1 00:00:00,000 --> 00:00:03,980 [Music throughout] 2 00:00:04,000 --> 00:00:07,980 Narrator: When it opens its eyes to our universe in the mid-2020s, the 3 00:00:08,000 --> 00:00:11,980 Nancy Grace Roman Space Telescope, will capture images unlike any 4 00:00:12,000 --> 00:00:15,980 satellite before it. The Roman Space Telescope 5 00:00:16,000 --> 00:00:19,980 will have the same image resolution as Hubble, but will cover an area 6 00:00:20,000 --> 00:00:23,980 100 times larger. Roman will also view the sky 7 00:00:24,000 --> 00:00:27,980 in carefully selected wavelengths of infrared light which will allow it 8 00:00:28,000 --> 00:00:31,980 to see through obscuring dust to reveal hidden stars and 9 00:00:32,000 --> 00:00:35,980 watch the growth of galaxies over the last 10 billion years. 10 00:00:36,000 --> 00:00:39,980 To see what the sky will look like to Roman, 11 00:00:40,000 --> 00:00:43,980 scientists use special processing techniques to create simulated images. 12 00:00:44,000 --> 00:00:47,980 In this case, they began with a Hubble mosaic 13 00:00:48,000 --> 00:00:51,980 of Andromeda, one of the closest galaxies to our own. 14 00:00:52,000 --> 00:00:55,980 Released in 2015, this mosaic was created out of over 15 00:00:56,000 --> 00:00:59,980 400 individual Hubble images and took more than three years. 16 00:01:00,000 --> 00:01:03,980 Because of its enormous coverage, Roman 17 00:01:04,000 --> 00:01:07,980 will be able to create a similar mosaic with just two images, each 18 00:01:08,000 --> 00:01:11,980 taking about 90 minutes. Roman Space Telescope 19 00:01:12,000 --> 00:01:15,980 images are actually made of 18 separate panels, each one 20 00:01:16,000 --> 00:01:19,980 corresponding to a single 16-megapixel detector. The arrangement of 21 00:01:20,000 --> 00:01:23,980 these detectors creates the distinctive Roman image shape. 22 00:01:24,000 --> 00:01:27,980 The simulated image is not just special because of its 23 00:01:28,000 --> 00:01:31,980 size, however. It also shows Andromeda as it will appear through 24 00:01:32,000 --> 00:01:35,980 Roman’s optics and infrared filters. To achieve this, 25 00:01:36,000 --> 00:01:39,980 scientists started with Hubble filters that are closest to Roman's. 26 00:01:40,000 --> 00:01:43,980 Then they used software to measure the positions 27 00:01:44,000 --> 00:01:47,980 and brightnesses of the roughly 100 million stars in those images 28 00:01:48,000 --> 00:01:51,980 and applied those as input to Roman image simulation software 29 00:01:52,000 --> 00:01:55,980 which added each star back to the image after applying the expected 30 00:01:56,000 --> 00:01:59,980 effects of the Roman optics, filters, and detectors. 31 00:02:00,000 --> 00:02:03,980 The resulting image reveals many stars that were blocked 32 00:02:04,000 --> 00:02:07,980 by dust in visible light. It highlights the Roman Space 33 00:02:08,000 --> 00:02:11,980 Telescope’s role in providing a more comprehensive view of the stars in the local 34 00:02:12,000 --> 00:02:15,980 universe. Roman will also use its broad view to search 35 00:02:16,000 --> 00:02:19,980 for planets around other stars in our galaxy and to look for the 36 00:02:20,000 --> 00:02:23,980 fingerprint of dark matter and dark energy in the distant reaches of the universe. 37 00:02:24,000 --> 00:02:27,980 With an unprecedented combination of breadth and depth, 38 00:02:28,000 --> 00:02:31,980 the Nancy Grace Roman Space Telescope will open a new era 39 00:02:32,000 --> 00:02:35,980 in viewing our universe. 40 00:02:36,000 --> 00:02:42,800 [Explore: Solar system & beyond] 41 00:02:42,820 --> 00:02:42,743 [NASA]