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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:02,469 --> 00:00:04,803 Narrator: Black holes -- 2 00:00:04,805 --> 00:00:10,276 long considered the bullies of the cosmos, 3 00:00:10,278 --> 00:00:13,211 but are they really so bad? 4 00:00:13,213 --> 00:00:16,414 Black holes aren't violent. They are elegant. 5 00:00:16,416 --> 00:00:18,617 They're incredibly powerful objects, 6 00:00:18,619 --> 00:00:21,752 but they're beautifully simple. 7 00:00:21,754 --> 00:00:24,090 Narrator: Simple but unpredictable. 8 00:00:24,092 --> 00:00:26,891 Black holes rip planets to shreds, 9 00:00:26,893 --> 00:00:31,363 but they also give birth to stars. 10 00:00:31,365 --> 00:00:32,964 Black holes are like the ultimate 11 00:00:32,966 --> 00:00:36,101 recycling-trash-bin combination. 12 00:00:38,304 --> 00:00:40,905 Narrator: They build galaxies 13 00:00:40,907 --> 00:00:46,778 and may have lit up the dark infant universe. 14 00:00:46,780 --> 00:00:48,980 Tegmark: It's one of the biggest changes that happened. 15 00:00:48,982 --> 00:00:54,252 Someone switched the lights on and transforms our universe. 16 00:00:54,254 --> 00:00:55,720 Narrator: They come in all sizes, 17 00:00:55,722 --> 00:00:59,124 from microscopic to ultramassive, 18 00:00:59,126 --> 00:01:02,727 controlling the fate of everything around them. 19 00:01:02,729 --> 00:01:05,063 Thaller: The story of the universe and how it's arranged 20 00:01:05,065 --> 00:01:07,465 is the story of black holes. 21 00:01:07,467 --> 00:01:11,802 Narrator: Black holes are the master architects of the universe, 22 00:01:11,804 --> 00:01:15,273 and without them, we would not exist. 23 00:01:15,275 --> 00:01:18,342 -- Captions by vitac -- www.vitac.com 24 00:01:18,344 --> 00:01:21,313 captions paid for by discovery communications 25 00:01:31,024 --> 00:01:35,559 �� 26 00:01:35,561 --> 00:01:37,162 narrator: Black holes -- 27 00:01:37,164 --> 00:01:41,432 we're riveted by their destructive power. 28 00:01:41,434 --> 00:01:44,102 Black holes are dangerous. 29 00:01:44,104 --> 00:01:45,570 Black holes are hazards. 30 00:01:45,572 --> 00:01:50,976 Black holes are not friendly for their environments. 31 00:01:50,978 --> 00:01:53,044 There's just no good end to anything 32 00:01:53,046 --> 00:01:54,979 that falls into a black hole. 33 00:01:54,981 --> 00:01:57,449 Perhaps one of the most frightening objects 34 00:01:57,451 --> 00:02:00,585 in the universe. 35 00:02:00,587 --> 00:02:04,322 Narrator: But what exactly are these scary objects? 36 00:02:04,324 --> 00:02:06,524 Black holes are created when you get enough matter 37 00:02:06,526 --> 00:02:09,260 in a small region of space. 38 00:02:09,262 --> 00:02:11,796 Narrator: This happens when a massive star dies 39 00:02:11,798 --> 00:02:15,200 and collapses in on itself... 40 00:02:19,005 --> 00:02:20,672 ...a supernova. 41 00:02:23,877 --> 00:02:27,745 A black hole is the ultimate consequence of gravity. 42 00:02:27,747 --> 00:02:30,015 It's an object that has so much mass 43 00:02:30,017 --> 00:02:33,418 crushed into such a small space that its escape velocity 44 00:02:33,420 --> 00:02:35,520 becomes greater than the speed of light. 45 00:02:40,026 --> 00:02:43,695 Sutter: They are a one-way street. 46 00:02:43,697 --> 00:02:45,163 You go in. 47 00:02:45,165 --> 00:02:47,399 Nothing escapes, not even light. 48 00:02:50,703 --> 00:02:55,373 Narrator: But do black holes really deserve their bad rap? 49 00:02:55,375 --> 00:02:57,175 Thaller: In some ways, I think we set up black holes 50 00:02:57,177 --> 00:02:59,044 to be more villains than they actually are. 51 00:02:59,046 --> 00:03:02,580 Black holes suffer a bit of a p.R. Problem. 52 00:03:02,582 --> 00:03:04,916 I think they're a lot more menacing in science fiction 53 00:03:04,918 --> 00:03:07,452 and popular media than they really are. 54 00:03:07,454 --> 00:03:13,057 �� 55 00:03:13,059 --> 00:03:16,094 narrator: There are trillions of galaxies in the known universe. 56 00:03:18,065 --> 00:03:21,466 And most of them have a supermassive black hole 57 00:03:21,468 --> 00:03:23,101 at their center. 58 00:03:27,273 --> 00:03:32,143 These monsters are millions of times the mass of our sun. 59 00:03:32,145 --> 00:03:36,081 Their immense gravity can send stars flying. 60 00:03:36,083 --> 00:03:38,416 They're instrumental in choreographing 61 00:03:38,418 --> 00:03:40,785 the dance of stars in their vicinity. 62 00:03:43,422 --> 00:03:46,025 Narrator: Supermassive black holes shoot out torrents 63 00:03:46,027 --> 00:03:50,829 of lethal radiation and violent cosmic winds 64 00:03:50,831 --> 00:03:55,300 and gobble up anything that comes close. 65 00:03:55,302 --> 00:04:00,237 Now scientists are beginning to realize these cosmic giants 66 00:04:00,239 --> 00:04:02,807 may also have a creative side. 67 00:04:05,378 --> 00:04:06,777 Most people think of black holes 68 00:04:06,779 --> 00:04:08,713 as being like giant vacuum cleaners in space, 69 00:04:08,715 --> 00:04:10,915 and basically everything falls into them, 70 00:04:10,917 --> 00:04:13,117 but that's not actually the case. 71 00:04:13,119 --> 00:04:18,189 They're better thought of as the engines of cosmic change. 72 00:04:18,191 --> 00:04:22,161 Natarajan: Although black holes are the end states of stars, 73 00:04:22,163 --> 00:04:25,997 they can actually influence the formation of stars, 74 00:04:25,999 --> 00:04:29,667 as well, in a bunch of different ways. 75 00:04:29,669 --> 00:04:33,671 Narrator: A galaxy's job is to make stars, 76 00:04:33,673 --> 00:04:37,809 but uncontrolled star growth isn't healthy. 77 00:04:37,811 --> 00:04:42,346 Too many stars can drain a galaxy's gas supply. 78 00:04:42,348 --> 00:04:45,016 Black holes are very important. 79 00:04:45,018 --> 00:04:50,488 It appears that galaxy evolution is tied to black-hole evolution. 80 00:04:50,490 --> 00:04:52,957 We don't know exactly how yet, 81 00:04:52,959 --> 00:04:58,229 but the marriage appears certain. 82 00:04:58,231 --> 00:05:02,634 Narrator: One idea is that supermassive black holes 83 00:05:02,636 --> 00:05:06,637 act as cosmic control mechanisms. 84 00:05:06,639 --> 00:05:09,574 Black holes can act like a thermostat in your house. 85 00:05:09,576 --> 00:05:11,576 If your house gets too hot, 86 00:05:11,578 --> 00:05:14,045 the thermostat will kick on the air conditioner, 87 00:05:14,047 --> 00:05:16,981 and if it gets too cold, it'll kick on the heater. 88 00:05:16,983 --> 00:05:20,851 Black holes do the same things for galaxies. 89 00:05:20,853 --> 00:05:24,255 Narrator: Supermassive black holes regulate star formation 90 00:05:24,257 --> 00:05:30,528 by pulling gas in and shooting it back out into the galaxy. 