1 00:00:10,410 --> 00:00:11,311 I'm Nancy Szabo. 2 00:00:11,311 --> 00:00:14,581 I'm a planetary scientist at the Johns Hopkins Applied Physics Lab, 3 00:00:14,581 --> 00:00:18,551 and I'm the coordination lead on the DART mission. 4 00:00:23,223 --> 00:00:26,760 This mission is about NASA's purposely crashing a spacecraft 5 00:00:26,760 --> 00:00:31,398 into an asteroid as the first planetary defense test mission. 6 00:00:31,765 --> 00:00:35,101 That mission is DART, the double asteroid redirection test. 7 00:00:35,301 --> 00:00:37,771 T stands for test. That's very important here. 8 00:00:38,038 --> 00:00:39,472 This is not a threat to the earth. 9 00:00:39,472 --> 00:00:41,107 This asteroid is not a threat to the earth. 10 00:00:41,107 --> 00:00:43,443 And the DART test won't make it a threat to the earth. 11 00:00:43,443 --> 00:00:46,980 But we want to take the steps to develop technologies to potentially prevent 12 00:00:46,980 --> 00:00:50,083 asteroids from hitting the earth in the future if we needed to. 13 00:00:50,383 --> 00:00:52,786 So the DART spacecraft is going to come speeding in, 14 00:00:52,952 --> 00:00:56,256 hit this asteroid, and it's going to change that motion of that 15 00:00:56,256 --> 00:01:00,693 asteroid ever so slightly in space changing its future path. 16 00:01:01,094 --> 00:01:04,597 This is one technique that you might use to change the path of an asteroid 17 00:01:04,597 --> 00:01:08,134 if one was ever found to be a threat to the earth in the future. 18 00:01:08,501 --> 00:01:12,439 And we're doing this test now before we need it. 19 00:01:18,244 --> 00:01:19,079 This asteroid 20 00:01:19,079 --> 00:01:22,382 is the ideal target for this first planetary defense test mission. 21 00:01:22,916 --> 00:01:24,284 And because it's to asteroids 22 00:01:24,284 --> 00:01:27,420 like the name of the mission says, it's a double asteroid out there. 23 00:01:27,587 --> 00:01:31,091 There's a larger asteroid titmouse and there's the little moonlit asteroid. 24 00:01:31,091 --> 00:01:32,926 The folks that goes around it. 25 00:01:32,926 --> 00:01:36,663 So Dart is going to slam into that small asteroid to more focus 26 00:01:36,930 --> 00:01:40,567 and measure asteroid deflection within this asteroid system. 27 00:01:40,800 --> 00:01:42,001 This makes it a really safe 28 00:01:42,001 --> 00:01:43,903 way to do this test where we're just deflecting 29 00:01:43,903 --> 00:01:46,773 how a small moon asteroid goes around a larger asteroid 30 00:01:46,973 --> 00:01:50,243 with no measurable change about how this asteroid goes around the sun. 31 00:01:50,677 --> 00:01:53,880 But it also lets us use telescopes here on the earth 32 00:01:54,080 --> 00:01:56,049 in order to measure that deflection. 33 00:01:56,049 --> 00:01:58,418 So it allows the DART spacecraft to be very focused, 34 00:01:58,618 --> 00:02:01,621 but then use these telescopes that discover this asteroid system 35 00:02:01,621 --> 00:02:06,726 and have been studying it for years to figure out how much we moved it. 36 00:02:11,331 --> 00:02:13,433 So the asteroid that it's colliding with the DART 37 00:02:13,433 --> 00:02:17,704 spacecraft will collide with the Morpho is about 160 meters in diameter. 38 00:02:17,704 --> 00:02:20,006 It's a less than two football fields in length, 39 00:02:20,640 --> 00:02:23,343 and it goes around one that's about half a mile in diameter. 40 00:02:23,643 --> 00:02:26,446 But really, asteroids that are the size of dynamos 41 00:02:26,446 --> 00:02:30,016 we found the large majority of that population, and none of those 42 00:02:30,016 --> 00:02:34,320 asteroids at that larger size are a threat to the Earth for the foreseeable future. 