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These are the user uploaded subtitles that are being translated: 1 00:00:01,302 --> 00:00:04,703 An invisible danger hurtles towards Earth 2 00:00:04,804 --> 00:00:07,538 at close to the speed of light. 3 00:00:07,607 --> 00:00:12,310 These are intergalactic alien interlopers on our Milky Way. 4 00:00:12,413 --> 00:00:13,846 Cosmic rays. 5 00:00:13,948 --> 00:00:16,414 Getting hit by a cosmic ray is like 6 00:00:16,550 --> 00:00:18,951 getting hit by a cosmic bullet. 7 00:00:19,053 --> 00:00:22,420 Cosmic rays are billions of times more energetic than any 8 00:00:22,556 --> 00:00:23,621 other types of particles, 9 00:00:23,757 --> 00:00:25,524 vastly more energetic than anything 10 00:00:25,626 --> 00:00:26,702 we can even create in 11 00:00:26,727 --> 00:00:30,129 a laboratory, in a nuclear fusion reactor, anywhere. 12 00:00:30,231 --> 00:00:33,064 They pierce spaceships, putting our astronauts 13 00:00:33,100 --> 00:00:34,198 in danger. 14 00:00:34,301 --> 00:00:36,679 But the source of their power is a mystery. 15 00:00:36,704 --> 00:00:38,637 Are they coming from other galaxies? 16 00:00:38,706 --> 00:00:40,484 Are they coming from things in between the galaxies? 17 00:00:40,508 --> 00:00:41,939 Where do cosmic rays come from? 18 00:00:42,042 --> 00:00:43,942 Truth is, the most powerful ones, 19 00:00:44,043 --> 00:00:45,210 we haven't got a clue. 20 00:00:45,311 --> 00:00:47,691 The race is on to solve the mystery 21 00:00:47,715 --> 00:00:50,816 of the fastest particles in the universe. 22 00:01:05,533 --> 00:01:08,099 If I were to make a list of the dangers of space, 23 00:01:08,201 --> 00:01:10,079 it would be a long list. 24 00:01:10,103 --> 00:01:13,638 You know, there's hard vacuum, huge swings in temperatures, 25 00:01:13,706 --> 00:01:16,307 micro meteorites, all kinds of things. 26 00:01:16,409 --> 00:01:20,512 But probably at the very top of that list, cosmic rays. 27 00:01:20,614 --> 00:01:23,314 These space invaders are not what they seem. 28 00:01:23,417 --> 00:01:26,051 When you hear the name cosmic rays, 29 00:01:26,120 --> 00:01:27,798 you might think it's like a beam, 30 00:01:27,822 --> 00:01:30,299 like a laser beam of light. No, no, no, no, no, no. 31 00:01:30,323 --> 00:01:34,126 It's a tiny little death particle. 32 00:01:34,228 --> 00:01:35,204 To fight them, 33 00:01:35,228 --> 00:01:37,228 we must first understand them. 34 00:01:42,203 --> 00:01:44,203 April 2019. 35 00:01:45,939 --> 00:01:49,942 NASA's Parker probe flies closer to the sun than 36 00:01:50,009 --> 00:01:51,287 ever before. 37 00:01:51,311 --> 00:01:53,390 We know the sun produces some of 38 00:01:53,414 --> 00:01:56,593 the cosmic rays that fill the solar system, 39 00:01:56,616 --> 00:01:58,049 but we don't know how. 40 00:01:59,453 --> 00:02:05,102 Our sun looks like a beautiful glowing orb, 41 00:02:05,126 --> 00:02:08,326 bringing energy and light to Earth and allowing life 42 00:02:08,429 --> 00:02:09,661 to thrive. 43 00:02:09,729 --> 00:02:11,629 But if you look at it up close, 44 00:02:11,731 --> 00:02:14,633 you'll see a tumultuous storm of events. 45 00:02:16,103 --> 00:02:18,236 The amount of energy the sun is emitting every 46 00:02:18,305 --> 00:02:24,109 second is the equivalent of 100 billion one megaton bombs. 47 00:02:24,211 --> 00:02:25,443 It's a dangerous neighborhood. 48 00:02:26,614 --> 00:02:29,192 Suddenly, the probe is caught head-on 49 00:02:29,216 --> 00:02:30,915 in a powerful blast. 50 00:02:34,989 --> 00:02:37,322 It's perfectly positioned to monitor 51 00:02:37,424 --> 00:02:39,525 the outburst from the inside. 52 00:02:41,228 --> 00:02:44,462 The entire outer third of the sun is a boiling 53 00:02:44,564 --> 00:02:48,078 cauldron, and tied up in that plasma are magnetic fields. 54 00:02:48,102 --> 00:02:51,336 They get tied and twisted, and energy is stored in them, 55 00:02:51,405 --> 00:02:54,038 so they rise towards the surface, and there, 56 00:02:54,140 --> 00:02:57,287 they rearrange, they reconnect, they twist, they spin. 57 00:02:57,311 --> 00:03:00,344 When the magnetic field lines snap, 58 00:03:00,447 --> 00:03:03,649 energy bursts out. 59 00:03:03,750 --> 00:03:08,052 And sometimes, that energy release is explosive 60 00:03:08,121 --> 00:03:09,955 and that's what results in flares, 61 00:03:10,056 --> 00:03:11,657 which are these huge bursts of light. 62 00:03:13,060 --> 00:03:16,627 The probe discovers that after a solar flare, 63 00:03:16,729 --> 00:03:20,932 the sun's surface stores electrically charged particles. 64 00:03:21,034 --> 00:03:25,336 But sometimes, there's a second explosion called 65 00:03:25,406 --> 00:03:29,341 a coronal mass ejection, releasing superheated, 66 00:03:29,409 --> 00:03:32,444 electrically charged gas called plasma. 67 00:03:34,215 --> 00:03:37,748 These giant balls of plasma go flying off the surface of 68 00:03:37,817 --> 00:03:40,563 the sun, and in those balls of plasma 69 00:03:40,587 --> 00:03:43,222 are contained these charged particles. 70 00:03:45,825 --> 00:03:50,628 The charged particles move fast, but they hit a roadblock, 71 00:03:50,764 --> 00:03:53,064 a cloud of slower-moving particles 72 00:03:53,133 --> 00:03:56,801 that always surrounds the sun, the solar wind. 73 00:03:58,338 --> 00:04:01,439 Well, the coronal mass ejection is moving into the solar wind 74 00:04:01,540 --> 00:04:03,385 much faster than the wind is moving. 75 00:04:03,409 --> 00:04:07,090 So it sort of runs into it and creates this shockwave 76 00:04:07,114 --> 00:04:09,848 and ends up piling up particles at the edge. 77 00:04:09,983 --> 00:04:12,450 The shockwave and particles 78 00:04:12,519 --> 00:04:15,052 slam together... In the collision, 79 00:04:15,155 --> 00:04:17,956 the particles steal energy and speed, 80 00:04:18,057 --> 00:04:20,625 like a baseball accelerating off a bat. 81 00:04:21,995 --> 00:04:26,264 The particles transform into something far more powerful... 82 00:04:26,332 --> 00:04:28,834 A solar cosmic ray. 83 00:04:28,935 --> 00:04:31,036 They're light, but they're moving 84 00:04:31,105 --> 00:04:32,637 incredibly fast. 85 00:04:34,507 --> 00:04:37,843 The Earth is on average 93 million miles away from 86 00:04:37,944 --> 00:04:41,846 the sun, and these guys reach us in about an hour. 87 00:04:41,949 --> 00:04:43,548 That's 93 million miles an hour. 88 00:04:43,617 --> 00:04:45,617 That's pretty fast. 89 00:04:45,752 --> 00:04:48,819 The cosmic rays speed towards Earth. 90 00:04:48,954 --> 00:04:50,622 We're under attack. 91 00:04:50,691 --> 00:04:55,004 Cosmic rays are, by far, the most energetic 92 00:04:55,028 --> 00:04:58,730 particles that we know to exist in the universe. 93 00:04:58,831 --> 00:05:02,233 And when things with very high energy, no matter how small 94 00:05:02,302 --> 00:05:04,036 they are, impact something else, 95 00:05:04,137 --> 00:05:07,182 they deposit that energy, right, and so cosmic rays 96 00:05:07,206 --> 00:05:08,451 can be very dangerous. 97 00:05:08,475 --> 00:05:12,343 Solar cosmic rays aren't the only threat we face. 98 00:05:12,446 --> 00:05:16,747 Other space bullets arrive from beyond our solar system. 99 00:05:16,850 --> 00:05:18,894 There are different kinds of cosmic rays, 100 00:05:18,918 --> 00:05:21,752 just like there are different kinds of bullets. 