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These are the user uploaded subtitles that are being translated: 1 00:00:00,960 --> 00:00:02,920 - [Narrator] The building blocks of the solar system 2 00:00:02,920 --> 00:00:05,420 are quickly giving up their secrets. 3 00:00:05,420 --> 00:00:07,560 Two major missions are on their way. 4 00:00:07,560 --> 00:00:09,210 The NASA OSIRUS REx, 5 00:00:09,210 --> 00:00:12,540 which is now closing in on its target asteroid, Bennu, 6 00:00:12,540 --> 00:00:15,940 and the JAXA mission, Hyabusa 2 to Ryugu, 7 00:00:15,940 --> 00:00:18,710 which is well into it's observation leg of the mission, 8 00:00:18,710 --> 00:00:21,340 studying the asteroid up close. 9 00:00:21,340 --> 00:00:23,657 Both missions hope to return samples to earth 10 00:00:23,657 --> 00:00:25,824 for a more complete study. 11 00:00:26,916 --> 00:00:29,749 (computer noises) 12 00:00:30,759 --> 00:00:34,426 (intense orchestral music) 13 00:01:04,240 --> 00:01:07,550 A three and a half year journey to asteroid Ryugu is over, 14 00:01:07,550 --> 00:01:10,924 and the Hyabusa 2 science mission begins. 15 00:01:10,924 --> 00:01:12,980 Ryugu, part of the Apollo group, 16 00:01:12,980 --> 00:01:16,720 is potentially a threat to earth in the years to come. 17 00:01:16,720 --> 00:01:19,710 It's an unusual asteroid, a CG type, 18 00:01:19,710 --> 00:01:20,870 meaning it has qualities 19 00:01:20,870 --> 00:01:24,910 of both C type and G type carbonaceous asteroids. 20 00:01:24,910 --> 00:01:28,813 It is just under a kilometer in diameter and fast-moving. 21 00:01:29,680 --> 00:01:30,960 As part of its payload, 22 00:01:30,960 --> 00:01:34,120 the Hybusa 2 has several deployable landers. 23 00:01:34,120 --> 00:01:37,490 Two MINERVA II's, the Franco-German Mascot lander, 24 00:01:37,490 --> 00:01:40,450 and target acquisition markers for the touchdown. 25 00:01:40,450 --> 00:01:42,240 - Okay, we want to see the boulders, 26 00:01:42,240 --> 00:01:43,780 we have a chance to view the boulders 27 00:01:43,780 --> 00:01:45,432 in a vertical structure. 28 00:01:45,432 --> 00:01:47,304 We also see the crack in the boulders, 29 00:01:47,304 --> 00:01:49,730 there is also regulate. 30 00:01:49,730 --> 00:01:52,780 We know from the spectral information we have so far 31 00:01:52,780 --> 00:01:55,260 that there is something a little bit redder, 32 00:01:55,260 --> 00:01:57,600 something a little bit bluer on the surface, 33 00:01:57,600 --> 00:01:58,920 so that's very interesting. 34 00:01:58,920 --> 00:02:01,510 Because there are differences on the surface, 35 00:02:01,510 --> 00:02:03,000 we have the feeling that the bluer, 36 00:02:03,000 --> 00:02:05,780 it may be a little bit fresher than the redder. 37 00:02:05,780 --> 00:02:10,780 And that basically gives us a good idea of the history 38 00:02:12,480 --> 00:02:14,930 of the material on the surface. 39 00:02:14,930 --> 00:02:19,023 And of course there are a number of landing sites, 40 00:02:19,023 --> 00:02:21,070 which are red and blue, 41 00:02:21,070 --> 00:02:23,190 or which have red and blue in it, 42 00:02:23,190 --> 00:02:25,930 and that's probably preferred, at least for the camera, 43 00:02:25,930 --> 00:02:29,150 so we have chance to see both of the surfaces. 44 00:02:29,150 --> 00:02:31,780 - From the feedback I have obtained now 45 00:02:31,780 --> 00:02:36,780 from our principle investigators of the instruments, 46 00:02:37,130 --> 00:02:40,270 seems to be that it's a very interesting asteroid. 47 00:02:40,270 --> 00:02:43,260 And that there are several aspects 48 00:02:43,260 --> 00:02:48,260 which is covering the science objective of each instrument. 