1 00:00:17,590 --> 00:00:15,190 the james webb space telescope is what's 2 00:00:20,070 --> 00:00:17,600 known as a reflector telescope two 3 00:00:22,230 --> 00:00:20,080 mirrors one primary and one secondary 4 00:00:24,790 --> 00:00:22,240 used to collect and focus light coming 5 00:00:27,269 --> 00:00:24,800 from far away objects they're looking at 6 00:00:29,509 --> 00:00:27,279 the primary mirror on james webb is so 7 00:00:31,910 --> 00:00:29,519 huge it needs to be assembled from 18 8 00:00:33,670 --> 00:00:31,920 separate mirrors to find out more about 9 00:00:35,510 --> 00:00:33,680 these mirrors and how nasa is making 10 00:00:37,190 --> 00:00:35,520 sure they work as well in space as they 11 00:00:38,950 --> 00:00:37,200 do on the ground we've come to the 12 00:00:41,270 --> 00:00:38,960 marshall space flight center in 13 00:00:43,430 --> 00:00:41,280 huntsville alabama we're here with jeff 14 00:00:45,270 --> 00:00:43,440 cagley and he's the director of the 15 00:00:47,190 --> 00:00:45,280 x-ray and cryogenic facility here at 16 00:00:48,790 --> 00:00:47,200 marshall space flight center so jeff 17 00:00:50,470 --> 00:00:48,800 tell us a little bit about where we are 18 00:00:52,950 --> 00:00:50,480 and what are you about to see 19 00:00:54,790 --> 00:00:52,960 mary we are in the entry area for our 20 00:00:56,869 --> 00:00:54,800 large clean room 21 00:00:58,549 --> 00:00:56,879 these james webb space telescopes 22 00:01:00,229 --> 00:00:58,559 mirrors have to stay in a very clean 23 00:01:01,430 --> 00:01:00,239 environment and we have that type of 24 00:01:02,869 --> 00:01:01,440 environment here so we're going to see 25 00:01:04,869 --> 00:01:02,879 if we can get a better look at those 26 00:01:05,990 --> 00:01:04,879 mirrors and to do that we're going to 27 00:01:07,830 --> 00:01:06,000 have to 28 00:01:27,749 --> 00:01:07,840 get dressed up a little bit so that only 29 00:01:32,789 --> 00:01:29,990 we're just about to pull the entire test 30 00:01:36,550 --> 00:01:32,799 stand assembly into the vacuum chamber 31 00:01:38,550 --> 00:01:36,560 with the three james webb mirrors aboard 32 00:01:41,190 --> 00:01:38,560 i noticed there's just three mirrors why 33 00:01:42,950 --> 00:01:41,200 is that i think james webb has 18 right 34 00:01:44,870 --> 00:01:42,960 right the james webb telescope is made 35 00:01:46,310 --> 00:01:44,880 up of 18 mirrors we're going to have 36 00:01:47,670 --> 00:01:46,320 each one of those mirrors come through 37 00:01:49,429 --> 00:01:47,680 here twice 38 00:01:51,749 --> 00:01:49,439 the first time through we actually 39 00:01:53,830 --> 00:01:51,759 measure the deformation as a function of 40 00:01:56,389 --> 00:01:53,840 temperature as we transition down to 41 00:01:58,230 --> 00:01:56,399 minus 400 degrees fahrenheit 42 00:02:00,149 --> 00:01:58,240 the second time through we verify that 43 00:02:01,749 --> 00:02:00,159 the mirrors actually perform correctly 44 00:02:03,030 --> 00:02:01,759 at that temperature 45 00:02:04,389 --> 00:02:03,040 and you said it's about to go into the 46 00:02:05,670 --> 00:02:04,399 chamber can we go inside the chamber 47 00:02:07,429 --> 00:02:05,680 just to see what it's like and maybe 48 00:02:09,109 --> 00:02:07,439 tell us a little bit about the chamber 49 00:02:14,630 --> 00:02:09,119 yeah we'll try to run in there and see 50 00:02:18,630 --> 00:02:16,710 the mirrors behind us will be pulled in 51 00:02:20,630 --> 00:02:18,640 and we'll will actually reside just up 52 00:02:22,710 --> 00:02:20,640 in front of us here inside the chamber 53 00:02:25,510 --> 00:02:22,720 where they can be cooled to minus 400 54 00:02:27,270 --> 00:02:25,520 degrees why a vacuum chamber 55 00:02:29,350 --> 00:02:27,280 well we have to simulate not only the 56 00:02:31,990 --> 00:02:29,360 thermal environment but also the vacuum 57 00:02:34,150 --> 00:02:32,000 environment of space you pull these in 58 00:02:37,030 --> 00:02:34,160 and what kind of things are you looking 59 00:02:38,790 --> 00:02:37,040 for in the mirror well the the ball 60 00:02:40,390 --> 00:02:38,800 aerospace team is actually responsible 61 00:02:41,990 --> 00:02:40,400 for the testing and they will actually 62 00:02:44,309 --> 00:02:42,000 be looking at these 63 00:02:46,710 --> 00:02:44,319 mirrors as they transition to cryogenic 64 00:02:48,630 --> 00:02:46,720 temperature through a window up in the 65 00:02:50,550 --> 00:02:48,640 front of our vacuum chamber and they'll 66 00:02:52,869 --> 00:02:50,560 be looking at these mirrors with an 67 00:02:54,309 --> 00:02:52,879 instrument called an interferometer 68 00:02:56,550 --> 00:02:54,319 and that's going to give them a very 69 00:02:58,790 --> 00:02:56,560 detailed surface map 70 00:03:00,070 --> 00:02:58,800 of what that mirror looks like and how 71 00:03:02,149 --> 00:03:00,080 it deforms 72 00:03:04,309 --> 00:03:02,159 as a function of temperature and my last 73 00:03:06,550 --> 00:03:04,319 question is why is it so important to be 74 00:03:08,710 --> 00:03:06,560 so precise with these mirrors 75 00:03:09,750 --> 00:03:08,720 well the primary mirror for a telescope 76 00:03:11,030 --> 00:03:09,760 is the 77 00:03:13,350 --> 00:03:11,040 part of the telescope that really 78 00:03:15,110 --> 00:03:13,360 matters it's gathering all the light 79 00:03:16,229 --> 00:03:15,120 that ultimately gets focused on the 80 00:03:18,470 --> 00:03:16,239 instrument 81 00:03:29,990 --> 00:03:18,480 and the larger and the better the 82 00:03:33,910 --> 00:03:31,430 these mirrors will be in the vacuum 83 00:03:36,070 --> 00:03:33,920 chamber for about 15 weeks going through 84 00:03:38,390 --> 00:03:36,080 seven cycles of temperature changes from 85 00:03:39,390 --> 00:03:38,400 room temperature to the cold extreme of 86 00:03:42,949 --> 00:03:39,400 space