All language subtitles for D731F252ABE979BBE8F7C85636CD9C9D_eng

af Afrikaans
ak Akan
sq Albanian
am Amharic
ar Arabic Download
hy Armenian
az Azerbaijani
eu Basque
be Belarusian
bem Bemba
bn Bengali
bh Bihari
bs Bosnian
br Breton
bg Bulgarian
km Cambodian
ca Catalan
ceb Cebuano
chr Cherokee
ny Chichewa
zh-CN Chinese (Simplified)
zh-TW Chinese (Traditional)
co Corsican
hr Croatian
cs Czech
da Danish
nl Dutch
en English
eo Esperanto
et Estonian
ee Ewe
fo Faroese
tl Filipino
fi Finnish
fr French
fy Frisian
gaa Ga
gl Galician
ka Georgian
de German
el Greek
gn Guarani
gu Gujarati
ht Haitian Creole
ha Hausa
haw Hawaiian
iw Hebrew
hi Hindi
hmn Hmong
hu Hungarian
is Icelandic
ig Igbo
id Indonesian
ia Interlingua
ga Irish
it Italian
ja Japanese
jw Javanese
kn Kannada
kk Kazakh
rw Kinyarwanda
rn Kirundi
kg Kongo
ko Korean
kri Krio (Sierra Leone)
ku Kurdish
ckb Kurdish (Soranî)
ky Kyrgyz
lo Laothian
la Latin
lv Latvian
ln Lingala
lt Lithuanian
loz Lozi
lg Luganda
ach Luo
lb Luxembourgish
mk Macedonian
mg Malagasy
ms Malay
ml Malayalam
mt Maltese
mi Maori
mr Marathi
mfe Mauritian Creole
mo Moldavian
mn Mongolian
my Myanmar (Burmese)
sr-ME Montenegrin
ne Nepali
pcm Nigerian Pidgin
nso Northern Sotho
no Norwegian
nn Norwegian (Nynorsk)
oc Occitan
or Oriya
om Oromo
ps Pashto
fa Persian
pl Polish
pt-BR Portuguese (Brazil)
pt Portuguese (Portugal)
pa Punjabi
qu Quechua
ro Romanian
rm Romansh
nyn Runyakitara
ru Russian
sm Samoan
gd Scots Gaelic
sr Serbian
sh Serbo-Croatian
st Sesotho
tn Setswana
crs Seychellois Creole
sn Shona
sd Sindhi
si Sinhalese
sk Slovak
sl Slovenian
so Somali
es Spanish
es-419 Spanish (Latin American)
su Sundanese
sw Swahili
sv Swedish
tg Tajik
ta Tamil
tt Tatar
te Telugu
th Thai
ti Tigrinya
to Tonga
lua Tshiluba
tum Tumbuka
tr Turkish
tk Turkmen
tw Twi
ug Uighur
uk Ukrainian
ur Urdu
uz Uzbek
vi Vietnamese
cy Welsh
wo Wolof
xh Xhosa
yi Yiddish
yo Yoruba
zu Zulu
Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:00,960 --> 00:00:02,920 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 00:01:04,240 --> 00:01:07,550 A three and a half year journey to asteroid Ryugu is over, 12 00:01:07,550 --> 00:01:10,924 and the Hyabusa 2 science mission begins. 13 00:01:10,924 --> 00:01:12,980 Ryugu, part of the Apollo group, 14 00:01:12,980 --> 00:01:16,720 is potentially a threat to earth in the years to come. 15 00:01:16,720 --> 00:01:19,710 It's an unusual asteroid, a CG type, 16 00:01:19,710 --> 00:01:20,870 meaning it has qualities 17 00:01:20,870 --> 00:01:24,910 of both C type and G type carbonaceous asteroids. 18 00:01:24,910 --> 00:01:28,813 It is just under a kilometer in diameter and fast-moving. 19 00:01:29,680 --> 00:01:30,960 As part of its payload, 20 00:01:30,960 --> 00:01:34,120 the Hybusa 2 has several deployable landers. 21 00:01:34,120 --> 00:01:37,490 Two MINERVA II's, the Franco-German Mascot lander, 22 00:01:37,490 --> 00:01:40,450 and target acquisition markers for the touchdown. 23 00:01:40,450 --> 00:01:42,240 - Okay, we want to see the boulders, 24 00:01:42,240 --> 00:01:43,780 we have a chance to view the boulders 25 00:01:43,780 --> 00:01:45,432 in a vertical structure. 26 00:01:45,432 --> 00:01:47,304 We also see the crack in the boulders, 27 00:01:47,304 --> 00:01:49,730 there is also regulate. 28 00:01:49,730 --> 00:01:52,780 We know from the spectral information we have so far 29 00:01:52,780 --> 00:01:55,260 that there is something a little bit redder, 30 00:01:55,260 --> 00:01:57,600 something a little bit bluer on the surface, 31 00:01:57,600 --> 00:01:58,920 so that's very interesting. 32 00:01:58,920 --> 00:02:01,510 Because there are differences on the surface, 33 00:02:01,510 --> 00:02:03,000 we have the feeling that the bluer, 34 00:02:03,000 --> 00:02:05,780 it may be a little bit fresher than the redder. 