1 00:00:03,460 --> 00:00:05,220 The dream of becoming a citizen 2 00:00:05,260 --> 00:00:07,820 of the cosmos was born here 3 00:00:07,860 --> 00:00:11,820 more than two millennia ago, in the city of Alexandria 4 00:00:12,380 --> 00:00:13,740 named after and conceived 5 00:00:13,860 --> 00:00:17,540 by its dead conqueror, Alexander the Great. 6 00:00:18,220 --> 00:00:20,220 The Ptolemys, the Greek kings 7 00:00:20,300 --> 00:00:21,820 who inherited the Egyptian portion 8 00:00:21,900 --> 00:00:24,860 of Alexander's empire, built this library 9 00:00:24,940 --> 00:00:27,660 and its associated research institution. 10 00:00:28,380 --> 00:00:31,580 Rarely, if ever, before or since 11 00:00:31,740 --> 00:00:34,180 has there been a government that was willing to spend 12 00:00:34,260 --> 00:00:36,420 so much of its gross national product 13 00:00:36,460 --> 00:00:38,820 on the acquisition of knowledge. 14 00:00:39,420 --> 00:00:42,580 And it paid off. Big time. 15 00:00:42,740 --> 00:00:46,540 Every ship entering Alexandria's harbor was searched 16 00:00:46,580 --> 00:00:49,740 not for contraband, but for books that might be copied 17 00:00:49,820 --> 00:00:52,620 and stored here, in what was then 18 00:00:52,700 --> 00:00:55,260 the greatest library on Earth. 19 00:01:00,940 --> 00:01:04,340 Here, Eratosthenes, one of the chief librarians 20 00:01:04,420 --> 00:01:07,020 accurately calculated the size of the Earth 21 00:01:07,460 --> 00:01:09,300 and invented geography. 22 00:01:11,380 --> 00:01:12,820 Pythagoras. 23 00:01:14,580 --> 00:01:15,900 Hypatia. 24 00:01:17,460 --> 00:01:18,900 Euclid. 25 00:01:23,740 --> 00:01:27,060 Euclid set forth the precepts of geometry 26 00:01:27,180 --> 00:01:31,140 in a textbook that remained in use for 2,300 years. 27 00:01:37,980 --> 00:01:39,860 The Old Testament Bible comes down to us 28 00:01:40,020 --> 00:01:42,780 mainly from the Greek translations made here. 29 00:01:42,940 --> 00:01:45,060 The original manuscripts of the masterpieces 30 00:01:45,140 --> 00:01:47,220 of Greek comedy and drama 31 00:01:47,340 --> 00:01:50,420 poetry, science, engineering 32 00:01:50,820 --> 00:01:52,820 medicine and history 33 00:01:53,180 --> 00:01:55,060 the total work product of the awakening 34 00:01:55,140 --> 00:01:57,060 of ancient civilization 35 00:01:57,140 --> 00:01:58,540 were kept here. 36 00:01:59,300 --> 00:02:02,020 Estimates vary on the total number of scrolls. 37 00:02:02,180 --> 00:02:04,900 They range from 500,000 38 00:02:05,020 --> 00:02:06,660 to nearly a million. 39 00:02:07,700 --> 00:02:09,140 And all of it 40 00:02:09,820 --> 00:02:13,140 all of this is but a tiny fraction of the information 41 00:02:13,220 --> 00:02:17,180 that you have at your fingertips at this very moment. 42 00:02:19,860 --> 00:02:22,500 The collective knowledge of our species 43 00:02:22,580 --> 00:02:25,780 our own electronic Library of Alexandria 44 00:02:25,820 --> 00:02:28,820 may be accessed by anyone who has a device 45 00:02:28,900 --> 00:02:31,660 and the interest and the freedom to do so. 46 00:02:32,300 --> 00:02:34,500 This was not true in Alexandria 47 00:02:34,580 --> 00:02:37,140 where knowledge belonged to the elite. 48 00:02:37,340 --> 00:02:39,460 So, in the 4th century A.D. 49 00:02:39,580 --> 00:02:42,180 when the mob came to destroy the library 50 00:02:42,260 --> 00:02:45,100 and the genius of classical civilization 51 00:02:45,140 --> 00:02:48,220 there were not enough people to defend it. 52 00:02:48,580 --> 00:02:52,540 What will happen the next time the mob comes? 53 00:04:32,660 --> 00:04:34,820 We've come a long way together 54 00:04:34,860 --> 00:04:38,020 traveling from deep inside the heart of an atom 55 00:04:38,180 --> 00:04:40,460 clear out to the cosmic horizon 56 00:04:40,500 --> 00:04:44,060 and from the beginning of time to the distant future. 57 00:04:44,900 --> 00:04:47,820 I think we're ready to perform an experiment. 58 00:05:13,620 --> 00:05:16,780 It's not the kind of experiment that requires a laboratory. 59 00:05:17,100 --> 00:05:18,980 You can do it in your head. 60 00:05:19,060 --> 00:05:21,980 It's called a thought experiment. 61 00:05:23,340 --> 00:05:26,820 Pick a star, any one of the hundreds of billions 62 00:05:26,900 --> 00:05:29,420 of stars in our Milky Way Galaxy 63 00:05:29,500 --> 00:05:31,220 which is just one galaxy 64 00:05:31,340 --> 00:05:34,380 out of the hundred billion in the known universe. 65 00:05:34,740 --> 00:05:37,620 How about that star? Or that one? 66 00:05:38,100 --> 00:05:39,700 Okay, this one. 67 00:05:40,380 --> 00:05:43,660 It's orbited by dozens of planets and moons. 68 00:05:43,860 --> 00:05:45,340 Suppose on one of them 69 00:05:45,420 --> 00:05:47,900 there lives an intelligent species 70 00:05:47,980 --> 00:05:51,700 one the 10 million life-forms on that planet 71 00:05:52,180 --> 00:05:54,140 and there's a subgroup of that species 72 00:05:54,180 --> 00:05:56,940 who believe they have it all figured out. 73 00:05:57,020 --> 00:06:00,500 Their world is the center of the universe 74 00:06:00,580 --> 00:06:03,220 a universe made for them 75 00:06:03,380 --> 00:06:06,460 and that they know everything they need to know about it 76 00:06:06,820 --> 00:06:09,180 their knowledge is complete. 77 00:06:09,700 --> 00:06:12,700 How seriously would you take their claim? 78 00:06:18,020 --> 00:06:21,940 Our ancestors believed the universe was made for them. 79 00:06:22,020 --> 00:06:24,540 It was natural to assume that we were at the center. 80 00:06:24,660 --> 00:06:28,620 After all, it looks like the sun and stars all revolve around us. 81 00:06:29,100 --> 00:06:31,820 We still speak of the sun rising. 82 00:06:32,260 --> 00:06:33,940 The architecture of our language 83 00:06:34,020 --> 00:06:37,900 myths and dreams comes from that prescientific age. 84 00:06:38,540 --> 00:06:41,580 This is our planet as it was known then 85 00:06:41,820 --> 00:06:44,060 just before Columbus set sail. 86 00:06:44,580 --> 00:06:47,300 This first globe of the Earth was cutting-edge 87 00:06:47,420 --> 00:06:50,620 when Martin Behaim made it in 1492. 88 00:06:51,180 --> 00:06:52,340 Like everyone else 89 00:06:52,420 --> 00:06:53,980 he believed that the jigsaw puzzle 90 00:06:54,060 --> 00:06:56,580 of geography was complete. 91 00:06:56,620 --> 00:07:00,580 There were three continents. Europe, Africa and Asia 92 00:07:00,740 --> 00:07:03,420 and only the great world ocean in between. 93 00:07:03,700 --> 00:07:05,540 Behaim had no clue 94 00:07:05,580 --> 00:07:08,220 that North and South America even existed. 