1 00:00:00,000 --> 00:00:04,000 [Music Throughout] 2 00:00:04,000 --> 00:00:08,000 In 2004, NASA’s Hubble Space Telescope changed astronomy 3 00:00:08,000 --> 00:00:12,000 forever when astronomers revealed the first ultra-deep field 4 00:00:12,000 --> 00:00:16,000 image. Created with more than 270 hours 5 00:00:16,000 --> 00:00:20,000 of observation over the course of a year, it is our farthest ever 6 00:00:20,000 --> 00:00:24,000 visible-light image of the universe. This tiny window 7 00:00:24,000 --> 00:00:28,000 revealed thousands of galaxies in a seemingly empty patch of sky. 8 00:00:28,000 --> 00:00:32,000 We can’t see any farther in visible light 9 00:00:32,000 --> 00:00:36,000 because the unrelenting expansion of space has stretched galaxies’ 10 00:00:36,000 --> 00:00:40,000 ultraviolet glow into red light. More distant 11 00:00:40,000 --> 00:00:44,000 galaxies are mostly detectable in infrared. 12 00:00:44,000 --> 00:00:48,000 That’s why, in 2009, Hubble captured an infrared 13 00:00:48,000 --> 00:00:52,000 ultra-deep field image that probed even deeper into the same spot. 14 00:00:52,000 --> 00:00:56,000 It remains one of the most distant images ever 15 00:00:56,000 --> 00:01:00,000 made, and a key source of information about some of the universe’s 16 00:01:00,000 --> 00:01:04,000 early history. 17 00:01:04,000 --> 00:01:08,000 The Nancy Grace Roman Space Telescope will have infrared resolution 18 00:01:08,000 --> 00:01:12,000 and capabilities similar to Hubble, but each image will cover 19 00:01:12,000 --> 00:01:16,000 200 times the area of sky. A potential 20 00:01:16,000 --> 00:01:20,000 Roman ultra-deep field could be far faster to capture, yet cover 21 00:01:20,000 --> 00:01:24,000 hundreds of times as much of the early universe. 22 00:01:24,000 --> 00:01:28,000 To further explore this potential, a team of researchers 23 00:01:28,000 --> 00:01:32,000 has created a simulated ultra-deep field image. 24 00:01:32,000 --> 00:01:36,000 The entire image contains about one square degree of sky, 25 00:01:36,000 --> 00:01:40,000 or about 5 full moons. Even a single 26 00:01:40,000 --> 00:01:44,000 Roman field of view contains a staggering number of distant galaxies, 27 00:01:44,000 --> 00:01:48,000 each one filled with billions of stars. 28 00:01:48,000 --> 00:01:52,000 This computer-generated 29 00:01:52,000 --> 00:01:56,000 image represents the distribution of galaxies that researchers expect to find, 30 00:01:56,000 --> 00:02:00,000 based on the existing Hubble observations. It will 31 00:02:00,000 --> 00:02:04,000 help astronomers determine how best to conduct an actual Roman 32 00:02:04,000 --> 00:02:08,000 ultra-deep field and anticipate the measurements and conclusions they might 33 00:02:08,000 --> 00:02:12,000 be able to make. Because light travels 34 00:02:12,000 --> 00:02:16,000 at a finite speed, distant images are also snapshots 35 00:02:16,000 --> 00:02:20,000 earlier in time. Ultra-deep field images reveal a 36 00:02:20,000 --> 00:02:24,000 time from about 200 million to 1 billion years after the 37 00:02:24,000 --> 00:02:28,000 big bang. Roman’s image would be the largest 38 00:02:28,000 --> 00:02:32,000 observation of its kind for this time period and could reveal 39 00:02:32,000 --> 00:02:36,000 key features in the adolescent universe, including rare 40 00:02:36,000 --> 00:02:40,000 ‘infant’ galaxies that eventually evolve into mature galaxies 41 00:02:40,000 --> 00:02:44,000 like our own Milky Way. 42 00:02:44,000 --> 00:02:48,000 With Roman set to launch by 2027, this simulated 43 00:02:48,000 --> 00:02:52,000 ultra-deep field image is just one example of the 44 00:02:52,000 --> 00:02:56,000 fantastic results this upcoming mission could bring 45 00:02:56,000 --> 00:03:00,000 by the end of the decade. 46 00:03:00,000 --> 00:03:04,000 47 00:03:04,000 --> 00:03:05,963 [NASA]