All language subtitles for How.the.universe.works.S01E02.720p.HDTV.x264-DHD.English-WWW.MY-SUBS.CO

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
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 Download
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: 00:00:00,000 --> 00:00:04,162 Translated By The Community Of WWW.MY-SUBS.COM 1 00:01:12,536 --> 00:01:16,238 Nothing can escape. 2 00:01:16,239 --> 00:01:20,843 They can suck in whole galaxies. 3 00:01:20,844 --> 00:01:24,113 Black holes used to be science fiction. 4 00:01:24,114 --> 00:01:26,549 Now we know they're real. 5 00:01:26,550 --> 00:01:28,117 When I was a PhD student, 6 00:01:28,118 --> 00:01:31,554 People used to giggle when you'd hear about black holes. 7 00:01:31,555 --> 00:01:34,223 They're like unicorns, mythical creatures. 8 00:01:34,224 --> 00:01:35,991 We called this the "giggle factor." 9 00:01:35,992 --> 00:01:37,927 People would say, "beam me up, Scotty." 10 00:01:37,928 --> 00:01:40,796 Well, no one is laughing anymore. 11 00:01:42,032 --> 00:01:44,433 Krauss: So, they're not science fiction. 12 00:01:44,434 --> 00:01:46,569 Even though we've never landed in one, 13 00:01:46,570 --> 00:01:48,938 We have enough evidence to know that they're really out there. 14 00:01:54,778 --> 00:01:58,047 Narrator: This image might not look like much to you and me, 15 00:01:58,048 --> 00:02:02,785 But to a scientist, it's proof that black holes exist. 16 00:02:02,786 --> 00:02:07,356 It's an actual movie of a black hole devouring a star 17 00:02:07,357 --> 00:02:09,992 In the constellation of Aquila. 18 00:02:09,993 --> 00:02:12,161 Black holes are messy eaters. 19 00:02:12,162 --> 00:02:14,296 The red spots you see are gas 20 00:02:14,297 --> 00:02:18,801 That's being spit out of the hole, into space. 21 00:02:18,802 --> 00:02:21,904 Eventually, over the next million years, 22 00:02:21,905 --> 00:02:26,775 This star will be eaten alive and disappear. 23 00:02:34,851 --> 00:02:37,253 A black hole is pretty much the end point of everything. 24 00:02:37,254 --> 00:02:39,755 It's the end point of a star. It's the end point of matter. 25 00:02:39,756 --> 00:02:42,324 It's the end point of energy. It's the end point of gravity. 26 00:02:42,325 --> 00:02:46,996 I mean, that's really it. That's the top of the scale. 27 00:02:51,468 --> 00:02:53,903 Narrator: Although they have the power to destroy 28 00:02:53,904 --> 00:02:55,704 Like nothing else in the universe, 29 00:02:55,705 --> 00:02:59,742 Black holes also help build galaxies -- 30 00:02:59,743 --> 00:03:03,746 A vital part of the great cosmic machine. 31 00:03:03,747 --> 00:03:05,648 Some astronomers think 32 00:03:05,649 --> 00:03:09,585 They could even be gateways to parallel universes. 33 00:03:14,724 --> 00:03:17,793 Dr. Kaku: We are now entering the golden age of research 34 00:03:17,794 --> 00:03:19,061 In black-hole physics. 35 00:03:19,062 --> 00:03:21,730 They could be the key 36 00:03:21,731 --> 00:03:24,533 To understanding the birth of the universe, 37 00:03:24,534 --> 00:03:26,869 Its formation, and then its death. 38 00:03:31,741 --> 00:03:33,776 Dr. Krauss: Black holes really represent, 39 00:03:33,777 --> 00:03:36,045 In one sense, the frontier of modern astronomy. 40 00:03:36,046 --> 00:03:38,781 And they're changing our ideas about how galaxies form 41 00:03:38,782 --> 00:03:40,716 And, indeed, how the universe works. 42 00:03:40,717 --> 00:03:43,585 Narrator: Their power comes 43 00:03:43,586 --> 00:03:47,389 From one of the primary forces in nature -- gravity. 44 00:03:50,126 --> 00:03:52,294 Dr. Kaku: I teach astronomy. 45 00:03:52,295 --> 00:03:53,862 And we teach our students 46 00:03:53,863 --> 00:03:57,599 That the fundamental principle of gravity is, "gravity sucks." 47 00:03:57,600 --> 00:04:01,170 Narrator: Gravity keeps our feet on the ground 48 00:04:01,171 --> 00:04:04,273 And our planet orbiting around the sun. 49 00:04:06,609 --> 00:04:12,181 But in a black hole, the force of gravity is off the charts -- 50 00:04:12,182 --> 00:04:15,918 So strong, it sucks in anything nearby. 51 00:04:15,919 --> 00:04:21,457 It can even bend the light from distant stars. 52 00:04:21,458 --> 00:04:24,460 And if that light gets too close, 53 00:04:24,461 --> 00:04:26,729 The black hole swallows it. 54 00:04:26,730 --> 00:04:28,464 Think of it like this. 55 00:04:28,465 --> 00:04:31,333 Imagine a black hole as a waterfall. 56 00:04:31,334 --> 00:04:34,636 Gravity is the river flowing toward the falls, 57 00:04:34,637 --> 00:04:37,039 And a beam of light -- the kayak. 58 00:04:37,040 --> 00:04:40,275 Upriver from the waterfall, the current is weak. 59 00:04:40,276 --> 00:04:43,846 The kayaker can paddle against it and get away. 60 00:04:43,847 --> 00:04:47,349 But closer to the waterfall, the current is stronger, 61 00:04:47,350 --> 00:04:52,321 And the kayaker struggles to escape. 62 00:04:52,322 --> 00:04:58,260 The edge of the waterfall is like the edge of a black hole. 63 00:04:58,261 --> 00:05:03,165 No matter how strong the kayaker is, he's going down. 64 00:05:03,166 --> 00:05:04,900 It's the same in space. 65 00:05:04,901 --> 00:05:08,070 The way black holes are really devastating 66 00:05:08,071 --> 00:05:10,406 Is because when you get close to them, 67 00:05:10,407 --> 00:05:12,141 The gravity gets super-strong. 68 00:05:17,247 --> 00:05:20,249 Narrator: So strong that they eat light. 69 00:05:20,250 --> 00:05:23,685 That's why black holes are black. 70 00:05:28,391 --> 00:05:30,959 A black hole is like a roach motel. 71 00:05:30,960 --> 00:05:33,896 Everything checks in. Nothing checks out. 72 00:05:38,101 --> 00:05:41,203 Narrator: Anything that gets too close is doomed -- 73 00:05:41,204 --> 00:05:46,909 Planets, stars, even whole solar systems. 74 00:05:53,683 --> 00:05:57,186 And don't think this is some faraway phenomenon. 75 00:05:57,187 --> 00:05:59,521 Black holes are on the loose 76 00:05:59,522 --> 00:06:03,158 Right here in our own cosmic neighborhood. 77 00:06:03,159 --> 00:06:05,627 We now know there are wandering nomads 78 00:06:05,628 --> 00:06:07,863 Throughout the milky way galaxy -- 79 00:06:07,864 --> 00:06:10,966 Vagabonds throughout the galaxy, 80 00:06:10,967 --> 00:06:14,169 Where black holes can come up right behind you 81 00:06:14,170 --> 00:06:16,939 And perhaps gobble you up, and they won't even burp. 82 00:06:16,940 --> 00:06:20,576 If one ever comes close, watch out. 83 00:06:20,577 --> 00:06:25,080 Narrator: If a black hole found its way into our solar system, 84 00:06:25,081 --> 00:06:26,815 It would rip us apart. 