1 00:00:00,719 --> 00:00:04,580 NARRATOR: For thousands of years, the course of exploration had been determined by staring 2 00:00:04,580 --> 00:00:09,710 toward the stars and moving forward with bold progress into the vast unknown. 3 00:00:09,710 --> 00:00:12,280 STRAUGHN: Astronomy is the oldest science. 4 00:00:12,280 --> 00:00:16,660 People have been looking up at the stars since we sort of stopped walking around on our knuckles. 5 00:00:16,660 --> 00:00:20,099 The way astronomers become interested in astronomy to begin with is just by looking at the sky. 6 00:00:20,099 --> 00:00:21,099 TYSON: If it's happening outside of our atmosphere - comets, asteroids, planets, stars, galaxies 7 00:00:21,099 --> 00:00:28,730 - cosmology, the study of the birth, life, and fate of the universe, that's what we worry 8 00:00:28,730 --> 00:00:29,730 about. 9 00:00:29,730 --> 00:00:39,380 And we use the laws of physics as discovered here on Earth and apply them to phenomenon 10 00:00:39,380 --> 00:00:40,690 in the cosmos. 11 00:00:40,690 --> 00:00:47,500 NARRATOR: Humanity reached out and explored farther and farther, until a place once reserved 12 00:00:47,500 --> 00:00:55,300 for the imagination and the distant view of a telescope's lens was now walked upon by 13 00:00:55,300 --> 00:00:56,300 humankind. 14 00:00:56,300 --> 00:00:59,220 Music ARMSTRONG: That's one small step for man. 15 00:00:59,220 --> 00:01:03,910 MUSGRAVE: I had to run outside and look at the moon and say, "You see that thing? 16 00:01:03,910 --> 00:01:05,489 Well, there's people on there right now." 17 00:01:05,489 --> 00:01:08,550 ARMSTRONG: One giant leap for mankind. 18 00:01:08,550 --> 00:01:14,070 NARRATOR: It was 1969, as ticker tape fell from the sky and rock and roll blazed across 19 00:01:14,070 --> 00:01:16,850 the American landscape. 20 00:01:19,580 --> 00:01:18,210 Music 21 00:01:19,580 --> 00:01:25,030 MIKULSKI: America loves discovery. 22 00:01:25,030 --> 00:01:33,200 We just--that's in our national DNA. 23 00:01:33,200 --> 00:01:38,400 When Lewis and Clark was sent out on their expedition by a president of the United States, 24 00:01:38,400 --> 00:01:40,270 it was called discovery. 25 00:01:40,270 --> 00:01:43,140 And that's when we send out our astronauts. 26 00:01:43,140 --> 00:01:48,650 That's when we've now sent out a space telescope, to go where no other telescopes had gone before 27 00:01:48,650 --> 00:01:51,490 and to see things that had never been seen. 28 00:01:51,490 --> 00:01:53,200 MOUNTAIN: So, astronomy is about exploration. 29 00:01:53,200 --> 00:01:54,799 It's what NASA does. 30 00:01:54,799 --> 00:01:55,799 NASA explores. 31 00:01:55,799 --> 00:02:00,490 NARRATOR: A telescope that would go beyond the atmospheric limits of the Earth; it's 32 00:02:00,490 --> 00:02:01,900 a simple problem. 33 00:02:01,900 --> 00:02:06,650 When you desire to look at objects far away, there are limitations. 34 00:02:06,650 --> 00:02:10,479 Through technological advancement, you can remove these limitations. 35 00:02:10,479 --> 00:02:14,590 The handheld telescope supersedes the naked eye. 36 00:02:14,590 --> 00:02:19,900 That small glass telescope was replaced by larger models, then mirrors are added and 37 00:02:19,900 --> 00:02:22,080 then more advancements. 38 00:02:22,080 --> 00:02:28,640 As the size and capacities of the device grow so do the discoveries, from mapping a few 39 00:02:28,640 --> 00:02:34,200 heavenly bodies circling the sun to seeing beyond ours and into other galaxies. 40 00:02:34,200 --> 00:02:38,590 GARCIA: Before we ever put, you know, men in space, astronomers are already thinking 41 00:02:38,590 --> 00:02:43,880 about getting, you know, off of the planet above the atmosphere in order to get the crystal 42 00:02:43,880 --> 00:02:44,920 clear view. 43 00:02:44,920 --> 00:02:50,160 NARRATOR: But, obstacles such as atmosphere, clouds, light pollution, and even our own 44 00:02:50,160 --> 00:02:56,190 sun's brightness stand in our way of seeing things clearly or watching around the clock. 45 00:02:56,190 --> 00:02:57,290 The solution? 46 00:02:57,290 --> 00:03:00,239 A non ground-based robotic observatory. 47 00:03:00,239 --> 00:03:05,060 TYSON: Well, there's that famous song, twinkle, twinkle little star, how I wonder what you 48 00:03:05,060 --> 00:03:06,060 are. 49 00:03:06,060 --> 00:03:11,569 That left a lot of people thinking that twinkling stars is exactly what astronomers want, BUT 50 00:03:11,569 --> 00:03:13,849 it is the opposite of what they want. 51 00:03:13,849 --> 00:03:17,770 MASSIMINO: One thing I've noticed as an astronaut is that when you get into space and you look 52 00:03:17,770 --> 00:03:20,300 at stars, they don't twinkle like they do on Earth. 53 00:03:20,300 --> 00:03:23,520 What you're seeing in twinkle, twinkle little star is because the light is coming through 54 00:03:23,520 --> 00:03:26,660 the atmosphere and causing them to twinkle. 55 00:03:26,660 --> 00:03:28,890 TYSON: Starlight does not twinkle on its own. 56 00:03:28,890 --> 00:03:31,220 It twinkles coming through Earth's atmosphere. 57 00:03:31,220 --> 00:03:36,370 And it's that bump, AND grind and jiggle and wiggle, moving through the layers, different 58 00:03:36,370 --> 00:03:43,210 temperature layers of the atmosphere, that disrupts the precision of your imaging of 59 00:03:43,210 --> 00:03:44,210 the night sky. 60 00:03:44,210 --> 00:03:48,670 MASSIMINO: THE space telescope was thought of originally by--Lyman Spitzer had the idea 61 00:03:48,670 --> 00:03:53,090 that if you could get above the atmosphere you could see a lot more clearly. 62 00:03:53,090 --> 00:03:58,090 NARRATOR: Renowned astrophysicist Lyman Spitzer gathered support in the astronomy community 63 00:03:58,090 --> 00:04:04,409 for a large space telescope, which later on would be named in honor of astronomer Edwin 64 00:04:04,409 --> 00:04:05,970 Powell Hubble. 65 00:04:05,970 --> 00:04:08,930 It was Hubble who discovered the universe was expanding. 