49 00:02:51,610 --> 00:02:53,430 - [Narrator] First to be deployed to the asteroid 50 00:02:53,430 --> 00:02:55,173 were two MINERVA probes. 51 00:02:58,540 --> 00:03:01,140 These rovers are based on the original MINERVA craft 52 00:03:01,140 --> 00:03:02,713 flown on Hyabusa 1, 53 00:03:04,560 --> 00:03:08,340 which unfortunately failed to land on their target asteroid. 54 00:03:08,340 --> 00:03:10,423 These ones, however, were successful. 55 00:03:19,510 --> 00:03:22,400 They have radioed back several stunning photographs 56 00:03:22,400 --> 00:03:24,330 from the surface of the asteroid, 57 00:03:24,330 --> 00:03:27,850 including this sequence of the sun crossing the skyline 58 00:03:27,850 --> 00:03:29,573 as the asteroid tumbles. 59 00:03:38,600 --> 00:03:43,600 - Asteroid missions are very important and very interesting 60 00:03:43,620 --> 00:03:45,700 from the scientific point of view 61 00:03:45,700 --> 00:03:50,700 because it is believed that asteroid and comets 62 00:03:50,811 --> 00:03:54,380 are bringing water to the earth 63 00:03:54,380 --> 00:03:59,030 in the very early phase of the development of the earth. 64 00:03:59,030 --> 00:04:03,380 And with this water and also organic materials, 65 00:04:03,380 --> 00:04:08,380 it is believed that life on earth has developed 66 00:04:10,180 --> 00:04:12,150 and very importantly, 67 00:04:12,150 --> 00:04:17,150 is also to understand the evolution of the solar system, 68 00:04:18,030 --> 00:04:21,160 because asteroid are supposed to be building blocks 69 00:04:21,160 --> 00:04:23,453 of our early solar system. 70 00:04:28,602 --> 00:04:31,670 - The Hyabusa 2 mission has been years in the making. 71 00:04:31,670 --> 00:04:33,320 As with any deep space probe, 72 00:04:33,320 --> 00:04:35,210 years are spent on the drawing board 73 00:04:35,210 --> 00:04:37,810 developing the hardware and software. 74 00:04:37,810 --> 00:04:41,563 Then come years of construction and extensive testing. 75 00:04:47,680 --> 00:04:49,490 The aim of the Hyabusa 2 mission 76 00:04:49,490 --> 00:04:52,160 is to learn more about the origin and evolution 77 00:04:52,160 --> 00:04:54,170 of the solar system. 78 00:04:54,170 --> 00:04:55,510 As asteroids account 79 00:04:55,510 --> 00:04:58,330 for some of the most primordial celestial bodies, 80 00:04:58,330 --> 00:05:01,700 researching them gives us a glimpse into our cosmic past. 81 00:05:08,620 --> 00:05:10,210 Scientists are keen to learn more 82 00:05:10,210 --> 00:05:13,348 about the properties and structure of near earth asteroids 83 00:05:13,348 --> 00:05:15,470 in order to gain new insights 84 00:05:15,470 --> 00:05:17,830 into how our solar system formed, 85 00:05:17,830 --> 00:05:21,210 and how water and life emerged on earth. 86 00:05:21,210 --> 00:05:22,913 It's an audacious mission. 87 00:05:28,260 --> 00:05:33,020 - I mean, they're flying to an asteroid, 88 00:05:33,020 --> 00:05:38,000 now we map the asteroid, then a lander will be deployed, 89 00:05:38,000 --> 00:05:39,470 like Mascot or MINERVA. 90 00:05:39,470 --> 00:05:41,480 They're trying to do three samples 91 00:05:41,480 --> 00:05:44,880 and then they have also explosives on board 92 00:05:44,880 --> 00:05:48,500 to produce a crater on the surface in the asteroid. 93 00:05:48,500 --> 00:05:51,530 I mean, to me it's a unique mission they are doing, 94 00:05:51,530 --> 00:05:54,763 and we are a part of it, so I'm really proud of it. 95 00:05:54,763 --> 00:05:58,160 - And, of course, we are interested in the geology, 96 00:05:58,160 --> 00:06:01,300 the geomorphology, the structure, 97 00:06:01,300 --> 00:06:03,828 the size of the big boulders, 98 00:06:03,828 --> 00:06:07,530 and also the structure of the regulate, 99 00:06:07,530 --> 00:06:12,530 and giving some hints of the evolution of the surface, 100 00:06:14,820 --> 00:06:18,563 of the forming and evolution of the surface of Ryugu. 