35 00:02:05,780 --> 00:02:10,780 And that basically gives us a good idea of the history 36 00:02:12,480 --> 00:02:14,930 of the material on the surface. 37 00:02:14,930 --> 00:02:19,023 And of course there are a number of landing sites, 38 00:02:19,023 --> 00:02:21,070 which are red and blue, 39 00:02:21,070 --> 00:02:23,190 or which have red and blue in it, 40 00:02:23,190 --> 00:02:25,930 and that's probably preferred, at least for the camera, 41 00:02:25,930 --> 00:02:29,150 so we have chance to see both of the surfaces. 42 00:02:29,150 --> 00:02:31,780 - From the feedback I have obtained now 43 00:02:31,780 --> 00:02:36,780 from our principle investigators of the instruments, 44 00:02:37,130 --> 00:02:40,270 seems to be that it's a very interesting asteroid. 45 00:02:40,270 --> 00:02:43,260 And that there are several aspects 46 00:02:43,260 --> 00:02:48,260 which is covering the science objective of each instrument. 47 00:02:51,610 --> 00:02:53,430 First to be deployed to the asteroid 48 00:02:53,430 --> 00:02:55,173 were two MINERVA probes. 49 00:02:58,540 --> 00:03:01,140 These rovers are based on the original MINERVA craft 50 00:03:01,140 --> 00:03:02,713 flown on Hyabusa 1, 51 00:03:04,560 --> 00:03:08,340 which unfortunately failed to land on their target asteroid. 52 00:03:08,340 --> 00:03:10,423 These ones, however, were successful. 53 00:03:19,510 --> 00:03:22,400 They have radioed back several stunning photographs 54 00:03:22,400 --> 00:03:24,330 from the surface of the asteroid, 55 00:03:24,330 --> 00:03:27,850 including this sequence of the sun crossing the skyline 56 00:03:27,850 --> 00:03:29,573 as the asteroid tumbles. 57 00:03:38,600 --> 00:03:43,600 - Asteroid missions are very important and very interesting 58 00:03:43,620 --> 00:03:45,700 from the scientific point of view 59 00:03:45,700 --> 00:03:50,700 because it is believed that asteroid and comets 60 00:03:50,811 --> 00:03:54,380 are bringing water to the earth 61 00:03:54,380 --> 00:03:59,030 in the very early phase of the development of the earth. 62 00:03:59,030 --> 00:04:03,380 And with this water and also organic materials, 63 00:04:03,380 --> 00:04:08,380 it is believed that life on earth has developed 64 00:04:10,180 --> 00:04:12,150 and very importantly, 65 00:04:12,150 --> 00:04:17,150 is also to understand the evolution of the solar system, 66 00:04:18,030 --> 00:04:21,160 because asteroid are supposed to be building blocks 67 00:04:21,160 --> 00:04:23,453 of our early solar system. 68 00:04:28,602 --> 00:04:31,670 - The Hyabusa 2 mission has been years in the making. 69 00:04:31,670 --> 00:04:33,320 As with any deep space probe, 70 00:04:33,320 --> 00:04:35,210 years are spent on the drawing board 71 00:04:35,210 --> 00:04:37,810 developing the hardware and software. 72 00:04:37,810 --> 00:04:41,563 Then come years of construction and extensive testing. 73 00:04:47,680 --> 00:04:49,490 The aim of the Hyabusa 2 mission 74 00:04:49,490 --> 00:04:52,160 is to learn more about the origin and evolution 75 00:04:52,160 --> 00:04:54,170 of the solar system. 76 00:04:54,170 --> 00:04:55,510 As asteroids account 77 00:04:55,510 --> 00:04:58,330 for some of the most primordial celestial bodies, 78 00:04:58,330 --> 00:05:01,700 researching them gives us a glimpse into our cosmic past. 79 00:05:08,620 --> 00:05:10,210 Scientists are keen to learn more 80 00:05:10,210 --> 00:05:13,348 about the properties and structure of near earth asteroids 81 00:05:13,348 --> 00:05:15,470 in order to gain new insights 82 00:05:15,470 --> 00:05:17,830 into how our solar system formed, 83 00:05:17,830 --> 00:05:21,210 and how water and life emerged on earth. 