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These are the user uploaded subtitles that are being translated: 1 00:00:02,500 --> 00:00:05,068 The universe was born to die. 2 00:00:05,069 --> 00:00:09,472 But how and when will it all end? 3 00:00:09,473 --> 00:00:11,306 That's the reason i became a cosmologist. 4 00:00:11,307 --> 00:00:13,043 I wanted to be the first person that would know 5 00:00:13,044 --> 00:00:15,011 How the universe would end. 6 00:00:15,012 --> 00:00:18,782 Two cosmic heavyweights wrestle for control. 7 00:00:18,783 --> 00:00:21,283 The winner seals our fate. 8 00:00:21,284 --> 00:00:24,087 The tug of war is gravity, 9 00:00:24,088 --> 00:00:25,756 Which is trying to shrink it down, 10 00:00:25,757 --> 00:00:28,558 And the expansion of space and time itself. 11 00:00:28,559 --> 00:00:30,893 Will gravity triumph? 12 00:00:30,894 --> 00:00:34,063 The universe will get smaller and smaller, hotter and hotter. 13 00:00:34,064 --> 00:00:37,066 Or will expansion get the upper hand? 14 00:00:37,067 --> 00:00:41,038 Even the electrons around your atoms will be ripped apart. 15 00:00:41,039 --> 00:00:42,505 The end is coming, 16 00:00:42,506 --> 00:00:46,043 And it could be sooner than you think. 17 00:00:59,425 --> 00:01:02,494 The universe is everything 18 00:01:02,495 --> 00:01:06,198 All space, all time, all matter. 19 00:01:08,467 --> 00:01:11,436 The earth is a speck by comparison, 20 00:01:11,437 --> 00:01:16,007 A grain of rock orbiting just one of the 200 billion stars 21 00:01:16,008 --> 00:01:19,079 In our home galaxy, the milky way. 22 00:01:22,381 --> 00:01:26,184 In turn, this enormous structure is just a drop 23 00:01:26,185 --> 00:01:28,787 In an ocean of galaxies that stretch 24 00:01:28,788 --> 00:01:31,324 For 90 billion light years. 25 00:01:33,425 --> 00:01:35,526 And all of this, 26 00:01:35,527 --> 00:01:39,698 From the biggest galaxy to the smallest atom, 27 00:01:39,699 --> 00:01:41,902 Will one day die. 28 00:01:43,737 --> 00:01:46,138 We don't see evidence of anything being eternal. 29 00:01:46,139 --> 00:01:47,838 Eternity doesn't exist. 30 00:01:47,839 --> 00:01:50,109 Even space and time will come to an end. 31 00:01:51,445 --> 00:01:55,381 The universe has been expanding since its birth, 32 00:01:55,382 --> 00:01:59,551 Gradually burning through the fuel that lights its stars. 33 00:01:59,552 --> 00:02:02,554 But what happens when the fuel runs out? 34 00:02:02,555 --> 00:02:05,056 Will it all just fade away? 35 00:02:05,057 --> 00:02:07,460 Stars die out, use up their nuclear fuel. 36 00:02:07,461 --> 00:02:10,063 We have an empty, cold, desolate universe. 37 00:02:10,064 --> 00:02:12,132 Just dead remnants of stars -- 38 00:02:12,133 --> 00:02:14,234 Black holes, neutron stars. 39 00:02:14,235 --> 00:02:15,768 Eventually, they decay away, 40 00:02:15,769 --> 00:02:18,704 And you're left with a thin haze of very low energy light. 41 00:02:18,705 --> 00:02:20,039 That's it. 42 00:02:20,040 --> 00:02:21,806 We used to think the universe 43 00:02:21,807 --> 00:02:24,577 Would cruise gently into old age. 44 00:02:24,578 --> 00:02:26,679 But over the past few decades, 45 00:02:26,680 --> 00:02:30,149 Astronomers have revealed a very different 46 00:02:30,150 --> 00:02:31,918 And disturbing picture. 47 00:02:31,919 --> 00:02:34,853 The universe isn't cruising. 48 00:02:34,854 --> 00:02:36,688 It's fighting for its life. 49 00:02:36,689 --> 00:02:38,958 It may seem peaceful here on earth on a nice, sunny day, 50 00:02:38,959 --> 00:02:40,793 But in fact, above us and all around us, 51 00:02:40,794 --> 00:02:43,929 Throughout the universe, a battle is raging, 52 00:02:43,930 --> 00:02:45,967 And it has raged since the beginning of time. 53 00:02:46,835 --> 00:02:50,404 Two deadly forces grapple for control. 54 00:02:50,405 --> 00:02:54,941 The first, expansion, pulls galaxies apart, 55 00:02:54,942 --> 00:02:57,977 Cooling the universe and threatening it 56 00:02:57,978 --> 00:03:01,048 With a frozen extinction. 57 00:03:01,049 --> 00:03:05,585 The second, gravity, tries to crush everything back together, 58 00:03:05,586 --> 00:03:09,424 Annihilating the universe in a dense ball of fire. 59 00:03:11,992 --> 00:03:15,596 Will gravity or expansion win? 60 00:03:15,597 --> 00:03:17,631 Or will it end in a tie? 61 00:03:17,632 --> 00:03:21,437 These two colossal forces yield three endgames. 62 00:03:22,037 --> 00:03:24,104 One is the big freeze. 63 00:03:24,105 --> 00:03:27,073 Expansion wins, and the universe just expands forever. 64 00:03:27,074 --> 00:03:29,676 The second is that there is a delicate balance 65 00:03:29,677 --> 00:03:30,944 Between the expansion 66 00:03:30,945 --> 00:03:32,614 And the amount of gravitational attraction, 67 00:03:32,615 --> 00:03:34,715 And the universe gets to a particular size, 68 00:03:34,716 --> 00:03:36,184 And it pretty much stays there. 69 00:03:36,185 --> 00:03:37,853 And the third outcome is that 70 00:03:37,854 --> 00:03:39,688 The gravitational attraction wins, 71 00:03:39,689 --> 00:03:41,322 And the expansion stops, 72 00:03:41,323 --> 00:03:43,057 And the universe begins to get smaller 73 00:03:43,058 --> 00:03:46,228 Until, eventually, it goes back to a big crunch. 74 00:03:48,431 --> 00:03:50,765 So far, the universe seems balanced 75 00:03:50,766 --> 00:03:54,703 On a tightrope between expansion and contraction. 76 00:03:54,704 --> 00:03:58,107 But will it keep its equilibrium until it runs out of steam, 77 00:03:58,108 --> 00:04:00,911 Or will something tip the balance? 78 00:04:02,946 --> 00:04:05,882 I don't think there's any bigger question than, 79 00:04:05,883 --> 00:04:08,116 Where is the universe going? 80 00:04:08,117 --> 00:04:11,654 To predict the future, cosmologists have always looked 81 00:04:11,655 --> 00:04:15,858 To the past, back to the beginning of expansion, 82 00:04:15,859 --> 00:04:20,631 The beginning of gravity, the beginning of everything. 83 00:04:23,232 --> 00:04:28,202 13.8 billion years ago, an infinitely dense, 84 00:04:28,203 --> 00:04:32,908 Hot speck ignites and suddenly expands outward -- 85 00:04:32,909 --> 00:04:34,912 The big bang. 86 00:04:36,446 --> 00:04:40,016 All energy, all space, and all matter... 87 00:04:41,751 --> 00:04:44,786 ...the building blocks of the universe we see today, 88 00:04:44,787 --> 00:04:47,258 Are created and set in motion. 89 00:04:48,259 --> 00:04:50,494 Think of it. 90 00:04:50,495 --> 00:04:52,797 Everything you see around us 91 00:04:52,798 --> 00:04:57,434 Concentrated into a primordial fireball that exploded, 92 00:04:57,435 --> 00:05:00,238 Sending all the galaxies into motion. 93 00:05:04,309 --> 00:05:07,977 That outward blast, the birth of expansion, 94 00:05:07,978 --> 00:05:10,647 Is still going on today. 95 00:05:10,648 --> 00:05:14,051 Without it, we wouldn't have a universe big enough 96 00:05:14,052 --> 00:05:16,854 For stars and galaxies to exist in. 97 00:05:16,855 --> 00:05:20,123 Expansion is an astonishing force of nature. 