1 00:00:42,950 --> 00:00:40,150 in february of 1987 2 00:00:46,389 --> 00:00:42,960 astronomers looking at the nearby galaxy 3 00:00:50,869 --> 00:00:46,399 called the large magellanic cloud 4 00:00:56,709 --> 00:00:53,350 a supernova explosion 5 00:00:58,790 --> 00:00:56,719 the spectacular death of the star 6 00:01:02,150 --> 00:00:58,800 astronomers around the world have 7 00:01:04,789 --> 00:01:02,160 eagerly studied supernova 1987 a with 8 00:01:07,270 --> 00:01:04,799 sensitive telescopes hoping to learn 9 00:01:10,390 --> 00:01:07,280 what will happen to the expanding debris 10 00:01:12,310 --> 00:01:10,400 and the fiery core of the star 11 00:01:14,789 --> 00:01:12,320 has the inner core collapsed as 12 00:01:18,310 --> 00:01:14,799 scientists expect into a tiny dense 13 00:01:21,990 --> 00:01:18,320 pulsing neutron star at the center 14 00:01:25,109 --> 00:01:22,000 in the exploding gas in giant supernovas 15 00:01:28,469 --> 00:01:25,119 in hundreds of millions of stars 16 00:01:30,950 --> 00:01:28,479 in huge spiraling galaxies 17 00:01:32,789 --> 00:01:30,960 in distant quasars whose light has been 18 00:01:34,230 --> 00:01:32,799 traveling to us since the beginning of 19 00:01:36,550 --> 00:01:34,240 the universe 20 00:01:38,630 --> 00:01:36,560 in these fantastic objects 21 00:01:40,710 --> 00:01:38,640 astronomers have learned that great 22 00:01:43,429 --> 00:01:40,720 forces heat gasses to extreme 23 00:01:44,630 --> 00:01:43,439 temperatures above tens of millions of 24 00:01:46,870 --> 00:01:44,640 degrees 25 00:01:49,670 --> 00:01:46,880 causing them to emit massive amounts of 26 00:01:53,910 --> 00:01:51,670 the space shuttle will carry sensitive 27 00:01:55,590 --> 00:01:53,920 new telescopes into orbit to study the 28 00:01:57,830 --> 00:01:55,600 cosmos 29 00:02:00,389 --> 00:01:57,840 one telescope measures x-rays emitted 30 00:02:02,789 --> 00:02:00,399 from supernovas quasars and other high 31 00:02:04,550 --> 00:02:02,799 energy targets in space 32 00:02:07,190 --> 00:02:04,560 priceless new information from this 33 00:02:09,430 --> 00:02:07,200 broadband x-ray telescope will help 34 00:02:20,830 --> 00:02:09,440 scientists uncover more pieces in the 35 00:02:26,390 --> 00:02:24,150 universe go for main engine start 36 00:02:28,150 --> 00:02:26,400 four three two 37 00:02:29,110 --> 00:02:28,160 one 38 00:02:35,750 --> 00:02:29,120 and 39 00:02:40,550 --> 00:02:38,470 in the spring of 1990 the space shuttle 40 00:02:43,030 --> 00:02:40,560 columbia will lift off on a special 41 00:02:45,350 --> 00:02:43,040 mission called astro one 42 00:02:46,949 --> 00:02:45,360 dedicated to scientific observations of 43 00:02:49,430 --> 00:02:46,959 our universe 44 00:02:51,350 --> 00:02:49,440 once in orbit four new telescopes will 45 00:02:52,589 --> 00:02:51,360 be operated from the shuttle's payload 46 00:02:56,550 --> 00:02:52,599 bay 47 00:02:59,509 --> 00:02:56,560 bbxrt the broadband x-ray telescope 48 00:03:01,910 --> 00:02:59,519 analyzes x-rays emitted by extremely hot 49 00:03:02,830 --> 00:03:01,920 and energetic stars and galaxies in 50 00:03:05,670 --> 00:03:02,840 distant 51 00:03:08,309 --> 00:03:05,680 space three other telescopes mounted 52 00:03:10,390 --> 00:03:08,319 together on a pointing platform examine 53 00:03:12,630 --> 00:03:10,400 ultraviolet light emitted from nearby 54 00:03:15,509 --> 00:03:12,640 objects in our solar system and from 55 00:03:17,670 --> 