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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:00,000 --> 00:00:05,000 [Music] 2 00:00:05,000 --> 00:00:11,000 the study of extreme physics 3 00:00:11,000 --> 00:00:23,000 brought us the bomb 4 00:00:23,000 --> 00:00:32,000 it has taken us inside the violent death of a star 5 00:00:32,000 --> 00:00:37,000 and now it has brought us face to face with the most destructive force in 6 00:00:37,000 --> 00:00:44,000 nature a super massive black hole 7 00:00:44,000 --> 00:00:52,000 how large how powerful can these monsters get 8 00:00:52,000 --> 00:00:58,000 and what can they tell us about the extremes of time 9 00:00:58,000 --> 00:01:13,000 and space 10 00:01:13,000 --> 00:01:19,000 [Music] 11 00:01:19,000 --> 00:01:25,000 the year was 1990. [Music] hope for a new age of scientific 12 00:01:25,000 --> 00:01:36,000 discovery rose into orbit aboard the hubble space telescope [Music] 13 00:01:36,000 --> 00:01:44,000 a technical flaw in its optics requiring astronauts to fly up to repair it would delay but not stop 14 00:01:44,000 --> 00:01:54,000 this new age from dawning 15 00:01:54,000 --> 00:01:59,000 in 1994 astronomers pointed the newly repaired hubble at one of its most 16 00:01:59,000 --> 00:02:07,000 important targets a giant elliptical galaxy 50 million light years from earth called 17 00:02:07,000 --> 00:02:15,000 m87 18 00:02:15,000 --> 00:02:21,000 pushing deep into m87s core they glimpsed a powerful jet of super 19 00:02:21,000 --> 00:02:27,000 hot gas extending 5 000 light years into space 20 00:02:27,000 --> 00:02:33,000 with hubble's remarkable resolving power astronomers measured the speed of the gas racing 21 00:02:33,000 --> 00:02:38,000 around the center they concluded the gravitational source 22 00:02:38,000 --> 00:02:43,000 driving these motions is a black hole weighing in at 6.6 23 00:02:43,000 --> 00:02:51,000 billion times the mass of our sun news of m87 joined a flood of 24 00:02:51,000 --> 00:03:02,000 discoveries beaming down from hubble's instruments 25 00:03:02,000 --> 00:03:09,000 the public was captivated by strange and majestic shapes captured from mysterious realms far 26 00:03:09,000 --> 00:03:19,000 beyond earth 27 00:03:19,000 --> 00:03:26,000 to scientists hubble was part of a quickly expanding arsenal of observing tools 28 00:03:26,000 --> 00:03:33,000 a growing fleet of space observatories scanned the light of distant objects across the entire electromagnetic 29 00:03:33,000 --> 00:03:40,000 spectrum [Music] 30 00:03:40,000 --> 00:03:46,000 on the ground a new generation of giant telescopes with precision mirrors and dynamic 31 00:03:46,000 --> 00:03:55,000 optics allowed observers to look deep into the universe [Music] 32 00:03:55,000 --> 00:04:02,000 astronomers used to long nights of painstaking camera exposures were now a wash in data streaming in 33 00:04:02,000 --> 00:04:10,000 from distant corners of the cosmos [Music] 34 00:04:10,000 --> 00:04:21,000 a new vision of the universe emerged one defined by vast energy releases 35 00:04:21,000 --> 00:04:27,000 titanic collisions [Music] 36 00:04:27,000 --> 00:04:35,000 mysterious new forces [Music] and nature's strangest phenomenon 37 00:04:35,000 --> 00:04:42,000 the black hole 38 00:04:42,000 --> 00:04:47,000 once thought of as mere curiosities black holes have taken center stage in our 39 00:04:47,000 --> 00:05:04,000 understanding of the universe and how it came to be 40 00:05:04,000 --> 00:05:19,000 a black hole begins its life in the brilliant light of a dying star 41 00:05:19,000 --> 00:05:25,000 within the folds of our galaxy the energy let loose by supernovae stirs the 42 00:05:25,000 --> 00:05:35,000 celestial mix 43 00:05:35,000 --> 00:05:43,000 shock waves from these explosions cause gas to condense then ignite 44 00:05:43,000 --> 00:05:51,000 [Music] stars are born sometimes hundreds at a 45 00:05:51,000 --> 00:06:03,000 time [Music] 46 00:06:03,000 --> 00:06:10,000 intense stellar winds from these newborn stars sculpt majestic castles of gas 47 00:06:10,000 --> 00:06:18,000 the great nebulae long admired by 48 00:06:18,000 --> 00:06:25,000 astronomers 49 00:06:25,000 --> 00:06:35,000 yet for the giant stars that set this process in motion the consequences are grim 50 00:06:35,000 --> 00:06:41,000 back in the mid 1800s mariners plied southern seas by the light of a brilliant star 51 00:06:41,000 --> 00:06:48,000 just off the plane of the galaxy in the constellation karina 52 00:06:48,000 --> 00:06:55,000 for over a decade it was the second brightest star in the sky 53 00:06:55,000 --> 00:07:01,000 astronomers have been studying it intensively ever since 54 00:07:01,000 --> 00:07:08,000 the star named ada carine had undergone what's now known as the great eruption 55 00:07:08,000 --> 00:07:13,000 an outburst that expelled two luminous lobes of gas that stretched some 12 trillion 56 00:07:13,000 --> 00:07:24,000 kilometers from end to end [Music] 57 00:07:24,000 --> 00:07:31,000 [Music] 58 00:07:31,000 --> 00:07:38,000 astronomers recently found that ada carinae is actually two giant stars closely orbiting one 59 00:07:38,000 --> 00:07:45,000 another to explain the extreme turbulence of 60 00:07:45,000 --> 00:07:52,000 this scene scientists modeled the fierce hot winds roaring out of these two companions 61 00:07:52,000 --> 00:07:57,000 [Music] the orbital motions of the two stars 62 00:07:57,000 --> 00:08:03,000 allowed them to peg the larger one at 90 times the mass of the sun 63 00:08:03,000 --> 00:08:09,000 eta carinae is a supernova waiting to happen 64 00:08:09,000 --> 00:08:24,000 in time it will cease with convulsions then collapse and 65 00:08:24,000 --> 00:08:31,000 explode throughout history our understanding of 66 00:08:31,000 --> 00:08:40,000 space has been shaped by a handful of supernovae visible to the naked eye some 67 00:08:40,000 --> 00:08:46,000 archaeologists believe this drawing depicts a supernova spotted by north american stargazers 68 00:08:46,000 --> 00:08:52,000 in the year 1054. the same event was also recorded in 69 00:08:52,000 --> 00:08:57,000 china korea and the middle east 70 00:08:57,000 --> 00:09:06,000 in europe supernova sightings help dispel the prevailing belief that the heavens are static and 71 00:09:06,000 --> 00:09:14,000 unchanging the astronomer tycho brahe saw one in the year 1572 72 00:09:14,000 --> 00:09:21,000 i was led into such perplexity by the unbelievability of the thing he wrote that i began to doubt the faith 73 00:09:21,000 --> 00:09:32,000 of my own eyes 74 00:09:32,000 --> 00:09:38,000 in modern times astronomers have intensively studied the remnants of the 1054 75 00:09:38,000 --> 00:09:44,000 explosion the famous crab nebula 76 00:09:44,000 --> 00:09:51,000 [Music] waves of radiation roaring out of the explosion have etched circular patterns in the 77 00:09:51,000 --> 00:09:57,000 surrounding gas seen here in radio 78 00:09:57,000 --> 00:10:02,000 infrared [Music] 79 00:10:02,000 --> 00:10:09,000 optical ultraviolet and x-ray light 80 00:10:09,000 --> 00:10:15,000 you can see signs of a jet shooting out of the central region 81 00:10:15,000 --> 00:10:22,000 this energy is coming from a tiny spinning object in the center the size of a city 82 00:10:22,000 --> 00:10:29,000 this neutron star is not made of any elements but subatomic particles packed by 83 00:10:29,000 --> 00:10:35,000 gravity into an ultra dense sphere [Music] 84 00:10:35,000 --> 00:10:42,000 physicists think of it as a single huge atom it's roughly equivalent to packing 85 00:10:42,000 --> 00:10:49,000 mount everest into a sugar cube 86 00:10:49,000 --> 00:11:00,000 yet some dying stars meet a fate that is stranger still 87 00:11:00,000 --> 00:11:08,000 in 1796 pierre simon the marquis de la place imagined a breed of dark stars so heavy 88 00:11:08,000 --> 00:11:16,000 their gravity prevented any light from escaping [Music] this idea a head scratcher fell out of 89 00:11:16,000 --> 00:11:28,000 favor for more than a century 90 00:11:28,000 --> 00:11:40,000 isaac newton had described gravity as a force of attraction between two masses 91 00:11:40,000 --> 00:11:46,000 early in the 20th century albert einstein's equations showed that gravity is actually the 92 00:11:46,000 --> 00:11:52,000 distortion of space-time by massive objects 93 00:11:52,000 --> 00:11:58,000 thus a planet or star or even a galaxy creates a gravitational well that will 94 00:11:58,000 --> 00:12:07,000 bend the path of other objects or even beams of light 95 00:12:07,000 --> 00:12:15,000 as the physicist john archibald wheeler later put it space-time tells matter how to move 96 00:12:15,000 --> 00:12:22,000 matter tells space-time how to curve 97 00:12:22,000 --> 00:12:29,000 in 1919 the now famous eddington expeditions set out to test this wild idea