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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:03,000 --> 00:00:05,800 Our universe is at war. 2 00:00:05,880 --> 00:00:10,000 The universe is a very violent and deadly place. 3 00:00:11,040 --> 00:00:13,680 Entire galaxies fight to the death. 4 00:00:13,760 --> 00:00:16,200 Talk about clash of the titans. 5 00:00:16,280 --> 00:00:18,360 It doesn't get more titanic than this. 6 00:00:18,440 --> 00:00:21,320 It's a slaughter. It's a massacre. 7 00:00:21,400 --> 00:00:23,560 Only the strongest survive. 8 00:00:23,640 --> 00:00:27,800 If a galaxy wants to stay alive, it has to feed on other galaxies. 9 00:00:29,280 --> 00:00:32,080 Our own galaxy also fights for survival. 10 00:00:33,120 --> 00:00:36,600 We are facing the ultimate destruction 11 00:00:36,680 --> 00:00:38,560 of the Milky Way galaxy. 12 00:00:39,600 --> 00:00:44,760 These battles are how galaxies live, grow and die. 13 00:00:44,840 --> 00:00:47,840 These collisions got us to where we are today, 14 00:00:47,920 --> 00:00:51,040 and they're gonna determine the future of the universe. 15 00:01:04,240 --> 00:01:08,720 In 2018, astronomers used the Gaia space telescope 16 00:01:08,800 --> 00:01:10,880 to map our Milky Way galaxy. 17 00:01:12,480 --> 00:01:15,400 They tracked the movements of a billion stars. 18 00:01:16,480 --> 00:01:19,880 And they found that some behave very strangely. 19 00:01:21,200 --> 00:01:24,440 When astronomers were mapping stars in our galaxy, 20 00:01:24,520 --> 00:01:29,040 they found a whole bunch that were on similar but very strange orbits. 21 00:01:29,120 --> 00:01:30,360 Most stars in the Milky Way 22 00:01:30,440 --> 00:01:32,840 are orbiting in a sort of regular pattern, 23 00:01:32,920 --> 00:01:34,640 but these stars at the centre, 24 00:01:34,720 --> 00:01:37,360 they're in these highly elongated orbits. 25 00:01:37,440 --> 00:01:39,240 Coming in from very far, 26 00:01:39,320 --> 00:01:42,040 swinging around the centre of our galaxy, 27 00:01:42,120 --> 00:01:46,440 and then going back out again, a little bit like a comet does. 28 00:01:46,520 --> 00:01:51,120 This group of stars plunges wildly through the centre of our galaxy. 29 00:01:51,200 --> 00:01:54,920 When you track their direction and speed on a chart, 30 00:01:55,000 --> 00:01:58,760 you get a shape that looks a bit like a sausage. 31 00:02:01,080 --> 00:02:03,000 This doesn't sound very sciency, 32 00:02:03,080 --> 00:02:05,640 but this sausage is really what the stars look like 33 00:02:05,720 --> 00:02:07,480 if you look at the shapes of their orbits 34 00:02:07,560 --> 00:02:08,880 in a certain configuration. 35 00:02:10,560 --> 00:02:15,040 What sent so many stars on such a strange path? 36 00:02:15,120 --> 00:02:17,280 It must have been a huge event. 37 00:02:18,400 --> 00:02:22,880 We think these stars are the result of a past cosmic collision. 38 00:02:24,960 --> 00:02:27,680 They are casualties from an enormous battle 39 00:02:27,760 --> 00:02:32,000 between the Milky Way and a foreign galactic army. 40 00:02:34,800 --> 00:02:37,000 They don't move like stars in the Milky Way 41 00:02:37,080 --> 00:02:39,080 because they're not from the Milky Way. 42 00:02:39,160 --> 00:02:41,720 These stars are actually alien stars. 43 00:02:41,800 --> 00:02:44,040 They're invaders from outer, outer space 44 00:02:45,720 --> 00:02:48,920 The attackers left their mark on the Milky Way. 45 00:02:50,000 --> 00:02:54,880 We find similar battle scars on galaxies across the universe. 46 00:02:55,920 --> 00:02:58,800 Our models of galaxy formation are still pretty uncertain. 47 00:02:58,880 --> 00:03:02,600 We still don't really understand how galaxies got to where they are, 48 00:03:02,680 --> 00:03:04,920 how we go from the Big Bang to the Milky Way. 49 00:03:06,400 --> 00:03:10,280 Wars between galaxies have profound consequences. 50 00:03:10,360 --> 00:03:14,000 For the winners, the losers and for us. 51 00:03:15,040 --> 00:03:17,840 What we're learning is that these galactic battles 52 00:03:17,920 --> 00:03:21,880 have had a huge impact on what the universe looks like today. 53 00:03:21,960 --> 00:03:23,360 Our understanding of galaxies 54 00:03:23,440 --> 00:03:25,880 has changed entirely in the last few decades. 55 00:03:25,960 --> 00:03:28,840 We understand now that every big galaxy like the Milky Way 56 00:03:28,920 --> 00:03:30,960 started from many smaller things colliding, 57 00:03:31,040 --> 00:03:32,880 changing each other as they went. 58 00:03:34,280 --> 00:03:36,080 Nearly ten billion years ago, 59 00:03:36,160 --> 00:03:39,720 the sausage stars were part of a foreign galaxy. 60 00:03:41,400 --> 00:03:45,480 It was on a collision course with our home, the Milky Way. 61 00:03:46,520 --> 00:03:50,520 We call this invading army the Sausage Galaxy, 62 00:03:50,600 --> 00:03:52,840 or Gaia-Enceladus. 63 00:03:53,880 --> 00:03:58,320 The galaxy that we fought probably had about 50 billion stars, 64 00:03:58,400 --> 00:03:59,960 so we're talking about something 65 00:04:00,040 --> 00:04:03,200 that is a significant fraction of the size of the Milky Way. 66 00:04:05,240 --> 00:04:08,040 Gaia-Enceladus was a tough opponent. 67 00:04:09,920 --> 00:04:13,480 But the Milky Way was 20 times its mass, 68 00:04:13,560 --> 00:04:17,280 and that makes a huge difference. 69 00:04:17,360 --> 00:04:19,640 When galaxies interact with each other, 70 00:04:19,720 --> 00:04:21,280 size definitely matters. 71 00:04:21,360 --> 00:04:24,800 The bigger galaxies are gonna dominate over the smaller ones, 72 00:04:24,880 --> 00:04:28,520 ripping them apart and essentially consuming them. 73 00:04:28,600 --> 00:04:32,240 Galaxy interactions are all about bullies. 74 00:04:32,320 --> 00:04:34,800 The bigger you are, the badder you are. 75 00:04:34,880 --> 00:04:37,120 When two galaxies collide, 76 00:04:37,200 --> 00:04:42,600 it's like two massive armies marching towards each other. 77 00:04:42,680 --> 00:04:48,320 And these galaxies aren't fighting with knives or spears or guns, 78 00:04:48,400 --> 00:04:49,720 or even nuclear bombs, 79 00:04:49,800 --> 00:04:52,600 they're fighting with something much more powerful. 80 00:04:52,680 --> 00:04:54,480 Gravity itself. 81 00:04:56,080 --> 00:04:59,960 Each galaxy contains billions of stars and planets. 82 00:05:01,000 --> 00:05:03,160 And a supermassive black hole, 83 00:05:03,240 --> 00:05:05,480 millions of times the mass of the sun. 84 00:05:06,520 --> 00:05:09,520 That's a lot of gravitational firepower. 85 00:05:10,640 --> 00:05:13,360 As these galaxies approach each other, 86 00:05:13,440 --> 00:05:15,400 you can get tidal effects. 87 00:05:15,480 --> 00:05:18,720 The same way that the moon can raise tides 88 00:05:18,800 --> 00:05:21,200 on one side of the Earth and the opposite side, 89 00:05:21,280 --> 00:05:25,920 one galaxy can stretch another galaxy 90 00:05:26,000 --> 00:05:28,000 along a certain direction. 