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These are the user uploaded subtitles that are being translated: 1 00:00:02,460 --> 00:00:04,387 We've seen the movie. 2 00:00:04,412 --> 00:00:07,736 A huge asteroid heads towards Earth, 3 00:00:07,760 --> 00:00:10,263 It smashes through the atmosphere 4 00:00:10,288 --> 00:00:12,760 slams into the surface. 5 00:00:14,460 --> 00:00:17,413 Sends up a huge fireball 6 00:00:17,437 --> 00:00:19,935 and a deadly shockwave. 7 00:00:21,960 --> 00:00:24,736 The Earth dies screaming. 8 00:00:27,060 --> 00:00:30,536 But this is not one of those films. 9 00:00:30,760 --> 00:00:35,436 This is how the Earth and humans fight back. 10 00:00:36,560 --> 00:00:40,036 Putting the apocalypse on hold. 11 00:01:01,490 --> 00:01:03,266 Planet Earth. 12 00:01:04,190 --> 00:01:08,266 A cradle of life floating peacefully through space. 13 00:01:08,790 --> 00:01:10,766 Or is it? 14 00:01:11,367 --> 00:01:16,465 Our planet can be one of the most hostile places in the universe. 15 00:01:18,290 --> 00:01:21,680 Think about what natural disasters befall humanity. 16 00:01:21,760 --> 00:01:24,625 Earthquakes, hurricanes, tornadoes, 17 00:01:24,850 --> 00:01:27,874 all of these sorts of things, we can't do anything about those. 18 00:01:27,940 --> 00:01:28,990 But an asteroid? 19 00:01:29,140 --> 00:01:34,716 Hey, this is a huge natural disaster that we can actually prevent. 20 00:01:35,640 --> 00:01:38,386 When people hear the word asteroid the first thing that comes to mind 21 00:01:38,411 --> 00:01:42,416 are the Sci-Fi movies of these very dangerous asteroids coming to hit us. 22 00:01:42,440 --> 00:01:44,786 The story of how the dinosaurs became extinct. 23 00:01:45,011 --> 00:01:48,016 Yes, there are some asteroids out there that are dangerous. 24 00:01:48,640 --> 00:01:51,574 When it comes to finding asteroids in defending the Earth, 25 00:01:51,599 --> 00:01:54,454 Scientists are very solidly the heroes. 26 00:01:56,760 --> 00:02:00,136 Across the world, teams of planetary protectors 27 00:02:00,160 --> 00:02:03,536 are working out ways to cancel the apocalypse. 28 00:02:05,035 --> 00:02:07,235 They're scanning the skies, 29 00:02:08,260 --> 00:02:10,336 doing the math, 30 00:02:11,560 --> 00:02:13,636 designing the tech, 31 00:02:14,637 --> 00:02:20,335 and making the plans that could ensure planetary extinctions from space, 32 00:02:20,460 --> 00:02:24,436 are nothing more than science fiction. 33 00:02:26,760 --> 00:02:28,496 If you're facing an opponent. 34 00:02:28,520 --> 00:02:30,936 You need to know a lot about them in order to defeat them. 35 00:02:30,960 --> 00:02:34,980 Their size, their strength, what they're made of, how they move. 36 00:02:35,050 --> 00:02:37,760 Well, we need to know the same things about these asteroids. 37 00:02:37,810 --> 00:02:39,200 Cause we want to knock them out. 38 00:02:44,560 --> 00:02:46,536 To better understand this opponent, 39 00:02:46,560 --> 00:02:51,636 Cathy Plesko from Los Alamos National Laboratory travels to Arizona. 40 00:02:52,760 --> 00:02:54,836 Around 50 thousand years ago, 41 00:02:54,860 --> 00:02:58,236 this was Ground Zero for an impact 42 00:02:58,260 --> 00:03:02,536 that left a crater over 550 ft deep. 43 00:03:05,960 --> 00:03:09,036 This is Meteor Crater. 44 00:03:12,160 --> 00:03:18,736 This is, awe inspiring to stand on the rim of the crater like this and 45 00:03:18,760 --> 00:03:25,436 see the, the scale of something this large and feeling this small. 46 00:03:25,460 --> 00:03:27,636 Understanding just 47 00:03:27,660 --> 00:03:33,636 how much energy it must have taken to excavate this much rock. 48 00:03:38,760 --> 00:03:44,736 The meteor that carved out the crater landed with the power of a hydrogen bomb. 49 00:03:46,360 --> 00:03:50,936 But the sky rock was just 130 ft across. 50 00:03:52,760 --> 00:03:55,636 Meteor Crater is helping us understand 51 00:03:55,760 --> 00:03:59,536 how speed can turn a small projectile 52 00:04:00,760 --> 00:04:02,560 into a killer. 53 00:04:03,560 --> 00:04:08,636 The asteroid came in at about 27 thousand miles an hour 54 00:04:08,660 --> 00:04:13,936 that is ten times faster than the muzzle velocity of a bullet coming out of a rifle. 55 00:04:15,860 --> 00:04:19,436 It comes slamming into the surface and just explodes 56 00:04:20,060 --> 00:04:24,436 and that explosion then opens up the crater. 57 00:04:27,960 --> 00:04:32,836 The impact shocked the surrounding solid rock into dust 58 00:04:33,160 --> 00:04:37,736 and sent an immense shockwave barreling outwards. 59 00:04:38,360 --> 00:04:39,713 So it's pretty windy here today, 60 00:04:39,737 --> 00:04:41,412 but that's nothing like it would have been 61 00:04:41,436 --> 00:04:43,458 in the shockwave from an impact. 62 00:04:43,859 --> 00:04:46,836 Anywhere near by here would have seen winds 63 00:04:46,860 --> 00:04:50,260 of thousands of miles an hour as the shockwave came out. 64 00:04:53,960 --> 00:04:55,396 Scientists calculate 65 00:04:55,437 --> 00:05:01,359 there's a 20% chance of such a hit on earth every century. 66 00:05:01,760 --> 00:05:04,836 If an asteroid like this struck today, 67 00:05:04,960 --> 00:05:06,360 it could level a city. 68 00:05:08,360 --> 00:05:12,436 But Cathy's research is helping build up our defenses. 69 00:05:13,960 --> 00:05:16,278 So we think that there's a variety of ways that we might 70 00:05:16,303 --> 00:05:18,460 prevent an asteroid from hitting the Earth. 71 00:05:19,360 --> 00:05:21,353 My colleagues and I at Los Alamos 72 00:05:21,377 --> 00:05:23,277 and at Livermore and other places 73 00:05:23,301 --> 00:05:25,902 can use computer models on super computers 74 00:05:26,027 --> 00:05:29,360 to do very careful high-fidelity simulations. 75 00:05:29,460 --> 00:05:31,309 To tell us, what's a good idea. 76 00:05:31,510 --> 00:05:33,110 Maybe what's not a good idea. 77 00:05:33,150 --> 00:05:36,140 And then be able to present to policymakers 78 00:05:36,164 --> 00:05:38,164 okay here's what we can do. 79 00:05:38,230 --> 00:05:41,106 In comparison to what Bruce Willis could do. 80 00:05:45,230 --> 00:05:49,106 The most potent weapon in the planetary protectors arsenal, 81 00:05:49,330 --> 00:05:51,330 a nuclear bomb. 82 00:05:54,630 --> 00:05:58,706 Blowing up an asteroid this way has its drawbacks, 83 00:05:58,730 --> 00:06:03,906 it risks showering the Earth with hundreds of smaller meteors. 