1 00:00:25,429 --> 00:00:23,109 over the past 2 00:00:27,189 --> 00:00:25,439 decades we've struggled to see beyond 3 00:00:28,470 --> 00:00:27,199 the atmosphere lying between earth and 4 00:00:30,870 --> 00:00:28,480 space 5 00:00:32,870 --> 00:00:30,880 even from mountaintop observatories the 6 00:00:34,069 --> 00:00:32,880 atmosphere has blurred our view of the 7 00:00:35,990 --> 00:00:34,079 universe 8 00:00:37,670 --> 00:00:36,000 and because the atmosphere absorbs 9 00:00:39,670 --> 00:00:37,680 certain forms of energy 10 00:00:41,430 --> 00:00:39,680 our knowledge of celestial phenomena has 11 00:00:43,910 --> 00:00:41,440 been limited 12 00:00:45,270 --> 00:00:43,920 one answer has been to go beyond the 13 00:00:47,029 --> 00:00:45,280 atmosphere 14 00:00:49,830 --> 00:00:47,039 in fact between the late 60s and the 15 00:00:51,910 --> 00:00:49,840 late 70s nasa launched a series of 16 00:00:54,549 --> 00:00:51,920 special purpose observatories 17 00:00:56,830 --> 00:00:54,559 revealing ultraviolet sources such as 18 00:00:59,590 --> 00:00:56,840 very hot stars and very young 19 00:01:00,549 --> 00:00:59,600 stars these satellites made tremendous 20 00:01:02,790 --> 00:01:00,559 breakthroughs 21 00:01:04,710 --> 00:01:02,800 and encouraged astronomers to move on to 22 00:01:06,469 --> 00:01:04,720 larger observatories 23 00:01:09,190 --> 00:01:06,479 seeking answers about more distant 24 00:01:12,230 --> 00:01:09,200 galaxies mysterious pulsars 25 00:01:16,630 --> 00:01:12,240 and quasars and the universe 26 00:01:17,109 --> 00:01:16,640 itself astronomers envisioned the next 27 00:01:20,230 --> 00:01:17,119 step 28 00:01:21,990 --> 00:01:20,240 a multi-purpose observatory in space 29 00:01:23,910 --> 00:01:22,000 one that could image farther and more 30 00:01:26,310 --> 00:01:23,920 clearly than its predecessors 31 00:01:28,469 --> 00:01:26,320 uncovering phenomena in ultraviolet 32 00:01:29,510 --> 00:01:28,479 visible and near infrared regions of the 33 00:01:31,429 --> 00:01:29,520 spectrum 34 00:01:33,910 --> 00:01:31,439 an observatory that could expand our 35 00:01:35,109 --> 00:01:33,920 perception to the outer reaches of the 36 00:01:39,030 --> 00:01:35,119 universe 37 00:01:40,390 --> 00:01:39,040 that next step was hst nasa's hubble 38 00:01:42,469 --> 00:01:40,400 space telescope 39 00:01:48,149 --> 00:01:42,479 with its precision optics and diverse 40 00:01:51,910 --> 00:01:50,389 nasa is responsible for developing 41 00:01:54,389 --> 00:01:51,920 operating and maintaining this 42 00:01:56,469 --> 00:01:54,399 ground-sized space observatory 43 00:01:57,590 --> 00:01:56,479 with its unparalleled goals the hubble 44 00:01:59,270 --> 00:01:57,600 space telescope 45 00:02:01,990 --> 00:01:59,280 poses a much greater challenge to 46 00:02:20,830 --> 00:02:02,000 operate than ground-based observatories 47 00:02:20,840 --> 00:02:35,910 so 48 00:02:40,470 --> 00:02:38,470 led by nasa engineers scientists and 49 00:02:43,350 --> 00:02:40,480 researchers from universities 50 00:02:44,150 --> 00:02:43,360 industries and the european space agency 51 00:02:45,670 --> 00:02:44,160 have combined 52 00:02:48,229 --> 00:02:45,680 efforts to meet the challenge of 53 00:02:50,150 --> 00:02:48,239 operating hubble space telescope 54 00:02:51,830 --> 00:02:50,160 the result is one of the most complex 55 00:02:52,949 --> 00:02:51,840 operations and maintenance systems in 56 