98 00:05:20,124 --> 00:05:24,427 It works by inflating the fabric of space-Time. 99 00:05:24,428 --> 00:05:28,099 Space between galaxies expands, 100 00:05:28,100 --> 00:05:30,402 And it pushes the galaxies apart. 101 00:05:30,403 --> 00:05:35,506 Space carries objects with it like a surfer on a wave. 102 00:05:35,507 --> 00:05:37,909 It's going on in every part of space. 103 00:05:37,910 --> 00:05:39,578 Even inside your body right now, 104 00:05:39,579 --> 00:05:41,513 There's a pressure for space to expand. 105 00:05:42,380 --> 00:05:45,417 Expansion generated the vast, moving stage 106 00:05:45,418 --> 00:05:48,052 On which today's universe plays out. 107 00:05:48,053 --> 00:05:50,956 But left unchecked, it could have been a force 108 00:05:50,957 --> 00:05:53,090 For utter annihilation. 109 00:05:53,091 --> 00:05:55,326 If the universe had been expanding much faster, 110 00:05:55,327 --> 00:05:57,095 It would have emptied out so fast, 111 00:05:57,096 --> 00:05:59,364 You wouldn't have had time to make galaxies, 112 00:05:59,365 --> 00:06:00,500 Planets, people. 113 00:06:03,168 --> 00:06:04,770 The fact that we're here 114 00:06:04,771 --> 00:06:07,340 Means that something must have put on the brakes. 115 00:06:07,341 --> 00:06:11,943 It was, of course, our universal glue -- Gravity. 116 00:06:11,944 --> 00:06:15,413 Gravity and matter go hand in hand. 117 00:06:15,414 --> 00:06:18,316 The more massive the object, 118 00:06:18,317 --> 00:06:21,419 The more pull it exerts on everything around it. 119 00:06:21,420 --> 00:06:27,026 It draws atom to atom, particle to particle... 120 00:06:27,728 --> 00:06:33,032 ...building stars, nebulas, 121 00:06:33,033 --> 00:06:35,368 Galaxies -- 122 00:06:35,369 --> 00:06:39,506 The hardware of the universe we see today. 123 00:06:39,507 --> 00:06:42,340 But gravity is a double-Edged sword. 124 00:06:42,341 --> 00:06:45,244 Too much, and the early universe would never have gotten 125 00:06:45,245 --> 00:06:47,412 Out of the starting blocks. 126 00:06:47,413 --> 00:06:49,448 If it had been expanding more slowly, 127 00:06:49,449 --> 00:06:51,717 It would have re-Collapsed into another singularity. 128 00:06:51,718 --> 00:06:54,486 And again, you wouldn't have had the time to make galaxies, 129 00:06:54,487 --> 00:06:56,289 Planets, or people. 130 00:06:56,290 --> 00:06:57,924 So we live in the goldilocks universe. 131 00:06:57,925 --> 00:07:00,059 We live in the universe that lasts long enough 132 00:07:00,060 --> 00:07:02,561 That we can be here, but expands gently enough 133 00:07:02,562 --> 00:07:04,497 That we have time to form. 134 00:07:07,267 --> 00:07:11,069 The universe has lasted for 13.8 billion years, 135 00:07:11,070 --> 00:07:15,042 Thanks to the opposing forces of gravity and expansion. 136 00:07:15,043 --> 00:07:19,112 But just how stable is this balancing act? 137 00:07:19,113 --> 00:07:22,615 Does our universe have just the right amount of stuff in it 138 00:07:22,616 --> 00:07:24,716 To keep it from runaway expansion 139 00:07:24,717 --> 00:07:26,787 Or catastrophic collapse? 140 00:07:27,388 --> 00:07:30,257 In the 1920s, scientists did the math, 141 00:07:30,258 --> 00:07:34,094 And the results were anything but reassuring. 142 00:07:34,095 --> 00:07:37,331 The more matter you have, the more gravity you have. 143 00:07:37,332 --> 00:07:40,668 If you have lots of matter in a very dense universe, 144 00:07:40,669 --> 00:07:43,738 Perhaps the universe begins to re-Collapse. 145 00:07:43,739 --> 00:07:45,839 Or, if you have very little matter, 146 00:07:45,840 --> 00:07:48,209 The universe would freeze to death. 147 00:07:48,210 --> 00:07:52,379 So what is the critical density, the border between the two? 148 00:07:52,380 --> 00:07:56,916 It's approximately five hydrogen atoms per cubic meter. 149 00:07:56,917 --> 00:08:02,322 So think of a cubic yard, and put just five hydrogen atoms 150 00:08:02,323 --> 00:08:05,159 Inside, and that is the tipping point. 151 00:08:05,160 --> 00:08:07,293 If you put more than five atoms, 152 00:08:07,294 --> 00:08:09,296 Then the universe will begin to collapse. 153 00:08:09,297 --> 00:08:10,831 If you have less than five atoms, 154 00:08:10,832 --> 00:08:12,434 Then the universe just keeps on going. 155 00:08:13,435 --> 00:08:15,635 If we thought the universe was balanced 156 00:08:15,636 --> 00:08:18,806 On a tightrope before, the critical density question 157 00:08:18,807 --> 00:08:23,079 Showed us that the rope was more like a razor blade. 158 00:08:23,446 --> 00:08:26,382 Yet, when astronomers took additional measurements, 159 00:08:26,383 --> 00:08:28,816 They liked what they saw. 160 00:08:28,817 --> 00:08:32,220 The universe appeared to contain just the right amount 161 00:08:32,221 --> 00:08:35,158 Of matter to stay at the critical density. 162 00:08:36,293 --> 00:08:38,393 More and more, the indirect evidence 163 00:08:38,394 --> 00:08:41,229 And the theoretical arguments suggested 164 00:08:41,230 --> 00:08:43,932 That the universe must be exactly at the boundary 165 00:08:43,933 --> 00:08:45,768 Between a universe that would collapse 166 00:08:45,769 --> 00:08:48,070 And one that would expand forever, 167 00:08:48,071 --> 00:08:51,706 That we were teetering on the hairy edge of expansion. 168 00:08:51,707 --> 00:08:55,978 The universe seemed so perfectly balanced 169 00:08:55,979 --> 00:08:59,880 That it would head quietly into old age. 170 00:08:59,881 --> 00:09:03,418 Then, in the 1970s, astronomers made an observation 171 00:09:03,419 --> 00:09:05,421 That shocked them. 172 00:09:05,422 --> 00:09:09,325 The cosmos was filled with invisible stuff, 173 00:09:09,326 --> 00:09:14,031 And its gravity could cause a catastrophic collapse. 174 00:09:24,443 --> 00:09:27,578 The universe is balanced on a tightrope. 175 00:09:27,579 --> 00:09:31,715 On each side of the drop lies an early death -- 176 00:09:31,716 --> 00:09:35,454 A big freeze, fueled by the runaway stretching of space, 177 00:09:35,455 --> 00:09:41,358 Or a big crunch, the result of gravity overcoming expansion. 178 00:09:41,359 --> 00:09:44,828 40 years ago, scientists believed we'd stay balanced 179 00:09:44,829 --> 00:09:48,399 Between these fates for eternity. 180 00:09:48,400 --> 00:09:50,635 Now things have changed tremendously, 181 00:09:50,636 --> 00:09:53,371 Because we've discovered something we never knew about 182 00:09:53,372 --> 00:09:54,172 40 years ago. 183 00:09:54,773 --> 00:09:59,444 In the 1970s, astronomers are stunned. 184 00:09:59,445 --> 00:10:03,147 Some unknown form of matter, invisible to telescopes, 185 00:10:03,148 --> 00:10:05,849 Dwarfs what we thought was out there, 186 00:10:05,850 --> 00:10:09,621 Not a fraction more, but five times more. 187 00:10:09,622 --> 00:10:12,790 We used to think that gravity came from stars 188 00:10:12,791 --> 00:10:15,794 And objects you can see -- End of story. 189 00:10:15,795 --> 00:10:19,165 Now, we realize that that naive picture is actually wrong. 190 00:10:20,200 --> 00:10:22,501 Astronomers make the discovery, 191 00:10:22,502 --> 00:10:25,873 Studying the clockwork nature of our universe. 