00:07:37,160 at interacting with the outside world than big things. 118 00:07:39,960 --> 00:07:43,440 Here is a lump of titanium. It's a very reactive metal, 119 00:07:43,440 --> 00:07:45,880 and I'm going to try and burn it. 120 00:07:50,280 --> 00:07:51,560 Nothing. 121 00:07:53,560 --> 00:07:57,320 But here is also titanium 122 00:07:57,320 --> 00:08:00,560 that has been crushed down into a powder. 123 00:08:08,800 --> 00:08:12,160 Powder titanium has far more of its surface, 124 00:08:12,160 --> 00:08:15,640 relative to its volume, exposed to the air, 125 00:08:15,640 --> 00:08:19,560 so it's got much more access to the oxygen in the air 126 00:08:19,560 --> 00:08:22,200 to help it burn. 127 00:08:22,200 --> 00:08:25,160 This applies to cells, too. 128 00:08:25,160 --> 00:08:29,920 Cells absorb nutrients and oxygen from the outside. 129 00:08:29,920 --> 00:08:31,880 Being small and, therefore, 130 00:08:31,880 --> 00:08:35,320 having a large surface area to volume ratio, 131 00:08:35,320 --> 00:08:38,040 means they can do this very effectively. 132 00:08:38,040 --> 00:08:40,360 If they were significantly larger, 133 00:08:40,360 --> 00:08:44,040 they wouldn't be able to take in what they need to survive. 134 00:08:45,560 --> 00:08:49,840 Ultimately, though, there's a limit to how small they can be. 135 00:08:49,840 --> 00:08:51,800 Cells are full of stuff - 136 00:08:51,800 --> 00:08:55,160 the nucleus, mitochondria, ribosomes - 137 00:08:55,160 --> 00:08:58,280 so it's a balance between making them small enough 138 00:08:58,280 --> 00:09:02,000 to maximise their surface area to volume ratio, 139 00:09:02,000 --> 00:09:05,640 yet big enough for their parts to perform their function. 140 00:09:07,400 --> 00:09:10,240 And their shape is crucial, too. 141 00:09:10,240 --> 00:09:14,920 For instance, some cells have found a way to increase surface area 142 00:09:14,920 --> 00:09:16,760 without changing volume. 143 00:09:16,760 --> 00:09:19,920 The cells in the walls of our digestive tract 144 00:09:19,920 --> 00:09:24,360 absorb the nutrients needed to sustain our entire body 145 00:09:24,360 --> 00:09:26,240 through their surface, 146 00:09:26,240 --> 00:09:30,800 so this surface needs to be as large as possible. 147 00:09:30,800 --> 00:09:32,520 How do they do this? 148 00:09:32,520 --> 00:09:37,000 How can cells maximise their surface to volume ratio 149 00:09:37,000 --> 00:09:39,200 without getting any smaller? 150 00:09:39,200 --> 00:09:42,560 Well, imagine this balloon is one of those cells. 151 00:09:42,560 --> 00:09:45,360 How can I increase its surface area 152 00:09:45,360 --> 00:09:49,360 without making it significantly smaller? Well... 153 00:09:54,000 --> 00:09:56,120 ..I can give it fingers. 154 00:09:56,120 --> 00:10:00,000 I've calculated these five fingers increase the surface area 155 00:10:00,000 --> 00:10:03,480 of this rubber glove by about 50% 156 00:10:03,480 --> 00:10:08,120 and, remarkably, evolution has adopted precisely this strategy. 157 00:10:15,560 --> 00:10:18,640 Welcome to my digestive tract. 158 00:10:18,640 --> 00:10:22,640 These protuberances are called microvilli. 159 00:10:22,640 --> 00:10:25,760 They're each about a 1,000th of a millimetre long, 160 00:10:25,760 --> 00:10:28,280 but just a few molecules wide, 161 00:10:28,280 --> 00:10:31,920 and there are millions of them. They stick out from the cells, 162 00:10:31,920 --> 00:10:34,640 dramatically increasing their surface area, 163 00:10:34,640 --> 00:10:38,360 and therefore their ability to absorb nutrients. 164 00:10:40,280 --> 00:10:43,320 Of course, the real thing is rather more impressive. 165 00:10:43,320 --> 00:10:47,200 Scientists have calculated that, because of the microvilli, 166 00:10:47,200 --> 00:10:53,040 our intestines have increased their surface area by up to 15 times. 167 00:11:00,480 --> 00:11:04,480 Modern optical microscopes have uncovered a strange world 168 00:11:04,480 --> 00:11:08,640 just a few thousandths of a millimetre in scale. 169 00:11:08,640 --> 00:11:11,840 A world very different from our own. 170 00:11:25,720 --> 00:11:31,680 All revealed by a device that is essentially remarkably simple. 171 00:11:31,680 --> 00:11:35,960 This is a modern but pretty basic compound microscope, 172 00:11:35,960 --> 00:11:39,120 and it works on the same principles as Robert Hooke's microscope 173 00:11:39,120 --> 00:11:42,320 from 400 years ago. It's so simple, really, 174 00:11:42,320 --> 00:11:45,920 because you just have two lenses, one in front of the other, 175 00:11:45,920 --> 00:11:50,400 and adjust them until you get this sharp, magnified image. 176 00:11:51,560 --> 00:11:57,080 The second lens multiplies the magnification of the first. 177 00:11:59,680 --> 00:12:04,960 There is, however, a fundamental problem with optical microscopes. 178 00:12:04,960 --> 00:12:07,680 As we increase magnification, 179 00:12:07,680 --> 00:12:11,040 images get more and more blurry. 180 00:12:11,040 --> 00:12:13,680 This is because light is a wave, 181 00:12:13,680 --> 00:12:17,120 so objects which are smaller than its wavelength 182 00:12:17,120 --> 00:12:19,640 are impossible to see clearly, 183 00:12:19,640 --> 00:12:23,320 which means optical microscopes hit a wall 184 00:12:23,320 --> 00:12:26,320 at about 1,000th of a millimetre. 185 00:12:26,320 --> 00:12:28,880 So the next step downwards 186 00:12:28,880 --> 00:12:31,520 means ditching light entirely 187 00:12:31,520 --> 00:12:34,880 and finding something else to see with, 188 00:12:34,880 --> 00:12:39,040 like tiny subatomic particles. Electrons. 189 00:12:41,040 --> 00:12:43,240 I've found a bit of old technology, 190 00:12:43,240 --> 00:12:46,520 something older viewers might recognise. 191 00:12:46,520 --> 00:12:50,200 I've taken the back off this old TV set, 192 00:12:50,200 --> 00:12:54,080 so what you can see here is called a cathode-ray tube. 193 00:12:54,080 --> 00:12:58,280 This bit, the cathode, boils off electrons 194 00:12:58,280 --> 00:13:01,840 which are then accelerated in a vacuum 195 00:13:01,840 --> 00:13:05,280 to hit the phosphorous screen at the front. 196 00:13:07,160 --> 00:13:09,480 Now, ordinarily on a TV set, 197 00:13:09,480 --> 00:13:13,880 the electron beam scans across the whole surface of the screen 198 00:13:13,880 --> 00:13:16,680 to produce the picture. But I've rigged this now 199 00:13:16,680 --> 00:13:20,080 so that it produces just a single, narrow beam of electrons 200 00:13:20,080 --> 00:13:21,840 forming a spot in the middle. 201 00:13:21,840 --> 00:13:24,240 Now, because electrons are negatively charged, 202 00:13:24,240 --> 00:13:26,720 they're affected by a magnetic field. 203 00:13:26,720 --> 00:13:29,520 In fact, that's how we control the direction of the beam. 204 00:13:29,520 --> 00:13:33,400 And to show that, I've got a small magnet at the end of this stick, 205 00:13:33,400 --> 00:13:37,280 which I can use to distort 206 00:13:37,280 --> 00:13:40,480 and move the direction of the beam. 207 00:13:43,840 --> 00:13:46,440 In fact, you can see it's produced three spots. 208 00:13:46,440 --> 00:13:48,760 That's because there are three electron beams, 209 00:13:48,760 --> 00:13:51,160 because this is a colour TV. 210 00:13:51,160 --> 00:13:53,480 Now I've got it working normally. 211 00:13:53,480 --> 00:13:56,440 The electron beam is scanning across the whole screen 212 00:13:56,440 --> 00:13:58,120 to produce the full picture. 213 00:13:58,120 --> 00:14:02,440 But I can still distort this picture using my magnet. 214 00:14:11,360 --> 00:14:14,360 So, if magnets can be used to control and direct 215 00:14:14,360 --> 00:14:16,360 the path of an electron beam, 216 00:14:16,360 --> 00:14:19,560 they can also be used to focus a beam of electrons, 217 00:14:19,560 --> 00:14:21,920 in the same way that a glass lens 218 00:14:21,920 --> 00:14:24,280 can be used to focus a beam of light. 