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These are the user uploaded subtitles that are being translated: 1 00:00:02,120 --> 00:00:05,100 a dangerous asteroid is heading towards Earth. 2 00:00:05,840 --> 00:00:12,579 It's the size of the Empire State Building, and it's traveling at 16 ,000 3 00:00:12,580 --> 00:00:13,630 miles an hour. 4 00:00:14,520 --> 00:00:19,280 It's called Apophis, after the Egyptian god of chaos. 5 00:00:19,860 --> 00:00:22,760 It will fly close to us in 2029. 6 00:00:23,240 --> 00:00:26,440 It won't hit us this time. 7 00:00:27,040 --> 00:00:32,240 But when it returns in 2068, It could be another story. 8 00:00:33,340 --> 00:00:38,180 If it blows up over a city, millions of people will die. 9 00:00:40,560 --> 00:00:44,220 This could be the most devastating single event in U .S. 10 00:00:44,440 --> 00:00:45,490 history. 11 00:00:45,600 --> 00:00:49,940 Earth is stuck in the crosshairs of a potential asteroid strike. 12 00:00:52,040 --> 00:00:56,900 Apophis is one of around 2 ,000 potentially hazardous asteroids. 13 00:00:59,709 --> 00:01:03,790 Asteroids have hit us before, and they will hit us again. 14 00:01:07,890 --> 00:01:12,830 As far as cosmic dangers go, they're number one on the list. 15 00:01:13,290 --> 00:01:15,330 This is not a thrill. 16 00:01:15,750 --> 00:01:17,090 If we do nothing, 17 00:01:17,990 --> 00:01:20,530 this is our future. 18 00:01:38,860 --> 00:01:40,300 December 2018, 19 00:01:41,020 --> 00:01:42,070 the U .S. 20 00:01:42,620 --> 00:01:47,439 military detects a huge explosion in the Earth's atmosphere, high over the 21 00:01:47,440 --> 00:01:50,040 Bering Sea off the coast of Alaska. 22 00:01:51,520 --> 00:01:56,399 When an explosion of this magnitude is detected, everyone's mind goes to the 23 00:01:56,400 --> 00:01:57,740 same thing, nukes. 24 00:01:57,960 --> 00:02:02,939 But when the real answer was found, and it was determined that it didn't even 25 00:02:02,940 --> 00:02:05,960 originate from Earth, that was even more shocking. 26 00:02:06,650 --> 00:02:09,570 The cause of the blast was an asteroid. 27 00:02:10,830 --> 00:02:16,669 This asteroid was 30 feet across, something like that, over 1 ,000 tons. 28 00:02:16,670 --> 00:02:21,690 was moving at 20 miles per second, over 70 ,000 miles an hour. 29 00:02:22,970 --> 00:02:28,489 This asteroid was small, and it exploded in the atmosphere of the ocean, so 30 00:02:28,490 --> 00:02:29,540 nobody was hurt. 31 00:02:33,170 --> 00:02:34,690 But if it had been bigger? 32 00:02:35,290 --> 00:02:39,250 or it had come in over a different place, or it had been moving a lot 33 00:02:39,251 --> 00:02:41,249 this could have been a dangerous object. 34 00:02:41,250 --> 00:02:45,170 But the scariest thing about it is that we didn't see it coming. 35 00:02:51,250 --> 00:02:52,970 We've been lucky so far. 36 00:02:54,270 --> 00:02:57,030 But near misses happen all the time. 37 00:02:59,660 --> 00:03:04,579 About once a year, we get something the equivalent of a nuclear bomb going off 38 00:03:04,580 --> 00:03:10,719 in our atmosphere. And while that sounds horrible, most of these happen tens of 39 00:03:10,720 --> 00:03:17,279 miles over open ocean, where we go on completely 40 00:03:17,280 --> 00:03:18,330 oblivious. 41 00:03:20,620 --> 00:03:27,120 We may be oblivious to most of the threats from space, but they are very 42 00:03:27,530 --> 00:03:29,410 We are going to get hit. 43 00:03:29,790 --> 00:03:35,350 Over a certain amount of time, an asteroid impact is inevitable. It will 44 00:03:35,570 --> 00:03:37,310 100 % absolute certainty. 45 00:03:54,060 --> 00:03:58,819 NASA considers the threat from the sky so severe it has made protection from 46 00:03:58,820 --> 00:04:00,500 asteroids a top priority. 47 00:04:02,520 --> 00:04:04,340 These events are not rare. 48 00:04:04,600 --> 00:04:05,650 They happen. 49 00:04:06,000 --> 00:04:10,699 And, of course, it's up to us to make sure that we are detecting and 50 00:04:10,700 --> 00:04:14,919 characterizing, tracking all of the near -Earth objects that potentially could 51 00:04:14,920 --> 00:04:15,970 be a threat. 52 00:04:16,079 --> 00:04:20,559 This is not about Hollywood. It's not about movies. This is about ultimately 53 00:04:20,560 --> 00:04:26,009 protecting. the only planet we know right now to host life, and that is the 54 00:04:26,010 --> 00:04:27,060 planet Earth. 55 00:04:29,610 --> 00:04:34,170 To help protect our home, we carry out Earth defense simulations. 56 00:04:35,190 --> 00:04:41,489 For three days, 200 scientists at the Planetary Defense Conference battle a 57 00:04:41,490 --> 00:04:46,410 simulated asteroid 20 times larger than the Bering Sea space rock. 58 00:04:48,000 --> 00:04:52,240 We practice, all right, what if this hits a major city? 59 00:04:52,520 --> 00:04:53,720 What would we need to do? 60 00:04:55,740 --> 00:05:00,619 By running potential impact scenarios, we can prepare for a real asteroid 61 00:05:00,620 --> 00:05:01,670 strike. 62 00:05:01,671 --> 00:05:05,999 This is like a fire drill that you would do at school or at work, where you 63 00:05:06,000 --> 00:05:09,659 practice and think about, okay, what if? Where are the exits? How do I get out? 64 00:05:09,660 --> 00:05:11,040 How fast do I get out? 65 00:05:13,710 --> 00:05:18,510 The drill starts with the discovery of a simulated Earth -bound asteroid. 66 00:05:19,890 --> 00:05:23,800 So the first information is, there's a big asteroid coming towards the Earth. 67 00:05:24,030 --> 00:05:28,069 Then we get a better estimate of how big it is, how fast it's going, and where 68 00:05:28,070 --> 00:05:29,120 it's going to hit. 69 00:05:29,790 --> 00:05:34,730 The asteroid is heading straight for Earth, with Denver, Colorado in its 70 00:05:37,320 --> 00:05:42,579 The planetary defense scientists send up a simulated spacecraft to smash into 71 00:05:42,580 --> 00:05:47,020 the asteroid and push it off its path. But it's a big gamble. 72 00:05:48,040 --> 00:05:54,380 You can push it the wrong way. You can potentially have unintended 73 00:05:57,020 --> 00:06:03,839 In the simulation, the spacecraft strikes the asteroid, deflecting it 74 00:06:03,840 --> 00:06:04,890 away from Earth. 75 00:06:07,040 --> 00:06:12,619 dislodges a 200 -foot junk, which is now heading straight towards the eastern 76 00:06:12,620 --> 00:06:13,670 seaboard. 77 00:06:14,360 --> 00:06:18,980 So there's this one last piece that is now going to hit New York. 78 00:06:19,640 --> 00:06:26,459 We know that something that size is going to have citywide consequences. 79 00:06:26,460 --> 00:06:29,300 That is huge. That's a horrible impact. 80 00:06:29,301 --> 00:06:34,929 When you're actually in the conference room and you understand eventually that 81 00:06:34,930 --> 00:06:39,249 New York City is going to be destroyed, and you're having strategies about how 82 00:06:39,250 --> 00:06:43,269 to evacuate people, all the timing, when you're doing the simulation, you're in 83 00:06:43,270 --> 00:06:46,489 your head, you're thinking about these things, you're trying to reason them 84 00:06:46,490 --> 00:06:51,050 But can you imagine the feeling in your gut, in your heart, if this was real? 85 00:06:52,030 --> 00:06:57,109 If this were real, the chunk of asteroid would strike the Earth's atmosphere at 86 00:06:57,110 --> 00:06:59,490 43 ,000 miles an hour. 87 00:07:00,680 --> 00:07:06,579 As the space rock descends, it collides with molecules in the atmosphere, which 88 00:07:06,580 --> 00:07:08,120 buffets the falling rock. 89 00:07:10,000 --> 00:07:14,059 It's kind of like doing a belly flop into a pool, right? You're going from 90 00:07:14,060 --> 00:07:18,560 vacuum of space into the dense lower atmosphere in mere seconds. 91 00:07:18,900 --> 00:07:22,150 And that's an incredible amount of pressure to put on the object. 92 00:07:23,340 --> 00:07:28,060 The asteroid flams into the air ahead of it, compressing it violently. 93 00:07:28,780 --> 00:07:32,680 the surface of the asteroid gets hotter and brighter. 94 00:07:33,620 --> 00:07:37,679 It's actually the air itself that's glowing luminously from the heating of 95 00:07:37,680 --> 00:07:42,599 shockwave, the world's most intense sonic boom, if you will, that heats the 96 00:07:42,600 --> 00:07:46,419 to incandescence as the object passes through. So that's the source of that 97 00:07:46,420 --> 00:07:47,680 brilliant illumination. 98 00:07:49,540 --> 00:07:53,260 This bright -burning asteroid is called a bolide. 99 00:07:53,550 --> 00:07:59,410 We witnessed one descending over the Russian city of Chelyabinsk in 2013. 100 00:08:00,050 --> 00:08:04,289 All of a sudden, there was a huge fireball striking through the sky, and 101 00:08:04,290 --> 00:08:08,349 had no idea what they were witnessing because it looked like the sky was on 102 00:08:08,350 --> 00:08:10,190 fire. It was insanity. 103 00:08:11,350 --> 00:08:17,089 As the asteroid descends, the compression of the denser air lower down 104 00:08:17,090 --> 00:08:19,950 flatten and even disrupt the falling rock. 105 00:08:20,680 --> 00:08:24,839 There's a high pressure on the front, there's no pressure on the back, and 106 00:08:24,840 --> 00:08:30,559 being superheated. And that intense temperature causes the air to glow, 107 00:08:30,560 --> 00:08:32,559 how we see the streak of a meteor. 108 00:08:32,799 --> 00:08:38,038 And it also disintegrates the asteroid itself. It's hot enough to literally 109 00:08:38,039 --> 00:08:40,740 rock. This can often lead to them exploding. 110 00:08:41,880 --> 00:08:48,159 The combination of heat and pressure invade the falling asteroid, causing it 111 00:08:48,160 --> 00:08:49,210 blow up. 112 00:08:49,680 --> 00:08:54,439 Most asteroids don't reach the ground before they completely disintegrate in a 113 00:08:54,440 --> 00:08:59,319 tremendous release of energy. This is what we call an airburst, and we learned 114 00:08:59,320 --> 00:09:02,990 lot about these while we were testing nuclear weapons after World War II. 115 00:09:05,300 --> 00:09:09,319 Some of these bombs were blown up underground and on the ground, but they 116 00:09:09,320 --> 00:09:13,319 out when they blew up bombs above the ground, it actually did more damage. It 117 00:09:13,320 --> 00:09:14,880 was more widespread damage. 118 00:09:15,790 --> 00:09:21,429 The explosion of the Telebent asteroid sent out a powerful shockwave at 119 00:09:21,430 --> 00:09:23,070 thousands of miles an hour. 120 00:09:24,610 --> 00:09:28,310 The blast traveled over 100 miles. 121 00:09:28,810 --> 00:09:34,350 It damaged 7 ,000 buildings and put 1 ,500 people in the hospital. 122 00:09:35,240 --> 00:09:39,119 All of the injuries pretty much came from people who saw, oh, what's that 123 00:09:39,120 --> 00:09:40,170 flash in the sky? 124 00:09:40,240 --> 00:09:44,459 And they came close to a window to look and see what it was, and then the 125 00:09:44,460 --> 00:09:46,810 pressure wave hit and blew glass in their face. 126 00:09:49,620 --> 00:09:53,360 The Chelyabinsk asteroid was only 65 feet across. 127 00:09:56,300 --> 00:10:01,799 The rock in the defense simulation is three times more massive and is now 128 00:10:01,800 --> 00:10:03,220 heading for New York City. 129 00:10:05,510 --> 00:10:10,209 Imagine what would happen if an explosion a thousand times greater than 130 00:10:10,210 --> 00:10:12,010 over Hiroshima hit New York. 131 00:10:13,210 --> 00:10:18,149 We're talking about an utter, complete destruction of the city and millions of 132 00:10:18,150 --> 00:10:19,200 people. 133 00:10:20,250 --> 00:10:25,330 With so little warning, the only option would be to evacuate New York City. 134 00:10:26,610 --> 00:10:30,110 How do we get everybody out of New York City within just a few days? 135 00:10:30,111 --> 00:10:34,049 That's where panic sets in. That's where fear would really become the dominant 136 00:10:34,050 --> 00:10:35,100 emotion. 137 00:10:37,400 --> 00:10:41,620 Anyone left in New York would see the bolide race in, 138 00:10:41,880 --> 00:10:48,559 followed by a blinding light as the asteroid 139 00:10:48,560 --> 00:10:50,080 explodes above the city. 140 00:10:51,920 --> 00:10:57,799 The blast would be the equivalent to the largest nuclear weapon ever detonated 141 00:10:57,800 --> 00:10:58,819 on Earth. 142 00:10:58,820 --> 00:11:03,540 Buildings would be flattened, melted. There would be fires for miles around. 143 00:11:03,800 --> 00:11:08,259 In the first moments of the explosion, A million people could be killed 144 00:11:08,260 --> 00:11:12,799 instantly, and many more would die later in the rubble and the ruins of what 145 00:11:12,800 --> 00:11:13,850 would happen there. 146 00:11:15,300 --> 00:11:19,879 Everything within nine miles of the blast epicenter would be completely 147 00:11:19,880 --> 00:11:20,930 destroyed. 148 00:11:27,900 --> 00:11:31,720 The intense heat and pressure would wreck buildings. 149 00:11:33,610 --> 00:11:36,650 It's the worst possible day for New Yorkers. 150 00:11:36,950 --> 00:11:39,170 And not just the city itself. 151 00:11:39,430 --> 00:11:44,130 There's something like 15 million people living in the New York area. 152 00:11:47,170 --> 00:11:52,610 The destructive shockwave would race out over 250 square miles. 