00:03:15,519 stars and distant galaxies 56 00:03:18,550 --> 00:03:17,680 these telescopes must be operated in 57 00:03:20,630 --> 00:03:18,560 space 58 00:03:23,430 --> 00:03:20,640 because the earth's atmosphere prevents 59 00:03:25,270 --> 00:03:23,440 most radiation including x-rays and 60 00:03:27,110 --> 00:03:25,280 ultraviolet light from reaching the 61 00:03:29,190 --> 00:03:27,120 ground 62 00:03:31,110 --> 00:03:29,200 the visible light that we can see is a 63 00:03:33,990 --> 00:03:31,120 surprisingly small portion of the 64 00:03:35,589 --> 00:03:34,000 radiation that is emitted in space 65 00:03:37,670 --> 00:03:35,599 we know that massive amounts of 66 00:03:40,229 --> 00:03:37,680 radiation are emitted in the invisible 67 00:03:43,430 --> 00:03:40,239 portion of the electromagnetic spectrum 68 00:03:45,430 --> 00:03:43,440 including ultraviolet light and x-rays 69 00:03:47,270 --> 00:03:45,440 each type of radiation provides 70 00:03:48,630 --> 00:03:47,280 different clues about the nature of the 71 00:03:51,110 --> 00:03:48,640 object 72 00:03:53,429 --> 00:03:51,120 the broadband x-ray telescope studies 73 00:03:55,830 --> 00:03:53,439 radiation emitted in a large portion of 74 00:03:59,030 --> 00:03:55,840 the x-ray spectrum which has never been 75 00:04:02,229 --> 00:03:59,040 studied before in great detail 76 00:04:03,990 --> 00:04:02,239 for example bbxrt can detect which 77 00:04:07,830 --> 00:04:04,000 chemical elements are present in an 78 00:04:08,789 --> 00:04:07,840 x-ray source such as oxygen magnesium 79 00:04:10,949 --> 00:04:08,799 silicon 80 00:04:13,670 --> 00:04:10,959 sulfur and calcium 81 00:04:17,030 --> 00:04:13,680 elements that are abundant in space and 82 00:04:20,469 --> 00:04:17,040 essential to life on earth 83 00:04:22,629 --> 00:04:20,479 bbxrt is the first x-ray telescope used 84 00:04:25,590 --> 00:04:22,639 in space that can detect the presence of 85 00:04:27,830 --> 00:04:25,600 iron in a broad variety of targets 86 00:04:30,150 --> 00:04:27,840 because iron is one of the most abundant 87 00:04:32,390 --> 00:04:30,160 elements in the universe its presence in 88 00:04:34,870 --> 00:04:32,400 an x-ray source provides tell-tale 89 00:04:38,150 --> 00:04:34,880 evidence about that object for example 90 00:04:40,710 --> 00:04:38,160 its size temperature how old it is 91 00:04:46,469 --> 00:04:40,720 whether it rotates and at what speed and 92 00:04:50,710 --> 00:04:48,310 the dream of building and launching a 93 00:04:53,670 --> 00:04:50,720 broadband x-ray telescope into space 94 00:04:55,590 --> 00:04:53,680 began more than 12 years ago here at 95 00:04:57,430 --> 00:04:55,600 nasa's goddard space flight center in 96 00:04:59,670 --> 00:04:57,440 greenbelt maryland 97 00:05:02,070 --> 00:04:59,680 over 40 satellites have been built and 98 00:05:03,830 --> 00:05:02,080 tested at goddard countless others have 99 00:05:05,590 --> 00:05:03,840 been managed by nasa's greenbelt 100 00:05:07,749 --> 00:05:05,600 facility 101 00:05:10,070 --> 00:05:07,759 in the late 1970s 102 00:05:11,990 --> 00:05:10,080 dr peter cerlamitsos working in 103 00:05:14,230 --> 00:05:12,000 goddard's high energy astrophysics 104 00:05:16,710 --> 00:05:14,240 laboratory developed a light and 105 00:05:18,629 --> 00:05:16,720 inexpensive mirror sufficiently smooth 106 00:05:21,510 --> 00:05:18,639 to reflect x-rays 107 00:05:24,469 --> 00:05:21,520 it was made from shiny aluminum foil 108 