101 00:05:21,822 --> 00:05:23,487 At the lowest end of the spectrum 102 00:05:23,624 --> 00:05:26,625 are these solar cosmic rays. 103 00:05:26,726 --> 00:05:29,761 These are like the BBs, and when a BB hits you, 104 00:05:29,829 --> 00:05:32,108 it might sting for a little bit, but you're not gonna get 105 00:05:32,132 --> 00:05:33,465 too worried about it. 106 00:05:33,533 --> 00:05:37,601 A bigger concern... Galactic cosmic rays. 107 00:05:37,704 --> 00:05:41,038 They travel faster and have more energy. 108 00:05:41,141 --> 00:05:44,141 If solar rays are like BBs, 109 00:05:44,211 --> 00:05:47,312 the galactic cosmic rays are like rifle bullets. 110 00:05:47,413 --> 00:05:49,747 They're far more dangerous. 111 00:05:49,817 --> 00:05:51,750 They're moving a lot faster. 112 00:05:51,819 --> 00:05:54,418 But they're also more rare. 113 00:05:54,521 --> 00:05:57,000 Faster still are the universe's most wanted... 114 00:05:57,024 --> 00:05:59,524 Ultra-high-energy cosmic rays. 115 00:05:59,593 --> 00:06:02,259 If you thought galactic cosmic rays were bad, it's 116 00:06:02,362 --> 00:06:05,709 because you haven't met an ultra-high-energy cosmic ray. 117 00:06:05,733 --> 00:06:08,834 These are the biggest, baddest, 118 00:06:08,935 --> 00:06:12,838 meanest cosmic rays in the universe. 119 00:06:13,940 --> 00:06:16,408 These ultra-high-energy cosmic rays 120 00:06:16,509 --> 00:06:18,288 are like hypersonic missiles. 121 00:06:18,312 --> 00:06:20,411 They are screaming, and they come from 122 00:06:20,514 --> 00:06:23,514 the most energetic events in the universe. 123 00:06:27,454 --> 00:06:29,620 The ultra-high-energy cosmic missiles 124 00:06:29,723 --> 00:06:32,824 are the rarest but also the swiftest. 125 00:06:34,127 --> 00:06:37,963 These cosmic ray particles are moving fast. 126 00:06:38,064 --> 00:06:40,798 These mysterious particles are moving incredibly 127 00:06:40,933 --> 00:06:42,300 close to the speed of light. 128 00:06:42,403 --> 00:06:45,036 I'm not talking about 99 percent the speed of light. 129 00:06:45,072 --> 00:06:46,483 They're moving through space at 130 00:06:46,507 --> 00:06:48,740 like 99.999... 131 00:06:48,808 --> 00:06:51,487 - 9999... - 9999... 132 00:06:51,512 --> 00:06:53,889 - 99999... - 999999... 133 00:06:53,913 --> 00:06:56,047 99999... 21 nines. 134 00:06:56,149 --> 00:06:57,293 That's fast. 135 00:06:57,317 --> 00:06:59,451 That's wild. That's scary. 136 00:07:01,154 --> 00:07:03,154 All three types of cosmic rays 137 00:07:03,223 --> 00:07:05,322 are racing through the solar system. 138 00:07:06,360 --> 00:07:10,206 If I were to hold up a golf ball in the middle of space, 139 00:07:10,230 --> 00:07:16,178 almost 100 cosmic rays pass through that golf ball every 140 00:07:16,202 --> 00:07:18,036 single second. 141 00:07:18,137 --> 00:07:21,850 It's a deadly hail of particle bullets, 142 00:07:21,875 --> 00:07:23,185 and out in space, 143 00:07:23,209 --> 00:07:26,944 our astronauts are caught in the crossfire. 144 00:07:27,047 --> 00:07:29,047 Cosmic rays represent one of 145 00:07:29,115 --> 00:07:32,516 the greatest dangers for human space flight. 146 00:07:32,619 --> 00:07:35,899 NASA plans to send astronauts back to the moon, 147 00:07:35,923 --> 00:07:37,500 where radiation levels -OVER RADIO: Lift-off. 148 00:07:37,524 --> 00:07:40,903 From cosmic rays are 200 times greater than 149 00:07:40,927 --> 00:07:43,961 on Earth, and that is just the start. 150 00:07:44,064 --> 00:07:47,576 One of NASA's big goals is to send humans to Mars, 151 00:07:47,600 --> 00:07:49,401 and that is a long way away, 152 00:07:49,536 --> 00:07:52,081 at least a six-month journey, and more often, 153 00:07:52,105 --> 00:07:54,840 about a nine-month journey. That's a big problem. 154 00:07:55,908 --> 00:08:00,644 I am hoping that one day, I can go to Mars as an astronaut, 155 00:08:00,747 --> 00:08:02,848 but I'm definitely afraid of cosmic rays, 156 00:08:02,949 --> 00:08:04,269 and the more that I read about it, 157 00:08:04,350 --> 00:08:06,396 the bigger of a threat it seems. 158 00:08:06,420 --> 00:08:11,055 So I think that NASA and other space organizations 159 00:08:11,124 --> 00:08:13,257 are going to need to work on 160 00:08:13,326 --> 00:08:15,471 how to protect their astronauts in these 161 00:08:15,495 --> 00:08:17,329 really dangerous situations. 162 00:08:19,132 --> 00:08:20,976 Only one group of people have been 163 00:08:21,000 --> 00:08:24,101 exposed to these high levels of cosmic rays, 164 00:08:25,305 --> 00:08:27,738 the crew members of the Apollo missions 165 00:08:29,108 --> 00:08:31,643 July 1969. 166 00:08:31,711 --> 00:08:35,447 That's one small step for man, 167 00:08:35,548 --> 00:08:38,115 one giant leap for mankind. 168 00:08:39,418 --> 00:08:41,952 One of the astronauts, Buzz Aldrin, 169 00:08:42,022 --> 00:08:44,399 sees something strange. 170 00:08:44,423 --> 00:08:45,701 During Apollo 11, 171 00:08:45,725 --> 00:08:48,225 Buzz Aldrin reported seeing tiny little 172 00:08:48,294 --> 00:08:50,961 flashes sometimes when he was looking around. 173 00:08:51,063 --> 00:08:52,808 That's pretty weird. 174 00:08:52,832 --> 00:08:55,200 But what's weirder is that he saw them 175 00:08:55,335 --> 00:08:57,201 when his eyes were closed. 176 00:08:57,336 --> 00:09:01,505 Later missions also report seeing odd flashes of light. 177 00:09:02,842 --> 00:09:05,309 A streak in the lower left side of the... 178 00:09:05,412 --> 00:09:06,889 left eye, moving down. 179 00:09:06,913 --> 00:09:11,693 The astronauts describe the flashes as spots, 180 00:09:11,717 --> 00:09:13,796 streaks, and clouds. 181 00:09:13,820 --> 00:09:17,422 Apollo 15 Commander David Scott reported seeing one that 182 00:09:17,524 --> 00:09:20,702 was blue with a white cast, like a blue diamond. 183 00:09:20,726 --> 00:09:25,629 What's happening is that a cosmic ray is entering 184 00:09:25,764 --> 00:09:26,775 the eyeball 185 00:09:26,799 --> 00:09:30,501 and then striking molecules and giving off 186 00:09:30,604 --> 00:09:32,636 a flash of light. 187 00:09:32,706 --> 00:09:36,341 An alternative theory is that it triggers the layer of 188 00:09:36,442 --> 00:09:38,943 sensitive cells in your retina, 189 00:09:39,046 --> 00:09:42,392 so you perceive a streak of light even though 190 00:09:42,415 --> 00:09:44,215 no light ever actually existed. 191 00:09:45,519 --> 00:09:48,219 The cosmic rays cause long-term damage. 192 00:09:48,322 --> 00:09:50,154 Inside of the eye's lens, 193 00:09:50,222 --> 00:09:52,869 there are these fiber cells that are transparent. 194 00:09:52,893 --> 00:09:54,859 Well, when a cosmic ray travels through them, 195 00:09:54,995 --> 00:09:57,562 it can damage those cells and make them cloudy, 196 00:09:57,630 --> 00:09:58,830 causing cataracts. 197 00:09:58,932 --> 00:10:01,432 When NASA examines ROWE: the astronauts' helmets, 198 00:10:01,533 --> 00:10:04,535 they find tiny tracks etched through them, 199 00:10:04,605 --> 00:10:07,404 evidence of cosmic ray impacts. 200 00:10:07,539 --> 00:10:10,642 When we say that cosmic rays are like tiny little bullets, 201 00:10:10,744 --> 00:10:12,989 we're not joking around. 202 00:10:13,013 --> 00:10:16,793 And some of these burrowed all the way through the helmet, 203 00:10:16,817 --> 00:10:20,951 which means it ended up in the astronaut's brain, 204 00:10:21,020 --> 00:10:24,322 which just makes me feel weird to think about. 