WEBVTT FILE 1 00:00:00.000 --> 00:00:04.926 Fast radio bursts or FRBs, are extraordinary events 2 00:00:04.926 --> 00:00:08.220 that generate as much energy in a thousandth of a second 3 00:00:08.220 --> 00:00:12.089 as the Sun does in an entire year! 4 00:00:12.089 --> 00:00:15.061 Astronomers, using NASA’s Hubble Space Telescope 5 00:00:15.061 --> 00:00:18.130 have traced the locations of five brief, powerful 6 00:00:18.130 --> 00:00:23.050 radio blasts to the spiral arms of five distant galaxies. 7 00:00:23.050 --> 00:00:25.747 Because these radio pulses disappear in much 8 00:00:25.747 --> 00:00:28.060 less than the blink of an eye, researchers 9 00:00:28.060 --> 00:00:30.532 have had a hard time tracking down where they 10 00:00:30.532 --> 00:00:32.800 come from, and what causes them. 11 00:00:32.800 --> 00:00:35.095 Locating the galaxies where these blasts originate, 12 00:00:35.095 --> 00:00:37.719 is important in determining what astronomical 13 00:00:37.719 --> 00:00:41.644 events trigger such intense flashes of energy. 14 00:00:41.653 --> 00:00:44.090 The Hubble Space Telescope helped researchers 15 00:00:44.090 --> 00:00:47.530 narrow the list of possible FRB sources. 16 00:00:47.530 --> 00:00:51.355 Since their discovery in 2007, astronomers have uncovered 17 00:00:51.355 --> 00:00:53.890 up to 1,000 FRBs, but only 18 00:00:53.890 --> 00:00:58.143 about 15 are associated with particular galaxies. 19 00:00:58.151 --> 00:01:00.989 In this new Hubble study of FRBs, astronomers 20 00:01:00.989 --> 00:01:06.020 pinpointed where those bursts occurred within their specific galaxies. 21 00:01:06.020 --> 00:01:09.344 These images display a range of spiral-arm structures, 22 00:01:09.344 --> 00:01:11.790 from tightly wound to more open, 23 00:01:11.790 --> 00:01:16.050 revealing how stars are distributed along these prominent features. 24 00:01:16.050 --> 00:01:20.660 These clues helped researchers rule out some of the possible stellar objects originally 25 00:01:20.660 --> 00:01:23.620 thought to cause these brilliant flares, including 26 00:01:23.620 --> 00:01:25.710 the explosive deaths of the youngest, most 27 00:01:25.710 --> 00:01:31.490 massive stars, which create gamma-ray bursts and some types of supernovae. 28 00:01:31.490 --> 00:01:35.153 Another unlikely source is the merger of neutron stars, 29 00:01:35.153 --> 00:01:37.110 the crushed cores of stars that end 30 00:01:37.110 --> 00:01:42.950 their lives in supernova explosions. These mergers take billions of years to occur and 31 00:01:42.950 --> 00:01:48.440 are usually far from the spiral arms of older galaxies that no longer form stars. 32 00:01:48.440 --> 00:01:51.938 This study suggests that FRBs do not originate from the 33 00:01:51.976 --> 00:01:54.740 youngest, most massive stars or from 34 00:01:54.740 --> 00:01:57.722 older stars in a galaxy's central bulge. 35 00:01:57.722 --> 00:02:00.880 However, it is consistent with the leading model that 36 00:02:00.880 --> 00:02:05.507 FRBs originate from young magnetar outbursts. 37 00:02:05.507 --> 00:02:10.380 Magnetars are a type of neutron star with powerful magnetic fields. 38 00:02:10.380 --> 00:02:13.805 Called the strongest magnets in the universe, Magnetars possess 39 00:02:13.824 --> 00:02:15.940 a magnetic field 10 trillion 40 00:02:15.940 --> 00:02:20.510 times more powerful than the magnets on your refrigerator door! 41 00:02:20.510 --> 00:02:26.650 These magnetic fields lead to flares and magnetic processes that can emit radio light. 42 00:02:26.650 --> 00:02:29.503 Although the Hubble results are exciting, researchers 43 00:02:29.503 --> 00:02:31.060 need more observations to better 44 00:02:31.060 --> 00:02:33.967 pinpoint the source of FRBs so they can develop 45 00:02:33.967 --> 00:02:38.630 a stronger understanding of these enigmatic flashes. 46 00:02:38.630 --> 00:02:41.551 This field of study may need a lot more research, 47 00:02:41.551 --> 00:02:43.730 but thanks to observations made with the Hubble 48 00:02:43.730 --> 00:02:48.780 Space Telescope, we’re getting closer to understanding the mysteries of the universe. 49 00:02:48.780 --> 00:02:56.910 [ MUSIC ]