1 00:00:00,711 --> 00:00:03,984 Shuttle astronauts will visit the Hubble Space Telescope 2 00:00:04,019 --> 00:00:06,637 for the final time in May 2009. 3 00:00:06,638 --> 00:00:12,195 In five bold and daring spacewalks, they will upgrade Hubble's instruments, 4 00:00:12,196 --> 00:00:15,852 allowing it to continue making remarkable scientific discoveries 5 00:00:15,934 --> 00:00:18,745 well into the next decade. 6 00:00:36,964 --> 00:00:38,985 This is the Hubblecast. 7 00:00:38,986 --> 00:00:42,450 News and images from the NASA / ESA Hubble Space Telescope. 8 00:00:42,451 --> 00:00:46,226 Travelling through time and space with our host, Dr. J 9 00:00:46,227 --> 00:00:48,741 EPISODE 28: Servicing Mission 4 a. k. a. Dr. Joe Liske. 10 00:00:48,776 --> 00:00:50,639 To scientists and the public alike, 11 00:00:50,640 --> 00:00:54,639 the NASA / ESA Hubble Space Telescope is an icon of scientific progress. 12 00:00:54,640 --> 00:00:58,705 Although more than 100 space observatories have been put into orbit over the years 13 00:00:58,706 --> 00:01:00,796 Hubble remains the best known. 14 00:01:00,797 --> 00:01:05,718 Its success story is based on amazing scientific results and stunning images. 15 00:01:05,719 --> 00:01:08,777 But much of this was only possible because once in a while 16 00:01:12,116 --> 00:01:12,293 astronauts went up there and paid Hubble a visit. 17 00:01:12,315 --> 00:01:14,066 Welcome to the Hubblecast. 18 00:01:14,067 --> 00:01:16,942 I'm actually quite excited because today we're going to look 19 00:01:16,977 --> 00:01:20,375 at the fifth, and final, Hubble Servicing Mission. 20 00:01:21,826 --> 00:01:26,317 The NASA / ESA Hubble Space Telescope is a remarkable feat of engineering 21 00:01:26,318 --> 00:01:29,411 that enable scientists to produce the stunning results 22 00:01:29,446 --> 00:01:31,386 we have all come to love. 23 00:01:31,387 --> 00:01:35,280 From the very beginning, the design of Hubble allowed the various instruments 24 00:01:35,332 --> 00:01:38,833 to be replaced over time, as scientists on the ground 25 00:01:38,869 --> 00:01:41,635 developed new, more powerful instruments. 26 00:01:41,636 --> 00:01:45,953 Now, a team of astronauts is making one final journey to Hubble 27 00:01:45,954 --> 00:01:49,879 to give it a 100,000 orbit service. 28 00:01:49,880 --> 00:01:52,348 This is the fifth servicing mission to Hubble. 29 00:01:52,349 --> 00:01:58,033 The first took place back in 1993 when, in a series of landmark spacewalks, 30 00:01:58,034 --> 00:02:01,891 astronauts corrected Hubble's nearsighted vision. 31 00:02:01,892 --> 00:02:07,661 Three further missions in 1997, 1999 and 2002, 32 00:02:07,696 --> 00:02:11,959 replaced various instruments and other components on Hubble. 33 00:02:13,512 --> 00:02:17,174 This fifth servicing mission has two main parts: 34 00:02:17,175 --> 00:02:19,855 the first is to install two new instruments 35 00:02:19,856 --> 00:02:22,804 and the second is to repair two existing instruments 36 00:02:22,854 --> 00:02:24,645 that are already on-board Hubble: 37 00:02:24,646 --> 00:02:27,532 the ACS camera and the STIS spectrograph. 38 00:02:27,533 --> 00:02:31,213 The first new instrument, the Wide Field Camera 3, 39 00:02:31,214 --> 00:02:33,900 is essentially an improved digital camera, 40 00:02:33,901 --> 00:02:37,636 just like the ones you and I may use for our holiday snapshots, 41 00:02:37,637 --> 00:02:41,320 except that this one boasts 16-megapixels, 42 00:02:41,355 --> 00:02:44,807 can observe in the ultraviolet, visible and infrared regimes, 43 00:02:44,868 --> 00:02:48,079 and it weights several hundred kilos! 