91 00:05:30,530 --> 00:05:32,931 When these black holes are consuming matter, 92 00:05:32,933 --> 00:05:34,732 they're drawing matter into themselves, 93 00:05:34,734 --> 00:05:37,935 but they're also spewing stuff out. 94 00:05:37,937 --> 00:05:41,539 Basically, black holes eat like little babies -- 95 00:05:41,541 --> 00:05:43,074 very sloppily, 96 00:05:43,076 --> 00:05:47,078 so a lot of what they eat comes flying back out again. 97 00:05:47,080 --> 00:05:49,213 Oluseyi: They eat stars. They eat planets. 98 00:05:49,215 --> 00:05:52,950 But most often, they eat giant clouds of gas. 99 00:05:52,952 --> 00:05:55,086 Narrator: The black hole drags gas and dust 100 00:05:55,088 --> 00:05:57,756 into an accretion disk around it. 101 00:05:57,758 --> 00:06:01,759 This disk spins faster and faster. 102 00:06:01,761 --> 00:06:05,096 Magnetic energy builds up. 103 00:06:05,098 --> 00:06:07,899 With the accretion disk swirling around the black hole, 104 00:06:07,901 --> 00:06:10,568 there are also magnetic fields that are going on. 105 00:06:10,570 --> 00:06:12,169 The material is moving so rapidly 106 00:06:12,171 --> 00:06:15,573 that the magnetic field sort of winds up, coils up, 107 00:06:15,575 --> 00:06:17,441 and forms a vortex like a tornado. 108 00:06:17,443 --> 00:06:19,311 Astronomers call them jets. 109 00:06:19,313 --> 00:06:25,850 �� 110 00:06:25,852 --> 00:06:28,453 these jets propagate outward like freight trains 111 00:06:28,455 --> 00:06:30,120 plowing through the galaxy 112 00:06:30,122 --> 00:06:33,791 over hundreds and thousands of light-years. 113 00:06:33,793 --> 00:06:37,261 These are like death rays. 114 00:06:37,263 --> 00:06:40,464 Narrator: The jets disrupt the star-forming gas clouds, 115 00:06:40,466 --> 00:06:45,202 limiting excess star formation in the main body of the galaxy, 116 00:06:45,204 --> 00:06:48,272 but in the very outer reaches of the galaxy, 117 00:06:48,274 --> 00:06:51,809 they can spark star birth. 118 00:06:51,811 --> 00:06:53,277 Things are more gentle out there. 119 00:06:53,279 --> 00:06:55,546 You're not as close to the energetic heart, 120 00:06:55,548 --> 00:06:58,616 so stars, planets, and life can form out there 121 00:06:58,618 --> 00:07:00,418 partially because of the material 122 00:07:00,420 --> 00:07:03,287 that the black hole has moved out there. 123 00:07:03,289 --> 00:07:08,025 Natarajan: So black holes can have outsize influence 124 00:07:08,027 --> 00:07:10,428 on the regions that they inhabit. 125 00:07:10,430 --> 00:07:15,099 Right around them, they can prevent the formation of stars 126 00:07:15,101 --> 00:07:17,969 whereas, on very, very large scales, 127 00:07:17,971 --> 00:07:21,873 they can actually instigate the formation of stars. 128 00:07:25,911 --> 00:07:29,913 Narrator: 2018 -- black holes hit the front page. 129 00:07:29,915 --> 00:07:35,586 �� 130 00:07:35,588 --> 00:07:38,523 scientists discovered black holes gobbling up gas 131 00:07:38,525 --> 00:07:44,528 so fast that they seem to be outgrowing their host galaxies. 132 00:07:44,530 --> 00:07:47,598 It naturally makes the question come up -- 133 00:07:47,600 --> 00:07:50,736 how big can a black hole get? 134 00:07:50,738 --> 00:07:52,938 Narrator: Now we have the answer. 135 00:07:52,940 --> 00:07:56,140 They can reach size triple-xl, 136 00:07:56,142 --> 00:07:59,810 becoming ultramassive black holes. 137 00:07:59,812 --> 00:08:07,084 �� 138 00:08:07,086 --> 00:08:14,492 �� 139 00:08:14,494 --> 00:08:16,493 stricker: Ultramassive black holes are so cool 140 00:08:16,495 --> 00:08:18,830 because it's just mind-boggling 141 00:08:18,832 --> 00:08:22,232 that black holes so large can exist. 142 00:08:22,234 --> 00:08:24,702 Mingarelli: Ultramassive black holes are very rare 143 00:08:24,704 --> 00:08:28,706 and typically have masses of more than 10 billion times 144 00:08:28,708 --> 00:08:30,507 the mass of the sun. 145 00:08:30,509 --> 00:08:33,311 Narrator: 10 billion solar masses -- 146 00:08:33,313 --> 00:08:37,381 that's a 10 followed by nine zeros. 147 00:08:37,383 --> 00:08:41,052 Ultramassive black holes are real beasts. 148 00:08:41,054 --> 00:08:43,121 The black hole at the center of our galaxy 149 00:08:43,123 --> 00:08:45,056 is 4 million solar masses. 150 00:08:45,058 --> 00:08:49,193 Imagine black holes that are 2,500 times bigger. 151 00:08:49,195 --> 00:08:51,029 That's what we're talking about here. 152 00:08:54,667 --> 00:08:57,668 Narrator: An ultramassive black hole this big 153 00:08:57,670 --> 00:09:00,438 would be as wide as the solar system... 154 00:09:02,541 --> 00:09:06,577 ...and weigh as much as all the stars in the milky way. 155 00:09:09,416 --> 00:09:12,216 They're inside galaxies that aren't a whole lot bigger. 156 00:09:12,218 --> 00:09:16,687 That really surprised the hell out of everybody. 157 00:09:16,689 --> 00:09:20,023 Narrator: And in 2018, scientists discover 158 00:09:20,025 --> 00:09:24,696 a 20-billion-solar-mass ultramassive black hole 159 00:09:24,698 --> 00:09:27,799 growing faster than any other black hole. 160 00:09:30,503 --> 00:09:34,972 This ravenous behemoth devours the mass of our sun 161 00:09:34,974 --> 00:09:36,641 every two days. 162 00:09:38,846 --> 00:09:40,845 Bullock: These big black holes are really good 163 00:09:40,847 --> 00:09:43,248 at gobbling up other things. 164 00:09:43,250 --> 00:09:44,915 They'll literally eat anything. 165 00:09:44,917 --> 00:09:48,052 They're monsters of the universe. 166 00:09:48,054 --> 00:09:50,121 Narrator: This kind of voracious eating 167 00:09:50,123 --> 00:09:53,790 can have devastating consequences. 168 00:09:53,792 --> 00:09:58,262 It blasts so much energy and turbulence into the galaxy 169 00:09:58,264 --> 00:10:02,266 that stars no longer form, 170 00:10:02,268 --> 00:10:07,071 and the bigger the black hole, the faster the galaxy dies. 171 00:10:07,073 --> 00:10:09,673 The primary thing these ultramassive black holes 172 00:10:09,675 --> 00:10:13,010 do to galaxies is they shut down all star formation, 173 00:10:13,012 --> 00:10:15,746 and so in that sense, they kind of kill galaxies. 174 00:10:15,748 --> 00:10:17,148 Oluseyi: And so these things 175 00:10:17,150 --> 00:10:21,419 could even wipe out their host galaxies. 176 00:10:21,421 --> 00:10:26,290 Narrator: Ultramassive black holes are a problem for scientists, too. 177 00:10:26,292 --> 00:10:30,294 They might be the fastest eaters, 178 00:10:30,296 --> 00:10:35,499 but that doesn't explain how they got so large. 179 00:10:35,501 --> 00:10:37,368 With these ultramassive black holes, 180 00:10:37,370 --> 00:10:40,104 these black holes that are 10s of billions of times 181 00:10:40,106 --> 00:10:42,840 more massive than our sun, you can't just grow them 182 00:10:42,842 --> 00:10:45,376 from the slow accretion of gas over time. 183 00:10:45,378 --> 00:10:46,777 There's just not enough gas, 184 00:10:46,779 --> 00:10:48,513 and there's just not enough time. 185 00:10:51,050 --> 00:10:52,984 Bullock: It gives us a new mystery to solve. 