219 00:14:24,280 --> 00:14:27,440 And this means that we can use electrons 220 00:14:27,440 --> 00:14:30,080 to make an electron microscope. 221 00:14:44,040 --> 00:14:47,960 This is a modern electron microscope and, in many ways, 222 00:14:47,960 --> 00:14:52,280 it resembles Robert Hooke's optical microscope from 400 years ago. 223 00:14:52,280 --> 00:14:55,040 But this one uses a beam of electrons, 224 00:14:55,040 --> 00:14:57,960 just like in the back of that old TV set. 225 00:14:59,640 --> 00:15:02,240 Here's where the electron beam is generated. 226 00:15:02,240 --> 00:15:05,400 Electromagnetic lenses focus the beam here. 227 00:15:05,400 --> 00:15:07,920 This is where the object is placed. 228 00:15:07,920 --> 00:15:12,120 More lenses here magnify the image thousands of times. 229 00:15:12,120 --> 00:15:15,560 And this is a screen which turns the electron image 230 00:15:15,560 --> 00:15:17,760 into something we can see. 231 00:15:17,760 --> 00:15:19,240 With microscopes like this, 232 00:15:19,240 --> 00:15:22,400 scientists were suddenly able to see objects hundreds, 233 00:15:22,400 --> 00:15:26,760 even thousands of times smaller than they'd ever been able to before. 234 00:15:28,680 --> 00:15:33,440 We could see tiny details on the bodies of insects 235 00:15:33,440 --> 00:15:38,360 and the machinery within cells that made them function. 236 00:15:38,360 --> 00:15:44,160 And then we came face-to-face with one of our deadliest enemies. 237 00:15:47,280 --> 00:15:52,400 This is an infectious bronchitis virus. 238 00:15:52,400 --> 00:15:55,480 And these are common cold viruses. 239 00:15:56,520 --> 00:15:59,760 On them, you can see something strange, 240 00:15:59,760 --> 00:16:04,320 a kind of halo surrounding the virus. 241 00:16:04,320 --> 00:16:06,840 They were, in fact, tiny spikes, 242 00:16:06,840 --> 00:16:11,040 each one just 100 millionth of a metre across, 243 00:16:11,040 --> 00:16:13,720 and they gave the virus a crown shape. 244 00:16:13,720 --> 00:16:16,640 So they named this new class of viruses 245 00:16:16,640 --> 00:16:19,200 after the corona of the sun. 246 00:16:19,200 --> 00:16:22,400 These are all coronaviruses. 247 00:16:25,240 --> 00:16:31,880 In 2020, electron microscopes helped to identify a new virus - 248 00:16:31,880 --> 00:16:36,480 SARS-CoV-2, or Covid-19. 249 00:16:40,760 --> 00:16:45,440 Professor Pippa Hawes studies viruses like Covid-19 250 00:16:45,440 --> 00:16:47,280 for the Pirbright Institute. 251 00:16:47,280 --> 00:16:51,920 How have electron microscopes allowed us to understand Covid-19? 252 00:16:51,920 --> 00:16:55,120 They've been crucial because they've allowed us to investigate 253 00:16:55,120 --> 00:16:58,480 the structure of the virus, so we can actually identify it. 254 00:16:58,480 --> 00:17:02,640 So here we have the Covid-19 virus itself. Yeah. 255 00:17:02,640 --> 00:17:05,920 We can see the spike protein very, very clearly here, 256 00:17:05,920 --> 00:17:07,520 around the outside of the virus. 257 00:17:07,520 --> 00:17:10,280 And inside is the viral RNA. 258 00:17:11,760 --> 00:17:17,840 Like all viruses, Covid needs to hijack another cell to reproduce. 259 00:17:17,840 --> 00:17:20,880 What does the virus do inside the cell? 260 00:17:20,880 --> 00:17:23,280 It takes over the cell machinery. 261 00:17:23,280 --> 00:17:27,280 The RNA gets placed inside the cytoplasm of the cell. 262 00:17:27,280 --> 00:17:30,560 This RNA is read by the cellular machinery 263 00:17:30,560 --> 00:17:33,200 and it's translated into viral proteins 264 00:17:33,200 --> 00:17:36,400 that the virus is using in order to replicate. 265 00:17:36,400 --> 00:17:39,320 So, by giving it its RNA, 266 00:17:39,320 --> 00:17:42,400 the virus is basically reprogramming the cell 267 00:17:42,400 --> 00:17:45,640 to get it to do its bidding. Yes, exactly. 268 00:17:48,200 --> 00:17:53,680 Incredibly, we can now see exactly how this happens. 269 00:17:53,680 --> 00:17:57,600 What are we looking at here? Where's the cell and where's the virus? 270 00:17:57,600 --> 00:18:00,960 The outside of the cell is outside of our field of view. Oh, OK, right. 271 00:18:00,960 --> 00:18:04,160 Yeah. So this is zooming in now on an infected cell. 272 00:18:04,160 --> 00:18:08,480 These are parts of the cell that the virus has taken over 273 00:18:08,480 --> 00:18:12,080 and formed into these double-membrane vesicles. 274 00:18:12,080 --> 00:18:15,960 So, these vesicles, then, are like the viruses' nest that it builds, 275 00:18:15,960 --> 00:18:18,760 to make a home for itself so that it can replicate? 276 00:18:18,760 --> 00:18:20,840 Yes, exactly. It's sometimes called a factory. 277 00:18:20,840 --> 00:18:24,160 It's where it produces more copies of the viral proteins, 278 00:18:24,160 --> 00:18:25,760 it produces more of the RNA 279 00:18:25,760 --> 00:18:28,240 and where it all comes together in the new viruses. 280 00:18:28,240 --> 00:18:32,840 And can we see the individual viruses? Yes, if we go... 281 00:18:32,840 --> 00:18:34,240 Ooh. 282 00:18:34,240 --> 00:18:36,960 Here, these two are viruses 283 00:18:36,960 --> 00:18:40,120 that are actually budding into this vesicle, 284 00:18:40,120 --> 00:18:42,720 so these are forming viruses. 285 00:18:42,720 --> 00:18:47,200 Sneaky. Yes! And so, understanding this, 286 00:18:47,200 --> 00:18:50,480 I mean, does it allow us, then, to combat Covid-19? 287 00:18:50,480 --> 00:18:53,320 We need to know how the virus infects, 288 00:18:53,320 --> 00:18:55,480 how it replicates and how it leaves, 289 00:18:55,480 --> 00:18:59,960 which would help with antiviral treatments to prevent the disease. 290 00:19:02,000 --> 00:19:05,480 Seeing things at this scale has revealed 291 00:19:05,480 --> 00:19:09,360 an incredible new world to scientists. 292 00:19:24,680 --> 00:19:29,320 They could see and begin to understand how genetics worked 293 00:19:29,320 --> 00:19:32,760 by seeing single chromosomes. 294 00:19:32,760 --> 00:19:37,400 They could watch a white blood cell attacking an infection. 295 00:19:37,400 --> 00:19:40,080 And they could now see beyond the living world, 296 00:19:40,080 --> 00:19:44,120 deep into the materials that surround us. 297 00:19:45,760 --> 00:19:48,640 How cracks move through metals. 298 00:19:53,000 --> 00:19:58,400 Then, in 1991, a group in Japan saw this - 299 00:19:58,400 --> 00:20:03,040 strange shapes forming at the end of a sparking filament. 300 00:20:04,960 --> 00:20:08,040 Ten times smaller than a virus. 301 00:20:08,040 --> 00:20:11,000 They were carbon nanotubes, 302 00:20:11,000 --> 00:20:13,120 each a long cylinder 303 00:20:13,120 --> 00:20:17,360 whose walls were just a single carbon atom thick. 304 00:20:17,360 --> 00:20:20,600 And they had unexpected properties, 305 00:20:20,600 --> 00:20:25,240 which has led to an explosion of fascinating new materials. 306 00:20:27,240 --> 00:20:31,520 This is one of the blackest materials in the world. 307 00:20:31,520 --> 00:20:34,600 See, it might look to you like a flat black square 308 00:20:34,600 --> 00:20:37,360 but, in fact, if you look at it side on, 309 00:20:37,360 --> 00:20:41,000 or even at the back, you can see it's got contours, it's got dents. 310 00:20:41,000 --> 00:20:43,400 And yet, looking at it face on, 311 00:20:43,400 --> 00:20:46,280 there's nothing, just pure blackness. 312 00:20:47,960 --> 00:20:49,880 Now, normally when we see objects, 313 00:20:49,880 --> 00:20:52,640 light bounces off of them into our eyes 314 00:20:52,640 --> 00:20:54,800 at different wavelengths and different angles 315 00:20:54,800 --> 00:20:59,480 so we can see colour and shape. But this is like a Harry Potter spell. 316 00:20:59,480 --> 00:21:03,520 Light falls on the surface and then just disappears forever. 317 00:21:05,200 --> 00:21:07,320 What's perhaps most surprising 318 00:21:07,320 --> 00:21:11,440 is that this paint is made of nanotubes. 