85 00:06:26,816 --> 00:06:28,784 Dr. Plait: Any kind of black hole 86 00:06:28,785 --> 00:06:31,053 That could pass through the solar system 87 00:06:31,054 --> 00:06:32,788 Would be pulling on all the planets 88 00:06:32,789 --> 00:06:34,189 Harder than the sun does. 89 00:06:34,190 --> 00:06:35,858 And so it's just gonna totally disrupt 90 00:06:35,859 --> 00:06:38,026 The gravitational balance of the solar system. 91 00:06:38,027 --> 00:06:43,499 Narrator: The black hole would literally tear planets from their orbits 92 00:06:43,500 --> 00:06:45,701 And smash them into each other. 93 00:06:52,942 --> 00:06:56,945 It's just an epic disaster. It's a bull in a china shop. 94 00:07:00,016 --> 00:07:03,418 If it got close enough to, say, Jupiter, 95 00:07:03,419 --> 00:07:05,954 It could actually pull the moons of Jupiter 96 00:07:05,955 --> 00:07:08,157 Away from the planet itself. 97 00:07:10,260 --> 00:07:12,594 It would just be flinging planets left and right 98 00:07:12,595 --> 00:07:14,930 Everywhere as it whipped through the solar system, 99 00:07:14,931 --> 00:07:17,332 Leaving disaster in its wake. 100 00:07:22,071 --> 00:07:25,107 Narrator: If a black hole approached earth, 101 00:07:25,108 --> 00:07:28,810 All that gravity would rip asteroids from their orbits 102 00:07:28,811 --> 00:07:30,979 And hurl them toward our planet. 103 00:07:39,622 --> 00:07:42,591 The earth's surface would become an inferno. 104 00:07:42,592 --> 00:07:46,361 It would be the beginning of the end. 105 00:07:50,967 --> 00:07:53,635 First, it would swallow up the atmosphere, 106 00:07:53,636 --> 00:07:56,205 Then the planet itself. 107 00:08:01,511 --> 00:08:03,946 Destroying an entire solar system 108 00:08:03,947 --> 00:08:06,381 Is nothing to a black hole. 109 00:08:06,382 --> 00:08:11,353 But it's more than just a big, empty, sucking piece of space. 110 00:08:11,354 --> 00:08:14,156 It's incredibly heavy. 111 00:08:14,157 --> 00:08:18,627 To get an idea just how heavy and Dee a black hole is, 112 00:08:18,628 --> 00:08:20,329 Imagine the earth. 113 00:08:20,330 --> 00:08:23,665 Now start to crush it... 114 00:08:26,269 --> 00:08:29,705 ...And keep crushing until it's packed so tight 115 00:08:29,706 --> 00:08:32,874 Even the atoms themselves collapse. 116 00:08:35,712 --> 00:08:40,015 When the earth crushes down to just 2 inches across, 117 00:08:40,016 --> 00:08:42,985 That's the density of a black hole. 118 00:08:42,986 --> 00:08:45,754 It would be the size of a golf ball, 119 00:08:45,755 --> 00:08:51,627 Yet weigh the same as e earth, with the same amount of gravity. 120 00:08:51,628 --> 00:08:55,230 What can make something that small, 121 00:08:55,231 --> 00:08:59,101 That dense, and that powerful? 122 00:08:59,102 --> 00:09:03,305 We don't have external forces, large pistons in the universe, 123 00:09:03,306 --> 00:09:04,906 To create black holes. 124 00:09:04,907 --> 00:09:07,676 So the only way the real black holes of the universe form 125 00:09:07,677 --> 00:09:09,544 Is if gravity can do the job itself. 126 00:09:09,545 --> 00:09:13,415 Narrator: There is only one place in the universe 127 00:09:13,416 --> 00:09:16,218 That generates that much gravity. 128 00:09:16,219 --> 00:09:19,087 And it's inside the largest stars. 129 00:09:19,088 --> 00:09:24,426 When massive stars 10 times heavier than our sun die, 130 00:09:24,427 --> 00:09:26,295 Gravity crushes them, 131 00:09:26,296 --> 00:09:29,898 Creating a huge explosion, a supernova. 132 00:09:40,109 --> 00:09:45,514 But some stars are even bigger than that. 133 00:09:45,515 --> 00:09:50,552 These supermassive stars weigh 100 times more than our sun 134 00:09:50,553 --> 00:09:53,422 And have 100 times more gravity. 135 00:09:53,423 --> 00:09:55,824 When one of these stars dies, 136 00:09:55,825 --> 00:10:01,563 It sets off the biggest explosion in the universe... 137 00:10:01,564 --> 00:10:03,565 A hypernova. 138 00:10:13,576 --> 00:10:17,946 This is the birth of a black hole. 139 00:10:28,946 --> 00:10:33,483 Narrator: Our universe is full of stars. 140 00:10:33,484 --> 00:10:37,854 At the end of their lives, some die quietly. 141 00:10:37,855 --> 00:10:42,159 Others go out in spectacular explosions. 142 00:10:42,160 --> 00:10:47,631 And some give birth to black holes. 143 00:10:47,632 --> 00:10:49,566 Dr. Plait: If you have a star, 144 00:10:49,567 --> 00:10:52,869 A supermassive star that's 100 times the mass of the sun, 145 00:10:52,870 --> 00:10:55,839 At the end of its life, the core runs out of fuel. 146 00:10:55,840 --> 00:10:57,741 There's nothing left to hold it up, 147 00:10:57,742 --> 00:11:00,110 And the core collapses down into a black hole. 148 00:11:00,111 --> 00:11:03,847 Narrator: When that happens, the enormous gravity 149 00:11:03,848 --> 00:11:08,919 Generated at the heart of supermassive stars runs wild. 150 00:11:11,723 --> 00:11:16,593 This is the dying star v.Y. Canis majoris. 151 00:11:16,594 --> 00:11:21,198 It's more than a billion miles across. 152 00:11:24,369 --> 00:11:28,805 Like all stars, it's a giant nuclear-fusion reactor, 153 00:11:28,806 --> 00:11:31,208 Pumping energy outward. 154 00:11:31,209 --> 00:11:36,713 At the same time, the star's extreme gravity crushes inward. 155 00:11:36,714 --> 00:11:38,749 For a few million years, 156 00:11:38,750 --> 00:11:42,853 Fusion and gravity are locked in standoff. 157 00:11:42,854 --> 00:11:45,922 But when the star runs out of fuel, 158 00:11:45,923 --> 00:11:49,826 Fusion stops and the stalemate ends. 159 00:11:49,827 --> 00:11:51,628 Gravity wins. 160 00:11:54,031 --> 00:11:56,099 In a millisecond, 161 00:11:56,100 --> 00:11:59,436 The core shrinks to a fraction of its original size 162 00:11:59,437 --> 00:12:03,573 And a baby black hole is born. 163 00:12:03,574 --> 00:12:05,175 Immediately, 164 00:12:05,176 --> 00:12:09,012 It starts to cannibalize what's left of the star. 165 00:12:09,013 --> 00:12:12,449 As matter swirls into the black hole, it gets incredibly hot. 166 00:12:12,450 --> 00:12:14,985 And there are magnetic forces and frictional forces, 167 00:12:14,986 --> 00:12:17,087 And it's just a witch's brew, a nightmare, 168 00:12:17,088 --> 00:12:19,856 What's going on right above the surface of the black hole. 169 00:12:19,857 --> 00:12:22,526 Narrator: The new black hole in the middle 170 00:12:22,527 --> 00:12:25,495 Keeps feeding on the body of the star around it. 171 00:12:25,496 --> 00:12:30,267 It eats the gas so fast, it chokes and coughs, 172 00:12:30,268 --> 00:12:33,503 Blasting out huge beams of energy. 