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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:02,720 --> 00:00:05,120 You might have seen a boxing match on TV. 2 00:00:06,400 --> 00:00:10,120 Maybe you've even seen one live. But you have never seen 3 00:00:10,200 --> 00:00:12,960 a contest like this. 4 00:00:13,040 --> 00:00:17,640 Take your ringside seat to the fight of the cosmos. 5 00:00:18,920 --> 00:00:21,120 This is gonna be a wonderful fight to witness, 6 00:00:21,200 --> 00:00:24,680 but you ought to be a few million, billion light years away. 7 00:00:24,760 --> 00:00:28,800 It's like being punched by the ghost of Muhammad Ali. 8 00:00:28,880 --> 00:00:31,280 You don't even see it coming. 9 00:00:31,360 --> 00:00:34,880 Our fighters don't float like a butterfly or sting like a bee. 10 00:00:34,960 --> 00:00:38,560 But they can deliver the ultimate knockout blow. 11 00:00:39,800 --> 00:00:41,920 It is a soul-chilling, 12 00:00:42,000 --> 00:00:46,360 mind-crushing amount of energy. It's just unbelievable. 13 00:00:46,440 --> 00:00:50,760 It's a fight between two supermassive black holes. 14 00:00:50,840 --> 00:00:53,640 Forget about the World Heavyweight Championships, 15 00:00:53,720 --> 00:00:56,840 this is the universe's heavyweight championships. 16 00:00:57,840 --> 00:01:01,560 Get ready for the heavyweight championship of the universe. 17 00:01:18,440 --> 00:01:21,120 2021. Scientists detect 18 00:01:21,200 --> 00:01:23,680 a gigantic rumble deep in space. 19 00:01:23,760 --> 00:01:26,680 A tsunami of gravitational waves. 20 00:01:26,760 --> 00:01:30,800 Giant ripples racing across the universe. 21 00:01:31,560 --> 00:01:34,640 Gravitational waves that big have to come from 22 00:01:34,720 --> 00:01:37,280 a giant, cataclysmic event. 23 00:01:37,360 --> 00:01:39,920 The universe is immense 24 00:01:40,000 --> 00:01:42,440 and full of very violent events 25 00:01:42,520 --> 00:01:44,440 that are happening every single day. 26 00:01:44,520 --> 00:01:47,720 The universe is a scary place. 27 00:01:47,800 --> 00:01:51,200 There is violence everywhere we look. 28 00:01:52,240 --> 00:01:54,760 The growls and roars are clues 29 00:01:54,840 --> 00:01:57,280 about the ultimate cosmic brawl. 30 00:01:58,680 --> 00:02:01,520 The most violent event in the universe. 31 00:02:03,920 --> 00:02:06,560 But we don't know where they're coming from. 32 00:02:07,960 --> 00:02:10,960 Imagine a storm is coming in the middle of the night. 33 00:02:11,040 --> 00:02:13,480 You can't see the storm, you can't see the lightning, 34 00:02:13,560 --> 00:02:16,840 but you can hear that rumble of the distant thunder 35 00:02:16,920 --> 00:02:19,000 and you know that it's coming. 36 00:02:20,920 --> 00:02:23,560 This distant rumble of gravitational waves 37 00:02:23,640 --> 00:02:26,000 is like the footwork of heavyweights 38 00:02:26,080 --> 00:02:28,760 pounding the canvas of the boxing ring. 39 00:02:30,320 --> 00:02:32,760 The waves are caused by something massive 40 00:02:32,840 --> 00:02:34,840 throwing its weight around. 41 00:02:36,200 --> 00:02:40,040 It's not the first time we've detected gravitational waves. 42 00:02:42,360 --> 00:02:45,280 Our experiments have picked up the signal 43 00:02:45,360 --> 00:02:49,440 of two small stellar mass black holes colliding. 44 00:02:49,520 --> 00:02:51,520 These waves are high-pitched 45 00:02:51,600 --> 00:02:54,360 and ring like a boxing bell. 46 00:02:54,440 --> 00:02:58,040 The deep space growl is a much lower frequency. 47 00:02:58,120 --> 00:03:00,080 Like the roar of a crowd. 48 00:03:02,240 --> 00:03:06,320 The difference in frequencies would be even more exaggerated 49 00:03:06,400 --> 00:03:08,960 than the difference between a sparrow chirping 50 00:03:09,040 --> 00:03:12,440 and the sound coming from a blue whale underwater. 51 00:03:12,520 --> 00:03:16,800 It would be orders of magnitude more different than that. 52 00:03:18,760 --> 00:03:21,400 The low frequency of the deep-space rumble 53 00:03:21,480 --> 00:03:24,240 tells us that the waves are colossal. 54 00:03:25,360 --> 00:03:27,920 Imagine throwing a stone in the water 55 00:03:28,000 --> 00:03:30,240 and watching the little ripples come out. 56 00:03:30,320 --> 00:03:34,720 Now imagine throwing in a boulder a billion times more massive 57 00:03:34,800 --> 00:03:37,240 and watching the huge waves that come from that. 58 00:03:37,320 --> 00:03:39,720 Those are the waves that we're looking at. 59 00:03:41,240 --> 00:03:43,080 These are more difficult to detect 60 00:03:43,160 --> 00:03:45,440 because the waves are so big. 61 00:03:45,520 --> 00:03:49,040 One of their wavelengths is about 15 light years. 62 00:03:50,120 --> 00:03:52,360 You could wait for 15 years 63 00:03:52,440 --> 00:03:54,880 and only have one wavelength go by the Earth. 64 00:03:55,960 --> 00:03:59,360 The waves are too big for an Earth-bound detector to pick up. 65 00:04:00,440 --> 00:04:03,760 So, to search for the source of these giant waves 66 00:04:03,840 --> 00:04:06,120 Chiara Mingarelli and her team 67 00:04:06,200 --> 00:04:09,240 use a detector already in space. 68 00:04:10,240 --> 00:04:14,520 Something large enough to pick up these galactic heavyweights. 69 00:04:14,600 --> 00:04:18,360 Spinning dead stars called pulsars. 70 00:04:19,440 --> 00:04:23,120 Our galaxy is awash with pulsars. 71 00:04:23,200 --> 00:04:27,160 Now they're called pulsars because they pulsate very regularly. 72 00:04:27,240 --> 00:04:29,240 They're like cosmic lighthouses. 73 00:04:29,320 --> 00:04:33,360 The lighthouse beams are so regular you can set your watch by them. 74 00:04:34,880 --> 00:04:38,080 But when a huge gravitational wave hits them, 75 00:04:38,160 --> 00:04:40,160 the timing gets knocked out of whack. 76 00:04:41,320 --> 00:04:44,960 That pulsar's gonna basically rock back and forth, 77 00:04:45,040 --> 00:04:47,680 and that's going to change the timing of the pulses 78 00:04:47,760 --> 00:04:49,440 that we measure from that object. 79 00:04:51,040 --> 00:04:53,880 To identify the source of the gravitational waves, 80 00:04:53,960 --> 00:04:57,240 Chiara and her team measure the wobbles 81 00:04:57,320 --> 00:05:01,160 of 100 pulsars spread across light years of space. 82 00:05:02,720 --> 00:05:04,720 It's like a tsunami. 83 00:05:04,800 --> 00:05:08,680 And the pulsars are like the buoys on the surface of the ocean. 84 00:05:08,760 --> 00:05:10,760 And as the tsunami passes by, 85 00:05:10,840 --> 00:05:14,040 we can watch all of them moving and shifting up and down. 86 00:05:14,120 --> 00:05:16,080 So our pulsar timing array 87 00:05:16,160 --> 00:05:19,040 is a gravitational wave warning system. 88 00:05:20,040 --> 00:05:24,040 The pulsar array has identified the source of the tsunami 89 00:05:24,120 --> 00:05:26,120 of gravitational waves. 90 00:05:27,400 --> 00:05:30,720 The only thing we know of that can makes these very long wavelength, 91 00:05:30,800 --> 00:05:33,440 very low-pitch gravitational waves 92 00:05:33,520 --> 00:05:36,720 would be the collisions of supermassive black holes. 93 00:05:36,800 --> 00:05:38,480 They're massive. They're huge. 94 00:05:38,560 --> 00:05:41,200 And they know how to throw their weight around. 