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These are the user uploaded subtitles that are being translated: 1 00:00:01,335 --> 00:00:04,837 Narrator: Our milky way is under threat. 2 00:00:04,839 --> 00:00:08,774 Across the universe, galaxies are going dark, 3 00:00:08,776 --> 00:00:12,478 And scientists are trying to find out why. 4 00:00:12,480 --> 00:00:17,616 Something is slowly drawing the curtains closed on the universe. 5 00:00:17,618 --> 00:00:23,022 Narrator: Why are the stars in our galaxy losing their shine? 6 00:00:23,024 --> 00:00:26,125 Will the milky way slowly fade to black? 7 00:00:26,127 --> 00:00:27,960 If our home galaxy is getting dimmer, 8 00:00:27,962 --> 00:00:30,029 What does it mean for us? 9 00:00:30,031 --> 00:00:33,032 Narrator: Astronomers are now racing to unlock the mystery 10 00:00:33,034 --> 00:00:36,502 Of why galaxies are darkening. 11 00:00:36,504 --> 00:00:39,872 Is there a link to massive bubbles of dust and gas, 12 00:00:39,874 --> 00:00:42,508 That shoot out from the center of the milky way? 13 00:00:42,510 --> 00:00:45,711 We have discovered something truly extraordinary. 14 00:00:45,713 --> 00:00:47,980 Can the biggest collisions in the universe 15 00:00:47,982 --> 00:00:51,650 Switch the lights back on? 16 00:00:51,652 --> 00:00:52,951 Oluseyi: We thought galaxy collisions 17 00:00:52,953 --> 00:00:55,154 Would be very violent and destructive, 18 00:00:55,156 --> 00:00:56,722 But what we find is that they're one of 19 00:00:56,724 --> 00:01:00,092 The most creative processes in the universe. 20 00:01:00,094 --> 00:01:02,261 Narrator: Scientists are gathering evidence 21 00:01:02,263 --> 00:01:04,763 For a startling theory... 22 00:01:04,765 --> 00:01:07,232 Of how galaxies are born... 23 00:01:07,234 --> 00:01:10,102 Live... 24 00:01:10,104 --> 00:01:11,737 And die. 25 00:01:11,739 --> 00:01:14,740 -- Captions by vitac -- www.Vitac.Com 26 00:01:14,742 --> 00:01:17,743 Captions paid for by discovery communications 27 00:01:17,745 --> 00:01:24,917 ♪♪ 28 00:01:24,919 --> 00:01:28,454 Our galaxy, the milky way, 29 00:01:28,456 --> 00:01:31,390 Is just one of many hundreds of billions of galaxies 30 00:01:31,392 --> 00:01:33,025 In the universe. 31 00:01:37,298 --> 00:01:39,932 Galaxies are huge, glowing concentrations 32 00:01:39,934 --> 00:01:43,702 Of gas, dust, stars, and planets. 33 00:01:46,140 --> 00:01:48,207 Telescopes capture breathtaking pictures 34 00:01:48,209 --> 00:01:52,044 Of bright, shining galaxies millions of light years away. 35 00:01:55,182 --> 00:01:57,616 Thaller: There are few things that make my jaw drop 36 00:01:57,618 --> 00:01:59,251 Like images of galaxies -- 37 00:01:59,253 --> 00:02:02,488 When you think about how vast they are and just how beautiful 38 00:02:02,490 --> 00:02:04,123 And also just how recent it is 39 00:02:04,125 --> 00:02:07,626 That we understand what these things really are. 40 00:02:07,628 --> 00:02:12,197 The basic component that we see of galaxies are stars, 41 00:02:12,199 --> 00:02:16,401 And that's what keeps these galaxies shining. 42 00:02:16,403 --> 00:02:19,505 The milky way is an enormous disc galaxy, 43 00:02:19,507 --> 00:02:22,474 About 120,000 light years across, 44 00:02:22,476 --> 00:02:25,611 And it has several hundred billion stars in it. 45 00:02:28,549 --> 00:02:34,653 Narrator: In 2015, astronomers make a worrying discovery. 46 00:02:34,655 --> 00:02:37,156 They report that something strange is happening 47 00:02:37,158 --> 00:02:39,992 Across the universe. 48 00:02:39,994 --> 00:02:44,863 Hundreds of thousands of galaxies are getting dimmer. 49 00:02:44,865 --> 00:02:47,199 Some have lost 50 percent of their brightness 50 00:02:47,201 --> 00:02:50,269 Over the past two billion years, 51 00:02:50,271 --> 00:02:53,639 And the milky way is one of them. 52 00:02:53,641 --> 00:02:55,507 Tremblay: This isn't just happening somewhere 53 00:02:55,509 --> 00:02:58,177 In the deep void of space in an unknown galaxy. 54 00:02:58,179 --> 00:02:59,711 This is our home galaxy, 55 00:02:59,713 --> 00:03:04,816 And anything that affects our home galaxy affects us. 56 00:03:04,818 --> 00:03:06,351 Narrator: The way the galaxies recycle 57 00:03:06,353 --> 00:03:08,420 Their precious star-building material 58 00:03:08,422 --> 00:03:10,689 Should keep them shining brightly. 59 00:03:15,296 --> 00:03:19,031 As some stars reach the end of their lives, 60 00:03:19,033 --> 00:03:23,001 They go supernova. 61 00:03:23,003 --> 00:03:24,503 This giant explosion 62 00:03:24,505 --> 00:03:29,274 Catapults a huge wave of gas across the galaxy. 63 00:03:29,276 --> 00:03:34,112 This wave injects new material into interstellar gas clouds 64 00:03:34,114 --> 00:03:39,318 And compresses them to the point where gravity takes hold. 65 00:03:39,320 --> 00:03:42,187 Gravity pulls the material tighter together 66 00:03:42,189 --> 00:03:46,124 And triggers the formation of a new generation of stars. 67 00:03:48,796 --> 00:03:52,631 Over time, this process keeps the milky way bright 68 00:03:52,633 --> 00:03:55,267 As billions of stars burst into life. 69 00:03:55,269 --> 00:04:02,107 ♪♪ 70 00:04:02,109 --> 00:04:04,476 Thaller: To me, one of the most beautiful stories ever told 71 00:04:04,478 --> 00:04:07,713 Is the cycle of star formation. 72 00:04:07,715 --> 00:04:10,916 So in a galaxy, you have these giant clouds of dust and gas 73 00:04:10,918 --> 00:04:13,285 That collapse into massive stars. 74 00:04:13,287 --> 00:04:15,988 Those stars then live their lives and blow up 75 00:04:15,990 --> 00:04:18,557 And distribute their material back into the galaxy 76 00:04:18,559 --> 00:04:21,627 For new stars and new planets to be made of. 77 00:04:21,629 --> 00:04:25,430 So that cycle of star formation is what keeps galaxies bright. 78 00:04:25,432 --> 00:04:30,402 ♪♪ 79 00:04:30,404 --> 00:04:32,971 Narrator: But it appears that something is going wrong 80 00:04:32,973 --> 00:04:37,542 With this galactic circle of life across the universe. 81 00:04:37,544 --> 00:04:41,146 The shocking thing is that our own galaxy could be in decline, 82 00:04:41,148 --> 00:04:44,449 So the lights could go out in our night sky. 83 00:04:44,451 --> 00:04:48,553 Galaxies are huge systems of gas and dust and stars. 84 00:04:48,555 --> 00:04:53,292 So whatever's turning them off must be something major. 85 00:04:53,294 --> 00:04:56,595 Narrator: Why are galaxies losing their shine? 86 00:04:56,597 --> 00:04:59,965 And what does this process, called galactic dimming, 87 00:04:59,967 --> 00:05:03,702 Mean for our own milky way? 88 00:05:03,704 --> 00:05:06,438 Astronomers believe that the heart of our own galaxy 89 00:05:06,440 --> 00:05:09,975 Is a good place to search for answers. 