173 00:12:37,608 --> 00:12:40,610 Dr. Plait: They basically eat their way out from the star. 174 00:12:40,611 --> 00:12:42,446 This happens in milliseconds. 175 00:12:42,447 --> 00:12:45,282 It happens before the rest of the star even knows 176 00:12:45,283 --> 00:12:46,783 The core is gone. 177 00:12:46,784 --> 00:12:51,288 And so basically, the star is dead before it hits the ground. 178 00:12:54,892 --> 00:12:58,762 Narrator: Finally, the star explodes. 179 00:13:01,432 --> 00:13:06,703 In one second, it blasts out 100 times more energy 180 00:13:06,704 --> 00:13:10,974 Than our sun will produce over its entire life. 181 00:13:13,377 --> 00:13:18,181 What's left is a new black hole and two jets of energy 182 00:13:18,182 --> 00:13:22,853 Hurtling through the universe at the speed of light. 183 00:13:22,854 --> 00:13:26,556 These jets are called "gamma-ray bursts." 184 00:13:31,929 --> 00:13:35,065 Dr. Plait: They're incredibly energetic events. 185 00:13:35,066 --> 00:13:37,400 In terms of raw energy and power, 186 00:13:37,401 --> 00:13:40,570 Gamma ray bursts are second only to the big bang itself. 187 00:13:42,273 --> 00:13:45,275 Narrator: Most of them last only a few seconds. 188 00:13:45,276 --> 00:13:48,778 And they fry anything in their way. 189 00:13:52,617 --> 00:13:55,986 They're so intense that if there was a gamma-ray burster 190 00:13:55,987 --> 00:13:59,022 In the region of our galaxy near our solar system, 191 00:13:59,023 --> 00:14:02,425 It could literally vaporize the entire planet. 192 00:14:02,426 --> 00:14:07,531 Narrator: Fortunately, most gamma-ray bursts occur outside our galaxy. 193 00:14:14,472 --> 00:14:17,440 But they tell us something important 194 00:14:17,441 --> 00:14:22,479 About black holes and how our universe works. 195 00:14:22,480 --> 00:14:25,849 What we were seeing every time a gamma-ray burst went off 196 00:14:25,850 --> 00:14:28,552 Was basically the birth cry of a black hole. 197 00:14:28,553 --> 00:14:33,757 Narrator: By counting gamma-ray bursts, astronomers can figure out 198 00:14:33,758 --> 00:14:36,459 How many black holes are being created. 199 00:14:36,460 --> 00:14:40,730 In 2004, NASA launched the swift probe 200 00:14:40,731 --> 00:14:43,867 To scan the universe for gamma-ray bursts. 201 00:14:43,868 --> 00:14:44,868 Man: Five... 202 00:14:44,869 --> 00:14:45,902 Four... 203 00:14:45,903 --> 00:14:46,937 Three... 204 00:14:46,938 --> 00:14:48,071 Two... 205 00:14:48,072 --> 00:14:50,206 One... We have ignition. 206 00:14:50,207 --> 00:14:53,610 And we have lift-off of NASA's swift spacecraft, 207 00:14:53,611 --> 00:14:56,913 On a mission to study and understand gamma-ray bursts 208 00:14:56,914 --> 00:14:58,448 Throughout the universe. 209 00:15:04,789 --> 00:15:07,891 Narrator: This is the most powerful gamma-ray burst 210 00:15:07,892 --> 00:15:10,060 Swift has detected so far. 211 00:15:10,061 --> 00:15:14,030 The flash of light announces the birth of a new black hole 212 00:15:14,031 --> 00:15:16,566 On the other side of the universe. 213 00:15:20,771 --> 00:15:25,609 Swift can only look at a fraction of what's out there. 214 00:15:29,714 --> 00:15:34,584 Still, it detects at least one gamma-ray burst every day. 215 00:15:36,487 --> 00:15:41,157 That discovery rocked astronomy to its foundations. 216 00:15:43,527 --> 00:15:46,363 Dr. Kaku: We once thought that black holes, like unicorns, 217 00:15:46,364 --> 00:15:48,999 Could never be found. 218 00:15:49,000 --> 00:15:52,402 We now believe that there are perhaps billions of black holes 219 00:15:52,403 --> 00:15:53,703 In the night sky. 220 00:15:53,704 --> 00:15:56,406 When we look around our galaxy and other galaxies, 221 00:15:56,407 --> 00:16:01,277 It's clear that the universe is full of powerful black holes. 222 00:16:01,278 --> 00:16:03,847 Narrator: Finding black holes is one thing. 223 00:16:03,848 --> 00:16:05,515 Figuring out how they work -- 224 00:16:05,516 --> 00:16:07,684 That's a whole different ball game. 225 00:16:07,685 --> 00:16:10,453 The only way to find out is to visit one. 226 00:16:10,454 --> 00:16:14,858 You'd have to take a spacecraft across the vastness of space 227 00:16:14,859 --> 00:16:16,693 Just to get close to it. 228 00:16:16,694 --> 00:16:20,930 Then you'd have to go inside the black hole. 229 00:16:20,931 --> 00:16:22,832 There, you'd find a place 230 00:16:22,833 --> 00:16:27,070 Where reality breaks down and time stands still. 231 00:16:34,762 --> 00:16:38,532 Narrator: There are billions of black holes in the universe. 232 00:16:38,533 --> 00:16:41,902 We can detect them with telescopes and satellites. 233 00:16:41,903 --> 00:16:46,573 But we don't actually know what they're like up-close. 234 00:16:46,574 --> 00:16:47,975 It's a long way off, 235 00:16:47,976 --> 00:16:50,611 But scientists are already speculating 236 00:16:50,612 --> 00:16:53,981 About a mission to a black hole... 237 00:16:53,982 --> 00:16:58,785 A one-way trip to the most dangerous place in the universe. 238 00:17:02,457 --> 00:17:04,158 Dr. Kaku: Originally, 239 00:17:04,159 --> 00:17:08,495 Physicists were horrified at the idea of black holes. 240 00:17:08,496 --> 00:17:10,130 They wanted to banish them, 241 00:17:10,131 --> 00:17:12,900 Because the laws of physics, as we know them, 242 00:17:12,901 --> 00:17:15,903 Seem to break down at the instant of a black hole. 243 00:17:15,904 --> 00:17:17,404 Time stops. 244 00:17:18,806 --> 00:17:21,375 Gravity becomes infinite. 245 00:17:21,376 --> 00:17:24,978 This is a nightmare. 246 00:17:24,979 --> 00:17:28,815 Narrator: Obviously, we can't send humans anywhere near a black hole. 247 00:17:28,816 --> 00:17:31,552 But a robot? Well, sure. 248 00:17:31,553 --> 00:17:34,688 A robotic probe could transmit data back 249 00:17:34,689 --> 00:17:37,424 Just before it goes over the edge. 250 00:17:37,425 --> 00:17:41,929 That edge of a black hole is called the "event horizon." 