43 00:02:34,721 --> 00:02:38,424 Now, there are no known asteroid threats that are a threat to the Earth 44 00:02:38,424 --> 00:02:39,926 for the foreseeable future. 45 00:02:39,926 --> 00:02:41,127 But the size of the more folks, 46 00:02:41,127 --> 00:02:45,265 we actually have found less than 50% of that asteroid population. 47 00:02:45,598 --> 00:02:49,135 And so along with finding all of these asteroids, figuring out where they are 48 00:02:49,135 --> 00:02:53,039 and keeping track of them, we want to take steps to be ready in case 49 00:02:53,039 --> 00:02:55,241 we need to in case we need to protect the earth 50 00:02:55,475 --> 00:02:58,578 from an asteroid, impact the size of something like tomatoes. 51 00:02:58,778 --> 00:03:01,614 And so this target asteroid is really the ideal way 52 00:03:01,614 --> 00:03:10,523 to do this first test, 53 00:03:10,523 --> 00:03:14,294 the way that you would use technology like this in the future, if you needed to 54 00:03:14,294 --> 00:03:17,830 if you needed to deflect an asteroid that was on the course with the Earth 55 00:03:18,131 --> 00:03:21,901 is not the Hollywood blockbuster last minute kind of scenario. 56 00:03:21,901 --> 00:03:24,137 It's something that you need to do years in advance. 57 00:03:24,571 --> 00:03:27,974 And so you would do this five, ten, 15, 20 years in advance. 58 00:03:27,974 --> 00:03:32,378 A small nudge adds up to a big change in position over that time. 59 00:03:32,378 --> 00:03:35,381 And that's why you need this warning time, which is why DART is just 60 00:03:35,381 --> 00:03:38,251 one part of a larger planetary defense strategy. 61 00:03:38,451 --> 00:03:41,254 Planetary defense is not just about deflecting asteroids. 62 00:03:41,254 --> 00:03:44,190 You can't do anything about the asteroids if you don't know where they are. 63 00:03:44,490 --> 00:03:48,494 So Planetary Defense, really Key Foundation is finding the asteroids, 64 00:03:48,494 --> 00:03:52,632 characterizing them, assessing them, and then taking steps to potentially 65 00:03:52,632 --> 00:03:56,836 prevent these natural disasters in the future. 66 00:04:01,774 --> 00:04:04,244 I am excited about everything about this mission. 67 00:04:04,577 --> 00:04:07,680 We've been working on this here at the Johns Hopkins Applied Physics Lab 68 00:04:07,847 --> 00:04:11,184 since 2015, and literally thousands of people 69 00:04:11,184 --> 00:04:13,620 have contributed to this to get us to this moment. 70 00:04:14,187 --> 00:04:17,490 From the people who developed and designed it, built the spacecraft. 71 00:04:17,624 --> 00:04:19,325 Our partners across the country, 72 00:04:19,325 --> 00:04:21,094 those who have been operating the spacecraft 73 00:04:21,094 --> 00:04:24,931 for the last ten months in space, over 200,000 images 74 00:04:24,931 --> 00:04:28,034 taken already to calibrate that spacecraft know what's going to happen. 75 00:04:28,301 --> 00:04:31,271 Telescopes around the world on all seven continents 76 00:04:31,471 --> 00:04:34,474 and in space, everybody's ready for this moment. 77 00:04:34,474 --> 00:04:45,151 And I'm excited about it finally being here. 78 00:04:45,285 --> 00:04:48,421 Well, certainly before the collision, actually, we're going to get 79 00:04:48,421 --> 00:04:52,358 some spectacular extreme close ups of the asteroid to our foes. 80 00:04:52,558 --> 00:04:55,161 And I'm really looking forward to this moment personally 81 00:04:55,261 --> 00:04:57,930 where we'll see what this asteroid looks like for the first time. 82 00:04:58,197 --> 00:05:01,968 So these images will be taken by the DART spacecraft every second 83 00:05:02,168 --> 00:05:05,104 as that spacecraft streams towards this asteroid 84 00:05:05,104 --> 00:05:07,874 at 14,000 miles per hour. 85 00:05:08,141 --> 00:05:09,942 These images will come back here to Earth. 