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These are the user uploaded subtitles that are being translated: 0 00:00:00,010 --> 00:00:07,777 SUB BY : DENI AUROR@ https://aurorarental.blogspot.com/ 1 00:00:02,902 --> 00:00:05,737 Two black holes circle each other 2 00:00:05,739 --> 00:00:08,640 in a dance of death. 3 00:00:08,642 --> 00:00:10,642 They spiral inwards, 4 00:00:10,644 --> 00:00:14,246 their immense gravities pulling them ever closer. 5 00:00:17,984 --> 00:00:19,417 When they finally collide, 6 00:00:19,419 --> 00:00:22,020 it's one of the most powerful events 7 00:00:22,022 --> 00:00:25,357 since the big bang. 8 00:00:25,359 --> 00:00:27,526 This explosive mystery 9 00:00:27,528 --> 00:00:31,462 sends ripples across the world of science. 10 00:00:31,464 --> 00:00:33,098 But can it also answer 11 00:00:33,100 --> 00:00:37,102 one of the most pressing questions in cosmology? 12 00:00:37,104 --> 00:00:42,307 How do supermassive black holes grow so large? 13 00:00:45,312 --> 00:00:48,513 Captions paid for by discovery communications 14 00:00:58,692 --> 00:00:59,958 in the known universe, 15 00:00:59,960 --> 00:01:04,529 there are roughly 2,000 billion galaxies. 16 00:01:04,531 --> 00:01:07,833 Each one has a different shape and size. 17 00:01:07,835 --> 00:01:11,637 But they may all have one feature in common ... 18 00:01:11,639 --> 00:01:17,076 a supermassive black hole buried at their center. 19 00:01:17,078 --> 00:01:20,145 As its name says, it is supermassive. 20 00:01:20,147 --> 00:01:21,580 And here, we're talking about objects 21 00:01:21,582 --> 00:01:24,182 that are millions or billions of times 22 00:01:24,184 --> 00:01:25,818 the mass of the sun. 23 00:01:28,855 --> 00:01:30,522 Supermassive black holes 24 00:01:30,524 --> 00:01:33,125 are so big that we need a special scale 25 00:01:33,127 --> 00:01:34,626 for measuring them. 26 00:01:37,297 --> 00:01:39,431 A solar mass is the mass of the sun. 27 00:01:39,433 --> 00:01:42,868 So when we study the universe, 28 00:01:42,870 --> 00:01:44,803 we have to use the tools that we have in hand. 29 00:01:44,805 --> 00:01:47,439 And what's the most massive thing that we have around us? 30 00:01:47,441 --> 00:01:49,508 It's the sun. And so we refer to things 31 00:01:49,510 --> 00:01:51,643 in multiples of the mass of the sun 32 00:01:51,645 --> 00:01:55,314 because it just makes it easier to wrap our heads around. 33 00:01:55,316 --> 00:01:57,616 However, if you have something that's 17 billion times 34 00:01:57,618 --> 00:01:59,952 the mass of the sun, that's pretty difficult 35 00:01:59,954 --> 00:02:02,086 to wrap your head around anyway. 36 00:02:02,088 --> 00:02:04,156 But we know that those kinds of black holes 37 00:02:04,158 --> 00:02:07,926 live in the centers of galaxies. 38 00:02:07,928 --> 00:02:11,463 The supermassive black hole at the center of our galaxy, 39 00:02:11,465 --> 00:02:15,500 the milky way, is called sagittarius "a"-star. 40 00:02:15,502 --> 00:02:19,404 It weighs in at 4 million solar masses. 41 00:02:19,406 --> 00:02:22,106 But compared to the other supermassive black holes 42 00:02:22,108 --> 00:02:24,810 out there, it's puny. 43 00:02:24,812 --> 00:02:27,078 This is probably one of the only contexts 44 00:02:27,080 --> 00:02:30,381 where you would think that our supermassive black hole 45 00:02:30,383 --> 00:02:32,150 isn't very supermassive. 46 00:02:34,820 --> 00:02:36,155 The supermassive black hole 47 00:02:36,157 --> 00:02:38,456 in our neighboring galaxy, Andromeda, 48 00:02:38,458 --> 00:02:42,727 is 25 times larger than sagittarius "a"-star, 49 00:02:42,729 --> 00:02:46,632 coming in at 100 million solar masses. 50 00:02:46,634 --> 00:02:48,700 But compared to the largest monsters 51 00:02:48,702 --> 00:02:51,703 out in the universe, it's a runt. 52 00:02:51,705 --> 00:02:55,874 O.j. 287's primary supermassive black hole 53 00:02:55,876 --> 00:03:00,078 weighs in at 18 billion solar masses. 54 00:03:00,080 --> 00:03:04,583 And the black hole in the core of galaxy ngc 4889 55 00:03:04,585 --> 00:03:08,886 in the coma cluster weighs 21 billion solar stars. 56 00:03:08,888 --> 00:03:11,056 That's over 5,000 times larger 57 00:03:11,058 --> 00:03:13,091 than sagittarius "a"-star. 58 00:03:15,094 --> 00:03:16,728 These are incredible things 59 00:03:16,730 --> 00:03:21,366 that are more massive than some galaxies. 60 00:03:21,368 --> 00:03:25,938 Now astronomers may have made a remarkable discovery ... 61 00:03:25,940 --> 00:03:29,141 a giant, new supermassive black hole 62 00:03:29,143 --> 00:03:32,410 that's a mind-blowing 30 billion times 63 00:03:32,412 --> 00:03:34,079 the mass of the sun. 64 00:03:34,081 --> 00:03:35,413 It's a huge puzzle. 65 00:03:35,415 --> 00:03:40,185 And we have simply no idea how it got so big. 66 00:03:40,187 --> 00:03:44,222 It's a huge mystery how black holes have become so enormous. 67 00:03:44,224 --> 00:03:46,157 We started finding black holes with millions 68 00:03:46,159 --> 00:03:48,527 and billions of times the sun's mass. 69 00:03:48,529 --> 00:03:49,927 No one expected that. 70 00:03:49,929 --> 00:03:53,798 And we have no idea how they got to be so big. 71 00:03:53,800 --> 00:03:56,434 It's not entirely clear at this point 72 00:03:56,436 --> 00:04:00,004 how supermassive black holes can get to be the masses 73 00:04:00,006 --> 00:04:01,273 that they are today. 74 00:04:07,714 --> 00:04:09,881 Regular-sized black holes form 75 00:04:09,883 --> 00:04:13,651 when large stars over 20 times the mass of our sun 76 00:04:13,653 --> 00:04:15,053 crash and burn. 77 00:04:17,190 --> 00:04:19,124 When a large star runs out of fuel, 78 00:04:19,126 --> 00:04:22,327 the core stops generating enough outward force 79 00:04:22,329 --> 00:04:26,231 to counteract the power of gravity crushing inwards. 80 00:04:26,233 --> 00:04:27,766 As the star collapses, 81 00:04:27,768 --> 00:04:31,236 the outer part explodes in a supernova. 82 00:04:36,776 --> 00:04:38,744 The inner core shrinks 83 00:04:38,746 --> 00:04:41,746 from a sphere millions of miles wide 84 00:04:41,748 --> 00:04:44,449 to one just 10 miles across. 85 00:04:47,387 --> 00:04:49,187 It's like shrinking the earth down 86 00:04:49,189 --> 00:04:53,225 to the size of a golf ball. 87 00:04:53,227 --> 00:04:57,862 This rapid collapse creates a black hole. 88 00:04:57,864 --> 00:04:59,464 So we now have seen black holes 89 00:04:59,466 --> 00:05:01,833 that are solar-mass black holes 90 00:05:01,835 --> 00:05:03,268 and black holes that are million 91 00:05:03,270 --> 00:05:05,036 or billion-solar-mass black holes. 92 00:05:05,038 --> 00:05:08,406 And the question is, how do you get from one to the other? 93 00:05:10,977 --> 00:05:12,844 Do the giants somehow grow 94 00:05:12,846 --> 00:05:16,181 from a solar-mass black hole? 95 00:05:16,183 --> 00:05:18,316 Bullock: One of the big puzzles today is, 96 00:05:18,318 --> 00:05:21,986 how do you make one of these supermassive black holes? 97 00:05:21,988 --> 00:05:24,456 One idea is, you get there by starting 98 00:05:24,458 --> 00:05:26,324 with a solar-mass black hole, 99 00:05:26,326 --> 00:05:27,725 having it grow through a stage 100 00:05:27,727 --> 00:05:29,294 of being an intermediate-mass black hole 101 00:05:29,296 --> 00:05:30,895 and then eventually getting to be 102 00:05:30,897 --> 00:05:33,799 a supermassive black hole. 103 00:05:33,801 --> 00:05:36,835 Theoretically, intermediate-mass black holes 104 00:05:36,837 --> 00:05:41,239 should be between 100 and 100,000 solar masses. 