66 00:04:08,930 --> 00:04:15,159 Through the lens of a hundred inch telescope, he made calculations that the universe was 67 00:04:15,159 --> 00:04:20,160 made up of billions of galaxies, well beyond the visible Milky Way. 68 00:04:20,160 --> 00:04:24,790 His observations pointed out that these galaxies seemed to be moving away from us. 69 00:04:24,790 --> 00:04:28,370 IDLE: (Singing) We're 30,000 light years from galactic central point. 70 00:04:28,370 --> 00:04:30,920 We go around every 200 million years. 71 00:04:30,920 --> 00:04:37,300 And our galaxy is only one of millions of billions in this amazing and expanding universe. 72 00:04:37,300 --> 00:04:46,000 NARRATOR: Using known stars to calculate distances between galaxies, Edwin Hubble confirmed this 73 00:04:46,000 --> 00:04:47,000 galactic retreat. 74 00:04:47,000 --> 00:04:48,900 WEILER: Now, let's take it ever further back. 75 00:04:48,900 --> 00:04:53,530 A lot of people don't realize this, but the Huddle Space Telescope was dreamed up by Lyman 76 00:04:53,530 --> 00:04:56,150 Spitzer back in 1948. 77 00:04:56,150 --> 00:04:59,990 And he wrote a paper on the advantages of putting a telescope in space to get above 78 00:04:59,990 --> 00:05:02,360 the atmosphere, etc. 79 00:05:02,360 --> 00:05:07,240 And that started a lifelong--a quest by Lyman to get the Hubble Space Telescope up there. 80 00:05:07,240 --> 00:05:12,280 He fought with the Congress with the able help of John Bahcall, who I consider the granduncle 81 00:05:12,280 --> 00:05:14,419 of Hubble, both at Princeton. 82 00:05:14,419 --> 00:05:20,850 And he and John fought with Congress and convinced Congress to provide the early funding in the 83 00:05:20,850 --> 00:05:21,850 late '70s. 84 00:05:21,850 --> 00:05:27,151 ALTMAN: It looks out at galaxies and brings them to us, crosses vast distances that we 85 00:05:27,151 --> 00:05:28,990 don't have the technology to travel. 86 00:05:28,990 --> 00:05:34,259 But, we can travel in a time machine using the Huddle to show us what the universe was 87 00:05:34,259 --> 00:05:40,000 like 13 billion years ago with the light that it pulls in, and also exposes us to just how 88 00:05:40,000 --> 00:05:46,710 vast the universe really is, with billions and billions of galaxies full of billions 89 00:05:46,710 --> 00:05:47,710 of stars. 90 00:05:47,710 --> 00:05:52,979 NARRATOR: To build a telescope in many ways is a decision to build a time machine. 91 00:05:52,979 --> 00:06:00,760 The United States Congress approved a large space telescope in 1977, sparking work to 92 00:06:00,760 --> 00:06:06,330 begin on creating this large, complex, and capable orbiting telescope. 93 00:06:06,330 --> 00:06:08,800 LECKRONE: Well, it wasn't easy. 94 00:06:08,800 --> 00:06:15,050 It was a long slog, difficult politically at first to have it accepted and funded in 95 00:06:15,050 --> 00:06:16,580 the US Congress. 96 00:06:16,580 --> 00:06:18,220 And then, technically it was difficult. 97 00:06:18,220 --> 00:06:25,389 CEPOLLINA: We need to find a new way and the new technology to approach the development 98 00:06:25,389 --> 00:06:33,590 of expensive satellites that would go to orbit, that could somehow take advantage of human 99 00:06:33,590 --> 00:06:37,220 repair and perhaps a space transportation system. 100 00:06:37,220 --> 00:06:42,320 NARRATOR: An advanced international observatory with multiple tools, multiple cameras, instruments, 101 00:06:42,320 --> 00:06:43,320 and capabilities. 102 00:06:43,320 --> 00:06:45,570 MASSIMINO: It's an amazing machine. 103 00:06:45,570 --> 00:06:51,430 It can orbit around the Earth at 17,500 miles an hour. 104 00:06:51,430 --> 00:06:55,500 And the reason it can take all these great images is not only because it's above the 105 00:06:55,500 --> 00:07:03,020 atmosphere, but because it can very steadily hold its gaze on an object in space. 106 00:07:03,020 --> 00:07:10,880 ROMAN: Aerospace companies came in with proposals for a space telescope, a large space telescope. 107 00:07:10,880 --> 00:07:15,139 All of them had men riding around with the telescope. 108 00:07:15,139 --> 00:07:17,590 This was the last thing that astronomers wanted. 109 00:07:17,590 --> 00:07:22,250 In the first place, we were trying to get rid of the atmosphere, and a man needs an 110 00:07:22,250 --> 00:07:23,250 atmosphere. 111 00:07:23,250 --> 00:07:25,630 In the second place, a man's going to wiggle. 112 00:07:25,630 --> 00:07:31,260 I don't care how careful he is, when you're taking a half hour or an hour exposures, he's 113 00:07:31,260 --> 00:07:33,170 going to wiggle sometimes. 114 00:07:33,170 --> 00:07:37,500 And when you wiggle in space, the spacecraft wiggles the opposite way. 115 00:07:37,500 --> 00:07:42,240 NARRATOR: A globally connected telescope, built through a partnership with the European 116 00:07:42,240 --> 00:07:47,419 Space Agency, which would look into the stars well beyond international borders. 117 00:07:47,419 --> 00:07:49,009 SCOLESE: It takes a lot of people. 118 00:07:49,009 --> 00:07:54,500 You know, it takes people that--obviously the scientists to conceive of it. 119 00:07:54,500 --> 00:07:58,880 It takes engineers to design it and build it and test it. 120 00:07:58,880 --> 00:08:02,051 It takes technicians to actually build it. 121 00:08:02,051 --> 00:08:07,510 It takes the people to keep the rooms clean, the facilities up and operating. 122 00:08:07,510 --> 00:08:14,270 So, it takes people from every walk of life in order to do it, every skill set that you 123 00:08:14,270 --> 00:08:15,270 can think of. 124 00:08:15,270 --> 00:08:20,710 NARRATOR: To then place this telescope into orbit to send back to us the data that scientists 125 00:08:20,710 --> 00:08:23,460 needed, unobstructed and unencumbered. 126 00:08:23,460 --> 00:08:28,130 WISEMAN: And when it was launched in 1990, it really opened a new vista on the whole 127 00:08:28,130 --> 00:08:32,550 universe simply by enabling us to get sharper images above the atmosphere. 