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These are the user uploaded subtitles that are being translated: 1 00:00:00,672 --> 00:00:04,255 (intense orchestral music) 2 00:00:06,950 --> 00:00:09,973 Everything in the universe has its size. 3 00:00:11,560 --> 00:00:13,223 Planets are big. 4 00:00:14,270 --> 00:00:15,913 Insects are small. 5 00:00:18,070 --> 00:00:20,033 People are somewhere in between. 6 00:00:21,390 --> 00:00:24,900 Everything has its place in the grand order. 7 00:00:24,900 --> 00:00:26,783 Things are as they should be. 8 00:00:27,920 --> 00:00:30,306 But does it have to be that way? 9 00:00:30,306 --> 00:00:34,163 Does size really matter or could things be different? 10 00:00:35,140 --> 00:00:38,123 After all, short people live longer than tall people. 11 00:00:39,440 --> 00:00:41,833 Small things are stronger than big things. 12 00:00:43,304 --> 00:00:46,510 And really tiny creatures can do things 13 00:00:46,510 --> 00:00:48,640 we can only dream of. 14 00:00:48,640 --> 00:00:50,670 So why are things the size they are 15 00:00:50,670 --> 00:00:53,393 and what if we could change that? 16 00:00:54,910 --> 00:00:56,710 Using the latest science, 17 00:00:56,710 --> 00:00:59,640 we are going to do the ultimate thought experiment. 18 00:00:59,640 --> 00:01:02,200 We are going to shrink everything in our world 19 00:01:04,140 --> 00:01:05,460 including us 20 00:01:05,460 --> 00:01:09,900 to see whether a smaller world really is more beautiful. 21 00:01:09,900 --> 00:01:11,670 Along the way, we're going to discover 22 00:01:11,670 --> 00:01:14,320 just how much size matters, 23 00:01:14,320 --> 00:01:16,904 how it defines everything. 24 00:01:16,904 --> 00:01:20,160 You'll never look at yourself or your world 25 00:01:20,160 --> 00:01:21,853 the same way again. 26 00:01:24,002 --> 00:01:27,085 (explosion blasting) 27 00:01:35,470 --> 00:01:37,790 You might think this looks like an ordinary house 28 00:01:37,790 --> 00:01:40,060 on an ordinary sunny morning. 29 00:01:40,060 --> 00:01:41,750 If you watched the last program, 30 00:01:41,750 --> 00:01:44,800 then you'll know that this is a parallel universe, 31 00:01:44,800 --> 00:01:48,520 one just like our own, but with one important difference. 32 00:01:48,520 --> 00:01:51,818 In this universe, we can change the size of things 33 00:01:51,818 --> 00:01:53,511 just to see what happens. 34 00:01:53,511 --> 00:01:56,840 (alarm beeping) (man sighing) 35 00:01:56,840 --> 00:01:59,450 We're going to change the size of stars, 36 00:01:59,450 --> 00:02:01,603 planets, and living things, 37 00:02:01,603 --> 00:02:04,090 and see the surprising effect it has 38 00:02:04,090 --> 00:02:08,290 on a normal guy going about his normal day. 39 00:02:08,290 --> 00:02:09,890 We'll find out if the way things are 40 00:02:09,890 --> 00:02:13,373 is the only way they can be or if size is just an accident. 41 00:02:15,330 --> 00:02:17,650 In our last grand thought experiment, 42 00:02:17,650 --> 00:02:22,650 we made everything big, but it all went wrong, badly wrong. 43 00:02:25,690 --> 00:02:27,640 So now, we're going to go the other way 44 00:02:27,640 --> 00:02:30,223 to see if small really could be beautiful. 45 00:02:31,268 --> 00:02:34,851 (intense orchestral music) 46 00:02:39,090 --> 00:02:40,393 So where do we start? 47 00:02:42,010 --> 00:02:43,550 Since this is a thought experiment, 48 00:02:43,550 --> 00:02:45,550 we can start anywhere we like. 49 00:02:45,550 --> 00:02:46,503 So how about here? 50 00:02:48,030 --> 00:02:50,703 Home, our planet. 51 00:02:52,080 --> 00:02:54,929 Earth is the fifth largest planet in the solar system 52 00:02:54,929 --> 00:02:56,423 or the fourth smallest. 53 00:02:57,984 --> 00:02:59,890 Maybe we could move it down the scale 54 00:02:59,890 --> 00:03:03,183 towards Venus, Mars, or Mercury. 55 00:03:06,400 --> 00:03:08,050 This is the Earth you're used to, 56 00:03:09,130 --> 00:03:12,480 12,756 kilometers across 57 00:03:12,480 --> 00:03:15,960 with a circumference of 40,000 kilometers 58 00:03:15,960 --> 00:03:18,793 which takes an airliner about two days to fly around. 59 00:03:24,514 --> 00:03:25,710 There's an atmosphere 60 00:03:25,710 --> 00:03:28,490 100 kilometers deep all the way around, 61 00:03:28,490 --> 00:03:30,492 then a thin layer of solid rock, 62 00:03:30,492 --> 00:03:34,560 five thousand kilometers of rock and molten metal, 63 00:03:34,560 --> 00:03:37,890 and finally, a 2,600 kilometer ball 64 00:03:37,890 --> 00:03:40,160 of solid iron at the core. 65 00:03:40,160 --> 00:03:41,510 But these are just numbers. 66 00:03:42,360 --> 00:03:44,910 The question is do they matter? 67 00:03:44,910 --> 00:03:46,710 Is it important that our world 68 00:03:46,710 --> 00:03:48,667 is exactly the size it is now? 69 00:03:49,850 --> 00:03:52,100 Surely, it's simple enough to imagine our Earth 70 00:03:52,100 --> 00:03:54,393 but say half the size across. 71 00:03:55,430 --> 00:03:57,970 All made of the same stuff, same proportions, 72 00:03:57,970 --> 00:03:59,093 just a bit smaller. 73 00:04:00,980 --> 00:04:03,414 Problem is changing Earth's size 74 00:04:03,414 --> 00:04:07,010 changes things you don't want to be changing 75 00:04:07,010 --> 00:04:09,860 and one of those is gravity. 76 00:04:09,860 --> 00:04:12,280 Gravity, basically a very, 77 00:04:12,280 --> 00:04:14,700 very important force in the universe. 78 00:04:14,700 --> 00:04:16,240 Whenever you have an object, 79 00:04:16,240 --> 00:04:19,380 it will attract everything that you have around you. 80 00:04:19,380 --> 00:04:20,980 So this works for planets, 81 00:04:20,980 --> 00:04:23,947 but it also works for everything in the universe. 82 00:04:23,947 --> 00:04:26,930 For instance, galaxies or stars. 83 00:04:26,930 --> 00:04:29,973 Everything attracts everything. 84 00:04:32,720 --> 00:04:34,060 A half-sized planet 85 00:04:34,060 --> 00:04:36,963 means half the normal gravity at the surface, 86 00:04:38,248 --> 00:04:41,643 enough of a change to put a spring in your step. 87 00:04:44,686 --> 00:04:46,100 And if you're athletic, 88 00:04:46,100 --> 00:04:48,193 who knows what you would be capable of. 89 00:04:55,300 --> 00:04:57,790 Half gravity means you can jump higher 90 00:05:05,270 --> 00:05:06,683 and fall slower. 91 00:05:11,208 --> 00:05:15,533 So far, so good, but then the fun would stop. 92 00:05:18,620 --> 00:05:20,770 The universe is a system basically, 93 00:05:20,770 --> 00:05:23,300 so size is important in the sense 94 00:05:23,300 --> 00:05:26,128 that if you change the size of one single element 95 00:05:26,128 --> 00:05:29,913 with respect to the others, then the whole thing breaks. 96 00:05:31,210 --> 00:05:32,850 For starters, half gravity 97 00:05:32,850 --> 00:05:35,140 means air pressure is half what it was 98 00:05:35,140 --> 00:05:38,683 as the planet pulls the atmosphere less strongly towards it. 99 00:05:41,100 --> 00:05:42,610 Pressure at sea level is now 100 00:05:42,610 --> 00:05:47,010 the same as it used to be 5,500 meters up a mountain. 101 00:05:49,016 --> 00:05:51,673 There is less oxygen in every breath. 102 00:05:54,500 --> 00:05:58,130 Within a few hours, humanity would have oxygen deficiency, 103 00:05:58,130 --> 00:06:00,343 otherwise known as altitude sickness. 104 00:06:02,932 --> 00:06:05,890 Humans can adapt to thinner air. 105 00:06:05,890 --> 00:06:07,946 After a few days, red blood cell counts 106 00:06:07,946 --> 00:06:09,710 would begin to increase 107 00:06:09,710 --> 00:06:11,743 to compensate for the reduced oxygen. 108 00:06:13,390 --> 00:06:16,033 Just in time to notice the next strange change. 109 00:06:19,910 --> 00:06:22,820 The aurora is an amazing display of light 110 00:06:22,820 --> 00:06:25,710 sometimes visible near the North and South Poles, 111 00:06:25,710 --> 00:06:27,830 but why does the aurora exist 112 00:06:27,830 --> 00:06:29,620 and what has made it turn up 113 00:06:29,620 --> 00:06:32,260 far from where it's supposed to be? 114 00:06:32,260 --> 00:06:34,360 It's a puzzle, and to solve it, 115 00:06:34,360 --> 00:06:36,730 we need to look not to outer space, 116 00:06:36,730 --> 00:06:39,320 but to the University of Maryland. 117 00:06:39,320 --> 00:06:41,810 Daniel Lathrop has spent 20 years 118 00:06:41,810 --> 00:06:44,299 building models of the inside of planet Earth 119 00:06:44,299 --> 00:06:46,931 to help him understand just how our planet 120 00:06:46,931 --> 00:06:49,057 generates a magnetic field, 121 00:06:49,057 --> 00:06:52,173 work that is vital for understanding the aurora. 122 00:06:55,190 --> 00:06:58,620 Dan's model has a solid metal ball at its center 123 00:06:58,620 --> 00:07:01,252 surrounded by a thick layer of molten metal 124 00:07:01,252 --> 00:07:03,033 just like planet Earth. 125 00:07:04,010 --> 00:07:06,850 As the Earth rotates, the currents of molten metal 126 00:07:06,850 --> 00:07:08,593 generate a magnetic field. 127 00:07:09,780 --> 00:07:12,473 Dan built his model to study how this happens. 128 00:07:14,270 --> 00:07:15,953 You may wonder why he bothered. 