105 00:05:41,241 --> 00:05:43,908 But we've never seen one. 106 00:05:43,910 --> 00:05:46,111 Part of the mystery of supermassive black holes 107 00:05:46,113 --> 00:05:49,147 is that black holes seem to occur in two flavors. 108 00:05:49,149 --> 00:05:50,982 You have ones that are only a couple times 109 00:05:50,984 --> 00:05:52,117 the mass of the sun. 110 00:05:52,119 --> 00:05:53,752 And you have ones that are millions 111 00:05:53,754 --> 00:05:55,954 or billions of times the mass of the sun. 112 00:05:55,956 --> 00:05:59,358 So we have small and extra large. 113 00:05:59,360 --> 00:06:01,559 If we think of the stellar-mass black hole 114 00:06:01,561 --> 00:06:02,961 as sort of the baby black holes, 115 00:06:02,963 --> 00:06:06,297 and the supermassive black holes as the grown-up black holes, 116 00:06:06,299 --> 00:06:07,966 we're missing the teenage black holes. 117 00:06:07,968 --> 00:06:09,968 Where are these black holes that have masses 118 00:06:09,970 --> 00:06:13,405 that are between stellar mass and supermassive? 119 00:06:15,641 --> 00:06:17,642 Bullock: They're sort of like a holy grail 120 00:06:17,644 --> 00:06:19,511 for black hole hunters. 121 00:06:19,513 --> 00:06:21,613 Where are these things? Where can we find them? 122 00:06:21,615 --> 00:06:24,216 And how do you make them? 123 00:06:24,218 --> 00:06:27,085 Then astronomers caught a break. 124 00:06:27,087 --> 00:06:29,254 They picked up a burst of energy 125 00:06:29,256 --> 00:06:34,760 coming from the ngc 1399 galaxy. 126 00:06:34,762 --> 00:06:35,594 It was the death throes 127 00:06:35,596 --> 00:06:40,298 of a star being eaten by a black hole. 128 00:06:40,300 --> 00:06:42,633 When they measured its size, they discovered it was 129 00:06:42,635 --> 00:06:45,937 an elusive intermediate-mass black hole. 130 00:06:45,939 --> 00:06:49,841 The missing link had been found. 131 00:06:49,843 --> 00:06:51,910 But when scientists did the math 132 00:06:51,912 --> 00:06:55,180 to see if such an intermediate-mass black hole 133 00:06:55,182 --> 00:06:58,049 could grow into a supermassive black hole, 134 00:06:58,051 --> 00:06:59,751 they hit a snag. 135 00:06:59,753 --> 00:07:01,753 There hasn't been enough time 136 00:07:01,755 --> 00:07:03,488 since the birth of the universe 137 00:07:03,490 --> 00:07:05,790 for an intermediate-mass black hole 138 00:07:05,792 --> 00:07:07,659 to eat enough stars 139 00:07:07,661 --> 00:07:10,962 to grow into a supermassive black hole. 140 00:07:10,964 --> 00:07:13,431 Bullock: It doesn't seem like there's enough time 141 00:07:13,433 --> 00:07:17,101 for black holes to get as big as we see them. 142 00:07:17,103 --> 00:07:20,772 But supermassives are everywhere we look. 143 00:07:20,774 --> 00:07:22,106 How did they get there? 144 00:07:22,108 --> 00:07:24,543 And how did they grow so huge? 145 00:07:38,591 --> 00:07:42,060 In our universe, we've detected small black holes. 146 00:07:42,062 --> 00:07:44,262 And we've seen monsters, 147 00:07:44,264 --> 00:07:46,497 supermassive black holes 148 00:07:46,499 --> 00:07:49,267 billions of times the mass of our sun. 149 00:07:49,269 --> 00:07:53,371 But we'd found almost none in between. 150 00:07:53,373 --> 00:07:58,009 So how do you get from a small black hole to a giant one? 151 00:07:58,011 --> 00:08:00,111 One of the most important outstanding questions 152 00:08:00,113 --> 00:08:01,313 in cosmology is, 153 00:08:01,315 --> 00:08:03,281 how did supermassive black holes 154 00:08:03,283 --> 00:08:04,915 get as big as they are? 155 00:08:04,917 --> 00:08:08,019 And when did that happen? 156 00:08:08,021 --> 00:08:12,023 Black holes are normally surrounded by gas and stars, 157 00:08:12,025 --> 00:08:15,393 an all-you-can-eat buffet. 158 00:08:15,395 --> 00:08:17,595 One of the best ideas for how black holes grow 159 00:08:17,597 --> 00:08:18,830 is that black holes do 160 00:08:18,832 --> 00:08:20,464 what we expect black holes to do, 161 00:08:20,466 --> 00:08:21,699 and that is eat stuff. 162 00:08:21,701 --> 00:08:23,034 For a black hole, 163 00:08:23,036 --> 00:08:25,370 it's almost as if the universe is its restaurant. 164 00:08:25,372 --> 00:08:29,074 And on its menu, you'll find stars, planets, 165 00:08:29,076 --> 00:08:32,010 and clouds of gas and dust. 166 00:08:32,012 --> 00:08:33,979 So is binge-eating the answer 167 00:08:33,981 --> 00:08:37,315 to growing a supermassive black hole? 168 00:08:37,317 --> 00:08:40,819 Theoretically, black holes should keep on growing forever 169 00:08:40,821 --> 00:08:43,821 as they consume more and more food. 170 00:08:43,823 --> 00:08:45,656 But recent discoveries suggest 171 00:08:45,658 --> 00:08:48,393 that the universe puts them on a diet, 172 00:08:48,395 --> 00:08:50,695 controlling how much they eat. 173 00:08:50,697 --> 00:08:52,597 Black holes are hungry. They like to eat. 174 00:08:52,599 --> 00:08:54,032 But sometimes, they eat too much, 175 00:08:54,034 --> 00:08:55,667 and they burp it up. 176 00:09:04,142 --> 00:09:06,144 February 2015. 177 00:09:06,146 --> 00:09:08,880 Astronomers report something unusual 178 00:09:08,882 --> 00:09:12,217 in the galaxy ngc 2276. 179 00:09:14,621 --> 00:09:17,288 it looked like something had taken a bite 180 00:09:17,290 --> 00:09:19,557 out of one of its spiral arms. 181 00:09:21,226 --> 00:09:22,827 Sitting alone in the void 182 00:09:22,829 --> 00:09:25,162 was an intermediate-mass black hole, 183 00:09:25,164 --> 00:09:29,834 about 50,000 times the mass of the sun. 184 00:09:29,836 --> 00:09:31,702 One theory was that the black hole 185 00:09:31,704 --> 00:09:33,738 had eaten everything around it, 186 00:09:33,740 --> 00:09:35,807 creating the dead zone. 187 00:09:35,809 --> 00:09:37,909 But the detection of a burst of energy 188 00:09:37,911 --> 00:09:39,543 from the black hole suggests 189 00:09:39,545 --> 00:09:41,613 it may have tried to eat too much 190 00:09:41,615 --> 00:09:45,183 and, in the process, destroyed its food source, 191 00:09:45,185 --> 00:09:48,820 burping so hard, its food was blasted away. 192 00:09:54,594 --> 00:09:57,529 Turns out that black holes are actually very messy eaters. 193 00:09:57,531 --> 00:10:00,932 A lot of matter gets thrown off as it tries to absorb it. 194 00:10:00,934 --> 00:10:02,967 So things move in, gets hot. 195 00:10:02,969 --> 00:10:06,804 But then a lot of it gets thrown all the way back out. 196 00:10:06,806 --> 00:10:09,106 Isler: Black holes are not vacuums in space. 197 00:10:09,108 --> 00:10:11,309 They do not just eat everything around them. 198 00:10:11,311 --> 00:10:13,645 And so they are messy. Some things get in. 199 00:10:13,647 --> 00:10:15,547 And they take that on. And it grows their mass. 200 00:10:15,549 --> 00:10:20,151 And some things are just flung out as they're eating. 201 00:10:20,153 --> 00:10:23,855 The enormous gravity of black holes sucks gas, dust, 202 00:10:23,857 --> 00:10:25,690 and even stars towards them. 203 00:10:25,692 --> 00:10:28,025 Everybody's been to an all-you-can-eat buffet. 204 00:10:28,027 --> 00:10:30,261 But let's be honest. There really is a limit 205 00:10:30,263 --> 00:10:32,563 to how much you can eat. 206 00:10:32,565 --> 00:10:35,767 Black holes are gluttons. They're greedy. 