All language subtitles for S05E03 - Black Holes - The Secret Origin.en

af Afrikaans
sq Albanian
am Amharic
ar Arabic
hy Armenian
az Azerbaijani
eu Basque
be Belarusian
bn Bengali
bs Bosnian
bg Bulgarian
ca Catalan
ceb Cebuano
ny Chichewa
zh-CN Chinese (Simplified)
zh-TW Chinese (Traditional)
co Corsican
hr Croatian
cs Czech
da Danish
nl Dutch
en English
eo Esperanto
et Estonian
tl Filipino
fi Finnish
fr French
fy Frisian
gl Galician
ka Georgian
de German
el Greek
gu Gujarati
ht Haitian Creole
ha Hausa
haw Hawaiian
iw Hebrew
hi Hindi
hmn Hmong
hu Hungarian
is Icelandic
ig Igbo
id Indonesian
ga Irish
it Italian
ja Japanese
jw Javanese
kn Kannada
kk Kazakh
km Khmer
ko Korean
ku Kurdish (Kurmanji)
ky Kyrgyz
lo Lao
la Latin
lv Latvian
lt Lithuanian
lb Luxembourgish
mk Macedonian
mg Malagasy
ms Malay
ml Malayalam
mt Maltese
mi Maori
mr Marathi
mn Mongolian
my Myanmar (Burmese)
ne Nepali
no Norwegian
ps Pashto
fa Persian
pl Polish
pt Portuguese
pa Punjabi
ro Romanian Download
ru Russian
sm Samoan
gd Scots Gaelic
sr Serbian
st Sesotho
sn Shona
sd Sindhi
si Sinhala
sk Slovak
sl Slovenian
so Somali
es Spanish
su Sundanese
sw Swahili
sv Swedish
tg Tajik
ta Tamil
te Telugu
th Thai
tr Turkish
uk Ukrainian
ur Urdu
uz Uzbek
vi Vietnamese
cy Welsh
xh Xhosa
yi Yiddish
yo Yoruba
zu Zulu
or Odia (Oriya)
rw Kinyarwanda
tk Turkmen
tt Tatar
ug Uyghur
Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:02,498 --> 00:00:05,306 Two black holes circle each other 2 00:00:05,307 --> 00:00:08,175 in a dance of death. 3 00:00:08,176 --> 00:00:10,153 They spiral inwards, 4 00:00:10,154 --> 00:00:13,715 their immense gravities pulling them ever closer. 5 00:00:17,415 --> 00:00:18,838 When they finally collide, 6 00:00:18,839 --> 00:00:21,410 it's one of the most powerful events 7 00:00:21,411 --> 00:00:24,714 since the big bang. 8 00:00:24,715 --> 00:00:26,851 This explosive mystery 9 00:00:26,861 --> 00:00:30,748 sends ripples across the world of science. 10 00:00:30,749 --> 00:00:32,400 But can it also answer 11 00:00:32,401 --> 00:00:36,357 one of the most pressing questions in cosmology? 12 00:00:36,367 --> 00:00:41,510 How do supermassive black holes grow so large? 13 00:00:41,511 --> 00:00:44,478 ...Captions by Vitac... www.Vitac.Com 14 00:00:44,478 --> 00:00:47,654 Captions paid for by Discovery communications 15 00:00:57,714 --> 00:00:58,969 In the known universe, 16 00:00:58,970 --> 00:01:03,430 there are roughly 2,000 billion galaxies. 17 00:01:03,431 --> 00:01:06,724 Each one has a different shape and size. 18 00:01:06,725 --> 00:01:10,493 But they may all have one feature in common... 19 00:01:10,494 --> 00:01:15,865 a supermassive black hole buried at their center. 20 00:01:15,875 --> 00:01:18,902 As its name says, it is supermassive. 21 00:01:18,912 --> 00:01:20,325 And here, we're talking about objects 22 00:01:20,326 --> 00:01:22,897 that are millions or billions of times 23 00:01:22,898 --> 00:01:24,520 the mass of the Sun. 24 00:01:27,517 --> 00:01:29,168 Supermassive black holes 25 00:01:29,169 --> 00:01:31,741 are so big that we need a special scale 26 00:01:31,751 --> 00:01:33,235 for measuring them. 27 00:01:35,876 --> 00:01:37,982 A solar mass is the mass of the Sun. 28 00:01:37,983 --> 00:01:41,414 So when we study the universe, 29 00:01:41,415 --> 00:01:43,333 we have to use the tools that we have in hand. 30 00:01:43,334 --> 00:01:45,935 And what's the most massive thing that we have around us? 31 00:01:45,936 --> 00:01:47,982 It's the Sun. And so we refer to things 32 00:01:47,983 --> 00:01:50,099 in multiples of the mass of the Sun 33 00:01:50,100 --> 00:01:53,759 because it just makes it easier to wrap our heads around. 34 00:01:53,760 --> 00:01:56,004 However, if you have something that's 17 billion times 35 00:01:56,005 --> 00:01:58,349 the mass of the Sun, that's pretty difficult 36 00:01:58,350 --> 00:02:00,357 to wrap your head around anyway. 37 00:02:00,358 --> 00:02:02,404 But we know that those kinds of black holes 38 00:02:02,405 --> 00:02:06,134 live in the centers of galaxies. 39 00:02:06,135 --> 00:02:09,635 The supermassive black hole 40 00:02:09,636 --> 00:02:13,661 the milky way, is called Sagittarius "a" -star. 41 00:02:13,662 --> 00:02:17,520 It weighs in at 4 million solar masses. 42 00:02:17,530 --> 00:02:20,200 But compared to the other supermassive black holes 43 00:02:20,201 --> 00:02:22,870 out there, it's puny. 44 00:02:22,871 --> 00:02:25,116 This is probably one of the only contexts 45 00:02:25,117 --> 00:02:28,380 where you would think that our supermassive black hole 46 00:02:28,381 --> 00:02:30,132 isn't very supermassive. 47 00:02:32,773 --> 00:02:34,089 The supermassive black hole 48 00:02:34,098 --> 00:02:36,372 in our neighboring galaxy, Andromeda, 49 00:02:36,373 --> 00:02:40,596 is 25 times larger than Sagittarius "A" -star, 50 00:02:40,597 --> 00:02:44,485 coming in at 100 million solar masses. 51 00:02:44,495 --> 00:02:46,531 But compared to the largest monsters 52 00:02:46,532 --> 00:02:49,509 out in the universe, it's a runt. 53 00:02:49,510 --> 00:02:53,634 O.J. 287's primary supermassive black hole 54 00:02:53,635 --> 00:02:57,720 weighs in at 18 billion solar masses. 55 00:02:57,730 --> 00:03:02,180 And the black hole in the core of galaxy NGC 4889 56 00:03:02,181 --> 00:03:06,433 in the coma cluster weighs 21 billion solar stars. 57 00:03:06,434 --> 00:03:08,580 That's over 5,000 times larger 58 00:03:08,581 --> 00:03:10,599 than Sagittarius "a" -star. 59 00:03:12,577 --> 00:03:14,189 These are incredible things 60 00:03:14,199 --> 00:03:18,818 that are more massive than some galaxies. 61 00:03:18,819 --> 00:03:23,338 Now astronomers may have ma 62 00:03:23,339 --> 00:03:26,504 a giant, new supermassive black hole 63 00:03:26,505 --> 00:03:29,738 that's a mind-blowing 30 billion times 64 00:03:29,739 --> 00:03:31,390 the mass of the Sun. 65 00:03:31,391 --> 00:03:32,706 It's a huge puzzle. 66 00:03:32,707 --> 00:03:37,425 And we have simply no idea how it got so big. 67 00:03:37,435 --> 00:03:41,451 It's a huge mystery how black 68 00:03:41,461 --> 00:03:43,339 we started finding black holes with millions 69 00:03:43,340 --> 00:03:45,684 and billions of times the Sun's mass. 70 00:03:45,685 --> 00:03:47,069 No one expected that. 71 00:03:47,070 --> 00:03:50,926 And we have no idea how they got to be so big. 72 00:03:50,927 --> 00:03:53,538 It's not entirely clear at this point 73 00:03:53,539 --> 00:03:57,000 how supermassive black holes can get to be the masses 74 00:03:57,001 --> 00:03:58,257 that they are today. 75 00:04:04,627 --> 00:04:06,773 Regular-sized black holes form 76 00:04:06,774 --> 00:04:10,502 when large stars over 20 times the mass of our sun 77 00:04:10,503 --> 00:04:11,917 crash and burn. 78 00:04:14,005 --> 00:04:15,913 When a large star runs out of fuel, 79 00:04:15,914 --> 00:04:19,078 the core stops generating enough outward force 80 00:04:19,079 --> 00:04:22,946 to counteract the power of gravity crushing inwards. 81 00:04:22,947 --> 00:04:24,490 As the star collapses, 82 00:04:24,500 --> 00:04:27,922 the outer part explodes in a supernova. 83 00:04:33,412 --> 00:04:35,350 The inner core shrinks 84 00:04:35,351 --> 00:04:38,327 from a sphere millions of miles wide 85 00:04:38,328 --> 00:04:40,999 to one just 10 miles across. 86 00:04:43,907 --> 00:04:45,687 It's like shrinking the earth down 87 00:04:45,688 --> 00:04:49,674 to the size of a golf ball. 88 00:04:49,684 --> 00:04:54,332 This rapid collapse creates a black hole. 89 00:04:54,333 --> 00:04:55,847 So we now have seen black holes 90 00:04:55,856 --> 00:04:58,160 that are solar-mass black holes 91 00:04:58,161 --> 00:04:59,576 and black holes that are million 92 00:04:59,586 --> 00:05:01,326 or billion-solar-mass black holes. 