84 00:05:21,210 --> 00:05:22,913 It's an audacious mission. 85 00:05:28,260 --> 00:05:33,020 - I mean, they're flying to an asteroid, 86 00:05:33,020 --> 00:05:38,000 now we map the asteroid, then a lander will be deployed, 87 00:05:38,000 --> 00:05:39,470 like Mascot or MINERVA. 88 00:05:39,470 --> 00:05:41,480 They're trying to do three samples 89 00:05:41,480 --> 00:05:44,880 and then they have also explosives on board 90 00:05:44,880 --> 00:05:48,500 to produce a crater on the surface in the asteroid. 91 00:05:48,500 --> 00:05:51,530 I mean, to me it's a unique mission they are doing, 92 00:05:51,530 --> 00:05:54,763 and we are a part of it, so I'm really proud of it. 93 00:05:54,763 --> 00:05:58,160 - And, of course, we are interested in the geology, 94 00:05:58,160 --> 00:06:01,300 the geomorphology, the structure, 95 00:06:01,300 --> 00:06:03,828 the size of the big boulders, 96 00:06:03,828 --> 00:06:07,530 and also the structure of the regulate, 97 00:06:07,530 --> 00:06:12,530 and giving some hints of the evolution of the surface, 98 00:06:14,820 --> 00:06:18,563 of the forming and evolution of the surface of Ryugu. 99 00:06:19,962 --> 00:06:21,110 And I think for a camera, 100 00:06:21,110 --> 00:06:23,980 all of the landing sites are quite okay. 101 00:06:23,980 --> 00:06:26,566 So the most interesting thing is to see the big boulders 102 00:06:26,566 --> 00:06:28,490 from the vertical structure. 103 00:06:28,490 --> 00:06:32,453 We really can look how deep they are in the surface, 104 00:06:34,320 --> 00:06:36,230 and there are many boulders on Ryugu, 105 00:06:36,230 --> 00:06:38,316 so I'm pretty sure we'll get a good view 106 00:06:38,316 --> 00:06:41,723 of this interesting part of this asteroid. 107 00:06:52,040 --> 00:06:54,050 The second batch of asteroid landers, 108 00:06:54,050 --> 00:06:57,260 developed by the German and French space organizations, 109 00:06:57,260 --> 00:06:59,860 were launched and after a short free fall, 110 00:06:59,860 --> 00:07:02,270 successfully landed at the southern hemisphere 111 00:07:02,270 --> 00:07:04,000 of asteroid Ryugu. 112 00:07:04,000 --> 00:07:07,540 After bouncing several times on the rock strewn surface, 113 00:07:07,540 --> 00:07:10,563 the two landers have begun their scientific research. 114 00:07:11,640 --> 00:07:15,502 - And you know that Mascot is made to bounce. 115 00:07:15,502 --> 00:07:17,280 That makes it robust, 116 00:07:17,280 --> 00:07:21,260 but it also means that the final resting location 117 00:07:21,260 --> 00:07:25,560 is not exactly possible to calculate it. 118 00:07:25,560 --> 00:07:27,870 So there's a dispersion of possible sites 119 00:07:27,870 --> 00:07:30,700 and there are some variation in between. 120 00:07:30,700 --> 00:07:33,760 There could be, among these many, many possibilities, 121 00:07:33,760 --> 00:07:37,210 some bad ones, and we have to go to places 122 00:07:37,210 --> 00:07:39,580 where the chance to hit a good one is highest, 123 00:07:39,580 --> 00:07:44,090 but it does exclude that we end up in a bad one. 124 00:07:44,090 --> 00:07:45,680 - Autonomous handling doesn't mean 125 00:07:45,680 --> 00:07:49,511 that Mascot is doing everything as he likes to, 126 00:07:49,511 --> 00:07:54,511 so there is lots of sequences and commands that's behind, 127 00:07:54,710 --> 00:07:56,610 which are carefully tested and planned. 128 00:07:56,610 --> 00:08:00,310 So the robustness of these sequences have to be tested 129 00:08:00,310 --> 00:08:03,460 against all these difficult, different conditions 130 00:08:03,460 --> 00:08:05,160 we can meet on the asteroid. 