129 00:07:16,988 --> 00:07:19,755 The fact is the Earth's magnetic field 130 00:07:19,755 --> 00:07:22,430 is very important indeed. 131 00:07:22,430 --> 00:07:24,820 So the Earth's magnetic field serves as a shield 132 00:07:24,820 --> 00:07:27,810 against the worst parts of bad solar weather. 133 00:07:27,810 --> 00:07:29,420 So the sun has storms 134 00:07:29,420 --> 00:07:31,190 that occasionally give large amounts of radiation 135 00:07:31,190 --> 00:07:32,290 aimed at the Earth. 136 00:07:32,290 --> 00:07:33,560 And the Earth's magnetic field 137 00:07:33,560 --> 00:07:35,750 inflates something like a bubble around the Earth. 138 00:07:35,750 --> 00:07:38,480 The magnetosphere that acts as a primary barrier 139 00:07:38,480 --> 00:07:40,320 to the worst of the radiation. 140 00:07:40,320 --> 00:07:42,210 It's this solar radiation 141 00:07:42,210 --> 00:07:43,900 that causes the aurora. 142 00:07:43,900 --> 00:07:46,700 The shape of the planet's protective magnetic field 143 00:07:46,700 --> 00:07:49,280 tunnels the sun's radiation towards the poles 144 00:07:49,280 --> 00:07:52,180 where it hits the upper atmosphere. 145 00:07:52,180 --> 00:07:56,243 This makes the gases glow, giving us a beautiful light show. 146 00:07:57,710 --> 00:08:00,460 But Dan's machine can also help us find out 147 00:08:00,460 --> 00:08:04,240 why a smaller Earth has auroras in unexpected places 148 00:08:06,480 --> 00:08:07,810 because over the years, 149 00:08:07,810 --> 00:08:11,303 he's built several smaller versions of his model Earth. 150 00:08:12,570 --> 00:08:15,730 So these actually are the first three sodium experiments 151 00:08:15,730 --> 00:08:17,860 we built to try to understand the Earth's magnetic field. 152 00:08:17,860 --> 00:08:19,210 So the first one, 153 00:08:19,210 --> 00:08:22,080 20 centimeter diameter model rapidly rotating. 154 00:08:22,080 --> 00:08:24,145 Next came a 30 centimeter experiment. 155 00:08:24,145 --> 00:08:26,090 There's an inner sphere deep inside there 156 00:08:26,090 --> 00:08:26,940 that you can't see. 157 00:08:26,940 --> 00:08:29,380 And the third experiment at 60 centimeters. 158 00:08:29,380 --> 00:08:31,304 Here's the bottom half of the outer sphere 159 00:08:31,304 --> 00:08:34,812 and then a solid copper model of the inner core 160 00:08:34,812 --> 00:08:36,530 that independently rotates. 161 00:08:36,530 --> 00:08:37,650 And then the whole thing 162 00:08:37,650 --> 00:08:40,190 would be filled with liquid sodium in the experiments. 163 00:08:40,190 --> 00:08:41,950 Thinking about what it would be like 164 00:08:41,950 --> 00:08:43,210 if the Earth were half sized, 165 00:08:43,210 --> 00:08:44,680 we could then examine data 166 00:08:44,680 --> 00:08:46,040 between the different size experiments 167 00:08:46,040 --> 00:08:48,290 to see how the magnetic fields are different. 168 00:08:50,310 --> 00:08:52,778 Dan's model is filled with the metal sodium 169 00:08:52,778 --> 00:08:55,430 because of its low melting point, 170 00:08:55,430 --> 00:08:57,023 but it still takes three days 171 00:08:57,023 --> 00:08:59,870 before it's fully melted and ready to spin. 172 00:09:01,540 --> 00:09:05,123 (intense orchestral music) 173 00:09:22,040 --> 00:09:23,710 So here, we see magnetic field data 174 00:09:23,710 --> 00:09:26,120 from the 30 centimeter smaller experiment 175 00:09:26,120 --> 00:09:30,465 and comparing it then to more recent data from three meter, 176 00:09:30,465 --> 00:09:31,700 it's very evident 177 00:09:31,700 --> 00:09:34,558 that as our experiments have gotten larger, 178 00:09:34,558 --> 00:09:37,390 we have much more magnetic induction, 179 00:09:37,390 --> 00:09:39,953 much stronger magnetic fields overall. 180 00:09:40,940 --> 00:09:42,010 So smaller Earth 181 00:09:42,010 --> 00:09:44,230 would have a weaker magnetosphere. 182 00:09:44,230 --> 00:09:46,720 But that's not all the experiments reveal. 183 00:09:46,720 --> 00:09:49,130 When we go from larger to a smaller experiment, 184 00:09:49,130 --> 00:09:52,439 the magnetic field strengths have both become weaker 185 00:09:52,439 --> 00:09:54,511 and have changed pattern. 186 00:09:54,511 --> 00:09:57,355 If you look at the data in the larger model, 187 00:09:57,355 --> 00:10:00,533 there's a kind of well-defined north, south magnetic poles, 188 00:10:00,533 --> 00:10:03,384 where in the smaller experiment at these parameters, 189 00:10:03,384 --> 00:10:06,920 we have like a ring of south poles around the equator 190 00:10:06,920 --> 00:10:10,480 and then two magnetic norths at either end. 191 00:10:10,480 --> 00:10:11,313 So it is possible 192 00:10:11,313 --> 00:10:13,025 for the shape of the magnetic fields to change 193 00:10:13,025 --> 00:10:15,163 when you change its size. 194 00:10:16,720 --> 00:10:18,670 A smaller Earth would be likely 195 00:10:18,670 --> 00:10:22,280 to have many magnetic poles spread around its surface 196 00:10:24,280 --> 00:10:27,620 meaning auroras could show up where you least expect them 197 00:10:29,240 --> 00:10:30,890 and they'd be stronger than ever, 198 00:10:32,176 --> 00:10:36,000 but that's a bad thing, a very bad thing. 199 00:10:36,000 --> 00:10:39,203 It's a sign that our magnetic field is being overwhelmed. 200 00:10:47,320 --> 00:10:49,150 If you have a smaller planet 201 00:10:49,150 --> 00:10:51,430 with a weaker magnetic field, 202 00:10:51,430 --> 00:10:53,840 there would be more problems with telecommunications. 203 00:10:53,840 --> 00:10:57,663 The sun still has these big angry things 204 00:10:57,663 --> 00:10:59,860 that could (mumbling) mass ejections 205 00:10:59,860 --> 00:11:02,743 where it really sends a burst of radiation in space. 206 00:11:05,180 --> 00:11:07,970 We have systems on Earth which are so big 207 00:11:07,970 --> 00:11:11,380 depending on electricity that when the sun is angry, 208 00:11:11,380 --> 00:11:14,193 potentially, you have (mumbling) and it causes problems. 209 00:11:15,930 --> 00:11:17,390 The sun's outbursts 210 00:11:17,390 --> 00:11:21,530 would cause a weaker magnetic field to wobble violently 211 00:11:21,530 --> 00:11:23,923 inducing surges in electrical systems. 212 00:11:24,760 --> 00:11:27,690 The result is havoc to power supplies, 213 00:11:27,690 --> 00:11:32,420 communications, and in fact, just about all electronics. 214 00:11:32,420 --> 00:11:35,350 Then things go from bad to worse. 215 00:11:35,350 --> 00:11:36,880 If we had no magnetic field 216 00:11:36,880 --> 00:11:38,120 around the Earth at all, 217 00:11:38,120 --> 00:11:39,790 then we would be directly hit 218 00:11:39,790 --> 00:11:41,500 by the radiation from the sun 219 00:11:41,500 --> 00:11:44,400 and the Earth would become a very, very toxic environment. 220 00:11:45,410 --> 00:11:46,810 Without the protective effect 221 00:11:46,810 --> 00:11:50,173 of a strong magnetic field, Earth is in real trouble. 222 00:11:51,710 --> 00:11:55,390 Lower gravity means gases can escape into space. 223 00:11:55,390 --> 00:11:58,063 Cosmic radiation supercharges the process. 224 00:12:00,229 --> 00:12:03,393 Eventually, there would be no air left to breathe, 225 00:12:04,720 --> 00:12:09,393 its precious atmosphere stripped and blasted away. 226 00:12:10,342 --> 00:12:14,009 (dramatic orchestral music) 227 00:12:15,188 --> 00:12:17,938 The Earth would end up like Mars. 228 00:12:20,390 --> 00:12:22,723 It's the curse of small planets. 229 00:12:25,060 --> 00:12:29,113 Small planets are not really up to supporting human life, 230 00:12:30,850 --> 00:12:33,927 so it's time to put things back to how they were. 231 00:12:35,010 --> 00:12:38,910 A planet 12,756 kilometers across 232 00:12:38,910 --> 00:12:42,273 with an atmosphere 100 kilometers deep all the way around 233 00:12:42,273 --> 00:12:45,570 and a circumference of 40,000 kilometers. 234 00:12:45,570 --> 00:12:48,763 Planet Earth just as it should be. 235 00:12:48,763 --> 00:12:51,253 Not too big, not too small. 236 00:12:59,208 --> 00:13:01,875 (alarm beeping) 237 00:13:07,790 --> 00:13:09,990 So far, so not so good. 238 00:13:09,990 --> 00:13:12,690 In pursuit of a smaller, more beautiful world, 239 00:13:12,690 --> 00:13:14,773 we turned it into an inhabitable desert. 240 00:13:17,836 --> 00:13:20,700 Maybe it's time to try something a little less risky 241 00:13:23,694 --> 00:13:25,273 like human beings. 242 00:13:28,550 --> 00:13:30,973 So how big are people anyway? 243 00:13:31,860 --> 00:13:35,310 There are about 4,000 mammal species in the world 244 00:13:35,310 --> 00:13:38,110 and they come in all different shapes and sizes. 245 00:13:38,110 --> 00:13:40,050 The largest, of course, are the whales. 246 00:13:40,050 --> 00:13:42,389 The blue whale is absolutely enormous, 247 00:13:42,389 --> 00:13:44,847 the size of several school buses put together. 248 00:13:44,847 --> 00:13:47,680 And the smallest mammal is very small. 249 00:13:47,680 --> 00:13:48,513 Two grams. 250 00:13:48,513 --> 00:13:50,650 It's essentially the size of your thumb. 251 00:13:50,650 --> 00:13:53,740 And the typical size of a mammal however, 252 00:13:53,740 --> 00:13:55,670 it not sort of in the middle. 