192 00:10:27,275 --> 00:10:29,942 The huge gravity of the sun holds the earth 193 00:10:29,943 --> 00:10:34,082 And all the other planets in a delicate circular dance. 194 00:10:37,951 --> 00:10:41,487 The sun's mass controls the speed of these orbits. 195 00:10:41,488 --> 00:10:44,657 If it were more massive, the planets would orbit 196 00:10:44,658 --> 00:10:46,325 Much more quickly. 197 00:10:46,326 --> 00:10:48,895 And if it were smaller, it would take much longer 198 00:10:48,896 --> 00:10:51,532 For a planet to complete an orbit. 199 00:10:53,733 --> 00:10:57,002 Galaxies run like clockwork, too. 200 00:10:57,003 --> 00:11:00,272 The vast mass at the center pulls the outer stars 201 00:11:00,273 --> 00:11:03,676 Into circular, planet-Like orbits. 202 00:11:03,677 --> 00:11:06,179 Astronomers make precise measurements 203 00:11:06,180 --> 00:11:09,848 Of these galactic orbits in the 1970s. 204 00:11:09,849 --> 00:11:13,021 The results change everything. 205 00:11:13,922 --> 00:11:16,489 The galaxies were spinning too fast. 206 00:11:16,490 --> 00:11:18,025 Way too fast. 207 00:11:21,096 --> 00:11:23,965 Even accounting for the supermassive black holes 208 00:11:23,966 --> 00:11:28,268 At their center, nine-Tenths of their mass was missing. 209 00:11:28,269 --> 00:11:31,105 By rights, the galaxy should fly apart. 210 00:11:31,106 --> 00:11:33,274 By rights, the earth should have been flung 211 00:11:33,275 --> 00:11:36,244 Into intergalactic space billions of years ago. 212 00:11:36,245 --> 00:11:39,446 We should have no milky way galaxy, and yet, 213 00:11:39,447 --> 00:11:41,183 Our universe is full of galaxies. 214 00:11:45,253 --> 00:11:48,188 An immense additional source of gravity 215 00:11:48,189 --> 00:11:51,091 Must be holding galaxies together. 216 00:11:51,092 --> 00:11:54,327 But no matter where astronomers point their telescopes, 217 00:11:54,328 --> 00:11:56,264 They see nothing. 218 00:11:56,265 --> 00:11:59,799 Not a glimmer, not a shadow. 219 00:11:59,800 --> 00:12:04,672 Whatever this new stuff is, it doesn't emit light, 220 00:12:04,673 --> 00:12:08,308 Reflect light, or even block light. 221 00:12:08,309 --> 00:12:11,213 They call it dark matter. 222 00:12:11,246 --> 00:12:14,584 What we've learned is that most of the matter in the universe 223 00:12:14,585 --> 00:12:17,220 Is not ordinary stuff. It's not atoms. 224 00:12:17,221 --> 00:12:20,022 It's not particles we've yet detected in any experiment 225 00:12:20,023 --> 00:12:21,724 Done here on earth. 226 00:12:21,725 --> 00:12:24,360 It's some new kind of particle that we call the dark matter. 227 00:12:27,496 --> 00:12:29,398 Dark matter fills the universe, 228 00:12:29,399 --> 00:12:32,502 Outstripping normal matter by 5-To-1. 229 00:12:36,105 --> 00:12:40,609 Vast filaments spread out throughout the cosmos, 230 00:12:40,610 --> 00:12:45,081 And bright galaxies cluster where dark matter is thickest. 231 00:12:47,417 --> 00:12:51,753 Dark matter provides the scaffolding that underlies 232 00:12:51,754 --> 00:12:54,623 How the matter in the universe structures itself, 233 00:12:54,624 --> 00:12:56,527 Where it goes, and what it does. 234 00:12:57,394 --> 00:12:59,329 So, dark matter dictated 235 00:12:59,330 --> 00:13:02,896 How the universe unfolded. 236 00:13:02,897 --> 00:13:05,035 It seems as if out of the hot big bang, 237 00:13:05,036 --> 00:13:08,671 Dark matter condensed first, before atoms, 238 00:13:08,672 --> 00:13:11,641 And dark matter began to become clumpy. 239 00:13:11,642 --> 00:13:14,844 The clumpiness then began to attract atoms 240 00:13:14,845 --> 00:13:18,547 As they were formed later, and that formed galaxies. 241 00:13:18,548 --> 00:13:20,584 And in some sense, the dark matter therefore 242 00:13:20,585 --> 00:13:24,189 Provides kind of a womb that allows the birth of our galaxy. 243 00:13:27,425 --> 00:13:30,594 Dark matter holds the universe together, 244 00:13:30,595 --> 00:13:33,064 But it also threatens to destroy it. 245 00:13:35,897 --> 00:13:36,598 One of the most amazing discoveries 246 00:13:36,599 --> 00:13:39,036 Of the past few decades is dark matter, 247 00:13:39,037 --> 00:13:41,002 The fact that there's much more matter in the universe 248 00:13:41,003 --> 00:13:42,472 Than we were aware of. 249 00:13:42,473 --> 00:13:44,976 And all of that matter has a lot of gravity. 250 00:13:44,977 --> 00:13:47,109 So all this new matter, all this new gravity 251 00:13:47,110 --> 00:13:49,513 Must be slowing down the expansion of the universe. 252 00:13:50,281 --> 00:13:53,217 Dark matter may even tip the cosmic scales 253 00:13:53,218 --> 00:13:55,218 In favor of gravity, 254 00:13:55,219 --> 00:13:58,988 Defeating expansion and pulling the entire universe 255 00:13:58,989 --> 00:14:01,593 Towards a death by fire. 256 00:14:01,594 --> 00:14:04,395 It's called the big crunch, 257 00:14:04,396 --> 00:14:06,765 And this is how it would play out. 258 00:14:08,467 --> 00:14:12,803 For a fraction of a second, the universe stalls, 259 00:14:12,804 --> 00:14:16,540 Poised between expansion and contraction. 260 00:14:16,541 --> 00:14:20,644 Then, gravity kicks off a cataclysm. 261 00:14:20,645 --> 00:14:23,113 When you looked out, the very first things 262 00:14:23,114 --> 00:14:25,049 As it began to turn around that you began to see 263 00:14:25,050 --> 00:14:27,684 Is that galaxies, instead of moving away from us on average, 264 00:14:27,685 --> 00:14:30,189 Would begin to be moving towards us on average. 265 00:14:31,323 --> 00:14:34,294 The whole universe would look like it was coming to get us. 266 00:14:36,096 --> 00:14:38,697 As space contracts further, 267 00:14:38,698 --> 00:14:42,533 The density of matter increases, gravity gets stronger, 268 00:14:42,534 --> 00:14:47,706 Temperatures soar as the crunch gathers momentum. 269 00:14:47,707 --> 00:14:50,042 Galaxies begin to collide, 270 00:14:50,043 --> 00:14:53,012 Gas clouds begin to collide, 271 00:14:53,013 --> 00:14:56,116 Planets slam into the earth. 272 00:14:59,885 --> 00:15:03,455 Black holes will execute a death dance around each other. 273 00:15:03,456 --> 00:15:06,892 Temperatures, of course, will continue to skyrocket. 274 00:15:06,893 --> 00:15:10,730 Matter, space, and time implode 275 00:15:10,731 --> 00:15:13,664 Until everything in the universe is compressed 276 00:15:13,665 --> 00:15:19,504 Into a tiny speck of infinite mass, heat, and pressure. 277 00:15:19,505 --> 00:15:22,273 For the last stages of the big crunch, 278 00:15:22,274 --> 00:15:25,476 Galaxies will collide and form a primordial atom. 279 00:15:25,477 --> 00:15:29,849 And then, life as we know it will be impossible. 280 00:15:29,850 --> 00:15:32,283 We're back to where it all began, 281 00:15:32,284 --> 00:15:33,421 Back at the big bang. 282 00:15:34,222 --> 00:15:37,959 The universe that we live in will cease to exist. 283 00:15:41,528 --> 00:15:47,266 But some believe a big crunch could herald a new beginning. 