131 00:08:05,160 --> 00:08:08,500 So if we bounce or land more in the west or more in the east 132 00:08:10,300 --> 00:08:12,610 for this the input Mascot has, 133 00:08:12,610 --> 00:08:16,110 which he uses for his autonomously, 134 00:08:16,110 --> 00:08:18,570 this is really carefully planned and tested. 135 00:08:18,570 --> 00:08:19,840 And so there's all the work, 136 00:08:19,840 --> 00:08:24,263 and I think we did a very well job, and so I'm relaxed. 137 00:08:27,350 --> 00:08:29,160 With it's four instruments, 138 00:08:29,160 --> 00:08:31,240 including the Micro-Mica spectrometer, 139 00:08:31,240 --> 00:08:35,460 developed by the IAS Space Astrophysics Institute at Oxate, 140 00:08:35,460 --> 00:08:37,600 with CNES oversight, 141 00:08:37,600 --> 00:08:40,810 Mascot is set to analyze the mineral composition of grains 142 00:08:40,810 --> 00:08:44,680 in the asteroid's soil in an attempt to unlock its secrets 143 00:08:44,680 --> 00:08:47,800 at two sites just a few meters apart. 144 00:08:47,800 --> 00:08:50,133 They also took some fascinating images. 145 00:08:53,750 --> 00:08:57,050 - I think, at least for me, the most important question 146 00:08:57,050 --> 00:08:59,710 is the big number of boulders. 147 00:08:59,710 --> 00:09:01,350 Where did they come from? 148 00:09:01,350 --> 00:09:04,120 Why has this asteroid so many boulders? 149 00:09:04,120 --> 00:09:07,793 Why are these boulders, to some extent, 150 00:09:08,944 --> 00:09:13,053 covered by the surface, so they are in the sub-surface? 151 00:09:15,110 --> 00:09:16,643 And the question here is, 152 00:09:18,180 --> 00:09:21,400 what are the source of the boulders? 153 00:09:21,400 --> 00:09:25,210 Are they from the interior or coming from outside, 154 00:09:25,210 --> 00:09:27,880 or they are linked from some kind of condition 155 00:09:27,880 --> 00:09:32,880 from bigger body where Ryugu is now a related part of it? 156 00:09:35,090 --> 00:09:38,543 So, I think that's the most important question. 157 00:09:43,330 --> 00:09:46,210 - Mascot was operational for over 17 hours, 158 00:09:46,210 --> 00:09:49,220 during which it collected data from the asteroid's surface 159 00:09:49,220 --> 00:09:52,430 and transmitted it back to Hyabusa 2 overhead, 160 00:09:52,430 --> 00:09:54,683 which relayed the data back to earth. 161 00:10:04,000 --> 00:10:07,360 The next probe to be released is the third MINERVA robot, 162 00:10:07,360 --> 00:10:09,400 the largest of the MINERVA's. 163 00:10:18,020 --> 00:10:23,020 - I would like just to express again this amazing work, 164 00:10:24,820 --> 00:10:27,433 which the whole team has done. 165 00:10:28,443 --> 00:10:33,443 DLR, as well as CNES, as well as JAXA surely. 166 00:10:33,640 --> 00:10:38,640 So, this was a very good example of very good collaboration 167 00:10:40,500 --> 00:10:42,480 on an international level, 168 00:10:42,480 --> 00:10:46,820 and I hope that it will go on in the future. 169 00:10:46,820 --> 00:10:51,190 - GNC that has to tell your autonomy manager, 170 00:10:51,190 --> 00:10:55,530 the right side or which side we should turn to upright. 171 00:10:58,020 --> 00:10:58,940 The entire mission 172 00:10:58,940 --> 00:11:01,840 has been a close collaboration between nations. 173 00:11:01,840 --> 00:11:04,870 Japanese, German, and French scientists and engineers 174 00:11:04,870 --> 00:11:07,920 have enjoyed over a decade of scientific cooperation, 175 00:11:07,920 --> 00:11:10,850 even if there are language barriers. 176 00:11:14,610 --> 00:11:15,443 - I like this because 177 00:11:15,443 --> 00:11:18,530 it's a small mission with little overhead. 