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These are the user uploaded subtitles that are being translated: 1 00:00:00,000 --> 00:00:02,000 * 2 00:00:02,080 --> 00:00:05,800 Did you ever stop to wonder where your car came from? 3 00:00:07,600 --> 00:00:10,080 Where it really came from? 4 00:00:10,160 --> 00:00:13,000 Every component has been on a mind-blowing journey, 5 00:00:13,080 --> 00:00:15,560 through time, space... 6 00:00:16,800 --> 00:00:20,440 ..and the most violent cosmic events since the Big Bang. 7 00:00:21,880 --> 00:00:25,920 The history of your car is the history of the universe. 8 00:00:48,000 --> 00:00:49,640 How old is a car? 9 00:00:50,840 --> 00:00:53,200 My car is about five years old. 10 00:00:53,280 --> 00:00:55,840 My car was assembled in 2001. 11 00:00:55,920 --> 00:00:57,560 The car I drive is pretty old. 12 00:00:57,640 --> 00:00:59,800 It was manufactured in 1991, 13 00:01:00,000 --> 00:01:02,800 but that's just when the pieces and parts were assembled. 14 00:01:04,440 --> 00:01:07,880 The materials that make up the cars we drive today 15 00:01:07,960 --> 00:01:10,640 were created long before 1991. 16 00:01:12,600 --> 00:01:16,960 Your car began its life billions of years ago, 17 00:01:17,040 --> 00:01:19,000 billions of miles away in deep space. 18 00:01:21,040 --> 00:01:24,840 The things that make up cars, those atoms, most of them were forged 19 00:01:24,920 --> 00:01:26,880 well before our Earth was born. 20 00:01:29,120 --> 00:01:30,960 You think your car is a clunker? 21 00:01:32,160 --> 00:01:35,920 It's actually 13.8 billion years old. 22 00:01:38,520 --> 00:01:40,240 All right. Let's do it, sir. 23 00:01:42,800 --> 00:01:46,400 The best way to find out what a car is made out of 24 00:01:46,480 --> 00:01:48,040 is to tear one apart. 25 00:01:52,680 --> 00:01:57,120 Iron, plastics, oils and rubber are the first to be removed. 26 00:01:59,760 --> 00:02:01,320 In another half-hour or so, 27 00:02:01,400 --> 00:02:03,520 this baby's going to be completely stripped. 28 00:02:04,800 --> 00:02:06,320 I can't wait to see it. 29 00:02:08,400 --> 00:02:11,960 Then aluminium, silicon, copper 30 00:02:12,040 --> 00:02:14,880 and finally, precious metals like platinum and gold. 31 00:02:19,600 --> 00:02:23,040 Each of these materials is crucial for building a car... 32 00:02:27,040 --> 00:02:29,960 ..but in the earliest days of the universe, 33 00:02:30,040 --> 00:02:31,520 none of them existed. 34 00:02:40,120 --> 00:02:42,280 13.8 billion years ago, 35 00:02:42,360 --> 00:02:44,760 the universe was born in a monumental event... 36 00:02:45,960 --> 00:02:47,200 ..the Big Bang. 37 00:02:48,280 --> 00:02:51,240 The early universe was filled with nothing but energy. 38 00:02:52,600 --> 00:02:54,240 After the Big Bang, 39 00:02:54,320 --> 00:02:58,600 it was just a chaotic glob of stuff, nothing like what you see today. 40 00:02:59,920 --> 00:03:02,120 As the early universe cools, 41 00:03:02,200 --> 00:03:05,360 the energy gave way to unstable matter and antimatter. 42 00:03:06,600 --> 00:03:09,000 Then protons and neutrons, 43 00:03:09,080 --> 00:03:11,880 and finally, atoms. 44 00:03:13,000 --> 00:03:17,320 But not the iron, silicon or carbon atoms that we use in a car, 45 00:03:17,400 --> 00:03:21,520 the universe was almost entirely made up of hydrogen. 46 00:03:21,600 --> 00:03:24,840 Something had to happen to give us everything else 47 00:03:24,920 --> 00:03:28,640 and everything was actually made from hydrogen building-blocks. 48 00:03:32,040 --> 00:03:36,160 An atom of hydrogen is the simplest and lightest atom in the universe - 49 00:03:36,240 --> 00:03:40,120 just a single positively-charged proton bound to a single electron. 50 00:03:43,000 --> 00:03:47,200 The universe built up bigger atoms such as carbon and iron 51 00:03:47,280 --> 00:03:49,560 by joining hydrogen atoms together. 52 00:03:51,760 --> 00:03:54,200 Everything starts from simpler origins. 53 00:03:54,280 --> 00:03:57,560 An iron atom is actually lots and lots of simple hydrogen atoms 54 00:03:57,640 --> 00:03:59,000 that were stuck together. 55 00:04:00,480 --> 00:04:03,840 But hydrogen atoms don't naturally stick together. 56 00:04:05,560 --> 00:04:08,240 Protons are positively charged. 57 00:04:08,320 --> 00:04:09,960 So as you push them closer together, 58 00:04:10,040 --> 00:04:12,200 they're gonna resist coming closer together. 59 00:04:12,280 --> 00:04:13,840 They really don't want to hang out. 60 00:04:15,560 --> 00:04:17,480 This repulsion makes the early universe 61 00:04:17,560 --> 00:04:21,160 a maelstrom of hydrogen atoms swerving to avoid each other. 62 00:04:22,600 --> 00:04:24,560 But if you can get them to a point 63 00:04:24,640 --> 00:04:26,600 where you can shove them together enough, 64 00:04:26,680 --> 00:04:29,000 at some point, they're going to lock together. 65 00:04:37,680 --> 00:04:40,720 Pushing atoms together so strongly that they fuse 66 00:04:40,800 --> 00:04:42,360 is called nuclear fusion. 67 00:04:43,960 --> 00:04:47,080 It's the first step in turning a universe full of gas 68 00:04:47,160 --> 00:04:49,960 into one filled with the ingredients for planets, 69 00:04:50,040 --> 00:04:52,880 people and cars. 70 00:04:54,520 --> 00:04:57,680 Getting two atoms to fuse is child's play... 71 00:04:57,760 --> 00:05:00,520 at least it is if your name's Taylor Wilson. 72 00:05:02,840 --> 00:05:06,360 Taylor's been fusing atoms in his garage since he was 14. 73 00:05:10,760 --> 00:05:13,280 Yeah, the neighbours know about the radioactive stuff 74 00:05:13,360 --> 00:05:15,800 that's in the garage, and so does the government. 75 00:05:15,880 --> 00:05:17,880 It's all relatively low-level. 76 00:05:17,960 --> 00:05:19,320 (BEEPING) 77 00:05:19,400 --> 00:05:20,680 It's my watch going off. 78 00:05:20,760 --> 00:05:22,000 I think I'm the only person 79 00:05:22,080 --> 00:05:24,080 I've ever met with a Geiger-counter watch. 80 00:05:27,720 --> 00:05:30,640 The centrepiece of Taylor's nuclear man cave 81 00:05:30,720 --> 00:05:33,720 is a precision-engineered fusion reactor 82 00:05:33,800 --> 00:05:36,760 which he built when he was still in high school. 83 00:05:36,840 --> 00:05:38,720 OK, I'll let in some gas now. 84 00:05:38,800 --> 00:05:42,040 The first ingredient - hydrogen gas. 85 00:05:42,120 --> 00:05:44,120 And it will be flowed into the chamber 86 00:05:44,200 --> 00:05:46,640 through this very precise sapphire leak valve. 87 00:05:47,720 --> 00:05:50,600 The next ingredient - high-voltage electricity. 88 00:05:54,840 --> 00:05:55,840 Hm. 89 00:05:55,920 --> 00:05:57,920 Oh, I wonder what the problem is! 90 00:05:58,280 --> 00:06:01,280 You forgot to plug it in. The power supply is not plugged in. 91 00:06:01,360 --> 00:06:03,560 OK, let's try that again. That's embarrassing. 