101 00:06:19,962 --> 00:06:21,110 And I think for a camera, 102 00:06:21,110 --> 00:06:23,980 all of the landing sites are quite okay. 103 00:06:23,980 --> 00:06:26,566 So the most interesting thing is to see the big boulders 104 00:06:26,566 --> 00:06:28,490 from the vertical structure. 105 00:06:28,490 --> 00:06:32,453 We really can look how deep they are in the surface, 106 00:06:34,320 --> 00:06:36,230 and there are many boulders on Ryugu, 107 00:06:36,230 --> 00:06:38,316 so I'm pretty sure we'll get a good view 108 00:06:38,316 --> 00:06:41,723 of this interesting part of this asteroid. 109 00:06:43,031 --> 00:06:46,281 (intense string music) 110 00:06:52,040 --> 00:06:54,050 - [Narrator] The second batch of asteroid landers, 111 00:06:54,050 --> 00:06:57,260 developed by the German and French space organizations, 112 00:06:57,260 --> 00:06:59,860 were launched and after a short free fall, 113 00:06:59,860 --> 00:07:02,270 successfully landed at the southern hemisphere 114 00:07:02,270 --> 00:07:04,000 of asteroid Ryugu. 115 00:07:04,000 --> 00:07:07,540 After bouncing several times on the rock strewn surface, 116 00:07:07,540 --> 00:07:10,563 the two landers have begun their scientific research. 117 00:07:11,640 --> 00:07:15,502 - And you know that Mascot is made to bounce. 118 00:07:15,502 --> 00:07:17,280 That makes it robust, 119 00:07:17,280 --> 00:07:21,260 but it also means that the final resting location 120 00:07:21,260 --> 00:07:25,560 is not exactly possible to calculate it. 121 00:07:25,560 --> 00:07:27,870 So there's a dispersion of possible sites 122 00:07:27,870 --> 00:07:30,700 and there are some variation in between. 123 00:07:30,700 --> 00:07:33,760 There could be, among these many, many possibilities, 124 00:07:33,760 --> 00:07:37,210 some bad ones, and we have to go to places 125 00:07:37,210 --> 00:07:39,580 where the chance to hit a good one is highest, 126 00:07:39,580 --> 00:07:44,090 but it does exclude that we end up in a bad one. 127 00:07:44,090 --> 00:07:45,680 - Autonomous handling doesn't mean 128 00:07:45,680 --> 00:07:49,511 that Mascot is doing everything as he likes to, 129 00:07:49,511 --> 00:07:54,511 so there is lots of sequences and commands that's behind, 130 00:07:54,710 --> 00:07:56,610 which are carefully tested and planned. 131 00:07:56,610 --> 00:08:00,310 So the robustness of these sequences have to be tested 132 00:08:00,310 --> 00:08:03,460 against all these difficult, different conditions 133 00:08:03,460 --> 00:08:05,160 we can meet on the asteroid. 134 00:08:05,160 --> 00:08:08,500 So if we bounce or land more in the west or more in the east 135 00:08:10,300 --> 00:08:12,610 for this the input Mascot has, 136 00:08:12,610 --> 00:08:16,110 which he uses for his autonomously, 137 00:08:16,110 --> 00:08:18,570 this is really carefully planned and tested. 138 00:08:18,570 --> 00:08:19,840 And so there's all the work, 139 00:08:19,840 --> 00:08:24,263 and I think we did a very well job, and so I'm relaxed. 140 00:08:27,350 --> 00:08:29,160 - [Narrator] With it's four instruments, 141 00:08:29,160 --> 00:08:31,240 including the Micro-Mica spectrometer, 142 00:08:31,240 --> 00:08:35,460 developed by the IAS Space Astrophysics Institute at Oxate, 143 00:08:35,460 --> 00:08:37,600 with CNES oversight, 144 00:08:37,600 --> 00:08:40,810 Mascot is set to analyze the mineral composition of grains 145 00:08:40,810 --> 00:08:44,680 in the asteroid's soil in an attempt to unlock its secrets 146 00:08:44,680 --> 00:08:47,800 at two sites just a few meters apart. 