WEBVTT FILE 1 00:00:00.020 --> 00:00:04.020 [Music] 2 00:00:04.040 --> 00:00:08.070 [Music] 3 00:00:08.090 --> 00:00:12.120 [Music] 4 00:00:12.140 --> 00:00:16.180 [Music] 5 00:00:16.200 --> 00:00:20.220 Narrator: Parkes 1441+25 is a distant 6 00:00:20.240 --> 00:00:24.270 galaxy powered by a supermassive black hole. It's so far away 7 00:00:24.290 --> 00:00:28.290 its light takes more than half the current age of the universe to reach us. 8 00:00:28.310 --> 00:00:32.370 This is NASA's Fermi Gamma-ray Space Telescope, 9 00:00:32.390 --> 00:00:36.450 our sharpest satellite eyes on the gamma-ray sky. But Fermi's 10 00:00:36.470 --> 00:00:40.510 effective collecting area is about the size of two office desks. It can't 11 00:00:40.530 --> 00:00:44.540 catch everything. Ground-based gamma-ray observatories sport 12 00:00:44.560 --> 00:00:48.570 much larger light collectors than Fermi, but like traditional telescopes, they 13 00:00:48.590 --> 00:00:52.590 only work at night. Both MAGIC and VERITAS work 14 00:00:52.610 --> 00:00:56.650 by catching faint flashes of visible light produced when a high-energy 15 00:00:56.670 --> 00:01:00.700 gamma ray strikes the upper atmosphere. This creates a shower 16 00:01:00.720 --> 00:01:04.740 of fast-moving charged particles that emit a glow called Cerenkov radiation. 17 00:01:04.760 --> 00:01:08.760 On April 16, 2015, 18 00:01:08.780 --> 00:01:12.810 Parkes 1441 was exhibiting high activity across all wavelengths. 19 00:01:12.830 --> 00:01:16.830 Scientists looking at Fermi data reported a strong gamma-ray 20 00:01:16.850 --> 00:01:20.840 outburst. Based on this alert, scientists on the MAGIC team began 21 00:01:20.860 --> 00:01:24.890 monitoring the galaxy and detected very-high-energy gamma rays. 22 00:01:24.910 --> 00:01:28.960 That was the cue for VERITAS to take a look, and it also captured the 23 00:01:28.980 --> 00:01:32.990 quasar's very-high-energy emission. These detections were 24 00:01:33.010 --> 00:01:37.020 remarkable because high-energy light usually can't travel extreme distances 25 00:01:37.040 --> 00:01:41.070 These gamma rays had been traveling for half the age of the cosmos 26 00:01:41.090 --> 00:01:45.120 passing through all the light emitted by stars, supernovae, and everything else 27 00:01:45.140 --> 00:01:49.140 that flashed and glowed across more than 7 billion years of cosmic history. 28 00:01:49.160 --> 00:01:53.170 Astronomers call this remnant glow is called the extragalactic background light 29 00:01:53.190 --> 00:01:57.210 background light. When a gamma ray strikes this lower-energy light, it converts into 30 00:01:57.230 --> 00:02:01.230 a pair of particles, an electron and a positron. The farther 31 00:02:01.250 --> 00:02:05.270 gamma rays travel the more likely it is they'll undergo this process, which effectively 32 00:02:05.290 --> 00:02:09.300 erases the gamma rays from the universe before we have the opportunity to detect 33 00:02:09.320 --> 00:02:13.370 them. Parkes 1441 is one of the most 34 00:02:13.390 --> 00:02:17.450 distant sources of gamma rays with energies above 100 GeV, 35 00:02:17.470 --> 00:02:21.490 tens of billions of times the energy in visible light. That the light 36 00:02:21.510 --> 00:02:25.530 reached us at all provides information about the extragalactic background light 37 00:02:25.550 --> 00:02:29.580 when the universe was half its present age. Those gamma rays 38 00:02:29.600 --> 00:02:33.730 originated from the particle jet produced by the galaxy's supermassive black hole. 39 00:02:33.750 --> 00:02:37.890 Astronomers think they started their journey only about 5 light-years from the 40 00:02:37.910 --> 00:02:41.960 black hole. Escaping the galaxy's crowded central regions 41 00:02:41.980 --> 00:02:46.050 means this high-energy light never interacted with matter or starlight, collisions 42 00:02:46.070 --> 00:02:50.120 that would have doomed them to convert into particles. This is one reason 43 00:02:50.140 --> 00:02:54.180 why extremely energetic gamma rays are few and far between, and why astronomers 44 00:02:54.200 --> 00:02:58.250 prize the relatively few photons they can find. 45 00:02:58.270 --> 00:03:02.270 The story of gamma rays from Parkes 1441 isn't a mere tale of survival. 46 00:03:02.290 --> 00:03:06.340 These photons executed a jailbreak of cosmic proportions, 47 00:03:06.360 --> 00:03:10.370 and it took Fermi, MAGIC, and VERTIAS to round them up. 48 00:03:10.390 --> 00:03:14.380 [Beeping] 49 00:03:14.400 --> 00:03:18.400 [Beeping] 50 00:03:18.420 --> 00:03:24.918 [Beeping]