92 00:06:05,200 --> 00:06:07,560 We'll get power from the laundry room now. 93 00:06:13,080 --> 00:06:14,600 Taylor passes a high voltage 94 00:06:14,680 --> 00:06:18,160 through a small spherical cage that sits inside the reactor. 95 00:06:19,680 --> 00:06:21,400 The negatively-charged cage 96 00:06:21,480 --> 00:06:24,160 quickly pulls the hydrogen ions towards it. 97 00:06:25,520 --> 00:06:28,680 So it's taking all those ions and sucking them towards the centre. 98 00:06:28,760 --> 00:06:31,120 And as they fly in, they get confined, 99 00:06:31,200 --> 00:06:33,760 and hopefully they collide with each other and fuse. 100 00:06:34,960 --> 00:06:38,720 The temperature of the atoms inside the cage is now so great 101 00:06:38,800 --> 00:06:41,800 that hydrogen atoms are fusing together, 102 00:06:41,880 --> 00:06:47,880 creating heavier helium atoms and a burst of energy hotter than the surface of the sun. 103 00:06:47,960 --> 00:06:52,240 That little tiny blob of plasma inside those grid wires, 104 00:06:52,320 --> 00:06:54,520 that's kind of like a star in a jar. 105 00:07:01,640 --> 00:07:03,400 13 billion years ago, 106 00:07:03,480 --> 00:07:07,160 the universe used gravity instead of an electrical cage 107 00:07:07,240 --> 00:07:09,080 to fuse atoms together. 108 00:07:12,520 --> 00:07:14,000 Across the cosmos, 109 00:07:14,080 --> 00:07:17,960 vast clouds of hydrogen gas collapsed under their own gravity. 110 00:07:20,840 --> 00:07:24,760 Pressure and temperature built as more and more gas was sucked in. 111 00:07:26,960 --> 00:07:33,200 Eventually, fusion sparked deep in the core of these giant balls of gas, 112 00:07:33,320 --> 00:07:35,520 and the first stars started to manufacture 113 00:07:35,600 --> 00:07:38,720 many of the heavy elements that make up cars today. 114 00:07:39,960 --> 00:07:41,920 A star is basically a machine 115 00:07:42,000 --> 00:07:44,520 for turning lighter elements into heavier elements. 116 00:07:46,360 --> 00:07:50,160 Fusion took place inside the core of these first stars, 117 00:07:50,240 --> 00:07:53,720 fusing hydrogen atoms together to create helium. 118 00:07:53,800 --> 00:07:57,080 And when all the hydrogen in the core had been used up, 119 00:07:57,160 --> 00:07:59,480 the star finds new fuel to burn. 120 00:08:01,320 --> 00:08:04,480 After you burn hydrogen to form helium, 121 00:08:04,560 --> 00:08:07,760 the core of the star begins to collapse and get hotter. 122 00:08:07,840 --> 00:08:09,480 And there is enough energy then 123 00:08:09,560 --> 00:08:12,560 to fuse three helium nuclei into carbon... 124 00:08:14,480 --> 00:08:19,200 ..and then that fuses to form nitrogen, oxygen, silicon, iron. 125 00:08:20,480 --> 00:08:24,800 But this incredible production line of elements can't go on forever. 126 00:08:26,200 --> 00:08:29,840 The heavier atoms you ram together, the less energy you get out. 127 00:08:29,920 --> 00:08:31,800 So you turn hydrogen into helium, 128 00:08:31,880 --> 00:08:34,560 helium becomes carbon, nitrogen, oxygen. 129 00:08:34,640 --> 00:08:37,920 But every time, there's a bit less energy to be had, 130 00:08:38,000 --> 00:08:39,400 until you get to iron. 131 00:08:40,680 --> 00:08:42,960 The iron that is in your car 132 00:08:43,040 --> 00:08:47,480 is actually, essentially, a deadly poison when it comes to a star. 133 00:08:48,760 --> 00:08:53,200 It's robbing that star of the heat needed to keep itself up. 134 00:08:57,520 --> 00:09:00,760 So the star collapses, dies and explodes 135 00:09:00,840 --> 00:09:03,600 at the moment you create iron in the core. 136 00:09:03,680 --> 00:09:05,760 I mean, literally, the fraction of a second. 137 00:09:05,840 --> 00:09:11,160 I'm not kidding. That's how dramatic and weird the steel in your car is. 138 00:09:13,520 --> 00:09:16,640 The explosion, called a supernova, 139 00:09:16,720 --> 00:09:20,200 is one of the brightest and most violent events in the universe. 140 00:09:21,920 --> 00:09:23,920 It releases enough energy 141 00:09:24,000 --> 00:09:27,840 to dwarf what the sun puts out over its entire lifetime. 142 00:09:27,920 --> 00:09:30,120 And all of the elements that it has created 143 00:09:30,200 --> 00:09:32,480 are then dispersed out into space. 144 00:09:33,680 --> 00:09:38,200 The gassy remains of the explosion are called a supernova remnant, 145 00:09:38,280 --> 00:09:43,560 an expanding bubble of gas containing hydrogen that survived in the star's outer layers, 146 00:09:43,640 --> 00:09:49,320 mixed in with carbon, oxygen, silicon and iron from the star's core. 147 00:09:51,240 --> 00:09:56,520 This 13 billion-year-old stardust helped you drive to work last week. 148 00:09:57,800 --> 00:10:00,600 This was once in the core of a dying star. 149 00:10:00,680 --> 00:10:04,080 And who knows? Maybe some of the iron atoms in this brake disc 150 00:10:04,160 --> 00:10:07,320 were forged in the heart of the very first generation of stars 151 00:10:07,400 --> 00:10:08,840 that illuminated the universe. 152 00:10:09,960 --> 00:10:13,120 When you're pumping iron, you're pumping the universe. 153 00:10:20,000 --> 00:10:23,600 The first stars created the materials in a car's chassis, 154 00:10:23,680 --> 00:10:25,520 body, windshield and seats. 155 00:10:26,640 --> 00:10:29,680 But key components, like the copper for the car's electronics, 156 00:10:29,760 --> 00:10:31,200 are yet to be manufactured. 157 00:10:32,400 --> 00:10:35,000 To create this crucial metal, 158 00:10:35,080 --> 00:10:39,360 a new generation of stars must die an even stranger death. 159 00:10:42,480 --> 00:10:44,480 * 160 00:10:46,000 --> 00:10:48,000 * 161 00:10:53,320 --> 00:10:56,280 Picture the scene 13 billion years ago... 162 00:10:57,320 --> 00:11:02,280 ..as the universe's very first stars are coming to the end of their lives. 163 00:11:05,640 --> 00:11:08,160 The sky is filled with flashes 164 00:11:08,240 --> 00:11:11,280 as star after star violently explodes. 165 00:11:13,080 --> 00:11:16,680 These supernovas hurl a rich cocktail of elements into space... 166 00:11:17,880 --> 00:11:22,040 ..carbon, silicon, aluminium and iron, 167 00:11:22,120 --> 00:11:25,840 materials that will one day be used to build cars on Earth. 168 00:11:32,120 --> 00:11:33,960 But some even heavier elements 169 00:11:34,040 --> 00:11:35,960 needed to build a car are still missing. 170 00:11:37,240 --> 00:11:40,720 Elements like copper and gold, used in the car's wiring. 171 00:11:42,160 --> 00:11:45,640 So far, the universe hasn't created these heavy metals, 172 00:11:45,720 --> 00:11:47,840 but it's about to. 173 00:11:47,920 --> 00:11:49,480 In the case of copper, 174 00:11:49,560 --> 00:11:53,080 the secret to its formation is reincarnation. 