95 00:05:41,280 --> 00:05:43,080 Supermassive black hole binaries 96 00:05:43,160 --> 00:05:46,640 produce the loudest gravitational waves in the universe. 97 00:05:48,080 --> 00:05:50,080 The gravitational waves' signal 98 00:05:50,160 --> 00:05:52,240 revealed something extraordinary. 99 00:05:52,320 --> 00:05:54,880 It's not just gravitational waves 100 00:05:54,960 --> 00:05:57,960 coming from one black hole binary pair, 101 00:05:58,040 --> 00:06:00,560 it's actually from the cosmic population 102 00:06:00,640 --> 00:06:03,040 of supermassive black hole binaries. 103 00:06:04,680 --> 00:06:08,160 Chiara and her team think there may be tens of thousands 104 00:06:08,240 --> 00:06:10,040 of heavyweight bouts going on. 105 00:06:11,240 --> 00:06:14,120 Now, the scientists want to pick out the sound 106 00:06:14,200 --> 00:06:16,200 of one single collision 107 00:06:16,280 --> 00:06:19,560 between two supermassive black holes 108 00:06:19,640 --> 00:06:22,040 from the background roar. 109 00:06:24,200 --> 00:06:28,160 If we were to hear a supermassive black hole merger, 110 00:06:28,240 --> 00:06:30,840 it would wound like a very low-frequency growl, 111 00:06:30,920 --> 00:06:33,280 this... whoooooooo 112 00:06:33,360 --> 00:06:35,360 that would last about 25 million years. 113 00:06:35,440 --> 00:06:39,840 To date, we haven't witnessed two supermassive black holes 114 00:06:39,920 --> 00:06:41,880 trading blows in real time. 115 00:06:41,960 --> 00:06:47,280 But we have seen events leading up to the championship bout. 116 00:06:47,360 --> 00:06:51,240 We've watched galaxies merge. We've seen stars explode. 117 00:06:51,320 --> 00:06:54,560 We've seen so many violent events in the universe. 118 00:06:54,640 --> 00:06:56,240 But we haven't seen this one. 119 00:06:57,200 --> 00:06:58,800 It's odd if you think about it. 120 00:06:58,880 --> 00:07:00,600 We haven't seen the biggest one. 121 00:07:00,680 --> 00:07:03,640 We haven't seen mergers between supermassive black holes. 122 00:07:03,720 --> 00:07:06,760 But that may be about to change. 123 00:07:08,520 --> 00:07:12,200 Chiara predicts there are 112 fighters 124 00:07:12,280 --> 00:07:15,200 who are pumped up and ready to enter the ring. 125 00:07:18,000 --> 00:07:21,120 In the next five years, we should be able to detect 126 00:07:21,200 --> 00:07:24,040 at least one supermassive black hole merger. 127 00:07:24,120 --> 00:07:29,000 It'll be the most violent event in the cosmos. 128 00:07:30,720 --> 00:07:32,960 Let's put that in context. 129 00:07:33,040 --> 00:07:35,680 We talk about how supernova are some of the most 130 00:07:35,760 --> 00:07:39,320 explosive, energetic things in our universe. 131 00:07:39,400 --> 00:07:42,440 Well, colliding supermassive black holes 132 00:07:42,520 --> 00:07:47,160 are a billion billion billion billion times more energetic 133 00:07:47,240 --> 00:07:49,240 than a supernova. 134 00:07:49,320 --> 00:07:50,960 Think about all of the light 135 00:07:51,040 --> 00:07:53,200 being emitted by everything in the universe, 136 00:07:53,280 --> 00:07:55,280 every star, every galaxy. 137 00:07:55,360 --> 00:07:58,960 In one instant, two supermassive black holes colliding 138 00:07:59,040 --> 00:08:02,200 could release 100 million times that energy. 139 00:08:03,800 --> 00:08:05,800 Imagine being punched in the face 140 00:08:05,880 --> 00:08:08,680 by the biggest, baddest heavyweight of all time. 141 00:08:10,240 --> 00:08:12,960 Ouch. This is way bigger than that. 142 00:08:14,680 --> 00:08:16,960 Where does all this energy come from? 143 00:08:17,040 --> 00:08:19,640 Surprisingly, it originates 144 00:08:19,720 --> 00:08:22,200 in the smallest atoms in the cosmos 145 00:08:22,280 --> 00:08:26,280 in a story that dates back billions of years, 146 00:08:26,360 --> 00:08:29,640 all the way to the birth of the universe. 147 00:08:36,360 --> 00:08:41,400 2020. The earthbound gravitational wave detector, LIGO, 148 00:08:41,480 --> 00:08:43,480 picks up the distinctive signal 149 00:08:43,560 --> 00:08:46,280 of a stellar mass black hole merger. 150 00:08:47,680 --> 00:08:49,680 What we saw was a black hole 151 00:08:49,760 --> 00:08:52,440 of 85 times the mass of our sun 152 00:08:52,520 --> 00:08:56,160 and another black hole of 66 times the mass of our sun 153 00:08:56,240 --> 00:08:59,680 smashing together to create a combined black hole. 154 00:09:01,760 --> 00:09:04,040 As someone who studies black hole mergers, 155 00:09:04,120 --> 00:09:05,920 this was a really exciting event. 156 00:09:06,000 --> 00:09:08,680 We're talking about the largest, the heaviest, 157 00:09:08,760 --> 00:09:12,440 the most massive black holes we have seen collide to date. 158 00:09:14,160 --> 00:09:18,080 It may be the largest detection, but on a universal scale 159 00:09:18,160 --> 00:09:20,160 it's still a small fry. 160 00:09:20,240 --> 00:09:24,480 Like lightweight boxers, the two black holes circle each other 161 00:09:24,560 --> 00:09:27,360 and emit low-energy gravitational waves. 162 00:09:28,520 --> 00:09:31,240 This energy loss causes the black holes 163 00:09:31,320 --> 00:09:33,960 to spiral in together. 164 00:09:34,040 --> 00:09:37,560 Finally, they collide in a cosmos-shattering event... 165 00:09:39,600 --> 00:09:41,800 ...forming a single black hole 166 00:09:41,880 --> 00:09:46,680 and releasing a huge blast of gravitational waves. 167 00:09:46,760 --> 00:09:50,640 But when astronomers examine the single merged black hole, 168 00:09:50,720 --> 00:09:53,160 something doesn't add up. 169 00:09:53,240 --> 00:09:56,280 If you take the combined mass of the two black holes, 170 00:09:56,360 --> 00:10:00,080 you get to 150 times the mass of our sun. 171 00:10:00,160 --> 00:10:02,920 But actually, the black hole that's left 172 00:10:03,000 --> 00:10:08,320 only has a mass of 142 times the mass of our sun. 173 00:10:08,400 --> 00:10:11,120 So the mass you have before the event 174 00:10:11,200 --> 00:10:14,080 does not equal the mass you have after the event. 175 00:10:14,160 --> 00:10:18,800 What happened to that missing eight solar masses? 176 00:10:18,880 --> 00:10:21,120 The way these black hole mergers work 177 00:10:21,200 --> 00:10:24,800 is very roughly five percent of the total mass of the system 178 00:10:24,880 --> 00:10:26,880 gets converted into energy. 179 00:10:28,200 --> 00:10:31,640 It all comes down to E=mc2. 180 00:10:32,960 --> 00:10:37,640 This is that beautiful equation that Einstein told us, E=mc2. 181 00:10:37,720 --> 00:10:40,600 E is the energy, and M is the mass. 182 00:10:40,680 --> 00:10:44,200 Einstein taught us that mass and energy are related. 183 00:10:44,280 --> 00:10:47,720 In fact, much of what we call mass is actually energy. 184 00:10:47,800 --> 00:10:51,120 In this case, the violence of the collision 185 00:10:51,200 --> 00:10:56,720 transforms 18,000 trillion trillion tons of matter 186 00:10:56,800 --> 00:10:59,960 into an explosion of gravitational waves. 187 00:11:01,120 --> 00:11:03,120 In just a fraction of a second, 188 00:11:03,200 --> 00:11:06,640 eight suns-worth of matter 189 00:11:06,720 --> 00:11:10,760 is converted into pure, unadulterated energy. 