251 00:17:41,930 --> 00:17:44,631 It's the edge of time and space -- 252 00:17:44,632 --> 00:17:47,768 At least, in the universe we know. 253 00:17:47,769 --> 00:17:49,870 We call the event horizon "event horizon" 254 00:17:49,871 --> 00:17:51,238 Quite simply because 255 00:17:51,239 --> 00:17:52,806 It separates space into two regions. 256 00:17:55,043 --> 00:17:56,877 It's not a physical surface. 257 00:17:56,878 --> 00:18:00,814 You might not even notice it if you were falling through it, 258 00:18:00,815 --> 00:18:03,417 But ultimately, once you're inside of it, you're doomed. 259 00:18:03,418 --> 00:18:06,286 Narrator: As you approach the event horizon, 260 00:18:06,287 --> 00:18:08,055 Gravity gets stronger 261 00:18:08,056 --> 00:18:12,159 And very strange things start to happen. 262 00:18:12,160 --> 00:18:14,828 Dr. Plait: As you fall into a black hole feet-first, 263 00:18:14,829 --> 00:18:16,930 Your feet are closer to the black hole. 264 00:18:16,931 --> 00:18:21,001 And so the gravity they feel is stronger. 265 00:18:21,002 --> 00:18:22,536 Your head is not quite as close, 266 00:18:22,537 --> 00:18:24,371 And so the gravity it feels is less. 267 00:18:24,372 --> 00:18:27,908 And basically, what happens is, you get stretched out. 268 00:18:27,909 --> 00:18:30,143 Your feet are being pulled much harder than your head, 269 00:18:30,144 --> 00:18:31,478 And you're like a piece of taffy 270 00:18:31,479 --> 00:18:33,180 Being pulled between two strong people. 271 00:18:36,317 --> 00:18:38,452 As you get thinner and thinner and thinner, 272 00:18:38,453 --> 00:18:40,487 As you get closer and closer and closer, 273 00:18:40,488 --> 00:18:44,057 You're undergoing a process we call "spaghettification" 274 00:18:44,058 --> 00:18:48,095 Because you're basically turned into a long, thin tube of pasta. 275 00:18:51,966 --> 00:18:55,502 Narrator: Gravity would stretch our robotic probe to the limit, 276 00:18:55,503 --> 00:18:57,271 Then rip it apart. 277 00:19:04,779 --> 00:19:07,648 But imagine if the probe was strong enough 278 00:19:07,649 --> 00:19:10,484 To survive and keep going. 279 00:19:12,854 --> 00:19:18,825 As it gets close to the event horizon, everything goes crazy. 280 00:19:18,826 --> 00:19:23,830 Gravity is so extreme, it stops time. 281 00:19:23,831 --> 00:19:26,199 Dr. Kaku: We think of time as being endless. 282 00:19:26,200 --> 00:19:29,403 However, in a black hole, in some sense, time stops. 283 00:19:33,274 --> 00:19:37,544 Dr. Plait: This sounds like it's nuts, but that's the way it works. 284 00:19:37,545 --> 00:19:38,979 It's in the math. 285 00:19:38,980 --> 00:19:42,449 It's actually woven into the fabric of the universe itself. 286 00:19:42,450 --> 00:19:45,218 Narrator: If you were to watch from a distance, 287 00:19:45,219 --> 00:19:47,587 The robot probe would seem to slow down 288 00:19:47,588 --> 00:19:50,624 As it gets closer to the black hole. 289 00:19:50,625 --> 00:19:53,927 Then it would appear to stop completely. 290 00:19:53,928 --> 00:19:57,064 The whole process might just take a brief moment. 291 00:19:57,065 --> 00:19:58,465 But from the outside, 292 00:19:58,466 --> 00:20:02,669 You appear to freeze and fall ever more slowly. 293 00:20:02,670 --> 00:20:05,372 You actually can never observe an object fall 294 00:20:05,373 --> 00:20:07,741 All the way through the event horizon. 295 00:20:07,742 --> 00:20:10,077 It literally freezes at the surface 296 00:20:10,078 --> 00:20:13,347 Because its clock is going infinitely slowly 297 00:20:13,348 --> 00:20:14,748 Compared to yours. 298 00:20:14,749 --> 00:20:19,753 Narrator: In reality, the probe hasn't stopped at all. 299 00:20:19,754 --> 00:20:24,024 It keeps going and crosses the event horizon. 300 00:20:25,860 --> 00:20:28,829 If the probe points its cameras backwards, 301 00:20:28,830 --> 00:20:31,298 Towards the entrance of the black hole, 302 00:20:31,299 --> 00:20:36,970 It will see light being sucked in. 303 00:20:36,971 --> 00:20:42,042 If it points the camera forward, at first it sees only black, 304 00:20:42,043 --> 00:20:45,445 But as it moves toward the heart of the black hole, 305 00:20:45,446 --> 00:20:50,283 It encounters the most bizarre place in the universe. 306 00:20:51,853 --> 00:20:55,856 The black hole's immense gravity pulls everything down 307 00:20:55,857 --> 00:20:59,259 To an unimaginably small point at its center. 308 00:20:59,260 --> 00:21:03,864 Scientists call it the "singularity." 309 00:21:03,865 --> 00:21:06,433 We really just don't know 310 00:21:06,434 --> 00:21:08,468 What happens at the center of a black hole. 311 00:21:08,469 --> 00:21:09,936 The densities are so great 312 00:21:09,937 --> 00:21:12,205 That the laws of physics break down, as we know them. 313 00:21:12,206 --> 00:21:17,043 A singularity is a point of infinite gravity, 314 00:21:17,044 --> 00:21:20,213 Where space and time become meaningless. 315 00:21:20,214 --> 00:21:22,082 Now, that is ridiculous. 316 00:21:22,083 --> 00:21:26,720 A singularity is basically a word for saying "I don't know." 317 00:21:26,721 --> 00:21:29,189 It's a word for saying "I'm clueless." 318 00:21:32,927 --> 00:21:34,127 Narrator: Even now, 319 00:21:34,128 --> 00:21:36,696 Scientists can't really answer the question, 320 00:21:36,697 --> 00:21:38,064 "what is a black hole?" 321 00:21:38,065 --> 00:21:39,800 Dr. Plait: It's upsetting, a little bit, 322 00:21:39,801 --> 00:21:41,568 To think that there are objects out there 323 00:21:41,569 --> 00:21:44,171 That are breaking the laws of physics. 324 00:21:44,172 --> 00:21:46,072 There must be bigger laws 325 00:21:46,073 --> 00:21:48,108 That are being used by these black holes, 326 00:21:48,109 --> 00:21:50,243 That are being obeyed by these black holes, 327 00:21:50,244 --> 00:21:51,978 That we just don't understand yet. 328 00:21:54,982 --> 00:21:58,151 Narrator: Okay, so, the one thing we do understand 329 00:21:58,152 --> 00:22:01,655 Is that black holes are born from dying stars. 330 00:22:04,358 --> 00:22:07,894 And most are small -- around 20 miles across. 331 00:22:11,165 --> 00:22:14,201 But now scientists have discovered 332 00:22:14,202 --> 00:22:17,504 That some black holes are much bigger. 