WEBVTT FILE 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]