147 00:08:47,800 --> 00:08:50,133 They also took some fascinating images. 148 00:08:53,750 --> 00:08:57,050 - I think, at least for me, the most important question 149 00:08:57,050 --> 00:08:59,710 is the big number of boulders. 150 00:08:59,710 --> 00:09:01,350 Where did they come from? 151 00:09:01,350 --> 00:09:04,120 Why has this asteroid so many boulders? 152 00:09:04,120 --> 00:09:07,793 Why are these boulders, to some extent, 153 00:09:08,944 --> 00:09:13,053 covered by the surface, so they are in the sub-surface? 154 00:09:15,110 --> 00:09:16,643 And the question here is, 155 00:09:18,180 --> 00:09:21,400 what are the source of the boulders? 156 00:09:21,400 --> 00:09:25,210 Are they from the interior or coming from outside, 157 00:09:25,210 --> 00:09:27,880 or they are linked from some kind of condition 158 00:09:27,880 --> 00:09:32,880 from bigger body where Ryugu is now a related part of it? 159 00:09:35,090 --> 00:09:38,543 So, I think that's the most important question. 160 00:09:43,330 --> 00:09:46,210 - Mascot was operational for over 17 hours, 161 00:09:46,210 --> 00:09:49,220 during which it collected data from the asteroid's surface 162 00:09:49,220 --> 00:09:52,430 and transmitted it back to Hyabusa 2 overhead, 163 00:09:52,430 --> 00:09:54,683 which relayed the data back to earth. 164 00:10:04,000 --> 00:10:07,360 The next probe to be released is the third MINERVA robot, 165 00:10:07,360 --> 00:10:09,400 the largest of the MINERVA's. 166 00:10:18,020 --> 00:10:23,020 - I would like just to express again this amazing work, 167 00:10:24,820 --> 00:10:27,433 which the whole team has done. 168 00:10:28,443 --> 00:10:33,443 DLR, as well as CNES, as well as JAXA surely. 169 00:10:33,640 --> 00:10:38,640 So, this was a very good example of very good collaboration 170 00:10:40,500 --> 00:10:42,480 on an international level, 171 00:10:42,480 --> 00:10:46,820 and I hope that it will go on in the future. 172 00:10:46,820 --> 00:10:51,190 - GNC that has to tell your autonomy manager, 173 00:10:51,190 --> 00:10:55,530 the right side or which side we should turn to upright. 174 00:10:58,020 --> 00:10:58,940 - [Narrator] The entire mission 175 00:10:58,940 --> 00:11:01,840 has been a close collaboration between nations. 176 00:11:01,840 --> 00:11:04,870 Japanese, German, and French scientists and engineers 177 00:11:04,870 --> 00:11:07,920 have enjoyed over a decade of scientific cooperation, 178 00:11:07,920 --> 00:11:10,850 even if there are language barriers. 179 00:11:10,850 --> 00:11:14,610 (foreign language spoken) 180 00:11:14,610 --> 00:11:15,443 - I like this because 181 00:11:15,443 --> 00:11:18,530 it's a small mission with little overhead. 182 00:11:18,530 --> 00:11:23,230 And it's very nice to work with the Japanese, 183 00:11:23,230 --> 00:11:26,360 because they are very success oriented, 184 00:11:29,420 --> 00:11:32,140 they are willing to take risks, 185 00:11:32,140 --> 00:11:35,460 they have also, because of language issues, 186 00:11:35,460 --> 00:11:39,380 much less paperwork than NASA or ESA does. 187 00:11:39,380 --> 00:11:42,050 So most things are done in discussions, 188 00:11:42,050 --> 00:11:44,350 and you agree on something, you look into your eyes 189 00:11:44,350 --> 00:11:48,120 and say yes we do it, yes, and you rely on the words. 190 00:11:48,120 --> 00:11:52,310 You don't sign big papers, and that's something I like, 191 00:11:52,310 --> 00:11:56,340 because it makes work so much easier and smooth and quick. 