00:02:55,190 --> 00:02:52,959 the world 57 00:02:57,030 --> 00:02:55,200 one that ensures quality observations 58 00:03:01,910 --> 00:02:57,040 and spacecraft performance 59 00:03:06,149 --> 00:03:03,830 to take a closer look we started the 60 00:03:07,990 --> 00:03:06,159 space telescope science institute in 61 00:03:10,070 --> 00:03:08,000 baltimore maryland 62 00:03:12,309 --> 00:03:10,080 aura a consortium of american 63 00:03:13,910 --> 00:03:12,319 universities operates the institute for 64 00:03:16,229 --> 00:03:13,920 nasa 65 00:03:18,149 --> 00:03:16,239 the space telescope science institute is 66 00:03:20,070 --> 00:03:18,159 the international center for science 67 00:03:22,550 --> 00:03:20,080 activities with hst 68 00:03:23,910 --> 00:03:22,560 it plans the day-to-day observations and 69 00:03:26,949 --> 00:03:23,920 sets up the long-term 70 00:03:28,630 --> 00:03:26,959 science program astronomers first come 71 00:03:31,430 --> 00:03:28,640 in contact with the institute when they 72 00:03:33,750 --> 00:03:31,440 submit their proposed science program 73 00:03:34,710 --> 00:03:33,760 as with any major observatory the demand 74 00:03:37,270 --> 00:03:34,720 for the telescope 75 00:03:37,830 --> 00:03:37,280 exceeds the time available we expect to 76 00:03:40,149 --> 00:03:37,840 receive 77 00:03:42,550 --> 00:03:40,159 over a thousand proposals a year and 78 00:03:44,630 --> 00:03:42,560 only 200 can be conducted 79 00:03:46,470 --> 00:03:44,640 a committee of international astronomers 80 00:03:48,390 --> 00:03:46,480 selects the proposals based on their 81 00:03:51,350 --> 00:03:48,400 scientific merit 82 00:03:53,270 --> 00:03:51,360 because the hst offers several hundred 83 00:03:55,190 --> 00:03:53,280 instrument configurations 84 00:03:58,710 --> 00:03:55,200 our scientists work with the selected 85 00:04:01,270 --> 00:03:58,720 researchers to detail their observations 86 00:04:02,309 --> 00:04:01,280 next numerous proposals are incorporated 87 00:04:04,390 --> 00:04:02,319 into a week-long 88 00:04:07,350 --> 00:04:04,400 observing schedule that ensures the 89 00:04:09,110 --> 00:04:07,360 efficient use of every telescope minute 90 00:04:10,789 --> 00:04:09,120 there are many many factors involved in 91 00:04:11,990 --> 00:04:10,799 scheduling observations with the space 92 00:04:13,429 --> 00:04:12,000 telescope 93 00:04:15,589 --> 00:04:13,439 there are many instruments onboard a 94 00:04:16,150 --> 00:04:15,599 space telescope within the same 95 00:04:18,710 --> 00:04:16,160 instrument 96 00:04:19,749 --> 00:04:18,720 there are several observing modes even 97 00:04:22,550 --> 00:04:19,759 the simplest 98 00:04:24,310 --> 00:04:22,560 observation requires using different 99 00:04:26,790 --> 00:04:24,320 filters 100 00:04:29,110 --> 00:04:26,800 we may also have to revisit the same 101 00:04:31,430 --> 00:04:29,120 target at different times of the year 102 00:04:34,070 --> 00:04:31,440 we want to maximize the time spent 103 00:04:35,990 --> 00:04:34,080 observing with the space telescope 104 00:04:37,430 --> 00:04:36,000 and minimize the time wasted moving the 105 00:04:39,749 --> 00:04:37,440 telescope around 106 00:04:42,710 --> 00:04:39,759 therefore we will group the observations 107 00:04:45,350 --> 00:04:42,720 to happen in the same area of the sky 108 00:04:45,909 --> 00:04:45,360 we also want to use the same instrument 109 00:04:47,749 --> 00:04:45,919 for 