84 00:06:04,730 --> 00:06:08,906 But Cathy's team is working on plans that would avoid this risk, 85 00:06:08,930 --> 00:06:13,906 instead, they use a nuclear weapon to deflect an asteroid. 86 00:06:15,730 --> 00:06:18,806 So one of the things I do study is nuclear deflection. 87 00:06:19,030 --> 00:06:22,583 In some cases and in the near-term future 88 00:06:22,607 --> 00:06:26,829 there could be a scenario where we might need to 89 00:06:26,853 --> 00:06:29,229 shove something fairly large out of the way 90 00:06:29,330 --> 00:06:33,340 and those sorts of things, if they're large enough, 91 00:06:33,540 --> 00:06:36,816 we might need to use a nuclear device to do that. 92 00:06:36,915 --> 00:06:39,415 We might launch a nuclear device 93 00:06:39,440 --> 00:06:42,716 detonate it above the surface of the object 94 00:06:42,740 --> 00:06:44,940 changing its velocity a little bit. 95 00:06:46,040 --> 00:06:49,516 Detonating a nuclear device near an asteroid 96 00:06:49,540 --> 00:06:51,739 vaporizes part of its surface 97 00:06:51,840 --> 00:06:54,516 pushing the asteroid off course. 98 00:06:58,340 --> 00:07:01,716 But firing nuclear weapons into space 99 00:07:01,740 --> 00:07:03,839 is no one's first choice. 100 00:07:04,640 --> 00:07:07,016 So there's some pros and cons to using nuclear deflection 101 00:07:07,040 --> 00:07:09,616 there's some situations where it is definitely 102 00:07:09,640 --> 00:07:11,316 an appropriate technology 103 00:07:11,340 --> 00:07:14,340 where it may be the only option at the time. 104 00:07:14,364 --> 00:07:15,964 But we hope in the future, 105 00:07:16,040 --> 00:07:21,416 that will have other methods at our disposal that are not as 106 00:07:21,540 --> 00:07:25,216 challenging, diplomatically or politically. 107 00:07:27,040 --> 00:07:31,817 The race is on, for scientists to find a way to deflect an asteroid 108 00:07:31,864 --> 00:07:34,864 without using nuclear weapons. 109 00:07:37,540 --> 00:07:39,593 We're discovering more and more about the asteroids 110 00:07:39,617 --> 00:07:40,639 we're understanding them 111 00:07:40,740 --> 00:07:43,451 and we're realizing that there really are ways we can mitigate 112 00:07:43,475 --> 00:07:46,116 the destructive effects of an impact on Earth. 113 00:07:46,440 --> 00:07:53,416 This could be the most important scientific endeavor humanity has ever undertaken. 114 00:07:53,440 --> 00:07:58,916 And the best way to cancel the asteroid apocalypse could be to take them out 115 00:07:58,940 --> 00:08:02,416 before they even become a threat. 116 00:08:17,770 --> 00:08:21,346 Our solar system is a dangerous place. 117 00:08:23,370 --> 00:08:27,046 Fast moving asteroids hurtle through space. 118 00:08:29,570 --> 00:08:33,646 And many of these rocks are headed our way. 119 00:08:34,970 --> 00:08:36,946 To counter the asteroid threat 120 00:08:36,970 --> 00:08:40,570 scientists are drawing up battle plans. 121 00:08:46,150 --> 00:08:48,916 The very first step in understanding this hazard 122 00:08:48,940 --> 00:08:52,256 and in preventing this hazard, is to find them. 123 00:08:52,949 --> 00:08:55,149 Not just the big ones that could end our civilization 124 00:08:55,250 --> 00:08:58,050 but even the small that could devastate your city. 125 00:09:05,000 --> 00:09:09,576 High in the mountains at the Catalina Sky survey in Arizona 126 00:09:09,700 --> 00:09:13,876 asteroid Hunter Greg Leonard is leading the search. 127 00:09:14,300 --> 00:09:17,276 We are the eyes for the world 128 00:09:17,300 --> 00:09:20,900 on this night, at this telescope, on the summit of this mountain. 129 00:09:21,850 --> 00:09:26,162 By comparing four images of the same patch of sky 130 00:09:26,186 --> 00:09:29,376 taken over a 20 minute period. 131 00:09:29,400 --> 00:09:35,776 Greg can hunt for elusive asteroids hidden among the stars. 132 00:09:35,800 --> 00:09:39,776 Because in these images, stars don't move. 133 00:09:39,800 --> 00:09:42,576 But asteroids do. 134 00:09:42,600 --> 00:09:44,776 If it's a really bright asteroid, 135 00:09:44,800 --> 00:09:50,576 we will see some bright points of light tracking across the four images. 136 00:09:55,800 --> 00:09:58,776 You have to kiss a lot of frogs before you get a prince or a princess 137 00:09:58,800 --> 00:10:02,376 and this is the case tonight as it is almost every night. 138 00:10:05,200 --> 00:10:06,576 Here we go! 139 00:10:07,200 --> 00:10:08,976 This is a real object. 140 00:10:09,000 --> 00:10:10,676 You can see it's moving 141 00:10:10,700 --> 00:10:14,300 across the sky hear from the lower right to the upper left 142 00:10:14,324 --> 00:10:17,601 we are very, very excited to have discovered one tonight. 143 00:10:17,625 --> 00:10:21,476 Because this is an object that's approaching near Earth space. 144 00:10:21,500 --> 00:10:23,776 Likely in the neighborhood of Earth. 145 00:10:25,000 --> 00:10:26,976 Greg's research reveals 146 00:10:27,000 --> 00:10:34,376 this 100 ft asteroid could get as close as 630 thousand miles to Earth. 147 00:10:34,400 --> 00:10:38,176 That's less than three times the distance to the Moon. 148 00:10:39,600 --> 00:10:42,676 And in the future, this asteroid's orbit 149 00:10:42,700 --> 00:10:45,120 could move closer to Earth. 150 00:10:45,400 --> 00:10:48,229 Even onto a collision course. 151 00:10:48,854 --> 00:10:52,076 If that happens, we need to be ready for it. 152 00:10:54,000 --> 00:10:55,513 The earlier we spot it, 153 00:10:55,538 --> 00:10:58,974 the best chance we have of altering its course. 154 00:10:59,970 --> 00:11:02,440 Space is so big and the Earth is so small 155 00:11:02,470 --> 00:11:05,210 and the asteroid would be starting from so far away, 156 00:11:05,340 --> 00:11:07,176 that if you just deflected it a little bit 157 00:11:07,200 --> 00:11:09,865 gave it a little nudge, a tiny course correction 158 00:11:09,950 --> 00:11:13,270 by the time it got to where the Earth's region is, 159 00:11:13,300 --> 00:11:15,620 it would miss us completely. 