192 00:11:56,340 --> 00:11:58,690 - [Raf] Oh yes, the mission is very good. 193 00:11:58,690 --> 00:12:02,540 There are in all the teams from Hyabusa Mascot, 194 00:12:02,540 --> 00:12:05,280 there are very excellent engineers 195 00:12:05,280 --> 00:12:06,960 and also very excellent scientists, 196 00:12:06,960 --> 00:12:10,620 so I'm really, really confident and excited. 197 00:12:10,620 --> 00:12:12,963 And that's the first time we do this. 198 00:12:13,820 --> 00:12:16,921 - [Tra] The Hyabusa 2 mission is very interesting 199 00:12:16,921 --> 00:12:18,870 from the point of view 200 00:12:18,870 --> 00:12:23,110 because Hyabusa 2 is investigating a C type asteroid. 201 00:12:23,110 --> 00:12:25,940 Ryugu is a very primitive asteroid, 202 00:12:25,940 --> 00:12:30,940 which is supposed to have organic material on the surface. 203 00:12:31,260 --> 00:12:35,277 In addition, Hyabusa 2 has got in situ signs 204 00:12:35,277 --> 00:12:37,610 provided by the Mascot lander, 205 00:12:37,610 --> 00:12:42,110 and also two to three further small MINERVA landers, 206 00:12:42,110 --> 00:12:47,050 and it is, or it will bring some samples back to earth, 207 00:12:47,050 --> 00:12:50,183 so that we can investigate it then on earth in the labs. 208 00:12:52,221 --> 00:12:55,471 (intense string music) 209 00:13:04,209 --> 00:13:06,210 - [Narrator] In the spirit of friendly competition, 210 00:13:06,210 --> 00:13:08,390 NASA was quick to congratulate JAXA 211 00:13:08,390 --> 00:13:10,753 for reaching their asteroid first. 212 00:13:11,940 --> 00:13:15,320 - This is Dante Lauretta, leader of the NASA OSIRUS REx 213 00:13:15,320 --> 00:13:17,320 asteroid sample return mission, 214 00:13:17,320 --> 00:13:19,590 congratulating you on the successful approach 215 00:13:19,590 --> 00:13:21,060 to asteroid Ryugu. 216 00:13:21,060 --> 00:13:24,420 We're all very proud of your amazing accomplishments so far, 217 00:13:24,420 --> 00:13:26,190 and we look forward to working with you together 218 00:13:26,190 --> 00:13:29,100 over the next year to maximize the scientific return 219 00:13:29,100 --> 00:13:30,200 from our two missions. 220 00:13:31,546 --> 00:13:33,190 - NASA's OSIRUS REx probe 221 00:13:33,190 --> 00:13:35,560 is about to reach its target, Bennu, 222 00:13:35,560 --> 00:13:38,453 another CG type asteroid close to earth's orbit. 223 00:13:39,300 --> 00:13:42,630 A less ambitious mission, OSIRUS REx will touch down 224 00:13:42,630 --> 00:13:45,863 and retrieve a surface sample, then return it to earth. 225 00:13:46,780 --> 00:13:48,440 - Asteroids are very interesting objects, 226 00:13:48,440 --> 00:13:52,819 so they are very primary. 227 00:13:52,819 --> 00:13:55,620 They are the fundamental things 228 00:13:55,620 --> 00:13:58,240 and fundamental material of the solar system. 229 00:13:58,240 --> 00:14:01,400 And on the other hand they have, to some extent, 230 00:14:01,400 --> 00:14:03,580 they cross the orbit of the earth, 231 00:14:03,580 --> 00:14:07,840 they are dangerous, and just to know their structure, 232 00:14:07,840 --> 00:14:09,320 composition will help 233 00:14:09,320 --> 00:14:13,788 in order to avoid a collision with the earth 234 00:14:13,788 --> 00:14:14,838 if this might happen. 235 00:14:15,683 --> 00:14:17,470 And that will give us enough information 236 00:14:17,470 --> 00:14:20,580 in order to really find a way to mitigate 237 00:14:20,580 --> 00:14:22,373 this kind of catastrophic future. 238 00:14:26,350 --> 00:14:27,720 - [Narrator] And there is no shortage 239 00:14:27,720 --> 00:14:30,313 of conceivably dangerous asteroids out there. 240 00:14:32,920 --> 00:14:35,380 - It's one of the main points, of course. 