207 00:10:35,769 --> 00:10:38,703 They don't really know when they've eaten too much. 208 00:10:38,705 --> 00:10:42,807 They just keep on cramming in more and more food. 209 00:10:42,809 --> 00:10:44,175 It doesn't just fall in. 210 00:10:44,177 --> 00:10:46,744 It has to go down the drain, more or less. 211 00:10:46,746 --> 00:10:50,080 And so it forms this disk around the hole. 212 00:10:50,082 --> 00:10:52,150 And as it does that, there's a lot of turbulence 213 00:10:52,152 --> 00:10:53,351 and magnetic fields 214 00:10:53,353 --> 00:10:55,987 and a witch's brew of forces going on there 215 00:10:55,989 --> 00:10:59,090 that get it really hot. 216 00:10:59,092 --> 00:11:01,526 As the gas and dust swirls around, 217 00:11:01,528 --> 00:11:03,027 it heats up, 218 00:11:03,029 --> 00:11:06,431 pushing temperatures to millions of degrees fahrenheit. 219 00:11:10,035 --> 00:11:12,637 This swirl, called the accretion disk, 220 00:11:12,639 --> 00:11:15,606 also generates powerful magnetic fields. 221 00:11:17,743 --> 00:11:20,712 These fields are dragged by the spin of the black hole 222 00:11:20,714 --> 00:11:25,015 and become focused above the poles. 223 00:11:25,017 --> 00:11:26,150 As energy builds up, 224 00:11:26,152 --> 00:11:28,753 the magnetic fields become so compressed 225 00:11:28,755 --> 00:11:33,658 they blast out super-energized particles. 226 00:11:33,660 --> 00:11:36,627 These beams can actually be incredibly violent. 227 00:11:36,629 --> 00:11:38,062 Matter is flung out 228 00:11:38,064 --> 00:11:40,531 at a large fraction of the speed of light. 229 00:11:40,533 --> 00:11:42,133 It's a tremendous wind 230 00:11:42,135 --> 00:11:46,271 that blows very hard away from the black hole. 231 00:11:46,273 --> 00:11:48,106 The jet hits the gas clouds 232 00:11:48,108 --> 00:11:49,674 surrounding the black hole, 233 00:11:49,676 --> 00:11:52,143 blowing the buffet away. 234 00:11:52,145 --> 00:11:54,478 If they eat too much, 235 00:11:54,480 --> 00:11:56,281 they can basically blow everything 236 00:11:56,283 --> 00:11:58,483 that's in their vicinity away. 237 00:11:58,485 --> 00:12:03,054 They lose their food supply. And then they're gonna starve. 238 00:12:03,056 --> 00:12:05,656 They can kind of shoot themselves in the foot. 239 00:12:05,658 --> 00:12:07,558 With no food available, 240 00:12:07,560 --> 00:12:09,994 the black hole stops growing. 241 00:12:09,996 --> 00:12:12,330 Astronomers think that's what happened 242 00:12:12,332 --> 00:12:14,098 to the intermediate-mass black hole 243 00:12:14,100 --> 00:12:16,067 they discovered in the dead zone. 244 00:12:21,440 --> 00:12:23,775 These burps may regulate star formation 245 00:12:23,777 --> 00:12:28,079 and stop the black hole from getting obese. 246 00:12:28,081 --> 00:12:29,647 But over time, 247 00:12:29,649 --> 00:12:31,749 the black hole will start eating again 248 00:12:31,751 --> 00:12:34,285 as gas falls back towards it. 249 00:12:34,287 --> 00:12:37,355 But can an intermediate-mass black hole eat enough 250 00:12:37,357 --> 00:12:39,991 to become a supermassive black hole 251 00:12:39,993 --> 00:12:43,495 weighing billions of solar masses? 252 00:12:43,497 --> 00:12:47,198 Could that black hole become so obese by eating? 253 00:12:47,200 --> 00:12:49,066 That's a really interesting question. 254 00:12:49,068 --> 00:12:51,636 You'd have to eat a heck of a lot 255 00:12:51,638 --> 00:12:54,839 to get that fat. 256 00:12:54,841 --> 00:12:57,675 When you think about it, if you imagine an average galaxy 257 00:12:57,677 --> 00:12:59,676 has 100 billion stars, 258 00:12:59,678 --> 00:13:01,479 the black hole would have to eat one 259 00:13:01,481 --> 00:13:04,081 in every five stars in the galaxy. 260 00:13:04,083 --> 00:13:06,785 The universe is old. But is it really old enough 261 00:13:06,787 --> 00:13:10,688 that black holes have had time to consume billions of stars? 262 00:13:10,690 --> 00:13:12,690 That seems kind of unlikely. 263 00:13:12,692 --> 00:13:14,425 Bullock: It doesn't seem to add up. 264 00:13:14,427 --> 00:13:15,960 We need some other way 265 00:13:15,962 --> 00:13:17,962 to make these supermassive black holes. 266 00:13:17,964 --> 00:13:21,065 And the question is, what is that? 267 00:13:21,067 --> 00:13:23,734 Maybe we've been making this all too complicated. 268 00:13:23,736 --> 00:13:28,406 Maybe to get a big black hole is to start big in the first place. 269 00:13:28,408 --> 00:13:31,876 So how can black holes start big? 270 00:13:31,878 --> 00:13:35,280 To answer that question, scientists had to journey back 271 00:13:35,282 --> 00:13:37,849 to the very start of the universe, 272 00:13:37,851 --> 00:13:41,419 to a mysterious time called the dark ages. 273 00:14:01,006 --> 00:14:03,441 As we look out into the universe, 274 00:14:03,443 --> 00:14:08,012 we're seeing farther and farther back in time. 275 00:14:08,014 --> 00:14:09,313 We have now looked back 276 00:14:09,315 --> 00:14:12,449 over 12 billion years 277 00:14:12,451 --> 00:14:15,920 to the time when the cosmos was still an infant. 278 00:14:15,922 --> 00:14:21,225 And what we found was a huge surprise. 279 00:14:21,227 --> 00:14:22,827 We had made the assumption 280 00:14:22,829 --> 00:14:25,129 that as you look farther out into the universe, 281 00:14:25,131 --> 00:14:26,464 the black holes would be smaller. 282 00:14:26,466 --> 00:14:28,166 They haven't had much time to grow. 283 00:14:28,168 --> 00:14:30,801 But now we've found a 12-billion-solar-mass 284 00:14:30,803 --> 00:14:33,104 black hole that's actually less 285 00:14:33,106 --> 00:14:34,772 than a billion years into the universe. 286 00:14:34,774 --> 00:14:36,641 How did this thing form so early? 287 00:14:36,643 --> 00:14:38,176 How did it grow so fast? 288 00:14:38,178 --> 00:14:40,577 This is like walking into a delivery room 289 00:14:40,579 --> 00:14:42,747 and finding a 100-pound baby. 290 00:14:42,749 --> 00:14:45,449 I mean, how does that even happen? 291 00:14:45,451 --> 00:14:47,084 It doesn't make any sense. 292 00:14:47,086 --> 00:14:51,155 Physics tells us no black hole could swallow enough stuff 293 00:14:51,157 --> 00:14:54,392 to get that big that quickly. 294 00:14:54,394 --> 00:14:56,794 There really wasn't enough time between the big bang 295 00:14:56,796 --> 00:14:58,763 and when we're studying these things 296 00:14:58,765 --> 00:15:01,299 for them to grow to such large sizes 297 00:15:01,301 --> 00:15:03,902 just by eating matter around them. 298 00:15:03,904 --> 00:15:07,839 So if there's not enough time for them to grow so large, 299 00:15:07,841 --> 00:15:12,109 maybe they're born supermassive. 300 00:15:12,111 --> 00:15:17,214 To understand how, we have to travel back even farther, 301 00:15:17,216 --> 00:15:20,084 to not long after the birth of the universe. 302 00:15:22,822 --> 00:15:24,888 isler: The early universe was definitely 303 00:15:24,890 --> 00:15:27,492 a much more compact 304 00:15:27,494 --> 00:15:29,093 and richer place for material. 305 00:15:29,095 --> 00:15:31,462 It was smaller, and it was denser. 306 00:15:31,464 --> 00:15:33,464 Things were much closer. It was hotter. 307 00:15:33,466 --> 00:15:38,869 It was just a much more intense place to be. 308 00:15:38,871 --> 00:15:43,274 Clouds of hydrogen and helium gas clumped together. 309 00:15:43,276 --> 00:15:46,577 As the clouds grew, so did their gravity, 310 00:15:46,579 --> 00:15:50,114 sucking in more and more gas. 311 00:15:50,116 --> 00:15:51,783 Eventually, the ball of gas 312 00:15:51,785 --> 00:15:54,819 became so dense, it collapsed, 313 00:15:54,821 --> 00:15:58,789 triggering nuclear fusion. 