93 00:05:01,327 --> 00:05:04,660 And the question is, how do you get from one to the other? 94 00:05:07,202 --> 00:05:09,051 Do the giants somehow grow 95 00:05:09,052 --> 00:05:12,355 from a solar-mass black hole? 96 00:05:12,356 --> 00:05:14,462 One of the big puzzles today is, 97 00:05:14,463 --> 00:05:18,092 how do you make one of these supermassive black holes? 98 00:05:18,093 --> 00:05:20,535 One idea is, you get there by starting 99 00:05:20,536 --> 00:05:22,385 with a solar-mass black hole, 100 00:05:22,386 --> 00:05:23,770 having it grow through a stage 101 00:05:23,771 --> 00:05:25,323 of being an intermediate-mass black hole 102 00:05:25,324 --> 00:05:26,906 and then eventually getting to be 103 00:05:26,907 --> 00:05:29,814 a supermassive black hole. 104 00:05:29,815 --> 00:05:32,812 Theoretically, intermediate-mass black holes 105 00:05:32,822 --> 00:05:37,173 should be between 100 and 100,000 solar masses. 106 00:05:37,174 --> 00:05:39,814 But we've never seen one. 107 00:05:39,815 --> 00:05:41,990 Part of the mystery of supermassive black holes 108 00:05:41,991 --> 00:05:45,057 is that black holes seem to occur in two flavors. 109 00:05:45,058 --> 00:05:46,808 You have ones that are only a couple times 110 00:05:46,809 --> 00:05:47,935 the mass of the Sun. 111 00:05:47,936 --> 00:05:49,548 And you have ones that are millions 112 00:05:49,549 --> 00:05:51,793 or billions of times the mass of the Sun. 113 00:05:51,794 --> 00:05:55,097 So we have small and extra large. 114 00:05:55,098 --> 00:05:57,204 If we think of the stellar-mass black hole 115 00:05:57,205 --> 00:05:58,955 as sort of the baby black holes, 116 00:05:58,956 --> 00:06:01,893 and the supermassive black holes as the grown-up black holes, 117 00:06:01,893 --> 00:06:03,574 we're missing the teenage black holes. 118 00:06:03,575 --> 00:06:05,553 Where are these black holes that have masses 119 00:06:05,563 --> 00:06:08,956 that are between stellar mass and supermassive? 120 00:06:11,172 --> 00:06:13,179 They're sort of like a holy grail 121 00:06:13,180 --> 00:06:14,999 for black hole hunters. 122 00:06:15,000 --> 00:06:17,076 Where are these things? Where can we find them? 123 00:06:17,077 --> 00:06:19,648 And how do you make them? 124 00:06:19,649 --> 00:06:22,487 Then astronomers caught a break. 125 00:06:22,488 --> 00:06:24,634 They picked up a burst of energy 126 00:06:24,635 --> 00:06:30,075 coming from the NGC 1399 galaxy. 127 00:06:30,085 --> 00:06:31,301 It was the death throes 128 00:06:31,302 --> 00:06:35,594 of a star being eaten by a black hole. 129 00:06:35,595 --> 00:06:37,898 When they measured its size, they discovered it was 130 00:06:37,899 --> 00:06:41,172 an elusive intermediate-mass black hole. 131 00:06:41,173 --> 00:06:45,030 The missing link had been found. 132 00:06:45,031 --> 00:06:47,078 But when scientists did the math 133 00:06:47,079 --> 00:06:50,312 to see if such an intermediate-mass black hole 134 00:06:50,313 --> 00:06:53,151 could grow into a supermassive black hole, 135 00:06:53,152 --> 00:06:54,833 they hit a snag. 136 00:06:54,834 --> 00:06:56,752 There hasn't been enough time 137 00:06:56,753 --> 00:06:58,463 since the birth of the universe 138 00:06:58,464 --> 00:07:00,738 for an intermediate-mass black hole 139 00:07:00,739 --> 00:07:02,588 to eat enough stars 140 00:07:02,589 --> 00:07:05,853 to grow into a supermassive black hole. 141 00:07:05,863 --> 00:07:08,297 It doesn't seem like there's enough time 142 00:07:08,306 --> 00:07:11,965 for black holes to get as big as we see them. 143 00:07:11,966 --> 00:07:15,596 But supermassives are everywhere we look. 144 00:07:15,597 --> 00:07:16,911 How did they get there? 145 00:07:16,912 --> 00:07:19,326 And how did they grow so huge? 146 00:07:33,283 --> 00:07:36,655 In our universe, we've detected small black holes. 147 00:07:36,656 --> 00:07:38,831 And we've seen monsters, 148 00:07:38,832 --> 00:07:41,038 supermassive black holes 149 00:07:41,048 --> 00:07:43,817 billions of times the mass of our sun. 150 00:07:43,818 --> 00:07:47,872 But we'd found almost none in between. 151 00:07:47,873 --> 00:07:52,462 So how do you get from a small black hole to a giant one? 152 00:07:52,463 --> 00:07:54,471 One of the most important outstanding questions 153 00:07:54,481 --> 00:07:55,658 in cosmology is, 154 00:07:55,668 --> 00:07:57,607 how did supermassive black holes 155 00:07:57,617 --> 00:07:59,228 get as big as they are? 156 00:07:59,229 --> 00:08:02,294 And when did that happen? 157 00:08:02,295 --> 00:08:06,261 Black holes are normally S 158 00:08:06,262 --> 00:08:09,594 an all-you-can-eat buffet. 159 00:08:09,595 --> 00:08:11,771 One of the best ideas for how black holes grow 160 00:08:11,772 --> 00:08:12,987 is that black holes do 161 00:08:12,988 --> 00:08:14,610 what we expect black holes to do, 162 00:08:14,611 --> 00:08:15,866 and that is eat stuff. 163 00:08:15,867 --> 00:08:17,280 For a black hole, 164 00:08:17,281 --> 00:08:19,496 it's almost as if the universe is its restaurant. 165 00:08:19,497 --> 00:08:23,156 And on its menu, you'll find stars, planets, 166 00:08:23,157 --> 00:08:26,064 and clouds of gas and dust. 167 00:08:26,065 --> 00:08:28,004 So is binge-eating the answer 168 00:08:28,014 --> 00:08:31,307 to growing a supermassive black hole? 169 00:08:31,308 --> 00:08:34,770 Theoretically, black holes should keep on growing forever 170 00:08:34,780 --> 00:08:37,746 as they consume more and more food. 171 00:08:37,747 --> 00:08:39,556 But recent discoveries suggest 172 00:08:39,557 --> 00:08:42,267 that the universe puts them on a diet, 173 00:08:42,268 --> 00:08:44,542 controlling how much they eat. 174 00:08:44,543 --> 00:08:46,421 Black holes are hungry. They like to eat. 175 00:08:46,422 --> 00:08:47,875 But sometimes, they eat too much, 176 00:08:47,876 --> 00:08:49,499 and they burp it up. 177 00:08:57,818 --> 00:08:59,795 February 2015. 178 00:08:59,796 --> 00:09:02,495 Astronomers report something unusual 179 00:09:02,496 --> 00:09:05,800 in the galaxy NGC 2276. 180 00:09:08,174 --> 00:09:10,814 It looked like something had taken a bite 181 00:09:10,815 --> 00:09:13,061 out of one of its spiral arms. 182 00:09:14,713 --> 00:09:16,294 Sitting alone in the void 183 00:09:16,295 --> 00:09:18,639 was an intermediate-mass black hole, 184 00:09:18,640 --> 00:09:23,258 about 50,000 times the mass of the Sun. 185 00:09:23,259 --> 00:09:25,108 One theory was that the black hole 186 00:09:25,109 --> 00:09:27,117 had eaten everything around it, 187 00:09:27,127 --> 00:09:29,163 creating the dead zone. 188 00:09:29,164 --> 00:09:31,242 But the detection of a burst of energy 189 00:09:31,251 --> 00:09:32,863 from the black hole suggests 190 00:09:32,864 --> 00:09:34,910 it may have tried to eat too much 191 00:09:34,911 --> 00:09:38,442 and, in the process, destroyed its food source, 192 00:09:38,443 --> 00:09:42,043 burping so hard, its food was blasted away. 193 00:09:47,751 --> 00:09:50,649 Turns out that black holes are actually very messy 194 00:09:50,659 --> 00:09:54,051 a lot of matter gets thrown off as it tries to absorb it. 195 00:09:54,052 --> 00:09:56,069 So things move in, gets hot. 196 00:09:56,070 --> 00:09:59,858 But then a lot of it gets thrown all the way back out. 197 00:09:59,868 --> 00:10:02,142 Black holes are not vacuums in space. 