175 00:11:53,160 --> 00:11:56,080 Copper is one metal that your car can't live without. 176 00:11:57,440 --> 00:12:00,440 It turns out, there's over a mile of copper in the average car. 177 00:12:00,520 --> 00:12:01,600 And the reason why 178 00:12:01,680 --> 00:12:05,920 is because copper is an excellent electrical conductor. 179 00:12:08,400 --> 00:12:11,600 Copper's also used to conduct heat in radiators. 180 00:12:15,160 --> 00:12:18,920 It stops bearings from failing when you need to go fast. 181 00:12:19,000 --> 00:12:20,720 And when you need to stop... 182 00:12:21,840 --> 00:12:24,880 ..copper provides the friction in your brake pads. 183 00:12:24,960 --> 00:12:29,320 But the story of how that copper came to exist and be on Earth, 184 00:12:29,400 --> 00:12:31,080 that's a truly remarkable story. 185 00:12:34,320 --> 00:12:35,960 Copper can't begin to form 186 00:12:36,040 --> 00:12:39,080 until the first generation of stars have died. 187 00:12:41,720 --> 00:12:43,840 The expanding supernova remnants 188 00:12:43,920 --> 00:12:46,040 crash into neighbouring clouds of gas... 189 00:12:47,280 --> 00:12:50,240 ..creating a shock wave of pressure, 190 00:12:50,320 --> 00:12:53,720 a perfect nursery for a new generation of stars. 191 00:12:59,800 --> 00:13:01,800 There are cycles to the universe. 192 00:13:01,880 --> 00:13:04,080 Stars form, they live out their lives. 193 00:13:04,160 --> 00:13:06,960 They die, they blow off winds and they explode, 194 00:13:07,040 --> 00:13:11,520 seeding their material into gas clouds which then form new stars 195 00:13:11,600 --> 00:13:15,120 with heavier elements in them, which will repeat the cycle again. 196 00:13:16,680 --> 00:13:18,560 So if you wanna think about it that way, 197 00:13:18,640 --> 00:13:20,880 the universe is the ultimate recycler. 198 00:13:24,040 --> 00:13:26,960 The gas that forms these second-generation stars 199 00:13:27,040 --> 00:13:30,160 is peppered with the carbon, aluminium and iron 200 00:13:30,240 --> 00:13:32,240 thrown out by the supernova. 201 00:13:33,360 --> 00:13:37,400 The biggest of these new stars burn extremely brightly, 202 00:13:37,480 --> 00:13:39,560 but only for a few million years... 203 00:13:40,840 --> 00:13:43,720 ..then they undergo an incredible metamorphosis. 204 00:13:48,960 --> 00:13:53,600 The star rapidly expands to 100 times its previous size... 205 00:13:55,640 --> 00:13:58,760 ..then it cools and turns a ghostly red. 206 00:14:00,360 --> 00:14:02,960 A second-generation star has transformed 207 00:14:03,040 --> 00:14:04,680 into a red supergiant. 208 00:14:06,800 --> 00:14:09,560 And in its diffuse outer layers, 209 00:14:09,640 --> 00:14:12,960 iron is slowly converted into copper... 210 00:14:14,600 --> 00:14:16,040 ..but not by fusion. 211 00:14:17,320 --> 00:14:20,440 That iron nucleus has 26 protons. 212 00:14:20,520 --> 00:14:22,520 That's a serious electric charge, 213 00:14:22,600 --> 00:14:25,680 so it's going to repel any protons we try to shoot in there. 214 00:14:28,480 --> 00:14:30,080 How do we get more protons in? 215 00:14:31,720 --> 00:14:35,280 The way we get those protons in there is we trick the nucleus. 216 00:14:35,360 --> 00:14:38,640 Instead of shooting in protons, we shoot in neutrons. 217 00:14:42,440 --> 00:14:44,840 Colliding atoms in the outer layers of a star 218 00:14:44,920 --> 00:14:47,280 sometimes spit out neutrons. 219 00:14:48,760 --> 00:14:52,280 Neutrons don't have a charge, so they're not repelled 220 00:14:52,360 --> 00:14:55,520 by the positively-charged protons in the iron stardust. 221 00:14:57,240 --> 00:15:00,880 These neutrons are able to stick to the iron atoms around them. 222 00:15:03,840 --> 00:15:07,080 An atom is a very tiny thing and makes a very small target. 223 00:15:07,160 --> 00:15:10,120 But there's a lot of particles flying around near a star, 224 00:15:10,200 --> 00:15:14,720 and if, by chance, a neutron can hit an atom, it can stick, 225 00:15:14,800 --> 00:15:17,720 and that will actually make the nucleus of the atom larger. 226 00:15:19,200 --> 00:15:21,840 Neutron by neutron can hit an atom 227 00:15:21,920 --> 00:15:25,120 and then that neutron can actually decay into a proton. 228 00:15:26,360 --> 00:15:30,280 The neutron spontaneously splits into an electron, which is ejected, 229 00:15:30,360 --> 00:15:32,480 and a proton, which is left behind. 230 00:15:33,520 --> 00:15:37,360 The process transforms iron into copper. 231 00:15:37,440 --> 00:15:41,400 Scientists call this magical conversion "beta decay". 232 00:15:41,480 --> 00:15:44,600 So you can build up heavy elements very slowly 233 00:15:44,680 --> 00:15:47,160 over the course of thousands or millions of years, 234 00:15:47,240 --> 00:15:48,680 just by capturing neutrons. 235 00:15:53,360 --> 00:15:57,520 Eventually, the core of the red supergiant runs out of fuel 236 00:15:57,600 --> 00:15:59,160 and the star explodes... 237 00:16:00,440 --> 00:16:03,680 ..blasting its copper-rich outer layer into space. 238 00:16:06,840 --> 00:16:10,600 Thanks to the life and death of two generations of stars... 239 00:16:11,720 --> 00:16:14,240 ..we can equip our car with copper wiring. 240 00:16:16,560 --> 00:16:19,320 But we're still short of some even heavier metals, 241 00:16:19,400 --> 00:16:21,480 such as lead for the battery, 242 00:16:21,560 --> 00:16:23,960 and gold for the electrical connectors. 243 00:16:25,720 --> 00:16:28,200 To make these truly massive atoms... 244 00:16:29,280 --> 00:16:33,040 ..the universe must create the most spectacular explosions 245 00:16:33,120 --> 00:16:34,640 since the Big Bang. 246 00:16:42,760 --> 00:16:46,120 To make a car, you need some seriously heavy metal. 247 00:16:47,680 --> 00:16:49,920 Metal like iridium, 248 00:16:50,000 --> 00:16:53,320 a supersized atom with 77 protons 249 00:16:53,400 --> 00:16:55,960 that's used to coat the tips of spark plugs. 250 00:16:59,080 --> 00:17:03,320 Heavier still is gold, with 79 protons. 251 00:17:04,400 --> 00:17:07,040 This shiny conductor resists corrosion, 252 00:17:07,120 --> 00:17:10,240 making it ideal for exposed electrical connections. 253 00:17:12,440 --> 00:17:16,400 These connectors here for this airbag assembly are gold, 254 00:17:16,480 --> 00:17:18,560 and so this thing can react really quickly 255 00:17:18,640 --> 00:17:20,680 if there's an accident and save your life. 256 00:17:24,760 --> 00:17:28,080 The heaviest atom found in a car is lead, 257 00:17:28,160 --> 00:17:30,000 with 82 protons. 258 00:17:32,000 --> 00:17:34,800 Only lead can deliver the short burst of high power 259 00:17:34,880 --> 00:17:38,200 needed to start an engine over and over again. 