190 00:11:10,840 --> 00:11:13,320 The amount of energy released was so great 191 00:11:13,400 --> 00:11:16,320 that if you add up all the energy of all the stars 192 00:11:16,400 --> 00:11:20,000 burning in the universe, it was bigger than that. 193 00:11:21,120 --> 00:11:25,880 This event was a collision between relative lightweights. 194 00:11:25,960 --> 00:11:28,200 Two stellar mass black holes. 195 00:11:31,280 --> 00:11:35,440 To understand heavyweight bouts, we need to scale up 196 00:11:35,520 --> 00:11:38,120 to supermassive black holes. 197 00:11:40,960 --> 00:11:42,960 In the universe of sports, 198 00:11:43,040 --> 00:11:46,440 supermassive black holes are the heavyweight contenders. 199 00:11:46,520 --> 00:11:50,960 With these big black holes, size matters. The bigger the better. 200 00:11:51,040 --> 00:11:55,320 More mass means more energy, which means more destructive power. 201 00:11:56,320 --> 00:12:00,480 We don't need to look too far to find this devastating muscle. 202 00:12:00,560 --> 00:12:03,800 This is M87 star, 203 00:12:03,880 --> 00:12:06,800 one of the largest supermassive black holes 204 00:12:06,880 --> 00:12:09,640 in our cosmic zip code. 205 00:12:09,720 --> 00:12:12,320 M87 star is huge. 206 00:12:12,400 --> 00:12:15,440 It weighs about six billion solar masses, 207 00:12:15,520 --> 00:12:19,520 about six billion suns, and it's the size of our solar system. 208 00:12:19,600 --> 00:12:24,600 A collision between two six billion solar mass supermassive black holes 209 00:12:24,680 --> 00:12:29,400 would release around five times ten to the power of 56 joules. 210 00:12:30,440 --> 00:12:33,400 So, what does that mean in real-world terms? 211 00:12:33,480 --> 00:12:35,880 It's hard to use words 212 00:12:35,960 --> 00:12:37,760 to express how much energy this is 213 00:12:37,840 --> 00:12:40,600 and the numbers are so huge, they're almost meaningless. 214 00:12:40,680 --> 00:12:44,600 The only way I can really explain this is... argh! 215 00:12:46,520 --> 00:12:48,760 In physics, we have these comparisons 216 00:12:48,840 --> 00:12:50,360 so we can get a mental picture, 217 00:12:50,440 --> 00:12:53,160 but for something like this there is no mental picture. 218 00:12:53,240 --> 00:12:55,240 That is so big! 219 00:12:58,400 --> 00:13:01,960 So where does this destructive mass and energy come from? 220 00:13:06,120 --> 00:13:11,040 It starts with the simplest ingredient, hydrogen. 221 00:13:13,680 --> 00:13:17,000 Hydrogen is the basic building block of the universe. 222 00:13:18,200 --> 00:13:22,600 Each atom is tiny, but it contains a lot of energy. 223 00:13:23,920 --> 00:13:26,600 Hydrogen atoms contain a huge amount of energy, 224 00:13:26,680 --> 00:13:28,680 just like all matter does. 225 00:13:28,760 --> 00:13:31,080 And if it's unlocked in a certain way, 226 00:13:31,160 --> 00:13:33,160 there can be huge explosions. 227 00:13:36,040 --> 00:13:38,280 You take the mass contained simply in my hand 228 00:13:38,360 --> 00:13:40,840 and you could blow up pretty much the entire Earth. 229 00:13:41,960 --> 00:13:45,800 Matter has energy because it formed from energy 230 00:13:45,880 --> 00:13:48,000 in the early moments of the universe. 231 00:13:49,040 --> 00:13:51,520 In many ways, atoms are reservoirs 232 00:13:51,600 --> 00:13:53,880 of stored energy from the big bang. 233 00:13:55,640 --> 00:13:57,760 13.8 billion years ago, 234 00:13:57,840 --> 00:14:00,200 the universe ignites 235 00:14:00,280 --> 00:14:03,920 in a super-hot ball of intense energy. 236 00:14:05,160 --> 00:14:08,400 Right after the big bang, there's a tremendous amount of energy. 237 00:14:08,480 --> 00:14:11,320 So much energy, in fact, that normal atoms can't exist. 238 00:14:13,160 --> 00:14:16,600 As that early energy starts to cool, 239 00:14:16,680 --> 00:14:19,400 it can start to form primitive matter. 240 00:14:21,960 --> 00:14:25,160 The universe takes that first matter and energy 241 00:14:25,240 --> 00:14:27,280 in the form of hydrogen atoms 242 00:14:27,360 --> 00:14:31,800 and starts the process of creating a supermassive black hole. 243 00:14:31,880 --> 00:14:35,000 Step one, build giant stars. 244 00:14:36,640 --> 00:14:38,640 So, gravity brings together 245 00:14:38,720 --> 00:14:41,440 gas, dust, hydrogen, all of that stuff, 246 00:14:41,520 --> 00:14:43,720 and as the clouds become more dense, 247 00:14:43,800 --> 00:14:45,800 they attract even more material. 248 00:14:46,800 --> 00:14:49,120 As they spin, they get hotter and hotter. 249 00:14:49,200 --> 00:14:52,600 And as that temperature and pressure increase, 250 00:14:52,680 --> 00:14:55,880 finally it ignites nuclear fusion within the core 251 00:14:55,960 --> 00:14:58,040 and creates an actual star. 252 00:15:00,480 --> 00:15:03,760 These huge stars are like cosmic rock stars. 253 00:15:03,840 --> 00:15:06,240 They live fast and die young. 254 00:15:07,800 --> 00:15:11,720 When they die, they flame out in a huge explosion. 255 00:15:12,800 --> 00:15:14,680 A supernova. 256 00:15:14,760 --> 00:15:18,800 The entire star turns itself inside out 257 00:15:18,880 --> 00:15:21,600 and releases a shockwave, 258 00:15:21,680 --> 00:15:24,160 going a good fraction of the speed of light, 259 00:15:24,240 --> 00:15:27,720 and releases enough energy to just obliterate you. 260 00:15:29,600 --> 00:15:33,120 If the dying star is more than 15 stellar masses, 261 00:15:33,200 --> 00:15:36,320 its core collapses into a black hole. 262 00:15:38,040 --> 00:15:40,640 It's kind of astounding what the universe is doing. 263 00:15:40,720 --> 00:15:44,560 It's taking incredibly simple things like hydrogen atoms and using gravity 264 00:15:44,640 --> 00:15:47,000 to ultimately bring all this stuff together 265 00:15:47,080 --> 00:15:49,640 and make things like black holes. 266 00:15:49,720 --> 00:15:53,480 I find it quite beautiful how our whole cosmic history 267 00:15:53,560 --> 00:15:55,320 is the story of 268 00:15:55,400 --> 00:15:58,040 little things coming together into bigger things. 269 00:15:58,120 --> 00:16:02,520 But these stellar mass black holes are tiny flyweights. 270 00:16:02,600 --> 00:16:04,960 To step up to the heavyweight division, 271 00:16:05,040 --> 00:16:08,720 they have to grow billions of times more massive. 272 00:16:08,800 --> 00:16:11,040 But how? 273 00:16:11,120 --> 00:16:13,520 How do black holes become supermassive? 274 00:16:14,840 --> 00:16:18,240 This is the age-old question. We're not really sure. 275 00:16:19,280 --> 00:16:21,840 The current stated understanding 276 00:16:21,920 --> 00:16:25,400 of how black holes become supermassive is like... uh, 277 00:16:25,480 --> 00:16:27,440 we're confused, we really don't know. 278 00:16:27,520 --> 00:16:29,560 In June of 2018, 279 00:16:29,640 --> 00:16:31,640 we spotted a clue. 280 00:16:31,720 --> 00:16:33,720 An enormous flash of light. 281 00:16:34,720 --> 00:16:37,200 AT2018cow, 282 00:16:37,280 --> 00:16:39,040 nicknamed "The Cow", 283 00:16:39,120 --> 00:16:41,480 was the brightest explosion ever recorded. 284 00:16:42,600 --> 00:16:44,640 A huge amount of energy was released 285 00:16:44,720 --> 00:16:47,400 and then, all of a sudden, everything was gone. 286 00:16:47,480 --> 00:16:50,160 This explosion was incredibly violent. 287 00:16:50,240 --> 00:16:53,640 At first, it was thought to just be a supernova, a flash of light. 