90 00:05:09,977 --> 00:05:11,543 The center of the milky way 91 00:05:11,545 --> 00:05:15,814 Contains the greatest concentration of stars. 92 00:05:15,816 --> 00:05:18,116 Focusing on this area gives scientists 93 00:05:18,118 --> 00:05:21,520 Studying galactic dimming a huge sample size 94 00:05:21,522 --> 00:05:23,422 Compared to smaller clusters of stars 95 00:05:23,424 --> 00:05:26,558 On the edges of the galaxy. 96 00:05:26,560 --> 00:05:27,859 Thaller: If you want to study the history 97 00:05:27,861 --> 00:05:29,728 Of star formation in the milky way, 98 00:05:29,730 --> 00:05:31,897 Why not look towards where there are most stars? 99 00:05:31,899 --> 00:05:34,099 And that's the center of the galaxy. 100 00:05:34,101 --> 00:05:36,768 Narrator: But astronomers face a big problem -- 101 00:05:36,770 --> 00:05:41,039 Seeing clearly this far into space from earth. 102 00:05:41,041 --> 00:05:44,376 Thick clouds of dust and gas lie between us 103 00:05:44,378 --> 00:05:47,245 And the center of the galaxy. 104 00:05:47,247 --> 00:05:52,250 These clouds block the visible light that our eyes see. 105 00:05:52,252 --> 00:05:57,489 Infrared light passes through this dense gas. 106 00:05:57,491 --> 00:06:01,293 Astronomers use special infrared detectors to study objects 107 00:06:01,295 --> 00:06:05,564 That other types of telescopes cannot see. 108 00:06:05,566 --> 00:06:08,333 But the water molecules in earth's atmosphere 109 00:06:08,335 --> 00:06:10,802 Absorb almost all of the infrared light 110 00:06:10,804 --> 00:06:14,773 Before it reaches the planet's surface. 111 00:06:14,775 --> 00:06:17,008 This reduces the level of detail 112 00:06:17,010 --> 00:06:20,078 That the telescopes on the ground see, 113 00:06:20,080 --> 00:06:21,980 Even telescopes on mountaintops 114 00:06:21,982 --> 00:06:25,183 Higher than 16,000 feet above sea level 115 00:06:25,185 --> 00:06:28,420 Struggle for clear view. 116 00:06:28,422 --> 00:06:31,089 To overcome the problem, 117 00:06:31,091 --> 00:06:35,427 Nasa and the german aerospace agency build this -- 118 00:06:35,429 --> 00:06:39,765 The stratospheric observatory for infrared astronomy, 119 00:06:39,767 --> 00:06:42,467 Or sofia for short. 120 00:06:42,469 --> 00:06:45,570 Sofia is a modified boeing 747 121 00:06:45,572 --> 00:06:49,674 That flies in the stratosphere above the clouds 122 00:06:49,676 --> 00:06:52,210 And carries a high-powered telescope. 123 00:06:55,149 --> 00:06:58,316 With its eight-foot mirror and infrared sensor, 124 00:06:58,318 --> 00:07:02,654 The telescope sees past galactic gas and dust 125 00:07:02,656 --> 00:07:08,026 To detect objects far out in space. 126 00:07:08,028 --> 00:07:13,231 Sofia looks through a corridor 650 light years wide, 127 00:07:13,233 --> 00:07:16,568 Right into the super bright center of the milky way. 128 00:07:19,072 --> 00:07:23,041 This has the most star-forming matter in the galaxy, 129 00:07:23,043 --> 00:07:25,544 So sofia's infrared sensors 130 00:07:25,546 --> 00:07:28,580 Can count the number of newly born stars. 131 00:07:31,151 --> 00:07:34,019 The data from sofia, combined with the data 132 00:07:34,021 --> 00:07:37,422 From space telescopes in orbit around the earth, 133 00:07:37,424 --> 00:07:41,092 Builds up a super detailed image of the center of the milky way, 134 00:07:44,231 --> 00:07:47,065 Sofia's observations confirm 135 00:07:47,067 --> 00:07:49,367 That the galactic center contains the largest 136 00:07:49,369 --> 00:07:55,173 And densest concentrations of gas in the galaxy, 137 00:07:55,175 --> 00:07:58,276 These dense gas concentrations should collapse 138 00:07:58,278 --> 00:08:00,879 To make new stars. 139 00:08:00,881 --> 00:08:02,981 The more gas that collapses, 140 00:08:02,983 --> 00:08:07,352 The more stars that a galaxy creates. 141 00:08:07,354 --> 00:08:09,454 But the telescope data shows 142 00:08:09,456 --> 00:08:13,158 That this isn't what is happening in the milky way. 143 00:08:13,160 --> 00:08:15,060 Thaller: As we look into the center of the galaxy, 144 00:08:15,062 --> 00:08:18,463 We see these dense, dark regions that should be forming stars. 145 00:08:18,465 --> 00:08:20,999 But for some reason, they're not. 146 00:08:21,001 --> 00:08:23,902 Something is damping down star formation 147 00:08:23,904 --> 00:08:26,404 In the heart of the milky way. 148 00:08:26,406 --> 00:08:29,875 Narrator: The gasses left over from the death of one generation of stars 149 00:08:29,877 --> 00:08:34,179 Should help give birth to the next generation. 150 00:08:34,181 --> 00:08:37,282 But sofia discovers that many of the giant gas clouds 151 00:08:37,284 --> 00:08:39,050 In the center of the milky way 152 00:08:39,052 --> 00:08:43,255 Are not collapsing into new stars. 153 00:08:43,257 --> 00:08:46,258 Astronomers find that these gas clouds are giving birth 154 00:08:46,260 --> 00:08:49,127 To ten times fewer stars than expected. 155 00:08:52,466 --> 00:08:54,099 Tremblay: Though there are some regions 156 00:08:54,101 --> 00:08:57,402 That are very dense with gas and forming stars very actively, 157 00:08:57,404 --> 00:09:00,405 Some places in our galaxy still host gas, 158 00:09:00,407 --> 00:09:02,841 And yet they're not forming stars at all. 159 00:09:02,843 --> 00:09:05,076 Without the light from these new stars, 160 00:09:05,078 --> 00:09:08,580 The galaxy is losing its brightness. 161 00:09:08,582 --> 00:09:10,682 Oluseyi: Stars are temporary things. 162 00:09:10,684 --> 00:09:12,584 They're born, and they die, 163 00:09:12,586 --> 00:09:15,954 So in order for a galaxy to stay the same brightness, 164 00:09:15,956 --> 00:09:18,857 You need to have a relative equilibrium 165 00:09:18,859 --> 00:09:20,525 With the number of stars being born 166 00:09:20,527 --> 00:09:22,494 And a number of stars dying equaling 167 00:09:22,496 --> 00:09:25,730 So that the lights don't really change. 168 00:09:25,732 --> 00:09:27,132 And we had an image of the milky way 169 00:09:27,134 --> 00:09:29,768 From a few billion years ago, what we notice 170 00:09:29,770 --> 00:09:34,172 Is that the cumulative amount of starlight has dropped. 171 00:09:36,443 --> 00:09:38,577 Narrator: The evidence is clear. 172 00:09:38,579 --> 00:09:40,745 The milky way produces fewer stars 173 00:09:40,747 --> 00:09:43,148 Now than it did in the past, 174 00:09:43,150 --> 00:09:45,250 And that is why it is dimming. 175 00:09:47,788 --> 00:09:51,489 Fewer new stars means that our galaxy is slowly dying. 176 00:09:53,660 --> 00:09:56,461 What is putting the brakes on star formation in galaxies 177 00:09:56,463 --> 00:10:00,031 Like the milky way? 178 00:10:00,033 --> 00:10:01,833 Are mysterious galactic bubbles, 179 00:10:01,835 --> 00:10:05,036 The key to solving what is killing our galaxy. 