284 00:15:47,267 --> 00:15:49,602 We don't know what the end point of a big crunch would be, 285 00:15:49,603 --> 00:15:52,338 Because the laws of physics break down. 286 00:15:52,339 --> 00:15:55,809 It's possible, and indeed, philosophically very pleasant, 287 00:15:55,810 --> 00:16:00,045 To imagine that that crunch would somehow end up evolving 288 00:16:00,046 --> 00:16:03,348 Into an expansion again, and you could have a cyclic universe 289 00:16:03,349 --> 00:16:04,883 Which goes on forever. 290 00:16:04,884 --> 00:16:08,623 Perhaps at that point, we will recreate another big bang. 291 00:16:12,560 --> 00:16:14,928 It's conceivable that as everything comes together 292 00:16:14,929 --> 00:16:18,463 In the crunch, something sort of keeps it from just continuing 293 00:16:18,464 --> 00:16:22,135 And pushes out in a hot, dense, smooth state, 294 00:16:22,136 --> 00:16:24,838 And from the other side, it looks like a big bang, 295 00:16:24,839 --> 00:16:26,573 And a new universe has been created. 296 00:16:26,574 --> 00:16:29,442 Our big bang might have been someone else's big crunch. 297 00:16:29,443 --> 00:16:31,745 But just when scientists came to terms 298 00:16:31,746 --> 00:16:35,216 With dark matter's big crunch, the universe threw them 299 00:16:35,217 --> 00:16:37,618 Another, even bigger curve. 300 00:16:37,619 --> 00:16:42,156 Some ghostly force seemed to be sending us hurtling toward 301 00:16:42,157 --> 00:16:44,257 A completely different death. 302 00:16:44,258 --> 00:16:47,061 My postdoctoral scholar showed me the results. 303 00:16:47,062 --> 00:16:48,230 I nearly fell off my chair. 304 00:16:58,374 --> 00:17:00,710 Gravity and expansion battle for control 305 00:17:00,711 --> 00:17:04,181 Of our universe for 14 billion years... 306 00:17:08,352 --> 00:17:12,787 ...expansion pushing it outwards, 307 00:17:12,788 --> 00:17:15,393 Gravity pulling it in. 308 00:17:16,894 --> 00:17:18,995 With dark matter in its corner, 309 00:17:18,996 --> 00:17:21,497 Gravity seems to be the inevitable winner. 310 00:17:21,498 --> 00:17:26,068 The extra mass will drag the universe into a big crunch, 311 00:17:26,069 --> 00:17:28,104 Until a stunning discovery 312 00:17:28,105 --> 00:17:32,610 Revolutionizes our understanding of the universe. 313 00:17:34,944 --> 00:17:39,883 Around 1990, two teams of researchers decided to measure 314 00:17:39,884 --> 00:17:41,950 The expansion history of the universe 315 00:17:41,951 --> 00:17:45,054 To determine whether it's been slowing down so much 316 00:17:45,055 --> 00:17:47,291 That it'll eventually have a big crunch, 317 00:17:47,292 --> 00:17:49,825 Or whether it hasn't been slowing down much 318 00:17:49,826 --> 00:17:51,795 And will eternally expand. 319 00:17:51,796 --> 00:17:56,298 Astronomer alex filippenko was on one team. 320 00:17:56,299 --> 00:17:58,901 Saul perlmutter led the other. 321 00:17:58,902 --> 00:18:01,938 We realized that it was possible for the first time 322 00:18:01,939 --> 00:18:05,608 To go and actually make a direct measurement 323 00:18:05,609 --> 00:18:08,111 Of how much the universe had been slowing down in the past. 324 00:18:08,313 --> 00:18:09,847 Both teams want to measure 325 00:18:09,848 --> 00:18:12,148 The speed of distant galaxies. 326 00:18:12,149 --> 00:18:16,020 But because the galaxies are too dim and too far away, 327 00:18:16,021 --> 00:18:18,057 They look for something brighter. 328 00:18:22,961 --> 00:18:27,431 Billions of light years from earth, a star detonates. 329 00:18:27,432 --> 00:18:30,100 This is a supernova, 330 00:18:30,101 --> 00:18:34,105 A dying star's brilliant final gasp. 331 00:18:34,106 --> 00:18:38,041 It burns brightly, 5 billion times brighter than the sun, 332 00:18:38,042 --> 00:18:40,712 But briefly. 333 00:18:40,713 --> 00:18:42,879 Perlmutter and filippenko have a window 334 00:18:42,880 --> 00:18:45,448 Of just one or two weeks to measure 335 00:18:45,449 --> 00:18:48,752 How much the galaxy it sits in is slowing down 336 00:18:48,753 --> 00:18:51,023 As it moves away from us. 337 00:18:55,128 --> 00:18:58,364 The teams look for supernovas for eight years. 338 00:18:58,365 --> 00:19:04,170 They measure 42, and the results seem impossible. 339 00:19:04,171 --> 00:19:06,771 We plotted the points on the graphs, 340 00:19:06,772 --> 00:19:09,508 And...it didn't make any sense. 341 00:19:09,509 --> 00:19:11,376 They were not slowing down at all. 342 00:19:11,377 --> 00:19:13,313 They were actually speeding up. 343 00:19:14,480 --> 00:19:18,084 What both groups found stunned the world. 344 00:19:18,085 --> 00:19:20,920 In the last 4 or 5 billion years, 345 00:19:20,921 --> 00:19:25,089 The universe has actually been speeding up in its expansion. 346 00:19:25,090 --> 00:19:26,925 An accelerating universe, 347 00:19:26,926 --> 00:19:30,896 Propelled by something mysterious. 348 00:19:30,897 --> 00:19:33,365 For so long, we've been arguing whether the universe would 349 00:19:33,366 --> 00:19:36,201 Expand forever or collapse back in on itself, 350 00:19:36,202 --> 00:19:38,570 But nobody thought the answer was going to be 351 00:19:38,571 --> 00:19:40,873 That the universe was accelerating, 352 00:19:40,874 --> 00:19:42,675 Going faster and faster all the time. 353 00:19:44,245 --> 00:19:47,615 The acceleration bewilders the scientists. 354 00:19:47,616 --> 00:19:50,718 It seems to defy the laws of physics. 355 00:19:50,719 --> 00:19:52,987 Imagine i've got a baseball 356 00:19:52,988 --> 00:19:54,654 And i throw it straight up. 357 00:19:54,655 --> 00:19:57,458 And instead of slowing down once it leaves my hand, 358 00:19:57,459 --> 00:19:59,292 Which is what normally it will do, 359 00:19:59,293 --> 00:20:01,161 It begins to slow down at first, 360 00:20:01,162 --> 00:20:03,064 But then it starts speeding away. 361 00:20:03,065 --> 00:20:04,699 Somehow, it's getting energy. 362 00:20:04,700 --> 00:20:10,170 The new energy seemed to be coming from nothing, 363 00:20:10,171 --> 00:20:12,405 The vacuum of space. 364 00:20:12,406 --> 00:20:16,176 The word "vacuum" to a scientist means completely empty space, 365 00:20:16,177 --> 00:20:18,778 No particles there at all, no temperature, 366 00:20:18,779 --> 00:20:20,379 No energy to speak of. 367 00:20:20,380 --> 00:20:23,683 But there's an intrinsic energy in space and time. 368 00:20:23,684 --> 00:20:27,386 Empty space has energy, and that energy produces 369 00:20:27,387 --> 00:20:30,523 A gravitational repulsion, a kind of anti-Gravity. 370 00:20:30,524 --> 00:20:34,962 Without a clue what this force is or how it works, 371 00:20:34,963 --> 00:20:40,534 All scientists can do is give it a name -- Dark energy. 372 00:20:40,903 --> 00:20:43,304 We could have called it we-Don't-Know energy. 373 00:20:43,305 --> 00:20:44,773 We could have called it anything. 374 00:20:44,774 --> 00:20:47,176 But we don't know what it is, and dark or not, 375 00:20:47,177 --> 00:20:49,311 It's the biggest mystery in physics. 376 00:20:52,480 --> 00:20:55,516 Nasa calibrates its finest space telescopes 377 00:20:55,517 --> 00:20:58,652 To measure how much dark energy is out there, 378 00:20:58,653 --> 00:21:01,989 And the result is mind-Blowing. 379 00:21:01,990 --> 00:21:06,795 It dominates the mass of the universe by nearly 3-To-1. 