205 00:10:24,423 --> 00:10:27,458 What might that long-term radiation 206 00:10:27,559 --> 00:10:30,562 do to your brain, to your ability to reason 207 00:10:30,629 --> 00:10:33,664 and problem solve in one of the most dangerous environments 208 00:10:33,700 --> 00:10:35,200 that humanity has ever placed itself? 209 00:10:36,403 --> 00:10:39,282 The farther we venture from our home planet, 210 00:10:39,306 --> 00:10:41,105 the more danger we face. 211 00:10:51,018 --> 00:10:54,797 Cosmic rays, highly energetic space particles, 212 00:10:54,821 --> 00:10:58,722 may be the most serious threat to human space exploration. 213 00:10:59,759 --> 00:11:02,904 The Hollywood conception of outer space is 214 00:11:02,928 --> 00:11:05,274 it's full of dangers like aliens 215 00:11:05,298 --> 00:11:08,099 wielding ray guns or black holes 216 00:11:08,201 --> 00:11:09,533 or asteroid showers. 217 00:11:09,602 --> 00:11:11,279 But in reality, the biggest 218 00:11:11,303 --> 00:11:13,937 danger facing astronauts is invisible. 219 00:11:14,006 --> 00:11:15,240 It's the cosmic radiation. 220 00:11:16,308 --> 00:11:19,811 Cosmic rays damaged ROWE: Apollo astronauts' eyes 221 00:11:19,913 --> 00:11:22,746 after just a few days' exposure. 222 00:11:22,816 --> 00:11:26,650 A one-way trip to Mars takes nine months. 223 00:11:26,720 --> 00:11:28,297 Future missions are going to be 224 00:11:28,321 --> 00:11:30,455 spending much longer times in space, 225 00:11:30,557 --> 00:11:31,716 which means we really need to 226 00:11:31,758 --> 00:11:34,703 consider how cosmic rays will impact us. 227 00:11:34,727 --> 00:11:38,807 We don't understand all the long-term effects 228 00:11:38,831 --> 00:11:42,801 from a steady rain of cosmic rays, 229 00:11:42,903 --> 00:11:46,104 but the astronauts are gonna have to deal with it. 230 00:11:46,206 --> 00:11:48,684 To find out more, scientists bombarded 231 00:11:48,709 --> 00:11:52,688 human cells with manmade cosmic ray particles. 232 00:11:52,712 --> 00:11:58,450 They discovered cosmic rays physically cut through DNA, 233 00:11:58,551 --> 00:12:00,697 chopping it apart. 234 00:12:00,721 --> 00:12:04,755 Damage to DNA in your cell is 235 00:12:04,857 --> 00:12:09,259 by far the worst kind, because your DNA 236 00:12:09,361 --> 00:12:11,807 is the cell's operating manuals, the blueprints 237 00:12:11,831 --> 00:12:15,778 so the cell knows how it should be functioning normally. 238 00:12:15,802 --> 00:12:17,836 You can trigger that cell to 239 00:12:17,937 --> 00:12:21,306 turn tumorous, to start producing cancer. 240 00:12:23,110 --> 00:12:26,288 In 2019, scientists ROWE: took the experiment 241 00:12:26,312 --> 00:12:29,114 further and simulated a trip to Mars... 242 00:12:30,116 --> 00:12:32,549 for mice... For six months, 243 00:12:32,619 --> 00:12:34,652 they blasted the rodents with a steady 244 00:12:34,721 --> 00:12:38,756 stream of lab-made cosmic ray particles. 245 00:12:38,857 --> 00:12:42,460 The experiment found profound alterations 246 00:12:42,528 --> 00:12:45,429 to the mice's normal behavior. 247 00:12:45,565 --> 00:12:49,100 They learned new tasks much more slowly. 248 00:12:49,201 --> 00:12:50,580 Their memory was affected, and they 249 00:12:50,604 --> 00:12:53,638 forgot things they had already learned. 250 00:12:53,706 --> 00:12:55,440 They were more anxious and prone to 251 00:12:55,542 --> 00:12:58,888 giving up on tasks they'd normally complete. 252 00:12:58,912 --> 00:13:01,312 If you put some of these irradiated mice into 253 00:13:01,447 --> 00:13:05,595 a swimming test, rather than trying to swim to safety, 254 00:13:05,619 --> 00:13:07,217 many of them just simply gave up. 255 00:13:09,054 --> 00:13:10,721 This is important, because we need 256 00:13:10,823 --> 00:13:13,101 our astronauts to be fully functioning. 257 00:13:13,125 --> 00:13:16,628 The reason why you do crewed missions is because 258 00:13:16,730 --> 00:13:20,831 the human brain is much better than any computer. 259 00:13:20,933 --> 00:13:23,134 If even one of them has a problem, 260 00:13:23,202 --> 00:13:26,203 it can even put the mission and their lives in jeopardy. 261 00:13:27,706 --> 00:13:31,109 Other studies discover cosmic rays can accelerate 262 00:13:31,211 --> 00:13:35,312 aging, alter genes, and cause cardiovascular disease. 263 00:13:37,049 --> 00:13:38,850 That sounds bad enough, 264 00:13:38,951 --> 00:13:41,952 but there's a more immediate danger. 265 00:13:42,022 --> 00:13:44,767 When cosmic rays penetrate spaceships, 266 00:13:44,790 --> 00:13:47,903 they can fry electronic systems, and that's enough to 267 00:13:47,927 --> 00:13:49,561 jeopardize a mission. 268 00:13:49,629 --> 00:13:54,876 Our operations in space depend on electronics, on computers. 269 00:13:54,900 --> 00:13:59,604 And the worst case scenario is that the wrong cosmic ray comes 270 00:13:59,706 --> 00:14:01,639 at the wrong time and hits 271 00:14:01,740 --> 00:14:06,344 the wrong circuit, and it leads to a cascading series of 272 00:14:06,446 --> 00:14:10,014 failures that can totally jeopardize a mission. 273 00:14:11,051 --> 00:14:13,918 We see evidence of this onslaught in mission cameras. 274 00:14:15,254 --> 00:14:17,120 Even when we have a detector in space 275 00:14:17,256 --> 00:14:18,822 like on the Hubble Space Telescope, 276 00:14:18,924 --> 00:14:20,357 if you saw a raw image, 277 00:14:20,460 --> 00:14:23,061 it doesn't look like the beautiful images 278 00:14:23,129 --> 00:14:24,328 that are shown to the public. 279 00:14:24,463 --> 00:14:26,865 They're just crossed with cosmic rays, and those 280 00:14:26,966 --> 00:14:31,201 cosmic rays are destroying that detector slowly over time. 281 00:14:33,105 --> 00:14:36,039 So how can we protect astronauts and their equipment? 282 00:14:37,443 --> 00:14:39,711 The obvious answer is to add shielding. 283 00:14:41,715 --> 00:14:45,048 It's one thing to say like, oh, just add more stuff. 284 00:14:45,150 --> 00:14:48,820 But have you seen rocket launches and how hard they are, 285 00:14:48,922 --> 00:14:51,822 how expensive it is to get stuff up into space? 286 00:14:53,225 --> 00:14:55,960 NASA does have a plan. 287 00:14:56,062 --> 00:14:58,763 The spacecraft for the Artemis moon landing mission 288 00:14:58,831 --> 00:15:02,033 will be packed for optimum cosmic ray protection. 289 00:15:02,101 --> 00:15:05,035 So one of the ways you can get around 290 00:15:05,138 --> 00:15:08,306 the mass limit is to basically get dual use 291 00:15:08,408 --> 00:15:10,041 out of everything... Your supplies, 292 00:15:10,110 --> 00:15:13,788 your fuel, your water, and you can use those as shielding. 293 00:15:13,812 --> 00:15:15,791 But it's not that simple. 294 00:15:15,815 --> 00:15:18,995 Just as more powerful bullets penetrate armor, 295 00:15:19,019 --> 00:15:22,352 more energetic cosmic rays pierce the shielding 296 00:15:22,422 --> 00:15:24,000 on spaceships. 297 00:15:24,024 --> 00:15:26,124 The solar ones... Yeah, you can just put up some 298 00:15:26,259 --> 00:15:28,960 material, some shielding, and it'll generally block them. 299 00:15:29,062 --> 00:15:31,863 But the higher energy ones, they can just burrow 300 00:15:31,998 --> 00:15:33,197 on through. 301 00:15:33,232 --> 00:15:37,302 If they hit one of the atoms in the shielding that is 302 00:15:37,403 --> 00:15:38,836 protecting our astronauts, 303 00:15:38,937 --> 00:15:42,039 it can create a shower of particles. 