1 00:00:10,310 --> 00:00:08,070 we are locked and we are going to send 2 00:00:11,910 --> 00:00:10,320 that command 3 00:00:12,870 --> 00:00:11,920 31 minutes and 32 seconds for our 4 00:00:15,270 --> 00:00:12,880 support 5 00:00:18,310 --> 00:00:15,280 [Music] 6 00:00:19,910 --> 00:00:18,320 go for status buffer dump 7 00:00:21,830 --> 00:00:19,920 what you're looking at with a telescope 8 00:00:24,310 --> 00:00:21,840 of course is the light from billions of 9 00:00:25,990 --> 00:00:24,320 light years away so the further you look 10 00:00:28,150 --> 00:00:26,000 the more you're going back towards the 11 00:00:30,710 --> 00:00:28,160 big bang and understanding how the 12 00:00:32,470 --> 00:00:30,720 universe was formed 13 00:00:35,430 --> 00:00:32,480 the webb telescope will be ground 14 00:00:37,110 --> 00:00:35,440 breaking because it has capabilities 15 00:00:38,950 --> 00:00:37,120 that are different than the hubble space 16 00:00:40,790 --> 00:00:38,960 telescope 17 00:00:42,470 --> 00:00:40,800 we have equipment that is so much more 18 00:00:44,790 --> 00:00:42,480 powerful than anything we've ever had 19 00:00:47,420 --> 00:00:44,800 before that it's almost impossible to 20 00:00:59,029 --> 00:00:47,430 tell what we will discover 21 00:01:03,830 --> 00:01:01,510 hubble's accomplishments include 22 00:01:05,429 --> 00:01:03,840 something called the deep feels 23 00:01:06,789 --> 00:01:05,439 looking out 24 00:01:08,870 --> 00:01:06,799 into space 25 00:01:11,590 --> 00:01:08,880 and collecting light sometimes for many 26 00:01:13,190 --> 00:01:11,600 days these deep feels have revealed 27 00:01:15,749 --> 00:01:13,200 visually to us 28 00:01:17,590 --> 00:01:15,759 a universe absolutely teeming with 29 00:01:20,290 --> 00:01:17,600 galaxies hundreds of billions of 30 00:01:23,590 --> 00:01:22,070 [Music] 31 00:01:25,109 --> 00:01:23,600 one of the neat things about the ultra 32 00:01:27,749 --> 00:01:25,119 deep field and one of the things that 33 00:01:29,910 --> 00:01:27,759 made it so unique was was how long it 34 00:01:31,510 --> 00:01:29,920 took us to take that image there's an 35 00:01:34,230 --> 00:01:31,520 exposure time that's expressed i think 36 00:01:36,310 --> 00:01:34,240 it's 11.2 days it's a very very long 37 00:01:38,870 --> 00:01:36,320 exposure time but probably what's more 38 00:01:42,710 --> 00:01:38,880 important is how many orbits it took us 39 00:01:45,109 --> 00:01:42,720 to do that 400 orbits of hubble data to 40 00:01:48,149 --> 00:01:45,119 take that image you only get 15 orbits a 41 00:01:49,910 --> 00:01:48,159 day to take 400 orbits 42 00:01:53,190 --> 00:01:49,920 and say we're going to observe this one 43 00:01:55,510 --> 00:01:53,200 spot in the sky for 400 orbits and the 44 00:01:57,190 --> 00:01:55,520 really unique thing about that was they 45 00:01:59,270 --> 00:01:57,200 picked a spot where there wasn't 46 00:02:01,350 --> 00:01:59,280 anything they looked and they said 47 00:02:04,230 --> 00:02:01,360 there's absolutely nothing here and they 48 00:02:06,230 --> 00:02:04,240 said you want to spend 400 hubble orbits 49 00:02:08,389 --> 00:02:06,240 looking at nothing and they said yes 50 00:02:10,150 --> 00:02:08,399 because we want to see what it can see 51 00:02:12,070 --> 00:02:10,160 and i think the results from the science 52 00:02:15,190 --> 00:02:12,080 i mean it was amazing what they saw was 53 00:02:15,200 --> 00:02:18,550 [Music] 54 00:02:22,390 --> 00:02:20,470 hubble spent two weeks taking pictures 55 00:02:23,750 --> 00:02:22,400 of empty places in sky 56 00:02:25,030 --> 00:02:23,760 and they saw they weren't empty at all 57 00:02:28,630 --> 00:02:25,040 they were thousands and thousands of 58 00:02:33,190 --> 00:02:30,949 we were amazed how many galaxies we've 59 00:02:35,589 --> 00:02:33,200 we've found and we continue to go back 60 00:02:40,229 --> 00:02:35,599 to that portion of the sky to increase 61 00:02:44,550 --> 00:02:42,949 the hubble space telescope is 62 00:02:47,030 --> 00:02:44,560 an outstanding 63 00:02:49,030 --> 00:02:47,040 time machine 64 00:02:50,949 --> 00:02:49,040 it's incredibly important for our 65 00:02:53,750 --> 00:02:50,959 studies with the hubble space telescope 66 00:02:56,869 --> 00:02:53,760 to realize that when we're looking at a 67 00:02:59,030 --> 00:02:56,879 galaxy we're seeing it as it was 68 00:03:01,270 --> 00:02:59,040 millions of years ago sometimes billions 69 00:03:03,270 --> 00:03:01,280 of years ago it's taken that long for 70 00:03:04,869 --> 00:03:03,280 the light to get to us 71 00:03:06,790 --> 00:03:04,879 what you're looking at with a telescope 72 00:03:09,270 --> 00:03:06,800 of course is the light from billions of 73 00:03:10,949 --> 00:03:09,280 light years away so the further you look 74 00:03:13,110 --> 00:03:10,959 the more you're going back towards the 75 00:03:15,910 --> 00:03:13,120 big bang and understanding how the 76 00:03:18,229 --> 00:03:15,920 universe was formed 77 00:03:21,110 --> 00:03:18,239 what hubble has revealed is that the 78 00:03:23,670 --> 00:03:21,120 universe has in fact changed over these 79 00:03:25,990 --> 00:03:23,680 billions of years of time the early 80 00:03:26,949 --> 00:03:26,000 galaxies the very distant ones as we see 81 00:03:27,750 --> 00:03:26,959 them 82 00:03:29,750 --> 00:03:27,760 are 83 00:03:32,149 --> 00:03:29,760 simple sometimes they're messy looking 84 00:03:35,190 --> 00:03:32,159 they're small they haven't had time yet 85 00:03:37,670 --> 00:03:35,200 to form that grand spiral structure 86 00:03:40,070 --> 00:03:37,680 over time we see galaxies actually 87 00:03:42,229 --> 00:03:40,080 merging with other galaxies and growing 88 00:03:44,149 --> 00:03:42,239 bigger and bigger and those mergers can 89 00:03:45,840 --> 00:03:44,159 look like train wrecks in our hubble 90 00:03:51,509 --> 00:03:45,850 images 91 00:03:53,350 --> 00:03:51,519 [Music] 92 00:03:54,630 --> 00:03:53,360 these very very deep exposures that 93 00:03:57,110 --> 00:03:54,640 hubble has been able to take we have 94 00:04:00,869 --> 00:03:57,120 seen right to the edge of the universe 95 00:04:02,470 --> 00:04:00,879 13 and a half billion years 96 00:04:04,070 --> 00:04:02,480 when hubble was first designed and 97 00:04:06,869 --> 00:04:04,080 envisioned it was never thought it could 98 00:04:08,630 --> 00:04:06,879 actually see that far out but because of 99 00:04:09,750 --> 00:04:08,640 the advances in the instruments that 100 00:04:11,910 --> 00:04:09,760 we've been able to put up on the 101 00:04:13,589 --> 00:04:11,920 telescope and also the cleverness of the 102 00:04:15,509 --> 00:04:13,599 scientists they've come up with very 103 00:04:17,430 --> 00:04:15,519 interesting observing scenarios doing 104 00:04:19,110 --> 00:04:17,440 these really deep exposures where we 105 00:04:20,310 --> 00:04:19,120 just sit there for orbit after orbit 106 00:04:22,390 --> 00:04:20,320 after orbit 107 00:04:24,100 --> 00:04:22,400 gathering the photons we've been able to 108 00:04:26,629 --> 00:04:24,110 push hubble out very very far 109 00:04:29,670 --> 00:04:26,639 [Music] 110 00:04:32,150 --> 00:04:29,680 as hubble looks out into these 111 00:04:34,310 --> 00:04:32,160 fields of galaxies we sometimes see 112 00:04:36,150 --> 00:04:34,320 clusters of galaxies these are galaxies 113 00:04:38,629 --> 00:04:36,160 that are held nearby each other by their 114 00:04:41,110 --> 00:04:38,639 mutual gravity 115 00:04:44,230 --> 00:04:41,120 these clusters are 116 00:04:47,749 --> 00:04:44,240 massive conglomerations there's so much 117 00:04:51,030 --> 00:04:47,759 mass that they have an actual observable 118 00:04:54,230 --> 00:04:51,040 impact on space time itself 119 00:04:56,070 --> 00:04:54,240 einstein predicted that mass distorts 120 00:04:58,070 --> 00:04:56,080 space but we didn't realize we could 121 00:05:00,710 --> 00:04:58,080 actually see the effects of that but 122 00:05:03,189 --> 00:05:00,720 with hubble we have been able to see 123 00:05:05,909 --> 00:05:03,199 distortions in space around clusters of 124 00:05:08,790 --> 