128 00:08:32,550 --> 00:08:37,119 MUSGRAVE: Humanity has always looked out there, to the heavens, to get the meaning and the 129 00:08:37,119 --> 00:08:39,089 hope of their life here. 130 00:08:39,089 --> 00:08:42,739 So, you look out there for what's going on down here. 131 00:08:42,739 --> 00:08:48,249 People understood that about Hubble before we carried it up there, and so that's the 132 00:08:48,249 --> 00:08:49,249 magic. 133 00:08:49,249 --> 00:08:53,839 Bolden: And at the time, I was the--what we called the PLT, or the pilot for the Hubble 134 00:08:53,839 --> 00:08:58,209 deploy mission, which was STS-31 aboard the Shuttle Discovery. 135 00:08:58,209 --> 00:09:02,499 All of us in the crew had a certain feeling of exhilaration and excitement. 136 00:09:02,499 --> 00:09:06,160 We knew that this was going to be an important mission. 137 00:09:06,160 --> 00:09:09,820 UNIDENTIFIED: Two, one, and liftoff of the Space Shuttle Discovery with the Hubble Space 138 00:09:09,820 --> 00:09:14,070 Telescope, our window on the universe. 139 00:09:14,070 --> 00:09:20,089 NARRATOR: On the 25th of April in 1990, the Space Shuttle Discovery, piloted by a future 140 00:09:20,089 --> 00:09:24,940 administrator of NASA, deployed the Hubble Space Telescope into an orbit around Earth. 141 00:09:24,940 --> 00:09:25,940 UNIDENTIFIED: Discovery, Houston. 142 00:09:25,940 --> 00:09:32,001 You have a go to open the doors. 143 00:09:32,001 --> 00:09:33,001 UNIDENTIFIED: Roger, Houston. 144 00:09:33,001 --> 00:09:37,839 BOLDEN: The mission itself was pretty intense in training, because we had to train for any 145 00:09:37,839 --> 00:09:42,160 number of contingencies that we all prayed would not happen. 146 00:09:42,160 --> 00:09:43,420 UNIDENTIFIED: Morning, Story. 147 00:09:43,420 --> 00:09:44,420 REEVES: Good morning, Discovery. 148 00:09:44,420 --> 00:09:49,550 Good morning from Bill Reeves and the Orbit One Team, and you got a go for HST deploy 149 00:09:49,550 --> 00:09:50,550 ops. 150 00:09:50,550 --> 00:09:52,480 UNIDENTIFIED: And Houston, Discovery. 151 00:09:52,480 --> 00:09:56,589 The transfer to internal power is complete. 152 00:09:56,589 --> 00:10:01,059 The umbilical is dead-faced, and we'll be standing by for your go for umbilical release. 153 00:10:01,059 --> 00:10:04,172 MUSGRAVE It was the people's instrument long before we launched it. 154 00:10:04,172 --> 00:10:12,490 So, and like I said, I was the lead communicator in the carry-up and deploy mission, STS-31, 155 00:10:12,490 --> 00:10:14,690 but it was the people's machine then. 156 00:10:14,690 --> 00:10:18,079 UNIDENTIFIED CHATTER BOLDEN: Ironically, one of those contingencies 157 00:10:18,079 --> 00:10:21,410 was failure of the solar array to deploy. 158 00:10:21,410 --> 00:10:25,809 It took us much of the day for the flight control team to say, "Look, we--this is not 159 00:10:25,809 --> 00:10:26,809 working out. 160 00:10:26,809 --> 00:10:29,189 We don't think we're going to get the solar arrays deployed." 161 00:10:29,189 --> 00:10:37,709 All of a sudden this great experience turned out to just go, "This is not good," when the 162 00:10:37,709 --> 00:10:40,399 ground control team called and said, "Stop, stop. 163 00:10:40,399 --> 00:10:42,170 We think we found a solution. 164 00:10:42,170 --> 00:10:44,809 You know, just stop where you are. 165 00:10:44,809 --> 00:10:45,809 We're going to try this." 166 00:10:45,809 --> 00:10:49,399 And they did and it worked, and so we went ahead and deployed. 167 00:10:49,399 --> 00:10:51,410 UNIDENTIFIED: The deploy activity so far is going very smoothly. 168 00:10:51,410 --> 00:10:53,299 BOLDEN: Okay, they copy you, Story. 169 00:10:53,299 --> 00:10:54,559 And we're at five--. 170 00:10:54,559 --> 00:10:59,809 BOLDEN: --It all worked out because of the incredible work of the combination of the 171 00:10:59,809 --> 00:11:06,910 crew onboard, the flight control team in Houston, but most especially very smart people at the 172 00:11:06,910 --> 00:11:13,079 Goddard Space Flight Center who actually knew the Hubble Space Telescope about as well as 173 00:11:13,079 --> 00:11:14,369 any people around. 174 00:11:14,369 --> 00:11:15,369 UNIDENTIFIED: J.C.? 175 00:11:15,369 --> 00:11:16,369 UNIDENTIFIED: Go. 176 00:11:16,369 --> 00:11:17,379 UNIDENTIFIED: Network go. 177 00:11:17,379 --> 00:11:19,100 Payloads, waiting on you. 178 00:11:19,100 --> 00:11:20,389 UNIDENTIFIED: Flight payloads. 179 00:11:20,389 --> 00:11:21,679 We are go. 180 00:11:21,679 --> 00:11:22,970 UNIDENTIFIED: Go ahead. 181 00:11:22,970 --> 00:11:25,410 CapCom, we have a go for release. 182 00:11:25,410 --> 00:11:27,989 UNIDENTIFIED: Discovery, go for Hubble release. 183 00:11:27,989 --> 00:11:29,279 BOLDEN: Houston, Discovery. 184 00:11:29,279 --> 00:11:30,999 MUSGRAVE: Go ahead, Charlie. 185 00:11:30,999 --> 00:11:32,290 BOLDEN: Okay, Story. 186 00:11:32,290 --> 00:11:34,009 We've been taking marks. 187 00:11:34,009 --> 00:11:38,970 Residuals and ratios look good, and we'd like to go ahead and go to the filter state. 188 00:11:38,970 --> 00:11:41,499 MUSGRAVE: We concur, Charlie. 189 00:11:41,499 --> 00:11:46,660 WEILER: We launched Hubble April 24th, 1990, and we were all on top of the world. 190 00:11:46,660 --> 00:11:52,269 Many of us astronomers had never done an interview, and suddenly we were on Today and Nightline 191 00:11:52,269 --> 00:11:54,920 and Good Morning America, etc. 192 00:11:54,920 --> 00:11:56,489 And the media loved us. 193 00:11:56,489 --> 00:11:58,889 The Hubble was big news across the country. 194 00:11:58,889 --> 00:12:00,149 Everybody loved us. 195 00:12:00,149 --> 00:12:05,299 UNIDENTIFIED: And it's here, 381 miles up, where the telescope is to be place in orbit 196 00:12:05,299 --> 00:12:06,299 tomorrow. 197 00:12:06,299 --> 00:12:08,160 So, the celebration will continue. 198 00:12:08,160 --> 00:12:09,399 UNIDENTIFIED: Oh, yes. 199 00:12:09,399 --> 00:12:12,850 Hey, I get to launch something here, guys. 200 00:12:12,850 --> 00:12:17,819 UNIDENTIFIED: Westfall’s family, neighbors, and colleagues who had traveled here from 201 00:12:17,819 --> 00:12:19,759 California toasted the telescope. 