304 00:15:42,140 --> 00:15:44,709 That radiation particle might have missed 305 00:15:44,811 --> 00:15:46,210 any of the cells in your body. 306 00:15:46,312 --> 00:15:47,644 But you've now turned it into 307 00:15:47,746 --> 00:15:51,548 a blast, shredding through everything in the spacecraft. 308 00:15:51,618 --> 00:15:55,664 And so it turns out your shielding becomes 309 00:15:55,688 --> 00:15:59,222 the weapon that the cosmic rays use against you. 310 00:15:59,325 --> 00:16:04,528 But NASA is recruiting an unexpected ally... the sun. 311 00:16:04,630 --> 00:16:09,299 Can we protect our astronauts by fighting fire with fire? 312 00:16:17,911 --> 00:16:22,413 Powerful cosmic rays smash through spaceships. 313 00:16:22,514 --> 00:16:27,518 But how can objects smaller than an atom carry enough 314 00:16:27,653 --> 00:16:30,455 energy to be dangerous to astronauts? 315 00:16:30,556 --> 00:16:33,423 Moving objects carry energy. 316 00:16:33,525 --> 00:16:35,960 We call this kinetic energy, and when 317 00:16:36,028 --> 00:16:39,529 they strike something, they transform that energy. 318 00:16:40,933 --> 00:16:44,201 When I hit my hand, the kinetic energy of 319 00:16:44,336 --> 00:16:49,639 my fist transforms into sound and heat and vibration. 320 00:16:49,709 --> 00:16:51,743 My hand hurts a little from 321 00:16:51,811 --> 00:16:55,613 that impact, from the transformation of energy. 322 00:16:55,715 --> 00:16:58,149 It's the same thing with cosmic rays. 323 00:16:58,217 --> 00:17:02,253 When they slam into a human brain cell or a computer chip, 324 00:17:02,355 --> 00:17:04,955 they dump some energy, causing damage. 325 00:17:06,326 --> 00:17:09,704 How much damage depends on their kinetic energy, 326 00:17:09,729 --> 00:17:12,063 and that comes down to two things... 327 00:17:12,132 --> 00:17:13,964 Mass and speed. 328 00:17:15,000 --> 00:17:18,935 Intuitively, things that are moving at the same speed, 329 00:17:19,038 --> 00:17:21,384 if they're more massive, they carry more energy. 330 00:17:21,407 --> 00:17:23,941 A bigger asteroid slamming into Earth will 331 00:17:24,009 --> 00:17:26,711 do more damage than a smaller asteroid. 332 00:17:26,813 --> 00:17:29,413 If you double the mass of an object, 333 00:17:29,516 --> 00:17:32,294 its kinetic energy also doubles. 334 00:17:32,317 --> 00:17:35,052 Although mass is important, 335 00:17:35,153 --> 00:17:36,721 it's not as important as speed. 336 00:17:39,625 --> 00:17:42,704 Speed matters even more than mass. 337 00:17:42,729 --> 00:17:46,064 The kinetic energy depends directly on the mass, 338 00:17:46,132 --> 00:17:48,676 but it depends on the square of the speed. 339 00:17:48,701 --> 00:17:51,380 Here's what that means... You double the mass, 340 00:17:51,403 --> 00:17:54,439 you have double the kinetic energy, you double the speed, 341 00:17:54,539 --> 00:17:56,807 you have four times the kinetic energy. 342 00:17:59,711 --> 00:18:05,650 When it comes to speed, cosmic rays are the elite. 343 00:18:05,750 --> 00:18:07,896 An ultra-high-energy cosmic ray 344 00:18:07,921 --> 00:18:12,500 detected in 1991 hit the atmosphere so fast, 345 00:18:12,525 --> 00:18:15,960 scientists called it the "Oh My God Particle." 346 00:18:19,231 --> 00:18:22,500 This particle was higher energy than they thought 347 00:18:22,602 --> 00:18:24,335 they would ever, ever see. 348 00:18:24,436 --> 00:18:27,805 Until this fluorescent streak in the Utah sky, 349 00:18:27,906 --> 00:18:31,186 no one believed a particle could reach the Earth traveling 350 00:18:31,211 --> 00:18:33,288 so close to the speed of light, 351 00:18:33,313 --> 00:18:36,614 making cosmic ray particles far more dangerous 352 00:18:36,715 --> 00:18:37,949 than expected. 353 00:18:38,049 --> 00:18:40,218 As you approach the speed of light, 354 00:18:40,319 --> 00:18:42,752 energy, momentum, mass, they start 355 00:18:42,822 --> 00:18:44,721 to act a little bit differently. 356 00:18:44,856 --> 00:18:47,525 Einstein's equations of relativity become important, 357 00:18:47,626 --> 00:18:50,327 because the physics changes, and the energy it has 358 00:18:50,462 --> 00:18:53,463 becomes much, much, much stronger. 359 00:18:53,532 --> 00:18:56,377 If a particle is moving at close to the speed of light, 360 00:18:56,402 --> 00:19:00,505 that means that its energy is almost at the maximum allowed 361 00:19:00,606 --> 00:19:02,606 by the laws of physics. 362 00:19:04,711 --> 00:19:06,788 It's amazing to think that something as tiny as 363 00:19:06,813 --> 00:19:09,814 a proton could actually be dangerous to a human being. 364 00:19:09,949 --> 00:19:13,217 But amazingly, that proton is moving so fast, 365 00:19:13,318 --> 00:19:15,564 it carries as much energy as a baseball 366 00:19:15,587 --> 00:19:17,255 thrown at 100 miles an hour. 367 00:19:17,323 --> 00:19:21,159 A baseball contains over a trillion, trillion protons. 368 00:19:21,259 --> 00:19:25,229 Imagine all that energy carried by just one particle. 369 00:19:25,330 --> 00:19:29,178 So now you get a sense of just how risky these can be. 370 00:19:29,201 --> 00:19:31,602 Ultra-high-energy cosmic rays like 371 00:19:31,703 --> 00:19:35,683 the Oh My God Particle are like supersonic missiles. 372 00:19:35,708 --> 00:19:38,608 They are the fastest, but they're so rare, 373 00:19:38,711 --> 00:19:41,811 astronauts are unlikely to be hit by one. 374 00:19:41,914 --> 00:19:45,994 Solar cosmic rays are like BB pellets... abundant, 375 00:19:46,019 --> 00:19:48,719 but our spacecraft can block them. 376 00:19:48,788 --> 00:19:50,453 The biggest threat to our astronauts, 377 00:19:50,522 --> 00:19:53,124 however, are galactic cosmic rays. 378 00:19:53,226 --> 00:19:56,105 They come from elsewhere in the Milky Way. 379 00:19:56,128 --> 00:19:57,862 The combination of their speed 380 00:19:57,997 --> 00:20:01,576 and frequency makes them the most dangerous. 381 00:20:01,601 --> 00:20:05,681 These galactic cosmic rays are much more powerful than 382 00:20:05,704 --> 00:20:07,404 the solar cosmic rays, 383 00:20:07,507 --> 00:20:10,786 and they've traveled enormous distances 384 00:20:10,809 --> 00:20:13,544 to mess you up. 385 00:20:13,613 --> 00:20:17,992 Luckily, our astronauts have a surprising protector, 386 00:20:18,017 --> 00:20:21,618 a guardian of the solar system, the sun. 387 00:20:23,155 --> 00:20:24,622 As well as spitting out these 388 00:20:24,723 --> 00:20:29,104 high-energy solar cosmic ray particles, 389 00:20:29,127 --> 00:20:33,431 the sun is also streaming out lots of much lower energy 390 00:20:33,499 --> 00:20:36,032 particles of the solar wind. 391 00:20:36,134 --> 00:20:38,180 That outward moving solar wind acts 392 00:20:38,203 --> 00:20:41,750 as a force field, and the cosmic rays have to work 393 00:20:41,773 --> 00:20:46,989 their way upstream to get to Earth far inside this bubble. 394 00:20:47,012 --> 00:20:51,715 The solar wind extends 11 billion miles 395 00:20:51,817 --> 00:20:53,116 around the solar system, 396 00:20:53,251 --> 00:20:57,098 generating a magnetic field that repels incoming 397 00:20:57,123 --> 00:20:59,423 galactic cosmic rays. 398 00:20:59,525 --> 00:21:01,869 It's almost like the deflector shield 399 00:21:01,894 --> 00:21:04,105 of the Starship Enterprise. 400 00:21:04,130 --> 00:21:08,932 So the sun's magnetic field partially helps protect 401 00:21:09,001 --> 00:21:11,335 the Earth and any astronauts 402 00:21:11,403 --> 00:21:12,803 from the incoming radiation. 