180 00:10:15,315 --> 00:10:20,051 Narrator: Galaxies across the universe are getting dimmer. 181 00:10:20,053 --> 00:10:22,821 Telescope observations reveal that something 182 00:10:22,823 --> 00:10:26,157 Is preventing the formation of new stars in the milky way. 183 00:10:28,362 --> 00:10:30,862 Thaller: Star formation is a powerful process. 184 00:10:30,864 --> 00:10:34,199 The scales are unbelievable, and yet all over the galaxy, 185 00:10:34,201 --> 00:10:35,700 Things seem to be shutting down. 186 00:10:35,702 --> 00:10:37,068 Did something happen in the past -- 187 00:10:37,070 --> 00:10:39,571 Something huge, some cataclysm 188 00:10:39,573 --> 00:10:41,373 That actually shut off star formation? 189 00:10:41,375 --> 00:10:43,575 And can we find any evidence of this? 190 00:10:45,646 --> 00:10:47,979 Narrator: That evidence could lie in data 191 00:10:47,981 --> 00:10:50,548 From nasa's fermi telescope. 192 00:10:50,550 --> 00:10:55,887 Fermi scans space for super high energy light called gamma rays. 193 00:10:55,889 --> 00:10:58,623 Tremblay: The gamma ray sky is a completely different view 194 00:10:58,625 --> 00:11:00,191 Of the universe. 195 00:11:00,193 --> 00:11:02,060 The fermi telescope is able to witness 196 00:11:02,062 --> 00:11:06,031 The most energetic events that are happening throughout it. 197 00:11:06,033 --> 00:11:10,835 Narrator: The telescope discovers something incredible... 198 00:11:10,837 --> 00:11:13,872 Two super huge bubbles of gamma radiation 199 00:11:13,874 --> 00:11:18,610 Emanating from the center of our galaxy. 200 00:11:18,612 --> 00:11:22,213 The bubbles extend 25,000 light years above 201 00:11:22,215 --> 00:11:26,351 And below the spiral of the milky way. 202 00:11:26,353 --> 00:11:29,554 Plait: The scale of these fermi bubbles is enormous. 203 00:11:29,556 --> 00:11:31,756 They're roughly the radius of the galaxy -- 204 00:11:31,758 --> 00:11:33,992 Half the width of the galaxy. 205 00:11:33,994 --> 00:11:36,428 If you were to go outside and look up in the sky, 206 00:11:36,430 --> 00:11:39,831 They would cover 2/3 of the size of the sky. 207 00:11:42,769 --> 00:11:45,537 Narrator: Only the most violent events in the universe 208 00:11:45,539 --> 00:11:49,140 Have the power to produce gamma rays... 209 00:11:49,142 --> 00:11:52,177 Like supernova explosions... 210 00:11:52,179 --> 00:11:54,245 And neutron star quakes. 211 00:11:56,616 --> 00:11:57,916 Neither is powerful enough 212 00:11:57,918 --> 00:12:00,218 To unleash the amount of gamma radiation 213 00:12:00,220 --> 00:12:03,722 That turns into the fermi bubbles. 214 00:12:03,724 --> 00:12:05,657 So what made them? 215 00:12:08,161 --> 00:12:10,562 Scientists think an invisible monster 216 00:12:10,564 --> 00:12:13,698 At the center of the milky way could be responsible. 217 00:12:16,002 --> 00:12:17,769 At the heart of every galaxy 218 00:12:17,771 --> 00:12:21,639 Lurks a supermassive black hole... 219 00:12:21,641 --> 00:12:25,543 A point in space so dense that nothing can escape its gravity. 220 00:12:27,681 --> 00:12:29,380 Oluseyi: From what we've observed, 221 00:12:29,382 --> 00:12:32,751 Every galaxy has a supermassive black hole at its core, 222 00:12:32,753 --> 00:12:35,820 And there are at least two trillion galaxies 223 00:12:35,822 --> 00:12:37,922 In the observable universe, so this means 224 00:12:37,924 --> 00:12:42,660 There are trillions of supermassive black holes. 225 00:12:42,662 --> 00:12:45,730 Narrator: The supermassive black hole at the center of the milky way 226 00:12:45,732 --> 00:12:49,667 Is called sagittarius a-star. 227 00:12:49,669 --> 00:12:54,105 It weighs the equivalent of four million suns. 228 00:12:54,107 --> 00:12:56,307 This black hole's enormous gravity 229 00:12:56,309 --> 00:12:58,977 Draws in anything that gets too close. 230 00:13:01,848 --> 00:13:05,784 The energy unleashed when this gravity rips apart stray stars 231 00:13:05,786 --> 00:13:11,556 Could unlock the mystery of what makes the fermi bubbles. 232 00:13:11,558 --> 00:13:15,026 Black holes don't eat like a nice, distinguished, 233 00:13:15,028 --> 00:13:16,628 Gentrified person. 234 00:13:16,630 --> 00:13:18,997 You know, they're sloppy. They're like the cookie monster. 235 00:13:18,999 --> 00:13:20,265 When the cookie monster eats cookies, 236 00:13:20,267 --> 00:13:22,233 More comes out than goes into his mouth. 237 00:13:22,235 --> 00:13:25,069 Well, supermassive black holes are just like that. 238 00:13:25,071 --> 00:13:28,807 Stuff is moving incredibly fast, approaching the speed of light, 239 00:13:28,809 --> 00:13:31,276 And the density and pressures are incredible. 240 00:13:31,278 --> 00:13:34,913 And so it's almost as if there are explosions 241 00:13:34,915 --> 00:13:37,081 In this traffic jam of material 242 00:13:37,083 --> 00:13:38,850 Trying to get into the black hole. 243 00:13:38,852 --> 00:13:41,653 And so a lot of material gets shot out 244 00:13:41,655 --> 00:13:45,390 Away from the black hole rather than ending up inside it. 245 00:13:45,392 --> 00:13:49,627 Narrator: The more massive the objects that the black hole consumes, 246 00:13:49,629 --> 00:13:51,362 The higher the densities and pressures 247 00:13:51,364 --> 00:13:54,065 Around the black hole become. 248 00:13:54,067 --> 00:13:55,667 And the greater the amount of energy 249 00:13:55,669 --> 00:13:59,370 That blasts into space as gamma radiation. 250 00:14:02,209 --> 00:14:06,477 Scientists rewind the milky way's galactic clock. 251 00:14:06,479 --> 00:14:09,848 They predict when sagittarius a-star feasts 252 00:14:09,850 --> 00:14:13,051 On a meal large enough to forge the fermi bubbles. 253 00:14:15,488 --> 00:14:19,090 Some scientists estimate that around three million years ago, 254 00:14:19,092 --> 00:14:24,162 Sagittarius a-star draws in a vast amount of matter. 255 00:14:24,164 --> 00:14:30,268 That flattens out into a huge, glowing, spinning disk. 256 00:14:30,270 --> 00:14:34,272 As the black hole devours this matter. 257 00:14:34,274 --> 00:14:38,042 Two immense jets of energy blast out from its poles. 258 00:14:40,881 --> 00:14:43,648 These jets blast gas out of the galaxy 259 00:14:43,650 --> 00:14:46,751 25,000 light years into space. 260 00:14:48,889 --> 00:14:53,157 The jets turn off when the black hole finishes its feast. 261 00:14:53,159 --> 00:14:56,995 All that remains are the fermi bubbles we see today. 262 00:15:01,401 --> 00:15:04,035 Scientists think that multiple events like this one 263 00:15:04,037 --> 00:15:06,037 Throughout the history of the milky way 264 00:15:06,039 --> 00:15:09,574 Could unlock the mystery of, "why are galaxies dimming?" 265 00:15:12,045 --> 00:15:15,713 The reason lies in the huge amount of heat they unleash. 