178 00:11:18,530 --> 00:11:23,230 And it's very nice to work with the Japanese, 179 00:11:23,230 --> 00:11:26,360 because they are very success oriented, 180 00:11:29,420 --> 00:11:32,140 they are willing to take risks, 181 00:11:32,140 --> 00:11:35,460 they have also, because of language issues, 182 00:11:35,460 --> 00:11:39,380 much less paperwork than NASA or ESA does. 183 00:11:39,380 --> 00:11:42,050 So most things are done in discussions, 184 00:11:42,050 --> 00:11:44,350 and you agree on something, you look into your eyes 185 00:11:44,350 --> 00:11:48,120 and say yes we do it, yes, and you rely on the words. 186 00:11:48,120 --> 00:11:52,310 You don't sign big papers, and that's something I like, 187 00:11:52,310 --> 00:11:56,340 because it makes work so much easier and smooth and quick. 188 00:11:56,340 --> 00:11:58,690 Oh yes, the mission is very good. 189 00:11:58,690 --> 00:12:02,540 There are in all the teams from Hyabusa Mascot, 190 00:12:02,540 --> 00:12:05,280 there are very excellent engineers 191 00:12:05,280 --> 00:12:06,960 and also very excellent scientists, 192 00:12:06,960 --> 00:12:10,620 so I'm really, really confident and excited. 193 00:12:10,620 --> 00:12:12,963 And that's the first time we do this. 194 00:12:13,820 --> 00:12:16,921 The Hyabusa 2 mission is very interesting 195 00:12:16,921 --> 00:12:18,870 from the point of view 196 00:12:18,870 --> 00:12:23,110 because Hyabusa 2 is investigating a C type asteroid. 197 00:12:23,110 --> 00:12:25,940 Ryugu is a very primitive asteroid, 198 00:12:25,940 --> 00:12:30,940 which is supposed to have organic material on the surface. 199 00:12:31,260 --> 00:12:35,277 In addition, Hyabusa 2 has got in situ signs 200 00:12:35,277 --> 00:12:37,610 provided by the Mascot lander, 201 00:12:37,610 --> 00:12:42,110 and also two to three further small MINERVA landers, 202 00:12:42,110 --> 00:12:47,050 and it is, or it will bring some samples back to earth, 203 00:12:47,050 --> 00:12:50,183 so that we can investigate it then on earth in the labs. 204 00:13:04,209 --> 00:13:06,210 In the spirit of friendly competition, 205 00:13:06,210 --> 00:13:08,390 NASA was quick to congratulate JAXA 206 00:13:08,390 --> 00:13:10,753 for reaching their asteroid first. 207 00:13:11,940 --> 00:13:15,320 - This is Dante Lauretta, leader of the NASA OSIRUS REx 208 00:13:15,320 --> 00:13:17,320 asteroid sample return mission, 209 00:13:17,320 --> 00:13:19,590 congratulating you on the successful approach 210 00:13:19,590 --> 00:13:21,060 to asteroid Ryugu. 211 00:13:21,060 --> 00:13:24,420 We're all very proud of your amazing accomplishments so far, 212 00:13:24,420 --> 00:13:26,190 and we look forward to working with you together 213 00:13:26,190 --> 00:13:29,100 over the next year to maximize the scientific return 214 00:13:29,100 --> 00:13:30,200 from our two missions. 215 00:13:31,546 --> 00:13:33,190 - NASA's OSIRUS REx probe 216 00:13:33,190 --> 00:13:35,560 is about to reach its target, Bennu, 217 00:13:35,560 --> 00:13:38,453 another CG type asteroid close to earth's orbit. 218 00:13:39,300 --> 00:13:42,630 A less ambitious mission, OSIRUS REx will touch down 219 00:13:42,630 --> 00:13:45,863 and retrieve a surface sample, then return it to earth. 220 00:13:46,780 --> 00:13:48,440 - Asteroids are very interesting objects, 221 00:13:48,440 --> 00:13:52,819 so they are very primary. 222 00:13:52,819 --> 00:13:55,620 They are the fundamental things 223 00:13:55,620 --> 00:13:58,240 and fundamental material of the solar system. 224 00:13:58,240 --> 00:14:01,400 And on the other hand they have, to some extent, 225 00:14:01,400 --> 00:14:03,580 they cross the orbit of the earth, 226 00:14:03,580 --> 00:14:07,840 they are dangerous, and just to know their structure, 227 00:14:07,840 --> 00:14:09,320 composition will help 228 00:14:09,320 --> 00:14:13,788 in order to avoid a collision with the earth 229 00:14:13,788 --> 00:14:14,838 if this might happen. 