288 00:16:53,720 --> 00:16:56,440 But over time, it became clear that this was something 289 00:16:56,520 --> 00:16:58,400 much more powerful. 290 00:16:58,480 --> 00:17:01,360 It was too bright, basically, to be a supernova. 291 00:17:01,440 --> 00:17:04,520 It was extremely bright and it didn't fit into 292 00:17:04,600 --> 00:17:06,920 any of our theoretical understandings 293 00:17:07,000 --> 00:17:09,600 of how bright supernovas should be. 294 00:17:09,680 --> 00:17:13,200 One explanation is that the light may have come from 295 00:17:13,280 --> 00:17:16,480 a black hole feeding on a small, white dwarf star, 296 00:17:16,560 --> 00:17:18,600 weighing less than the Sun. 297 00:17:19,800 --> 00:17:21,800 What really seemed to fit that model 298 00:17:21,880 --> 00:17:24,680 was a star getting too close to a black hole 299 00:17:24,760 --> 00:17:26,240 and getting ripped apart, 300 00:17:26,320 --> 00:17:29,040 and then everything going right down the black hole. 301 00:17:29,120 --> 00:17:32,960 A black hole gains mass every time it eats something. 302 00:17:33,040 --> 00:17:35,920 That's how they grow. Whether it's a gas cloud or a star 303 00:17:36,000 --> 00:17:37,360 or another black hole, 304 00:17:37,440 --> 00:17:40,120 once it gains that mass it's gained that mass. 305 00:17:42,760 --> 00:17:45,280 People often ask me, What happens to the mass 306 00:17:45,360 --> 00:17:48,200 that falls into a black hole? Does it go to another dimension? 307 00:17:48,280 --> 00:17:49,440 And the answer is no. 308 00:17:49,520 --> 00:17:52,280 It's still there. It's inside the black hole. 309 00:17:52,360 --> 00:17:54,880 They get bigger. They grow. 310 00:17:54,960 --> 00:17:58,920 Could this be how weak, flyweight black holes 311 00:17:59,000 --> 00:18:02,920 turn into mean and powerful supermassive heavyweights? 312 00:18:03,000 --> 00:18:05,000 The star is like protein, 313 00:18:05,080 --> 00:18:08,040 and the black hole is like a boxer. 314 00:18:09,840 --> 00:18:13,080 And so, the more protein they get, the more stars they consume, 315 00:18:13,160 --> 00:18:16,360 the stronger they get, the more destructive they can be. 316 00:18:18,960 --> 00:18:22,520 But there's a problem with the training program explanation. 317 00:18:24,320 --> 00:18:26,880 Eating small stars one at a time 318 00:18:26,960 --> 00:18:29,480 just doesn't add enough mass fast enough 319 00:18:29,560 --> 00:18:32,760 to grow the supermassive black holes that we see today. 320 00:18:32,840 --> 00:18:37,080 That's like boxers eating just one egg per day. 321 00:18:38,240 --> 00:18:41,720 Like them, black holes need much bigger meals. 322 00:18:43,160 --> 00:18:45,800 And in 2020, we detected one. 323 00:18:47,520 --> 00:18:49,960 A sudden burst of gravitational waves 324 00:18:50,040 --> 00:18:53,040 from a black hole gorging on the remains 325 00:18:53,120 --> 00:18:55,160 of a dead star... 326 00:18:56,560 --> 00:18:58,320 ...called a neutron star. 327 00:18:59,760 --> 00:19:03,080 For scientists, January 2020 was exciting 328 00:19:03,160 --> 00:19:05,880 because it was the first time LIGO observed 329 00:19:05,960 --> 00:19:09,280 the very first black hole neutron star merger. 330 00:19:10,320 --> 00:19:12,600 Neutron stars may be small 331 00:19:12,680 --> 00:19:15,920 but they are inconceivably dense. 332 00:19:16,000 --> 00:19:19,000 You want to talk about an enormous mass, talk about a neutron star. 333 00:19:19,080 --> 00:19:20,680 That's one heck of a snack. 334 00:19:20,760 --> 00:19:25,000 The black hole swallowed the neutron star in one gulp. 335 00:19:26,560 --> 00:19:30,280 So, this black hole ate a whole neutron star, 336 00:19:30,360 --> 00:19:34,400 which means it gained just over ten percent of its entire body weight 337 00:19:34,480 --> 00:19:36,480 in one shot. 338 00:19:36,560 --> 00:19:38,880 Ten percent doesn't sound like a lot, 339 00:19:38,960 --> 00:19:42,000 but then we detected another black hole 340 00:19:42,080 --> 00:19:45,160 swallowing a neutron star just ten days later, 341 00:19:45,240 --> 00:19:48,280 suggesting that there are lots of black holes 342 00:19:48,360 --> 00:19:50,360 bulking up across the universe. 343 00:19:51,560 --> 00:19:53,640 But even with this extreme weight gain, 344 00:19:53,720 --> 00:19:57,320 it's probably not enough to get supermassive. 345 00:19:57,400 --> 00:19:59,240 They need to eat even more. 346 00:20:00,240 --> 00:20:02,880 If you're a black hole and you want to get bigger, 347 00:20:02,960 --> 00:20:05,800 your best bet is to merge with another black hole. 348 00:20:06,800 --> 00:20:08,800 But there's a catch. 349 00:20:08,880 --> 00:20:11,720 So, if you're a flyweight black hole, 350 00:20:11,800 --> 00:20:13,800 and you try to eat 351 00:20:13,880 --> 00:20:16,720 all of the other flyweight black holes, 352 00:20:16,800 --> 00:20:20,080 there's just not enough time in the history of the universe 353 00:20:20,160 --> 00:20:22,640 for you to become a supermassive black hole. 354 00:20:22,720 --> 00:20:25,280 But you can make it to middleweight. 355 00:20:26,280 --> 00:20:30,440 So, exactly how supermassive black holes grow so large 356 00:20:30,520 --> 00:20:32,680 remains an open question. 357 00:20:32,760 --> 00:20:37,120 We do know that the process started in the very early universe 358 00:20:37,200 --> 00:20:39,520 with a journey from the lightest element 359 00:20:39,600 --> 00:20:42,720 to the most intimidating object in the cosmos. 360 00:20:42,800 --> 00:20:45,840 It's so interesting how the cosmos can take something 361 00:20:45,920 --> 00:20:47,920 as simple as a hydrogen atom 362 00:20:48,000 --> 00:20:50,760 and build stellar-mass black holes 363 00:20:50,840 --> 00:20:53,400 and intermediate-mass black holes 364 00:20:53,480 --> 00:20:55,720 and even supermassive black holes 365 00:20:55,800 --> 00:21:00,360 out of these really densely compressed hydrogen atoms. 366 00:21:00,440 --> 00:21:02,320 It's really a wonder. 367 00:21:02,400 --> 00:21:07,440 Now, 13.8 billion years after the big bang, 368 00:21:07,520 --> 00:21:11,440 supermassive black holes feed and flex their muscles 369 00:21:11,520 --> 00:21:15,720 ready to fight for the heavyweight championship of the universe. 370 00:21:15,800 --> 00:21:17,800 These supermassive black holes 371 00:21:17,880 --> 00:21:20,640 have been bulking up since the age of the universe. 372 00:21:20,720 --> 00:21:24,520 These black holes have been getting ready for the fight. 373 00:21:24,600 --> 00:21:28,600 They have been bulking up, they have been eating entire stars 374 00:21:28,680 --> 00:21:31,960 as snacks, to get the mass they need. 375 00:21:32,040 --> 00:21:33,960 So they are ready to rumble. 376 00:21:34,960 --> 00:21:36,960 It's not The Rumble in the Jungle. 377 00:21:37,040 --> 00:21:40,920 This is the battle to be the boss of the cosmos. 378 00:21:41,000 --> 00:21:46,720 Supermassive black hole versus supermassive black hole. 379 00:21:46,800 --> 00:21:48,840 Fought in the grandest arena. 380 00:21:50,560 --> 00:21:53,600 The fighters' entourage, their host galaxies, 381 00:21:53,680 --> 00:21:55,680 escort them to the ring. 382 00:21:55,760 --> 00:21:58,800 But even this journey is violent, triggering starbursts, 383 00:21:58,880 --> 00:22:01,640 jets, and carnage. 384 00:22:04,240 --> 00:22:06,520 Things are about to get nasty. 