95 00:07:10,140 --> 00:07:12,860 It's easy to feel smug, right? 96 00:07:14,140 --> 00:07:17,220 Well, the fact is Martin Behaim 97 00:07:17,300 --> 00:07:20,500 knew infinitely more about his world, the Earth 98 00:07:20,540 --> 00:07:24,140 than we know about ours, the universe. 99 00:07:24,900 --> 00:07:28,820 A recent lesson in humility will serve to illustrate. 100 00:07:29,900 --> 00:07:32,460 In 1912, Victor Hess 101 00:07:32,540 --> 00:07:35,900 made a series of voyages into the sky above Austria 102 00:07:36,340 --> 00:07:39,980 and found the thing that scientists love best 103 00:07:40,980 --> 00:07:43,540 a mystery that defied understanding 104 00:07:43,700 --> 00:07:46,940 in terms of conventional scientific wisdom. 105 00:07:49,260 --> 00:07:51,820 And even today, a century later 106 00:07:51,860 --> 00:07:54,380 we are still searching for a complete explanation 107 00:07:54,420 --> 00:07:56,220 of what Hess found. 108 00:07:58,220 --> 00:08:01,180 A new kind of energy had recently been discovered 109 00:08:01,340 --> 00:08:02,980 radioactivity. 110 00:08:03,060 --> 00:08:06,140 It was given off by certain elements, like radium. 111 00:08:06,700 --> 00:08:08,820 But it was also found in the air 112 00:08:08,900 --> 00:08:11,660 even far away from radioactive rocks. 113 00:08:11,740 --> 00:08:13,660 It was everywhere. 114 00:08:15,100 --> 00:08:17,660 Where did this strange energy come from? 115 00:08:17,900 --> 00:08:19,260 No one knew. 116 00:08:19,340 --> 00:08:22,980 Hess suspected that it might come from above the Earth. 117 00:08:23,020 --> 00:08:24,460 To test his hypothesis 118 00:08:24,580 --> 00:08:28,460 he carried radiation detectors high into the sky. 119 00:08:28,860 --> 00:08:31,580 During a risky ascent in a hydrogen balloon 120 00:08:31,660 --> 00:08:35,100 he attained an altitude of more than three miles. 121 00:08:36,660 --> 00:08:40,420 When he reached the thin, cold, upper half of the atmosphere 122 00:08:50,860 --> 00:08:52,620 he found that the radiation 123 00:08:52,700 --> 00:08:55,540 was more than twice as strong as on the ground. 124 00:08:56,140 --> 00:08:58,940 The radiation must be coming from above. 125 00:08:59,100 --> 00:09:02,220 That's why its intensity was weaker on the ground 126 00:09:02,260 --> 00:09:05,260 the Earth's atmosphere was absorbing most of it. 127 00:09:06,180 --> 00:09:09,540 Some thought that the radiation might come from the Sun. 128 00:09:09,620 --> 00:09:12,860 To test that idea, Hess timed one of his ascents 129 00:09:12,900 --> 00:09:15,820 to coincide with a solar eclipse. 130 00:09:23,140 --> 00:09:26,540 But the eclipse had no effect on the radiation. 131 00:09:26,860 --> 00:09:29,100 Hess also found that the radiation 132 00:09:29,140 --> 00:09:32,100 was just as strong at night as in daylight. 133 00:09:32,300 --> 00:09:35,540 It was coming from above, but not from the sun. 134 00:09:36,140 --> 00:09:39,340 What Hess did not know was that the solar wind 135 00:09:39,460 --> 00:09:41,260 doesn't move that quickly. 136 00:09:41,620 --> 00:09:45,580 And so, for the wrong reason, he came to the right conclusion. 137 00:09:46,660 --> 00:09:49,740 Hess had discovered cosmic rays 138 00:09:49,900 --> 00:09:53,540 showers of subatomic particles that crisscross the universe 139 00:09:53,620 --> 00:09:55,580 at nearly the speed of light. 140 00:09:55,940 --> 00:09:58,740 Without the shielding effect of the Earth's atmosphere 141 00:09:58,820 --> 00:10:00,300 they would be lethal. 142 00:10:00,540 --> 00:10:03,180 Some cosmic rays can carry as much energy 143 00:10:03,260 --> 00:10:05,500 as a bullet fired from a rifle. 144 00:10:06,100 --> 00:10:09,540 It would take decades to trace those cosmic rays back 145 00:10:09,660 --> 00:10:13,020 to a death of unimaginable violence. 146 00:10:23,300 --> 00:10:25,620 The cosmic rays that Victor Hess detected 147 00:10:25,660 --> 00:10:27,420 in the skies above Austria 148 00:10:27,460 --> 00:10:29,860 posed a mystery to scientists. 149 00:10:31,660 --> 00:10:35,620 Radioactivity in minerals on Earth, like uranium ore 150 00:10:35,740 --> 00:10:38,220 comes from the disintegration of atoms. 151 00:10:38,380 --> 00:10:41,420 But cosmic rays were of a different nature. 152 00:10:42,180 --> 00:10:46,140 They were far more powerful than anything known in Hess's world. 153 00:10:46,900 --> 00:10:48,500 Scientists wondered for two decades 154 00:10:48,540 --> 00:10:51,220 what could possibly produce cosmic rays. 155 00:10:51,860 --> 00:10:55,780 Enter Fritz Zwicky, the most brilliant man 156 00:10:55,820 --> 00:10:57,620 you've never heard of. 157 00:10:58,700 --> 00:11:02,660 In 1933, he and a colleague discovered that some stars 158 00:11:02,940 --> 00:11:05,780 flare up to become as bright as their entire galaxy 159 00:11:05,860 --> 00:11:09,020 for a few weeks, before fading out again. 160 00:11:09,180 --> 00:11:13,060 Fritz Zwicky was the first person to understand what just happened. 161 00:11:13,180 --> 00:11:14,980 He correctly surmised 162 00:11:15,020 --> 00:11:17,940 that this is the way a massive star dies. 163 00:11:18,060 --> 00:11:20,820 It blows its guts out into space. 164 00:11:21,060 --> 00:11:24,340 He called this kind of stellar death a supernova 165 00:11:29,620 --> 00:11:31,980 and predicted that the dying star would shrink 166 00:11:32,020 --> 00:11:35,260 from about a million miles across to only 10. 167 00:11:35,980 --> 00:11:38,300 This corpse would be so dense 168 00:11:38,780 --> 00:11:40,260 that a single grain of it 169 00:11:40,300 --> 00:11:43,180 would weigh as much as the Great Pyramid in Egypt. 170 00:11:43,220 --> 00:11:44,900 It would consist almost entirely 171 00:11:44,940 --> 00:11:47,460 of subatomic particles called neutrons 172 00:11:47,620 --> 00:11:51,180 so he named these bizarre objects neutron stars. 173 00:11:51,260 --> 00:11:54,380 And 35 years after Zwicky predicted their existence 174 00:11:54,460 --> 00:11:56,500 astronomers began to find them. 175 00:11:56,660 --> 00:11:58,740 We call them pulsars when they spin rapidly 176 00:11:58,780 --> 00:12:01,620 and emit regular pulses of radio energy. 177 00:12:01,860 --> 00:12:04,340 Supernovas and neutron stars could account 178 00:12:04,380 --> 00:12:06,820 for a wide range of cosmic rays 179 00:12:07,020 --> 00:12:09,180 but not the most energetic ones. 180 00:12:09,540 --> 00:12:11,980 Nothing yet known to science can explain them 181 00:12:12,100 --> 00:12:13,900 and we're fine with that. 182 00:12:13,980 --> 00:12:15,820 It's one of the things I love about science. 