260 00:17:46,360 --> 00:17:48,360 But until very recently, 261 00:17:48,440 --> 00:17:51,880 how the universe made these oversized atoms 262 00:17:51,960 --> 00:17:53,360 was a complete mystery. 263 00:17:54,720 --> 00:17:57,320 You can't make gold atoms in a normal star. 264 00:17:58,800 --> 00:18:02,040 You can't make gold atoms in a massive star that's dying. 265 00:18:03,880 --> 00:18:07,080 In order to make atoms this big, with this many neutrons, 266 00:18:07,160 --> 00:18:09,320 you need a truly cataclysmic event. 267 00:18:13,160 --> 00:18:14,440 Just a few years ago, 268 00:18:14,520 --> 00:18:16,800 most scientists believed that supernovas 269 00:18:16,880 --> 00:18:19,440 were cataclysmic enough to do the job. 270 00:18:23,400 --> 00:18:26,160 But astronomer Edo Berger had doubts. 271 00:18:27,640 --> 00:18:30,800 If you open any one of these books and flip to the page 272 00:18:30,880 --> 00:18:32,640 that tells you where gold came from, 273 00:18:32,720 --> 00:18:35,480 it will tell you that gold came from supernova explosions. 274 00:18:36,600 --> 00:18:38,880 But nobody had directly observed supernovas 275 00:18:38,960 --> 00:18:41,640 producing elements like gold. 276 00:18:41,720 --> 00:18:44,200 And inside computer simulations, 277 00:18:44,280 --> 00:18:48,240 virtual supernovas lacked the energy to forge these oversized atoms. 278 00:18:49,320 --> 00:18:51,600 Clearly, something was wrong. 279 00:18:51,680 --> 00:18:54,640 But if supernovas weren't powerful enough, 280 00:18:54,720 --> 00:18:56,880 what in the universe was? 281 00:18:56,960 --> 00:18:59,400 To form heavy elements requires a lot of neutrons, 282 00:18:59,480 --> 00:19:03,400 and so another possible theory was that the heaviest elements 283 00:19:03,480 --> 00:19:06,880 were produced in the mergers of two neutron stars in a binary system. 284 00:19:11,320 --> 00:19:14,600 Neutron stars are some of the strangest objects in the universe. 285 00:19:15,680 --> 00:19:19,160 They're formed from the collapsed cores of giant stars. 286 00:19:20,560 --> 00:19:23,280 You're taking a couple of times the mass of the sun 287 00:19:23,360 --> 00:19:27,200 and squeezing it down into a ball that's only a few miles across. 288 00:19:27,280 --> 00:19:30,560 The electrons and the protons that are flitting around inside of that 289 00:19:30,640 --> 00:19:32,480 combine to form neutrons. 290 00:19:32,560 --> 00:19:37,960 And what you're left with is an extremely dense ball of neutrons 291 00:19:38,040 --> 00:19:39,960 about the size of a city. 292 00:19:42,360 --> 00:19:44,960 Neutron stars are extremely dense. 293 00:19:45,040 --> 00:19:48,480 If you take just a teaspoon of the neutron star material, 294 00:19:48,560 --> 00:19:50,600 it's actually a billion tonnes. 295 00:19:51,720 --> 00:19:54,240 If neighbouring stars die together, 296 00:19:54,320 --> 00:19:57,200 it's possible for the two neutron stars they leave behind 297 00:19:57,280 --> 00:19:59,560 to form a spinning binary pair. 298 00:20:00,880 --> 00:20:03,560 But the partnership is doomed. 299 00:20:03,640 --> 00:20:06,600 What you're left over with is two incredibly compact, 300 00:20:06,680 --> 00:20:09,040 dramatic objects spiralling around each other. 301 00:20:12,320 --> 00:20:17,480 Over time, they move in together, until finally, they can coalesce 302 00:20:17,560 --> 00:20:20,280 in the most violent explosion since the Big Bang. 303 00:20:25,320 --> 00:20:28,920 The explosion is called a neutron-star merger. 304 00:20:30,360 --> 00:20:33,840 The amount of energy in this explosion is crushing. 305 00:20:33,920 --> 00:20:36,000 There's almost no way to describe it. 306 00:20:36,080 --> 00:20:38,120 It's like taking all of the sun's energy 307 00:20:38,200 --> 00:20:40,760 that it will ever emit over its entire lifetime 308 00:20:40,840 --> 00:20:43,000 and releasing it in a single second. 309 00:20:48,440 --> 00:20:51,160 Berger suspected that this colossal explosion 310 00:20:51,240 --> 00:20:53,560 forged iridium, gold and lead... 311 00:20:54,640 --> 00:20:58,160 ..but to rewrite the textbooks, he needed hard evidence. 312 00:20:59,240 --> 00:21:01,800 It was difficult to convince the community 313 00:21:01,880 --> 00:21:04,040 that this was a potential channel 314 00:21:04,120 --> 00:21:05,960 for the production of heavy elements. 315 00:21:10,160 --> 00:21:13,720 The proof is to actually see this process happening in the universe. 316 00:21:17,080 --> 00:21:18,440 June 2013. 317 00:21:19,720 --> 00:21:23,520 NASA's Swift satellite spotted a short burst of gamma rays 318 00:21:23,600 --> 00:21:24,960 from a nearby galaxy... 319 00:21:26,360 --> 00:21:30,640 ..a sign that a neutron-star merger had just taken place. 320 00:21:30,720 --> 00:21:33,680 For Berger, it was the lucky break he'd been waiting for. 321 00:21:36,720 --> 00:21:40,000 As soon as we knew that there was a gamma-ray burst nearby, 322 00:21:40,080 --> 00:21:44,480 we knew that this was our one chance, for perhaps several years, 323 00:21:44,560 --> 00:21:49,440 to obtain the right kind of measurements to test the formation of heavy elements. 324 00:21:51,320 --> 00:21:53,840 Once Swift had identified the burst, 325 00:21:53,920 --> 00:21:57,760 the Hubble Space Telescope swung into action to capture images. 326 00:22:01,680 --> 00:22:04,080 We grabbed them right away and we just looked. 327 00:22:04,160 --> 00:22:07,200 We knew exactly where to look, at the centre of this red circle. 328 00:22:07,280 --> 00:22:10,320 And what we saw was this source right there in the middle 329 00:22:10,400 --> 00:22:13,560 that is the direct signature 330 00:22:13,640 --> 00:22:16,440 of the production of very heavy elements, including gold. 331 00:22:20,360 --> 00:22:22,520 Berger's theory was right, 332 00:22:22,600 --> 00:22:25,840 but the rate of production was far higher than he'd expected. 333 00:22:27,440 --> 00:22:28,800 Well, in that one event, 334 00:22:28,880 --> 00:22:32,280 the amount of gold that was produced was more than the mass of the Earth. 335 00:22:34,000 --> 00:22:35,360 If we can bring it all here, 336 00:22:35,440 --> 00:22:38,600 it would be worth quadrillions and quadrillions of dollars. 337 00:22:40,720 --> 00:22:43,360 The theory is still very new, 338 00:22:43,440 --> 00:22:46,760 but it's possible that ancient neutron-star mergers 339 00:22:46,840 --> 00:22:49,560 made all the heavy metals we see in the world today... 340 00:22:51,720 --> 00:22:55,800 ..including the last remaining ingredients for our car. 341 00:23:03,080 --> 00:23:06,080 But all these elements were floating free in space. 342 00:23:07,680 --> 00:23:12,240 They still have to be pulled together into one giant fabrication plant... 