333 00:22:17,505 --> 00:22:20,707 They're called "supermassive black holes." 334 00:22:20,708 --> 00:22:24,511 They're the same size as our entire solar system. 335 00:22:24,512 --> 00:22:30,684 And one of these monsters lies at the heart of our own galaxy. 336 00:22:38,827 --> 00:22:43,297 Narrator: Our solar system lies in the milky way galaxy. 337 00:22:43,298 --> 00:22:47,969 It's made up of billions of stars, including our sun... 338 00:22:49,972 --> 00:22:53,674 ...All revolving around a mysterious region 339 00:22:53,675 --> 00:22:56,344 Right at the center. 340 00:22:56,345 --> 00:22:59,213 Dr. Kaku: Children ask the question -- 341 00:22:59,214 --> 00:23:00,915 If the moon goes around the earth, 342 00:23:00,916 --> 00:23:02,283 The earth goes around the sun, 343 00:23:02,284 --> 00:23:03,951 Then what does the sun go around? 344 00:23:03,952 --> 00:23:06,087 Narrator: It's a good question. 345 00:23:06,088 --> 00:23:08,456 And astronomers ask the same thing. 346 00:23:08,457 --> 00:23:10,558 Maybe there was something going on 347 00:23:10,559 --> 00:23:12,360 At the heart of the milky way -- 348 00:23:12,361 --> 00:23:17,799 Perhaps a black hole at the very center. 349 00:23:17,800 --> 00:23:21,269 But because we can't actually see a black hole, 350 00:23:21,270 --> 00:23:26,441 The best they could do was look for telltale signs. 351 00:23:26,442 --> 00:23:28,176 Using infrared telescopes, 352 00:23:28,177 --> 00:23:30,878 They looked at the middle of the galaxy 353 00:23:30,879 --> 00:23:34,248 And discovered a densely packed swarm 354 00:23:34,249 --> 00:23:36,150 Of millions of stars. 355 00:23:36,151 --> 00:23:40,087 But they couldn't see what was at the center. 356 00:23:45,060 --> 00:23:49,630 One team has spent 15 years looking for clues. 357 00:23:54,236 --> 00:23:57,538 High above the clouds on Mauna Kea, in Hawaii, 358 00:23:57,539 --> 00:24:00,908 The giant Keck telescope has the power 359 00:24:00,909 --> 00:24:05,313 To see right through to the center of the milky way. 360 00:24:12,120 --> 00:24:14,822 The region which we have to study 361 00:24:14,823 --> 00:24:18,192 To prove that there's a black hole is incredibly small. 362 00:24:18,193 --> 00:24:19,827 It is absolutely the case 363 00:24:19,828 --> 00:24:22,363 Of looking for a needle in a haystack, 364 00:24:22,364 --> 00:24:25,166 Except we know exactly where the needle is. 365 00:24:27,169 --> 00:24:30,104 Narrator: Andrea Ghez has spent countless nights 366 00:24:30,105 --> 00:24:32,240 Scanning the center of the galaxy 367 00:24:32,241 --> 00:24:35,376 For signs of a black hole. 368 00:24:35,377 --> 00:24:37,245 To be able to do this experiment, 369 00:24:37,246 --> 00:24:38,880 One has to be able to see 370 00:24:38,881 --> 00:24:41,516 The stars that are very close to the center of the galaxy 371 00:24:41,517 --> 00:24:44,352 And to position them incredibly accurately. 372 00:24:44,353 --> 00:24:46,153 And this would be equivalent 373 00:24:46,154 --> 00:24:49,223 To me in Los Angeles looking at you in new York 374 00:24:49,224 --> 00:24:53,227 And seeing you be able to move your finger like this. 375 00:24:56,932 --> 00:24:59,267 [ motors whirring ] 376 00:25:06,942 --> 00:25:08,943 Narrator: As the Keck kicks into action, 377 00:25:08,944 --> 00:25:13,047 A laser beam detects tiny disturbances in the atmosphere 378 00:25:13,048 --> 00:25:15,483 That would distort the image. 379 00:25:18,153 --> 00:25:24,091 Motors then adjust the huge 30-foot mirror to compensate. 380 00:25:24,092 --> 00:25:26,327 The image is clear enough 381 00:25:26,328 --> 00:25:30,431 To track the stars at the heart of our galaxy. 382 00:25:32,701 --> 00:25:37,138 Ghez has taken thousands of images over the last 15 years. 383 00:25:37,139 --> 00:25:42,677 And what they reveal is amazing. 384 00:25:42,678 --> 00:25:45,379 The stars at the center of the galaxy 385 00:25:45,380 --> 00:25:48,316 Are moving at millions of miles an hour. 386 00:25:54,723 --> 00:25:59,160 The center of the galaxy is a very extreme environment. 387 00:25:59,161 --> 00:26:01,128 The speeds with which stars move 388 00:26:01,129 --> 00:26:04,165 Is much higher than anywhere else in our galaxy. 389 00:26:04,166 --> 00:26:06,934 And that is absolutely the signpost of the black hole. 390 00:26:12,274 --> 00:26:18,079 Narrator: They look like tiny planets racing around an invisible sun. 391 00:26:18,080 --> 00:26:21,616 But they're not planets. They're stars. 392 00:26:21,617 --> 00:26:23,684 It takes a lot of gravity 393 00:26:23,685 --> 00:26:28,022 To swing huge stars around in such fast, tight orbits. 394 00:26:28,023 --> 00:26:33,060 There's only one thing in the universe with that much pull... 395 00:26:33,061 --> 00:26:38,099 A supermassive black hole. 396 00:26:38,100 --> 00:26:40,368 Watching these things shows the presence 397 00:26:40,369 --> 00:26:43,237 Of a 4-million-times- the-mass-of-our-sun black hole, 398 00:26:43,238 --> 00:26:45,573 Located right at the heart of our galaxy. 399 00:26:47,175 --> 00:26:49,377 Narrator: It is a huge discovery. 400 00:26:49,378 --> 00:26:53,214 Everything in our galaxy, including our own solar system, 401 00:26:53,215 --> 00:26:57,952 Orbits around a supermassive black hole. 402 00:26:57,953 --> 00:27:01,055 But the milky way isn't the only galaxy 403 00:27:01,056 --> 00:27:03,424 With a black hole in the middle. 404 00:27:03,425 --> 00:27:05,660 There are supermassive black holes 405 00:27:05,661 --> 00:27:09,130 At the heart of most galaxies in the universe. 406 00:27:09,131 --> 00:27:12,700 The Andromeda galaxy is our closest neighbor. 407 00:27:12,701 --> 00:27:16,203 It circles around a supermassive black hole 408 00:27:16,204 --> 00:27:20,808 Weighing 140 million times more than our sun. 409 00:27:20,809 --> 00:27:24,178 Other galaxies, like this one, m87, 410 00:27:24,179 --> 00:27:30,117 Have black holes weighing as much as 20 billion suns. 411 00:27:30,118 --> 00:27:32,753 How do black holes get so big, 412 00:27:32,754 --> 00:27:37,191 And what are they doing at the center of galaxies? 413 00:27:37,192 --> 00:27:42,663 For answers, we have to go back nearly 14 billion years 414 00:27:42,664 --> 00:27:46,667 To the beginning of the universe. 