241 00:14:35,380 --> 00:14:38,630 Because we really cannot exclude it 242 00:14:38,630 --> 00:14:41,410 but it's on a long time scale, 243 00:14:41,410 --> 00:14:44,980 but in any case, we know from the past, 244 00:14:44,980 --> 00:14:48,050 and we know from the past four billion years 245 00:14:48,050 --> 00:14:50,623 that this is a real danger for planets. 246 00:14:56,850 --> 00:14:59,000 - Sixty six million years ago 247 00:14:59,000 --> 00:15:01,750 one asteroid measuring 10 kilometers across 248 00:15:01,750 --> 00:15:04,170 completely changed earth's climate, 249 00:15:04,170 --> 00:15:06,890 wiping out two thirds of living species, 250 00:15:06,890 --> 00:15:08,500 and consigning the dinosaurs 251 00:15:08,500 --> 00:15:11,093 to history books and museum displays. 252 00:15:13,268 --> 00:15:16,018 (mystical music) 253 00:15:35,740 --> 00:15:39,280 Fortunately, large asteroid strikes are very rare, 254 00:15:39,280 --> 00:15:42,510 but smaller ones can still be dangerous. 255 00:15:42,510 --> 00:15:45,380 Along with other organizations across the world, 256 00:15:45,380 --> 00:15:48,763 ESA is working hard to identify and track them. 257 00:15:50,178 --> 00:15:52,928 (mystical music) 258 00:16:11,320 --> 00:16:13,480 - We currently have a detection rate of something like 259 00:16:13,480 --> 00:16:18,480 200 asteroids per month, and maybe 3, 4, 5 of them 260 00:16:19,144 --> 00:16:22,660 are objects which might hit the earth. 261 00:16:22,660 --> 00:16:26,780 So, currently we have 740 objects where we don't know 262 00:16:26,780 --> 00:16:28,300 if they will hit the earth of not. 263 00:16:28,300 --> 00:16:30,720 There's none which is really a serious threat, 264 00:16:30,720 --> 00:16:32,966 which we currently know of. 265 00:16:32,966 --> 00:16:33,799 There's plenty of things out there 266 00:16:33,799 --> 00:16:35,170 which we have not yet detected, 267 00:16:35,170 --> 00:16:36,890 which we are still searching for, 268 00:16:36,890 --> 00:16:39,219 but from what we know right now, 269 00:16:39,219 --> 00:16:42,850 there's nothing which we have to really worry about. 270 00:16:42,850 --> 00:16:43,720 What we have already seen, 271 00:16:43,720 --> 00:16:47,160 is if a 20 meter object would approach, 272 00:16:47,160 --> 00:16:49,790 that was the case five years ago in Chely, Binsk, 273 00:16:49,790 --> 00:16:53,840 when a 20 meter object exploded over a city in Russia, 274 00:16:53,840 --> 00:16:56,870 and 1,500 people went to hospital 275 00:16:56,870 --> 00:16:58,960 because they were close to a window, 276 00:16:58,960 --> 00:17:02,510 they were hit by fragments, and they were not aware, 277 00:17:02,510 --> 00:17:04,830 nobody knew that this object would come. 278 00:17:04,830 --> 00:17:08,380 And this is what we could improve in the future, 279 00:17:08,380 --> 00:17:10,910 that our telescope would detect this 280 00:17:10,910 --> 00:17:13,460 a week maybe in advance. 281 00:17:13,460 --> 00:17:15,500 - [Narrator] ESA's new Fly Eye telescope 282 00:17:15,500 --> 00:17:18,760 will conduct automated nightly sky surveys. 283 00:17:18,760 --> 00:17:22,630 It works by splitting the image into 16 smaller sub images, 284 00:17:22,630 --> 00:17:24,923 greatly expanding the field of view. 285 00:17:26,420 --> 00:17:28,580 - We planned our Fly Eye telescope, 286 00:17:28,580 --> 00:17:32,680 and easily we can scan the sky within 48 hours, 287 00:17:32,680 --> 00:17:34,420 so whenever an object 288 00:17:34,420 --> 00:17:37,570 bigger than 10-15 meters would approach, 289 00:17:37,570 --> 00:17:39,840 we should be able to see it beforehand, 290 00:17:39,840 --> 00:17:44,700 and then we would pass this information to the authorities. 