230 00:14:15,683 --> 00:14:17,470 And that will give us enough information 231 00:14:17,470 --> 00:14:20,580 in order to really find a way to mitigate 232 00:14:20,580 --> 00:14:22,373 this kind of catastrophic future. 233 00:14:26,350 --> 00:14:27,720 And there is no shortage 234 00:14:27,720 --> 00:14:30,313 of conceivably dangerous asteroids out there. 235 00:14:32,920 --> 00:14:35,380 - It's one of the main points, of course. 236 00:14:35,380 --> 00:14:38,630 Because we really cannot exclude it 237 00:14:38,630 --> 00:14:41,410 but it's on a long time scale, 238 00:14:41,410 --> 00:14:44,980 but in any case, we know from the past, 239 00:14:44,980 --> 00:14:48,050 and we know from the past four billion years 240 00:14:48,050 --> 00:14:50,623 that this is a real danger for planets. 241 00:14:56,850 --> 00:14:59,000 - Sixty six million years ago 242 00:14:59,000 --> 00:15:01,750 one asteroid measuring 10 kilometers across 243 00:15:01,750 --> 00:15:04,170 completely changed earth's climate, 244 00:15:04,170 --> 00:15:06,890 wiping out two thirds of living species, 245 00:15:06,890 --> 00:15:08,500 and consigning the dinosaurs 246 00:15:08,500 --> 00:15:11,093 to history books and museum displays. 247 00:15:35,740 --> 00:15:39,280 Fortunately, large asteroid strikes are very rare, 248 00:15:39,280 --> 00:15:42,510 but smaller ones can still be dangerous. 249 00:15:42,510 --> 00:15:45,380 Along with other organizations across the world, 250 00:15:45,380 --> 00:15:48,763 ESA is working hard to identify and track them. 251 00:16:11,320 --> 00:16:13,480 - We currently have a detection rate of something like 252 00:16:13,480 --> 00:16:18,480 200 asteroids per month, and maybe 3, 4, 5 of them 253 00:16:19,144 --> 00:16:22,660 are objects which might hit the earth. 254 00:16:22,660 --> 00:16:26,780 So, currently we have 740 objects where we don't know 255 00:16:26,780 --> 00:16:28,300 if they will hit the earth of not. 256 00:16:28,300 --> 00:16:30,720 There's none which is really a serious threat, 257 00:16:30,720 --> 00:16:32,966 which we currently know of. 258 00:16:32,966 --> 00:16:33,799 There's plenty of things out there 259 00:16:33,799 --> 00:16:35,170 which we have not yet detected, 260 00:16:35,170 --> 00:16:36,890 which we are still searching for, 261 00:16:36,890 --> 00:16:39,219 but from what we know right now, 262 00:16:39,219 --> 00:16:42,850 there's nothing which we have to really worry about. 263 00:16:42,850 --> 00:16:43,720 What we have already seen, 264 00:16:43,720 --> 00:16:47,160 is if a 20 meter object would approach, 265 00:16:47,160 --> 00:16:49,790 that was the case five years ago in Chely, Binsk, 266 00:16:49,790 --> 00:16:53,840 when a 20 meter object exploded over a city in Russia, 267 00:16:53,840 --> 00:16:56,870 and 1,500 people went to hospital 268 00:16:56,870 --> 00:16:58,960 because they were close to a window, 269 00:16:58,960 --> 00:17:02,510 they were hit by fragments, and they were not aware, 270 00:17:02,510 --> 00:17:04,830 nobody knew that this object would come. 271 00:17:04,830 --> 00:17:08,380 And this is what we could improve in the future, 272 00:17:08,380 --> 00:17:10,910 that our telescope would detect this 273 00:17:10,910 --> 00:17:13,460 a week maybe in advance. 274 00:17:13,460 --> 00:17:15,500 ESA's new Fly Eye telescope 275 00:17:15,500 --> 00:17:18,760 will conduct automated nightly sky surveys. 