202 00:12:19,759 --> 00:12:23,859 BRAD BIRD: The science that is astronomy would never be the same. 203 00:12:23,859 --> 00:12:28,179 STRAUGHN: When people think about a telescope here on Earth, they think about a mirror with 204 00:12:28,179 --> 00:12:29,439 a tube around it. 205 00:12:29,439 --> 00:12:31,540 And that's exactly what Hubble is. 206 00:12:31,540 --> 00:12:35,889 It's a huge mirror with a huge tube around it in space. 207 00:12:35,889 --> 00:12:39,649 And the--of course, the purpose of Hubble is to take these beautiful images that we 208 00:12:39,649 --> 00:12:40,649 learn about. 209 00:12:40,649 --> 00:12:45,670 And so, the images are recorded on cameras, and then the data is sent back to Earth for 210 00:12:45,670 --> 00:12:46,670 us to study. 211 00:12:46,670 --> 00:12:51,429 NARRATOR: The Hubble Space Telescope powered up, all systems nominal, and the data began 212 00:12:51,429 --> 00:12:56,799 to stream in; images of far off distances, galaxies, and stars, but there was something 213 00:12:56,799 --> 00:12:57,799 wrong. 214 00:12:57,799 --> 00:13:02,579 The magnificent space observatory's imagery was not clear, not crisp. 215 00:13:02,579 --> 00:13:06,619 BOLDEN: As a member of the deploy crew, we had come back, done our debrief, and, you 216 00:13:06,619 --> 00:13:07,619 know, we had done our job. 217 00:13:07,619 --> 00:13:08,670 And so, we were happy. 218 00:13:08,670 --> 00:13:13,069 We thought everything was okay until the word came that, ah, we saw the first light images. 219 00:13:13,069 --> 00:13:18,059 And to the amateur like me, it looked great because we had made this great discovery right 220 00:13:18,059 --> 00:13:22,230 off the bat; what we thought was a single star turned out to be a binary star, when 221 00:13:22,230 --> 00:13:25,079 we learned that no, it's not really that good an image. 222 00:13:25,079 --> 00:13:27,589 It's kind of blurred because we have this thing. 223 00:13:27,589 --> 00:13:33,639 FRANK CEPOLLINA: From an agency perspective and from a public perspective and a Congressional 224 00:13:33,639 --> 00:13:35,519 perspective, it was doom and gloom. 225 00:13:35,519 --> 00:13:42,359 MIKULSKI: Working on a bipartisan basis, we used the best tools to identify was this a 226 00:13:42,359 --> 00:13:48,980 techno turkey that we would just bag as a terrible mistake and say bye-bye boondoggle, 227 00:13:48,980 --> 00:13:51,180 or were we really going to try to fix it? 228 00:13:51,180 --> 00:13:56,639 WEILER: Couldn't get the telescope focused, had trouble pointing it sometimes, and that 229 00:13:56,639 --> 00:14:01,250 went on until about early June when people, smart people, finally figured out that what 230 00:14:01,250 --> 00:14:02,709 we had was a spherical aberration. 231 00:14:02,709 --> 00:14:04,529 CEPOLLINA: The mirror was polished incorrectly. 232 00:14:04,529 --> 00:14:06,369 And it wasn't by much. 233 00:14:06,369 --> 00:14:09,749 It was half the thickness of a human hair across 100 inches. 234 00:14:09,749 --> 00:14:17,169 You know, you can try to imagine what--how much sag something that weighed 2,300 pounds 235 00:14:17,169 --> 00:14:18,169 would have. 236 00:14:18,169 --> 00:14:24,540 And yet, we were off by half the thickness of a human hair from center to edge. 237 00:14:24,540 --> 00:14:30,639 And that's pretty astounding, that, you know, we could come so close and yet not make it. 238 00:14:30,639 --> 00:14:34,439 WEILER: The mirror was still a perfect smooth curve, but it had the wrong prescription. 239 00:14:34,439 --> 00:14:36,899 It wasn't the right curve. 240 00:14:36,899 --> 00:14:40,610 Just like my eye is a perfectly good eye, it's got a smooth curve to it, but it's the 241 00:14:40,610 --> 00:14:41,739 wrong prescription. 242 00:14:41,739 --> 00:14:43,939 Light doesn't come to a focus at the right spot. 243 00:14:43,939 --> 00:14:45,699 So, how do we fix it? 244 00:14:45,699 --> 00:14:50,169 Well, we fix it with corrective lenses, the opposite prescription. 245 00:14:50,169 --> 00:14:56,269 And that's what we talked about on the famous press conference of June 27th, 1990, where 246 00:14:56,269 --> 00:15:00,899 I had the unique honor of explaining to the American people and the press that Hubble 247 00:15:00,899 --> 00:15:02,879 wouldn't be doing the science we had promised. 248 00:15:02,879 --> 00:15:09,119 WEILER: I'm going to try to give you a perspective on the short term ramifications of this particular 249 00:15:09,119 --> 00:15:14,869 issue and also the long term ramifications in terms of what we can do, the science we 250 00:15:14,869 --> 00:15:20,970 can do, the science we won't be able to do for a while in the short term, and most importantly, 251 00:15:20,970 --> 00:15:23,889 the solutions to this problem in the future. 252 00:15:23,889 --> 00:15:28,559 NARRATOR: Decades of planning and hope seemed extinguished by a blurring spherical aberration 253 00:15:28,559 --> 00:15:30,429 in Hubble's primary mirror. 254 00:15:30,429 --> 00:15:36,139 WEILER: We feel that we can characterize the problem, this spherical aberration problem, 255 00:15:36,139 --> 00:15:40,579 well enough that we can take advantage of an insurance policy that we haven't talked 256 00:15:40,579 --> 00:15:43,239 much about and that hasn't been in the press much. 257 00:15:43,239 --> 00:15:46,449 And that is we started a long time ago to plan a maintenance program. 258 00:15:46,449 --> 00:15:51,459 GRUNSFELD: The truly remarkable feature of the Hubble Space Telescope is that it was 259 00:15:51,459 --> 00:15:54,350 designed to be upgraded and fixed. 260 00:15:54,350 --> 00:15:58,569 NARRATOR: On Earth, you'd order a replacement part and correct the problem when the shipment 261 00:15:58,569 --> 00:15:59,569 arrived. 262 00:15:59,569 --> 00:16:06,819 But, Hubble was over 340 miles from the Earth's surface, moving at nearly 18,000 miles per 263 00:16:06,819 --> 00:16:07,819 hour. 264 00:16:07,819 --> 00:16:09,380 You'd need a special repair team. 265 00:16:09,380 --> 00:16:15,079 MUSGRAVE: The team comes together through multiple domains, multiple disciplines, and 266 00:16:15,079 --> 00:16:17,739 multiple organizations, multiple divisions. 