1 00:00:11,469 --> 00:00:13,596 So to celebrate Hubble's 35th 2 00:00:13,596 --> 00:00:17,642 birthday, we're releasing four new images from Hubble. 3 00:00:17,934 --> 00:00:20,103 There are different parts of the universe. 4 00:00:20,103 --> 00:00:22,981 One of them is the Rosette Nebula. 5 00:00:22,981 --> 00:00:25,900 Or a part of it where stars are still forming. 6 00:00:25,900 --> 00:00:30,280 And you can see dark clouds and then lit up clouds behind those 7 00:00:30,280 --> 00:00:34,534 where new stars are ionizing the gas and showing off this glow. 8 00:00:35,285 --> 00:00:39,372 We also are releasing an image of a planetary nebula. 9 00:00:39,748 --> 00:00:43,209 Now, this colorful nebula really has nothing to do with planets. 10 00:00:43,543 --> 00:00:44,878 That's just what they called it 11 00:00:44,878 --> 00:00:46,296 decades ago. 12 00:00:46,296 --> 00:00:51,217 But it is really the remnants of a dead star system, 13 00:00:51,217 --> 00:00:56,931 and the outflows from the remaining white dwarf star are creating 14 00:00:56,931 --> 00:01:01,811 this glowing cloud that's expanding away from the central sources there. 15 00:01:02,353 --> 00:01:06,941 We have an image from outside of our galaxy, of another galaxy. 16 00:01:07,067 --> 00:01:09,444 This is a spiral galaxy. 17 00:01:09,444 --> 00:01:12,489 It doesn't look quite like we think our Milky Way does, 18 00:01:12,489 --> 00:01:15,575 because the spiral arms are kind of smudged together. 19 00:01:15,575 --> 00:01:18,078 We call it a flocculant spiral. 20 00:01:18,078 --> 00:01:22,082 But in the middle, you see this amazing bar like structure. 21 00:01:22,415 --> 00:01:26,336 These are common in some types of spiral galaxies, and they are the 22 00:01:26,336 --> 00:01:30,507 mechanism by which gas and dust from the outer parts of the galaxy 23 00:01:30,507 --> 00:01:35,053 are funneled in toward the middle and can fuel the formation of new stars. 24 00:01:35,345 --> 00:01:39,099 We think our Milky Way also has some kind of a bar in the center. 25 00:01:39,766 --> 00:01:42,727 And then much closer to home in our own solar system. 26 00:01:43,061 --> 00:01:48,191 We've taken new pictures of Mars. These really wonderful clear 27 00:01:48,191 --> 00:01:53,404 shots of Mars show different features on the planet from different perspectives. 28 00:01:53,446 --> 00:01:58,034 As Mars is rotating, we see the icy poles on the top. 29 00:01:58,034 --> 00:02:01,830 We see clouds, and we can also see mountain ranges 30 00:02:01,830 --> 00:02:05,458 and deep canyons and plane structures. 31 00:02:05,792 --> 00:02:08,962 Mars is an interesting planet to study, both for what 32 00:02:08,962 --> 00:02:11,965 it's doing now, but for what it was like in the past. 33 00:02:12,090 --> 00:02:15,885 These images from the Hubble Space Telescope show us the variety 34 00:02:15,885 --> 00:02:19,013 of scientific discovery that Hubble is capable of doing. 35 00:02:26,312 --> 00:02:31,526 We're using Hubble in new, exciting ways because Hubble sees wavelengths 36 00:02:31,526 --> 00:02:34,529 or colors of light that other observatories 37 00:02:34,529 --> 00:02:38,116 don't see, and vice versa, so we use them in complement. 38 00:02:38,783 --> 00:02:42,579 Scientists are using Hubble's ultraviolet light capabilities 39 00:02:42,579 --> 00:02:46,499 to see this energetic light that comes from star forming regions, 40 00:02:46,499 --> 00:02:50,837 and also explosive events out in the universe from energetic stars. 41 00:02:51,504 --> 00:02:55,258 We're using Hubble to complement the infrared light 42 00:02:55,258 --> 00:02:58,803 observations that the newer Webb Space Telescope can do. 43 00:02:58,928 --> 00:03:02,807 Webb can see deep into the universe some of the earliest galaxies. 44 00:03:03,057 --> 00:03:05,143 Hubble sees nearer galaxies 45 00:03:05,143 --> 00:03:08,730 in all the detail, seeing its hot spots of star formation. 46 00:03:08,980 --> 00:03:12,483 With this information, together, scientists are piecing together 47 00:03:12,483 --> 00:03:18,072 how galaxies have grown and merged and changed over all of cosmic history. 48 00:03:18,198 --> 00:03:20,909 It's a very exciting new dual tool. 49 00:03:28,583 --> 00:03:29,000 Well, when 50 00:03:29,000 --> 00:03:32,879 Hubble was first launched, we were still just trying to understand 51 00:03:32,879 --> 00:03:37,175 some very basics, like how fast is the universe expanding 52 00:03:37,383 --> 00:03:40,929 and what are some of the processes by which stars form. 53 00:03:41,471 --> 00:03:45,183 Hubble has given us an avalanche of information. 