415 00:27:46,668 --> 00:27:48,402 Back then, 416 00:27:48,403 --> 00:27:53,040 The universe was filled with clouds of gas from the big bang. 417 00:27:53,041 --> 00:27:54,642 In some places, 418 00:27:54,643 --> 00:27:58,546 The gas was thick enough for millions of stars to form. 419 00:28:03,385 --> 00:28:06,520 Most of these new stars were supermassive. 420 00:28:06,521 --> 00:28:08,589 They burned hot and fast 421 00:28:08,590 --> 00:28:12,693 And then exploded, creating lots of black holes. 422 00:28:23,205 --> 00:28:26,040 The early universe was a wild-and-crazy place 423 00:28:26,041 --> 00:28:29,677 Where huge regions of mass were collapsing catastrophically, 424 00:28:29,678 --> 00:28:31,011 Producing black holes. 425 00:28:31,012 --> 00:28:33,781 And, in fact, the early universe might have been 426 00:28:33,782 --> 00:28:36,217 Full of emerging black holes everywhere. 427 00:28:38,854 --> 00:28:41,622 Narrator: Gravity pulled many of them together. 428 00:28:41,623 --> 00:28:43,958 All over the early universe, 429 00:28:43,959 --> 00:28:48,229 They merged, creating larger and larger black holes. 430 00:28:51,166 --> 00:28:54,969 Over hundreds of millions of years, each black hole grew, 431 00:28:54,970 --> 00:28:59,406 Producing stronger gravity and pulling in more and more gas. 432 00:28:59,407 --> 00:29:04,078 New stars were born from the gas, forming primitive galaxies. 433 00:29:06,081 --> 00:29:09,950 But the black hole kept on sucking in gas, 434 00:29:09,951 --> 00:29:11,819 Until it could take no more, 435 00:29:11,820 --> 00:29:15,990 Igniting the most powerful flamethrower in the universe. 436 00:29:34,507 --> 00:29:38,343 Narrator: A young galaxy is a vast cluster of stars, 437 00:29:38,344 --> 00:29:41,446 Stars that formed from clouds of gas. 438 00:29:46,319 --> 00:29:48,854 At the center of the new galaxy 439 00:29:48,855 --> 00:29:53,325 Is a young, supermassive black hole feeding on the gas, 440 00:29:53,326 --> 00:29:55,327 Getting bigger and bigger. 441 00:29:55,328 --> 00:29:57,129 Dr. Plait: If you can imagine, 442 00:29:57,130 --> 00:29:59,665 When a galaxy is very young and still forming, 443 00:29:59,666 --> 00:30:02,501 There's a supermassive black hole forming at the core, 444 00:30:02,502 --> 00:30:04,503 And the gas is still falling into it 445 00:30:04,504 --> 00:30:06,038 And still forming the galaxy. 446 00:30:06,039 --> 00:30:08,340 Well, near that central black hole, 447 00:30:08,341 --> 00:30:10,042 Things are getting very hot. 448 00:30:10,043 --> 00:30:11,743 That material is heating up. 449 00:30:11,744 --> 00:30:15,380 Narrator: Gas is speeding into the black hole. 450 00:30:15,381 --> 00:30:17,883 But it overloads, 451 00:30:17,884 --> 00:30:22,621 And there is no room for all that excess hot gas. 452 00:30:22,622 --> 00:30:26,992 It has nowhere to go but out. 453 00:30:26,993 --> 00:30:32,130 It's blasted into space in huge jets of energy. 454 00:30:36,669 --> 00:30:40,205 Each jet is 20 times wider than our solar system 455 00:30:40,206 --> 00:30:44,443 And shoots clear through the galaxy. 456 00:30:44,444 --> 00:30:50,349 The supermassive black hole has ignited a quasar. 457 00:30:50,350 --> 00:30:52,117 Quasars are literally 458 00:30:52,118 --> 00:30:54,286 The brightest objects in the universe. 459 00:30:54,287 --> 00:30:57,222 They're so intense, they can outshine an entire galaxy. 460 00:30:57,223 --> 00:31:00,058 Narrator: This is a real photograph 461 00:31:00,059 --> 00:31:03,929 Of a real quasar in the galaxy m87, 462 00:31:03,930 --> 00:31:07,599 50 million light-years away. 463 00:31:11,003 --> 00:31:14,673 Quasars blast away huge quantities of gas 464 00:31:14,674 --> 00:31:16,675 From the surrounding galaxy... 465 00:31:19,312 --> 00:31:23,915 ...The equivalent of 10 earths every minute. 466 00:31:27,286 --> 00:31:31,523 Dr. Plait: When you heat up a gas, it tends to expand and it blows outward. 467 00:31:31,524 --> 00:31:34,359 And it's sort of like a wind, but on a huge scale. 468 00:31:34,360 --> 00:31:36,395 And you get a black-hole wind, 469 00:31:36,396 --> 00:31:38,997 Gas blowing out from the black hole. 470 00:31:38,998 --> 00:31:43,635 Narrator: Black holes suck gas in. Quasars blow it out. 471 00:31:43,636 --> 00:31:48,273 But eventually there's no gas left to make stars, 472 00:31:48,274 --> 00:31:50,041 And the galaxy stops growing. 473 00:31:50,042 --> 00:31:52,811 Dr. Plait: So we think that the eventual size 474 00:31:52,812 --> 00:31:54,379 That a galaxy can achieve 475 00:31:54,380 --> 00:31:56,948 Depends on the black hole in its center. 476 00:31:56,949 --> 00:31:58,550 The two are tied together. 477 00:32:00,453 --> 00:32:05,323 Narrator: With no gas left to feed on, the quasar jets shrink and die. 478 00:32:06,726 --> 00:32:09,795 What's left is a supermassive black hole 479 00:32:09,796 --> 00:32:14,266 At the center of the galaxy, with a whole lot of young stars, 480 00:32:14,267 --> 00:32:18,270 Just like our milky way back when it was young. 481 00:32:18,271 --> 00:32:21,006 Dr. Plait: Early on in the history of the milky way, 482 00:32:21,007 --> 00:32:24,409 When it was a young galaxy, we were probably a quasar. 483 00:32:24,410 --> 00:32:27,913 Probably every big galaxy was a quasar when it was young. 484 00:32:27,914 --> 00:32:29,481 But right now we're old enough 485 00:32:29,482 --> 00:32:31,383 That the galaxy has quieted down. 486 00:32:33,219 --> 00:32:37,155 Narrator: Now astronomers are looking for quasars, 487 00:32:37,156 --> 00:32:40,559 The secret to finding more black holes 488 00:32:40,560 --> 00:32:43,195 And figuring out how they work. 489 00:32:43,196 --> 00:32:46,264 The Chandra observatory is a space telescope 490 00:32:46,265 --> 00:32:52,237 That can detect the powerful x-rays quasars send out. 491 00:32:52,238 --> 00:32:55,140 It's found thousands. 492 00:32:55,141 --> 00:32:57,676 These remarkable images show 493 00:32:57,677 --> 00:33:02,647 Quasars of all shapes and sizes firing out into space. 494 00:33:06,652 --> 00:33:08,854 Each one is a signpost 495 00:33:08,855 --> 00:33:12,958 For a young galaxy with a new black hole at its center. 496 00:33:16,729 --> 00:33:19,798 These quasars will eventually calm down 497 00:33:19,799 --> 00:33:25,136 As their galaxy matures and takes its final shape. 