380 00:21:06,796 --> 00:21:08,462 And the more space expands, 381 00:21:08,463 --> 00:21:11,632 The more dark energy there seems to be. 382 00:21:11,633 --> 00:21:14,568 Dark energy is the energy of nothing, 383 00:21:14,569 --> 00:21:16,104 And it's repulsive. 384 00:21:16,105 --> 00:21:19,908 Therefore, as this dark energy repels galaxies, 385 00:21:19,909 --> 00:21:21,843 There's more of it, there's more vacuum. 386 00:21:21,844 --> 00:21:23,946 And so there's more repulsion, 387 00:21:23,947 --> 00:21:26,881 And perhaps that's the reason why the universe is accelerating 388 00:21:26,882 --> 00:21:30,218 Right now rather than slowing down. 389 00:21:30,219 --> 00:21:33,689 Dark energy seems to kill the big crunch theory, 390 00:21:33,690 --> 00:21:36,757 But scientists aren't yet sure how dark energy, 391 00:21:36,758 --> 00:21:40,295 Expansion, and space are connected. 392 00:21:40,296 --> 00:21:43,631 If a volume of space doubles in size, 393 00:21:43,632 --> 00:21:46,534 Does the dark energy inside it double, too? 394 00:21:46,535 --> 00:21:48,637 Or does it increase more? 395 00:21:48,638 --> 00:21:52,173 A 1-To-1 relationship leads to a steady expansion. 396 00:21:52,174 --> 00:21:55,310 The universe ends in a big freeze. 397 00:21:55,311 --> 00:21:59,881 But if dark energy increases above and beyond expansion, 398 00:21:59,882 --> 00:22:04,455 A new, even more terrifying end awaits the universe -- A big rip. 399 00:22:05,256 --> 00:22:09,291 In a big rip scenario, the expansion is so great 400 00:22:09,292 --> 00:22:13,496 That even the galaxies begin to expand internally, 401 00:22:13,497 --> 00:22:14,831 Which means that literally 402 00:22:14,832 --> 00:22:16,768 Our bodies are going to be ripped apart. 403 00:22:18,067 --> 00:22:19,568 Scientists calculate 404 00:22:19,569 --> 00:22:21,905 Just how the big rip will play out. 405 00:22:24,240 --> 00:22:28,310 One by one, the galaxies in the night sky will blink out 406 00:22:28,311 --> 00:22:31,279 As space pulls them away from the earth 407 00:22:31,280 --> 00:22:33,082 Faster than the speed of light. 408 00:22:34,786 --> 00:22:39,189 60 million years before the end, dark energy overcomes gravity 409 00:22:39,190 --> 00:22:42,124 On smaller and smaller scales. 410 00:22:42,125 --> 00:22:45,428 First galaxies start to rip apart, 411 00:22:45,429 --> 00:22:49,298 Then insides of galaxies will begin to rip apart, 412 00:22:49,299 --> 00:22:51,969 And then solar systems will begin to rip apart... 413 00:22:54,239 --> 00:22:57,208 then planets... 414 00:22:57,209 --> 00:23:02,614 and then rocks, people, atoms. 415 00:23:02,615 --> 00:23:05,918 The end will be mercifully quick. 416 00:23:07,219 --> 00:23:09,487 In the space of a few minutes, 417 00:23:09,488 --> 00:23:13,658 All the stars and planets in the universe will be destroyed, 418 00:23:13,659 --> 00:23:18,429 Their remains pulled apart into ever-Smaller pieces 419 00:23:18,430 --> 00:23:21,099 Until finally, when the universe has 420 00:23:21,100 --> 00:23:22,833 Less than a second to live, 421 00:23:22,834 --> 00:23:26,304 The subatomic particles that made all matter 422 00:23:26,305 --> 00:23:27,971 Will be destroyed, 423 00:23:27,972 --> 00:23:31,275 And all that remains will be individual photons 424 00:23:31,276 --> 00:23:33,577 Becoming scarcer and scarcer 425 00:23:33,578 --> 00:23:36,314 As the space between them expands. 426 00:23:36,315 --> 00:23:38,783 All you're left with is very low energy light 427 00:23:38,784 --> 00:23:40,252 That gets stretched and stretched 428 00:23:40,253 --> 00:23:42,354 Until it might as well not exist at all. 429 00:23:42,355 --> 00:23:44,354 The last thing to go -- 430 00:23:44,355 --> 00:23:47,859 The empty vacuum of space itself. 431 00:23:49,396 --> 00:23:51,897 It'll be pulling on the universe so hard, 432 00:23:51,898 --> 00:23:54,800 It could tear the fabric of the universe apart. 433 00:23:54,801 --> 00:23:58,203 Reality could dissolve. 434 00:23:58,204 --> 00:24:01,540 Will the universe end with a big rip, 435 00:24:01,541 --> 00:24:03,875 Or a big freeze? 436 00:24:03,876 --> 00:24:08,347 The answer is locked inside the mystery of dark energy. 437 00:24:08,348 --> 00:24:13,119 Solve that, and the fate of the universe becomes clear. 438 00:24:26,000 --> 00:24:28,366 The end of the universe is coming. 439 00:24:28,367 --> 00:24:30,537 But how will it play out? 440 00:24:30,538 --> 00:24:34,406 For a time, a big crunch was the likely answer. 441 00:24:34,407 --> 00:24:38,177 Dark matter, the invisible bulk of the universe, 442 00:24:38,178 --> 00:24:41,482 Causes space to fall in on itself. 443 00:24:42,750 --> 00:24:47,119 Galaxies collide. Planet merges with planet. 444 00:24:47,120 --> 00:24:51,892 Everything becomes hotter and hotter, denser and denser. 445 00:24:51,893 --> 00:24:54,462 The universe is like one giant star. 446 00:24:58,232 --> 00:25:02,268 Dark energy kills the big crunch theory. 447 00:25:02,269 --> 00:25:05,404 It acts like rocket fuel for the expansion of space 448 00:25:05,405 --> 00:25:07,641 Between galaxies. 449 00:25:07,642 --> 00:25:10,879 They're not just coasting. They're getting pushed outward. 450 00:25:14,213 --> 00:25:16,415 Only two possible fates remain -- 451 00:25:16,416 --> 00:25:19,118 A big rip or a big freeze. 452 00:25:19,119 --> 00:25:22,020 Both scenarios rely on dark energy. 453 00:25:22,021 --> 00:25:24,958 For the universe to be torn to shreds in a big rip, 454 00:25:24,959 --> 00:25:28,662 Dark energy must increase exponentially in the future. 455 00:25:28,663 --> 00:25:31,998 But a big freeze requires a steady increase 456 00:25:31,999 --> 00:25:33,500 In dark energy, 457 00:25:33,501 --> 00:25:35,402 Pushing galaxies away from each other. 458 00:25:35,503 --> 00:25:38,472 We can't write the last chapter of our universe 459 00:25:38,473 --> 00:25:41,944 Until we understand the nature of dark energy. 460 00:25:43,545 --> 00:25:46,414 May 2009. 461 00:25:46,415 --> 00:25:50,019 The european space agency launches the planck satellite 462 00:25:50,020 --> 00:25:53,921 To search for the birth of dark energy. 463 00:25:53,922 --> 00:25:58,392 Its ultra-Sensitive telescope peers through space and time 464 00:25:58,393 --> 00:26:00,928 Back through billions of years, 465 00:26:00,929 --> 00:26:05,500 Towards the beginning of everything, to capture this. 466 00:26:05,501 --> 00:26:08,003 This is our universe as it appeared 467 00:26:08,004 --> 00:26:10,938 Over 13 billion years ago, 468 00:26:10,939 --> 00:26:14,977 380,000 years after the big bang. 469 00:26:16,545 --> 00:26:19,147 So what planck has done is take a picture 470 00:26:19,148 --> 00:26:21,416 Of the early universe 471 00:26:21,417 --> 00:26:24,552 And told us about what the early universe is like 472 00:26:24,553 --> 00:26:26,988 And given us our most detailed and accurate picture 473 00:26:26,989 --> 00:26:28,322 Of that moment in time. 474 00:26:28,323 --> 00:26:30,757 The universe in this picture 475 00:26:30,758 --> 00:26:35,264 Is a hot soup of protons, electrons, and photons. 