1 00:00:00,020 --> 00:00:04,050 2 00:00:04,070 --> 00:00:09,070 Hubble is profoundly significant 3 00:00:09,090 --> 00:00:12,180 I think for humanity. 4 00:00:12,200 --> 00:00:14,220 We work together, we launched this telescope 5 00:00:14,240 --> 00:00:17,250 that's now in orbit that's now in orbit Earth 6 00:00:17,270 --> 00:00:20,290 and has been in orbit for 25 years 7 00:00:20,310 --> 00:00:23,350 revealing things about the universe that we never knew before. 8 00:00:23,370 --> 00:00:26,400 So because of Hubble we been able to learn 9 00:00:26,420 --> 00:00:30,420 about other galaxies and even the expansion 10 00:00:30,440 --> 00:00:34,440 of the entire universe and details about our own 11 00:00:34,460 --> 00:00:38,480 neighborhood and solar system with detail that we could never have had before. 12 00:00:38,500 --> 00:00:44,510 13 00:00:44,530 --> 00:00:47,530 It was hoped from the outset that Hubble 14 00:00:47,550 --> 00:00:50,580 would help us understand how fast the universe was stretching apart 15 00:00:50,600 --> 00:00:52,620 and it has done that. 16 00:00:52,640 --> 00:00:54,650 But one surprise is that in recent years 17 00:00:54,670 --> 00:00:56,680 Hubble along with ground based telescopes 18 00:00:56,700 --> 00:00:59,740 have been used to determine 19 00:00:59,760 --> 00:00:59,800 that expansion rate is actually getting faster 20 00:00:59,820 --> 00:01:03,850 that expansion rate is actually getting faster, it's accelerating. 21 00:01:03,870 --> 00:01:06,870 Something we call "dark energy" is pushing the universe apart, 22 00:01:06,890 --> 00:01:08,940 that's a big unexpected surprise. 23 00:01:08,960 --> 00:01:11,980 We're also doing things with Hubble that 24 00:01:12,000 --> 00:01:15,000 are innovative that weren't planned from the outset. 25 00:01:15,020 --> 00:01:18,030 One is, we're using Hubble to study the atmosphere's 26 00:01:18,050 --> 00:01:21,080 of planets outside our own solar system. 27 00:01:21,100 --> 00:01:25,140 So we have only known for a few years now 28 00:01:25,160 --> 00:01:28,220 that there are planets outside our solar system 29 00:01:28,240 --> 00:01:31,260 Hubble has not made most of those discoveries of exoplanets 30 00:01:31,280 --> 00:01:34,280 but what Hubble is doing is analyzing the 31 00:01:34,300 --> 00:01:37,310 composition of some of those atmosphere of exoplanets. 32 00:01:37,330 --> 00:01:41,340 And that's a very innovative use of Hubble. 33 00:01:41,360 --> 00:01:45,360 34 00:01:45,380 --> 00:01:50,390 Hubble, even after 25 years is actually 35 00:01:50,410 --> 00:01:54,420 working as well or better then ever 36 00:01:54,440 --> 00:01:56,440 and the reason that is the case is that 37 00:01:56,460 --> 00:01:59,480 the last servicing mission that astronauts did 38 00:01:59,500 --> 00:02:01,530 in 2009 was very successful. 39 00:02:01,550 --> 00:02:04,550 We were able through their hard work and 40 00:02:04,570 --> 00:02:06,700 hard work of many many people on the ground 41 00:02:06,720 --> 00:02:10,730 to install 2 brand new state of the art instruments. 42 00:02:10,750 --> 00:02:12,730 A new camera, a new spectrograph, 43 00:02:12,750 --> 00:02:14,780 and also the astronauts repaired another camera 44 00:02:14,800 --> 00:02:17,880 and spectrograph already on the observatory. 45 00:02:17,900 --> 00:02:21,920 So now we have this full suite of several science instruments. 46 00:02:21,940 --> 00:02:24,970 We also have good batteries and gyroscopes 47 00:02:24,990 --> 00:02:29,010 all the things we need to keep the telescope pointing and operating stability. 48 00:02:29,030 --> 00:02:32,040 So we can get better science now from Hubble 49 00:02:32,060 --> 00:02:34,090 then ever before. 50 00:02:34,110 --> 00:02:36,120 In fact, scientist around the world are proposing 51 00:02:36,140 --> 00:02:40,160 to use Hubble at the highest rates ever in recent years. 