314 00:15:58,791 --> 00:16:00,892 A star was born. 315 00:16:00,894 --> 00:16:03,494 These massive first stars 316 00:16:03,496 --> 00:16:07,098 are called population III stars. 317 00:16:07,100 --> 00:16:09,500 Because there was so much food around, 318 00:16:09,502 --> 00:16:12,503 these stars were huge, 319 00:16:12,505 --> 00:16:16,774 many times bigger than any stars that exist today. 320 00:16:16,776 --> 00:16:19,310 Bullock: We think a lot of these population III stars 321 00:16:19,312 --> 00:16:21,579 probably were incredibly massive, 322 00:16:21,581 --> 00:16:24,782 incredibly short-lived, and just blew up right away. 323 00:16:24,784 --> 00:16:28,219 They would've left massive black holes behind. 324 00:16:39,398 --> 00:16:41,065 With so much food available, 325 00:16:41,067 --> 00:16:45,036 these young, ravenous black holes, called quasars, 326 00:16:45,038 --> 00:16:47,505 started binge-eating 327 00:16:47,507 --> 00:16:50,408 and became incredibly bright. 328 00:16:50,410 --> 00:16:54,212 Billions of years later, we can still see their gluttony. 329 00:16:56,215 --> 00:16:59,383 The most luminous, bright objects in the universe 330 00:16:59,385 --> 00:17:00,918 are things called quasars. 331 00:17:00,920 --> 00:17:02,319 And it may seem kind of ironic. 332 00:17:02,321 --> 00:17:05,389 But what these really are are supermassive black holes. 333 00:17:05,391 --> 00:17:07,392 There's so much stuff trying to cram itself down 334 00:17:07,394 --> 00:17:10,961 the black hole that everything gets very hot, very energetic. 335 00:17:10,963 --> 00:17:13,597 And you can see them clear across the universe. 336 00:17:13,599 --> 00:17:16,567 But when we measured the size of the young quasars, 337 00:17:16,569 --> 00:17:20,705 we discovered they were already billions of solar masses. 338 00:17:20,707 --> 00:17:22,573 Isler: There's not enough time, 339 00:17:22,575 --> 00:17:25,043 a billion years after the universe was created, 340 00:17:25,045 --> 00:17:28,512 for them to get to a billion solar masses in ... 341 00:17:28,514 --> 00:17:30,714 it's just too short a time. 342 00:17:30,716 --> 00:17:33,684 Bullock: So the question becomes, how do you make black holes 343 00:17:33,686 --> 00:17:36,888 that are this big in that small amount of time? 344 00:17:36,890 --> 00:17:38,089 We need some other way 345 00:17:38,091 --> 00:17:40,624 of growing these supermassive black holes. 346 00:17:40,626 --> 00:17:42,559 There needs to be some other mechanism 347 00:17:42,561 --> 00:17:44,829 that allows them to get that massive so early. 348 00:17:44,831 --> 00:17:47,731 But what is that? 349 00:17:47,733 --> 00:17:52,803 A clue can be found in the very early universe. 350 00:17:52,805 --> 00:17:55,473 The early universe is still so much of a mystery to us. 351 00:17:55,475 --> 00:17:57,475 We know that conditions were very different. 352 00:17:57,477 --> 00:18:00,545 It was denser. There was a lot more material. 353 00:18:00,547 --> 00:18:03,815 This period is called the dark ages. 354 00:18:03,817 --> 00:18:05,616 Bullock: During the dark age, we know 355 00:18:05,618 --> 00:18:08,452 that there was basically nothing happening. 356 00:18:08,454 --> 00:18:09,720 Matter existed. 357 00:18:09,722 --> 00:18:11,856 We think that there was hydrogen and helium gas 358 00:18:11,858 --> 00:18:14,758 but really not much else. 359 00:18:14,760 --> 00:18:16,760 There were a few stars around, 360 00:18:16,762 --> 00:18:20,097 but nothing large enough to form giant black holes. 361 00:18:20,099 --> 00:18:22,967 But there were huge clouds of gas. 362 00:18:22,969 --> 00:18:26,070 And because the universe was much smaller and denser, 363 00:18:26,072 --> 00:18:29,740 the clouds were much thicker. 364 00:18:29,742 --> 00:18:33,043 The idea is that from these basic ingredients, 365 00:18:33,045 --> 00:18:34,912 gravity and gas, 366 00:18:34,914 --> 00:18:38,983 the cosmos built massive black holes. 367 00:18:38,985 --> 00:18:41,218 Somehow, the universe has created a shortcut 368 00:18:41,220 --> 00:18:42,253 to the black hole. 369 00:18:42,255 --> 00:18:44,188 We've typically thought of it as, 370 00:18:44,190 --> 00:18:46,424 cloud of gas collapses into a star, 371 00:18:46,426 --> 00:18:49,960 star evolves, star dies, leaves behind a black hole. 372 00:18:49,962 --> 00:18:51,596 Perhaps the universe has found a way 373 00:18:51,598 --> 00:18:53,697 to skip the star phase 374 00:18:53,699 --> 00:18:55,599 and go directly to the black hole. 375 00:18:58,737 --> 00:19:03,407 Clouds of gas may have built massive black holes 376 00:19:03,409 --> 00:19:06,944 in a process called direct collapse. 377 00:19:06,946 --> 00:19:09,780 As they collapsed, they never even formed a star. 378 00:19:09,782 --> 00:19:12,783 They just collapsed straight into a giant black hole. 379 00:19:12,785 --> 00:19:14,351 Through this direct collapse theory, 380 00:19:14,353 --> 00:19:16,687 you can form really big black holes. 381 00:19:16,689 --> 00:19:19,189 Imagine what it's like seeing one of these giant clouds 382 00:19:19,191 --> 00:19:21,359 of gas collapsing down into a black hole. 383 00:19:21,361 --> 00:19:23,294 You might think you start with, okay, 384 00:19:23,296 --> 00:19:25,296 cloud of gas slowly collapsing, 385 00:19:25,298 --> 00:19:27,231 and, boop, it's a black hole. 386 00:19:27,233 --> 00:19:29,466 That wouldn't be the case. It would be more like 387 00:19:29,468 --> 00:19:31,702 giant cloud of gas starts collapsing, 388 00:19:31,704 --> 00:19:34,638 then ... aah! ... Black hole. 389 00:19:34,640 --> 00:19:36,707 It's believed that direct collapse 390 00:19:36,709 --> 00:19:38,609 could have created black holes 391 00:19:38,611 --> 00:19:41,412 up to a million times the mass of the sun, 392 00:19:41,414 --> 00:19:43,214 much bigger than from the collapse 393 00:19:43,216 --> 00:19:44,882 of a single star. 394 00:19:44,884 --> 00:19:46,317 Bullock: These early black holes 395 00:19:46,319 --> 00:19:48,619 are sort of like the galaxies that never were. 396 00:19:48,621 --> 00:19:50,054 They were gonna make galaxies. 397 00:19:50,056 --> 00:19:53,457 But instead, they collapsed into very massive black holes. 398 00:19:55,460 --> 00:19:58,094 For direct collapse to form a black hole, 399 00:19:58,096 --> 00:20:01,299 the conditions need to be precise. 400 00:20:01,301 --> 00:20:04,035 The clouds must be very symmetrical, 401 00:20:04,037 --> 00:20:06,571 forming a smooth ball. 402 00:20:06,573 --> 00:20:09,406 If you have a ball of gas that isn't quite a ball, 403 00:20:09,408 --> 00:20:11,175 that's not quite homogeneous, 404 00:20:11,177 --> 00:20:13,243 as it collapses, it'll fragment. 405 00:20:13,245 --> 00:20:15,613 And it'll fragment into objects that won't form black holes. 406 00:20:15,615 --> 00:20:18,249 So you want it to be hot enough 407 00:20:18,251 --> 00:20:22,119 that it stays one big, giant thing. 408 00:20:22,121 --> 00:20:23,954 But it does need to cool a little bit, right, 409 00:20:23,956 --> 00:20:26,824 so that you get it to collapse in on itself. 410 00:20:30,295 --> 00:20:34,064 You have to get uniform collapse over time 411 00:20:34,066 --> 00:20:37,401 of a very large amount of hydrogen gas, presumably, 412 00:20:37,403 --> 00:20:40,604 which is the original matter in the universe, 413 00:20:40,606 --> 00:20:43,907 collapsing spherically symmetrically, 414 00:20:43,909 --> 00:20:45,643 without fragmenting, 415 00:20:45,645 --> 00:20:49,380 over a period of less than 500 million years. 