54 00:03:45,183 --> 00:03:49,062 We've now measured very precisely the expansion rate of the universe. 55 00:03:49,395 --> 00:03:53,650 And in fact, now, thanks to Hubble working with telescopes on the ground, 56 00:03:53,650 --> 00:03:57,320 we know that that expansion of the universe is accelerating 57 00:03:57,612 --> 00:03:59,656 by something called dark energy. 58 00:03:59,656 --> 00:04:04,535 We've understood that Hubble is picking up signs of dark matter in the universe. 59 00:04:04,535 --> 00:04:10,124 This is mass we can't see, but we see its gravitational effects by distorted light. 60 00:04:10,375 --> 00:04:15,421 Hubble's picked up lots of regions in the universe where dark matter is prevalent, 61 00:04:22,053 --> 00:04:25,598 Scientists are using in particular the Hubble and the Webb space 62 00:04:25,598 --> 00:04:30,687 telescopes in complement because they see different wavelengths of light. 63 00:04:30,728 --> 00:04:35,316 Hubble concentrates on visible light and the energetic ultraviolet 64 00:04:35,316 --> 00:04:40,530 light, and Webb concentrates on red light and infrared light. 65 00:04:40,530 --> 00:04:43,866 And so when we have these observatories used in complement, 66 00:04:44,284 --> 00:04:49,163 we see this whole spectrum of colors that enable us to learn a whole 67 00:04:49,163 --> 00:04:52,458 lot more about whatever we're studying, whether it's the solar system 68 00:04:52,917 --> 00:04:56,629 or other star systems or distant galaxies. 69 00:04:57,630 --> 00:05:00,758 One of the new branches of science newer 70 00:05:01,301 --> 00:05:05,346 is the study of exoplanets planets outside our solar system. 71 00:05:05,930 --> 00:05:09,600 When Hubble was launched, we didn't even know if there were 72 00:05:09,600 --> 00:05:13,104 exoplanetary systems outside of our own solar system. 73 00:05:13,730 --> 00:05:18,860 And in subsequent years, many exoplanets have been discovered by other facilities. 74 00:05:19,319 --> 00:05:22,196 Hubble is now honing in on understanding 75 00:05:22,196 --> 00:05:25,241 the nature of the atmospheres of these exoplanets. 76 00:05:25,241 --> 00:05:30,830 Hubble was the pioneer of a technique of actually understanding the composition 77 00:05:31,205 --> 00:05:35,376 of exoplanet atmospheres, and now that same technique is being used by Webb. 78 00:05:35,626 --> 00:05:38,880 Astronomers are using the Webb and Hubble telescopes together 79 00:05:38,880 --> 00:05:44,093 to get a full spectrum of information about exoplanet atmospheres 80 00:05:44,093 --> 00:05:47,138 from the infrared all the way into the ultraviolet, 81 00:05:47,472 --> 00:05:50,850 and that helps us understand how exoplanet atmospheres 82 00:05:50,850 --> 00:05:54,604 compare to the atmospheres of planets in our own solar system. 83 00:05:55,021 --> 00:05:58,232 This is an example of how Hubble is being used for science 84 00:05:58,232 --> 00:06:01,861 now that was never envisioned when Hubble was designed. 85 00:06:02,278 --> 00:06:07,408 Hubble gave us many discoveries right off the bat that then gave us new questions. 86 00:06:07,742 --> 00:06:11,120 So now scientists are using Hubble to address questions 87 00:06:11,120 --> 00:06:13,873 that were not even imagined when Hubble was designed. 88 00:06:21,547 --> 00:06:22,006 I have 89 00:06:22,006 --> 00:06:25,176 many favorite images from the Hubble Space Telescope. 90 00:06:25,176 --> 00:06:27,095 I love the colorful nebulae 91 00:06:27,095 --> 00:06:30,515 because they show us that star formation is still going on. 92 00:06:31,057 --> 00:06:34,018 But I think my favorite image from Hubble 93 00:06:34,018 --> 00:06:37,063 is something called the Ultra Deep Field. 94 00:06:37,480 --> 00:06:42,235 This was an image taken by simply pointing the telescope in a direction of the sky, 95 00:06:42,235 --> 00:06:45,571 that didn't have a lot of nearby stars to drown out the image, 96 00:06:45,696 --> 00:06:49,075 and just collecting faint light for days and days with Hubble. 97 00:06:49,409 --> 00:06:53,996 The resulting image is famous now it's covered with little splotches of light. 98 00:06:53,996 --> 00:06:56,541 Well, those little splotches are galaxies. 99 00:06:56,541 --> 00:06:59,377 Galaxies outside of our own Milky Way. 100 00:06:59,377 --> 00:07:02,755 And these galaxies can contain hundreds of billions of stars. 