153 00:11:53,330 --> 00:11:56,809 This would certainly be the worst disaster that the U .S. has ever 154 00:11:56,810 --> 00:12:01,769 We're talking about millions and millions of people displaced, affected 155 00:12:01,770 --> 00:12:02,820 an instant. 156 00:12:08,840 --> 00:12:12,400 This scenario is just a simulation, for now. 157 00:12:17,980 --> 00:12:21,400 The asteroid Apophis is heading our way. 158 00:12:23,920 --> 00:12:29,720 If it hits Earth, it might not just kill a city. It could kill a whole region. 159 00:12:30,480 --> 00:12:33,280 I wouldn't exactly want to be there when that happens. 160 00:12:33,780 --> 00:12:35,520 I want to be very, very far away. 161 00:12:37,750 --> 00:12:44,569 Apophis will skim Earth in 2029, but its path will 162 00:12:44,570 --> 00:12:45,620 change, 163 00:12:46,070 --> 00:12:50,970 possibly turning a future myth into a direct hit. 164 00:12:58,850 --> 00:13:01,790 April 13, 2029. 165 00:13:02,070 --> 00:13:05,750 A speck of light races towards Earth. 166 00:13:06,280 --> 00:13:10,660 It's an 1 ,100 -foot -wide asteroid called Apophis. 167 00:13:10,900 --> 00:13:15,100 We are about to have an extremely close shave. 168 00:13:15,920 --> 00:13:21,139 It's the closest approach of any asteroid that didn't actually hit us for 169 00:13:21,140 --> 00:13:27,099 long, long time. It will be ten times closer than the moon itself. It will be 170 00:13:27,100 --> 00:13:29,800 close it will be brighter than some stars. 171 00:13:30,280 --> 00:13:33,260 The football stadium -sized Apophis. 172 00:13:33,520 --> 00:13:35,220 will race over the Atlantic. 173 00:13:35,221 --> 00:13:39,859 If it were sitting on the surface of the Earth, it would weigh about 50 million 174 00:13:39,860 --> 00:13:41,460 tons, something like that. 175 00:13:41,860 --> 00:13:47,879 And that is not the place you want it to be. You want it to be in space and far 176 00:13:47,880 --> 00:13:48,930 away. 177 00:13:49,440 --> 00:13:55,179 When we discovered Apophis in 2004, we thought it might be on a collision 178 00:13:55,180 --> 00:13:56,230 with Earth. 179 00:13:56,300 --> 00:14:01,780 With a potential impact greater than the largest atomic bomb ever exploded. 180 00:14:02,870 --> 00:14:07,849 The largest nuclear device, atomic device, ever detonated on our planet was 181 00:14:07,850 --> 00:14:12,270 Tsar Bomba bomb in Russia. It was something like 55 or 56 megatons. 182 00:14:12,890 --> 00:14:18,970 When Krakatoa exploded in 1883, that was something like 200 megatons. 183 00:14:19,450 --> 00:14:22,050 Apophis impact would be 450 megatons. 184 00:14:22,051 --> 00:14:26,009 If something like that were to happen over New York City or Washington, D .C., 185 00:14:26,010 --> 00:14:27,670 you're going to lose the city. 186 00:14:30,030 --> 00:14:34,989 The impact would be at least ten times greater than the simulated asteroid 187 00:14:34,990 --> 00:14:36,050 strike on New York. 188 00:14:42,770 --> 00:14:47,170 When you put it in those terms, that's just plain scary. 189 00:14:47,650 --> 00:14:53,490 In a word, an impact from an apophysized asteroid would be bad. 190 00:14:53,910 --> 00:14:56,010 Very, very bad. 191 00:14:57,449 --> 00:15:03,009 Apophis' orbit will cross Earth every seven years this century, but it won't 192 00:15:03,010 --> 00:15:04,290 us in 2029. 193 00:15:04,830 --> 00:15:09,110 But this close encounter will change Apophis' orbit. 194 00:15:10,290 --> 00:15:16,449 When a small asteroid encounters a bigger body like a planet, it's like a 195 00:15:16,450 --> 00:15:17,850 of roller derby players. 196 00:15:20,540 --> 00:15:24,619 Most of them are clumped together, but maybe there's one just on their own 197 00:15:24,620 --> 00:15:25,670 particular orbit. 198 00:15:25,860 --> 00:15:29,979 And as they circle around, as they get close to that larger clump, there'll be 199 00:15:29,980 --> 00:15:35,759 some interactions, potentially violent interactions, that will change the 200 00:15:35,760 --> 00:15:41,139 trajectory of that lone roller derby skater. And the next time around, it 201 00:15:41,140 --> 00:15:44,620 be a wide miss, or it might be a head -on impact. 202 00:15:49,100 --> 00:15:51,340 It's the same in the solar system. 203 00:15:51,700 --> 00:15:57,019 The combined gravity of the Earth and Moon creates what's called a 204 00:15:57,020 --> 00:16:03,900 keyhole, a gravitational sweet spot, which could change Apophis' 205 00:16:04,080 --> 00:16:05,130 orbit. 206 00:16:05,780 --> 00:16:11,219 That will change the potential future trajectory of this rock and might make 207 00:16:11,220 --> 00:16:15,999 totally harmless or might increase the chances of an impact even further in the 208 00:16:16,000 --> 00:16:17,050 future. 209 00:16:20,050 --> 00:16:24,949 Because of the gravitational keyhole, there is still a small chance that 210 00:16:24,950 --> 00:16:26,930 will hit Earth in 2068. 211 00:16:31,070 --> 00:16:35,969 That is the important lesson that Apophis taught us. You can miss the 212 00:16:35,970 --> 00:16:40,329 if you pass through one of these keyholes at some time later, you will 213 00:16:40,330 --> 00:16:41,380 Earth. 214 00:16:41,710 --> 00:16:48,690 We now know Apophis will miss the keyhole in 2029, but there are other 215 00:16:49,160 --> 00:16:50,800 and other close passes. 216 00:16:57,000 --> 00:16:59,560 Apophis is not a lone threat. 217 00:16:59,880 --> 00:17:06,618 There are an estimated 832 ,557 asteroids orbiting the 218 00:17:06,619 --> 00:17:07,669 sun. 219 00:17:08,980 --> 00:17:13,420 Most asteroids live their lives perfectly peacefully. 220 00:17:14,520 --> 00:17:20,399 past the orbit of Mars or trailing Jupiter and don't mind anybody else and 221 00:17:20,400 --> 00:17:26,858 cause any troubles. But some asteroids are on very particular orbits that cross 222 00:17:26,859 --> 00:17:28,440 the orbit of the Earth. 223 00:17:30,180 --> 00:17:35,439 These asteroids have left the stable orbit of the asteroid belt and moved 224 00:17:35,440 --> 00:17:37,680 orbits that get near our own. 225 00:17:37,980 --> 00:17:43,940 These asteroids are called near -Earth asteroids, or NEAs for short. 226 00:17:43,941 --> 00:17:48,259 The near -Earth asteroid population is interesting and potentially dangerous 227 00:17:48,260 --> 00:17:51,259 because they're the ones that actually cross the orbit of the Earth. So they're 228 00:17:51,260 --> 00:17:55,800 most likely to have, at some point in the future, an impact with the Earth. 229 00:17:57,620 --> 00:18:01,300 Most NEAs pose little or no threat to Earth. 230 00:18:02,040 --> 00:18:07,020 But we've detected over 2 ,000 that do, including apophis. 231 00:18:09,380 --> 00:18:12,020 These are called PHAs. 232 00:18:12,220 --> 00:18:14,320 Potentially hazardous asteroids. 233 00:18:15,620 --> 00:18:19,479 The difference between a near -Earth asteroid and a potentially hazardous 234 00:18:19,480 --> 00:18:22,680 asteroid is distance and size. 235 00:18:23,640 --> 00:18:27,740 Anything can get near the Earth, and that could be 20 million miles away, 236 00:18:27,860 --> 00:18:31,379 something like that, and be a near -Earth asteroid. But a potentially 237 00:18:31,380 --> 00:18:34,680 one can hit us, and it's big enough to do damage. 238 00:18:35,231 --> 00:18:42,879 So something that over the next hundred years or so has a chance of hitting us 239 00:18:42,880 --> 00:18:46,860 and doing damage when it does, that's a potentially hazardous object. 240 00:18:49,500 --> 00:18:54,380 PHAs are asteroids 500 foot or larger that could collide with Earth. 241 00:18:57,220 --> 00:18:59,320 Take a 400 foot asteroid. 242 00:18:59,620 --> 00:19:05,380 If it hit, it would release as much energy as 3 ,000 Hiroshima nuclear 243 00:19:12,520 --> 00:19:18,740 In July 2018, NASA published a map of all known NEAs and PHAs. 244 00:19:21,960 --> 00:19:27,820 The animation tracks their discovery from 1999 through 2018. 245 00:19:27,821 --> 00:19:33,419 Every time I look at this animation, it does make my heart stop a little bit 246 00:19:33,420 --> 00:19:37,199 because it looks like we're in the middle of this swarm of angry bees 247 00:19:37,200 --> 00:19:38,250 all around us. 248 00:19:38,410 --> 00:19:39,530 In 1999, 249 00:19:40,410 --> 00:19:45,390 we'd identified under 300 NEAs scattered through the inner solar system. 250 00:19:45,770 --> 00:19:49,490 Ten years later, we discovered 500 more. 251 00:19:49,930 --> 00:19:55,030 By 2018, we discovered 18 ,000 near -Earth asteroids. 252 00:19:55,250 --> 00:19:59,070 But we estimate there are millions out there. 253 00:19:59,970 --> 00:20:04,190 It seems like we can never find all the asteroids. They just keep coming. 254 00:20:04,410 --> 00:20:06,640 It's like we're fighting an army of zombies. 255 00:20:07,820 --> 00:20:14,379 Zombies that keep hurtling our way, hitting Earth at up to 64 ,000 miles an 256 00:20:14,380 --> 00:20:15,430 hour. 257 00:20:16,740 --> 00:20:21,739 That is very, very fast. That is much faster than a rifle bullet. And that's 258 00:20:21,740 --> 00:20:23,320 key to its destructive power. 259 00:20:25,640 --> 00:20:32,359 When a really fast and really large asteroid hits, the impact is off the 260 00:20:32,360 --> 00:20:35,640 chart. The blast is so intense. 261 00:20:36,240 --> 00:20:39,580 It can melt or even vaporize rock. 262 00:20:45,440 --> 00:20:47,100 January 2019. 263 00:20:47,620 --> 00:20:50,140 A total eclipse of the moon. 264 00:20:51,100 --> 00:20:55,360 Astronomers train their telescopes on the darkening lunar surface. 265 00:20:55,820 --> 00:21:00,920 They capture a bright flash that lasts around a quarter of a second. 266 00:21:00,921 --> 00:21:06,119 It was recorded. There were a lot of live webcasts and things like that going 267 00:21:06,120 --> 00:21:06,939 at the time. 268 00:21:06,940 --> 00:21:10,200 And you can see this flash of light. What the heck was that? 269 00:21:11,900 --> 00:21:15,260 At first, the cause of the flash was a mystery. 270 00:21:16,840 --> 00:21:22,619 It turns out it was actually a meteorite hitting the surface of the moon. And 271 00:21:22,620 --> 00:21:25,899 because it was dark, and because we were all looking at it, we could actually 272 00:21:25,900 --> 00:21:26,679 see it. 273 00:21:26,680 --> 00:21:32,759 The moon's dark surface gave us a unique view into what happens when an asteroid 274 00:21:32,760 --> 00:21:38,039 strikes. What was so exciting about being able to see this impact on the 275 00:21:38,040 --> 00:21:42,079 a dark area is that we could actually look at the light that it produced and 276 00:21:42,080 --> 00:21:45,460 then back calculate exactly what the size of the impactor was. 277 00:21:45,780 --> 00:21:52,219 We worked out that the impacting asteroid was just 20 inches wide. The 278 00:21:52,220 --> 00:21:54,960 blew out was 45 feet across. 279 00:21:55,450 --> 00:21:59,410 How could something so small be so destructive? 280 00:22:00,230 --> 00:22:04,309 The two things that matter the most are how fast it's going and how massive is 281 00:22:04,310 --> 00:22:07,489 the thing. The more massive, the bigger the boom, the faster, the bigger the 282 00:22:07,490 --> 00:22:11,949 boom. Speed and weight are two very important factors to assess how much 283 00:22:11,950 --> 00:22:13,000 an asteroid will do. 284 00:22:13,110 --> 00:22:17,349 Just like a boxer, if a tiny person like me were to swing a punch, it would do a 285 00:22:17,350 --> 00:22:19,710 lot less damage than a heavyweight champion. 286 00:22:19,711 --> 00:22:21,629 Same thing with asteroids. 287 00:22:21,630 --> 00:22:23,499 The bigger they are, the bigger the punch. 288 00:22:23,500 --> 00:22:25,180 But the same thing is fast, right? 289 00:22:25,181 --> 00:22:28,759 If I hit you really slowly, it's not going to hurt. I have to really wind 290 00:22:28,760 --> 00:22:29,659 and pop. 291 00:22:29,660 --> 00:22:31,520 That's what happens with an asteroid. 292 00:22:33,040 --> 00:22:38,800 The damage from an asteroid strike is determined by its kinetic energy. 293 00:22:39,580 --> 00:22:43,980 Kinetic energy depends on two things, speed and weight. 294 00:22:44,680 --> 00:22:47,080 Speed is the most important. 295 00:22:49,840 --> 00:22:53,639 If you double the mass, you double the kinetic energy. But if you double the 296 00:22:53,640 --> 00:22:56,560 velocity, you get four times the kinetic energy. 297 00:22:56,800 --> 00:23:01,259 Three times the speed, nine times the impact energy. Ten times as fast, it has 298 00:23:01,260 --> 00:23:05,380 hundred times the energy. So the velocity is what's really critical here. 299 00:23:07,760 --> 00:23:14,239 The lunar asteroid weighed only 100 pounds, but it was traveling at 38 ,000 300 00:23:14,240 --> 00:23:15,290 miles an hour. 301 00:23:15,580 --> 00:23:20,140 carrying a huge kinetic energy which gouged out the crater. 302 00:23:21,500 --> 00:23:24,740 It's the same principle for impacts on Earth. 303 00:23:25,620 --> 00:23:32,220 50 ,000 years ago, a 150 -foot asteroid hit what is now Arizona. 304 00:23:32,820 --> 00:23:39,480 The impact blasted out an impressive hole, now called Beringer Crater. 