All language subtitles for How the Universe Works s09e06 War of the Galaxies.eng

af Afrikaans
sq Albanian
am Amharic
ar Arabic
hy Armenian
az Azerbaijani
eu Basque
be Belarusian
bn Bengali
bs Bosnian
bg Bulgarian
ca Catalan
ceb Cebuano
ny Chichewa
zh-CN Chinese (Simplified)
zh-TW Chinese (Traditional)
co Corsican
hr Croatian
cs Czech
da Danish
nl Dutch Download
en English
eo Esperanto
et Estonian
tl Filipino
fi Finnish
fr French
fy Frisian
gl Galician
ka Georgian
de German
el Greek
gu Gujarati
ht Haitian Creole
ha Hausa
haw Hawaiian
iw Hebrew
hi Hindi
hmn Hmong
hu Hungarian
is Icelandic
ig Igbo
id Indonesian
ga Irish
it Italian
ja Japanese
jw Javanese
kn Kannada
kk Kazakh
km Khmer
ko Korean
ku Kurdish (Kurmanji)
ky Kyrgyz
lo Lao
la Latin
lv Latvian
lt Lithuanian
lb Luxembourgish
mk Macedonian
mg Malagasy
ms Malay
ml Malayalam
mt Maltese
mi Maori
mr Marathi
mn Mongolian
my Myanmar (Burmese)
ne Nepali
no Norwegian
ps Pashto
fa Persian
pl Polish
pt Portuguese
pa Punjabi
ro Romanian
ru Russian
sm Samoan
gd Scots Gaelic
sr Serbian
st Sesotho
sn Shona
sd Sindhi
si Sinhala
sk Slovak
sl Slovenian
so Somali
es Spanish
su Sundanese
sw Swahili
sv Swedish
tg Tajik
ta Tamil
te Telugu
th Thai
tr Turkish
uk Ukrainian
ur Urdu
uz Uzbek
vi Vietnamese
cy Welsh
xh Xhosa
yi Yiddish
yo Yoruba
zu Zulu
or Odia (Oriya)
rw Kinyarwanda
tk Turkmen
tt Tatar
ug Uyghur
Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:03,290 --> 00:00:06,090 Our universe is at war. 2 00:00:06,190 --> 00:00:10,990 The universe is a very violent and deadly place. 3 00:00:11,090 --> 00:00:14,160 Entire galaxies fight to the death. 4 00:00:14,260 --> 00:00:16,600 Talk about clash of the Titans. 5 00:00:16,700 --> 00:00:19,170 It doesn't get more titanic than this. 6 00:00:19,270 --> 00:00:21,170 It's a slaughter. It's a massacre. 7 00:00:21,270 --> 00:00:23,810 Only the strongest survive. 8 00:00:23,910 --> 00:00:25,610 If a galaxy wants to stay alive, 9 00:00:25,710 --> 00:00:28,610 it has to feed on other galaxies. 10 00:00:28,710 --> 00:00:32,080 Our own galaxy also fights for survival. 11 00:00:33,080 --> 00:00:36,620 We are facing the ultimate destruction 12 00:00:36,720 --> 00:00:38,990 of the Milky Way Galaxy. 13 00:00:39,090 --> 00:00:42,490 These battles are how galaxies live, 14 00:00:42,590 --> 00:00:44,960 grow, and die. 15 00:00:45,060 --> 00:00:48,030 These collisions got us to where we are today, 16 00:00:48,130 --> 00:00:50,570 and they're going to determine the future of the universe. 17 00:01:04,650 --> 00:01:07,420 In 2018, astronomers used the Gaia 18 00:01:07,520 --> 00:01:10,850 space telescope to map our Milky Way Galaxy. 19 00:01:12,690 --> 00:01:16,090 They tracked the movements of a billion stars, 20 00:01:16,190 --> 00:01:19,860 and they found that some behave very strangely. 21 00:01:21,400 --> 00:01:24,470 When astronomers were mapping stars in our galaxy, 22 00:01:24,570 --> 00:01:27,300 they found a whole bunch that we're on similar 23 00:01:27,400 --> 00:01:29,300 but very strange orbits. 24 00:01:29,410 --> 00:01:31,840 Most stars of the Milky Way are orbiting in a sort of 25 00:01:31,940 --> 00:01:34,140 regular pattern, but these stars 26 00:01:34,280 --> 00:01:37,510 at the center, they're in these highly elongated orbits. 27 00:01:37,610 --> 00:01:39,550 Coming in from very far, 28 00:01:39,650 --> 00:01:43,080 swinging around the center of our galaxy, and then going back 29 00:01:43,190 --> 00:01:46,690 out again, a little bit like a comet does. 30 00:01:46,790 --> 00:01:48,420 This group of stars plunges 31 00:01:48,520 --> 00:01:51,860 wildly through the center of our galaxy. 32 00:01:51,960 --> 00:01:55,230 When you track their direction and speed on a chart, 33 00:01:55,330 --> 00:01:58,970 you get a shape that looks a bit like a sausage. 34 00:02:01,440 --> 00:02:02,800 This doesn't sound very science-y, 35 00:02:02,940 --> 00:02:05,870 but this sausage is really what the stars look like 36 00:02:05,980 --> 00:02:06,980 if you look at the shapes 37 00:02:07,010 --> 00:02:09,140 of their orbits in a certain configuration. 38 00:02:10,750 --> 00:02:14,620 What sent so many stars on such a strange path? 39 00:02:14,720 --> 00:02:17,790 It must have been a huge event. 40 00:02:18,890 --> 00:02:21,720 We think these stars are the result of a past 41 00:02:21,820 --> 00:02:22,920 cosmic collision. 42 00:02:25,260 --> 00:02:28,200 They are casualties from an enormous battle between 43 00:02:28,300 --> 00:02:31,830 the Milky Way and a foreign galactic army. 44 00:02:35,000 --> 00:02:36,870 They don't move like stars in the Milky Way, 45 00:02:36,970 --> 00:02:39,210 because they're not from the Milky Way. 46 00:02:39,310 --> 00:02:41,810 These stars are actually alien stars. 47 00:02:41,910 --> 00:02:44,380 They're invaders from outer, outer space. 48 00:02:46,320 --> 00:02:49,180 The attackers left their mark on the Milky Way. 49 00:02:50,390 --> 00:02:53,720 We find similar battle scars on galaxies across 50 00:02:53,820 --> 00:02:55,860 the universe. 51 00:02:55,960 --> 00:02:57,730 Our models of galaxy information are still 52 00:02:57,830 --> 00:02:58,930 pretty uncertain. 53 00:02:59,030 --> 00:03:01,960 We still don't really understand how galaxies got to 54 00:03:02,060 --> 00:03:05,230 where they are, how we go from the Big Bang to the Milky Way. 55 00:03:06,740 --> 00:03:10,740 Wars between galaxies have profound consequences, for 56 00:03:10,840 --> 00:03:14,080 the winners, the losers, and for us. 57 00:03:14,180 --> 00:03:18,450 What we're learning is that these galactic battles have had 58 00:03:18,550 --> 00:03:22,120 a huge impact on what the universe looks like today. 59 00:03:22,220 --> 00:03:24,020 Our understanding of galaxies has changed 60 00:03:24,120 --> 00:03:25,850 entirely in the last few decades. 61 00:03:25,960 --> 00:03:28,620 We understand now that every big galaxy like the Milky Way 62 00:03:28,720 --> 00:03:31,160 started from many smaller things colliding, 63 00:03:31,260 --> 00:03:32,830 changing each other as they went. 64 00:03:34,500 --> 00:03:36,360 Nearly 10 billion years ago, 65 00:03:36,470 --> 00:03:39,730 the sausage stars were part of a foreign galaxy. 66 00:03:41,700 --> 00:03:45,570 It was on a collision course with our home, the Milky Way. 67 00:03:47,110 --> 00:03:51,250 We call this invading army the Sausage Galaxy, 68 00:03:51,350 --> 00:03:53,880 or Gaia-Enceladus. 69 00:03:53,980 --> 00:03:56,720 The galaxy that we fought probably had 70 00:03:56,820 --> 00:03:58,450 about 50 billion stars, 71 00:03:58,550 --> 00:04:00,720 so we're talking about something that is a significant 72 00:04:00,820 --> 00:04:02,860 fraction of the size of the Milky Way. 73 00:04:05,530 --> 00:04:08,030 Gaia-Enceladus was a tough opponent, 74 00:04:09,730 --> 00:04:14,140 but the Milky Way was 20 times its mass, 75 00:04:14,240 --> 00:04:16,600 and that makes a huge difference. 76 00:04:16,710 --> 00:04:19,640 When galaxies interact with each other, 77 00:04:19,740 --> 00:04:21,410 size definitely matters. 