91 00:05:32,320 --> 00:05:35,640 As Gaia-Enceladus advanced towards us, 92 00:05:35,720 --> 00:05:40,360 our galaxy's superior gravity grabbed hold of the smaller galaxy. 93 00:05:41,800 --> 00:05:42,800 As it approached, 94 00:05:42,880 --> 00:05:45,600 the gravity from the Milky Way would've stretched it out. 95 00:05:47,400 --> 00:05:51,640 Gaia-Enceladus was distorted, but not defeated. 96 00:05:51,720 --> 00:05:54,200 The battle was just beginning. 97 00:05:54,280 --> 00:05:56,440 It would've passed through our galaxy, 98 00:05:56,520 --> 00:05:58,360 maybe orbiting a couple of times, 99 00:05:58,440 --> 00:06:01,680 before being torn apart by our gravity. 100 00:06:04,560 --> 00:06:10,200 The Milky Way's gravitational power ripped Gaia-Enceladus apart 101 00:06:10,280 --> 00:06:13,000 and captured billions of its stars. 102 00:06:14,800 --> 00:06:18,200 And eventually most of those stars would have then settled down 103 00:06:18,280 --> 00:06:21,960 into the disc of the Milky Way and become a part of it. 104 00:06:22,040 --> 00:06:24,000 Little galaxy try to take on the Milky Way, 105 00:06:24,080 --> 00:06:26,640 you gonna get what's coming to you. 106 00:06:26,720 --> 00:06:28,360 Despite winning the battle, 107 00:06:28,440 --> 00:06:31,520 the Milky Way suffered serious damage. 108 00:06:33,000 --> 00:06:35,080 The collision with the Sausage Galaxy 109 00:06:35,160 --> 00:06:37,040 left a scar on the Milky Way, 110 00:06:37,120 --> 00:06:39,280 and when we look near the centre of our galaxy, 111 00:06:39,360 --> 00:06:42,680 we see a bulge just left over from that collision. 112 00:06:44,160 --> 00:06:48,240 The Milky Way isn't the only galaxy scarred by war. 113 00:06:49,640 --> 00:06:54,720 Across the universe, rival armies made up of billions of stars 114 00:06:54,800 --> 00:06:55,880 slug it out, 115 00:06:57,080 --> 00:07:02,240 leaving behind distorted and damaged casualties of war. 116 00:07:04,200 --> 00:07:06,600 There's a million different subcategories of them. 117 00:07:06,680 --> 00:07:09,320 There's tadpole galaxies that have long tails, 118 00:07:09,400 --> 00:07:11,040 longer than our own galaxy. 119 00:07:11,120 --> 00:07:13,760 There are things like Arp-Madore 2026, 120 00:07:13,840 --> 00:07:15,960 where you see this eerie glowing face, 121 00:07:16,040 --> 00:07:19,800 two big eyes looking right at you from across the universe. 122 00:07:19,880 --> 00:07:21,400 There are galaxies that look like 123 00:07:21,480 --> 00:07:24,960 they might've collided and blown holes through each other. 124 00:07:27,560 --> 00:07:30,640 These battle scars give us important clues 125 00:07:30,720 --> 00:07:34,360 about one of the biggest mysteries in astronomy. 126 00:07:34,440 --> 00:07:36,920 How galaxies develop and grow. 127 00:07:38,080 --> 00:07:40,320 But there's a problem. 128 00:07:40,400 --> 00:07:43,880 We can't watch these battles in real time. 129 00:07:44,920 --> 00:07:46,800 The scale of galaxies is huge. 130 00:07:46,880 --> 00:07:49,280 They're hundreds of thousands of light years across. 131 00:07:49,360 --> 00:07:53,520 It's going to take them millions or billions of years to come together. 132 00:07:53,600 --> 00:07:56,000 So it's like looking at one frame 133 00:07:56,080 --> 00:07:58,640 from a really energetic fight scene in a movie. 134 00:08:00,000 --> 00:08:02,240 By piecing these snapshots together, 135 00:08:02,320 --> 00:08:05,720 astronomers can build up a detailed picture 136 00:08:05,800 --> 00:08:07,280 of past conflicts, 137 00:08:07,360 --> 00:08:11,520 and discover how these battles transformed galaxies 138 00:08:11,600 --> 00:08:13,160 over billions of years. 139 00:08:14,200 --> 00:08:16,280 We have pictures of isolated galaxies, 140 00:08:16,360 --> 00:08:18,320 we have pictures of interacting galaxies, 141 00:08:18,400 --> 00:08:21,080 and we have pictures of aftermath galaxies. 142 00:08:22,120 --> 00:08:26,000 And that's helped us discover something alarming. 143 00:08:26,080 --> 00:08:30,040 The Milky Way faces yet another attack. 144 00:08:30,120 --> 00:08:34,680 From an enemy armed with an enormous secret weapon. 145 00:08:34,760 --> 00:08:37,920 Will our solar system survive the onslaught? 146 00:08:46,000 --> 00:08:49,800 Across the universe, galaxies are at war. 147 00:08:51,280 --> 00:08:55,080 Their main weapon? Gravity. 148 00:08:55,160 --> 00:08:59,320 It tears the combatants into weird and wonderful shapes. 149 00:09:00,360 --> 00:09:06,000 Our galaxy didn't escape the mayhem. It's peppered with battle scars. 150 00:09:08,160 --> 00:09:12,560 The overall shape of the Milky Way is a flat disc of stars and gas. 151 00:09:12,640 --> 00:09:15,880 Except recently we have found out that at the edges, 152 00:09:15,960 --> 00:09:19,440 it's actually warped a little bit like the brim of a fedora. 153 00:09:19,520 --> 00:09:22,760 The stars actually dip down below the plane on one side, 154 00:09:22,840 --> 00:09:24,400 and dip above it on the other. 155 00:09:25,800 --> 00:09:28,960 We think the attacker was one of our satellites. 156 00:09:29,040 --> 00:09:34,040 A galaxy that orbits the Milky Way like the moon orbits the Earth. 157 00:09:34,120 --> 00:09:38,360 It's called the Sagittarius Dwarf Galaxy. 158 00:09:38,440 --> 00:09:41,040 From looking at how the stars move in the Milky Way, 159 00:09:41,120 --> 00:09:44,360 we suspect that the Sagittarius Dwarf Galaxy 160 00:09:44,440 --> 00:09:47,920 has actually crashed through the Milky Way a few times 161 00:09:48,000 --> 00:09:50,600 on its course of its orbit around the galaxy. 162 00:09:50,680 --> 00:09:52,680 It came in about six billion years ago, 163 00:09:52,760 --> 00:09:54,840 hit the disc hard about two billion years ago, 164 00:09:54,920 --> 00:09:57,480 and crashed again about a billion years ago. 165 00:09:57,560 --> 00:09:59,520 And our gravity has pulled it out 166 00:09:59,600 --> 00:10:02,400 into a gigantic looping stream of stars 167 00:10:02,480 --> 00:10:04,640 that is moving in and out of our Milky Way. 168 00:10:07,320 --> 00:10:09,120 The war is not over. 169 00:10:09,200 --> 00:10:12,200 The insurgent galaxy will return. 170 00:10:14,360 --> 00:10:15,760 When galaxies interact, 171 00:10:15,840 --> 00:10:18,440 often they're caught in this huge cosmic dance 172 00:10:18,520 --> 00:10:21,080 where they revolve around each other a few times, 173 00:10:21,160 --> 00:10:23,120 or they even crash through each other 174 00:10:23,200 --> 00:10:24,600 and then come back around. 175 00:10:24,680 --> 00:10:27,680 The Sagittarius Dwarf Galaxy looks like it's crashing in 176 00:10:27,760 --> 00:10:29,600 with ever-increasing frequency. 177 00:10:30,880 --> 00:10:35,040 A new skirmish could take place in the next 100 million years. 178 00:10:36,080 --> 00:10:40,320 So, should we be worried about these attacks? 