1 00:00:08,030 --> 00:00:05,930 when it comes to learning about stars 2 00:00:11,900 --> 00:00:08,040 there is no closer classroom than our 3 00:00:13,970 --> 00:00:11,910 Sun that's why NASA began an in-depth 4 00:00:16,570 --> 00:00:13,980 study of the Sun and Earth relationship 5 00:00:19,040 --> 00:00:16,580 in a program dubbed living with a star 6 00:00:20,840 --> 00:00:19,050 the first mission in the space weather 7 00:00:24,019 --> 00:00:20,850 program is the Solar Dynamics 8 00:00:25,910 --> 00:00:24,029 Observatory or sdo scheduled to launch 9 00:00:35,270 --> 00:00:25,920 from Cape Canaveral Air Force Station in 10 00:00:39,170 --> 00:00:35,280 Florida welcome to the Solar Dynamics 11 00:00:41,840 --> 00:00:39,180 Observatory webcast I'm Tiffany now with 12 00:00:44,600 --> 00:00:41,850 NASA's launch services program in the 13 00:00:48,020 --> 00:00:44,610 next few minutes we'll tell you what sdo 14 00:00:50,750 --> 00:00:48,030 might uncover about the Sun and how all 15 00:00:53,779 --> 00:00:50,760 of us on earth can benefit from finding 16 00:00:57,380 --> 00:00:53,789 out more about that bright orange disk 17 00:01:00,080 --> 00:00:57,390 in the sky but sto is not NASA's first 18 00:01:02,500 --> 00:01:00,090 mission to study the Sun several of 19 00:01:05,630 --> 00:01:02,510 NASA's past missions focused on the Sun 20 00:01:08,300 --> 00:01:05,640 pioneer 5 was the first it launched in 21 00:01:11,090 --> 00:01:08,310 1960 with instruments to study the solar 22 00:01:12,890 --> 00:01:11,100 wind and other phenomena the instruments 23 00:01:15,590 --> 00:01:12,900 are primitive by today's standards but 24 00:01:19,880 --> 00:01:15,600 back then pioneer gave researchers their 25 00:01:22,399 --> 00:01:19,890 first up-close look at a star in 1973 26 00:01:25,130 --> 00:01:22,409 NASA made observing the Sun a central 27 00:01:27,170 --> 00:01:25,140 goal of the skylab space station the 28 00:01:28,969 --> 00:01:27,180 agency's first space station included a 29 00:01:31,429 --> 00:01:28,979 telescope designed to look closely at 30 00:01:33,170 --> 00:01:31,439 the Sun astronauts living on the station 31 00:01:36,469 --> 00:01:33,180 spent hours making specialized 32 00:01:39,289 --> 00:01:36,479 observations what they found on Skylab 33 00:01:41,359 --> 00:01:39,299 with what we call coronal holes and we 34 00:01:43,789 --> 00:01:41,369 did not know about coronal holes until 35 00:01:46,160 --> 00:01:43,799 they started taking these images I would 36 00:01:50,330 --> 00:01:46,170 say thats Skylab coming out with that 37 00:01:53,149 --> 00:01:50,340 type of photography was one of its most 38 00:01:54,950 --> 00:01:53,159 important things SDO is cutting edge 39 00:01:57,499 --> 00:01:54,960 instruments offer researchers an 40 00:01:59,600 --> 00:01:57,509 unprecedented opportunity to examine the 41 00:02:02,330 --> 00:01:59,610 star at the center of our solar system 42 00:02:04,370 --> 00:02:02,340 in fact the readings are expected to be 43 00:02:06,980 --> 00:02:04,380 precise enough for researchers to 44 00:02:09,770 --> 00:02:06,990 forecast solar weather and predict when 45 00:02:11,900 --> 00:02:09,780 satellites in space and even electronics 46 00:02:16,370 --> 00:02:11,910 on earth will be endangered by a store 47 00:02:19,070 --> 00:02:16,380 on the Sun we had 15 years of fairly 48 00:02:21,680 --> 00:02:19,080 constant industry and we've taken that 49 00:02:24,950 --> 00:02:21,690 data and designed us do to improve the 50 00:02:27,980 --> 00:02:24,960 ability to do science and to the ability 51 00:02:29,990 --> 00:02:27,990 to predict space weather we measure not 52 00:02:32,900 --> 00:02:30,000 just a strength of the magnetic field we 53 00:02:35,360 --> 00:02:32,910 measure also its direction and we think 54 00:02:37,880 --> 00:02:35,370 that the how much the magnetic field 55 00:02:40,550 --> 00:02:37,890 direction changes over a small part of 56 00:02:42,500 --> 00:02:40,560 the Sun is probably related to whether 57 00:02:44,990 --> 00:02:42,510 or not space weather things are going to 58 00:02:47,600 --> 00:02:45,000 happen solar flares can cause