160 00:11:16,600 --> 00:11:21,040 To do that, we need to move asteroids off their trajectory. 161 00:11:23,800 --> 00:11:25,392 Think of a golf swing, 162 00:11:25,417 --> 00:11:27,969 hook or shank the ball by just 163 00:11:27,993 --> 00:11:29,792 one degree off of the tee 164 00:11:29,860 --> 00:11:32,143 and you'll miss the green completely. 165 00:11:33,600 --> 00:11:36,745 Now, scale that up to asteroids. 166 00:11:37,070 --> 00:11:41,776 Over time, space rocks can leave their home turf of the asteroid belt 167 00:11:41,900 --> 00:11:44,876 becoming threatening near-earth objects 168 00:11:44,900 --> 00:11:49,276 30 million miles away that could one day hit our planet. 169 00:11:50,900 --> 00:11:55,902 But if planetary protectors can change the course of a dangerous object 170 00:11:55,927 --> 00:11:58,300 by just a tenth of a degree, 171 00:11:58,525 --> 00:12:00,876 they'd miss the Earth completely. 172 00:12:02,400 --> 00:12:07,076 And scientists have come up with a very direct way to do it. 173 00:12:09,700 --> 00:12:12,176 In a football game, if somebody on the defense has 174 00:12:12,200 --> 00:12:15,286 seen the quarterback running into the endzone, what do they do? 175 00:12:15,310 --> 00:12:19,050 Boom, hit him, knock him out of bounds, knock them down, do something like that. 176 00:12:19,100 --> 00:12:21,773 That's what we want to do with asteroids. 177 00:12:21,798 --> 00:12:25,714 So if we send something moving towards an asteroid very quickly to hit it 178 00:12:25,800 --> 00:12:27,650 we call that a kinetic impactor. 179 00:12:27,690 --> 00:12:29,546 Slams into it really hard, 180 00:12:29,570 --> 00:12:34,046 changes not just the velocity of the asteroid but also its trajectory. 181 00:12:38,470 --> 00:12:43,546 Scientists have already intercepted asteroid like objects in space 182 00:12:46,645 --> 00:12:52,045 2005, the Deep Impact Spacecraft arrived at Temple One 183 00:12:52,070 --> 00:12:55,746 a comet half the size of Manhattan. 184 00:12:58,670 --> 00:13:02,946 This spacecraft shot a little probe at the comet. 185 00:13:06,170 --> 00:13:09,711 Like a bullet, it slammed into Temple One 186 00:13:09,736 --> 00:13:12,546 picking up material from the surface. 187 00:13:15,470 --> 00:13:18,546 Research into kinetics impactors continues. 188 00:13:19,670 --> 00:13:24,046 In 2022, a spacecraft called Dart 189 00:13:24,070 --> 00:13:26,445 will slam into an asteroid 190 00:13:26,470 --> 00:13:30,646 at over 13 thousand miles an hour. 191 00:13:30,670 --> 00:13:32,617 That transfer of momentum, 192 00:13:32,642 --> 00:13:36,915 would change the velocity of the asteroid, just a little bit 193 00:13:36,990 --> 00:13:40,620 maybe, a fraction of a mile per hour. 194 00:13:40,650 --> 00:13:42,944 But over maybe a decade 195 00:13:42,969 --> 00:13:46,926 that change in velocity, even though it's very tiny, would add up 196 00:13:46,950 --> 00:13:51,426 to a change in position big enough to completely miss the Earth. 197 00:13:56,150 --> 00:14:00,726 Knocking a giant space rock off course may sound unusual 198 00:14:02,350 --> 00:14:04,528 but astronomers have discovered, 199 00:14:04,552 --> 00:14:07,750 that in space, it's happened a lot. 200 00:14:10,250 --> 00:14:12,376 When you have a lot of traffic driving on the highway 201 00:14:12,400 --> 00:14:13,996 and a lot of lane changing going on. 202 00:14:14,020 --> 00:14:16,157 Sooner or later there's going to be a fender bender 203 00:14:16,182 --> 00:14:18,696 and that happens in our solar system as well. 204 00:14:19,720 --> 00:14:21,758 It's a busy place out there in the asteroid belt 205 00:14:21,783 --> 00:14:25,896 asteroids will run into each other at many miles per second. 206 00:14:25,920 --> 00:14:29,750 Relative speeds. And when that happens, the sparks fly. 207 00:14:33,810 --> 00:14:37,310 If you started with two asteroids and they collided, 208 00:14:37,350 --> 00:14:39,200 suddenly, you'd have ten asteroids. 209 00:14:39,240 --> 00:14:41,831 Those ten asteroids are now going to collide again 210 00:14:41,856 --> 00:14:43,744 and now you have a hundred asteroids. 211 00:14:43,790 --> 00:14:45,616 Those asteroids will collide and now you have 212 00:14:45,640 --> 00:14:49,870 a thousand, a million, a billion, possible impactors for the Earth. 213 00:14:51,980 --> 00:14:55,356 But this war isn't just a numbers game, 214 00:14:55,380 --> 00:15:00,185 because asteroids aren't all built out of the same stuff. 215 00:15:00,210 --> 00:15:01,756 So we're going to need, 216 00:15:01,880 --> 00:15:07,056 different kinds of weapons to take each type out. 217 00:15:23,810 --> 00:15:24,955 Across the world 218 00:15:24,979 --> 00:15:28,386 planetary protectors are developing battle strategies 219 00:15:28,410 --> 00:15:32,786 to save us from a major asteroid impact. 220 00:15:34,710 --> 00:15:37,457 But there's millions of asteroids in the solar system 221 00:15:37,482 --> 00:15:40,386 and each one presents a different type of threat. 222 00:15:42,410 --> 00:15:45,690 Their speed, size and distance from the earth 223 00:15:45,715 --> 00:15:48,786 help dictate the degree of danger. 224 00:15:49,910 --> 00:15:52,513 The more we can really understand about an asteroid, 225 00:15:52,538 --> 00:15:56,186 the better prepared we are to be able to defend against it. 226 00:15:57,510 --> 00:15:59,635 This is definitely a case of 'Know thy enemy' 227 00:15:59,660 --> 00:16:02,272 we need to know something about the properties of these objects 228 00:16:02,297 --> 00:16:07,830 if we have any hope of a moving a threatening one out of our path one day. 229 00:16:10,690 --> 00:16:12,613 But scientists are realizing 230 00:16:12,638 --> 00:16:16,690 that an asteroid's composition could be the deadliest factor. 231 00:16:20,390 --> 00:16:24,566 Knowing what asteroids are made of can help us find chinks in their armor. 232 00:16:27,890 --> 00:16:31,766 Marina Brozovic from the center for near-earth object studies 233 00:16:31,790 --> 00:16:35,166 uses a technology developed during World War II. 234 00:16:36,190 --> 00:16:37,589 Radar. 