276 00:17:18,760 --> 00:17:22,630 It works by splitting the image into 16 smaller sub images, 277 00:17:22,630 --> 00:17:24,923 greatly expanding the field of view. 278 00:17:26,420 --> 00:17:28,580 - We planned our Fly Eye telescope, 279 00:17:28,580 --> 00:17:32,680 and easily we can scan the sky within 48 hours, 280 00:17:32,680 --> 00:17:34,420 so whenever an object 281 00:17:34,420 --> 00:17:37,570 bigger than 10-15 meters would approach, 282 00:17:37,570 --> 00:17:39,840 we should be able to see it beforehand, 283 00:17:39,840 --> 00:17:44,700 and then we would pass this information to the authorities. 284 00:17:44,700 --> 00:17:46,650 - Currently, the first Fly Eye telescope 285 00:17:46,650 --> 00:17:50,047 is foreseen to be placed in Sicily near the. 286 00:17:52,330 --> 00:17:55,648 There are other free telescope for seeing the frame 287 00:17:55,648 --> 00:17:57,613 of the the NASA project, 288 00:17:58,500 --> 00:18:00,390 and there are many advantages 289 00:18:00,390 --> 00:18:03,670 in it for identical telescopes, 290 00:18:03,670 --> 00:18:07,100 both placed in northern and southern hemisphere. 291 00:18:07,100 --> 00:18:09,610 The coverage of the both hemisphere 292 00:18:09,610 --> 00:18:12,100 is due to geometric reasons in order to cover 293 00:18:12,100 --> 00:18:14,490 the full celestial sphere. 294 00:18:14,490 --> 00:18:19,010 Then considering that a telescope needs a clear sky 295 00:18:19,010 --> 00:18:22,180 for observation, doubling the number of telescope 296 00:18:22,180 --> 00:18:25,630 allow us to compensate in case of bad weather conditions. 297 00:18:36,160 --> 00:18:37,610 ESA's Fly Eye telescope 298 00:18:37,610 --> 00:18:39,500 will improve our chances of detecting 299 00:18:39,500 --> 00:18:41,910 these potentially dangerous objects, 300 00:18:41,910 --> 00:18:44,130 while the asteroid missions will increase our knowledge 301 00:18:44,130 --> 00:18:47,863 of asteroids and look at ways of protecting our planet. 302 00:18:51,870 --> 00:18:53,590 The telescope was designed and built 303 00:18:53,590 --> 00:18:55,020 by a consortium of companies 304 00:18:55,020 --> 00:18:57,383 from Italy, Poland, and Romania. 305 00:18:58,940 --> 00:19:01,740 - The Fly Eye telescope is based on novel and regional 306 00:19:01,740 --> 00:19:05,100 optical architecture, that makes, as the name says, 307 00:19:05,100 --> 00:19:07,170 the eye of the insects. 308 00:19:07,170 --> 00:19:08,810 In fact, it is composed by 309 00:19:08,810 --> 00:19:12,230 16 independent, single telescopes 310 00:19:12,230 --> 00:19:15,230 that share a common primary mirror. 311 00:19:15,230 --> 00:19:19,080 This way we can join together different optical features 312 00:19:19,080 --> 00:19:20,980 that are difficult to combine together 313 00:19:20,980 --> 00:19:22,940 in a single telescope. 314 00:19:22,940 --> 00:19:27,940 And every single optical channel, every single telescope 315 00:19:28,760 --> 00:19:30,870 that composes the Fly Eye telescope 316 00:19:30,870 --> 00:19:33,415 is provided with a focal plane, 317 00:19:33,415 --> 00:19:37,860 which already provides a large field of view. 318 00:19:37,860 --> 00:19:40,170 The combination of the 16 field of views, 319 00:19:40,170 --> 00:19:42,150 creates a very huge field of view. 320 00:19:42,150 --> 00:19:45,070 In fact, we have for each single telescope 321 00:19:45,070 --> 00:19:47,940 2.75 square degrees of field of view. 322 00:19:47,940 --> 00:19:51,630 That multiplied by 16 gives the 44 feet field of view 323 00:19:51,630 --> 00:19:53,620 of the overall instrument. 324 00:19:53,620 --> 00:19:55,240 This is very important due to the fact 325 00:19:55,240 --> 00:19:56,930 that with such a large field of view, 326 00:19:56,930 --> 00:20:01,030 you can map large ares of the sky very quickly, 327 00:20:01,030 --> 00:20:04,690 and you can, this way, scan the full visible sky 328 00:20:04,690 --> 00:20:07,130 at least three times per night. 