253 00:13:55,670 --> 00:13:57,970 Instead, it's much closer to the smallest size, 254 00:13:57,970 --> 00:14:01,130 about 40 grams which is the size of a rat. 255 00:14:01,130 --> 00:14:05,820 Humans are about 65 kilos on average, give or take, 256 00:14:05,820 --> 00:14:08,763 and so that makes us enormous. 257 00:14:10,300 --> 00:14:11,680 When we look at an elephant, 258 00:14:11,680 --> 00:14:14,160 we may feel small, but in fact, 259 00:14:14,160 --> 00:14:17,800 human beings are around 1,600 times heavier 260 00:14:17,800 --> 00:14:19,000 than the average mammal, 261 00:14:20,110 --> 00:14:22,123 but that's not necessarily good news. 262 00:14:23,283 --> 00:14:25,760 Aaron Clauset is a data scientist 263 00:14:25,760 --> 00:14:29,193 who studies the relationship between size and extinction. 264 00:14:30,540 --> 00:14:33,313 What we've found is that the larger an animal is, 265 00:14:33,313 --> 00:14:34,810 the more likely that species is 266 00:14:34,810 --> 00:14:36,460 to go extinct in the long run, 267 00:14:36,460 --> 00:14:38,990 and there are various reasons for this. 268 00:14:38,990 --> 00:14:42,205 Typically, species that are larger have smaller populations 269 00:14:42,205 --> 00:14:44,870 and so if there happen to be a few bad years 270 00:14:44,870 --> 00:14:46,399 in terms of reproduction or food, 271 00:14:46,399 --> 00:14:48,300 then their population could crash, 272 00:14:48,300 --> 00:14:50,230 and as a result, they can become extinct. 273 00:14:50,230 --> 00:14:52,070 Whereas much smaller animals 274 00:14:52,070 --> 00:14:54,080 typically have much larger populations 275 00:14:54,080 --> 00:14:57,793 and so they are robust to these kinds of events. 276 00:15:01,511 --> 00:15:04,030 In the extinction that wiped out the dinosaurs, 277 00:15:04,030 --> 00:15:07,763 every land creature that weighed over 25 kilograms died 278 00:15:07,763 --> 00:15:11,493 which is why the only dinosaurs we have today are the birds. 279 00:15:13,220 --> 00:15:15,040 So in general, the larger the animal is, 280 00:15:15,040 --> 00:15:16,713 the faster it goes extinct. 281 00:15:17,837 --> 00:15:18,670 Bye-bye. 282 00:15:20,560 --> 00:15:21,810 For living things, 283 00:15:21,810 --> 00:15:24,500 size is a matter of life or death, 284 00:15:24,500 --> 00:15:27,160 but human size is not fixed. 285 00:15:27,160 --> 00:15:29,903 It has changed a lot over the course of history. 286 00:15:31,549 --> 00:15:35,330 Back in the Stone Age when humans lived as hunter-gatherers, 287 00:15:35,330 --> 00:15:37,480 the average male height was similar to now. 288 00:15:39,000 --> 00:15:42,456 During the Neolithic Revolution when we started farming, 289 00:15:42,456 --> 00:15:46,136 we shrunk hugely as our new grain-based diet 290 00:15:46,136 --> 00:15:48,203 had a lower nutritional value. 291 00:15:49,500 --> 00:15:52,521 Humans stayed short for several thousand years. 292 00:15:52,521 --> 00:15:54,820 It's only in the last 200 years 293 00:15:54,820 --> 00:15:57,570 that we finally got back to hunter-gatherer size 294 00:15:57,570 --> 00:15:59,910 and beyond thanks to modern improvements 295 00:15:59,910 --> 00:16:01,660 in food and medicine. 296 00:16:01,660 --> 00:16:06,010 But paradoxically, getting taller isn't always a good thing. 297 00:16:06,010 --> 00:16:07,100 Although big animals 298 00:16:07,100 --> 00:16:09,435 have longer lifespans than smaller ones, 299 00:16:09,435 --> 00:16:12,900 within each species, the story is different. 300 00:16:12,900 --> 00:16:14,870 It's been observed that in many species, 301 00:16:14,870 --> 00:16:17,840 it's the shorter individuals that actually live longer 302 00:16:17,840 --> 00:16:19,450 like in dogs. 303 00:16:19,450 --> 00:16:22,283 Could the same also be true for humans? 304 00:16:29,434 --> 00:16:31,120 I guess in a lot of species 305 00:16:31,120 --> 00:16:34,520 and if we look at dogs, horses, elephants, 306 00:16:34,520 --> 00:16:37,167 it's actually the smaller variants of that species 307 00:16:37,167 --> 00:16:39,170 that seem to live longer. 308 00:16:39,170 --> 00:16:41,100 And of course, then the real question is 309 00:16:41,100 --> 00:16:43,340 does it also apply to humans? 310 00:16:43,340 --> 00:16:45,620 But that's not so easy to answer. 311 00:16:45,620 --> 00:16:48,120 There are so many influences on our lives. 312 00:16:48,120 --> 00:16:50,120 How can you tell what's due to size 313 00:16:50,120 --> 00:16:52,563 and what's due to, say, diet or exercise? 314 00:16:53,645 --> 00:16:57,250 Geneticist Diana van Heemst has been reexamining 315 00:16:57,250 --> 00:17:01,280 a remarkable 1970's study that found a solution. 316 00:17:01,280 --> 00:17:03,081 It honed in on a group of people 317 00:17:03,081 --> 00:17:06,880 with very similar lifestyles, but varying heights. 318 00:17:06,880 --> 00:17:08,183 Professional athletes. 319 00:17:09,310 --> 00:17:11,083 For example, American baseball players, 320 00:17:11,083 --> 00:17:13,566 there's a nice encyclopedia 321 00:17:13,566 --> 00:17:16,450 which is actually a rich source of information 322 00:17:16,450 --> 00:17:18,607 not only for the baseball fans 323 00:17:18,607 --> 00:17:22,820 about all the details of batting performances and nicknames, 324 00:17:22,820 --> 00:17:25,510 but also actually, it contains date of birth, 325 00:17:25,510 --> 00:17:30,200 date of death, their adult height, and their weight. 326 00:17:30,200 --> 00:17:31,870 The study took this information 327 00:17:31,870 --> 00:17:35,660 on height and age of death and looked for a pattern. 328 00:17:35,660 --> 00:17:38,033 Wally Burnette, one meter 83. 329 00:17:42,120 --> 00:17:45,053 Murry Dickson, one meter 78. 330 00:17:46,904 --> 00:17:48,980 The original study used data 331 00:17:48,980 --> 00:17:50,940 from thousands of players, 332 00:17:50,940 --> 00:17:52,390 but we can see what they discovered 333 00:17:52,390 --> 00:17:53,753 by looking at just a few. 334 00:17:56,739 --> 00:17:59,740 I took from the encyclopedia of baseball 335 00:17:59,740 --> 00:18:02,891 nine representative examples of baseball players, 336 00:18:02,891 --> 00:18:06,970 and we have, you know, attached them to the wall 337 00:18:06,970 --> 00:18:10,020 based on the height and the age at death. 338 00:18:10,020 --> 00:18:13,160 And this kindly mimics the original study 339 00:18:13,160 --> 00:18:16,618 which made use of the full sample of the encyclopedia 340 00:18:16,618 --> 00:18:19,550 which found there's negative correlation 341 00:18:19,550 --> 00:18:22,417 between height and the age at death. 342 00:18:22,417 --> 00:18:26,830 The 1970s study found that size did matter. 343 00:18:26,830 --> 00:18:30,070 Being five centimeters shorter meant on average 344 00:18:30,070 --> 00:18:32,650 you would live two years longer. 345 00:18:32,650 --> 00:18:35,070 The big question is why. 346 00:18:35,070 --> 00:18:38,246 Although the original work was conducted in the 1970s, 347 00:18:38,246 --> 00:18:40,870 it's only now researchers like Diana 348 00:18:40,870 --> 00:18:43,490 have come up with a possible explanation. 349 00:18:43,490 --> 00:18:46,610 In order to grow, our body makes growth hormone 350 00:18:46,610 --> 00:18:48,670 which stimulates growth, 351 00:18:48,670 --> 00:18:51,240 but at the same time, it also influences 352 00:18:51,240 --> 00:18:54,071 lots of other processes in our body. 353 00:18:54,071 --> 00:18:56,133 And if you look at the data 354 00:18:56,133 --> 00:18:59,618 that have been derived from work on other animals, 355 00:18:59,618 --> 00:19:03,370 we can see that those growth hormones, 356 00:19:03,370 --> 00:19:05,590 they stimulate the body to grow 357 00:19:05,590 --> 00:19:07,330 and this is kind of a signal 358 00:19:07,330 --> 00:19:08,770 that there's enough food, 359 00:19:08,770 --> 00:19:10,817 that there's favorable conditions 360 00:19:10,817 --> 00:19:14,834 that it would be wise to invest as much as possible energy 361 00:19:14,834 --> 00:19:16,700 in growth and reproduction. 362 00:19:16,700 --> 00:19:18,510 And this may come at a cost 363 00:19:18,510 --> 00:19:20,700 because it means there's less energy available 364 00:19:20,700 --> 00:19:24,250 to invest simply in maintaining our bodies in good shape. 365 00:19:24,250 --> 00:19:27,600 And actually, when conditions get adverse 366 00:19:27,600 --> 00:19:31,120 or become less favorable like when there is a food shortage 367 00:19:31,120 --> 00:19:32,550 or lots of toxins, 368 00:19:32,550 --> 00:19:36,776 then as a consequence, as a response to that, we don't grow. 369 00:19:36,776 --> 00:19:38,300 We kind of stop growth 370 00:19:38,300 --> 00:19:40,260 and we really invest the available energy 371 00:19:40,260 --> 00:19:41,620 in maintaining our body 372 00:19:41,620 --> 00:19:46,438 and trying to kind of survive this period of hardship 373 00:19:46,438 --> 00:19:48,343 until things get better. 374 00:19:49,280 --> 00:19:52,622 It seems being big comes at a price. 