235 00:16:40,390 --> 00:16:45,766 Planetary radar is really like a big cousin of airport radar and so 236 00:16:45,790 --> 00:16:50,490 the same way like the airport is tracking airplanes we are tracking asteroids. 237 00:16:50,590 --> 00:16:54,966 That are, you know, hundreds of thousands sometimes millions of kilometers away. 238 00:16:54,990 --> 00:16:57,177 Another thing that radars do is 239 00:16:57,202 --> 00:17:01,266 they tell us about how this asteroid looks like. 240 00:17:01,290 --> 00:17:04,262 You to know: What's their size? What's their shape? 241 00:17:04,287 --> 00:17:06,666 What's their chemical composition? 242 00:17:06,690 --> 00:17:08,885 Considering the detail that we see on the surface, 243 00:17:08,910 --> 00:17:11,824 short of sending a spacecraft, you cannot achieve that. 244 00:17:11,849 --> 00:17:15,090 So radar is, in a way, it's own little space mission. 245 00:17:16,090 --> 00:17:19,766 Radar shows that asteroids can be made of rock, 246 00:17:20,990 --> 00:17:22,284 metal, 247 00:17:23,109 --> 00:17:26,166 or a combination of the two. 248 00:17:27,190 --> 00:17:31,966 This is crucial information for calculating how to deal with them. 249 00:17:33,690 --> 00:17:37,300 So metallic asteroids are far more dense 250 00:17:37,370 --> 00:17:39,113 then a normal rocky asteroid. 251 00:17:39,138 --> 00:17:43,733 So an impact from a big iron asteroid could have much more energy 252 00:17:43,770 --> 00:17:47,140 for the same size asteroid that was just rocky. 253 00:17:48,030 --> 00:17:49,630 Just as a metal cannonball 254 00:17:49,655 --> 00:17:53,006 would do more damage than a similar sized rock, 255 00:17:53,030 --> 00:17:58,406 metallic asteroids could be far more deadly than rocky asteroids. 256 00:17:59,430 --> 00:18:04,106 But scientists have now discovered that most asteroids are less like cannonballs 257 00:18:04,130 --> 00:18:08,106 and more like vast cosmic shotgun shells. 258 00:18:10,130 --> 00:18:12,176 Most of the asteroids, they're not a single object, 259 00:18:12,201 --> 00:18:15,130 they're not monolithic but instead, their rubble piles. 260 00:18:15,230 --> 00:18:18,278 So they consist of many smaller rocks and pebbles 261 00:18:18,303 --> 00:18:21,370 and grains and pieces of sand. 262 00:18:21,470 --> 00:18:24,846 And all of this is held very loosely with gravity. 263 00:18:25,770 --> 00:18:29,813 Rubble pile asteroids like the peanut shaped Itokawa 264 00:18:29,838 --> 00:18:34,246 probably formed from violent collisions between asteroids. 265 00:18:36,370 --> 00:18:41,546 Initially, the rocky debris from these collisions scatters like shrapnel. 266 00:18:42,170 --> 00:18:48,146 Then gravity can draw some of the rocks loosely back together again. 267 00:18:50,970 --> 00:18:53,689 The structure of rubble pile asteroids presents 268 00:18:53,714 --> 00:18:57,370 a major challenge to our planetary protectors. 269 00:18:59,370 --> 00:19:04,346 How can our science heroes save us from a pile of rubble? 270 00:19:04,370 --> 00:19:06,570 If the object is a solid mass of metal. 271 00:19:06,720 --> 00:19:11,090 It's going to respond to an impact or an explosion in a far different way 272 00:19:11,140 --> 00:19:14,100 than if it's just a loosely bound rubble pile 273 00:19:14,125 --> 00:19:16,340 barely held together by its own gravity. 274 00:19:16,440 --> 00:19:18,709 Well, they're very, very delicate objects 275 00:19:18,734 --> 00:19:22,516 and so those objects need some special consideration. 276 00:19:22,540 --> 00:19:26,316 We can't just go slamming into them necessarily. 277 00:19:28,040 --> 00:19:30,633 Smashing into a rubble pile asteroid 278 00:19:30,658 --> 00:19:34,340 would be like kicking a pile of leaves. 279 00:19:34,440 --> 00:19:39,516 Thousands of smaller rocks would go hurtling out in every direction. 280 00:19:39,915 --> 00:19:45,915 They'd be undetectable, unpredictable and could continue to head our way. 281 00:19:47,340 --> 00:19:50,816 But we have a plan. 282 00:19:52,040 --> 00:19:54,530 Instead of using violent force, 283 00:19:54,555 --> 00:19:58,716 we could use the gentle tug of gravity. 284 00:20:00,040 --> 00:20:03,950 So instead of this ham-fisted approach of whacking it and then just walking away. 285 00:20:04,020 --> 00:20:05,096 We need something. 286 00:20:05,220 --> 00:20:07,911 We need something more careful, something more precise 287 00:20:07,936 --> 00:20:11,020 and that's where the gravity tractor comes in. 288 00:20:14,120 --> 00:20:16,996 Rubble piles of rock may be small, 289 00:20:17,020 --> 00:20:18,535 but it has gravity. 290 00:20:18,560 --> 00:20:21,904 And if we send up a probe that has the mass of say, a ton. 291 00:20:21,970 --> 00:20:24,150 It has gravity too. Now, not much. 292 00:20:24,230 --> 00:20:25,430 But it's there. 293 00:20:25,560 --> 00:20:27,916 And if you put it near the asteroid, 294 00:20:27,940 --> 00:20:30,107 You can actually use the mutual gravity, 295 00:20:30,132 --> 00:20:35,340 the attraction between them, to tug the asteroid into a safe orbit. 296 00:20:37,090 --> 00:20:40,266 All you have to do is park a spacecraft next to the asteroid, 297 00:20:40,290 --> 00:20:41,317 Hover it there, 298 00:20:41,342 --> 00:20:44,926 don't let the gravity of the asteroid and the spacecraft pull each other together, 299 00:20:44,950 --> 00:20:47,492 and let the gravity of the spacecraft 300 00:20:47,517 --> 00:20:51,250 act as a tow line to pull the asteroid out of the way. 301 00:20:53,450 --> 00:20:55,089 This sounds like science fiction, 302 00:20:55,114 --> 00:20:58,844 but it turns out the physics of this is relatively simple. 303 00:20:58,880 --> 00:21:00,956 And we can do it. 304 00:21:04,180 --> 00:21:06,329 But gravity tractors only work 305 00:21:06,354 --> 00:21:10,380 if we can accurately track the movements of these asteroids. 306 00:21:12,480 --> 00:21:16,756 Problem is, there's a massive complicating factor 307 00:21:16,780 --> 00:21:19,570 at the center of our solar system. 308 00:21:20,500 --> 00:21:22,776 The Sun. 309 00:21:40,500 --> 00:21:45,376 Planetary protectors want to put the apocalypse on hold. 310 00:21:48,000 --> 00:21:49,569 Their mission: 311 00:21:49,594 --> 00:21:54,800 Protect the Earth from these seemingly inevitable asteroid impacts. 