183 00:12:15,940 --> 00:12:18,740 We don't have to pretend we have all the answers. 184 00:12:19,340 --> 00:12:21,420 Zwicky also came up with the idea that 185 00:12:21,460 --> 00:12:24,820 the gravity of a galaxy warps the fabric of space around it 186 00:12:24,940 --> 00:12:26,660 to act like a lens. 187 00:12:26,740 --> 00:12:28,660 This distorts and magnifies light 188 00:12:28,740 --> 00:12:31,660 from any other galaxy lying directly behind it. 189 00:12:31,860 --> 00:12:34,860 So, astronomers on Earth would see multiple images 190 00:12:34,900 --> 00:12:36,860 of that same distant galaxy 191 00:12:37,060 --> 00:12:40,100 deformed, as in a funhouse mirror. 192 00:12:40,780 --> 00:12:42,980 40 years after this prediction 193 00:12:43,580 --> 00:12:45,460 we started finding them, too. 194 00:12:47,460 --> 00:12:51,300 And Zwicky made yet another discovery back in the 1930s. 195 00:12:52,300 --> 00:12:54,900 While studying the Coma Cluster of galaxies 196 00:12:55,020 --> 00:12:58,380 he noticed something funny about the way they moved. 197 00:12:59,340 --> 00:13:02,380 The galaxies were going way too fast. 198 00:13:02,420 --> 00:13:05,740 So fast that they should've been flying apart from each other 199 00:13:05,780 --> 00:13:07,900 because all the stars in all those galaxies 200 00:13:08,020 --> 00:13:11,580 had far too little gravity to hold the cluster together. 201 00:13:12,180 --> 00:13:13,900 Zwicky thought that something else 202 00:13:13,940 --> 00:13:16,100 must be binding them to each other. 203 00:13:16,300 --> 00:13:18,900 That mysterious missing component 204 00:13:18,940 --> 00:13:20,660 would have to weigh something like 205 00:13:20,700 --> 00:13:23,620 50 times as much as the stars themselves. 206 00:13:23,780 --> 00:13:26,940 But no one paid much attention to this wild notion. 207 00:13:27,060 --> 00:13:30,100 Just another one of Zwicky's crazy ideas. 208 00:13:30,260 --> 00:13:32,940 In our solar system, the innermost planet, Mercury 209 00:13:33,460 --> 00:13:36,420 moves much faster than the outermost one, Neptune. 210 00:13:36,460 --> 00:13:38,100 And that makes sense, right? 211 00:13:38,140 --> 00:13:41,580 The harder you push or pull on something, the faster it goes. 212 00:13:41,780 --> 00:13:44,580 The sun's gravity weakens with increasing distance 213 00:13:44,700 --> 00:13:48,660 so the planets that are farther from the sun move more slowly. 214 00:13:49,340 --> 00:13:52,060 Everyone expected that the outermost stars 215 00:13:52,100 --> 00:13:55,060 in a galaxy would act the same way. 216 00:13:56,380 --> 00:13:58,980 Most of the stars are concentrated towards the center 217 00:13:59,140 --> 00:14:01,060 so, their collective gravity 218 00:14:01,220 --> 00:14:03,300 pulls on the other stars the same way 219 00:14:03,420 --> 00:14:05,540 the sun pulls on the planets. 220 00:14:05,780 --> 00:14:07,300 But in the 1970s 221 00:14:07,380 --> 00:14:10,700 when astronomer Vera Rubin studied the Andromeda Galaxy 222 00:14:10,820 --> 00:14:14,700 she discovered that the outer stars obeyed no such rule. 223 00:14:15,340 --> 00:14:17,780 Unlike the outer planets in the solar system 224 00:14:17,820 --> 00:14:21,460 the outer stars in the galaxy were all going at the same speed 225 00:14:21,540 --> 00:14:23,460 as the stars that were closer in 226 00:14:23,660 --> 00:14:26,580 and they were moving way faster than expected. 227 00:14:27,020 --> 00:14:28,900 "That's funny," Vera thought. 228 00:14:29,220 --> 00:14:32,500 "There must be something weird about the Andromeda Galaxy." 229 00:14:32,740 --> 00:14:35,060 So she looked at another galaxy. 230 00:14:35,260 --> 00:14:37,980 Same story. And another. 231 00:14:38,020 --> 00:14:41,980 Vera studied 60 galaxies and found that all of them 232 00:14:42,100 --> 00:14:44,300 seemed to be violating the Law of Gravity 233 00:14:44,380 --> 00:14:46,540 a core principle of physics. 234 00:14:47,260 --> 00:14:49,620 After some initial healthy skepticism 235 00:14:49,740 --> 00:14:52,020 her colleagues looked for themselves 236 00:14:52,100 --> 00:14:54,500 and found that Vera was right. 237 00:14:54,900 --> 00:14:58,140 It's not that Isaac Newton had gotten the Law of Gravity wrong 238 00:14:58,380 --> 00:15:00,100 Vera Rubin had discovered 239 00:15:00,140 --> 00:15:03,020 that the gravity of something massive and invisible 240 00:15:03,060 --> 00:15:05,580 was forcing the stars to go fast. 241 00:15:06,820 --> 00:15:09,460 And then, someone remembered 242 00:15:09,500 --> 00:15:11,620 crazy old Fritz Zwicky 243 00:15:13,460 --> 00:15:16,820 and the unknown source of gravity in the galaxy clusters 244 00:15:16,900 --> 00:15:19,180 that he called dark matter 245 00:15:19,220 --> 00:15:21,340 back in 1933. 246 00:15:27,180 --> 00:15:30,020 Vera Rubin had verified the existence of a new 247 00:15:30,060 --> 00:15:31,980 much larger cosmos. 248 00:15:32,100 --> 00:15:34,540 And just like the one we thought we knew 249 00:15:34,580 --> 00:15:36,660 it was filled with mystery. 250 00:15:37,780 --> 00:15:40,540 Dark matter is completely unobservable 251 00:15:40,580 --> 00:15:42,540 except for its gravitational effect 252 00:15:42,620 --> 00:15:45,940 which makes visible stars and galaxies move faster. 253 00:15:46,860 --> 00:15:49,980 Its nature is another deep mystery. 254 00:15:50,300 --> 00:15:53,540 Rubin had provided the evidence for an invisible universe 255 00:15:53,580 --> 00:15:57,500 nearly 10 times more massive than the one we thought we knew. 256 00:15:58,140 --> 00:16:01,220 It was as if we had been standing on the seashore at night 257 00:16:01,300 --> 00:16:04,260 mistakenly believing that the froth on the waves 258 00:16:04,340 --> 00:16:06,700 was all there was to the ocean. 259 00:16:06,860 --> 00:16:10,300 Vera Rubin looked at the stars and realized 260 00:16:10,460 --> 00:16:13,460 they were merely the foam on the waves 261 00:16:13,740 --> 00:16:17,620 and that the greatest part of the ocean remained unknown. 262 00:16:17,900 --> 00:16:21,300 But wait. It gets crazier. 263 00:16:22,500 --> 00:16:24,300 Our Milky Way galaxy 264 00:16:24,340 --> 00:16:26,780 a few hundred billion stars 265 00:16:26,820 --> 00:16:29,020 plus the clouds of gas and dust 266 00:16:29,300 --> 00:16:31,940 the stuff of once and future stars 267 00:16:31,980 --> 00:16:34,940 and about a hundred billion other galaxies 268 00:16:35,140 --> 00:16:38,820 all of that, including those uncounted billions 269 00:16:38,860 --> 00:16:42,740 of trillions of planets, moons, and comets 270 00:16:43,260 --> 00:16:45,740 amounts to only 5% 271 00:16:45,780 --> 00:16:47,780 of what is actually there. 