403 00:21:12,904 --> 00:21:16,707 Not long ago, our Voyager spacecraft 404 00:21:16,808 --> 00:21:19,943 made it to that boundary between the sun's bubble 405 00:21:20,046 --> 00:21:21,444 and the galaxy and was able 406 00:21:21,547 --> 00:21:24,648 to study that region, and we see the difference between 407 00:21:24,750 --> 00:21:27,496 inside the sun's bubble and what's going on 408 00:21:27,519 --> 00:21:29,097 outside the sun's bubble. 409 00:21:29,122 --> 00:21:31,521 The sun has our back, billions 410 00:21:31,624 --> 00:21:34,659 of miles away, and that's pretty cool. 411 00:21:34,759 --> 00:21:37,806 The Voyager space probes discovered 412 00:21:37,829 --> 00:21:40,664 a moving battlefield. 413 00:21:40,732 --> 00:21:44,579 The solar wind behaves a bit like a storm front on Earth. 414 00:21:44,604 --> 00:21:46,481 Sometimes, it advances. 415 00:21:46,506 --> 00:21:48,739 Sometimes, it retreats. 416 00:21:49,808 --> 00:21:51,808 When the sun's activity is the highest, 417 00:21:51,911 --> 00:21:54,811 it's spitting out more solar energetic protons, 418 00:21:54,913 --> 00:21:58,749 but those solar cosmic rays are much less damaging 419 00:21:58,817 --> 00:21:59,994 than the galactic ones, 420 00:22:00,019 --> 00:22:02,519 so the net is a benefit. 421 00:22:03,690 --> 00:22:06,501 So actually, ironically, you might find that, 422 00:22:06,526 --> 00:22:10,105 for astronauts, it is safer to launch missions to Mars 423 00:22:10,128 --> 00:22:14,065 during a period of higher solar activity, because although 424 00:22:14,133 --> 00:22:18,579 you have more of the solar particle radiation, 425 00:22:18,604 --> 00:22:22,084 you also get a better shielding effect 426 00:22:22,107 --> 00:22:23,786 from the solar wind. 427 00:22:23,809 --> 00:22:25,843 The sun's activity goes through 428 00:22:25,944 --> 00:22:28,390 an 11-year cycle of highs and lows. 429 00:22:28,413 --> 00:22:32,094 The protective bubble follows the same cycle, 430 00:22:32,117 --> 00:22:36,597 allowing NASA to predict the safest times to launch. 431 00:22:36,622 --> 00:22:38,521 This is a thorny problem, and, you know, 432 00:22:38,624 --> 00:22:41,759 we have very smart people working on it, but we want to 433 00:22:41,861 --> 00:22:44,205 explore space as much as we can, 434 00:22:44,230 --> 00:22:45,829 but we have to lower the risk 435 00:22:45,932 --> 00:22:47,832 to the astronauts as much as possible. 436 00:22:49,935 --> 00:22:53,436 NASA's fight against the cosmic invaders continues, 437 00:22:53,506 --> 00:22:56,240 but the biggest mystery remains. 438 00:22:56,308 --> 00:22:59,743 What exactly is launching the deadliest 439 00:22:59,811 --> 00:23:02,046 galactic cosmic rays? 440 00:23:10,323 --> 00:23:12,901 Every second, quadrillions of bits 441 00:23:12,924 --> 00:23:15,358 of space shrapnel race towards Earth 442 00:23:15,428 --> 00:23:17,361 at close to the speed of light... 443 00:23:17,430 --> 00:23:20,029 Galactic cosmic rays. 444 00:23:21,099 --> 00:23:24,380 The galactic cosmic rays are like a rifle bullet. 445 00:23:24,403 --> 00:23:27,404 You do not want to get hit by one of these. 446 00:23:27,539 --> 00:23:31,307 They are invaders from outside the solar system. 447 00:23:31,411 --> 00:23:34,044 We know they're made by something powerful 448 00:23:34,113 --> 00:23:35,391 within our galaxy, 449 00:23:35,414 --> 00:23:39,048 so the source should be easy to detect. 450 00:23:39,151 --> 00:23:41,551 You'd think if one of them 451 00:23:41,653 --> 00:23:44,320 hits a detector on Earth, that we'd just be able 452 00:23:44,423 --> 00:23:46,056 to point back in a straight line and say, 453 00:23:46,125 --> 00:23:47,290 "It came from over there." 454 00:23:47,326 --> 00:23:49,104 And then look, is there something else over there, 455 00:23:49,127 --> 00:23:51,006 like a supernova explosion that 456 00:23:51,029 --> 00:23:52,962 could explain the source of this? 457 00:23:53,031 --> 00:23:55,576 The problem is that cosmic rays get 458 00:23:55,601 --> 00:23:59,981 bent as they move by magnetic fields. 459 00:24:00,006 --> 00:24:01,939 The electric charge on a cosmic ray 460 00:24:02,040 --> 00:24:04,107 makes it act like a little magnet, 461 00:24:05,178 --> 00:24:08,045 and the Milky Way is full of other magnets. 462 00:24:08,114 --> 00:24:12,249 If I'm a cosmic ray just barreling through the galaxy, 463 00:24:12,351 --> 00:24:14,751 and I encounter a magnetic field, 464 00:24:14,820 --> 00:24:17,121 I'm gonna slightly change directions. 465 00:24:17,222 --> 00:24:20,201 Maybe here, maybe there, maybe up there. 466 00:24:20,226 --> 00:24:23,259 My trajectory is going to become scrambled. 467 00:24:23,328 --> 00:24:25,962 And after a few million years or so, 468 00:24:26,065 --> 00:24:28,731 basically all the information about where it started has 469 00:24:28,800 --> 00:24:30,334 been lost... It's going in a completely 470 00:24:30,403 --> 00:24:34,305 random direction for all practical purposes. 471 00:24:34,406 --> 00:24:38,308 But galactic cosmic rays also have a sidekick, 472 00:24:38,411 --> 00:24:44,048 one that is far less elusive... Gamma rays. 473 00:24:44,148 --> 00:24:47,351 When a galactic cosmic ray hits a regular atom out 474 00:24:47,452 --> 00:24:50,320 in space, it causes this big reaction. 475 00:24:51,624 --> 00:24:53,868 It emits all sorts of other particles, 476 00:24:53,893 --> 00:24:55,226 including gamma rays, 477 00:24:55,361 --> 00:24:58,729 which are basically extremely energetic photons of light. 478 00:24:58,830 --> 00:25:02,700 Critically, gamma rays don't get bent by magnetic fields, 479 00:25:02,835 --> 00:25:04,515 because they don't have an electric charge, 480 00:25:04,604 --> 00:25:07,538 so they just beeline off in a straight line along whatever 481 00:25:07,640 --> 00:25:10,840 direction the cosmic ray was moving in the first place. 482 00:25:10,942 --> 00:25:14,944 So we can look back at where gamma rays are coming from in 483 00:25:15,013 --> 00:25:18,393 the sky, and that tells us where there are a lot of 484 00:25:18,416 --> 00:25:19,750 cosmic rays having collisions. 485 00:25:21,053 --> 00:25:24,855 And they've led us to a prime suspect... 486 00:25:26,125 --> 00:25:27,125 supernovas. 487 00:25:30,695 --> 00:25:31,961 Supernova are some of 488 00:25:32,064 --> 00:25:34,375 the most powerful explosions in the universe, 489 00:25:34,400 --> 00:25:37,433 and so they're ripe grounds for these highly energetic, 490 00:25:37,536 --> 00:25:41,704 extremely fast particles to be created. 491 00:25:41,807 --> 00:25:44,040 When a giant star runs out of fuel, 492 00:25:44,109 --> 00:25:46,954 it can no longer support its own weight. 493 00:25:46,979 --> 00:25:48,612 It collapses inward, 494 00:25:50,549 --> 00:25:54,050 triggering a huge explosion, powerful enough 495 00:25:54,119 --> 00:25:57,699 to smash atoms into tiny pieces. 496 00:25:57,722 --> 00:26:01,002 The explosion pushes out an expanding cloud 497 00:26:01,027 --> 00:26:04,806 of gas and dust, the supernova remnant. 498 00:26:04,829 --> 00:26:06,963 And that material, as it's moving out at 499 00:26:07,066 --> 00:26:08,164 1,000 miles a second, 500 00:26:08,232 --> 00:26:11,535 generates an incredibly powerful shockwave. 501 00:26:11,604 --> 00:26:14,038 And that shockwave could be where 502 00:26:14,105 --> 00:26:19,442 a particle swept up in the shock gets accelerated. 