1 00:00:01,668 --> 00:00:04,471 [Music throughout] Satellite names aren't always easy to understand, 2 00:00:04,471 --> 00:00:09,976 but NASA's Neil Gehrels Swift Observatory states its key ability up front. 3 00:00:10,043 --> 00:00:12,946 Launched on Nov. 20, 2004, 4 00:00:12,946 --> 00:00:15,849 Swift is first and foremost a rapid response 5 00:00:15,849 --> 00:00:18,852 gamma-ray burst explorer. 6 00:00:18,985 --> 00:00:21,354 Gamma-ray bursts, or GRBs, 7 00:00:21,354 --> 00:00:24,290 are the most powerful explosions in the universe. 8 00:00:24,290 --> 00:00:27,827 They arise when massive stars run out of fuel and collapse, 9 00:00:27,894 --> 00:00:32,232 or when pairs of orbiting neutron stars collide. 10 00:00:32,298 --> 00:00:36,269 GRBs can be as brief as a few milliseconds, are very rare, 11 00:00:36,436 --> 00:00:40,640 and happen in distant galaxies, which makes them hard to spot. 12 00:00:40,740 --> 00:00:45,912 Despite this, Swift has managed to observe 1,800 GRBs. 13 00:00:47,514 --> 00:00:49,482 Scientists and engineers designed 14 00:00:49,482 --> 00:00:53,620 Swift's GRB detector to see large portions of the sky and quickly 15 00:00:53,620 --> 00:00:58,525 relay a GRB’s location to the ground so other missions could follow up. 16 00:00:58,591 --> 00:01:03,329 They also enabled Swift to change where it's looking very rapidly so it can target 17 00:01:03,329 --> 00:01:08,201 its X-ray and ultraviolet/optical telescopes on any detected event. 18 00:01:09,235 --> 00:01:12,739 Swift owes much of its existence to Neil Gehrels, 19 00:01:12,806 --> 00:01:16,276 who was a scientist at NASA's Goddard Space Flight Center. 20 00:01:16,342 --> 00:01:19,079 Neil was a global figure in gamma-ray astronomy 21 00:01:19,079 --> 00:01:21,281 and gamma-ray bursts in particular. 22 00:01:21,915 --> 00:01:26,286 He was part of the small group that first imagined Swift in 1998 23 00:01:26,352 --> 00:01:30,824 and was instrumental in seeing it through to launch and into its early mission. 24 00:01:30,890 --> 00:01:33,726 After Neil passed away in 2017, 25 00:01:33,726 --> 00:01:36,729 Swift was renamed in his honor. 26 00:01:36,863 --> 00:01:39,265 Over its 20 years of operation, 27 00:01:39,265 --> 00:01:42,268 Swift has proven incredibly useful and versatile. 28 00:01:42,469 --> 00:01:46,806 Its rapid detection, alerts, and repointing have allowed missions 29 00:01:46,806 --> 00:01:51,711 like NASA's Chandra, Webb and Hubble to quickly follow up on transient events. 30 00:01:51,811 --> 00:01:56,549 Beyond GRB detections, Swift's X-ray and ultraviolet/optical telescopes 31 00:01:56,783 --> 00:02:01,054 have enabled it to perform science that no one imagined prior to launch. 32 00:02:01,154 --> 00:02:03,890 Swift has tracked near-Earth asteroids, 33 00:02:03,890 --> 00:02:08,661 observed more distant asteroid collisions, studied comets, 34 00:02:08,661 --> 00:02:10,997 seen massive flares on distant stars, 35 00:02:10,997 --> 00:02:14,067 taken ultraviolet surveys of nearby galaxies, 36 00:02:14,167 --> 00:02:18,338 and made countless observations of short-lived cosmic phenomena. 37 00:02:19,305 --> 00:02:22,308 Despite the failure of one of the spinning reaction wheels 38 00:02:22,308 --> 00:02:24,410 that enable Swift's rapid turning, 39 00:02:24,477 --> 00:02:28,114 the spacecraft remains as nimble as it was in its first year, 40 00:02:28,214 --> 00:02:30,850 and it promises to remain a critical first 41 00:02:30,850 --> 00:02:34,087 responder in NASA's astrophysics fleet. 42 00:02:35,989 --> 00:02:40,693 [NASA]