272 00:16:47,860 --> 00:16:51,700 Because there's a bigger unsolved mystery than dark matter 273 00:16:52,100 --> 00:16:55,580 dark energy, which makes up even more of the cosmos 274 00:16:55,660 --> 00:16:57,620 and drives its expansion. 275 00:16:58,060 --> 00:17:01,620 And it was Fritz Zwicky's supernovas that lit the way 276 00:17:01,700 --> 00:17:04,460 to the revelation of its existence. 277 00:17:06,740 --> 00:17:08,020 In one scenario 278 00:17:08,060 --> 00:17:11,260 a star consumes all of its nuclear fuel 279 00:17:14,660 --> 00:17:18,620 then cools, and suddenly collapses under its own gravity. 280 00:17:18,820 --> 00:17:22,460 The star rebounds in a massive explosion 281 00:17:22,740 --> 00:17:26,700 leaving behind a neutron star or a black hole. 282 00:17:28,220 --> 00:17:30,260 Since the mass of the original star 283 00:17:30,340 --> 00:17:32,540 can fall within a wide range 284 00:17:32,660 --> 00:17:34,460 its peak brightness as a supernova 285 00:17:34,580 --> 00:17:36,180 can also vary widely. 286 00:17:36,340 --> 00:17:38,700 So, you can't tell how far away it is 287 00:17:38,820 --> 00:17:40,660 just from how bright it looks. 288 00:17:40,740 --> 00:17:44,180 A relatively nearby supernova might appear just as bright 289 00:17:44,300 --> 00:17:47,220 as one that was more powerful, but farther away. 290 00:17:48,020 --> 00:17:50,060 But there's another kind of supernova 291 00:17:50,180 --> 00:17:52,540 that comes in only one strength. 292 00:17:52,740 --> 00:17:55,860 It marks the violent grand finale of a tango 293 00:17:55,980 --> 00:17:59,660 danced by a giant star and a dwarf. 294 00:18:01,140 --> 00:18:04,020 As the two stars orbit closely around each other 295 00:18:04,180 --> 00:18:07,860 the giant sheds its outer layers of gas onto the dwarf. 296 00:18:09,100 --> 00:18:12,260 When the added weight becomes too much for it to bear 297 00:18:12,580 --> 00:18:14,020 the dwarf detonates 298 00:18:14,060 --> 00:18:16,940 like a stupendous thermonuclear bomb. 299 00:18:18,460 --> 00:18:21,420 For a few weeks, the brilliance of such a supernova 300 00:18:21,460 --> 00:18:25,420 rivals the combined light of all the stars in its galaxy. 301 00:18:25,860 --> 00:18:29,820 This kind of supernova always has the same maximum power output 302 00:18:30,100 --> 00:18:33,340 about five billion times brighter than our sun. 303 00:18:34,020 --> 00:18:37,980 With big telescopes, we can see them in galaxies very far away 304 00:18:38,100 --> 00:18:41,420 out toward the edge of the observable universe. 305 00:18:50,220 --> 00:18:53,380 Because all such supernovas have the same wattage 306 00:18:53,540 --> 00:18:55,980 they're ideal tools for measuring distances 307 00:18:56,020 --> 00:18:58,500 to the farthest reaches of the universe. 308 00:18:58,540 --> 00:19:01,580 We call them standard candles. 309 00:19:05,940 --> 00:19:09,100 In 1929, Edwin Hubble discovered 310 00:19:09,140 --> 00:19:11,340 that the universe is expanding. 311 00:19:11,740 --> 00:19:15,020 The distant galaxies are drifting away from one another. 312 00:19:15,460 --> 00:19:17,340 Later, we learned that the expansion began 313 00:19:17,420 --> 00:19:19,660 some 14 billion years ago 314 00:19:19,700 --> 00:19:22,500 with the explosive birth of the universe 315 00:19:22,540 --> 00:19:24,300 the big bang. 316 00:19:26,820 --> 00:19:28,620 Everybody assumed that the rate of expansion 317 00:19:28,700 --> 00:19:31,380 would be slowing down due to the mutual pull of gravity 318 00:19:31,460 --> 00:19:33,820 between all the parts of the universe. 319 00:19:33,980 --> 00:19:35,500 If there is enough dark matter 320 00:19:35,660 --> 00:19:39,060 its gravity would eventually bring the expansion to a stop 321 00:19:39,180 --> 00:19:42,100 and the universe would then fall back on itself. 322 00:19:42,420 --> 00:19:45,180 In that case, everything would eventually collapse 323 00:19:45,260 --> 00:19:47,060 in a big crunch. 324 00:19:47,100 --> 00:19:48,060 On the other hand 325 00:19:48,140 --> 00:19:50,300 if the universe had less dark matter 326 00:19:50,380 --> 00:19:52,500 the expansion would continue forever 327 00:19:52,740 --> 00:19:54,940 just getting slower and slower. 328 00:19:55,620 --> 00:19:57,620 Two competing teams of astronomers 329 00:19:57,780 --> 00:20:00,860 were observing those supernovas in distant galaxies. 330 00:20:00,980 --> 00:20:04,940 It turned out to be another one of those "that's funny" moments. 331 00:20:05,540 --> 00:20:06,660 In 1998 332 00:20:06,700 --> 00:20:09,980 both teams independently came to the same conclusion. 333 00:20:10,060 --> 00:20:12,340 The expansion isn't slowing down at all 334 00:20:12,420 --> 00:20:13,940 it's speeding up. 335 00:20:14,460 --> 00:20:18,100 This means the universe will continue to expand forever. 336 00:20:18,620 --> 00:20:21,660 There seems to be a mysterious force in the universe 337 00:20:21,980 --> 00:20:24,860 one that overwhelms gravity on the grandest scale 338 00:20:24,940 --> 00:20:27,140 to push the cosmos apart. 339 00:20:27,700 --> 00:20:29,060 Most of the energy of the universe 340 00:20:29,220 --> 00:20:31,540 is bound up in this unknown force. 341 00:20:31,620 --> 00:20:34,020 We call it dark energy. 342 00:20:34,300 --> 00:20:36,940 But that name, like dark matter 343 00:20:37,140 --> 00:20:39,980 is merely a code word for our ignorance. 344 00:20:40,620 --> 00:20:42,940 It's okay not to know all the answers. 345 00:20:43,020 --> 00:20:44,540 It's better to admit our ignorance 346 00:20:44,660 --> 00:20:47,020 than to believe answers that might be wrong. 347 00:20:47,420 --> 00:20:49,220 Pretending to know everything 348 00:20:49,540 --> 00:20:52,780 closes the door to finding out what's really there. 349 00:20:54,020 --> 00:20:56,500 Tonight, our ships sail 350 00:20:56,580 --> 00:20:59,340 into even more exotic waters. 351 00:20:59,660 --> 00:21:01,220 Come with me. 352 00:21:08,260 --> 00:21:09,660 Only two of our ships 353 00:21:09,740 --> 00:21:12,060 have ventured into the great dark ocean 354 00:21:12,140 --> 00:21:13,780 of interstellar space. 355 00:21:14,300 --> 00:21:17,340 The longest odyssey in all of history 356 00:21:17,780 --> 00:21:20,780 was launched back in 1977 357 00:21:21,340 --> 00:21:24,460 NASA's Voyager I and II. 358 00:21:25,780 --> 00:21:29,740 The Voyagers move about 40,000 miles an hour. 359 00:21:30,300 --> 00:21:32,540 They gave us our first close-up look 360 00:21:32,580 --> 00:21:34,740 at Jupiter's Great Red Spot 361 00:21:34,780 --> 00:21:38,180 a hurricane three times the size of Earth 362 00:21:38,260 --> 00:21:41,820 and one that's been raging since at least 1644 363 00:21:41,900 --> 00:21:43,460 when it was first observed. 