186 00:10:52,986 --> 00:10:55,386 How do you make black holes that are just that big? 187 00:10:55,388 --> 00:10:57,721 There's not a clear answer so far 188 00:10:57,723 --> 00:11:01,192 as to how these ultramassive black holes were formed. 189 00:11:01,194 --> 00:11:03,461 People wonder if there's some other mechanism 190 00:11:03,463 --> 00:11:05,930 by which you could make black holes. 191 00:11:05,932 --> 00:11:08,665 Narrator: A mechanism so violent it also throws 192 00:11:08,667 --> 00:11:13,003 supermassive black holes clean out of galaxies. 193 00:11:13,005 --> 00:11:16,474 �� 194 00:11:23,015 --> 00:11:29,820 �� 195 00:11:29,822 --> 00:11:32,890 narrator: We now know that ultramassive black holes 196 00:11:32,892 --> 00:11:36,961 billions of times the mass of the sun exist, 197 00:11:36,963 --> 00:11:42,165 but we have no idea how they got so big. 198 00:11:42,167 --> 00:11:44,502 We've detected lightweight stellar-mass 199 00:11:44,504 --> 00:11:47,238 black holes colliding. 200 00:11:47,240 --> 00:11:51,242 They merged into a new larger black hole 201 00:11:51,244 --> 00:11:53,544 and generated huge amounts of energy. 202 00:11:57,784 --> 00:12:01,452 But what about supermassive black holes? 203 00:12:01,454 --> 00:12:02,787 When galaxies merge, 204 00:12:02,789 --> 00:12:05,122 their central supermassive black holes 205 00:12:05,124 --> 00:12:08,326 will fall to the center of the newly formed galaxy. 206 00:12:10,729 --> 00:12:13,197 Narrator: Could these supermassive black holes 207 00:12:13,199 --> 00:12:15,399 caught up in galactic mergers 208 00:12:15,401 --> 00:12:19,804 combine to form an ultramassive black hole? 209 00:12:19,806 --> 00:12:26,545 �� 210 00:12:26,547 --> 00:12:30,014 in 2017, the hubble space telescope spotted 211 00:12:30,016 --> 00:12:35,987 something strange in a distant galaxy called 3c186. 212 00:12:38,157 --> 00:12:41,626 It detected an incredibly bright spot 213 00:12:41,628 --> 00:12:46,229 thousands of light-years from the galaxy center. 214 00:12:46,231 --> 00:12:50,569 Scientists suspect it's a quasar. 215 00:12:50,571 --> 00:12:54,839 A quasar is an incredibly bright, active galactic nucleus 216 00:12:54,841 --> 00:12:57,141 that's powered by a supermassive black hole. 217 00:13:00,512 --> 00:13:03,581 Narrator: We regularly spot black-hole-powered quasars, 218 00:13:03,583 --> 00:13:07,117 but always at the centers of galaxies, 219 00:13:07,119 --> 00:13:10,120 until now. 220 00:13:10,122 --> 00:13:12,590 When we actually got this data from hubble, 221 00:13:12,592 --> 00:13:14,792 we were absolutely stunned to discover 222 00:13:14,794 --> 00:13:17,127 that the quasar that we've long known to exist 223 00:13:17,129 --> 00:13:20,464 in the center of this galaxy wasn't actually at the center. 224 00:13:20,466 --> 00:13:23,067 This black hole is offset from the center of the galaxy 225 00:13:23,069 --> 00:13:25,469 by about 35,000 light-years. 226 00:13:25,471 --> 00:13:27,071 That's really weird. 227 00:13:27,073 --> 00:13:30,607 Tremblay: What is an incredibly rare and bizarre event 228 00:13:30,609 --> 00:13:33,210 to find a quasar, a supermassive black hole, 229 00:13:33,212 --> 00:13:36,414 that is not at the center of the galaxy. 230 00:13:36,416 --> 00:13:38,482 Narrator: When scientists looked closer, 231 00:13:38,484 --> 00:13:42,553 they discovered that the quasar is hurtling through space 232 00:13:42,555 --> 00:13:46,023 away from the center of the galaxy. 233 00:13:46,025 --> 00:13:47,758 Now, mind you, this is a black hole 234 00:13:47,760 --> 00:13:50,894 with the mass of about a billion times the sun, 235 00:13:50,896 --> 00:13:55,700 and it's screaming away at 4 million miles an hour. 236 00:13:55,702 --> 00:13:56,967 Tremblay: This black hole, 237 00:13:56,969 --> 00:13:59,504 which was probably originally in the galaxy center, 238 00:13:59,506 --> 00:14:02,439 has somehow been shot out at high velocity 239 00:14:02,441 --> 00:14:05,243 by some incredibly violent event. 240 00:14:05,245 --> 00:14:07,645 It's hard to imagine what kind of event 241 00:14:07,647 --> 00:14:10,915 would pump that much energy into such a huge object 242 00:14:10,917 --> 00:14:14,118 to shoot it away from the center of a galaxy. 243 00:14:14,120 --> 00:14:18,055 Who kicked it out, how, and why? 244 00:14:18,057 --> 00:14:20,591 Narrator: Scientists have an idea. 245 00:14:20,593 --> 00:14:24,795 3c186 may be the remnant of a galaxy merger. 246 00:14:24,797 --> 00:14:28,132 Narrator: The merged galaxies' supermassive black holes 247 00:14:28,134 --> 00:14:30,534 circle each other, 248 00:14:30,536 --> 00:14:35,106 sending out blasts of energy in the form of gravitational waves. 249 00:14:38,745 --> 00:14:42,012 Gravitational waves are all around us. 250 00:14:42,014 --> 00:14:46,350 They're ripples in the fabric of space-time. 251 00:14:46,352 --> 00:14:48,352 Every time mass moves, 252 00:14:48,354 --> 00:14:50,487 gravitational waves are produced, 253 00:14:50,489 --> 00:14:55,025 so if I wave my hand, I am making gravitational waves. 254 00:14:55,027 --> 00:15:00,198 Narrator: A hand produces imperceptible waves. 255 00:15:00,200 --> 00:15:01,632 When objects as huge 256 00:15:01,634 --> 00:15:05,435 as supermassive black holes collide, 257 00:15:05,437 --> 00:15:08,773 the energy released as gravitational waves 258 00:15:08,775 --> 00:15:12,109 is phenomenal. 259 00:15:12,111 --> 00:15:14,244 Scientists think these black holes 260 00:15:14,246 --> 00:15:17,581 might have been different sizes. 261 00:15:17,583 --> 00:15:19,650 It's possible that if one of the black holes 262 00:15:19,652 --> 00:15:20,717 is really massive 263 00:15:20,719 --> 00:15:22,652 and the other one isn't quite as massive, 264 00:15:22,654 --> 00:15:25,255 that when they spiral around and merge, 265 00:15:25,257 --> 00:15:28,726 they send out gravitational waves in an asymmetric way. 266 00:15:28,728 --> 00:15:35,399 �� 267 00:15:35,401 --> 00:15:38,469 narrator: This asymmetry has a catastrophic effect. 268 00:15:41,474 --> 00:15:44,074 As the two black holes collide and merge, 269 00:15:44,076 --> 00:15:47,545 they shoot out a huge blast of gravitational waves, 270 00:15:47,547 --> 00:15:49,847 but only in one direction. 271 00:15:52,151 --> 00:15:56,353 This blast of energy kicks the newly combined black hole 272 00:15:56,355 --> 00:15:59,490 out of the galactic center. 273 00:15:59,492 --> 00:16:03,327 Think of a shotgun recoil, but supersized. 