during a 98 00:12:29,000 --> 00:12:36,000 solar eclipse [Music] their data showed that the sun's gravity 99 00:12:36,000 --> 00:12:43,000 bent the path of starlight just as einstein had predicted 100 00:12:43,000 --> 00:12:48,000 but also hiding in einstein's equations was a very strange prospect that 101 00:12:48,000 --> 00:12:55,000 recalled pierre simon's speculation if an object is dense enough it will 102 00:12:55,000 --> 00:13:05,000 bend a beam of light back onto itself causing that light to disappear 103 00:13:05,000 --> 00:13:11,000 physicist carl schwarzfield director of the astrophysical observatory in potsdam germany 104 00:13:11,000 --> 00:13:17,000 took this idea to its logical conclusion working as an artillery lieutenant on 105 00:13:17,000 --> 00:13:24,000 the battlefront of world war one he stole moments to pour over einstein's new theory 106 00:13:24,000 --> 00:13:32,000 as you see he wrote to einstein the war treated me kindly enough in spite of the heavy gunfire to allow 107 00:13:32,000 --> 00:13:37,000 me to get away from it all and take this walk in the land of your ideas 108 00:13:37,000 --> 00:13:43,000 schwarzeeld realized that objects could become so dense their mass would be packed into an 109 00:13:43,000 --> 00:13:49,000 infinitesimal point a singularity 110 00:13:49,000 --> 00:13:55,000 he calculated that these odd creations must be bounded by a larger spherical region 111 00:13:55,000 --> 00:14:02,000 beyond which no light can escape the so-called event horizon 112 00:14:02,000 --> 00:14:08,000 but how could such objects actually exist 113 00:14:08,000 --> 00:14:14,000 in 1939 einstein himself wrote a paper that sought to prove that these strange objects 114 00:14:14,000 --> 00:14:20,000 were impossible but just a few months later physicist 115 00:14:20,000 --> 00:14:27,000 j robert oppenheimer and his graduate students published their own paper on the subject 116 00:14:27,000 --> 00:14:33,000 taking a fresh look at the mathematics of collapsing stars they show that if the parent star is 117 00:14:33,000 --> 00:14:39,000 sufficiently massive the force of the collapse will literally crush its core 118 00:14:39,000 --> 00:14:45,000 down to a point an infinitely dense infinitely curved speck of pure 119 00:14:45,000 --> 00:14:53,000 gravitational energy 120 00:14:53,000 --> 00:14:58,000 oppenheimer went off to spearhead the design of the atomic bomb 121 00:14:58,000 --> 00:15:07,000 having laid the foundations of the modern science of black holes 122 00:15:07,000 --> 00:15:17,000 the atomic age brought a whole new focus on the study of extreme physics 123 00:15:17,000 --> 00:15:24,000 the bomb was terrifying proof as einstein conjectured that a small amount of mass could 124 00:15:24,000 --> 00:15:31,000 convert to a huge amount of energy researchers studied the enormous forces 125 00:15:31,000 --> 00:15:37,000 released when atoms are split apart in chain reactions at the heart of 126 00:15:37,000 --> 00:15:45,000 atomic and thermonuclear bombs 127 00:15:45,000 --> 00:15:54,000 using advanced new computers developed to model and forecast these explosions astrophysicists 128 00:15:54,000 --> 00:16:00,000 began probing the mechanisms at work deep inside stars where lighter elements 129 00:16:00,000 --> 00:16:06,000 burn and fuse into heavier ones they saw how this can eventually lead 130 00:16:06,000 --> 00:16:26,000 large stars to collapse and explode 131 00:16:26,000 --> 00:16:32,000 this grim product of star death entered the popular imagination in 1967 132 00:16:32,000 --> 00:16:38,000 when physicist john wheeler called it a black hole 133 00:16:38,000 --> 00:16:47,000 [Music] 134 00:16:47,000 --> 00:16:53,000 astronomers were already at work looking for these monsters 135 00:16:53,000 --> 00:16:59,000 in 1964 a sounding rocket recorded a high-energy x-ray source in the southern 136 00:16:59,000 --> 00:17:05,000 constellation of cygnus [Music] later satellites recorded a pulsing 137 00:17:05,000 --> 00:17:12,000 rhythm in its light punctuated by outlandish bursts of energy [Music] 138 00:17:12,000 --> 00:17:18,000 after pinpointing its exact location ground-based observatories detected a giant star 139 00:17:18,000 --> 00:17:24,000 that could not by itself emit x-rays 140 00:17:24,000 --> 00:17:31,000 astronomers deduced that cygnus x1 is a star with an unseen companion one 141 00:17:31,000 --> 00:17:37,000 that is