364 00:21:43,580 --> 00:21:44,700 For all we know 365 00:21:44,780 --> 00:21:47,220 it could be thousands of years old. 366 00:21:47,620 --> 00:21:50,820 The Voyagers discovered the first active volcano 367 00:21:50,940 --> 00:21:52,220 on another world 368 00:21:52,420 --> 00:21:54,580 on Jupiter's moon Io 369 00:21:56,340 --> 00:22:00,300 and an ocean beneath the icy surface of the moon Europa 370 00:22:03,860 --> 00:22:07,820 with at least twice as much water as we have here on Earth. 371 00:22:10,460 --> 00:22:14,140 The Voyagers dared to fly across Saturn's rings 372 00:22:14,220 --> 00:22:17,740 and revealed that they were made of hundreds of thin bands 373 00:22:17,820 --> 00:22:19,940 of orbiting snowballs. 374 00:22:23,300 --> 00:22:25,620 On Saturn's giant moon Titan 375 00:22:25,740 --> 00:22:27,740 Voyager detected an atmosphere 376 00:22:27,780 --> 00:22:30,180 four times denser than Earth's. 377 00:22:30,300 --> 00:22:34,260 That hinted at the existence of hydrocarbon seas on Titan 378 00:22:34,820 --> 00:22:37,100 which we later confirmed. 379 00:22:38,660 --> 00:22:41,140 Voyager II gave us our first portrait 380 00:22:41,220 --> 00:22:44,300 of the outermost planet, Neptune 381 00:22:45,220 --> 00:22:48,900 where the winds roar at 1000 miles per hour 382 00:22:50,260 --> 00:22:51,940 and its moon Triton 383 00:22:52,140 --> 00:22:55,180 where geysers of boiling nitrogen 384 00:22:55,340 --> 00:22:57,940 shoot five miles high. 385 00:23:01,060 --> 00:23:04,140 Voyager successfully completed its mission of discovery 386 00:23:04,260 --> 00:23:05,500 to the outer planets 387 00:23:05,620 --> 00:23:09,620 but its odyssey into the darkness was just beginning. 388 00:23:11,900 --> 00:23:13,780 35 years after its launch 389 00:23:13,900 --> 00:23:16,500 Voyager I became the first of our spacecraft 390 00:23:16,740 --> 00:23:19,540 to enter an uncharted realm. 391 00:23:20,260 --> 00:23:22,580 The Sun is constantly shooting out streams 392 00:23:22,660 --> 00:23:24,900 of charged particles in all directions 393 00:23:25,020 --> 00:23:27,460 moving at a million miles an hour. 394 00:23:27,540 --> 00:23:29,300 This solar wind 395 00:23:29,340 --> 00:23:31,940 blows a vast magnetic bubble 396 00:23:32,140 --> 00:23:36,100 our heliosphere, that extends beyond the outer planets. 397 00:23:36,420 --> 00:23:40,380 It pushes out against the thin gas of interstellar space. 398 00:23:40,860 --> 00:23:43,500 There's a border where one ends 399 00:23:43,540 --> 00:23:45,380 and the other begins. 400 00:23:45,500 --> 00:23:47,700 Voyager I reported back to Earth 401 00:23:47,780 --> 00:23:49,860 that its detectors were being pummeled 402 00:23:49,980 --> 00:23:52,420 by more and more cosmic rays. 403 00:23:52,580 --> 00:23:56,500 Until then, we didn't know where the interstellar ocean began. 404 00:23:56,580 --> 00:23:59,580 Voyager I pressed on past a boundary 405 00:23:59,660 --> 00:24:01,900 we had never crossed before. 406 00:24:01,980 --> 00:24:05,940 The heliosphere shields us from most of the deadly cosmic rays. 407 00:24:06,020 --> 00:24:07,940 When stormy solar winds blow 408 00:24:08,060 --> 00:24:10,220 this zone of protection grows 409 00:24:10,300 --> 00:24:12,460 and calm solar weather, it shrinks. 410 00:24:12,540 --> 00:24:16,100 When a star goes supernova in our galactic neighborhood 411 00:24:17,620 --> 00:24:19,660 the debris from the exploded star 412 00:24:20,300 --> 00:24:23,300 pushes the heliosphere back towards the sun. 413 00:24:23,460 --> 00:24:26,700 If it's strong enough to push it all the way back to Earth's orbit 414 00:24:26,980 --> 00:24:30,940 our planet gets a radioactive bath of supernova debris. 415 00:24:32,020 --> 00:24:34,740 Luckily, this doesn't happen very often. 416 00:24:34,900 --> 00:24:37,900 The last one was perhaps two million years ago. 417 00:24:38,260 --> 00:24:39,940 A neighboring star explodes 418 00:24:40,060 --> 00:24:42,740 a million years before there's even such a thing 419 00:24:43,180 --> 00:24:45,060 as the human species. 420 00:24:45,500 --> 00:24:47,420 How can we possibly know this? 421 00:24:47,740 --> 00:24:49,180 Because the dying star 422 00:24:49,340 --> 00:24:52,820 left its traces miles below the surface of the ocean. 423 00:24:53,300 --> 00:24:55,180 Manganese nodules 424 00:24:55,380 --> 00:24:57,340 small rocks like this one 425 00:24:57,580 --> 00:25:00,780 are scattered over much of the deep sea floor. 426 00:25:02,300 --> 00:25:04,580 They grow very slowly. 427 00:25:04,740 --> 00:25:06,740 I'm talking a millimeter 428 00:25:07,260 --> 00:25:09,180 in a million years 429 00:25:10,020 --> 00:25:11,780 layer upon layer. 430 00:25:13,540 --> 00:25:16,740 These nodules grow in partnership with bacteria 431 00:25:16,820 --> 00:25:20,300 by taking up minerals dissolved in the seawater. 432 00:25:21,460 --> 00:25:24,900 A supernova produces a radioactive form of iron 433 00:25:25,380 --> 00:25:28,940 unlike anything made by natural processes on Earth. 434 00:25:29,260 --> 00:25:31,820 Researchers found telltale traces of this iron 435 00:25:32,100 --> 00:25:35,860 in a thin layer below the surface of the manganese nodules. 436 00:25:36,180 --> 00:25:38,780 They used the known rate of growth of the nodules 437 00:25:38,980 --> 00:25:40,300 to date that layer 438 00:25:40,380 --> 00:25:44,340 and to connect it to the fate of a star that perished eons ago. 439 00:25:47,140 --> 00:25:50,060 The difference between seeing nothing but a pebble 440 00:25:50,380 --> 00:25:54,340 and reading the history of the cosmos inscribed inside it 441 00:25:54,740 --> 00:25:56,420 is science. 442 00:25:59,020 --> 00:26:02,900 The interstellar ocean is dark and deep. 443 00:26:03,500 --> 00:26:07,100 Out here, the sun is just the brightest star in the sky. 444 00:26:07,180 --> 00:26:08,140 Yet the Voyagers 445 00:26:08,340 --> 00:26:10,020 maintain their regular communications 446 00:26:10,100 --> 00:26:12,580 with NASA's Jet Propulsion Laboratory 447 00:26:12,660 --> 00:26:14,740 talking back and forth across the light-hours 448 00:26:14,860 --> 00:26:18,420 that separate these ships from their home port. 449 00:26:18,700 --> 00:26:21,860 No other objects touched by human hands 450 00:26:21,980 --> 00:26:24,700 have ever ventured this far from home. 451 00:26:30,900 --> 00:26:34,220 Even after they lose their ability to respond to our command 452 00:26:34,420 --> 00:26:35,900 the last and, by far 453 00:26:35,980 --> 00:26:39,340 the longest phase of the Voyager mission will begin. 