WEBVTT FILE 1 00:00:00.000 --> 00:00:13.580 (music) 2 00:00:13.580 --> 00:00:17.580 I'm Kathy Thornton. I was a mission specialist on the first service mission 3 00:00:17.580 --> 00:00:22.980 on Hubble Space Telescope in 1993. It's amazing to me when I was flying 4 00:00:22.980 --> 00:00:26.880 in space, orbiting, that I could look back at the Earth and you don't see a lot of 5 00:00:26.880 --> 00:00:31.829 evidence that we're here, but yet those little tiny beings down on Earth that I 6 00:00:31.829 --> 00:00:42.240 can't see we're smart enough to get me there. We were not the most significant 7 00:00:42.240 --> 00:00:46.140 part. We might have been the most visible, but the real heroes of the service 8 00:00:46.140 --> 00:00:50.430 missions are the people who figure out how to do it. The people who came up with 9 00:00:50.430 --> 00:01:06.750 Russ: My name is Russ Werneth. I've been involved with all five of the 10 00:01:06.750 --> 00:01:11.880 Hubble Servicing Missions. Back in 1993 when we did our first servicing mission, 11 00:01:11.880 --> 00:01:19.409 I was involved in designing all the tools that we use. Kathy: On that mission, we did 12 00:01:19.409 --> 00:01:25.320 five spacewalks. I did the second and the fourth one. On my spacewalks we put in a 13 00:01:25.320 --> 00:01:30.810 new solar array and we installed the COSTAR, which included the corrective 14 00:01:30.810 --> 00:01:38.950 optics for all the axial instruments in the bottom part of the telescope. 15 00:01:39.490 --> 00:01:44.330 Kathy: We think a lot about the engineering technology that goes into Hubble 16 00:01:44.330 --> 00:01:50.240 and makes it work, and the innovation and design that goes into the fixes for the 17 00:01:50.240 --> 00:01:53.990 Hubble and every new instrument that goes up in the Hubble. And those are 18 00:01:53.990 --> 00:01:59.110 pretty amazing, but the purpose of the Hubble is science. 19 00:02:00.200 --> 00:02:06.780 The purpose of Hubble is to help us learn about where we came from. About 20 00:02:06.780 --> 00:02:14.729 what happened before us in this universe. 21 00:02:15.290 --> 00:02:19.939 Kathy: Servicing the Hubble one more time is well worth the risk to 22 00:02:19.939 --> 00:02:24.170 the crew and to the vehicle and to the Hubble itself. Every time we touch it you 23 00:02:24.170 --> 00:02:27.829 know, we plan to make it better, but you could always make it worse. 24 00:02:27.829 --> 00:02:32.329 And so there's some risk to the telescope as well. Russ: When we plan for a 25 00:02:32.329 --> 00:02:37.340 servicing mission with the astronauts, we always ask ourselves the questions 'what if.' 26 00:02:37.340 --> 00:02:44.049 What if this tool were to fail? What if this procedure wouldn't work? And 27 00:02:44.049 --> 00:02:47.780 therefore we do all the training that's necessary. 28 00:02:47.780 --> 00:02:57.090 We have contingency tools, we have backup tools, we have backup procedures. 29 00:02:57.090 --> 00:03:02.470 There was a hand rail that had to be removed, and as much as we practiced on 30 00:03:02.470 --> 00:03:06.760 the ground with tools and procedures, that hand rail couldn't be removed 31 00:03:06.760 --> 00:03:14.260 because of one of the bolts. As Mike Massimino was working, in real time with his 32 00:03:14.260 --> 00:03:19.330 EVA, his spacewalk, we were working on the ground to figure out how we could 33 00:03:19.330 --> 00:03:27.930 solve that problem. And we went through several levels of contingency. 34 00:03:28.470 --> 00:03:36.160 Then ultimately, it came down to just using brute force on that hand rail to 35 00:03:36.160 --> 00:03:43.180 get that bolt to break. And we've essentially been able to leave a new telescope every 36 00:03:43.180 --> 00:03:47.670 time we finish up a servicing mission. Kathy: I 37 00:03:47.670 --> 00:03:53.170 have a picture on my wall of the first Hubble Deep Field photos, where 38 00:03:53.170 --> 00:03:57.989 Hubble was pointed at place in the sky where there wasn't anything. 39 00:03:58.350 --> 00:04:03.370 But imagine that you could look through a straw or a pinhole and find a place 40 00:04:03.370 --> 00:04:07.480 in the sky where there's absolutely nothing, and know that there are millions 41 00:04:07.480 --> 00:04:13.150 of galaxies in that little pinhole that you're looking at. I think more than 42 00:04:13.150 --> 00:04:18.910 anything else Hubble is an icon of science, of exploration, and of the things 43 00:04:18.910 --> 00:04:23.100 we as humans can do. 44 00:04:23.100 --> 00:04:30.200 (music)