179 00:10:40,400 --> 00:10:42,280 Because the Sagittarius Dwarf Galaxy 180 00:10:42,360 --> 00:10:44,240 is so small compared to the Milky Way, 181 00:10:44,320 --> 00:10:46,800 it will do some damage at the beginning. 182 00:10:46,880 --> 00:10:50,440 But because we're so massive, we can absorb the impact. 183 00:10:50,520 --> 00:10:53,040 I mean, this galaxy, it's looking for a fight, 184 00:10:53,120 --> 00:10:56,520 but it's also 10,000 times smaller than us, 185 00:10:56,600 --> 00:10:58,760 so this is gonna be no sweat at all. 186 00:11:02,000 --> 00:11:05,560 So far, the Milky Way has been victorious. 187 00:11:06,640 --> 00:11:09,160 But the danger isn't over. 188 00:11:10,280 --> 00:11:13,160 We are surrounded by enemies. 189 00:11:13,240 --> 00:11:17,640 Our local neighbourhood of galaxies has three major galaxies, 190 00:11:17,720 --> 00:11:20,880 but up to 50 smaller ones. 191 00:11:20,960 --> 00:11:24,520 All these galaxies are potential troublemakers. 192 00:11:24,600 --> 00:11:28,240 Each one of these could be armies that rise up against us. 193 00:11:29,640 --> 00:11:32,960 The two most famous galaxies that orbit the Milky Way 194 00:11:33,040 --> 00:11:35,560 are the Large and Small Magellanic Clouds. 195 00:11:36,680 --> 00:11:39,200 These are two independent dwarf galaxies 196 00:11:39,280 --> 00:11:42,520 that you can see in the night sky from the southern hemisphere. 197 00:11:46,000 --> 00:11:48,720 We thought the Large Magellanic Cloud 198 00:11:48,800 --> 00:11:51,440 orbited our galaxy at a safe distance 199 00:11:51,520 --> 00:11:54,320 of 160,000 light years. 200 00:11:55,400 --> 00:11:59,120 We thought it would stay that way and we thought it was harmless. 201 00:12:00,200 --> 00:12:05,000 Now a new discovery shows we were wrong on all counts. 202 00:12:06,400 --> 00:12:10,360 The new factor that changed our view of the Magellanic Cloud 203 00:12:10,440 --> 00:12:13,080 is we found out it has a lot more dark matter 204 00:12:13,160 --> 00:12:14,160 than we thought. 205 00:12:16,000 --> 00:12:17,640 Dark matter. 206 00:12:17,720 --> 00:12:21,280 The most mysterious stuff in the universe. 207 00:12:22,320 --> 00:12:25,040 Dark matter is literally what it sounds like. 208 00:12:25,120 --> 00:12:26,760 It's matter that we cannot see. 209 00:12:26,840 --> 00:12:27,840 But it has gravity 210 00:12:27,920 --> 00:12:30,040 and can affect objects that we can see. 211 00:12:33,440 --> 00:12:38,320 Adding in this extra dark matter makes the Large Magellanic Cloud 212 00:12:38,400 --> 00:12:41,480 at least twice as massive as predicted, 213 00:12:41,560 --> 00:12:45,200 so its gravity is double what we thought. 214 00:12:46,800 --> 00:12:49,720 And it's secretly been gathering allies, 215 00:12:49,800 --> 00:12:53,600 has been gathering dark matter on its side, 216 00:12:53,680 --> 00:12:57,000 and now it's a much bigger threat than we thought before. 217 00:12:58,280 --> 00:13:00,120 So it's not just going to orbit us, 218 00:13:00,200 --> 00:13:02,160 it's gonna collide with the Milky Way. 219 00:13:03,480 --> 00:13:06,560 Moving at nearly a million miles an hour, 220 00:13:06,640 --> 00:13:11,120 the Large Magellanic Cloud will not swing past us, 221 00:13:11,200 --> 00:13:12,360 it will attack. 222 00:13:13,560 --> 00:13:15,400 The Large Magellanic Cloud 223 00:13:15,480 --> 00:13:19,280 is one tenth the mass of the Milky Way. 224 00:13:19,360 --> 00:13:22,080 That's enough to make a pretty big punch. 225 00:13:24,000 --> 00:13:26,480 In about two-and-a-half billion years, 226 00:13:26,560 --> 00:13:28,960 it will smash into our galaxy. 227 00:13:32,000 --> 00:13:35,320 It's gonna plough through the disc of the Milky Way. 228 00:13:35,400 --> 00:13:36,880 It's gonna blow a cavity. 229 00:13:36,960 --> 00:13:39,960 It might even damage our spiral arms. 230 00:13:41,960 --> 00:13:45,520 Earth sits in one of those spiral arms. 231 00:13:47,640 --> 00:13:50,640 Could our planet become collateral damage? 232 00:13:51,720 --> 00:13:53,360 If the Large Magellanic Cloud 233 00:13:53,440 --> 00:13:55,600 passes through the plane of our galaxy 234 00:13:55,680 --> 00:13:59,680 near our location, that could have dire consequences. 235 00:14:01,000 --> 00:14:03,960 The gravitational clash between the invader 236 00:14:04,040 --> 00:14:05,280 and the Milky Way 237 00:14:05,360 --> 00:14:08,560 could hurl stars and planets out of our galaxy. 238 00:14:10,000 --> 00:14:12,480 Earth could be one of them. 239 00:14:13,640 --> 00:14:16,640 Our planet's very close to its own star, 240 00:14:16,720 --> 00:14:21,200 so the odds are that you'll just get ripped out along with your star, 241 00:14:21,280 --> 00:14:23,200 so we'd be moving along with the sun 242 00:14:23,280 --> 00:14:26,840 even as the sun gets jettisoned from our galaxy. 243 00:14:26,920 --> 00:14:29,920 And it'll move off out into intergalactic space. 244 00:14:30,000 --> 00:14:33,120 And that's not terrible, I mean, it's not gonna get destroyed, 245 00:14:33,200 --> 00:14:34,800 but it's a little lonely. 246 00:14:37,880 --> 00:14:41,960 Our view of the night sky would radically change. 247 00:14:43,400 --> 00:14:46,480 We'd be able to see much more of the Milky Way, 248 00:14:46,560 --> 00:14:50,120 especially if we got kicked up above the plane of the galaxy. 249 00:14:50,200 --> 00:14:52,680 We'd be able to see the whole shebang. 250 00:14:52,760 --> 00:14:56,640 Just look at any image of a spiral galaxy, 251 00:14:56,720 --> 00:14:57,880 they're gorgeous. 252 00:14:57,960 --> 00:15:00,200 Now, imagine seeing your night sky 253 00:15:00,280 --> 00:15:03,080 filled with the face-on spiral galaxy. 254 00:15:04,200 --> 00:15:07,440 That would be like waking up to my face every morning. 255 00:15:07,520 --> 00:15:08,760 Spectacular. 256 00:15:09,880 --> 00:15:11,440 (LAUGHS) 257 00:15:14,000 --> 00:15:16,160 If we were unlucky, 258 00:15:16,240 --> 00:15:18,720 our home planet could have a close encounter 259 00:15:18,800 --> 00:15:20,440 with an invading star. 260 00:15:21,520 --> 00:15:23,680 The odds are very low 261 00:15:23,760 --> 00:15:26,840 that another star will pass close by the sun. 262 00:15:26,920 --> 00:15:28,720 But those odds aren't zero. 263 00:15:28,800 --> 00:15:31,520 It could happen that another star passes close enough 264 00:15:31,600 --> 00:15:32,840 to affect the planets. 265 00:15:32,920 --> 00:15:34,480 And if that were to happen, 266 00:15:34,560 --> 00:15:39,280 it could upset the delicate balance in the solar system. 267 00:15:40,320 --> 00:15:42,640 We don't know where the Earth could end up. 268 00:15:43,880 --> 00:15:47,080 It might find its way into the sun. You just don't know. 269 00:15:47,160 --> 00:15:49,400 Or there might just be a rain of comets 270 00:15:49,480 --> 00:15:51,280 into our inner solar system. 271 00:15:51,360 --> 00:15:53,920 Our own planet might be flung out, 272 00:15:54,000 --> 00:15:58,400 in which case this would be a death knell for all life on Earth. 