1 00:00:05,670 --> 00:00:03,429 fast radio bursts or frbs are 2 00:00:08,150 --> 00:00:05,680 extraordinary events that generate as 3 00:00:11,830 --> 00:00:08,160 much energy in a thousandth of a second 4 00:00:14,070 --> 00:00:11,840 as the sun does in an entire year 5 00:00:16,390 --> 00:00:14,080 astronomers using nasa's hubble space 6 00:00:19,109 --> 00:00:16,400 telescope have traced the locations of 7 00:00:22,790 --> 00:00:19,119 five brief powerful radio blasts to the 8 00:00:25,189 --> 00:00:22,800 spiral arms of five distant galaxies 9 00:00:27,349 --> 00:00:25,199 because these radio pulses disappear in 10 00:00:29,109 --> 00:00:27,359 much less than the blink of an eye 11 00:00:30,870 --> 00:00:29,119 researchers have had a hard time 12 00:00:32,310 --> 00:00:30,880 tracking down where they come from and 13 00:00:34,389 --> 00:00:32,320 what causes them 14 00:00:36,549 --> 00:00:34,399 locating the galaxies where these blasts 15 00:00:38,869 --> 00:00:36,559 originate is important in determining 16 00:00:41,430 --> 00:00:38,879 what astronomical events trigger such 17 00:00:43,350 --> 00:00:41,440 intense flashes of energy 18 00:00:45,590 --> 00:00:43,360 the hubble space telescope helped 19 00:00:47,670 --> 00:00:45,600 researchers narrow the list of possible 20 00:00:49,670 --> 00:00:47,680 frb sources 21 00:00:53,189 --> 00:00:49,680 since their discovery astronomers have 22 00:00:55,430 --> 00:00:53,199 uncovered up to 1000 frbs but only about 23 00:00:57,270 --> 00:00:55,440 15 are associated with particular 24 00:00:59,590 --> 00:00:57,280 galaxies 25 00:01:01,510 --> 00:00:59,600 in this new hubble study of frbs 26 00:01:03,349 --> 00:01:01,520 astronomers pinpointed where those 27 00:01:05,670 --> 00:01:03,359 bursts occurred within their specific 28 00:01:08,149 --> 00:01:05,680 galaxies 29 00:01:10,630 --> 00:01:08,159 these images display a range of spiral 30 00:01:13,109 --> 00:01:10,640 arm structures from tightly wound to 31 00:01:14,789 --> 00:01:13,119 more open revealing how stars are 32 00:01:16,550 --> 00:01:14,799 distributed along these prominent 33 00:01:18,710 --> 00:01:16,560 features 34 00:01:20,710 --> 00:01:18,720 these clues helped researchers rule out 35 00:01:22,390 --> 00:01:20,720 some of the possible stellar objects 36 00:01:25,030 --> 00:01:22,400 originally thought to cause these 37 00:01:26,950 --> 00:01:25,040 brilliant flares including the explosive 38 00:01:29,590 --> 00:01:26,960 deaths of the youngest most massive 39 00:01:32,069 --> 00:01:29,600 stars which create gamma-ray bursts and 40 00:01:34,550 --> 00:01:32,079 some type of supernova 41 00:01:37,429 --> 00:01:34,560 another unlikely source is the merger of 42 00:01:39,270 --> 00:01:37,439 neutron stars the crushed cores of stars 43 00:01:40,710 --> 00:01:39,280 that end their lives in supernova 44 00:01:42,870 --> 00:01:40,720 explosions 45 00:01:44,950 --> 00:01:42,880 these mergers take billions of years to 46 00:01:47,670 --> 00:01:44,960 occur and are usually far from the 47 00:01:49,429 --> 00:01:47,680 spiral arms of older galaxies that no 48 00:01:51,830 --> 00:01:49,439 longer form stars 49 00:01:54,069 --> 00:01:51,840 this study suggests that frbs do not 50 00:01:57,109 --> 00:01:54,079 originate from the youngest most massive 51 00:02:00,149 --> 00:01:57,119 stars or from older stars in a galaxy's 52 00:02:02,389 --> 00:02:00,159 central bulge however it is consistent 53 00:02:06,230 --> 00:02:02,399 with the leading model that frbs 54 00:02:08,469 --> 00:02:06,240 originate from young magnetar outbursts 55 00:02:11,510 --> 00:02:08,479 magnetars are a type of neutron star 56 00:02:13,510 --> 00:02:11,520 with powerful magnetic fields called the 57 00:02:16,150 --> 00:02:13,520 strongest magnets in the universe 58 00:02:18,550 --> 00:02:16,160 magnetars possess a magnetic field 10 59 00:02:20,949 --> 00:02:18,560 trillion times more powerful than the 60 00:02:23,510 --> 00:02:20,959 magnets on your refrigerator door 61 00:02:25,750 --> 00:02:23,520 these magnetic fields lead to flares and 62 00:02:27,350 --> 00:02:25,760 magnetic processes that can emit radio 63 00:02:29,510 --> 00:02:27,360 light 64 00:02:31,509 --> 00:02:29,520 although the hubble results are exciting 65 00:02:33,990 --> 00:02:31,519 researchers need more observations to 66 00:02:35,350 --> 00:02:34,000 better pinpoint the source of frbs so 67 00:02:39,190 --> 00:02:35,360 they can develop a stronger 68 00:02:41,350 --> 00:02:39,200 understanding of these enigmatic flashes 69 00:02:43,910 --> 00:02:41,360 this field of study may need a lot more 70 00:02:45,830 --> 00:02:43,920 research but thanks to observations made 71 00:02:47,830 --> 00:02:45,840 with the hubble space telescope we're