WEBVTT FILE 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.