101 00:07:03,297 --> 00:07:07,385 I like to imagine being able to go to each one of them and check it out. 102 00:07:07,385 --> 00:07:11,222 We can't do that yet with our technology, but we can do it with our eyes 103 00:07:11,222 --> 00:07:15,560 and just see how galaxies fill the universe, how rich they are. 104 00:07:15,810 --> 00:07:20,148 And of course, scientists are now learning about the history of the universe 105 00:07:20,481 --> 00:07:23,734 by looking at how the more distant galaxies 106 00:07:23,734 --> 00:07:26,737 in this image compare to ones closer to us. 107 00:07:26,946 --> 00:07:30,032 Because astronomy is like a time machine, it's taken time for the light 108 00:07:30,032 --> 00:07:34,704 to get to us and for the more distant ones we're seeing farther back in time. 109 00:07:41,836 --> 00:07:42,670 The Hubble Space 110 00:07:42,670 --> 00:07:46,299 Telescope is in excellent technical condition. 111 00:07:46,716 --> 00:07:50,219 For something that's 35 years old, it's really incredible. 112 00:07:50,219 --> 00:07:53,764 And the reason that Hubble is in good shape is because, first of all, 113 00:07:53,973 --> 00:07:56,976 we've had these series of astronaut servicing 114 00:07:56,976 --> 00:07:59,979 missions where astronauts have returned to the telescope, 115 00:08:00,062 --> 00:08:03,691 put in new and improved instrumentation and repaired components. 116 00:08:04,233 --> 00:08:07,945 And now we have this excellent team of experts on the ground 117 00:08:07,945 --> 00:08:10,990 who are constantly monitoring Hubble's technical health. 118 00:08:11,324 --> 00:08:16,120 They can address any glitches remotely from the ground is pretty incredible. 119 00:08:16,537 --> 00:08:20,791 And we're even learning to operate the observatory in different ways 120 00:08:20,791 --> 00:08:25,671 so that as it ages, we can continue to get excellent scientific results. 121 00:08:32,470 --> 00:08:33,054 The Hubble 122 00:08:33,054 --> 00:08:36,933 team and astronomers everywhere are excited 123 00:08:36,933 --> 00:08:41,145 and very gratified that we're reaching this 35th anniversary 124 00:08:41,854 --> 00:08:44,857 milestone for the Hubble Space Telescope mission. 125 00:08:45,149 --> 00:08:49,111 This mission is older than many people on planet Earth. 126 00:08:49,111 --> 00:08:53,074 A lot of people today have grown up with the Hubble Space Telescope as being a 127 00:08:53,074 --> 00:08:56,619 part of their lives, and that's something I think we can be very proud of, 128 00:08:56,619 --> 00:09:00,957 that this eye on the sky has given people around the world 129 00:09:01,207 --> 00:09:06,629 a new view of the universe, how vast it is, how beautiful it is, 130 00:09:06,879 --> 00:09:10,716 and how active it is, and how we are all fellow citizens 131 00:09:10,716 --> 00:09:15,179 of planet Earth just looking up in awe and wonder at what we're discovering 132 00:09:15,346 --> 00:09:18,349 because of this wonderful miracle of technology. 133 00:09:24,230 --> 00:09:27,233 One of the reasons the world loves the Hubble Space 134 00:09:27,233 --> 00:09:31,070 Telescope is that we've made our images accessible 135 00:09:31,237 --> 00:09:35,032 to people around the world as long as we could do it. 136 00:09:35,032 --> 00:09:39,495 And, you know, with the internet coming on board after Hubble was launched, 137 00:09:39,912 --> 00:09:43,958 it really created a new portal for sharing the observations 138 00:09:43,958 --> 00:09:46,961 of this major space observatory with the world. 139 00:09:47,044 --> 00:09:49,964 And now people are using these Hubble images 140 00:09:49,964 --> 00:09:52,967 for education, for inspiration. 141 00:09:53,092 --> 00:09:56,804 And just to be curious about what's in the universe. 142 00:09:56,804 --> 00:10:01,309 And I love that fact about this mission, and I'm looking forward to many more 143 00:10:01,517 --> 00:10:04,770 images and spectra from Hubble to inspire people 144 00:10:04,770 --> 00:10:07,773 for years to come. 145 00:10:13,154 --> 00:10:16,449 NASA has a wonderful website for information 146 00:10:16,449 --> 00:10:18,492 about the Hubble Space Telescope. 147 00:10:18,492 --> 00:10:21,537 It's nasa.gov/hubble, 148 00:10:22,163 --> 00:10:26,000 and we're also very active on social media at NASA Hubble. 149 00:10:26,417 --> 00:10:29,378 So there's lots of information, all the Hubble images, 150 00:10:29,378 --> 00:10:31,547 a lot of information about Hubble's history, 151 00:10:31,547 --> 00:10:33,799 and a lot of information about Hubble's future. 152 00:10:33,799 --> 00:10:35,760 So I encourage everyone to look.