1 00:00:00,980 --> 00:00:04,080 For the first time ever, scientists using NASA's 2 00:00:04,080 --> 00:00:08,860 Fermi Gamma-ray Space Telescope have found the source of a high-energy neutrino 3 00:00:08,860 --> 00:00:12,380 from outside our galaxy. The neutrino came from the 4 00:00:12,380 --> 00:00:16,160 eruption of a supermassive black hole at the center of a type of galaxy called 5 00:00:16,160 --> 00:00:20,620 a blazar. The eruption jetted out particles moving near the speed of light. 6 00:00:22,580 --> 00:00:24,500 Collisions inside the jet produced 7 00:00:24,500 --> 00:00:28,400 gamma rays, the highest-energy form of light, and neutrinos, 8 00:00:28,400 --> 00:00:30,900 ghostly particles that rarely interact with matter. 9 00:00:32,200 --> 00:00:36,340 3.7 billion years later, they reached Earth. 10 00:00:37,360 --> 00:00:41,120 On September 22, 2017, a single 11 00:00:41,120 --> 00:00:45,300 high-energy neutrino struck an atom in a water molecule in the Antarctic ice. 12 00:00:45,300 --> 00:00:48,260 The crash produced a particle called a muon. 13 00:00:49,080 --> 00:00:52,800 It raced through the ice so fast it emitted a faint blue glow. 14 00:00:54,220 --> 00:00:57,620 When the muon reached the South Pole, it was tracked by the 15 00:00:57,630 --> 00:01:01,680 IceCube Neutrino Observatory. IceCube scientists found 16 00:01:01,680 --> 00:01:04,520 the original neutrino likely came from beyond our solar system. 17 00:01:05,320 --> 00:01:09,900 They alerted astronomers to be on the lookout for cosmic outbursts possibly 18 00:01:09,910 --> 00:01:14,100 associated with it. NASA's Fermi Gamma-ray Space 19 00:01:14,100 --> 00:01:17,760 Telescope found the source, a blazar it had been watching for some time. 20 00:01:19,540 --> 00:01:22,240 When the neutrino arrived, Fermi saw the blazar 21 00:01:22,240 --> 00:01:24,700 was brighter than it had been over the previous decade. 22 00:01:25,740 --> 00:01:29,940 It's the first time a neutrino could be traced back to a black hole, or to any 23 00:01:29,940 --> 00:01:34,000 source beyond our immediate galactic neighborhood. And it's an important 24 00:01:34,180 --> 00:01:38,260 step forward for a growing field scientists call multimessenger astronomy, 25 00:01:38,860 --> 00:01:42,560 which combines light with new signals like gravitational waves 26 00:01:42,560 --> 00:01:46,360 and neutrinos, to provide new insights on the most 27 00:01:46,360 --> 00:01:50,400 extreme cosmic phenomena. 28 00:01:50,800 --> 00:01:54,880 [Music fades] NASA Astrophysics