power 59 00:02:49,520 --> 00:02:47,610 surges on earth and wreak havoc on space 60 00:02:52,310 --> 00:02:49,530 stations and satellites orbiting the 61 00:02:54,110 --> 00:02:52,320 planet so researchers want to find out 62 00:02:56,330 --> 00:02:54,120 what makes solar flares and other 63 00:02:58,580 --> 00:02:56,340 turbulent events occur on the Sun and 64 00:03:00,620 --> 00:02:58,590 then find out if there's a pattern or 65 00:03:04,310 --> 00:03:00,630 signs that we could use on earth to 66 00:03:07,010 --> 00:03:04,320 predict future flares sto will look at 67 00:03:09,680 --> 00:03:07,020 the Sun and try to understand where the 68 00:03:11,690 --> 00:03:09,690 magnetic field comes from when we talk 69 00:03:14,690 --> 00:03:11,700 about flares and coronal mass ejections 70 00:03:17,120 --> 00:03:14,700 that's the Sun getting rid of stuff that 71 00:03:19,370 --> 00:03:17,130 magnetic field is no longer in the Sun 72 00:03:22,270 --> 00:03:19,380 it wants it gone and it gets rid of the 73 00:03:25,430 --> 00:03:22,280 energy by having magnetic flares that 74 00:03:27,350 --> 00:03:25,440 release bright flashes of light and it 75 00:03:29,600 --> 00:03:27,360 gets rid of the leftover magnetic field 76 00:03:31,580 --> 00:03:29,610 by just throwing it off the spacecraft 77 00:03:33,470 --> 00:03:31,590 will use three instruments to examine 78 00:03:35,600 --> 00:03:33,480 the Sun including one that will take 79 00:03:38,060 --> 00:03:35,610 pictures rivaling the resolution of an 80 00:03:41,210 --> 00:03:38,070 IMAX movie another instrument called the 81 00:03:43,580 --> 00:03:41,220 helioseismic and magnetic imager or hm I 82 00:03:45,860 --> 00:03:43,590 will measure the sound waves bouncing 83 00:03:48,260 --> 00:03:45,870 around inside the Sun to construct an 84 00:03:50,420 --> 00:03:48,270 image of the stars inner workings the 85 00:03:53,150 --> 00:03:50,430 data could reveal why the Sun operates 86 00:03:55,160 --> 00:03:53,160 in an 11-year cycle of activity the 87 00:03:57,080 --> 00:03:55,170 extreme ultraviolet variability 88 00:03:59,030 --> 00:03:57,090 experiment will monitor the sun's 89 00:04:01,729 --> 00:03:59,040 brightness in the extreme ultraviolet 90 00:04:04,699 --> 00:04:01,739 wavelength which changes constantly are 91 00:04:07,430 --> 00:04:04,709 three instruments on here are really new 92 00:04:09,979 --> 00:04:07,440 and improved versions of some other 93 00:04:12,020 --> 00:04:09,989 instruments that have flown and of 94 00:04:14,540 --> 00:04:12,030 course we have a lot more data and we 95 00:04:16,039 --> 00:04:14,550 take a lot more pictures so then that's 96 00:04:18,110 --> 00:04:16,049 one thing the scientist love because as 97 00:04:19,310 --> 00:04:18,120 they say the Sun changes time it changes 98 00:04:21,860 --> 00:04:19,320 every second and we're going to be 99 00:04:24,920 --> 00:04:21,870 imaging it every second and we image the 100 00:04:26,120 --> 00:04:24,930 full disk of the Sun taken together the 101 00:04:28,100 --> 00:04:26,130 information s do 102 00:04:30,050 --> 00:04:28,110 collects could give scientists ways to 103 00:04:32,570 --> 00:04:30,060 predict future solar disturbances and 104 00:04:34,850 --> 00:04:32,580 help developers on earth come up with 105 00:04:37,940 --> 00:04:34,860 ways to protect sensitive electronics in 106 00:04:39,590 --> 00:04:37,950 space and on the planet while the work 107 00:04:41,390 --> 00:04:39,600 from s do is expected to be 108 00:04:42,980 --> 00:04:41,400 groundbreaking it took a lot of 109 00:04:45,440 --> 00:04:42,990 researchers and several previous 110 00:04:47,090 --> 00:04:45,450 missions to show scientist what kind of 111 00:04:49,910 --> 00:04:47,100 instruments they would need to put on 112 00:04:52,100 --> 00:04:49,920 the spacecraft solar studies have relied 113 00:04:53,950 --> 00:04:52,110 on data from a host of missions looking 114 00:04:56,710 --> 00:04:53,960 at the Sun from different perspectives 115 00:04:59,330 --> 00:04:56,720 the solar maximum mission launched in 116 00:05:01,700 --> 00:04:59,340 1982 look at solar flares and other 117 00:05:04,610 --> 