266 00:15:18,652 --> 00:15:22,553 Stars form when huge quantities of gas and dust collapse 267 00:15:22,555 --> 00:15:24,722 Under gravity. 268 00:15:24,724 --> 00:15:27,425 The process triggers a nuclear reaction. 269 00:15:31,564 --> 00:15:33,564 Scientists calculate that this reaction 270 00:15:33,566 --> 00:15:36,100 Happens only when the gas is cold. 271 00:15:38,171 --> 00:15:39,604 Plait: Star formation is a battle 272 00:15:39,606 --> 00:15:41,606 Between these two forces of gravity, 273 00:15:41,608 --> 00:15:43,708 Which is trying to collapse the cloud, 274 00:15:43,710 --> 00:15:46,577 And its own internal heat, which is trying to inflate it. 275 00:15:46,579 --> 00:15:50,081 For gravity to win, for stars to get made, 276 00:15:50,083 --> 00:15:53,084 The gas has to be cool enough that it doesn't stay inflated, 277 00:15:53,086 --> 00:15:55,153 That it's able to collapse. 278 00:15:57,724 --> 00:16:00,792 Narrator: The jets that sagittarius a-star releases 279 00:16:00,794 --> 00:16:03,494 Hurl some of the richest star-building material 280 00:16:03,496 --> 00:16:07,031 Into intergalactic space. 281 00:16:07,033 --> 00:16:11,836 This superheats the gas at the center of the milky way. 282 00:16:11,838 --> 00:16:17,008 The clouds of gas become too hot to collapse into stars. 283 00:16:17,010 --> 00:16:20,578 Oluseyi: All of this heat and power and light and force 284 00:16:20,580 --> 00:16:22,780 Would have stripped out all this material 285 00:16:22,782 --> 00:16:24,449 From the center of the galaxy. 286 00:16:24,451 --> 00:16:28,353 So it just would not have been available to form new stars. 287 00:16:28,355 --> 00:16:30,455 Narrator: A series of events like these 288 00:16:30,457 --> 00:16:33,224 Happening at different times in our galaxy's history 289 00:16:33,226 --> 00:16:34,993 Could put the brakes on star formation 290 00:16:34,995 --> 00:16:37,295 At the heart of the milky way. 291 00:16:41,534 --> 00:16:43,468 Telescopes look millions of light years 292 00:16:43,470 --> 00:16:47,171 Through space at other galaxies. 293 00:16:47,173 --> 00:16:50,441 They discover that the damage sagittarius a-star wreaks 294 00:16:50,443 --> 00:16:52,777 On the milky way throughout its past 295 00:16:52,779 --> 00:16:55,613 Is not unique. 296 00:16:55,615 --> 00:16:57,949 Astronomers observe 2,000 galaxies 297 00:16:57,951 --> 00:17:01,352 That show evidence of huge blast of gamma radiation 298 00:17:01,354 --> 00:17:05,189 Coming from the black holes at their centers. 299 00:17:05,191 --> 00:17:09,894 And the vast majority of these galaxies are now getting dimmer. 300 00:17:09,896 --> 00:17:12,096 Tremblay: We see it in an enormous number of galaxies 301 00:17:12,098 --> 00:17:13,398 Throughout the universe -- 302 00:17:13,400 --> 00:17:16,701 Direct signatures of violent black hole activity 303 00:17:16,703 --> 00:17:18,669 And a depressed star formation rate. 304 00:17:18,671 --> 00:17:22,006 There's definitely a clear connection. 305 00:17:22,008 --> 00:17:26,044 Narrator: But do bursts of radiation from a supermassive black hole 306 00:17:26,046 --> 00:17:29,847 Spell doom for a galaxy indefinitely? 307 00:17:29,849 --> 00:17:33,051 And do mysterious alien stars unlock 308 00:17:33,053 --> 00:17:36,521 How it might be possible to reverse galactic dimming? 309 00:17:47,300 --> 00:17:50,435 Narrator: Jets that blast out from supermassive black holes 310 00:17:50,437 --> 00:17:53,337 Kill star birth at the center of galaxies. 311 00:17:55,508 --> 00:18:00,344 They could explain why our milky way is dimming. 312 00:18:00,346 --> 00:18:04,148 Will the curtains close on our galaxy forever, 313 00:18:04,150 --> 00:18:07,785 Or is there a way it can get a new lease of life? 314 00:18:10,156 --> 00:18:13,991 Scientists believe a clue could lie inside a space rock 315 00:18:13,993 --> 00:18:15,626 That fell to earth. 316 00:18:17,964 --> 00:18:20,765 In 1969, a meteorite lands 317 00:18:20,767 --> 00:18:24,769 Near to the small town of murchison, australia, 318 00:18:24,771 --> 00:18:26,771 One hundred miles north of melbourne. 319 00:18:30,343 --> 00:18:35,913 It shatters into pieces, and locals gather over 100 kilograms 320 00:18:35,915 --> 00:18:38,916 Of the black, smelly meteorite fragments. 321 00:18:42,222 --> 00:18:46,591 In 2019, scientists grind down a sample 322 00:18:46,593 --> 00:18:49,160 To analyze what it is made of. 323 00:18:49,162 --> 00:18:51,295 They get a big surprise. 324 00:18:54,134 --> 00:18:57,935 They find grains of dust from alien stars that died 325 00:18:57,937 --> 00:19:03,407 4.6 billion years ago, before our sun was even born. 326 00:19:05,712 --> 00:19:09,213 These grains of stardust become locked inside space rocks 327 00:19:09,215 --> 00:19:11,582 Through the stars' never ending cycle of birth 328 00:19:11,584 --> 00:19:13,217 And rebirth. 329 00:19:15,822 --> 00:19:19,457 Billions of years ago, an ancient star in the milky way 330 00:19:19,459 --> 00:19:21,225 Reaches the end of its life. 331 00:19:23,329 --> 00:19:27,832 Chemical reactions inside the star makes it grow rapidly. 332 00:19:27,834 --> 00:19:32,170 It transforms into a red giant. 333 00:19:32,172 --> 00:19:36,941 The outer layers of the star shed grains of stardust. 334 00:19:36,943 --> 00:19:39,777 These grains travel light years through space 335 00:19:39,779 --> 00:19:42,880 And merge with the spinning disc of gas and dust 336 00:19:42,882 --> 00:19:47,151 Surrounding newly formed stars. 337 00:19:47,153 --> 00:19:49,921 The stardust from the dead red giant 338 00:19:49,923 --> 00:19:53,991 Combines with the material in the disk to make asteroids. 339 00:19:57,263 --> 00:19:59,697 It is a part of just such an asteroid 340 00:19:59,699 --> 00:20:04,168 That falls on murchison as a meteorite in 1969. 341 00:20:08,474 --> 00:20:12,076 These grains of dead stars might reveal if galactic dimming 342 00:20:12,078 --> 00:20:15,513 Caused by blast of gamma radiation spells doom 343 00:20:15,515 --> 00:20:19,550 For galaxies like the milky way. 344 00:20:19,552 --> 00:20:23,888 Different types of grains come from different dead stars. 345 00:20:23,890 --> 00:20:26,357 Adding up the unique grains tells astronomers 346 00:20:26,359 --> 00:20:28,593 How many stars existed in the milky way 347 00:20:28,595 --> 00:20:30,695 At certain times in the past. 348 00:20:33,099 --> 00:20:36,601 These little pieces of stardust inside this meteorite tell us 349 00:20:36,603 --> 00:20:39,971 The story of what was happening in our galaxy 350 00:20:39,973 --> 00:20:42,139 Before our sun even formed. 351 00:20:42,141 --> 00:20:44,642 They're little tracers. 352 00:20:44,644 --> 00:20:48,379 Narrator: The stars that eject the grains found in the murchison meteorite 353 00:20:48,381 --> 00:20:52,917 Lived for between two to 2.5 billion years. 