454 00:26:46,580 --> 00:26:49,980 Back in 1979, when both Voyagers rounded Jupiter 455 00:26:50,100 --> 00:26:52,620 its massive gravity acted as a slingshot 456 00:26:52,700 --> 00:26:54,340 flinging them out of the solar system 457 00:26:54,420 --> 00:26:56,900 to travel among the stars of our galaxy 458 00:26:57,180 --> 00:26:58,860 for a billion years. 459 00:26:59,060 --> 00:27:00,500 Carl Sagan recognized 460 00:27:00,580 --> 00:27:03,220 that the Voyager mission offered two free tickets 461 00:27:03,300 --> 00:27:06,140 to something approaching eternity. 462 00:27:06,500 --> 00:27:09,220 He assembled a small team to create a message 463 00:27:09,340 --> 00:27:12,140 to any civilization that might, one day 464 00:27:12,380 --> 00:27:14,900 encounter the derelict spacecraft. 465 00:27:18,620 --> 00:27:20,420 26 centuries ago 466 00:27:20,500 --> 00:27:23,420 the Assyrian king Esarhaddon wrote 467 00:27:23,540 --> 00:27:26,020 "I had monuments made of bronze" 468 00:27:26,100 --> 00:27:28,500 "and inscriptions of baked clay." 469 00:27:28,700 --> 00:27:32,300 "I left them in the foundations for future times." 470 00:27:32,860 --> 00:27:36,820 These hieroglyphics continue that ancient tradition. 471 00:27:36,940 --> 00:27:38,500 They are inscribed on the cover 472 00:27:38,580 --> 00:27:40,260 of a message designed to be read 473 00:27:40,340 --> 00:27:44,300 by the beings of other worlds and times. 474 00:27:45,340 --> 00:27:48,620 What could we possibly have in common with an alien civilization 475 00:27:48,820 --> 00:27:51,620 with its own separate evolutionary history 476 00:27:51,700 --> 00:27:53,820 and one so far advanced beyond us 477 00:27:54,060 --> 00:27:56,980 that they can patrol interstellar space? 478 00:27:57,700 --> 00:27:59,100 One thing at least 479 00:27:59,260 --> 00:28:00,940 a universal language 480 00:28:01,580 --> 00:28:02,820 science. 481 00:28:04,140 --> 00:28:06,180 It's hard to break the bonds of gravity. 482 00:28:06,460 --> 00:28:08,460 You can only sail the cosmic seas 483 00:28:08,580 --> 00:28:11,540 if you speak mathematics and physics. 484 00:28:11,900 --> 00:28:14,780 Hydrogen is the most common element in the universe. 485 00:28:15,060 --> 00:28:16,780 The electron in a hydrogen atom 486 00:28:16,860 --> 00:28:20,820 flips the direction of its spin at a constant rate, or frequency. 487 00:28:21,180 --> 00:28:24,500 Hydrogen atoms are like tiny natural clocks 488 00:28:24,940 --> 00:28:26,860 tick, tock. 489 00:28:27,100 --> 00:28:28,620 Now we have a unit of time 490 00:28:28,700 --> 00:28:31,180 in common with the extraterrestrials. 491 00:28:31,700 --> 00:28:34,740 This will come in handy when we get to the next level of the message. 492 00:28:34,940 --> 00:28:37,540 Here's our return address in space. 493 00:28:37,820 --> 00:28:40,300 Pulsars are rapidly-spinning neutron stars 494 00:28:40,380 --> 00:28:43,500 that give off regular bursts of radio waves. 495 00:28:44,020 --> 00:28:46,220 You can set your clock by them. 496 00:28:46,340 --> 00:28:48,940 The sun is at the center of this diagram 497 00:28:49,100 --> 00:28:52,540 and the lines point to the 14 nearest pulsars. 498 00:28:52,820 --> 00:28:56,300 A simple code labels each pulsar with its unique frequency 499 00:28:56,540 --> 00:28:58,340 using the ticktock of the hydrogen atom 500 00:28:58,460 --> 00:28:59,780 as the unit of time. 501 00:29:00,300 --> 00:29:03,020 So, alien astronomers could use this diagram 502 00:29:03,100 --> 00:29:07,060 to locate the home star of the Voyager spacecraft in our galaxy. 503 00:29:08,180 --> 00:29:11,340 They could also tell how long ago the spacecraft was launched. 504 00:29:11,500 --> 00:29:12,460 And that's important 505 00:29:12,500 --> 00:29:13,620 because the Voyager record 506 00:29:13,700 --> 00:29:17,580 has a projected shelf life of a 1,000 million years. 507 00:29:20,340 --> 00:29:23,860 Become an extraterrestrial archaeologist for a few moments. 508 00:29:24,060 --> 00:29:27,620 An artifact has been fished out of the interstellar ocean. 509 00:29:27,700 --> 00:29:31,660 It was made by beings that lived about a billion years ago. 510 00:29:31,860 --> 00:29:34,460 What would you make of them and their world? 511 00:29:34,980 --> 00:29:37,780 They've sent us their music 512 00:29:39,020 --> 00:29:42,860 and greetings in 59 human languages. 513 00:29:46,540 --> 00:29:49,140 'Hello from the children of planet Earth.' 514 00:29:49,260 --> 00:29:50,900 And one whale language. 515 00:29:51,660 --> 00:29:55,620 And a sound essay that includes a Saturn-V rocket launch. 516 00:29:57,580 --> 00:30:01,060 A mother's first words to her newborn baby. 517 00:30:01,460 --> 00:30:03,980 'Oh, come on now. Be a good boy..' 518 00:30:04,940 --> 00:30:08,420 The brain waves of a young woman newly fallen in love. 519 00:30:11,380 --> 00:30:14,300 And the sound of a pulsar. 520 00:30:19,420 --> 00:30:23,380 All of that will live for a billion years. 521 00:30:36,060 --> 00:30:39,140 How long is a billion years? 522 00:30:44,420 --> 00:30:47,380 If you compress all the time since the big bang 523 00:30:47,460 --> 00:30:49,220 the explosive birth of the universe 524 00:30:49,300 --> 00:30:51,100 into a single Earth year 525 00:30:51,300 --> 00:30:54,580 a billion years is about one month of that year. 526 00:30:54,860 --> 00:30:58,620 What was happening on Earth a billion years ago? 527 00:31:01,780 --> 00:31:03,660 Most of Earth's land was amassed 528 00:31:03,740 --> 00:31:06,380 into a supercontinent called Rodinia. 529 00:31:06,580 --> 00:31:10,140 It was a barren desert, no animals, no plants. 530 00:31:10,180 --> 00:31:12,300 A billion years ago, there wasn't enough oxygen 531 00:31:12,380 --> 00:31:14,500 in our atmosphere to form an ozone layer 532 00:31:14,660 --> 00:31:15,540 and without it 533 00:31:15,780 --> 00:31:17,300 ultraviolet radiation 534 00:31:17,340 --> 00:31:20,220 prevented life from colonizing the land. 535 00:31:20,460 --> 00:31:22,500 Rodinia probably looked more like Mars 536 00:31:22,580 --> 00:31:24,100 than present-day Earth. 537 00:31:25,060 --> 00:31:28,100 The giant world ocean produced huge rainstorms 538 00:31:28,180 --> 00:31:30,420 causing flooding and erosion. 539 00:31:30,500 --> 00:31:31,620 Glaciers formed 540 00:31:31,820 --> 00:31:33,860 and their slow but relentless movements 541 00:31:33,900 --> 00:31:36,340 carved the land into new shapes. 542 00:31:37,140 --> 00:31:40,220 Single-celled organisms dominated the oceans 543 00:31:40,340 --> 00:31:43,940 but some existed in colonies called microbial mats 544 00:31:44,020 --> 00:31:47,980 and the first multicellular organisms would soon evolve. 