503 00:26:19,545 --> 00:26:21,990 The magnetic fields inside the cloud 504 00:26:22,013 --> 00:26:24,615 trap the subatomic particles. 505 00:26:24,683 --> 00:26:27,550 Cosmic rays inside of the supernova remnant 506 00:26:27,619 --> 00:26:29,452 are a lot like being in a pinball machine. 507 00:26:31,523 --> 00:26:35,503 So you have the shockwave as the flipper, and then your 508 00:26:35,528 --> 00:26:37,806 magnetic fields are these bumpers, 509 00:26:37,829 --> 00:26:40,064 prohibiting it from actually leaving. 510 00:26:41,433 --> 00:26:42,877 They're bouncing back and forth across 511 00:26:42,902 --> 00:26:45,881 this incredibly energetic shock, and each time 512 00:26:45,904 --> 00:26:47,037 they bounce back and forth, 513 00:26:47,105 --> 00:26:49,606 the key is they pick up a little more energy. 514 00:26:50,643 --> 00:26:53,943 When a galactic cosmic ray gains enough energy, 515 00:26:54,012 --> 00:26:57,259 the magnetic fields can no longer hold on to it. 516 00:26:57,282 --> 00:26:58,515 It escapes. 517 00:27:01,153 --> 00:27:03,798 The supernova theory explains the birth 518 00:27:03,823 --> 00:27:06,457 of many of these cosmic bullets. 519 00:27:06,557 --> 00:27:09,371 But then we discovered a super gamma ray 520 00:27:09,394 --> 00:27:13,130 so powerful, it must have a completely different 521 00:27:13,231 --> 00:27:14,565 origin story. 522 00:27:14,633 --> 00:27:17,500 So this gamma ray was incredibly high energy, 523 00:27:17,635 --> 00:27:20,781 which means that the cosmic ray responsible for it was 524 00:27:20,806 --> 00:27:23,539 probably also extremely high in energy. 525 00:27:23,642 --> 00:27:25,742 If you fire a bullet into a pinball machine, 526 00:27:25,778 --> 00:27:27,443 it's not gonna bounce back and forth. 527 00:27:29,248 --> 00:27:30,948 I'm just gonna break through the machinery. 528 00:27:31,049 --> 00:27:32,394 The problem is that these 529 00:27:32,417 --> 00:27:35,219 are vastly more energetic than that. 530 00:27:35,320 --> 00:27:38,099 So there's no way they could have been bouncing around all 531 00:27:38,124 --> 00:27:41,557 the way up to their current energies inside of that 532 00:27:41,626 --> 00:27:45,007 particular pinball machine. 533 00:27:45,030 --> 00:27:48,065 There must be something else in the Milky Way 534 00:27:48,133 --> 00:27:50,433 creating galactic cosmic rays, 535 00:27:50,502 --> 00:27:54,704 something more powerful than a supernova. 536 00:27:56,307 --> 00:27:59,509 The question is, what? 537 00:27:59,612 --> 00:28:03,047 January 2021. 538 00:28:03,147 --> 00:28:04,792 At an observatory 539 00:28:04,817 --> 00:28:07,796 high up on the side of a Mexican volcano, 540 00:28:07,819 --> 00:28:11,320 blue light zaps through water tanks, 541 00:28:12,424 --> 00:28:15,025 signs of incoming gamma rays. 542 00:28:16,828 --> 00:28:19,807 Their trail stretches back across the Milky Way, 543 00:28:19,832 --> 00:28:24,101 crossing billions of miles, but suddenly goes cold. 544 00:28:25,336 --> 00:28:28,439 Instead of originating in a huge explosion, 545 00:28:28,507 --> 00:28:33,443 the trail ends in a cold, sparse cloud of dust. 546 00:28:33,545 --> 00:28:36,713 Molecular clouds, at first glance, seem like 547 00:28:36,816 --> 00:28:38,292 one of the most boring, 548 00:28:38,317 --> 00:28:41,117 innocuous places in the universe. 549 00:28:41,220 --> 00:28:45,500 You can barely even see them without an infrared telescope. 550 00:28:45,523 --> 00:28:48,258 They're not events like supernova 551 00:28:48,359 --> 00:28:50,326 that have enormously high energies. 552 00:28:50,429 --> 00:28:52,462 So you wouldn't expect it to create super 553 00:28:52,530 --> 00:28:54,276 energetic particles. 554 00:28:54,299 --> 00:28:57,034 Something must be hidden in the cloud, 555 00:28:57,103 --> 00:29:01,383 something powerful enough to accelerate the cosmic rays. 556 00:29:01,406 --> 00:29:03,484 We just don't know what. 557 00:29:03,509 --> 00:29:06,410 We can't see inside the molecular clouds, 558 00:29:06,545 --> 00:29:09,747 so it could be that, deep inside them, 559 00:29:09,847 --> 00:29:13,317 there are clusters of newborn stars that are cranking out 560 00:29:13,419 --> 00:29:14,796 these cosmic rays, 561 00:29:14,819 --> 00:29:18,756 but we don't know if even the crankiest of stars are 562 00:29:18,824 --> 00:29:23,505 capable of producing cosmic rays at these energies. 563 00:29:23,528 --> 00:29:25,662 Just two months later, 564 00:29:25,763 --> 00:29:29,232 in March of 2021, we get another clue. 565 00:29:29,334 --> 00:29:31,934 Scientists detect gamma rays coming 566 00:29:32,037 --> 00:29:35,239 from the Cygnus Cocoon Nebula. 567 00:29:35,339 --> 00:29:37,941 It's a dense molecular cloud with 568 00:29:38,042 --> 00:29:41,612 a difference... At the center is a cavity. 569 00:29:41,713 --> 00:29:46,450 Hundreds of closely packed stars push against the dust 570 00:29:46,551 --> 00:29:48,818 and gas, including 571 00:29:48,887 --> 00:29:52,855 huge bright stars called spectral type O and B 572 00:29:53,925 --> 00:29:56,160 Spectral type O and B stars are 573 00:29:56,228 --> 00:29:58,362 some of the hottest stars in our universe. 574 00:30:00,031 --> 00:30:02,598 The massive stars blast out solar winds far 575 00:30:02,733 --> 00:30:05,035 stronger than the wind produced by our sun. 576 00:30:06,704 --> 00:30:09,038 When you think about all these stars forming together, 577 00:30:09,141 --> 00:30:12,342 they are all putting off a wind of high-energy particles 578 00:30:12,443 --> 00:30:13,644 from their surfaces. 579 00:30:13,679 --> 00:30:16,712 These winds collide and form big shock structures 580 00:30:16,816 --> 00:30:18,648 between all of these young stars. 581 00:30:18,750 --> 00:30:20,951 You're getting so much energy from 582 00:30:21,053 --> 00:30:22,772 so many different winds, coming from so many 583 00:30:22,855 --> 00:30:27,356 different directions, that it forms a boiling mass of 584 00:30:27,425 --> 00:30:29,471 shockwaves and magnetic fields. 585 00:30:29,494 --> 00:30:30,961 It's a pinball machine 586 00:30:31,029 --> 00:30:34,964 on a far bigger scale... The magnetic fields are stronger 587 00:30:35,034 --> 00:30:36,278 than a supernova's, 588 00:30:36,301 --> 00:30:40,582 trapping and accelerating the more energetic cosmic rays 589 00:30:40,605 --> 00:30:41,782 for longer. 590 00:30:41,807 --> 00:30:44,240 One important thing about star clusters is that 591 00:30:44,343 --> 00:30:46,988 they are around for millions and millions of years. 592 00:30:47,011 --> 00:30:49,947 It's not just a one-off event like a supernova. 593 00:30:49,981 --> 00:30:52,894 And so you've got this magnetic field 594 00:30:52,917 --> 00:30:56,118 and these shocks happening over a long period of time, 595 00:30:56,255 --> 00:30:58,521 and that may be what you need to accelerate cosmic rays. 596 00:30:59,924 --> 00:31:04,428 Molecular clouds may shoot out galactic cosmic rays, 597 00:31:04,529 --> 00:31:07,663 but what fires the hypersonic space missiles, 598 00:31:07,732 --> 00:31:10,800 the ultra-high-energy cosmic rays? 599 00:31:10,935 --> 00:31:14,805 The culprit may be hiding out in distant galaxies... 600 00:31:14,940 --> 00:31:18,107 Supermassive black holes. 601 00:31:25,217 --> 00:31:27,517 Ultra-high-energy cosmic rays are 602 00:31:27,619 --> 00:31:31,221 the hypersonic missiles of the particle world. 