416 00:20:55,153 --> 00:20:57,622 Direct collapse may have created black holes 417 00:20:57,624 --> 00:21:00,224 a million times the mass of the sun. 418 00:21:00,226 --> 00:21:02,126 But it can't completely explain 419 00:21:02,128 --> 00:21:06,697 the 12 billion solar-mass supermassive black holes 420 00:21:06,699 --> 00:21:09,300 we see in the early universe. 421 00:21:09,302 --> 00:21:13,703 Maybe gigantic supermassive black holes were created 422 00:21:13,705 --> 00:21:16,774 by strange, unseen forces. 423 00:21:16,776 --> 00:21:18,675 Maybe they were created 424 00:21:18,677 --> 00:21:22,079 by the mysterious dark universe. 425 00:21:35,126 --> 00:21:39,229 Astronomers looking deep into the early universe 426 00:21:39,231 --> 00:21:43,868 have discovered gigantic supermassive black holes. 427 00:21:43,870 --> 00:21:45,602 Bullock: This is a pretty deep mystery. 428 00:21:45,604 --> 00:21:47,671 There are these supermassive black holes 429 00:21:47,673 --> 00:21:49,606 that exist in the very early universe. 430 00:21:49,608 --> 00:21:52,609 And by all accounts, they should not exist. 431 00:21:52,611 --> 00:21:55,312 According to the normal laws of physics, 432 00:21:55,314 --> 00:21:56,647 it shouldn't have been possible 433 00:21:56,649 --> 00:21:59,650 for them to grow so big so quickly. 434 00:21:59,652 --> 00:22:02,653 For astrophysicists, understanding how black holes 435 00:22:02,655 --> 00:22:06,023 have grown to be so large is one of our biggest mysteries. 436 00:22:06,025 --> 00:22:07,625 Bullock: We need some other way 437 00:22:07,627 --> 00:22:09,693 of growing these supermassive black holes. 438 00:22:09,695 --> 00:22:11,495 There needs to be some other mechanism 439 00:22:11,497 --> 00:22:14,030 that allows them to get that massive so early. 440 00:22:14,032 --> 00:22:16,433 But what is that? 441 00:22:16,435 --> 00:22:18,903 Everything we can see in the night sky 442 00:22:18,905 --> 00:22:21,371 makes up just 4.8% 443 00:22:21,373 --> 00:22:24,107 of all the matter in the cosmos. 444 00:22:24,109 --> 00:22:26,410 The rest is the dark universe, 445 00:22:26,412 --> 00:22:28,746 including dark matter. 446 00:22:28,748 --> 00:22:33,083 We can't see it, feel it, or detect it directly. 447 00:22:33,085 --> 00:22:35,753 But we know dark matter is there. 448 00:22:35,755 --> 00:22:39,456 Its gravity is tugging on everything around it. 449 00:22:39,458 --> 00:22:41,058 And we're beginning to understand 450 00:22:41,060 --> 00:22:43,160 it plays a fundamental role 451 00:22:43,162 --> 00:22:45,662 in the formation of the universe. 452 00:22:45,664 --> 00:22:47,965 Most of the stuff that collects together 453 00:22:47,967 --> 00:22:49,933 gravitationally is dark matter. 454 00:22:49,935 --> 00:22:52,736 So perhaps black holes form 455 00:22:52,738 --> 00:22:55,673 somehow with the inclusion of dark matter. 456 00:22:55,675 --> 00:22:57,508 One way of looking at it is there's six times 457 00:22:57,510 --> 00:22:59,110 as much dark matter as normal matter. 458 00:22:59,112 --> 00:23:01,712 So there's six times as much food out there 459 00:23:01,714 --> 00:23:03,047 for the black holes to eat 460 00:23:03,049 --> 00:23:05,850 if they're able to tap into this dark stuff. 461 00:23:05,852 --> 00:23:08,852 Maybe these supermassive black holes are growing 462 00:23:08,854 --> 00:23:11,021 by eating dark matter. 463 00:23:11,023 --> 00:23:13,891 There are some tantalizing clues. 464 00:23:13,893 --> 00:23:16,526 The largest supermassive black holes 465 00:23:16,528 --> 00:23:19,563 don't live in the galaxies with the most regular matter. 466 00:23:19,565 --> 00:23:23,366 They live in the galaxies with the most dark matter. 467 00:23:23,368 --> 00:23:26,136 The one thing we know about dark matter right now 468 00:23:26,138 --> 00:23:28,071 is that it has gravity. 469 00:23:28,073 --> 00:23:30,074 And a black hole runs on gravity. 470 00:23:30,076 --> 00:23:31,709 It attracts anything with mass. 471 00:23:31,711 --> 00:23:33,577 So there's no reason to assume 472 00:23:33,579 --> 00:23:35,912 that black holes would only eat regular matter. 473 00:23:35,914 --> 00:23:40,251 And now we know that there's far more dark matter out there. 474 00:23:40,253 --> 00:23:45,322 Maybe dark matter helps the black holes eat. 475 00:23:45,324 --> 00:23:47,825 Maybe in some ways, dark matter is a feeder 476 00:23:47,827 --> 00:23:50,161 for these supermassive black holes. 477 00:23:50,163 --> 00:23:53,063 Perhaps what really grows a supermassive black hole 478 00:23:53,065 --> 00:23:56,133 is all of the regular matter being directed into the center 479 00:23:56,135 --> 00:23:59,103 by the dark matter around it. 480 00:23:59,105 --> 00:24:02,106 Maybe the dark matter's powerful gravity 481 00:24:02,108 --> 00:24:03,908 sucks in regular matter 482 00:24:03,910 --> 00:24:07,511 and funnels it into the black hole. 483 00:24:07,513 --> 00:24:10,548 In a sense, the dark matter is greasing the wheels. 484 00:24:10,550 --> 00:24:12,282 It's sort of tilting the table up 485 00:24:12,284 --> 00:24:14,384 so that that food can slide right in. 486 00:24:18,124 --> 00:24:21,091 But now scientists think the dark matter 487 00:24:21,093 --> 00:24:25,028 may create gigantic black holes directly 488 00:24:25,030 --> 00:24:29,333 by igniting dark stars. 489 00:24:29,335 --> 00:24:30,968 Some believe that dark matter 490 00:24:30,970 --> 00:24:33,704 sparked early universe super stars. 491 00:24:33,706 --> 00:24:39,009 When they die, they leave behind supermassive black holes. 492 00:24:39,011 --> 00:24:40,511 Dark stars sound like 493 00:24:40,513 --> 00:24:42,546 they come from the fertile imagination 494 00:24:42,548 --> 00:24:44,615 of some Sci-Fi writer. 495 00:24:44,617 --> 00:24:47,684 But Dr. Katie freese believes they may explain 496 00:24:47,686 --> 00:24:53,056 how early supermassive black holes grew so fast. 497 00:24:53,058 --> 00:24:54,491 Dark stars are amazing. 498 00:24:54,493 --> 00:24:56,893 So, when we first had this idea, 499 00:24:56,895 --> 00:24:58,195 we got excited really quickly, 500 00:24:58,197 --> 00:25:00,464 because this is a new type of star 501 00:25:00,466 --> 00:25:03,667 that has never been seen before. 502 00:25:03,669 --> 00:25:06,437 Dark stars may have been some of the first stars 503 00:25:06,439 --> 00:25:08,672 to form in the universe. 504 00:25:08,674 --> 00:25:09,873 They sparked into life 505 00:25:09,875 --> 00:25:14,078 when the universe was just 200 million years old. 506 00:25:14,080 --> 00:25:19,616 But how could dark stars form really massive black holes? 507 00:25:19,618 --> 00:25:24,488 A newborn black hole can't weigh more than its parent star. 508 00:25:24,490 --> 00:25:28,792 So in order to give birth to a really massive black hole, 509 00:25:28,794 --> 00:25:33,297 the parent star has to be supermassive, as well. 510 00:25:33,299 --> 00:25:35,833 Freese: These early objects are really strange. 511 00:25:35,835 --> 00:25:38,001 They're very cool. 512 00:25:38,003 --> 00:25:40,437 And they're really, really big. 513 00:25:40,439 --> 00:25:43,874 The size of these things is 10 times the distance 514 00:25:43,876 --> 00:25:46,476 between the sun and the earth. 515 00:25:48,679 --> 00:25:51,215 But how is that possible? 516 00:25:51,217 --> 00:25:55,619 Regular stars have an upper size limit. 517 00:25:55,621 --> 00:25:59,389 A star is a battle between gravity pushing inwards 518 00:25:59,391 --> 00:26:01,725 and nuclear fusion pushing out. 519 00:26:05,162 --> 00:26:06,730 When the star grows too big, 520 00:26:06,732 --> 00:26:11,101 its gravity becomes overwhelming. 