198 00:10:02,143 --> 00:10:04,318 They do not just eat everything around them. 199 00:10:04,319 --> 00:10:06,624 And so they are messy. Some things get in. 200 00:10:06,634 --> 00:10:08,513 And they take that on. And it grows their mass. 201 00:10:08,514 --> 00:10:13,063 And some things are just flung out as they're eating. 202 00:10:13,064 --> 00:10:16,724 The enormous gravity of black holes sucks gas, dust, 203 00:10:16,734 --> 00:10:18,543 and even stars towards them. 204 00:10:18,544 --> 00:10:20,849 Everybody's been to an all-you-can-eat buffet. 205 00:10:20,858 --> 00:10:23,063 But let's be honest. There really is a limit 206 00:10:23,064 --> 00:10:25,338 to how much you can eat. 207 00:10:25,339 --> 00:10:28,543 Black holes are gluttons. They're greedy. 208 00:10:28,544 --> 00:10:31,451 They don't really know when they've eaten too much. 209 00:10:31,452 --> 00:10:35,507 They just keep on cramming in more and more food. 210 00:10:35,508 --> 00:10:36,862 It doesn't just fall in. 211 00:10:36,863 --> 00:10:39,404 It has to go down the drain, more or less. 212 00:10:39,405 --> 00:10:42,699 And so it forms this disk around the hole. 213 00:10:42,709 --> 00:10:44,746 And as it does that, there's a lot of turbulence 214 00:10:44,747 --> 00:10:46,002 and magnetic fields 215 00:10:46,003 --> 00:10:48,544 and a witch's brew of forces going on there 216 00:10:48,545 --> 00:10:51,611 that get it really hot. 217 00:10:51,612 --> 00:10:54,024 As the gas and dust swirls around, 218 00:10:54,025 --> 00:10:55,539 it heats up, 219 00:10:55,549 --> 00:10:58,813 pushing temperatures to millions of degrees Fahrenheit. 220 00:11:02,413 --> 00:11:04,984 This swirl, called the accretion disk, 221 00:11:04,985 --> 00:11:07,923 also generates powerful magnetic fields. 222 00:11:10,030 --> 00:11:12,967 These fields are dragged by the SPiN of the black hole 223 00:11:12,968 --> 00:11:17,221 and become focused above the poles. 224 00:11:17,231 --> 00:11:18,477 As energy builds up, 225 00:11:18,478 --> 00:11:20,920 the magnetic fields become so compressed 226 00:11:20,921 --> 00:11:25,777 they blast out super-energized particles. 227 00:11:25,778 --> 00:11:28,775 These beams can actually be incredibly violent. 228 00:11:28,785 --> 00:11:30,129 Matter is flung out 229 00:11:30,130 --> 00:11:32,572 at a large fraction of the speed of light. 230 00:11:32,573 --> 00:11:34,195 It's a tremendous wind 231 00:11:34,196 --> 00:11:38,280 that blows very hard away from the black hole. 232 00:11:38,281 --> 00:11:40,100 The jet hits the gas clouds 233 00:11:40,101 --> 00:11:41,653 surrounding the black hole, 234 00:11:41,654 --> 00:11:44,096 blowing the buffet away. 235 00:11:44,097 --> 00:11:46,401 If they eat too much, 236 00:11:46,402 --> 00:11:48,181 they can basically blow everything 237 00:11:48,182 --> 00:11:50,367 that's in their vicinity away. 238 00:11:50,368 --> 00:11:54,819 They lose their food supply. And then they're gonna starve. 239 00:11:54,820 --> 00:11:57,391 They can kind of shoot themselves in the foot. 240 00:11:57,392 --> 00:11:59,271 With no food available, 241 00:11:59,281 --> 00:12:01,684 the black hole stops growing. 242 00:12:01,685 --> 00:12:03,998 Astronomers think that's what happened 243 00:12:03,999 --> 00:12:05,779 to the intermediate-mass black hole 244 00:12:05,780 --> 00:12:07,728 they discovered in the dead zone. 245 00:12:13,040 --> 00:12:15,345 These burps may regulate star formation 246 00:12:15,355 --> 00:12:19,607 and stop the black hole from getting obese. 247 00:12:19,608 --> 00:12:21,160 But over time, 248 00:12:21,161 --> 00:12:23,238 the black hole will start eating again 249 00:12:23,239 --> 00:12:25,809 as gas falls back towards it. 250 00:12:25,810 --> 00:12:28,778 But can an intermediate-mass black hole eat enough 251 00:12:28,788 --> 00:12:31,388 to become a supermassive black hole 252 00:12:31,389 --> 00:12:34,851 weighing billions of solar masses? 253 00:12:34,861 --> 00:12:38,550 Could that black hole become so obese by eating? 254 00:12:38,551 --> 00:12:40,400 That's a really interesting question. 255 00:12:40,401 --> 00:12:42,942 You'd have to eat a heck of a lot 256 00:12:42,943 --> 00:12:46,107 to get that fat. 257 00:12:46,108 --> 00:12:48,916 When you think about it, if you imagine an average galaxy 258 00:12:48,917 --> 00:12:50,895 has 100 billion stars, 259 00:12:50,896 --> 00:12:52,607 the black hole would have to eat one 260 00:12:52,617 --> 00:12:55,188 in every five stars in the galaxy. 261 00:12:55,189 --> 00:12:57,859 The universe is old. But is it really old enough 262 00:12:57,860 --> 00:13:01,717 that black holes have had time to consume billions of stars? 263 00:13:01,727 --> 00:13:03,705 That seems kind of unlikely. 264 00:13:03,706 --> 00:13:05,416 It doesn't seem to add up. 265 00:13:05,417 --> 00:13:06,939 We need some other way 266 00:13:06,940 --> 00:13:08,918 to make these supermassive black holes. 267 00:13:08,919 --> 00:13:12,015 And the question is, what is that? 268 00:13:12,025 --> 00:13:14,656 Maybe we've been making this all too complicated. 269 00:13:14,666 --> 00:13:19,275 Maybe to get a big black hole is to start big in the first place. 270 00:13:19,285 --> 00:13:22,708 So how can black holes start big? 271 00:13:22,717 --> 00:13:26,080 To answer that question, scientists had to journey back 272 00:13:26,081 --> 00:13:28,622 to the very start of the universe, 273 00:13:28,623 --> 00:13:32,154 to a mysterious time called the dark ages. 274 00:13:51,492 --> 00:13:53,905 As we look out into the universe, 275 00:13:53,906 --> 00:13:58,426 we're seeing farther and farther back in time. 276 00:13:58,427 --> 00:13:59,711 We have now looked back 277 00:13:59,712 --> 00:14:02,817 over 12 billion years 278 00:14:02,818 --> 00:14:06,250 to the time when the cosmos was still an infant. 279 00:14:06,251 --> 00:14:11,492 And what we found was a huge surprise. 280 00:14:11,493 --> 00:14:13,075 We had made the assumption 281 00:14:13,076 --> 00:14:15,351 that as you look farther out into the universe, 282 00:14:15,361 --> 00:14:16,676 the black holes would be smaller. 283 00:14:16,677 --> 00:14:18,388 They haven't had much time to grow. 284 00:14:18,398 --> 00:14:20,998 But now we've found a 12-billion-solar-mass 285 00:14:20,999 --> 00:14:23,343 black hole that's actually less 286 00:14:23,344 --> 00:14:24,925 than a billion years into the universe. 287 00:14:24,926 --> 00:14:26,775 How did this thing form so early? 288 00:14:26,776 --> 00:14:28,328 How did it grow so fast? 289 00:14:28,329 --> 00:14:30,672 This is like walking into a delivery room 290 00:14:30,673 --> 00:14:32,819 and finding a 100-pound baby. 291 00:14:32,820 --> 00:14:35,490 I mean, how does that even happen? 292 00:14:35,491 --> 00:14:37,103 It doesn't make any sense. 293 00:14:37,113 --> 00:14:41,129 Physics tells us no black hole could swallow enough stuff 294 00:14:41,139 --> 00:14:44,333 to get that big that quickly. 295 00:14:44,334 --> 00:14:46,708 There really wasn't enough time between the big bang 296 00:14:46,718 --> 00:14:48,656 and when we're studying these things 297 00:14:48,657 --> 00:14:51,130 for them to grow to such large sizes 298 00:14:51,139 --> 00:14:53,710 just by eating matter around them. 299 00:14:53,711 --> 00:14:57,599 So if there's not enough time 300 00:14:57,609 --> 00:15:01,831 maybe they're born supermassive. 301 00:15:01,832 --> 00:15:06,907 To understand how, we have to travel back even farther, 302 00:15:06,917 --> 00:15:09,716 to not long after the birth of the universe. 303 00:15:12,426 --> 00:15:14,464 The early universe was definitely 304 00:15:14,474 --> 00:15:17,045 a much more compact 305 00:15:17,046 --> 00:15:18,627 and richer place for material. 