52 00:02:40,180 --> 00:02:45,180 So, Hubble is bringing excellent science and we anticipate this for several years to come. 53 00:02:45,200 --> 00:02:50,210 54 00:02:50,230 --> 00:02:54,250 I think Hubble has become a cultural icon 55 00:02:54,270 --> 00:02:58,260 because the beautiful images that it sends down 56 00:02:58,280 --> 00:03:02,280 and one thing I'm pleased that NASA has done 57 00:03:02,300 --> 00:03:05,400 and also the European Space Agency 58 00:03:05,420 --> 00:03:09,440 is to make these images easily available to the public. 59 00:03:09,460 --> 00:03:13,450 60 00:03:13,470 --> 00:03:17,500 This is an image taken by pointing Hubble 61 00:03:17,520 --> 00:03:21,530 at a relatively boring position in the sky 62 00:03:21,550 --> 00:03:25,610 where there aren't any nearby star or galaxies 63 00:03:25,630 --> 00:03:27,630 and Hubble was allowed to collect light 64 00:03:27,650 --> 00:03:30,490 for days on end, so you could see the faintest galaxies 65 00:03:30,510 --> 00:03:31,490 and faintest objects. 66 00:03:31,510 --> 00:03:34,530 What appeared in that image were thousands 67 00:03:34,550 --> 00:03:37,590 of galaxies, most of them never discovered before 68 00:03:37,610 --> 00:03:40,630 and that's just in a soda straw area of the sky. 69 00:03:40,650 --> 00:03:44,640 If you imagine these galaxies extrapolated 70 00:03:44,660 --> 00:03:46,700 around the whole sky, you get a visual image for 71 00:03:46,720 --> 00:03:50,730 how many galaxies there are. 72 00:03:50,750 --> 00:03:53,810 73 00:03:53,830 --> 00:03:58,870 We are always getting surprised by what we are discovering with Hubble. 74 00:03:58,890 --> 00:04:02,920 We are now looking into the atmospheres of exoplanets. 75 00:04:02,940 --> 00:04:04,950 These are planets outside our solar system. 76 00:04:04,970 --> 00:04:07,970 Nobody ever envisioned that for Hubble when it was first launched. 77 00:04:07,990 --> 00:04:11,000 We are able to watch and see 78 00:04:11,020 --> 00:04:14,060 how things change in our own solar system, 79 00:04:14,080 --> 00:04:16,110 we're able to see how planets and comets change, 80 00:04:16,130 --> 00:04:18,110 sometimes on a daily basis. 81 00:04:18,130 --> 00:04:20,200 That's very exciting and we are able to 82 00:04:20,220 --> 00:04:24,280 compare the make up of extremely distant galaxies, 83 00:04:24,300 --> 00:04:26,330 with galaxies like our own, 84 00:04:26,350 --> 00:04:31,380 using Hubble's sensitive cameras and spectrographs. 85 00:04:31,400 --> 00:04:34,390 86 00:04:34,410 --> 00:04:37,440 Different kinds of telescopes have 87 00:04:37,460 --> 00:04:40,460 different strengths and capabilites, 88 00:04:40,480 --> 00:04:43,510 so Hubble is very good at doing observations in 89 00:04:43,530 --> 00:04:45,560 visible optical light and some what into 90 00:04:45,580 --> 00:04:48,600 near infered light and ultraviolet light. 91 00:04:48,620 --> 00:04:51,640 But Hubble is not capable of looking far 92 00:04:51,660 --> 00:04:54,660 into infered light into these 93 00:04:54,680 --> 00:04:58,710 reddened and lower energy light forms 94 00:04:58,730 --> 00:05:01,730 that are sometimes emitted from objects 95 00:05:01,750 --> 00:05:03,810 especially distant galaxies. 96 00:05:03,830 --> 00:05:05,820 The James Webb Space Telescope, 97 00:05:05,840 --> 00:05:07,850 to be launched in 2018, 98 00:05:07,870 --> 00:05:09,860 will be an infered observatory and 99 00:05:09,880 --> 00:05:12,920 it will be able to see galaxies that are farther away 100 00:05:12,940 --> 00:05:13,990 then what Hubble can see. 101 00:05:14,010 --> 00:05:17,010 It will also be able to peer into some of these 102 00:05:17,030 --> 00:05:17,040 dusty regions around stars where we think 103 00:05:17,060 --> 00:05:21,090 dusty regions around stars where we think planets form. 104 00:05:21,110 --> 00:05:25,140 So James Webb will pick up on some of the science that Hubble 105 00:05:25,160 --> 00:05:28,260 has revealed and take us a little bit farther. 106 00:05:28,280 --> 00:05:33,260 So we're excited about James Webb and we hope it will overlap with Hubble some years. 107 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