305 00:23:40,160 --> 00:23:42,540 It's about three -quarters of a mile across. 306 00:23:42,541 --> 00:23:47,139 Over 500 feet deep, you could put the Washington Monument in the bottom of the 307 00:23:47,140 --> 00:23:51,059 crater, and the top of the monument wouldn't quite clear the rim. It's a 308 00:23:51,060 --> 00:23:52,560 impressive hole in the ground. 309 00:23:56,260 --> 00:23:57,540 In 2016, 310 00:23:58,380 --> 00:24:03,979 impact specialist Kathy Plesko visited Beringer Crater to see firsthand what 311 00:24:03,980 --> 00:24:06,920 mass and speed do to the surface of the Earth. 312 00:24:10,800 --> 00:24:11,850 The food. 313 00:24:12,270 --> 00:24:17,389 It's awe -inspiring to stand on the rim of a crater like this, understanding 314 00:24:17,390 --> 00:24:23,810 just how much energy it must have taken to excavate this much rock. 315 00:24:27,210 --> 00:24:32,470 An asteroid came in at about 27 ,000 miles an hour. 316 00:24:34,330 --> 00:24:37,590 It comes slamming into the surface and just explodes. 317 00:24:38,010 --> 00:24:42,709 Anywhere nearby here would have seen winds of thousands of miles an hour as 318 00:24:42,710 --> 00:24:43,890 shockwave came out. 319 00:24:49,990 --> 00:24:55,189 The immense power of an asteroid impact comes from the kinetic energy being 320 00:24:55,190 --> 00:24:58,730 transferred from the space rock into the surface rock. 321 00:25:01,230 --> 00:25:06,269 It's an extremely violent process, and it starts with the moment of contact of 322 00:25:06,270 --> 00:25:08,250 the projectile with the surface itself. 323 00:25:10,010 --> 00:25:16,530 It pushes into the crust, and at first it's just almost punching, 324 00:25:16,830 --> 00:25:20,750 like sticking your thumb into dough. It's only about as wide as the object 325 00:25:20,910 --> 00:25:26,169 It's going straight down in, but then it's meeting resistance from the surface 326 00:25:26,170 --> 00:25:26,999 of the Earth. 327 00:25:27,000 --> 00:25:32,079 And so it squishes, squishes, squishes until it runs out of momentum, but then 328 00:25:32,080 --> 00:25:35,459 it's very compressed, and all of that energy is in a very small space. 329 00:25:35,460 --> 00:25:39,919 As it releases, it detonates like a bomb, and that's what makes the impact 330 00:25:39,920 --> 00:25:40,970 crater. 331 00:25:43,720 --> 00:25:48,960 Simulations of an asteroid strike in the lab reveal the impact in slow motion. 332 00:25:52,140 --> 00:25:58,329 As the high -speed pellet hits the surface, The sand compresses downwards, 333 00:25:58,330 --> 00:25:59,380 rebounds. 334 00:26:00,590 --> 00:26:05,589 As that rebound is occurring, that's when the material is being ejected out 335 00:26:05,590 --> 00:26:06,640 the crater itself. 336 00:26:07,850 --> 00:26:12,149 You'll see the surface erupting outwards like the blooming petals of some big 337 00:26:12,150 --> 00:26:15,830 rocky flower as all this debris goes spraying out in every direction. 338 00:26:21,130 --> 00:26:25,290 The 150 -foot Behringer asteroid turned the rock to powder. 339 00:26:26,430 --> 00:26:33,229 66 million years ago, an asteroid around 200 times larger and moving one and a 340 00:26:33,230 --> 00:26:36,070 half times faster than Behringer hit Earth. 341 00:26:37,210 --> 00:26:44,210 This asteroid, called KPG, had so much energy, it turned rock to liquid. 342 00:26:44,610 --> 00:26:48,649 The thing was immense. It's really hard to wrap your head around just how big it 343 00:26:48,650 --> 00:26:55,119 is. When the back end of it is so far back that it's where a modern 344 00:26:55,120 --> 00:26:56,300 jetliner would fly. 345 00:26:58,660 --> 00:27:05,479 The KPG asteroid hit the ground with a lethal combination of mass and speed. A 346 00:27:05,480 --> 00:27:09,940 trillion tons traveling at 45 ,000 miles an hour. 347 00:27:11,700 --> 00:27:15,220 Some rock is completely vaporized. It just becomes a gas. 348 00:27:15,770 --> 00:27:17,550 You have some rock that has melted. 349 00:27:17,870 --> 00:27:20,850 You have some that's thrown out into space. 350 00:27:22,770 --> 00:27:27,129 This material goes up through that and then falls down and settles down over a 351 00:27:27,130 --> 00:27:31,669 huge area. That might be dust. It might be pulverized rock. It might be 352 00:27:31,670 --> 00:27:32,720 vaporized metal. 353 00:27:32,990 --> 00:27:35,950 It's all of this hot material raining down everywhere. 354 00:27:38,310 --> 00:27:41,070 As some rock exploded skyward. 355 00:27:41,550 --> 00:27:47,089 Rock below the surface was slammed by a shockwave that was completely off the 356 00:27:47,090 --> 00:27:48,140 charts. 357 00:27:48,250 --> 00:27:51,230 Rock stopped, behaving like rock. 358 00:27:52,270 --> 00:27:57,469 We experience rocks as solid objects, but if you hit a rock hard enough, it 359 00:27:57,470 --> 00:27:58,520 flows like water. 360 00:27:58,750 --> 00:28:05,690 The KPG impact hits so hard, it pulverized the rock and turned it into a 361 00:28:05,910 --> 00:28:10,269 Almost like ripples on a pond moving away from a stone that's been dropped in 362 00:28:10,270 --> 00:28:14,340 it. It's almost like a splash in the solid body of the Earth itself. 363 00:28:14,540 --> 00:28:19,039 And like the water droplets splashing in water, you'll see that central peak 364 00:28:19,040 --> 00:28:22,559 will kind of splash up and rise to a high altitude and then come back down 365 00:28:22,560 --> 00:28:26,979 again. We think a process very similar to that probably happened in the rock 366 00:28:26,980 --> 00:28:31,779 itself at the center of the crater, rising up as high as the Himalayas 367 00:28:31,780 --> 00:28:34,279 relaxing back down into their current position again. 368 00:28:34,280 --> 00:28:35,330 The material... 369 00:28:36,560 --> 00:28:41,619 And so these ripples are frozen in the rock. And there are other fragments that 370 00:28:41,620 --> 00:28:45,999 go away radially, almost like the spiderweb pattern in glass that you get 371 00:28:46,000 --> 00:28:47,480 it's shot with a bullet. 372 00:28:49,000 --> 00:28:54,180 The KPG impact blew out a 111 -mile -wide crater. 373 00:28:56,780 --> 00:29:03,640 A large and fast asteroid heading our way is always going to be a problem. 374 00:29:04,680 --> 00:29:05,940 So what do we do? 375 00:29:06,940 --> 00:29:08,620 Wait for oblivion? 376 00:29:10,920 --> 00:29:12,520 Or fight back? 377 00:29:21,780 --> 00:29:28,400 The space in the inner solar system seems calm, stable, and empty. 378 00:29:28,720 --> 00:29:30,060 But it's not. 379 00:29:31,820 --> 00:29:35,780 There are tens of thousands of near -Earth objects just whizzing around 380 00:29:36,000 --> 00:29:37,960 Now, space is big. 381 00:29:38,320 --> 00:29:44,379 They're not going to hit us every time they orbit the sun. But this does set up 382 00:29:44,380 --> 00:29:49,459 the possibility that one of these years, we're going to end up at the same spot 383 00:29:49,460 --> 00:29:52,920 in space at the same time as that asteroid. 384 00:29:53,260 --> 00:29:54,880 And then it's going to be an event. 385 00:29:57,360 --> 00:29:59,530 We're living in a cosmic shooting gallery. 386 00:29:59,540 --> 00:30:03,459 Asteroids strike the Earth all the time through history, and it's going to 387 00:30:03,460 --> 00:30:04,510 happen again. 388 00:30:04,660 --> 00:30:09,740 Scientists are developing strategies to stop an asteroid hitting our planet. 389 00:30:10,180 --> 00:30:14,800 Our options, destroy or deflect the space rock. 390 00:30:15,120 --> 00:30:19,380 But first, we need to detect any dangerous asteroids. 391 00:30:20,880 --> 00:30:24,799 It's a little bit unnerving to know that we haven't yet detected all of the 392 00:30:24,800 --> 00:30:29,039 asteroids that exist that could possibly cross our path. We've discovered a lot 393 00:30:29,040 --> 00:30:32,340 of asteroids now, but we typically discover the big ones. 394 00:30:33,720 --> 00:30:38,559 But for asteroids that are below 100 feet, there's a lot still out there that 395 00:30:38,560 --> 00:30:39,579 haven't discovered. 396 00:30:39,580 --> 00:30:43,839 And such an asteroid can do some real damage if it were to explode over a 397 00:30:43,840 --> 00:30:44,890 populated area. 398 00:30:44,920 --> 00:30:46,760 To prevent such a catastrophe... 399 00:30:47,290 --> 00:30:51,730 We need to find all asteroids whose orbits cross our own. 400 00:30:52,550 --> 00:30:55,510 Detection is crucial in our defense against asteroids. 401 00:30:55,750 --> 00:31:00,649 And the reason is, the earlier they're detected, the easier it is to deflect 402 00:31:00,650 --> 00:31:02,270 them away from hitting the Earth. 403 00:31:02,630 --> 00:31:05,400 You want to do deflection, the first step is detection. 404 00:31:07,490 --> 00:31:11,470 The problem is, asteroids are very hard to detect. 405 00:31:12,410 --> 00:31:16,730 Finding asteroids and cataloging all their orbits is really challenging. 406 00:31:17,100 --> 00:31:21,699 They can move quite fast across the sky, and they might go away on the other 407 00:31:21,700 --> 00:31:23,930 side of the sun for years and years and years. 408 00:31:26,140 --> 00:31:27,780 So we can't see them. 409 00:31:28,840 --> 00:31:33,380 And even when they are this side of the sun, they're hard to spot. 410 00:31:34,820 --> 00:31:37,830 But the problem is they're very small and they're very dark. 411 00:31:38,020 --> 00:31:41,580 And when I say very dark, I mean really dark like a lump of coal. 412 00:31:41,800 --> 00:31:45,639 So how do you find a small, dark rock just wandering around out there in the 413 00:31:45,640 --> 00:31:46,690 solar system? 414 00:31:51,820 --> 00:31:54,600 The Catalina Sky Survey has the answer. 415 00:31:56,280 --> 00:32:01,699 The huge telescope in the mountains above Tucson, Arizona takes a series of 416 00:32:01,700 --> 00:32:03,900 images over a 20 -minute period. 417 00:32:04,340 --> 00:32:07,640 It's looking for anything that moves. 418 00:32:07,860 --> 00:32:12,260 Because stars don't move, but asteroids do. 419 00:32:14,700 --> 00:32:20,220 If it's a really bright asteroid, we will see some bright points of light. 420 00:32:20,720 --> 00:32:22,360 tracking across the four images. 421 00:32:23,680 --> 00:32:25,420 Ah, here we go. 422 00:32:26,360 --> 00:32:27,660 This is a real object. 423 00:32:28,220 --> 00:32:33,079 You can see it's moving across the sky here from the lower right to the upper 424 00:32:33,080 --> 00:32:37,919 left. We are very, very excited to have discovered one tonight because this is 425 00:32:37,920 --> 00:32:42,580 an object that's approaching nearer space, likely in the neighborhood of 426 00:32:47,720 --> 00:32:49,340 Catalina has limitations. 427 00:32:50,030 --> 00:32:52,530 it can only see visible light. 428 00:32:52,770 --> 00:32:55,930 So a particularly dim asteroid could be missed. 429 00:32:58,310 --> 00:32:59,610 Asteroids are very cold. 430 00:32:59,611 --> 00:33:01,509 They're usually quite far away from the sun. 431 00:33:01,510 --> 00:33:05,170 But amazingly, the best way we have to find these is infrared light. 432 00:33:05,570 --> 00:33:09,589 Because things that are cold by human scale can still be very warm to an 433 00:33:09,590 --> 00:33:10,640 infrared telescope. 434 00:33:10,690 --> 00:33:15,169 So even if asteroids are just a few tens of degrees above absolute zero, that's 435 00:33:15,170 --> 00:33:16,790 still enough heat to detect them. 436 00:33:18,030 --> 00:33:24,369 When the infrared space telescope NEOWISE turned its gaze onto asteroids, 437 00:33:24,370 --> 00:33:25,550 immediate results. 438 00:33:26,810 --> 00:33:32,449 NEOWISE has now detected close to 160 ,000 new asteroids and comets in our 439 00:33:32,450 --> 00:33:36,270 system, and about 780 of those are things that are near the Earth. 440 00:33:36,970 --> 00:33:43,589 Ten of those near objects have been classified as PHAs, potentially 441 00:33:43,590 --> 00:33:46,610 asteroids, without NEOWISE. 442 00:33:47,080 --> 00:33:48,340 we would have missed them. 443 00:33:48,660 --> 00:33:53,499 Using an infrared space telescope is a way of better detecting some of the 444 00:33:53,500 --> 00:33:57,280 smaller asteroids and comets in the near -Earth vicinity. 445 00:33:58,080 --> 00:34:04,019 Detection is an important first step, but it only tells us there's another 446 00:34:04,020 --> 00:34:05,320 asteroid out there. 447 00:34:05,660 --> 00:34:10,520 Once we've spotted an asteroid... All we know is that it's a tiny dot of light. 448 00:34:10,540 --> 00:34:15,339 We don't know anything else about it. So when a new asteroid is discovered, the 449 00:34:15,340 --> 00:34:18,979 most important thing is to determine its path, to track it, to figure out 450 00:34:18,980 --> 00:34:22,019 exactly how it's orbiting around the sun and how close it's going to get to 451 00:34:22,020 --> 00:34:25,579 Earth. For that, we have to know where they are now, so its current location, 452 00:34:25,580 --> 00:34:29,500 and measure how fast it's going and which direction it's traveling. 