354 00:20:52,919 --> 00:20:55,786 So it is possible for scientists to calculate 355 00:20:55,788 --> 00:20:59,557 When these ancient stars were born. 356 00:20:59,559 --> 00:21:03,160 By knowing that these grains came from dying stars, 357 00:21:03,162 --> 00:21:05,863 We can actually trace backwards in time 358 00:21:05,865 --> 00:21:11,435 To when those dying stars were actually first forming. 359 00:21:11,437 --> 00:21:13,504 Narrator: Scientists discover that these grains 360 00:21:13,506 --> 00:21:17,675 Come from different stars from all over the galaxy, 361 00:21:17,677 --> 00:21:21,779 But they share one thing in common. 362 00:21:21,781 --> 00:21:26,183 They are all born seven billion years ago. 363 00:21:26,185 --> 00:21:29,053 Calculations reveal that the rate of star birth 364 00:21:29,055 --> 00:21:33,758 In the milky way at that time is double the average. 365 00:21:33,760 --> 00:21:35,926 Tremblay: This was a beautiful and exciting result. 366 00:21:35,928 --> 00:21:37,995 It showed that the milky way experienced 367 00:21:37,997 --> 00:21:39,563 What might have been a sudden 368 00:21:39,565 --> 00:21:41,532 And unexpected burst of star formation 369 00:21:41,534 --> 00:21:43,434 About seven billion years ago, 370 00:21:43,436 --> 00:21:45,269 And this might not have been a localized event. 371 00:21:45,271 --> 00:21:48,239 It might have been galaxy wide. 372 00:21:48,241 --> 00:21:53,411 Narrator: These grains show that galactic dimming is not inevitable. 373 00:21:53,413 --> 00:21:55,212 Galaxies like the milky way 374 00:21:55,214 --> 00:21:59,817 Experience periods of intense star building. 375 00:21:59,819 --> 00:22:03,020 These events, counter galactic dimming. 376 00:22:03,022 --> 00:22:06,924 They make galaxies much brighter. 377 00:22:06,926 --> 00:22:09,327 Thaller: A galaxy is such a rich and complex thing, 378 00:22:09,329 --> 00:22:12,129 It turns out that its life cycle is not very simple. 379 00:22:12,131 --> 00:22:15,266 They grow, they change, they evolve, 380 00:22:15,268 --> 00:22:20,071 And in fact, their story may not be so doomed after all. 381 00:22:20,073 --> 00:22:22,773 Narrator: What triggers these sudden bursts of star creation 382 00:22:22,775 --> 00:22:25,009 Within galaxies like the milky way? 383 00:22:25,011 --> 00:22:30,448 ♪♪ 384 00:22:30,450 --> 00:22:33,751 A clue lies in the findings from an observatory 385 00:22:33,753 --> 00:22:35,386 In new mexico. 386 00:22:37,357 --> 00:22:42,326 This is the sloan 100-inch telescope. 387 00:22:42,328 --> 00:22:45,529 Sloan's apogee project studies hundreds of stars 388 00:22:45,531 --> 00:22:47,732 In the milky way simultaneously 389 00:22:47,734 --> 00:22:50,801 During a single observation session. 390 00:22:50,803 --> 00:22:53,838 One of the most powerful things that we can do as astronomers 391 00:22:53,840 --> 00:22:55,673 Is take a survey of the night sky, 392 00:22:55,675 --> 00:22:59,043 Of looking at huge chunks of the sky at the same time, 393 00:22:59,045 --> 00:23:03,681 And mapping out all of the stars there. 394 00:23:03,683 --> 00:23:06,083 Narrator: The light from a star reveals information 395 00:23:06,085 --> 00:23:09,253 About the chemicals it contains. 396 00:23:09,255 --> 00:23:11,455 Apogee analyzes this starlight 397 00:23:11,457 --> 00:23:16,694 To unlock the precise chemical makeup of thousands of stars. 398 00:23:16,696 --> 00:23:19,330 So you take the light that any particular star emits, 399 00:23:19,332 --> 00:23:22,666 You break it up into a rainbow, and you can see the fingerprints 400 00:23:22,668 --> 00:23:25,202 Of all the different chemicals in there, the ratios of them, 401 00:23:25,204 --> 00:23:27,938 How much there is of one thing versus another. 402 00:23:27,940 --> 00:23:32,676 Every single chemical has its own rainbow fingerprint. 403 00:23:32,678 --> 00:23:35,746 Narrator: The results from sloan's apogee project reveal 404 00:23:35,748 --> 00:23:38,149 That there's something very strange about the chemicals 405 00:23:38,151 --> 00:23:40,718 Inside some of the stars in the milky way. 406 00:23:42,755 --> 00:23:47,291 Stars contain 98 percent hydrogen and helium. 407 00:23:47,293 --> 00:23:51,896 And traces of other elements like iron, magnesium, or carbon. 408 00:23:55,668 --> 00:24:00,971 Apogee analyzes the light from over 600,000 stars 409 00:24:00,973 --> 00:24:04,241 To decode the chemical signature of each one. 410 00:24:07,413 --> 00:24:11,015 It finds that nearly all stars in our galaxy, 411 00:24:11,017 --> 00:24:13,317 Regardless of their size or color, 412 00:24:13,319 --> 00:24:15,319 Share a common signature. 413 00:24:18,958 --> 00:24:24,528 But every now and again, apogee finds a rogue star... 414 00:24:24,530 --> 00:24:27,498 With a different signature. 415 00:24:27,500 --> 00:24:31,068 How is this possible? 416 00:24:31,070 --> 00:24:33,838 Astronomers studying these odd stars out 417 00:24:33,840 --> 00:24:36,540 Come to an astonishing conclusion. 418 00:24:36,542 --> 00:24:38,843 Oluseyi: Their ratios don't match 419 00:24:38,845 --> 00:24:40,878 Everything else in the milky way. 420 00:24:40,880 --> 00:24:44,415 By identifying stars that have a different chemical signature 421 00:24:44,417 --> 00:24:46,317 Than other stars in the milky way, 422 00:24:46,319 --> 00:24:48,853 The implication is clear -- 423 00:24:48,855 --> 00:24:54,058 These stars did not originate in the milky way galaxy. 424 00:24:54,060 --> 00:24:57,194 Narrator: If these stars weren't born in the milky way, 425 00:24:57,196 --> 00:25:00,498 Then where do they come from? 426 00:25:00,500 --> 00:25:04,969 And do they unlock how to reverse galactic dimming? 427 00:25:14,881 --> 00:25:17,147 Narrator: Astronomers discover that our milky way 428 00:25:17,149 --> 00:25:19,416 Contains mysterious alien stars 429 00:25:19,418 --> 00:25:21,652 That were not born in our galaxy. 430 00:25:24,490 --> 00:25:27,625 So where do they come from? 431 00:25:27,627 --> 00:25:31,228 And what is their connection to galactic dimming? 432 00:25:34,534 --> 00:25:40,137 The european space agency's gaia telescope finds a clue. 433 00:25:40,139 --> 00:25:43,173 The telescope maps the motion of over a billion stars 434 00:25:43,175 --> 00:25:46,043 In the milky way. 435 00:25:46,045 --> 00:25:49,980 It discovers that these odd stars out all travel 436 00:25:49,982 --> 00:25:51,482 On different orbits to stars 437 00:25:51,484 --> 00:25:56,387 That share the typical chemical profiles for the milky way. 438 00:25:56,389 --> 00:25:58,355 They circle the galactic center 439 00:25:58,357 --> 00:26:01,559 In the opposite direction to other stars 440 00:26:01,561 --> 00:26:06,230 And move on elongated oval-shaped orbits. 441 00:26:06,232 --> 00:26:11,135 The results from gaia lead to a startling conclusion. 