498 00:33:25,137 --> 00:33:27,072 I guess the universe is a lot like people -- 499 00:33:27,073 --> 00:33:28,807 Active when they're young, 500 00:33:28,808 --> 00:33:30,675 A little bit quieter and more relaxed when they get older. 501 00:33:33,045 --> 00:33:36,081 Narrator: We now know that supermassive black holes 502 00:33:36,082 --> 00:33:40,151 And the quasars they create control galaxies. 503 00:33:40,152 --> 00:33:44,189 Dr. Ghez: Black holes are central to understanding how galaxies form. 504 00:33:44,190 --> 00:33:47,225 They're a key to understanding how they evolve with time. 505 00:33:47,226 --> 00:33:49,394 So, in fact, rather than being obscura, 506 00:33:49,395 --> 00:33:51,463 They're fundamental to our understanding 507 00:33:51,464 --> 00:33:53,265 Of our galaxies and our universe. 508 00:33:53,266 --> 00:33:57,536 Narrator: The only way to find out more about black holes 509 00:33:57,537 --> 00:33:59,571 Is to get a good look at one. 510 00:33:59,572 --> 00:34:03,375 And since an up-close visit is, well, not a good idea, 511 00:34:03,376 --> 00:34:06,344 Astronomers are trying to devise a way to take a picture 512 00:34:06,345 --> 00:34:10,215 Of the supermassive black hole at the heart of our own galaxy. 513 00:34:10,216 --> 00:34:11,917 To get it, 514 00:34:11,918 --> 00:34:15,887 They'll need a telescope as large as earth itself. 515 00:34:33,316 --> 00:34:36,552 Narrator: There's a supermassive black hole 516 00:34:36,553 --> 00:34:40,222 At the center of the milky way. 517 00:34:42,392 --> 00:34:45,361 It's hidden by a dense cluster of stars 518 00:34:45,362 --> 00:34:47,930 Circling the heart of the galaxy. 519 00:34:50,700 --> 00:34:55,204 But soon, we hope we'll be able to see it. 520 00:34:55,205 --> 00:34:58,040 Dr. Kaku: Seeing is believing. 521 00:34:58,041 --> 00:35:01,877 It would be spectacular if we can go right up there, 522 00:35:01,878 --> 00:35:04,780 Nose-to-nose with the event horizon 523 00:35:04,781 --> 00:35:08,250 Of the black hole at the center of the milky way galaxy. 524 00:35:08,251 --> 00:35:11,553 And that's the holy grail. 525 00:35:11,554 --> 00:35:14,857 Narrator: A supermassive black hole lies hidden 526 00:35:14,858 --> 00:35:16,959 At the center of most galaxies. 527 00:35:16,960 --> 00:35:18,761 We only know they're there 528 00:35:18,762 --> 00:35:21,730 Because the stars around them are drawn in 529 00:35:21,731 --> 00:35:23,966 At millions of miles per hour. 530 00:35:23,967 --> 00:35:25,667 But there might still be a way 531 00:35:25,668 --> 00:35:29,238 To take a picture of the very edge of the black hole -- 532 00:35:29,239 --> 00:35:31,407 The event horizon. 533 00:35:31,408 --> 00:35:35,210 Shep Doeleman and his team are trying to capture an image 534 00:35:35,211 --> 00:35:37,346 That shows its outline. 535 00:35:37,347 --> 00:35:39,615 We're essentially looking for the shadow, 536 00:35:39,616 --> 00:35:41,650 Or the silhouette, of the black hole, 537 00:35:41,651 --> 00:35:45,154 Within this cloud of gas that's swirling around it. 538 00:35:45,155 --> 00:35:48,891 This technique that we're exploiting 539 00:35:48,892 --> 00:35:51,960 Is the best hope I think we have 540 00:35:51,961 --> 00:35:54,763 To actually image a region of the universe 541 00:35:54,764 --> 00:35:58,067 Which has hitherto been completely invisible to us. 542 00:35:58,068 --> 00:36:00,369 Narrator: Optical telescopes 543 00:36:00,370 --> 00:36:03,906 Can't see the black hole directly. 544 00:36:03,907 --> 00:36:07,776 But the glowing, super-heated gas surrounding the black hole 545 00:36:07,777 --> 00:36:11,447 Sends out radio waves that can be used to make an image. 546 00:36:13,416 --> 00:36:18,687 Huge radio telescopes pick up these signals from space. 547 00:36:18,688 --> 00:36:21,290 The antenna will move in azimuth and elevation. 548 00:36:21,291 --> 00:36:23,625 [ beeping ] 549 00:36:23,626 --> 00:36:26,161 [ whirring ] 550 00:36:27,864 --> 00:36:31,633 Narrator: This one, at the m.I.T. Observatory near Boston, 551 00:36:31,634 --> 00:36:34,369 Is more than 100 feet wide. 552 00:36:34,370 --> 00:36:38,474 It's big enough to detect very faint radio emissions 553 00:36:38,475 --> 00:36:43,445 From the black hole in our own galaxy, 25,000 light-years away. 554 00:36:43,446 --> 00:36:47,716 But it's not nearly big enough to capture an image. 555 00:36:47,717 --> 00:36:51,253 We need to take multiple copies of these telescopes, 556 00:36:51,254 --> 00:36:53,122 Place them around the world 557 00:36:53,123 --> 00:36:57,726 To create a virtual telescope as large as the earth itself. 558 00:36:57,727 --> 00:37:00,696 Narrator: Doeleman's team will link up radio telescopes 559 00:37:00,697 --> 00:37:04,933 Around the globe, from Hawaii to Chile to Africa. 560 00:37:11,107 --> 00:37:13,775 When the whole network is connected, 561 00:37:13,776 --> 00:37:17,946 They'll have a virtual dish over 10,000 miles across, 562 00:37:17,947 --> 00:37:22,518 With 500 times the power of a single telescope. 563 00:37:25,889 --> 00:37:28,457 They think it will be powerful enough 564 00:37:28,458 --> 00:37:31,093 To take a picture of the event horizon 565 00:37:31,094 --> 00:37:36,598 Of the supermassive black hole at the center of the milky way. 566 00:37:36,599 --> 00:37:39,067 They're already picking up signals 567 00:37:39,068 --> 00:37:41,570 From the dark heart of our galaxy. 568 00:37:41,571 --> 00:37:44,206 Dr. Doeleman: When we saw the first detection, 569 00:37:44,207 --> 00:37:46,942 It was a moment where I just looked at the computer screen 570 00:37:46,943 --> 00:37:49,711 And said to myself, "my god, we've done it. 571 00:37:49,712 --> 00:37:52,648 "we've actually seen something that's so small 572 00:37:52,649 --> 00:37:56,718 That it has to be coming from right around the event horizon." 573 00:37:56,719 --> 00:38:00,255 Narrator: The signals are still too weak to give a complete picture, 574 00:38:00,256 --> 00:38:03,892 But doeleman expects the images to improve 575 00:38:03,893 --> 00:38:08,864 As more telescopes come online over the next few years. 576 00:38:08,865 --> 00:38:14,169 Eventually, the outline of the black hole itself should emerge. 577 00:38:16,739 --> 00:38:21,977 But even a picture can't compare to witnessing it for yourself. 