385 00:22:07,640 --> 00:22:09,960 Galaxies can look calm and serene, 386 00:22:10,040 --> 00:22:12,520 but they can get into pretty big scraps. 387 00:22:15,240 --> 00:22:17,440 There's a lot of them that are totally messed up, 388 00:22:17,520 --> 00:22:19,320 and are clearly merging with each other. 389 00:22:24,960 --> 00:22:29,320 Eventually, even our own galaxy will merge with another galaxy. 390 00:22:30,320 --> 00:22:32,240 In a few billion years, 391 00:22:32,320 --> 00:22:35,080 a timescale that I'm not too worried about myself, 392 00:22:35,160 --> 00:22:38,400 the Milky Way and the Andromeda Galaxy will collide. 393 00:22:38,480 --> 00:22:41,560 The Milky Way and Andromeda each have supermassive black holes. 394 00:22:41,640 --> 00:22:43,080 And when they collide, 395 00:22:43,160 --> 00:22:45,200 their supermassive black holes will collide too. 396 00:22:49,320 --> 00:22:52,520 This is an incredibly dangerous event for our solar system. 397 00:22:52,600 --> 00:22:55,240 Our solar system could be swept out 398 00:22:55,320 --> 00:22:58,200 to be somewhere else in this newly-formed galaxy, 399 00:22:58,280 --> 00:23:01,680 or it could be completely ejected from the galaxy. 400 00:23:03,360 --> 00:23:06,280 If there's any life around near the merger 401 00:23:06,360 --> 00:23:09,720 of these supermassive black holes, it would be obliterated. 402 00:23:12,200 --> 00:23:15,880 When galaxies fight, their gravity pulls on each other, 403 00:23:15,960 --> 00:23:18,600 twisting and distorting their structures. 404 00:23:20,040 --> 00:23:22,840 The galaxy will be warped and morphed into 405 00:23:22,920 --> 00:23:25,840 different ways that we can only imagine 406 00:23:25,920 --> 00:23:27,920 how twisted it would be. 407 00:23:29,400 --> 00:23:31,040 This violent cosmic tango 408 00:23:31,120 --> 00:23:33,880 brings the two supermassive black holes together. 409 00:23:35,480 --> 00:23:39,560 It's elegant. It's beautiful. It's this billion-year 410 00:23:39,640 --> 00:23:44,200 choreographed dance that is entirely conducted by gravity. 411 00:23:47,560 --> 00:23:50,280 The two heavyweight fighters approach each other. 412 00:23:50,360 --> 00:23:53,680 Their feet beat out a rhythm on the canvas, 413 00:23:53,760 --> 00:23:55,760 just like circling black holes 414 00:23:55,840 --> 00:23:58,760 release low-energy gravitational waves. 415 00:24:00,160 --> 00:24:02,000 You have these giant beasts 416 00:24:02,080 --> 00:24:04,840 that are stalking around each other 417 00:24:04,920 --> 00:24:09,600 and as they do, they create these gravitational waves. 418 00:24:11,120 --> 00:24:13,080 June, 2021. 419 00:24:13,160 --> 00:24:16,480 Astronomers photograph a galactic collision 420 00:24:16,560 --> 00:24:20,840 and witness a spectacular pre-fight fireworks show. 421 00:24:22,120 --> 00:24:25,200 One of the amazing things that can happen when galaxies collide is 422 00:24:25,280 --> 00:24:27,680 they can create tremendous starbursts. 423 00:24:29,160 --> 00:24:32,760 There is a big in-rush as all of that gas follows that gravity. 424 00:24:32,840 --> 00:24:36,880 As the gas gets hotter and denser, it creates shockwaves. 425 00:24:38,360 --> 00:24:41,520 And each shockwave actually creates a new generation of stars 426 00:24:41,600 --> 00:24:44,160 going out around the core of the galaxy. 427 00:24:44,240 --> 00:24:47,400 The sudden starburst lights up the merging galaxies. 428 00:24:47,480 --> 00:24:51,640 The in-rushing gas also fuels the prize-fighters, 429 00:24:51,720 --> 00:24:54,160 the supermassive black holes 430 00:24:54,240 --> 00:24:57,800 spiraling towards the merging galactic center. 431 00:25:00,520 --> 00:25:03,440 But only if the galaxies approach at the right angle. 432 00:25:03,520 --> 00:25:07,840 It's not the case that every merger feeds a black hole. 433 00:25:07,920 --> 00:25:11,320 Sometimes it actually strips material 434 00:25:11,400 --> 00:25:13,920 away from the central regions 435 00:25:14,000 --> 00:25:17,240 and then there's no food there for the black holes to eat. 436 00:25:19,040 --> 00:25:21,720 A head-on collision with another black hole 437 00:25:21,800 --> 00:25:25,720 could strip the material around the supermassive black hole. 438 00:25:25,800 --> 00:25:27,800 With nothing there, 439 00:25:27,880 --> 00:25:30,080 the black holes can't power themselves. 440 00:25:32,000 --> 00:25:35,680 To get the biggest bang requires an attacking angle 441 00:25:35,760 --> 00:25:38,360 that'll help feed a starving black hole. 442 00:25:39,520 --> 00:25:41,640 With a grazing collision, 443 00:25:41,720 --> 00:25:45,880 the gas pockets surrounding the black hole survive 444 00:25:45,960 --> 00:25:47,960 and gain more mass. 445 00:25:48,040 --> 00:25:49,760 And that can power it even more. 446 00:25:49,840 --> 00:25:52,320 It can make it even more spectacular. 447 00:25:52,400 --> 00:25:55,280 If there's a big supermassive black hole, 448 00:25:55,360 --> 00:25:58,760 that suddenly finds it surrounded by loads of gas 449 00:25:58,840 --> 00:26:00,920 and other material it can eat, 450 00:26:01,000 --> 00:26:04,120 it goes on a kind of feeding frenzy. 451 00:26:04,200 --> 00:26:06,760 If you're a hungry supermassive black hole, 452 00:26:06,840 --> 00:26:09,120 then this is your lunchtime buffet. 453 00:26:10,720 --> 00:26:14,040 Not all the gas falls into the supermassive black hole. 454 00:26:15,640 --> 00:26:18,640 Other parts of the matter actually gets caught up in what we call 455 00:26:18,720 --> 00:26:22,280 an "accretion disk" rotating around the outside of the black hole. 456 00:26:23,360 --> 00:26:26,960 This bright vortex spins around the supermassive black hole 457 00:26:27,040 --> 00:26:29,200 at over two million miles an hour. 458 00:26:30,720 --> 00:26:33,800 The material in the disk rubs against itself, 459 00:26:33,880 --> 00:26:35,880 creating friction. 460 00:26:35,960 --> 00:26:39,680 Friction generates heat. If I rub my hands together, 461 00:26:39,760 --> 00:26:41,760 they get a little bit warm. 462 00:26:41,840 --> 00:26:43,840 If I rub my hands together 463 00:26:43,920 --> 00:26:46,560 at hundreds of thousands of miles per hour, 464 00:26:46,640 --> 00:26:48,760 it's gonna get very, very, very warm. 465 00:26:50,440 --> 00:26:54,880 The accretion disk keeps up blasting out intense light. 466 00:26:57,360 --> 00:27:00,440 In 2020, NASA's Hubble Space Telescope 467 00:27:00,520 --> 00:27:04,120 saw two fueled-up supermassive black holes 468 00:27:04,200 --> 00:27:06,680 lighting up for the fight. 469 00:27:07,640 --> 00:27:09,360 We call them quasars. 470 00:27:11,160 --> 00:27:16,120 Quasars are a sub-class of very bright black holes 471 00:27:16,200 --> 00:27:18,320 that are emitting huge amounts of power. 472 00:27:18,400 --> 00:27:21,440 So these can be seen at the far reaches of the universe. 473 00:27:24,240 --> 00:27:27,040 Black holes, these so-called dark things, 474 00:27:27,120 --> 00:27:29,120 when they're growing at a very high rate, 475 00:27:29,200 --> 00:27:31,880 are some of the brightest lights in the universe. 476 00:27:33,160 --> 00:27:37,280 To date, we've detected over 100 pairs of quasars 477 00:27:37,360 --> 00:27:39,760 in the cores of merging galaxies. 478 00:27:39,840 --> 00:27:43,680 We think they will all eventually collide. 