442 00:26:11,137 --> 00:26:16,440 These alien stars come from a different galaxy. 443 00:26:16,442 --> 00:26:20,177 But how can a star jump between galaxies? 444 00:26:23,983 --> 00:26:28,919 A clue lies 250 million light years from earth. 445 00:26:28,921 --> 00:26:32,957 This is a galaxy named arp 220. 446 00:26:32,959 --> 00:26:35,960 It has one of the strangest shapes of any known galaxy 447 00:26:35,962 --> 00:26:38,963 In the visible universe. 448 00:26:38,965 --> 00:26:42,666 Arp 220 does not look like a regular calm, beautiful, 449 00:26:42,668 --> 00:26:45,269 Majestic spiral galaxy like the milky way. 450 00:26:45,271 --> 00:26:50,074 It is this train wreck blob. It's an absolute mess. 451 00:26:50,076 --> 00:26:55,446 Narrator: Why does arp 220 look so different to other galaxies? 452 00:26:55,448 --> 00:26:59,717 The answer is arp 220 isn't a single galaxy. 453 00:27:01,921 --> 00:27:04,221 Oluseyi: The bent shape of arp 220 454 00:27:04,223 --> 00:27:06,824 Isn't just because of aesthetic reasons. 455 00:27:06,826 --> 00:27:09,860 It tells us something about the galaxy's history. 456 00:27:09,862 --> 00:27:16,266 It appears to be the result of a merger between two galaxies. 457 00:27:16,268 --> 00:27:19,470 Narrator: The merger of two galaxies after a collision 458 00:27:19,472 --> 00:27:25,175 Explains how alien stars can jump from one galaxy to another. 459 00:27:25,177 --> 00:27:28,712 The discovery of odd stars out in the milky way 460 00:27:28,714 --> 00:27:30,748 Is evidence that our galaxy, too, 461 00:27:30,750 --> 00:27:34,451 Is involved in a collision billions of years ago. 462 00:27:34,453 --> 00:27:36,687 Now we understand that galactic collisions 463 00:27:36,689 --> 00:27:39,923 Are responsible for these odd stars in the sky. 464 00:27:39,925 --> 00:27:42,593 They didn't come from the milky way galaxy. 465 00:27:42,595 --> 00:27:43,961 So it's an amazing thing to think 466 00:27:43,963 --> 00:27:45,496 That when you look up in the sky, 467 00:27:45,498 --> 00:27:48,432 Some of even the nearest stars may have began their lives 468 00:27:48,434 --> 00:27:50,534 In an entirely different galaxy. 469 00:27:53,139 --> 00:27:55,739 Narrator: Astronomers believe that these galactic mergers 470 00:27:55,741 --> 00:27:58,876 Unlock what triggers intense periods of star birth 471 00:27:58,878 --> 00:28:01,178 In galaxies like our own. 472 00:28:03,549 --> 00:28:07,584 The clue is that merged galaxies like arp 220 473 00:28:07,586 --> 00:28:12,589 Are some of the most brilliant objects in the universe. 474 00:28:12,591 --> 00:28:14,158 There are some galaxies in the universe 475 00:28:14,160 --> 00:28:16,694 That are putting on a spectacular show. 476 00:28:16,696 --> 00:28:18,162 They're incredibly bright. 477 00:28:18,164 --> 00:28:23,233 Their name says it all -- ultra luminous starburst galaxies. 478 00:28:23,235 --> 00:28:26,136 Narrator: The brightness of a galaxy like arp 220 479 00:28:26,138 --> 00:28:27,971 Is a telltale sign 480 00:28:27,973 --> 00:28:32,910 That it is producing huge numbers of new stars. 481 00:28:32,912 --> 00:28:35,713 The raw ingredients for this starburst 482 00:28:35,715 --> 00:28:37,581 Are the vast clouds of gas 483 00:28:37,583 --> 00:28:40,417 That wrap themselves around every galaxy. 484 00:28:44,256 --> 00:28:45,989 Oluseyi: When two things merge together, 485 00:28:45,991 --> 00:28:48,759 There's a lot of reproduction of stars. 486 00:28:48,761 --> 00:28:51,495 New stars are being born. 487 00:28:51,497 --> 00:28:55,432 Just like we had a baby boom, we have a star boom. 488 00:28:57,703 --> 00:29:00,671 Narrator: 700 million years ago. 489 00:29:00,673 --> 00:29:04,842 Two enormous spiral galaxies are on a collision course. 490 00:29:07,079 --> 00:29:10,114 Stripping away their stars and planets 491 00:29:10,116 --> 00:29:14,618 Reveals what happens when they collide. 492 00:29:14,620 --> 00:29:20,858 The galactic gas and dust compress in the collision. 493 00:29:20,860 --> 00:29:25,596 This triggers the formation of billions of stars. 494 00:29:25,598 --> 00:29:30,134 Over millions of years and multiple collisions, 495 00:29:30,136 --> 00:29:33,437 The two galaxies merge into a new galaxy 496 00:29:33,439 --> 00:29:35,272 That is incredibly bright -- 497 00:29:35,274 --> 00:29:37,441 Arp 220. 498 00:29:40,179 --> 00:29:41,912 So a galaxy collision sounds 499 00:29:41,914 --> 00:29:43,814 Like a really violent event, right? 500 00:29:43,816 --> 00:29:47,117 But in fact, it can seed new life. 501 00:29:47,119 --> 00:29:49,720 Gas is the fuel from which all stars are born. 502 00:29:49,722 --> 00:29:53,323 So when you introduce new gas to emerging galaxy, 503 00:29:53,325 --> 00:29:55,626 You can form a new generation of stars. 504 00:29:59,532 --> 00:30:04,735 Narrator: Observations reveal arp 220's origin is not unique. 505 00:30:04,737 --> 00:30:07,271 Astronomers believe up to 80 percent 506 00:30:07,273 --> 00:30:09,940 Of ultra luminous starburst galaxies 507 00:30:09,942 --> 00:30:12,376 Are the result of galactic collisions. 508 00:30:14,513 --> 00:30:17,714 Could a cosmic merger be responsible for the epic periods 509 00:30:17,716 --> 00:30:22,719 Of intense star building and the milky way's past? 510 00:30:22,721 --> 00:30:24,354 And when will the milky way's 511 00:30:24,356 --> 00:30:27,491 Next galactic mega collision take place? 512 00:30:27,493 --> 00:30:33,964 ♪♪ 513 00:30:35,601 --> 00:30:40,404 ♪♪ 514 00:30:40,406 --> 00:30:43,240 Narrator: Scientists are on a mission to discover 515 00:30:43,242 --> 00:30:46,710 How galaxies can reverse the effects of galactic dimming. 516 00:30:49,582 --> 00:30:52,716 The brightest galaxies in the universe reveal 517 00:30:52,718 --> 00:30:58,255 That the galactic collisions breathe new life into a galaxy. 518 00:30:58,257 --> 00:31:01,892 So when was the milky way's last major collision? 519 00:31:05,965 --> 00:31:08,498 Astronomers plot the positions and movements 520 00:31:08,500 --> 00:31:13,136 Of both the old and new stars in our galaxy. 521 00:31:13,138 --> 00:31:16,940 They use this data to rewind time 522 00:31:16,942 --> 00:31:18,742 And reveal the event that triggers 523 00:31:18,744 --> 00:31:21,311 One of the greatest-ever periods of star building 524 00:31:21,313 --> 00:31:22,846 In the milky way. 525 00:31:25,251 --> 00:31:29,052 Around 10 billion years ago, the milky way collides 526 00:31:29,054 --> 00:31:34,658 With a smaller, ancient galaxy called gaia-enceladus. 527 00:31:34,660 --> 00:31:39,363 The impact compresses together huge clouds of gas. 528 00:31:39,365 --> 00:31:43,767 This gas collapses to make thousands of brand-new stars. 