476 00:26:35,265 --> 00:26:38,332 Hydrogen atoms have just started to form, 477 00:26:38,333 --> 00:26:41,069 And it's the light from this genesis of matter 478 00:26:41,070 --> 00:26:42,938 That we see here. 479 00:26:45,007 --> 00:26:48,244 Blue areas are colder. Reds are warm. 480 00:26:48,378 --> 00:26:50,480 Eventually, those hot spots, 481 00:26:50,481 --> 00:26:52,682 Those red spots you see in the map, 482 00:26:52,683 --> 00:26:55,318 Are going to form large superclusters 483 00:26:55,319 --> 00:26:59,790 Made up of hundreds or thousands of galaxies. 484 00:26:59,791 --> 00:27:03,927 Each one of those galaxies will contain billions of stars. 485 00:27:05,561 --> 00:27:07,864 Gravity and expansion alone 486 00:27:07,865 --> 00:27:12,568 Appear to drive the formation of these embryonic galaxies. 487 00:27:12,569 --> 00:27:16,839 Dark energy doesn't seem to have switched on yet. 488 00:27:16,840 --> 00:27:21,678 So, when did dark energy take control of the universe? 489 00:27:28,185 --> 00:27:31,387 Astronomer brenda frye is part of a team 490 00:27:31,388 --> 00:27:33,991 Using massive ground-Based telescopes 491 00:27:33,992 --> 00:27:36,792 Like this one at kitt peak, arizona. 492 00:27:36,793 --> 00:27:41,164 She peers back in time to capture the universe 493 00:27:41,165 --> 00:27:44,069 Through its childhood as it was growing. 494 00:27:46,104 --> 00:27:48,672 Right. So this is an aluminum plate, 495 00:27:48,673 --> 00:27:52,875 And into this plate are drilled 640 individual holes. 496 00:27:52,876 --> 00:27:55,945 Each one is put at a very specific place on the mask 497 00:27:55,946 --> 00:28:00,017 Which will correspond to one particular galaxy in the sky. 498 00:28:02,386 --> 00:28:04,119 During each observation, 499 00:28:04,120 --> 00:28:08,625 The light from 640 individual galaxies is collected 500 00:28:08,626 --> 00:28:12,029 Using fiber optic cables. 501 00:28:12,030 --> 00:28:15,499 The speed and relative position of each galaxy is measured 502 00:28:15,500 --> 00:28:19,371 To pinpoint exactly where it is in space. 503 00:28:19,472 --> 00:28:22,107 So far, the team has accurately mapped 504 00:28:22,108 --> 00:28:24,943 Around a million galaxies in 3d, 505 00:28:24,944 --> 00:28:26,812 And this is what they look like. 506 00:28:28,046 --> 00:28:30,682 Each one of these fuzzy patches 507 00:28:30,683 --> 00:28:32,516 Is a fully grown galaxy 508 00:28:32,517 --> 00:28:36,553 Containing around 200 billion stars. 509 00:28:36,554 --> 00:28:38,223 This is a very basic measurement, 510 00:28:38,224 --> 00:28:40,390 And we think that this will be able to help us 511 00:28:40,391 --> 00:28:43,395 To get a grasp into the nature of dark energy. 512 00:28:43,396 --> 00:28:47,697 Scientists compare this adolescent universe 513 00:28:47,698 --> 00:28:49,567 To its baby pictures. 514 00:28:49,568 --> 00:28:51,802 It shows dark energy emerging 515 00:28:51,803 --> 00:28:55,008 When the universe is half as old as it is today. 516 00:28:56,276 --> 00:28:59,011 About 8 billion years after the big bang, 517 00:28:59,012 --> 00:29:03,248 This expansion of the universe begins to accelerate, 518 00:29:03,249 --> 00:29:05,884 And we're in the middle of this acceleration. 519 00:29:05,885 --> 00:29:10,589 The data also shows that as space expands, 520 00:29:10,590 --> 00:29:15,226 Dark energy increases in lockstep with it. 521 00:29:15,227 --> 00:29:17,562 If you had a box and you put some dark energy in it, 522 00:29:17,563 --> 00:29:19,898 And then you went and you weighed that box... 523 00:29:19,899 --> 00:29:21,800 now you take the box, you make it twice as big. 524 00:29:21,801 --> 00:29:23,668 You don't open it. You don't put anything in it. 525 00:29:23,669 --> 00:29:26,205 You weigh it again, it's gonna weigh twice as much. 526 00:29:26,206 --> 00:29:28,541 This remarkable observation means 527 00:29:28,542 --> 00:29:32,011 That we should be safe from a big rip. 528 00:29:32,012 --> 00:29:35,447 Dark energy will continue to increase gradually. 529 00:29:35,448 --> 00:29:39,016 The universe is heading for a big freeze, 530 00:29:39,017 --> 00:29:43,054 And scientists can finally calculate a timeline 531 00:29:43,055 --> 00:29:45,925 For the end of everything. 532 00:29:55,102 --> 00:29:56,637 It now seems that we live 533 00:29:56,638 --> 00:29:59,272 In an almost perfect universe, 534 00:29:59,273 --> 00:30:02,842 With just enough gravity to hold the galaxies together 535 00:30:02,843 --> 00:30:06,748 And just enough dark energy that it will expand forever 536 00:30:06,749 --> 00:30:09,385 Without ripping itself to shreds. 537 00:30:11,320 --> 00:30:15,992 Cosmologists can finally envision the end of it all. 538 00:30:17,326 --> 00:30:19,894 30 years ago, it was debatable. 539 00:30:19,895 --> 00:30:22,762 But now, it appears that the universe most likely 540 00:30:22,763 --> 00:30:24,331 Will suffer a deep freeze. 541 00:30:24,332 --> 00:30:27,637 If you look at the data, it stares out at you. 542 00:30:28,803 --> 00:30:30,370 In a big freeze, 543 00:30:30,371 --> 00:30:34,509 Dark energy pushes galaxies further and further apart, 544 00:30:34,510 --> 00:30:37,380 But they remain intact. 545 00:30:37,413 --> 00:30:41,083 The stars inside them fade away. 546 00:30:41,084 --> 00:30:43,619 Every star you see in the sky, including our sun, 547 00:30:43,620 --> 00:30:45,722 Is burning through its nuclear fuel. 548 00:30:45,723 --> 00:30:48,923 The gas will run out, stars will stop being made, 549 00:30:48,924 --> 00:30:52,562 And the ones that exist are it. Those are the last ones. 550 00:30:56,967 --> 00:30:59,267 A hundred trillion years from now, 551 00:30:59,268 --> 00:31:03,573 The biggest stars will be the first to go extinct. 552 00:31:03,574 --> 00:31:06,708 Big stars burn bright and die hard. 553 00:31:06,709 --> 00:31:11,147 The star's core collapses, 554 00:31:11,148 --> 00:31:13,284 Unleashing a supernova. 555 00:31:14,584 --> 00:31:17,920 Then gravity crushes the dead star down 556 00:31:17,921 --> 00:31:20,590 To a single dense spot. 557 00:31:20,591 --> 00:31:24,027 The bright star is now a black hole. 558 00:31:26,397 --> 00:31:28,967 Sun-Like stars go next. 559 00:31:30,434 --> 00:31:33,035 As their supply of hydrogen runs out, 560 00:31:33,036 --> 00:31:35,405 They swell to a bloated fireball 561 00:31:35,406 --> 00:31:38,342 Over 200 times their current size. 562 00:31:44,215 --> 00:31:46,450 And when the core has no more hydrogen, 563 00:31:46,451 --> 00:31:49,720 It's going to bloat up into a red giant star. 564 00:31:49,721 --> 00:31:52,089 Now, red giant stars are so big, they will actually 565 00:31:52,090 --> 00:31:54,090 Eat up their own planets. 566 00:31:54,091 --> 00:31:55,925 We know of examples of red giants 567 00:31:55,926 --> 00:31:57,994 That go all the way out to where the orbit of jupiter is 568 00:31:57,995 --> 00:31:59,929 In our solar system. 569 00:31:59,930 --> 00:32:02,899 Its fuel exhausted, 570 00:32:02,900 --> 00:32:05,602 The sun-Like star gives in to gravity 571 00:32:05,603 --> 00:32:07,704 And shrinks to a white dwarf, 572 00:32:07,705 --> 00:32:09,473 A dense ball of matter 573 00:32:09,474 --> 00:32:12,608 Just a few thousand miles in diameter. 