1 00:00:05,349 --> 00:00:03,669 on august 21st 2019 nasa's nicer 2 00:00:07,349 --> 00:00:05,359 telescope on the international space 3 00:00:08,950 --> 00:00:07,359 station observed its brightest x-ray 4 00:00:12,070 --> 00:00:08,960 burst to date 5 00:00:14,390 --> 00:00:12,080 the flare-up came from saks j1808 a 6 00:00:15,589 --> 00:00:14,400 binary system about 11 000 light years 7 00:00:18,230 --> 00:00:15,599 away 8 00:00:20,950 --> 00:00:18,240 here a pulsar a rapidly spinning neutron 9 00:00:22,630 --> 00:00:20,960 star draws gas from its companion an 10 00:00:24,550 --> 00:00:22,640 object called a brown dwarf that is 11 00:00:26,070 --> 00:00:24,560 larger than a planet but less massive 12 00:00:28,230 --> 00:00:26,080 than a star 13 00:00:30,790 --> 00:00:28,240 hydrogen gas from the brown dwarf forms 14 00:00:32,549 --> 00:00:30,800 an accretion disk around the pulsar 15 00:00:33,830 --> 00:00:32,559 every few years the disk becomes 16 00:00:35,510 --> 00:00:33,840 unstable 17 00:00:38,229 --> 00:00:35,520 this sends a rush of gas toward the 18 00:00:40,310 --> 00:00:38,239 pulsar that makes it brighten and x-rays 19 00:00:42,470 --> 00:00:40,320 the pulsar super-strong magnetic field 20 00:00:44,549 --> 00:00:42,480 sweeps up the gas and channels it to the 21 00:00:46,549 --> 00:00:44,559 object's surface 22 00:00:48,869 --> 00:00:46,559 hydrogen nuclei falling to the pulsar 23 00:00:51,029 --> 00:00:48,879 surface fuse together producing energy 24 00:00:52,150 --> 00:00:51,039 and forming helium nuclei which settle 25 00:00:54,150 --> 00:00:52,160 out below 26 00:00:55,670 --> 00:00:54,160 this process is similar to what happens 27 00:00:57,830 --> 00:00:55,680 inside our sun 28 00:00:59,830 --> 00:00:57,840 then when the conditions are just right 29 00:01:02,709 --> 00:00:59,840 the entire helium layer ignites in a 30 00:01:05,030 --> 00:01:02,719 brief but intense thermonuclear fireball 31 00:01:07,270 --> 00:01:05,040 astronomers call this a type 1 x-ray 32 00:01:08,789 --> 00:01:07,280 burst here's how it happened 33 00:01:10,870 --> 00:01:08,799 the explosion first blows off the 34 00:01:12,630 --> 00:01:10,880 hydrogen layer which expands and 35 00:01:14,710 --> 00:01:12,640 ultimately dissipates 36 00:01:16,230 --> 00:01:14,720 then the rising radiation builds to the 37 00:01:18,950 --> 00:01:16,240 point where it blows off the helium 38 00:01:20,950 --> 00:01:18,960 layer which overtakes the hydrogen shell 39 00:01:23,910 --> 00:01:20,960 some of the x-rays emitted in the blast 40 00:01:25,990 --> 00:01:23,920 scatter off of the accretion disk 41 00:01:29,510 --> 00:01:26,000 the fireball then quickly cools and the 42 00:01:31,910 --> 00:01:29,520 helium settles back onto the surface 43 00:01:33,910 --> 00:01:31,920 it was all over in 20 seconds but nicer 44 00:01:35,510 --> 00:01:33,920 data clearly show important details that 45 00:01:36,870 --> 00:01:35,520 haven't been seen together in other 46 00:01:38,230 --> 00:01:36,880 bursts 47 00:01:40,069 --> 00:01:38,240 this will help scientists better