00:05:26,390 --> 00:05:24,479 coated with acrylic and gold the mirrors 109 00:05:28,550 --> 00:05:26,400 were nested together in a housing to 110 00:05:30,469 --> 00:05:28,560 provide the large surface area needed to 111 00:05:32,950 --> 00:05:30,479 gather x-rays 112 00:05:34,870 --> 00:05:32,960 these foil mirrors made the telescope 113 00:05:36,790 --> 00:05:34,880 light enough to be carried into space on 114 00:05:38,469 --> 00:05:36,800 the shuttle 115 00:05:41,029 --> 00:05:38,479 once the telescope was approved for 116 00:05:43,670 --> 00:05:41,039 flight teams of up to 100 goddard 117 00:05:45,670 --> 00:05:43,680 scientists engineers and technicians 118 00:05:47,749 --> 00:05:45,680 worked for five years to build the 119 00:05:50,469 --> 00:05:47,759 instrument and a unique reusable 120 00:05:52,710 --> 00:05:50,479 pointing system for the telescope 121 00:05:55,830 --> 00:05:52,720 payload manager frank volpe describes 122 00:05:57,909 --> 00:05:55,840 the challenges of building the telescope 123 00:06:01,189 --> 00:05:57,919 when you fly in the orbiter the the key 124 00:06:02,870 --> 00:06:01,199 most criteria is to make sure it's safe 125 00:06:05,510 --> 00:06:02,880 so we have gone through extensive 126 00:06:07,749 --> 00:06:05,520 testing and design to ensure that in no 127 00:06:09,749 --> 00:06:07,759 way jeopardize the health and safety of 128 00:06:11,990 --> 00:06:09,759 the crew and the orbiter 129 00:06:15,189 --> 00:06:12,000 to that extent you also must make sure 130 00:06:17,830 --> 00:06:15,199 that it is its limits of weight 131 00:06:19,909 --> 00:06:17,840 and power and thermal requirements all 132 00:06:22,309 --> 00:06:19,919 within the constraints of the orbiter 133 00:06:24,309 --> 00:06:22,319 itself we had to take some 134 00:06:26,230 --> 00:06:24,319 exceptional uh 135 00:06:28,309 --> 00:06:26,240 steps to ensure that 136 00:06:30,710 --> 00:06:28,319 the thermal systems remained within its 137 00:06:33,110 --> 00:06:30,720 limits at one end of the telescope 138 00:06:35,670 --> 00:06:33,120 we have elements operating at a very 139 00:06:36,629 --> 00:06:35,680 very cold temperature around 40 degrees 140 00:06:38,950 --> 00:06:36,639 kelvin 141 00:06:40,629 --> 00:06:38,960 at other places on the telescope and the 142 00:06:43,029 --> 00:06:40,639 payload we have 143 00:06:44,309 --> 00:06:43,039 boxes that like to operate near room 144 00:06:46,629 --> 00:06:44,319 temperature 145 00:06:48,309 --> 00:06:46,639 once the telescope was built it was 146 00:06:50,309 --> 00:06:48,319 lowered into the two-axis pointing 147 00:06:52,629 --> 00:06:50,319 system structure 148 00:06:54,550 --> 00:06:52,639 during the integration and testing phase 149 00:06:56,230 --> 00:06:54,560 the complex electronic systems 150 00:06:58,469 --> 00:06:56,240 controlling the telescope and the 151 00:07:00,550 --> 00:06:58,479 support structure were wired together 152 00:07:02,309 --> 00:07:00,560 and repeatedly checked 153 00:07:05,270 --> 00:07:02,319 blankets were attached to achieve the 154 00:07:08,070 --> 00:07:05,280 required thermal insulation in space 155 00:07:10,710 --> 00:07:08,080 vibration acoustics and thermal vacuum 156 00:07:12,629 --> 00:07:10,720 tests were conducted on the telescope to 157 00:07:14,309 --> 00:07:12,639 simulate conditions encountered during 158 00:07:16,230 --> 00:07:14,319 the mission 159 00:07:18,629 --> 00:07:16,240 some of the shuttle astronauts shown 160 