545 00:31:48,540 --> 00:31:50,660 And a billion years from now 546 00:31:50,900 --> 00:31:52,420 what will Earth be like 547 00:31:52,860 --> 00:31:55,300 long after our cities, the Egyptian pyramids 548 00:31:55,500 --> 00:31:58,540 the Rocky Mountains have all been eroded to dust? 549 00:31:58,860 --> 00:32:01,020 There are few things we can say with confidence 550 00:32:01,260 --> 00:32:03,660 about such a far distant time. 551 00:32:08,020 --> 00:32:10,380 The only thing we can say for sure 552 00:32:10,580 --> 00:32:12,300 is that Earth as we know it 553 00:32:12,540 --> 00:32:13,820 will be so changed 554 00:32:14,100 --> 00:32:17,180 that we would scarcely recognize it as home. 555 00:32:17,780 --> 00:32:20,900 But even a thousand million years from now 556 00:32:21,140 --> 00:32:23,060 something of who we were 557 00:32:23,180 --> 00:32:26,100 and the music that we made in that long-ago spring 558 00:32:26,860 --> 00:32:28,380 will live on. 559 00:32:34,060 --> 00:32:35,460 In that distant future 560 00:32:35,580 --> 00:32:38,260 our sun will have completed another four orbits 561 00:32:38,380 --> 00:32:40,580 around the centre of the galaxy. 562 00:32:48,460 --> 00:32:51,060 And the Voyagers will have ventured 563 00:32:51,180 --> 00:32:53,020 far from the sun. 564 00:32:56,140 --> 00:32:58,820 Carl Sagan was a member of Voyager's imaging team 565 00:32:59,340 --> 00:33:03,140 and it was his idea that Voyager take one last picture. 566 00:33:04,020 --> 00:33:05,300 A generation before 567 00:33:05,420 --> 00:33:08,020 an astronaut on the last Apollo flight to the moon 568 00:33:08,180 --> 00:33:10,740 had taken a picture of the whole Earth 569 00:33:10,980 --> 00:33:14,180 the planet as a world without borders. 570 00:33:14,300 --> 00:33:17,420 It became an icon of a new consciousness. 571 00:33:17,900 --> 00:33:21,620 Carl realized the next step in this process. 572 00:33:21,740 --> 00:33:22,940 He convinced NASA 573 00:33:23,060 --> 00:33:25,860 to turn the Voyager I camera back towards Earth 574 00:33:25,980 --> 00:33:28,300 when the spacecraft went beyond Neptune 575 00:33:28,580 --> 00:33:30,860 for one last look homeward 576 00:33:31,020 --> 00:33:34,980 at what he called the Pale Blue Dot. 577 00:33:41,300 --> 00:33:42,780 That's here. 578 00:33:42,860 --> 00:33:44,060 That's home. 579 00:33:44,260 --> 00:33:45,660 That's us. 580 00:33:45,980 --> 00:33:48,900 On it, everyone you love 581 00:33:49,060 --> 00:33:50,340 everyone you know 582 00:33:50,660 --> 00:33:52,260 everyone you ever heard of 583 00:33:52,580 --> 00:33:55,380 every human being whoever was 584 00:33:55,460 --> 00:33:57,540 lived out their lives. 585 00:33:57,980 --> 00:34:01,140 The aggregate of our joy and suffering 586 00:34:01,460 --> 00:34:04,380 thousands of confident religions, ideologies 587 00:34:04,460 --> 00:34:06,420 and economic doctrines 588 00:34:06,460 --> 00:34:08,460 every hunter and forager 589 00:34:08,540 --> 00:34:10,420 every hero and coward 590 00:34:10,460 --> 00:34:13,740 every creator and destroyer of civilization 591 00:34:13,860 --> 00:34:15,940 every king and peasant 592 00:34:16,060 --> 00:34:18,100 every young couple in love 593 00:34:18,180 --> 00:34:21,340 every mother and father, hopeful child 594 00:34:21,380 --> 00:34:23,780 inventor and explorer 595 00:34:23,820 --> 00:34:27,220 every teacher of morals, every corrupt politician 596 00:34:27,300 --> 00:34:29,140 every superstar 597 00:34:29,220 --> 00:34:31,380 every supreme leader 598 00:34:31,540 --> 00:34:35,380 every saint and sinner in the history of our species 599 00:34:35,540 --> 00:34:37,020 lived there 600 00:34:37,260 --> 00:34:38,860 on a mote of dust 601 00:34:38,980 --> 00:34:42,380 suspended in a sunbeam. 602 00:34:42,420 --> 00:34:46,380 The Earth is a very small stage 603 00:34:46,660 --> 00:34:50,620 in a vast, cosmic arena. 604 00:34:50,660 --> 00:34:53,540 Think of the rivers of blood 605 00:34:53,620 --> 00:34:57,340 spilled by all those generals and emperors 606 00:34:57,460 --> 00:34:59,660 so that in glory and triumph 607 00:34:59,780 --> 00:35:02,220 they could become the momentary masters 608 00:35:02,780 --> 00:35:06,300 of a fraction of a dot. 609 00:35:06,460 --> 00:35:09,220 Think of the endless cruelties visited 610 00:35:09,340 --> 00:35:12,580 by the inhabitants of one corner of this pixel 611 00:35:12,740 --> 00:35:15,940 on the scarcely distinguishable inhabitants 612 00:35:16,020 --> 00:35:17,580 of some other corner. 613 00:35:17,700 --> 00:35:20,700 How frequent their misunderstandings 614 00:35:20,860 --> 00:35:23,540 how eager they are to kill one another 615 00:35:23,740 --> 00:35:26,740 how fervent their hatreds. 616 00:35:27,380 --> 00:35:29,780 Our posturings 617 00:35:29,900 --> 00:35:32,660 our imagined self-importance 618 00:35:32,780 --> 00:35:35,540 the delusion that we have some privileged position 619 00:35:35,620 --> 00:35:36,860 in the universe 620 00:35:36,900 --> 00:35:39,580 are challenged by this point 621 00:35:39,620 --> 00:35:41,180 of pale light. 622 00:35:42,220 --> 00:35:46,180 Our planet is a lonely speck 623 00:35:46,220 --> 00:35:49,980 in the great, enveloping cosmic dark. 624 00:35:50,060 --> 00:35:52,380 In our obscurity 625 00:35:52,860 --> 00:35:55,300 in all this vastness 626 00:35:55,580 --> 00:35:57,260 there is no hint 627 00:35:57,300 --> 00:35:59,300 that help will come from elsewhere 628 00:35:59,380 --> 00:36:02,260 to save us from ourselves. 629 00:36:02,380 --> 00:36:06,340 The Earth is the only world known so far to harbour life. 630 00:36:06,980 --> 00:36:08,460 There is nowhere else 631 00:36:08,580 --> 00:36:10,260 at least in the near future 632 00:36:10,380 --> 00:36:13,220 to which our species could migrate. 633 00:36:13,300 --> 00:36:15,980 Visit, yes. 634 00:36:16,060 --> 00:36:18,900 Settle, not yet. 635 00:36:19,020 --> 00:36:20,180 Like it or not 636 00:36:20,380 --> 00:36:21,940 for the moment 637 00:36:21,980 --> 00:36:25,180 the Earth is where we make our stand. 638 00:36:25,460 --> 00:36:28,380 It has been said that astronomy is a humbling 639 00:36:28,420 --> 00:36:31,980 and character-building experience. 640 00:36:32,420 --> 00:36:34,940 There is perhaps no better demonstration 641 00:36:35,020 --> 00:36:37,660 of the folly of human conceits 642 00:36:37,820 --> 00:36:40,900 than this distant image. 