274 00:16:05,498 --> 00:16:08,031 Plait: And there's so much energy in that emission 275 00:16:08,033 --> 00:16:09,433 that it acts like a rocket, 276 00:16:09,435 --> 00:16:12,636 and it actually pushes the merged black hole away. 277 00:16:12,638 --> 00:16:14,705 It would have been one of the most energetic events 278 00:16:14,707 --> 00:16:16,574 ever witnessed. 279 00:16:16,576 --> 00:16:18,242 Plait: They're so energetic, 280 00:16:18,244 --> 00:16:21,479 they are literally shaking the fabric of space. 281 00:16:25,184 --> 00:16:28,452 Narrator: We didn't witness the actual collision, 282 00:16:28,454 --> 00:16:31,855 but 3c186 could be evidence 283 00:16:31,857 --> 00:16:37,061 that supermassive black holes can collide and merge, 284 00:16:37,063 --> 00:16:41,198 building even larger black holes. 285 00:16:41,200 --> 00:16:43,734 This would be a mechanism by which you would create, 286 00:16:43,736 --> 00:16:47,004 ultimately, an ultramassive black hole. 287 00:16:47,006 --> 00:16:49,206 Narrator: As for the ejected black hole, 288 00:16:49,208 --> 00:16:52,209 the gravitational recoil sent it 289 00:16:52,211 --> 00:16:56,013 on a one-way ride to oblivion. 290 00:16:56,015 --> 00:17:00,350 So gravitational waves kicked this supermassive black hole 291 00:17:00,352 --> 00:17:02,219 and sent it flying through space. 292 00:17:02,221 --> 00:17:07,024 In 20 million years, it's expected to exit its galaxy. 293 00:17:07,026 --> 00:17:09,760 Narrator: The ejected supermassive black hole 294 00:17:09,762 --> 00:17:12,363 may eventually hit another galaxy 295 00:17:12,365 --> 00:17:16,100 and merge with its supermassive black hole. 296 00:17:16,102 --> 00:17:22,105 �� 297 00:17:22,107 --> 00:17:23,974 these largest of black holes 298 00:17:23,976 --> 00:17:26,844 seem to throw their weight around, 299 00:17:26,846 --> 00:17:31,649 bullying galaxies and other black holes. 300 00:17:31,651 --> 00:17:35,919 Now researchers have discovered a vampire black hole 301 00:17:35,921 --> 00:17:39,389 that's draining the lifeblood of its neighbor. 302 00:17:39,391 --> 00:17:43,794 �� 303 00:17:50,402 --> 00:18:00,411 �� 304 00:18:00,413 --> 00:18:02,346 narrator: Ultramassive black holes 305 00:18:02,348 --> 00:18:05,148 seem to destroy their galaxies, 306 00:18:05,150 --> 00:18:10,888 while supermassive black holes seem to regulate star formation. 307 00:18:10,890 --> 00:18:15,559 But are all supermassive black holes forces for good? 308 00:18:15,561 --> 00:18:20,864 �� 309 00:18:20,866 --> 00:18:25,370 hundreds of galaxies surround the milky way, 310 00:18:25,372 --> 00:18:28,571 large and small, 311 00:18:28,573 --> 00:18:33,844 but most of the largest galaxies are red. 312 00:18:33,846 --> 00:18:35,979 This is not a good omen. 313 00:18:35,981 --> 00:18:39,350 In space, red means danger. 314 00:18:41,520 --> 00:18:43,721 If you have active ongoing star birth, 315 00:18:43,723 --> 00:18:45,055 then you have massive stars, 316 00:18:45,057 --> 00:18:46,856 and massive stars tend to be blue, 317 00:18:46,858 --> 00:18:49,226 but they don't live very long, and they blow up. 318 00:18:53,132 --> 00:18:55,665 Once you stop star formation, after some amount of time, 319 00:18:55,667 --> 00:18:59,336 the galaxy turns red. 320 00:18:59,338 --> 00:19:01,137 Narrator: The only stars left alive 321 00:19:01,139 --> 00:19:06,944 are small, long-lived red stars called red dwarfs. 322 00:19:06,946 --> 00:19:10,414 A red galaxy with only red dwarfs 323 00:19:10,416 --> 00:19:13,750 is a dying galaxy. 324 00:19:13,752 --> 00:19:17,420 The Sloan digital sky survey found an entire population 325 00:19:17,422 --> 00:19:20,557 of these luminous red galaxies 326 00:19:20,559 --> 00:19:22,961 that were no longer forming stars 327 00:19:22,963 --> 00:19:23,994 that were dead. 328 00:19:26,899 --> 00:19:31,602 Narrator: One galaxy around 340 million light-years away stood out. 329 00:19:35,440 --> 00:19:40,444 It was named after a Japanese anime character, Akira. 330 00:19:40,446 --> 00:19:42,046 Plait: It's very red. 331 00:19:42,048 --> 00:19:44,514 All the stars in it are red, and that means they're old, 332 00:19:44,516 --> 00:19:45,983 so we know that Akira has not had 333 00:19:45,985 --> 00:19:48,452 any active star formation in a long time. 334 00:19:51,390 --> 00:19:53,323 Narrator: The Akira galaxy doesn't form stars 335 00:19:53,325 --> 00:19:55,793 because it doesn't have the cool, calm gas 336 00:19:55,795 --> 00:19:57,061 needed to build them. 337 00:19:59,264 --> 00:20:02,933 Something is heating the gas, making it turbulent. 338 00:20:05,004 --> 00:20:07,337 One of the ways in which a black hole can drive 339 00:20:07,339 --> 00:20:09,806 the evolution of the galaxy in which it resides 340 00:20:09,808 --> 00:20:13,410 is by simply powering a wind. 341 00:20:13,412 --> 00:20:16,714 These are winds that are literally driven by light. 342 00:20:19,551 --> 00:20:21,151 Narrator: When a black hole feeds, 343 00:20:21,153 --> 00:20:25,889 it drags gas into an accretion disk. 344 00:20:25,891 --> 00:20:29,326 The disk heats up and gives off light radiation. 345 00:20:31,763 --> 00:20:35,432 The radiation pressure from the accretion disk around this black hole 346 00:20:35,434 --> 00:20:37,767 couples to the ambient gas and dust 347 00:20:37,769 --> 00:20:42,040 and pushes it outwards at very high velocity. 348 00:20:42,042 --> 00:20:45,976 These winds that are driven out by the black hole 349 00:20:45,978 --> 00:20:49,779 essentially warm up the gas in the galaxy, 350 00:20:49,781 --> 00:20:52,349 preventing further star formation. 351 00:20:54,453 --> 00:20:58,121 Narrator: However, whatever's fueling the black hole in Akira 352 00:20:58,123 --> 00:20:59,990 is a mystery. 353 00:20:59,992 --> 00:21:02,793 Here's a weird thing -- there is an outflow, 354 00:21:02,795 --> 00:21:04,928 a wind coming out of this galaxy, 355 00:21:04,930 --> 00:21:06,864 and that means there's gas feeding 356 00:21:06,866 --> 00:21:10,000 that black hole in the center, and it's blowing it out. 357 00:21:10,002 --> 00:21:13,604 Where is this gas coming from? 358 00:21:13,606 --> 00:21:16,606 Ah, it's stealing it. 359 00:21:16,608 --> 00:21:20,344 It has a small companion galaxy, which is nicknamed tetsuo, 360 00:21:20,346 --> 00:21:22,080 and that has gas in it. 361 00:21:24,950 --> 00:21:29,219 Narrator: Akira's supermassive black hole pulls gas from tetsuo 362 00:21:29,221 --> 00:21:31,923 and drags it into the center of the galaxy. 363 00:21:34,827 --> 00:21:38,094 The black hole is taking the gas from this companion galaxy, 364 00:21:38,096 --> 00:21:39,897 and that's what's falling around the black hole 365 00:21:39,899 --> 00:21:41,632 and creating this wind, 366 00:21:41,634 --> 00:21:44,234 so Akira is actually sort of a dead galaxy, 367 00:21:44,236 --> 00:21:47,404 but it's being rejuvenated by its companion, tetsuo. 