1 00:00:06,309 --> 00:00:04,470 in april 2020 astronomers detected an 2 00:00:08,629 --> 00:00:06,319 unusually bright and powerful radio 3 00:00:09,990 --> 00:00:08,639 signal never before recorded in our home 4 00:00:12,470 --> 00:00:10,000 galaxy 5 00:00:14,390 --> 00:00:12,480 the source is a magnetar a type of 6 00:00:16,870 --> 00:00:14,400 compact object with the strongest 7 00:00:19,670 --> 00:00:16,880 magnetic fields in the cosmos 8 00:00:21,670 --> 00:00:19,680 like pulsars and neutron stars magnetars 9 00:00:24,150 --> 00:00:21,680 are the crushed cores left behind when a 10 00:00:25,910 --> 00:00:24,160 massive star explodes but their super 11 00:00:27,670 --> 00:00:25,920 strong magnetic fields put them in a 12 00:00:29,349 --> 00:00:27,680 class by themselves 13 00:00:31,750 --> 00:00:29,359 the fields are up to a thousand times 14 00:00:33,750 --> 00:00:31,760 stronger than typical neutron stars and 15 00:00:35,750 --> 00:00:33,760 over 10 trillion times stronger than a 16 00:00:37,590 --> 00:00:35,760 refrigerator magnet 17 00:00:39,350 --> 00:00:37,600 they can rip molecules apart from 18 00:00:41,750 --> 00:00:39,360 thousands of miles away 19 00:00:45,190 --> 00:00:41,760 distort the shapes of atoms and store 20 00:00:49,270 --> 00:00:45,200 enormous amounts of energy on april 27th 21 00:00:51,830 --> 00:00:49,280 the magnetar named sgr 1935 produced a 22 00:00:54,470 --> 00:00:51,840 rapid-fire storm of short powerful x-ray 23 00:00:57,110 --> 00:00:54,480 bursts that lasted hours 24 00:00:59,270 --> 00:00:57,120 the activity first spotted by swift was 25 00:01:01,590 --> 00:00:59,280 also monitored by nasa's fermi gamma-ray 26 00:01:03,349 --> 00:01:01,600 space telescope and the nicer x-ray 27 00:01:04,390 --> 00:01:03,359 telescope on the international space 28 00:01:07,350 --> 00:01:04,400 station 29 00:01:09,510 --> 00:01:07,360 along with other space missions 30 00:01:10,550 --> 00:01:09,520 as the storm wound down early on april 31 00:01:13,429 --> 00:01:10,560 28th 32 00:01:15,670 --> 00:01:13,439 nicer recorded some 200 x-ray bursts in 33 00:01:18,870 --> 00:01:15,680 just 20 minutes 34 00:01:20,469 --> 00:01:18,880 later that day sgr 1935 fired off 35 00:01:22,390 --> 00:01:20,479 another x-ray burst 36 00:01:23,670 --> 00:01:22,400 this time though it was accompanied by 37 00:01:26,310 --> 00:01:23,680 something new 38 00:01:29,350 --> 00:01:26,320 a powerful pulse of radio waves lasting 39 00:01:31,429 --> 00:01:29,360 a thousandth of a second 40 00:01:33,190 --> 00:01:31,439 chime a radio telescope in british 41 00:01:35,510 --> 00:01:33,200 columbia led by several canadian 42 00:01:37,270 --> 00:01:35,520 universities discovered the signal and 43 00:01:39,830 --> 00:01:37,280 determined it came from the vicinity of 44 00:01:42,469 --> 00:01:39,840 sgr 1935 45 00:01:44,469 --> 00:01:42,479 another experiment called stair 2 and 46 00:01:46,710 --> 00:01:44,479 operated by caltech and nasa's jet 47 00:01:48,389 --> 00:01:46,720 propulsion laboratory saw an even 48 00:01:50,630 --> 00:01:48,399 brighter signal at different radio 49 00:01:53,109 --> 00:01:50,640 wavelengths 50 00:01:55,190 --> 00:01:53,119 since 2007 astronomers have been trying 51 00:01:57,749 --> 00:01:55,200 to understand the sources of powerful 52 00:02:00,789 --> 00:01:57,759 millisecond radio signals called fast 53 00:02:03,990 --> 00:02:00,799 radio bursts seen from other galaxies 54 00:02:06,550 --> 00:02:04,000 magnetars have been prominent suspects 55 00:02:09,510 --> 00:02:06,560 the duration and energy release of sgr 56 00:02:12,470 --> 00:02:09,520 1935's radio signal is closer to fast 57 00:02:14,470 --> 00:02:12,480 radio bursts than any other source 58 00:02:16,869 --> 00:02:14,480 for the first time astronomers saw 59 00:02:18,710 --> 00:02:16,879 magnetar in our own backyard produce a 60 00:02:20,229 --> 00:02:18,720 signal only previously seen in other 61 00:02:22,229 --> 00:02:20,239 galaxies 62 00:02:24,309 --> 00:02:22,239 the discovery strengthens the case that 63 00:02:26,020 --> 00:02:24,319 magnetars are responsible for at least 64 00:02:27,270 --> 00:02:26,030 some fast radio bursts 65 00:02:29,350 --> 00:02:27,280 [Music] 66 00:02:31,110 --> 00:02:29,360 data from nyser and fermi on x-ray 67 00:02:32,470 --> 00:02:31,120 bursts at the end of the storm 68 00:02:35,190 --> 00:02:32,480 showed that they differed from the one 69 00:02:37,030 --> 00:02:35,200 that coincided with the radio signal 70 00:02:39,030 --> 00:02:37,040 this event's characteristics set it 71 00:02:41,190 --> 00:02:39,040 apart from the other eruptions 72 00:02:42,790 --> 00:02:41,200 and further study may provide clues 73 00:02:44,070 --> 00:02:42,800 about how it also powered the radio 74 00:02:45,910 --> 00:02:44,080 burst 75 00:02:48,229 --> 00:02:45,920 radio waves from normal pulsars 76 00:02:51,190 --> 00:02:48,239 originate high above their surfaces 77 00:02:53,509 --> 00:02:51,200 exactly where and how we don't know 78 00:02:55,750 --> 00:02:53,519 a big eruption could launch a cloud of 79 00:02:57,750 --> 00:02:55,760 plasma to high enough that a radio burst 80 00:02:59,670 --> 00:02:57,760 could form 81 00:03:02,550 --> 00:02:59,680 never before have astronomers seen a 82 00:03:04,390 --> 00:03:02,560 fast radio burst so close to home 83 00:03:05,589 --> 00:03:04,400 it's just one more reason to watch the 84 00:03:07,830 --> 00:03:05,599 skies 85 00:03:14,550 --> 00:03:07,840 and to keep tabs on the strongest