eating it alive enveloped in a halo of glowing gas 142 00:17:37,000 --> 00:17:42,000 streaming in from the star that partner weighs in at 15 times the 143 00:17:42,000 --> 00:17:47,000 mass of our sun the first confirmed black hole 144 00:17:47,000 --> 00:17:55,000 [Music] 145 00:17:55,000 --> 00:18:01,000 this computer simulation shows how a black hole makes its presence known 146 00:18:01,000 --> 00:18:12,000 matter spiraling into the abyss forms what's called an accretion disc 147 00:18:12,000 --> 00:18:19,000 the spinning motion generates powerful magnetic fields that whip up a hurricane of particles 148 00:18:19,000 --> 00:18:26,000 and propel them from the poles at nearly the speed of light [Music] 149 00:18:26,000 --> 00:18:33,000 if you were to fall into a star-sized black hole the pull of its gravity rises so sharply 150 00:18:33,000 --> 00:18:40,000 you'd be stretched out until just your atoms remained what physicist stephen hawking once 151 00:18:40,000 --> 00:18:47,000 called spaghettification [Music] 152 00:18:47,000 --> 00:18:56,000 stellar evolution models suggest there could be as many as a billion black holes in our milky way alone 153 00:18:56,000 --> 00:19:03,000 yet they are dwarfed by a far larger and far more powerful presence lurking in the very 154 00:19:03,000 --> 00:19:10,000 core of the galaxy 155 00:19:10,000 --> 00:19:15,000 [Music] the first hints of this presence came in 156 00:19:15,000 --> 00:19:20,000 1932. the bell telephone company was concerned 157 00:19:20,000 --> 00:19:26,000 about static interfering with what it saw as a revolutionary new technology 158 00:19:26,000 --> 00:19:32,000 long-distance radio communications 159 00:19:32,000 --> 00:19:39,000 the company tasked the radio astronomer karl jansky with finding the sources 160 00:19:39,000 --> 00:19:47,000 using this ungainly radio receiver jansky methodically scanned the airwaves 161 00:19:47,000 --> 00:19:55,000 he traced most of the static to thunderstorms some nearby and others far away 162 00:19:55,000 --> 00:20:01,000 then on september 16 1932 he picked up a rumble that he could not 163 00:20:01,000 --> 00:20:07,000 explain this particular noise appeared when the 164 00:20:07,000 --> 00:20:13,000 antenna was pointed at the constellation sagittarius toward the center of the galaxy 165 00:20:13,000 --> 00:20:19,000 it returned every 23 hours and 56 minutes exactly one earth day in relation to the 166 00:20:19,000 --> 00:20:27,000 stars [Music] word of jjansky's findings got out 167 00:20:27,000 --> 00:20:33,000 he assured the public it was not aliens seeking contact [Music] 168 00:20:33,000 --> 00:20:45,000 but it would take another 30 years for astronomers to find out what it was 169 00:20:45,000 --> 00:20:50,000 in the 1960s advanced radio telescopes began picking up signals from distant 170 00:20:50,000 --> 00:20:56,000 space not knowing just what they were observers called them 171 00:20:56,000 --> 00:21:04,000 quasi-stellar radio sources quasars for short 172 00:21:04,000 --> 00:21:15,000 [Music] these bright bluish beacons emitted far greater energy than a star 173 00:21:15,000 --> 00:21:21,000 one cosmic engine was driving them 174 00:21:21,000 --> 00:21:28,000 radio astronomers found that some featured brilliant extensions originating in the centers of galaxies 175 00:21:28,000 --> 00:21:44,000 and reaching millions of light years into space 176 00:21:44,000 --> 00:21:51,000 looking at their light spectra researchers realized that these were actually jets of super hot gas speeding 177 00:21:51,000 --> 00:21:57,000 away at hundreds of thousands of kilometers each second 178 00:21:57,000 --> 00:22:08,000 could such a feature finally explain jansky's findings 179 00:22:08,000 --> 00:22:22,000 it would take a new generation of giant telescopes to reveal the answer [Music] 180 00:22:22,000 --> 00:22:28,000 just as the hubble space telescope began its sensational run several new observatories were 181 00:22:28,000 --> 00:22:33,000 christened on the mountains in hawaii in the north and the andes 182 00:22:33,000 --> 00:22:39,000 mountains in the south [Music] 183 00:22:39,000 --> 00:22:46,000 two rival teams of astronomers each zeroed in on the galactic center to see what was 184 00:22:46,000 --> 00:22:52,000 [Music] 185 00:22:52,000 --> 00:22:58,000 there 186 00:22:58,000 --> 00:23:07,000 [Music] 187 00:23:07,000 --> 00:23:14,000 these teams each