86 00:05:09,942 --> 00:05:12,645 And when they make it to the mission operations center here at the Johns 87 00:05:12,645 --> 00:05:16,983 Hopkins Applied Physics Lab, they'll be broadcast live on NASA TV, 88 00:05:17,183 --> 00:05:20,787 where the whole world can see this data at the same time that the team is. 89 00:05:21,120 --> 00:05:23,256 And so this will be really spectacular 90 00:05:23,256 --> 00:05:27,026 and tell the final moments and the story of the DART spacecraft. 91 00:05:27,560 --> 00:05:30,063 But this obviously won't tell us how much we deflected the asteroid 92 00:05:30,063 --> 00:05:32,598 because the DART spacecraft will be totally destroyed at this point. 93 00:05:32,865 --> 00:05:35,401 We're going to use the telescopes here on the earth in order to do that. 94 00:05:35,601 --> 00:05:39,872 And telescopes across the across the world on all seven continents 95 00:05:39,872 --> 00:05:43,209 and in space are being used to help characterize and make this measurement. 96 00:05:43,443 --> 00:05:46,846 This will take a few days and weeks in order to really come up with that. 97 00:05:46,846 --> 00:05:52,352 But we're ready to have this next stage of the mission begin. 98 00:05:58,157 --> 00:06:00,960 So Dart's companion, CubeSat is called the Feature Cube. 99 00:06:00,993 --> 00:06:04,030 It's the light Italian CubeSat for imaging of asteroids. 100 00:06:04,330 --> 00:06:08,301 It's contributed by the Italian space agency, and it has two cameras on it. 101 00:06:08,568 --> 00:06:12,538 And so what this CubeSat is going to do, it was actually deployed an ejected 102 00:06:12,538 --> 00:06:15,608 successfully from the DART spacecraft about two weeks ago 103 00:06:15,775 --> 00:06:18,978 and it's been operating on its own in space ever since then. 104 00:06:19,212 --> 00:06:23,516 It's going to take direct images of Dart's collision into the asteroid 105 00:06:23,649 --> 00:06:28,321 and then fly by that asteroid its closest 3 minutes after Dart's collision. 106 00:06:28,321 --> 00:06:29,922 Taking even more images. 107 00:06:29,922 --> 00:06:33,793 Now, it'll store all those images on board and then send it back after its 108 00:06:33,793 --> 00:06:34,727 flyby is over. 109 00:06:34,727 --> 00:06:36,929 So we'll have to wait days to see what it finds. 110 00:06:37,463 --> 00:06:40,666 But we're so excited to have this international collaboration on DART 111 00:06:41,000 --> 00:06:44,670 for this first planetary defense test mission, because planetary defense 112 00:06:44,670 --> 00:06:48,141 is really an international issue. 113 00:06:53,246 --> 00:06:55,448 Well, here at APL, like you might imagine, 114 00:06:55,448 --> 00:06:59,118 there's a lot of excitement building and there's a lot of activities going on. 115 00:06:59,819 --> 00:07:02,622 The Mission Operations Center is extremely busy 116 00:07:03,156 --> 00:07:04,791 and so they will all be there. 117 00:07:04,791 --> 00:07:08,094 And one of the main challenges actually for this mission is hitting 118 00:07:08,094 --> 00:07:12,932 a small asteroid in space that you have limited information about at high speed. 