319 00:21:14,320 --> 00:21:16,520 The paint, called Vantablack, 320 00:21:16,520 --> 00:21:20,760 is the invention of nanotechnology scientist Ben Jensen. 321 00:21:23,320 --> 00:21:25,680 So it just looks like a black surface here, 322 00:21:25,680 --> 00:21:29,320 but talk me through what it looks like if you zoom in. 323 00:21:29,320 --> 00:21:32,280 So, if you imagine a forest of trees, 324 00:21:32,280 --> 00:21:34,720 but the trees are thousands of metres tall 325 00:21:34,720 --> 00:21:37,440 and they're all straight and they're all equally spaced. 326 00:21:37,440 --> 00:21:39,760 So light comes in, photons come in, 327 00:21:39,760 --> 00:21:42,160 and they effectively bounce between the trees 328 00:21:42,160 --> 00:21:44,600 and then they're absorbed after a number of bounces. 329 00:21:44,600 --> 00:21:46,600 So, as you can see on here, 330 00:21:46,600 --> 00:21:50,160 it looks like a very, very thick, lush carpet. 331 00:21:50,160 --> 00:21:53,760 So light coming in gets in between the nanotubes and bounces around 332 00:21:53,760 --> 00:21:56,960 and is eventually absorbed into the substrate. 333 00:21:56,960 --> 00:21:59,680 It looks like a brush. Yes, exactly. 334 00:22:03,320 --> 00:22:07,040 I want to get across to you just how black this material is. 335 00:22:08,280 --> 00:22:10,480 This card has been painted with the blackest 336 00:22:10,480 --> 00:22:12,320 commercially available paint. 337 00:22:12,320 --> 00:22:14,840 It's called Black 3.0. 338 00:22:14,840 --> 00:22:17,120 And, yeah, it looks very black. 339 00:22:17,120 --> 00:22:20,640 But put it alongside the Vantablack, 340 00:22:20,640 --> 00:22:23,520 and if I shine a light on them, 341 00:22:23,520 --> 00:22:27,360 you can see the paint just looks grey in comparison. 342 00:22:27,360 --> 00:22:29,080 And even more impressive, 343 00:22:29,080 --> 00:22:33,200 if I make an angle so that the light bounces off the surface 344 00:22:33,200 --> 00:22:34,960 and hopefully into the camera, 345 00:22:34,960 --> 00:22:38,280 you can see that this paint looks a lot brighter 346 00:22:38,280 --> 00:22:40,320 because the light has been reflected. 347 00:22:40,320 --> 00:22:43,320 But if I do the same thing with the Vantablack, 348 00:22:43,320 --> 00:22:45,640 you should see no difference at all. 349 00:22:45,640 --> 00:22:49,520 All the light is being absorbed. None of it is reflected. 350 00:22:52,000 --> 00:22:56,960 What is it useful for? So its main uses are in satellite systems, 351 00:22:56,960 --> 00:22:59,520 for controlling stray light from the sun, 352 00:22:59,520 --> 00:23:02,000 the moon and the Earth when you're looking out at stars. 353 00:23:02,000 --> 00:23:04,280 It's also used for calibrating infrared cameras 354 00:23:04,280 --> 00:23:07,920 that look at the Earth for global warming studies. And terrestrially, 355 00:23:07,920 --> 00:23:11,760 it's used to protect cars with autonomous driving modes 356 00:23:11,760 --> 00:23:13,880 from sunlight entering the camera systems 357 00:23:13,880 --> 00:23:16,560 and causing ghosting and loss of signal. 358 00:23:19,160 --> 00:23:21,760 For me, this is an entirely unexpected 359 00:23:21,760 --> 00:23:26,720 and surprising property of nanotubes and, more importantly, 360 00:23:26,720 --> 00:23:32,040 this is nanotechnology that we can see. Or, rather, not see. 361 00:23:33,600 --> 00:23:36,920 Glimpsing tiny nanotubes was impressive, 362 00:23:36,920 --> 00:23:39,400 but could we go even further? 363 00:23:39,400 --> 00:23:44,320 By the 1980s, scientists were trying to see ever smaller things, 364 00:23:44,320 --> 00:23:47,040 using a completely different approach. 365 00:23:47,040 --> 00:23:50,920 They wondered if they could see by feeling. 366 00:23:50,920 --> 00:23:54,000 Basically, the idea was to mimic the way the needle 367 00:23:54,000 --> 00:23:56,040 on an old record player works. 368 00:24:01,000 --> 00:24:04,480 A stylus passes along a groove on a record 369 00:24:04,480 --> 00:24:07,800 and the tiny bumps vibrate the needle, 370 00:24:07,800 --> 00:24:09,880 making music. 371 00:24:09,880 --> 00:24:11,880 MUSIC PLAYS 372 00:24:11,880 --> 00:24:12,920 MUSIC STOPS 373 00:24:14,040 --> 00:24:17,720 But, of course, the tip of a record player stylus 374 00:24:17,720 --> 00:24:21,920 is far too big to feel something as small as an atom. 375 00:24:21,920 --> 00:24:25,160 But then, in 1982, two scientists - 376 00:24:25,160 --> 00:24:28,000 Heinrich Rohrer and Gerd Binnig - 377 00:24:28,000 --> 00:24:30,000 had an ingenious idea. 378 00:24:30,000 --> 00:24:34,520 They put a thin metal spike into a corrosive liquid. 379 00:24:34,520 --> 00:24:36,120 Using electrical currents, 380 00:24:36,120 --> 00:24:39,600 they slowly dissolved away the tip of the spike 381 00:24:39,600 --> 00:24:43,040 so that just a very thin needle of metal remained. 382 00:24:43,040 --> 00:24:46,720 Its tip was just a few atoms in diameter. 383 00:24:48,000 --> 00:24:51,040 But how could this needle see? 384 00:24:51,040 --> 00:24:55,120 One idea was to harness an unusual force of nature. 385 00:24:57,640 --> 00:24:59,800 This is a gecko. 386 00:24:59,800 --> 00:25:04,000 Its feet stick to the glass using a tiny attractive force 387 00:25:04,000 --> 00:25:06,240 called the van der Waals force. 388 00:25:09,000 --> 00:25:13,240 Van der Waals forces exist because of a rather quirky aspect 389 00:25:13,240 --> 00:25:15,640 of atoms and molecules. 390 00:25:15,640 --> 00:25:19,200 Think of an atom as a tiny positively charged nucleus 391 00:25:19,200 --> 00:25:23,360 surrounded by a cloud of negatively charged electrons. 392 00:25:25,640 --> 00:25:29,600 But, crucially, these electron clouds aren't static, 393 00:25:29,600 --> 00:25:33,440 they fluctuate in shape, often randomly. 394 00:25:33,440 --> 00:25:35,720 So the clouds can become lopsided, 395 00:25:35,720 --> 00:25:38,840 with more electrons on one side than on the other. 396 00:25:40,800 --> 00:25:43,520 Because opposite charges attract, 397 00:25:43,520 --> 00:25:45,720 the negative end of one molecule 398 00:25:45,720 --> 00:25:48,800 is pulled towards the positive end of another. 399 00:25:48,800 --> 00:25:53,160 The force that an individual atom feels is, of course, minuscule. 400 00:25:53,160 --> 00:25:56,640 But these effects can add up. 401 00:25:56,640 --> 00:26:00,000 And this, in turn, means that the molecules on the surface 402 00:26:00,000 --> 00:26:02,080 of an object can sometimes 403 00:26:02,080 --> 00:26:07,120 feel pulled towards the molecules on the surface of a nearby object. 404 00:26:09,000 --> 00:26:12,800 And that's what the gecko is taking advantage of. 405 00:26:14,000 --> 00:26:18,720 A gecko's feet are covered with billions of tiny structures 406 00:26:18,720 --> 00:26:20,520 called spatulae. 407 00:26:21,760 --> 00:26:24,040 When these press against the glass, 408 00:26:24,040 --> 00:26:28,120 they flatten out, creating a huge surface area. 409 00:26:30,520 --> 00:26:33,640 Billions of atoms are now in contact. 410 00:26:37,720 --> 00:26:40,080 Then the tiny van der Waals forces 411 00:26:40,080 --> 00:26:43,920 combine and hold the gecko in place. 412 00:26:43,920 --> 00:26:46,080 And this was one of the forces 413 00:26:46,080 --> 00:26:50,360 Binnig and Rohrer believed they could harness. 414 00:26:50,360 --> 00:26:52,440 When a tiny stylus - 415 00:26:52,440 --> 00:26:55,920 and remember, its tip is just a few atoms wide - 416 00:26:55,920 --> 00:26:59,000 approaches atoms on the surface of the material, 417 00:26:59,000 --> 00:27:02,000 this is when the van der Waals forces come into play. 418 00:27:02,000 --> 00:27:05,560 Just like the spatulae on the foot of a gecko 419 00:27:05,560 --> 00:27:09,400 feels an attractive force between it and the molecules on the surface 420 00:27:09,400 --> 00:27:14,440 of the glass, so the stylus feels a force pulling it towards 421 00:27:14,440 --> 00:27:19,560 or pushing it away from the atoms as it passes over the surface. 