1 00:00:00,020 --> 00:00:04,030 [Music throughout] The Wide Field Instrument is the heart of the Nancy Grace 2 00:00:04,050 --> 00:00:08,120 Roman Space Telescope. The basic design is the same as 3 00:00:08,140 --> 00:00:12,160 telescopes around the world. Light enters through Roman's 2.4-meter 4 00:00:12,180 --> 00:00:16,210 aperture, and is reflected and focused by the curved main mirror. 5 00:00:16,230 --> 00:00:20,260 More elements tighten the beam, and strip it of stray light rays 6 00:00:20,280 --> 00:00:24,440 before it passes through the filter wheel. This wheel has a 7 00:00:24,460 --> 00:00:28,540 variety of filters that allow different wavelengths of light to pass through. 8 00:00:28,560 --> 00:00:32,640 It spins from one to another depending on what the researcher is looking for. 9 00:00:32,660 --> 00:00:36,830 FInally, the focused and filtered light reaches the focal plane, 10 00:00:36,850 --> 00:00:41,020 where it creates an image on the detectors. In Roman's case, 11 00:00:41,040 --> 00:00:45,200 there are 18 detectors, allowing it to create 300-million-pixel images 12 00:00:45,220 --> 00:00:49,350 of large patches of the sky. This combination of image size 13 00:00:49,370 --> 00:00:53,430 and detail has never been possible on a space-based telescope before, 14 00:00:53,450 --> 00:00:57,560 and will make the Nancy Grace Roman Space Telescope an indispensible 15 00:00:57,580 --> 00:00:59,640 tool in the future.