110 00:04:49,430 --> 00:04:47,759 long periods of time even weeks at a 111 00:04:50,870 --> 00:04:49,440 time to minimize 112 00:04:54,550 --> 00:04:50,880 switching instruments on and off 113 00:04:58,629 --> 00:04:56,469 before the telescope schedule can be 114 00:04:59,430 --> 00:04:58,639 completed another essential factor is 115 00:05:03,110 --> 00:04:59,440 entered 116 00:05:04,310 --> 00:05:03,120 the guide stars to establish guide stars 117 00:05:06,710 --> 00:05:04,320 for operations 118 00:05:08,870 --> 00:05:06,720 the institute has converted 1500 119 00:05:12,710 --> 00:05:08,880 photographic plates of the sky 120 00:05:14,550 --> 00:05:12,720 into a catalog of 15 million stars 121 00:05:15,909 --> 00:05:14,560 using the catalog the institute's 122 00:05:19,270 --> 00:05:15,919 computer selects 123 00:05:21,510 --> 00:05:19,280 guide stars for each target hst 124 00:05:22,710 --> 00:05:21,520 stabilizes on a target by finding and 125 00:05:24,950 --> 00:05:22,720 locking onto 126 00:05:26,790 --> 00:05:24,960 two guide stars with its precision 127 00:05:29,110 --> 00:05:26,800 guidance sensors 128 00:05:30,390 --> 00:05:29,120 the sensors detect any minor drift from 129 00:05:32,550 --> 00:05:30,400 the guide stars 130 00:05:34,469 --> 00:05:32,560 and correct the spacecraft's position 131 00:05:36,550 --> 00:05:34,479 through the onboard computers 132 00:05:38,070 --> 00:05:36,560 with the guide stars and other system 133 00:05:40,230 --> 00:05:38,080 factors incorporated 134 00:05:42,390 --> 00:05:40,240 the institute produces a week-long 135 00:05:45,270 --> 00:05:42,400 schedule which specifies 136 00:05:52,629 --> 00:05:45,280 when where and how hst science 137 00:05:54,550 --> 00:05:52,639 instruments will be used 138 00:05:56,070 --> 00:05:54,560 from the institute the science schedule 139 00:05:59,270 --> 00:05:56,080 is transmitted to the space 140 00:06:01,350 --> 00:05:59,280 telescope operations control center 141 00:06:03,110 --> 00:06:01,360 located at goddard space flight center 142 00:06:05,749 --> 00:06:03,120 in greenbelt maryland 143 00:06:07,029 --> 00:06:05,759 this is the nerve center of hst's ground 144 00:06:09,189 --> 00:06:07,039 system 145 00:06:11,029 --> 00:06:09,199 the science schedule automatically goes 146 00:06:11,830 --> 00:06:11,039 into one of the control center computer 147 00:06:13,909 --> 00:06:11,840 systems 148 00:06:16,710 --> 00:06:13,919 which adds commands for operating and 149 00:06:18,950 --> 00:06:16,720 maintaining the observatory 150 00:06:20,710 --> 00:06:18,960 these new commands cover such operations 151 00:06:24,309 --> 00:06:20,720 as moving the telescope 152 00:06:26,550 --> 00:06:24,319 or pointing its communications antennas 153 00:06:29,830 --> 00:06:26,560 the system also schedules links to 154 00:06:32,230 --> 00:06:29,840 nasa's communications satellites 155 00:06:32,950 --> 00:06:32,240 merging both the science and spacecraft 156 00:06:35,270 --> 00:06:32,960 commands 157 00:06:36,390 --> 00:06:35,280 the computer generates a master schedule 158 00:06:38,070 --> 00:06:36,400 for the week 159 00:06:39,990 --> 00:06:38,080 if this second by second schedule 160 00:06:41,990 --> 00:06:40,000 printed out the stack would be one to 161 00:06:44,790 --> 00:06:42,000 two feet high 162 00:06:45,749 --> 00:06:44,800 commands are sent to hst's two on-board 163 00:06:47,909 --> 00:06:45,759 computers 164 00:06:50,790 --> 00:06:47,919 which on an average day carry out over 165 00:06:52,790 --> 00:06:50,800 12 000 commands 166 00:06:57,510 --> 00:06:52,800 the spacecraft's safety is also 167 00:07:02,870 --> 00:07:00,070 a typical satellite has about a thousand 168 00:07:06,230 --> 00:07:02,880 parameters that must be monitored 169 00:07:08,150 --> 00:07:06,240 hst has about six thousand 170 00:07:09,589 --> 00:07:08,160 these parameters include specific 171 00:07:12,150 --> 00:07:09,599 spacecraft temperatures 172 00:07:14,629 --> 00:07:12,160 voltages electrical currents and the 173 00:07:17,029 --> 00:07:14,639 condition of its computers 174 00:07:18,790 --> 00:07:17,039 our engineers must instantly recognize 175 00:07:20,309 --> 00:07:18,800 the codes for each function 176 00:07:23,430 --> 00:07:20,319 interpret their measurements and take 177 00:07:25,430 --> 00:07:23,440 immediate action if something is unusual 178 00:07:27,350 --> 00:07:25,440 because the engineers are overrun with 179 00:07:29,270 --> 00:07:27,360 data we became concerned about the 180 00:07:31,110 --> 00:07:29,280 potential for human error 181 00:07:32,790 --> 00:07:31,120 to minimize this possibility we are 182 00:07:33,430 --> 00:07:32,800 developing an artificial intelligence 183 00:07:37,029 --> 00:07:33,440 system 184 00:07:39,350 --> 00:07:37,039 that automates much of the analysis 185 00:07:40,870 --> 00:07:39,360 if the system finds something amiss it 186 00:07:43,350 --> 00:07:40,880 tells the operator 187 00:07:44,309 --> 00:07:43,360 eventually it will also prescribe a 188 00:07:48,150 --> 00:07:44,319 solution 189 00:07:53,189 --> 00:07:50,710 before the actual observations begin 190 00:07:54,070 --> 00:07:53,199 nasa must calibrate hst's various 191 00:07:56,150 --> 00:07:54,080 systems 192 00:07:59,110 --> 00:07:56,160 during a crucial seven-month period 193 00:08:01,589 --> 00:07:59,120 following launch marshall space flight 194 00:08:04,629 --> 00:08:01,599 center located in huntsville alabama 195 00:08:06,390 --> 00:08:04,639 was responsible for building hst 196 00:08:07,990 --> 00:08:06,400 early in the calibration process 197 00:08:09,749 --> 00:08:08,000 marshall personnel managed the 198 00:08:12,950 --> 00:08:09,759 spacecraft's initial checkout 199 00:08:14,469 --> 00:08:12,960 from goddard's control center 200 00:08:16,150 --> 00:08:14,479 at the beginning of deployment the 201 00:08:19,189 --> 00:08:16,160 shuttle bay doors open 202 00:08:21,270 --> 00:08:19,199 and the arbiter applies power to hst 203 00:08:23,270 --> 00:08:21,280 communication is then established 204 00:08:25,909 --> 00:08:23,280 between the ground control center 205 00:08:26,950 --> 00:08:25,919 and the spacecraft to verify proper 206 00:08:29,029 --> 00:08:26,960 configuration 207 00:08:31,350 --> 00:08:29,039 and to activate basic systems for 208 00:08:34,230 --> 00:08:31,360 thermal safety 209 00:08:35,029 --> 00:08:34,240 next the arbiter's arm lifts hst out of 210 00:08:36,949 --> 00:08:35,039 the bay 211 00:08:39,269 --> 00:08:36,959 so the telescope's solar arrays and 212 00:08:41,350 --> 00:08:39,279 antennas can be extended 213 00:08:44,790 --> 00:08:41,360 the arm releases the observatory into 214 00:08:47,910 --> 00:08:44,800 orbit some 300 miles above the earth 215 00:08:49,670 --> 00:08:47,920 hst's solar arrays are oriented properly 216 00:08:53,190 --> 00:08:49,680 to convert the sun's energy into 217 