422 00:27:20,680 --> 00:27:24,800 Measuring minuscule forces like these can paint a picture 423 00:27:24,800 --> 00:27:27,880 of the surface at the tiniest scale. 424 00:27:29,120 --> 00:27:32,440 This is a modern atomic force microscope. 425 00:27:33,720 --> 00:27:36,120 Dr Georgina Benn is using it 426 00:27:36,120 --> 00:27:39,080 to understand one of our deadliest enemies. 427 00:27:40,360 --> 00:27:43,400 I'm going to be imaging E coli, 428 00:27:43,400 --> 00:27:45,000 which are a type of bacteria. 429 00:27:45,000 --> 00:27:48,520 So, with a normal microscope, we could look at just the bacteria. 430 00:27:48,520 --> 00:27:51,200 But we need our atomic force microscope to be able to see 431 00:27:51,200 --> 00:27:52,440 the details on the surface. 432 00:27:53,720 --> 00:27:56,160 Why are we looking at the surface of E coli? 433 00:27:56,160 --> 00:27:59,680 So, E coli are really good at resisting antibiotics 434 00:27:59,680 --> 00:28:02,120 because they have this extra protective layer 435 00:28:02,120 --> 00:28:05,360 around the outside, and we want to know how the protective layer 436 00:28:05,360 --> 00:28:09,040 is arranged so that we can help people design antibiotics 437 00:28:09,040 --> 00:28:12,840 that can get through the protective layer more efficiently. 438 00:28:12,840 --> 00:28:16,800 So this is the full cell? The full bacteria? Yeah. 439 00:28:16,800 --> 00:28:21,320 So you can sort of start to see features on the surface. 440 00:28:23,200 --> 00:28:28,280 And these are already well below optical microscopy kind of sizes. 441 00:28:28,280 --> 00:28:31,840 Right. My scan's going to be 500 nanometres wide. 442 00:28:31,840 --> 00:28:35,200 So we're now looking at the surface of the bacteria? Yes. Yes. 443 00:28:35,200 --> 00:28:38,480 This is really impressive. 444 00:28:38,480 --> 00:28:41,120 What we're looking at here is bacteria skin 445 00:28:41,120 --> 00:28:43,920 and, you know, you're looking at the craters and bumps 446 00:28:43,920 --> 00:28:46,800 and hills on the skin of bacteria, 447 00:28:46,800 --> 00:28:51,920 to find these weak spots that we can attack with antibiotics. 448 00:28:53,920 --> 00:28:58,080 Each one of these black spots is a hole on the bacteria, 449 00:28:58,080 --> 00:29:02,520 which is about three millionths of a millimetre wide. 450 00:29:02,520 --> 00:29:06,600 These are the holes that let water and nutrients 451 00:29:06,600 --> 00:29:09,040 in and out of the cell. Right. 452 00:29:09,040 --> 00:29:12,840 So we're looking at how they're arranged, relative to each other. 453 00:29:12,840 --> 00:29:14,640 And what's interesting is that 454 00:29:14,640 --> 00:29:18,560 we've got this really tight lattice of pores. 455 00:29:18,560 --> 00:29:21,960 And then sometimes there are these gaps in your lattice. 456 00:29:21,960 --> 00:29:25,920 So those are the weak spots? We don't know. Oh, OK. 457 00:29:25,920 --> 00:29:28,480 So we want to know... That's, like, a next question - 458 00:29:28,480 --> 00:29:32,880 why these are important, why they would be there in the first place? 459 00:29:32,880 --> 00:29:38,120 So we know that some kind of patches will make the membrane weaker. 460 00:29:39,480 --> 00:29:41,080 And some of them will not. 461 00:29:41,080 --> 00:29:44,400 So, if you could get the bacteria to mutate 462 00:29:44,400 --> 00:29:48,680 so that it generates these weak spots... Yeah, or maybe... 463 00:29:48,680 --> 00:29:52,080 ..then you can attack it? Yes, or maybe get a drug 464 00:29:52,080 --> 00:29:56,680 that will make these weak spots, and then we could apply antibiotic. 465 00:30:01,000 --> 00:30:03,120 With the atomic force microscope, 466 00:30:03,120 --> 00:30:07,760 we began to see more detail of the world than ever before. 467 00:30:07,760 --> 00:30:10,520 But it had its limitations. 468 00:30:10,520 --> 00:30:15,320 They are most effective at seeing features on a flat surface. 469 00:30:16,960 --> 00:30:19,880 But atoms also connect up in three dimensions, 470 00:30:19,880 --> 00:30:22,720 often forming very complicated shapes which, in turn, 471 00:30:22,720 --> 00:30:24,680 affects their behaviour. 472 00:30:24,680 --> 00:30:27,880 How, then, can we see these shapes? 473 00:30:27,880 --> 00:30:32,440 Remember how visible light has a limit because of its wavelength? 474 00:30:32,440 --> 00:30:35,200 Well, it turns out there's another form of light 475 00:30:35,200 --> 00:30:38,200 which has a much, much smaller wavelength. 476 00:30:42,600 --> 00:30:44,320 X-rays. 477 00:30:44,320 --> 00:30:47,680 Crucially, X-rays have very short wavelength 478 00:30:47,680 --> 00:30:51,360 when compared to visible light. Now, the wavelengths of visible lights 479 00:30:51,360 --> 00:30:54,360 are just under a millionth of a metre 480 00:30:54,360 --> 00:30:55,960 but the wavelengths of X-rays 481 00:30:55,960 --> 00:30:59,000 are typically several thousand times shorter, 482 00:30:59,000 --> 00:31:02,600 at around a tenth of a billionth of a metre. 483 00:31:04,520 --> 00:31:06,920 But there are many differences. 484 00:31:06,920 --> 00:31:09,400 Our eyes can't detect X-rays. 485 00:31:09,400 --> 00:31:11,800 More importantly, they pack a punch. 486 00:31:11,800 --> 00:31:15,600 X-rays contain much more energy than rays of visible light. 487 00:31:15,600 --> 00:31:20,000 The intense energy of X-rays enables them to pass unhindered 488 00:31:20,000 --> 00:31:23,040 through soft tissue, like flesh and blood, 489 00:31:23,040 --> 00:31:28,920 which is as transparent to X-rays as glass is to visible light. 490 00:31:28,920 --> 00:31:33,560 The larger atoms that make up our bones do stop X-rays, 491 00:31:33,560 --> 00:31:36,560 so when you see an image like this, 492 00:31:36,560 --> 00:31:39,520 you're literally seeing an X-ray shadow, 493 00:31:39,520 --> 00:31:43,520 cast by your bones on photographic paper. 494 00:31:43,520 --> 00:31:45,560 This begs the question, 495 00:31:45,560 --> 00:31:49,600 can X-rays, which have such short wavelengths, 496 00:31:49,600 --> 00:31:54,400 be used to see things that are just too small for visible light? 497 00:31:55,960 --> 00:31:58,840 The first hints that this might be possible 498 00:31:58,840 --> 00:32:01,280 came in the early 20th century. 499 00:32:01,280 --> 00:32:06,000 Scientists noticed that when they shone X-rays through crystals, 500 00:32:06,000 --> 00:32:10,760 they produced weird spots arranged in patterns. 501 00:32:10,760 --> 00:32:12,920 These images may not look like much, 502 00:32:12,920 --> 00:32:15,000 but think of them as a kind of code. 503 00:32:15,000 --> 00:32:19,120 And by crackling it, you can deduce the way the atoms 504 00:32:19,120 --> 00:32:21,680 in the crystal are arranged. 505 00:32:21,680 --> 00:32:24,920 This process of turning images like these into an understanding 506 00:32:24,920 --> 00:32:29,000 of how substances are structured down at the atomic scale 507 00:32:29,000 --> 00:32:31,400 is known as X-ray crystallography. 508 00:32:35,400 --> 00:32:38,560 For a sense of how X-ray crystallography works, 509 00:32:38,560 --> 00:32:41,080 let's say each of these Christmas trees 510 00:32:41,080 --> 00:32:44,800 represents one of the atoms that makes up the crystal. 511 00:32:44,800 --> 00:32:48,920 To keep it simple, let's say they're all arranged in neat rows, 512 00:32:48,920 --> 00:32:50,520 just like these trees. 513 00:32:53,960 --> 00:32:57,640 What's important is that the wavelength of the X-rays 514 00:32:57,640 --> 00:33:01,360 striking the crystal is about the same as the distance 515 00:33:01,360 --> 00:33:06,360 between the rows of atoms, or the rows of trees in our analogy. 516 00:33:08,800 --> 00:33:11,920 Imagine an X-ray reflecting off the surface 517 00:33:11,920 --> 00:33:14,280 and the layer beneath. 