375 00:19:52,622 --> 00:19:54,150 But for tall people, 376 00:19:54,150 --> 00:19:56,550 there is some light at the end of the tunnel. 377 00:19:56,550 --> 00:19:59,000 However, height is not the only thing that matters. 378 00:19:59,000 --> 00:20:01,130 There's lots of things that people can do themselves 379 00:20:01,130 --> 00:20:02,609 to adopt a healthy lifestyle 380 00:20:02,609 --> 00:20:06,650 like not smoking, healthy food, lots of exercise. 381 00:20:06,650 --> 00:20:11,417 So it matters, but it's not the only thing that matters. 382 00:20:19,640 --> 00:20:21,690 So just how small can we go? 383 00:20:22,980 --> 00:20:25,567 Well, let's start with what we know. 384 00:20:25,567 --> 00:20:28,346 The smallest adult humans known to science 385 00:20:28,346 --> 00:20:31,370 are just over 50 centimeters tall 386 00:20:31,370 --> 00:20:34,563 like Jyoti Amge, the world's smallest woman. 387 00:20:48,580 --> 00:20:50,650 24 year old student Jyoti 388 00:20:50,650 --> 00:20:53,040 is on a sight seeing trip to London. 389 00:20:53,040 --> 00:20:55,470 Wherever she goes, she gets as much attention 390 00:20:55,470 --> 00:20:56,933 as the biggest attractions. 391 00:21:02,230 --> 00:21:03,880 When I go outside, 392 00:21:05,270 --> 00:21:07,833 then everyone gathers together and stares at me. 393 00:21:09,900 --> 00:21:13,743 Then I feel a bit strange, but at the same time, 394 00:21:15,340 --> 00:21:17,290 it feels good that they all look at me. 395 00:21:20,210 --> 00:21:21,600 In our last episode, 396 00:21:21,600 --> 00:21:25,290 we met Sultan Kosen, the world's tallest man. 397 00:21:25,290 --> 00:21:27,100 Sultan is so tall because his body 398 00:21:27,100 --> 00:21:29,063 produces too much growth hormone. 399 00:21:30,100 --> 00:21:32,663 For Jyoti, the opposite is true. 400 00:21:33,964 --> 00:21:38,524 While Sultan has various health issues caused by being tall, 401 00:21:38,524 --> 00:21:40,693 for Jyoti, the story is different. 402 00:21:42,097 --> 00:21:43,680 The doctors told me 403 00:21:43,680 --> 00:21:45,433 I have hormone deficiency. 404 00:21:46,880 --> 00:21:48,993 This is the reason I can't grow taller. 405 00:21:50,040 --> 00:21:52,033 I don't have any other health problems. 406 00:21:53,070 --> 00:21:55,400 Jyoti's main complaint is simple. 407 00:21:55,400 --> 00:21:57,100 The world is just too big for her. 408 00:21:59,530 --> 00:22:00,940 One thing which I can't do 409 00:22:00,940 --> 00:22:03,283 because of my height is drive cars, 410 00:22:04,290 --> 00:22:08,013 and when I want to go out, I can't go out alone. 411 00:22:10,130 --> 00:22:12,220 I always have to have help from my family 412 00:22:13,830 --> 00:22:15,500 like my sisters and brothers. 413 00:22:15,500 --> 00:22:17,220 I always need help. 414 00:22:17,220 --> 00:22:19,660 These are the problems I face. 415 00:22:19,660 --> 00:22:22,110 But in a specially adapted environment, 416 00:22:22,110 --> 00:22:23,293 it's a different story. 417 00:22:26,080 --> 00:22:26,970 In my house, 418 00:22:26,970 --> 00:22:29,123 everything is specially made for me. 419 00:22:30,860 --> 00:22:35,860 In my bedroom, I have a small bed, cupboard, chair, table, 420 00:22:39,410 --> 00:22:42,533 and everything made in my size, all my furniture. 421 00:22:45,090 --> 00:22:47,423 I don't have any problems in my house. 422 00:22:52,637 --> 00:22:55,693 So what if we were all the size of Jyoti? 423 00:22:57,530 --> 00:23:00,630 We could adapt our environment to suit our smaller size. 424 00:23:09,540 --> 00:23:11,800 We would need less food and energy, 425 00:23:11,800 --> 00:23:13,250 which has to be a good thing. 426 00:23:16,254 --> 00:23:18,593 But surely, we can go further than this. 427 00:23:21,490 --> 00:23:23,573 Could a mammal this small survive? 428 00:23:25,220 --> 00:23:26,920 The answer is yes. 429 00:23:26,920 --> 00:23:30,880 In the wild, Etruscan shrews weigh just two grams 430 00:23:32,920 --> 00:23:35,820 which makes them one of the smallest mammals in the world. 431 00:23:37,060 --> 00:23:40,480 So it's a good role model for a miniature human being. 432 00:23:40,480 --> 00:23:42,430 Each one has a heart, lungs, 433 00:23:42,430 --> 00:23:44,434 and all the organs you would expect, 434 00:23:44,434 --> 00:23:47,473 but the similarities with human beings stop there. 435 00:23:48,370 --> 00:23:50,600 This tiny mammal lives its life 436 00:23:50,600 --> 00:23:52,733 right at the edge of what is possible. 437 00:23:53,730 --> 00:23:56,873 Professor Michael Brecht has studied them for years. 438 00:23:58,160 --> 00:23:59,153 Here they are. 439 00:24:00,353 --> 00:24:03,330 And I want to chase them into this. 440 00:24:03,330 --> 00:24:05,610 So now, here we have him. 441 00:24:05,610 --> 00:24:09,480 Let me show you what we do for gender determination. 442 00:24:09,480 --> 00:24:12,460 So the sexes, they look quite similar. 443 00:24:12,460 --> 00:24:16,330 The really foolproof sex testing 444 00:24:16,330 --> 00:24:17,800 is what I'm gonna do now. 445 00:24:17,800 --> 00:24:20,853 So we actually use this box here 446 00:24:20,853 --> 00:24:24,304 and what you do is you carefully, 447 00:24:24,304 --> 00:24:27,440 you put the shrew into the little box 448 00:24:27,440 --> 00:24:29,320 and you carefully sniff on it. 449 00:24:29,320 --> 00:24:34,320 Now, if it's very, very stinky, it turns out it's a female. 450 00:24:34,786 --> 00:24:38,763 If you sniff on it and you pass out, it's a male. 451 00:24:40,160 --> 00:24:41,793 So let me do this here. 452 00:24:43,180 --> 00:24:44,740 Female. 453 00:24:44,740 --> 00:24:47,233 Okay, now let's figure out how much she weighs. 454 00:24:49,040 --> 00:24:52,110 This is on the higher side for these animals. 455 00:24:52,110 --> 00:24:54,950 Many of the adults are just two grams. 456 00:24:54,950 --> 00:24:59,630 They have perfectly the same mammalian equipment. 457 00:24:59,630 --> 00:25:01,250 It's all there. 458 00:25:01,250 --> 00:25:03,154 It's just very tiny. 459 00:25:03,154 --> 00:25:06,840 It's very difficult to circulate blood 460 00:25:06,840 --> 00:25:08,370 through such a small body. 461 00:25:08,370 --> 00:25:10,300 The circulation system of mammals, 462 00:25:10,300 --> 00:25:13,679 it's much more suitable for bigger bodies. 463 00:25:13,679 --> 00:25:17,216 And both the respiration and the blood supply 464 00:25:17,216 --> 00:25:20,700 are a huge challenge for such a small body. 465 00:25:20,700 --> 00:25:24,430 So what we would see is they have a (mumbling) heart 466 00:25:24,430 --> 00:25:28,860 of 5% of the body weight or so, a really big heart. 467 00:25:28,860 --> 00:25:30,960 What we also see 468 00:25:30,960 --> 00:25:34,460 is that they have unheard of respiration rates. 469 00:25:34,460 --> 00:25:37,490 So when they are very excited, very nervous, 470 00:25:37,490 --> 00:25:39,910 one would see breaths per minute 471 00:25:39,910 --> 00:25:43,440 go up to about 1,000 breaths per minute, 472 00:25:43,440 --> 00:25:46,610 an absolutely unheard of rate in mammals. 473 00:25:46,610 --> 00:25:48,500 Really, also difficult to understand 474 00:25:48,500 --> 00:25:53,143 how a mammalian brain and lung could do that. 475 00:25:54,070 --> 00:25:57,628 Almost a thousand breaths a minute is certainly fast, 476 00:25:57,628 --> 00:26:00,780 but their hearts push things even further, 477 00:26:00,780 --> 00:26:03,430 beating up to 1,500 times a minute. 478 00:26:03,430 --> 00:26:06,303 That's 20 beat for every beat of a human heart. 479 00:26:07,210 --> 00:26:10,630 It's clearly hard work for a mammal to be so small. 480 00:26:10,630 --> 00:26:12,850 The question is why bother? 481 00:26:12,850 --> 00:26:17,468 The idea that ecologists have about these animals 482 00:26:17,468 --> 00:26:21,339 is that they are specialists for small spaces, yeah? 483 00:26:21,339 --> 00:26:26,339 For tunnels, and that they go into small spaces 484 00:26:26,368 --> 00:26:28,590 where no other predator can go 485 00:26:28,590 --> 00:26:30,360 and where they're then paradoxically, 486 00:26:30,360 --> 00:26:32,880 are again big predators. 487 00:26:32,880 --> 00:26:34,800 Matching your size to your environment 488 00:26:34,800 --> 00:26:37,060 is an important part of evolution, 489 00:26:37,060 --> 00:26:40,975 but filling this niche comes at an incredible cost. 490 00:26:40,975 --> 00:26:43,943 The biggest problem they face is heat loss. 491 00:26:45,158 --> 00:26:47,640 You see him in a thermal camera 492 00:26:47,640 --> 00:26:51,599 and you see how much heat he gives off, 493 00:26:51,599 --> 00:26:53,550 how much he lights up. 494 00:26:53,550 --> 00:26:57,365 And this is actually a central problem of their life. 495 00:26:57,365 --> 00:27:02,322 Their immense heat loss they have or energy loss they have 496 00:27:02,322 --> 00:27:06,863 as a result of their unfavorable surface to volume ratio. 