453 00:34:29,501 --> 00:34:33,419 All of these things together are really important for tracking where it's going 454 00:34:33,420 --> 00:34:36,010 to be next and whether or not they're going to hit us. 455 00:34:38,120 --> 00:34:43,739 To get this information, we need something much bigger and more powerful. 456 00:34:44,120 --> 00:34:46,540 The Arecibo Observatory. 457 00:34:46,840 --> 00:34:52,119 Once Catalina or another telescope detects a near -Earth asteroid in our 458 00:34:52,120 --> 00:34:57,860 neighborhood, Arecibo's 1 ,000 -foot dish swings into action. 459 00:34:58,730 --> 00:35:04,349 They discover these asteroids, and then once we know where they were, we can try 460 00:35:04,350 --> 00:35:09,789 and point the radio telescope and see where they are at the moment and measure 461 00:35:09,790 --> 00:35:12,170 their exact location and their trajectory. 462 00:35:12,870 --> 00:35:18,370 Arecibo achieves this level of precision by using radio detection and ranging, 463 00:35:18,770 --> 00:35:20,270 more commonly known. 464 00:35:21,730 --> 00:35:26,429 The planetary radar system at Arecibo Observatory is the most powerful radar 465 00:35:26,430 --> 00:35:27,590 system in the world. 466 00:35:27,890 --> 00:35:32,649 We focus on potentially hazardous asteroids, which are those that have a 467 00:35:32,650 --> 00:35:34,290 probability of impacting Earth. 468 00:35:35,470 --> 00:35:39,930 Arecibo sends out radio signals towards the newly detected asteroid. 469 00:35:40,310 --> 00:35:42,330 It emanates radio signals. 470 00:35:42,570 --> 00:35:47,689 Some of them hit the asteroid, just like a radar gun from a cop might hit the 471 00:35:47,690 --> 00:35:48,740 side of your car. 472 00:35:48,960 --> 00:35:53,040 It's pretty similar, but instead of doing it with a radar gun on a small 473 00:35:53,260 --> 00:35:57,219 we're doing it at a really big scale with one megawatt power hitting objects 474 00:35:57,220 --> 00:35:59,560 that are tens of them are distances away. 475 00:36:00,040 --> 00:36:06,239 And then those radio waves bounce back to Earth and we detect them again. And 476 00:36:06,240 --> 00:36:11,819 comparing the differences between what we sent and what we received, we can get 477 00:36:11,820 --> 00:36:17,199 a map of the asteroid itself and we can get where it's moving and how fast it's 478 00:36:17,200 --> 00:36:18,250 moving. 479 00:36:20,300 --> 00:36:24,020 But asteroids may not be the biggest threat from faith. 480 00:36:25,100 --> 00:36:27,660 November 25, 2018. 481 00:36:28,800 --> 00:36:34,639 Cameras on board the solar and heliospheric observatory film a large 482 00:36:34,640 --> 00:36:36,160 crashing into the sun. 483 00:36:38,140 --> 00:36:43,019 We recorded the impact of an object into the sun at over a million miles per 484 00:36:43,020 --> 00:36:44,070 hour. 485 00:36:45,060 --> 00:36:46,740 The incredible speed. 486 00:36:47,040 --> 00:36:49,120 tells us that this was not an asteroid. 487 00:36:49,400 --> 00:36:55,019 It was the death plunge of something much more unpredictable and dangerous, a 488 00:36:55,020 --> 00:36:58,440 killer object from the outer reaches of the solar system. 489 00:36:59,560 --> 00:37:03,739 Comets, in some way, you could consider maybe being more dangerous than near 490 00:37:03,740 --> 00:37:04,790 -Earth asteroids. 491 00:37:04,791 --> 00:37:08,559 With near -Earth asteroids, you could imagine that we would discover all of 492 00:37:08,560 --> 00:37:12,819 them. And if we get perfect knowledge of all of their orbits, we can predict 493 00:37:12,820 --> 00:37:16,520 into the future where they'll be and when they may or may not. 494 00:37:16,810 --> 00:37:20,370 have an orbit that crosses the actual Earth and could be an impact. 495 00:37:21,350 --> 00:37:24,470 Comets, a large part of that population, we only see once. 496 00:37:24,471 --> 00:37:28,649 They come in from way out in the distant part of the solar system, they do one 497 00:37:28,650 --> 00:37:32,130 lap around the sun, and they go back out there for millions of years. 498 00:37:35,270 --> 00:37:39,590 Comets are dirty snowballs, huge lumps of ice and dust. 499 00:37:39,970 --> 00:37:42,430 They come in two flavors. 500 00:37:42,431 --> 00:37:45,979 There's something we call short -period comet. 501 00:37:45,980 --> 00:37:49,999 These are comets that are kind of constrained to the solar system, the 502 00:37:50,000 --> 00:37:53,550 solar system, and their orbits are never more than a few hundred years. 503 00:37:54,480 --> 00:37:59,119 Short -period comets come from the Kuiper Belt, a region of the solar 504 00:37:59,120 --> 00:38:00,880 beyond the orbit of Neptune. 505 00:38:02,380 --> 00:38:06,440 These comets have short orbits on the same plane as Earth. 506 00:38:12,940 --> 00:38:14,540 The second type of comet. 507 00:38:14,800 --> 00:38:17,180 are called long -period comets. 508 00:38:17,620 --> 00:38:23,279 They originate in the Oort Cloud, a sphere of icy objects located at the 509 00:38:23,280 --> 00:38:24,880 edges of the solar system. 510 00:38:27,580 --> 00:38:31,619 There are thousands and thousands of comets out there in the Oort Cloud. 511 00:38:31,620 --> 00:38:32,579 just waiting. 512 00:38:32,580 --> 00:38:35,819 And so, in principle, one of them can get knocked off course and come raining 513 00:38:35,820 --> 00:38:37,700 down into the inner solar system. 514 00:38:41,770 --> 00:38:47,290 Long period comets are very large, and they travel very fast. 515 00:38:48,130 --> 00:38:51,130 Comets can get really big, and they're really heavy. 516 00:38:51,390 --> 00:38:55,510 And essentially, they're falling to Earth from 2 billion light years away. 517 00:38:55,770 --> 00:38:58,490 So imagine how fast they're going. 518 00:38:59,270 --> 00:39:04,829 We know from studying asteroids that the faster they go, the more kinetic energy 519 00:39:04,830 --> 00:39:06,070 they release on impact. 520 00:39:10,130 --> 00:39:11,270 Comet travel. 521 00:39:11,550 --> 00:39:13,330 even faster than asteroids. 522 00:39:14,210 --> 00:39:17,450 In general, they're moving 50 % faster, something like that. 523 00:39:17,650 --> 00:39:21,990 But that doubles their impact energy. And that's sort of a best -case 524 00:39:22,190 --> 00:39:26,369 In a worst -case scenario, pound for pound, they could have five or up to 525 00:39:26,370 --> 00:39:29,210 ten times as much energy as an asteroid impact. 526 00:39:33,550 --> 00:39:37,070 The Bering Sea asteroid blew up in the atmosphere. 527 00:39:37,800 --> 00:39:42,660 But the Beringer crater asteroid hit the ground intact with its full force. 528 00:39:45,300 --> 00:39:48,880 Why do different asteroids behave differently? 529 00:39:49,360 --> 00:39:53,380 And what will Apophis do when it heads our way? 530 00:39:54,520 --> 00:39:57,400 Arecibo's radar may have the answer. 531 00:39:58,200 --> 00:40:03,239 When we bounce radar waves off of these objects, we can get... effectively 532 00:40:03,240 --> 00:40:07,919 imagery of the surface of some of these small objects that we just cannot do 533 00:40:07,920 --> 00:40:09,180 with optical telescopes. 534 00:40:09,740 --> 00:40:12,760 This is the radar image of Apophis. 535 00:40:13,180 --> 00:40:17,880 It's so far away that all we could image was a few pixels. 536 00:40:19,500 --> 00:40:24,040 So this is our most recent radar image of asteroid Apophis. 537 00:40:25,120 --> 00:40:31,359 And you can see it's only a few pixels, but it does give us... information on 538 00:40:31,360 --> 00:40:33,020 what it actually is. 539 00:40:34,320 --> 00:40:38,980 These few pixels are enough to work out how big a pofis is. 540 00:40:40,520 --> 00:40:46,699 From this image, we can constrain the size to be about 1 ,000 feet, which is 541 00:40:46,700 --> 00:40:50,480 about the same size as our receiver radio telescope. 542 00:40:51,000 --> 00:40:53,900 All of that from a weird bunch of pixels. 543 00:41:00,140 --> 00:41:05,179 Knowing the size and mass of an asteroid is critical to understanding what an 544 00:41:05,180 --> 00:41:06,600 asteroid is made of. 545 00:41:07,560 --> 00:41:10,300 If we have the size and the mass, we get the density. 546 00:41:10,520 --> 00:41:12,930 If we have the density, we know what it's made of. 547 00:41:13,120 --> 00:41:14,800 Rock has some density. 548 00:41:15,180 --> 00:41:16,720 Metal has a different density. 549 00:41:16,920 --> 00:41:21,799 So we can determine a huge amount about the asteroid simply by pinging it with 550 00:41:21,800 --> 00:41:22,850 radar. 551 00:41:25,620 --> 00:41:29,790 Arecibo's data reveals... that not all asteroids are alike. 552 00:41:31,390 --> 00:41:35,000 There's not just one kind of asteroid. There are actually several kinds. 553 00:41:35,250 --> 00:41:38,890 And this is important to understand because they behave differently. 554 00:41:38,891 --> 00:41:42,629 They behave differently if they impact us, and they behave differently if we're 555 00:41:42,630 --> 00:41:48,089 trying to prevent them from impacting us. We need to know what these asteroids 556 00:41:48,090 --> 00:41:52,849 are made of, if they're going to hit the Earth, because that drastically alters 557 00:41:52,850 --> 00:41:54,130 the potential effects. 558 00:41:54,350 --> 00:41:58,790 Asteroids come in different shapes, different sizes, and different 559 00:41:59,110 --> 00:42:03,210 And we think that is because they are the leftovers of planet formation. 560 00:42:03,590 --> 00:42:09,289 To understand how each asteroid formed and its threat level, we have to go back 561 00:42:09,290 --> 00:42:13,670 4 .6 billion years to the start of the solar system. 562 00:42:14,030 --> 00:42:18,069 The reason that there are all these asteroids floating around in our solar 563 00:42:18,070 --> 00:42:22,089 system today is just because of the early violence of the solar system as it 564 00:42:22,090 --> 00:42:23,140 forming. 565 00:42:25,040 --> 00:42:31,619 At the birth of the solar system, the sun ignited, leaving a 566 00:42:31,620 --> 00:42:33,480 disk of gas and dust. 567 00:42:37,000 --> 00:42:40,200 Slowly over time, planets formed. 568 00:42:40,940 --> 00:42:42,360 Many planets. 569 00:42:43,660 --> 00:42:49,159 The early solar system was a messy place. There were a lot more planets, a 570 00:42:49,160 --> 00:42:53,639 more forming planets. They would crash into each other. They would merge. They 571 00:42:53,640 --> 00:42:55,640 would disintegrate. They would reform. 572 00:42:59,120 --> 00:43:04,780 This process of accretion, of building planetary worlds, was not just, you 573 00:43:04,840 --> 00:43:07,280 kind of gentle and happy. It was violent. 574 00:43:09,040 --> 00:43:12,620 It was like a giant cosmic game of pool. 575 00:43:14,199 --> 00:43:16,720 planets smashing into planets. 576 00:43:17,200 --> 00:43:22,960 The leftovers from this violence formed a ring of junk between Mars and Jupiter. 577 00:43:23,420 --> 00:43:25,840 And now we call that junk asteroids. 578 00:43:26,240 --> 00:43:30,270 They're just basically rubble left over from the formation of the solar system. 579 00:43:32,140 --> 00:43:36,500 Rocky leftovers became C -type, or chondrite asteroids. 580 00:43:36,980 --> 00:43:42,260 They are quite dense, so big ones can punch through the atmosphere. 581 00:43:42,720 --> 00:43:43,800 and hit the ground. 582 00:43:49,660 --> 00:43:52,840 Radar reveals a rarer type of asteroid. 583 00:43:54,100 --> 00:43:58,419 Some of them really stand out because their density is so much higher than the 584 00:43:58,420 --> 00:43:59,800 rest of the other asteroids. 585 00:44:00,720 --> 00:44:04,000 These asteroids are M -type, or metal. 586 00:44:06,140 --> 00:44:11,140 Because their mass is great, they carry more kinetic energy. 587 00:44:11,470 --> 00:44:12,520 During a strike. 588 00:44:13,250 --> 00:44:17,310 By far the worst one is this iron meteorite. 589 00:44:17,530 --> 00:44:18,830 This is really heavy. 590 00:44:18,831 --> 00:44:22,529 So the difference, if you were being hit by this, would be the difference 591 00:44:22,530 --> 00:44:26,050 between being hit by a rock and being hit by a metal hammer. 592 00:44:27,750 --> 00:44:34,429 We think that both the Behringer and the KPG dinosaur killer events were 593 00:44:34,430 --> 00:44:36,570 caused by metal asteroids. 594 00:44:40,080 --> 00:44:44,540 There is another, more mysterious type floating through space. 595 00:44:47,980 --> 00:44:49,460 December 2018. 596 00:44:50,180 --> 00:44:55,740 NASA spacecraft OSIRIS -REx approached the near -Earth asteroid Bennu. 597 00:44:57,700 --> 00:45:01,999 Over time, it drifted out of the main asteroid belt, made its way into the 598 00:45:02,000 --> 00:45:06,319 solar system, until it became a near -Earth asteroid accessible for our 599 00:45:06,320 --> 00:45:07,760 spacecraft to go in business. 600 00:45:08,960 --> 00:45:12,140 Osiris -Rex trained its camera on Bennu. 601 00:45:18,580 --> 00:45:23,979 One of the biggest surprises on arrival at Bennu was the large number of large 602 00:45:23,980 --> 00:45:25,180 boulders on its surface. 