1 00:00:12,060 --> 00:00:10,040 Music 2 00:00:12,080 --> 00:00:16,100 Narrator: Most big galaxies contain big black holes. Not just big, 3 00:00:16,120 --> 00:00:20,160 supersized, with millions of times the sun's mass 4 00:00:20,180 --> 00:00:24,190 Some of these black holes are actively devouring gas. This drives 5 00:00:24,210 --> 00:00:28,280 particle jets that can spew matter millions of light-years into space, and it 6 00:00:28,300 --> 00:00:32,430 also makes the holes a source of penetrating, or hard, X-rays. 7 00:00:32,450 --> 00:00:36,460 At these energies, the sky glows in every direction, even far away 8 00:00:36,480 --> 00:00:40,500 from bright sources. Astronomers have long suspected that active 9 00:00:40,520 --> 00:00:44,550 supermassive black holes in galaxies were responsible, but they just couldn't find 10 00:00:44,570 --> 00:00:48,560 enough of them to account for the X-ray glow--especially the peak of the energy spectrum. 11 00:00:48,580 --> 00:00:52,610 Now, astronomers using NASA's 12 00:00:52,630 --> 00:00:56,680 Swift satellite confirm that a largely unseen population of black-hole-powered 13 00:00:56,700 --> 00:01:00,710 galaxies is out there. There are so many that scientists say they might fully 14 00:01:00,730 --> 00:01:04,750 account for the cosmic X-ray background. What emission we 15 00:01:04,770 --> 00:01:08,830 detect from an active black hole is a function of how we see it--whether we're looking 16 00:01:08,850 --> 00:01:12,860 face-on and into one of it's jets, or viewing it from the side, through the disk of gas 17 00:01:12,880 --> 00:01:16,900 and dust that surrounds it. The brightest active black 18 00:01:16,920 --> 00:01:20,980 holes, which include quasars and blazars, are those we see face-on. 19 00:01:21,000 --> 00:01:25,010 But as the viewing angle increases, the surrounding disk absorbs increasing 20 00:01:25,030 --> 00:01:29,070 amounts of radiation. Astronomers have always assumed that many 21 00:01:29,090 --> 00:01:33,090 active galaxies were oriented edgewise to us, but because the disk of gas 22 00:01:33,110 --> 00:01:37,110 smothers most of their X-rays, these sideways black holes just weren't detected. 23 00:01:37,130 --> 00:01:41,160 And that's where Swift comes in. Since 24 00:01:41,180 --> 00:01:45,180 2004, the satellites Burst Alert Telescope has been building up the largest, most 25 00:01:45,200 --> 00:01:49,210 sensitive X-ray map of the sky. Using these data, 26 00:01:49,230 --> 00:01:53,260 astronomers found that the most heavily absorbed galaxies create the energy peak in the 27 00:01:53,280 --> 00:01:57,260 cosmic X-ray background. What does it all mean? 28 00:01:57,280 --> 00:02:01,300 When the universe was about half its present age, about 7 billion years ago, galaxies 29 00:02:01,320 --> 00:02:05,370 crashed together more frequently and these collisions produced gas rich galaxies 30 00:02:05,390 --> 00:02:09,370 with heavily obscured black holes. The Swift survey shows that 31 00:02:09,390 --> 00:02:13,410 galaxy mergers helped activate these black holes by feeding them torrents of fresh gas. 32 00:02:13,430 --> 00:02:17,490 The new findings are consistent with idea that the X-ray background 33 00:02:17,510 --> 00:02:21,500 peaked around this time, when our own galaxy was young and before our