1 00:00:05,990 --> 00:00:03,669 now and then an obscure star briefly 2 00:00:07,030 --> 00:00:06,000 flares up brightening up to a million 3 00:00:09,990 --> 00:00:07,040 times 4 00:00:13,589 --> 00:00:10,000 it's an event called a nova 5 00:00:16,790 --> 00:00:13,599 the star v906 karani erupted as anova in 6 00:00:19,830 --> 00:00:16,800 2018. observations from three satellites 7 00:00:22,230 --> 00:00:19,840 provide new insights into what happened 8 00:00:24,070 --> 00:00:22,240 nasa's fermi mission has seen 14 novi 9 00:00:26,230 --> 00:00:24,080 since 2010. 10 00:00:28,150 --> 00:00:26,240 before then astronomers didn't think 11 00:00:30,470 --> 00:00:28,160 novae could glow in gamma rays the 12 00:00:32,389 --> 00:00:30,480 highest energy light 13 00:00:34,709 --> 00:00:32,399 when a white dwarf pulls material from a 14 00:00:36,870 --> 00:00:34,719 companion star the gas forms a 15 00:00:39,110 --> 00:00:36,880 thickening layer that eventually erupts 16 00:00:41,110 --> 00:00:39,120 in a thermonuclear fireball 17 00:00:42,790 --> 00:00:41,120 a nova is born 18 00:00:45,750 --> 00:00:42,800 led by a team from michigan state 19 00:00:48,709 --> 00:00:45,760 university astronomers studied v906 20 00:00:51,430 --> 00:00:48,719 karani using high energy data from fermi 21 00:00:53,510 --> 00:00:51,440 nasa's nustar x-ray telescope 22 00:00:55,990 --> 00:00:53,520 and invisible light from a canadian 23 00:00:57,590 --> 00:00:56,000 satellite named bright toronto 24 00:01:00,549 --> 00:00:57,600 shaped by the orbital motion of the 25 00:01:03,430 --> 00:01:00,559 stars the explosion debris first forms a 26 00:01:04,310 --> 00:01:03,440 thick expanding ring around the system 27 00:01:06,310 --> 00:01:04,320 then 28 00:01:09,030 --> 00:01:06,320 after 10 days or so 29 00:01:11,270 --> 00:01:09,040 fast outflows likely driven by residual 30 00:01:13,590 --> 00:01:11,280 fusion on the white dwarf strike the 31 00:01:15,910 --> 00:01:13,600 ring the resulting shock waves produce 32 00:01:19,350 --> 00:01:15,920 gamma-ray and optical flares that 33 00:01:21,670 --> 00:01:19,360 radiate away most of the novus energy 34 00:01:23,910 --> 00:01:21,680 these observations provide the first 35 00:01:25,270 --> 00:01:23,920 direct evidence that shockwaves can 36 00:01:28,230 --> 00:01:25,280 power most of 37 00:01:29,910 --> 00:01:28,240 explosion's visible light 38 00:01:32,149 --> 00:01:29,920 figuring out how they work in nearby 39 00:01:34,469 --> 00:01:32,159 novi will help us understand more