574 00:32:12,609 --> 00:32:16,647 It will glow with heat for a further 10 billion years 575 00:32:16,648 --> 00:32:19,215 Before cooling to a black dwarf, 576 00:32:19,216 --> 00:32:24,255 A ball of compressed carbon, perhaps even diamond. 577 00:32:26,959 --> 00:32:29,293 As the biggest stars die, 578 00:32:29,294 --> 00:32:32,830 The universe will slowly turn red. 579 00:32:32,831 --> 00:32:34,598 The blue stars will blow up, 580 00:32:34,599 --> 00:32:36,767 And then the slightly less blue stars will blow up, 581 00:32:36,768 --> 00:32:39,136 And then stars like the sun will fade away and die, 582 00:32:39,137 --> 00:32:41,808 Leaving just the red stars to exist. 583 00:32:43,376 --> 00:32:45,211 Red stars are the smallest 584 00:32:45,212 --> 00:32:47,113 And coolest in the universe. 585 00:32:47,114 --> 00:32:49,382 They burn their fuel slowly. 586 00:32:49,383 --> 00:32:52,116 But, after another 10 trillion years, 587 00:32:52,117 --> 00:32:54,520 Even these smallest of dwarf stars 588 00:32:54,521 --> 00:32:56,789 Will use up their fuel. 589 00:32:56,790 --> 00:33:00,358 Stars as we know them will cease to burn energy, 590 00:33:00,359 --> 00:33:02,828 And the night sky will turn black. 591 00:33:02,829 --> 00:33:06,699 Black holes, the corpses of dead stars, 592 00:33:06,700 --> 00:33:11,338 And cold clouds of gas and dust are all that remains. 593 00:33:13,140 --> 00:33:15,909 The age of stars is over. 594 00:33:15,910 --> 00:33:19,645 The age of black holes begins. 595 00:33:19,646 --> 00:33:21,848 Black holes become the fundamental building block 596 00:33:21,849 --> 00:33:23,515 Of the universe. 597 00:33:23,516 --> 00:33:25,884 A galaxy will basically be a supermassive black hole 598 00:33:25,885 --> 00:33:27,919 In the center, with smaller black holes orbiting it. 599 00:33:27,920 --> 00:33:30,455 In some ways, it's kind of a ghost universe. 600 00:33:30,456 --> 00:33:32,292 It's the corpses, the zombie stars, 601 00:33:32,293 --> 00:33:33,993 That will take us into the future. 602 00:33:33,994 --> 00:33:37,163 Zombie galaxies filled with black holes 603 00:33:37,164 --> 00:33:38,964 Continue to evolve. 604 00:33:38,965 --> 00:33:42,335 They sweep up the dead remains of stars. 605 00:33:42,336 --> 00:33:46,439 Black hole merges with black hole. 606 00:33:46,440 --> 00:33:48,540 They'll eat each other and they'll get bigger, 607 00:33:48,541 --> 00:33:50,375 And maybe they'll fall into the supermassive black hole 608 00:33:50,376 --> 00:33:51,844 And it'll get bigger. 609 00:33:51,845 --> 00:33:54,846 The universe will still be an exciting, dynamic place, 610 00:33:54,847 --> 00:33:57,149 It's just that the time scales you're talking about 611 00:33:57,150 --> 00:33:58,718 Are now trillions of years 612 00:33:58,719 --> 00:34:01,420 Instead of thousands or millions of years. 613 00:34:01,421 --> 00:34:05,591 Any material that evades the pull of a black hole 614 00:34:05,592 --> 00:34:10,862 Eventually dies away as its protons disintegrate. 615 00:34:10,863 --> 00:34:14,000 A proton, one of the fundamental building blocks 616 00:34:14,001 --> 00:34:16,835 Of atomic matter, of what makes us up, 617 00:34:16,836 --> 00:34:19,337 Can just spontaneously fall apart, 618 00:34:19,338 --> 00:34:23,210 And it turns out this takes a tremendously long time. 619 00:34:23,211 --> 00:34:25,310 But even that will go away. 620 00:34:25,311 --> 00:34:30,382 All that will be left is a sea of black holes. 621 00:34:30,383 --> 00:34:33,652 Scientists used to think black holes were immortal, 622 00:34:33,653 --> 00:34:35,323 But even these will one day die. 623 00:34:35,424 --> 00:34:38,125 Now we're talking about time scales 624 00:34:38,126 --> 00:34:39,794 Of unimaginable length -- 625 00:34:39,795 --> 00:34:42,331 Quadrillions of years into the future. 626 00:34:42,432 --> 00:34:43,898 But on that time scale, 627 00:34:43,899 --> 00:34:48,001 Even the black holes begin to evaporate. 628 00:34:48,002 --> 00:34:50,238 They'll get smaller and smaller and smaller, 629 00:34:50,239 --> 00:34:52,173 And then, poof, they'll be gone. 630 00:34:52,174 --> 00:34:54,642 The universe will end 631 00:34:54,643 --> 00:34:57,477 When the last remaining black hole dies. 632 00:34:57,478 --> 00:35:00,280 As it gets smaller, the evaporation rate 633 00:35:00,281 --> 00:35:02,316 Increases exponentially. 634 00:35:02,317 --> 00:35:04,517 Before long, it reaches a size 635 00:35:04,518 --> 00:35:09,523 A billionth of a trillionth of a trillionth of an inch. 636 00:35:09,524 --> 00:35:12,927 At that instant, the laws of physics break down, 637 00:35:12,928 --> 00:35:17,097 And the last black hole explodes in a flash of gamma rays, 638 00:35:17,098 --> 00:35:19,867 Leaving nothing. 639 00:35:19,868 --> 00:35:23,470 And it will die in a sudden burst of light, 640 00:35:23,471 --> 00:35:25,139 The last burst of light 641 00:35:25,140 --> 00:35:27,475 In the entire history of the universe. 642 00:35:28,111 --> 00:35:30,112 The big freeze is coming. 643 00:35:30,113 --> 00:35:34,416 The universe will suffer a cold, slow, dark death 644 00:35:34,417 --> 00:35:35,784 Which will play out 645 00:35:35,785 --> 00:35:39,521 Over trillions upon trillions of years. 646 00:35:39,522 --> 00:35:42,925 But quantum physics leaves the door open 647 00:35:42,926 --> 00:35:44,693 For an alternative end, 648 00:35:44,694 --> 00:35:48,130 An event so powerful, so destructive, 649 00:35:48,131 --> 00:35:53,836 That it could destroy everything we see in the blink of an eye. 650 00:35:53,837 --> 00:35:57,007 And it could happen tomorrow. 651 00:36:06,251 --> 00:36:08,085 The end of the universe -- 652 00:36:08,086 --> 00:36:09,618 It's coming. 653 00:36:09,619 --> 00:36:13,022 Dark energy accelerates the space between galaxies, 654 00:36:13,023 --> 00:36:16,593 Pushing everything we see to a long, cold, 655 00:36:16,594 --> 00:36:19,330 And very slow death. 656 00:36:19,331 --> 00:36:23,199 Unless, that is, something bizarre happens first. 657 00:36:23,200 --> 00:36:27,004 A monster called phase transition 658 00:36:27,005 --> 00:36:28,638 Is lurking in the shadows, 659 00:36:28,639 --> 00:36:32,576 And it could annihilate the fabric of space and time 660 00:36:32,577 --> 00:36:35,678 At any moment. 661 00:36:35,679 --> 00:36:39,449 When we cool down water, it turns into ice. 662 00:36:39,450 --> 00:36:40,951 The properties change. 663 00:36:40,952 --> 00:36:43,154 If you lived in the water, when it changed to ice, 664 00:36:43,155 --> 00:36:44,989 Your world would be very different. 665 00:36:44,990 --> 00:36:50,194 Water phase changes into ice when it loses energy. 666 00:36:50,195 --> 00:36:53,230 I once left a water bottle in my car overnight. 667 00:36:53,231 --> 00:36:56,132 It was still liquid, but the moment i touched it, 668 00:36:56,133 --> 00:36:57,533 The slight imperfection, 669 00:36:57,534 --> 00:36:59,402 The little bit of ice that it formed, spread, 670 00:36:59,403 --> 00:37:01,270 Poof, and filled up the whole bottle. 671 00:37:01,271 --> 00:37:04,474 That rapid change to something new 672 00:37:04,475 --> 00:37:06,644 Is called a phase transition, 673 00:37:06,645 --> 00:37:12,048 And bizarrely, the same thing could happen to empty space. 