273 00:15:58,480 --> 00:16:01,280 I'm not someone who's like a doom and gloom person, 274 00:16:01,360 --> 00:16:03,000 but, like, that would be insane. 275 00:16:04,400 --> 00:16:09,400 You don't know what's gonna happen, but most of the options are bad. 276 00:16:10,480 --> 00:16:14,280 All these nightmare scenarios will extinguish life. 277 00:16:18,000 --> 00:16:20,080 Earth might survive, 278 00:16:20,160 --> 00:16:23,720 but our cosmic zipcode will take a severe beating. 279 00:16:25,040 --> 00:16:28,600 The Milky Way galaxy is bigger than the Large Magellanic Cloud, 280 00:16:28,680 --> 00:16:31,000 so we are gonna win, 281 00:16:31,080 --> 00:16:33,480 but it's gonna hurt us for a long time. 282 00:16:34,880 --> 00:16:38,600 The Large Magellanic Cloud will leave our galaxy battered, 283 00:16:38,680 --> 00:16:41,680 bruised, but ultimately undefeated. 284 00:16:42,720 --> 00:16:47,680 But there's a far bigger threat looming over the Milky Way. 285 00:16:47,760 --> 00:16:50,960 It's gonna face an opponent that it can't defeat. 286 00:16:52,000 --> 00:16:56,560 Will this mega-collision be the Milky Way's last stand? 287 00:16:59,600 --> 00:17:03,480 In the not-too-distant future, galactically speaking, 288 00:17:03,560 --> 00:17:07,560 a much, much larger battle is due for the Milky Way. 289 00:17:09,000 --> 00:17:14,080 A battle with a local superpower, the Andromeda Galaxy. 290 00:17:15,480 --> 00:17:19,360 We thought this huge galaxy might wound us in the future. 291 00:17:20,680 --> 00:17:23,160 Now recent evidence reveals 292 00:17:23,240 --> 00:17:26,400 it's going to make a full-scale assault. 293 00:17:27,720 --> 00:17:29,200 We've known for a long time 294 00:17:29,280 --> 00:17:32,880 that Andromeda is heading more or less toward us, 295 00:17:32,960 --> 00:17:35,440 but we didn't know exactly in what direction. 296 00:17:35,520 --> 00:17:39,240 But in recent years, we've been able to pinpoint this a lot better, 297 00:17:39,320 --> 00:17:43,160 and, uh, yeah, it's heading right for us. 298 00:17:45,400 --> 00:17:47,400 Data from the Hubble Space Telescope 299 00:17:47,480 --> 00:17:52,880 shows the two galaxies will collide in about four billion years. 300 00:17:55,120 --> 00:17:58,520 And it will be a monumental battle. 301 00:17:59,560 --> 00:18:02,680 This collision that is coming, and it is coming, 302 00:18:02,760 --> 00:18:05,920 is not gonna be anything like the Milky Way has experienced before 303 00:18:06,000 --> 00:18:08,000 in its 10 or 12-billion-year history. 304 00:18:08,080 --> 00:18:10,880 This is galaxy of comparable size. 305 00:18:10,960 --> 00:18:14,520 This is two heavyweight prizefighters coming at it. 306 00:18:14,600 --> 00:18:19,240 Warriors with the same gravitational firepower. 307 00:18:19,320 --> 00:18:23,280 Simulations suggest a clash of the titans. 308 00:18:23,360 --> 00:18:26,000 Each of them with half a trillion stars in them. 309 00:18:26,080 --> 00:18:28,600 Well, that sounds like a pretty spectacular collision. 310 00:18:30,240 --> 00:18:34,400 Fights between equally-matched galaxies are rare 311 00:18:34,480 --> 00:18:35,480 and messy. 312 00:18:36,720 --> 00:18:38,200 When the battle kicks off, 313 00:18:38,280 --> 00:18:41,360 there will be no good news for either side. 314 00:18:43,240 --> 00:18:46,040 When the Andromeda Galaxy and the Milky Way galaxy 315 00:18:46,120 --> 00:18:47,440 start to get close, 316 00:18:47,520 --> 00:18:50,080 they're gonna start affecting each other profoundly. 317 00:18:50,160 --> 00:18:52,480 Tendrils of stars are gonna be thrown out. 318 00:18:52,560 --> 00:18:54,800 Gas is gonna be thrown out. 319 00:18:56,320 --> 00:18:59,000 It won't be a single impact. 320 00:19:00,040 --> 00:19:05,120 Gravity will send the two opponents into a spiralling dance of death. 321 00:19:06,800 --> 00:19:09,400 The first pass is actually not a direct hit. 322 00:19:09,480 --> 00:19:12,480 They're gonna swing past each other, in fact. 323 00:19:12,560 --> 00:19:13,720 And at this point, 324 00:19:13,800 --> 00:19:16,440 their gravitational interaction is gonna slow 'em down, 325 00:19:16,520 --> 00:19:18,680 and they're gonna come back toward each other. 326 00:19:18,760 --> 00:19:22,320 The galaxies will collide and fly apart again, 327 00:19:22,400 --> 00:19:25,960 inflicting more and more damage with each clash. 328 00:19:27,160 --> 00:19:29,240 If you were to go outside and look up, 329 00:19:29,320 --> 00:19:32,640 you could see the disc of our galaxy getting ripped apart 330 00:19:32,720 --> 00:19:35,120 by tidal interactions with Andromeda. 331 00:19:38,320 --> 00:19:43,720 The two beautiful spiral galaxies will tear each other apart, 332 00:19:45,000 --> 00:19:48,880 leaving one vast, elliptical galaxy. 333 00:19:50,720 --> 00:19:54,720 The fate of - the Andromeda/ - Milky Way battle 334 00:19:54,800 --> 00:19:57,200 is that they will merge. 335 00:19:57,280 --> 00:20:01,080 This is going to be one gigantic galaxy. 336 00:20:03,840 --> 00:20:05,240 And that presents a problem. 337 00:20:05,320 --> 00:20:07,120 What are we gonna call this new galaxy? 338 00:20:07,200 --> 00:20:10,640 Of course, my nerd colleagues have come up with names 339 00:20:10,720 --> 00:20:13,520 like Milkomeda, Andromoway, whatever. 340 00:20:13,600 --> 00:20:14,960 Those are corny. 341 00:20:15,040 --> 00:20:17,600 We should just call it Hakeem. 342 00:20:23,240 --> 00:20:25,200 With a trillion stars, 343 00:20:25,280 --> 00:20:29,160 it will be one of the biggest galaxies in the universe. 344 00:20:31,320 --> 00:20:34,880 In the Hakeem galaxy, things gonna be completely new. 345 00:20:34,960 --> 00:20:38,120 First off, it's gonna be a really good-looking galaxy, 346 00:20:38,200 --> 00:20:40,200 let's get that straight from the get-go. 347 00:20:40,280 --> 00:20:42,840 Second, it's gonna be powerful. 348 00:20:42,920 --> 00:20:44,960 And I'm talking powerful. 349 00:20:45,040 --> 00:20:47,440 This may be the most remarkable galaxy 350 00:20:47,520 --> 00:20:49,240 in the history of the universe. 351 00:20:51,560 --> 00:20:55,520 Milkomeda, or Hakeem if you prefer, 352 00:20:55,600 --> 00:20:59,040 will become the undisputed boss of our cosmic neighbourhood. 353 00:21:00,400 --> 00:21:04,480 Its calm appearance concealing a history of violence. 354 00:21:07,000 --> 00:21:09,960 It's the result of a complete war zone of mergers 355 00:21:10,040 --> 00:21:11,840 over the course of billions of years. 356 00:21:11,920 --> 00:21:15,720 Many galaxies crashing together, fully reconfiguring each time. 357 00:21:15,800 --> 00:21:20,520 And slowly you grow this smooth, placid, big blob of stars. 358 00:21:23,000 --> 00:21:29,000 After billions of years of warfare, our galaxy will finally be peaceful. 