312 00:21:57,100 --> 00:22:02,176 But to do that, they need to predict their every move. 313 00:22:03,600 --> 00:22:07,961 In a constantly changing Solar system, that's not easy. 314 00:22:07,986 --> 00:22:10,957 We measure their orbits and we can draw up maps of 315 00:22:10,982 --> 00:22:13,724 all their orbits as we see them today. 316 00:22:13,780 --> 00:22:16,398 But we know that it's not a static population, 317 00:22:16,423 --> 00:22:22,356 that it's dynamic, things are constantly evolving in the asteroid belt. 318 00:22:22,380 --> 00:22:24,895 It's not just about size with asteroids. 319 00:22:24,920 --> 00:22:26,656 You have to understand the density, 320 00:22:26,680 --> 00:22:30,556 the orbit, the speed, in order to really tackle it. 321 00:22:32,180 --> 00:22:36,856 Collisions can set asteroid debris off on new orbits. 322 00:22:38,880 --> 00:22:46,656 But there's another factor at play, the immense gravity of the gas giant, Jupiter. 323 00:22:46,680 --> 00:22:49,422 Jupiter is the most massive planet in the solar system and 324 00:22:49,447 --> 00:22:51,556 it's sitting outside the asteroid belt. 325 00:22:51,600 --> 00:22:54,333 It's gravity can tweak and tug these asteroids 326 00:22:54,358 --> 00:22:56,306 and make their orbits more elliptical. 327 00:22:56,330 --> 00:22:58,120 Sending them in towards the Sun. 328 00:22:58,170 --> 00:23:00,050 Crossing Earth's orbit. 329 00:23:01,570 --> 00:23:06,846 Modeling Jupiter's effect on millions of asteroids is hard enough. 330 00:23:06,870 --> 00:23:13,146 Now add the influence of some of the asteroid belts biggest bruisers. 331 00:23:13,170 --> 00:23:16,539 300 mile wide rocks like Vesta 332 00:23:17,464 --> 00:23:20,546 and Pallas. 333 00:23:21,370 --> 00:23:26,146 A tricky task becomes near impossible. 334 00:23:29,670 --> 00:23:36,646 But gravity isn't the only force creating orbital chaos. 335 00:23:36,670 --> 00:23:41,048 This is the asteroid Bennu. 336 00:23:41,073 --> 00:23:46,346 There's one chance in 2700 it'll hit the Earth. 337 00:23:46,370 --> 00:23:50,068 But Bennu's orbit keeps changing. 338 00:23:50,093 --> 00:23:56,546 In the last 18 years, it shifted over a hundred miles off course 339 00:23:56,570 --> 00:24:00,746 and the culprit could be the Sun. 340 00:24:00,770 --> 00:24:03,086 So what can change the orbit of an asteroid? 341 00:24:03,110 --> 00:24:05,300 It's easy to think of these large rocks 342 00:24:05,325 --> 00:24:08,386 passing by each other tugging on each other gravitationally. 343 00:24:08,410 --> 00:24:12,786 But could the most dramatic changes be due something as gentle as sunlight? 344 00:24:12,810 --> 00:24:15,092 It might feel very subtle, but the sunlight, 345 00:24:15,117 --> 00:24:18,614 on our bodies, exerts a subtle pressure. 346 00:24:18,680 --> 00:24:22,340 The fact that you're hotter on one side than on the other side, 347 00:24:22,390 --> 00:24:27,080 actually exerts a kind of a thrust that can move you around. 348 00:24:27,670 --> 00:24:32,646 Sunlight is made up of tiny packets of energy called photons. 349 00:24:32,670 --> 00:24:34,649 When photons hit an asteroid 350 00:24:34,674 --> 00:24:37,546 they pass on a tiny amount of momentum 351 00:24:37,570 --> 00:24:40,446 and a tiny amount of heat. 352 00:24:41,570 --> 00:24:44,006 Let's actually, you know, let's imagine this situation, 353 00:24:44,031 --> 00:24:47,037 here's our asteroid, in reality, this might be, 354 00:24:47,062 --> 00:24:49,593 10 miles across or a mile across, something like that. 355 00:24:49,620 --> 00:24:52,320 Here's our asteroid, here's the Sun. 356 00:24:52,390 --> 00:24:55,120 This asteroid is orbiting the Sun this way. 357 00:24:55,150 --> 00:24:58,916 This face of the asteroid is being warmed by the heat from the Sun. 358 00:24:58,940 --> 00:25:03,261 Out here on the back side facing the cold vacuum of space it's a lot colder. 359 00:25:03,286 --> 00:25:06,754 In fact, I can even feel it already with my hands. 360 00:25:06,800 --> 00:25:09,490 The warm side that's being illuminated by sunshine 361 00:25:09,530 --> 00:25:13,710 actually re-radiates that heat in the infrared portion of the spectrum. 362 00:25:13,760 --> 00:25:17,050 All of that infrared radiation off the side of the asteroid 363 00:25:17,075 --> 00:25:19,536 acts like a like a little rocket motor in a way. 364 00:25:19,560 --> 00:25:22,936 It actually pushes on the asteroid. 365 00:25:22,960 --> 00:25:26,551 This is known as the Yarkovsky effect, 366 00:25:26,576 --> 00:25:29,036 it's a slow process. 367 00:25:29,060 --> 00:25:31,900 The asteroid is pushed by a force 368 00:25:31,925 --> 00:25:37,660 equal to the weight of a few grapes on Earth. 369 00:25:37,760 --> 00:25:43,136 But as Bennu circles the Sun it heats up on one side 370 00:25:43,160 --> 00:25:47,236 which moves it into a different orbit. 371 00:25:49,760 --> 00:25:52,536 The Yarkovsky effect is actually a bit of a problem. 372 00:25:52,560 --> 00:25:55,217 If there were just gravity acting on these asteroids 373 00:25:55,242 --> 00:25:58,125 then we can predict where all the asteroids and planets will be 374 00:25:58,150 --> 00:26:01,086 and we'd be able to figure out the trajectory of these asteroids 375 00:26:01,111 --> 00:26:02,608 many years in the future. 376 00:26:02,660 --> 00:26:04,450 But with the Yarkovsky effect, 377 00:26:04,490 --> 00:26:07,276 that actually changes it in ways that are difficult to predict. 378 00:26:07,301 --> 00:26:09,877 Because it depends on how dark the asteroid is, 379 00:26:09,902 --> 00:26:12,214 whether it's spinning, what shape it is 380 00:26:12,290 --> 00:26:15,830 and so it makes the orbit of the asteroid much, much more difficult to predict 381 00:26:15,920 --> 00:26:18,441 a long time into the future. 382 00:26:19,766 --> 00:26:24,938 The Yarkovsky effect makes predicting the movement of asteroids like Bennu, 383 00:26:24,963 --> 00:26:26,795 even harder. 384 00:26:26,820 --> 00:26:31,324 But our planetary protectors are an ingenious bunch 385 00:26:31,349 --> 00:26:34,189 and they're attempting to use the Yarkovsky effect 386 00:26:34,214 --> 00:26:37,621 to create a new weapon for their armory. 