518 00:33:14,280 --> 00:33:17,000 The beam that travels down to the next layer 519 00:33:17,000 --> 00:33:21,040 has a longer journey, and that is key. 520 00:33:22,760 --> 00:33:25,200 If the waves are now out of step 521 00:33:25,200 --> 00:33:28,760 and the peak of one coincides with the trough of the other, 522 00:33:28,760 --> 00:33:31,720 they then combine and cancel out. 523 00:33:33,080 --> 00:33:35,400 But if they're in step, 524 00:33:35,400 --> 00:33:37,360 the peaks combine, 525 00:33:37,360 --> 00:33:41,440 making a larger wave and a bright dot on the screen. 526 00:33:44,520 --> 00:33:46,000 By carefully measuring 527 00:33:46,000 --> 00:33:48,720 the angle at which the X-rays strike the crystal, 528 00:33:48,720 --> 00:33:51,440 where the dots appear, where they disappear, 529 00:33:51,440 --> 00:33:54,280 you can deduce the structure of the crystal. 530 00:33:56,440 --> 00:33:58,880 By decoding images like this, 531 00:33:58,880 --> 00:34:02,320 scientists in the early 20th century were able to deduce 532 00:34:02,320 --> 00:34:05,720 the structures of simple crystals, like rock salt. 533 00:34:05,720 --> 00:34:09,160 The atoms are arranged at each corner of a cube 534 00:34:09,160 --> 00:34:13,400 and the cubes repeat to form a 3D lattice. 535 00:34:13,400 --> 00:34:16,440 Most importantly, it meant we now knew the distance 536 00:34:16,440 --> 00:34:20,880 between the atoms. It's a third of a billionth of a metre. 537 00:34:23,320 --> 00:34:26,840 But for me, the story of X-ray crystallography 538 00:34:26,840 --> 00:34:28,960 really comes into its own 539 00:34:28,960 --> 00:34:33,160 because of one of the great heroes of British science - 540 00:34:33,160 --> 00:34:35,920 Dorothy Crowfoot Hodgkin. 541 00:34:37,200 --> 00:34:41,000 At Cambridge and Oxford in the 1930s and '40s, 542 00:34:41,000 --> 00:34:45,760 Hodgkin became fascinated by X-ray crystallography 543 00:34:45,760 --> 00:34:50,040 and she quickly established herself as one of the leading researchers. 544 00:34:52,360 --> 00:34:55,720 Her first big challenge came during the Second World War 545 00:34:55,720 --> 00:34:58,720 and her work on penicillin. 546 00:34:58,720 --> 00:35:02,400 Scientists had already noticed that the newly discovered penicillin 547 00:35:02,400 --> 00:35:05,520 had incredible antibacterial properties. 548 00:35:05,520 --> 00:35:08,240 It could stop infections in their tracks, 549 00:35:08,240 --> 00:35:11,800 literally bringing patients back from the brink of death. 550 00:35:11,800 --> 00:35:15,680 Now in the throws of war, understanding it and producing it 551 00:35:15,680 --> 00:35:18,280 in quantity was more important than ever. 552 00:35:21,080 --> 00:35:23,920 But penicillin was still a mystery, 553 00:35:23,920 --> 00:35:27,680 with a handful of atoms arranged in an unknown structure. 554 00:35:27,680 --> 00:35:31,000 So Hodgkin set her laboratory a challenge - 555 00:35:31,000 --> 00:35:35,160 use X-ray crystallography to learn its structure. 556 00:35:38,520 --> 00:35:43,560 Georgina Ferry is a science writer and biographer of Dorothy Hodgkin. 557 00:35:43,560 --> 00:35:44,920 Tell me about penicillin. 558 00:35:44,920 --> 00:35:48,600 What was so difficult about understanding its structure? 559 00:35:48,600 --> 00:35:51,920 The structure was unknown and, naturally, 560 00:35:51,920 --> 00:35:54,480 the organic chemists all came to Dorothy and said 561 00:35:54,480 --> 00:35:58,880 would she like to have a go at this? The first problem with it was that 562 00:35:58,880 --> 00:36:01,240 it doesn't make terribly good crystals. 563 00:36:01,240 --> 00:36:05,760 These are not ideal for putting into the X-ray apparatus. 564 00:36:05,760 --> 00:36:09,200 It took a while before they managed to get a version of penicillin 565 00:36:09,200 --> 00:36:14,160 that she was able to get a good image from. That image... 566 00:36:16,960 --> 00:36:18,560 ..looks like this. 567 00:36:18,560 --> 00:36:24,000 These are spots on photographic film that have been made by X-rays 568 00:36:24,000 --> 00:36:27,560 coming out of the crystal and hitting the photographic film. 569 00:36:27,560 --> 00:36:29,720 The dots are at different intensities. Some of them 570 00:36:29,720 --> 00:36:32,480 are very black, there's some down here that are very faint. 571 00:36:32,480 --> 00:36:36,560 And what she had to do was carry out a complicated 572 00:36:36,560 --> 00:36:38,720 mathematical calculation, 573 00:36:38,720 --> 00:36:42,040 which then enabled her to begin to understand 574 00:36:42,040 --> 00:36:45,880 where there was what's known as density 575 00:36:45,880 --> 00:36:47,640 in the molecule and in the crystal. 576 00:36:47,640 --> 00:36:50,840 And density means there's an atom there. And the final stage 577 00:36:50,840 --> 00:36:54,520 once you've done all those calculations, is to... 578 00:36:58,600 --> 00:37:02,000 ..to...essentially draw a contour map. 579 00:37:02,000 --> 00:37:04,640 This represents a slice through the molecule 580 00:37:04,640 --> 00:37:06,920 and the numbers that are written down 581 00:37:06,920 --> 00:37:09,920 represent the density of the electrons. 582 00:37:09,920 --> 00:37:13,600 And what she's done is join up areas of equivalent density, 583 00:37:13,600 --> 00:37:15,880 and that shows you that's a place where there's an atom, 584 00:37:15,880 --> 00:37:17,840 because there's a lot of intensity there. 585 00:37:17,840 --> 00:37:19,760 We're looking at a 2D picture here. 586 00:37:19,760 --> 00:37:23,960 So how did Hodgkin then go to the full 3D structure? 587 00:37:23,960 --> 00:37:27,920 What you want to do is take a number of slices, 588 00:37:27,920 --> 00:37:31,280 stack those one above the other, and that'll show you 589 00:37:31,280 --> 00:37:34,280 the three dimensional structure of the molecule. 590 00:37:37,320 --> 00:37:41,600 So, you can see, what we've got here is a stack of Perspex sheets 591 00:37:41,600 --> 00:37:43,640 of equal distances apart. 592 00:37:43,640 --> 00:37:47,800 And on each sheet, you've got the contour lines drawn, 593 00:37:47,800 --> 00:37:49,360 as we were looking at before. Mm. 594 00:37:49,360 --> 00:37:51,240 And if you're looking down from the top, 595 00:37:51,240 --> 00:37:54,480 you can see the three dimensional structure. 596 00:37:54,480 --> 00:37:57,920 This is the structure of penicillin 597 00:37:57,920 --> 00:38:02,600 that Hodgkin came up with after some four years of research. 598 00:38:02,600 --> 00:38:04,880 These are the carbon atoms, 599 00:38:04,880 --> 00:38:08,520 and they're connected by chemical bonds to other atoms. 600 00:38:08,520 --> 00:38:12,960 Oxygen, hydrogen, nitrogen, sulphur. 601 00:38:12,960 --> 00:38:15,440 But it's this section here 602 00:38:15,440 --> 00:38:19,000 that explains its incredible efficacy. 603 00:38:19,000 --> 00:38:21,960 It's called a beta-lactam ring 604 00:38:21,960 --> 00:38:26,040 and it seems to give penicillin its wondrous ability. 605 00:38:26,040 --> 00:38:30,320 It binds to a part of the cell wall of most bacteria, 606 00:38:30,320 --> 00:38:32,040 killing them dead. 607 00:38:32,040 --> 00:38:37,640 Understanding how penicillin works was a revolution in medicine. 608 00:38:37,640 --> 00:38:41,400 Hodgkin's work spawned a generation of new antibiotics, 609 00:38:41,400 --> 00:38:44,640 effective against many aggressive bacteria, 610 00:38:44,640 --> 00:38:47,680 saving millions of lives. 611 00:38:49,520 --> 00:38:53,400 And these techniques, still widely used today, 612 00:38:53,400 --> 00:38:57,840 famously went on to unlock the structure of DNA. 613 00:39:00,640 --> 00:39:04,200 Despite the achievements of X-ray crystallography, 614 00:39:04,200 --> 00:39:07,680 it was still an indirect method of seeing, 615 00:39:07,680 --> 00:39:10,040 and only worked for crystals. 