674 00:37:12,049 --> 00:37:14,753 We've really come to understand 675 00:37:14,754 --> 00:37:17,956 That we shouldn't take for granted that...vacuum, 676 00:37:17,957 --> 00:37:20,691 What we call nothing, is actually stable. 677 00:37:20,692 --> 00:37:23,594 It could be that the energy stored in empty space 678 00:37:23,595 --> 00:37:26,398 Is just waiting to be released in a phase transition. 679 00:37:26,399 --> 00:37:29,535 If it is, the laws of physics will change. 680 00:37:31,404 --> 00:37:35,106 A spontaneous glitch in the fabric of space-Time 681 00:37:35,107 --> 00:37:39,010 Could trigger a phase transition of space, 682 00:37:39,011 --> 00:37:43,414 A tiny bubble of new universe that spreads out, 683 00:37:43,415 --> 00:37:45,715 Overwriting the old. 684 00:37:45,716 --> 00:37:49,387 We know it can happen, because it's happened before. 685 00:37:53,192 --> 00:37:55,193 At the moment of the big bang, 686 00:37:55,194 --> 00:37:57,262 The universe that's first created 687 00:37:57,263 --> 00:38:00,632 Is completely different to the one we see today. 688 00:38:00,633 --> 00:38:03,568 Hot and without form, 689 00:38:03,569 --> 00:38:06,170 There's no matter, no time. 690 00:38:06,171 --> 00:38:09,740 The laws of physics are different. 691 00:38:09,741 --> 00:38:13,445 Suddenly, less than a trillionth of a second later, 692 00:38:13,446 --> 00:38:16,514 A glitch triggers a phase transition. 693 00:38:16,515 --> 00:38:20,152 A tiny bubble of the universe we live in today forms, 694 00:38:20,153 --> 00:38:22,387 And it races outward, 695 00:38:22,388 --> 00:38:24,356 Destroying everything it touches 696 00:38:24,357 --> 00:38:27,525 Like ice spreading through water. 697 00:38:27,526 --> 00:38:31,262 The energy that spills out creates the space and time 698 00:38:31,263 --> 00:38:32,898 That we exist in, 699 00:38:32,899 --> 00:38:37,503 The building blocks of matter and the forces that govern them. 700 00:38:37,504 --> 00:38:40,239 All that energy was released, producing all the matter 701 00:38:40,240 --> 00:38:42,175 And radiation we observe in the universe today. 702 00:38:42,375 --> 00:38:45,211 The old universe gives up its energy 703 00:38:45,212 --> 00:38:46,847 To create the new. 704 00:38:46,848 --> 00:38:48,982 But it holds some back. 705 00:38:48,983 --> 00:38:53,419 The vacuum of space still has energy bound to it. 706 00:38:53,420 --> 00:38:57,957 Perhaps this is the dark energy we see today. 707 00:38:57,958 --> 00:39:01,261 Physicists believe that someday in the future, 708 00:39:01,262 --> 00:39:04,763 A brand new glitch in the fabric of space-Time 709 00:39:04,764 --> 00:39:07,300 May trigger another phase transition, 710 00:39:07,301 --> 00:39:10,870 One that wipes us and everything we see 711 00:39:10,871 --> 00:39:12,805 Out of existence. 712 00:39:12,806 --> 00:39:16,309 This is a way to destroy an entire universe, 713 00:39:16,310 --> 00:39:18,077 Because within your universe 714 00:39:18,078 --> 00:39:20,579 Are the seeds of its own destruction. 715 00:39:20,580 --> 00:39:23,550 It would spread out at the speed of light in a death bubble, 716 00:39:23,551 --> 00:39:26,519 Ruining all the galaxies as it passes through, 717 00:39:26,520 --> 00:39:29,822 And ultimately completely destroying our universe. 718 00:39:29,823 --> 00:39:33,327 Nothing can survive the expanding phase transition. 719 00:39:33,328 --> 00:39:38,132 Planets, nebulas, galaxies -- All are ripped apart 720 00:39:38,133 --> 00:39:40,434 As the boundary of the bubble reaches them. 721 00:39:40,435 --> 00:39:43,670 Inside this bubble, protons are unstable, 722 00:39:43,671 --> 00:39:47,507 Atoms begin to rearrange in a new form of matter. 723 00:39:47,508 --> 00:39:49,543 As these bubbles begin to expand, 724 00:39:49,544 --> 00:39:52,179 A new universe is being born 725 00:39:52,180 --> 00:39:54,847 In the corpse of the old universe, 726 00:39:54,848 --> 00:39:58,186 And the beginning of a new law of physics. 727 00:39:58,387 --> 00:40:02,022 And so, the expanding universe we now see 728 00:40:02,023 --> 00:40:05,460 May end in a phase transition, but we won't know what hit us, 729 00:40:05,461 --> 00:40:07,395 'Cause the laws of physics will change, 730 00:40:07,396 --> 00:40:10,131 And we will essentially most likely disappear 731 00:40:10,132 --> 00:40:11,899 At the instant it happens. 732 00:40:11,900 --> 00:40:15,569 This bubble will expand at the speed of light, 733 00:40:15,570 --> 00:40:17,439 And as the bubble passes you, 734 00:40:17,440 --> 00:40:20,475 All the atoms of your body rearrange themselves, 735 00:40:20,476 --> 00:40:22,178 And you would never know it. 736 00:40:22,179 --> 00:40:24,879 You would have no warning, because the bubble itself 737 00:40:24,880 --> 00:40:26,448 Is expanding at the speed of light. 738 00:40:26,449 --> 00:40:29,052 You can't predict precisely when it could happen. 739 00:40:29,053 --> 00:40:30,684 You only have a probability. 740 00:40:30,685 --> 00:40:32,921 So what you really are predicting is a rate. 741 00:40:32,922 --> 00:40:36,092 Does it happen once a year? Once every 10 billion years? 742 00:40:36,093 --> 00:40:38,325 Once every googol years? Or whatever. 743 00:40:38,326 --> 00:40:41,628 It's very possible that these bubbles get nucleated 744 00:40:41,629 --> 00:40:45,267 And grow about once every 10 or 20 billion years. 745 00:40:45,268 --> 00:40:47,903 So it hasn't happened yet because we got lucky. 746 00:40:47,904 --> 00:40:50,840 It's unlikely it would happen the next year or the next day, 747 00:40:50,841 --> 00:40:52,908 But the laws of physics absolutely allow it. 748 00:40:56,245 --> 00:41:00,516 A phase change may happen, or it may not. 749 00:41:01,650 --> 00:41:05,790 The universe plays its cards close to its chest. 750 00:41:09,625 --> 00:41:12,829 And, like dark energy and dark matter, 751 00:41:12,830 --> 00:41:14,799 There may be more surprises to come... 752 00:41:16,600 --> 00:41:21,470 ...surprises that will only add to the mystery and wonder 753 00:41:21,471 --> 00:41:24,108 Our universe holds for us. 754 00:41:27,478 --> 00:41:29,113 Whatever the universe is up to, 755 00:41:29,114 --> 00:41:30,479 We still don't know enough. 756 00:41:30,480 --> 00:41:32,582 We're in an age of discovery right now. 757 00:41:32,583 --> 00:41:34,483 Perhaps there is something else out there 758 00:41:34,484 --> 00:41:35,852 That we don't know about. 759 00:41:35,853 --> 00:41:38,255 So, i'm not going to draw any conclusions 760 00:41:38,256 --> 00:41:39,957 Until things are conclusive. 761 00:41:42,659 --> 00:41:45,160 We don't understand the nature of dark energy. 762 00:41:45,161 --> 00:41:48,765 And without that understanding, virtually anything is possible. 763 00:41:48,766 --> 00:41:50,800 The future is still uncertain, 764 00:41:50,801 --> 00:41:53,135 And that means there's still a mystery. 765 00:41:53,136 --> 00:41:56,507 And for me, that's the most exciting possibility of all. 61288

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