1 00:00:00,010 --> 00:00:04,010 Music 2 00:00:04,030 --> 00:00:08,030 Hi, I'm Elizabeth Hayes, a scientist working on NASA's 3 00:00:08,050 --> 00:00:12,050 Fermi Gamma-ray Space Telescope. Every 3 hours, the 4 00:00:12,070 --> 00:00:16,070 Large Area Telescope onboard Fermi builds up a picture of the sky in gamma-rays, 5 00:00:16,090 --> 00:00:20,100 the most energetic form of light. One thing it sees a lot of is 6 00:00:20,120 --> 00:00:24,130 blazars, active galaxies whose emissions are powered by supermassive black 7 00:00:24,150 --> 00:00:28,140 holes. Blazars are extremely active objects. 8 00:00:28,160 --> 00:00:32,150 Here's one of the most extreme Fermi has seen. It's been known to flare up so brightly 9 00:00:32,170 --> 00:00:36,190 that, for a few days, it outshines every other gamma-ray source. 10 00:00:36,210 --> 00:00:40,210 Considering that it's more than 7 billion light-years away, this is an immense 11 00:00:40,230 --> 00:00:44,230 energy output. At the core of an active galaxy is a supermassive 12 00:00:44,250 --> 00:00:48,250 black hole that powers jets of particles moving near the speed of light. 13 00:00:48,270 --> 00:00:52,280 We call it a blazar when one of the jets is pointed in our direction. 14 00:00:52,300 --> 00:00:56,280 This offers us the best view for seeing dramatic flares when there are changes along 15 00:00:56,300 --> 00:01:00,300 the jet. Fermi has found about a thousand gamma-ray blazars so far. 16 00:01:00,320 --> 00:01:04,320 Every day, the gamma-ray sky changes depending on which galaxies are 17 00:01:04,340 --> 00:01:08,370 in outburst and which are in a quiet phase. Because we're watching them all the time, 18 00:01:08,390 --> 00:01:12,390 we can track their activity and alert other telescopes to new flare-ups. 19 00:01:12,410 --> 00:01:16,430 As Fermi continues to watch the sky, it builds a more complete picture of the 20 00:01:16,450 --> 00:01:20,460 daily lives of these powerful objects. Some of the flares we 21 00:01:20,480 --> 00:01:24,490 see announce the presence of blazars we've never seen before. And sometimes 22 00:01:24,510 --> 00:01:28,520 we find a gamma-ray flare that is not from a blazar, which is very exciting. 23 00:01:28,540 --> 00:01:32,550 We hope to discover new types of gamma-ray-emitting objects that we don't yet know 24 00:01:32,570 --> 00:01:36,590 about. Right now, nearly one third of Fermi sources cannot be connected 25 00:01:36,600 --> 00:01:40,620 to any known type of gamma-ray source. Out there in the dark, 26 00:01:40,640 --> 00:01:44,650 what new discoveries await us?