1 00:00:00,000 --> 00:00:07,215 [ INTENSE MUSIC ] 2 00:00:07,215 --> 00:00:11,302 -We have lock, and are good to send that command. We have thirty-one minutes and thirty-two 3 00:00:11,302 --> 00:00:15,432 seconds for our support. 4 00:00:15,432 --> 00:00:18,309 Go for status buffer dump. 5 00:00:18,309 --> 00:00:23,982 -Because the Hubble Space Telescope is so scientifically effective right now, scientists are using 6 00:00:23,982 --> 00:00:29,571 Hubble to investigate some of the deepest mysteries of the universe. 7 00:00:29,571 --> 00:00:32,282 -One of the primary things Hubble has been doing is looking at 8 00:00:32,282 --> 00:00:35,618 the atmospheres around exoplanets. 9 00:00:35,618 --> 00:00:39,080 -If you had asked the guys who built Hubble and designed Hubble, they would have sworn 10 00:00:39,080 --> 00:00:41,124 that Hubble could never ever do this. 11 00:00:41,124 --> 00:00:46,129 -That's one of the things I love about Hubble is that it ends up giving us new questions, 12 00:00:46,129 --> 00:00:51,009 new mysteries to explore. 13 00:00:51,009 --> 00:00:51,426 Hubble In The Sky 14 00:00:51,426 --> 00:00:54,554 Hubble In The Sky 15 00:00:54,554 --> 00:00:57,724 Episode 2: An Unexpected Journey 16 00:00:57,724 --> 00:01:00,935 -My name is Larry Dunham. I'm the chief systems engineer 17 00:01:00,935 --> 00:01:03,897 for flight systems here on the Hubble Space Telescope. 18 00:01:03,897 --> 00:01:09,736 I started on the Hubble program back in the summer of 1982, when Hubble was being built 19 00:01:09,736 --> 00:01:16,242 out in California. First telescope, in space, to be designed so that we've got what we call 20 00:01:16,242 --> 00:01:21,122 orbital replacement units. They're modular boxes with handrails on them so the astronauts 21 00:01:21,122 --> 00:01:25,794 can go up and just pick and play. They've got nice connectors on them that make it easy 22 00:01:25,794 --> 00:01:31,966 for the astronauts with their big gloves to be able to put them in and out. 23 00:01:31,966 --> 00:01:34,344 -We've had five servicing missions. 24 00:01:34,344 --> 00:01:38,098 We have replaced some equipment multiple times, 25 00:01:38,098 --> 00:01:43,019 especially the instruments. We're always going with the advanced technology. 26 00:01:43,019 --> 00:01:48,108 -The telescope we have today on orbit is not the telescope that we launched originally. 27 00:01:48,108 --> 00:01:53,196 We've been able to replace all five of our science instruments with instruments that 28 00:01:53,196 --> 00:01:58,368 have the technology that didn't even exist when Hubble was being built originally. 29 00:01:58,368 --> 00:02:02,122 -The Hubble Space Telescope is really an observatory 30 00:02:02,122 --> 00:02:04,958 because it has several science instruments, 31 00:02:04,958 --> 00:02:10,296 several modes of operation. We have multiple cameras, multiple spectrographs. They each 32 00:02:10,296 --> 00:02:15,051 have different capabilities in terms of their sensitivities or the kinds of frequencies 33 00:02:15,051 --> 00:02:20,014 they can receive of the electromagnetic spectrum. We can also use Hubble in different kinds 34 00:02:20,014 --> 00:02:23,476 of intriguing modes depending on what we're trying to observe. 35 00:02:23,476 --> 00:02:26,146 -There are different types of observing scenarios, 36 00:02:26,146 --> 00:02:28,439 and one of the things the scientists have been able to do 37 00:02:28,439 --> 00:02:31,651 is they've been able to come up with very interesting and unique observing 38 00:02:31,651 --> 00:02:36,489 scenarios that allow them to do science that they never thought they could do before. 39 00:02:36,489 --> 00:02:41,744 -Because the Hubble Space Telescope has been operating for a long time, it's giving us 40 00:02:41,744 --> 00:02:47,500 what we need to explore the universe in deep ways that would never have been possible when 41 00:02:47,500 --> 00:02:53,715 Hubble was first launched. For example, scientists wondered whether we could use Hubble in an 42 00:02:53,715 --> 00:03:01,055 innovative mode in recent years, basically scanning objects slowly, instead of just staring 43 00:03:01,055 --> 00:03:06,227 at them. In some cases that gives us a higher sensitivity to what we're trying to observe. 44 00:03:06,227 --> 00:03:11,983 And we're using that special mode on Hubble now to get better information about many types 45 00:03:11,983 --> 00:03:18,281 of things in space, including to be able to study planets around other stars, what we 46 00:03:18,281 --> 00:03:22,076 call exoplanets, planets outside of our own solar system. 47 00:03:22,076 --> 00:03:27,040 -What Hubble’s been able to do is as the planets go in front of the stars that they're 48 00:03:27,040 --> 00:03:30,126 going around, the spectrographs can detect changes, 49 00:03:30,126 --> 00:03:37,217 very small changes in the spectrum. This has allowed them to do exoplanet atmospheric studies. 