1 00:00:09,030 --> 00:00:05,670 black holes are the strongest test of 2 00:00:10,870 --> 00:00:09,040 what the theory of gravity really is 3 00:00:13,270 --> 00:00:10,880 space is just bent and warped and 4 00:00:14,950 --> 00:00:13,280 twisted in some incredibly complex way 5 00:00:17,029 --> 00:00:14,960 and if one could only understand that 6 00:00:18,950 --> 00:00:17,039 one would have a fundamental insight 7 00:00:20,710 --> 00:00:18,960 into the theory of gravity 8 00:00:23,429 --> 00:00:20,720 in the past five years our knowledge of 9 00:00:25,590 --> 00:00:23,439 black holes has really exploded 10 00:00:27,269 --> 00:00:25,600 by using space-based and ground-based 11 00:00:29,669 --> 00:00:27,279 telescopes covering the full 12 00:00:31,269 --> 00:00:29,679 electromagnetic spectrum astronomers 13 00:00:32,790 --> 00:00:31,279 have found that black holes are 14 00:00:34,950 --> 00:00:32,800 everywhere 15 00:00:36,549 --> 00:00:34,960 they come in a variety of sizes and they 16 00:00:38,069 --> 00:00:36,559 are integral to the formation of 17 00:00:40,069 --> 00:00:38,079 galaxies 18 00:00:42,470 --> 00:00:40,079 one way to find a black hole is to look 19 00:00:44,630 --> 00:00:42,480 for x-rays that are produced by matter 20 00:00:46,229 --> 00:00:44,640 caught up in its violent and extreme 21 00:00:48,310 --> 00:00:46,239 environment 22 00:00:50,549 --> 00:00:48,320 in fact we are extremely close to 23 00:00:54,470 --> 00:00:50,559 looking at the very edge of a black hole 24 00:00:56,950 --> 00:00:54,480 something einstein never imagined 25 00:00:59,110 --> 00:00:56,960 what happens to matter and energy as it 26 00:01:01,270 --> 00:00:59,120 moves closer to a black hole 27 00:01:02,709 --> 00:01:01,280 and crosses the event horizon 28 00:01:04,310 --> 00:01:02,719 the theoretical border from which 29 00:01:06,870 --> 00:01:04,320 nothing can escape 30 00:01:08,630 --> 00:01:06,880 does time really come to a standstill 31 00:01:10,830 --> 00:01:08,640 will we see a breakdown in general 32 00:01:13,750 --> 00:01:10,840 relativity in the environment of extreme 33 00:01:15,750 --> 00:01:13,760 gravity general relativity makes 34 00:01:18,310 --> 00:01:15,760 specific predictions about matter and 35 00:01:20,950 --> 00:01:18,320 energy close to a black hole 36 00:01:23,030 --> 00:01:20,960 if upon close scrutiny we see the 37 00:01:24,390 --> 00:01:23,040 slightest deviation between theory and 38 00:01:26,469 --> 00:01:24,400 observation 39 00:01:29,749 --> 00:01:26,479 we will understand limitations in 40 00:01:32,069 --> 00:01:29,759 einstein's equations 41 00:01:34,469 --> 00:01:32,079 two space missions will take us closer 42 00:01:36,390 --> 00:01:34,479 to a black hole event horizon than we've 43 00:01:38,950 --> 00:01:36,400 ever been 44 00:01:40,710 --> 00:01:38,960 lisa a joint nasa european mission now 45 00:01:43,190 --> 00:01:40,720 and formulation will listen for 46 00:01:44,870 --> 00:01:43,200 gravitational waves created by merging 47 00:01:47,429 --> 00:01:44,880 black holes 48 00:01:49,270 --> 00:01:47,439 now we're talking about opening a window 49 00:01:51,590 --> 00:01:49,280 that's not even 50 00:01:54,230 --> 00:01:51,600 based on electromagnetism it's a window 51 00:01:56,710 --> 00:01:54,240 that's based on gravitational radiation 52 00:01:58,870 --> 00:01:56,720 the gravity wave spectrum 53 00:02:00,630 --> 00:01:58,880 is kind of a new and really unexplored 54 00:02:04,630 --> 00:02:00,640 frontier 55 00:02:06,469 --> 00:02:04,640 no one's directly detected gravity waves 56 00:02:09,029 --> 00:02:06,479 as we start to open up this next 57 00:02:11,110 --> 00:02:09,039 frontier which i think many of us think 58 00:02:13,030 --> 00:02:11,120 of as the great frontier for 21st 59 00:02:14,550 --> 00:02:13,040 century astronomy 60 00:02:15,990 --> 00:02:14,560 i think we're going to learn about 61 00:02:17,270 --> 00:02:16,000 different things from different parts of 62 00:02:19,030 --> 00:02:17,280 that spectrum 63 00:02:21,190 --> 00:02:19,040 another mission will give us a closer 64 00:02:23,270 --> 00:02:21,200 look at black holes and probe the 65 00:02:26,150 --> 00:02:23,280 mystery of dark energy 66 00:02:28,309 --> 00:02:26,160 constellation x an x-ray observatory 67 00:02:29,910 --> 00:02:28,319 will make movies of the material falling 68 00:02:37,830 --> 00:02:29,920 into a black hole 69 00:02:42,790 --> 00:02:40,070 constellation x will let us watch how 70 00:02:45,670 --> 00:02:42,800 that matter approaches the event horizon 71 00:02:46,869 --> 00:02:45,680 and how from our perspective time creeps 72 00:02:49,589 --> 00:02:46,879 to a halt 73 00:02:52,070 --> 00:02:49,599 we'll be able to watch the final x-ray 74 00:02:54,710 --> 00:02:52,080 flicker of light as