78 00:04:21,510 --> 00:04:24,980 The bigger galaxies are gonna dominate over the smaller ones, 79 00:04:25,080 --> 00:04:28,720 ripping them apart and essentially consuming them. 80 00:04:28,820 --> 00:04:32,220 Galaxy interactions are all about bullies. 81 00:04:32,320 --> 00:04:35,120 The bigger you are, the badder you are. 82 00:04:35,220 --> 00:04:37,260 When two galaxies collide, 83 00:04:37,360 --> 00:04:42,660 it's like two massive armies marching towards each other. 84 00:04:42,770 --> 00:04:45,400 These galaxies aren't fighting 85 00:04:45,500 --> 00:04:50,100 with knives or spears or guns or even nuclear bombs. 86 00:04:50,210 --> 00:04:51,346 They're fighting with something 87 00:04:51,370 --> 00:04:54,710 much more powerful... Gravity itself. 88 00:04:56,310 --> 00:05:00,650 Each galaxy contains billions of stars and planets 89 00:05:00,750 --> 00:05:03,320 and a supermassive black hole, 90 00:05:03,420 --> 00:05:06,420 millions of times the mass of the sun. 91 00:05:06,520 --> 00:05:09,460 That's a lot of gravitational firepower. 92 00:05:11,030 --> 00:05:13,460 As these galaxies approach each other, 93 00:05:13,560 --> 00:05:17,630 you can get tidal effects... The same way that the moon can 94 00:05:17,730 --> 00:05:21,440 raise tides on one side of the Earth and the opposite side, 95 00:05:21,540 --> 00:05:25,210 one galaxy can stretch another 96 00:05:25,310 --> 00:05:27,940 galaxy along a certain direction. 97 00:05:32,650 --> 00:05:35,820 As Gaia-Enceladus advanced towards us, 98 00:05:35,920 --> 00:05:38,550 our galaxy's superior gravity grabbed 99 00:05:38,650 --> 00:05:40,520 hold of the smaller galaxy. 100 00:05:41,990 --> 00:05:44,530 As it approached, the gravity from the Milky Way 101 00:05:44,630 --> 00:05:46,330 would have stretched it out. 102 00:05:47,700 --> 00:05:52,000 Gaia-Enceladus was distorted but not defeated. 103 00:05:52,100 --> 00:05:54,840 The battle was just beginning. 104 00:05:54,940 --> 00:05:56,640 It would have passed through our galaxy, 105 00:05:56,740 --> 00:05:59,810 maybe orbiting a couple of times before being torn 106 00:05:59,910 --> 00:06:03,280 apart by our gravity. 107 00:06:04,980 --> 00:06:07,180 The Milky Way's gravitational power 108 00:06:07,280 --> 00:06:10,250 ripped Gaia-Enceladus apart 109 00:06:10,350 --> 00:06:12,850 and captured billions of its stars. 110 00:06:15,120 --> 00:06:17,190 Eventually, most of those stars would have 111 00:06:17,290 --> 00:06:18,730 then settled down into 112 00:06:18,830 --> 00:06:21,800 the disk of the Milky Way and become a part of it. 113 00:06:21,900 --> 00:06:24,230 Little galaxy try to take on the Milky Way... 114 00:06:24,330 --> 00:06:25,810 You're gonna get what's coming to you. 115 00:06:27,040 --> 00:06:28,640 Despite winning the battle, 116 00:06:28,740 --> 00:06:32,010 the Milky Way suffered serious damage. 117 00:06:33,580 --> 00:06:35,310 The collision with the Sausage Galaxy 118 00:06:35,410 --> 00:06:37,250 left a scar on the Milky Way. 119 00:06:37,380 --> 00:06:39,310 And when we look near the center of our galaxy, 120 00:06:39,380 --> 00:06:43,950 we see a bulge that's left over from that collision. 121 00:06:44,050 --> 00:06:48,020 The Milky Way isn't the only galaxy scarred by war. 122 00:06:49,790 --> 00:06:51,030 Across the universe, 123 00:06:51,130 --> 00:06:57,200 rival armies made up of billions of stars slug it out, 124 00:06:57,300 --> 00:07:02,270 leaving behind distorted and damaged casualties of war. 125 00:07:04,370 --> 00:07:05,450 There's a million different 126 00:07:05,540 --> 00:07:06,940 sub-categories of them. 127 00:07:07,040 --> 00:07:09,610 There's tadpole galaxies that have long tails, 128 00:07:09,710 --> 00:07:11,450 longer than our own galaxy. 129 00:07:11,550 --> 00:07:14,380 There are things like Arp-Madore 2026, where you see 130 00:07:14,480 --> 00:07:16,050 this eerie, glowing face, 131 00:07:16,150 --> 00:07:19,920 two big eyes looking right at you from across the universe. 132 00:07:20,020 --> 00:07:22,266 There are galaxies that looked like they might have collided 133 00:07:22,290 --> 00:07:24,860 with one another and blown holes through each other. 134 00:07:28,030 --> 00:07:30,670 These battle scars give us important clues 135 00:07:30,770 --> 00:07:34,440 about one of the biggest mysteries in astronomy... 136 00:07:34,540 --> 00:07:36,970 How galaxies develop and grow. 137 00:07:38,410 --> 00:07:40,540 But there's a problem. 138 00:07:40,640 --> 00:07:44,510 We can't watch these battles in real time. 139 00:07:44,610 --> 00:07:47,250 The scale of galaxies is huge. 140 00:07:47,350 --> 00:07:49,356 They're hundreds of thousands of light years across. 141 00:07:49,380 --> 00:07:50,660 It's going to take them millions 142 00:07:50,690 --> 00:07:52,590 or billions of years to come together. 143 00:07:53,890 --> 00:07:56,220 So it's like looking at one frame 144 00:07:56,330 --> 00:07:58,630 from a really energetic fight scene in a movie. 145 00:08:00,200 --> 00:08:02,260 By piecing these snapshots together, 146 00:08:02,360 --> 00:08:06,330 astronomers can build up a detailed picture of past 147 00:08:06,440 --> 00:08:10,540 conflicts and discover how these battles transformed 148 00:08:10,640 --> 00:08:13,640 galaxies over billions of years. 149 00:08:13,740 --> 00:08:16,380 We have pictures of isolated galaxies, 150 00:08:16,480 --> 00:08:18,380 we have pictures of interacting galaxies, 151 00:08:18,480 --> 00:08:21,150 and we have pictures of aftermath galaxies. 152 00:08:22,520 --> 00:08:26,220 And that's helped us discover something alarming. 153 00:08:26,320 --> 00:08:30,360 The Milky Way faces yet another attack from 154 00:08:30,460 --> 00:08:34,930 an enemy armed with an enormous secret weapon. 155 00:08:35,030 --> 00:08:38,330 Will our solar system survive the onslaught? 156 00:08:50,150 --> 00:08:51,610 Across the universe, 157 00:08:51,710 --> 00:08:53,610 galaxies are at war, 158 00:08:55,780 --> 00:08:57,490 Their main weapon... 159 00:08:57,590 --> 00:08:59,050 Gravity. 160 00:08:59,150 --> 00:09:03,590 It tears the combatants into weird and wonderful shapes. 161 00:09:03,690 --> 00:09:07,660 Our galaxy didn't escape the mayhem. 162 00:09:07,760 --> 00:09:10,060 It's peppered with battle scars. 163 00:09:12,370 --> 00:09:13,730 The overall shape of the Milky Way 164 00:09:13,840 --> 00:09:16,470 is a flat disk of stars and gas. 165 00:09:16,570 --> 00:09:20,110 Except recently, we have found out that at the edges, 166 00:09:20,210 --> 00:09:23,480 it's actually warped a little bit like the brim of a fedora. 167 00:09:23,580 --> 00:09:26,310 The stars actually dip down below the plane on 168 00:09:26,380 --> 00:09:29,820 one side and dip above it on the other. 169 00:09:29,920 --> 00:09:32,590 We think the attacker was one of our satellites, 170 00:09:32,690 --> 00:09:36,490 a galaxy that orbits the Milky Way like the moon 171 00:09:36,590 --> 00:09:38,030 orbits the Earth. 