479 00:27:45,400 --> 00:27:47,440 But before they do, they'll put on 480 00:27:47,520 --> 00:27:50,640 a spectacular and lethal light show... 481 00:27:52,560 --> 00:27:54,560 A common theme in science fiction 482 00:27:54,640 --> 00:27:57,240 are different kinds of jets of energy or beams 483 00:27:57,320 --> 00:27:59,720 that people shoot out of their eyes or their hands. 484 00:27:59,800 --> 00:28:02,800 Well, supermassive black holes do that, too. 485 00:28:02,880 --> 00:28:05,720 ...firing out relativistic jets. 486 00:28:07,840 --> 00:28:09,840 When those jets fire up, 487 00:28:09,920 --> 00:28:13,240 that's when you're talking about superstar. 488 00:28:13,320 --> 00:28:15,040 Really, really bright lights. 489 00:28:15,120 --> 00:28:17,720 And at this point, the galaxy is lit up and ready to go. 490 00:28:19,840 --> 00:28:24,040 These are the spotlights on Madison Square Garden. 491 00:28:24,120 --> 00:28:27,160 This is telling you that the event is going down. 492 00:28:29,520 --> 00:28:31,840 A single supermassive black hole jet 493 00:28:31,920 --> 00:28:34,520 will produce more energy in a second 494 00:28:34,600 --> 00:28:38,880 than the sun will produce in its entire ten-billion-year lifetime. 495 00:28:43,560 --> 00:28:46,680 Imagine a laser of radiation 496 00:28:46,760 --> 00:28:49,520 that is light years in length and across. 497 00:28:49,600 --> 00:28:53,880 That's what we're talking about. This thing would fry a planet. 498 00:28:54,800 --> 00:28:56,400 This is no pre-fight hype. 499 00:28:57,600 --> 00:29:01,440 In February, 2020 we saw the impact of a jet. 500 00:29:03,080 --> 00:29:05,120 So in the Ophiuchus galaxy cluster, 501 00:29:05,200 --> 00:29:06,840 there's an enormous void 502 00:29:06,920 --> 00:29:09,480 that is 15 times wider than the Milky Way galaxy. 503 00:29:09,560 --> 00:29:11,880 And this has all been sculpted, carved 504 00:29:11,960 --> 00:29:15,680 by jets from a supermassive black hole. 505 00:29:15,760 --> 00:29:17,800 It's like this scar on the universe. 506 00:29:17,880 --> 00:29:21,080 It's a million light years across. It's huge. 507 00:29:21,160 --> 00:29:25,560 Scientists calculate the impact of the jet hitting the cluster 508 00:29:25,640 --> 00:29:30,640 was equivalent to a 20 billion billion megaton TNT explosion 509 00:29:30,720 --> 00:29:33,040 every thousandth of a second 510 00:29:33,120 --> 00:29:35,640 for 240 million years. 511 00:29:39,520 --> 00:29:42,480 But how does a black hole generate so much power? 512 00:29:42,560 --> 00:29:44,920 Even though there's a lot of energy 513 00:29:45,000 --> 00:29:47,640 in the accretion disk surrounding a black hole, 514 00:29:47,720 --> 00:29:51,400 there's not enough to launch these really powerful jets. 515 00:29:51,480 --> 00:29:54,600 Because we can't account for it any other way, 516 00:29:54,680 --> 00:29:56,400 there must be something else 517 00:29:56,480 --> 00:29:58,920 that's contributing energy to these jets. 518 00:30:01,040 --> 00:30:03,400 We get a clue in 2021 519 00:30:03,480 --> 00:30:06,360 when scientists publish a new photo 520 00:30:06,440 --> 00:30:10,560 of the supermassive black hole M87 star. 521 00:30:11,880 --> 00:30:13,880 It shows the accretion disk. 522 00:30:13,960 --> 00:30:17,720 The lines represent magnetic field lines. 523 00:30:19,080 --> 00:30:22,520 The fast-spinning accretion disk drags the magnetic field 524 00:30:22,600 --> 00:30:24,680 around the supermassive black hole, 525 00:30:24,760 --> 00:30:26,760 charging it up for the battle. 526 00:30:28,160 --> 00:30:30,800 The accretion disk around a black hole 527 00:30:30,880 --> 00:30:33,840 isn't just swirling around like crazy. 528 00:30:33,920 --> 00:30:37,280 It's also undulating and moving and wiggling, 529 00:30:37,360 --> 00:30:41,000 and this causes the magnetic field to fold in on itself. 530 00:30:41,080 --> 00:30:43,640 And every time it folds, it amplifies itself, 531 00:30:43,720 --> 00:30:46,120 getting stronger and stronger and stronger. 532 00:30:46,200 --> 00:30:50,800 This is a dynamo that powers this incredible magnetic field. 533 00:30:50,880 --> 00:30:55,240 The magnetic field can't hold onto the building energy any longer. 534 00:30:56,400 --> 00:30:58,000 It erupts. 535 00:30:58,080 --> 00:31:00,480 These magnetic field lines then sweep up and away 536 00:31:00,560 --> 00:31:03,040 like a tornado. And that can lift material 537 00:31:03,120 --> 00:31:05,600 away from the black hole and the accretion disk 538 00:31:05,680 --> 00:31:08,080 and shoot it out into intergalactic space. 539 00:31:09,560 --> 00:31:11,920 The relativistic jet's immense power 540 00:31:12,000 --> 00:31:15,720 may be a showstopper, but when it's time to land the killer punch 541 00:31:15,800 --> 00:31:17,800 supermassive black holes 542 00:31:17,880 --> 00:31:21,680 draw on an even more powerful force, gravity. 543 00:31:21,760 --> 00:31:26,680 Jets are very powerful, but really only on a relatively small scale. 544 00:31:26,760 --> 00:31:29,040 When you're talking about cosmic scale, 545 00:31:29,120 --> 00:31:30,840 gravity always wins. 546 00:31:30,920 --> 00:31:33,160 Nothing is as powerful as gravity. 547 00:31:35,680 --> 00:31:41,480 Across the universe, supermassive black holes duke it out 548 00:31:41,560 --> 00:31:45,480 in the cosmos' version of heavyweight superfights. 549 00:31:45,560 --> 00:31:50,400 Supermassive black holes are merging around us all the time. 550 00:31:50,480 --> 00:31:52,760 It's only our ability to detect them 551 00:31:52,840 --> 00:31:55,360 that's preventing us from seeing them. 552 00:31:57,040 --> 00:32:00,160 Scientists have identified at least a dozen pairs 553 00:32:00,240 --> 00:32:03,400 of supermassive black holes circling each other. 554 00:32:04,560 --> 00:32:07,080 We have some hints of some galaxies 555 00:32:07,160 --> 00:32:09,000 where we think it might happen, 556 00:32:09,080 --> 00:32:12,280 where we see two glowing black holes that are getting very close. 557 00:32:13,800 --> 00:32:16,520 But not all these matches will end with a knockout. 558 00:32:17,880 --> 00:32:20,280 Black hole collisions happen all the time, 559 00:32:20,360 --> 00:32:23,000 but they don't always go according to plan. 560 00:32:23,080 --> 00:32:26,640 When black holes come together, really strange things can happen. 561 00:32:29,160 --> 00:32:32,320 The Hubble Space Telescope spots something strange 562 00:32:32,400 --> 00:32:36,160 in a distant galaxy called 3C186. 563 00:32:38,080 --> 00:32:41,360 It's a quasar, an active supermassive black hole. 564 00:32:43,640 --> 00:32:45,640 But it's in the wrong place. 565 00:32:46,640 --> 00:32:48,560 In nearly every galaxy, we see 566 00:32:48,640 --> 00:32:51,400 the supermassive black hole sits right at the center. 567 00:32:51,480 --> 00:32:53,120 That makes sense. 568 00:32:53,200 --> 00:32:56,680 Because that's the only place with enough material to power them. 569 00:32:56,760 --> 00:33:00,320 But in 3C186, that's not what we see. 570 00:33:00,400 --> 00:33:03,480 The supermassive black hole is displaced from the center. 571 00:33:03,560 --> 00:33:06,880 And not a little bit. It's 35,000 light years. 572 00:33:06,960 --> 00:33:10,320 So to see a quasar 35,000 light years away from the core 573 00:33:10,400 --> 00:33:13,640 means something really violent had to happen there. 