368 00:21:50,976 --> 00:21:52,844 Narrator: Like a cosmic vampire, 369 00:21:52,846 --> 00:21:57,514 Akira's supermassive black hole feeds off tetsuo. 370 00:22:00,053 --> 00:22:04,521 The black hole drags gas and dust into its accretion disk, 371 00:22:04,523 --> 00:22:08,525 which spins faster and faster. 372 00:22:08,527 --> 00:22:10,793 Plait: When these particles are rubbing against each other, 373 00:22:10,795 --> 00:22:13,131 well, that generates friction. 374 00:22:13,133 --> 00:22:15,532 Friction may not seem like that big of a deal. 375 00:22:15,534 --> 00:22:16,800 I mean, you can rub your hands together 376 00:22:16,802 --> 00:22:18,535 on a cold day to get warm, 377 00:22:18,537 --> 00:22:20,070 but imagine rubbing your hands together 378 00:22:20,072 --> 00:22:22,472 at very nearly the speed of light. 379 00:22:22,474 --> 00:22:24,074 How much friction is that gonna generate? 380 00:22:24,076 --> 00:22:27,076 It's gonna make a lot of heat. 381 00:22:27,078 --> 00:22:31,415 Narrator: Over a million degrees fahrenheit -- 382 00:22:31,417 --> 00:22:35,185 so hot the accretion disk lights up. 383 00:22:38,024 --> 00:22:41,558 Its temperature goes up, and he starts emitting light. 384 00:22:41,560 --> 00:22:44,494 It becomes incredibly bright. 385 00:22:44,496 --> 00:22:46,563 Even though there's a black hole in the core, 386 00:22:46,565 --> 00:22:51,902 its surroundings are intensely bright. 387 00:22:51,904 --> 00:22:54,338 Narrator: This heats up the surrounding gas, 388 00:22:54,340 --> 00:22:56,239 generating a hot wind, 389 00:22:56,241 --> 00:23:01,444 which extends thousands of light-years from the black hole. 390 00:23:01,446 --> 00:23:04,515 Tremblay: And those winds carry with them a lot of energy, 391 00:23:04,517 --> 00:23:08,051 and that energy, if it couples to the gas in the galaxy, 392 00:23:08,053 --> 00:23:10,053 can blow that gas out. 393 00:23:10,055 --> 00:23:12,455 They inject energy into nearby gas clouds 394 00:23:12,457 --> 00:23:17,127 and heat them up and prevent them from forming stars. 395 00:23:17,129 --> 00:23:20,731 Narrator: Stars don't form -- the galaxy dies. 396 00:23:23,335 --> 00:23:26,870 These dying galaxies are called red geysers. 397 00:23:30,476 --> 00:23:33,810 Scientists think around 10% of the red galaxies 398 00:23:33,812 --> 00:23:37,014 we see around us died this way... 399 00:23:39,352 --> 00:23:42,386 ...heated up by this galactic warming. 400 00:23:45,156 --> 00:23:48,158 We think that the source of some of this galactic warming 401 00:23:48,160 --> 00:23:50,961 is in the growth of supermassive black holes themselves 402 00:23:50,963 --> 00:23:53,297 because when you grow a supermassive black hole, 403 00:23:53,299 --> 00:23:56,833 you must liberate an enormous amount of energy. 404 00:23:56,835 --> 00:23:59,503 You can't grow a black hole for free, 405 00:23:59,505 --> 00:24:03,240 and that energy gets dumped back into the ambient surroundings 406 00:24:03,242 --> 00:24:05,175 and keeps this halo of gas hot. 407 00:24:05,177 --> 00:24:08,012 It prevents it from cooling and forming stars. 408 00:24:11,450 --> 00:24:13,317 Narrator: Sagittarius a-star, 409 00:24:13,319 --> 00:24:16,919 the supermassive black hole at the heart of our galaxy, 410 00:24:16,921 --> 00:24:21,525 the milky way, could turn into a red geyser. 411 00:24:21,527 --> 00:24:24,528 If you were suddenly to dump an enormous amount of gas 412 00:24:24,530 --> 00:24:26,463 onto sagittarius a-star, 413 00:24:26,465 --> 00:24:29,199 you could have what is effectively a red-geyser effect, 414 00:24:29,201 --> 00:24:33,203 a very powerful wind driven by all of this energy. 415 00:24:37,475 --> 00:24:40,010 Narrator: Star formation would stop, 416 00:24:40,012 --> 00:24:44,782 and our milky way would become another dying red galaxy. 417 00:24:49,754 --> 00:24:53,690 Now new research suggests that sagittarius a-star 418 00:24:53,692 --> 00:24:57,761 has already affected the inner region of our galaxy, 419 00:24:57,763 --> 00:24:59,762 not by killing stars, 420 00:24:59,764 --> 00:25:05,269 but by transforming planets from gas giants into super-earths. 421 00:25:05,271 --> 00:25:08,772 �� 422 00:25:15,314 --> 00:25:20,517 �� 423 00:25:20,519 --> 00:25:25,655 �� 424 00:25:25,657 --> 00:25:27,390 narrator: At the center of our galaxy 425 00:25:27,392 --> 00:25:32,295 lies a supermassive black hole, sagittarius a-star. 426 00:25:35,467 --> 00:25:40,337 We think it's calm, dormant, safe. 427 00:25:40,339 --> 00:25:42,405 Relative to other supermassive black holes 428 00:25:42,407 --> 00:25:45,875 in the universe, ours is relatively quiet. 429 00:25:45,877 --> 00:25:48,678 Narrator: It's been active in the past, 430 00:25:48,680 --> 00:25:52,081 and it could flare up in the future. 431 00:25:52,083 --> 00:25:54,350 Tremblay: It could be active tomorrow, for all we know. 432 00:25:54,352 --> 00:25:55,952 All you need to do to light it up 433 00:25:55,954 --> 00:25:58,088 is start dumping some gas on it, 434 00:25:58,090 --> 00:26:00,824 and there is almost certainly a giant cloud of gas 435 00:26:00,826 --> 00:26:02,225 that we don't currently know of 436 00:26:02,227 --> 00:26:04,427 on its way to the center of our galaxy, 437 00:26:04,429 --> 00:26:06,362 and it will find itself one day in the vicinity 438 00:26:06,364 --> 00:26:07,965 of our supermassive black hole, 439 00:26:07,967 --> 00:26:11,701 and it will start to light up like a Christmas tree. 440 00:26:11,703 --> 00:26:16,040 Narrator: In February of 2018, scientists at Harvard 441 00:26:16,042 --> 00:26:20,910 simulated sagittarius a-star during a feeding frenzy 442 00:26:20,912 --> 00:26:25,381 to understand the impact of an active supermassive black hole 443 00:26:25,383 --> 00:26:26,917 on its local environment. 444 00:26:30,722 --> 00:26:31,854 They found that, 445 00:26:31,856 --> 00:26:35,058 as sagittarius a-star gobbled up gas and dust, 446 00:26:35,060 --> 00:26:40,930 it belched out bright flares of high-energy radiation, 447 00:26:40,932 --> 00:26:45,936 which radically affected the region around the black hole. 448 00:26:45,938 --> 00:26:48,605 Plait: The environment near the center of a galaxy 449 00:26:48,607 --> 00:26:51,007 that has an actively feeding black hole 450 00:26:51,009 --> 00:26:53,943 is the worst place in the universe. 451 00:26:53,945 --> 00:26:55,946 You've got this tremendous object 452 00:26:55,948 --> 00:26:59,483 which is heating up this gas to millions of degrees. 453 00:26:59,485 --> 00:27:01,818 This is no place that you want to be. 454 00:27:04,822 --> 00:27:06,857 Narrator: The model revealed what would happen 455 00:27:06,859 --> 00:27:10,360 to any planets in the line of fire. 456 00:27:10,362 --> 00:27:11,427 Thaller: Think about being in the way 457 00:27:11,429 --> 00:27:13,896 of one of these black-hole burps. 