172 00:09:38,130 --> 00:09:42,230 It's called the Sagittarius Dwarf Galaxy. 173 00:09:42,330 --> 00:09:45,200 From looking at how the stars move in the Milky Way, 174 00:09:45,300 --> 00:09:48,640 we suspect that the Sagittarius Dwarf Galaxy has 175 00:09:48,740 --> 00:09:52,010 actually crashed through the Milky Way a few times on 176 00:09:52,110 --> 00:09:54,540 its course of its orbit around the galaxy. 177 00:09:54,640 --> 00:09:56,440 It came in about six billion years ago, 178 00:09:56,550 --> 00:09:59,350 hit the disk hard about two billion years ago, and crashed 179 00:09:59,450 --> 00:10:01,580 again about a billion years ago. 180 00:10:01,680 --> 00:10:04,620 And our gravity has pulled it out into a gigantic, 181 00:10:04,720 --> 00:10:07,520 looping stream of stars that is moving in and out 182 00:10:07,620 --> 00:10:09,320 of our Milky Way. 183 00:10:11,390 --> 00:10:13,190 The war is not over. 184 00:10:13,300 --> 00:10:16,700 The insurgent galaxy will return. 185 00:10:16,800 --> 00:10:19,700 When galaxies interact, 186 00:10:19,800 --> 00:10:22,470 often they're caught in this huge cosmic dance 187 00:10:22,570 --> 00:10:25,010 where they revolve around each other a few times, 188 00:10:25,110 --> 00:10:27,480 or they even crash through each other and then come 189 00:10:27,580 --> 00:10:28,580 back around. 190 00:10:28,610 --> 00:10:30,610 The Sagittarius Dwarf Galaxy looks like 191 00:10:30,710 --> 00:10:34,380 it's crashing in with ever increasing frequency. 192 00:10:34,480 --> 00:10:37,590 A new skirmish could take place in the next 193 00:10:37,690 --> 00:10:40,050 100 million years. 194 00:10:40,160 --> 00:10:44,060 So should we be worried about these attacks? 195 00:10:44,160 --> 00:10:46,990 Because the Sagittarius Dwarf Galaxy is so small 196 00:10:47,100 --> 00:10:48,460 compared to the Milky Way, 197 00:10:48,560 --> 00:10:50,500 it will do some damage at the beginning, 198 00:10:50,600 --> 00:10:54,570 but because we're so massive, we can absorb the impact. 199 00:10:54,670 --> 00:10:56,970 I mean, this galaxy, it's looking for a fight, 200 00:10:57,070 --> 00:11:00,470 but it's also 10,000 times smaller than us. 201 00:11:00,580 --> 00:11:02,640 So this is gonna be no sweat at all. 202 00:11:06,250 --> 00:11:09,350 So far, the Milky Way has been victorious. 203 00:11:10,790 --> 00:11:12,820 But the danger isn't over. 204 00:11:14,390 --> 00:11:17,290 We are surrounded by enemies. 205 00:11:17,390 --> 00:11:19,260 Our local neighborhood of galaxies 206 00:11:19,360 --> 00:11:21,560 has three major galaxies, 207 00:11:21,660 --> 00:11:24,600 but up to 50 smaller ones. 208 00:11:24,700 --> 00:11:28,440 All these galaxies are potential troublemakers. 209 00:11:28,540 --> 00:11:32,140 Each one of these could be armies that rise up against us. 210 00:11:33,810 --> 00:11:36,280 The two most famous galaxies that orbit 211 00:11:36,380 --> 00:11:39,880 the Milky Way are the Large and Small Magellanic Clouds. 212 00:11:39,980 --> 00:11:43,380 These are two independent dwarf galaxies that you can 213 00:11:43,490 --> 00:11:45,990 see in the night sky from the Southern Hemisphere. 214 00:11:50,060 --> 00:11:53,330 We thought the Large Magellanic Cloud orbited 215 00:11:53,430 --> 00:11:58,500 our galaxy at a safe distance of 160,000 light years. 216 00:11:59,740 --> 00:12:01,170 We thought it would stay that way, 217 00:12:01,270 --> 00:12:04,040 and we thought it was harmless. 218 00:12:04,140 --> 00:12:09,110 Now, a new discovery shows we were wrong on all counts. 219 00:12:10,550 --> 00:12:14,280 The new factor that changed our view of the Magellanic Cloud 220 00:12:14,380 --> 00:12:15,380 is we found out 221 00:12:15,450 --> 00:12:18,120 it has a lot more dark matter than we thought. 222 00:12:20,090 --> 00:12:21,690 Dark matter, 223 00:12:21,790 --> 00:12:25,330 the most mysterious stuff in the universe. 224 00:12:25,430 --> 00:12:29,000 A dark matter is literally what it sounds like. 225 00:12:29,100 --> 00:12:30,660 It's matter that we cannot see. 226 00:12:30,770 --> 00:12:32,900 But it has gravity and can affect objects 227 00:12:33,000 --> 00:12:34,300 that we can see. 228 00:12:37,610 --> 00:12:41,010 Adding in this extra dark matter makes the Large 229 00:12:41,110 --> 00:12:45,710 Magellanic Cloud at least twice a massive as predicted. 230 00:12:45,810 --> 00:12:48,980 So its gravity is double what we thought. 231 00:12:50,550 --> 00:12:53,090 It's secretly been gathering 232 00:12:53,190 --> 00:12:57,460 allies, has been gathering dark matter on its side, 233 00:12:57,560 --> 00:13:00,860 and now it's a much bigger threat than we thought before. 234 00:13:02,430 --> 00:13:04,270 So it's not just going to orbit us. 235 00:13:04,370 --> 00:13:06,070 It's gonna collide with the Milky Way. 236 00:13:07,740 --> 00:13:10,540 Moving at nearly a million miles an hour, 237 00:13:10,640 --> 00:13:15,240 the Large Magellanic Cloud will not swing past us. 238 00:13:15,340 --> 00:13:17,550 It will attack. 239 00:13:17,650 --> 00:13:20,010 The large Magellanic Cloud is 240 00:13:20,120 --> 00:13:23,380 1/10 the mass of the Milky Way. 241 00:13:23,490 --> 00:13:26,320 That's enough to make a pretty big punch. 242 00:13:28,120 --> 00:13:30,090 In about 2.5 billion years, 243 00:13:30,190 --> 00:13:32,790 it will smash into our galaxy. 244 00:13:36,100 --> 00:13:39,230 It's gonna plow through the disk of the Milky Way, 245 00:13:39,330 --> 00:13:40,840 it's gonna blow a cavity. 246 00:13:40,940 --> 00:13:43,640 It might even damage our spiral arms. 247 00:13:46,010 --> 00:13:49,340 Earth sits in one of those spiral arms. 248 00:13:51,610 --> 00:13:54,380 Could our planet become collateral damage? 249 00:13:55,850 --> 00:13:58,450 If the Large Magellanic Cloud passes through the plane 250 00:13:58,550 --> 00:14:01,260 of our galaxy near our location, 251 00:14:01,360 --> 00:14:03,320 that can have dire consequences. 252 00:14:05,030 --> 00:14:07,090 The gravitational clash between 253 00:14:07,200 --> 00:14:09,160 the invader on the Milky Way 254 00:14:09,260 --> 00:14:12,370 could hurl stars and planets out of our galaxy. 255 00:14:14,240 --> 00:14:16,100 Earth could be one of them. 256 00:14:17,740 --> 00:14:20,540 Our planet's very close to its own star, 257 00:14:20,640 --> 00:14:23,840 so the odds are that you'll just get ripped out 258 00:14:23,950 --> 00:14:25,110 along with your star, 259 00:14:25,210 --> 00:14:28,150 so we'd be moving along with the sun even as the sun gets 260 00:14:28,250 --> 00:14:30,890 jettisoned from our galaxy. 261 00:14:30,990 --> 00:14:33,720 And it'll move off out into intergalactic space. 262 00:14:33,820 --> 00:14:35,520 And that's not terrible. 263 00:14:35,620 --> 00:14:37,390 I mean, it's not gonna get destroyed, 264 00:14:37,490 --> 00:14:38,730 but it's a little lonely. 265 00:14:42,030 --> 00:14:44,500 Our view of the night sky 266 00:14:44,600 --> 00:14:46,000 would radically change. 