643 00:36:41,420 --> 00:36:44,780 To me, it underscores our responsibility 644 00:36:44,940 --> 00:36:47,740 to deal more kindly with one another 645 00:36:47,780 --> 00:36:50,700 and to preserve and cherish 646 00:36:50,740 --> 00:36:52,220 the pale blue dot 647 00:36:52,340 --> 00:36:55,820 the only home we've ever known. 648 00:37:02,580 --> 00:37:04,780 How did we, tiny creatures 649 00:37:04,860 --> 00:37:06,860 living on that speck of dust 650 00:37:06,940 --> 00:37:08,540 ever manage to figure out 651 00:37:08,580 --> 00:37:12,540 how to send spacecraft out among the stars of the Milky Way? 652 00:37:13,020 --> 00:37:14,740 Only a few centuries ago 653 00:37:14,860 --> 00:37:17,020 a mere second of cosmic time 654 00:37:17,300 --> 00:37:20,820 we knew nothing of where or when we were. 655 00:37:20,900 --> 00:37:23,340 Oblivious to the rest of the cosmos 656 00:37:23,380 --> 00:37:25,620 we inhabited a kind of prison 657 00:37:25,700 --> 00:37:29,660 a tiny universe bounded by a nutshell. 658 00:37:33,980 --> 00:37:36,780 How did we escape from the prison? 659 00:37:37,940 --> 00:37:40,700 It was the work of generations of searchers 660 00:37:40,780 --> 00:37:44,460 who took five simple rules to heart. 661 00:37:48,860 --> 00:37:50,820 Question authority. 662 00:37:50,860 --> 00:37:52,460 No idea is true 663 00:37:52,540 --> 00:37:56,140 just because someone says so, including me. 664 00:37:57,500 --> 00:37:59,620 Think for yourself. 665 00:38:03,180 --> 00:38:05,700 Question yourself. 666 00:38:06,740 --> 00:38:10,180 Don't believe anything just because you want to. 667 00:38:10,300 --> 00:38:13,500 Believing something doesn't make it so. 668 00:38:14,020 --> 00:38:16,180 Test ideas by the evidence gained 669 00:38:16,260 --> 00:38:18,860 from observation and experiment. 670 00:38:20,820 --> 00:38:24,780 If a favourite idea fails a well-designed test, it's wrong! 671 00:38:25,420 --> 00:38:26,740 Get over it. 672 00:38:28,060 --> 00:38:31,460 Follow the evidence, wherever it leads. 673 00:38:33,140 --> 00:38:36,900 If you have no evidence, reserve judgment. 674 00:38:37,100 --> 00:38:39,620 And perhaps the most important rule of all 675 00:38:40,260 --> 00:38:42,900 remember, you could be wrong. 676 00:38:42,980 --> 00:38:46,740 Even the best scientists have been wrong about some things. 677 00:38:46,940 --> 00:38:49,060 Newton, Einstein 678 00:38:49,140 --> 00:38:52,540 and every other great scientist in history 679 00:38:52,620 --> 00:38:54,300 they all made mistakes. 680 00:38:54,380 --> 00:38:57,500 Of course they did, they were human. 681 00:38:57,860 --> 00:39:01,620 Science is a way to keep from fooling ourselves 682 00:39:02,100 --> 00:39:03,620 and each other. 683 00:39:04,780 --> 00:39:07,300 Have scientists known sin? 684 00:39:10,300 --> 00:39:11,340 Of course. 685 00:39:11,900 --> 00:39:13,940 We have misused science 686 00:39:14,020 --> 00:39:17,540 just as we have every other tool at our disposal 687 00:39:17,780 --> 00:39:20,380 and that's why we can't afford to leave it 688 00:39:20,500 --> 00:39:22,900 in the hands of a powerful few. 689 00:39:23,700 --> 00:39:26,300 The more science belongs to all of us 690 00:39:26,540 --> 00:39:29,220 the less likely it is to be misused. 691 00:39:31,940 --> 00:39:33,660 These values undermine 692 00:39:33,700 --> 00:39:36,820 the appeals of fanaticism and ignorance. 693 00:39:36,860 --> 00:39:38,780 And, after all 694 00:39:38,860 --> 00:39:41,220 the universe is mostly dark 695 00:39:41,300 --> 00:39:43,860 dotted by islands of light. 696 00:39:45,060 --> 00:39:48,380 Learning the age of the Earth or the distance to the stars or 697 00:39:48,420 --> 00:39:50,060 how life evolves 698 00:39:50,180 --> 00:39:52,140 what difference does that make? 699 00:39:52,340 --> 00:39:53,980 Well, part of it depends on 700 00:39:54,020 --> 00:39:56,620 how big a universe you're willing to live in. 701 00:39:57,020 --> 00:39:58,820 Some of us like it small. 702 00:39:59,020 --> 00:40:00,420 That's fine. 703 00:40:00,500 --> 00:40:02,180 Understandable. 704 00:40:02,220 --> 00:40:03,780 But I like it big. 705 00:40:03,860 --> 00:40:06,900 And when I take all of this into my heart and my mind 706 00:40:06,940 --> 00:40:08,580 I'm uplifted by it. 707 00:40:08,660 --> 00:40:10,180 And when I have that feeling 708 00:40:10,260 --> 00:40:12,460 I want to know that it's real 709 00:40:12,500 --> 00:40:16,060 that it's not just something happening inside my own head 710 00:40:16,300 --> 00:40:18,140 because it matters what's true 711 00:40:18,220 --> 00:40:19,780 and our imagination 712 00:40:19,900 --> 00:40:23,860 is nothing compared with nature's awesome reality. 713 00:40:28,300 --> 00:40:31,620 I want to know what's in those dark places 714 00:40:32,860 --> 00:40:36,140 and what happened before the big bang. 715 00:40:38,020 --> 00:40:41,220 I want to know what lies beyond the cosmic horizon 716 00:40:41,300 --> 00:40:43,540 and how life began. 717 00:40:43,620 --> 00:40:45,580 Are there other places in the cosmos 718 00:40:45,780 --> 00:40:49,500 where matter and energy have become alive 719 00:40:50,740 --> 00:40:52,860 and aware? 720 00:40:59,940 --> 00:41:03,460 I want to know my ancestors, all of them. 721 00:41:03,500 --> 00:41:05,580 I want to be a good, strong link 722 00:41:05,660 --> 00:41:07,780 in the chain of generations. 723 00:41:07,900 --> 00:41:09,820 I want to protect my children 724 00:41:09,860 --> 00:41:12,740 and the children of ages to come. 725 00:41:12,980 --> 00:41:16,180 We, who embody the local eyes and ears 726 00:41:16,260 --> 00:41:18,940 and thoughts and feelings of the cosmos. 727 00:41:19,020 --> 00:41:21,820 We've begun to learn the story of our origins 728 00:41:22,220 --> 00:41:26,100 star stuff contemplating the evolution of matter 729 00:41:26,340 --> 00:41:30,220 tracing that long path by which it arrived at consciousness. 730 00:41:30,540 --> 00:41:32,860 We and the other living things on this planet 731 00:41:32,900 --> 00:41:35,100 carry a legacy of cosmic evolution 732 00:41:35,220 --> 00:41:37,740 spanning billions of years. 733 00:41:37,780 --> 00:41:39,940 If we take that knowledge to heart 734 00:41:39,980 --> 00:41:43,620 if we come to know and love nature as it really is 735 00:41:43,660 --> 00:41:46,540 then we will surely be remembered by our descendants 736 00:41:46,580 --> 00:41:49,540 as good, strong links in the chain of life. 737 00:41:49,620 --> 00:41:52,820 And our children will continue this sacred searching 738 00:41:53,020 --> 00:41:56,700 seeing for us as we have seen for those who came before 739 00:41:56,780 --> 00:41:59,940 discovering wonders yet undreamt of 740 00:42:00,100 --> 00:42:02,220 in the cosmos.