00:08:55,430 --> 00:08:53,200 electrical power for the observatory 218 00:08:56,870 --> 00:08:55,440 the arbiter stays nearby for about two 219 00:08:59,430 --> 00:08:56,880 days after release 220 00:09:02,230 --> 00:08:59,440 in case hst needs further assistance 221 00:09:04,070 --> 00:09:02,240 during this early critical period 222 00:09:05,750 --> 00:09:04,080 once we establish that the spacecraft 223 00:09:08,949 --> 00:09:05,760 can operate on its own 224 00:09:10,949 --> 00:09:08,959 the arbiter returns to earth meanwhile 225 00:09:11,590 --> 00:09:10,959 ground control engineers continue to 226 00:09:14,070 --> 00:09:11,600 verify 227 00:09:15,750 --> 00:09:14,080 that major components are up and running 228 00:09:17,750 --> 00:09:15,760 and that the telescope is pointing 229 00:09:19,430 --> 00:09:17,760 properly 230 00:09:21,110 --> 00:09:19,440 next through a long series of 231 00:09:23,350 --> 00:09:21,120 calibrations the telescope 232 00:09:25,829 --> 00:09:23,360 mirrors star trackers fine guidance 233 00:09:27,829 --> 00:09:25,839 sensors and rate gyros are aligned 234 00:09:30,070 --> 00:09:27,839 at approximately the end of the first 235 00:09:32,630 --> 00:09:30,080 month marshall officially turns 236 00:09:34,310 --> 00:09:32,640 responsibility for hst operations over 237 00:09:36,310 --> 00:09:34,320 to goddard 238 00:09:38,230 --> 00:09:36,320 during the second month goddard conducts 239 00:09:39,750 --> 00:09:38,240 further telescope calibrations 240 00:09:41,269 --> 00:09:39,760 and early checkout of the science 241 00:09:43,030 --> 00:09:41,279 instruments 242 00:09:44,550 --> 00:09:43,040 subsequent checkout of the optics and 243 00:09:46,790 --> 00:09:44,560 the instruments occurs during the 244 00:09:48,550 --> 00:09:46,800 remaining five months 245 00:09:59,670 --> 00:09:48,560 only then can the long-awaited 246 00:10:02,790 --> 00:10:02,150 to make these observations hst's 247 00:10:05,030 --> 00:10:02,800 commands 248 00:10:07,190 --> 00:10:05,040 must travel an intricate path the 249 00:10:08,150 --> 00:10:07,200 science commands from the institute are 250 00:10:10,710 --> 00:10:08,160 integrated with 251 00:10:11,990 --> 00:10:10,720 spacecraft commands at goddard's control 252 00:10:14,470 --> 00:10:12,000 center 253 00:10:15,190 --> 00:10:14,480 ultimately the signals are relayed to a 254 00:10:17,750 --> 00:10:15,200 nasa 255 00:10:20,870 --> 00:10:17,760 tracking and data relay satellite 256 00:10:23,509 --> 00:10:20,880 orbiting 23 000 miles above earth 257 00:10:25,750 --> 00:10:23,519 the commands then go into hst's onboard 258 00:10:28,389 --> 00:10:25,760 computers to be implemented 259 00:10:31,670 --> 00:10:28,399 this path reverses when data gathered by 260 00:10:33,670 --> 00:10:31,680 an observation is sent back to earth 261 00:10:35,509 --> 00:10:33,680 with commands loaded into its computers 262 00:10:36,949 --> 00:10:35,519 the telescope automatically proceeds 263 00:10:39,750 --> 00:10:36,959 with observations 264 00:10:41,509 --> 00:10:39,760 in this case hst pivots slowly to its 265 00:10:43,110 --> 00:10:41,519 new target 266 00:10:45,670 --> 00:10:43,120 light from the target goes down the 267 00:10:48,550 --> 00:10:45,680 telescope and hits the primary mirror 268 00:10:50,710 --> 00:10:48,560 it reflects back to the secondary mirror 269 00:10:52,630 --> 00:10:50,720 reduced to a narrow beam the light is 270 00:10:54,150 --> 