616 00:39:10,040 --> 00:39:15,040 To see even smaller things would require something else. 617 00:39:15,040 --> 00:39:19,760 It seemed electron microscopes held the most potential, 618 00:39:19,760 --> 00:39:23,520 but they had a huge technical problem. 619 00:39:23,520 --> 00:39:25,680 Their electromagnetic lenses 620 00:39:25,680 --> 00:39:29,680 were fundamentally different from glass ones. 621 00:39:29,680 --> 00:39:33,320 One of the most common problems that affects lenses 622 00:39:33,320 --> 00:39:35,800 is called spherical aberration. 623 00:39:35,800 --> 00:39:38,800 You see, the way lenses work is that they bend the light 624 00:39:38,800 --> 00:39:42,080 that travels through them. But the amount of bending 625 00:39:42,080 --> 00:39:45,840 depends on which part of the lens the light travels through. 626 00:39:47,000 --> 00:39:50,640 So, when I try to focus the sun, for instance, 627 00:39:50,640 --> 00:39:53,840 I can never quite focus to a point. 628 00:39:53,840 --> 00:39:57,840 Which means, at high magnifications especially, 629 00:39:57,840 --> 00:40:01,520 parts of the image will always blur. 630 00:40:01,520 --> 00:40:04,920 Electron microscope lenses are exactly the same, 631 00:40:04,920 --> 00:40:08,520 they also suffer from spherical aberration. 632 00:40:08,520 --> 00:40:10,520 And at high magnification, 633 00:40:10,520 --> 00:40:14,040 the blurring was making the images unusable. 634 00:40:14,040 --> 00:40:17,720 Now, for glass lenses, this issue can be minimised. 635 00:40:17,720 --> 00:40:21,000 You add a second lens, a concave lens, 636 00:40:21,000 --> 00:40:23,440 which corrects for the first one, 637 00:40:23,440 --> 00:40:26,440 giving us a much sharper point. 638 00:40:26,440 --> 00:40:30,760 But this solution doesn't work with electron microscopes. 639 00:40:30,760 --> 00:40:33,920 The lenses of electron microscopes are fundamentally different 640 00:40:33,920 --> 00:40:38,840 from glass ones. There simply is no equivalent of a concave lens. 641 00:40:38,840 --> 00:40:43,640 The physics of electrons and electromagnetic fields forbids it. 642 00:40:43,640 --> 00:40:46,040 So it seemed that electron microscopes 643 00:40:46,040 --> 00:40:48,080 would always suffer from blurriness 644 00:40:48,080 --> 00:40:50,440 at very high levels of magnification. 645 00:40:56,560 --> 00:41:02,160 The question was whether we could delve deeper to see even smaller. 646 00:41:02,160 --> 00:41:06,000 Well, the next breakthrough that changed everything 647 00:41:06,000 --> 00:41:08,360 took place here in Germany. 648 00:41:13,080 --> 00:41:18,720 Two teams of headstrong scientists started to question the orthodoxy. 649 00:41:18,720 --> 00:41:20,840 There were three in Germany - 650 00:41:20,840 --> 00:41:23,080 Theoretician Harald Rose, 651 00:41:23,080 --> 00:41:25,840 experimentalist Max Haider, 652 00:41:25,840 --> 00:41:28,560 material scientist Knut Urban - 653 00:41:28,560 --> 00:41:33,560 and an American team led by Ondrej Krivanek. 654 00:41:33,560 --> 00:41:35,680 Everybody expected us to fail, 655 00:41:35,680 --> 00:41:39,040 and so we knew we could only exceed expectations. 656 00:41:39,040 --> 00:41:43,080 Each stubbornly believed that they could somehow overturn 657 00:41:43,080 --> 00:41:45,640 the established prevailing science 658 00:41:45,640 --> 00:41:49,040 and make an electron microscope that could see more. 659 00:41:49,040 --> 00:41:51,640 Perhaps even atoms. 660 00:41:51,640 --> 00:41:56,720 Was it a big challenge, then, to persuade the science world 661 00:41:56,720 --> 00:42:01,240 that here was something that was going to change the field? 662 00:42:01,240 --> 00:42:05,520 The science world, at that time, had essentially given up 663 00:42:05,520 --> 00:42:08,640 to have aberration-corrected electron optics. 664 00:42:08,640 --> 00:42:13,840 They decided that hardware aberration correction 665 00:42:13,840 --> 00:42:17,480 will be unthinkable. They said it was impossible? 666 00:42:17,480 --> 00:42:21,000 That it was impossible. We had three different people. 667 00:42:21,000 --> 00:42:24,000 Theoretician, experimentalist and material scientists, 668 00:42:24,000 --> 00:42:26,080 and I think this three together, 669 00:42:26,080 --> 00:42:28,240 that was just a point for its success. 670 00:42:28,240 --> 00:42:32,160 Their approach used multiple electron magnets, 671 00:42:32,160 --> 00:42:35,160 multipoles to distort the image, 672 00:42:35,160 --> 00:42:38,040 squeezing out the worst of the aberration. 673 00:42:38,040 --> 00:42:40,920 Then a second lens reformed the image, 674 00:42:40,920 --> 00:42:45,120 now almost aberration free. But getting it right was challenging. 675 00:42:45,120 --> 00:42:48,960 It would require sophisticated arrangements of multipoles, 676 00:42:48,960 --> 00:42:52,280 sensitive cameras and powerful computers. 677 00:43:18,200 --> 00:43:19,600 To bring it back again. 678 00:43:22,000 --> 00:43:25,840 For years, they struggled to get their new lenses to work, 679 00:43:25,840 --> 00:43:29,680 and the rest of the scientific community remained sceptical. 680 00:43:29,680 --> 00:43:33,520 I had a lovely comment from a professor at Stanford 681 00:43:33,520 --> 00:43:36,920 who told me, "Ondrej, you're burying your career." 682 00:43:36,920 --> 00:43:40,400 But then, in June 1997, 683 00:43:40,400 --> 00:43:43,280 their stubbornness began to pay off. 684 00:43:43,280 --> 00:43:48,280 And soon they caught glimpses of the building blocks of all matter 685 00:43:48,280 --> 00:43:51,640 with unprecedented clarity. 686 00:43:51,640 --> 00:43:55,400 Here's a typical image without aberration correction. 687 00:43:55,400 --> 00:43:58,400 Now watch as it's added in. 688 00:43:58,400 --> 00:44:03,000 The white blurs resolve into two clear dots, 689 00:44:03,000 --> 00:44:07,080 each one a single atom of silicone. 690 00:44:09,960 --> 00:44:12,000 Finally, you could see atoms. 691 00:44:12,000 --> 00:44:14,960 This was a real jump in innovation. 692 00:44:14,960 --> 00:44:17,360 This was a real paradigm change. 693 00:44:17,360 --> 00:44:20,240 What was it like when you saw those first images? 694 00:44:20,240 --> 00:44:21,800 Seeing is believing, 695 00:44:21,800 --> 00:44:25,360 and the mission impossible was not impossible. 696 00:44:25,360 --> 00:44:29,560 They had achieved a scientific miracle. 697 00:44:29,560 --> 00:44:33,120 It was like if you have a huge fog. 698 00:44:33,120 --> 00:44:35,560 But suddenly, the fog goes. 699 00:44:35,560 --> 00:44:37,600 Suddenly, you see everything. 700 00:44:37,600 --> 00:44:40,480 A new kind of electron microscope. 701 00:44:40,480 --> 00:44:43,480 It was brilliant. It was so unbelievable. 702 00:44:43,480 --> 00:44:48,240 And it's the most important effect of aberration correction. 703 00:44:48,240 --> 00:44:52,600 By 2020, they'd gone from academic outcasts 704 00:44:52,600 --> 00:44:56,360 to world-renowned scientists. 705 00:44:56,360 --> 00:44:58,800 The images that came out are truly spectacular, 706 00:44:58,800 --> 00:45:01,200 like the one on the cover of Nature. That's kind of like 707 00:45:01,200 --> 00:45:03,600 if you're a model and you get on the cover of Vogue. 708 00:45:03,600 --> 00:45:08,400 And they had defined a new kind of science. 709 00:45:08,400 --> 00:45:10,280 I think we are on the way 710 00:45:10,280 --> 00:45:13,800 to make high precision electron microscopy 711 00:45:13,800 --> 00:45:17,000 a part of science in general. 712 00:45:33,880 --> 00:45:36,880 The next stage of this journey downwards 713 00:45:36,880 --> 00:45:38,720 happened in Manchester, 714 00:45:38,720 --> 00:45:42,720 with the discovery of an incredible new material - 715 00:45:42,720 --> 00:45:44,160 graphene. 716 00:45:44,160 --> 00:45:47,680 The new electron microscopes revealed that graphene 717 00:45:47,680 --> 00:45:52,240 was a sheet of carbon just a single atom thick. 718 00:45:52,240 --> 00:45:57,440 And incredible strength was just one of its unexpected properties. 