497 00:27:07,910 --> 00:27:09,460 For every gram of body mass, 498 00:27:09,460 --> 00:27:11,010 small creatures like the shrew 499 00:27:11,010 --> 00:27:13,890 have more skin than bigger creatures like us. 500 00:27:13,890 --> 00:27:15,963 A human has a quarter of a square centimeter 501 00:27:15,963 --> 00:27:20,930 of skin for every gram, but a shrew has much more, 502 00:27:20,930 --> 00:27:23,536 almost 20 times more, in fact. 503 00:27:23,536 --> 00:27:26,620 So a shrew loses heat much more easily, 504 00:27:26,620 --> 00:27:29,670 which is particularly bad news for a mammal. 505 00:27:29,670 --> 00:27:31,560 Unlike insects and reptiles, 506 00:27:31,560 --> 00:27:33,770 mammals have to keep their bodies at a temperature 507 00:27:33,770 --> 00:27:36,603 of around 37 degrees centigrade to survive. 508 00:27:38,070 --> 00:27:40,440 Only one mammal has the heat loss problem 509 00:27:40,440 --> 00:27:43,573 worse than Etruscan shrews, their babies. 510 00:27:45,720 --> 00:27:50,160 But somehow, with the help of their parents, they survive. 511 00:27:50,160 --> 00:27:52,500 The newborn shrews are incredibly small, 512 00:27:52,500 --> 00:27:55,210 inconceivably small, 0.2 grams. 513 00:27:55,210 --> 00:27:57,640 It's just absolutely incredible. 514 00:27:57,640 --> 00:27:59,780 And they look kind of unreal. 515 00:27:59,780 --> 00:28:02,370 I mean, the whole body is totally transparent. 516 00:28:02,370 --> 00:28:04,611 They huddle together very heavenly. 517 00:28:04,611 --> 00:28:07,160 The mother is very protective 518 00:28:07,160 --> 00:28:12,160 and obviously also supplies a lot of energy. 519 00:28:15,740 --> 00:28:17,730 If mammals can get this small, 520 00:28:17,730 --> 00:28:19,033 then why not a human? 521 00:28:22,880 --> 00:28:24,630 It's feasible that the human body 522 00:28:24,630 --> 00:28:27,650 could work at just five centimeters tall, 523 00:28:27,650 --> 00:28:30,970 but of course, we'd face all the same problems as the shrew. 524 00:28:30,970 --> 00:28:34,353 An insane heart rate and a constant battle to keep warm. 525 00:28:37,700 --> 00:28:41,653 Life at this size requires a totally different lifestyle. 526 00:28:44,500 --> 00:28:48,250 It's not just about huddling together for warmth, 527 00:28:48,250 --> 00:28:50,260 if you're losing energy fast, 528 00:28:50,260 --> 00:28:52,750 you need to be very good at replacing it. 529 00:28:52,750 --> 00:28:54,540 In fact, scientists have discovered 530 00:28:54,540 --> 00:28:56,490 that small animals have to have 531 00:28:56,490 --> 00:28:58,643 a completely different relationship to food 532 00:28:58,643 --> 00:29:00,700 than big animals. 533 00:29:00,700 --> 00:29:01,920 More than 100 years ago, 534 00:29:01,920 --> 00:29:04,800 a scientist named Kleiber observed empirically 535 00:29:04,800 --> 00:29:07,414 that the amount of food that an animal requires 536 00:29:07,414 --> 00:29:10,780 increases, of course, with how big the animal is. 537 00:29:10,780 --> 00:29:13,411 So an elephant eats more than a deer does. 538 00:29:13,411 --> 00:29:16,700 But the relationship doesn't go up proportionately. 539 00:29:16,700 --> 00:29:19,642 So an elephant eats a little bit less than you'd expect 540 00:29:19,642 --> 00:29:22,583 than an equal number of deers would. 541 00:29:25,860 --> 00:29:28,942 An Asian elephant weighs about 5,000 kilograms, 542 00:29:28,942 --> 00:29:30,593 but how much does it eat? 543 00:29:31,776 --> 00:29:33,633 Just ask a zookeeper. 544 00:29:37,154 --> 00:29:38,460 This is the amount of hay 545 00:29:38,460 --> 00:29:40,710 one of our male elephants get every day. 546 00:29:40,710 --> 00:29:43,530 43 kilos to 45 kilos. 547 00:29:43,530 --> 00:29:46,440 Which is about 1% of its body weight. 548 00:29:46,440 --> 00:29:49,780 For the dik-dik, their mass is about seven kilos. 549 00:29:49,780 --> 00:29:51,240 This is amount of alfalfa 550 00:29:51,240 --> 00:29:53,317 our dik-dik get on a daily basis. 551 00:29:53,317 --> 00:29:55,440 0.5 kilos. 552 00:29:55,440 --> 00:29:57,933 Around 7% of its body mass. 553 00:29:59,852 --> 00:30:02,540 Repeat this for all kinds of different animals 554 00:30:02,540 --> 00:30:04,070 and a clear pattern emerges. 555 00:30:04,070 --> 00:30:05,870 The smaller the animal, 556 00:30:05,870 --> 00:30:08,917 the more food energy they need per kilo of body mass. 557 00:30:08,917 --> 00:30:10,499 And for the smallest animals, 558 00:30:10,499 --> 00:30:13,633 the amount of food they need goes through the roof. 559 00:30:17,000 --> 00:30:19,300 Applied to our five centimeter human, 560 00:30:19,300 --> 00:30:20,680 Kleiber's Law reveals 561 00:30:20,680 --> 00:30:23,343 we'd have to eat our own body weight every day. 562 00:30:26,923 --> 00:30:29,830 Most of our life would be spent looking for food 563 00:30:31,070 --> 00:30:32,623 just like the Etruscan shrew. 564 00:30:38,631 --> 00:30:41,403 But what if we went smaller still? 565 00:30:42,240 --> 00:30:43,841 So if you were to take a mammal 566 00:30:43,841 --> 00:30:47,660 and to make it smaller than the smallest current mammal, 567 00:30:47,660 --> 00:30:49,709 then it would cease to be a mammal as we know it 568 00:30:49,709 --> 00:30:53,220 because the rate at which it would lose heat 569 00:30:53,220 --> 00:30:54,500 into the environment would be so great, 570 00:30:54,500 --> 00:30:57,225 it couldn't maintain its internal temperature 571 00:30:57,225 --> 00:30:58,850 to be warm blooded. 572 00:30:58,850 --> 00:31:00,990 And so it would have to change its physiology. 573 00:31:00,990 --> 00:31:02,240 It would have to become cold blooded 574 00:31:02,240 --> 00:31:03,830 and use different strategies 575 00:31:03,830 --> 00:31:05,680 in order to regulate its temperature. 576 00:31:07,660 --> 00:31:08,760 So going smaller 577 00:31:08,760 --> 00:31:11,620 means saying goodbye to being a mammal. 578 00:31:11,620 --> 00:31:13,319 From here on, we'll need to be cold blooded 579 00:31:13,319 --> 00:31:15,403 with organs more like an insect. 580 00:31:17,220 --> 00:31:19,954 But it's worth it because incredible things start happening 581 00:31:19,954 --> 00:31:22,403 once you get down to the size of a wasp. 582 00:31:25,590 --> 00:31:28,000 At Cambridge University, they're finding 583 00:31:28,000 --> 00:31:29,920 that for very small creatures, 584 00:31:29,920 --> 00:31:31,920 the world is a completely different place 585 00:31:31,920 --> 00:31:33,600 to the one we experience. 586 00:31:35,163 --> 00:31:38,763 It's as if they're ruled by separate laws of physics. 587 00:31:39,780 --> 00:31:41,120 In terms of their relative strength, 588 00:31:41,120 --> 00:31:43,519 you might almost say that insects are superheroes. 589 00:31:43,519 --> 00:31:45,350 So some of the strongest ants 590 00:31:45,350 --> 00:31:47,560 can easily carry four or five times their own body weight 591 00:31:47,560 --> 00:31:49,960 which for us is the equivalent of of almost a small car 592 00:31:49,960 --> 00:31:52,150 if you're a relatively big human. 593 00:31:52,150 --> 00:31:54,290 This is all because volume, area, 594 00:31:54,290 --> 00:31:56,880 and length change by different amounts 595 00:31:56,880 --> 00:31:58,363 when you make things small. 596 00:31:59,330 --> 00:32:01,770 The overall effect is to make small creatures 597 00:32:01,770 --> 00:32:04,163 relatively much stronger than big ones. 598 00:32:05,490 --> 00:32:08,600 Professor David Labonte carries out tests on ants 599 00:32:08,600 --> 00:32:10,103 to see just how strong. 600 00:32:11,467 --> 00:32:13,180 Ants support the weight of a paintbrush 601 00:32:13,180 --> 00:32:15,010 which is roughly 2.5 grams. 602 00:32:15,010 --> 00:32:17,960 That corresponds to around 500 times its own weight 603 00:32:17,960 --> 00:32:20,860 which would be the equivalent of me for 40 tonnes 604 00:32:20,860 --> 00:32:23,760 which is probably about six, seven lorries. 605 00:32:23,760 --> 00:32:25,480 So it's really quite impressive. 606 00:32:30,667 --> 00:32:32,530 But there's more to being small 607 00:32:32,530 --> 00:32:34,464 than just strength. 608 00:32:34,464 --> 00:32:37,214 (insect buzzing) 609 00:32:38,310 --> 00:32:39,860 As we know, small creatures 610 00:32:39,860 --> 00:32:42,057 have bigger surface area for their weight, 611 00:32:50,070 --> 00:32:52,213 a fact that can be a life saver. 612 00:32:54,370 --> 00:32:55,610 So one of the very first studies 613 00:32:55,610 --> 00:32:57,920 that thought about the question how size matters 614 00:32:57,920 --> 00:32:59,889 and what the right size for an animal is 615 00:32:59,889 --> 00:33:00,980 thought about the problem 616 00:33:00,980 --> 00:33:03,059 of why you can drop an ant down a shaft 617 00:33:03,059 --> 00:33:05,756 and the ant just falls down the ground and walks away, 618 00:33:05,756 --> 00:33:07,562 but if you would do the same to a human, 619 00:33:07,562 --> 00:33:09,000 the human would break. 620 00:33:09,000 --> 00:33:10,590 Because the ant is so small, 621 00:33:10,590 --> 00:33:12,940 air resistance is much more important for the ant. 622 00:33:12,940 --> 00:33:14,880 So the velocity with which the ant hits the ground 623 00:33:14,880 --> 00:33:17,923 is much slower than what would happen to a human. 624 00:33:20,191 --> 00:33:21,520 Taken to an extreme, 625 00:33:21,520 --> 00:33:25,096 it's why rock dust floats in the air but rocks don't 626 00:33:25,096 --> 00:33:28,260 even though they're made of the same stuff. 