521 00:26:11,103 --> 00:26:12,703 The delicate balance 522 00:26:12,705 --> 00:26:16,640 between gravity and fusion is broken. 523 00:26:16,642 --> 00:26:21,544 Gravity wins out, and the star collapses. 524 00:26:21,546 --> 00:26:24,414 But dark stars may have a work-around 525 00:26:24,416 --> 00:26:28,686 that lets them become supermassive. 526 00:26:28,688 --> 00:26:30,654 Freese: So, they are made of ordinary matter. 527 00:26:30,656 --> 00:26:33,256 They're made of hydrogen and helium. 528 00:26:33,258 --> 00:26:36,226 But they're powered by dark matter. 529 00:26:36,228 --> 00:26:39,196 We don't know what dark matter is made from. 530 00:26:39,198 --> 00:26:44,301 But we do have theories on how it might power a star. 531 00:26:44,303 --> 00:26:46,903 Freese: One of the best ideas we have for dark matter 532 00:26:46,905 --> 00:26:50,908 is that it's made of weakly interacting massive particles, 533 00:26:50,910 --> 00:26:52,977 or wimps for short. 534 00:26:52,979 --> 00:26:55,378 So, these wimps are their own antimatter. 535 00:26:55,380 --> 00:26:57,915 And that means, whenever they encounter each other, 536 00:26:57,917 --> 00:27:01,818 they annihilate and turn into something else. 537 00:27:01,820 --> 00:27:04,621 That means a lot of heat is released, a lot of energy. 538 00:27:04,623 --> 00:27:07,958 And it's that energy that could power stars. 539 00:27:10,895 --> 00:27:13,364 The energy from the wimps' annihilations 540 00:27:13,366 --> 00:27:18,101 keeps the star from collapsing like a normal star. 541 00:27:18,103 --> 00:27:20,404 Bullock: So it's possible that, in some stars, 542 00:27:20,406 --> 00:27:22,205 their internal reactions 543 00:27:22,207 --> 00:27:25,242 are actually being powered by dark matter. 544 00:27:25,244 --> 00:27:28,144 If that's the case, then you could imagine situations 545 00:27:28,146 --> 00:27:29,646 where, when that burns out, 546 00:27:29,648 --> 00:27:32,616 you produce very massive black holes. 547 00:27:32,618 --> 00:27:34,251 So it could be that dark matter, 548 00:27:34,253 --> 00:27:35,652 the physics of dark matter, 549 00:27:35,654 --> 00:27:38,955 plays really important roles in creating black holes 550 00:27:38,957 --> 00:27:41,491 and their prevalence in the universe. 551 00:27:49,668 --> 00:27:51,935 The energy from the dark matter 552 00:27:51,937 --> 00:27:56,907 allows the dark stars to grow huge. 553 00:27:56,909 --> 00:27:58,575 When they first form, they're small. 554 00:27:58,577 --> 00:28:01,512 They're about the mass of the sun. 555 00:28:01,514 --> 00:28:03,546 But because they're so cool, 556 00:28:03,548 --> 00:28:04,848 they keep accumulating matter 557 00:28:04,850 --> 00:28:06,416 and growing, growing, growing. 558 00:28:06,418 --> 00:28:08,852 And some of them will get to be a million times 559 00:28:08,854 --> 00:28:13,356 as massive as the sun and a billion times as bright. 560 00:28:13,358 --> 00:28:15,893 But these giants don't live for long. 561 00:28:15,895 --> 00:28:18,294 Eventually, the dark matter particles 562 00:28:18,296 --> 00:28:20,698 wipe each other out completely. 563 00:28:20,700 --> 00:28:22,198 And there is no more fuel 564 00:28:22,200 --> 00:28:24,835 to keep the massive amount of ordinary matter 565 00:28:24,837 --> 00:28:27,371 from collapsing. 566 00:28:27,373 --> 00:28:28,806 And then that's it. 567 00:28:28,808 --> 00:28:31,442 There's nothing to sustain this big, puffy object. 568 00:28:31,444 --> 00:28:36,346 If it's big enough, you collapse directly to a black hole. 569 00:28:36,348 --> 00:28:40,951 A monster supermassive black hole. 570 00:28:40,953 --> 00:28:43,287 Bullock: It's really fun to think about the possibility 571 00:28:43,289 --> 00:28:44,755 that the physics of dark matter 572 00:28:44,757 --> 00:28:47,157 is actually helping to power stars. 573 00:28:47,159 --> 00:28:48,892 If so, it would bring, you know, 574 00:28:48,894 --> 00:28:51,328 a whole new window into our understanding 575 00:28:51,330 --> 00:28:53,597 of stars and their evolution. 576 00:28:56,134 --> 00:29:00,771 At the moment, dark stars are just theoretical. 577 00:29:00,773 --> 00:29:03,607 But when the powerful James webb telescope 578 00:29:03,609 --> 00:29:05,909 comes online in 2018, 579 00:29:05,911 --> 00:29:08,011 we may get our first glimpse. 580 00:29:09,914 --> 00:29:13,616 Freese: We're gonna do an observing run and look for these things. 581 00:29:13,618 --> 00:29:14,551 And so we're very excited. 582 00:29:14,553 --> 00:29:16,686 If you would find an entirely new type of star, 583 00:29:16,688 --> 00:29:19,923 that would be huge. 584 00:29:19,925 --> 00:29:22,459 While Katie freese looks for dark stars, 585 00:29:22,461 --> 00:29:26,196 another team is investigating another radical idea 586 00:29:26,198 --> 00:29:27,997 that offers new insight 587 00:29:27,999 --> 00:29:33,370 into how supermassive black holes grow so huge. 588 00:29:33,372 --> 00:29:35,705 They detect the faint echoes 589 00:29:35,707 --> 00:29:39,809 of a violent event from across the universe, 590 00:29:39,811 --> 00:29:43,280 the remnants of an extraordinary collision, 591 00:29:43,282 --> 00:29:45,215 a supremely energetic event 592 00:29:45,217 --> 00:29:49,486 that reveals black holes are cannibals. 593 00:30:04,102 --> 00:30:06,803 Our universe is filled with enormous 594 00:30:06,805 --> 00:30:11,508 supermassive black holes that defy explanation. 595 00:30:11,510 --> 00:30:13,443 Supermassive black holes are one of the things 596 00:30:13,445 --> 00:30:15,512 in the universe that, when you run the physics, 597 00:30:15,514 --> 00:30:17,780 when you run the math of how did they evolve, 598 00:30:17,782 --> 00:30:19,849 they really shouldn't be there. 599 00:30:19,851 --> 00:30:22,853 It's still a profound mystery. 600 00:30:22,855 --> 00:30:24,855 The universe hasn't been around long enough 601 00:30:24,857 --> 00:30:26,323 for regular black holes 602 00:30:26,325 --> 00:30:29,759 to eat enough matter to get supermassive. 603 00:30:29,761 --> 00:30:31,795 So how did they get so big? 604 00:30:31,797 --> 00:30:33,197 The most logical answer 605 00:30:33,199 --> 00:30:36,333 is that large black holes are born large, 606 00:30:36,335 --> 00:30:39,202 around 1 to 2 billion solar masses. 607 00:30:39,204 --> 00:30:41,771 But that's still over 10 times smaller 608 00:30:41,773 --> 00:30:46,242 than the largest supermassive black holes out there. 609 00:30:46,244 --> 00:30:48,311 Bullock: Given the time scales, it doesn't seem to add up. 610 00:30:48,313 --> 00:30:49,980 We need some other way 611 00:30:49,982 --> 00:30:52,081 to make these supermassive black holes. 612 00:30:52,083 --> 00:30:53,950 And the question is, what is that? 613 00:30:56,254 --> 00:30:59,790 A clue came from a large, isolated galaxy 614 00:30:59,792 --> 00:31:02,092 200 million light-years away 615 00:31:02,094 --> 00:31:04,394 in a quiet part of the universe. 616 00:31:06,331 --> 00:31:10,200 nestling alone was a supermassive black hole 617 00:31:10,202 --> 00:31:15,472 with a mass of 17 billion suns. 618 00:31:15,474 --> 00:31:17,073 Normally, such monsters 619 00:31:17,075 --> 00:31:19,943 are found in dense regions of space 620 00:31:19,945 --> 00:31:24,414 with lots of galaxies and lots of stars. 621 00:31:24,416 --> 00:31:26,883 This black holes doesn't match its surroundings at all. 622 00:31:26,885 --> 00:31:29,152 It's kind of like driving to the middle of a desert 623 00:31:29,154 --> 00:31:31,120 and coming across the empire state building. 