719 00:45:58,760 --> 00:46:03,400 So, just how impressive is graphene? Well, I've come here to this lab 720 00:46:03,400 --> 00:46:06,000 to carry out what's called a stress test. 721 00:46:06,000 --> 00:46:08,440 I've got two strips of plastic here. 722 00:46:08,440 --> 00:46:12,480 It's a stretchy polymer. One of them is just the pure polymer, 723 00:46:12,480 --> 00:46:17,080 the other contains just 3% graphene mixed in with it. 724 00:46:17,080 --> 00:46:21,360 And I want to stretch them to find out how much force is needed 725 00:46:21,360 --> 00:46:23,360 to snap these strips. 726 00:46:25,960 --> 00:46:28,640 First up is the pure polymer. 727 00:46:34,920 --> 00:46:37,480 Ah. There we go. It's gone? It's gone. 728 00:46:37,480 --> 00:46:42,920 So that snapped at...? 533 newtons. 729 00:46:42,920 --> 00:46:44,800 533 newtons. 730 00:46:44,800 --> 00:46:48,720 So that's about two... Two bags of cement. Two bags of cement. 731 00:46:48,720 --> 00:46:50,840 So now you're going to swap it with the graphene... 732 00:46:50,840 --> 00:46:52,720 Yes, I'm going to reset... ..implanted one. 733 00:46:52,720 --> 00:46:56,640 ..reset the machine with the graphene ones. OK? OK. 734 00:47:03,720 --> 00:47:04,760 OK. 735 00:47:17,080 --> 00:47:20,200 OK, so it's now hit 500 newtons. 736 00:47:20,200 --> 00:47:24,480 We've now already overtaken the non-graphene. Yes. 737 00:47:24,480 --> 00:47:29,000 And it looks pretty healthy, as far as I can tell. It's healthy, yes. 738 00:47:30,400 --> 00:47:34,480 It's coming up to 750 newtons now. 740, 750. 739 00:47:39,400 --> 00:47:43,520 We're now... And now it's coming up to 1,000 newtons. 740 00:47:43,520 --> 00:47:45,320 And still going strong. 741 00:47:47,880 --> 00:47:49,360 And... 742 00:47:57,800 --> 00:48:00,000 STRIP SNAPS Oh! So that was about... 743 00:48:00,000 --> 00:48:04,640 So the final force was 1,074. 744 00:48:04,640 --> 00:48:06,360 So that's double. 745 00:48:06,360 --> 00:48:09,320 Twice as much force was needed to snap this polymer, 746 00:48:09,320 --> 00:48:13,680 compared with the one without the graphene. That is pretty impressive. 747 00:48:13,680 --> 00:48:16,440 A huge improvement with just a few percent 748 00:48:16,440 --> 00:48:21,320 of graphene mixed in with the polymer. Yeah. That's incredible. 749 00:48:22,720 --> 00:48:27,120 Graphene has shaken the scientific community to its core, 750 00:48:27,120 --> 00:48:30,720 and yet was discovered almost by chance 751 00:48:30,720 --> 00:48:33,160 by scientist Andre Geim 752 00:48:33,160 --> 00:48:37,240 as he was searching for ever thinner slithers of graphite. 753 00:48:37,240 --> 00:48:41,000 Talk to me through what happened on that night, 754 00:48:41,000 --> 00:48:45,000 when you realised your eureka moment. 20 years ago, 755 00:48:45,000 --> 00:48:48,840 I realised that just taking Scotch tape, 756 00:48:48,840 --> 00:48:52,840 putting piece of graphite between the Scotch tape, 757 00:48:52,840 --> 00:48:57,840 peeling the Scotch tape like that, leaves small pieces of graphite. 758 00:48:57,840 --> 00:48:59,920 Is that something we can demonstrate here? Yeah. 759 00:48:59,920 --> 00:49:02,000 Because, we have a piece of graphite. Yeah. 760 00:49:02,000 --> 00:49:07,480 You can take this piece of graphite... 761 00:49:07,480 --> 00:49:10,600 ..and without much trouble... 762 00:49:10,600 --> 00:49:15,360 You can, of course, make it thinner by repeating this procedure. 763 00:49:15,360 --> 00:49:17,360 But if you shine lights through, 764 00:49:17,360 --> 00:49:22,040 you eventually start finding flakes which are transparent, 765 00:49:22,040 --> 00:49:24,480 and that actually was the Eureka moment. 766 00:49:24,480 --> 00:49:27,400 Because being reasonably well educated, 767 00:49:27,400 --> 00:49:33,280 I realised that if flakes of graphite are transparent, 768 00:49:33,280 --> 00:49:35,120 they're really, really thin. 769 00:49:35,120 --> 00:49:38,440 Probably initially those were ten layers thick 770 00:49:38,440 --> 00:49:41,880 but eventually we went down to a single layer. 771 00:49:45,200 --> 00:49:48,520 It's hard to overstate just how excited scientists 772 00:49:48,520 --> 00:49:51,000 and engineers are about graphene, 773 00:49:51,000 --> 00:49:54,400 so let me just remind you what graphene is. 774 00:49:54,400 --> 00:49:58,960 It's just a single flat sheet of carbon atoms all bonded together. 775 00:49:58,960 --> 00:50:01,320 But that would be really under-selling it 776 00:50:01,320 --> 00:50:04,320 because at around a third of a nanometre, 777 00:50:04,320 --> 00:50:07,600 it's just a single carbon atom thick, 778 00:50:07,600 --> 00:50:11,360 making it the thinnest material ever made. 779 00:50:11,360 --> 00:50:15,640 For a sense of why graphene is so extraordinary, 780 00:50:15,640 --> 00:50:19,720 we have to understand its physics at the atomic scale. 781 00:50:19,720 --> 00:50:23,240 Each sheet is made up of repeating hexagons. 782 00:50:23,240 --> 00:50:25,480 At each corner is a carbon atom 783 00:50:25,480 --> 00:50:28,760 that's bonded powerfully to three others. 784 00:50:28,760 --> 00:50:32,680 Those bonds are the source of the material's strength, 785 00:50:32,680 --> 00:50:36,160 but they also seem to produce other strange properties. 786 00:50:36,160 --> 00:50:39,280 Each carbon atom bonds to its three neighbours 787 00:50:39,280 --> 00:50:41,680 by sharing electrons with them. 788 00:50:41,680 --> 00:50:44,160 But not all the electrons are used for this. 789 00:50:44,160 --> 00:50:47,280 One electron from each atom is spare. 790 00:50:47,280 --> 00:50:50,840 These free electrons can zip around unhindered, 791 00:50:50,840 --> 00:50:54,560 and this has huge consequences because it means that graphene 792 00:50:54,560 --> 00:50:58,720 can be made to conduct electricity incredibly efficiently. 793 00:50:59,920 --> 00:51:02,960 There are high hopes that it will enable new kinds 794 00:51:02,960 --> 00:51:05,120 of electronic components, 795 00:51:05,120 --> 00:51:08,960 revolutionising batteries with much greater storage, 796 00:51:08,960 --> 00:51:11,280 and also solar power generation, 797 00:51:11,280 --> 00:51:16,560 water filtration, material science and quantum computing. 798 00:51:17,800 --> 00:51:20,200 Of course, this is still early days in graphene research 799 00:51:20,200 --> 00:51:24,440 but there is, without doubt, much to play for. 800 00:51:24,440 --> 00:51:29,080 The discovery of graphene brings us towards the end of this story, 801 00:51:29,080 --> 00:51:30,520 because with the newest 802 00:51:30,520 --> 00:51:33,520 aberration-corrected electron microscopes, 803 00:51:33,520 --> 00:51:37,560 we're now able to see on the smallest scales imaginable. 804 00:51:43,440 --> 00:51:45,440 Professor Quentin Ramasse 805 00:51:45,440 --> 00:51:49,480 runs some of the biggest electron microscopes in the world. 806 00:51:49,480 --> 00:51:52,680 He's going to zoom into a sample of graphene, 807 00:51:52,680 --> 00:51:56,480 until we can see individual atoms. 808 00:51:56,480 --> 00:51:59,560 OK, what are you going to show me here? 809 00:51:59,560 --> 00:52:03,840 So, we've prepared some graphene samples for you. 810 00:52:03,840 --> 00:52:07,800 The samples are on a copper grid just millimetres wide. 811 00:52:07,800 --> 00:52:12,240 Let me put it here and actually place it into the sample holder. 812 00:52:12,240 --> 00:52:15,520 That's the three millimetre sample? That's the three millimetre sample, 813 00:52:15,520 --> 00:52:18,040 and now, hopefully, you can already see... I can see the grid. 814 00:52:18,040 --> 00:52:20,920 So they're essentially just copper bars. 815 00:52:23,440 --> 00:52:25,200 Under the optical microscope, 816 00:52:25,200 --> 00:52:28,640 I can just make out holes in the sheet of carbon 817 00:52:28,640 --> 00:52:31,560 within the grid, where the graphene flakes are. 818 00:52:31,560 --> 00:52:33,240 To see them in more detail, 819 00:52:33,240 --> 00:52:37,960 he now switches the sample into a powerful electron microscope. 