574 00:33:13,720 --> 00:33:17,720 The quasar is racing away from the center of the galaxy 575 00:33:17,800 --> 00:33:20,240 at over four million miles an hour. 576 00:33:20,320 --> 00:33:23,200 That is insane! 577 00:33:23,280 --> 00:33:26,360 The magnitude of the energy and the forces required 578 00:33:26,440 --> 00:33:28,880 are just something unimaginable. 579 00:33:28,960 --> 00:33:31,360 So what can kick 580 00:33:31,440 --> 00:33:34,000 a giant black hole out of a galaxy? 581 00:33:35,280 --> 00:33:37,280 What has that kind of power? 582 00:33:37,360 --> 00:33:41,200 The answer is a clash that wasn't evenly matched. 583 00:33:42,200 --> 00:33:46,840 The two supermassive black holes were different sizes, 584 00:33:46,920 --> 00:33:50,520 a middleweight boxer taking on a heavyweight. 585 00:33:52,000 --> 00:33:54,400 When humans set up a fight, we like to make it fair 586 00:33:54,480 --> 00:33:57,120 because it's sport. Nature doesn't care about sport. 587 00:33:57,200 --> 00:33:58,440 It's survival of the fittest. 588 00:33:58,520 --> 00:34:03,280 This is not a fair fight. It's over before it even begins. 589 00:34:03,360 --> 00:34:06,080 One punch and it's a K-O. 590 00:34:08,120 --> 00:34:10,640 As these two black holes are merging, 591 00:34:10,720 --> 00:34:12,480 there's one really small black hole 592 00:34:12,560 --> 00:34:14,400 and one much bigger black hole. 593 00:34:14,480 --> 00:34:16,240 The whole system wobbles around 594 00:34:16,320 --> 00:34:18,480 and it can get more of a gravitational wave kick 595 00:34:18,560 --> 00:34:20,280 in one direction than the other. 596 00:34:20,360 --> 00:34:23,640 And that's momentum. That's a push. That's enough energy 597 00:34:23,720 --> 00:34:26,200 to kick the black hole out. 598 00:34:28,200 --> 00:34:30,560 The lopsided gravitational punch 599 00:34:30,640 --> 00:34:33,600 sends the merged supermassive black hole 600 00:34:33,680 --> 00:34:35,680 on a one-way trip to oblivion. 601 00:34:37,200 --> 00:34:39,800 This tells us that gravitational waves can be 602 00:34:39,880 --> 00:34:43,960 tremendously powerful. They can move a supermassive black hole 603 00:34:44,040 --> 00:34:46,880 out from the center of a galaxy and send it on its way. 604 00:34:47,920 --> 00:34:50,520 But it just carries on drifting. There's no way to stop it. 605 00:34:50,600 --> 00:34:53,200 And who knows? In a few million years, 606 00:34:53,280 --> 00:34:56,080 it could just drift entirely out of its galaxy 607 00:34:56,160 --> 00:34:58,760 and go floating off into deep space. 608 00:35:00,560 --> 00:35:04,400 In some matches, the fighters don't even land a punch. 609 00:35:06,400 --> 00:35:09,760 Scientists spot a supermassive black hole 610 00:35:09,840 --> 00:35:14,200 named B3 1715+425. 611 00:35:15,440 --> 00:35:17,640 This black hole is strange. 612 00:35:19,400 --> 00:35:21,280 Stripped of all its stars, 613 00:35:21,360 --> 00:35:25,720 it hurtles through empty space at 4.5 million miles an hour. 614 00:35:25,800 --> 00:35:28,040 The first thing that draws our attention 615 00:35:28,120 --> 00:35:31,360 is this faint trail of debris across the sky. 616 00:35:31,440 --> 00:35:35,880 There is actually a trail leading back to the center of the galaxy. 617 00:35:35,960 --> 00:35:38,800 It's kinda like a dump truck that's filled with dirt 618 00:35:38,880 --> 00:35:42,000 driving down the highway, and the dirt's flying off behind it. 619 00:35:42,080 --> 00:35:44,080 This is a naked black hole. 620 00:35:44,160 --> 00:35:48,520 The exposed supermassive black hole has lost its stars and galaxy. 621 00:35:48,600 --> 00:35:52,680 A champion stripped of its fans and entourage. 622 00:35:52,760 --> 00:35:55,680 So what event is powerful enough 623 00:35:55,760 --> 00:36:00,800 to strip a supermassive black hole of its entire host galaxy? 624 00:36:00,880 --> 00:36:03,520 That has to be something really big. 625 00:36:05,720 --> 00:36:07,720 B3 is a smallish galaxy 626 00:36:07,800 --> 00:36:10,320 and it got into a scrap with a much bigger one. 627 00:36:10,400 --> 00:36:12,480 The stronger gravity of the bigger galaxy 628 00:36:12,560 --> 00:36:16,320 stripped the stars away from that black hole and shot it out. 629 00:36:17,160 --> 00:36:20,040 Typically, in the universe when something's bigger and more massive, 630 00:36:20,120 --> 00:36:22,800 it wins. So this is true for galaxies. 631 00:36:22,880 --> 00:36:25,160 A big galaxy versus a little galaxy, 632 00:36:25,240 --> 00:36:27,040 put your money on the big one. 633 00:36:28,520 --> 00:36:32,280 But when two evenly-matched heavyweights enter the ring... 634 00:36:33,760 --> 00:36:36,120 ...it's time for the main event. 635 00:36:37,880 --> 00:36:39,880 A clash of the titans. 636 00:36:41,000 --> 00:36:43,040 I grew up watching boxing with my dad, 637 00:36:43,120 --> 00:36:45,000 so I've always been a boxing fan. 638 00:36:45,080 --> 00:36:48,920 And I love a great battle. And what's a bigger battle 639 00:36:49,000 --> 00:36:53,080 than a head-on collision between two supermassive black holes? 640 00:36:53,160 --> 00:36:55,840 If you're a boxing fan, this is the big one. 641 00:36:55,920 --> 00:36:59,400 We are ready. We are on the edge of our seats. 642 00:37:00,760 --> 00:37:02,920 We've got two supermassive black holes, 643 00:37:03,000 --> 00:37:05,720 each one is in their corner, and they're getting ready 644 00:37:05,800 --> 00:37:07,800 for the fight of the century. 645 00:37:09,320 --> 00:37:12,400 I mean, they're just gonna go at it, like goosh, goosh. 646 00:37:12,480 --> 00:37:15,400 I would watch that. I'd pay-per-view that. 647 00:37:15,480 --> 00:37:18,280 It doesn't get any better than this. These are prize-fighters 648 00:37:18,360 --> 00:37:21,240 at the top of their game, they're trained to a T, 649 00:37:21,320 --> 00:37:24,600 they're beefed up, they are ready to rumble. 650 00:37:28,760 --> 00:37:32,200 Welcome to the heavyweight championship of the universe. 651 00:37:32,280 --> 00:37:35,800 Weighing in at eight billion solar masses, 652 00:37:35,880 --> 00:37:38,720 we have The Galactic Destroyer, 653 00:37:38,800 --> 00:37:40,800 M101 star. 654 00:37:40,880 --> 00:37:46,200 And in the other corner, at a punishing 7.8 billion suns, 655 00:37:46,280 --> 00:37:50,480 The Star Crusher, NSC 47 star. 656 00:37:50,560 --> 00:37:54,520 They are pumped and ready to rumble. 657 00:37:54,600 --> 00:37:57,160 So here it is. We're finally here. 658 00:37:57,240 --> 00:37:59,560 The crowd is roaring. 659 00:37:59,640 --> 00:38:03,800 The bell has rung and the fighters are approaching each other. 660 00:38:03,880 --> 00:38:05,880 They are ready to go at it. 661 00:38:07,680 --> 00:38:10,800 Let's have a clean fight, fellas. Touch hands 662 00:38:10,880 --> 00:38:13,840 and go back to your corners. 663 00:38:13,920 --> 00:38:17,120 Round One. The two heavyweights circle, 664 00:38:17,200 --> 00:38:19,160 testing the other's defenses. 665 00:38:19,240 --> 00:38:21,920 The black holes are gonna do what the boxers are gonna do. 666 00:38:22,000 --> 00:38:25,360 They're gonna circle each other and they're gonna orbit each other 667 00:38:25,440 --> 00:38:28,320 and they're gonna size each other up. 668 00:38:28,400 --> 00:38:31,760 Once these two supermassive black holes are close enough, 669 00:38:31,840 --> 00:38:35,120 they're gravity inexorably is gonna draw them together. 