343 00:23:16,760 --> 00:23:18,000 ..the Earth. 344 00:23:21,440 --> 00:23:23,440 * 345 00:23:25,000 --> 00:23:27,000 * 346 00:23:34,480 --> 00:23:36,240 Before the Earth was born, 347 00:23:36,320 --> 00:23:39,960 all the materials that would one day go into making your car 348 00:23:40,040 --> 00:23:41,560 looked like this. 349 00:23:41,640 --> 00:23:45,840 A vast, swirling cloud of gas and stardust, 350 00:23:45,920 --> 00:23:48,640 the exploded remnants of ancient stars. 351 00:23:48,720 --> 00:23:50,880 The clouds between the stars of the galaxy 352 00:23:50,960 --> 00:23:53,400 are made of everything that the Earth, your body 353 00:23:53,480 --> 00:23:54,640 and your car is made of. 354 00:23:54,720 --> 00:23:56,880 There's everything that you need floating 355 00:23:56,960 --> 00:23:59,200 in gaseous form between the stars. 356 00:24:00,560 --> 00:24:02,520 Four-and-a-half billion years ago, 357 00:24:02,600 --> 00:24:05,240 this interstellar gas collapsed once more. 358 00:24:06,520 --> 00:24:10,000 This time to create a rather ordinary mid-sized star... 359 00:24:11,960 --> 00:24:13,040 ..our sun. 360 00:24:13,840 --> 00:24:17,560 Close to the young sun, all of the lighter stuff got blown away. 361 00:24:17,640 --> 00:24:20,640 What was left behind was the heavier, denser stuff. 362 00:24:23,360 --> 00:24:26,200 There was carbon, there was iron, there was gold, 363 00:24:26,280 --> 00:24:27,800 everything in-between. 364 00:24:29,880 --> 00:24:34,520 Over time, these free-floating elements began to coalesce. 365 00:24:34,600 --> 00:24:37,840 Dust became rock. 366 00:24:39,320 --> 00:24:43,280 Rocks joined to form larger objects called planetesimals. 367 00:24:44,880 --> 00:24:48,680 Finally, planetesimals joined to form the Earth. 368 00:24:52,520 --> 00:24:56,440 Our planet was born with all the ingredients needed to build a car... 369 00:24:57,600 --> 00:25:01,240 ..but these ingredients were about to go their separate ways. 370 00:25:03,400 --> 00:25:04,680 The Earth is a big planet 371 00:25:04,760 --> 00:25:07,080 and it's done something that not all planets do, 372 00:25:07,160 --> 00:25:08,920 it's differentiated, it melted. 373 00:25:11,480 --> 00:25:13,720 Copper and lead dissolved in sulphur 374 00:25:13,800 --> 00:25:16,760 and floated to the top of the molten Earth, 375 00:25:16,840 --> 00:25:19,760 making these metals easy to mine today. 376 00:25:22,480 --> 00:25:25,320 But precious metals like iridium and gold 377 00:25:25,400 --> 00:25:29,840 sunk to the Earth's core and most of the iron sunk with them. 378 00:25:30,920 --> 00:25:32,440 It's kind of a pain, actually. 379 00:25:32,520 --> 00:25:35,160 All the heavy elements that are super-useful, like iron, 380 00:25:35,240 --> 00:25:38,080 they've sunk to the middle of the Earth where we can't reach them 381 00:25:38,160 --> 00:25:40,560 and there's not a whole lot of it in the crust. 382 00:25:44,600 --> 00:25:47,960 3.8 billion years ago, the oceans formed 383 00:25:48,040 --> 00:25:50,840 and water dissolved the last remaining traces of iron 384 00:25:50,920 --> 00:25:52,400 from the Earth's surface. 385 00:25:55,440 --> 00:25:57,440 In fact, there was so much iron in the sea 386 00:25:57,520 --> 00:26:01,120 that the Earth would've been green, not blue like it is today. 387 00:26:02,800 --> 00:26:06,200 The Earth's crust seemed destined to be practically iron-free. 388 00:26:07,560 --> 00:26:10,120 Then along came the most unlikely saviour... 389 00:26:11,880 --> 00:26:13,360 ..green slime. 390 00:26:15,800 --> 00:26:18,400 I want to show you a couple of examples of rocks 391 00:26:18,480 --> 00:26:20,800 that we recently brought back from South Africa. 392 00:26:22,000 --> 00:26:24,240 Caltech geobiologist Woody Fischer 393 00:26:24,320 --> 00:26:27,320 traced the history of iron through the Earth's earliest rocks. 394 00:26:29,240 --> 00:26:32,240 This is an example of a rock that was deposited on the seafloor 395 00:26:32,320 --> 00:26:34,560 a little over two-and-a-half billion years ago, 396 00:26:34,640 --> 00:26:36,840 and there's not a lot of iron in this sample. 397 00:26:36,920 --> 00:26:41,040 Now, what's so interesting is you go to the same place on the Earth 398 00:26:41,120 --> 00:26:43,000 200 million years later, 399 00:26:43,080 --> 00:26:45,920 and what you find is that things have really changed. 400 00:26:46,000 --> 00:26:49,040 And you'll note this very rusty colour to it. 401 00:26:49,120 --> 00:26:51,080 This is from the presence of iron oxides, 402 00:26:51,160 --> 00:26:55,320 and in fact, the rock itself is incredibly heavy, very dense. 403 00:26:57,400 --> 00:27:02,200 Why did the Earth's geological record change so quickly and so profoundly? 404 00:27:03,720 --> 00:27:07,360 One clue is that the sudden appearance of iron-rich rocks 405 00:27:07,440 --> 00:27:10,720 coincides with the rise of the first simple plants. 406 00:27:13,720 --> 00:27:17,480 This is a microorganism called a cyanobacterium. 407 00:27:17,560 --> 00:27:20,480 Each of the individual cells that are present in that medium 408 00:27:20,560 --> 00:27:23,360 are green and they're conducting photosynthesis. 409 00:27:23,440 --> 00:27:28,160 This group of cyanobacteria is gathering energy from light, 410 00:27:28,240 --> 00:27:32,280 using that to split water, and in so doing, 411 00:27:32,360 --> 00:27:34,280 they produce copious amounts of oxygen. 412 00:27:37,240 --> 00:27:38,760 In the early oceans, 413 00:27:38,840 --> 00:27:43,040 this newly formed oxygen reacted with the dissolved iron, 414 00:27:43,120 --> 00:27:46,560 forming a heavy rust that settled on the ocean-floor. 415 00:27:48,360 --> 00:27:51,000 For the first time in Earth's history, there was oxygen, 416 00:27:51,080 --> 00:27:52,720 free oxygen, in the air. 417 00:27:52,800 --> 00:27:54,760 That combined with the iron 418 00:27:54,840 --> 00:27:57,600 and the iron, basically, sank to the bottom of the ocean. 419 00:27:59,560 --> 00:28:04,360 These ancient rusty deposits form the iron ore that we mine today. 