820 00:52:37,960 --> 00:52:41,120 So what we're looking at now is the same image 821 00:52:41,120 --> 00:52:43,760 as we had under the optical microscope? 822 00:52:43,760 --> 00:52:46,520 You can already recognise there's two shadows here, 823 00:52:46,520 --> 00:52:49,120 the corners of those grid squares. 824 00:52:49,120 --> 00:52:51,640 But in the middle here, you recognise what you also saw 825 00:52:51,640 --> 00:52:55,000 on the optical microscope, which are those circle holes, 826 00:52:55,000 --> 00:52:59,920 inside which is the graphene that we're going to go and look at. 827 00:53:01,800 --> 00:53:06,560 Slowly getting closer and closer and closer. 828 00:53:06,560 --> 00:53:10,240 We're going to be zooming into graphene much further in. 829 00:53:10,240 --> 00:53:13,160 Almost gives you vertigo when... A little bit, yes. 830 00:53:13,160 --> 00:53:15,960 ..you realise how much we're zooming in. 831 00:53:15,960 --> 00:53:17,880 OK, so, what are we looking at here? 832 00:53:17,880 --> 00:53:22,360 This is a patch of graphene that's about 500 nanometres across. 833 00:53:22,360 --> 00:53:25,520 How does this, then, compare to the thickness of a human hair? 834 00:53:25,520 --> 00:53:27,720 It would be...? Several metres across. 835 00:53:27,720 --> 00:53:29,880 Several metres across in diameter? Yes. 836 00:53:29,880 --> 00:53:32,080 That's how... OK, right. That's how small it is. 837 00:53:32,080 --> 00:53:34,640 And yet, we're still only halfway in our journey down. 838 00:53:34,640 --> 00:53:37,600 Not even... Not even halfway. ..of the way there. OK. 839 00:53:37,600 --> 00:53:41,080 And so what we're trying to do, really, is zoom in even further 840 00:53:41,080 --> 00:53:43,760 on that little black speck. Go for it. 841 00:53:43,760 --> 00:53:47,800 So we'll start reducing the magnification slowly. 842 00:53:47,800 --> 00:53:50,760 I'll go to magnify it ten times this time, 843 00:53:50,760 --> 00:53:53,800 trying to not go too fast so that you can really keep... 844 00:53:53,800 --> 00:53:55,720 You don't want to spoil the surprise for me. 845 00:53:55,720 --> 00:53:57,720 You don't want to spoil the surprise, no. 846 00:54:01,400 --> 00:54:03,640 If you notice, the shape of this hole, 847 00:54:03,640 --> 00:54:06,240 it's about the shape of Africa, I would say. 848 00:54:06,240 --> 00:54:10,800 It's now getting to a size that is more foreign to everyday life, 849 00:54:10,800 --> 00:54:14,760 especially when you start realising that this patch is going to be 850 00:54:14,760 --> 00:54:17,000 100 times smaller still. 851 00:54:17,000 --> 00:54:19,760 But let's zoom in and hopefully see 852 00:54:19,760 --> 00:54:22,560 what we are here to see, which are single atoms. 853 00:54:24,200 --> 00:54:25,800 So this is now that same patch, 854 00:54:25,800 --> 00:54:27,680 and you notice that it is very dark. 855 00:54:27,680 --> 00:54:30,640 You might just about start being able to recognise 856 00:54:30,640 --> 00:54:33,880 some pattern in the middle, some very faint lines 857 00:54:33,880 --> 00:54:37,360 which correspond to the hexagonal lattice in graphene. 858 00:54:37,360 --> 00:54:39,880 But if you look closely on the original image 859 00:54:39,880 --> 00:54:41,880 that we still have on screen here, 860 00:54:41,880 --> 00:54:45,880 you see small, round blobs that are perhaps a little bit brighter. 861 00:54:45,880 --> 00:54:48,960 And they are brighter because, those atoms are heavier, 862 00:54:48,960 --> 00:54:50,840 and we happen to know they're silicone. 863 00:54:50,840 --> 00:54:53,200 But just to demonstrate, I can move that scan box 864 00:54:53,200 --> 00:54:55,560 around one of those single atoms and, hopefully, 865 00:54:55,560 --> 00:54:58,000 it'll light up like a Christmas light in the middle. 866 00:55:00,520 --> 00:55:02,280 And there it is. 867 00:55:02,280 --> 00:55:05,280 Because it is heavier, it appears brighter on the image. 868 00:55:05,280 --> 00:55:07,840 So that entire bright patch 869 00:55:07,840 --> 00:55:10,600 is a single atom of silicone? 870 00:55:10,600 --> 00:55:15,120 And yet it's a blob, it's a patch. It's not the picture of an atom 871 00:55:15,120 --> 00:55:17,600 that we learn about at school, with a nucleus and electrons 872 00:55:17,600 --> 00:55:20,280 buzzing around the outside. So what is exactly...? 873 00:55:20,280 --> 00:55:24,720 It remains reasonably abstract. What we see is this average structure 874 00:55:24,720 --> 00:55:29,040 of subatomic particles, and that gives us this average round shape. 875 00:55:29,040 --> 00:55:32,520 We've magnified this sample that we've taken out 876 00:55:32,520 --> 00:55:36,960 from a sample box and put into the microscope by several million times 877 00:55:36,960 --> 00:55:39,080 to see on the screen this magnification. 878 00:55:39,080 --> 00:55:40,840 So a tenth of a billionth of a metre. 879 00:55:40,840 --> 00:55:43,280 We've come a long way since Robert Hooke. 880 00:55:43,280 --> 00:55:45,520 THEY LAUGH 881 00:55:45,520 --> 00:55:48,000 For me, as a theoretical physicist, 882 00:55:48,000 --> 00:55:51,160 an atom is just abstract mathematics - 883 00:55:51,160 --> 00:55:56,200 an equation, an idea. But to see one of them with my own eyes, 884 00:55:56,200 --> 00:55:58,360 the building blocks of everything, 885 00:55:58,360 --> 00:56:01,600 just ten millionths of a millimetre across, 886 00:56:01,600 --> 00:56:04,120 is nothing less than miraculous. 887 00:56:04,120 --> 00:56:08,040 I still can't get my head around the fact 888 00:56:08,040 --> 00:56:11,440 that I'm looking at individual atoms. 889 00:56:11,440 --> 00:56:14,160 Well, look, I'll tell you. Yeah. 890 00:56:14,160 --> 00:56:19,680 I mean, I've spent my career studying atomic nuclei, 891 00:56:19,680 --> 00:56:22,400 but, for me, it's always been abstract. 892 00:56:22,400 --> 00:56:28,640 The notion that we're looking at an individual atom here... 893 00:56:28,640 --> 00:56:30,360 And I love the analogy 894 00:56:30,360 --> 00:56:34,560 that there are more atoms in a single glass of water 895 00:56:34,560 --> 00:56:39,640 than there are glasses of water in all the oceans of the world, right? 896 00:56:39,640 --> 00:56:43,640 Atoms are tiny. They are tiny. The fact that we have an instrument 897 00:56:43,640 --> 00:56:47,800 here that allows you to look at an atom... 898 00:56:47,800 --> 00:56:50,720 I... The novelty doesn't wear off? 899 00:56:50,720 --> 00:56:52,480 It definitely doesn't, no. 900 00:56:52,480 --> 00:56:55,320 I might be either simple-minded or single-minded, 901 00:56:55,320 --> 00:56:58,680 but seeing those single atoms is, 902 00:56:58,680 --> 00:57:01,840 I think, something I'll want to do for the rest of my life. 903 00:57:01,840 --> 00:57:04,760 And it's just a wonderful thing to see. 904 00:57:14,320 --> 00:57:18,960 We've now entered a realm in which we can see individual atoms, 905 00:57:18,960 --> 00:57:23,160 and it's leading us into a new world of single atom physics, 906 00:57:23,160 --> 00:57:27,080 chemistry, biology, engineering and medicine. 907 00:57:27,080 --> 00:57:32,480 It's all so new that it's impossible to say where it's going to take us. 908 00:57:32,480 --> 00:57:35,960 But as we learn more about our world, 909 00:57:35,960 --> 00:57:38,480 from insects, to cells, 910 00:57:38,480 --> 00:57:40,960 to the atoms that make us, 911 00:57:40,960 --> 00:57:45,040 I know there'll be many more wonders to discover. 912 00:57:46,480 --> 00:57:49,160 Next time, I go big. 913 00:57:49,160 --> 00:57:53,920 As I journey from our solar system out to galactic superclusters, 914 00:57:53,920 --> 00:57:57,680 I'll confront the biggest mysteries in our universe. 74040

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