50 00:03:37,217 --> 00:03:40,678 This is something that Hubble has sort of really stepped up to the plate. It has been 51 00:03:40,678 --> 00:03:43,306 just phenomenally good at. 52 00:03:43,306 --> 00:03:46,309 The spectrographs have really sort of been leading that, if you ever see things about, 53 00:03:46,309 --> 00:03:50,688 oh, a new exoplanet was discovered that has this in the atmosphere or that in the atmosphere, 54 00:03:50,688 --> 00:03:56,236 and we think it's made of this, it's the spectrographs which have shown you that kind of information. 55 00:03:56,236 --> 00:04:00,198 For doing a lot of the exoplanet observations, you have to catch what's known as a transit. 56 00:04:00,198 --> 00:04:02,492 One, the orbit of the exoplanet has to be 57 00:04:02,492 --> 00:04:04,911 such that it's going to go between you and 58 00:04:04,911 --> 00:04:07,372 the star it's going around. 59 00:04:07,372 --> 00:04:10,625 We can't just do an exoplanet observation whenever we want 60 00:04:10,625 --> 00:04:12,543 or whenever it's convenient. We have to do 61 00:04:12,543 --> 00:04:15,171 an exoplanet observation when it's first starting 62 00:04:15,171 --> 00:04:20,134 to go into the star, and so they have to know very accurately the timing of that. 63 00:04:20,134 --> 00:04:23,429 We have to schedule it ahead of time. This is not something that Hubble can get around 64 00:04:23,429 --> 00:04:28,309 to when it wants to. We have to say no, at this point in time on this date, you have 65 00:04:28,309 --> 00:04:32,313 to be pointed here and you have to be looking here. We had to really think about how to 66 00:04:32,313 --> 00:04:35,942 schedule this. A lot of thought goes into it. A lot of thought goes into the planning 67 00:04:35,942 --> 00:04:38,569 and of the execution. 68 00:04:38,569 --> 00:04:44,867 -The Hubble operations team are quite willing and capable of using the telescope in new 69 00:04:44,867 --> 00:04:49,789 modes and new, innovative ways that enable us to accomplish science that we wouldn't 70 00:04:49,789 --> 00:04:53,293 otherwise be able to accomplish. 71 00:04:53,293 --> 00:04:58,798 We asked them, would it be possible to use Hubble to track something moving quickly 72 00:04:58,798 --> 00:05:04,053 across the sky? And they figured out a way to use Hubble in a fast-tracking mode that 73 00:05:04,053 --> 00:05:09,434 enabled us to do explorations and discoveries that astronomers didn't envision using Hubble 74 00:05:09,434 --> 00:05:12,812 for when it was first designed. 75 00:05:12,812 --> 00:05:17,483 -Now when we're observing our planets, when we're observing Jupiter, or Saturn, or Uranus, 76 00:05:17,483 --> 00:05:22,238 or Neptune, they move also. You have to move the telescope because they're just going around 77 00:05:22,238 --> 00:05:25,408 the Sun. They're actually moving because they're really moving, so we have to move with them. 78 00:05:25,408 --> 00:05:31,581 Or if we’re observing asteroids or comets you have to chase after them. 79 00:05:31,581 --> 00:05:35,626 -'Oumuamua, we know came from outside of our solar system, 80 00:05:35,626 --> 00:05:38,463 is like a big asteroid that was detected 81 00:05:38,463 --> 00:05:41,424 whizzing through our solar system. We wanted to use Hubble 82 00:05:41,424 --> 00:05:44,385 to observe this as well. And we were able to track it 83 00:05:44,385 --> 00:05:47,305 and this was not a simple operation. It's moving at 84 00:05:47,305 --> 00:05:51,517 more than a hundred thousand miles an hour, so being able to observe this and track it is 85 00:05:51,517 --> 00:05:53,102 a wonderful capability that the operations team has enabled Hubble to have. 86 00:05:53,102 --> 00:05:54,854 spot, now we have to get in the exact location to put the target in 87 00:05:54,854 --> 00:05:57,690 the science instrument aperture. 88 00:05:57,690 --> 00:06:02,862 -The telescope is big, it's massive. It moves about the same speed as the minute hand on 89 00:06:02,862 --> 00:06:07,492 a clock, so to move from pointing at one thing to go completely around the other one, takes 90 00:06:07,492 --> 00:06:12,538 us a half an hour. It is not a very fast motion. 91 00:06:12,538 --> 00:06:16,834 We actually use a very interesting technique. It's using Newton's third law. We have these 92 00:06:16,834 --> 00:06:20,922 very large reaction wheels on it. They're about two feet across, very very heavy, 93 00:06:20,922 --> 00:06:26,594 very very massive wheels. You start spinning those wheels one way, the telescope will spin a little 94 00:06:26,594 --> 00:06:31,140 bit in the opposite direction. This is how we can move the telescope from 95 00:06:31,140 --> 00:06:34,143 one part of the sky to another part of the sky. 96 00:06:34,143 --> 00:06:37,480 -Once we've moved the reaction wheels and we've moved the telescope so we're in the right 97 00:06:37,480 --> 00:06:42,193 spot, now we have to get in the exact location to put the target in 98 00:06:42,193 --> 00:06:46,114 the science instrument aperture. 