627 00:33:28,260 --> 00:33:31,160 And there are even more advantages to being so small. 628 00:33:31,160 --> 00:33:32,890 So one of the things we're interested in 629 00:33:32,890 --> 00:33:35,042 is how well insects stick. 630 00:33:35,042 --> 00:33:37,550 And one of the techniques we use to measure that 631 00:33:37,550 --> 00:33:38,628 is a centrifuge. 632 00:33:38,628 --> 00:33:41,600 So we take a little ant, put it on a centrifuge, 633 00:33:41,600 --> 00:33:43,379 and start spinning it around. 634 00:33:43,379 --> 00:33:46,120 And we then try and measure at what acceleration 635 00:33:46,120 --> 00:33:48,270 these ants actually fall of the centrifuge. 636 00:33:49,872 --> 00:33:51,360 Wow. 637 00:33:51,360 --> 00:33:52,470 G-force is the name 638 00:33:52,470 --> 00:33:55,313 for the feeling you might get on a steep rollercoaster. 639 00:33:56,600 --> 00:33:59,443 In the tightest turn, you might experience six G. 640 00:34:00,720 --> 00:34:03,660 But even with much, much higher g-forces, 641 00:34:03,660 --> 00:34:06,210 somehow, the ants hang on. 642 00:34:06,210 --> 00:34:07,250 And during these measurements, 643 00:34:07,250 --> 00:34:09,780 we've seen ants withstand 500 G, 1,000 G 644 00:34:09,780 --> 00:34:11,660 for 10, 20, even 30 seconds, 645 00:34:11,660 --> 00:34:14,740 and then they fall off and walk off as if nothing happened. 646 00:34:14,740 --> 00:34:16,570 It's this same ability to hang on 647 00:34:16,570 --> 00:34:19,980 that allows insects to walk up the smoothest of walls, 648 00:34:19,980 --> 00:34:21,800 even hang on to the ceiling. 649 00:34:21,800 --> 00:34:23,260 So how does it work? 650 00:34:23,260 --> 00:34:25,130 Insects, or geckos, or any animal 651 00:34:25,130 --> 00:34:26,367 that climbs with adhesive feet, 652 00:34:26,367 --> 00:34:27,640 they can't use a glue 653 00:34:27,640 --> 00:34:29,310 because it would take a long time 654 00:34:29,310 --> 00:34:30,810 to activate and deactivate. 655 00:34:30,810 --> 00:34:32,730 So as far as we know, climbing animals 656 00:34:32,730 --> 00:34:35,750 use intermolecular forces to stick to surfaces. 657 00:34:35,750 --> 00:34:36,583 It's still under debate 658 00:34:36,583 --> 00:34:38,640 what exactly these intermolecular forces are. 659 00:34:38,640 --> 00:34:40,023 If you have two molecules and they attract each other, 660 00:34:40,023 --> 00:34:43,050 then you have to convince them to split apart 661 00:34:43,050 --> 00:34:45,363 and that's when helps these animals to stick. 662 00:34:46,250 --> 00:34:47,160 We experience 663 00:34:47,160 --> 00:34:49,836 these intramolecular sticking forces too, 664 00:34:49,836 --> 00:34:51,978 but at our normal human size, 665 00:34:51,978 --> 00:34:53,730 we're not even aware of them 666 00:34:53,730 --> 00:34:55,913 because they're tiny compared to gravity. 667 00:34:56,840 --> 00:35:00,383 But once more, being small changes the rules. 668 00:35:00,383 --> 00:35:04,673 A five millimeter human could climb a wall just like an ant. 669 00:35:06,110 --> 00:35:09,080 But it's not all good news for small creatures. 670 00:35:09,080 --> 00:35:11,760 A five millimeter human may be good at climbing, 671 00:35:11,760 --> 00:35:14,060 but he might not understand why he's doing it. 672 00:35:14,966 --> 00:35:19,040 It's a problem that affects all very small creatures. 673 00:35:19,040 --> 00:35:20,113 Brain size. 674 00:35:21,721 --> 00:35:23,624 Our brains rely on our neurons 675 00:35:23,624 --> 00:35:25,250 and it looks like that neurons 676 00:35:25,250 --> 00:35:28,260 remain relatively constant in size across different animals. 677 00:35:28,260 --> 00:35:30,890 So whether you're a very small or a very big animal, 678 00:35:30,890 --> 00:35:33,460 the neuron is approximately the same size. 679 00:35:33,460 --> 00:35:35,610 Now, this immediately means that if you're very small, 680 00:35:35,610 --> 00:35:37,150 you have fewer neurons, 681 00:35:37,150 --> 00:35:38,590 and that might present you with a problem 682 00:35:38,590 --> 00:35:40,560 regarding your cognitive abilities. 683 00:35:40,560 --> 00:35:41,550 The bottom line is 684 00:35:41,550 --> 00:35:43,240 if you're going to get really small, 685 00:35:43,240 --> 00:35:44,963 you're going to lose brain power. 686 00:35:49,719 --> 00:35:51,020 A five millimeter human 687 00:35:51,020 --> 00:35:53,270 would only have around two million neurons 688 00:35:53,270 --> 00:35:55,940 which puts him somewhere between a cockroach 689 00:35:55,940 --> 00:35:57,542 and a small fish. 690 00:35:57,542 --> 00:35:58,983 Smart enough to spot food, 691 00:36:02,554 --> 00:36:04,440 but probably not smart enough 692 00:36:04,440 --> 00:36:06,693 to worry about the puddle of coffee in the way. 693 00:36:09,070 --> 00:36:10,490 For normal size people, 694 00:36:10,490 --> 00:36:12,463 surface tension is barely noticeable, 695 00:36:13,340 --> 00:36:16,910 but when you're tiny, it's suddenly deadly. 696 00:36:16,910 --> 00:36:17,930 Surface tension is a force 697 00:36:17,930 --> 00:36:19,400 that becomes very, very powerful 698 00:36:19,400 --> 00:36:20,800 if you're very small, 699 00:36:20,800 --> 00:36:23,090 and really unimportant if you're really big. 700 00:36:23,090 --> 00:36:24,451 So for very small animals, 701 00:36:24,451 --> 00:36:26,552 a droplet of water can be very dangerous 702 00:36:26,552 --> 00:36:29,352 while very large animals will hardly notice the droplet. 703 00:36:31,490 --> 00:36:33,040 Super powers or not, 704 00:36:33,040 --> 00:36:35,006 being small has too many downsides 705 00:36:35,006 --> 00:36:38,290 like tiny brains, constantly looking for food, 706 00:36:38,290 --> 00:36:40,170 and of course, if you're that small, 707 00:36:40,170 --> 00:36:42,570 almost everything in the world wants to eat you. 708 00:36:44,152 --> 00:36:47,690 So it's for the best that we return things to how they were 709 00:36:53,140 --> 00:36:54,810 because the size we are now 710 00:36:54,810 --> 00:36:56,960 is a perfect fit for the way we live 711 00:36:56,960 --> 00:36:58,533 and the world we live in today. 712 00:36:59,380 --> 00:37:02,193 Lifespan, health, food, society, resources, 713 00:37:02,193 --> 00:37:05,423 it all goes hand in hand with our size. 714 00:37:10,340 --> 00:37:13,750 We've tried shrinking the planet and even ourselves, 715 00:37:13,750 --> 00:37:17,810 but so far, small has not proved to be beautiful, 716 00:37:17,810 --> 00:37:20,290 but there's one thing we haven't tried, 717 00:37:20,290 --> 00:37:22,030 something so big that surely, 718 00:37:22,030 --> 00:37:23,460 we could make it a little smaller 719 00:37:23,460 --> 00:37:25,173 without ending life as we know it. 720 00:37:26,740 --> 00:37:27,573 The sun. 721 00:37:28,443 --> 00:37:32,060 Perhaps a smaller sun would be a good idea. 722 00:37:32,060 --> 00:37:35,283 Less skin cancer, a cooler climate. 723 00:37:35,283 --> 00:37:37,700 The sun we have is a kind of star 724 00:37:37,700 --> 00:37:40,780 known to astronomers as a G2 drawf, 725 00:37:40,780 --> 00:37:43,750 but it's not really much of a dwarf by human standards. 726 00:37:43,750 --> 00:37:47,470 In fact, it's 1.4 million kilometers wide. 727 00:37:47,470 --> 00:37:50,543 That's 109 times wider than the Earth. 728 00:37:51,860 --> 00:37:54,805 But does it have to be so preposterously large 729 00:37:54,805 --> 00:37:57,980 or would everything work out fine with a smaller, 730 00:37:57,980 --> 00:38:00,540 gentler sun that wouldn't damage our skin 731 00:38:00,540 --> 00:38:03,053 and we can look at without sunglasses? 732 00:38:04,660 --> 00:38:05,900 The key to this question 733 00:38:05,900 --> 00:38:08,563 is understanding what makes a star shine. 734 00:38:09,730 --> 00:38:11,510 Stars are big balls of gas 735 00:38:11,510 --> 00:38:14,210 which have been pulled together by gravity. 736 00:38:14,210 --> 00:38:17,890 At some point, the gases literally fuse. 737 00:38:17,890 --> 00:38:19,540 Subatomic hydrogen particles 738 00:38:19,540 --> 00:38:22,100 get squashed together to make helium. 739 00:38:22,100 --> 00:38:24,462 This is nuclear fusion 740 00:38:24,462 --> 00:38:27,900 which generates such enormous amounts of energy 741 00:38:27,900 --> 00:38:30,400 that we've been trying to replicate the process on Earth 742 00:38:30,400 --> 00:38:32,650 ever since it was discovered. 743 00:38:32,650 --> 00:38:36,563 The problem is that it turns out it's incredibly hard to do. 744 00:38:37,950 --> 00:38:40,930 This is one of the world's best attempts, 745 00:38:40,930 --> 00:38:43,850 JET, Joint European Torus, 746 00:38:43,850 --> 00:38:46,187 based at Culham in the U.K. 747 00:38:46,187 --> 00:38:47,709 The first place on Earth 748 00:38:47,709 --> 00:38:51,133 that they managed to achieve controlled nuclear fusion, 749 00:38:52,599 --> 00:38:56,176 a phenomenally complicated and expensive facility 750 00:38:56,176 --> 00:38:58,850 where they use as much power as a small (mumbling) 751 00:38:58,850 --> 00:39:01,203 to superheat the gases until they fuse. 752 00:39:02,680 --> 00:39:07,170 Jet physicist Ivor Coffey knows just how intense things get. 753 00:39:07,170 --> 00:39:09,350 The fusion takes place inside this chamber. 