603 00:45:25,380 --> 00:45:29,719 Bennu is really littered with huge boulders and littered with medium -sized 604 00:45:29,720 --> 00:45:34,700 boulders and littered with small boulders. Bennu is not a solid lump of 605 00:45:34,990 --> 00:45:40,590 It's made up of thousands of bits of rock forming what we call a rubble pile. 606 00:45:40,990 --> 00:45:46,709 These asteroids aren't big, singular, spherical balls of rock, but rather 607 00:45:46,710 --> 00:45:48,450 they're literally piles of rubble. 608 00:45:48,451 --> 00:45:51,909 They're all sorts of pieces and fragments from another asteroid that had 609 00:45:51,910 --> 00:45:56,249 previously been disrupted that have all come back together and formed literally 610 00:45:56,250 --> 00:45:59,150 a pile of rocks held together by their own gravity. 611 00:45:59,630 --> 00:46:04,370 We think rubble piles form from collisions inside the asteroid belt. 612 00:46:04,830 --> 00:46:11,109 Each impact blasted bits off. Then over time, they came back together to form 613 00:46:11,110 --> 00:46:12,770 the loose pile of rocks. 614 00:46:13,230 --> 00:46:18,529 Imagine taking a big cosmic dump truck full of gravel and rubble and dumping it 615 00:46:18,530 --> 00:46:22,250 out there into space and letting gravity weakly hold it together. 616 00:46:23,630 --> 00:46:28,670 When scientists probed deeper into Bennu, they had another surprise. 617 00:46:29,210 --> 00:46:32,790 It's full of holes, like Swiss cheese. 618 00:46:33,610 --> 00:46:37,749 If you could slice open one of these asteroids, you'd see there are a lot of 619 00:46:37,750 --> 00:46:42,110 voids. In fact, 60 % of what we're looking at is a void space. 620 00:46:42,350 --> 00:46:44,090 So they're actually really fluffy. 621 00:46:44,330 --> 00:46:47,880 So even though they're made of rocks, they're sort of the lint of rocks. 622 00:46:48,290 --> 00:46:51,070 Bennu helps us understand a pulpit. 623 00:46:51,730 --> 00:46:56,550 Radar data shows that a pulpit is also a rubble pile. 624 00:46:56,551 --> 00:47:00,479 If you look at Apophis, we really want to know how its orbit will evolve in the 625 00:47:00,480 --> 00:47:05,339 future. What we learn at Bennu about similar -sized rubble pile asteroids 626 00:47:05,340 --> 00:47:08,290 help us understand the future of an asteroid like Apophis. 627 00:47:08,760 --> 00:47:12,840 So what would happen if rubble pile Apophis hits Earth? 628 00:47:12,841 --> 00:47:16,979 You probably don't want that to hit you still, but it definitely makes it a lot 629 00:47:16,980 --> 00:47:22,559 weaker than something like a solid rock or, even more, a chunk of nickel -iron 630 00:47:22,560 --> 00:47:25,420 metal. Does its rubble pile composition? 631 00:47:25,960 --> 00:47:27,780 make it any less of a threat. 632 00:47:28,180 --> 00:47:32,999 A rubble pile like Apophis is especially unnerving because we don't know when it 633 00:47:33,000 --> 00:47:36,139 interacts with the atmosphere if it's going to stay as one solid piece. 634 00:47:36,140 --> 00:47:37,190 Will it break up? 635 00:47:38,380 --> 00:47:42,979 When these rubble piles start interacting with planets, if they fly 636 00:47:42,980 --> 00:47:46,059 planet, they can get pulled apart into all of their little pieces. 637 00:47:46,060 --> 00:47:50,899 Or if they enter the atmosphere of a planet to impact the surface, they might 638 00:47:50,900 --> 00:47:53,620 slowly get pulled apart as they enter the atmosphere. 639 00:47:54,750 --> 00:47:58,510 and end up being an array of little impacts instead of one big single 640 00:48:03,590 --> 00:48:07,310 In 2017, we had another wake -up call. 641 00:48:07,650 --> 00:48:11,370 A strange base rock arrived in our neighborhood. 642 00:48:11,790 --> 00:48:15,590 Its shape was unlike anything we'd seen before. 643 00:48:16,650 --> 00:48:20,849 The thing that made Oumuamua different from anything else we'd ever seen is it 644 00:48:20,850 --> 00:48:25,090 seemed to be almost a shard, a sharp piece of metal tumbling through space. 645 00:48:26,390 --> 00:48:30,350 Typically, things that move around our solar system are somewhat spherical. 646 00:48:31,470 --> 00:48:35,110 This in no way was spherical. It was almost cigar -shaped. 647 00:48:35,640 --> 00:48:39,540 So it kind of really plugged into all those alien theories. 648 00:48:39,940 --> 00:48:43,820 But we were able to confirm that it didn't flow down as it went by the 649 00:48:43,821 --> 00:48:47,239 which was, we figured if it was an alien craft, it would probably stop and have 650 00:48:47,240 --> 00:48:49,950 a little bit of a look. But it carried on its trajectory. 651 00:48:50,380 --> 00:48:54,660 It wasn't a comet or an asteroid from the asteroid belt. 652 00:48:55,100 --> 00:48:58,560 It was a space rock from interstellar space. 653 00:48:58,561 --> 00:49:03,619 Interstellar asteroids are probably pretty rare, but the thing about them is 654 00:49:03,620 --> 00:49:05,020 they're moving really fast. 655 00:49:05,460 --> 00:49:08,500 So if they happen to hit us, it's really bad. 656 00:49:09,580 --> 00:49:14,560 Oumuamua was traveling over 100 times faster than a fighter jet. 657 00:49:14,840 --> 00:49:17,920 And as we know, speed means danger. 658 00:49:18,980 --> 00:49:23,599 Had Oumuamua been on an impact trajectory with the Earth, at those 659 00:49:23,600 --> 00:49:27,480 speeds, very much faster than anything in our solar system, 660 00:49:28,400 --> 00:49:33,879 remember the kinetic energy goes as the square of the impact speed. At those 661 00:49:33,880 --> 00:49:34,930 kinds of speeds, 662 00:49:35,760 --> 00:49:40,859 imagine it hitting us at 196 ,000 miles per hour, that carries an incredibly 663 00:49:40,860 --> 00:49:46,439 powerful punch. And so for a given size object, the impact of Oumuamua compared 664 00:49:46,440 --> 00:49:50,720 to a... regular solar system objects would have been absolutely devastating. 665 00:49:51,680 --> 00:49:56,619 Oumuamua passed safely through the solar system, but it won't be the last 666 00:49:56,620 --> 00:49:58,660 invader from interstellar space. 667 00:49:59,180 --> 00:50:05,079 Astronomers estimate that one alien object visits our cosmic neighborhood 668 00:50:05,080 --> 00:50:06,130 year. 669 00:50:09,700 --> 00:50:10,750 2019. 670 00:50:11,600 --> 00:50:12,650 U .S. 671 00:50:12,880 --> 00:50:15,240 researchers discovered deposits of fossils. 672 00:50:15,980 --> 00:50:20,400 They contain both the remnants of land and sea creatures. 673 00:50:20,920 --> 00:50:26,599 You see things that are all jumbled together. So you'll have fossils of sea 674 00:50:26,600 --> 00:50:32,779 creatures. You'll have ocean deposits that are mixed up with coastal deposits 675 00:50:32,780 --> 00:50:38,519 and onshore deposits. And you see those deposits in places that are very, very 676 00:50:38,520 --> 00:50:42,719 far away from where you would expect them to be. And so this material was 677 00:50:42,720 --> 00:50:44,840 obviously thrown very far inland. 678 00:50:46,760 --> 00:50:52,639 The jumbled deposits suggest the creatures were killed at the same time 679 00:50:52,640 --> 00:50:57,799 huge and violent event, something powerful enough to sweep ocean -dwelling 680 00:50:57,800 --> 00:50:59,840 creatures far inland. 681 00:51:00,940 --> 00:51:02,300 A tsunami. 682 00:51:03,080 --> 00:51:07,920 Tsunamis are usually created when the ocean floor suddenly moves. 683 00:51:08,420 --> 00:51:14,199 The ground picks up the entire ocean and shakes it up and down, and it's sort of 684 00:51:14,200 --> 00:51:15,820 like taking a rope and shaking it. 685 00:51:15,900 --> 00:51:20,820 and it moves all across the ocean floor and ocean surface until it reaches land. 686 00:51:21,020 --> 00:51:26,019 The biggest recent tsunami was caused by the Earth's crust at the bottom of the 687 00:51:26,020 --> 00:51:31,379 ocean lifting slightly. So this means that that entire length of crust that 688 00:51:31,380 --> 00:51:37,619 lifted displaced the water above it. So the waves, the tsunamis that result, are 689 00:51:37,620 --> 00:51:42,919 really long and wide, and it can travel across the ocean at tremendous speeds 690 00:51:42,920 --> 00:51:44,020 and up on land. 691 00:51:46,350 --> 00:51:49,130 Is this what happened to the fossilized creatures? 692 00:51:49,530 --> 00:51:52,370 Were they killed by a huge tsunami? 693 00:51:53,030 --> 00:51:55,690 Clues come from dating the preserved remains. 694 00:51:56,910 --> 00:51:59,850 They are 66 million years old. 695 00:52:00,070 --> 00:52:05,889 From the same time, a six -mile -wide asteroid crashed into the sea off the 696 00:52:05,890 --> 00:52:07,510 Yucatan Peninsula, Mexico. 697 00:52:11,290 --> 00:52:13,350 Are the two events connected? 698 00:52:14,190 --> 00:52:17,930 Do ocean -impacting asteroids trigger tsunamis? 699 00:52:18,490 --> 00:52:22,589 We used to think that a big asteroid impacting in the ocean would drive a 700 00:52:22,590 --> 00:52:28,189 tremendous tsunami, a huge wall of water, out at very rapid speeds, which 701 00:52:28,190 --> 00:52:29,930 basically scour clean everything. 702 00:52:30,770 --> 00:52:36,110 Now, new research from 2018 suggests a very different scenario. 703 00:52:36,690 --> 00:52:41,910 Scientists used supercomputers to model asteroids hitting the deep ocean. 704 00:52:42,480 --> 00:52:47,819 to work out how much of the asteroid's kinetic energy is converted into a 705 00:52:47,820 --> 00:52:48,870 tsunami wave. 706 00:52:50,200 --> 00:52:56,999 In the simulations, a 1600 -foot asteroid hits the ocean at 20 ,000 miles 707 00:52:57,000 --> 00:52:59,640 an hour and dives into the water. 708 00:53:01,040 --> 00:53:05,859 As it goes deeper in, of course it's meeting a lot of resistance, and it 709 00:53:05,860 --> 00:53:10,179 down and it compresses up. It compresses and compresses and compresses. And then 710 00:53:10,180 --> 00:53:14,940 finally it runs out of momentum, and it's at an extremely high pressure. 711 00:53:15,880 --> 00:53:21,060 The huge pressure causes the asteroid to explode and vaporize. 712 00:53:21,880 --> 00:53:26,779 Temperatures hotter than the surface of the sun turn trillions of gallons of 713 00:53:26,780 --> 00:53:27,960 water into steam. 714 00:53:28,360 --> 00:53:29,520 The blast. 715 00:53:29,820 --> 00:53:36,339 creates a huge short -lived cavity in the water surface and a splash curtain, 716 00:53:36,340 --> 00:53:39,100 wall of water that leaps up several miles. 717 00:53:39,540 --> 00:53:45,339 This curtain then collapses and water falls back into the cavity, shooting a 718 00:53:45,340 --> 00:53:48,220 column of water five miles up. 719 00:53:48,460 --> 00:53:53,840 This very tall column can't support its own weight and collapses back down. 720 00:53:54,760 --> 00:53:57,060 The collapse of so much water. 721 00:53:57,390 --> 00:53:59,790 triggers a 1 ,200 -foot -high wave. 722 00:54:00,230 --> 00:54:02,970 Could this become a huge tsunami? 723 00:54:08,470 --> 00:54:12,869 If we think about a meteor striking the ocean, we want to understand how far the 724 00:54:12,870 --> 00:54:16,089 waves might propagate from the site. We could actually just use a stone and 725 00:54:16,090 --> 00:54:17,390 throw it into a pond. 726 00:54:17,391 --> 00:54:21,089 And you might think, OK, well, it's a big stone. It's going to make a really 727 00:54:21,090 --> 00:54:23,689 splash, and that's just going to extend out a long distance. 728 00:54:23,690 --> 00:54:27,299 But it turns out the splash stays... the biggest, really close to where it 729 00:54:27,300 --> 00:54:30,670 impacts, and then the ripples die down after that. So let's try that. 730 00:54:32,240 --> 00:54:33,540 Big splash in the middle. 731 00:54:33,541 --> 00:54:38,079 And we see the ripples going outward, but they're really pretty small compared 732 00:54:38,080 --> 00:54:39,520 with that initial big splash. 733 00:54:41,560 --> 00:54:44,900 It's the same with an ocean -impacting asteroid. 734 00:54:45,920 --> 00:54:51,519 The impact creates surface waves that die away quickly because only a small 735 00:54:51,520 --> 00:54:54,600 amount of the asteroid's kinetic energy gets into the water. 736 00:54:55,160 --> 00:54:59,179 It's actually pretty tough to make a tsunami like that. The energy of the 737 00:54:59,180 --> 00:55:03,000 asteroid doesn't couple well with the water to drive this wave. 738 00:55:03,400 --> 00:55:08,779 Instead, most of the energy goes into vaporizing the asteroid itself, as well 739 00:55:08,780 --> 00:55:10,320 all of the water around it. 740 00:55:11,000 --> 00:55:16,080 Only 1 % of the asteroid's kinetic energy goes into making a wave. 741 00:55:16,520 --> 00:55:23,079 So only low -energy waves form, too weak to become giant tsunamis traveling 742 00:55:23,080 --> 00:55:24,280 hundreds of miles. 743 00:55:25,040 --> 00:55:30,339 So what caused the jumbled fossil deposit thousands of miles away from the 744 00:55:30,340 --> 00:55:31,390 impact site? 745 00:55:31,500 --> 00:55:36,219 We don't think there could be that much energy still transmitted that far away 746 00:55:36,220 --> 00:55:37,270 from the impact site. 747 00:55:37,780 --> 00:55:42,159 Instead, there has to be a different source of energy that created different 748 00:55:42,160 --> 00:55:45,180 waves right about the same time as that impact event. 749 00:55:47,180 --> 00:55:50,320 Research from 2019 may have the answer. 