267 00:14:47,600 --> 00:14:50,470 We'd be able to see much more of the Milky Way, 268 00:14:50,570 --> 00:14:54,240 especially if we got kicked up above the plane of the galaxy. 269 00:14:54,340 --> 00:14:56,810 We'd be able to see the whole shebang. 270 00:14:56,910 --> 00:15:00,550 Just look at any image of a spiral galaxy. 271 00:15:00,650 --> 00:15:03,780 They're gorgeous. Now imagine seeing your night 272 00:15:03,890 --> 00:15:07,350 sky filled with a face-on spiral galaxy. 273 00:15:07,460 --> 00:15:09,920 That would be like waking up to my face 274 00:15:10,030 --> 00:15:12,830 every morning... spectacular. 275 00:15:17,470 --> 00:15:19,970 If we were unlucky, 276 00:15:20,070 --> 00:15:21,640 our home planet could have 277 00:15:21,740 --> 00:15:25,040 a close encounter with an invading star. 278 00:15:25,140 --> 00:15:28,940 The odds are very low that another star 279 00:15:29,040 --> 00:15:30,740 will pass close by the sun, 280 00:15:30,850 --> 00:15:32,780 but those odds aren't zero. 281 00:15:32,880 --> 00:15:34,580 It could happen that another star 282 00:15:34,680 --> 00:15:36,750 passes close enough to affect the planets. 283 00:15:36,850 --> 00:15:38,520 And if that were to happen, 284 00:15:38,620 --> 00:15:43,560 it could upset the delicate balance in the solar system. 285 00:15:44,590 --> 00:15:47,800 We don't know where the Earth could end up. 286 00:15:47,900 --> 00:15:49,860 It might find its way into the sun. 287 00:15:49,970 --> 00:15:51,000 You just don't know. 288 00:15:51,100 --> 00:15:52,870 Or there might just be a rain 289 00:15:52,970 --> 00:15:55,400 of comets into our inner solar system. 290 00:15:55,500 --> 00:15:57,940 Our own planet might be flung out, 291 00:15:58,040 --> 00:16:01,240 in which case, this would be a death knell for all life 292 00:16:01,340 --> 00:16:02,580 on Earth. 293 00:16:02,680 --> 00:16:05,280 I'm not someone who is like a doom and gloom person, 294 00:16:05,380 --> 00:16:07,180 but, like, that would be insane. 295 00:16:08,520 --> 00:16:10,080 You don't know what's gonna happen, 296 00:16:10,190 --> 00:16:13,350 but most of the options are bad. 297 00:16:13,460 --> 00:16:16,660 All these nightmare scenarios 298 00:16:16,760 --> 00:16:18,490 will extinguish life. 299 00:16:22,130 --> 00:16:25,000 Earth might survive, but our cosmic 300 00:16:25,100 --> 00:16:27,630 zip code will take a severe beating. 301 00:16:29,240 --> 00:16:31,440 The Milky Way Galaxy is bigger than 302 00:16:31,540 --> 00:16:32,640 the Large Magellanic Cloud, 303 00:16:32,710 --> 00:16:35,440 so we are gonna win, [exhales heavily] 304 00:16:35,540 --> 00:16:37,340 but it's gonna hurt us for a long time. 305 00:16:39,050 --> 00:16:40,610 The Large Magellanic Cloud 306 00:16:40,720 --> 00:16:42,680 will leave our galaxy battered, 307 00:16:42,780 --> 00:16:45,750 bruised, but ultimately undefeated. 308 00:16:45,850 --> 00:16:49,760 But there's a far bigger threat looming 309 00:16:49,860 --> 00:16:51,590 over the Milky Way. 310 00:16:51,690 --> 00:16:54,630 It's gonna face an opponent that it can't defeat. 311 00:16:56,000 --> 00:16:58,200 Will this mega collision be 312 00:16:58,300 --> 00:17:00,600 the Milky Way's last stand? 313 00:17:11,650 --> 00:17:13,150 For billions of years, 314 00:17:13,250 --> 00:17:16,250 the Milky Way conquered galaxy after galaxy, 315 00:17:16,350 --> 00:17:19,850 tearing its smaller rivals to pieces. 316 00:17:21,120 --> 00:17:24,090 But our galaxy is about to meet its match. 317 00:17:27,130 --> 00:17:31,100 In the not-too-distant future, galactically speaking, 318 00:17:31,200 --> 00:17:34,840 a much, much larger battle is due for the Milky Way. 319 00:17:36,540 --> 00:17:38,940 A battle with a local superpower, 320 00:17:40,240 --> 00:17:41,540 the Andromeda Galaxy. 321 00:17:43,110 --> 00:17:46,750 We thought this huge galaxy might wound us in the future. 322 00:17:48,180 --> 00:17:51,720 Now, recent evidence reveals it's going to make 323 00:17:51,820 --> 00:17:54,490 a full-scale assault. 324 00:17:54,590 --> 00:17:58,130 We've known for a long time that Andromeda is heading 325 00:17:58,230 --> 00:18:00,390 more or less toward us, 326 00:18:00,500 --> 00:18:02,860 but we didn't know exactly in what direction. 327 00:18:02,960 --> 00:18:04,570 But in recent years, we've been 328 00:18:04,670 --> 00:18:06,670 able to pinpoint this a lot better. 329 00:18:06,770 --> 00:18:10,370 And, uh, yeah, it's... It's heading right for us. 330 00:18:13,110 --> 00:18:16,180 Data from the Hubble Space Telescope shows 331 00:18:16,280 --> 00:18:20,180 two galaxies will collide in about four billion years, 332 00:18:23,020 --> 00:18:26,890 and it will be a monumental battle. 333 00:18:26,990 --> 00:18:30,890 This collision that is coming, and it is coming, is not gonna 334 00:18:30,990 --> 00:18:33,430 be anything like the Milky Way has experienced before 335 00:18:33,530 --> 00:18:35,630 in its 10- or 12-billion-year history. 336 00:18:35,730 --> 00:18:38,330 This is a galaxy of comparable size. 337 00:18:38,430 --> 00:18:42,740 This is two heavyweight prize fighters coming at it. 338 00:18:42,840 --> 00:18:46,940 Warriors with the same gravitational firepower. 339 00:18:47,040 --> 00:18:50,810 Simulations suggest a clash of the Titans. 340 00:18:50,910 --> 00:18:53,350 Each of them with half a trillion stars in them. 341 00:18:53,450 --> 00:18:55,920 That sounds like a pretty spectacular collision. 342 00:18:57,990 --> 00:19:00,920 Fights between equally matched galaxies 343 00:19:01,020 --> 00:19:03,520 are rare and messy. 344 00:19:03,630 --> 00:19:05,590 When the battle kicks off, 345 00:19:05,690 --> 00:19:08,600 there will be no good news for either side. 346 00:19:10,770 --> 00:19:13,400 When the Andromeda Galaxy and the Milky Way Galaxy 347 00:19:13,500 --> 00:19:14,870 start to get close, 348 00:19:14,970 --> 00:19:16,540 they're gonna start affecting each 349 00:19:16,640 --> 00:19:17,700 other profoundly. 350 00:19:17,810 --> 00:19:20,070 Tendrils of stars are gonna be thrown out. 351 00:19:20,180 --> 00:19:23,980 Gas is gonna be thrown out. 352 00:19:24,080 --> 00:19:26,580 It won't be a single impact. 353 00:19:26,680 --> 00:19:29,620 Gravity will send the two opponents 354 00:19:29,720 --> 00:19:32,450 into a spiraling dance of death. 355 00:19:34,620 --> 00:19:36,890 The first pass is actually not a direct hit. 356 00:19:36,990 --> 00:19:39,690 They're gonna swing past each other, in fact. 357 00:19:39,790 --> 00:19:42,200 And at this point, their gravitational 358 00:19:42,300 --> 00:19:43,800 interaction is gonna slow them down, 359 00:19:43,900 --> 00:19:46,030 and they're gonna come back toward each other. 360 00:19:46,130 --> 00:19:49,670 The galaxies will collide and fly apart again, 361 00:19:49,770 --> 00:19:54,310 inflicting more and more damage with each clash. 362 00:19:54,410 --> 00:19:56,940 If you were to go outside and look up, 363 00:19:57,050 --> 00:20:00,050 you could see the disk of our galaxy getting ripped apart 364 00:20:00,150 --> 00:20:02,320 by tidal interactions with Andromeda. 