undertook a multi-decade effort to track a population of stars that seem 188 00:23:14,000 --> 00:23:25,000 to orbit a concentrated source of energetic emission called sagittarius a star 189 00:23:25,000 --> 00:23:33,000 finally in the spring of 2002 a star labeled s2 swooped in close accelerating to a 190 00:23:33,000 --> 00:23:41,000 remarkable 18 million kilometers per hour 191 00:23:41,000 --> 00:23:47,000 [Music] if its path near sagittarius a star proved erratic 192 00:23:47,000 --> 00:23:54,000 astronomers would know the galactic center was packed with multiple massive objects 193 00:23:54,000 --> 00:24:01,000 instead its path was smooth they concluded that s2 and its 194 00:24:01,000 --> 00:24:09,000 companions must be orbiting a single object weighing several million times the mass of our sun 195 00:24:09,000 --> 00:24:19,000 a supermassive black hole 196 00:24:19,000 --> 00:24:25,000 this effort more than two and a half decades after it began was recognized with the nobel prize in 197 00:24:25,000 --> 00:24:31,000 physics since that discovery astrophysicists 198 00:24:31,000 --> 00:24:37,000 have been feeding additional observation data into their supercomputers to better understand 199 00:24:37,000 --> 00:24:44,000 how clouds of gas flow around and into the monster and how its immense 200 00:24:44,000 --> 00:24:50,000 gravity drives the motions of stars at the center of our galaxy 201 00:24:50,000 --> 00:24:57,000 [Music] the star s2 will inevitably return to 202 00:24:57,000 --> 00:25:03,000 the black hole the pull of gravity will cause its orbit 203 00:25:03,000 --> 00:25:11,000 to shrink pulling it ever closer 204 00:25:11,000 --> 00:25:17,000 astronomers recently caught a glimpse of what would then happen 205 00:25:17,000 --> 00:25:23,000 a survey telescope in the andes mountains recorded the sudden brightening of a galaxy 206 00:25:23,000 --> 00:25:29,000 in distant space astronomers at the european southern observatory 207 00:25:29,000 --> 00:25:34,000 turned their telescopes toward the source [Music] 208 00:25:34,000 --> 00:25:42,000 the light had come from a galaxy 215 million light years away astronomers tracked the 209 00:25:42,000 --> 00:25:47,000 event through to its ultimate demise six months later 210 00:25:47,000 --> 00:25:55,000 they deduced that a star had wandered a little too close to a supermassive black hole 211 00:25:55,000 --> 00:26:03,000 the giant began to tear it apart turning the star into a river of hot gas 212 00:26:03,000 --> 00:26:18,000 fueling a high-energy jet bright enough to be detected from earth 213 00:26:18,000 --> 00:26:23,000 astronomers have long nurtured the hope of seeing a black hole directly 214 00:26:23,000 --> 00:26:34,000 to understand its properties and how it disrupts the space around it 215 00:26:34,000 --> 00:26:40,000 in recent years an international group of astronomers has been working on just such an 216 00:26:40,000 --> 00:26:45,000 audacious goal like the eddington expeditions a century 217 00:26:45,000 --> 00:26:50,000 before these scientists hope to test einstein's theories 218 00:26:50,000 --> 00:27:07,000 only this time in the most extreme laboratory the universe has to offer a black hole 219 00:27:07,000 --> 00:27:12,000 the idea was to adapt a technique developed over 60 years ago 220 00:27:12,000 --> 00:27:17,000 called long baseline interferometry [Music] 221 00:27:17,000 --> 00:27:24,000 by synchronizing radio telescopes all around our planet a team of 400 scientists and engineers 222 00:27:24,000 --> 00:27:32,000 created a much larger virtual telescope with an aperture the diameter of earth 223 00:27:32,000 --> 00:27:40,000 itself it has a resolution equivalent to being able to read a newspaper in paris 224 00:27:40,000 --> 00:27:46,000 while sitting in new york 225 00:27:46,000 --> 00:27:54,000 they call it the event horizon telescope 226 00:27:54,000 --> 00:28:00,000 their goal to capture the first ever image of a black hole 227 00:28:00,000 --> 00:28:13,000 their target the monster at the center of m87 228 00:28:13,000 --> 00:28:18,000 probing deep into m87s luminous core the astronomers struck a delicate 229 00:28:18,000 --> 00:28:23,000 balance between filtering out interstellar dust and finding the outlines 230 00:28:23,000 --> 00:28:32,000 of their quarry at a radio wavelength of about one millimeter all the dust and gas 231 00:28:32,000 --> 00:28:39,000 obscuring the