00:07:20,790 --> 00:07:18,639 here in their anti-contamination suits 161 00:07:22,390 --> 00:07:20,800 came to goddard to get a first-hand look 162 00:07:24,629 --> 00:07:22,400 at the new telescope that they will 163 00:07:26,790 --> 00:07:24,639 carry into orbit 164 00:07:29,430 --> 00:07:26,800 goddard scientists have carefully chosen 165 00:07:30,790 --> 00:07:29,440 the x-ray sources that the bbxrt will 166 00:07:33,110 --> 00:07:30,800 observe 167 00:07:36,469 --> 00:07:33,120 these unusually hot and energetic 168 00:07:39,270 --> 00:07:36,479 targets vary from tiny neutron stars 169 00:07:45,189 --> 00:07:39,280 drawing gas from a larger companion star 170 00:07:51,510 --> 00:07:48,710 a prime bbxrt target is a supernova 171 00:07:55,749 --> 00:07:51,520 remnant the exploded outer shell of a 172 00:07:58,390 --> 00:07:55,759 star which occupies vast areas in space 173 00:08:01,110 --> 00:07:58,400 the outer edges heated to extreme 174 00:08:03,589 --> 00:08:01,120 temperatures by shock waves emit 175 00:08:05,070 --> 00:08:03,599 millions of x-rays 176 00:08:08,070 --> 00:08:05,080 in these regions 177 00:08:10,309 --> 00:08:08,080 bbxrt can detect the presence of heavy 178 00:08:13,510 --> 00:08:10,319 elements such as iron and many other 179 00:08:16,150 --> 00:08:13,520 elements that make up our own bodies 180 00:08:17,830 --> 00:08:16,160 by studying the supernova the x-ray 181 00:08:19,990 --> 00:08:17,840 telescope will contribute new 182 00:08:23,589 --> 00:08:20,000 information about how these important 183 00:08:26,950 --> 00:08:23,599 elements are manufactured inside stars 184 00:08:28,629 --> 00:08:26,960 bbxrt principal investigator dr peter 185 00:08:30,869 --> 00:08:28,639 cerlemitsos 186 00:08:34,230 --> 00:08:30,879 everything we learn from it is telltale 187 00:08:36,230 --> 00:08:34,240 evidence of what was inside the star 188 00:08:38,310 --> 00:08:36,240 you know how we're going to study what 189 00:08:40,709 --> 00:08:38,320 the star is forming inside we're waiting 190 00:08:43,029 --> 00:08:40,719 for it to spew this matter out in the 191 00:08:45,430 --> 00:08:43,039 interstellar space and therefore 192 00:08:47,990 --> 00:08:45,440 from the pieces out there we see the 193 00:08:50,470 --> 00:08:48,000 x-ray emission that tells us what was 194 00:08:53,190 --> 00:08:50,480 forming the star what how much iron how 195 00:08:56,030 --> 00:08:53,200 much silicon and so forth 196 00:08:59,030 --> 00:08:56,040 as the exploded outer shell of supernova 197 00:09:02,070 --> 00:08:59,040 1987a dissipates into space 198 00:09:04,790 --> 00:09:02,080 it may be possible for bbxrt to observe 199 00:09:06,310 --> 00:09:04,800 the existence of a neutron star at the 200 00:09:08,470 --> 00:09:06,320 center 201 00:09:10,790 --> 00:09:08,480 neutron stars are formed during a 202 00:09:13,430 --> 00:09:10,800 supernova explosion when the inner 203 00:09:15,269 --> 00:09:13,440 region of a star collapses into a tiny 204 00:09:17,829 --> 00:09:15,279 core 205 00:09:20,710 --> 00:09:17,839 pulsars are neutron stars that rotate 206 00:09:22,870 --> 00:09:20,720 extremely quickly some as fast as one 207 00:09:25,030 --> 00:09:22,880 thousand times a second 208 00:09:27,670 --> 00:09:25,040 they emit light and x-rays in 209 00:09:29,430 --> 00:09:27,680 searchlight beams making them appear to 210 00:09:31,430 --> 00:09:29,440 blink on and off 211 00:09:33,750 --> 00:09:31,440 scientists believe that