1 00:00:10,390 --> 00:00:05,749 why won't the supernova explode 2 00:00:16,150 --> 00:00:12,549 somewhere in the milky way a massive 3 00:00:18,630 --> 00:00:16,160 star is about to die a spectacular death 4 00:00:20,230 --> 00:00:18,640 as its nuclear fuel runs out the star 5 00:00:22,390 --> 00:00:20,240 begins to collapse under its own 6 00:00:24,390 --> 00:00:22,400 tremendous weight 7 00:00:25,509 --> 00:00:24,400 crushing pressure triggers new nuclear 8 00:00:28,070 --> 00:00:25,519 reactions 9 00:00:29,349 --> 00:00:28,080 setting the stage for a terrifying blast 10 00:00:31,750 --> 00:00:29,359 and then 11 00:00:33,350 --> 00:00:31,760 nothing happens 12 00:00:36,229 --> 00:00:33,360 at least that's what supercomputers have 13 00:00:37,750 --> 00:00:36,239 been telling astrophysicists for decades 14 00:00:41,590 --> 00:00:37,760 many of the best computer models of 15 00:00:43,670 --> 00:00:41,600 supernovas fail to produce an explosion 16 00:00:45,830 --> 00:00:43,680 at the end of the simulation gravity 17 00:00:47,350 --> 00:00:45,840 wins the day and the star simply 18 00:00:50,790 --> 00:00:47,360 collapses 19 00:00:52,790 --> 00:00:50,800 clearly physicists are missing something 20 00:00:55,189 --> 00:00:52,800 we don't fully understand how supernovas 21 00:00:57,350 --> 00:00:55,199 of massive stars work yet says fiona 22 00:01:00,950 --> 00:00:57,360 harrison an astrophysicist at the 23 00:01:02,869 --> 00:01:00,960 california institute of technology 24 00:01:04,950 --> 00:01:02,879 to figure out what's going on 25 00:01:07,990 --> 00:01:04,960 scientists need to examine the inside of 26 00:01:10,950 --> 00:01:08,000 a real supernova while it's exploding 27 00:01:13,670 --> 00:01:10,960 not a particularly easy thing to do 28 00:01:15,910 --> 00:01:13,680 so instead they examine the remnant of 29 00:01:17,590 --> 00:01:15,920 the exploded star as soon after the 30 00:01:19,190 --> 00:01:17,600 explosion as possible 31 00:01:21,270 --> 00:01:19,200 harrison and colleagues have figured out 32 00:01:23,030 --> 00:01:21,280 how to do this using a new space 33 00:01:25,350 --> 00:01:23,040 telescope called the nuclear 34 00:01:27,749 --> 00:01:25,360 spectroscopic telescope array 35 00:01:30,390 --> 00:01:27,759 nustar for short 36 00:01:32,310 --> 00:01:30,400 launched on june 13th 2012 onboard a 37 00:01:34,950 --> 00:01:32,320 pegasus xl rocket dropped from an 38 00:01:37,429 --> 00:01:34,960 airplane high above the pacific ocean 39 00:01:39,429 --> 00:01:37,439 nustar is a small explorer satellite 40 00:01:42,469 --> 00:01:39,439 that carries the first space telescope 41 00:01:44,789 --> 00:01:42,479 that can focus very high energy x-rays 42 00:01:46,789 --> 00:01:44,799 nustar will produce images roughly 100 43 00:01:49,990 --> 00:01:46,799 times sharper than those possible with 44 00:01:52,149 --> 00:01:50,000 previous high-energy x-ray telescopes 45 00:01:54,630 --> 00:01:52,159 when nustar finishes its checkout and 46 00:01:56,469 --> 00:01:54,640 becomes fully operational scientists 47 00:01:58,389 --> 00:01:56,479 will use it to scan supernova remnants 48 00:01:59,670 --> 00:01:58,399 for clues etched into the pattern of 49 00:02:01,749 --> 00:01:59,680 elements spread throughout the 50 00:02:03,429 --> 00:02:01,759 explosion's debris 51 00:02:05,590 --> 00:02:03,439 the distribution of the material in a 52 00:02:08,630 --> 00:02:05,600 supernova remnant tells you a lot about 53 00:02:10,710 --> 00:02:08,640 the original explosion says harrison 54 00:02:13,030 --> 00:02:10,720 an element of particular interest is 55 00:02:14,869 --> 00:02:13,040 titanium 44. 