754 00:39:09,350 --> 00:39:12,390 We actually create a highly ionized gas or plasma. 755 00:39:12,390 --> 00:39:13,620 Sort of the center of the plasma 756 00:39:13,620 --> 00:39:15,852 which is probably roughly just above my head 757 00:39:15,852 --> 00:39:18,270 would be where the temperature 758 00:39:18,270 --> 00:39:20,780 and density are at the maximum temperature. 759 00:39:20,780 --> 00:39:22,084 There could be something in the reads 760 00:39:22,084 --> 00:39:24,643 in between 100 and 150 million degrees centigrade. 761 00:39:26,110 --> 00:39:28,200 Conditions in here are so extreme 762 00:39:28,200 --> 00:39:31,463 that they can only run the machine for 30 seconds at a time. 763 00:39:34,100 --> 00:39:36,030 Today, they're running the fusion test 764 00:39:36,030 --> 00:39:38,807 at even higher power levels than they've tried before. 765 00:39:41,203 --> 00:39:45,363 10, nine, eight, seven, six, 766 00:39:45,363 --> 00:39:48,196 five, four, three, two, one, zero. 767 00:39:51,255 --> 00:39:54,838 (intense orchestral music) 768 00:39:57,280 --> 00:39:59,420 What you are looking at right now 769 00:39:59,420 --> 00:40:01,380 is actual fusion. 770 00:40:01,380 --> 00:40:03,090 This is the very same process 771 00:40:03,090 --> 00:40:05,213 that happens at the heart of a star. 772 00:40:06,131 --> 00:40:09,714 (intense orchestral music) 773 00:40:14,870 --> 00:40:17,420 The problem of making fusion happen on Earth 774 00:40:17,420 --> 00:40:20,870 is no different to the problem of making it happen in space, 775 00:40:20,870 --> 00:40:23,148 but stars manage to solve this problem 776 00:40:23,148 --> 00:40:25,103 by being incredibly big. 777 00:40:26,350 --> 00:40:29,530 The main requirement if you want to trigger fusion 778 00:40:29,530 --> 00:40:30,800 anywhere in the universe, 779 00:40:30,800 --> 00:40:33,550 inside of stars or in a laboratory on Earth 780 00:40:33,550 --> 00:40:35,205 is that you have to create conditions 781 00:40:35,205 --> 00:40:37,440 of very high temperature. 782 00:40:37,440 --> 00:40:40,480 And the problem then is that if you have high temperature, 783 00:40:40,480 --> 00:40:42,350 you will also basically have the problem 784 00:40:42,350 --> 00:40:44,490 that this high temperature ball of material 785 00:40:44,490 --> 00:40:47,670 wants to be pushed out by the pressure. 786 00:40:47,670 --> 00:40:49,770 So you have to somehow overcome the pressure. 787 00:40:49,770 --> 00:40:53,110 And the stars do this by having all the gravity 788 00:40:53,110 --> 00:40:54,130 of the overlying material. 789 00:40:54,130 --> 00:40:55,430 The gravity of the star 790 00:40:55,430 --> 00:40:57,903 is confining the pressure of the hot material. 791 00:40:59,980 --> 00:41:02,420 For stars, size matters. 792 00:41:02,420 --> 00:41:05,260 If they're not big enough, fusion can't happen. 793 00:41:05,260 --> 00:41:07,833 And without fusion, it's not a star at all. 794 00:41:09,910 --> 00:41:12,680 If we make stars smaller, less massive, 795 00:41:12,680 --> 00:41:15,560 and the temperature of the star 796 00:41:15,560 --> 00:41:16,690 in the center will also go down, 797 00:41:16,690 --> 00:41:17,610 and at some point, 798 00:41:17,610 --> 00:41:20,240 the temperature is not sufficient any longer 799 00:41:20,240 --> 00:41:22,552 to ignite nuclear fusion. 800 00:41:22,552 --> 00:41:25,290 And this really is the fundamental limit, 801 00:41:25,290 --> 00:41:26,850 if you like, for stardom. 802 00:41:26,850 --> 00:41:29,030 The very smallest we could make our sun 803 00:41:29,030 --> 00:41:30,450 or indeed any star 804 00:41:30,450 --> 00:41:33,260 is around 10 times the width of the Earth. 805 00:41:33,260 --> 00:41:34,922 But with a sun this size, 806 00:41:34,922 --> 00:41:37,333 what kind of Earth would we wake up to? 807 00:41:40,536 --> 00:41:43,203 (alarm beeping) 808 00:41:44,360 --> 00:41:46,973 For starters, you'd be seeing red. 809 00:41:49,520 --> 00:41:52,560 The reason that this low mass star would be red 810 00:41:52,560 --> 00:41:56,000 is that this star would have much reduced gravity, 811 00:41:56,000 --> 00:42:00,150 and therefore also it would have much reduced temperature. 812 00:42:00,150 --> 00:42:04,830 It would shift the peak wavelength of your photons 813 00:42:04,830 --> 00:42:06,358 that the star is emitting 814 00:42:06,358 --> 00:42:08,550 into longer and longer wavelengths. 815 00:42:08,550 --> 00:42:11,457 This means that we shifted from the yellow that our sun has 816 00:42:11,457 --> 00:42:15,540 into the red that those red dwarf stars would have. 817 00:42:16,610 --> 00:42:17,720 A star this size 818 00:42:17,720 --> 00:42:19,970 would be no brighter than the moon, 819 00:42:19,970 --> 00:42:22,710 but light isn't the only casualty. 820 00:42:22,710 --> 00:42:25,822 Within hours, we'd feel a bigger problem. 821 00:42:25,822 --> 00:42:27,520 What would happen to a planet 822 00:42:27,520 --> 00:42:30,460 around such a red dwarf central star? 823 00:42:30,460 --> 00:42:31,370 The most dramatic thing 824 00:42:31,370 --> 00:42:36,118 is that because of the very, very much reduced temperature, 825 00:42:36,118 --> 00:42:39,293 we would basically experience a deep freeze. 826 00:42:40,430 --> 00:42:42,430 Temperatures would plummet. 827 00:42:43,470 --> 00:42:46,490 A star this size gives off just one six thousandth 828 00:42:46,490 --> 00:42:48,343 of the heat of our sun. 829 00:42:50,176 --> 00:42:54,133 All the liquid water would be converted into ice. 830 00:42:54,133 --> 00:42:58,520 Even our atmosphere would begin to freeze out. 831 00:42:58,520 --> 00:43:02,030 We would enter into a state of complete cold, 832 00:43:02,030 --> 00:43:03,847 deep desperate freeze. 833 00:43:05,200 --> 00:43:06,970 As the Earth cools further, 834 00:43:06,970 --> 00:43:09,300 all the gases in the air solidify 835 00:43:09,300 --> 00:43:11,413 causing the atmosphere to collapse. 836 00:43:13,660 --> 00:43:15,083 So how do we save the world? 837 00:43:16,870 --> 00:43:18,790 The answer may seem obvious. 838 00:43:18,790 --> 00:43:23,033 We move the planet closer to the sun so that things warm up. 839 00:43:24,040 --> 00:43:25,663 But would that actually work? 840 00:43:27,459 --> 00:43:29,060 Earth's normal orbit 841 00:43:29,060 --> 00:43:33,010 is about 150 million kilometers from the sun. 842 00:43:33,010 --> 00:43:35,070 This is the middle of the habitable zone, 843 00:43:35,070 --> 00:43:37,830 the region of the solar system where it's not too hot 844 00:43:37,830 --> 00:43:38,983 and not too cold. 845 00:43:41,270 --> 00:43:42,227 Now, we've moved the Earth 846 00:43:42,227 --> 00:43:45,633 nearly 100 times closer to the tiny sun. 847 00:43:47,066 --> 00:43:50,649 (intense orchestral music) 848 00:43:51,831 --> 00:43:54,590 At this distance, our planet gets the same energy 849 00:43:54,590 --> 00:43:56,090 from the sun as we're used to, 850 00:43:57,310 --> 00:43:58,810 but this is a different world. 851 00:44:01,410 --> 00:44:04,098 The sun may be tiny, but we are so close 852 00:44:04,098 --> 00:44:06,770 that it would look big in the sky. 853 00:44:06,770 --> 00:44:09,193 Around 10 times bigger than we're used to. 854 00:44:12,530 --> 00:44:14,830 But there are problems to face, 855 00:44:14,830 --> 00:44:17,050 problems that the best scientists in the world 856 00:44:17,050 --> 00:44:18,713 are trying to solve 857 00:44:18,713 --> 00:44:22,300 because they've recently discovered a planet just like this 858 00:44:22,300 --> 00:44:24,503 and it turns out it's our nearest neighbor. 859 00:44:25,800 --> 00:44:28,270 If you look at the many stars in the night sky, 860 00:44:28,270 --> 00:44:30,670 you probably won't even notice Proxima Centauri. 861 00:44:31,917 --> 00:44:34,400 It's actually the closest of them all, 862 00:44:34,400 --> 00:44:35,880 but it's very small, 863 00:44:35,880 --> 00:44:40,490 just one seventh the size of the sun, but it's up there. 864 00:44:40,490 --> 00:44:42,905 And at Queen Mary University London, 865 00:44:42,905 --> 00:44:45,210 astronomers have been looking very hard 866 00:44:45,210 --> 00:44:46,925 at the faint light it gives off 867 00:44:46,925 --> 00:44:48,860 to see what they can discover 868 00:44:48,860 --> 00:44:50,793 about the sun's tiny neighbor. 869 00:44:53,720 --> 00:44:56,353 Proxima Centauri is the nearest star to the sun. 870 00:44:57,370 --> 00:44:59,210 This is where astronomy begins. 871 00:44:59,210 --> 00:45:02,910 So it's really the first spot in the next frontier. 872 00:45:02,910 --> 00:45:07,550 So the first place to go when we go beyond our solar system. 873 00:45:07,550 --> 00:45:09,523 So that makes it very special. 874 00:45:10,540 --> 00:45:12,350 In August 2016, 875 00:45:12,350 --> 00:45:14,140 they made an astonishing discovery 876 00:45:14,140 --> 00:45:17,623 by analyzing the light that Proxima Centauri gives off. 877 00:45:18,910 --> 00:45:21,350 So basically what we do, we go to a telescope. 