750 00:55:50,910 --> 00:55:56,869 The KPG asteroid struck on the continental shelf, the shallow region 751 00:55:56,870 --> 00:55:58,690 land and deep ocean. 752 00:55:59,050 --> 00:56:04,709 The impact triggered a localized tsunami, large enough to kill creatures 753 00:56:04,710 --> 00:56:09,570 region. But it also sent a huge shockwave into the bedrock. 754 00:56:09,950 --> 00:56:14,289 There's going to be a shockwave driven through the ground. That probably would 755 00:56:14,290 --> 00:56:20,450 have killed anything in the area. If you had a dinosaur that was standing on... 756 00:56:20,620 --> 00:56:27,319 The Gulf Coast of what is now the United States, that animal would have 757 00:56:27,320 --> 00:56:33,879 experienced a seismic pulse, an earthquake that is stronger than 758 00:56:33,880 --> 00:56:38,159 current Richter scale. It would have actually driven its legs up into its 759 00:56:38,160 --> 00:56:39,660 cavity, killing it instantly. 760 00:56:39,720 --> 00:56:44,719 There's all manner of mayhem and death taking place at this time. There was no 761 00:56:44,720 --> 00:56:45,770 escape in this event. 762 00:56:48,880 --> 00:56:52,780 The initial shockwave would have traveled through the Earth's crust. 763 00:56:54,560 --> 00:56:59,779 The impact would have shaken the crust of the Earth, which also would have 764 00:56:59,780 --> 00:57:03,819 triggered earthquakes around the world, which themselves may have triggered 765 00:57:03,820 --> 00:57:05,080 secondary tsunamis. 766 00:57:08,240 --> 00:57:14,039 Secondary tsunamis, thousands of miles from the impact site, killed both land 767 00:57:14,040 --> 00:57:15,260 and sea creatures. 768 00:57:15,780 --> 00:57:17,700 The KPG impact. 769 00:57:18,000 --> 00:57:22,400 went on to wipe out 70 % of all life on Earth. 770 00:57:28,580 --> 00:57:34,000 How could one space rock hitting the sea cause a global catastrophe? 771 00:57:35,760 --> 00:57:40,879 When you have a big rock hitting the ocean, the biggest danger is not from 772 00:57:40,880 --> 00:57:43,700 waves, but actually from the steam that it creates. 773 00:57:44,280 --> 00:57:45,330 The impact. 774 00:57:45,760 --> 00:57:48,620 vaporized trillions of tons of seawater. 775 00:57:48,940 --> 00:57:54,800 This steam rose up into the atmosphere where it condensed into water vapor. 776 00:57:55,460 --> 00:57:57,480 Water vapor is a greenhouse gas. 777 00:57:57,710 --> 00:58:04,149 So that's then going up into the upper atmosphere, and it's trapping heat, but 778 00:58:04,150 --> 00:58:08,069 at different layers it's making clouds. It's just throwing everything off 779 00:58:08,070 --> 00:58:12,889 kilter. Water is a very effective greenhouse gas. You will actually affect 780 00:58:12,890 --> 00:58:16,950 very significant climate change very quickly as a result of that impact. 781 00:58:19,050 --> 00:58:24,229 Within weeks of the asteroid strike, water vapor in the atmosphere caused 782 00:58:24,230 --> 00:58:25,470 temperatures to rise. 783 00:58:26,920 --> 00:58:28,700 But that was only the start. 784 00:58:29,500 --> 00:58:35,700 The impact also blew out 10 trillion tons of rock, ash, and dust. 785 00:58:38,000 --> 00:58:43,440 This asteroid is so big, it's six miles wide. It's punched a hole in the air. 786 00:58:43,560 --> 00:58:47,699 There's like a column of low density, a chimney, that goes from the ground up to 787 00:58:47,700 --> 00:58:48,919 the top of the atmosphere. 788 00:58:48,920 --> 00:58:52,340 And that means there's very little air resistance in that tunnel. 789 00:58:52,970 --> 00:58:57,629 These rocks can actually blast up into the chimney and find it easier to get up 790 00:58:57,630 --> 00:59:03,149 out of the atmosphere. It sent that material flying up halfway to the orbit 791 00:59:03,150 --> 00:59:08,769 the moon, circled around the Earth, all this ring of material falling back onto 792 00:59:08,770 --> 00:59:12,450 the Earth, and it was like the sky itself was on fire. 793 00:59:13,030 --> 00:59:17,069 So you not only do have rocks falling on you, but they're molten, and these 794 00:59:17,070 --> 00:59:21,050 rocks will start catching plants and anything else on fire. 795 00:59:26,920 --> 00:59:31,940 Soot and ash rose up into the atmosphere, blocking the sun. 796 00:59:35,000 --> 00:59:39,439 Material was thrown into the atmosphere, plunging the planet into a nuclear 797 00:59:39,440 --> 00:59:44,580 winter. It was complete chaos, and it went dark for two full years. 798 00:59:46,200 --> 00:59:49,820 Without sunlight, temperatures seesawed. 799 00:59:50,520 --> 00:59:55,680 Just months after the impact, the planet cooled by 20 degrees. 800 00:59:57,100 --> 01:00:00,230 In the immediate area, there's just tremendous destruction. 801 01:00:00,231 --> 01:00:01,839 Just everything gets destroyed. 802 01:00:01,840 --> 01:00:06,040 But over the long term, you're talking about ash kicked up in the atmosphere, 803 01:00:06,320 --> 01:00:09,880 extremely cold weather, basically a global ice age. 804 01:00:11,480 --> 01:00:14,620 The freezing temperatures killed off most plant life. 805 01:00:15,700 --> 01:00:17,880 Imagine how that affected life on Earth. 806 01:00:18,160 --> 01:00:21,600 No plants, and the base of the ecosystem collapses. 807 01:00:24,720 --> 01:00:30,819 This dark nuclear winter lasted two years and prevented plants from 808 01:00:30,820 --> 01:00:32,100 photosynthesizing. 809 01:00:33,280 --> 01:00:38,499 So if plants can no longer use photosynthesis to live, they'll die. And 810 01:00:38,500 --> 01:00:42,220 with no plants, then you have no food for these larger animals. 811 01:00:42,500 --> 01:00:46,720 And so anything that eats those animals will also die. If you lose your plants, 812 01:00:46,880 --> 01:00:49,110 you're going to lose your large -scale life. 813 01:00:50,040 --> 01:00:53,100 First, plant -eating herbivores died off. 814 01:00:53,420 --> 01:00:55,500 than meat -eating carnivores. 815 01:00:56,660 --> 01:01:02,019 Most of the dinosaurs were just unable to find food and to survive through the 816 01:01:02,020 --> 01:01:03,440 cold, long night. 817 01:01:04,460 --> 01:01:08,040 The global devastation wasn't over yet. 818 01:01:08,340 --> 01:01:14,259 The rock of the continental shelf, where the asteroid hit, contained carbon and 819 01:01:14,260 --> 01:01:15,310 sulfur. 820 01:01:15,820 --> 01:01:21,759 These carbonate rocks were heated and vaporized and released carbon dioxide 821 01:01:21,760 --> 01:01:27,039 the atmosphere, yet another greenhouse gas. So you're vaporizing a lot of 822 01:01:27,040 --> 01:01:33,279 sulfur, a lot of salt of different kinds that are then lofted up into the upper 823 01:01:33,280 --> 01:01:35,880 atmosphere that then plays havoc on the climate. 824 01:01:40,840 --> 01:01:44,080 These greenhouse gases built up in the atmosphere. 825 01:01:44,780 --> 01:01:46,560 forming a warming blanket. 826 01:01:49,600 --> 01:01:53,900 These gases triggered the next phase of destruction. 827 01:01:55,460 --> 01:01:58,620 Global warming on steroids. 828 01:02:00,880 --> 01:02:04,680 Temperatures rose 10 degrees above normal. 829 01:02:05,020 --> 01:02:07,820 Then the oceans warmed as well. 830 01:02:08,680 --> 01:02:12,980 Oxygen levels dropped and the seas became toxic. 831 01:02:13,400 --> 01:02:14,900 To simple life forms. 832 01:02:16,640 --> 01:02:21,559 That actually made it impossible for certain microbes to actually live. And 833 01:02:21,560 --> 01:02:26,319 they're the basis of the food system. So really it changed what could actually 834 01:02:26,320 --> 01:02:28,680 live in the ocean and how much could live there. 835 01:02:30,360 --> 01:02:34,980 Dead zones appeared in the oceans just as they had on land. 836 01:02:36,100 --> 01:02:39,180 Nearly three quarters of life on Earth died. 837 01:02:41,840 --> 01:02:44,580 All from what asteroid impact? 838 01:02:48,520 --> 01:02:54,079 To prevent it from happening again, we need to track all potentially dangerous 839 01:02:54,080 --> 01:03:00,999 asteroids. But that's not easy, because these floating space rocks can change 840 01:03:01,000 --> 01:03:02,050 direction. 841 01:03:11,220 --> 01:03:14,200 Security cameras record a flash in the sky. 842 01:03:16,800 --> 01:03:21,520 The flash was from a three -foot asteroid exploding in the atmosphere. 843 01:03:28,020 --> 01:03:32,699 It blew up in the atmosphere and rained down. And people saw that. It was very 844 01:03:32,700 --> 01:03:37,399 noticeable. And they went and they collected those meteorites. And then 845 01:03:37,400 --> 01:03:39,690 tried to figure out what they were looking at. 846 01:03:42,280 --> 01:03:45,240 The debris was sent for fragment analysis. 847 01:03:47,300 --> 01:03:48,940 I have a piece of one here. 848 01:03:49,180 --> 01:03:53,199 So first, on the outside, you can see it has a really black fusion crust. This 849 01:03:53,200 --> 01:03:56,039 is from when it fell into the Earth's atmosphere, so it was melted. 850 01:03:56,040 --> 01:04:01,240 But when you look on the inside, it reveals this beautiful, very light 851 01:04:01,300 --> 01:04:02,500 fine -grained material. 852 01:04:02,760 --> 01:04:06,550 And so these meteorites are incredibly distinctive and really beautiful. 853 01:04:07,080 --> 01:04:08,960 The meteorites are rocky. 854 01:04:09,520 --> 01:04:14,060 Their beautiful color comes from a mineral called Howardite. 855 01:04:14,440 --> 01:04:17,520 It's rare, and it doesn't form on Earth. 856 01:04:18,860 --> 01:04:23,439 Howardite meteorites come from the asteroid Vesta, and we know that because 857 01:04:23,440 --> 01:04:27,139 the Dawn mission that actually went to Vesta and took a look at it very 858 01:04:27,140 --> 01:04:29,620 carefully, so we know the composition very well. 859 01:04:29,860 --> 01:04:34,359 And so now suddenly here was a new kind of meteorite that's in Turkey that 860 01:04:34,360 --> 01:04:37,360 matches the Vesta family of meteorites. 861 01:04:41,130 --> 01:04:45,830 But how can we be sure that these bits of space rock come from Vesta? 862 01:04:47,630 --> 01:04:52,389 It was a fall meteorite, and so what that means is that someone saw it. You 863 01:04:52,390 --> 01:04:56,949 know, we saw it fall, and so we knew its trajectory, so we could actually work 864 01:04:56,950 --> 01:05:00,130 backwards to say, where did that meteorite come from? 865 01:05:01,210 --> 01:05:06,169 Tracing the trajectory of the Turkish meteorite back took the scientists all 866 01:05:06,170 --> 01:05:09,430 way to the 328 -mile -wide Vesta. 867 01:05:13,040 --> 01:05:17,620 When they studied Vesta's surface, they found further evidence. 868 01:05:18,540 --> 01:05:23,339 On the surface of Vesta, there's actually a very large and fresh impact 869 01:05:23,340 --> 01:05:29,099 that is around the same age of the Turkish meteorite. So that really 870 01:05:29,100 --> 01:05:32,080 it. This thing is definitely from Vesta, and we proved it. 871 01:05:32,720 --> 01:05:36,620 So how did bits of Vesta end up here on Earth? 872 01:05:37,070 --> 01:05:43,409 22 million years ago, some very large impactor struck Vesta and made a huge 873 01:05:43,410 --> 01:05:48,349 crater. And some of the rocks from that crater actually escaped from Vesta's 874 01:05:48,350 --> 01:05:50,890 gravity and were lofted into space. 875 01:05:53,150 --> 01:05:58,050 Some of these rocks from Vesta went into orbit that intersected with Earth. 876 01:05:58,510 --> 01:06:03,130 22 million years later, one blew up over Sarah Chichak. 877 01:06:05,230 --> 01:06:10,930 The Saracicic meteor shows that the asteroid belt is an unstable 878 01:06:13,610 --> 01:06:17,270 Asteroids frequently strike other asteroids. 879 01:06:17,271 --> 01:06:23,399 That's actually happening all the time. Things are running into each other in 880 01:06:23,400 --> 01:06:28,139 our solar system right now. And so that makes it really hard for us to track all 881 01:06:28,140 --> 01:06:31,899 of those objects because we don't actually know what happens after they 882 01:06:31,900 --> 01:06:35,079 with each other. Now things are totally different. That changes the whole 883 01:06:35,080 --> 01:06:36,130 system. 884 01:06:36,660 --> 01:06:39,140 Each collision makes more asteroids. 885 01:06:39,141 --> 01:06:44,679 There's many different possibilities of what could happen when asteroids 886 01:06:44,680 --> 01:06:47,900 collide. Imagine a roller derby situation. 887 01:06:50,570 --> 01:06:55,169 You have two groups of players that run into each other. That could be like two 888 01:06:55,170 --> 01:06:56,910 asteroids running into each other. 889 01:06:57,190 --> 01:07:02,829 And one possible outcome is that one stays intact while the other is 890 01:07:02,830 --> 01:07:03,880 blown apart. 891 01:07:06,650 --> 01:07:09,900 That sends fragments flying all through the main asteroid belt. 892 01:07:09,901 --> 01:07:14,029 And then those little asteroid fragments are on their own independent orbits 893 01:07:14,030 --> 01:07:15,080 around the sun. 894 01:07:16,310 --> 01:07:20,350 A problem with asteroid impacts is that we're always making new asteroids. 