458 00:27:13,898 --> 00:27:16,499 All of a sudden, there's a tremendous wind of radiation 459 00:27:16,501 --> 00:27:18,167 that comes through your solar system. 460 00:27:18,169 --> 00:27:21,103 That could actually strip away the outer layers of gas 461 00:27:21,105 --> 00:27:22,572 of a planet like Neptune. 462 00:27:25,310 --> 00:27:26,709 Narrator: The high-energy radiation 463 00:27:26,711 --> 00:27:28,845 from the supermassive black holes 464 00:27:28,847 --> 00:27:33,317 would hit the gas planets and heat up their atmospheres. 465 00:27:33,319 --> 00:27:35,919 Thaller: Maybe this would actually strip away the outer layers, 466 00:27:35,921 --> 00:27:38,054 leaving the solid material in the middle. 467 00:27:38,056 --> 00:27:40,256 You could actually turn a gas-giant planet 468 00:27:40,258 --> 00:27:42,325 into a terrestrial solid planet 469 00:27:42,327 --> 00:27:46,062 all because you're close to a black hole. 470 00:27:46,064 --> 00:27:50,734 Narrator: This radiation strips away the gas, leaving the core, 471 00:27:50,736 --> 00:27:54,137 now a new rocky planet 472 00:27:54,139 --> 00:27:58,074 but a giant one -- a super-earth. 473 00:27:58,076 --> 00:27:59,977 Normally, you think of rocky planets 474 00:27:59,979 --> 00:28:01,745 being about the size of the earth, 475 00:28:01,747 --> 00:28:05,882 but this would be a way of making so called super-earths. 476 00:28:05,884 --> 00:28:07,884 Narrator: Super-earths are one of the most common 477 00:28:07,886 --> 00:28:11,888 type of planets discovered in our galaxy. 478 00:28:11,890 --> 00:28:14,291 It's possible that any super-earths 479 00:28:14,293 --> 00:28:16,626 close to sagittarius a-star 480 00:28:16,628 --> 00:28:19,729 were created by these blasts of energy. 481 00:28:23,969 --> 00:28:26,235 Away from our galactic center, 482 00:28:26,237 --> 00:28:29,706 a much smaller stellar-mass black hole 483 00:28:29,708 --> 00:28:33,143 is also radically transforming its environment. 484 00:28:36,114 --> 00:28:38,715 January 2017 -- 485 00:28:38,717 --> 00:28:41,851 researchers discover something strange 486 00:28:41,853 --> 00:28:46,589 in a cloud of gas called w44. 487 00:28:46,591 --> 00:28:48,526 Plait: W44 is a supernova remnant. 488 00:28:48,528 --> 00:28:53,797 It's the debris -- the expanding cloud from a star that blew up. 489 00:28:53,799 --> 00:28:57,934 Narrator: The explosive shock wave from a supernova 490 00:28:57,936 --> 00:29:01,671 pushes gas and dust out from the dead star, 491 00:29:01,673 --> 00:29:05,275 forming a huge nebula. 492 00:29:05,277 --> 00:29:06,743 Plait: We see a lot of these. 493 00:29:06,745 --> 00:29:09,280 I mean, they're catastrophic, amazing, incredible events, 494 00:29:09,282 --> 00:29:10,480 but as far as they go, 495 00:29:10,482 --> 00:29:13,483 this one appears to be pretty standard, 496 00:29:13,485 --> 00:29:15,752 except for one weird thing. 497 00:29:15,754 --> 00:29:16,952 Thaller: In the heart of it, 498 00:29:16,954 --> 00:29:18,822 there's something very mysterious going on. 499 00:29:18,824 --> 00:29:20,957 There seems to be something shooting out 500 00:29:20,959 --> 00:29:23,493 of the very center of this explosion. 501 00:29:23,495 --> 00:29:29,566 �� 502 00:29:29,568 --> 00:29:32,435 narrator: A thin protrusion trillions of miles long 503 00:29:32,437 --> 00:29:36,573 streams out from the cloud. 504 00:29:36,575 --> 00:29:39,241 It's moving at over 60 miles a second 505 00:29:39,243 --> 00:29:42,779 against the flow of the galaxy. 506 00:29:42,781 --> 00:29:45,114 It's very strange that it's moving backwards 507 00:29:45,116 --> 00:29:47,517 against the rotation of the milky way. 508 00:29:47,519 --> 00:29:51,321 Tremblay: When you see a giant, giant, very massive cloud of gas 509 00:29:51,323 --> 00:29:53,856 that is moving counter to the rotation of the milky way, 510 00:29:53,858 --> 00:29:55,792 it needed to be like a bullet from a gun 511 00:29:55,794 --> 00:29:59,395 fired against a headwind in the opposite direction. 512 00:29:59,397 --> 00:30:00,797 So what is that gun? 513 00:30:00,799 --> 00:30:04,934 You know, what fired that bullet of gas? 514 00:30:04,936 --> 00:30:07,404 Narrator: The tip of the bullet cloud is expanding 515 00:30:07,406 --> 00:30:09,806 at 75 miles a second. 516 00:30:09,808 --> 00:30:12,809 That's 270,000 miles an hour, 517 00:30:12,811 --> 00:30:17,080 over 150 times faster than a bullet. 518 00:30:17,082 --> 00:30:20,884 What in the cosmos has the power to accelerate gas 519 00:30:20,886 --> 00:30:23,553 to such high speed? 520 00:30:23,555 --> 00:30:25,488 Could that actually be a black hole 521 00:30:25,490 --> 00:30:28,491 moving very, very quickly? 522 00:30:28,493 --> 00:30:31,628 Narrator: Researchers think a stellar-mass black hole 523 00:30:31,630 --> 00:30:33,296 hidden in the bullet cloud 524 00:30:33,298 --> 00:30:36,165 is powering the movement of the gas. 525 00:30:36,167 --> 00:30:38,568 Gravity from this black hole is incredibly strong, 526 00:30:38,570 --> 00:30:40,570 and so it will latch onto this gas cloud 527 00:30:40,572 --> 00:30:42,038 as it passes through it, 528 00:30:42,040 --> 00:30:45,308 and it can completely disrupt the motions of this cloud. 529 00:30:45,310 --> 00:30:47,711 Bullock: This is a very interesting stream of gas 530 00:30:47,713 --> 00:30:50,246 that's somehow connected to a black hole, 531 00:30:50,248 --> 00:30:51,581 and we don't know whether it's there 532 00:30:51,583 --> 00:30:53,717 because the black hole is moving through the gas, 533 00:30:53,719 --> 00:30:55,317 and it's creating a wake, 534 00:30:55,319 --> 00:30:57,520 or whether somehow this black hole 535 00:30:57,522 --> 00:31:01,924 is spitting out a stream of material in some way. 536 00:31:01,926 --> 00:31:03,927 Narrator: The black hole could be dragging gas 537 00:31:03,929 --> 00:31:06,930 into an accretion disk around it. 538 00:31:06,932 --> 00:31:09,199 The gas heats up and expands, 539 00:31:09,201 --> 00:31:15,538 giving the initial supernova explosion, w44, an extra kick, 540 00:31:15,540 --> 00:31:19,942 driving this bullet-like cloud out in front of it. 541 00:31:19,944 --> 00:31:23,613 Or the black hole could be racing away from the nebula, 542 00:31:23,615 --> 00:31:27,082 dragging the gas behind it like a wake. 543 00:31:27,084 --> 00:31:33,289 �� 544 00:31:33,291 --> 00:31:37,827 ultramassive, supermassive, and stellar-mass black holes 545 00:31:37,829 --> 00:31:41,564 all play a role in shaping the cosmos, 546 00:31:41,566 --> 00:31:44,767 but there may be another type of black hole 547 00:31:44,769 --> 00:31:49,105 even more dangerous than the rest -- 548 00:31:49,107 --> 00:31:51,841 a microscopic black hole. 549 00:31:51,843 --> 00:31:55,912 �� 550 00:32:02,387 --> 00:32:09,058 �� 551 00:32:09,060 --> 00:32:15,732 �� 552 00:32:15,734 --> 00:32:18,735 narrator: We have so far detected triple-xl 553 00:32:18,737 --> 00:32:24,206 ultramassive black holes, large supermassive black holes, 554 00:32:24,208 --> 00:32:28,545 medium-sized intermediate black holes, 555 00:32:28,547 --> 00:32:32,215 and small stellar-mass black holes. 