matter plunges into 75 00:02:56,790 --> 00:02:54,720 the black hole and disappears forever 76 00:02:58,710 --> 00:02:56,800 this is where we'll be able to probe the 77 00:03:00,869 --> 00:02:58,720 most extreme conditions of gravity that 78 00:03:03,110 --> 00:03:00,879 we know of and really put einstein's 79 00:03:12,869 --> 00:03:03,120 theories to the test 80 00:03:18,309 --> 00:03:16,229 in 1992 the nasa kobe mission discovered 81 00:03:20,630 --> 00:03:18,319 slight temperature fluctuations in the 82 00:03:21,670 --> 00:03:20,640 nearly uniform cosmic microwave 83 00:03:23,830 --> 00:03:21,680 background 84 00:03:25,990 --> 00:03:23,840 that's the blanket of light encompassing 85 00:03:27,589 --> 00:03:26,000 the universe that is the after glow of 86 00:03:30,710 --> 00:03:27,599 the big bang 87 00:03:32,710 --> 00:03:30,720 kobe's successor nasa's wmap mission 88 00:03:35,509 --> 00:03:32,720 produced this much higher resolution 89 00:03:37,589 --> 00:03:35,519 image of the cosmic microwave background 90 00:03:40,710 --> 00:03:37,599 becoming one of the most scientifically 91 00:03:43,270 --> 00:03:40,720 significant images of cosmology today 92 00:03:45,589 --> 00:03:43,280 we look at the wmap data 93 00:03:47,589 --> 00:03:45,599 much of what we see in the data has the 94 00:03:50,390 --> 00:03:47,599 imprint of the physical processes that 95 00:03:51,830 --> 00:03:50,400 took place about 300 000 years after the 96 00:03:53,830 --> 00:03:51,840 big bang 97 00:03:55,750 --> 00:03:53,840 the basic properties that we've inferred 98 00:03:58,390 --> 00:03:55,760 from this is that the geometry of the 99 00:04:00,710 --> 00:03:58,400 universe is flat or nearly flat we also 100 00:04:05,270 --> 00:04:00,720 know it's pretty old today we know it's 101 00:04:07,589 --> 00:04:05,280 about 13.6 13.7 billion years old and 102 00:04:09,350 --> 00:04:07,599 the stars formed about 100 million years 103 00:04:11,670 --> 00:04:09,360 after the big bang 104 00:04:13,910 --> 00:04:11,680 the information obtained by wmap and 105 00:04:15,990 --> 00:04:13,920 proposed missions will help distinguish 106 00:04:19,189 --> 00:04:16,000 between competing theories of what 107 00:04:21,749 --> 00:04:19,199 sparked inflation and the big bang 108 00:04:23,909 --> 00:04:21,759 einstein hoped to fold the quantum force 109 00:04:27,350 --> 00:04:23,919 of electromagnetism into general 110 00:04:28,950 --> 00:04:27,360 relativity and to find a unified theory 111 00:04:31,030 --> 00:04:28,960 much of what he could not answer and 112 00:04:33,110 --> 00:04:31,040 struggled with until the day he died 113 00:04:35,670 --> 00:04:33,120 remains unanswered today 114 00:04:38,230 --> 00:04:35,680 these questions about dark energy black 115 00:04:40,790 --> 00:04:38,240 holes the big bang and the nature of 116 00:04:43,510 --> 00:04:40,800 gravity have come to define the cutting 117 00:04:46,230 --> 00:04:43,520 edge 118 00:04:47,030 --> 00:04:46,240 the next revolution that i think could 119 00:04:49,189 --> 00:04:47,040 be 120 00:04:52,310 --> 00:04:49,199 in the not too distant future 121 00:04:54,870 --> 00:04:52,320 is to really learn what space and time 122 00:04:56,230 --> 00:04:54,880 actually are and i think as to others 123 00:04:58,310 --> 00:04:56,240 that we will learn that space and time 124 00:04:59,670 --> 00:04:58,320 are not fundamental there are more 125 00:05:03,189 --> 00:04:59,680 fundamental 126 00:05:05,110 --> 00:05:03,199 entities that make up space and time and 127 00:05:07,189 --> 00:05:05,120 when we can figure out what they are the 128 00:05:09,430 --> 00:05:07,199 atoms if you will of space and time 129 00:05:11,029 --> 00:05:09,440 themselves i think that will take our 130 00:05:13,350 --> 00:05:11,039 understanding of the universe to a 131 00:05:17,029 --> 00:05:13,360 completely new level and i think that 132 00:05:19,510 --> 00:05:17,039 discovery may be on the horizon 133 00:05:21,270 --> 00:05:19,520 like einstein's theories modern theories 134 00:05:22,790 --> 00:05:21,280 make fantastic predictions that seem 135 00:05:25,270 --> 00:05:22,800 hard to believe 136 00:05:26,710 --> 00:05:25,280 unseen dimensions and entire universes 137 00:05:29,590 --> 00:05:26,720 beyond our own 138 00:05:31,189 --> 00:05:29,600 we must find facts to confront and guide 139 00:05:33,430 --> 00:05:31,199 these new theories 140 00:05:35,749 --> 00:05:33,440 thus we follow matter to the very brink 141 00:05:37,830 --> 00:05:35,759 of black holes and detect particles of 142 00:05:38,870 --> 00:05:37,840 time left over from the beginning of the 143 00:05:40,390 --> 00:05:38,880 universe 144 00:05:42,469 --> 00:05:40,400 and we will use breakthrough 145 00:05:45,270 --> 00:05:42,479 technologies to see beyond the vision of