359 00:21:30,920 --> 00:21:34,160 But before its honourable discharge, 360 00:21:34,240 --> 00:21:39,480 Milkomeda may produce one final devastating act of war. 361 00:21:40,640 --> 00:21:43,120 Imagine World War Two, 362 00:21:43,200 --> 00:21:44,440 and then all of a sudden 363 00:21:44,520 --> 00:21:47,400 one of the sides comes up with the Death Star. 364 00:21:47,480 --> 00:21:49,560 That's what we're talking about here. 365 00:21:51,480 --> 00:21:54,280 A weapon of cosmic destruction. 366 00:22:06,560 --> 00:22:08,600 When giant galaxies clash, 367 00:22:08,680 --> 00:22:11,920 the battles are spectacular and destructive. 368 00:22:15,320 --> 00:22:18,400 The victors steal huge numbers of stars 369 00:22:18,480 --> 00:22:20,120 and vast amounts of gas 370 00:22:20,200 --> 00:22:24,200 as fuel for the ultimate super weapon. 371 00:22:26,400 --> 00:22:29,800 This special weapon that these monster galaxies have 372 00:22:29,880 --> 00:22:32,280 is a giant death ray, 373 00:22:32,360 --> 00:22:37,160 a jet of material racing across thousands of light years. 374 00:22:39,480 --> 00:22:41,800 These huge outbursts of energy 375 00:22:41,880 --> 00:22:45,440 blast out of the centre of the colliding galaxies. 376 00:22:45,520 --> 00:22:48,520 They produce more energy in one second 377 00:22:48,600 --> 00:22:53,120 than the sun will in its entire ten-billion-year lifetime. 378 00:22:54,160 --> 00:22:56,320 We call them jets. 379 00:22:57,880 --> 00:23:01,960 These incredibly powerful jets aren't just brief features. 380 00:23:02,040 --> 00:23:05,280 They can be sustained for millions of years. 381 00:23:05,360 --> 00:23:07,480 And they can maintain their structure 382 00:23:07,560 --> 00:23:09,360 for thousands of light years. 383 00:23:10,560 --> 00:23:13,440 It's like turning on a garden hose in Chicago 384 00:23:13,520 --> 00:23:16,640 and using it to water a garden in London. 385 00:23:18,240 --> 00:23:21,240 Exactly what triggered these jets was a mystery. 386 00:23:21,320 --> 00:23:23,960 Then, in June 2018, 387 00:23:24,040 --> 00:23:27,880 astronomers in Hawaii captured something stunning, 388 00:23:27,960 --> 00:23:31,840 a jet forming during a galactic collision. 389 00:23:34,000 --> 00:23:36,520 The team found something really incredible. 390 00:23:36,600 --> 00:23:39,920 They found two galaxies that were in a cosmic collision, 391 00:23:40,000 --> 00:23:43,200 and actually found an active jet in one of these galaxies. 392 00:23:43,280 --> 00:23:46,440 It was the first time anything like this has been discovered. 393 00:23:48,640 --> 00:23:50,280 When galaxies collide, 394 00:23:50,360 --> 00:23:54,160 the clash drives huge clouds of gas and dust 395 00:23:54,240 --> 00:23:56,240 towards their centres. 396 00:23:56,320 --> 00:24:00,560 The supermassive black holes start to feed. 397 00:24:02,080 --> 00:24:04,080 The gas that was in those galaxies 398 00:24:04,160 --> 00:24:06,040 starts to funnel toward the black hole 399 00:24:06,120 --> 00:24:07,600 and will fall upon it. 400 00:24:08,640 --> 00:24:12,960 Not all this gas ends up inside the supermassive black hole, 401 00:24:13,040 --> 00:24:16,200 powerful magnetic fields carry some of this matter 402 00:24:16,280 --> 00:24:17,280 to the poles, 403 00:24:18,400 --> 00:24:21,800 and blast it out in tight, narrow jets. 404 00:24:21,880 --> 00:24:23,680 A super weapon is born. 405 00:24:24,720 --> 00:24:29,640 This discovery helps us understand how giant elliptical galaxies form. 406 00:24:30,800 --> 00:24:35,000 Knowing that mergers of spiral galaxies can cause these jets 407 00:24:35,080 --> 00:24:37,280 helps us put together a complete picture 408 00:24:37,360 --> 00:24:40,360 of how these huge elliptical galaxies might be formed. 409 00:24:43,160 --> 00:24:46,880 The discovery doesn't answer all our questions. 410 00:24:46,960 --> 00:24:48,400 There's another mystery. 411 00:24:48,480 --> 00:24:53,560 How did the super giant galaxies that dwarf the Milky Way get so big? 412 00:24:54,600 --> 00:25:00,120 Our Milky Way galaxy is big-ish. It's slightly bigger than average. 413 00:25:00,200 --> 00:25:02,760 But IC 1101, for example, 414 00:25:02,840 --> 00:25:06,000 is more than 50 times larger than our home galaxy, 415 00:25:06,080 --> 00:25:09,160 and has more than a trillion, with a T, 416 00:25:09,240 --> 00:25:11,240 a trillion stars in it. 417 00:25:11,320 --> 00:25:15,120 The biggest galaxies make the Milky Way look like an ant. 418 00:25:16,160 --> 00:25:19,800 These galactic giants pose a problem. 419 00:25:19,880 --> 00:25:23,280 There hasn't been enough time since the birth of the universe 420 00:25:23,360 --> 00:25:25,800 for them to become so large. 421 00:25:26,840 --> 00:25:29,960 Even by conquering smaller galaxies. 422 00:25:30,040 --> 00:25:32,040 When we look into the distant universe, 423 00:25:32,120 --> 00:25:35,520 we see something very strange that we don't quite understand. 424 00:25:35,600 --> 00:25:37,480 We see enormous galaxies 425 00:25:37,560 --> 00:25:40,440 that existed just a billion years after the Big Bang. 426 00:25:40,520 --> 00:25:42,600 And even though these cosmic collisions 427 00:25:42,680 --> 00:25:44,920 help explain how galaxies get bigger, 428 00:25:45,000 --> 00:25:48,800 they don't quite explain everything about how galaxies grow over time. 429 00:25:48,880 --> 00:25:51,160 So we still have a big mystery on our hands here. 430 00:25:54,880 --> 00:25:57,200 So, in 2019, 431 00:25:57,280 --> 00:26:01,160 an international team investigated a very large galaxy 432 00:26:01,240 --> 00:26:03,640 over 300 million light years away. 433 00:26:03,720 --> 00:26:07,880 We call it NGC 6240. 434 00:26:09,000 --> 00:26:11,800 NGC 6240 was being steadied 435 00:26:11,880 --> 00:26:14,440 because it had two supermassive black holes in it. 436 00:26:14,520 --> 00:26:17,800 Now, the galaxy itself looked like it had been disturbed, 437 00:26:17,880 --> 00:26:19,280 like something had happened, 438 00:26:19,360 --> 00:26:22,840 so they thought that potentially it had had a recent merger. 439 00:26:28,080 --> 00:26:32,080 They were expecting to see two supermassive black holes 440 00:26:32,160 --> 00:26:33,960 in the galaxy's heart. 441 00:26:34,040 --> 00:26:38,200 As the researchers peered through the layers of gas and dust, 442 00:26:38,280 --> 00:26:41,160 they discovered something surprising. 443 00:26:41,240 --> 00:26:43,640 What we found was staggering. 444 00:26:43,720 --> 00:26:47,720 We found not two, but three supermassive black holes 445 00:26:47,800 --> 00:26:49,280 lurking in the centre. 446 00:26:55,240 --> 00:26:57,600 It's the first time we've found a galaxy 447 00:26:57,680 --> 00:27:00,240 with three supermassive black holes. 448 00:27:01,280 --> 00:27:04,280 Evidence of a three galaxy pile up. 449 00:27:05,520 --> 00:27:10,240 This galaxy is an active battlefield of not two, 450 00:27:10,320 --> 00:27:14,560 but three armies colliding at once. 451 00:27:14,640 --> 00:27:16,800 And because there are three armies involved, 452 00:27:16,880 --> 00:27:20,760 there are three galaxies involved with three times as much mass, 453 00:27:20,840 --> 00:27:24,160 three times as many stars, three times as much material, 454 00:27:24,240 --> 00:27:26,400 and three times as much violence. 