387 00:26:37,720 --> 00:26:39,860 So the Yarkovsky effect we know can 388 00:26:39,885 --> 00:26:44,095 change asteroid orbits pretty dramatically. 389 00:26:44,119 --> 00:26:46,544 It's an effect that we could use 390 00:26:46,620 --> 00:26:48,540 to move asteroids ourselves. 391 00:26:48,570 --> 00:26:51,456 If we could change the way the asteroid is heated by the Sun. 392 00:26:51,480 --> 00:26:54,020 By changing its color or 393 00:26:54,080 --> 00:26:57,456 changing its shape so that it gets heated in a very specific way, 394 00:26:57,480 --> 00:27:00,656 That we could change its orbit that way. 395 00:27:01,580 --> 00:27:05,280 If scientists could send a satellite to an asteroid, 396 00:27:05,305 --> 00:27:08,040 it could use black or white paint 397 00:27:08,065 --> 00:27:11,604 to increase or decrease the heating effect. 398 00:27:12,780 --> 00:27:15,556 But at the University of Southern California, 399 00:27:15,580 --> 00:27:19,666 a team of scientists are working on a higher tech solution. 400 00:27:19,691 --> 00:27:22,380 They're trying to one-up the Yarkovsky effect 401 00:27:22,480 --> 00:27:28,256 using a space-based laser called D-Star. 402 00:27:28,280 --> 00:27:31,880 Let's say we see an asteroid that's on its way towards the Earth. 403 00:27:31,940 --> 00:27:35,452 We can use space lasers to zap the asteroid. 404 00:27:35,477 --> 00:27:37,454 You vaporize the surface material. 405 00:27:37,530 --> 00:27:40,602 That turns into a gas which expands very quickly 406 00:27:40,627 --> 00:27:42,526 and that acts like a rocket. 407 00:27:42,550 --> 00:27:45,485 And so you can use that to push the asteroid 408 00:27:45,510 --> 00:27:47,750 into a safer path as well. 409 00:27:49,650 --> 00:27:52,435 Space lasers are another powerful weapon 410 00:27:52,460 --> 00:27:56,776 for our planetary protectors fight against asteroids. 411 00:27:57,950 --> 00:28:00,726 They joined gravity tractors, 412 00:28:00,750 --> 00:28:03,767 kinetic impactors 413 00:28:03,792 --> 00:28:07,650 and nuclear weapons in the armory. 414 00:28:07,750 --> 00:28:11,626 But there is one very big problem. 415 00:28:11,750 --> 00:28:14,651 All of the methods of defending against asteroids that we've mentioned 416 00:28:14,776 --> 00:28:16,550 are technologically possible. 417 00:28:16,650 --> 00:28:18,828 The thing that's a little bit nerve-wracking is that 418 00:28:18,853 --> 00:28:23,526 none of them are actually ready to go right now. 419 00:28:23,550 --> 00:28:26,700 So it's not time to cancel the apocalypse yet. 420 00:28:26,725 --> 00:28:29,712 We've made a lot of progress especially in the last few years. 421 00:28:29,737 --> 00:28:31,406 But we're not really there yet. 422 00:28:31,431 --> 00:28:36,974 But we could get to that point within the next maybe 10 or 15 years. 423 00:28:39,850 --> 00:28:42,326 But don't panic just yet. 424 00:28:42,350 --> 00:28:46,481 Turns out the Earth has a built-in defense system 425 00:28:46,506 --> 00:28:51,826 that can burn up asteroids, before they ever hit the ground. 426 00:29:08,930 --> 00:29:14,106 Arizona, June 2nd 2016. 427 00:29:14,130 --> 00:29:19,506 A 5 ft wide rock hurdles towards the Earth. 428 00:29:19,530 --> 00:29:24,606 It's moving at over 40 thousand miles per hour 429 00:29:24,630 --> 00:29:29,706 and as it streaks overhead, it lights up the sky. 430 00:29:32,030 --> 00:29:33,951 In the very early morning hours, 431 00:29:33,976 --> 00:29:37,206 an asteroid came screaming into the Earth's atmosphere 432 00:29:37,230 --> 00:29:39,020 far faster than a rifle bullet. 433 00:29:39,060 --> 00:29:43,616 There was a fireball that lit up the Red Rocks all around us that night. 434 00:29:43,640 --> 00:29:46,127 It was bright enough to burn out cameras on the ground 435 00:29:46,152 --> 00:29:48,840 from NASA that were watching for fireballs. 436 00:29:49,940 --> 00:29:53,134 The asteroid is just seconds away from impact 437 00:29:53,159 --> 00:29:56,540 and major damage seems inevitable. 438 00:29:59,240 --> 00:30:05,734 But the asteroid never makes it to the ground, why? 439 00:30:05,759 --> 00:30:10,930 We do have a natural barrier against at least small asteroid impacts. 440 00:30:11,010 --> 00:30:12,880 And let me give you a hint about what that is. 441 00:30:18,650 --> 00:30:20,811 The air around us seems too tenuous 442 00:30:20,836 --> 00:30:23,126 to actually defend against a threat from space. 443 00:30:23,150 --> 00:30:28,526 But in fact, the atmosphere is sort of the last line of defense against asteroids. 444 00:30:29,450 --> 00:30:35,926 One day our planetary protectors will be ready to save us from asteroid strikes. 445 00:30:35,950 --> 00:30:42,126 Until then, we'll have to rely on the Earth's built in defense system, 446 00:30:42,150 --> 00:30:45,226 the atmosphere. 447 00:30:45,250 --> 00:30:48,230 We know for a fact that our atmosphere acts like a shield. 448 00:30:48,260 --> 00:30:52,613 Because space rocks come the earth every day. 449 00:30:52,637 --> 00:30:54,835 Some of them are tiny, some of them are a bit larger. 450 00:30:54,860 --> 00:30:58,463 But what's happening is that as they enter the atmosphere at high speed 451 00:30:58,488 --> 00:31:01,160 the friction burns them up. 452 00:31:01,960 --> 00:31:05,736 Even though the top layers of the atmosphere are very thin, 453 00:31:05,760 --> 00:31:12,336 compared to the vacuum of space, they're extremely dense. 454 00:31:12,360 --> 00:31:15,242 As rocky asteroids hurtle through the atmosphere, 455 00:31:15,267 --> 00:31:21,836 friction and air pressure can heat them to over 3 thousand degrees Fahrenheit. 456 00:31:21,860 --> 00:31:25,536 The larger the asteroid, the longer it takes to burn up. 457 00:31:25,560 --> 00:31:31,936 And for these larger rocks, the effects can be dramatic. 458 00:31:31,960 --> 00:31:35,216 If there's a rock that's big enough that it doesn't burn out very quickly. 459 00:31:35,240 --> 00:31:38,879 We call that a bolide, and as the bolide falls through the atmosphere, 460 00:31:38,904 --> 00:31:42,858 it creates a spectacular show, called a fireball. 