329 00:20:07,130 --> 00:20:09,656 A typical observation of the telescope 330 00:20:09,656 --> 00:20:14,656 is about 40 to 60 seconds exposure time. 331 00:20:15,150 --> 00:20:16,140 During this time, of course, 332 00:20:16,140 --> 00:20:19,490 the structure must be very stiff in order to avoid 333 00:20:19,490 --> 00:20:22,330 the vibration that could blur the image 334 00:20:22,330 --> 00:20:26,367 and diminish the possibility of the telescope 335 00:20:26,367 --> 00:20:29,740 to look for faint objects. 336 00:20:29,740 --> 00:20:33,740 And this is very important from the optical point of view, 337 00:20:33,740 --> 00:20:36,810 due to the fact that all the performances 338 00:20:36,810 --> 00:20:39,250 that are collected together in the telescope 339 00:20:39,250 --> 00:20:42,423 must be maintained also from a mechanical point of view. 340 00:20:55,210 --> 00:21:00,210 - Fly Eye telescope, due to its large field of view 341 00:21:00,500 --> 00:21:05,500 and also the capability to quick scan the sky, 342 00:21:05,770 --> 00:21:08,320 allow to arrive up to three 343 00:21:09,390 --> 00:21:12,023 complete scanning of the sky per night. 344 00:21:13,410 --> 00:21:18,410 This feature allow to implement what we call wide survey, 345 00:21:19,030 --> 00:21:23,380 what exist today is what is called the deep survey. 346 00:21:23,380 --> 00:21:28,100 So specific observation of an asteroid very far. 347 00:21:28,100 --> 00:21:33,100 But today we think we are the first, 348 00:21:33,170 --> 00:21:36,523 we are offering a service to cover all of the world. 349 00:21:37,410 --> 00:21:41,347 Because we can inform the population with a week in advance 350 00:21:41,347 --> 00:21:43,690 that an asteroid can hit to the earth, 351 00:21:43,690 --> 00:21:46,470 so we can protect the population. 352 00:21:46,470 --> 00:21:51,470 This instrument can detect an object like a tennis ball 353 00:21:51,800 --> 00:21:54,480 at an orbit 1000 kilometer 354 00:21:55,880 --> 00:21:57,823 moving at 10 kilometer per second. 355 00:21:58,700 --> 00:22:02,594 After 10 detections, we can calculate the orbit 356 00:22:02,594 --> 00:22:06,110 to with an accuracy of 20 meter along a track. 357 00:22:06,110 --> 00:22:07,930 So an important feature, 358 00:22:07,930 --> 00:22:11,730 and we can implement aerial cooperative way, 359 00:22:11,730 --> 00:22:13,133 between aerial and optical. 360 00:22:15,540 --> 00:22:16,890 ESA is currently working 361 00:22:16,890 --> 00:22:19,630 on a set of space safety and security activities, 362 00:22:19,630 --> 00:22:22,410 which focus on threats, such as space weather, 363 00:22:22,410 --> 00:22:25,810 artificial debris, and asteroids. 364 00:22:25,810 --> 00:22:27,230 By enhancing the existing 365 00:22:27,230 --> 00:22:29,670 space situational awareness program, 366 00:22:29,670 --> 00:22:31,990 these will help us better understand the risks 367 00:22:31,990 --> 00:22:34,513 to our planet and prevent disaster. 368 00:22:37,580 --> 00:22:40,756 - Searching for asteroids and mitigating the risk of impact, 369 00:22:40,756 --> 00:22:42,660 while at the same time 370 00:22:42,660 --> 00:22:44,810 collaborating with international partners, 371 00:22:44,810 --> 00:22:47,560 that's how I see how ESA can contribute 372 00:22:47,560 --> 00:22:50,613 to fulfill UN sustainable development goals. 373 00:23:02,700 --> 00:23:05,200 All going well, the Hyabusa 2 sample 374 00:23:05,200 --> 00:23:09,280 will land in the Australian outback sometime in 2020. 375 00:23:09,280 --> 00:23:13,713 OSIRUS REx will follow with a sample for return in 2023. 30431

Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.