529 00:31:43,769 --> 00:31:47,671 The milky way brightens as more and more stars form. 530 00:31:47,673 --> 00:31:50,841 The past collision of the milky way with gaia-enceladus 531 00:31:50,843 --> 00:31:53,777 Might have introduced an enormous new reservoir of gas 532 00:31:53,779 --> 00:31:56,480 Into our home galaxy, and that gas could have gone 533 00:31:56,482 --> 00:31:59,783 Into forming a new generation of stars. 534 00:31:59,785 --> 00:32:01,385 Thaller: When you think galaxy collision, 535 00:32:01,387 --> 00:32:03,186 It sounds like something destructive. 536 00:32:03,188 --> 00:32:05,489 But in fact, when one galaxy collides with another, 537 00:32:05,491 --> 00:32:07,257 That's a harbinger of the creation 538 00:32:07,259 --> 00:32:10,227 Of a brand-new generation of stars. 539 00:32:10,229 --> 00:32:12,629 Our own sun may have formed when a small galaxy 540 00:32:12,631 --> 00:32:15,032 Collided with the milky way billions of years ago. 541 00:32:15,034 --> 00:32:19,536 It's an act of violent creation. 542 00:32:19,538 --> 00:32:22,439 Narrator: A mega collision 10 billion years ago 543 00:32:22,441 --> 00:32:26,243 Reversed the milky way's galactic dimming. 544 00:32:26,245 --> 00:32:27,678 Where else has the gas needed 545 00:32:27,680 --> 00:32:30,614 To make new stars come from since then? 546 00:32:34,620 --> 00:32:39,556 In 2020, astronomers using data from the gaia space probe 547 00:32:39,558 --> 00:32:41,191 Uncover a clue. 548 00:32:43,495 --> 00:32:47,531 Gaia spots a cluster of a few thousand bright young blue stars 549 00:32:47,533 --> 00:32:50,267 In an ancient outer region of the milky way. 550 00:32:53,105 --> 00:32:55,205 These stars burst into life 551 00:32:55,207 --> 00:32:58,008 Along a stream of fresh hydrogen gas. 552 00:33:00,946 --> 00:33:06,016 Gaia follows the gas trail into intergalactic space 553 00:33:06,018 --> 00:33:10,620 To a cluster of stars outside the milky way. 554 00:33:10,622 --> 00:33:13,323 Our galaxy is not alone in space, 555 00:33:13,325 --> 00:33:18,128 The milky way is surrounded by dozens of smaller galaxies. 556 00:33:18,130 --> 00:33:19,463 And where we have maybe a hundred 557 00:33:19,465 --> 00:33:21,365 Or a few hundred billion stars, 558 00:33:21,367 --> 00:33:24,468 These galaxies only have about a billion. 559 00:33:24,470 --> 00:33:26,370 It's like we're a whale in the ocean 560 00:33:26,372 --> 00:33:29,006 Surrounded by a school of little fish. 561 00:33:32,911 --> 00:33:35,078 Narrator: The new star-building gas 562 00:33:35,080 --> 00:33:37,848 Comes from the largest of these dwarf galaxies, 563 00:33:37,850 --> 00:33:41,318 Called the large magellanic cloud. 564 00:33:41,320 --> 00:33:44,087 The huge gravity of the larger milky way 565 00:33:44,089 --> 00:33:47,758 Continually strips gas from the smaller dwarf galaxy. 566 00:33:50,696 --> 00:33:55,632 The new gas collides with the outer regions of our galaxy. 567 00:33:55,634 --> 00:33:59,436 Thousands of bright, young blue stars burst into light. 568 00:34:01,907 --> 00:34:04,174 Astronomers estimate that the milky way 569 00:34:04,176 --> 00:34:06,043 Will completely tear apart the cloud 570 00:34:06,045 --> 00:34:08,912 Within the next two and a half billion years. 571 00:34:08,914 --> 00:34:16,586 ♪♪ 572 00:34:16,588 --> 00:34:19,790 Dwarf galaxies like the large magellanic cloud 573 00:34:19,792 --> 00:34:23,760 Keep the milky way topped with star-building gas. 574 00:34:23,762 --> 00:34:25,595 Oluseyi: The milky way isn't isolated. 575 00:34:25,597 --> 00:34:26,963 It has a lot of neighbors, 576 00:34:26,965 --> 00:34:29,366 And it's stealing gas from some of them. 577 00:34:29,368 --> 00:34:30,667 It's ripping them apart 578 00:34:30,669 --> 00:34:33,603 And incorporating that material into itself. 579 00:34:33,605 --> 00:34:37,974 And that's the material that may form new stars of the future. 580 00:34:37,976 --> 00:34:40,310 The milky way is literally sucking the gas 581 00:34:40,312 --> 00:34:44,347 Off of its neighbors to keep itself alive. 582 00:34:44,349 --> 00:34:46,416 Narrator: Astronomers think that there is enough gas 583 00:34:46,418 --> 00:34:48,218 In these satellite galaxies 584 00:34:48,220 --> 00:34:53,290 To keep the milky way fed for a few billion years. 585 00:34:53,292 --> 00:34:56,560 But where will the critical supplies of gas come from 586 00:34:56,562 --> 00:35:00,564 Once these smaller galaxies are exhausted? 587 00:35:00,566 --> 00:35:02,499 Thaller: We want to know what's going to happen to us, 588 00:35:02,501 --> 00:35:05,001 To our star, in the very distant future, 589 00:35:05,003 --> 00:35:06,736 And knowing the future of the milky way 590 00:35:06,738 --> 00:35:09,873 Will help us understand what's gonna happen to our home. 591 00:35:12,544 --> 00:35:14,911 Narrator: Astronomers scan the cosmos to identify 592 00:35:14,913 --> 00:35:19,683 Where the milky way's next meal will come from. 593 00:35:19,685 --> 00:35:22,419 They discover that it is our own galaxy 594 00:35:22,421 --> 00:35:25,989 That might be next on the menu. 595 00:35:25,991 --> 00:35:28,058 The milky way has fed off the gas 596 00:35:28,060 --> 00:35:33,563 From around 50 smaller satellite galaxies for billions of years, 597 00:35:33,565 --> 00:35:36,266 But it might be about to meet its match. 598 00:35:38,871 --> 00:35:42,439 Nearby on a cosmic scale is andromeda 599 00:35:42,441 --> 00:35:45,442 And its satellite galaxies. 600 00:35:45,444 --> 00:35:48,612 Andromeda has over 800 billion stars, 601 00:35:48,614 --> 00:35:52,816 More than double the number in the milky way. 602 00:35:52,818 --> 00:35:56,620 This juggernaut is hurtling towards us. 603 00:35:56,622 --> 00:35:59,789 The stage is set for a mighty cosmic showdown. 604 00:36:02,761 --> 00:36:06,229 When will this clash of the galactic titans happen? 605 00:36:08,333 --> 00:36:11,067 And what will it do to the milky way? 606 00:36:11,069 --> 00:36:16,072 ♪♪ 607 00:36:17,576 --> 00:36:22,646 ♪♪ 608 00:36:22,648 --> 00:36:24,948 Narrator: Astronomers believe the milky way is destined 609 00:36:24,950 --> 00:36:27,984 To collide with our galactic neighbor, andromeda. 610 00:36:31,156 --> 00:36:34,758 They race to discover when this mighty cosmic faceoff 611 00:36:34,760 --> 00:36:36,393 Will take place. 612 00:36:38,564 --> 00:36:39,963 Tremblay: The milky way and andromeda 613 00:36:39,965 --> 00:36:42,599 Are two of the most massive galaxies in our local group, 614 00:36:42,601 --> 00:36:44,668 And we know that they're moving toward one another 615 00:36:44,670 --> 00:36:46,136 And will eventually collide. 616 00:36:46,138 --> 00:36:48,071 So what we want to discover now 617 00:36:48,073 --> 00:36:49,873 Is whether they're on a direct collision course 618 00:36:49,875 --> 00:36:51,608 And they're headed right for one another 619 00:36:51,610 --> 00:36:53,043 Or whether they're gonna continue to dance 620 00:36:53,045 --> 00:36:56,813 Around each other for several billion more years. 