455 00:27:27,440 --> 00:27:31,840 This three-way battle may explain how the largest galaxies 456 00:27:31,920 --> 00:27:34,080 got so big so fast. 457 00:27:35,120 --> 00:27:38,080 It could be that galaxy mergers are more frequent 458 00:27:38,160 --> 00:27:39,880 than what we thought previously. 459 00:27:39,960 --> 00:27:43,600 And therefore, galaxies become more massive 460 00:27:43,680 --> 00:27:45,400 faster than previously expected. 461 00:27:47,480 --> 00:27:48,560 In the past, 462 00:27:48,640 --> 00:27:52,640 galaxies may have battled and collided more often than today. 463 00:27:52,720 --> 00:27:57,280 Back then, galaxies were more densely packed together. 464 00:27:58,560 --> 00:28:01,440 Our universe is expanding as it ages, 465 00:28:01,520 --> 00:28:05,000 which means in the past all the galaxies in the universe 466 00:28:05,080 --> 00:28:06,920 were closer together. 467 00:28:07,000 --> 00:28:08,720 That means they've had greater chance 468 00:28:08,800 --> 00:28:10,560 for their gravitational interactions 469 00:28:10,640 --> 00:28:12,960 to pull them together and smash them together. 470 00:28:15,960 --> 00:28:18,960 When galaxies fight, the big get bigger. 471 00:28:20,000 --> 00:28:24,160 More mass means more gravity. The vital ingredient for victory. 472 00:28:26,400 --> 00:28:30,320 But galactic conflict doesn't always result in growth. 473 00:28:31,360 --> 00:28:36,000 A strange new astronomical object had scientists confused. 474 00:28:38,640 --> 00:28:41,640 They just look like stars from the ground. 475 00:28:41,720 --> 00:28:43,880 However, with the advent of Hubble 476 00:28:43,960 --> 00:28:46,600 and beautiful space-based telescopes, 477 00:28:46,680 --> 00:28:50,160 it was possible to look at these "stars" again 478 00:28:50,240 --> 00:28:52,560 and actually discover that they were galaxies. 479 00:28:58,000 --> 00:29:02,640 They're kind of crazy. They're a huge number of stars, 480 00:29:02,720 --> 00:29:05,360 but crammed into an incredibly tiny space 481 00:29:05,440 --> 00:29:06,760 on an astrophysical scale, 482 00:29:06,840 --> 00:29:10,320 something 500 times smaller than our Milky Way galaxy. 483 00:29:11,560 --> 00:29:15,200 We call them ultra-compact dwarf galaxies, 484 00:29:15,280 --> 00:29:16,520 or UCDs. 485 00:29:17,800 --> 00:29:20,760 You might imagine the difference between 486 00:29:20,840 --> 00:29:23,720 the Milky Way galaxy and a UCD 487 00:29:23,800 --> 00:29:27,960 as the difference between a cloud and a rock, 488 00:29:28,040 --> 00:29:31,520 where the rock is just the same kind of material, 489 00:29:31,600 --> 00:29:34,000 but compressed to just incredibly high densities 490 00:29:34,080 --> 00:29:36,320 compared to some fluffy, gaseous thing. 491 00:29:39,400 --> 00:29:43,960 What are these strange galaxies? They seem to break all the rules. 492 00:29:45,000 --> 00:29:47,480 To find out, astronomers zoomed in 493 00:29:47,560 --> 00:29:51,640 to a particularly dense ultra-compact dwarf galaxy 494 00:29:51,720 --> 00:29:55,440 called M60-UCD1. 495 00:29:56,720 --> 00:30:00,520 M60-UCD1 is 300 light years across. 496 00:30:00,600 --> 00:30:04,080 It's tiny. It's a pinpoint compared to our enormous galaxy. 497 00:30:04,160 --> 00:30:08,040 Our galaxy has 200 or more billion stars in it. 498 00:30:08,120 --> 00:30:11,000 M60-UCD1 only has 140 million, 499 00:30:11,080 --> 00:30:14,880 but they're packed into this incredibly tight volume. 500 00:30:14,960 --> 00:30:17,440 The night sky inside the galaxy 501 00:30:17,520 --> 00:30:19,760 would look very different from our own. 502 00:30:20,840 --> 00:30:22,800 On Earth, when you look at the night sky, 503 00:30:22,880 --> 00:30:24,880 you see a few thousand stars. 504 00:30:24,960 --> 00:30:27,440 But if you were in M60-UCD1, 505 00:30:27,520 --> 00:30:29,920 you wouldn't just see a few thousand stars, 506 00:30:30,000 --> 00:30:34,160 you would see hundreds of thousands of stars in the night sky. 507 00:30:34,240 --> 00:30:35,880 That would be amazing. 508 00:30:41,920 --> 00:30:46,320 As the astronomers looked deeper into the heart of this tiny galaxy, 509 00:30:47,560 --> 00:30:50,040 things got even weirder. 510 00:30:50,120 --> 00:30:54,560 They found a supermassive black hole much bigger than expected. 511 00:30:56,800 --> 00:31:00,600 It actually has a black hole that's bigger, five times bigger, 512 00:31:00,680 --> 00:31:03,840 than the black hole at the centre of our Milky Way galaxy. 513 00:31:03,920 --> 00:31:07,400 When we see supermassive black holes inside of galaxies, 514 00:31:07,480 --> 00:31:10,880 they tend to scale with the size of the galaxy itself. 515 00:31:10,960 --> 00:31:14,640 A bigger galaxy has a bigger supermassive black hole. 516 00:31:14,720 --> 00:31:16,880 Why does such a tiny little object 517 00:31:16,960 --> 00:31:19,880 have such an oversized central black hole? 518 00:31:19,960 --> 00:31:22,520 The only possible explanation? 519 00:31:22,600 --> 00:31:26,400 This tiny galaxy was once much larger. 520 00:31:27,440 --> 00:31:29,880 These galaxies might have begun their lives 521 00:31:29,960 --> 00:31:32,360 as, in fact, much bigger galaxies. 522 00:31:32,440 --> 00:31:36,240 And that what we see today is really just the very central densest part 523 00:31:36,320 --> 00:31:37,960 of a much larger galaxy. 524 00:31:39,560 --> 00:31:42,880 Based on the size of its supermassive black hole, 525 00:31:42,960 --> 00:31:49,600 M60-UCD1 may once have contained many billions of stars. 526 00:31:49,680 --> 00:31:52,320 Something captured them, 527 00:31:52,400 --> 00:31:55,720 and we don't have to look far to find the aggressor. 528 00:31:55,800 --> 00:31:57,440 A nearby super galaxy 529 00:31:57,520 --> 00:32:01,680 with lots of gravitational firepower, M60. 530 00:32:02,800 --> 00:32:06,120 M60's a monster. It has a trillion stars in it. 531 00:32:06,200 --> 00:32:09,000 It's bigger than the Milky Way and we're pretty big. 532 00:32:09,080 --> 00:32:12,400 The battle was not a full-on frontal assault. 533 00:32:12,480 --> 00:32:17,960 M60 raided its smaller opponent, capturing its troops. 534 00:32:18,040 --> 00:32:21,520 This is more of a stealthy, guerrilla hit and run, 535 00:32:21,600 --> 00:32:24,400 where we're gonna move in, pick off some of your troops 536 00:32:24,480 --> 00:32:27,200 and then get out before you even notice. 537 00:32:28,320 --> 00:32:32,640 All that's left from one of these drive-by galaxy interactions 538 00:32:32,720 --> 00:32:35,040 is this supermassive black hole 539 00:32:35,120 --> 00:32:37,400 with a fraction of its original stars. 540 00:32:38,560 --> 00:32:42,560 The conflict devastated M60-UCD1. 