WEBVTT FILE 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 00:05:33.280 --> 00:05:34.148