44 00:02:48,666 --> 00:02:52,232 The second new instrument is the Cosmic Origin Spectrograph, 45 00:02:52,267 --> 00:02:54,083 which will work in the ultraviolet. 46 00:02:54,084 --> 00:02:57,488 Unlike cameras, a spectrograph doesn't take images, 47 00:02:57,489 --> 00:03:01,076 instead it breaks up the light into its constituent colours 48 00:03:01,111 --> 00:03:04,659 to show it spectrum, a bit like a rainbow. 49 00:03:05,283 --> 00:03:09,570 Because the new Wide Field Camera 3 images in several colours, 50 00:03:09,605 --> 00:03:13,095 making it the firs panchromatic instrument on Hubble, 51 00:03:13,096 --> 00:03:17,058 we can learn much about the composition of distant objects. 52 00:03:17,059 --> 00:03:21,476 Ultraviolet light reveals hot young stars burning brightly, 53 00:03:21,477 --> 00:03:24,997 yellow light reveals clouds of hydrogen gas, 54 00:03:24,998 --> 00:03:29,060 and red light reveals the glowing embers of oldest stars. 55 00:03:29,438 --> 00:03:32,075 By combining images taken in each colour, 56 00:03:32,076 --> 00:03:34,823 astronomers can see structure within galaxies 57 00:03:34,873 --> 00:03:38,462 and begin to learn how it changes over time. 58 00:03:38,463 --> 00:03:43,538 A young proto-galaxy in the early Universe blazes brightly in the ultraviolet. 59 00:03:43,539 --> 00:03:47,221 This light travels for 13 billion years to reach us, 60 00:03:47,222 --> 00:03:52,643 by which time this light is shifted into the red and near-infrared part of the spectrum, 61 00:03:52,644 --> 00:03:57,048 and allows astronomers to see galaxies in the early stages of evolution. 62 00:03:57,049 --> 00:04:00,843 The powerful new Cosmic Origin Spectrograph, COS, 63 00:04:00,844 --> 00:04:03,461 will investigate the gas between galaxies 64 00:04:03,462 --> 00:04:06,141 to learn more about its chemical composition 65 00:04:06,142 --> 00:04:08,881 and the early growth of stars in the Universe. 66 00:04:08,882 --> 00:04:13,044 It will do this by looking at how the light from very distant quasars 67 00:04:13,045 --> 00:04:16,092 is absorbed as it passes through the gas. 68 00:04:16,270 --> 00:04:20,736 Closer to home, this improved spectrograph can also detect young stars 69 00:04:20,771 --> 00:04:25,042 burning hotter than our Sun, embedded in the thick dust clouds 70 00:04:25,077 --> 00:04:30,013 that gave rise to their birth, clarifying the phenomenon of star formation. 71 00:04:30,767 --> 00:04:32,284 The second task on this mission 72 00:04:32,319 --> 00:04:35,183 is going to be a huge challenge for the astronauts. 73 00:04:35,184 --> 00:04:38,426 They have to repair two instruments that are already on-board Hubble, 74 00:04:38,427 --> 00:04:41,681 but which haven't been working properly for some time now. 75 00:04:41,682 --> 00:04:43,942 The problem is that these instruments 76 00:04:43,943 --> 00:04:46,376 were never designed to be repaired in space. 77 00:04:46,377 --> 00:04:49,159 That means that some very clever people have to invent 78 00:04:49,194 --> 00:04:52,786 new and dexterous tools to help them carry out the repairs. 79 00:04:53,323 --> 00:04:54,407 The second problem is 80 00:04:54,408 --> 00:04:57,659 that it is actually not that easy to play electrician in space. 