420 00:28:09,040 --> 00:28:12,840 So in the process of making a car, mining the iron ore, 421 00:28:12,920 --> 00:28:15,320 life was an essential part of that first step. 422 00:28:17,080 --> 00:28:20,320 You have to wait until after these guys evolve 423 00:28:20,400 --> 00:28:23,840 in order to be able to concentrate the raw materials that you need. 424 00:28:33,520 --> 00:28:36,800 The life of early plants brought us iron, 425 00:28:36,880 --> 00:28:40,080 but their death was perhaps even more helpful, 426 00:28:40,160 --> 00:28:44,240 because without dead plants, most cars wouldn't run. 427 00:28:46,920 --> 00:28:49,960 So what's the final ingredient for getting a car to actually go? 428 00:28:51,160 --> 00:28:52,560 You need to add fuel, 429 00:28:52,640 --> 00:28:55,640 and we, right now, use hydrocarbon-based fuel. 430 00:28:55,720 --> 00:28:56,960 We use oil. 431 00:28:58,880 --> 00:29:02,120 Oil is actually the remnant of dead plant life 432 00:29:02,200 --> 00:29:03,680 from billions of years ago. 433 00:29:04,880 --> 00:29:07,800 It amazes me to think that as you're driving your car around, 434 00:29:07,880 --> 00:29:09,960 what you're actually running the car on 435 00:29:10,040 --> 00:29:11,840 is ancient dead life. 436 00:29:13,440 --> 00:29:15,720 These hydrocarbons are also processed 437 00:29:15,800 --> 00:29:19,920 to help make rubber and plastics for the tyres and interior trim. 438 00:29:27,760 --> 00:29:31,160 Now we have almost all the components needed to complete a car. 439 00:29:32,360 --> 00:29:36,640 All that remains is a spark to bring the engine to life... 440 00:29:38,640 --> 00:29:40,880 ..but to get that spark, 441 00:29:40,960 --> 00:29:43,480 the Earth must pay a catastrophic price. 442 00:29:46,800 --> 00:29:50,600 65 million years ago, the Earth's crust is missing 443 00:29:50,680 --> 00:29:53,800 one crucial group of super-tough metals. 444 00:29:58,840 --> 00:30:00,760 This is a spark plug. 445 00:30:00,840 --> 00:30:04,320 And the way it works is that 100,000 volts are put 446 00:30:04,400 --> 00:30:05,600 across this gap here... 447 00:30:06,880 --> 00:30:10,760 ..and that ignites gasoline vapour in the cylinder of your motor. 448 00:30:12,160 --> 00:30:15,200 This tip has to survive in very harsh conditions... 449 00:30:17,000 --> 00:30:21,520 ..so it must be made of a very, very sturdy, robust material, 450 00:30:21,600 --> 00:30:25,800 and the material in this spark plug is a metal known as iridium. 451 00:30:29,000 --> 00:30:30,520 Like gold and lead, 452 00:30:30,600 --> 00:30:35,080 iridium was created inside the biggest bang since the Big Bang - 453 00:30:35,160 --> 00:30:37,120 a neutron star merger. 454 00:30:39,680 --> 00:30:43,240 Although the Earth originally contained a large amount of iridium, 455 00:30:43,320 --> 00:30:47,280 it sank out of reach while the Earth was still molten, 456 00:30:47,360 --> 00:30:50,520 falling to the core under the influence of gravity. 457 00:30:53,320 --> 00:30:56,640 The iridium that we mine on the Earth's surface today 458 00:30:56,720 --> 00:30:58,200 came from somewhere else. 459 00:31:00,200 --> 00:31:04,560 This exposed rock face in Colorado reveals a clue - 460 00:31:04,640 --> 00:31:07,560 a mysterious layer in the Earth's geological record 461 00:31:07,640 --> 00:31:10,000 that wraps around the entire planet. 462 00:31:10,080 --> 00:31:12,240 There's something particularly interesting 463 00:31:12,320 --> 00:31:13,760 about this clay layer here. 464 00:31:13,840 --> 00:31:18,160 If you analyse the concentration of rare metals like iridium in this layer, 465 00:31:18,240 --> 00:31:21,320 you'll find that there's about 100 times as much iridium here 466 00:31:21,400 --> 00:31:24,160 as in the other rocks around us in the crust of the Earth. 467 00:31:24,240 --> 00:31:25,680 It's rather bizarre, actually, 468 00:31:25,760 --> 00:31:28,360 to find so much iridium concentrated in one place 469 00:31:28,440 --> 00:31:29,960 here in crustal rocks. 470 00:31:30,040 --> 00:31:31,880 And it turns out that the entire budget 471 00:31:31,960 --> 00:31:33,640 of the iridium in the Earth's crust 472 00:31:33,720 --> 00:31:35,560 is pretty much contained in this layer. 473 00:31:38,040 --> 00:31:41,960 When geologists discovered the iridium layer in the late '70s, 474 00:31:42,040 --> 00:31:44,440 it became one of the biggest mysteries in science. 475 00:31:46,040 --> 00:31:49,560 How could so much of this rare metal end up concentrated 476 00:31:49,640 --> 00:31:51,280 in such a thin layer? 477 00:31:56,320 --> 00:31:59,920 Astronomers had measured similar concentrations of iridium before... 478 00:32:01,440 --> 00:32:04,640 ..inside rocks that had come from the asteroid belt. 479 00:32:05,800 --> 00:32:09,400 Billions of years ago, planets were forming all over our solar system, 480 00:32:09,480 --> 00:32:11,840 but there was an area in-between Mars and Jupiter 481 00:32:11,920 --> 00:32:15,920 where the gravity of Jupiter pretty much pulled apart anything that tried to form. 482 00:32:16,000 --> 00:32:19,200 And what got left over were a bunch of large, rocky chunks 483 00:32:19,280 --> 00:32:21,520 that we call the asteroid belt. 484 00:32:21,600 --> 00:32:24,160 Now, some of the asteroid belt is made of rock. 485 00:32:25,480 --> 00:32:27,600 Other asteroids are richer in metals. 486 00:32:30,920 --> 00:32:32,360 From time to time, 487 00:32:32,440 --> 00:32:35,640 asteroids are thrown out of orbit by another asteroid, 488 00:32:35,720 --> 00:32:38,280 or by the long reach of Jupiter's gravity. 489 00:32:40,120 --> 00:32:43,320 Sometimes these asteroids smash into the Earth. 490 00:32:46,800 --> 00:32:48,080 Could the iridium layer 491 00:32:48,160 --> 00:32:52,880 be the scattered remains of a single giant, metal-rich asteroid impact? 492 00:32:59,280 --> 00:33:02,320 30 years ago, this idea sounded far-fetched. 493 00:33:03,440 --> 00:33:06,840 Only an asteroid the size of a city would've had enough power 494 00:33:06,920 --> 00:33:09,560 to blast debris around the entire planet. 495 00:33:11,000 --> 00:33:12,720 If you could imagine the magnitude, 496 00:33:12,800 --> 00:33:15,360 the enormity of the violence of an event like that. 497 00:33:15,440 --> 00:33:18,400 And to have inches of dusty debris 498 00:33:18,480 --> 00:33:21,320 come booming over the horizon and settling out of the sky 499 00:33:21,400 --> 00:33:24,560 and raining on top of you and burying you in this layer, 500 00:33:24,640 --> 00:33:27,600 that should make a pretty big crater someplace on the Earth. 501 00:33:29,680 --> 00:33:32,040 Although it sounded incredible, 502 00:33:32,120 --> 00:33:35,680 the asteroid hypothesis also solved a long-standing mystery. 503 00:33:37,680 --> 00:33:40,200 The dinosaurs were wiped out around the same time 504 00:33:40,280 --> 00:33:42,080 the iridium layer was laid down. 505 00:33:43,400 --> 00:33:45,720 Could the two events be linked? 506 00:33:47,000 --> 00:33:49,800 The puzzle was solved when an asteroid-impact crater 507 00:33:49,880 --> 00:33:52,240 was discovered down in the Yucatan. 508 00:33:52,320 --> 00:33:55,720 The crater age turned out to be exactly 65 million years old, 509 00:33:55,800 --> 00:33:57,840 the same age as this deposit. 