306 00:15:18,628 --> 00:15:20,972 It was smaller, and it was denser. 307 00:15:20,973 --> 00:15:22,950 Things were much closer. It was hotter. 308 00:15:22,951 --> 00:15:28,331 It was just a much more intense place to be. 309 00:15:28,332 --> 00:15:32,684 Clouds of hydrogen and helium gas clumped together. 310 00:15:32,685 --> 00:15:35,958 As the clouds grew, so did their gravity, 311 00:15:35,959 --> 00:15:39,451 sucking in more and more gas. 312 00:15:39,460 --> 00:15:41,132 Eventually, the ball of gas 313 00:15:41,142 --> 00:15:44,109 became so dense, it collapsed, 314 00:15:44,110 --> 00:15:48,036 triggering nuclear fusion. 315 00:15:48,037 --> 00:15:50,045 A star was born. 316 00:15:50,054 --> 00:15:52,625 These massive first stars 317 00:15:52,626 --> 00:15:56,256 are called population III stars. 318 00:15:56,257 --> 00:15:58,600 Because there was so much food around, 319 00:15:58,601 --> 00:16:01,567 these stars were huge, 320 00:16:01,568 --> 00:16:05,791 many times bigger than any stars that exist today. 321 00:16:05,792 --> 00:16:08,304 We think a lot of these population III stars 322 00:16:08,305 --> 00:16:10,540 probably were incredibly massive, 323 00:16:10,550 --> 00:16:13,714 incredibly short-lived, and just blew up right away. 324 00:16:13,715 --> 00:16:17,108 They would've left massive black holes behind. 325 00:16:28,167 --> 00:16:29,849 With so much food available, 326 00:16:29,859 --> 00:16:33,776 these young, ravenous black holes, called quasars, 327 00:16:33,786 --> 00:16:36,219 started binge-eating 328 00:16:36,229 --> 00:16:39,097 and became incredibly bright. 329 00:16:39,098 --> 00:16:42,856 Billions of years later, we can still see their gluttony. 330 00:16:44,835 --> 00:16:47,969 The most luminous, bright objects in the universe 331 00:16:47,970 --> 00:16:49,423 are things called quasars. 332 00:16:49,424 --> 00:16:50,907 And it may seem kind of ironic. 333 00:16:50,908 --> 00:16:53,845 But what these really are are supermassive black holes. 334 00:16:53,846 --> 00:16:55,824 There's so much stuff trying to cram itself down 335 00:16:55,834 --> 00:16:59,356 the black hole that everything gets very hot, very energetic. 336 00:16:59,366 --> 00:17:01,966 And you can see them clear across the universe. 337 00:17:01,967 --> 00:17:04,934 But when we measured the size of the young quasars, 338 00:17:04,935 --> 00:17:09,029 we discovered they were already billions of solar masses. 339 00:17:09,030 --> 00:17:10,879 There's not enough time, 340 00:17:10,880 --> 00:17:13,322 a billion years after the universe was created, 341 00:17:13,323 --> 00:17:16,754 for them to get to a billion solar masses in... 342 00:17:16,755 --> 00:17:18,930 it's just too short a time. 343 00:17:18,931 --> 00:17:21,868 So the question becomes, 344 00:17:21,869 --> 00:17:25,035 that are this big in that small amount of time? 345 00:17:25,044 --> 00:17:26,290 We need some other way 346 00:17:26,291 --> 00:17:28,733 of growing these supermassive black holes. 347 00:17:28,734 --> 00:17:30,652 There needs to be some other mechanism 348 00:17:30,653 --> 00:17:32,889 that allows them to get that massive so early. 349 00:17:32,899 --> 00:17:35,766 But what is that? 350 00:17:35,767 --> 00:17:40,811 A clue can be found in the very early universe. 351 00:17:40,812 --> 00:17:43,452 The early universe is still so much of a mystery to us. 352 00:17:43,453 --> 00:17:45,431 We know that conditions were very different. 353 00:17:45,441 --> 00:17:48,408 It was denser. There was a lot more material. 354 00:17:48,409 --> 00:17:51,642 This period is called the dark ages. 355 00:17:51,643 --> 00:17:53,423 During the dark age, we know 356 00:17:53,424 --> 00:17:56,223 that there was basically nothing happening. 357 00:17:56,233 --> 00:17:57,577 Matter existed. 358 00:17:57,578 --> 00:17:59,595 We think that there was hydrogen and helium gas 359 00:17:59,596 --> 00:18:02,464 but really not much else. 360 00:18:02,465 --> 00:18:04,442 There were a few stars around, 361 00:18:04,443 --> 00:18:07,746 but nothing large enough to form giant black holes. 362 00:18:07,747 --> 00:18:10,615 But there were huge clouds of gas. 363 00:18:10,616 --> 00:18:13,691 And because the universe was much smaller and denser, 364 00:18:13,692 --> 00:18:17,321 the clouds were much thicker. 365 00:18:17,322 --> 00:18:20,585 The idea is that from these basic ingredients, 366 00:18:20,586 --> 00:18:22,435 gravity and gas, 367 00:18:22,436 --> 00:18:26,461 the cosmos built massive black holes. 368 00:18:26,462 --> 00:18:28,668 Somehow, the universe has created a shortcut 369 00:18:28,678 --> 00:18:29,696 to the black hole. 370 00:18:29,697 --> 00:18:31,606 We've typically thought of it as, 371 00:18:31,616 --> 00:18:33,821 cloud of gas collapses into a star, 372 00:18:33,822 --> 00:18:37,322 star evolves, star dies, leaves behind a black hole. 373 00:18:37,323 --> 00:18:38,935 Perhaps the universe has found a way 374 00:18:38,936 --> 00:18:41,013 to skip the star phase 375 00:18:41,023 --> 00:18:42,902 and go directly to the black hole. 376 00:18:46,038 --> 00:18:50,587 Clouds of gas may have built massive black holes 377 00:18:50,588 --> 00:18:54,089 in a process called direct collapse. 378 00:18:54,090 --> 00:18:56,888 As they collapsed, they never even formed a star. 379 00:18:56,889 --> 00:18:59,865 They just collapsed straight into a giant black hole. 380 00:18:59,866 --> 00:19:01,410 Through this direct collapse theory, 381 00:19:01,419 --> 00:19:03,723 you can form really big black holes. 382 00:19:03,724 --> 00:19:06,236 Imagine what it's like seeing one of these giant clouds 383 00:19:06,237 --> 00:19:08,343 of gas collapsing down into a black hole. 384 00:19:08,344 --> 00:19:10,262 You might think you start with, okay, 385 00:19:10,263 --> 00:19:12,240 cloud of gas slowly collapsing, 386 00:19:12,241 --> 00:19:14,150 and, boop, it's a black hole. 387 00:19:14,160 --> 00:19:16,394 That wouldn't be the case. It would be more like 388 00:19:16,395 --> 00:19:18,610 giant cloud of gas starts collapsing, 389 00:19:18,611 --> 00:19:21,509 then... aah! Black hole. 390 00:19:21,519 --> 00:19:23,556 It's believed that direct collapse 391 00:19:23,557 --> 00:19:25,436 could have created black holes 392 00:19:25,446 --> 00:19:28,215 up to a million times the mass of the Sun, 393 00:19:28,216 --> 00:19:29,996 much bigger than from the collapse 394 00:19:29,997 --> 00:19:31,677 of a single star. 395 00:19:31,678 --> 00:19:33,062 These early black holes 396 00:19:33,063 --> 00:19:35,338 are sort of like the galaxies that never were. 397 00:19:35,348 --> 00:19:36,831 They were gonna make galaxies. 398 00:19:36,832 --> 00:19:40,126 But instead, they collapsed into very massive black holes. 399 00:19:42,114 --> 00:19:44,714 For direct collapse to form a black hole, 400 00:19:44,715 --> 00:19:47,919 the conditions need to be precise. 401 00:19:47,920 --> 00:19:50,621 The clouds must be very symmetrical, 402 00:19:50,631 --> 00:19:53,132 forming a smooth ball. 403 00:19:53,133 --> 00:19:55,941 If you have a ball of gas that isn't quite a ball, 404 00:19:55,942 --> 00:19:57,683 that's not quite homogeneous, 405 00:19:57,693 --> 00:19:59,730 as it collapses, it'll fragment. 406 00:19:59,731 --> 00:20:02,074 And it'll fragment into objects that won't form black holes. 407 00:20:02,075 --> 00:20:04,686 So you want it to be hot enough 408 00:20:04,687 --> 00:20:08,514 that it stays one big, giant thing. 409 00:20:08,515 --> 00:20:10,325 But it does need to cool a little bit, right, 410 00:20:10,335 --> 00:20:13,164 so that you get it to collapse in on itself. 