1 00:00:17,590 --> 00:00:15,350 the james webb space telescope is a 2 00:00:19,349 --> 00:00:17,600 reflecting telescope which means it 3 00:00:22,630 --> 00:00:19,359 images the universe with the help of 4 00:00:25,349 --> 00:00:22,640 mirrors we are here at l3 ios tinsley in 5 00:00:28,390 --> 00:00:25,359 richmond california to find out just how 6 00:00:30,710 --> 00:00:28,400 the observatory will work 7 00:00:33,030 --> 00:00:30,720 so i'd like to first show you one of our 8 00:00:34,630 --> 00:00:33,040 primary mirror segments and before we 9 00:00:38,389 --> 00:00:34,640 get too close we'll want to put our mask 10 00:00:40,150 --> 00:00:38,399 on to protect the optical surface okay 11 00:00:41,350 --> 00:00:40,160 this is one of our 18 primary mirror 12 00:00:43,590 --> 00:00:41,360 segments once they're all complete 13 00:00:45,110 --> 00:00:43,600 they'll combine to make one large 14 00:00:46,549 --> 00:00:45,120 primary mirror 15 00:00:49,029 --> 00:00:46,559 you can see the front side surface is 16 00:00:50,869 --> 00:00:49,039 highly polished and as we rotate to the 17 00:00:53,350 --> 00:00:50,879 backside surface you'll see that there 18 00:00:55,029 --> 00:00:53,360 is a honeycomb light waiting 19 00:00:57,430 --> 00:00:55,039 so it reduces the payload when it goes 20 00:00:58,869 --> 00:00:57,440 up into space and yet it's very stiff 21 00:01:01,750 --> 00:00:58,879 looks like you can attach things to it 22 00:01:04,469 --> 00:01:01,760 too yes they bond more hardware on the 23 00:01:06,310 --> 00:01:04,479 backside surface which makes it an even 24 00:01:08,230 --> 00:01:06,320 stronger structure and that's the way 25 00:01:09,350 --> 00:01:08,240 it'll go up in the space 26 00:01:10,950 --> 00:01:09,360 there are several other mirrors that 27 00:01:13,190 --> 00:01:10,960 we're doing here for james webb space 28 00:01:15,109 --> 00:01:13,200 telescope we have a 29 00:01:16,630 --> 00:01:15,119 secondary mirror element we have a 30 00:01:18,550 --> 00:01:16,640 tertiary mirror element and we're also 31 00:01:20,149 --> 00:01:18,560 doing the fine steering mirror that's 32 00:01:22,390 --> 00:01:20,159 for those of us who don't understand how 33 00:01:23,510 --> 00:01:22,400 a telescope works why do you have so 34 00:01:24,870 --> 00:01:23,520 many mirrors 35 00:01:26,550 --> 00:01:24,880 the light that comes from space is 36 00:01:29,190 --> 00:01:26,560 collected into the primary mirrors 37 00:01:30,789 --> 00:01:29,200 primary mirrors then take that light and 38 00:01:32,469 --> 00:01:30,799 image and bring it to the secondary 39 00:01:34,630 --> 00:01:32,479 mirror which 40 00:01:36,469 --> 00:01:34,640 projects it to the tertiary mirror and 41 00:01:37,590 --> 00:01:36,479 then that goes to the fine steering 42 00:01:39,590 --> 00:01:37,600 mirror and then with fine steering 43 00:01:41,590 --> 00:01:39,600 mirror they're able to adjust it move it 44 00:01:44,149 --> 00:01:41,600 around and get the images that they're 45 00:01:46,630 --> 00:01:44,159 looking for why all the bouncing around 46 00:01:49,429 --> 00:01:46,640 well the mirrors work together to 47 00:01:51,109 --> 00:01:49,439 reduce the aperture size to a format 48 00:01:52,630 --> 00:01:51,119 that can fit on a camera that we can 49 00:01:53,590 --> 00:01:52,640 image now that we've seen the primary 50 00:01:55,830 --> 00:01:53,600 mirror i'd love to show you the 51 00:01:57,749 --> 00:01:55,840 secondary mirror 52 00:02:00,389 --> 00:01:57,759 so andrea what's going on here 53 00:02:02,069 --> 00:02:00,399 we are performing a microscope 54 00:02:03,670 --> 00:02:02,079 inspection of the surface what he's 55 00:02:05,670 --> 00:02:03,680 doing here is he's getting very close to 56 00:02:06,789 --> 00:02:05,680 the optical surface so that he can 57 00:02:08,389 --> 00:02:06,799 capture 58 00:02:10,550 --> 00:02:08,399 surface data and then we can look at 59 00:02:12,790 --> 00:02:10,560 that later on and you can see this one 60 00:02:14,949 --> 00:02:12,800 is unique compared to the other mirrors 61 00:02:16,790 --> 00:02:14,959 this one is a convex hyperbola whereas 62 00:02:19,430 --> 00:02:16,800 the primary mirror and the tertiary 63 00:02:21,190 --> 00:02:19,440 mirror all concave 64 00:02:23,190 --> 00:02:21,200 and there's only one of these 65 00:02:25,110 --> 00:02:23,200 there's only one of these 66 00:02:26,949 --> 00:02:25,120 so on the telescope the 67 00:02:28,790 --> 00:02:26,959 light captured from the primary bounces 68 00:02:30,550 --> 00:02:28,800 onto this next right yep that's why they 69 00:02:33,190 --> 00:02:30,560 called the secondary element 70 00:02:34,949 --> 00:02:33,200 two switches i could pick two 71 00:02:37,190 --> 00:02:34,959 we also have the tertiary mirror which 72 00:02:38,710 --> 00:02:37,200 is a concave ellipse 73 00:02:40,309 --> 00:02:38,720 this is a onesie mirror just like the 74 00:02:43,110 --> 00:02:40,319 secondary in the fine steering mirror 75 00:02:45,030 --> 00:02:43,120 it's a one of a kind in a telescope 76 00:02:47,030 --> 00:02:45,040 and with this mirror we run through the 77 00:02:49,190 --> 00:02:47,040 same sort of rigorous testing that we do 78 00:02:50,470 --> 00:02:49,200 for the primary in the secondary mirror 79 00:02:52,309 --> 00:02:50,480 and we get down to those tight 80 00:02:54,710 --> 00:02:52,319 specifications that are required to 81 00:02:56,150 --> 00:02:54,720 maximize the image resolution thanks a 82 00:02:57,990 --> 00:02:56,160 lot for your time andrew and showing us 83 00:03:00,309 --> 00:02:58,000 your mirrors welcome 84 00:03:02,869 --> 00:03:00,319 andrea showed us a segment of the 85 00:03:04,949 --> 00:03:02,879 primary mirror the secondary mirror and 86 00:03:07,190 --> 00:03:04,959 the tertiary mirror she wasn't able to 87 00:03:09,589 --> 00:03:07,200 show us the fine steering mirror that's 88 00:03:11,750 --> 00:03:09,599 the mirror that keeps the beam of light 89 00:03:13,910 --> 00:03:11,760 collected by the telescope centered and 90 00:03:16,070 --> 00:03:13,920 stabilized that's because that fine 91 00:03:18,070 --> 00:03:16,080 steering mirror is inside this thermal 92 00:03:19,910 --> 00:03:18,080 chamber going through some extreme 93 00:03:21,509 --> 00:03:19,920 temperature changes to simulate the 94 00:03:23,030 --> 00:03:21,519 conditions of space