267 00:16:17,739 --> 00:16:22,639 You got to get a job done, and NASA is absolutely expertise on this. 268 00:16:22,639 --> 00:16:28,680 When you got to get the job done, the team comes from many different places. 269 00:16:28,680 --> 00:16:32,699 SEMBACH: When Hubble was first launched, it had the spherical aberration on its primary 270 00:16:32,699 --> 00:16:35,860 mirror, so the prescription for the mirror wasn't right. 271 00:16:35,860 --> 00:16:41,259 It took a team of people to figure out what that prescription actually was in practice 272 00:16:41,259 --> 00:16:45,359 as opposed to what it should have been, and then people to figure out how to actually 273 00:16:45,359 --> 00:16:49,489 solve Hubble's blurry vision at the time. 274 00:16:49,489 --> 00:16:59,819 This institute and NASA and its contractors figured out a way to put together a prescription 275 00:16:59,819 --> 00:17:03,009 for correcting that spherical aberration. 276 00:17:03,009 --> 00:17:08,290 MUSGRAVE: After those two failures, the big boss came over and looked at me and said, 277 00:17:08,290 --> 00:17:09,500 "Story, fix it." 278 00:17:09,500 --> 00:17:10,980 Okay, I'll fix it. 279 00:17:10,980 --> 00:17:12,600 UNIDENTIFIED: Two, one. 280 00:17:12,600 --> 00:17:16,990 And we have liftoff, liftoff of the Space Shuttle Endeavor on an ambitious mission to 281 00:17:16,990 --> 00:17:18,660 service the Hubble Space Telescope. 282 00:17:18,660 --> 00:17:23,429 MUSGRAVE: The real magic on the Hubble mission is almost 40 hours of spacewalking, and we 283 00:17:23,429 --> 00:17:25,079 had almost no surprises. 284 00:17:25,079 --> 00:17:27,389 We had 13 major systems to fix. 285 00:17:27,389 --> 00:17:31,299 And day after day we just kept working away getting the system fixed, and they'd tell 286 00:17:31,299 --> 00:17:35,970 us this one is up and running and it's fixed. 287 00:17:35,970 --> 00:17:39,830 And we kept on going through five days. 288 00:17:39,830 --> 00:17:44,220 And finally we finished the job and, hey, it's totally restored. 289 00:17:44,220 --> 00:17:49,340 MOUNTAIN: Because astronauts from NASA have been able to go back and refurbish it, put 290 00:17:49,340 --> 00:17:53,429 in new instruments, repair it, and so that 25 years has made it an increasingly more 291 00:17:53,429 --> 00:17:54,429 powerful telescope. 292 00:17:54,429 --> 00:17:58,460 And it's the fact the Hubble is so powerful today which is so remarkable. 293 00:17:58,460 --> 00:18:03,309 After 25 years, it's basically 10 to 100 times more powerful than when it was first launched. 294 00:18:03,309 --> 00:18:07,600 GRUNSFELD: Crew members, women and men in white spacesuits rode to the recue like a 295 00:18:07,600 --> 00:18:08,880 great Western. 296 00:18:08,880 --> 00:18:14,180 And so, this was a huge deal for me personally as an astronomer, astrophysicist, and astronaut, 297 00:18:14,180 --> 00:18:19,279 to have the privilege of going to Hubble on my first mission in 1999. 298 00:18:19,279 --> 00:18:22,480 GOOD: Like taking the car in for an oil change, rotate the tires. 299 00:18:22,480 --> 00:18:24,230 So, we were changing out batteries. 300 00:18:24,230 --> 00:18:29,549 We were changing out the gyros, things that just made the telescope work. 301 00:18:29,549 --> 00:18:33,909 MUSGRAVE: So, you have a satellite out there, and you got to maintain its attitude and you 302 00:18:33,909 --> 00:18:38,220 got to maneuver to point very closely. 303 00:18:38,220 --> 00:18:42,179 The only ultimate force that you impose on the machine is magnets. 304 00:18:42,179 --> 00:18:47,540 Now, as Hubble goes around the Earth, here's the magnetic field of Earth. 305 00:18:47,540 --> 00:18:54,820 And the magnetometers, which I replaced, those magnetometers, they sense where the magnetic 306 00:18:54,820 --> 00:18:59,789 field of the Earth is, and the computers say, "Okay, I'm going to turn these magnets on 307 00:18:59,789 --> 00:19:00,789 or off. 308 00:19:00,789 --> 00:19:02,360 And that's the way I'm going to control Hubble attitude." 309 00:19:02,360 --> 00:19:05,789 SEMBACH: Remember, up in space, you know, there isn't anything for Hubble to push against, 310 00:19:05,789 --> 00:19:09,289 so it has to push against something internal like these spinning wheels. 311 00:19:09,289 --> 00:19:15,910 FOALE: I did a mission to the Hubble Space Telescope, and it was a--it wasn't really 312 00:19:15,910 --> 00:19:16,970 a refurbishment. 313 00:19:16,970 --> 00:19:25,309 It was a rescue mission, because the Hubble Telescope uses gyroscopes to determine how 314 00:19:25,309 --> 00:19:30,000 it's moving and how to point, with absolutely no motion, at a star. 315 00:19:30,000 --> 00:19:32,549 And those gyroscopes, six of them, were failing. 316 00:19:32,549 --> 00:19:37,190 And then, by the time we got there, only one, I think, was working. 317 00:19:37,190 --> 00:19:44,009 And so, it was a dead telescope at that point, and our role on that mission was to basically 318 00:19:44,009 --> 00:19:45,769 repair the Hubble Telescope. 319 00:19:45,769 --> 00:19:50,870 It was a real repair mission, just like the first repair mission to change the optics. 320 00:19:50,870 --> 00:19:54,929 If I had messed that up, I would be the one that had broken the telescope forever. 321 00:19:54,929 --> 00:19:59,139 MCARTHUR: This amazing telescope with all this history and, you know, what if I wreck 322 00:19:59,139 --> 00:20:00,139 it? 323 00:20:00,139 --> 00:20:01,139 What if I do something bad? 324 00:20:01,139 --> 00:20:04,070 GRUNSFELD: Then I got the opportunity to go a second time as the payload commander on 325 00:20:04,070 --> 00:20:05,740 STS-109. 326 00:20:05,740 --> 00:20:10,769 And when we actually were doing the spacewalks and I went out and shook hands with Mr. Hubble, 327 00:20:10,769 --> 00:20:16,160 the telescope, you know, holding on to the side, I truly felt like, you know, this was 328 00:20:16,160 --> 00:20:19,250 my partner and that we were here, you know, to help. 329 00:20:19,250 --> 00:20:22,940 REZAC: I guess that's part of the excitement of having worked a Hubble mission, because 330 00:20:22,940 --> 00:20:27,710 you know you've got the best team on the ground, the best crew upstairs. 