1 00:00:00,000 --> 00:00:04,000 [Music throughout] 2 00:00:04,000 --> 00:00:08,000 Narrator: When it opens its eyes to our universe in the mid-2020s, WFIRST, 3 00:00:08,000 --> 00:00:12,000 the Wide Field Infrared Survey Telescope, will capture 4 00:00:12,000 --> 00:00:16,000 images unlike any satellite before it. WFIRST 5 00:00:16,000 --> 00:00:20,000 will have the same image resolution as Hubble, but will cover an area 6 00:00:20,000 --> 00:00:24,000 100 times larger. WFIRST will also view the sky 7 00:00:24,000 --> 00:00:28,000 in carefully selected wavelengths of infrared light which will allow it 8 00:00:28,000 --> 00:00:32,000 to see through obscuring dust to reveal hidden stars and 9 00:00:32,000 --> 00:00:36,000 watch the growth of galaxies over the last 10 billion years. 10 00:00:36,000 --> 00:00:40,000 To see what the sky will look like to WFIRST, 11 00:00:40,000 --> 00:00:44,000 scientists use special processing techniques to create simulated images. 12 00:00:44,000 --> 00:00:48,000 In this case, they began with a Hubble mosaic 13 00:00:48,000 --> 00:00:52,000 of Andromeda, one of the closest galaxies to our own. 14 00:00:52,000 --> 00:00:56,000 Released in 2015, this mosaic was created out of over 15 00:00:56,000 --> 00:01:00,000 400 individual Hubble images and took more than three years. 16 00:01:00,000 --> 00:01:04,000 Because of its enormous coverage, WFIRST 17 00:01:04,000 --> 00:01:08,000 will be able to create a similar mosaic with just two images, each 18 00:01:08,000 --> 00:01:12,000 taking about 90 minutes. WFIRST images are 19 00:01:12,000 --> 00:01:16,000 actually made of 18 separate panels, each one corresponding to 20 00:01:16,000 --> 00:01:20,000 a single 16-megapixel detector. The arrangement of these 21 00:01:20,000 --> 00:01:24,000 detectors creates the distinctive WFIRST image shape. 22 00:01:24,000 --> 00:01:28,000 The simulated image is not just special because of its 23 00:01:28,000 --> 00:01:32,000 size, however. It also shows Andromeda as it will appear through 24 00:01:32,000 --> 00:01:36,000 WFIRST’s optics and infrared filters. To achieve 25 00:01:36,000 --> 00:01:40,000 this, scientists started with Hubble filters that are closest to WFIRST's. 26 00:01:40,000 --> 00:01:44,000 Then they used software to measure the positions 27 00:01:44,000 --> 00:01:48,000 and brightnesses of the roughly 100 million stars in those images 28 00:01:48,000 --> 00:01:52,000 and applied those as input to WFIRST image simulation software 29 00:01:52,000 --> 00:01:56,000 which added each star back to the image after applying the expected 30 00:01:56,000 --> 00:02:00,000 effects of the WFIRST optics, filters, and detectors. 31 00:02:00,000 --> 00:02:04,000 The resulting image reveals many stars 32 00:02:04,000 --> 00:02:08,000 that were blocked by dust in visible light. It highlights 33 00:02:08,000 --> 00:02:12,000 WFIRST’s role in providing a more comprehensive view of the stars in the local 34 00:02:12,000 --> 00:02:16,000 universe. WFIRST will also use its broad view 35 00:02:16,000 --> 00:02:20,000 to search for planets around other stars in our galaxy and to look for the 36 00:02:20,000 --> 00:02:24,000 fingerprint of dark matter and dark energy in the distant reaches of the universe. 37 00:02:24,000 --> 00:02:28,000 With an unprecedented combination of breadth and 38 00:02:28,000 --> 00:02:32,000 depth, WFIRST will open a new era in 39 00:02:32,000 --> 00:02:36,000 viewing our universe. 40 00:02:36,000 --> 00:02:42,820 [Explore: Solar system & beyond] 41 00:02:42,820 --> 00:02:42,816 [NASA]