monster faded away leaving this ghostly silhouette 232 00:28:39,000 --> 00:28:51,000 a black hole an object that cannot by its very nature be seen 233 00:28:51,000 --> 00:28:59,000 the event horizon telescope relies on a tool that has transformed the study of the universe 234 00:28:59,000 --> 00:29:05,000 to make sense of the vast amount of data captured by the many receivers researchers developed a series of 235 00:29:05,000 --> 00:29:17,000 computer simulations visualizing the complexity of the scene 236 00:29:17,000 --> 00:29:25,000 here are some of the results the dark nucleus is the event horizon 237 00:29:25,000 --> 00:29:37,000 a shadow left when the object's immense gravity slows all light to a stop 238 00:29:37,000 --> 00:29:44,000 the singularity the black hole itself is hiding in the shadows 239 00:29:44,000 --> 00:29:51,000 the visible ring marks the spinning accretion disk 240 00:29:51,000 --> 00:29:57,000 it's brighter on one side because the gas there is spiraling towards the telescope its 241 00:29:57,000 --> 00:30:03,000 photons piling up the light from material moving away 242 00:30:03,000 --> 00:30:11,000 becomes dimmer as its wavelength stretches toward the red part of the electromagnetic spectrum 243 00:30:11,000 --> 00:30:17,000 from a slightly more distant perspective you can see how a portion of the inflowing matter 244 00:30:17,000 --> 00:30:28,000 is flung out in a fiery pulsating jet 245 00:30:28,000 --> 00:30:33,000 m87 is a black hole of truly cosmic proportions 246 00:30:33,000 --> 00:30:40,000 it has been bulking up for billions of years on a steady diet of gas dust planets 247 00:30:40,000 --> 00:30:46,000 and stars but it's not the only billion solar mass 248 00:30:46,000 --> 00:30:54,000 black hole out there or even the largest 249 00:30:54,000 --> 00:31:00,000 [Music] the coma cluster is a dense grouping of 250 00:31:00,000 --> 00:31:07,000 galaxies 321 million light years from earth 251 00:31:07,000 --> 00:31:16,000 its center is occupied by a colossal elliptical galaxy cataloged as ngc 4889 252 00:31:16,000 --> 00:31:25,000 it harbors a black hole estimated to be 21 billion times the mass of the sun 253 00:31:25,000 --> 00:31:31,000 j2157 is even larger 254 00:31:31,000 --> 00:31:37,000 at 34 billion times the mass of the sun this ultra massive black hole is 8 000 255 00:31:37,000 --> 00:31:44,000 times larger than the one at our milky way's core 256 00:31:44,000 --> 00:31:52,000 the largest black hole yet spotted ton 618 may weigh as much as 66 billion 257 00:31:52,000 --> 00:31:59,000 of our suns it drives a super luminous quasar shining 140 trillion times brighter than 258 00:31:59,000 --> 00:32:05,000 our star [Music] theoretically there is no limit to how 259 00:32:05,000 --> 00:32:23,000 large a black hole can grow all it takes is time and the right circumstances 260 00:32:23,000 --> 00:32:28,000 the building boom of ever larger telescope mirrors has given astronomers a whole new 261 00:32:28,000 --> 00:32:36,000 vantage point on the life cycle of ultramassive black holes 262 00:32:36,000 --> 00:32:44,000 here in the high northern deserts of chile they have been combing the early universe for dim clues of black holes on 263 00:32:44,000 --> 00:32:51,000 the rise out in the southern constellation of leo 264 00:32:51,000 --> 00:32:56,000 they spotted the most distant quasar yet observed just 770 265 00:32:56,000 --> 00:33:07,000 million years after the big bang [Music] 266 00:33:07,000 --> 00:33:13,000 the red dot is light energized by a black hole estimated at two billion times the mass 267 00:33:13,000 --> 00:33:21,000 of the sun how did it form and what impact will it 268 00:33:21,000 --> 00:33:26,000 have on its surroundings 269 00:33:26,000 --> 00:33:36,000 to find out scientists have launched a major international effort to simulate the early evolution of the 270 00:33:36,000 --> 00:33:50,000 universe 271 00:33:50,000 --> 00:33:58,000 the action starts a few million years after the big bang gravity begins to draw hydrogen gas into 272 00:33:58,000 --> 00:34:09,000 large halos and from there into concentrations dense enough for stars to form 273 00:34:09,000 --> 00:34:16,000 as some stars die they give rise to black holes these primordial monsters 274 00:34:16,000 --> 00:34:22,000 feed on in-rushing gas growing ever larger while blasting their 275 00:34:22,000 --> 00:34:29,000 environments with fierce