neutron stars 212 00:09:36,070 --> 00:09:33,760 are unimaginably dense 213 00:09:41,110 --> 00:09:36,080 one teaspoonful of matter from a neutron 214 00:09:43,430 --> 00:09:41,120 star would weigh over a billion tons 215 00:09:46,150 --> 00:09:43,440 many neutron stars are often paired with 216 00:09:48,710 --> 00:09:46,160 a much larger companion star 217 00:09:51,430 --> 00:09:48,720 in this binary star system the tiny 218 00:09:54,310 --> 00:09:51,440 neutron star exerts an extremely strong 219 00:09:56,470 --> 00:09:54,320 gravitational pull which draws gas from 220 00:09:58,790 --> 00:09:56,480 the companion star 221 00:10:01,110 --> 00:09:58,800 the gas flows into an accretion disk 222 00:10:03,030 --> 00:10:01,120 around the neutron star 223 00:10:06,069 --> 00:10:03,040 as it approaches the star 224 00:10:09,750 --> 00:10:06,079 the gas is heated to millions of degrees 225 00:10:11,670 --> 00:10:09,760 and emits large amounts of x-rays 226 00:10:13,750 --> 00:10:11,680 in some systems 227 00:10:18,470 --> 00:10:13,760 the gas flows onto the pole of the 228 00:10:20,389 --> 00:10:18,480 neutron star along its magnetic field 229 00:10:22,630 --> 00:10:20,399 scientists believe that some binary 230 00:10:25,990 --> 00:10:22,640 systems may contain a mysterious black 231 00:10:28,550 --> 00:10:26,000 hole instead of a neutron star 232 00:10:31,670 --> 00:10:28,560 x-rays are admitted as the swirling hot 233 00:10:33,750 --> 00:10:31,680 gas is drawn into the black hole 234 00:10:36,310 --> 00:10:33,760 the gravitational force exerted by the 235 00:10:38,710 --> 00:10:36,320 black hole is so strong that neither 236 00:10:40,630 --> 00:10:38,720 light nor matter can escape once they 237 00:10:42,710 --> 00:10:40,640 are drawn in 238 00:10:46,790 --> 00:10:42,720 the physical conditions found inside the 239 00:10:48,710 --> 00:10:46,800 black hole are totally unknown 240 00:10:50,870 --> 00:10:48,720 the x-ray telescope will study a 241 00:10:53,509 --> 00:10:50,880 suspected black hole in our galaxy 242 00:10:56,230 --> 00:10:53,519 called cygnus x1 243 00:10:58,550 --> 00:10:56,240 scientists hope bbxrt 244 00:11:01,190 --> 00:10:58,560 will confirm the theory that material is 245 00:11:04,069 --> 00:11:01,200 actually spiraling around the black hole 246 00:11:06,790 --> 00:11:04,079 as it is drawn into it 247 00:11:09,509 --> 00:11:06,800 perhaps none of bbxrt's targets are as 248 00:11:11,509 --> 00:11:09,519 mysterious as the quasars 249 00:11:13,910 --> 00:11:11,519 though they look like stars 250 00:11:16,150 --> 00:11:13,920 quasars are believed to be the center of 251 00:11:17,670 --> 00:11:16,160 distant galaxies formed billions of 252 00:11:20,470 --> 00:11:17,680 years ago 253 00:11:23,990 --> 00:11:20,480 yet a single quasar radiates more energy 254 00:11:26,069 --> 00:11:24,000 than 100 normal galaxies combined 255 00:11:29,430 --> 00:11:26,079 it is believed that quasars may be 256 00:11:31,829 --> 00:11:29,440 powered by a massive black hole 257 00:11:33,670 --> 00:11:31,839 quasars are the furthest objects from 258 00:11:35,750 --> 00:11:33,680 earth ever observed 259 00:11:38,069 --> 00:11:35,760 so the light emitted from them dates 260 00:11:38,949 --> 00:11:38,079 back to a time much closer to the big 261 00:11:41,829 --> 00:11:38,959 bang 262 00:11:43,750 --> 00:11:41,839 the indescribably huge explosion that 263 00:11:45,670 --> 00:11:43,760 scientists believe was the beginning of 