365 00:20:05,990 --> 00:20:09,320 The two beautiful spiral galaxies 366 00:20:09,420 --> 00:20:11,730 will tear each other apart, 367 00:20:11,830 --> 00:20:16,360 leaving one vast elliptical galaxy. 368 00:20:18,300 --> 00:20:21,370 The fate of the Andromeda, Milky Way 369 00:20:21,470 --> 00:20:24,710 battle is that they will merge. 370 00:20:24,810 --> 00:20:28,410 This is going to be one gigantic galaxy. 371 00:20:31,480 --> 00:20:32,750 And that presents a problem. 372 00:20:32,850 --> 00:20:34,510 What are we gonna call this new galaxy? 373 00:20:34,620 --> 00:20:37,580 Of course, my nerd colleagues have come up with 374 00:20:37,690 --> 00:20:40,520 names like Milkomeda, Andromeway. 375 00:20:40,620 --> 00:20:42,760 Whatever, those are corny. 376 00:20:42,860 --> 00:20:44,890 We should just call it Hakeem. 377 00:20:50,970 --> 00:20:53,500 With a trillion stars, it will be 378 00:20:53,600 --> 00:20:56,440 one of the biggest galaxies in the universe. 379 00:20:58,970 --> 00:21:00,140 In the Hakeem Galaxy, 380 00:21:00,240 --> 00:21:02,280 things gonna be completely new. 381 00:21:02,380 --> 00:21:05,680 First off, it's gonna be a really good-looking galaxy. 382 00:21:05,780 --> 00:21:07,510 Let's get that straight from the get-go. 383 00:21:07,620 --> 00:21:12,650 Second, it's gonna be powerful, and I'm talking powerful. 384 00:21:12,750 --> 00:21:14,390 This may be the most remarkable 385 00:21:14,490 --> 00:21:16,590 galaxy in the history of the universe. 386 00:21:19,130 --> 00:21:23,100 Milkomeda, or Hakeem, if you prefer, 387 00:21:23,200 --> 00:21:26,570 will become the undisputed boss of our cosmic neighborhood. 388 00:21:26,630 --> 00:21:30,140 It's calm appearance concealing 389 00:21:30,240 --> 00:21:31,810 a history of violence. 390 00:21:34,840 --> 00:21:37,980 It's the result of a complete war zone of mergers over 391 00:21:38,080 --> 00:21:39,326 the course of billions of years, 392 00:21:39,350 --> 00:21:42,350 many galaxies crashing together, fully reconfiguring 393 00:21:42,450 --> 00:21:44,520 each time and slowly, you grow 394 00:21:44,620 --> 00:21:48,190 this smooth, placid, big blob of stars. 395 00:21:50,260 --> 00:21:53,090 After billions of years of warfare, 396 00:21:53,190 --> 00:21:56,160 our galaxy will finally be peaceful. 397 00:21:58,770 --> 00:22:02,600 But before it's honorable discharge, Milkomeda 398 00:22:02,700 --> 00:22:04,770 may produce one final, 399 00:22:04,870 --> 00:22:07,640 devastating act of war. 400 00:22:07,740 --> 00:22:11,910 Imagine World War II, and then all of a sudden, 401 00:22:12,010 --> 00:22:14,880 one of the sides comes up with the Death Star. 402 00:22:14,980 --> 00:22:16,520 That's what we're talking about here. 403 00:22:19,090 --> 00:22:21,420 A weapon of cosmic destruction. 404 00:22:37,810 --> 00:22:40,040 When giant galaxies clash, 405 00:22:40,140 --> 00:22:43,110 the battles are spectacular and destructive. 406 00:22:46,280 --> 00:22:50,420 The victors steal huge numbers of stars and vast amounts 407 00:22:50,520 --> 00:22:55,290 of gas as fuel for the ultimate super weapon. 408 00:22:57,360 --> 00:23:00,230 The special weapon that these monster galaxies 409 00:23:00,330 --> 00:23:03,460 have is a giant Death Ray, 410 00:23:03,560 --> 00:23:08,440 a jet of material racing across thousands of light-years. 411 00:23:10,840 --> 00:23:13,540 These huge outbursts of energy blast out 412 00:23:13,640 --> 00:23:16,710 of the center of the colliding galaxies. 413 00:23:16,810 --> 00:23:20,050 They produce more energy in one second than 414 00:23:20,150 --> 00:23:25,190 the sun will in its entire 10-billion-year lifetime. 415 00:23:25,290 --> 00:23:27,220 We call them jets. 416 00:23:28,990 --> 00:23:33,160 These incredibly powerful jets aren't just brief features. 417 00:23:33,260 --> 00:23:36,400 They can be sustained for millions of years, 418 00:23:36,500 --> 00:23:38,570 and they can maintain their structure 419 00:23:38,670 --> 00:23:41,500 for thousands of light-years. 420 00:23:41,600 --> 00:23:43,470 It's like turning on a garden hose 421 00:23:43,570 --> 00:23:45,870 in Chicago and using it to water 422 00:23:45,970 --> 00:23:47,610 a garden in London. 423 00:23:49,580 --> 00:23:52,580 Exactly what triggered these jets was a mystery. 424 00:23:52,680 --> 00:23:57,120 Then, in June 2018, astronomers in Hawaii captured 425 00:23:57,220 --> 00:24:00,350 something stunning... A jet forming 426 00:24:00,460 --> 00:24:02,860 during a galactic collision. 427 00:24:05,430 --> 00:24:07,590 The team found something really incredible. 428 00:24:07,700 --> 00:24:11,030 They found two galaxies that were in a cosmic collision 429 00:24:11,130 --> 00:24:14,330 and actually found an active jet in one of these galaxies. 430 00:24:14,440 --> 00:24:16,840 It was the first time anything like this has been discovered. 431 00:24:20,340 --> 00:24:23,980 When galaxies collide, the clash drives huge clouds 432 00:24:24,080 --> 00:24:27,480 of gas and dust towards their centers. 433 00:24:27,580 --> 00:24:31,180 The supermassive black holes start to feed. 434 00:24:33,390 --> 00:24:35,590 The gas that was in those galaxies starts to 435 00:24:35,690 --> 00:24:39,390 funnel toward the black hole and then fall upon it. 436 00:24:39,490 --> 00:24:42,030 Not all this gas ends up inside 437 00:24:42,130 --> 00:24:44,160 the supermassive black hole. 438 00:24:44,270 --> 00:24:46,670 Powerful magnetic fields carry some of 439 00:24:46,770 --> 00:24:49,500 this matter to the poles 440 00:24:49,600 --> 00:24:52,740 and blast it out in tight, narrow jets. 441 00:24:52,840 --> 00:24:55,780 A super weapon is born. 442 00:24:55,880 --> 00:24:57,780 This discovery helps us understand 443 00:24:57,880 --> 00:25:01,850 how giant elliptical galaxies form. 444 00:25:01,950 --> 00:25:05,520 Knowing that mergers of spiral galaxies can cause 445 00:25:05,650 --> 00:25:07,220 these jets helps us put together 446 00:25:07,320 --> 00:25:09,820 a complete picture of how these huge elliptical 447 00:25:09,920 --> 00:25:11,420 galaxies might be formed. 448 00:25:14,430 --> 00:25:18,230 The discovery doesn't answer all our questions. 449 00:25:18,330 --> 00:25:19,630 There's another mystery. 450 00:25:19,730 --> 00:25:21,970 How did the super giant galaxies that 451 00:25:22,070 --> 00:25:25,070 dwarf the Milky Way get so big? 452 00:25:25,170 --> 00:25:29,380 Our Milky Way Galaxy is big-ish. 453 00:25:29,480 --> 00:25:31,550 It's... it's slightly bigger than average, 454 00:25:31,650 --> 00:25:33,880 but IC 1101, for example, 455 00:25:33,980 --> 00:25:37,650 is more than 50 times larger than our home galaxy and has 456 00:25:37,750 --> 00:25:42,020 more than a trillion, with a T, a trillion stars in it. 457 00:25:42,120 --> 00:25:47,190 The biggest galaxies make the Milky Way look like an ant. 458 00:25:47,300 --> 00:25:50,900 These galactic giants pose a problem. 