624 00:31:31,122 --> 00:31:33,857 Now, the empire state building belongs in the middle of a city. 625 00:31:33,859 --> 00:31:35,425 And a black hole this big 626 00:31:35,427 --> 00:31:38,962 belongs in a rich cluster of galaxies. 627 00:31:38,964 --> 00:31:41,698 This is the first time astronomers have found 628 00:31:41,700 --> 00:31:43,300 such a giant object 629 00:31:43,302 --> 00:31:47,571 lurking in such a relatively empty area of the universe. 630 00:31:47,573 --> 00:31:48,872 So you got to ask the question, 631 00:31:48,874 --> 00:31:52,041 if there's nothing else around, how exactly do you grow 632 00:31:52,043 --> 00:31:54,611 a 17-billion-solar-mass black hole? 633 00:31:57,815 --> 00:32:01,351 One possible answer is the stuff of nightmares. 634 00:32:01,353 --> 00:32:03,353 Maybe the story of this black hole 635 00:32:03,355 --> 00:32:05,756 is actually a little more scary than we thought. 636 00:32:05,758 --> 00:32:06,956 Maybe it's all alone 637 00:32:06,958 --> 00:32:09,259 because it ate all of its neighbors. 638 00:32:11,662 --> 00:32:14,898 Maybe it was eating more than galaxies. 639 00:32:14,900 --> 00:32:18,301 Maybe it was eating its own kind. 640 00:32:20,204 --> 00:32:22,405 The thing about black holes is they're omnivores. 641 00:32:22,407 --> 00:32:23,673 They'll eat anything. 642 00:32:23,675 --> 00:32:26,243 Anything that gets close them, they'll gobble up. 643 00:32:26,245 --> 00:32:28,244 One way black holes can grow so large 644 00:32:28,246 --> 00:32:29,880 is by eating other black holes. 645 00:32:29,882 --> 00:32:32,716 So in a sense, they may be cannibals. 646 00:32:32,718 --> 00:32:36,219 Cannibal black holes were just theoretical. 647 00:32:36,221 --> 00:32:39,156 We'd never actually seen them eat each other. 648 00:32:41,325 --> 00:32:45,128 Then scientists detected the faint echoes 649 00:32:45,130 --> 00:32:48,732 of actual ripples in space-time. 650 00:32:48,734 --> 00:32:50,267 When engineers turned on 651 00:32:50,269 --> 00:32:54,537 the laser interferometer gravitational-wave observatory, 652 00:32:54,539 --> 00:32:56,573 or ligo for short, 653 00:32:56,575 --> 00:32:58,475 they immediately picked up 654 00:32:58,477 --> 00:33:02,345 the faint signal of gravitational waves. 655 00:33:02,347 --> 00:33:04,114 Gravitational waves are created 656 00:33:04,116 --> 00:33:06,950 by huge explosions in space. 657 00:33:10,187 --> 00:33:14,924 To make them, you need an almost unimaginably energetic event, 658 00:33:14,926 --> 00:33:17,661 something really, really big... 659 00:33:19,897 --> 00:33:24,000 ...something like merging black holes. 660 00:33:26,003 --> 00:33:28,305 Bullock: A black hole merger is the most violent, 661 00:33:28,307 --> 00:33:29,606 the most energetic thing 662 00:33:29,608 --> 00:33:31,875 that happens in the universe, period. 663 00:33:34,745 --> 00:33:38,715 Picture the scene, 1.3 billion years ago. 664 00:33:38,717 --> 00:33:42,819 Two black holes circle each other in a dance of death. 665 00:33:42,821 --> 00:33:46,622 The larger black hole pulls the smaller one inwards 666 00:33:46,624 --> 00:33:50,093 until they're locked together in a spiral. 667 00:33:50,095 --> 00:33:52,562 Very, very slowly, that orbit is decaying. 668 00:33:52,564 --> 00:33:54,664 They're getting closer and closer and closer. 669 00:33:54,666 --> 00:33:58,101 And then they will merge into one giant black hole, 670 00:33:58,103 --> 00:34:01,971 truly one of the most dramatic events in the universe. 671 00:34:01,973 --> 00:34:04,074 Finally, they collide 672 00:34:04,076 --> 00:34:07,844 in one of the largest bangs since the big bang. 673 00:34:11,082 --> 00:34:13,016 I would have loved to have been able 674 00:34:13,018 --> 00:34:14,818 to safely view the collision 675 00:34:14,820 --> 00:34:16,953 of these two black holes up close. 676 00:34:16,955 --> 00:34:18,255 Imagine these two black holes 677 00:34:18,257 --> 00:34:20,123 as they spiral in toward each other, 678 00:34:20,125 --> 00:34:22,358 going faster and faster and faster and faster. 679 00:34:22,360 --> 00:34:24,928 And then, suddenly, where there appears to be nothing 680 00:34:24,930 --> 00:34:27,430 or just distortions in space in front of you, 681 00:34:27,432 --> 00:34:30,700 suddenly, there is this enormous burst of energy. 682 00:34:30,702 --> 00:34:33,870 And everything just rains around you. 683 00:34:33,872 --> 00:34:37,274 By measuring the frequency of the gravitational waves, 684 00:34:37,276 --> 00:34:41,544 we can calculate the size of the objects causing them. 685 00:34:41,546 --> 00:34:43,313 When those two black holes, 686 00:34:43,315 --> 00:34:45,881 weighing 29 solar masses 687 00:34:45,883 --> 00:34:49,652 and 36 solar masses, collided, 688 00:34:49,654 --> 00:34:53,757 they created a black hole around twice the size. 689 00:34:55,793 --> 00:34:58,327 In some ways, it's very elegant and simple. 690 00:34:58,329 --> 00:35:00,596 You take two black holes. You spiral them in together. 691 00:35:00,598 --> 00:35:03,567 And you end up with one big black hole. 692 00:35:05,702 --> 00:35:09,172 The event showed that black holes can double their mass 693 00:35:09,174 --> 00:35:12,875 through cannibalism...Almost. 694 00:35:12,877 --> 00:35:17,580 The final black hole was less than the sum of its parts. 695 00:35:17,582 --> 00:35:20,883 There were 3 solar masses missing. 696 00:35:20,885 --> 00:35:23,086 That may not sound like a lot. 697 00:35:23,088 --> 00:35:25,621 So let's put it in context. 698 00:35:25,623 --> 00:35:27,890 Our sun is burning 699 00:35:27,892 --> 00:35:30,827 about 100 billion hydrogen bombs every second. 700 00:35:30,829 --> 00:35:32,829 And over its 10-billion-year lifetime, 701 00:35:32,831 --> 00:35:35,298 it will convert less than maybe 1% of the mass 702 00:35:35,300 --> 00:35:36,500 of the sun to energy. 703 00:35:36,502 --> 00:35:38,702 In 2/10 of a second, 704 00:35:38,704 --> 00:35:41,505 3 times the mass of the sun in matter 705 00:35:41,507 --> 00:35:44,173 got converted to energy in that collision. 706 00:35:46,110 --> 00:35:50,046 It was 36 septillion yottawatts. 707 00:35:50,048 --> 00:35:52,616 What does that mean? A lot of freaking energy. 708 00:35:52,618 --> 00:35:55,851 That's more energy in that 2/10 of a second 709 00:35:55,853 --> 00:35:57,987 than is emitted by all the stars 710 00:35:57,989 --> 00:36:00,122 in the visible universe in the same time. 711 00:36:02,693 --> 00:36:06,095 In its first run, ligo detected two collisions. 712 00:36:08,232 --> 00:36:10,333 This suggests that cannibal black holes 713 00:36:10,335 --> 00:36:12,035 are relatively common 714 00:36:12,037 --> 00:36:16,206 and that each feast builds a larger black hole. 715 00:36:16,208 --> 00:36:18,541 But so far, the largest black hole 716 00:36:18,543 --> 00:36:20,343 these mergers have produced 717 00:36:20,345 --> 00:36:22,812 is 62 solar masses, 718 00:36:22,814 --> 00:36:28,018 not close to the largest supermassives we've found. 719 00:36:28,020 --> 00:36:30,220 It's hard to imagine, in 13.8 billion years, 720 00:36:30,222 --> 00:36:33,122 that there'd be enough collisions of 30-solar-mass 721 00:36:33,124 --> 00:36:37,460 black holes to build up to form a billion-solar-mass black hole. 722 00:36:37,462 --> 00:36:40,430 That's 100 million collisions. 723 00:36:40,432 --> 00:36:44,067 So maybe small black holes eating each other 724 00:36:44,069 --> 00:36:45,668 isn't the solution. 