411 00:20:16,596 --> 00:20:20,326 You have to get uniform collapse over time 412 00:20:20,335 --> 00:20:23,659 of a very large amount of hydrogen gas, presumably, 413 00:20:23,669 --> 00:20:26,833 which is the original matter in the universe, 414 00:20:26,834 --> 00:20:30,098 collapsing spherically symmetrically, 415 00:20:30,099 --> 00:20:31,819 without fragmenting, 416 00:20:31,820 --> 00:20:35,509 over a period of less than 500 million years. 417 00:20:41,227 --> 00:20:43,660 Direct collapse may have created black holes 418 00:20:43,670 --> 00:20:46,172 a million times the mass of the Sun. 419 00:20:46,173 --> 00:20:48,051 But it can't completely explain 420 00:20:48,052 --> 00:20:52,572 the 12 billion solar-mass supermassive black holes 421 00:20:52,573 --> 00:20:55,252 we see in the early universe. 422 00:20:55,253 --> 00:20:59,536 Maybe gigantic supermassive black holes were created 423 00:20:59,546 --> 00:21:02,572 by strange, unseen forces. 424 00:21:02,573 --> 00:21:04,452 Maybe they were created 425 00:21:04,462 --> 00:21:07,826 by the mysterious dark universe. 426 00:21:20,734 --> 00:21:24,858 Astronomers looking deep into the early universe 427 00:21:24,859 --> 00:21:29,408 have discovered gigantic supermassive black holes. 428 00:21:29,409 --> 00:21:31,120 This is a pretty deep mystery. 429 00:21:31,130 --> 00:21:33,168 There are these supermassive black holes 430 00:21:33,178 --> 00:21:35,086 that exist in the very early universe. 431 00:21:35,087 --> 00:21:38,054 And by all accounts, they should not exist. 432 00:21:38,055 --> 00:21:40,725 According to the normal laws of physics, 433 00:21:40,735 --> 00:21:42,050 it shouldn't have been possible 434 00:21:42,051 --> 00:21:45,017 for them to grow so big so quickly. 435 00:21:45,018 --> 00:21:47,926 For astrophysicists, understanding how black holes 436 00:21:47,927 --> 00:21:51,259 have grown to be so large is one of our biggest mysteries. 437 00:21:51,260 --> 00:21:52,842 We need some other way 438 00:21:52,843 --> 00:21:54,889 of growing these supermassive black holes. 439 00:21:54,890 --> 00:21:56,670 There needs to be some other mechanism 440 00:21:56,671 --> 00:21:59,182 that allows them to get that massive so early. 441 00:21:59,183 --> 00:22:01,626 But what is that? 442 00:22:01,627 --> 00:22:04,029 Everything we can see in the night sky 443 00:22:04,030 --> 00:22:06,472 makes up just 4.8% 444 00:22:06,473 --> 00:22:09,183 of all the matter in the cosmos. 445 00:22:09,184 --> 00:22:11,458 The rest is the dark universe, 446 00:22:11,459 --> 00:22:13,764 including dark matter. 447 00:22:13,774 --> 00:22:18,056 We can't see it, feel it, or detect it directly. 448 00:22:18,057 --> 00:22:20,697 But we know dark matter is there. 449 00:22:20,698 --> 00:22:24,367 Its gravity is tugging on everything around it. 450 00:22:24,368 --> 00:22:25,949 And we're beginning to understand 451 00:22:25,950 --> 00:22:28,027 it plays a fundamental role 452 00:22:28,027 --> 00:22:30,499 in the formation of the universe. 453 00:22:30,500 --> 00:22:32,874 Most of the stuff that collects together 454 00:22:32,884 --> 00:22:34,763 gravitationally is dark matter. 455 00:22:34,764 --> 00:22:37,532 So perhaps black holes form 456 00:22:37,533 --> 00:22:40,432 somehow with the inclusion of dark matter. 457 00:22:40,442 --> 00:22:42,251 One way of looking at it is there's six times 458 00:22:42,252 --> 00:22:43,903 as much dark matter as normal matter. 459 00:22:43,904 --> 00:22:46,346 So there's six times as much food out there 460 00:22:46,347 --> 00:22:47,662 for the black holes to eat 461 00:22:47,663 --> 00:22:50,441 if they're able to tap into this dark stuff. 462 00:22:50,442 --> 00:22:53,409 Maybe these supermassive black holes are growing 463 00:22:53,410 --> 00:22:55,555 by eating dark matter. 464 00:22:55,556 --> 00:22:58,394 There are some tantalizing clues. 465 00:22:58,395 --> 00:23:00,996 The largest supermassive black holes 466 00:23:00,997 --> 00:23:04,003 don't live in the galaxies with the most regular matter. 467 00:23:04,004 --> 00:23:07,801 They live in the galaxies with the most dark matter. 468 00:23:07,802 --> 00:23:10,541 The one thing we know about dark matter right now 469 00:23:10,542 --> 00:23:12,450 is that it has gravity. 470 00:23:12,451 --> 00:23:14,429 And a black hole runs on gravity. 471 00:23:14,429 --> 00:23:16,051 It attracts anything with mass. 472 00:23:16,052 --> 00:23:17,900 So there's no reason to assume 473 00:23:17,901 --> 00:23:20,205 that black holes would only eat regular matter. 474 00:23:20,206 --> 00:23:24,498 And now we know that there's far more dark matter out there. 475 00:23:24,499 --> 00:23:29,513 Maybe dark matter helps the black holes eat. 476 00:23:29,514 --> 00:23:31,987 Maybe in some ways, dark matter is a feeder 477 00:23:31,997 --> 00:23:34,301 for these supermassive black holes. 478 00:23:34,302 --> 00:23:37,170 Perhaps what really grows a supermassive black hole 479 00:23:37,171 --> 00:23:40,246 is all of the regular matter being directed into the center 480 00:23:40,247 --> 00:23:43,175 by the dark matter around it. 481 00:23:43,185 --> 00:23:46,082 Maybe the dark matter's powerful gravity 482 00:23:46,083 --> 00:23:47,863 sucks in regular matter 483 00:23:47,873 --> 00:23:51,433 and funnels it into the black hole. 484 00:23:51,434 --> 00:23:54,431 In a sense, the dark matter is greasing the wheels. 485 00:23:54,432 --> 00:23:56,152 It's sort of tilting the table up 486 00:23:56,153 --> 00:23:58,230 so that that food can slide right in. 487 00:24:01,929 --> 00:24:04,866 But now scientists think the dark matter 488 00:24:04,867 --> 00:24:08,755 may create gigantic black holes directly 489 00:24:08,765 --> 00:24:13,047 by igniting dark stars. 490 00:24:13,048 --> 00:24:14,669 Some believe that dark matter 491 00:24:14,670 --> 00:24:17,369 sparked early universe super stars. 492 00:24:17,370 --> 00:24:22,622 When they die, they leave behind supermassive black holes. 493 00:24:22,623 --> 00:24:24,106 Dark stars sound like 494 00:24:24,107 --> 00:24:26,115 they come from the fertile imagination 495 00:24:26,125 --> 00:24:28,162 of some Sci-Fi writer. 496 00:24:28,172 --> 00:24:31,199 But Dr. Katie Freese believes they may explain 497 00:24:31,209 --> 00:24:36,520 how early supermassive black holes grew so fast. 498 00:24:36,521 --> 00:24:37,934 Dark stars are amazing. 499 00:24:37,935 --> 00:24:40,308 So, when we first had this idea, 500 00:24:40,309 --> 00:24:41,595 we got excited really quickly, 501 00:24:41,605 --> 00:24:43,780 because this is a new type of star 502 00:24:43,781 --> 00:24:46,975 that has never been seen before. 503 00:24:46,976 --> 00:24:49,715 Dark stars may have been some of the first stars 504 00:24:49,716 --> 00:24:51,931 to form in the universe. 505 00:24:51,932 --> 00:24:53,444 They sparked into life 506 00:24:53,445 --> 00:24:57,274 when the universe was just 200 million years old. 507 00:24:57,283 --> 00:25:02,792 But how could dark stars form really massive black holes? 508 00:25:02,793 --> 00:25:07,571 A newborn black hole can't weigh more than its parent star. 509 00:25:07,581 --> 00:25:11,833 So in order to give birth to a really massive black hole, 510 00:25:11,834 --> 00:25:16,284 the parent star has to be supermassive, as well. 511 00:25:16,285 --> 00:25:18,827 These early objects are really strange. 512 00:25:18,828 --> 00:25:20,973 They're very cool. 513 00:25:20,974 --> 00:25:23,387 And they're really, really big. 514 00:25:23,388 --> 00:25:26,780 The size of these things is 10 times the distance 515 00:25:26,781 --> 00:25:29,362 between the Sun and the earth. 