541 00:32:42,640 --> 00:32:46,640 Over 98% of its stellar army were captured 542 00:32:46,720 --> 00:32:48,840 and became prisoners of war. 543 00:32:48,920 --> 00:32:52,480 It used to be a big galaxy, 544 00:32:52,560 --> 00:32:57,320 but it suffered one too many defeats and now it's a fallen empire. 545 00:32:58,360 --> 00:33:02,440 We can frame this battle between M60 and M60-UCD1 546 00:33:02,520 --> 00:33:03,760 as just a battle, 547 00:33:03,840 --> 00:33:07,080 but, in fact, it's a slaughter, it's a massacre. 548 00:33:08,120 --> 00:33:12,360 These small galaxies get all their troops removed, 549 00:33:12,440 --> 00:33:13,920 but the HQ, 550 00:33:14,000 --> 00:33:16,000 the supermassive black hole, remains, 551 00:33:16,080 --> 00:33:17,840 but it doesn't have any troops left. 552 00:33:19,000 --> 00:33:22,880 Eventually, M60 will conquer its battered opponent, 553 00:33:22,960 --> 00:33:26,120 destroying what's left of the compact galaxy. 554 00:33:27,200 --> 00:33:28,920 It'll get ripped apart even further, 555 00:33:29,000 --> 00:33:31,000 and more and more stars will be consumed 556 00:33:31,080 --> 00:33:32,280 by the bigger galaxy. 557 00:33:32,360 --> 00:33:37,080 So chances are this little dwarf is eventually going to be pulled apart 558 00:33:37,160 --> 00:33:39,520 and become a part of M60. 559 00:33:42,080 --> 00:33:44,560 But while this little galaxy is down, 560 00:33:44,640 --> 00:33:47,640 it is most certainly not yet out. 561 00:33:47,720 --> 00:33:49,960 It's likely to stage a counterattack. 562 00:33:51,080 --> 00:33:56,960 Its final mission? A kamikaze charge that will leave M60 reeling. 563 00:34:01,240 --> 00:34:04,400 It's absolutely chaotic. 564 00:34:04,480 --> 00:34:08,360 Stars are sent off flying in every direction, 565 00:34:08,440 --> 00:34:11,440 and they're moving at really high velocities. 566 00:34:12,560 --> 00:34:15,200 And when stars are stripped out of galaxies, 567 00:34:15,280 --> 00:34:17,280 they become what we call rogue stars. 568 00:34:19,880 --> 00:34:23,600 These ejected, runaway stars will leave the galaxy 569 00:34:23,680 --> 00:34:25,400 at two million miles an hour. 570 00:34:27,720 --> 00:34:30,360 They'll hurtle through the emptiness of space, 571 00:34:30,440 --> 00:34:32,440 never to be seen again. 572 00:34:35,720 --> 00:34:40,960 But even this dramatic assault can't change the inevitable outcome. 573 00:34:41,040 --> 00:34:45,120 M60-UCD1 is doomed. 574 00:34:50,640 --> 00:34:52,960 In the great game of galactic warfare, 575 00:34:53,040 --> 00:34:55,040 losing can be catastrophic. 576 00:34:55,120 --> 00:35:00,000 For weak and small galaxies, resistance is futile. 577 00:35:01,480 --> 00:35:04,880 Pillaged for resources by their more powerful opponents, 578 00:35:04,960 --> 00:35:07,680 they slowly become burnt-out wrecks. 579 00:35:10,000 --> 00:35:14,880 But some peaceful galaxies face an equally terrible fate. 580 00:35:15,920 --> 00:35:17,320 They starve to death. 581 00:35:24,320 --> 00:35:29,200 Cosmic wars are vicious. They destroy many galaxies. 582 00:35:30,240 --> 00:35:34,080 But violent conflicts can also give galaxies new life. 583 00:35:35,640 --> 00:35:41,640 Case in point, galaxy NGC 4485. 584 00:35:41,720 --> 00:35:44,880 NGC 4485 has a nickname of the Two-Face galaxy, 585 00:35:44,960 --> 00:35:46,280 like the Batman villain, 586 00:35:46,360 --> 00:35:48,840 because it has two different halves of the galaxy 587 00:35:48,920 --> 00:35:50,600 doing completely different things. 588 00:35:50,680 --> 00:35:55,080 Half of the galaxy is sort of old and calm and relatively quiescent, 589 00:35:55,160 --> 00:35:57,560 whereas half of it appears to be undergoing 590 00:35:57,640 --> 00:36:00,880 a sort of fireworks display of new star formation. 591 00:36:02,000 --> 00:36:06,640 Why are new stars only born in one half of this galaxy? 592 00:36:08,080 --> 00:36:10,720 We found a clue on the edge of a photo 593 00:36:10,800 --> 00:36:12,960 taken by the Hubble Space Telescope. 594 00:36:15,120 --> 00:36:18,680 It was evidence of an attack by another galaxy. 595 00:36:18,760 --> 00:36:23,080 We think that another galaxy passed through it just off centre 596 00:36:23,160 --> 00:36:25,960 in a way that strongly perturbed the gas 597 00:36:26,040 --> 00:36:28,040 on one half of the galaxy. 598 00:36:30,000 --> 00:36:34,400 The Two-Face galaxy skirmish gave it a gravitational jolt, 599 00:36:34,480 --> 00:36:37,120 forcing clouds of gas together. 600 00:36:38,240 --> 00:36:40,480 When we think of galaxies, we think of stars, 601 00:36:40,560 --> 00:36:42,520 and of course galaxies are made of stars, 602 00:36:42,600 --> 00:36:46,400 but of course gas is the stuff that stars are made of. 603 00:36:48,320 --> 00:36:50,280 When two galaxies collide, 604 00:36:50,360 --> 00:36:54,520 the gravitational duel can trigger a huge burst of star formation. 605 00:36:58,720 --> 00:37:01,200 You need something to give a galaxy a push, 606 00:37:01,280 --> 00:37:03,760 and that's exactly what a galaxy collision does. 607 00:37:03,840 --> 00:37:07,000 And when gas clouds collide, they compress. 608 00:37:07,080 --> 00:37:09,880 And when they compress, you get knots in them 609 00:37:09,960 --> 00:37:12,960 that can compress more and form stars. 610 00:37:15,000 --> 00:37:18,000 So you can think of these collisions as very violent events, 611 00:37:18,080 --> 00:37:21,080 but ultimately it can breathe new life into a galaxy. 612 00:37:22,120 --> 00:37:25,520 But the spoils of war don't last long. 613 00:37:25,600 --> 00:37:30,000 In the short term, the victor galaxy can come out glorious 614 00:37:30,080 --> 00:37:32,640 with so many new stars. 615 00:37:32,720 --> 00:37:36,760 But this celebration is short lived because that round of star formation 616 00:37:36,840 --> 00:37:40,560 quickly uses up the material available. 617 00:37:40,640 --> 00:37:45,480 If a galaxy wants to stay alive, it has to feed on other galaxies. 618 00:37:49,560 --> 00:37:52,480 But what happens when opponents are closely matched 619 00:37:52,560 --> 00:37:54,200 in gravitational firepower? 620 00:37:56,960 --> 00:38:02,920 When two equal mass galaxies meet, when two armies of equal size meet, 621 00:38:03,000 --> 00:38:07,800 they can exhaust all their fuel, they can kill all their troops, 622 00:38:07,880 --> 00:38:10,680 so at the end of it there's nobody left to fight. 623 00:38:10,760 --> 00:38:14,240 The galaxies themselves can be stripped of gas and dust, 624 00:38:14,320 --> 00:38:17,800 all the things you need to actually make star formation happen. 625 00:38:21,880 --> 00:38:23,840 Once the gas is used up, 626 00:38:23,920 --> 00:38:26,240 the galaxy can't create any new stars. 627 00:38:27,320 --> 00:38:31,320 It can only get more gas by looting other galaxies. 