99 00:06:46,114 --> 00:06:50,827 -What's going to happen now is the FGSs are going to start talking to the telescope, talking 100 00:06:50,827 --> 00:06:55,039 to the flight software computer and saying, I want you to move the telescope over here 101 00:06:55,039 --> 00:07:00,211 a little bit to be able to position the science for the science aperture. 102 00:07:00,211 --> 00:07:05,466 -Most of the time we use the Hubble Space Telescope to do observations that have been planned 103 00:07:05,466 --> 00:07:10,388 quite a bit in advance. Observers around the world, astronomers will write proposals. We 104 00:07:10,388 --> 00:07:16,018 will then take those accepted proposals and observe whatever it is that the astronomer 105 00:07:16,018 --> 00:07:22,525 has proposed, but sometimes there are things that happen that are unexpected or rapid events 106 00:07:22,525 --> 00:07:25,027 that we need a more rapid response. 107 00:07:25,027 --> 00:07:29,699 -We have a capability of what we call a target of opportunity, 108 00:07:29,699 --> 00:07:33,202 and that's when something unexpected 109 00:07:33,202 --> 00:07:38,791 happens in the universe that astronomers, they want to immediately jump on that as fast 110 00:07:38,791 --> 00:07:45,006 as possible with Hubble. Case in point was the gravitational wave detection of two neutron 111 00:07:45,006 --> 00:07:51,596 stars colliding. The target of opportunity was submitted for Hubble to actually go look 112 00:07:51,596 --> 00:07:56,767 at the remnant, and see if we could find it. 113 00:07:56,767 --> 00:08:01,397 -We had the engineers run through it, we got new commanding sequences from the Space Telescope 114 00:08:01,397 --> 00:08:04,108 Science Institute. We're able to run all that through and then 115 00:08:04,108 --> 00:08:05,568 we executed on orbit. 116 00:08:05,568 --> 00:08:13,159 -We have to respond very fast to produce a new schedule and set of command loads. 117 00:08:13,159 --> 00:08:18,289 -We can modify a lot of the flight software, modify how the instruments are commanded. 118 00:08:18,289 --> 00:08:23,878 It allows us to change. We can react very quickly. 119 00:08:23,878 --> 00:08:29,050 What Hubble has done compared to what we were thinking Hubble could do is just amazing. Hubble’s 120 00:08:29,050 --> 00:08:34,096 had its fingers in almost everything. The neutron star collision. Looking for all the 121 00:08:34,096 --> 00:08:39,977 supernovae, all this stuff going on with dark matter, dark energy, exoplanets. Hubble has 122 00:08:39,977 --> 00:08:44,482 just been constantly finding new things. Now we're looking at these interstellar comets 123 00:08:44,482 --> 00:08:50,279 and these interstellar asteroids visiting us. It's really been spectacular to watch. 124 00:08:50,279 --> 00:08:55,868 -There really are two key aspects to Hubble's design that have enabled us to last 125 00:08:55,868 --> 00:09:00,540 the 30 years that we have, and that is really the redundancy that we have on board, and 126 00:09:00,540 --> 00:09:05,127 then it's the servicing, putting in new and improved instruments, and being able to improve 127 00:09:05,127 --> 00:09:09,507 the hardware with lessons learned over the 30 years of Hubble operations. 128 00:09:09,507 --> 00:09:12,176 We are now at our peak performance. 129 00:09:12,176 --> 00:09:20,560 -The Hubble Space Telescope has had a profound impact, not only on astronomy. It showed that 130 00:09:20,560 --> 00:09:28,484 humans in space and science can go hand in hand to enable us to explore space in richer 131 00:09:28,484 --> 00:09:33,906 ways than we could ever do with either just astronauts alone or just with instrumentation 132 00:09:33,906 --> 00:09:39,870 alone. By using these skills together, new vistas of exploration are open to us, and 133 00:09:39,870 --> 00:09:44,500 that lesson is something we're still benefiting from as we envision future space exploration. 134 00:09:44,500 --> 00:09:50,047 “Go ahead?” “We have a go for release.” “Okay, Charlie." 135 00:09:50,047 --> 00:09:54,385 -It's amazing with a program that's lasted, the duration that Hubble has lasted, that 136 00:09:54,385 --> 00:09:58,180 the astronomers up at the Space Telescope Science Institute continue to come up with 137 00:09:58,180 --> 00:10:02,184 new things that they want to try to do with Hubble, and we certainly hope that we'll be 138 00:10:02,184 --> 00:10:07,064 able to continue to provide that kind of capability to them until the late 2020s and beyond. 139 00:10:07,064 --> 00:10:13,029 Hubble Eye In The Sky 140 00:10:13,029 --> 00:10:20,786 [ INTENSE MUSIC ]