331 00:20:27,710 --> 00:20:31,059 It's exciting, but there is a level of confidence you're going to pull through this. 332 00:20:31,059 --> 00:20:32,940 MCARTHUR: It's incredible, the things that they can come up with. 333 00:20:32,940 --> 00:20:36,659 And they have the time and the resources to develop that here, and then we take, you know, 334 00:20:36,659 --> 00:20:40,160 sort of the best solution up with us to implement in space. 335 00:20:40,160 --> 00:20:41,160 There is it. 336 00:20:41,160 --> 00:20:42,429 It looks exactly the way it's supposed to look. 337 00:20:42,429 --> 00:20:47,712 It's exactly where it's supposed to be and I'm just going to reach over and grab it. 338 00:20:47,712 --> 00:20:48,712 So, it was a really good feeling. 339 00:20:48,712 --> 00:20:52,919 And what we did after we grappled the telescope and put it in the payload bay was, every day 340 00:20:52,919 --> 00:20:57,169 that the spacewalks were going on, which was the five days after we grappled the telescope, 341 00:20:57,169 --> 00:21:00,730 the two guys go outside and one of them is pretty much always on the end of the arm. 342 00:21:00,730 --> 00:21:01,730 Unidentified: Go on three, bueno. 343 00:21:01,730 --> 00:21:02,730 GOOD: Copy. 344 00:21:02,730 --> 00:21:03,730 Go three. 345 00:21:03,730 --> 00:21:04,730 Unidentified: So, we'd drive them around and put them into position to do their work. 346 00:21:04,730 --> 00:21:05,730 Unidentified: You are clear to continue and increase the rate of your--. 347 00:21:05,730 --> 00:21:06,730 UNIDENTIFIED: --Yep. 348 00:21:06,730 --> 00:21:07,730 You can increase the rate, Megan. 349 00:21:07,730 --> 00:21:08,730 MCARTHUR: Copy, picking up the rate. 350 00:21:08,730 --> 00:21:11,030 Unidentified Man: Oh, what a beautiful view. 351 00:21:11,030 --> 00:21:19,710 MCARTHUR: They'd ask me to bring them in closer or move them by the telescope. 352 00:21:19,710 --> 00:21:23,240 I'd have to ask them, "Hey, you need to check and verify how much space do I have." 353 00:21:23,240 --> 00:21:26,570 And of course, their mind is on their job, the instrument that they're holding, the tools, 354 00:21:26,570 --> 00:21:27,570 whatever. 355 00:21:27,570 --> 00:21:30,539 And so, having to work that coordination, training really helps there. 356 00:21:30,539 --> 00:21:34,370 But, it is--it's delicate in the sense of you don't want to hurt the hardware, you don't 357 00:21:34,370 --> 00:21:36,330 want to hurt the person, and you certainly don't want to hurt the telescope. 358 00:21:36,330 --> 00:21:38,600 Unidentified Man: Okay, you can stop there, Megan. 359 00:21:38,600 --> 00:21:39,740 MCARTHUR: Motion stopped, check. 360 00:21:39,740 --> 00:21:40,870 Unidentified Man: Thank you. 361 00:21:40,870 --> 00:21:45,370 GOOD: It was 19 years old at the time when we went up there, and the batteries were original 362 00:21:45,370 --> 00:21:46,480 equipment. 363 00:21:46,480 --> 00:21:50,399 And so, they're charging and discharging, you know, like your--think about your phone, 364 00:21:50,399 --> 00:21:51,399 your cell phone. 365 00:21:51,399 --> 00:21:54,039 You know, you're lucky to get a year or two out of that battery, right? 366 00:21:54,039 --> 00:21:57,380 So, this is original batteries, so we replaced the batteries. 367 00:21:57,380 --> 00:21:58,539 Those are still working great. 368 00:21:58,539 --> 00:22:03,870 But, then some of the more interesting parts were actually replacing some of the science 369 00:22:03,870 --> 00:22:04,870 instruments. 370 00:22:04,870 --> 00:22:09,429 So, we took up a new camera and a new spectrograph and put those in. 371 00:22:09,429 --> 00:22:12,330 And then, we also fixed some broken instruments up there. 372 00:22:12,330 --> 00:22:15,210 There was a broken camera and a broken spectrograph. 373 00:22:15,210 --> 00:22:18,850 These are the science instruments so that when the light comes in the telescope, these 374 00:22:18,850 --> 00:22:23,910 are the things that take the pictures and do all the science for the--you know, for 375 00:22:23,910 --> 00:22:24,910 the astronomers and everybody back here on Earth. 376 00:22:24,910 --> 00:22:30,450 JOHNSON: The breaking off of one of the hand tools that Massimino--Mike Massimino had to 377 00:22:30,450 --> 00:22:31,450 do. 378 00:22:31,450 --> 00:22:32,450 Unidentified Man: Houston, you ready for this? 379 00:22:32,450 --> 00:22:33,450 Unidentified Man: Go. 380 00:22:33,450 --> 00:22:34,450 We're ready. 381 00:22:34,450 --> 00:22:35,450 Unidentified Man: Okay, Mass, you have a go. 382 00:22:35,450 --> 00:22:36,450 MASSIMINO: Here we go. 383 00:22:36,450 --> 00:22:38,410 It's off. 384 00:22:38,410 --> 00:22:41,550 Disposal bag, please? 385 00:22:41,550 --> 00:22:48,860 JOHNSON: It was pretty exciting watching that from inside, 'cause that had a lot of bearing 386 00:22:48,860 --> 00:22:51,720 on whether we got that part of the mission accomplished. 387 00:22:51,720 --> 00:22:52,970 So, it was pretty interesting. 388 00:22:52,970 --> 00:22:54,860 GRUNSFELD: A third time I got to go back. 389 00:22:54,860 --> 00:23:01,110 And, you know, I just can't tell you how thrilled I was and how thrilled I was that we had a 390 00:23:01,110 --> 00:23:05,350 great team and we were able to leave the Hubble in even better shape, such that now we're 391 00:23:05,350 --> 00:23:08,370 able to celebrate the 25th anniversary. 392 00:23:08,370 --> 00:23:12,769 I was a little bit worried that when we deployed the Hubble, you know, I'd feel really sad 393 00:23:12,769 --> 00:23:14,759 again, but this time I didn't. 394 00:23:14,759 --> 00:23:18,389 I just felt thrilled that we hadn't broken the Hubble, that we'd upgraded it, that it 395 00:23:18,389 --> 00:23:22,690 was in the best shape of its life, and that we'd done our job and a little bit more to 396 00:23:22,690 --> 00:23:28,120 give Hubble a very long life, bringing back all of its rewards to us here on planet Earth 397 00:23:28,120 --> 00:23:29,470 in terms of great discoveries. 