00:05:05,919 galaxies the way we see that is when 125 00:05:11,110 --> 00:05:08,800 light from a background galaxy travels 126 00:05:13,430 --> 00:05:11,120 through that cluster of galaxies or 127 00:05:15,749 --> 00:05:13,440 around it due to this gravitational 128 00:05:18,870 --> 00:05:15,759 lensing effect the lensing also 129 00:05:20,950 --> 00:05:18,880 magnifies that background galaxy so if 130 00:05:22,870 --> 00:05:20,960 we look in some of these distorted arcs 131 00:05:24,790 --> 00:05:22,880 we can see more detail than we would 132 00:05:27,830 --> 00:05:24,800 ever have been able to see 133 00:05:31,749 --> 00:05:27,840 without gravitational lensing nature's 134 00:05:36,150 --> 00:05:33,670 there are observations where we're 135 00:05:38,550 --> 00:05:36,160 explicitly looking for the lensing and 136 00:05:41,670 --> 00:05:38,560 they're getting science out of that that 137 00:05:44,469 --> 00:05:41,680 just otherwise would just not be doable 138 00:05:45,510 --> 00:05:44,479 hubble has really taken that to a next 139 00:05:48,150 --> 00:05:45,520 level 140 00:05:49,909 --> 00:05:48,160 it's doing large amounts of astrophysics 141 00:05:55,350 --> 00:05:49,919 that it's just never been able to do 142 00:05:59,990 --> 00:05:57,510 some of what we're doing with hubble is 143 00:06:02,230 --> 00:06:00,000 to prepare for the new james webb 144 00:06:05,510 --> 00:06:02,240 telescope which we anticipate launching 145 00:06:07,510 --> 00:06:05,520 in 2021 which will be able to see 146 00:06:10,390 --> 00:06:07,520 farther into the infrared part of the 147 00:06:13,510 --> 00:06:10,400 electromagnetic spectrum that enables us 148 00:06:15,749 --> 00:06:13,520 to see some galaxies that are 149 00:06:18,150 --> 00:06:15,759 difficult for hubble to see 150 00:06:20,550 --> 00:06:18,160 because they're so far away 151 00:06:22,309 --> 00:06:20,560 that their light is traveling through us 152 00:06:24,870 --> 00:06:22,319 through expanding space and gets 153 00:06:27,189 --> 00:06:24,880 stretched out into redder wavelengths 154 00:06:28,309 --> 00:06:27,199 often far into the infrared part of the 155 00:06:30,309 --> 00:06:28,319 spectrum 156 00:06:32,790 --> 00:06:30,319 even sometimes beyond what hubble is 157 00:06:34,390 --> 00:06:32,800 able to detect well the web telescope 158 00:06:38,230 --> 00:06:34,400 will give us more information about some 159 00:06:41,590 --> 00:06:40,070 the james webb space telescope is the 160 00:06:43,189 --> 00:06:41,600 follow-on telescope after the great 161 00:06:45,189 --> 00:06:43,199 hubble telescope 162 00:06:47,800 --> 00:06:45,199 it extends the discoveries of hubble 163 00:06:49,270 --> 00:06:47,810 into the infrared spectrum region 164 00:06:50,870 --> 00:06:49,280 [Music] 165 00:06:52,390 --> 00:06:50,880 we think that the first objects that 166 00:06:54,390 --> 00:06:52,400 grew out of the big bang material 167 00:06:57,350 --> 00:06:54,400 probably happened in about 100 million 168 00:06:59,029 --> 00:06:57,360 years after the start 169 00:07:00,790 --> 00:06:59,039 and we think the webb telescope can pick 170 00:07:04,070 --> 00:07:00,800 them up they're rare they're hard to 171 00:07:07,830 --> 00:07:05,430 the farthest we've been able to see with 172 00:07:09,990 --> 00:07:07,840 the hubble telescope goes back about 173 00:07:10,950 --> 00:07:10,000 6 800 million years after the expansion 174 00:07:11,670 --> 00:07:10,960 began 175 00:07:13,589 --> 00:07:11,680 so 176 00:07:17,749 --> 00:07:13,599 we think we'll get a much much closer to 177 00:07:19,510 --> 00:07:17,759 the first objects with the web telescope 178 00:07:21,749 --> 00:07:19,520 hubble gives information that the web 179 00:07:24,309 --> 00:07:21,759 telescope cannot give about visible and 180 00:07:25,830 --> 00:07:24,319 ultraviolet emission from things in the 181 00:07:28,390 --> 00:07:25,840 universe and when we have all that 182 00:07:32,390 --> 00:07:28,400 information coming in at the same time 183 00:07:34,309 --> 00:07:32,400 it's like a banquet of scientific