291 00:17:44,700 --> 00:17:46,650 - Currently, the first Fly Eye telescope 292 00:17:46,650 --> 00:17:50,047 is foreseen to be placed in Sicily near the (mumbles). 293 00:17:52,330 --> 00:17:55,648 There are other free telescope for seeing the frame 294 00:17:55,648 --> 00:17:57,613 of the the NASA project, 295 00:17:58,500 --> 00:18:00,390 and there are many advantages 296 00:18:00,390 --> 00:18:03,670 in it for identical telescopes, 297 00:18:03,670 --> 00:18:07,100 both placed in northern and southern hemisphere. 298 00:18:07,100 --> 00:18:09,610 The coverage of the both hemisphere 299 00:18:09,610 --> 00:18:12,100 is due to geometric reasons in order to cover 300 00:18:12,100 --> 00:18:14,490 the full celestial sphere. 301 00:18:14,490 --> 00:18:19,010 Then considering that a telescope needs a clear sky 302 00:18:19,010 --> 00:18:22,180 for observation, doubling the number of telescope 303 00:18:22,180 --> 00:18:25,630 allow us to compensate in case of bad weather conditions. 304 00:18:25,630 --> 00:18:29,213 (intense orchestral music) 305 00:18:36,160 --> 00:18:37,610 - [Narrator] ESA's Fly Eye telescope 306 00:18:37,610 --> 00:18:39,500 will improve our chances of detecting 307 00:18:39,500 --> 00:18:41,910 these potentially dangerous objects, 308 00:18:41,910 --> 00:18:44,130 while the asteroid missions will increase our knowledge 309 00:18:44,130 --> 00:18:47,863 of asteroids and look at ways of protecting our planet. 310 00:18:51,870 --> 00:18:53,590 The telescope was designed and built 311 00:18:53,590 --> 00:18:55,020 by a consortium of companies 312 00:18:55,020 --> 00:18:57,383 from Italy, Poland, and Romania. 313 00:18:58,940 --> 00:19:01,740 - The Fly Eye telescope is based on novel and regional 314 00:19:01,740 --> 00:19:05,100 optical architecture, that makes, as the name says, 315 00:19:05,100 --> 00:19:07,170 the eye of the insects. 316 00:19:07,170 --> 00:19:08,810 In fact, it is composed by 317 00:19:08,810 --> 00:19:12,230 16 independent, single telescopes 318 00:19:12,230 --> 00:19:15,230 that share a common primary mirror. 319 00:19:15,230 --> 00:19:19,080 This way we can join together different optical features 320 00:19:19,080 --> 00:19:20,980 that are difficult to combine together 321 00:19:20,980 --> 00:19:22,940 in a single telescope. 322 00:19:22,940 --> 00:19:27,940 And every single optical channel, every single telescope 323 00:19:28,760 --> 00:19:30,870 that composes the Fly Eye telescope 324 00:19:30,870 --> 00:19:33,415 is provided with a focal plane, 325 00:19:33,415 --> 00:19:37,860 which already provides a large field of view. 326 00:19:37,860 --> 00:19:40,170 The combination of the 16 field of views, 327 00:19:40,170 --> 00:19:42,150 creates a very huge field of view. 328 00:19:42,150 --> 00:19:45,070 In fact, we have for each single telescope 329 00:19:45,070 --> 00:19:47,940 2.75 square degrees of field of view. 330 00:19:47,940 --> 00:19:51,630 That multiplied by 16 gives the 44 feet field of view 331 00:19:51,630 --> 00:19:53,620 of the overall instrument. 332 00:19:53,620 --> 00:19:55,240 This is very important due to the fact 333 00:19:55,240 --> 00:19:56,930 that with such a large field of view, 334 00:19:56,930 --> 00:20:01,030 you can map large ares of the sky very quickly, 335 00:20:01,030 --> 00:20:04,690 and you can, this way, scan the full visible sky 336 00:20:04,690 --> 00:20:07,130 at least three times per night. 