398 00:23:29,470 --> 00:23:35,330 STRAUGHN: The fact that astronauts were able to go up and fix Hubble was really a groundbreaking 399 00:23:35,330 --> 00:23:36,330 thing. 400 00:23:36,330 --> 00:23:41,580 And it tells a really critical part of NASA's history, when science and human space exploration 401 00:23:41,580 --> 00:23:44,120 worked together really critically for the first time. 402 00:23:44,120 --> 00:23:50,930 SEMBACH: Without the repair missions, you wouldn't have Hubble lasting 25 years. 403 00:23:50,930 --> 00:23:53,510 Hubble's best days are still to come. 404 00:23:53,510 --> 00:23:57,279 NARRATOR: Astronauts and support staff on the ground had made tremendous improvements 405 00:23:57,279 --> 00:24:00,480 to Hubble's already majestic payload. 406 00:24:00,480 --> 00:24:05,940 With the repairs completed, Hubble blew the world away with what it saw and what we now 407 00:24:05,940 --> 00:24:13,740 could behold: sharp, clean, and crisp data, images of stars forming, and Ultra Deep Field 408 00:24:13,740 --> 00:24:19,529 images of thousands of galaxies showing just a glimpse at how big this universe is. 409 00:24:19,529 --> 00:24:22,049 MASSIMINO: I do have a favorite Hubble image. 410 00:24:22,049 --> 00:24:27,429 I have a couple of them, but the one that pops into my mind is the Cone Nebula. 411 00:24:27,429 --> 00:24:32,080 And it is an early release image, and the reason I like that is because it showed that 412 00:24:32,080 --> 00:24:35,200 we installed the advanced camera for surveys correctly. 413 00:24:35,200 --> 00:24:41,210 JOHNSON: Hubble has brought just knowledge of the universe that I think is beyond belief 414 00:24:41,210 --> 00:24:42,899 to the normal person. 415 00:24:42,899 --> 00:24:48,690 And some of the discoveries of the Hubble Space Telescope in terms of the universe expanding 416 00:24:48,690 --> 00:24:50,409 are just mindboggling. 417 00:24:50,409 --> 00:24:56,509 FLANAGAN: Every time I look at it, I stare and I stare and I want to see what's in that 418 00:24:56,509 --> 00:24:58,860 finger, you know, what's in that pillar? 419 00:24:58,860 --> 00:25:03,779 And interestingly, if you look at it in the infrared, you can actually see into it. 420 00:25:03,779 --> 00:25:06,809 STRAUGHN: The Hubble Ultra Deep Field was released in 2004 when I was in grad school. 421 00:25:06,809 --> 00:25:12,559 And to this day, I really remember the day when that image came out. 422 00:25:12,559 --> 00:25:18,399 My grad advisor printed this image, this beautiful image with galaxies that we'd never seen before 423 00:25:18,399 --> 00:25:22,529 on a huge sheet of paper and rolled it out on the table for us grad students to look 424 00:25:22,529 --> 00:25:24,879 at, and just said, you know, "Look at this image. 425 00:25:24,879 --> 00:25:25,970 Look what's here. 426 00:25:25,970 --> 00:25:28,179 What can we learn from this?" 427 00:25:28,179 --> 00:25:33,360 And so, I really loved that visual, sort of tangible representation of look at this beautiful 428 00:25:33,360 --> 00:25:34,870 thing and what can we learn. 429 00:25:34,870 --> 00:25:40,130 NARRATOR: Circling the globe at five miles per second, this school bus sized observatory 430 00:25:40,130 --> 00:25:45,760 was the most technologically advanced device ever launched, and has stayed amazingly advanced 431 00:25:45,760 --> 00:25:50,870 through five repair and upgrade missions, from the first mission critical optics repair 432 00:25:50,870 --> 00:25:58,289 on Space Shuttle mission STS-61 to the last servicing mission, STS-125, which added the 433 00:25:58,289 --> 00:26:04,129 wide field camera three and replaced or improved sensors, batteries, and numerous other components. 434 00:26:04,129 --> 00:26:07,610 BOLDEN: The Hubble was an incredible undertaking. 435 00:26:07,610 --> 00:26:13,909 If I look at the very last Hubble servicing mission, STS-125, it was perhaps the most 436 00:26:13,909 --> 00:26:18,659 ambitious single mission that this agency has ever undertaken. 437 00:26:18,659 --> 00:26:24,309 It was five spacewalks back to back to back to back to back. 438 00:26:24,309 --> 00:26:28,950 That's no break in between the spacewalks like we normally will do. 439 00:26:28,950 --> 00:26:34,570 The magnitude of the things that they wanted to accomplish almost meant certain failure 440 00:26:34,570 --> 00:26:35,570 somewhere. 441 00:26:35,570 --> 00:26:39,370 But, the crew said--the crew and the whole team, the team that put the mission together 442 00:26:39,370 --> 00:26:41,019 said, "Look, we can do this. 443 00:26:41,019 --> 00:26:45,779 You know, we will have accomplished so much more in making Hubble better than it is ever 444 00:26:45,779 --> 00:26:46,999 believed to be." 445 00:26:46,999 --> 00:26:53,929 So, Hubble gave us an excellent example of people, a team, that was not afraid of failure. 446 00:26:53,929 --> 00:26:55,889 SCOLESE: Failure was not an option. 447 00:26:55,889 --> 00:26:57,590 We were going to succeed. 448 00:26:57,590 --> 00:27:01,509 GRUNSFELD: What's really exciting to me is just the breadth of the scientific discoveries 449 00:27:01,509 --> 00:27:06,240 it's been able to make, everything from the age of the universe to proving the existence 450 00:27:06,240 --> 00:27:12,330 of black holes to discovering brand new things like the universe is accelerating due to mysterious 451 00:27:12,330 --> 00:27:13,330 dark energy. 452 00:27:13,330 --> 00:27:17,260 TYSON: I grew up, telescopes put into orbit wouldn't last more than three, at most five 453 00:27:17,260 --> 00:27:18,260 years. 454 00:27:18,260 --> 00:27:25,480 So, they never had a chance to grow on you, to become part of your soul of expectation 455 00:27:25,480 --> 00:27:28,110 for the next astronomical discovery. 456 00:27:28,110 --> 00:27:35,090 With Hubble, the fact--I think the fact that it was repairable meant it could just stay 457 00:27:35,090 --> 00:27:39,410 with you for decades, now 25 years. 458 00:27:39,410 --> 00:27:41,600 GARCIA: Everybody knows Hubble. 