603 00:31:31,289 --> 00:31:33,300 If a photon of light, the fastest thing in 604 00:31:33,325 --> 00:31:37,227 the universe, had a race with an ultra-high-energy cosmic ray, 605 00:31:37,328 --> 00:31:41,664 it would be so close, that after 200,000 years, 606 00:31:41,700 --> 00:31:44,500 that photon would be half an inch ahead of 607 00:31:44,635 --> 00:31:46,381 the ultra-high-energy cosmic ray. 608 00:31:46,404 --> 00:31:50,941 They appear to come from beyond our Milky Way galaxy. 609 00:31:51,042 --> 00:31:55,811 Our galaxy is 100,000 light years across. 610 00:31:55,914 --> 00:31:59,615 The next nearest galaxy to us is two million light years away. 611 00:31:59,718 --> 00:32:01,751 So these are traveling to us 612 00:32:01,853 --> 00:32:04,820 across millions and billions of light years. 613 00:32:04,923 --> 00:32:09,326 How do you accelerate this tiny 614 00:32:09,461 --> 00:32:13,963 little particle to such insane velocities? 615 00:32:14,066 --> 00:32:15,876 What is the power source? 616 00:32:15,901 --> 00:32:19,536 What in the universe has that kind of capability? 617 00:32:19,605 --> 00:32:22,405 Where's the Death Star here? 618 00:32:22,540 --> 00:32:25,142 Their speed makes them dangerous, 619 00:32:25,210 --> 00:32:29,046 but it also makes it easier to find their source. 620 00:32:29,114 --> 00:32:32,415 Ultra-high-energy cosmic rays are moving so rapidly, 621 00:32:32,550 --> 00:32:34,518 that they're really not affected that much by 622 00:32:34,619 --> 00:32:35,751 magnetic fields. 623 00:32:35,820 --> 00:32:37,999 It's like a bullet going through a fisherman's net. 624 00:32:38,022 --> 00:32:41,802 And so they're coming mostly in a straight line. 625 00:32:41,826 --> 00:32:44,161 When they're coming in a straight line, and we can point 626 00:32:44,229 --> 00:32:45,707 back to their origin, 627 00:32:45,730 --> 00:32:49,477 and that's something we can use to figure out where 628 00:32:49,500 --> 00:32:50,933 and how they're getting accelerated. 629 00:32:52,904 --> 00:32:54,604 In the Argentinian desert, 630 00:32:54,707 --> 00:32:58,240 the Pierre Auger Cosmic Ray Detector completes 631 00:32:58,309 --> 00:33:00,410 a 12-year study of the sky. 632 00:33:02,647 --> 00:33:05,548 It confirms that most galaxies have a supermassive 633 00:33:05,650 --> 00:33:07,351 black hole at their center, 634 00:33:07,419 --> 00:33:11,153 but only a few are active, shooting out energy. 635 00:33:11,256 --> 00:33:15,057 These active supermassive black holes also 636 00:33:15,126 --> 00:33:18,428 blast out ultra-high-energy cosmic rays. 637 00:33:19,431 --> 00:33:23,278 Supermassive black holes are already extremely powerful. 638 00:33:23,301 --> 00:33:25,035 So it makes a lot of sense to me that 639 00:33:25,136 --> 00:33:28,238 the ultra-high-energy cosmic rays could originate at 640 00:33:28,339 --> 00:33:30,440 supermassive black holes. 641 00:33:30,509 --> 00:33:35,690 The M87 galaxy is 54 million light years away. 642 00:33:35,713 --> 00:33:38,292 It's famous because we took a photo 643 00:33:38,317 --> 00:33:41,695 of the supermassive black hole at its core. 644 00:33:41,720 --> 00:33:45,967 So the event horizon telescope image of the swirling vortex of 645 00:33:45,990 --> 00:33:48,458 gas around that central black hole, 646 00:33:48,527 --> 00:33:50,559 that shadow that you can't actually see, 647 00:33:50,628 --> 00:33:55,432 that could be a site for the unbelievably energetic 648 00:33:55,534 --> 00:33:56,932 acceleration of cosmic rays. 649 00:33:57,035 --> 00:34:00,280 In March 2021, 650 00:34:00,305 --> 00:34:03,306 scientists analyze the data further. 651 00:34:03,442 --> 00:34:07,309 This new image of M87 shows very clear 652 00:34:07,445 --> 00:34:08,945 magnetic field lines, 653 00:34:09,047 --> 00:34:11,815 which is really stunning and reminds us of how much energy 654 00:34:11,916 --> 00:34:15,052 could be contained close to the supermassive black hole. 655 00:34:15,152 --> 00:34:17,820 Black holes have enormous power, 656 00:34:17,922 --> 00:34:20,902 but how do they transfer some of that energy 657 00:34:20,925 --> 00:34:22,159 to a tiny particle? 658 00:34:22,260 --> 00:34:25,327 One possibility for how supermassive black holes 659 00:34:25,463 --> 00:34:27,630 could accelerate such enormously energetic 660 00:34:27,733 --> 00:34:31,601 cosmic rays is that they actually drag or capture via 661 00:34:31,735 --> 00:34:32,936 their gravity 662 00:34:33,070 --> 00:34:36,405 preexisting normal cosmic rays, which are already 663 00:34:36,541 --> 00:34:37,840 extremely energetic, 664 00:34:37,943 --> 00:34:41,811 and then give them an extra boost to even higher energies. 665 00:34:41,914 --> 00:34:45,047 So supermassive black holes bend the fabric 666 00:34:45,117 --> 00:34:46,449 of spacetime around them, 667 00:34:46,550 --> 00:34:50,597 and even light particles can get stuck, and cosmic rays are 668 00:34:50,621 --> 00:34:53,657 no different... they can also be attracted by the supermassive 669 00:34:53,757 --> 00:34:57,360 black holes and get drawn into their orbit. 670 00:34:57,461 --> 00:35:00,809 It makes sense that the black hole captures 671 00:35:00,833 --> 00:35:02,498 passing cosmic rays, 672 00:35:02,601 --> 00:35:05,635 but how do the particles escape its clutches 673 00:35:05,737 --> 00:35:07,103 and hurtle towards us? 674 00:35:08,474 --> 00:35:12,253 M87 has a fearsome weapon in its arsenal. 675 00:35:12,277 --> 00:35:17,291 Enormous jets of energy blast out of its poles. 676 00:35:17,315 --> 00:35:20,851 So M87's jets are spectacularly large, 677 00:35:20,985 --> 00:35:23,954 larger than the entire galaxy that houses this black hole 678 00:35:24,056 --> 00:35:25,422 that's launching those jets. 679 00:35:25,523 --> 00:35:28,157 The powerful jets may give the cosmic rays 680 00:35:28,193 --> 00:35:29,559 a speed injection, 681 00:35:29,661 --> 00:35:33,163 transforming them from galactic rifle bullets into 682 00:35:33,264 --> 00:35:36,500 ultra-high-energy hypersonic missiles. 683 00:35:36,601 --> 00:35:41,036 So imagine if you had a regular bullet that 684 00:35:41,139 --> 00:35:43,784 you fired out of a gun at high speed, 685 00:35:43,809 --> 00:35:47,943 and as its flying, a little rocket motor in 686 00:35:48,079 --> 00:35:52,293 the bullet kicks in and takes it up to even higher speeds. 687 00:35:52,317 --> 00:35:54,650 That's sort of what's happening to 688 00:35:54,753 --> 00:35:57,119 the cosmic rays in these jets. 689 00:35:58,456 --> 00:36:00,356 Black holes may be the supervillains 690 00:36:00,458 --> 00:36:02,003 we've been looking for, 691 00:36:02,027 --> 00:36:04,905 firing out the fastest cosmic bullets, 692 00:36:04,929 --> 00:36:08,876 but cosmic rays have a superpower of their own. 693 00:36:08,900 --> 00:36:10,400 They're time travelers. 694 00:36:18,110 --> 00:36:20,710 Cosmic rays race through the universe at close 695 00:36:20,844 --> 00:36:24,813 to the speed of light... Like subatomic bullets, 696 00:36:24,916 --> 00:36:28,918 they can pierce spaceships and harm astronauts. 697 00:36:31,923 --> 00:36:34,623 But down on Earth, we're protected. 698 00:36:36,561 --> 00:36:41,675 Out of all of the rocky inner planets in the solar system, 699 00:36:41,699 --> 00:36:44,201 the Earth is the only one to generate 700 00:36:44,335 --> 00:36:48,304 its own deflector shield against this cosmic radiation. 701 00:36:48,373 --> 00:36:50,606 That's amazing. And that's where life is. 702 00:36:50,742 --> 00:36:54,210 I don't think that's actually all that much of a coincidence. 