510 00:33:57,920 --> 00:34:00,160 And the crater size turned out 511 00:34:00,240 --> 00:34:02,960 to be just the size of crater you would get 512 00:34:03,040 --> 00:34:06,040 from the size of an asteroid it would take to make this layer. 513 00:34:07,640 --> 00:34:09,360 So it turns out that in a lot of ways 514 00:34:09,440 --> 00:34:12,840 you can think of asteroids as sort of a cosmic iridium-delivery system 515 00:34:12,920 --> 00:34:14,840 for us here on the surface of the Earth. 516 00:34:14,920 --> 00:34:18,240 And it's not just iridium we have to thank asteroids for. 517 00:34:18,320 --> 00:34:19,960 There were probably several times 518 00:34:20,040 --> 00:34:23,320 in the history of our solar system where there was heavy bombardment, 519 00:34:23,400 --> 00:34:26,640 all kinds of asteroids and comets falling in toward the Earth. 520 00:34:26,720 --> 00:34:29,600 Well, the Earth had solidified to some degree by that time, 521 00:34:29,680 --> 00:34:31,960 so not everything sank down into the core. 522 00:34:32,040 --> 00:34:34,040 So some of the metals we find around us 523 00:34:34,120 --> 00:34:36,600 are products of this later era of bombardment. 524 00:34:40,400 --> 00:34:42,640 The Earth's history is a violent one. 525 00:34:42,720 --> 00:34:46,240 Over the course of time, we've been hit over and over and over again 526 00:34:46,320 --> 00:34:48,160 by asteroids of all sizes. 527 00:34:48,240 --> 00:34:50,440 Some of them have actually delivered 528 00:34:50,520 --> 00:34:53,440 quite a bit of heavy elements to the surface of the Earth. 529 00:34:56,120 --> 00:34:58,200 These asteroid-borne materials 530 00:34:58,280 --> 00:35:00,600 include most of the gold, platinum and nickel 531 00:35:00,680 --> 00:35:02,520 we use in cars today. 532 00:35:05,200 --> 00:35:09,280 Asteroid impacts will form little pockets of concentrations 533 00:35:09,360 --> 00:35:12,320 of some of those ore minerals and ore metals for us 534 00:35:12,400 --> 00:35:15,840 that we can then mine in greater abundance on the surface. 535 00:35:15,920 --> 00:35:19,360 In many cases, when you go to a mine to dig up these heavy elements, 536 00:35:19,440 --> 00:35:23,080 what you are doing is tapping into an asteroid impact. 537 00:35:27,480 --> 00:35:30,480 But these mines are relatively rare. 538 00:35:30,560 --> 00:35:33,000 As humanity continues to grow, 539 00:35:33,080 --> 00:35:35,920 our precious metals will be the first metals to run out. 540 00:35:37,520 --> 00:35:39,240 If we want to get more, 541 00:35:39,320 --> 00:35:42,520 the only option will be to mine the asteroid belt itself. 542 00:35:44,360 --> 00:35:46,360 I don't think we can keep making cars here 543 00:35:46,440 --> 00:35:48,160 on the surface of the Earth forever. 544 00:35:48,240 --> 00:35:52,040 And as population grows and our need for these minerals grows, 545 00:35:52,120 --> 00:35:54,120 at some point, you know, we're gonna... 546 00:35:54,200 --> 00:35:56,920 you're gonna mine the Earth as much as it can be mined 547 00:35:57,000 --> 00:35:59,560 and you have to start to look someplace else. 548 00:35:59,640 --> 00:36:00,800 And fortunately, 549 00:36:00,880 --> 00:36:03,440 there are mines in the sky out there by the billions, 550 00:36:03,520 --> 00:36:04,920 and they're called asteroids. 551 00:36:06,000 --> 00:36:10,400 A lot of asteroids have platinum, iron, nickel, gold in them. 552 00:36:10,480 --> 00:36:13,840 It's very expensive to go up there and grab them and tow them back, 553 00:36:13,920 --> 00:36:16,400 but just the raw materials in an asteroid 554 00:36:16,480 --> 00:36:18,720 could be worth hundreds of billions of dollars. 555 00:36:20,600 --> 00:36:23,040 NASA recently estimated the value 556 00:36:23,120 --> 00:36:25,920 of the precious metals and materials on the asteroid belt 557 00:36:26,000 --> 00:36:29,000 as being about $600 quintillion, 558 00:36:29,080 --> 00:36:32,880 or about $100 billion for every person alive on the Earth today. 559 00:36:32,960 --> 00:36:35,600 But I do not expect to be seeing any of that money myself. 560 00:36:36,720 --> 00:36:39,520 We'll have to wait for rocket technology to get cheaper 561 00:36:39,600 --> 00:36:42,480 before asteroid-mining becomes a viable proposition. 562 00:36:43,800 --> 00:36:47,000 Until then, we'll continue to rely on the asteroids 563 00:36:47,080 --> 00:36:48,640 that have hit the Earth. 564 00:36:52,040 --> 00:36:55,040 Metal-rich asteroids are the final piece of the puzzle. 565 00:36:56,840 --> 00:37:00,320 We can now reconstruct the journey of every atom of our car 566 00:37:00,400 --> 00:37:03,200 through time and space. 567 00:37:03,280 --> 00:37:08,440 From the moment of the Big Bang, through generations of stars 568 00:37:08,520 --> 00:37:12,160 to the birth of the Earth, and eventually, 569 00:37:12,240 --> 00:37:14,240 the showroom floor. 570 00:37:14,320 --> 00:37:17,680 Over the course of the multiple supernovae in our universe 571 00:37:17,760 --> 00:37:20,400 and the birth and death of stars, 572 00:37:20,480 --> 00:37:23,640 we were able to collect all of the materials needed 573 00:37:23,720 --> 00:37:25,320 to assemble these cars. 574 00:37:26,520 --> 00:37:27,880 That's pretty fantastic. 575 00:37:31,280 --> 00:37:34,040 I think we don't fully appreciate how complicated 576 00:37:34,120 --> 00:37:36,200 the elements that make up our car really are 577 00:37:36,280 --> 00:37:37,480 and how special they are. 578 00:37:37,560 --> 00:37:39,560 They really are star stuff. 579 00:37:49,400 --> 00:37:52,520 But not every car is like the one we've just pulled apart. 580 00:37:54,680 --> 00:37:57,880 These days, not every car runs on petrol. 581 00:37:59,680 --> 00:38:02,640 Electric vehicles require a magical element 582 00:38:02,720 --> 00:38:04,120 that's made in space... 583 00:38:05,200 --> 00:38:06,880 ..by cosmic ray guns. 584 00:38:09,200 --> 00:38:11,200 * 585 00:38:13,000 --> 00:38:15,000 * 586 00:38:19,520 --> 00:38:21,320 This car doesn't have a petrol tank. 587 00:38:22,640 --> 00:38:25,760 It's part of a new generation of electric vehicles. 588 00:38:27,640 --> 00:38:31,560 The key to these high-tech cars is their rechargeable batteries... 589 00:38:35,280 --> 00:38:39,080 ..a technology that relies on one of the Earth's rarest metals. 590 00:38:41,560 --> 00:38:44,680 This here is a battery pack from an electric car, 591 00:38:44,760 --> 00:38:48,640 and in today's electric cars, the metal of choice is lithium, 592 00:38:48,720 --> 00:38:52,960 and lithium has one of the most amazing stories in the universe. 593 00:38:55,880 --> 00:39:00,280 After hydrogen and helium, lithium is the lightest element, 594 00:39:00,360 --> 00:39:02,800 with just three protons and four neutrons. 