878 00:45:21,350 --> 00:45:24,820 The telescope has an optical fiber sitting at the focus 879 00:45:24,820 --> 00:45:26,310 and then the light from the star 880 00:45:26,310 --> 00:45:27,410 goes through the optical fiber 881 00:45:27,410 --> 00:45:28,834 to the basement of the observatory 882 00:45:28,834 --> 00:45:30,390 where there's a spectrometer. 883 00:45:30,390 --> 00:45:31,709 And what the spectrometer does. 884 00:45:31,709 --> 00:45:33,986 Takes the light coming from the optical fiber 885 00:45:33,986 --> 00:45:36,880 and these two elements here, a prism and a grating, 886 00:45:36,880 --> 00:45:38,648 separate the light into wavelengths. 887 00:45:38,648 --> 00:45:41,688 And we see that there are these dark spots 888 00:45:41,688 --> 00:45:43,750 in the middle of the traces. 889 00:45:43,750 --> 00:45:47,020 These are the footprints of molecules 890 00:45:47,020 --> 00:45:49,730 and atoms in the atmosphere of the star. 891 00:45:49,730 --> 00:45:51,650 When they observed the star again, 892 00:45:51,650 --> 00:45:54,883 they saw that the spectrum of Proxima Centauri was changing. 893 00:45:55,930 --> 00:45:58,887 So we come here to the telescope two months later. 894 00:45:58,887 --> 00:46:00,420 We take more data 895 00:46:00,420 --> 00:46:03,350 and then we see that the measurements start to trend. 896 00:46:03,350 --> 00:46:05,260 Something is happening, whether we don't know what. 897 00:46:05,260 --> 00:46:06,440 We got more measurements, 898 00:46:06,440 --> 00:46:07,970 more measurements, more measurements, 899 00:46:07,970 --> 00:46:09,080 and after two years, 900 00:46:09,080 --> 00:46:12,032 then we see that it reaches a peak 901 00:46:12,032 --> 00:46:14,860 and then you have this signal. 902 00:46:14,860 --> 00:46:15,790 And it's repeating also. 903 00:46:15,790 --> 00:46:17,501 If we keep observing the star, 904 00:46:17,501 --> 00:46:19,601 we see the same thing over and over again. 905 00:46:21,086 --> 00:46:22,829 These wobbles in the spectrum 906 00:46:22,829 --> 00:46:27,020 reveal that the star has been pulled backward and forwards. 907 00:46:27,020 --> 00:46:30,523 It's the telltale sign of a planet orbiting close by. 908 00:46:32,700 --> 00:46:35,952 Further study shows that this planet called Proxima b 909 00:46:35,952 --> 00:46:39,240 has a lot of similarities to our own. 910 00:46:39,240 --> 00:46:42,433 It's roughly Earth-sized and mostly made of rock, 911 00:46:43,570 --> 00:46:48,390 but unlike Earth, which takes 365 days to go around its sun, 912 00:46:48,390 --> 00:46:51,150 the spectrum patterns reveal that Proxima b 913 00:46:51,150 --> 00:46:52,670 takes a mere 11 days 914 00:46:52,670 --> 00:46:55,983 meaning it must be very close to its star. 915 00:46:57,900 --> 00:46:59,600 When the scientists did the maths, 916 00:46:59,600 --> 00:47:01,685 they realized it is at a perfect distance 917 00:47:01,685 --> 00:47:04,242 for the possibility of life. 918 00:47:04,242 --> 00:47:07,760 Not too hot and not too cold. 919 00:47:07,760 --> 00:47:10,010 There are many more factors to consider 920 00:47:10,010 --> 00:47:11,913 before they know if life is possible. 921 00:47:13,310 --> 00:47:14,840 It's only right to the solar system 922 00:47:14,840 --> 00:47:17,456 that we can expect to actually 923 00:47:17,456 --> 00:47:20,069 start to search for evidence of life 924 00:47:20,069 --> 00:47:23,410 in the planets like this one is Proxima Centauri 925 00:47:23,410 --> 00:47:25,010 and also some very nearby stars. 926 00:47:26,644 --> 00:47:29,660 As the search for life on Proxima b begins, 927 00:47:29,660 --> 00:47:33,870 what can we learn from it to help our thought experiment? 928 00:47:33,870 --> 00:47:36,463 Could life survive this close to a small sun? 929 00:47:37,830 --> 00:47:41,170 For a start, plants would have to be a different color. 930 00:47:41,170 --> 00:47:43,560 Plants are green because of the specific wavelength 931 00:47:43,560 --> 00:47:45,367 of light they use. 932 00:47:45,367 --> 00:47:49,258 But if our sun was red like Proxima Centauri, 933 00:47:49,258 --> 00:47:51,739 crucial wavelengths would be missing 934 00:47:51,739 --> 00:47:54,400 and green plants wouldn't work. 935 00:47:54,400 --> 00:47:55,770 They'd have to be black 936 00:47:55,770 --> 00:47:58,970 to absorb as much sunlight as possible. 937 00:47:58,970 --> 00:48:02,200 Our planet would look very different, 938 00:48:02,200 --> 00:48:04,121 but there's a much bigger problem. 939 00:48:04,121 --> 00:48:07,633 A possible side effect of being so close to a star. 940 00:48:08,600 --> 00:48:09,803 Tidal locking. 941 00:48:10,700 --> 00:48:12,800 So basically you have a small star. 942 00:48:12,800 --> 00:48:15,724 The small star makes very little energy. 943 00:48:15,724 --> 00:48:17,470 It's also faint. 944 00:48:17,470 --> 00:48:20,470 So you need to be warm, you need to be close to it. 945 00:48:20,470 --> 00:48:22,150 And the fact of being close to it 946 00:48:22,150 --> 00:48:25,390 means that you also have a very strong tidal forces then 947 00:48:25,390 --> 00:48:26,950 and most likely what will happen 948 00:48:26,950 --> 00:48:30,095 is like what happens with the moon to the Earth. 949 00:48:30,095 --> 00:48:31,940 The rotation of the planet 950 00:48:31,940 --> 00:48:34,340 is synchronized to the orbit of the planet 951 00:48:34,340 --> 00:48:36,823 so the same side faces the star. 952 00:48:38,340 --> 00:48:41,270 With one side frozen in perpetual night 953 00:48:41,270 --> 00:48:43,750 and the other in never-ending sun, 954 00:48:43,750 --> 00:48:46,190 planets that are fully tidally locked 955 00:48:46,190 --> 00:48:48,683 are sometimes called eyeball planets. 956 00:48:50,670 --> 00:48:53,110 The world we are used to isn't possible 957 00:48:53,110 --> 00:48:55,092 around a smaller sun. 958 00:48:55,092 --> 00:48:58,190 Even if we move close enough to the sun to be warm, 959 00:48:58,190 --> 00:49:00,663 Earth would be a very difficult place to live. 960 00:49:02,448 --> 00:49:05,400 (intense orchestral music) 961 00:49:05,400 --> 00:49:09,450 It turns out that the size of our sun is everything. 962 00:49:09,450 --> 00:49:12,760 Any smaller and we can't have a green world, 963 00:49:12,760 --> 00:49:14,577 can't have night and day, 964 00:49:14,577 --> 00:49:17,403 and most of our world becomes deadly. 965 00:49:22,010 --> 00:49:26,040 It seems we are better off with the sun the size it was, 966 00:49:26,040 --> 00:49:30,893 us the size we are, living on a planet that is just right. 967 00:49:33,880 --> 00:49:35,170 Size does matter. 968 00:49:35,170 --> 00:49:37,266 Size determines on the one hand 969 00:49:37,266 --> 00:49:39,400 the height we will achieve, 970 00:49:39,400 --> 00:49:42,905 but on the other hand, size determines our lifespan 971 00:49:42,905 --> 00:49:45,611 because size determines how much energy 972 00:49:45,611 --> 00:49:48,793 we invest in maintaining our body in good shape. 973 00:49:50,470 --> 00:49:52,310 A very large animal and a very small animal 974 00:49:52,310 --> 00:49:53,780 live in completely different worlds, 975 00:49:53,780 --> 00:49:56,180 so they face completely different problems. 976 00:49:56,180 --> 00:49:57,190 Evolution has produced 977 00:49:57,190 --> 00:49:59,160 completely different solutions to these problems. 978 00:49:59,160 --> 00:50:00,740 And for scientists, it's really interesting 979 00:50:00,740 --> 00:50:02,380 to try and understand how things work 980 00:50:02,380 --> 00:50:04,320 at small scales and big scales. 981 00:50:04,320 --> 00:50:05,500 How big you are 982 00:50:05,500 --> 00:50:07,610 determines the scale of the world around you 983 00:50:07,610 --> 00:50:08,637 and how you interact with it. 984 00:50:08,637 --> 00:50:10,483 The smaller you become, 985 00:50:10,483 --> 00:50:13,118 the kinds of things that are dangerous to you change. 986 00:50:13,118 --> 00:50:16,210 But size is also a very mutable variable. 987 00:50:16,210 --> 00:50:18,270 It's flexible and mammals have found a way 988 00:50:18,270 --> 00:50:21,919 to live very successfully at all different sizes. 989 00:50:21,919 --> 00:50:24,690 I think size is important in the universe. 990 00:50:24,690 --> 00:50:25,920 It's a clockwork really. 991 00:50:25,920 --> 00:50:27,860 You have your clock and everything works perfectly, 992 00:50:27,860 --> 00:50:30,137 but if you change the size of one of the cogs, 993 00:50:30,137 --> 00:50:32,370 then it doesn't fit with the rest anymore 994 00:50:32,370 --> 00:50:34,120 and the whole system will collapse. 995 00:50:36,317 --> 00:50:39,613 Size isn't like a color or clothing. 996 00:50:40,905 --> 00:50:42,843 It's not arbitrary. 997 00:50:43,788 --> 00:50:46,823 It goes hand in hand with so many things. 998 00:50:48,290 --> 00:50:53,290 Gravity, intelligence, the evolution of life itself. 999 00:50:55,339 --> 00:51:00,339 Our size is who we are and what we always will be. 1000 00:51:00,969 --> 00:51:04,552 (intense orchestral music) 78577

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