556 00:32:32,217 --> 00:32:36,419 Now scientists have another to add to the roster -- 557 00:32:36,421 --> 00:32:39,222 microscopic black holes. 558 00:32:39,224 --> 00:32:40,757 Carroll: We know there are supermassive black holes 559 00:32:40,759 --> 00:32:42,626 at the centers of galaxies. 560 00:32:42,628 --> 00:32:45,228 We know there are star-sized black holes 561 00:32:45,230 --> 00:32:46,562 from the deaths of stars. 562 00:32:46,564 --> 00:32:48,331 That's what we know for sure. 563 00:32:48,333 --> 00:32:50,900 It's possible there are much smaller black holes, 564 00:32:50,902 --> 00:32:53,970 microscopically small black holes. 565 00:32:53,972 --> 00:32:57,306 Narrator: Microscopic black holes are virtually invisible 566 00:32:57,308 --> 00:32:58,775 to the naked eye, 567 00:32:58,777 --> 00:33:04,648 but magnified, they look like regular stellar-mass black holes 568 00:33:04,650 --> 00:33:06,983 the definition of a black hole 569 00:33:06,985 --> 00:33:09,385 is an object that has so much mass 570 00:33:09,387 --> 00:33:12,756 crushed into such a small space that its escape velocity 571 00:33:12,758 --> 00:33:14,924 becomes greater than the speed of light, 572 00:33:14,926 --> 00:33:17,327 so it could be something the size of a star, 573 00:33:17,329 --> 00:33:18,928 the size of a galaxy. 574 00:33:18,930 --> 00:33:21,998 It could also be the mass of a planet. 575 00:33:22,000 --> 00:33:25,135 Narrator: If you could crush the earth down far enough, 576 00:33:25,137 --> 00:33:27,670 it could become a black hole. 577 00:33:27,672 --> 00:33:28,938 Thaller: The density of a black hole 578 00:33:28,940 --> 00:33:30,406 is something that the human brain 579 00:33:30,408 --> 00:33:32,408 really doesn't wrap itself around very easily. 580 00:33:32,410 --> 00:33:34,877 When you think about something the size of the earth, 581 00:33:34,879 --> 00:33:37,547 how small would the earth have to be to be a black hole? 582 00:33:37,549 --> 00:33:40,016 And the answer is something on the order of a marble. 583 00:33:40,018 --> 00:33:41,884 So think about taking the entire earth 584 00:33:41,886 --> 00:33:44,521 and compressing it down to the size of just a marble. 585 00:33:46,958 --> 00:33:51,561 Narrator: So where do these strange little black holes come from? 586 00:33:51,563 --> 00:33:54,897 These very small black holes can only be formed 587 00:33:54,899 --> 00:34:01,237 in the exotic conditions of the incredibly early universe. 588 00:34:01,239 --> 00:34:04,173 Our universe might get flooded with these small black holes 589 00:34:04,175 --> 00:34:09,112 that simply persist to the present day. 590 00:34:09,114 --> 00:34:10,580 It's the only time in the history of the universe 591 00:34:10,582 --> 00:34:12,448 where you could take a small amount of matter 592 00:34:12,450 --> 00:34:13,983 and crush it down so tightly 593 00:34:13,985 --> 00:34:15,652 that it could become a black hole. 594 00:34:15,654 --> 00:34:17,855 Those conditions don't exist anymore, 595 00:34:17,857 --> 00:34:21,457 so if these things exist, they would be primordial. 596 00:34:21,459 --> 00:34:24,060 They would be as old as the universe itself. 597 00:34:24,062 --> 00:34:30,199 �� 598 00:34:30,201 --> 00:34:33,603 narrator: These primordial black holes may be ancient, 599 00:34:33,605 --> 00:34:36,806 but they still pack a punch. 600 00:34:36,808 --> 00:34:38,408 When it comes to black holes, 601 00:34:38,410 --> 00:34:42,344 the smaller black holes are actually more dangerous 602 00:34:42,346 --> 00:34:44,480 because their mass is concentrated 603 00:34:44,482 --> 00:34:47,149 into such a small volume. 604 00:34:47,151 --> 00:34:51,621 Narrator: In fact, a tiny black hole would be lethal. 605 00:34:51,623 --> 00:34:55,091 If it were to pass in front of me, very quickly, 606 00:34:55,093 --> 00:34:58,761 almost instantly, I would be ripped apart head to toe, 607 00:34:58,763 --> 00:35:03,533 stretched into a long, thin stream of fundamental particles 608 00:35:03,535 --> 00:35:06,302 that would then wind their way into the black hole. 609 00:35:06,304 --> 00:35:12,041 It would actively feast on me in a matter of seconds. 610 00:35:12,043 --> 00:35:15,445 Narrator: But if Paul or an interstellar robotic probe 611 00:35:15,447 --> 00:35:17,780 visited a supermassive black hole 612 00:35:17,782 --> 00:35:20,316 or even an ultramassive black hole, 613 00:35:20,318 --> 00:35:25,121 they wouldn't be immediately ripped to shreds. 614 00:35:25,123 --> 00:35:27,190 One of the most fun questions about black holes is, 615 00:35:27,192 --> 00:35:29,125 how close could you get to a black hole 616 00:35:29,127 --> 00:35:31,327 before the gravity would rip you apart? 617 00:35:31,329 --> 00:35:34,597 And that actually depends on the volume of the black hole. 618 00:35:34,599 --> 00:35:38,936 If the black hole is very large, you could get very, very close. 619 00:35:38,938 --> 00:35:40,536 Bullock: The more massive they are, 620 00:35:40,538 --> 00:35:43,806 the slightly softer they are in how they tear things apart, 621 00:35:43,808 --> 00:35:45,876 so a supermassive black hole, actually -- 622 00:35:45,878 --> 00:35:48,077 you can cross within the event horizon 623 00:35:48,079 --> 00:35:50,546 and not really notice it. 624 00:35:50,548 --> 00:35:52,015 You're never gonna get back out, 625 00:35:52,017 --> 00:35:54,149 but you won't necessarily be stretched to your death 626 00:35:54,151 --> 00:35:55,818 while you cross inside. 627 00:35:58,556 --> 00:36:01,691 Narrator: So a probe could visit a supermassive black hole 628 00:36:01,693 --> 00:36:03,426 and not be destroyed... 629 00:36:05,830 --> 00:36:08,230 ...until it crossed the event horizon 630 00:36:08,232 --> 00:36:10,533 and traveled deep inside. 631 00:36:12,637 --> 00:36:15,238 Then it would be torn to pieces. 632 00:36:17,642 --> 00:36:23,512 But microscopic black holes are currently just a theory. 633 00:36:23,514 --> 00:36:26,782 Mingarelli: Microscopic black holes have been the focus 634 00:36:26,784 --> 00:36:29,051 for some researchers for many years, 635 00:36:29,053 --> 00:36:30,653 but currently there's no evidence 636 00:36:30,655 --> 00:36:32,689 to support their existence. 