56 00:02:16,869 --> 00:02:14,879 creating this isotope of titanium 57 00:02:19,430 --> 00:02:16,879 through nuclear fusion requires a 58 00:02:21,430 --> 00:02:19,440 certain combination of energy pressure 59 00:02:23,430 --> 00:02:21,440 and raw materials 60 00:02:25,270 --> 00:02:23,440 inside the collapsing star that 61 00:02:27,030 --> 00:02:25,280 combination occurs at a depth that's 62 00:02:29,110 --> 00:02:27,040 very special 63 00:02:31,270 --> 00:02:29,120 everything below that depth succumbs to 64 00:02:32,949 --> 00:02:31,280 gravity and collapses inward to form a 65 00:02:34,550 --> 00:02:32,959 black hole 66 00:02:37,030 --> 00:02:34,560 everything above that depth will be 67 00:02:39,589 --> 00:02:37,040 blown outward in the explosion 68 00:02:42,390 --> 00:02:39,599 titanium 44 is created just above the 69 00:02:44,309 --> 00:02:42,400 cusp so the pattern of how titanium 44 70 00:02:46,229 --> 00:02:44,319 is spread throughout a supernova remnant 71 00:02:47,750 --> 00:02:46,239 can reveal a lot about what happened at 72 00:02:50,390 --> 00:02:47,760 that crucial threshold during the 73 00:02:52,070 --> 00:02:50,400 explosion and with that information 74 00:02:53,350 --> 00:02:52,080 scientists might be able to figure out 75 00:02:55,830 --> 00:02:53,360 what's wrong with their computer 76 00:02:58,229 --> 00:02:55,840 simulations 77 00:03:00,390 --> 00:02:58,239 to detect titanium 44 78 00:03:02,470 --> 00:03:00,400 nustar needs to be able to focus very 79 00:03:05,190 --> 00:03:02,480 high energy x-rays 80 00:03:07,509 --> 00:03:05,200 titanium 44 is radioactive 81 00:03:11,910 --> 00:03:07,519 and when it decays it releases photons 82 00:03:14,470 --> 00:03:11,920 with an energy of 68 000 electron volts 83 00:03:16,949 --> 00:03:14,480 existing x-ray space telescopes such as 84 00:03:19,750 --> 00:03:16,959 nasa's chandra x-ray observatory can 85 00:03:22,149 --> 00:03:19,760 focus x-rays only up to about 15 000 86 00:03:25,270 --> 00:03:22,159 electron volts 87 00:03:27,509 --> 00:03:25,280 normal lenses can't focus x-rays at all 88 00:03:31,190 --> 00:03:27,519 glass bends x-rays only a minuscule 89 00:03:33,030 --> 00:03:31,200 amount not enough to form an image 90 00:03:34,710 --> 00:03:33,040 x-ray telescopes are an entirely 91 00:03:37,670 --> 00:03:34,720 different kind of telescope consisting 92 00:03:39,190 --> 00:03:37,680 of many concentric shells 93 00:03:41,110 --> 00:03:39,200 they look a bit like the layers of a 94 00:03:43,030 --> 00:03:41,120 cylindrical onion 95 00:03:45,270 --> 00:03:43,040 incoming x-rays pass between these 96 00:03:47,030 --> 00:03:45,280 layers which guide the x-rays to the 97 00:03:49,910 --> 00:03:47,040 focus by reflecting them off the 98 00:03:51,670 --> 00:03:49,920 surfaces of the shells 99 00:03:53,429 --> 00:03:51,680 the new star team has spent years 100 00:03:55,270 --> 00:03:53,439 perfecting delicate manufacturing 101 00:03:57,589 --> 00:03:55,280 techniques required to make 102 00:04:00,550 --> 00:03:57,599 high-precision x-ray optics for nustar 103 00:04:02,390 --> 00:04:00,560 that work at energies as high as 79 000 104 00:04:04,309 --> 00:04:02,400 electron volts 105 00:04:07,509 --> 00:04:04,319 their efforts could crack the mystery of 106 00:04:09,910 --> 00:04:07,519 the supernova that wouldn't explode 107 00:04:12,309 --> 00:04:09,920 and that's just for starters 108 00:04:15,750 --> 00:04:12,319 nustar will also study black holes 109 00:04:17,189 --> 00:04:15,760 blazars pulsars and many more exotic 110 00:04:18,949 --> 00:04:17,199 objects 111 00:04:20,870 --> 00:04:18,959 the high energy universe is about to 112 00:04:23,030 --> 00:04:20,880 come into sharper focus 113 00:04:24,629 --> 00:04:23,040 and no one can say what surprises may be 114 00:04:26,469 --> 00:04:24,639 in store