725 00:36:45,670 --> 00:36:48,905 Maybe supermassive black holes 726 00:36:48,907 --> 00:36:51,841 are eating each other. 727 00:36:51,843 --> 00:36:54,677 If so, could the supermassive black hole 728 00:36:54,679 --> 00:36:58,948 at the heart of our own galaxy be on the menu? 729 00:37:13,697 --> 00:37:16,132 We've found supermassive black holes 730 00:37:16,134 --> 00:37:19,969 so large, they defy explanation. 731 00:37:19,971 --> 00:37:21,371 They're too big to have grown 732 00:37:21,373 --> 00:37:25,642 by simply eating the matter around them. 733 00:37:25,644 --> 00:37:29,178 They can't form the same way that regular black holes do. 734 00:37:29,180 --> 00:37:31,848 There must be something else that happens that lets them grow 735 00:37:31,850 --> 00:37:34,684 to such enormous mass. 736 00:37:34,686 --> 00:37:37,553 Too large to have grown from dark stars 737 00:37:37,555 --> 00:37:41,391 and too big to have grown from regular black holes 738 00:37:41,393 --> 00:37:43,727 simply eating each other. 739 00:37:43,729 --> 00:37:46,129 Merging black holes almost certainly play a role 740 00:37:46,131 --> 00:37:48,965 in our understanding of supermassive black holes. 741 00:37:48,967 --> 00:37:52,201 We think that supermassive black holes themselves also merge 742 00:37:52,203 --> 00:37:55,271 and have merged regularly over the course of the universe. 743 00:37:55,273 --> 00:37:57,240 Now, whether this merging activity itself 744 00:37:57,242 --> 00:37:59,342 is enough to make them that big, 745 00:37:59,344 --> 00:38:01,811 the jury is still out on that. 746 00:38:01,813 --> 00:38:04,948 Now a newly discovered type of galaxy 747 00:38:04,950 --> 00:38:07,317 may provide an answer. 748 00:38:07,319 --> 00:38:13,189 It's called w2246-0526. 749 00:38:13,191 --> 00:38:14,724 And we can't see it. 750 00:38:14,726 --> 00:38:18,294 But we can detect the heat it gives off. 751 00:38:18,296 --> 00:38:20,429 This galaxy is an example 752 00:38:20,431 --> 00:38:24,501 of a rare class of objects called hot dogs. 753 00:38:24,503 --> 00:38:27,237 One of the funnier terms for an exotic type of galaxy 754 00:38:27,239 --> 00:38:28,838 is a hot dog galaxy. 755 00:38:28,840 --> 00:38:31,074 And no, this is not some delicious sausage snack. 756 00:38:31,076 --> 00:38:35,412 In fact, it means "hot, dust-obscured galaxy." 757 00:38:35,414 --> 00:38:37,980 It's called obscured because it's shrouded 758 00:38:37,982 --> 00:38:42,218 in so much dust and gas, the only light that escapes 759 00:38:42,220 --> 00:38:46,822 is infrared in the form of heat. 760 00:38:46,824 --> 00:38:48,691 All this heat must be coming from somewhere. 761 00:38:48,693 --> 00:38:51,494 So in the core, there is a cauldron, 762 00:38:51,496 --> 00:38:53,430 a seething supermassive black hole, 763 00:38:53,432 --> 00:38:55,298 the likes of which we can't even imagine. 764 00:38:58,470 --> 00:39:00,670 of all the supermassive black holes we know of, 765 00:39:00,672 --> 00:39:03,106 the ones that are obscured in these hot dog galaxies 766 00:39:03,108 --> 00:39:05,207 may be the ones that are the most ravenous, 767 00:39:05,209 --> 00:39:06,810 consuming many millions of times 768 00:39:06,812 --> 00:39:09,812 the mass of the sun. 769 00:39:09,814 --> 00:39:12,214 Scientists theorize that hot dogs 770 00:39:12,216 --> 00:39:14,450 could be the offspring 771 00:39:14,452 --> 00:39:18,020 of cannibal giant black holes. 772 00:39:18,022 --> 00:39:20,122 When the monstrous black holes merge, 773 00:39:20,124 --> 00:39:23,126 they drag gas and dust with them. 774 00:39:23,128 --> 00:39:25,695 This brings more food to the table, 775 00:39:25,697 --> 00:39:29,665 allowing the new black hole to gorge itself. 776 00:39:29,667 --> 00:39:32,369 When you have these two galaxies merging, 777 00:39:32,371 --> 00:39:35,271 they have all-new food. 778 00:39:35,273 --> 00:39:36,372 It's a brand-new dinner plate, 779 00:39:36,374 --> 00:39:40,310 a brand-new buffet of food to eat. 780 00:39:40,312 --> 00:39:43,546 The combination of cannibalism and fresh food 781 00:39:43,548 --> 00:39:46,649 allows the black holes to grow super large. 782 00:39:49,186 --> 00:39:52,222 Perhaps this is how the supermassive black hole 783 00:39:52,224 --> 00:39:53,956 at the center of our galaxy 784 00:39:53,958 --> 00:39:56,626 grew when it was young. 785 00:39:56,628 --> 00:39:58,228 But what's the future 786 00:39:58,230 --> 00:40:03,032 of our supermassive sagittarius "a"-star? 787 00:40:03,034 --> 00:40:05,101 As far as supermassive black holes go, 788 00:40:05,103 --> 00:40:06,335 sagittarius "a"-star 789 00:40:06,337 --> 00:40:08,404 is actually still kind of in the minor leagues. 790 00:40:08,406 --> 00:40:10,773 It's small. But it's not done yet. 791 00:40:10,775 --> 00:40:14,777 It's still eating. It's still growing. 792 00:40:14,779 --> 00:40:17,046 And in around 4 billion years, 793 00:40:17,048 --> 00:40:21,951 it's going to become 25 times larger, 794 00:40:21,953 --> 00:40:25,888 because it's going to be eaten by its neighbor. 795 00:40:30,761 --> 00:40:34,396 The giant Andromeda galaxy is heading our way. 796 00:40:34,398 --> 00:40:37,834 And it's going to engulf our milky way. 797 00:40:37,836 --> 00:40:39,302 When galaxies merge, 798 00:40:39,304 --> 00:40:43,405 their central supermassive black holes merge. 799 00:40:43,407 --> 00:40:46,476 Andromeda's huge supermassive black hole 800 00:40:46,478 --> 00:40:50,013 will drag sagittarius "a"-star into orbit... 801 00:40:52,216 --> 00:40:56,085 ...gradually drawing it closer and closer 802 00:40:56,087 --> 00:40:57,720 until it devours it. 803 00:41:00,791 --> 00:41:03,125 The new supermassive black hole will weigh 804 00:41:03,127 --> 00:41:06,729 around 100 million solar masses. 805 00:41:06,731 --> 00:41:09,198 But the disruption to the new galaxy 806 00:41:09,200 --> 00:41:12,535 will provide the new supermassive black hole 807 00:41:12,537 --> 00:41:13,836 with plenty to eat 808 00:41:13,838 --> 00:41:17,440 and the opportunity to grow a whole lot bigger. 809 00:41:20,110 --> 00:41:22,145 At present, there are many theories 810 00:41:22,147 --> 00:41:26,349 of how supermassive black holes get so big. 811 00:41:26,351 --> 00:41:30,086 Most likely, it's a combination of them all. 812 00:41:30,088 --> 00:41:34,224 But however it happens, we can be pretty sure 813 00:41:34,226 --> 00:41:38,828 it's one of the most spectacular things in the universe. 814 00:41:38,830 --> 00:41:40,930 The jury's still out on exactly 815 00:41:40,932 --> 00:41:44,033 how supermassive black holes become so massive. 816 00:41:47,372 --> 00:41:49,071 making all the black holes we see 817 00:41:49,073 --> 00:41:51,941 probably requires a pretty diverse cookbook. 818 00:41:51,943 --> 00:41:54,244 So any physicist who's looking for a really simple, 819 00:41:54,246 --> 00:41:56,479 single answer for how they get made, 820 00:41:56,481 --> 00:41:59,849 they're probably gonna be disappointed. 821 00:41:59,851 --> 00:42:02,785 It's probably a pretty complex thing that's going on. 822 00:42:06,557 --> 00:42:09,792 It could be through eating. It could be through merging. 823 00:42:09,794 --> 00:42:11,127 It could be through eating and merging. 824 00:42:11,129 --> 00:42:13,596 And usually, the answer is somewhere in the middle. 825 00:42:13,598 --> 00:42:15,932 So they will merge with other black holes. 826 00:42:15,934 --> 00:42:19,235 And they'll also have a few snacks between mergers. 64206

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