459 00:25:51,000 --> 00:25:53,500 There hasn't been enough time since the birth of 460 00:25:53,600 --> 00:25:57,740 the universe for them to become so large, 461 00:25:57,840 --> 00:26:00,110 even by conquering smaller galaxies. 462 00:26:00,210 --> 00:26:03,240 When we look into the distant universe, 463 00:26:03,340 --> 00:26:06,550 we see something very strange that we don't quite understand. 464 00:26:06,650 --> 00:26:09,620 We see enormous galaxies that existed just 465 00:26:09,720 --> 00:26:11,520 a billion years after the Big Bang. 466 00:26:11,620 --> 00:26:14,650 And even though these cosmic collisions help explain how 467 00:26:14,760 --> 00:26:16,020 galaxies get bigger, 468 00:26:16,120 --> 00:26:18,960 they don't quite explain everything about how galaxies 469 00:26:19,060 --> 00:26:20,090 grow over time. 470 00:26:20,190 --> 00:26:22,360 So we still have a big mystery on our hands here. 471 00:26:26,230 --> 00:26:29,800 So in 2019, an international team 472 00:26:29,900 --> 00:26:32,370 investigated a very large galaxy 473 00:26:32,470 --> 00:26:35,410 over 300 million light-years away. 474 00:26:35,510 --> 00:26:39,610 We call it NGC 6240. 475 00:26:39,710 --> 00:26:43,120 NGC 6240 was being studied because 476 00:26:43,220 --> 00:26:45,790 it had two supermassive black holes in it. 477 00:26:45,890 --> 00:26:48,090 Now the galaxy itself looked like it 478 00:26:48,160 --> 00:26:50,160 had been disturbed, like something had happened. 479 00:26:50,260 --> 00:26:53,730 They thought that potentially it had had a recent merger. 480 00:26:59,300 --> 00:27:01,270 They were expecting to see two 481 00:27:01,370 --> 00:27:05,270 supermassive black holes in the galaxy's heart. 482 00:27:05,370 --> 00:27:08,270 As the researchers peered through the layers of gas 483 00:27:08,380 --> 00:27:12,450 and dust, they discovered something surprising. 484 00:27:12,550 --> 00:27:14,710 What we found was staggering. 485 00:27:14,820 --> 00:27:17,380 We found not two but three 486 00:27:17,490 --> 00:27:20,250 supermassive black holes lurking in the center. 487 00:27:26,630 --> 00:27:27,830 It's the first time we found 488 00:27:27,930 --> 00:27:32,430 a galaxy with three supermassive black holes, 489 00:27:32,530 --> 00:27:36,000 evidence of a three-galaxy pile up. 490 00:27:36,100 --> 00:27:40,140 This galaxy is an active battlefield of 491 00:27:40,240 --> 00:27:46,110 not two but three armies colliding at once, 492 00:27:46,210 --> 00:27:47,950 and because there are three armies involved, 493 00:27:48,050 --> 00:27:50,180 there are three galaxies involved with 494 00:27:50,280 --> 00:27:53,520 three times as much mass, three times as many stars, 495 00:27:53,620 --> 00:27:56,220 three times as much material, and three times as 496 00:27:56,320 --> 00:27:58,490 much violence. 497 00:27:58,590 --> 00:28:01,460 This three-way battle may explain how 498 00:28:01,560 --> 00:28:06,270 the largest galaxies got so big so fast. 499 00:28:06,370 --> 00:28:08,130 It could be that galaxy mergers 500 00:28:08,240 --> 00:28:11,140 are more frequent than what we thought previously, 501 00:28:11,240 --> 00:28:14,740 and therefore, galaxies become more massive 502 00:28:14,840 --> 00:28:16,880 faster than previously expected. 503 00:28:18,910 --> 00:28:21,050 In the past, galaxies may have 504 00:28:21,150 --> 00:28:24,420 battled and collided more often than today. 505 00:28:24,520 --> 00:28:28,250 Back then, galaxies were more densely packed together. 506 00:28:29,820 --> 00:28:33,330 Our universe is expanding as it ages, which means in 507 00:28:33,430 --> 00:28:35,430 the past, all the galaxies in 508 00:28:35,530 --> 00:28:37,930 the universe were closer together, 509 00:28:38,030 --> 00:28:40,030 and that means they had greater chance for their 510 00:28:40,130 --> 00:28:41,630 gravitational interactions to 511 00:28:41,740 --> 00:28:43,940 pull them together and smash them together. 512 00:28:46,610 --> 00:28:49,610 The early universe was at war. 513 00:28:49,710 --> 00:28:52,650 Conflicts between galaxies were common. 514 00:28:52,750 --> 00:28:56,220 They collided frequently and grew quickly. 515 00:28:57,790 --> 00:29:01,820 But not every galaxy profited from the carnage. 516 00:29:01,920 --> 00:29:04,690 Some brave galaxies took on the big guns 517 00:29:04,790 --> 00:29:06,760 and nearly died as a result. 518 00:29:21,540 --> 00:29:24,180 When galaxies fight, the big get bigger. 519 00:29:24,280 --> 00:29:28,410 More mass means more gravity, the vital ingredient 520 00:29:28,520 --> 00:29:29,650 for victory. 521 00:29:31,820 --> 00:29:36,020 But galactic conflict doesn't always result in growth. 522 00:29:36,120 --> 00:29:39,790 A strange new astronomical object had 523 00:29:39,890 --> 00:29:41,260 scientists confused. 524 00:29:44,430 --> 00:29:46,730 They just looked like stars from the ground. 525 00:29:46,830 --> 00:29:50,170 However, with the advent of Hubble and beautiful 526 00:29:50,270 --> 00:29:51,970 space-based telescopes, 527 00:29:52,070 --> 00:29:56,080 it was possible to look at these stars again and actually 528 00:29:56,180 --> 00:29:58,040 discover that they were galaxies. 529 00:30:03,280 --> 00:30:04,650 They're kind of crazy. 530 00:30:04,750 --> 00:30:09,820 They're a huge number of stars, but crammed into an incredibly 531 00:30:09,920 --> 00:30:12,030 tiny space on an astrophysical scale, 532 00:30:12,130 --> 00:30:16,460 something 500 times smaller than our Milky Way Galaxy. 533 00:30:16,560 --> 00:30:20,400 We call them ultra-compact dwarf galaxies, 534 00:30:20,500 --> 00:30:21,840 or UCDs. 535 00:30:23,270 --> 00:30:25,770 You might imagine the difference between 536 00:30:25,870 --> 00:30:29,980 the Milky Way Galaxy and a UCD as 537 00:30:30,080 --> 00:30:33,280 the difference between a cloud and a rock, 538 00:30:33,380 --> 00:30:36,720 where the rock is just the same kind of material, 539 00:30:36,820 --> 00:30:39,250 but compressed to just incredibly high densities 540 00:30:39,350 --> 00:30:41,590 compared to some fluffy gaseous thing. 541 00:30:44,590 --> 00:30:46,860 What are these strange galaxies? 542 00:30:46,960 --> 00:30:49,560 They seem to break all the rules. 543 00:30:49,660 --> 00:30:53,000 To find out, astronomers zoomed in to 544 00:30:53,100 --> 00:30:54,700 a particularly dense, 545 00:30:54,800 --> 00:30:57,340 ultra-compact dwarf galaxy 546 00:30:57,440 --> 00:31:00,740 called M60-UCD1. 547 00:31:02,010 --> 00:31:05,980 M60-UCD1 is 300 light-years across. 548 00:31:06,080 --> 00:31:08,010 It's tiny. It's a pinpoint compared to 549 00:31:08,120 --> 00:31:09,450 our enormous galaxy. 550 00:31:09,550 --> 00:31:13,020 Our galaxy has 200 or more billion stars in it. 551 00:31:13,120 --> 00:31:16,390 And M60-UCD1 only has 140 million. 552 00:31:16,490 --> 00:31:20,390 But they're packed into this incredibly tight volume. 553 00:31:20,490 --> 00:31:22,700 The night sky inside the galaxy 554 00:31:22,800 --> 00:31:25,570 would look very different from our own. 555 00:31:25,670 --> 00:31:28,030 On Earth, when you look at the night sky, 556 00:31:28,140 --> 00:31:30,370 you see a few thousand stars. 