return 184 00:07:35,990 --> 00:07:34,319 now when we get the complete picture of 185 00:07:38,390 --> 00:07:36,000 every wavelength you can possibly see 186 00:07:40,070 --> 00:07:38,400 from ultraviolet to infrared we hope to 187 00:07:41,749 --> 00:07:40,080 have the story of the growth of the 188 00:07:44,070 --> 00:07:41,759 first galaxies from the primordial 189 00:07:46,070 --> 00:07:44,080 material so that will be a huge 190 00:07:47,990 --> 00:07:46,080 accomplishment that depends on both 191 00:07:49,909 --> 00:07:48,000 pieces of equipment the hubble telescope 192 00:07:51,830 --> 00:07:49,919 and the james webb telescope working 193 00:07:54,309 --> 00:07:51,840 together 194 00:07:55,990 --> 00:07:54,319 so astronomers are very excited about 195 00:07:57,909 --> 00:07:56,000 this probability that we'll have both 196 00:08:00,230 --> 00:07:57,919 the hubble space telescope and the webb 197 00:08:02,070 --> 00:08:00,240 telescope operating at the same time for 198 00:08:04,230 --> 00:08:02,080 quite a few years that will give us an 199 00:08:06,390 --> 00:08:04,240 abundance of new understanding about the 200 00:08:08,629 --> 00:08:06,400 universe and already right now with 201 00:08:11,430 --> 00:08:08,639 hubble we're doing preparatory 202 00:08:13,670 --> 00:08:11,440 observations for the web telescope we're 203 00:08:16,070 --> 00:08:13,680 using hubble to do things for example 204 00:08:19,510 --> 00:08:16,080 like surveying distant galaxies to find 205 00:08:21,670 --> 00:08:19,520 out which ones would be prime targets 206 00:08:23,430 --> 00:08:21,680 for the webb telescope in fact 207 00:08:25,430 --> 00:08:23,440 scientists around the world 208 00:08:26,390 --> 00:08:25,440 are proposing observations with hubble 209 00:08:28,390 --> 00:08:26,400 right now 210 00:08:30,629 --> 00:08:28,400 specifically to help us learn 211 00:08:32,550 --> 00:08:30,639 information that will be useful 212 00:08:34,949 --> 00:08:32,560 for making the best use of the web 213 00:08:39,269 --> 00:08:34,959 telescope as soon as it's launched and 214 00:08:42,389 --> 00:08:40,790 i think the hubble telescope has been 215 00:08:44,550 --> 00:08:42,399 the most productive science instrument 216 00:08:46,310 --> 00:08:44,560 ever built in astronomy there's what we 217 00:08:47,910 --> 00:08:46,320 knew before hubble and now there's what 218 00:08:49,829 --> 00:08:47,920 we know after hubble they're so 219 00:08:52,070 --> 00:08:49,839 different of course hubble has now had a 220 00:08:54,230 --> 00:08:52,080 life of 30 years so it's had a long time 221 00:08:56,630 --> 00:08:54,240 to make this revolution happen so it's 222 00:08:58,150 --> 00:08:56,640 not all at once it's a gradual 223 00:09:00,550 --> 00:08:58,160 revolution but it's still a huge 224 00:09:02,550 --> 00:09:00,560 revolution 225 00:09:04,310 --> 00:09:02,560 technology has changed dramatically over 226 00:09:06,870 --> 00:09:04,320 the 30 years of life of the hubble 227 00:09:08,550 --> 00:09:06,880 telescope so you couldn't even have 228 00:09:10,310 --> 00:09:08,560 imagined when the hubble was launched 229 00:09:12,949 --> 00:09:10,320 that we would have the wonderful cameras 230 00:09:14,870 --> 00:09:12,959 and spectrometers that we fly today 231 00:09:16,949 --> 00:09:14,880 we figured out how to send astronauts we 232 00:09:18,870 --> 00:09:16,959 trained the astronauts we figured out 233 00:09:20,150 --> 00:09:18,880 what instruments could be put in we 234 00:09:22,230 --> 00:09:20,160 figured out how to repair everything 235 00:09:24,710 --> 00:09:22,240 that went wrong on the hubble and it's 236 00:09:27,509 --> 00:09:24,720 still alive it's today 30 years after 237 00:09:29,750 --> 00:09:27,519 launch and i am so thrilled to say that 238 00:09:31,670 --> 00:09:29,760 our people were able to do that 239 00:09:33,670 --> 00:09:31,680 that's the operations team that makes 240 00:09:34,870 --> 00:09:33,680 this possible it's a miracle as far as 241 00:09:38,020 --> 00:09:34,880 i'm concerned because it didn't have to