459 00:27:41,600 --> 00:27:43,179 It's really true. 460 00:27:43,179 --> 00:27:48,669 Worldwide, all throughout the US, everybody, all ages, all walks of life, you say Hubble 461 00:27:48,669 --> 00:27:52,070 Space Telescope, people know what you're talking about. 462 00:27:52,070 --> 00:27:53,070 That's extraordinary. 463 00:27:53,070 --> 00:27:58,350 NARRATOR: More than a simple telescope, Hubble is humanity's grand observatory of the vastness 464 00:27:58,350 --> 00:27:59,870 of space. 465 00:27:59,870 --> 00:28:03,960 And we've kept exploring by staring into the universe and moving forward. 466 00:28:03,960 --> 00:28:07,789 STRAUGHN: The great thing about Hubble now, this year, is that it's still going strong. 467 00:28:07,789 --> 00:28:11,919 And we expect it to last out 'til 2020, maybe even longer. 468 00:28:11,919 --> 00:28:14,519 But, we definitely have to start thinking about the future. 469 00:28:14,519 --> 00:28:19,230 And NASA right now is building and putting together and testing the James Webb Space 470 00:28:19,230 --> 00:28:20,230 Telescope. 471 00:28:20,230 --> 00:28:24,090 MASSIMINO: That's going to be put even further away from the Earth than Hubble, and be able 472 00:28:24,090 --> 00:28:29,370 to see much further into the universe and provide even more information and even better 473 00:28:29,370 --> 00:28:30,370 images. 474 00:28:30,370 --> 00:28:32,980 I think that's going to be very exciting when we get that into space. 475 00:28:32,980 --> 00:28:38,230 NARRATOR:: The team here at NASA will continue that momentum with the next great observatory 476 00:28:38,230 --> 00:28:44,779 coming soon to the NASA inventory, the James Webb Space Telescope, with a primary mirror 477 00:28:44,779 --> 00:28:48,840 six times larger than Hubble's and over a hundred times more powerful. 478 00:28:48,840 --> 00:28:52,350 GRUNSFELD: There are places that the Hubble just can't see. 479 00:28:52,350 --> 00:28:58,179 The Hubble Space Telescope can't see inside the dark cocoons of dust and gas where baby 480 00:28:58,179 --> 00:29:01,659 stars are born and planets form. 481 00:29:01,659 --> 00:29:05,559 The James Webb Space Telescope and the infrared will be able to peer into those cocoons and 482 00:29:05,559 --> 00:29:09,160 show us the details of those first moments of star and planet formation. 483 00:29:09,160 --> 00:29:14,070 ALTMAN: The big thing is how exciting space is for the future. 484 00:29:14,070 --> 00:29:15,580 It's going to be incredible. 485 00:29:15,580 --> 00:29:21,710 We're at the cusp of a new era with new machines being designed, new missions being flown. 486 00:29:21,710 --> 00:29:27,039 We are going to visit other planets, and I'm--I just hope that young people can get excited 487 00:29:27,039 --> 00:29:29,009 about taking us that next step. 488 00:29:29,009 --> 00:29:31,169 I can't wait to watch them do it. 489 00:29:31,169 --> 00:29:32,179 It's a great time. 490 00:29:32,179 --> 00:29:37,710 JOHNSON: Growth in space; for kids that are involved in science and technology, I think 491 00:29:37,710 --> 00:29:42,029 space is a great way to aim your career at. 492 00:29:42,029 --> 00:29:44,230 I think we're going to discover new things. 493 00:29:44,230 --> 00:29:49,010 I'm really excited that NASA's got a number of programs going, including the James Webb 494 00:29:49,010 --> 00:29:53,179 Telescope, which'll bring the same kind of discoveries Hubble has. 495 00:29:53,179 --> 00:29:55,080 So, the future's pretty bright. 496 00:29:55,080 --> 00:30:00,169 NARRATOR: Today Hubble is still making new discoveries, seeing distant stars and galaxies 497 00:30:00,169 --> 00:30:05,590 that have never been seen before, improving our knowledge of the early universe, and clarifying 498 00:30:05,590 --> 00:30:07,409 images of our closest neighbors. 499 00:30:07,409 --> 00:30:08,830 CEPOLLINA: Look at the Washington Post. 500 00:30:08,830 --> 00:30:14,009 On the front page of the Washington Post there is a colored picture of a brand new galaxy 501 00:30:14,009 --> 00:30:15,730 just discovered by Hubble. 502 00:30:15,730 --> 00:30:22,010 And to be able to look at that picture and say, "My gosh, we did that," that's exciting. 503 00:30:22,010 --> 00:30:23,010 That's exciting. 504 00:30:23,010 --> 00:30:33,190 TYSON: Hubble has consistently taken us to places we've never been visually, of course, 505 00:30:33,190 --> 00:30:38,990 and given--and empowered us to answer questions that, in a previous generation of telescopes, 506 00:30:38,990 --> 00:30:40,940 we couldn't even pose. 507 00:30:40,940 --> 00:30:47,000 NARRATOR:: From comets and asteroids to some of the most distant galaxies yet discovered, 508 00:30:47,000 --> 00:30:52,059 Hubble continues to revolutionize astronomy in our solar system and beyond. 509 00:30:52,059 --> 00:30:56,090 Hubble has changed the way we view our universe and ourselves. 510 00:30:56,090 --> 00:30:59,941 STRAUGHN: There is no doubt that the Hubble Space Telescope has changed the way that we 511 00:30:59,941 --> 00:31:02,169 as astronomers understand the universe. 512 00:31:02,169 --> 00:31:06,909 But, I think even more significantly than that, Hubble's changed the way that the world 513 00:31:06,909 --> 00:31:07,909 views space. 514 00:31:07,909 --> 00:31:11,549 WEILER: You know, when you look back on the last 25 years of Hubble, it's just incredible 515 00:31:11,549 --> 00:31:19,389 because we have made major breakthroughs in almost every field of astrophysics, from planetary 516 00:31:19,389 --> 00:31:24,690 nearby to our own galaxy to the very, very beginning of time. 517 00:31:24,690 --> 00:31:32,279 And to think that we mere humans are sitting here and getting close to understanding this 518 00:31:32,279 --> 00:31:37,679 incredible universe that's around us, and Hubble has been a key component in that over 519 00:31:37,679 --> 00:31:38,740 the last 25 years. 520 00:31:38,740 --> 00:31:40,419 NARRATOR: We're on a never-ending journey. 521 00:31:40,419 --> 00:31:45,779 And the Hubble Space Telescope celebrates its quarter century of exploration as part