578 00:38:24,214 --> 00:38:27,616 In the distant future, we may have the technology 579 00:38:27,617 --> 00:38:32,087 To actually enter and pass through a black hole 580 00:38:32,088 --> 00:38:35,224 And maybe even survive the journey. 581 00:38:40,763 --> 00:38:44,132 Then we might finally answer the question -- 582 00:38:44,133 --> 00:38:48,170 What lies at the heart of a black hole? 583 00:38:50,273 --> 00:38:51,707 Some scientists believe 584 00:38:51,708 --> 00:38:54,476 We could use black holes as a kind of portal, 585 00:38:54,477 --> 00:38:57,779 With the potential for travel across the universe. 586 00:38:57,780 --> 00:39:00,582 Dr. Kaku: This is still very speculative, 587 00:39:00,583 --> 00:39:03,085 But the mathematics seem to indicate 588 00:39:03,086 --> 00:39:05,420 That as you fall through a black hole 589 00:39:05,421 --> 00:39:07,089 That you don't simply die -- 590 00:39:07,090 --> 00:39:09,791 You fall right through a wormhole, 591 00:39:09,792 --> 00:39:14,496 Which is a gateway, a shortcut through space and time. 592 00:39:14,497 --> 00:39:18,233 Perhaps we could simply rocket across the universe 593 00:39:18,234 --> 00:39:23,505 Through a subway system that we call a black hole. 594 00:39:23,506 --> 00:39:27,809 Narrator: If black holes are shortcuts through space and time, 595 00:39:27,810 --> 00:39:31,913 It could turn one of the coolest ideas from science fiction 596 00:39:31,914 --> 00:39:35,651 Into reality. 597 00:39:35,652 --> 00:39:39,221 Time travel is possible, but not very practical. 598 00:39:39,222 --> 00:39:42,791 You see, the energy source, the material that you need 599 00:39:42,792 --> 00:39:45,327 To keep the throat of a wormhole open 600 00:39:45,328 --> 00:39:46,795 Is something so exotic 601 00:39:46,796 --> 00:39:49,698 That we cannot produce it in the laboratory. 602 00:39:49,699 --> 00:39:52,668 But if you could, it might be possible 603 00:39:52,669 --> 00:39:56,738 To exploit the power of black holes to visit yesterday. 604 00:39:58,441 --> 00:40:01,209 Perhaps our descendants in the future 605 00:40:01,210 --> 00:40:04,012 Have already mastered this technology. 606 00:40:04,013 --> 00:40:06,214 So one day, if somebody knocks on your door 607 00:40:06,215 --> 00:40:07,816 And claims to be 608 00:40:07,817 --> 00:40:10,052 Your great-great-great-great- great-great granddaughter, 609 00:40:10,053 --> 00:40:11,119 Don't slam the door. 610 00:40:15,091 --> 00:40:19,461 Narrator: Black holes might even be gateways to other universes. 611 00:40:19,462 --> 00:40:22,030 On the other side of a black hole, 612 00:40:22,031 --> 00:40:25,100 There could even be... A big bang. 613 00:40:28,338 --> 00:40:32,007 As a black hole collapses and matter falls into it, 614 00:40:32,008 --> 00:40:35,477 Perhaps the matter is blown out the other side in a white hole. 615 00:40:35,478 --> 00:40:37,713 Doesn't that sound like the big bang? 616 00:40:43,252 --> 00:40:46,922 Narrator: If a big bang is just the flip side of a black hole, 617 00:40:46,923 --> 00:40:50,992 This could be how our own universe was born. 618 00:40:52,729 --> 00:40:55,263 If you look at the equations for a black hole 619 00:40:55,264 --> 00:40:57,165 And put in the parameters of the universe -- 620 00:40:57,166 --> 00:40:59,401 The mass of the universe, the size of the universe -- 621 00:40:59,402 --> 00:41:00,469 Bingo! 622 00:41:00,470 --> 00:41:01,903 You find that our universe 623 00:41:01,904 --> 00:41:04,539 Actually solves the equations for a black hole. 624 00:41:04,540 --> 00:41:07,776 In other words, we could be inside an event horizon. 625 00:41:07,777 --> 00:41:13,281 Perhaps we are actually living inside a black hole. 626 00:41:13,282 --> 00:41:16,752 Narrator: Every black hole might be the origin 627 00:41:16,753 --> 00:41:19,621 Of an entirely separate universe. 628 00:41:19,622 --> 00:41:20,989 If that's true, 629 00:41:20,990 --> 00:41:25,660 There could be billions of universes out there... 630 00:41:29,065 --> 00:41:34,436 ...Each one full of stars, planets, life. 631 00:41:34,437 --> 00:41:36,972 Whatever we figure out later, 632 00:41:36,973 --> 00:41:40,909 We know now that black holes are everywhere. 633 00:41:40,910 --> 00:41:42,144 They're bigger in size 634 00:41:42,145 --> 00:41:44,880 And more critical to the evolution of the universe 635 00:41:44,881 --> 00:41:47,082 Than we ever imagined. 636 00:41:58,394 --> 00:42:00,328 Dr. Krauss: Literally, our understanding 637 00:42:00,329 --> 00:42:02,397 Of the universe that's important around us, 638 00:42:02,398 --> 00:42:04,800 The universe that's visible to telescopes, 639 00:42:04,801 --> 00:42:06,668 Has been profoundly affected 640 00:42:06,669 --> 00:42:10,105 By our realization that black holes are everywhere. 641 00:42:13,009 --> 00:42:14,276 Dr. Kaku: Once upon a time, 642 00:42:14,277 --> 00:42:15,944 People thought that black-hole physics 643 00:42:15,945 --> 00:42:19,080 Was too fantastic to be true. 644 00:42:19,081 --> 00:42:21,650 And now they are center-stage. 645 00:42:21,651 --> 00:42:23,118 We now know they dominate 646 00:42:23,119 --> 00:42:25,387 The evolution of the universe itself. 647 00:42:27,290 --> 00:42:28,857 Dr. Plait: When I was a kid, 648 00:42:28,858 --> 00:42:30,959 Black holes basically played a part in science fiction. 649 00:42:30,960 --> 00:42:32,494 It was always something to avoid. 650 00:42:32,495 --> 00:42:34,029 Your spaceship -- 651 00:42:34,030 --> 00:42:35,764 You try to get around them before you get drawn in. 652 00:42:35,765 --> 00:42:37,833 But what we've learned since then 653 00:42:37,834 --> 00:42:40,068 Is that black holes play a huge role 654 00:42:40,069 --> 00:42:42,637 And a huge number of roles in the universe. 655 00:42:45,508 --> 00:42:47,843 It's not an exaggeration to say 656 00:42:47,844 --> 00:42:51,613 That if black holes did not exist, we wouldn't be here. 657 00:42:51,614 --> 00:42:54,416 We literally owe our existence to black holes. 658 00:42:58,521 --> 00:43:01,957 Narrator: The story's not over yet. 659 00:43:01,958 --> 00:43:04,593 There's still much more to be discovered 660 00:43:04,594 --> 00:43:09,531 About the mysterious objects called black holes... 661 00:43:09,532 --> 00:43:12,801 The masters of the universe. 662 00:43:12,849 --> 00:43:18,849 Sync by kuniva for MY-SUBS.com 54250

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