461 00:31:44,160 --> 00:31:50,336 In February 2013, the town of Chelyabinsk in Russia had it's own fireball 462 00:31:50,360 --> 00:31:55,036 when a 60 ft wide space rock barreled through the sky. 463 00:31:58,460 --> 00:32:03,436 This asteroid was bigger than a school bus 464 00:32:03,460 --> 00:32:07,250 and it traveled at 11 miles per second. 465 00:32:07,290 --> 00:32:10,389 It got super hot, broke up into small pieces, 466 00:32:10,414 --> 00:32:13,566 those pieces then rammed through the atmosphere. 467 00:32:13,590 --> 00:32:16,676 When all of that vast energy of motion of this rock 468 00:32:16,700 --> 00:32:21,154 was converted into light and heat, it exploded. 469 00:32:23,270 --> 00:32:27,346 The Chelyabinsk meteor is the largest natural object seen 470 00:32:27,371 --> 00:32:31,146 entering the atmosphere in over a hundred years. 471 00:32:33,370 --> 00:32:37,055 It explodes 12 miles above the Earth's surface 472 00:32:37,080 --> 00:32:40,146 with the power of 30 nuclear bombs. 473 00:32:43,970 --> 00:32:51,646 The blast causes over 15 hundred injuries and damages seven thousand buildings. 474 00:32:51,670 --> 00:32:54,846 But if it wasn't for the protective shielding of our atmosphere, 475 00:32:54,870 --> 00:32:59,046 the results would have been far worse. 476 00:33:01,270 --> 00:33:02,364 The problem is, 477 00:33:02,389 --> 00:33:06,750 the atmosphere can only protect us from rocky and rubble pile asteroids 478 00:33:06,775 --> 00:33:09,494 up to around 100 ft wide. 479 00:33:11,270 --> 00:33:15,246 And there is something else much more dangerous to consider, 480 00:33:15,270 --> 00:33:18,046 metallic asteroids. 481 00:33:18,070 --> 00:33:20,412 If you had a rocky asteroid hitting, 482 00:33:20,437 --> 00:33:22,724 or a rubbly rocky asteroid hitting, 483 00:33:22,800 --> 00:33:24,237 It wouldn't make it to the ground. 484 00:33:24,262 --> 00:33:26,555 An asteroid that's around a 100 ft across 485 00:33:26,580 --> 00:33:28,924 would actually blow up in the sky. 486 00:33:30,500 --> 00:33:33,030 But if a 100 ft metallic asteroid were to hit, 487 00:33:33,070 --> 00:33:34,800 First of all you wouldn't have much warning 488 00:33:34,825 --> 00:33:36,594 it would hit the top of the atmosphere 489 00:33:36,790 --> 00:33:39,907 and then would hit the ground about a second later. 490 00:33:39,932 --> 00:33:42,923 Causing an enormous explosion that would 491 00:33:42,948 --> 00:33:46,514 open up a crater that would be about a mile across. 492 00:33:46,560 --> 00:33:51,516 You'd have a flattened ruin of remnants of buildings. 493 00:33:51,540 --> 00:33:58,216 Millions dead from the shockwave that would be radiating out 494 00:33:58,240 --> 00:34:04,216 and layer of dust falling back down over the next minutes and hours. 495 00:34:05,640 --> 00:34:08,560 The metallic asteroid punches through the atmosphere 496 00:34:08,585 --> 00:34:13,916 because it's too hard for friction and air pressure to break up completely. 497 00:34:13,940 --> 00:34:20,316 So it slams into the ground in a catastrophic explosion. 498 00:34:20,340 --> 00:34:26,316 Metallic asteroids could be our planetary protectors greatest foe. 499 00:34:28,440 --> 00:34:34,416 But turns out the Earth could have another built in defense. 500 00:34:35,540 --> 00:34:41,916 We know an asteroid punched through the atmosphere and killed off the dinosaurs. 501 00:34:41,940 --> 00:34:46,716 But research is showing our planet could have saved them. 502 00:34:46,740 --> 00:34:49,416 The dinosaurs were incredibly unlucky. 503 00:34:49,440 --> 00:34:51,855 Even if the object does make it past our atmosphere 504 00:34:51,880 --> 00:34:55,540 we still have another line of defense. 505 00:34:55,640 --> 00:35:02,616 It's not always what an asteroid is made of that makes the difference. 506 00:35:02,640 --> 00:35:08,030 Sometimes, it's all about where it is. 507 00:35:25,850 --> 00:35:30,092 Our planetary protectors are creating technologies 508 00:35:30,417 --> 00:35:34,850 to divert a potentially catastrophic asteroid. 509 00:35:37,150 --> 00:35:40,026 But until their armory is complete, 510 00:35:40,050 --> 00:35:44,126 the Earth has its own defensive strategy. 511 00:35:45,950 --> 00:35:50,326 One of the things that is sure, is that we will be hit by an asteroid or comet again. 512 00:35:50,350 --> 00:35:53,090 It may not happen for millions of years, but it will happen. 513 00:35:53,130 --> 00:35:55,728 And on that day the thing that will differentiate 514 00:35:55,753 --> 00:35:59,545 between a just being a very bad day and it being a global catastrophe, 515 00:35:59,580 --> 00:36:02,160 is location, location, location. 516 00:36:04,990 --> 00:36:06,966 Some regions of the Earth 517 00:36:06,990 --> 00:36:12,566 could actually reduce the damage done by a killer asteroid. 518 00:36:12,590 --> 00:36:15,445 How do we know that? 519 00:36:15,470 --> 00:36:16,866 Dinosaurs. 520 00:36:16,890 --> 00:36:21,860 65 million years ago, the dinosaurs had a very bad day. 521 00:36:21,884 --> 00:36:26,986 They had the bad luck to be wiped out by an asteroid impact. 522 00:36:29,510 --> 00:36:32,588 We thought we knew the full story. 523 00:36:32,613 --> 00:36:37,886 But researchers have revealed something astonishing. 524 00:36:37,910 --> 00:36:43,186 If the asteroid had hit the earth just minutes later. 525 00:36:43,210 --> 00:36:50,420 Dinosaurs may still roam the planet today, but how? 526 00:36:50,470 --> 00:36:52,997 This object hit right at the Yucatan Peninsula. 527 00:36:53,022 --> 00:36:56,354 It caused an incredible tsunami that flooded North America 528 00:36:56,379 --> 00:36:59,670 but it also threw a lot of sulfates into the air. 529 00:37:02,970 --> 00:37:06,521 The six mile wide asteroid landed in shallow seas 530 00:37:06,546 --> 00:37:09,846 in what is now the Gulf of Mexico. 531 00:37:12,370 --> 00:37:17,446 It vaporized rocks in the sea floor of the continental shelf. 532 00:37:17,470 --> 00:37:23,546 The impact blasted out trillions of tons of gases into the atmosphere. 533 00:37:23,570 --> 00:37:26,792 Triggering catastrophic climate change. 534 00:37:26,817 --> 00:37:32,246 70% of all life on Earth became extinct. 