895 01:07:20,351 --> 01:07:24,489 There are big asteroids out there, and they get hit by other asteroids, and you 896 01:07:24,490 --> 01:07:28,649 get shrapnel. And now you've got not one big one and one smaller one. You've got 897 01:07:28,650 --> 01:07:31,540 one big one, one smaller one, and millions of little ones. 898 01:07:31,541 --> 01:07:35,369 Now, most of these aren't very big, but some of them might be bigger and could 899 01:07:35,370 --> 01:07:36,690 be potentially hazardous. 900 01:07:38,050 --> 01:07:42,410 As the solar system ages, the number of asteroids increases. 901 01:07:43,250 --> 01:07:44,710 Each new space rock. 902 01:07:44,940 --> 01:07:48,800 travels on a new course, which could intersect with Earth. 903 01:07:49,820 --> 01:07:54,059 So we're constantly producing new asteroids and big collisions in the main 904 01:07:54,060 --> 01:07:54,919 asteroid belt. 905 01:07:54,920 --> 01:07:58,419 And these are producing the small asteroids that will eventually drift 906 01:07:58,420 --> 01:07:59,470 the solar system. 907 01:08:00,700 --> 01:08:06,379 Tracking this constantly evolving population of asteroids gives scientists 908 01:08:06,380 --> 01:08:07,430 huge headache. 909 01:08:07,880 --> 01:08:12,119 If they break apart, then that gives you even more pieces of the asteroid to 910 01:08:12,120 --> 01:08:14,340 track. It's not a simple thing. 911 01:08:14,640 --> 01:08:19,160 to track and predict the orbit of asteroids and their movements. 912 01:08:19,460 --> 01:08:25,759 Because one tiny little change can have huge dramatic 913 01:08:25,760 --> 01:08:28,920 impacts for its possible future. 914 01:08:28,921 --> 01:08:32,978 Figuring out exactly where they're going to go and keeping track of how they 915 01:08:32,979 --> 01:08:35,509 interact with each other, this is a huge endeavor. 916 01:08:36,560 --> 01:08:42,339 The sheer volume of asteroids can affect the behavior of other asteroids as they 917 01:08:42,340 --> 01:08:43,720 gravitationally interact. 918 01:08:44,620 --> 01:08:48,020 Think about your roller derby player, skating in circles. 919 01:08:48,021 --> 01:08:52,159 The path they're going to follow will evolve the more people you plop down on 920 01:08:52,160 --> 01:08:53,039 that track. 921 01:08:53,040 --> 01:08:56,770 They start interacting with each other and their trajectory will change. 922 01:08:57,979 --> 01:09:02,318 The more crowded you make the solar system, the more things there are to 923 01:09:02,319 --> 01:09:04,899 your orbit of your individual asteroid. 924 01:09:07,060 --> 01:09:11,339 It's not like air traffic control where there's a known amount of airplanes and 925 01:09:11,340 --> 01:09:12,420 they all follow a plan. 926 01:09:13,260 --> 01:09:19,299 This situation is further complicated because asteroid orbits can be affected 927 01:09:19,300 --> 01:09:21,120 other, more subtle forces. 928 01:09:22,640 --> 01:09:26,160 One of these is called the Yarkovsky, or the Yorp effect. 929 01:09:26,600 --> 01:09:28,700 Honestly, Yorp is more fun to say. 930 01:09:29,260 --> 01:09:33,580 The Yorp effect is caused by sunlight hitting an asteroid. 931 01:09:34,060 --> 01:09:38,339 Light is made up of photons that are traveling, and these photons actually 932 01:09:38,340 --> 01:09:42,560 momentum. So when light shines on something, it actually pushes on it. 933 01:09:44,910 --> 01:09:51,228 When sunlight hits an asteroid, the photons give it a tiny push, enough 934 01:09:51,229 --> 01:09:54,350 to change the space rock's trajectory. 935 01:10:04,710 --> 01:10:08,710 Asteroids can change course, which makes tracking them hard. 936 01:10:09,330 --> 01:10:12,890 Comets stay on course, but they are much harder to track. 937 01:10:16,620 --> 01:10:21,559 We track asteroids pretty regularly because they hang out in the inner solar 938 01:10:21,560 --> 01:10:24,400 system. We can look for any potential dangerous ones. 939 01:10:24,600 --> 01:10:29,639 The comets are a completely different story because they come in from random 940 01:10:29,640 --> 01:10:31,760 directions at random times. 941 01:10:32,000 --> 01:10:34,240 They are completely unpredictable. 942 01:10:36,280 --> 01:10:40,340 Which is why we've only detected a fraction of what's out there. 943 01:10:42,000 --> 01:10:46,280 There are millions and tens of millions of them. Guess how many we found? 944 01:10:46,560 --> 01:10:47,900 6 ,300. 945 01:10:48,460 --> 01:10:50,740 That means that we virtually found zero. 946 01:10:51,800 --> 01:10:57,739 The low number is because long -period comets spend much of their orbit over 10 947 01:10:57,740 --> 01:11:00,560 billion miles away, where they are invisible. 948 01:11:03,260 --> 01:11:07,290 The trouble with long -period comets is, of course, their periods are very long. 949 01:11:07,320 --> 01:11:11,879 And so we only see a small part of their arc. They go very distant into the 950 01:11:11,880 --> 01:11:12,930 solar system. 951 01:11:13,660 --> 01:11:17,799 And so it just makes them difficult to follow when they get a very long way 952 01:11:17,800 --> 01:11:20,379 the sun. We're not able to track their orbits anymore. 953 01:11:20,380 --> 01:11:22,700 And so it becomes a little bit more guesswork. 954 01:11:23,720 --> 01:11:27,919 We don't see them until they're already in the inner solar system, inside the 955 01:11:27,920 --> 01:11:28,970 orbit of Jupiter. 956 01:11:30,830 --> 01:11:36,869 We never really know about them until they've already started their passage 957 01:11:36,870 --> 01:11:40,749 really far away and started their dive into the solar system at really high 958 01:11:40,750 --> 01:11:45,150 velocity. We really only discover these comets at the very last minute. 959 01:11:46,290 --> 01:11:49,150 You could spot an asteroid 10, 15 years in advance. 960 01:11:49,410 --> 01:11:51,700 These comets, that's basically impossible. 961 01:11:51,830 --> 01:11:54,120 We may have a couple of years warning for them. 962 01:12:01,990 --> 01:12:07,650 When we know an asteroid is really heading our way, it's time to fight 963 01:12:08,290 --> 01:12:11,180 So we've got an asteroid that's headed at us. What do we do? 964 01:12:11,370 --> 01:12:12,590 Two main possibilities. 965 01:12:12,850 --> 01:12:17,049 We deflect it, we nudge it a little bit so it misses, or we blow it up, we 966 01:12:17,050 --> 01:12:19,220 destroy it. Which of those do you want to do? 967 01:12:19,221 --> 01:12:23,889 This is something where our science fiction ideas have gotten it almost 968 01:12:23,890 --> 01:12:28,950 wrong. If you're in a bad movie, a really, really bad movie, movie. 969 01:12:29,170 --> 01:12:34,369 You can send astronauts to an asteroid, put a nuclear bomb in it, and blow it up 970 01:12:34,370 --> 01:12:37,809 into lots of little bits that then burn up harmlessly in our atmosphere. 971 01:12:37,810 --> 01:12:39,490 Yeah, it doesn't work that way. 972 01:12:40,110 --> 01:12:43,210 Blowing up an asteroid would make the problem much worse. 973 01:12:43,470 --> 01:12:47,230 You're no longer dealing with just one marauding space rock. 974 01:12:47,770 --> 01:12:51,970 My issue with this is that you may have turned one problem into 50. 975 01:12:51,971 --> 01:12:56,009 Instead of one regular -sized asteroid, now you have a whole bunch of littler 976 01:12:56,010 --> 01:12:59,569 ones, and these may still hit the Earth and cause damage. And you know what? 977 01:12:59,570 --> 01:13:03,610 That's not much less fun than just having a single big asteroid. 978 01:13:03,830 --> 01:13:07,189 Now you've just taken all that devastation and spread it out for 979 01:13:07,190 --> 01:13:08,240 enjoy. 980 01:13:08,270 --> 01:13:13,029 The problem with using a nuclear device is that the products that rain down on 981 01:13:13,030 --> 01:13:14,770 Earth are now radioactive. 982 01:13:22,210 --> 01:13:27,909 If a dangerous asteroid is on its way, blowing up an asteroid would be a last 983 01:13:27,910 --> 01:13:33,710 resort. A less risky method is to deflect it off its collision course. 984 01:13:34,090 --> 01:13:40,710 A small nudge early enough can change an asteroid's trajectory away from Earth. 985 01:13:42,530 --> 01:13:47,189 You don't have to nudge it very much for it to miss, right? So head it straight 986 01:13:47,190 --> 01:13:50,789 at it, just touch it slightly. By the time it gets to Earth, it's way off 987 01:13:50,790 --> 01:13:51,840 course. 988 01:13:54,800 --> 01:14:00,559 NASA is investigating several techniques to change an asteroid's path, including 989 01:14:00,560 --> 01:14:02,140 a nuclear burst. 990 01:14:02,760 --> 01:14:09,419 In a nuclear burst, what we do is we don't actually hit it. We come up to it 991 01:14:09,420 --> 01:14:14,439 with the device on a spacecraft, and then the device would be detonated at a 992 01:14:14,440 --> 01:14:16,120 certain height above the surface. 993 01:14:17,090 --> 01:14:21,329 That heats up the surface of the asteroid, which vaporizes. You get 994 01:14:21,330 --> 01:14:25,729 rock or metal, which blasts off the surface, and that's how a rocket works. 995 01:14:25,730 --> 01:14:29,449 you blow up a bomb here, and it winds up pushing the asteroid in the other 996 01:14:29,450 --> 01:14:30,500 direction. 997 01:14:31,170 --> 01:14:36,569 To prevent any potential nuclear fallout, NASA would detonate the bomb a 998 01:14:36,570 --> 01:14:37,620 way from Earth. 999 01:14:39,509 --> 01:14:43,689 Any deflection attempt has to be done years in advance, which means it would 1000 01:14:43,690 --> 01:14:47,969 done on the other side of the solar system from us, on the opposite side of 1001 01:14:47,970 --> 01:14:48,889 object's orbit. 1002 01:14:48,890 --> 01:14:53,309 That means that all of the vapor made during the explosion gets blown away by 1003 01:14:53,310 --> 01:14:54,360 the solar wind. 1004 01:14:55,190 --> 01:15:00,729 NASA is also investigating other less explosive methods of deflecting an 1005 01:15:00,730 --> 01:15:01,780 asteroid. 1006 01:15:02,210 --> 01:15:05,330 D -STAR would blast the asteroid with a laser. 1007 01:15:05,770 --> 01:15:10,690 We hit it with the laser, material vaporizes and flies off the asteroid. 1008 01:15:10,691 --> 01:15:14,449 And because of Newton's third law, which is that for every action there's an 1009 01:15:14,450 --> 01:15:19,109 opposite and equal reaction, this means that vaporized material moving off in 1010 01:15:19,110 --> 01:15:22,190 one direction moves the asteroid in the opposite direction. 1011 01:15:24,430 --> 01:15:29,770 Both the laser and nuclear burst are still just ideas on the drawing board. 1012 01:15:31,730 --> 01:15:36,740 But one asteroid deflection mission... called Double Asteroid Redirection Test, 1013 01:15:36,940 --> 01:15:42,840 or DART for short, is already up and running and scheduled for launch in 1014 01:15:45,140 --> 01:15:50,400 DART is a kinetic impactor and will try to knock the asteroid off work. 1015 01:15:50,401 --> 01:15:55,959 At NASA, for the longest time, all we've been able to do is theorize about how 1016 01:15:55,960 --> 01:15:59,039 we changed their path. But now, for the first time, we're actually going to 1017 01:15:59,040 --> 01:16:00,090 practice it. 1018 01:16:00,429 --> 01:16:05,690 Leading this groundbreaking mission to bump an asteroid off its course is Dr. 1019 01:16:05,990 --> 01:16:07,040 Andy Chang. 1020 01:16:07,630 --> 01:16:12,809 DART is the first planetary defense mission that we've ever done, where we 1021 01:16:12,810 --> 01:16:19,049 a spacecraft, we fly the spacecraft into the asteroid to change its course and 1022 01:16:19,050 --> 01:16:20,130 make it miss the Earth. 1023 01:16:20,970 --> 01:16:27,389 DART's target is a 525 -foot space rod orbiting the large near -Earth asteroid 1024 01:16:27,390 --> 01:16:31,579 Didymus. We picked the near -Earth asteroid Didymos as a target for the 1025 01:16:31,580 --> 01:16:34,899 mission because although it's a near -Earth asteroid, it's one that's very 1026 01:16:34,900 --> 01:16:38,939 safely parked away out there in space. There's no way we can move Didymos or 1027 01:16:38,940 --> 01:16:41,830 moon in any way big enough to cause a problem for the Earth. 1028 01:16:49,340 --> 01:16:55,419 The Didymoon asteroid is moving at over 36 ,000 miles an hour and is over 4 1029 01:16:55,420 --> 01:16:56,760 million miles away. 1030 01:16:57,280 --> 01:17:02,020 So how do you move a 10 .5 billion pound space rock? 1031 01:17:03,560 --> 01:17:06,500 You need to hit it really hard to change its orbit. 1032 01:17:06,740 --> 01:17:12,119 So it's going to be coming in at a super high velocity in order to impart a 1033 01:17:12,120 --> 01:17:14,230 bunch of energy and momentum to that moon. 1034 01:17:15,580 --> 01:17:20,240 DART will hit the target at around 14 ,000 miles an hour. 1035 01:17:20,600 --> 01:17:22,200 The speed of the DART impact. 1036 01:17:23,050 --> 01:17:27,930 will be more than nine times the speed of the rifle bullet from AK -47. 1037 01:17:29,930 --> 01:17:33,430 The impact will give the asteroid a small push. 1038 01:17:33,670 --> 01:17:39,390 To work out how big a push, we test impacts with the Ames vertical gun. 1039 01:17:40,360 --> 01:17:44,319 At the NASA Ames Research Center in California, there's a very special 1040 01:17:44,320 --> 01:17:46,120 called the Ames Vertical Gun Range. 