557 00:31:30,470 --> 00:31:32,770 But if you were in M60-UCD1, 558 00:31:32,870 --> 00:31:35,110 you wouldn't just see a few thousand stars. 559 00:31:35,210 --> 00:31:38,210 You would see hundreds of thousands of stars 560 00:31:38,310 --> 00:31:41,010 in the night sky. That would be amazing. 561 00:31:47,520 --> 00:31:49,290 As the astronomers look deeper 562 00:31:49,390 --> 00:31:51,930 into the heart of this tiny galaxy, 563 00:31:52,030 --> 00:31:55,230 Things got even weirder. 564 00:31:55,330 --> 00:31:58,930 They found a supermassive black hole much bigger 565 00:31:59,030 --> 00:32:01,300 than expected. 566 00:32:01,400 --> 00:32:05,840 It actually has a black hole that's bigger, five times bigger 567 00:32:05,940 --> 00:32:07,246 than the black hole at the center of 568 00:32:07,270 --> 00:32:09,210 our Milky Way Galaxy. 569 00:32:09,280 --> 00:32:12,810 When we see supermassive black holes inside of galaxies, 570 00:32:12,910 --> 00:32:16,220 they tend to scale with the size of the galaxy itself. 571 00:32:16,320 --> 00:32:19,990 A bigger galaxy has a bigger supermassive black hole. 572 00:32:20,090 --> 00:32:22,220 Why does such a tiny little object 573 00:32:22,320 --> 00:32:25,760 have such an oversized central black hole? 574 00:32:25,860 --> 00:32:27,960 The only possible explanation? 575 00:32:28,060 --> 00:32:32,700 This tiny galaxy was once much larger. 576 00:32:32,800 --> 00:32:35,770 These galaxies might have begun their lives as, in fact, 577 00:32:35,870 --> 00:32:37,840 much bigger galaxies. 578 00:32:37,940 --> 00:32:40,310 And that what we see today, it was really just the very 579 00:32:40,410 --> 00:32:43,310 central, densest part of a much larger galaxy 580 00:32:44,980 --> 00:32:48,310 Based on the size of its supermassive black hole, 581 00:32:48,380 --> 00:32:51,320 M60-UCD1 may once 582 00:32:51,420 --> 00:32:54,320 have contained many billions of stars. 583 00:32:54,420 --> 00:32:57,720 Something captured them, 584 00:32:57,830 --> 00:33:00,790 and we don't have to look far to find the aggressor... 585 00:33:00,890 --> 00:33:03,100 A nearby super galaxy with 586 00:33:03,200 --> 00:33:07,730 lots of gravitational firepower... M60. 587 00:33:07,840 --> 00:33:11,340 M60 is a monster. It has a trillion stars in it. 588 00:33:11,440 --> 00:33:12,710 It's bigger than the Milky Way, 589 00:33:12,810 --> 00:33:14,570 and we're pretty big. 590 00:33:14,680 --> 00:33:18,010 The battle was not a full-on frontal assault. 591 00:33:18,110 --> 00:33:23,380 M60 raided its smaller opponent, capturing its troops. 592 00:33:23,480 --> 00:33:26,690 This is more of a stealthy guerrilla hit and run 593 00:33:26,790 --> 00:33:28,290 where we're gonna move in, 594 00:33:28,390 --> 00:33:30,920 pick off some of your troops, and then get out 595 00:33:31,030 --> 00:33:33,530 before you even notice. 596 00:33:33,630 --> 00:33:36,660 All that's left from one of these drive-by 597 00:33:36,760 --> 00:33:38,030 galaxy interactions 598 00:33:38,130 --> 00:33:41,400 is this supermassive black hole with a fraction 599 00:33:41,500 --> 00:33:43,470 of its original stars. 600 00:33:43,570 --> 00:33:48,370 The conflict devastated M60-UCD1. 601 00:33:48,480 --> 00:33:51,980 Over 98% of its stellar army were captured 602 00:33:52,080 --> 00:33:54,450 and became prisoners of war. 603 00:33:54,550 --> 00:33:57,750 It used to be a big galaxy, 604 00:33:57,850 --> 00:34:00,220 but it suffered one too many defeats. 605 00:34:00,320 --> 00:34:02,620 And now it's a... It's a fallen empire. 606 00:34:02,720 --> 00:34:05,090 We can frame this battle 607 00:34:05,190 --> 00:34:09,100 between M60 and M60-UCD1 as just a battle. 608 00:34:09,200 --> 00:34:11,330 But in fact, it's a slaughter. 609 00:34:11,430 --> 00:34:13,430 It's a massacre. 610 00:34:13,530 --> 00:34:17,570 These small galaxies get all their troops removed, 611 00:34:17,670 --> 00:34:19,340 but the HQ, 612 00:34:19,440 --> 00:34:21,470 the supermassive black hole remains, 613 00:34:21,580 --> 00:34:24,310 but it doesn't have any troops left. 614 00:34:24,410 --> 00:34:28,050 Eventually, M60 will conquer its battered opponent, 615 00:34:28,150 --> 00:34:32,590 destroying what's left of the compact galaxy. 616 00:34:32,720 --> 00:34:34,320 It'll get ripped apart even further, 617 00:34:34,420 --> 00:34:36,520 and more and more stars will be consumed 618 00:34:36,620 --> 00:34:37,990 by the bigger galaxy. 619 00:34:38,090 --> 00:34:41,590 So chances are this little dwarf is eventually going to 620 00:34:41,700 --> 00:34:45,530 be pulled apart and become a part of M60. 621 00:34:45,630 --> 00:34:48,730 In the great game of galactic warfare, 622 00:34:48,840 --> 00:34:50,700 losing can be catastrophic. 623 00:34:50,800 --> 00:34:53,040 For weak and small galaxies, 624 00:34:53,110 --> 00:34:55,510 resistance is futile. 625 00:34:57,740 --> 00:35:00,550 Pillaged for resource is by their more powerful opponents, 626 00:35:00,650 --> 00:35:03,350 they slowly become burnt-out wrecks. 627 00:35:06,020 --> 00:35:11,020 But some peaceful galaxies face an equally terrible fate. 628 00:35:11,130 --> 00:35:12,930 They starve to death. 629 00:35:24,100 --> 00:35:26,240 Cosmic wars are vicious. 630 00:35:26,340 --> 00:35:29,210 They destroy many galaxies, 631 00:35:29,310 --> 00:35:33,480 but violent conflicts can also give galaxies new life. 632 00:35:35,380 --> 00:35:36,280 Case in point, 633 00:35:36,380 --> 00:35:40,590 galaxy NGC 4485. 634 00:35:41,720 --> 00:35:44,420 NGC 4485 has a nickname of the two-faced galaxy, 635 00:35:44,530 --> 00:35:45,760 like the Batman villain, 636 00:35:45,860 --> 00:35:48,630 because it has two different halves of the galaxy 637 00:35:48,730 --> 00:35:50,100 doing completely different things. 638 00:35:50,200 --> 00:35:53,170 Half of the galaxy is sort of old and calm 639 00:35:53,270 --> 00:35:54,530 and relatively quiescent, 640 00:35:54,600 --> 00:35:57,470 whereas half of it appears to be undergoing a sort of 641 00:35:57,570 --> 00:36:00,440 fireworks display of new star formation. 642 00:36:01,840 --> 00:36:04,080 Why are new stars only born 643 00:36:04,180 --> 00:36:06,350 in one half of this galaxy? 644 00:36:08,450 --> 00:36:09,750 We found a clue on the edge of 645 00:36:09,850 --> 00:36:14,520 a photo taken by the Hubble Space Telescope. 646 00:36:14,620 --> 00:36:18,460 It was evidence of an attack by another galaxy. 647 00:36:18,560 --> 00:36:22,200 We think that another galaxy passed through it just off 648 00:36:22,300 --> 00:36:24,830 center in a way that strongly perturbed 649 00:36:24,930 --> 00:36:27,770 the gas on one half of the galaxy. 650 00:36:29,900 --> 00:36:32,540 The two-faced galaxy skirmish gave it 651 00:36:32,640 --> 00:36:34,110 a gravitational jolt, 652 00:36:34,210 --> 00:36:37,110 forcing clouds of gas together. 653 00:36:37,210 --> 00:36:40,280 When we think of galaxies, we think of stars, 654 00:36:40,380 --> 00:36:42,050 and of course, galaxies are made of stars. 