winds and jets [Music] 276 00:34:29,000 --> 00:34:37,000 the scene shifts to visible light as the universe reaches its halfway point two galaxies 277 00:34:37,000 --> 00:34:45,000 are beginning to form each with a central region densely packed with stars 278 00:34:45,000 --> 00:34:51,000 gravity begins to draw the two into a cosmic embrace [Music] 279 00:34:51,000 --> 00:34:58,000 the black holes at their centers will inevitably meet and merge the end result 280 00:34:58,000 --> 00:35:08,000 a galaxy similar to our own with a super massive black hole hidden deep in its core 281 00:35:08,000 --> 00:35:15,000 we now move to a much larger scale the action starts 500 million years 282 00:35:15,000 --> 00:35:21,000 after the big bang matter coalesces in a spider web pattern 283 00:35:21,000 --> 00:35:31,000 of filaments and dense knots 284 00:35:31,000 --> 00:35:41,000 amid the formation of countless stars several larger galaxies develop 285 00:35:41,000 --> 00:35:50,000 as they merge so do the black holes in their cores [Music] 286 00:35:50,000 --> 00:36:04,000 a still larger view tracks the impact these supermassive black holes have on the surrounding universe 287 00:36:04,000 --> 00:36:12,000 you can see bubbles rising quickly from the largest galaxies these are waves of super hot gas pushed 288 00:36:12,000 --> 00:36:26,000 out by winds and jets powered by growing black holes 289 00:36:26,000 --> 00:36:33,000 such outbursts seed the universe with elements generated by large stars and supernovae 290 00:36:33,000 --> 00:36:45,000 elements that would one day come together in stars and planets like our own 291 00:36:45,000 --> 00:36:51,000 [Music] by pushing outward huge volumes of gas 292 00:36:51,000 --> 00:36:58,000 these hot bubbles slow the growth of their host galaxies while promoting the formation of smaller 293 00:36:58,000 --> 00:37:11,000 galaxies like our milky way 294 00:37:11,000 --> 00:37:18,000 [Music] quasars and the black hole jets powering 295 00:37:18,000 --> 00:37:25,000 them are among the most energetic phenomenon known [Music] 296 00:37:25,000 --> 00:37:33,000 this one spotted by the hubble space telescope in the early universe emits light 600 trillion times brighter 297 00:37:33,000 --> 00:37:43,000 than our sun [Music] 298 00:37:43,000 --> 00:37:49,000 and yet that hardly begins to describe the power unleashed when two supermassive black 299 00:37:49,000 --> 00:37:59,000 holes collide 300 00:37:59,000 --> 00:38:07,000 to find out what that will look like from earth scientists have simulated the moment just before two supermassive 301 00:38:07,000 --> 00:38:13,000 black holes merge magnetic and gravitational forces heat 302 00:38:13,000 --> 00:38:19,000 up the gas the pair is enveloped in ultraviolet 303 00:38:19,000 --> 00:38:24,000 light super hot plasma flowing around and into the black holes 304 00:38:24,000 --> 00:38:33,000 glows in x-ray light 305 00:38:33,000 --> 00:38:41,000 [Music] 306 00:38:41,000 --> 00:39:03,000 the intense gravity of the pair distorts and bends space time creating a lens 307 00:39:03,000 --> 00:39:08,000 albert einstein hinted that the energy of such a collision goes far beyond the emission of 308 00:39:08,000 --> 00:39:15,000 high-energy light his equations predicted that when massive bodies like black holes 309 00:39:15,000 --> 00:39:21,000 accelerate or whip around each other they would disturb the normally smooth fabric of space-time 310 00:39:21,000 --> 00:39:26,000 [Music] a series of powerful gravitational waves 311 00:39:26,000 --> 00:39:34,000 would move outward like ripples on a pond 312 00:39:34,000 --> 00:39:42,000 by the time these waves travel the breadth of the universe to reach us their energy will have nearly dissipated 313 00:39:42,000 --> 00:39:51,000 [Music] 314 00:39:51,000 --> 00:39:57,000 and yet scientists believe they have detected them 315 00:39:57,000 --> 00:40:03,000 at the laser interferometry gravitational wave observatory known as ligo they have assembled 316 00:40:03,000 --> 00:40:09,000 precision high-powered lasers and some of the most perfect large-scale 317 00:40:09,000 --> 00:40:17,000 vacuum chambers ever created 318 00:40:17,000 --> 00:40:23,000 the idea is that as a gravitational wave passes it will stretch and squeeze the distance 319 00:40:23,000 --> 00:40:30,000 between mirrors placed at the ends of four kilometer long tubes 320 00:40:30,000 --> 00:40:37,000 this distortion of space-time measured by lasers is incredibly subtle a thousand 321 00:40:37,000 --> 00:40:49,000 times smaller than the nucleus of an atom 322 00:40:49,000 --> 00:40:56,000 this ambitious undertaking decades in the making finally bore fruit in 2015. 