119 00:07:13,399 --> 00:07:17,170 In order to do that, the spacecraft actually will autonomously 120 00:07:17,170 --> 00:07:20,773 guide itself during the last 4 hours of the mission. 121 00:07:21,040 --> 00:07:23,876 And so that's all getting prepared, prepared for that, 122 00:07:24,076 --> 00:07:25,411 where we have to make sure 123 00:07:25,411 --> 00:07:28,915 the spacecraft is where it needs to be and then put on this autopilot and it will 124 00:07:29,215 --> 00:07:31,551 distinguish between these asteroids and bring itself in. 125 00:07:32,151 --> 00:07:36,222 We're really welcoming people in order to focus guests here at APL. 126 00:07:36,222 --> 00:07:39,559 But really the world to join and watch this event live 127 00:07:39,559 --> 00:07:48,734 when it's shown on NASA TV. 128 00:07:49,135 --> 00:07:50,203 So in order to figure out 129 00:07:50,203 --> 00:07:53,940 asteroid deflection, how much Dart's collision deflected the asteroid. 130 00:07:53,973 --> 00:07:57,176 We have telescopes across the planet and in space. 131 00:07:57,176 --> 00:07:58,010 This includes 132 00:07:58,010 --> 00:08:02,081 Hubble, this includes GWC, and it includes the Lucy spacecraft as well. 133 00:08:02,348 --> 00:08:03,783 They're going to be looking 134 00:08:03,783 --> 00:08:06,986 not just for how much deflection, but how much ejecta is thrown up. 135 00:08:07,153 --> 00:08:09,388 So when dart collides with this rocky asteroid, it's 136 00:08:09,388 --> 00:08:11,557 going to pulverize a bunch of rock and material 137 00:08:11,557 --> 00:08:14,293 and it's going to throw it up away from the asteroid. 138 00:08:14,494 --> 00:08:17,363 And this will result in the system getting a little brighter. 139 00:08:17,363 --> 00:08:18,130 And the telescopes 140 00:08:18,130 --> 00:08:21,000 are going to be looking, trying to capture that, characterize that. 141 00:08:21,367 --> 00:08:25,204 And it's really so great to have all of these facilities coming together 142 00:08:25,204 --> 00:08:32,044 to maximize what we learn from this first planetary defense test mission. 143 00:08:35,748 --> 00:08:37,450 Will So we 144 00:08:37,450 --> 00:08:40,953 know from other asteroids that have been visited by other missions 145 00:08:40,953 --> 00:08:44,991 that these are complicated things that are not just giant shards of rock out there 146 00:08:44,991 --> 00:08:45,525 in space. 147 00:08:45,525 --> 00:08:49,495 Those cirrus MCs Rex mission found that it was a pile of gravel 148 00:08:49,495 --> 00:08:52,698 loosely bound together in this very low gravity environment. 149 00:08:52,698 --> 00:08:55,868 And when they went to sample it, it went further into the asteroid 150 00:08:55,902 --> 00:08:58,437 than maybe people were initially expecting. 151 00:08:59,472 --> 00:09:01,140 We've never seen two more folks before. 152 00:09:01,140 --> 00:09:05,177 And in fact, it's going to be the smallest asteroid ever visited by a spacecraft. 153 00:09:05,211 --> 00:09:07,680 What is it, its internal structure? How strong is it? 154 00:09:07,947 --> 00:09:10,750 These are important components for planetary defense. 155 00:09:10,783 --> 00:09:13,853 If you wanted to protect the earth from an asteroid like this. 156 00:09:14,086 --> 00:09:17,223 And that's also why we need to do dart doing this full scale 157 00:09:17,223 --> 00:09:20,893 asteroid deflection test on an asteroid of the relevant size 158 00:09:21,160 --> 00:09:24,597 to see how that asteroid reacts to this kinetic impactor collision. 159 00:09:24,864 --> 00:09:27,166 So we've learned a lot from those other asteroid missions, 160 00:09:27,166 --> 00:09:28,601 and we're going to learn even more from DART.