637 00:36:35,527 --> 00:36:38,794 Narrator: Microscopic primordial black holes may or may not 638 00:36:38,796 --> 00:36:41,364 have been around since the big bang. 639 00:36:43,668 --> 00:36:48,137 Now scientists have discovered supermassive black holes 640 00:36:48,139 --> 00:36:51,340 from the very early universe. 641 00:36:51,342 --> 00:36:56,412 They're shedding light on one of the most mysterious eras, 642 00:36:56,414 --> 00:36:59,081 the cosmic dark ages. 643 00:36:59,083 --> 00:37:02,285 �� 644 00:37:08,759 --> 00:37:16,700 �� 645 00:37:16,702 --> 00:37:20,302 narrator: Black holes don't just shape the universe now. 646 00:37:20,304 --> 00:37:24,273 They've been shaping it from almost the dawn of time. 647 00:37:26,310 --> 00:37:29,044 Scientists think black holes may have triggered 648 00:37:29,046 --> 00:37:32,115 one of the universe's greatest transformations -- 649 00:37:32,117 --> 00:37:37,186 turning from dark and foggy to transparent and light. 650 00:37:37,188 --> 00:37:44,727 �� 651 00:37:44,729 --> 00:37:46,329 at the beginning of time, 652 00:37:46,331 --> 00:37:50,500 the universe was a tiny ball of super-hot energy -- 653 00:37:50,502 --> 00:37:53,536 the big bang. 654 00:37:53,538 --> 00:37:57,406 Shortly after our big bang, our universe was shining bright 655 00:37:57,408 --> 00:38:01,410 because it was full of hot, glowing gas. 656 00:38:01,412 --> 00:38:05,082 Then it cooled off and entered the so-called dark ages 657 00:38:05,084 --> 00:38:09,485 until eventually something lit it up again. 658 00:38:09,487 --> 00:38:12,221 It's one of the biggest changes that happened in our universe. 659 00:38:12,223 --> 00:38:17,492 Someone switched the lights on and transformed the universe. 660 00:38:17,494 --> 00:38:18,895 Narrator: During the dark ages, 661 00:38:18,897 --> 00:38:22,698 the universe was blanketed in a thick fog. 662 00:38:22,700 --> 00:38:24,900 Then something lit it up 663 00:38:24,902 --> 00:38:29,305 in a process called reionization. 664 00:38:29,307 --> 00:38:30,840 We still don't really know for sure 665 00:38:30,842 --> 00:38:35,377 whether reionization was mainly caused by young stars 666 00:38:35,379 --> 00:38:39,782 or whether it was mainly black holes that ate stuff 667 00:38:39,784 --> 00:38:42,219 and spewed out a bunch of radiation. 668 00:38:45,123 --> 00:38:48,458 Narrator: Then in December of 2017, 669 00:38:48,460 --> 00:38:52,995 researchers in Chile scan a region of space so far away 670 00:38:52,997 --> 00:38:58,267 it takes light 13 billion years to reach us. 671 00:38:58,269 --> 00:39:03,005 They spot an object from just 690 million years 672 00:39:03,007 --> 00:39:04,606 after the big bang 673 00:39:04,608 --> 00:39:10,345 when the universe was only 5% of its current age. 674 00:39:10,347 --> 00:39:16,652 It's called quasar j1342+0928. 675 00:39:19,757 --> 00:39:22,357 The thing that's so amazing about this farthest quasar 676 00:39:22,359 --> 00:39:27,096 is we may actually have seen the boundary of these dark ages. 677 00:39:27,098 --> 00:39:31,033 This particular supermassive black hole/quasar tells us 678 00:39:31,035 --> 00:39:35,237 something about the formation of the early universe. 679 00:39:35,239 --> 00:39:38,241 Narrator: It's thought that quasars helped drag the universe 680 00:39:38,243 --> 00:39:40,309 out of the dark ages. 681 00:39:40,311 --> 00:39:42,845 They gobbled up so much hydrogen gas 682 00:39:42,847 --> 00:39:46,650 and belched out jets of energy 683 00:39:46,652 --> 00:39:49,185 and cleared up the fog. 684 00:39:49,187 --> 00:39:51,988 Those jets could have actually put so much energy 685 00:39:51,990 --> 00:39:55,257 into the universe that it made it clear again. 686 00:39:55,259 --> 00:39:57,260 We may actually be seeing the moment 687 00:39:57,262 --> 00:40:00,830 where something punches through this boundary of the dark ages. 688 00:40:05,269 --> 00:40:07,670 Narrator: Pockets of reionization opened up 689 00:40:07,672 --> 00:40:10,540 throughout the early universe. 690 00:40:10,542 --> 00:40:14,644 They came in different sizes, depending on what created them. 691 00:40:17,415 --> 00:40:19,348 Tegmark: While our universe was being reionized, 692 00:40:19,350 --> 00:40:21,417 there was kind of, like, all these holes 693 00:40:21,419 --> 00:40:23,485 that kept growing. 694 00:40:23,487 --> 00:40:27,823 If the reionization was made by a large number of little stars, 695 00:40:27,825 --> 00:40:29,759 you would have many, many small holes, 696 00:40:29,761 --> 00:40:32,762 much like a sponge, 697 00:40:32,764 --> 00:40:36,098 whereas if you had a small number 698 00:40:36,100 --> 00:40:37,501 of monster black holes doing it, 699 00:40:37,503 --> 00:40:41,805 you'd have a lot of big holes, like in Swiss cheese. 700 00:40:46,711 --> 00:40:49,979 Narrator: At present, we can't measure the ionized pockets 701 00:40:49,981 --> 00:40:53,049 to determine if it was stars or black holes 702 00:40:53,051 --> 00:40:55,117 that lit up the early universe. 703 00:40:55,119 --> 00:40:58,187 Perhaps it was both -- 704 00:40:58,189 --> 00:41:02,058 black holes and stars working together. 705 00:41:02,060 --> 00:41:07,730 �� 706 00:41:07,732 --> 00:41:09,799 the more we investigate black holes, 707 00:41:09,801 --> 00:41:11,801 the more we learn about their role 708 00:41:11,803 --> 00:41:14,136 as architects of the universe. 709 00:41:14,138 --> 00:41:23,145 �� 710 00:41:23,147 --> 00:41:25,748 I think scientists of my generation are very lucky 711 00:41:25,750 --> 00:41:31,487 to be able to be at the beginning of this revolution. 712 00:41:31,489 --> 00:41:34,623 Narrator: We used to portray black holes as monsters. 713 00:41:34,625 --> 00:41:37,159 Now we know that, without them, 714 00:41:37,161 --> 00:41:40,162 the universe would be a very different place. 715 00:41:40,164 --> 00:41:42,032 They made life possible. 716 00:41:42,034 --> 00:41:45,701 Without black holes, we probably wouldn't exist. 717 00:41:45,703 --> 00:41:46,970 Narrator: We're discovering 718 00:41:46,972 --> 00:41:50,239 just how black holes shaped the universe, 719 00:41:50,241 --> 00:41:56,378 but the more we learn, the more questions they pose. 720 00:41:56,380 --> 00:41:58,513 I've spent my career studying black holes, 721 00:41:58,515 --> 00:42:01,917 and I want to spend the rest of my career studying black holes, 722 00:42:01,919 --> 00:42:05,255 and I guarantee you that, at the end of my career, 723 00:42:05,257 --> 00:42:07,857 on the day I retire, I will probably have 724 00:42:07,859 --> 00:42:11,360 more questions about black holes than I do today. 725 00:42:13,931 --> 00:42:15,664 This is an incredibly exciting time 726 00:42:15,666 --> 00:42:17,266 for black-hole science. 727 00:42:17,268 --> 00:42:19,135 Who knows what we're gonna discover? 728 00:42:19,137 --> 00:42:28,511 �� 58574

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