81 00:04:57,660 --> 00:05:00,528 Astronauts wear really thick gloves. 82 00:05:00,529 --> 00:05:03,910 For them, any task is kind of like trying to peel an egg 83 00:05:03,955 --> 00:05:06,135 with really thick oven gloves. 84 00:05:10,235 --> 00:05:12,841 Except for them, it would be even harder. 85 00:05:12,842 --> 00:05:15,801 For example, they will have to undo more than one hundred screws 86 00:05:15,841 --> 00:05:17,620 without losing any. 87 00:05:17,621 --> 00:05:20,698 I'm sure they'll be doing a better job than me... 88 00:05:21,898 --> 00:05:25,636 The repaired STIS instrument will obtain spectra from objects, 89 00:05:25,637 --> 00:05:29,308 but at different wavelengths to the new COS instrument. 90 00:05:29,309 --> 00:05:32,619 For the first time, scientists will be able to simultaneously 91 00:05:32,681 --> 00:05:36,904 see spectra from across a wide range of wavelengths. 92 00:05:37,170 --> 00:05:40,021 Even with the introduction of the new Wide Field Camera, 93 00:05:40,022 --> 00:05:44,575 the repaired ACS instrument remains Hubble's most sensitive 94 00:05:44,576 --> 00:05:46,581 in the visible light range. 95 00:05:46,582 --> 00:05:49,379 It will continue to capture stunning images 96 00:05:49,380 --> 00:05:53,003 and help scientists unravel the mysteries of the Universe. 97 00:05:53,664 --> 00:05:58,017 In addition to the work on the instruments, Hubble itself will also get a service. 98 00:05:58,018 --> 00:06:00,596 Just like your car, after 100,000 orbits 99 00:06:00,631 --> 00:06:04,239 Hubble needs the equivalent of an oil change and a new set of tires. 100 00:06:04,240 --> 00:06:08,262 Astronauts will carry out extra spacewalks to replace some parts 101 00:06:08,263 --> 00:06:12,161 that will keep Hubble flying hopefully well into the next decade. 102 00:06:12,162 --> 00:06:14,505 They will also attach a special mechanism 103 00:06:14,540 --> 00:06:18,163 that will allow a future robotic spacecraft to dock with Hubble 104 00:06:18,198 --> 00:06:21,589 in order to steer it to a peaceful, final resting place in the ocean. 105 00:06:24,790 --> 00:06:29,544 Upgrades to the power and guidance systems will give Hubble a new lease of life. 106 00:06:29,545 --> 00:06:31,936 A rejuvenated Hubble will allow astronomers 107 00:06:31,971 --> 00:06:36,856 to continue making remarkable discoveries for many years to come. 108 00:06:46,283 --> 00:06:47,395 Impressive, isn't it? 109 00:06:47,396 --> 00:06:51,240 It looks like this servicing mission is going to make Hubble better than ever. 110 00:06:51,241 --> 00:06:53,094 I'm already looking forward to bringing you 111 00:06:53,151 --> 00:06:56,560 the exciting discoveries from these instruments later this year. 112 00:06:56,561 --> 00:07:01,584 Look out for updates on the servicing mission on our website at spacetelescope.org 113 00:07:01,585 --> 00:07:04,131 This is Dr. J signing off for the Hubblecast. 114 00:07:04,132 --> 00:07:08,868 Once again, nature has surprised us beyond our wildest imagination... 115 00:07:12,427 --> 00:07:14,427 Hubblecast is produced by ESA / Hubble 116 00:07:14,428 --> 00:07:16,428 at the European Southern Observatory in Germany. 117 00:07:17,444 --> 00:07:19,444 The Hubble mission is a project of international cooperation 118 00:07:19,445 --> 00:07:21,445 between NASA and the European Space Agency.