516 00:25:31,538 --> 00:25:34,041 But how is that possible? 517 00:25:34,051 --> 00:25:38,402 Regular stars have an upper size limit. 518 00:25:38,403 --> 00:25:42,131 A star is a battle between gravity pushing inwards 519 00:25:42,132 --> 00:25:44,378 and nuclear fusion pushing out. 520 00:25:47,781 --> 00:25:49,323 When the star grows too big, 521 00:25:49,324 --> 00:25:53,685 its gravity becomes overwhelming. 522 00:25:53,686 --> 00:25:55,268 The delicate balance 523 00:25:55,269 --> 00:25:59,165 between gravity and fusion is broken. 524 00:25:59,166 --> 00:26:04,012 Gravity wins out, and the star collapses. 525 00:26:04,013 --> 00:26:06,851 But dark stars may have a work-around 526 00:26:06,852 --> 00:26:11,075 that lets them become supermassive. 527 00:26:11,076 --> 00:26:13,023 So, they are made of ordinary matter. 528 00:26:13,024 --> 00:26:15,595 They're made of hydrogen and helium. 529 00:26:15,596 --> 00:26:18,533 But they're powered by dark matter. 530 00:26:18,534 --> 00:26:21,471 We don't know what dark matter is made from. 531 00:26:21,472 --> 00:26:26,555 But we do have theories on how it might power a star. 532 00:26:26,556 --> 00:26:29,127 One of the best ideas we have for dark matter 533 00:26:29,128 --> 00:26:33,094 is that it's made of weakly interacting massive particles, 534 00:26:33,095 --> 00:26:35,141 or wimps for short. 535 00:26:35,142 --> 00:26:37,515 So, these wimps are their own antimatter. 536 00:26:37,516 --> 00:26:40,019 And that means, whenever they encounter each other, 537 00:26:40,029 --> 00:26:43,816 they annihilate and turn into something else. 538 00:26:43,817 --> 00:26:46,587 That means a lot of heat is released, a lot of energy. 539 00:26:46,597 --> 00:26:49,891 And it's that energy that could power stars. 540 00:26:52,799 --> 00:26:55,241 The energy from the wimps' annihilations 541 00:26:55,242 --> 00:26:59,959 keeps the star from collapsing like a normal star. 542 00:26:59,960 --> 00:27:02,235 So it's possible that, in some stars, 543 00:27:02,236 --> 00:27:04,015 their internal reactions 544 00:27:04,016 --> 00:27:07,022 are actually being powered by dark matter. 545 00:27:07,023 --> 00:27:09,891 If that's the case, then you could imagine situations 546 00:27:09,892 --> 00:27:11,374 where, when that burns out, 547 00:27:11,375 --> 00:27:14,312 you produce very massive black holes. 548 00:27:14,313 --> 00:27:15,935 So it could be that dark matter, 549 00:27:15,936 --> 00:27:17,319 the physics of dark matter, 550 00:27:17,320 --> 00:27:20,584 plays really important roles in creating black holes 551 00:27:20,585 --> 00:27:23,097 and their prevalence in the universe. 552 00:27:31,218 --> 00:27:33,454 The energy from the dark matter 553 00:27:33,464 --> 00:27:38,379 allows the dark stars to grow huge. 554 00:27:38,380 --> 00:27:40,022 When they first form, they're small. 555 00:27:40,032 --> 00:27:42,861 They're about the mass of the Sun. 556 00:27:42,871 --> 00:27:44,878 But because they're so cool, 557 00:27:44,879 --> 00:27:46,164 they keep accumulating matter 558 00:27:46,165 --> 00:27:47,717 and growing, growing, growing. 559 00:27:47,718 --> 00:27:50,121 And some of them will get to be a million times 560 00:27:50,131 --> 00:27:54,581 as massive as the Sun and a billion times as bright. 561 00:27:54,582 --> 00:27:57,085 But these giants don't live for long. 562 00:27:57,095 --> 00:27:59,468 Eventually, the dark matter particles 563 00:27:59,469 --> 00:28:01,941 wipe each other out completely. 564 00:28:01,942 --> 00:28:03,425 And there is no more fuel 565 00:28:03,426 --> 00:28:05,967 to keep the massive amount of ordinary matter 566 00:28:05,968 --> 00:28:08,479 from collapsing. 567 00:28:08,480 --> 00:28:09,894 And then that's it. 568 00:28:09,895 --> 00:28:12,505 There's nothing to sustain this big, puffy object. 569 00:28:12,506 --> 00:28:17,352 If it's big enough, you collapse directly to a black hole. 570 00:28:17,353 --> 00:28:21,912 A monster supermassive black hole. 571 00:28:21,913 --> 00:28:24,217 It's really fun to think about the possibility 572 00:28:24,218 --> 00:28:25,671 that the physics of dark matter 573 00:28:25,672 --> 00:28:28,045 is actually helping to power stars. 574 00:28:28,046 --> 00:28:29,766 If so, it would bring, you know, 575 00:28:29,767 --> 00:28:32,171 a whole new window into our understanding 576 00:28:32,181 --> 00:28:34,416 of stars and their evolution. 577 00:28:36,959 --> 00:28:41,478 At the moment, dark stars are just theoretical. 578 00:28:41,479 --> 00:28:44,287 But when the powerful James Webb telescope 579 00:28:44,288 --> 00:28:46,562 comes online in 2018, 580 00:28:46,563 --> 00:28:50,529 we may get our first glimpse. 581 00:28:50,530 --> 00:28:54,189 We're gonna do an observing run and look f 582 00:28:54,190 --> 00:28:55,544 and so we're very excited. 583 00:28:55,545 --> 00:28:57,226 If you would find an entirely new type of star, 584 00:28:57,227 --> 00:29:00,431 that would be huge. 585 00:29:00,432 --> 00:29:02,933 While Katie Freese looks for dark stars, 586 00:29:02,934 --> 00:29:06,633 another team is investigating another radical idea 587 00:29:06,634 --> 00:29:08,413 that offers new insight 588 00:29:08,414 --> 00:29:13,765 into how supermassive black holes grow so huge. 589 00:29:13,766 --> 00:29:16,069 They detect the faint echoes 590 00:29:16,070 --> 00:29:20,135 of a violent event from across the universe, 591 00:29:20,136 --> 00:29:23,567 the remnants of an extraordinary collision, 592 00:29:23,568 --> 00:29:25,476 a supremely energetic event 593 00:29:25,477 --> 00:29:29,701 that reveals black holes are cannibals. 594 00:29:44,192 --> 00:29:46,862 Our universe is filled with enormous 595 00:29:46,863 --> 00:29:51,521 supermassive black holes that defy explanation. 596 00:29:51,522 --> 00:29:53,430 Supermassive black holes are one of the things 597 00:29:53,431 --> 00:29:55,478 in the universe that, when you run the physics, 598 00:29:55,479 --> 00:29:57,723 when you run the math of how did they evolve, 599 00:29:57,724 --> 00:29:59,771 they really shouldn't be there. 600 00:29:59,772 --> 00:30:02,738 It's still a profound mystery. 601 00:30:02,739 --> 00:30:04,718 The universe hasn't been around long enough 602 00:30:04,728 --> 00:30:06,171 for regular black holes 603 00:30:06,172 --> 00:30:09,574 to eat enough matter to get supermassive. 604 00:30:09,575 --> 00:30:11,583 So how did they get so big? 605 00:30:11,592 --> 00:30:12,976 The most logical answer 606 00:30:12,977 --> 00:30:16,112 is that large black holes are born large, 607 00:30:16,113 --> 00:30:18,942 around 1 to 2 billion solar masses. 608 00:30:18,952 --> 00:30:21,484 But that's still over 10 times smaller 609 00:30:21,494 --> 00:30:25,915 than the largest supermassive black holes out there. 610 00:30:25,916 --> 00:30:27,953 Given the time scales, it doesn't seem to add up. 611 00:30:27,963 --> 00:30:29,604 We need some other way 612 00:30:29,605 --> 00:30:31,683 to make these supermassive black holes. 613 00:30:31,692 --> 00:30:33,532 And the question is, what is that? 614 00:30:35,817 --> 00:30:39,308 A clue came from a large, isolated galaxy 615 00:30:39,309 --> 00:30:41,524 200 million light-years away 616 00:30:41,525 --> 00:30:43,800 in a quiet part of the universe. 617 00:30:45,719 --> 00:30:49,576 Nestling alone was a supermassive black hole 618 00:30:49,577 --> 00:30:54,789 with a mass of 17 billion suns. 619 00:30:54,790 --> 00:30:56,411 Normally, such monsters 620 00:30:56,412 --> 00:30:59,210 are found in dense regions of space 621 00:30:59,211 --> 00:31:03,671 with lots of galaxies and lots of stars. 