703 00:36:54,346 --> 00:36:58,047 The Earth creates its own magnetic field. 704 00:36:58,115 --> 00:37:01,217 The Earth has this wonderful active molten core of metal. 705 00:37:01,320 --> 00:37:04,766 All of that metal is moving around inside the Earth, 706 00:37:04,789 --> 00:37:07,556 and that moving metal generates a strong magnetic field. 707 00:37:07,659 --> 00:37:09,903 These cosmic rays are electrically charged. 708 00:37:09,927 --> 00:37:11,561 They follow a magnetic field. 709 00:37:11,663 --> 00:37:13,963 So our magnetic field deflects most 710 00:37:14,065 --> 00:37:15,931 of the cosmic rays around it. 711 00:37:16,034 --> 00:37:18,179 The shield is not perfect. 712 00:37:18,202 --> 00:37:21,248 Some cosmic rays do get through, 713 00:37:21,273 --> 00:37:24,284 but then they hit our second line of defense... 714 00:37:24,309 --> 00:37:25,786 The atmosphere. 715 00:37:25,811 --> 00:37:27,844 One of the things we have to be thankful for is 716 00:37:27,978 --> 00:37:30,512 our atmosphere... not only does it give us air to breathe, 717 00:37:30,648 --> 00:37:32,492 but it protects us from these space bullets. 718 00:37:32,516 --> 00:37:37,753 The atmosphere is like a missile defense system. 719 00:37:37,822 --> 00:37:40,601 Cosmic rays collide with air molecules, 720 00:37:40,626 --> 00:37:44,126 shattering into safer, smaller particles. 721 00:37:44,262 --> 00:37:48,364 The most common ones are called muons. 722 00:37:49,701 --> 00:37:54,204 The muons are the children of the cosmic rays. 723 00:37:54,306 --> 00:37:57,539 They're produced by these high-energy collisions 724 00:37:57,608 --> 00:37:58,885 in our upper atmosphere that 725 00:37:58,909 --> 00:38:02,545 create these showers of muons that then come down to 726 00:38:02,646 --> 00:38:03,757 the surface. 727 00:38:03,780 --> 00:38:05,994 There's as many as four of these cosmic rays passing 728 00:38:06,018 --> 00:38:07,594 through my hand every second. 729 00:38:07,619 --> 00:38:09,719 They're passing through your body right now. 730 00:38:09,788 --> 00:38:11,755 Muons are so abundant, 731 00:38:11,856 --> 00:38:14,824 we don't need a high-tech observatory to detect them, 732 00:38:14,958 --> 00:38:18,762 just a few things you'd find in a high school science lab. 733 00:38:18,829 --> 00:38:23,132 A small aquarium that I've attached a small piece of felt 734 00:38:23,233 --> 00:38:24,778 to the bottom. 735 00:38:24,802 --> 00:38:27,804 Some frozen carbon dioxide, some dry ice, 736 00:38:27,905 --> 00:38:33,788 hence the safety gloves, a flat piece of metal like this, 737 00:38:33,811 --> 00:38:35,644 some isopropyl alcohol. 738 00:38:37,416 --> 00:38:40,050 Then I flip the whole thing over 739 00:38:40,150 --> 00:38:43,320 onto the bottom, and I wait. 740 00:38:45,523 --> 00:38:49,503 So what's happening is that the alcohol in the felt is 741 00:38:49,527 --> 00:38:52,907 evaporating in sinking down, and because 742 00:38:52,931 --> 00:38:55,710 that bottom layer is so cold from the dry ice, 743 00:38:55,733 --> 00:39:00,135 it forms a super saturated cloud of alcohol vapor. 744 00:39:01,505 --> 00:39:05,286 When the charged particles pass through the cold vapor, 745 00:39:05,309 --> 00:39:09,713 they create tiny ghostly trails. 746 00:39:09,815 --> 00:39:12,592 What we're looking for are the muons, 747 00:39:12,617 --> 00:39:16,219 the subatomic particles generated when a cosmic ray 748 00:39:16,353 --> 00:39:18,699 strikes the upper atmosphere. 749 00:39:18,724 --> 00:39:21,824 Each silvery thread in the cloud chamber 750 00:39:21,960 --> 00:39:25,005 is the sign of a cosmic ray. 751 00:39:25,030 --> 00:39:28,876 These muons should never make it down to Earth at all. 752 00:39:28,900 --> 00:39:33,981 They only live for 2.2 microseconds before breaking up, 753 00:39:34,005 --> 00:39:35,704 not enough time to travel 754 00:39:35,806 --> 00:39:38,686 through six miles of Earth's atmosphere. 755 00:39:38,710 --> 00:39:41,844 Naively, we would think there's no way that a muon could make it 756 00:39:41,980 --> 00:39:44,146 from the upper atmosphere to where we are now 757 00:39:44,248 --> 00:39:45,193 without decaying. 758 00:39:45,217 --> 00:39:46,994 It turns out they do, and the only 759 00:39:47,018 --> 00:39:50,898 way they do this is they effectively time travel. 760 00:39:50,922 --> 00:39:54,423 The muons move at 98 percent the speed of light. 761 00:39:55,827 --> 00:39:57,505 They move so fast, 762 00:39:57,528 --> 00:40:01,063 they experience what Einstein called time dilation. 763 00:40:01,132 --> 00:40:04,733 Albert Einstein taught us that we live 764 00:40:04,802 --> 00:40:06,735 in a space time, and so that means 765 00:40:06,804 --> 00:40:10,340 that all measurements of lengths and durations of time 766 00:40:10,409 --> 00:40:11,940 are relative. 767 00:40:12,043 --> 00:40:13,809 From a muon's perspective, 768 00:40:13,911 --> 00:40:17,447 we humans move incredibly slowly. 769 00:40:17,516 --> 00:40:20,795 They're moving so fast that, for them, 770 00:40:20,818 --> 00:40:23,719 time is stretched out. 771 00:40:23,822 --> 00:40:27,856 What we found by measuring the energy and the lifetime of 772 00:40:27,958 --> 00:40:33,228 muons is that as muons got closer to the speed of light, 773 00:40:33,331 --> 00:40:37,733 their lifetime increased, because to them, time is 774 00:40:37,802 --> 00:40:41,237 slowing down, exactly the way Einstein predicted. 775 00:40:41,338 --> 00:40:45,385 Their lifespan is extended by more than 20 times 776 00:40:45,409 --> 00:40:46,608 from our perspective, 777 00:40:46,710 --> 00:40:49,012 so they make it to the ground. 778 00:40:51,949 --> 00:40:55,952 Cosmic rays are the ultimate space travelers. 779 00:40:56,054 --> 00:40:59,722 They're awe-inspiring speed allows us to unlock 780 00:40:59,824 --> 00:41:03,425 hidden processes and test our theories of physics. 781 00:41:04,728 --> 00:41:06,463 They're way more energetic than anything 782 00:41:06,530 --> 00:41:08,465 we can do in a laboratory on Earth. 783 00:41:08,532 --> 00:41:10,400 So that means we can unlock all kinds of 784 00:41:10,501 --> 00:41:13,036 new domains about physics at the highest, 785 00:41:13,137 --> 00:41:15,237 most extreme energies. 786 00:41:15,306 --> 00:41:17,851 They're our best link to the farthest reaches of 787 00:41:17,876 --> 00:41:19,641 the cosmos. 788 00:41:19,710 --> 00:41:23,445 To me, it's really exciting that we're actually sampling 789 00:41:23,547 --> 00:41:26,315 pieces of matter from distant 790 00:41:26,418 --> 00:41:30,197 stars, from distant galaxies, and we're getting them here at 791 00:41:30,222 --> 00:41:31,954 Earth and studying them. 792 00:41:33,925 --> 00:41:37,405 There are so many amazingly violent events in the universe, 793 00:41:37,429 --> 00:41:40,307 the birth of black holes, exploding stars. 794 00:41:40,331 --> 00:41:42,364 These cosmic rays that are going through your body 795 00:41:42,432 --> 00:41:45,579 right now are messengers from those events. 796 00:41:45,603 --> 00:41:47,503 In some way, you're still connected to 797 00:41:47,606 --> 00:41:49,938 those events, millions of light years away. 798 00:41:51,842 --> 00:41:54,043 These are messengers from the universe, 799 00:41:54,112 --> 00:41:56,012 telling us about how it works. 63837

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