337 00:20:07,130 --> 00:20:09,656 A typical observation of the telescope 338 00:20:09,656 --> 00:20:14,656 is about 40 to 60 seconds exposure time. 339 00:20:15,150 --> 00:20:16,140 During this time, of course, 340 00:20:16,140 --> 00:20:19,490 the structure must be very stiff in order to avoid 341 00:20:19,490 --> 00:20:22,330 the vibration that could blur the image 342 00:20:22,330 --> 00:20:26,367 and diminish the possibility of the telescope 343 00:20:26,367 --> 00:20:29,740 to look for faint objects. 344 00:20:29,740 --> 00:20:33,740 And this is very important from the optical point of view, 345 00:20:33,740 --> 00:20:36,810 due to the fact that all the performances 346 00:20:36,810 --> 00:20:39,250 that are collected together in the telescope 347 00:20:39,250 --> 00:20:42,423 must be maintained also from a mechanical point of view. 348 00:20:45,595 --> 00:20:48,762 (mellow guitar music) 349 00:20:55,210 --> 00:21:00,210 - Fly Eye telescope, due to its large field of view 350 00:21:00,500 --> 00:21:05,500 and also the capability to quick scan the sky, 351 00:21:05,770 --> 00:21:08,320 allow to arrive up to three 352 00:21:09,390 --> 00:21:12,023 complete scanning of the sky per night. 353 00:21:13,410 --> 00:21:18,410 This feature allow to implement what we call wide survey, 354 00:21:19,030 --> 00:21:23,380 what exist today is what is called the deep survey. 355 00:21:23,380 --> 00:21:28,100 So specific observation of an asteroid very far. 356 00:21:28,100 --> 00:21:33,100 But today we think we are the first, 357 00:21:33,170 --> 00:21:36,523 we are offering a service to cover all of the world. 358 00:21:37,410 --> 00:21:41,347 Because we can inform the population with a week in advance 359 00:21:41,347 --> 00:21:43,690 that an asteroid can hit to the earth, 360 00:21:43,690 --> 00:21:46,470 so we can protect the population. 361 00:21:46,470 --> 00:21:51,470 This instrument can detect an object like a tennis ball 362 00:21:51,800 --> 00:21:54,480 at an orbit 1000 kilometer 363 00:21:55,880 --> 00:21:57,823 moving at 10 kilometer per second. 364 00:21:58,700 --> 00:22:02,594 After 10 detections, we can calculate the orbit 365 00:22:02,594 --> 00:22:06,110 to with an accuracy of 20 meter along a track. 366 00:22:06,110 --> 00:22:07,930 So an important feature, 367 00:22:07,930 --> 00:22:11,730 and we can implement aerial cooperative way, 368 00:22:11,730 --> 00:22:13,133 between aerial and optical. 369 00:22:15,540 --> 00:22:16,890 - [Narrator] ESA is currently working 370 00:22:16,890 --> 00:22:19,630 on a set of space safety and security activities, 371 00:22:19,630 --> 00:22:22,410 which focus on threats, such as space weather, 372 00:22:22,410 --> 00:22:25,810 artificial debris, and asteroids. 373 00:22:25,810 --> 00:22:27,230 By enhancing the existing 374 00:22:27,230 --> 00:22:29,670 space situational awareness program, 375 00:22:29,670 --> 00:22:31,990 these will help us better understand the risks 376 00:22:31,990 --> 00:22:34,513 to our planet and prevent disaster. 377 00:22:37,580 --> 00:22:40,756 - Searching for asteroids and mitigating the risk of impact, 378 00:22:40,756 --> 00:22:42,660 while at the same time 379 00:22:42,660 --> 00:22:44,810 collaborating with international partners, 380 00:22:44,810 --> 00:22:47,560 that's how I see how ESA can contribute 381 00:22:47,560 --> 00:22:50,613 to fulfill UN sustainable development goals. 382 00:22:51,641 --> 00:22:54,391 (mystical music) 383 00:23:02,700 --> 00:23:05,200 - [Narrator] All going well, the Hyabusa 2 sample 384 00:23:05,200 --> 00:23:09,280 will land in the Australian outback sometime in 2020. 385 00:23:09,280 --> 00:23:13,713 OSIRUS REx will follow with a sample for return in 2023. 386 00:23:15,598 --> 00:23:19,181 (intense orchestral music) 387 00:23:39,581 --> 00:23:41,998 (wind blows) 31325

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