264 00:11:49,430 --> 00:11:45,680 the universe 265 00:11:51,509 --> 00:11:49,440 bb xrt co-investigator frank marshall 266 00:11:53,750 --> 00:11:51,519 quasars have been known for i guess more 267 00:11:55,590 --> 00:11:53,760 than 20 years now but it's still not 268 00:11:58,069 --> 00:11:55,600 known what the 269 00:12:00,470 --> 00:11:58,079 real energy generation mechanism 270 00:12:02,710 --> 00:12:00,480 in quasars is but x-rays allow you to 271 00:12:05,110 --> 00:12:02,720 look very close into the central engine 272 00:12:07,269 --> 00:12:05,120 of quasars which is where most of the 273 00:12:09,590 --> 00:12:07,279 action is going on so we'll look very 274 00:12:13,190 --> 00:12:09,600 close to what we think is the black hole 275 00:12:15,509 --> 00:12:13,200 at the at the center of the quasar and 276 00:12:17,750 --> 00:12:15,519 get a measurement of perhaps how the 277 00:12:18,949 --> 00:12:17,760 material is is falling into the into the 278 00:12:21,190 --> 00:12:18,959 quasar 279 00:12:25,030 --> 00:12:21,200 and how large the object the center of 280 00:12:30,790 --> 00:12:27,910 the largest areas bbxrt will study are 281 00:12:32,949 --> 00:12:30,800 clusters of galaxies where hundreds of 282 00:12:35,269 --> 00:12:32,959 galaxies move around each other in their 283 00:12:36,870 --> 00:12:35,279 own gravitational system 284 00:12:39,670 --> 00:12:36,880 previous x-ray instruments have 285 00:12:41,829 --> 00:12:39,680 discovered an extremely hot gas that 286 00:12:43,190 --> 00:12:41,839 covers an enormous region within the 287 00:12:46,069 --> 00:12:43,200 cluster 288 00:12:47,750 --> 00:12:46,079 bbxrt will analyze the chemical makeup 289 00:12:50,470 --> 00:12:47,760 of the gas 290 00:12:52,470 --> 00:12:50,480 clusters of galaxies what is the gas 291 00:12:53,430 --> 00:12:52,480 that is in them how hot it is and what 292 00:12:56,230 --> 00:12:53,440 it is 293 00:12:58,230 --> 00:12:56,240 is it just hydrogen from from the big 294 00:13:00,949 --> 00:12:58,240 bang or is it something that the 295 00:13:02,230 --> 00:13:00,959 galaxies that are going in this cluster 296 00:13:04,629 --> 00:13:02,240 that has 297 00:13:06,069 --> 00:13:04,639 been spewing out and now it's heated up 298 00:13:07,350 --> 00:13:06,079 in the middle of the cluster in 299 00:13:09,829 --> 00:13:07,360 astrophysics this is important 300 00:13:12,310 --> 00:13:09,839 information and instruments like bbxrt 301 00:13:14,150 --> 00:13:12,320 give you that information it's just that 302 00:13:16,550 --> 00:13:14,160 a lot of this information simply does 303 00:13:19,509 --> 00:13:16,560 not exist right now and bbxrt will be 304 00:13:21,590 --> 00:13:19,519 producing this information 305 00:13:23,430 --> 00:13:21,600 the weeks prior to the launch are a time 306 00:13:26,230 --> 00:13:23,440 of great anticipation for the men and 307 00:13:28,629 --> 00:13:26,240 women who work to build a telescope 308 00:13:31,350 --> 00:13:28,639 together with the ultraviolet telescopes 309 00:13:34,870 --> 00:13:31,360 bbxrt is positioned into the shuttle's 310 00:13:37,430 --> 00:13:34,880 payload bay at the kennedy space center 311 00:13:38,949 --> 00:13:37,440 during the mission the x-ray telescope 312 00:13:40,710 --> 00:13:38,959 will be controlled from the goddard 313 00:13:42,550 --> 00:13:40,720 space flight center 314 00:13:44,230 --> 00:13:42,560 several flight simulations are held 315 00:13:46,230 --> 00:13:44,240 prior