1 00:00:05,269 --> 00:00:03,510 [Music] 2 00:00:08,150 --> 00:00:05,279 the wide field instrument is the heart 3 00:00:09,669 --> 00:00:08,160 of the nancy grace roman space telescope 4 00:00:11,669 --> 00:00:09,679 it is what allows the roman space 5 00:00:14,150 --> 00:00:11,679 telescope to take pictures with the same 6 00:00:17,269 --> 00:00:14,160 detail as hubble but covering an area 7 00:00:19,670 --> 00:00:17,279 100 times larger despite this incredible 8 00:00:21,830 --> 00:00:19,680 power the basic design is the same as 9 00:00:24,150 --> 00:00:21,840 telescopes around the world 10 00:00:25,269 --> 00:00:24,160 light enters through roman's 2.4 meter 11 00:00:27,029 --> 00:00:25,279 aperture 12 00:00:29,349 --> 00:00:27,039 and is reflected and focused by the 13 00:00:31,990 --> 00:00:29,359 curved main mirror which is also the 14 00:00:34,229 --> 00:00:32,000 largest mirror in the telescope 15 00:00:36,389 --> 00:00:34,239 this light is reflected and focused once 16 00:00:38,630 --> 00:00:36,399 more by the secondary mirror 17 00:00:40,549 --> 00:00:38,640 more elements tighten the beam and strip 18 00:00:42,630 --> 00:00:40,559 it of stray light rays before it passes 19 00:00:44,790 --> 00:00:42,640 through the filter wheel 20 00:00:46,470 --> 00:00:44,800 this wheel has a variety of filters that 21 00:00:47,910 --> 00:00:46,480 allow different wavelengths of light to 22 00:00:50,229 --> 00:00:47,920 pass through 23 00:00:52,790 --> 00:00:50,239 it spins from one to another depending 24 00:00:54,950 --> 00:00:52,800 on what the researcher is looking for 25 00:00:57,029 --> 00:00:54,960 finally the focused and filtered light 26 00:00:58,950 --> 00:00:57,039 reaches the focal plane where it creates 27 00:01:00,869 --> 00:00:58,960 an image on the detectors 28 00:01:03,029 --> 00:01:00,879 these detectors use the photoelectric 29 00:01:05,270 --> 00:01:03,039 effect to convert photons into an 30 00:01:07,190 --> 00:01:05,280 electrical signal that is then decoded 31 00:01:09,990 --> 00:01:07,200 into an image 32 00:01:12,230 --> 00:01:10,000 in roman's case there are 18 detectors 33 00:01:15,990 --> 00:01:12,240 allowing it to create 300 million pixel 34 00:01:18,550 --> 00:01:16,000 images of large patches of the sky 35 00:01:21,270 --> 00:01:18,560 the large number of detectors and pixels 36 00:01:23,030 --> 00:01:21,280 gives roman its wide field of view 37 00:01:25,190 --> 00:01:23,040 the size of the mirror and the precision 38 00:01:26,950 --> 00:01:25,200 of its optics gives roman its fine 39 00:01:29,030 --> 00:01:26,960 imaging 40 00:01:31,270 --> 00:01:29,040 this combination of image size and 41 00:01:33,350 --> 00:01:31,280 detail has never been possible on a 42 00:01:35,190 --> 00:01:33,360 space-based telescope before and will 43 00:01:37,830 --> 00:01:35,200 make the nancy grace roman space