00:10:52,640 aimed back to the focal plane just 271 00:10:56,630 --> 00:10:54,160 behind it 272 00:10:57,990 --> 00:10:56,640 the image is directed to hst's fine 273 00:11:00,550 --> 00:10:58,000 guidance sensors 274 00:11:03,110 --> 00:11:00,560 which locate and lock onto guide stars 275 00:11:05,829 --> 00:11:03,120 on either side of the target 276 00:11:07,509 --> 00:11:05,839 with hst now centered on its target the 277 00:11:08,710 --> 00:11:07,519 light travels into the science 278 00:11:10,870 --> 00:11:08,720 instruments which will make the 279 00:11:13,990 --> 00:11:10,880 observation 280 00:11:17,670 --> 00:11:14,000 the instrument shutters open the correct 281 00:11:21,430 --> 00:11:17,680 filter is selected and hst begins its 282 00:11:26,470 --> 00:11:23,910 while most observations are pre-planned 283 00:11:30,150 --> 00:11:26,480 10 percent require real-time interaction 284 00:11:32,310 --> 00:11:30,160 at the institute by scientists 285 00:11:34,630 --> 00:11:32,320 real-time observations with the space 286 00:11:37,350 --> 00:11:34,640 telescope defy pre-programming 287 00:11:37,829 --> 00:11:37,360 for example we want to observe the red 288 00:11:40,389 --> 00:11:37,839 spots 289 00:11:43,269 --> 00:11:40,399 on jupiter this is a complicated 290 00:11:46,230 --> 00:11:43,279 operation because the planet moves 291 00:11:47,829 --> 00:11:46,240 and it also rotates in order to be able 292 00:11:49,190 --> 00:11:47,839 to do this we have to take an early 293 00:11:52,150 --> 00:11:49,200 picture of the planet 294 00:11:52,550 --> 00:11:52,160 send information down to the ground and 295 00:11:54,870 --> 00:11:52,560 then 296 00:11:56,710 --> 00:11:54,880 have an operator make a very quick 297 00:11:59,269 --> 00:11:56,720 decision as to exactly 298 00:12:00,790 --> 00:11:59,279 where the instrument that is being used 299 00:12:02,389 --> 00:12:00,800 has to be pointed 300 00:12:04,389 --> 00:12:02,399 this is a very challenging operation 301 00:12:06,710 --> 00:12:04,399 indeed 302 00:12:08,470 --> 00:12:06,720 within 24 hours of an observation the 303 00:12:10,069 --> 00:12:08,480 observer can obtain the data from the 304 00:12:13,110 --> 00:12:10,079 science institute's data 305 00:12:15,350 --> 00:12:13,120 archive and distribution service the 306 00:12:17,509 --> 00:12:15,360 investigator who submitted the proposal 307 00:12:19,269 --> 00:12:17,519 has exclusive rights to this information 308 00:12:21,590 --> 00:12:19,279 for one year 309 00:12:24,310 --> 00:12:21,600 after this period the data is available 310 00:12:26,069 --> 00:12:24,320 to scientists around the world serving 311 00:12:27,670 --> 00:12:26,079 as an hst library 312 00:12:30,310 --> 00:12:27,680 the archive will distribute an 313 00:12:31,110 --> 00:12:30,320 equivalent of 500 million pages of 314 00:12:34,150 --> 00:12:31,120 information 315 00:12:35,670 --> 00:12:34,160 over a single year the observations are 316 00:12:38,310 --> 00:12:35,680 distributed through worldwide 317 00:12:42,870 --> 00:12:38,320 astronomical computer networks 318 00:12:45,829 --> 00:12:42,880 are through optical disks magnetic tapes 319 00:12:48,150 --> 00:12:45,839 and photographs astronomers can use this 320 00:12:52,949 --> 00:12:48,160 information at their home institution 321 00:12:55,110 --> 00:12:52,959 to further their own research 322 00:12:56,710 --> 00:12:55,120 from this data who can say what great 323 00:12:59,030 --> 00:12:56,720 discoveries will be made 324 00:13:00,230 --> 00:12:59,040 astronomers hope for answers about black 325 00:13:02,870 --> 00:13:00,240 holes 326 00:13:04,389 --> 00:13:02,880 the evolution of galaxies and the size 327 00:13:06,230 --> 00:13:04,399 of our universe 328 00:13:08,870 --> 00:13:06,240 looking to the future to ensure the 329 00:13:12,389 --> 00:13:08,880 continuous flow of such exciting data 330 00:13:14,790 --> 00:13:12,399 nasa has created contingency plans 331 00:13:17,190 --> 00:13:14,800 in contrast to the unexpected repair of 332 00:13:18,629 --> 00:13:17,200 the solar maximum mission spacecraft in 333 00:13:21,430 --> 00:13:18,639 1984 334 00:13:24,470 --> 00:13:21,440 nasa has prepared for hst's on orbit 335 00:13:30,150 --> 00:13:26,870 hst is designed and developed by nasa 336 00:13:32,790 --> 00:13:30,160 for on-orbit servicing by astronauts 337 00:13:37,670 --> 00:13:32,800 consequently hst instruments and various 338 00:13:41,590 --> 00:13:39,269 this allows the astronauts to replace 339 00:13:44,150 --> 00:13:41,600 degradable parts such as solar arrays 340 00:13:45,829 --> 00:13:44,160 and batteries during routine servicing 341 00:13:47,750 --> 00:13:45,839 missions 342 00:13:49,990 --> 00:13:47,760 the modular design also makes it 343 00:13:51,990 --> 00:13:50,000 possible to update the observatory with 344 00:13:54,069 --> 00:13:52,000 new instruments 345 00:13:55,829 --> 00:13:54,079 during the first planned maintenance 346 00:13:57,910 --> 00:13:55,839 mission for the hst 347 00:13:59,829 --> 00:13:57,920 we expect to remove one of the original 348 00:14:02,389 --> 00:13:59,839 scientific instruments and replace it 349 00:14:04,150 --> 00:14:02,399 with a near-infrared instrument 350 00:14:07,269 --> 00:14:04,160 the first scientific instruments on the 351 00:14:08,949 --> 00:14:07,279 hst are sensitive to the ultraviolet 352 00:14:10,710 --> 00:14:08,959 and visible portions of the 353 00:14:13,670 --> 00:14:10,720 electromagnetic spectrum 354 00:14:15,750 --> 00:14:13,680 when we add an infrared capability we 355 00:14:16,550 --> 00:14:15,760 will be able to examine regions such as 356 00:14:18,150 --> 00:14:16,560 this 357 00:14:19,750 --> 00:14:18,160 where stars are in the process of 358 00:14:21,750 --> 00:14:19,760 formation today 359 00:14:22,790 --> 00:14:21,760 and we'll also be able to probe still 360 00:14:33,910 --> 00:14:22,800 further back 361 00:14:38,470 --> 00:14:36,310 hubble space telescope operations can be 362 00:14:40,710 --> 00:14:38,480 compared to the complexity and challenge 363 00:14:43,990 --> 00:14:40,720 of the operations necessary to send 364 00:14:46,069 --> 00:14:44,000 astronauts to the moon the expertise of 365 00:14:47,509 --> 00:14:46,079 thousands of individuals has contributed 366 00:14:50,790 --> 00:14:47,519 to the innovative 367 00:14:53,030 --> 00:14:50,800 science instruments computer systems 368 00:14:55,269 --> 00:14:53,040 information systems and maintenance 369 00:14:57,509 --> 00:14:55,279 hardware that constitute hst's 370 00:14:59,670 --> 00:14:57,519 operations network 371 00:15:01,030 --> 00:14:59,680 this elaborate system supporting hubble 372 00:15:02,949 --> 00:15:01,040 space telescope 373 00:15:04,470 --> 00:15:02,959 promises long-sought answers to 374 00:15:07,030 --> 00:15:04,480 universal questions 375 00:15:07,990 --> 00:15:07,040 exciting discoveries to ponder and