670 00:38:37,320 --> 00:38:40,400 As the two supermassive black holes get closer, 671 00:38:40,480 --> 00:38:42,960 they throw a few exploratory jabs... 672 00:38:46,160 --> 00:38:49,360 ...triggering bursts of gravitational waves 673 00:38:49,440 --> 00:38:51,920 that warp everything in their path. 674 00:38:52,000 --> 00:38:55,000 These enormous gravitational waves 675 00:38:55,080 --> 00:38:59,520 are completely deforming the fabric of space time around them. 676 00:38:59,600 --> 00:39:01,760 Not just a little bit, but a lot! 677 00:39:01,840 --> 00:39:06,280 It's like feeling the fighters approach in the boxing ring 678 00:39:06,360 --> 00:39:08,960 from the next town over. 679 00:39:14,320 --> 00:39:17,640 Next, the supermassive black holes' gravity 680 00:39:17,720 --> 00:39:19,720 throws in a couple of right hooks 681 00:39:19,800 --> 00:39:22,600 straight into the accretion disks. 682 00:39:25,360 --> 00:39:28,320 What could happen is that they start to form like 683 00:39:28,400 --> 00:39:30,920 an angle grinder. You'll see sparks flying 684 00:39:31,000 --> 00:39:35,040 as they try to merge and form a new, single accretion disk. 685 00:39:35,120 --> 00:39:37,560 When those accretion disks collide, 686 00:39:37,640 --> 00:39:40,440 the whole thing is gonna light up like the 4th of July. 687 00:39:42,560 --> 00:39:45,200 Spiraling in at millions of miles an hour 688 00:39:45,280 --> 00:39:47,800 the heavyweight fighters get close, 689 00:39:47,880 --> 00:39:50,200 delivering punishing body blows. 690 00:39:54,280 --> 00:39:58,720 The event horizons, the surface of the supermassive black holes, 691 00:39:58,800 --> 00:40:00,800 are about to touch. 692 00:40:02,320 --> 00:40:05,360 In their final moments, these two supermassive black holes 693 00:40:05,440 --> 00:40:08,040 are orbiting each other at a significant fraction 694 00:40:08,120 --> 00:40:09,440 of the speed of light, 695 00:40:09,520 --> 00:40:11,720 and their event horizons will touch. 696 00:40:13,440 --> 00:40:16,880 And they'll eventually merge into one new supermassive black hole. 697 00:40:18,000 --> 00:40:20,600 You might think: don't they bump into each other 698 00:40:20,680 --> 00:40:22,360 like bowling balls? No, they don't. 699 00:40:22,440 --> 00:40:25,040 Because what we're calling the edge of the black hole 700 00:40:25,120 --> 00:40:28,040 is actually not a thing. That's just the surface 701 00:40:28,120 --> 00:40:31,240 around the black hole. Gravity is so strong, nothing can come out. 702 00:40:31,320 --> 00:40:36,200 The two supermassive black holes finally merge, 703 00:40:36,280 --> 00:40:39,680 releasing around five percent of the mass they've gathered 704 00:40:39,760 --> 00:40:43,640 over billions of years in an enormous burst 705 00:40:43,720 --> 00:40:46,200 of gravitational waves. 706 00:40:46,280 --> 00:40:48,600 The amount of energy we're talking about... 707 00:40:50,400 --> 00:40:53,360 There's nothing to compare it to. It's mind-crushing. 708 00:40:53,440 --> 00:40:56,520 There's really almost no point in thinking about it. 709 00:40:56,600 --> 00:41:00,240 It's just not something I think that I can wrap my head around. 710 00:41:00,320 --> 00:41:02,320 Coming from where I come from, 711 00:41:02,400 --> 00:41:04,400 you know, you don't show weakness. 712 00:41:04,480 --> 00:41:07,320 So I'm not gonna say that the collision of two black holes 713 00:41:07,400 --> 00:41:09,560 is more powerful than one of my punches, 714 00:41:09,640 --> 00:41:12,200 but... it's close. 715 00:41:14,160 --> 00:41:17,040 The gigantic and powerful gravitational waves 716 00:41:17,120 --> 00:41:20,000 race out from the collision zone, 717 00:41:20,080 --> 00:41:23,240 leaving a single merged black hole. 718 00:41:24,440 --> 00:41:27,040 This supermassive black hole, after it merges, 719 00:41:27,120 --> 00:41:30,360 permanently deforms the fabric of space time around it. 720 00:41:30,440 --> 00:41:33,600 And this deformation travels out at the speed of light. 721 00:41:35,320 --> 00:41:37,800 The surviving 95 percent of mass 722 00:41:37,880 --> 00:41:40,800 from the two colliding supermassive black holes 723 00:41:40,880 --> 00:41:45,440 is now locked in a single ultramassive black hole. 724 00:41:46,440 --> 00:41:50,480 The undisputed super heavyweight champion of the universe. 725 00:41:50,560 --> 00:41:52,560 At least for now. 726 00:41:53,800 --> 00:41:56,040 It seems the universe is always upping the ante. 727 00:41:56,120 --> 00:41:59,440 Could there be something even more violent we haven't discovered yet? 728 00:41:59,520 --> 00:42:03,360 The universe keeps wanting to give us something more violent all the time. 729 00:42:04,960 --> 00:42:07,680 Energy locked in hydrogen atoms 730 00:42:07,760 --> 00:42:09,760 formed at the birth of the universe 731 00:42:09,840 --> 00:42:13,280 is finally released in the violent collision 732 00:42:13,360 --> 00:42:17,480 and builds an ultramassive black hole. 733 00:42:20,360 --> 00:42:23,920 This is one of the most beautiful stories in our universe. 734 00:42:24,000 --> 00:42:26,560 You have the most energetic collision, 735 00:42:26,640 --> 00:42:29,480 the most amount of energy released, the most violent event 736 00:42:29,560 --> 00:42:34,080 can trace its origins to the humble hydrogen atom. 737 00:42:34,160 --> 00:42:38,000 There are things constantly being built up and then destroyed. 738 00:42:38,080 --> 00:42:42,320 It's sort of the cycle of life in our universe 739 00:42:42,400 --> 00:42:46,600 that evolves various exotic phenomenon 740 00:42:46,680 --> 00:42:51,160 and makes them into something more beautiful and transformative. 741 00:42:51,240 --> 00:42:53,240 Our universe has managed to create 742 00:42:53,320 --> 00:42:56,280 both these fearsome weapons of mass destruction, 743 00:42:56,360 --> 00:42:58,360 monster black holes, 744 00:42:58,440 --> 00:43:01,240 and also conscious life 745 00:43:01,320 --> 00:43:04,520 that can write poetry and ponder the meaning of it all. 746 00:43:09,440 --> 00:43:11,560 So, we have our champion. 747 00:43:11,640 --> 00:43:14,560 Matter compressed and then smashed together 748 00:43:14,640 --> 00:43:16,640 by supermassive black holes 749 00:43:16,720 --> 00:43:20,160 creates the most violent event in the universe. 750 00:43:21,600 --> 00:43:23,480 I don't think there's a contest. 751 00:43:23,560 --> 00:43:25,680 The supermassive black hole collisions 752 00:43:25,760 --> 00:43:30,120 are the most energetic, just like mind-numbingly large 753 00:43:30,200 --> 00:43:32,880 amounts of energy in these collisions. 754 00:43:35,560 --> 00:43:38,480 A merger of two supermassive black holes 755 00:43:38,560 --> 00:43:41,760 is at the absolute top end extreme of that 756 00:43:41,840 --> 00:43:45,560 for all possible events in the entire universe. 757 00:43:45,640 --> 00:43:47,960 A supermassive black hole merger 758 00:43:48,040 --> 00:43:52,000 is the most violent thing that we can observe in the universe. 759 00:43:52,080 --> 00:43:54,080 Subtitling by Iyuno 62640

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