655 00:36:42,150 --> 00:36:44,380 But, of course, gas is the stuff that 656 00:36:44,480 --> 00:36:45,720 stars are made of. 657 00:36:48,190 --> 00:36:49,890 When two galaxies collide, 658 00:36:49,990 --> 00:36:51,760 the gravitational duel can trigger 659 00:36:51,890 --> 00:36:54,090 a huge burst of star formation. 660 00:36:58,370 --> 00:37:00,670 You need something to give a galaxy a push, 661 00:37:00,770 --> 00:37:03,500 and that's exactly what a galaxy collision does. 662 00:37:03,600 --> 00:37:06,840 And when gas clouds collide, they compress. 663 00:37:06,940 --> 00:37:10,110 And when they compress, you get knots in them that can 664 00:37:10,210 --> 00:37:12,710 compress more and form stars. 665 00:37:14,750 --> 00:37:16,550 So you can think of these collisions as very 666 00:37:16,650 --> 00:37:17,780 violent events, 667 00:37:17,880 --> 00:37:21,190 but ultimately, it can breathe new life into a galaxy. 668 00:37:21,290 --> 00:37:25,320 But the spoils of war don't last long. 669 00:37:25,430 --> 00:37:28,460 In the short term, the victor galaxy can 670 00:37:28,560 --> 00:37:31,960 come out glorious with... With so many new stars. 671 00:37:32,070 --> 00:37:35,370 But this celebration is short-lived, because that round 672 00:37:35,470 --> 00:37:41,010 of star formation quickly uses up the material available. 673 00:37:41,110 --> 00:37:44,140 If a galaxy wants to stay alive, it has to feed on 674 00:37:44,240 --> 00:37:46,180 other galaxies. 675 00:37:46,280 --> 00:37:50,080 So galaxies constantly need to raid new targets, 676 00:37:50,180 --> 00:37:52,620 and that raises an important question. 677 00:37:52,720 --> 00:37:55,550 What happens if there's a galaxy just alone in space? 678 00:37:55,660 --> 00:37:58,690 Nothing else is colliding with it, sort of a pacifist galaxy. 679 00:38:00,260 --> 00:38:03,360 The poster child for these peace-loving galaxies 680 00:38:03,460 --> 00:38:06,230 is NGC 1277. 681 00:38:07,530 --> 00:38:11,340 NGC 1277 is a very peculiar galaxy. 682 00:38:11,440 --> 00:38:15,940 It's pretty big, and its stars are extremely old. 683 00:38:16,040 --> 00:38:18,480 It basically hasn't formed new stars in the last 684 00:38:18,580 --> 00:38:19,980 10 billion years, 685 00:38:20,080 --> 00:38:23,320 so it's kind of the veterans home of galaxies. 686 00:38:24,380 --> 00:38:26,790 NGC 1277 lives in a rough 687 00:38:26,890 --> 00:38:29,520 part of the cosmos called the Perseus Cluster. 688 00:38:30,890 --> 00:38:35,030 Thousands of other galaxies surround NGC 1277, 689 00:38:35,130 --> 00:38:38,200 and they are all ready for a fight. 690 00:38:38,270 --> 00:38:40,030 So you might ask, why hasn't it had 691 00:38:40,130 --> 00:38:43,140 encounters with other galaxies that might rejuvenate it? 692 00:38:44,640 --> 00:38:47,710 The answer, once again, is gravity. 693 00:38:47,810 --> 00:38:53,250 NGC 1277 sits inside this massive galaxy cluster 694 00:38:53,350 --> 00:38:54,580 that has a ton of mass, 695 00:38:54,720 --> 00:38:56,920 and if you look at its position, it's fairly near 696 00:38:57,020 --> 00:38:58,480 the center of the cluster. 697 00:39:00,820 --> 00:39:03,520 The combined gravity of thousands of galaxies 698 00:39:03,620 --> 00:39:06,130 pulls on NGC 1277, 699 00:39:06,230 --> 00:39:10,530 accelerating it to two million miles an hour. 700 00:39:13,270 --> 00:39:15,000 And so it has spent the last 701 00:39:15,100 --> 00:39:17,670 few billion years traveling faster and faster. 702 00:39:17,770 --> 00:39:19,910 Until now, it's almost at its fastest pace. 703 00:39:22,810 --> 00:39:24,240 It's very hard for gravity 704 00:39:24,340 --> 00:39:26,780 to catch it or catch one of its neighbors 705 00:39:26,880 --> 00:39:30,750 and bring them together to merge with each other. 706 00:39:30,850 --> 00:39:34,490 NGC 1277 has no chance of 707 00:39:34,590 --> 00:39:37,590 grabbing new gas to make new stars. 708 00:39:37,690 --> 00:39:43,300 It's dying. All that has left are old red stars. 709 00:39:43,400 --> 00:39:46,670 When it comes to galaxies, red is dead. 710 00:39:46,770 --> 00:39:49,170 No new stars means no big stars, 711 00:39:49,270 --> 00:39:52,940 no blue stars, just small dim red dwarfs. 712 00:39:57,980 --> 00:40:01,780 Galaxies that don't fight just fade away. 713 00:40:01,880 --> 00:40:03,480 And at that point, the history of 714 00:40:03,580 --> 00:40:05,520 the universe becomes really kind of boring. 715 00:40:05,620 --> 00:40:08,190 All the stars will simply start to die out. 716 00:40:08,290 --> 00:40:09,760 Eventually, there will be the last 717 00:40:09,860 --> 00:40:11,360 star formed in the Milky Way, 718 00:40:11,460 --> 00:40:13,890 with no new galaxy bringing fresh material. 719 00:40:13,990 --> 00:40:17,060 Without galaxy collisions, the universe dies. 720 00:40:24,240 --> 00:40:27,110 Galactic battles mix things up 721 00:40:27,210 --> 00:40:29,540 and replenish gas supplies, 722 00:40:29,640 --> 00:40:33,550 and our own galaxy has reaped the benefits. 723 00:40:33,650 --> 00:40:38,420 Our Milky Way Galaxy fought a massive battle, 724 00:40:38,520 --> 00:40:41,820 but that battle may have been necessary to build 725 00:40:41,920 --> 00:40:44,920 solar systems like the one we live in right now. 726 00:40:48,800 --> 00:40:51,400 Clashes with the Sagittarius Dwarf Galaxy 727 00:40:51,500 --> 00:40:54,530 occurred at the same time the sun formed. 728 00:40:56,100 --> 00:40:58,340 It's possible that we owe our very 729 00:40:58,440 --> 00:41:02,810 existence to the collision with the Sagittarius Dwarf Galaxy. 730 00:41:02,910 --> 00:41:05,710 Maybe the gas that ultimately gave rise 731 00:41:05,850 --> 00:41:07,780 to the birth of our solar system 732 00:41:07,880 --> 00:41:10,080 once came from another galaxy entirely. 733 00:41:12,390 --> 00:41:16,360 So galactic wars are both creative and destructive. 734 00:41:17,660 --> 00:41:21,260 Galaxies are built from collisions, 735 00:41:21,360 --> 00:41:24,300 galaxies survive from collisions, 736 00:41:24,400 --> 00:41:29,070 and galaxies can also die from collisions. 737 00:41:29,170 --> 00:41:31,000 Far from being destructive events, 738 00:41:31,100 --> 00:41:32,710 colliding galaxies may be the reason 739 00:41:32,810 --> 00:41:34,140 that you and I are here. 740 00:41:37,140 --> 00:41:39,550 Intergalactic warfare has revolutionized 741 00:41:39,650 --> 00:41:44,350 our understanding of how galaxies live and die. 742 00:41:44,450 --> 00:41:47,820 Ultimately, it's these galaxy mergers that are one of 743 00:41:47,920 --> 00:41:50,190 the great engines of all structure growth 744 00:41:50,290 --> 00:41:52,020 in the universe. 745 00:41:52,130 --> 00:41:55,260 These collisions got us to where we are today, 746 00:41:55,360 --> 00:41:58,330 and they're gonna determine the future of all the universe. 747 00:41:58,380 --> 00:42:02,930 Repair and Synchronization by Easy Subtitles Synchronizer 1.0.0.0 58987

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