323 00:40:56,000 --> 00:41:02,000 the instruments at ligo and its european counterpart each recorded a signal consistent with 324 00:41:02,000 --> 00:41:12,000 the merger of two black holes of 29 and 36 solar masses 325 00:41:12,000 --> 00:41:20,000 [Music] scientists calculate that the collision converted the mass of up to three suns 326 00:41:20,000 --> 00:41:34,000 to pure energy in the form of gravitational waves 327 00:41:34,000 --> 00:41:45,000 ligo's founders would win the nobel prize for physics in 2017 328 00:41:45,000 --> 00:41:53,000 this simulation shows the pattern of gravitational waves that the pair would have emitted in the final moments of the merger and 329 00:41:53,000 --> 00:42:01,000 just after as the object spiral together the energy 330 00:42:01,000 --> 00:42:07,000 carried by each successive wave rises for the briefest of moments to a hundred 331 00:42:07,000 --> 00:42:14,000 billion trillion times the power of our sun [Music] 332 00:42:14,000 --> 00:42:24,000 collisions like this are extremely rare but the universe is very large 333 00:42:24,000 --> 00:42:29,000 as their sensitivity improves ligo and similar instruments will detect more and more such 334 00:42:29,000 --> 00:42:35,000 reverberations in space-time 335 00:42:35,000 --> 00:42:40,000 remarkably even this does not begin to describe the power 336 00:42:40,000 --> 00:42:49,000 held within a black hole 337 00:42:49,000 --> 00:42:57,000 [Music] 338 00:42:57,000 --> 00:43:02,000 imagine a spaceship in the distant future on a rendezvous with a supermassive 339 00:43:02,000 --> 00:43:08,000 black hole [Music] 340 00:43:08,000 --> 00:43:15,000 because of the object's immense size the stretching force is small allowing the ship to survive as it falls 341 00:43:15,000 --> 00:43:29,000 through the event horizon but not for long 342 00:43:29,000 --> 00:43:38,000 as the ship spirals down it hits a wall of energy what scientists describe as the inner 343 00:43:38,000 --> 00:43:44,000 horizon [Music] 344 00:43:44,000 --> 00:43:51,000 at a black hole's event horizon matter accelerates to the speed of light 345 00:43:51,000 --> 00:43:58,000 it is then whipped around so fast that some of it gets flung back out and into a collision with 346 00:43:58,000 --> 00:44:04,000 inflowing matter 347 00:44:04,000 --> 00:44:12,000 at the inner horizon the energy rises so sharply it may well reach nature's limit 348 00:44:12,000 --> 00:44:20,000 equivalent perhaps to the big bang [Applause] 349 00:44:20,000 --> 00:44:34,000 itself [Music] 350 00:44:34,000 --> 00:44:41,000 fortunately for us gravity walls off such extremes behind the event horizon of black holes 351 00:44:41,000 --> 00:44:46,000 [Music] 352 00:44:46,000 --> 00:44:54,000 waiting long enough trillions upon trillions of years to a time when theory says all matter 353 00:44:54,000 --> 00:45:04,000 and energy will likely fall inside black holes 354 00:45:04,000 --> 00:45:11,000 [Music] gravity may well draw the entire 355 00:45:11,000 --> 00:45:21,000 universe inside a single ultimate black hole 356 00:45:21,000 --> 00:45:31,000 some theories suggest that it could erupt 357 00:45:31,000 --> 00:45:36,000 in a flurry of matter and anti-matter 358 00:45:36,000 --> 00:45:42,000 [Music] in gases that cool and coalesce into stars 359 00:45:42,000 --> 00:45:51,000 [Music] explosions that give rise to black holes 360 00:45:51,000 --> 00:46:00,000 [Music] galaxies that envelope and nurture them 361 00:46:00,000 --> 00:46:14,000 while giving birth to solar systems like ours 362 00:46:14,000 --> 00:46:21,000 [Music] and so here we sit on a planet that is 363 00:46:21,000 --> 00:46:31,000 an infinitesimally small by-product of the universe at large 364 00:46:31,000 --> 00:46:36,000 our imaginations though are unbounded 365 00:46:36,000 --> 00:47:00,000 as we contemplate the strange and powerful forces that have shaped all we see 366 00:47:00,000 --> 00:47:30,000 [Music] 367 00:47:30,000 --> 00:47:37,000 [Music] 368 00:47:37,000 --> 00:47:50,000 [Music] 369 00:47:50,000 --> 00:47:59,000 so 370 00:47:59,000 --> 00:48:00,000 you37359

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