535 00:37:32,270 --> 00:37:35,146 Including the dinosaurs. 536 00:37:35,170 --> 00:37:36,840 The thing that's kind of tragic 537 00:37:36,870 --> 00:37:39,433 is that the Earth had rotated just a little bit more, 538 00:37:39,458 --> 00:37:42,490 when that impact hit, it would have been in deeper ocean. 539 00:37:42,520 --> 00:37:46,596 And there wouldn't have been all that vaporized rock and sulphur. 540 00:37:50,520 --> 00:37:54,796 Our planet spins at a thousand miles an hour. 541 00:37:54,820 --> 00:38:01,196 70% of the earth's surface is covered by ocean. 542 00:38:01,220 --> 00:38:07,196 With a little luck, the dinosaur destroyer could have struck in deeper water. 543 00:38:07,420 --> 00:38:08,944 There's no good place on the earth 544 00:38:08,969 --> 00:38:13,514 to take a five mile wide asteroid strike, there's just no good place. 545 00:38:13,539 --> 00:38:15,855 Some places are worse than others and 546 00:38:15,880 --> 00:38:20,896 the Yucatan Peninsula with that much sulfur was one of the worst possible. 547 00:38:20,920 --> 00:38:23,890 So it's just not going to be a good day. 548 00:38:25,990 --> 00:38:32,666 The asteroid that killed the dinosaurs, allowed us mammals to take over the Earth. 549 00:38:32,690 --> 00:38:39,466 Fortunately, these giant asteroids only strike once every few million years. 550 00:38:39,790 --> 00:38:44,163 But every two thousand years or so, 551 00:38:44,188 --> 00:38:50,066 a rock about the size of a football field hits Earth. 552 00:38:50,090 --> 00:38:52,784 What would happen if one of these smaller, 553 00:38:52,809 --> 00:38:56,666 more common asteroids, were to hit the ocean? 554 00:38:56,690 --> 00:38:58,346 Think of something like the Pacific Ocean, 555 00:38:58,371 --> 00:39:00,052 there's a lot of coastline there. 556 00:39:00,076 --> 00:39:02,866 And so you have many, many people that are at risk. 557 00:39:02,965 --> 00:39:05,465 Most of the Earth's surface is ocean. 558 00:39:05,490 --> 00:39:08,137 So it's a much more likely scenario, 559 00:39:08,162 --> 00:39:10,066 for an asteroid to hit the ocean. 560 00:39:10,090 --> 00:39:13,896 And so the question is, how much of a tsunami risk is there? 561 00:39:16,620 --> 00:39:19,496 Scientist have modeled what would happen. 562 00:39:19,520 --> 00:39:24,796 If an asteroid strikes different places in the ocean. 563 00:39:24,820 --> 00:39:26,863 It was studied in three dimensions 564 00:39:26,888 --> 00:39:30,275 with different types of compositions, different ocean depths, 565 00:39:30,300 --> 00:39:32,220 different entry angles 566 00:39:32,320 --> 00:39:39,396 and found out that the continental shelf actually saves us. 567 00:39:39,420 --> 00:39:43,496 The continental shelf is an underwater landmass that extends 568 00:39:43,520 --> 00:39:47,496 around 50 miles beyond the coast. 569 00:39:47,520 --> 00:39:50,917 So when an asteroid hundreds of feet across 570 00:39:50,942 --> 00:39:53,596 slams into the deep ocean, 571 00:39:53,620 --> 00:39:57,219 the shallow sea created by the continental shelf 572 00:39:57,244 --> 00:40:02,296 could force a tsunami to collapse before it hits land. 573 00:40:02,320 --> 00:40:07,296 It seems, the ocean has our back. 574 00:40:07,320 --> 00:40:11,802 For the deep ocean we think that asteroids smaller than 400 ft across, 575 00:40:11,827 --> 00:40:15,096 which is quite large, are not a tsunami risk 576 00:40:15,120 --> 00:40:19,996 and so we don't need to worry as much as we thought we did, about it. 577 00:40:20,020 --> 00:40:22,012 That shallow part of the water 578 00:40:22,037 --> 00:40:26,020 actually buffers any tsunami wave that might be coming in. 579 00:40:32,720 --> 00:40:35,896 So our planet has defense mechanisms 580 00:40:35,920 --> 00:40:41,896 and our scientists are devising plans that will take the fight to the asteroids. 581 00:40:43,620 --> 00:40:46,696 What they need is time. 582 00:40:48,320 --> 00:40:52,385 Astronomy very well can save the world, because we're on the lookout 583 00:40:52,410 --> 00:40:55,596 for all the asteroids that may someday collide with Earth 584 00:40:55,620 --> 00:41:00,696 and if we find them we could avoid a civilization ending event. 585 00:41:00,720 --> 00:41:03,820 If we have warning time, we then have the advantage of 586 00:41:03,845 --> 00:41:06,802 being able to think about the problem, plan for it 587 00:41:06,827 --> 00:41:10,220 and actually build up the technologies practice the techniques that it's gonna 588 00:41:10,244 --> 00:41:15,396 take to push that asteroid out of the way, time is definitely an ally for us. 589 00:41:15,420 --> 00:41:20,196 We're not ready to cancel the apocalypse just yet. 590 00:41:20,220 --> 00:41:24,896 But with the planetary protection team on the case, 591 00:41:24,920 --> 00:41:27,535 soon, we'll have a fighting chance. 592 00:41:29,060 --> 00:41:32,296 If you want to know what, like an astronomer's sweatiest nightmare is. 593 00:41:32,320 --> 00:41:37,196 It's an asteroid impact. It's kinda personal, right? 594 00:41:37,220 --> 00:41:40,228 This is happening right here on Earth. 595 00:41:40,253 --> 00:41:45,196 It's a challenge to us and that's why we want to prevent them. 596 00:41:45,820 --> 00:41:50,496 The good news is, we actually are on the cusp of being able to deflect them. 597 00:41:50,520 --> 00:41:55,996 We're almost there we just have to push it through. 598 00:41:56,020 --> 00:41:58,164 The planet is incredibly resilient. 599 00:41:58,189 --> 00:42:02,824 Even if one specific species or one specific individual is very fragile, 600 00:42:02,849 --> 00:42:07,596 as a whole, the Earth is actually quite tough. 601 00:42:07,620 --> 00:42:09,903 It really comes back to, as human beings: 602 00:42:09,928 --> 00:42:14,096 What is our will to discover, to explore and understand the solar system? 603 00:42:14,120 --> 00:42:17,247 It becomes very important when you think about asteroids. 604 00:42:17,272 --> 00:42:19,596 We need to keep scanning the skies. 605 00:42:19,620 --> 00:42:23,696 We need to keep being scientists to defend the Earth. 606 00:42:26,700 --> 00:42:28,900 Subtitles by FlyingK 52780

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