1 00:00:00,960 --> 00:00:07,550 \h The Chandra X-ray Observatory orbits high above the Earth, peering into the blackest reaches of space. 2 00:00:07,550 --> 00:00:13,700 \h Exploring the most menacing and magnificent features of the cosmos, this remarkable telescope is revealing what 3 00:00:13,700 --> 00:00:31,290 \h our eyes can't, taking us beyond visible light. 4 00:00:31,290 --> 00:00:38,350 \h The bad boys of astronomy, black holes inspire well-deserved wariness and strange fascination. 5 00:00:38,350 --> 00:00:41,710 \h But what exactly are they? 6 00:00:41,710 --> 00:00:47,140 \h Scientists harnessing the incredible power of Chandra have discovered that black holes play a 7 00:00:47,140 --> 00:00:53,700 \h critical role in both the development and demise of stars and galaxies. 8 00:00:53,700 --> 00:00:59,290 \h While astronomers have long known that black holes existed, it wasn't until Chandra was launched in 9 00:00:59,290 --> 00:01:04,760 \h 1999 that some of their elusive secrets were revealed. 10 00:01:04,760 --> 00:01:12,250 \h With its insightful perspective, Chandra has shed a revealing light on the dark mysteries of black holes. 11 00:01:12,250 --> 00:01:19,750 \h Focusing on the deepest depths of space, Chandra has witnessed the gluttonous eating habits of some black holes. 12 00:01:19,750 --> 00:01:24,200 \h HARVEY TANANBAUM: And in those regions where the X-rays are deficient, 13 00:01:24,200 --> 00:01:28,750 \h where the gas voids exist, is the same regions where you see the radio lobes, 14 00:01:28,750 --> 00:01:31,300 \h these jets and lobes that are formed from the radios. 15 00:01:31,300 --> 00:01:36,480 \h So you know that energetic particles are being shot away from the black hole by some kind of mysterious process, 16 00:01:36,480 --> 00:01:38,430 \h and they're clearing the gas away. 17 00:01:38,430 --> 00:01:40,350 \h They're pushing the gas aside. 18 00:01:40,350 --> 00:01:44,900 \h Because the gas has a density and a temperature, properties that we measure in the X-rays, 19 00:01:44,900 --> 00:01:49,630 \h it's very easy to calculate the amount of work that's needed to clear these voids. 20 00:01:49,630 --> 00:01:54,980 \h So you can actually measure the energy that's carried out by these jets of particles. 21 00:01:54,980 --> 00:02:01,240 \h However, not all black holes mean certain doom for their neighbors. 22 00:02:01,240 --> 00:02:10,430 \h Consider for example, one known as Sagittarius A Star, a black hole churning at the center of our own Milky Way galaxy. 23 00:02:10,430 --> 00:02:17,710 \h Unlike its more malicious siblings, this black hole appears to be protecting a flock of young stars instead of eating them. 24 00:02:17,710 --> 00:02:22,010 \h TANANBAUM: With Chandra, we're able to measure the density and temperature of the gas just outside 25 00:02:22,010 --> 00:02:24,980 \h the black hole at the center of the Milky Way galaxy, 26 00:02:24,980 --> 00:02:28,940 \h and there's plenty of gas there and it's hot! 27 00:02:28,940 --> 00:02:38,210 \h And we should see, even with conservative theories, instead of 100 billion times the amount of radiation that we see, 28 00:02:38,210 --> 00:02:46,890 \h we should see a billion times or some 100 million times; it doesn't matter, it's a large factor greater than what we see. 29 00:02:46,890 --> 00:02:55,320 \h Equal parts stellar destroyers and cosmic creators, Chandra's black holes exhibit dual nature.