628 00:38:32,400 --> 00:38:36,400 We can sometimes see a gas stream coming from one galaxy 629 00:38:36,480 --> 00:38:37,880 and joining to the other, 630 00:38:37,960 --> 00:38:40,360 and then the gas from that galaxy is now free 631 00:38:40,440 --> 00:38:42,600 and it starts to make stars again. 632 00:38:44,000 --> 00:38:46,880 You're bringing in new ingredients to form stars, 633 00:38:46,960 --> 00:38:50,440 new gas, new dust to become part of this larger galaxy. 634 00:38:50,520 --> 00:38:54,360 All sorts of weird and wonderful things can happen in galaxy mergers. 635 00:38:58,320 --> 00:38:59,560 A star is born 636 00:38:59,640 --> 00:39:02,960 when a huge cloud of gas collapses under gravity, 637 00:39:03,040 --> 00:39:05,040 triggering nuclear fusion. 638 00:39:06,080 --> 00:39:08,640 The star ignites and begins to shine. 639 00:39:09,800 --> 00:39:11,040 It's a glorious sight 640 00:39:11,120 --> 00:39:15,200 and often a sign that the war is finally ending. 641 00:39:17,240 --> 00:39:20,040 When two galaxies come together, boom, 642 00:39:20,120 --> 00:39:22,840 all of a sudden, stars light up all over the place. 643 00:39:23,880 --> 00:39:27,160 In this moment, as you catch this system getting excited, 644 00:39:27,240 --> 00:39:28,960 the star formation rate's ramping up 645 00:39:29,040 --> 00:39:31,040 and it's sort of a cosmic fireworks display, 646 00:39:31,120 --> 00:39:34,280 as if they're celebrating the end of this hostile encounter 647 00:39:34,360 --> 00:39:36,160 with the other galaxy, this war. 648 00:39:38,480 --> 00:39:41,720 But it's also a sign that the victorious galaxy 649 00:39:41,800 --> 00:39:43,800 is using up its gas supply. 650 00:39:46,160 --> 00:39:50,320 So galaxies constantly need to raid new targets 651 00:39:50,400 --> 00:39:53,200 and that raises an important question. 652 00:39:53,280 --> 00:39:55,680 What happens if there's a galaxy just alone in space, 653 00:39:55,760 --> 00:39:59,160 nothing else is colliding with it, sort of a pacifist galaxy. 654 00:40:00,200 --> 00:40:03,440 The poster child for these peace-loving galaxies 655 00:40:03,520 --> 00:40:06,400 is NGC 1277. 656 00:40:07,640 --> 00:40:11,440 NGC 1277 is a very peculiar galaxy. 657 00:40:11,520 --> 00:40:15,920 It's pretty big and its stars are extremely old. 658 00:40:16,000 --> 00:40:20,200 It basically hasn't formed new stars in the last ten billion years, 659 00:40:20,280 --> 00:40:23,280 so it's kind of the veterans home of galaxies. 660 00:40:24,320 --> 00:40:27,880 NGC 1277 lives in a rough part of the cosmos 661 00:40:27,960 --> 00:40:29,600 called the Perseus Cluster. 662 00:40:30,680 --> 00:40:35,000 Thousands of other galaxies surround NGC 1277 663 00:40:35,080 --> 00:40:37,400 and they are all ready for a fight. 664 00:40:38,560 --> 00:40:41,720 So, you might ask why hasn't it had encounters with other galaxies 665 00:40:41,800 --> 00:40:43,440 that might rejuvenate it? 666 00:40:44,480 --> 00:40:47,280 The answer, once again, is gravity. 667 00:40:48,480 --> 00:40:53,440 NGC 1277 sits inside this massive galaxy cluster 668 00:40:53,520 --> 00:40:54,600 that has a ton of mass. 669 00:40:54,680 --> 00:40:56,160 And if you look at its position, 670 00:40:56,240 --> 00:40:58,280 it's fairly near the centre of the cluster. 671 00:41:00,640 --> 00:41:03,600 The combined gravity of thousands of galaxies 672 00:41:03,680 --> 00:41:06,400 pulls on NGC 1277, 673 00:41:06,480 --> 00:41:10,200 accelerating it to two million miles an hour. 674 00:41:12,880 --> 00:41:16,040 And so it has spent the last few billion years 675 00:41:16,120 --> 00:41:17,680 travelling faster and faster, 676 00:41:17,760 --> 00:41:20,400 until now it's almost at its fastest pace. 677 00:41:22,640 --> 00:41:25,440 It's very hard for gravity to catch it, 678 00:41:25,520 --> 00:41:26,920 or catch one of its neighbours, 679 00:41:27,000 --> 00:41:29,680 and bring them together to merge with each other. 680 00:41:31,080 --> 00:41:37,480 NGC 1277 has no chance of grabbing new gas to make new stars. 681 00:41:37,560 --> 00:41:38,800 It's dying. 682 00:41:38,880 --> 00:41:42,120 All it has left are old red stars. 683 00:41:43,320 --> 00:41:46,880 When it comes to galaxies, red is dead. 684 00:41:46,960 --> 00:41:50,360 No new stars means no big stars, no blue stars, 685 00:41:50,440 --> 00:41:52,920 just small, dim, red dwarfs. 686 00:41:57,400 --> 00:42:00,400 Galaxies that don't fight just fade away. 687 00:42:01,560 --> 00:42:02,720 At that point, 688 00:42:02,800 --> 00:42:05,680 the history of the universe becomes really kind of boring. 689 00:42:05,760 --> 00:42:08,080 All the stars will simply start to die out. 690 00:42:08,160 --> 00:42:09,960 Eventually there will be the last star 691 00:42:10,040 --> 00:42:11,280 formed in the Milky Way, 692 00:42:11,360 --> 00:42:13,760 with no new galaxy bringing fresh material. 693 00:42:13,840 --> 00:42:17,400 Without galaxy collisions, the universe dies. 694 00:42:24,000 --> 00:42:29,080 Galactic battles mix things up and replenish gas supplies. 695 00:42:30,360 --> 00:42:33,000 And our own galaxy has reaped the benefits. 696 00:42:34,240 --> 00:42:38,200 Our Milky Way galaxy fought a massive battle, 697 00:42:38,280 --> 00:42:40,800 but that battle may have been necessary 698 00:42:40,880 --> 00:42:45,040 to build solar systems like the one we live in right now. 699 00:42:48,240 --> 00:42:51,400 Clashes with the Sagittarius Dwarf Galaxy 700 00:42:51,480 --> 00:42:54,200 occurred at the same time the sun formed. 701 00:42:56,160 --> 00:42:59,040 It's possible that we owe our very existence 702 00:42:59,120 --> 00:43:01,920 to the collision with the Sagittarius Dwarf Galaxy. 703 00:43:03,000 --> 00:43:04,160 Maybe the gas 704 00:43:04,240 --> 00:43:07,400 that ultimately gave rise to the birth of our solar system 705 00:43:07,480 --> 00:43:10,000 once came from another galaxy entirely. 706 00:43:12,400 --> 00:43:16,280 So, galactic wars are both creative and destructive. 707 00:43:17,320 --> 00:43:20,960 Galaxies are built from collisions. 708 00:43:21,040 --> 00:43:24,440 Galaxies survive from collisions. 709 00:43:24,520 --> 00:43:27,840 And galaxies can also die from collisions. 710 00:43:29,240 --> 00:43:30,880 Far from being destructive events, 711 00:43:30,960 --> 00:43:33,920 colliding galaxies may be the reason that you and I are here. 712 00:43:36,760 --> 00:43:38,760 Intergalactic warfare 713 00:43:38,840 --> 00:43:44,080 has revolutionised our understanding of how galaxies live and die. 714 00:43:45,120 --> 00:43:46,920 Ultimately, it's these galaxy mergers 715 00:43:47,000 --> 00:43:48,800 that are one of the great engines 716 00:43:48,880 --> 00:43:51,200 of all structured growth in the universe. 717 00:43:52,240 --> 00:43:55,040 These collisions got us to where we are today, 718 00:43:55,120 --> 00:43:58,440 and they're gonna determine the future of all the universe. 719 00:43:58,520 --> 00:44:00,520 subtitles by Deluxe 59451

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