1041 01:17:46,440 --> 01:17:51,339 It's a hypervelocity gas gun that allows us to shoot little metal BBs at rock 1042 01:17:51,340 --> 01:17:55,920 targets at speeds up to like 13 ,000, 14 ,000 miles per hour. 1043 01:17:56,340 --> 01:18:00,020 The gun replicates the impact the DART mission will make. 1044 01:18:00,260 --> 01:18:05,559 It reveals that an impact will blow off a small amount of debris, but at an 1045 01:18:05,560 --> 01:18:09,060 extremely high speed, enough to get the asteroid. 1046 01:18:09,390 --> 01:18:10,810 An additional kick. 1047 01:18:11,250 --> 01:18:15,649 The impact will blow off pieces of the asteroid. So the pieces are thrown off 1048 01:18:15,650 --> 01:18:19,930 the back. And so that process acts like a little rocket engine. 1049 01:18:20,150 --> 01:18:24,689 That provides an additional momentum change, momentum push, to the target 1050 01:18:24,690 --> 01:18:25,740 itself. 1051 01:18:26,210 --> 01:18:30,630 The combined push from the kinetic impactor and the ejected debris is tiny, 1052 01:18:30,910 --> 01:18:33,990 around 9, 10 thousandths of a mile per hour. 1053 01:18:34,290 --> 01:18:38,130 But hopefully it's enough to change the asteroid's orbit. 1054 01:18:38,590 --> 01:18:44,169 If DART works, we could then use a similar mission to defend Earth when the 1055 01:18:44,170 --> 01:18:45,220 comes. 1056 01:18:45,690 --> 01:18:50,089 This isn't some small rock prototype that we're doing this test on. This is a 1057 01:18:50,090 --> 01:18:55,849 real dress rehearsal for an asteroid that could destroy cities or even maybe 1058 01:18:55,850 --> 01:18:56,990 send the Earth in chaos. 1059 01:18:57,790 --> 01:19:01,150 The moon of Didymus is a solid lump of rock. 1060 01:19:01,370 --> 01:19:06,389 Will a kinetic impactor like DART work with a rubble pile asteroid like a 1061 01:19:06,390 --> 01:19:10,019 Pophis? When you shoot a rubble pile with a projectile, it's a little bit 1062 01:19:10,020 --> 01:19:13,999 like trying to punch a sandbag. You get a lot more of the energy that's absorbed 1063 01:19:14,000 --> 01:19:17,760 into just moving the sand around inside the bag than ejecting it. 1064 01:19:18,000 --> 01:19:21,310 And so rubble piles might be a little harder to move by this method. 1065 01:19:23,180 --> 01:19:27,740 We don't know if we can deflect a rubble pile asteroid like Apophis. 1066 01:19:28,000 --> 01:19:33,640 They remain a clear and present danger and something we might not buy. 1067 01:19:40,620 --> 01:19:44,160 But there may be a space lifeboat. 1068 01:19:49,500 --> 01:19:56,339 In 2018, scientists re -examined rocks collected by Apollo 14 astronauts from 1069 01:19:56,340 --> 01:19:57,390 the moon. 1070 01:20:00,900 --> 01:20:04,900 Buried in the samples was a rock that shouldn't be there. 1071 01:20:06,879 --> 01:20:11,440 They got something they didn't expect, and that was an Earth rock. 1072 01:20:11,640 --> 01:20:15,600 They actually picked up a rock from Earth on the moon. 1073 01:20:15,820 --> 01:20:17,320 They didn't bring it with them. 1074 01:20:17,460 --> 01:20:21,399 It's very likely that it was something that was lofted up. When something hit 1075 01:20:21,400 --> 01:20:22,450 Earth, 1076 01:20:24,180 --> 01:20:29,279 threw up a bunch of rocks, some of those rocks fell onto the moon. And that's a 1077 01:20:29,280 --> 01:20:31,480 meteorite on the moon, but it's from Earth. 1078 01:20:36,940 --> 01:20:42,079 Supercomputer simulations of the KPG asteroid strike reveal how the impact 1079 01:20:42,080 --> 01:20:47,019 so much energy that it catapulted rocks out of Earth's atmosphere and into 1080 01:20:47,020 --> 01:20:53,019 space. They were then caught by the moon's gravity and pulled down to the 1081 01:20:53,020 --> 01:20:54,070 surface. 1082 01:20:55,160 --> 01:21:00,679 We now know that material ejected into space from asteroid impacts can travel 1083 01:21:00,680 --> 01:21:06,959 other planets as well, which would explain the 100 Mars meteorites. we 1084 01:21:06,960 --> 01:21:08,010 here on Earth. 1085 01:21:08,011 --> 01:21:14,459 We think that there was probably the exchange of a huge amount of material 1086 01:21:14,460 --> 01:21:18,200 between different bodies, Earth to the moon and back again into Mars. 1087 01:21:21,620 --> 01:21:25,799 With each impact that occurs in our solar system, that ejects all types of 1088 01:21:25,800 --> 01:21:30,220 material that allows material to swap from planet to planet, moon to planet, 1089 01:21:30,560 --> 01:21:34,859 moon to moon. And so there's all of this material that eventually travels from 1090 01:21:34,860 --> 01:21:35,910 place to place. 1091 01:21:36,589 --> 01:21:42,629 This planetary interchange may give life on Earth a lifeboat should another 1092 01:21:42,630 --> 01:21:44,590 giant asteroid hit our planet. 1093 01:21:45,590 --> 01:21:51,009 If you think about such an impact today, you know, the chances are high that a 1094 01:21:51,010 --> 01:21:54,790 lot of life will be wiped out. Much of life, probably all of human life. 1095 01:21:56,070 --> 01:22:00,249 It's certainly possible that a big enough asteroid strike can completely 1096 01:22:00,250 --> 01:22:01,350 sterilize a planet. 1097 01:22:01,570 --> 01:22:03,250 Talking about no life whatsoever. 1098 01:22:04,050 --> 01:22:08,109 Not to put too fine a point on it, but if there's a dinosaur killer asteroid 1099 01:22:08,110 --> 01:22:11,849 there and it hits the Earth, the chance of humanity's survival of such a thing 1100 01:22:11,850 --> 01:22:14,350 as a species, not great. 1101 01:22:19,250 --> 01:22:24,769 Humans may not survive, but some scientists believe some simple life 1102 01:22:24,770 --> 01:22:25,820 could. 1103 01:22:27,550 --> 01:22:33,609 If a giant rock hits the Earth and kills almost all life on Earth... There is a 1104 01:22:33,610 --> 01:22:40,469 slim line of hope. And that's because the dirt, the rocks on 1105 01:22:40,470 --> 01:22:45,570 Earth are infused with bacterial life, with microscopic life. 1106 01:22:45,850 --> 01:22:51,749 And in the event of a giant impact, some of these bits of rock will be ejected 1107 01:22:51,750 --> 01:22:52,699 into space. 1108 01:22:52,700 --> 01:22:57,699 and might float around. After an asteroid impact, whatever ejected into 1109 01:22:57,700 --> 01:23:01,979 atmosphere could contain microbial life that, when it falls back down onto the 1110 01:23:01,980 --> 01:23:04,600 ground, could reseed the life on that planet. 1111 01:23:08,140 --> 01:23:12,600 Some bacteria can survive the harsh conditions of space. 1112 01:23:13,060 --> 01:23:19,079 These creatures can cope with an asteroid strike, reentry, and landing 1113 01:23:19,080 --> 01:23:20,130 Earth's surface. 1114 01:23:29,900 --> 01:23:34,559 I think in terms of life on planet Earth, I think we've learned that we 1115 01:23:34,560 --> 01:23:36,000 a very resilient planet. 1116 01:23:36,240 --> 01:23:39,839 And I think life in some form, even if it has to crawl its way back from 1117 01:23:39,840 --> 01:23:44,160 bacterial stage, I think life on this planet is going to eke through. 1118 01:23:47,120 --> 01:23:50,320 Life is pretty good at figuring out a way of surviving. 1119 01:23:51,320 --> 01:23:53,580 We know that life first formed on the Earth. 1120 01:23:53,870 --> 01:23:58,910 well over 4 billion years ago, and has never been wiped out in all of that 1121 01:23:59,070 --> 01:24:02,610 There's always been something after every major mass extinction. 1122 01:24:02,850 --> 01:24:07,290 So life will continue. It just won't necessarily be us. 1123 01:24:08,550 --> 01:24:13,669 An asteroid strike on another world may be how life started on Earth in the 1124 01:24:13,670 --> 01:24:14,669 first place. 1125 01:24:14,670 --> 01:24:19,289 There's an interesting idea that an asteroid strike on another planet could 1126 01:24:19,290 --> 01:24:23,429 actually seeded life on Earth. And the way this works is you have life that's 1127 01:24:23,430 --> 01:24:27,789 somehow gotten a foothold on some other planet like Mars. A big asteroid strike 1128 01:24:27,790 --> 01:24:32,030 hits that planet and knocks a piece of it off, eventually rains down on Earth, 1129 01:24:32,250 --> 01:24:33,330 carrying with it life. 1130 01:24:35,590 --> 01:24:40,270 We may owe the existence of life here to asteroid impacts. 1131 01:24:44,090 --> 01:24:46,380 Speculative, but it's kind of a cool thought. 1132 01:24:48,590 --> 01:24:55,129 Life -seeding asteroids may have hit us in the past, and other asteroids will 1133 01:24:55,130 --> 01:24:56,180 hit us in the future. 1134 01:24:58,230 --> 01:25:03,710 One of them may be a pulpit, arriving in less than half a century. 1135 01:25:04,970 --> 01:25:06,750 Maybe we will deflect it. 1136 01:25:08,010 --> 01:25:11,050 Maybe it will miss us all on its own. 1137 01:25:12,130 --> 01:25:15,670 Either way, We need to keep tabs on it. 1138 01:25:15,671 --> 01:25:20,489 The best thing we can do as a species, and it's funny because it almost sounds 1139 01:25:20,490 --> 01:25:24,109 like I'm advocating for more jobs for astronomers, we need to keep looking at 1140 01:25:24,110 --> 01:25:24,629 the sky. 1141 01:25:24,630 --> 01:25:28,889 We need to look at the sky longer and deeper with more sensitive instruments 1142 01:25:28,890 --> 01:25:32,289 get more of a sense of what out there is around us. That's what our species 1143 01:25:32,290 --> 01:25:34,130 needs to do to ultimately survive. 1144 01:25:35,490 --> 01:25:40,129 Because now we have the ability to see these things a little bit better, we 1145 01:25:40,130 --> 01:25:43,329 the ability to protect ourselves better. It doesn't have to be a surprise. 1146 01:25:43,330 --> 01:25:46,509 You know, the first time we see a big impact doesn't have to be as it's 1147 01:25:46,510 --> 01:25:47,950 down, destroying our planet. 1148 01:25:48,070 --> 01:25:52,209 We can actually see it before it gets to us and decide what we want to do about 1149 01:25:52,210 --> 01:25:53,260 it. 1150 01:25:53,550 --> 01:25:56,630 Earth's history is littered with asteroid strikes. 1151 01:25:57,470 --> 01:26:00,130 Some wiped out millions of feces. 1152 01:26:00,990 --> 01:26:04,050 Some may have seeded life in the first place. 1153 01:26:04,490 --> 01:26:11,150 What the future holds in our relationship with these space rocks, no 1154 01:26:12,290 --> 01:26:17,109 Even though the chances of something really large hitting the Earth are 1155 01:26:17,110 --> 01:26:19,910 small, the consequences are dire. 1156 01:26:20,210 --> 01:26:24,510 It would really destroy our planet, or at least life as we understand it. 1157 01:26:24,910 --> 01:26:29,450 And so in many ways, asteroids are the greatest threat that we face. 1158 01:26:29,870 --> 01:26:31,250 Life is fragile. 1159 01:26:31,850 --> 01:26:35,669 So, of course, we live in a larger environment where something could come 1160 01:26:35,670 --> 01:26:36,720 hit us at any time. 1161 01:26:36,850 --> 01:26:38,210 That's part of being alive. 1162 01:26:38,470 --> 01:26:42,669 There's no guarantee tomorrow will happen. But what there is is a high 1163 01:26:42,670 --> 01:26:45,080 likelihood that you'll still be safe tomorrow. 1164 01:26:48,150 --> 01:26:50,110 Impacts from space are rare. 1165 01:26:50,610 --> 01:26:54,569 But if they do happen, it's a huge deal. And so you've got to put those two 1166 01:26:54,570 --> 01:26:55,529 things together. 1167 01:26:55,530 --> 01:26:57,390 That means we've got to pay attention. 1168 01:26:57,391 --> 01:27:01,829 Those impacts have happened many times in the past, and they're going to 1169 01:27:01,830 --> 01:27:04,060 continue to happen many times in the future. 1170 01:27:04,330 --> 01:27:07,220 Fortunately, it's not probably in our immediate future. 1171 01:27:07,650 --> 01:27:10,570 Impacts are rare, but the Earth lives a long time. 1172 01:27:11,950 --> 01:27:15,449 So you're unlikely to get in a car accident, but if you drive enough, 1173 01:27:15,450 --> 01:27:16,890 going to get in a car accident. 1174 01:27:20,130 --> 01:27:24,289 Over a century timescale, yes, we should be concerned about these. But over the 1175 01:27:24,290 --> 01:27:29,419 daily, weekly, monthly, even yearly timescale... I wouldn't sweat it too 1176 01:27:29,420 --> 01:27:33,559 wouldn't say we should lose sleep over an asteroid or comet striking Earth, but 1177 01:27:33,560 --> 01:27:35,880 the reality is it will happen again. 1178 01:27:39,450 --> 01:27:43,589 about asteroid strikes remember this wonderful dramatic universe you find 1179 01:27:43,590 --> 01:27:48,449 yourself in we're here because stars died and exploded life on earth wouldn't 1180 01:27:48,450 --> 01:27:52,109 the same if we didn't find ourselves in this dramatic and even dangerous 1181 01:27:52,110 --> 01:27:56,749 environment in space but this is who we are this is nothing new and this will 1182 01:27:56,750 --> 01:27:58,479 continue for the future of our planet 1183 01:27:58,480 --> 01:28:03,030 Repair and Synchronization by Easy Subtitles Synchronizer 1.0.0.0 112332

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