622 00:31:03,672 --> 00:31:06,075 This black holes doesn't match its surroundings at all. 623 00:31:06,076 --> 00:31:08,320 It's kind of like driving to the middle of a desert 624 00:31:08,321 --> 00:31:10,269 and coming across the empire state building. 625 00:31:10,270 --> 00:31:12,979 Now, the empire state building belongs in the middle of a city. 626 00:31:12,980 --> 00:31:14,524 And a black hole this big 627 00:31:14,533 --> 00:31:18,024 belongs in a rich cluster of galaxies. 628 00:31:18,025 --> 00:31:20,764 This is the first time astronomers have found 629 00:31:20,765 --> 00:31:22,347 such a giant object 630 00:31:22,348 --> 00:31:26,571 lurking in such a relatively empty area of the universe. 631 00:31:26,572 --> 00:31:28,094 So you got to ask the question, 632 00:31:28,095 --> 00:31:30,993 if there's nothing else around, how exactly do you grow 633 00:31:31,003 --> 00:31:33,535 a 17-billion-solar-mass black hole? 634 00:31:36,711 --> 00:31:40,142 One possible answer is the stuff of nightmares. 635 00:31:40,143 --> 00:31:42,190 Maybe the story of this black hole 636 00:31:42,191 --> 00:31:44,494 is actually a little more scary than we thought. 637 00:31:44,495 --> 00:31:45,681 Maybe it's all alone 638 00:31:45,682 --> 00:31:47,957 because it ate all of its neighbors. 639 00:31:50,341 --> 00:31:53,575 Maybe it was eating more than galaxies. 640 00:31:53,576 --> 00:31:56,939 Maybe it was eating its own kind. 641 00:31:58,819 --> 00:32:00,995 The thing about black holes is they're omnivores. 642 00:32:01,005 --> 00:32:02,418 They'll eat anything. 643 00:32:02,419 --> 00:32:04,792 Anything that gets close them, they'll gobble up. 644 00:32:04,793 --> 00:32:06,772 One way black holes can grow so large 645 00:32:06,781 --> 00:32:08,393 is by eating other black holes. 646 00:32:08,394 --> 00:32:11,193 So in a sense, they may be cannibals. 647 00:32:11,203 --> 00:32:14,694 Cannibal black holes were just theoretical. 648 00:32:14,695 --> 00:32:17,563 We'd never actually seen them eat each other. 649 00:32:19,720 --> 00:32:23,478 Then scientists detected the faint echoes 650 00:32:23,479 --> 00:32:27,108 of actual ripples in space-time. 651 00:32:27,109 --> 00:32:28,661 When engineers turned on 652 00:32:28,662 --> 00:32:32,815 the laser interferometer gravitational-wave observatory, 653 00:32:32,816 --> 00:32:34,833 or LIGO for short, 654 00:32:34,834 --> 00:32:36,713 they immediately picked up 655 00:32:36,714 --> 00:32:40,472 the faint signal of gravitational waves. 656 00:32:40,473 --> 00:32:42,222 Gravitational waves are created 657 00:32:42,223 --> 00:32:45,033 by huge explosions in space. 658 00:32:48,228 --> 00:32:52,915 To make them, you need an almost unimaginably energetic event, 659 00:32:52,916 --> 00:32:55,627 something really, really big... 660 00:32:57,833 --> 00:33:01,997 ...something like merging black holes. 661 00:33:03,906 --> 00:33:06,181 A black hole merger is the most violent, 662 00:33:06,191 --> 00:33:07,467 the most energetic thing 663 00:33:07,477 --> 00:33:09,712 that happens in the universe, period. 664 00:33:12,561 --> 00:33:16,478 Picture the scene, 1.3 billion years ago. 665 00:33:16,488 --> 00:33:20,543 Two black holes circle each other in a dance of death. 666 00:33:20,544 --> 00:33:24,302 The larger black hole pulls the smaller one inwards 667 00:33:24,303 --> 00:33:27,734 until they're locked together in a spiral. 668 00:33:27,735 --> 00:33:30,177 Very, very slowly, that orbit is decaying. 669 00:33:30,178 --> 00:33:32,256 They're getting closer and closer and closer. 670 00:33:32,266 --> 00:33:35,688 And then they will merge into one giant black hole, 671 00:33:35,698 --> 00:33:39,485 truly one of the most dramatic events in the universe. 672 00:33:39,486 --> 00:33:41,533 Finally, they collide 673 00:33:41,534 --> 00:33:45,263 in one of the largest bangs since the big bang. 674 00:33:48,468 --> 00:33:50,376 I would have loved to have been able 675 00:33:50,377 --> 00:33:52,158 to safely view the collision 676 00:33:52,168 --> 00:33:54,274 of these two black holes up close. 677 00:33:54,275 --> 00:33:55,560 Imagine these two black holes 678 00:33:55,561 --> 00:33:57,439 as they spiral in toward each other, 679 00:33:57,440 --> 00:33:59,616 going faster and faster and faster and faster. 680 00:33:59,626 --> 00:34:02,158 And then, suddenly, where there appears to be nothing 681 00:34:02,168 --> 00:34:04,640 or just distortions in space in front of you, 682 00:34:04,641 --> 00:34:07,904 suddenly, there is this enormous burst of energy. 683 00:34:07,905 --> 00:34:11,040 And everything just rains around you. 684 00:34:11,041 --> 00:34:14,403 By measuring the frequency 685 00:34:14,404 --> 00:34:18,628 we can calculate the size of the objects causing them. 686 00:34:18,638 --> 00:34:20,378 When those two black holes, 687 00:34:20,379 --> 00:34:22,920 weighing 29 solar masses 688 00:34:22,921 --> 00:34:26,649 and 36 solar masses, collided, 689 00:34:26,650 --> 00:34:30,716 they created a black hole around twice the size. 690 00:34:32,724 --> 00:34:35,235 In some ways, it's very elegant and simple. 691 00:34:35,236 --> 00:34:37,411 You take two black holes. You spiral them in together. 692 00:34:37,412 --> 00:34:40,380 And you end up with one big black hole. 693 00:34:42,497 --> 00:34:45,928 The event showed that black holes can double their mass 694 00:34:45,929 --> 00:34:49,588 through cannibalism... Almost. 695 00:34:49,589 --> 00:34:54,247 The final black hole was less than the sum of its parts. 696 00:34:54,248 --> 00:34:57,511 There were 3 solar masses missing. 697 00:34:57,512 --> 00:34:59,687 That may not sound like a lot. 698 00:34:59,688 --> 00:35:02,260 So let's put it in context. 699 00:35:02,270 --> 00:35:04,445 Our sun is burning 700 00:35:04,446 --> 00:35:07,344 about 100 billion hydrogen bombs every second. 701 00:35:07,345 --> 00:35:09,323 And over its 10-billion-year lifetime, 702 00:35:09,333 --> 00:35:11,805 it will convert less than maybe 1% of the mass 703 00:35:11,806 --> 00:35:12,992 of the Sun to energy. 704 00:35:12,993 --> 00:35:15,168 In 2/10 of a second, 705 00:35:15,169 --> 00:35:17,939 3 times the mass of the Sun in matter 706 00:35:17,949 --> 00:35:20,580 got converted to energy in that collision. 707 00:35:22,499 --> 00:35:26,395 It was 36 septillion yottawatts. 708 00:35:26,396 --> 00:35:28,928 What does that mean? A lot of freaking energy. 709 00:35:28,938 --> 00:35:32,132 That's more energy in that 2/10 of a second 710 00:35:32,133 --> 00:35:34,249 than is emitted by all the stars 711 00:35:34,250 --> 00:35:36,298 in the visible universe in the same time. 712 00:35:38,840 --> 00:35:42,203 In its first run, LIGO detected two collisions. 713 00:35:44,320 --> 00:35:46,426 This suggests that cannibal black holes 714 00:35:46,427 --> 00:35:48,107 are relatively common 715 00:35:48,108 --> 00:35:52,232 and that each feast builds a larger black hole. 716 00:35:52,233 --> 00:35:54,547 But so far, the largest black hole 717 00:35:54,548 --> 00:35:56,327 these mergers have produced 718 00:35:56,328 --> 00:35:58,771 is 62 solar masses, 719 00:35:58,772 --> 00:36:03,915 not close to the largest supermassives we've found. 720 00:36:03,925 --> 00:36:06,100 It's hard to imagine, in 13.8 billion years, 721 00:36:06,101 --> 00:36:08,969 that there'd be enough collisions of 30-solar-mass 722 00:36:08,970 --> 00:36:13,262 black holes to build up to form a billion-solar-mass black hole. 723 00:36:13,263 --> 00:36:16,200 That's 100 million collisions. 