621 00:36:56,815 --> 00:37:00,050 Tremblay: Telescopes from around the world scan andromeda 622 00:37:00,052 --> 00:37:04,554 To unlock its speed and trajectory. 623 00:37:04,556 --> 00:37:07,090 They discover that andromeda and the milky way 624 00:37:07,092 --> 00:37:09,092 Will smash into one another 625 00:37:09,094 --> 00:37:11,795 Within the next five billion years. 626 00:37:14,733 --> 00:37:17,801 The result will be a period of star creation 627 00:37:17,803 --> 00:37:21,871 Unmatched in the history of our galaxy. 628 00:37:21,873 --> 00:37:23,940 Oluseyi: We now have the most accurate prediction 629 00:37:23,942 --> 00:37:25,709 Of when this collision is gonna take place, 630 00:37:25,711 --> 00:37:29,179 And when it does, it's gonna set the skies alight 631 00:37:29,181 --> 00:37:32,382 Because there's gonna be a huge burst of star formation. 632 00:37:36,355 --> 00:37:39,322 Narrator: The massive sizes of the milky way and andromeda 633 00:37:39,324 --> 00:37:42,525 Give them huge gravity. 634 00:37:42,527 --> 00:37:44,828 The two galaxies speed towards each other 635 00:37:44,830 --> 00:37:49,699 At over 250,000 miles per hour. 636 00:37:49,701 --> 00:37:54,704 Their gas reserves smash together when they meet. 637 00:37:54,706 --> 00:37:58,308 This triggers a super intense period of star creation. 638 00:38:01,780 --> 00:38:04,848 Billions of new stars burst into life. 639 00:38:07,653 --> 00:38:12,355 The spiral arms of the milky way and andromeda tangle together. 640 00:38:12,357 --> 00:38:18,928 They eventually form a giant super galaxy called milkomeda. 641 00:38:18,930 --> 00:38:21,031 What a sight that will be. 642 00:38:21,033 --> 00:38:22,866 I mean, it's beautiful enough going out now 643 00:38:22,868 --> 00:38:24,834 And seeing our galaxy as it is, 644 00:38:24,836 --> 00:38:28,705 But we're adding a whole other galaxy to our own. 645 00:38:28,707 --> 00:38:31,408 There will be more stars, more gas out there, 646 00:38:31,410 --> 00:38:35,312 More things to see, more structures in the sky. 647 00:38:35,314 --> 00:38:37,747 It will be fantastic. 648 00:38:41,453 --> 00:38:43,920 Narrator: Today, a drop off in star formation 649 00:38:43,922 --> 00:38:45,622 At the center of the milky way 650 00:38:45,624 --> 00:38:48,358 Means our galaxy is losing its shine. 651 00:38:50,962 --> 00:38:52,696 The creation of milkomeda 652 00:38:52,698 --> 00:38:56,833 Will throw this galactic dimming into reverse. 653 00:38:56,835 --> 00:39:00,036 This new galaxy will make billions of bright, new stars 654 00:39:00,038 --> 00:39:04,708 In the space of a few hundred million years. 655 00:39:04,710 --> 00:39:07,410 But scientists believe that our galaxy will then move 656 00:39:07,412 --> 00:39:13,149 Into the final stage of its life after this dramatic merger. 657 00:39:13,151 --> 00:39:15,485 The light from a billion new stars 658 00:39:15,487 --> 00:39:17,587 Bursting into life so quickly 659 00:39:17,589 --> 00:39:21,558 Blasts away surplus gas. 660 00:39:21,560 --> 00:39:26,162 This prevents the birth of new stars in the future. 661 00:39:26,164 --> 00:39:28,732 Oluseyi: The formation of bright stars 662 00:39:28,734 --> 00:39:30,767 Is gonna drive out gas and dust, 663 00:39:30,769 --> 00:39:33,737 And then when the big stars start exploding, 664 00:39:33,739 --> 00:39:35,905 That's gonna drive out even more. 665 00:39:35,907 --> 00:39:40,043 So this birth may just lead to the end of star formation 666 00:39:40,045 --> 00:39:41,845 In the galaxy. 667 00:39:41,847 --> 00:39:45,081 Tremblay: We think of galaxies as these immortal structures, 668 00:39:45,083 --> 00:39:48,918 These vast swirling voids of hundreds of billions of stars 669 00:39:48,920 --> 00:39:52,088 That live for all of time, but in fact, it's not true. 670 00:39:52,090 --> 00:39:56,659 Galaxies change and evolve and eventually die. 671 00:39:56,661 --> 00:39:59,529 Narrator: Milkomeda will inhabit a sparsely populated part 672 00:39:59,531 --> 00:40:02,399 Of the universe. 673 00:40:02,401 --> 00:40:05,635 There will be no nearby galaxies to feed from 674 00:40:05,637 --> 00:40:09,806 To rejuvenate the lost gas supply. 675 00:40:09,808 --> 00:40:11,941 Oluseyi: Once the milky way and andromeda merge 676 00:40:11,943 --> 00:40:13,676 And form a new, larger galaxy, 677 00:40:13,678 --> 00:40:16,379 It has this huge burst of star formation. 678 00:40:16,381 --> 00:40:19,716 After that, things are gonna go a lot quieter 679 00:40:19,718 --> 00:40:22,852 Because we're relatively isolated right now. 680 00:40:22,854 --> 00:40:24,487 It's just the two of us. 681 00:40:26,591 --> 00:40:29,993 Narrator: Milkomeda is condemned to terminal decline 682 00:40:29,995 --> 00:40:32,595 And extinction. 683 00:40:32,597 --> 00:40:34,798 After the giant galactic fireworks show 684 00:40:34,800 --> 00:40:37,400 That will be the collision of the milky way and andromeda, 685 00:40:37,402 --> 00:40:39,302 We're live in this simmering ember 686 00:40:39,304 --> 00:40:42,672 That will continue to cool off for billions of years more. 687 00:40:42,674 --> 00:40:45,775 Ultimately, our existence as a civilization is nothing 688 00:40:45,777 --> 00:40:48,445 But a sentence in the book of the universe. 689 00:40:51,249 --> 00:40:55,285 Narrator: Astronomers are now unlocking the life story of our milky way. 690 00:40:58,857 --> 00:41:00,123 Mega bubbles of gas 691 00:41:00,125 --> 00:41:03,993 Reveal how supermassive black holes generate heat 692 00:41:03,995 --> 00:41:07,797 That stops star birth and makes galaxies grow dim. 693 00:41:10,836 --> 00:41:14,204 Weird alien stars show how galactic collisions 694 00:41:14,206 --> 00:41:17,774 Rejuvenate galaxies and make them grow bright again. 695 00:41:20,312 --> 00:41:24,881 Today, the milky way is passing through a phase of dimming. 696 00:41:24,883 --> 00:41:30,119 But the light show we see from earth is still spectacular. 697 00:41:30,121 --> 00:41:32,222 Thaller: I want you to realize that we live 698 00:41:32,224 --> 00:41:34,991 In this tremendously fortunate time. 699 00:41:34,993 --> 00:41:37,594 Go outside and look at the stars. 700 00:41:37,596 --> 00:41:39,762 Feel this joy seep through you. 701 00:41:39,764 --> 00:41:42,565 You are standing in this wondrous moment. 702 00:41:42,567 --> 00:41:44,667 Enjoy it and celebrate it. 703 00:41:46,705 --> 00:41:50,006 Narrator: The milky way will enter a new stage of its evolution 704 00:41:50,008 --> 00:41:53,309 And five billion years' time -- 705 00:41:53,311 --> 00:41:56,613 One final cosmic blowout. 706 00:41:56,615 --> 00:42:01,551 Before it slowly fades away into the darkness. 64624

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