to launch 316 00:13:48,629 --> 00:13:46,240 many of the scientists and engineers who 317 00:13:50,629 --> 00:13:48,639 built and tested the telescope practiced 318 00:13:52,629 --> 00:13:50,639 the commands and procedures to be used 319 00:13:55,990 --> 00:13:52,639 during the mission you can enable taps 320 00:13:59,350 --> 00:13:56,000 in bbxrt for command at this time 321 00:14:01,750 --> 00:13:59,360 astro will be around the clock mission 322 00:14:04,230 --> 00:14:01,760 nearly every orbit the astronauts will 323 00:14:05,990 --> 00:14:04,240 adjust the orientation of the shuttle 324 00:14:08,470 --> 00:14:06,000 then the telescopes will make fine 325 00:14:10,230 --> 00:14:08,480 adjustments toward new targets 326 00:14:12,710 --> 00:14:10,240 for part of the mission all the 327 00:14:14,829 --> 00:14:12,720 telescopes will point at the same target 328 00:14:17,590 --> 00:14:14,839 such as supernova 329 00:14:19,990 --> 00:14:17,600 1987a by comparing simultaneous 330 00:14:22,069 --> 00:14:20,000 information taken in two different bands 331 00:14:24,069 --> 00:14:22,079 of the electromagnetic spectrum 332 00:14:26,550 --> 00:14:24,079 scientists will gain a more complete 333 00:14:29,430 --> 00:14:26,560 understanding of these targets 334 00:14:31,590 --> 00:14:29,440 at other times the x-ray and ultraviolet 335 00:14:32,870 --> 00:14:31,600 telescopes will be pointed at different 336 00:14:34,870 --> 00:14:32,880 targets 337 00:14:37,829 --> 00:14:34,880 all data from the telescopes will be 338 00:14:39,590 --> 00:14:37,839 analyzed over the coming years 339 00:14:42,550 --> 00:14:39,600 what's been exciting about this project 340 00:14:45,350 --> 00:14:42,560 is that science was conceived here 341 00:14:47,269 --> 00:14:45,360 the instrument was developed here the 342 00:14:49,350 --> 00:14:47,279 rest of the payload was developed and 343 00:14:51,990 --> 00:14:49,360 integrated and tested here 344 00:14:53,670 --> 00:14:52,000 and the whole payload will be controlled 345 00:14:55,189 --> 00:14:53,680 from the goddard space flight center 346 00:14:57,189 --> 00:14:55,199 control center 347 00:14:59,590 --> 00:14:57,199 largely we don't know 348 00:15:01,030 --> 00:14:59,600 exactly what we're going to see which is 349 00:15:03,590 --> 00:15:01,040 part of the excitement 350 00:15:05,750 --> 00:15:03,600 the 10 days will produce for us and 351 00:15:07,990 --> 00:15:05,760 discovering exactly what 352 00:15:09,990 --> 00:15:08,000 what we do find because in the past 353 00:15:11,430 --> 00:15:10,000 x-ray astronomy new x-ray astronomy 354 00:15:12,870 --> 00:15:11,440 missions have always produced something 355 00:15:14,949 --> 00:15:12,880 we didn't anticipate 356 00:15:17,110 --> 00:15:14,959 in many circumstances those are the most 357 00:15:19,269 --> 00:15:17,120 have been the most exciting results 358 00:15:24,870 --> 00:15:19,279 and i'm very hopeful that the same will 359 00:15:29,590 --> 00:15:27,670 the broadband x-ray telescope 360 00:15:30,949 --> 00:15:29,600 along with the astro ultraviolet 361 00:15:33,110 --> 00:15:30,959 telescopes 362 00:15:35,430 --> 00:15:33,120 stands ready to deliver brand new 363 00:15:36,470 --> 00:15:35,440 information to scientists all over the 364 00:15:38,829 --> 00:15:36,480 world 365 00:15:41,509 --> 00:15:38,839 about the greatest mysteries in the 366 00:15:43,110 --> 00:15:41,519 universe its origin 367 00:16:27,990 --> 00:15:43,120 its evolution