724 00:36:16,201 --> 00:36:19,830 So maybe small black holes eating each other 725 00:36:19,831 --> 00:36:21,413 isn't the solution. 726 00:36:21,414 --> 00:36:24,609 Maybe supermassive black holes 727 00:36:24,619 --> 00:36:27,516 are eating each other. 728 00:36:27,517 --> 00:36:30,325 If so, could the supermassive black hole 729 00:36:30,326 --> 00:36:34,550 at the heart of our own galaxy be on the menu? 730 00:36:49,071 --> 00:36:51,513 We've found supermassive black holes 731 00:36:51,514 --> 00:36:55,303 so large, they defy explanation. 732 00:36:55,313 --> 00:36:56,696 They're too big to have grown 733 00:36:56,697 --> 00:37:00,920 by simply eating the matter around them. 734 00:37:00,921 --> 00:37:04,413 They can't form the same way that regular black holes do. 735 00:37:04,423 --> 00:37:07,054 There must be something else that happens that lets them grow 736 00:37:07,064 --> 00:37:09,862 to such enormous mass. 737 00:37:09,863 --> 00:37:12,701 Too large to have grown from dark stars 738 00:37:12,702 --> 00:37:16,500 and too big to have grown from regular black holes 739 00:37:16,501 --> 00:37:18,804 simply eating each other. 740 00:37:18,805 --> 00:37:21,179 Merging black holes almost certainly play a role 741 00:37:21,189 --> 00:37:24,018 in our understanding of supermassive black holes. 742 00:37:24,028 --> 00:37:27,222 We think that supermassive black holes themselves also merge 743 00:37:27,223 --> 00:37:30,259 and have merged regularly over the course of the universe. 744 00:37:30,260 --> 00:37:32,208 Now, whether this merging activity itself 745 00:37:32,209 --> 00:37:34,285 is enough to make them that big, 746 00:37:34,286 --> 00:37:36,660 the jury is still out on that. 747 00:37:36,670 --> 00:37:39,765 Now a newly discovered type of galaxy 748 00:37:39,766 --> 00:37:42,109 may provide an answer. 749 00:37:42,110 --> 00:37:47,916 It's called w2246-0526. 750 00:37:47,917 --> 00:37:49,439 And we can't see it. 751 00:37:49,440 --> 00:37:52,970 But we can detect the heat it gives off. 752 00:37:52,971 --> 00:37:55,077 This galaxy is an example 753 00:37:55,078 --> 00:37:59,202 of a rare class of objects called hot dogs. 754 00:37:59,203 --> 00:38:01,843 One of the funnier terms f 755 00:38:01,844 --> 00:38:03,427 is a hot dog galaxy. 756 00:38:03,437 --> 00:38:05,711 And no, this is not some delicious sausage snack. 757 00:38:05,712 --> 00:38:09,935 In fact, it means "hot, dust-obscured galaxy." 758 00:38:09,936 --> 00:38:12,477 It's called obscured because it's shrouded 759 00:38:12,478 --> 00:38:16,662 in so much dust and gas, the only light that escapes 760 00:38:16,672 --> 00:38:21,221 is infrared in the form of heat. 761 00:38:21,222 --> 00:38:23,071 All this heat must be coming from somewhere. 762 00:38:23,072 --> 00:38:25,841 So in the core, there is a cauldron, 763 00:38:25,842 --> 00:38:27,751 a seething supermassive black hole, 764 00:38:27,761 --> 00:38:29,600 the likes of which we can't even imagine. 765 00:38:32,776 --> 00:38:34,882 Of all the supermassive black holes we know of, 766 00:38:34,883 --> 00:38:37,325 the ones that are obscured in these hot dog galaxies 767 00:38:37,326 --> 00:38:39,372 may be the ones that are the most ravenous, 768 00:38:39,373 --> 00:38:40,955 consuming many millions of times 769 00:38:40,956 --> 00:38:43,924 the mass of the Sun. 770 00:38:43,933 --> 00:38:46,306 Scientists theorize that hot dogs 771 00:38:46,307 --> 00:38:48,512 could be the offspring 772 00:38:48,513 --> 00:38:52,044 of cannibal giant black holes. 773 00:38:52,045 --> 00:38:54,122 When the monstrous black holes merge, 774 00:38:54,132 --> 00:38:57,098 they drag gas and dust with them. 775 00:38:57,099 --> 00:38:59,641 This brings more food to the table, 776 00:38:59,641 --> 00:39:03,597 allowing the new black hole to gorge itself. 777 00:39:03,598 --> 00:39:06,269 When you have these two galaxies merging, 778 00:39:06,279 --> 00:39:09,146 they have all-new food. 779 00:39:09,147 --> 00:39:10,235 It's a brand-new dinner plate, 780 00:39:10,236 --> 00:39:14,132 a brand-new buffet of food to eat. 781 00:39:14,133 --> 00:39:17,327 The combination of cannibalism and fresh food 782 00:39:17,328 --> 00:39:20,394 allows the black holes to grow super large. 783 00:39:22,907 --> 00:39:25,913 Perhaps this is how the supermassive black hole 784 00:39:25,914 --> 00:39:27,624 at the center of our galaxy 785 00:39:27,625 --> 00:39:30,265 grew when it was young. 786 00:39:30,266 --> 00:39:31,849 But what's the future 787 00:39:31,859 --> 00:39:36,635 of our supermassive Sagittarius "a" -star? 788 00:39:36,636 --> 00:39:38,683 As far as supermassive black holes go, 789 00:39:38,684 --> 00:39:40,038 Sagittarius "a" -star 790 00:39:40,039 --> 00:39:41,948 is actually still kind of in the minor leagues. 791 00:39:41,958 --> 00:39:44,292 It's small. But it's not done yet. 792 00:39:44,293 --> 00:39:48,258 It's still eating. It's still growing. 793 00:39:48,259 --> 00:39:50,504 And in around 4 billion years, 794 00:39:50,505 --> 00:39:55,351 it's going to become 25 times larger, 795 00:39:55,352 --> 00:39:59,249 because it's going to be eaten by its neighbor. 796 00:40:04,066 --> 00:40:07,666 The giant Andromeda galaxy is heading our way. 797 00:40:07,667 --> 00:40:11,098 And it's going to engulf our milky way. 798 00:40:11,099 --> 00:40:12,543 When galaxies merge, 799 00:40:12,553 --> 00:40:16,608 their central supermassive black holes merge. 800 00:40:16,609 --> 00:40:19,645 Andromeda's huge supermassive black hole 801 00:40:19,646 --> 00:40:23,137 will drag Sagittarius "a" -star into orbit... 802 00:40:25,323 --> 00:40:29,151 ...gradually drawing it closer and closer 803 00:40:29,152 --> 00:40:30,764 until it devours it. 804 00:40:33,741 --> 00:40:36,045 The new supermassive black hole will weigh 805 00:40:36,046 --> 00:40:39,607 around 100 million solar masses. 806 00:40:39,617 --> 00:40:42,089 But the disruption to the new galaxy 807 00:40:42,090 --> 00:40:45,384 will provide the new supermassive black hole 808 00:40:45,394 --> 00:40:46,738 with plenty to eat 809 00:40:46,739 --> 00:40:50,241 and the opportunity to grow a whole lot bigger. 810 00:40:52,882 --> 00:40:54,890 At present, there are many theories 811 00:40:54,900 --> 00:40:59,083 of how supermassive black holes get so big. 812 00:40:59,084 --> 00:41:02,744 Most likely, it's a combination of them all. 813 00:41:02,754 --> 00:41:06,838 But however it happens, we can be pretty sure 814 00:41:06,839 --> 00:41:11,398 it's one of the most spectacular things in the universe. 815 00:41:11,399 --> 00:41:13,475 The jury's still out on exactly 816 00:41:13,476 --> 00:41:16,612 how supermassive black holes become so massive. 817 00:41:19,876 --> 00:41:21,558 Making all the black holes we see 818 00:41:21,568 --> 00:41:24,397 probably requires a pretty diverse cookbook. 819 00:41:24,407 --> 00:41:26,681 So any physicist who's looking for a really simple, 820 00:41:26,682 --> 00:41:28,887 single answer for how they get made, 821 00:41:28,888 --> 00:41:32,220 they're probably gonna be disappointed. 822 00:41:32,221 --> 00:41:35,060 It's probably a pretty complex thing that's going on. 823 00:41:38,789 --> 00:41:41,993 It could be through eating. 824 00:41:41,994 --> 00:41:43,309 It could be through eating and merging. 825 00:41:43,310 --> 00:41:45,752 And usually, the answer is somewhere in the middle. 826 00:41:45,753 --> 00:41:48,096 So they will merge with other black holes. 827 00:41:48,097 --> 00:41:51,362 And they'll also have a few snacks between mergers. 64197

Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.