595 00:39:04,000 --> 00:39:07,200 Its lightness makes it ideal for electric cars. 596 00:39:08,760 --> 00:39:10,960 If the battery weighs more than the car, 597 00:39:11,040 --> 00:39:14,160 then we are just wasting energy on moving the battery around. 598 00:39:14,240 --> 00:39:18,040 If we can build a light battery, for example, a lithium-ion battery, 599 00:39:18,120 --> 00:39:21,600 then we can provide the power without the penalty 600 00:39:21,680 --> 00:39:24,680 of having to carry those heavy batteries along with the car. 601 00:39:27,040 --> 00:39:28,400 Lithium is rapidly becoming 602 00:39:28,480 --> 00:39:31,520 one of the most sought-after metals on Earth, 603 00:39:31,600 --> 00:39:33,840 but it's also a cosmic curiosity. 604 00:39:36,600 --> 00:39:39,360 The Big Bang creates a trace of lithium, 605 00:39:39,440 --> 00:39:42,120 but as the first stars form, 606 00:39:42,200 --> 00:39:44,960 this lithium disappears. 607 00:39:45,040 --> 00:39:46,360 Unlike hydrogen and helium, 608 00:39:46,440 --> 00:39:48,920 which are fairly stable on an atomic scale, 609 00:39:49,000 --> 00:39:51,120 lithium is a little bit fragile. 610 00:39:51,200 --> 00:39:54,200 It can actually be broken apart into its components. 611 00:39:56,040 --> 00:39:58,400 As time goes by, these first stars 612 00:39:58,480 --> 00:40:01,400 manufacture a little lithium on their own, 613 00:40:01,480 --> 00:40:03,040 but it doesn't last long. 614 00:40:04,640 --> 00:40:06,880 It is so fragile that the instant it's made, 615 00:40:06,960 --> 00:40:10,440 it's destroyed once again by the conditions in the core of the star. 616 00:40:12,280 --> 00:40:13,640 The lithium we have on Earth 617 00:40:13,720 --> 00:40:17,040 isn't made in a star like iron, copper and iridium. 618 00:40:18,320 --> 00:40:21,200 Instead of fusing lighter elements together, 619 00:40:21,280 --> 00:40:24,480 lithium is created when larger atoms are blasted apart. 620 00:40:25,560 --> 00:40:27,840 The answer for where lithium comes from 621 00:40:27,920 --> 00:40:31,000 is an amazing thing, it's almost like a sci-fi answer. 622 00:40:31,080 --> 00:40:33,200 It kind of comes from ray guns from space. 623 00:40:39,800 --> 00:40:44,680 The ray guns are supernovas and their bullets are cosmic rays... 624 00:40:46,240 --> 00:40:48,960 ..high-velocity particles that streak through space 625 00:40:49,040 --> 00:40:50,680 at close to the speed of light. 626 00:40:51,800 --> 00:40:54,080 Cosmic rays are subatomic particles. 627 00:40:54,160 --> 00:40:58,240 They are atomic nuclei that are accelerated to high speed 628 00:40:58,320 --> 00:40:59,840 in a supernova explosion. 629 00:41:01,000 --> 00:41:03,200 If another atomic nucleus gets in the way, 630 00:41:03,280 --> 00:41:05,360 it can hit them and shatter them, 631 00:41:05,440 --> 00:41:09,040 and one of the pieces of shrapnel from this explosion is lithium. 632 00:41:19,120 --> 00:41:21,160 The process is a bit like going bowling, 633 00:41:21,240 --> 00:41:23,200 where the bowling ball is the cosmic ray 634 00:41:23,280 --> 00:41:26,400 and the pins together are some other atomic nucleus. 635 00:41:33,960 --> 00:41:36,680 When the bowling ball smashes into the pins, 636 00:41:36,760 --> 00:41:38,920 it sends them scattered in all directions... 637 00:41:43,280 --> 00:41:45,440 ..and one of those pins could be lithium. 638 00:41:57,880 --> 00:42:00,400 Cosmic rays are travelling throughout all of space, 639 00:42:00,480 --> 00:42:02,120 between galaxies and in galaxies. 640 00:42:02,200 --> 00:42:04,480 So the cosmic rays that are forming lithium 641 00:42:04,560 --> 00:42:06,360 by breaking other elements apart 642 00:42:06,440 --> 00:42:09,160 are literally doing it in the space between the stars. 643 00:42:10,600 --> 00:42:14,680 Almost all the lithium on Earth today was made this way, 644 00:42:14,760 --> 00:42:17,360 atom by atom in the vastness of space. 645 00:42:18,480 --> 00:42:20,560 And then swept up into the clouds of gas 646 00:42:20,640 --> 00:42:22,760 that formed our solar system. 647 00:42:29,800 --> 00:42:31,920 Oh, yeah, baby. 648 00:42:32,000 --> 00:42:36,040 For our cosmic car, this may look like the end of the line, 649 00:42:36,120 --> 00:42:39,680 but the production line for the universe keeps on rolling. 650 00:42:41,480 --> 00:42:42,840 This is pretty awesome. 651 00:42:42,920 --> 00:42:44,680 These atoms in this car here 652 00:42:44,760 --> 00:42:46,920 have been travelling across the cosmos. 653 00:42:47,000 --> 00:42:49,840 They came to us from, maybe, 13 billion years ago, 654 00:42:49,920 --> 00:42:52,680 a billion years after the formation of the universe. 655 00:42:52,760 --> 00:42:53,840 Now guess what? 656 00:42:53,920 --> 00:42:57,200 They were used and we're returning them back to where they came from. 657 00:42:58,280 --> 00:43:00,920 The atoms in our car will not be in our car forever. 658 00:43:01,000 --> 00:43:03,160 In fact, our car will probably be destroyed 659 00:43:03,240 --> 00:43:05,120 within a single human lifetime. 660 00:43:05,200 --> 00:43:06,520 Time to crush. 661 00:43:06,600 --> 00:43:08,800 It'll be recycled into other things on Earth, 662 00:43:08,880 --> 00:43:12,240 but eventually, even the atoms on Earth will be recycled 663 00:43:12,320 --> 00:43:13,880 with the rest of the cosmos. 664 00:43:18,520 --> 00:43:19,720 How cool was that? 665 00:43:21,440 --> 00:43:25,480 You could imagine my car gets destroyed with the Earth 666 00:43:25,560 --> 00:43:28,160 and eventually makes its way to another planet. 667 00:43:28,240 --> 00:43:32,000 It gets built into some other kind of transportation mode 668 00:43:32,080 --> 00:43:33,160 by an alien race. 669 00:43:33,240 --> 00:43:34,880 I mean, that's totally possible, 670 00:43:34,960 --> 00:43:36,960 and I think that's kind of a cool idea. 671 00:43:40,080 --> 00:43:42,960 From stars being born billions of years ago, 672 00:43:43,040 --> 00:43:46,520 to cosmic rays, to even the Big Bang itself. 673 00:43:46,600 --> 00:43:48,880 It's amazing to contemplate all of the things 674 00:43:48,960 --> 00:43:52,360 that had to come together in the universe for us to have cars. 675 00:43:52,440 --> 00:43:54,480 You really are driving around 676 00:43:54,560 --> 00:43:56,880 in the end product of something that started 677 00:43:56,960 --> 00:43:58,720 13.7 billion years ago. 678 00:43:58,800 --> 00:44:03,440 That "new car" smell, that's actually "old universe" smell, 679 00:44:03,520 --> 00:44:07,760 because that smell is traceable all the way back to the Big Bang. 680 00:44:07,960 --> 00:44:08,960 subtitles by Deluxe 681 00:44:09,800 --> 00:44:11,080 How do you like that? 682 00:44:11,880 --> 00:44:13,880 That guarantees the last word in the show. 57644

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