00:05:01,710 events the mission was extended by 118 00:05:07,040 --> 00:05:04,620 shuttle astronauts in 1984 who repaired 119 00:05:10,490 --> 00:05:07,050 the spacecraft in orbit solar max 120 00:05:12,680 --> 00:05:10,500 operated until nineteen eighty nine NASA 121 00:05:14,750 --> 00:05:12,690 and the European Space Agency jointly 122 00:05:17,380 --> 00:05:14,760 developed the Ulysses spacecraft which 123 00:05:20,570 --> 00:05:17,390 launched on shuttle discovery in 1990 124 00:05:23,990 --> 00:05:20,580 alessi k researchers unique looks at the 125 00:05:26,360 --> 00:05:24,000 sun's North and South Poles the Solar 126 00:05:30,430 --> 00:05:26,370 and Heliospheric Observatory known as 127 00:05:33,350 --> 00:05:30,440 Soho launched in 1995 aboard an atlas to 128 00:05:36,320 --> 00:05:33,360 sohos observations are similar to those 129 00:05:38,990 --> 00:05:36,330 in vision for s do although s do is 130 00:05:41,840 --> 00:05:39,000 carrying more advanced instruments well 131 00:05:44,450 --> 00:05:41,850 the big challenge of this mission is its 132 00:05:47,810 --> 00:05:44,460 data rate it's a hundred and 50 megabits 133 00:05:51,500 --> 00:05:47,820 per second 24 hours a day it's 134 00:05:53,360 --> 00:05:51,510 relentless most of the astronomical 135 00:05:54,650 --> 00:05:53,370 spacecraft are looking at sort of faint 136 00:05:56,450 --> 00:05:54,660 sources so they don't have that much 137 00:05:59,150 --> 00:05:56,460 like we're looking at the Sun right a 138 00:06:00,740 --> 00:05:59,160 lot of photons come off the Sun and we 139 00:06:03,410 --> 00:06:00,750 gotta process those and get them down to 140 00:06:05,500 --> 00:06:03,420 the ground but before SDO can start its 141 00:06:08,420 --> 00:06:05,510 observations it has to get into space 142 00:06:11,660 --> 00:06:08,430 that's the job of a powerful Atlas 5 143 00:06:13,450 --> 00:06:11,670 rocket the Atlas will lift the 6800 144 00:06:17,210 --> 00:06:13,460 pound spacecraft to an orbit about 145 00:06:19,220 --> 00:06:17,220 22,000 miles above Earth the Atlas 5 is 146 00:06:21,590 --> 00:06:19,230 one of the largest boosters available to 147 00:06:23,270 --> 00:06:21,600 NASA and was used to launch the lunar 148 00:06:26,720 --> 00:06:23,280 reconnaissance orbiter and moon 149 00:06:28,310 --> 00:06:26,730 impacting el crossface craft sto is one 150 00:06:30,680 --> 00:06:28,320 of the largest solar observatories we've 151 00:06:32,690 --> 00:06:30,690 ever launched it had a heavy lift 152 00:06:33,270 --> 00:06:32,700 requirement so we chose the Atlas 5 is 153 00:06:36,930 --> 00:06:33,280 the rocket 154 00:06:39,510 --> 00:06:36,940 this mission the Atlas 5 is unique for 155 00:06:41,670 --> 00:06:39,520 its launch structure Alice fire has been 156 00:06:44,129 --> 00:06:41,680 a very reliable rocket we've used it on 157 00:06:46,530 --> 00:06:44,139 a couple of NASA missions it's unique in 158 00:06:49,140 --> 00:06:46,540 that it's chosen a clean pad concept for 159 00:06:50,640 --> 00:06:49,150 it so launch processing the Rockets 160 00:06:52,680 --> 00:06:50,650 actually built on a mobile launch 161 00:06:54,510 --> 00:06:52,690 platform in the vehicle behind me the 162 00:06:56,250 --> 00:06:54,520 vertical integration facility and then 163 00:06:59,100 --> 00:06:56,260 rolled out with rail cars out to the pad 164 00:07:01,050 --> 00:06:59,110 the day of launch one advantage of this 165 00:07:03,450 --> 00:07:01,060 clean pad concept that they chose is 166 00:07:05,340 --> 00:07:03,460 that the rocket is processed safe and 167 00:07:07,440 --> 00:07:05,350 secure in a building and then it rolls 168 00:07:09,180 --> 00:07:07,450 out the day of launch and that way if 169 00:07:10,409 --> 00:07:09,190 they have a problem a storm or something 170 00:07:12,090 --> 00:07:10,419 like that they can roll back in the 171 00:07:14,520 --> 00:07:12,100 facility it's not exposed to the 172 00:07:15,600 --> 00:07:14,530 elements for very long it just gives 173 00:07:16,980 --> 00:07:15,610 them a lot of flexibility in the 174 00:07:19,680 --> 00:07:16,990 processing a lot of protection for the 175 00:07:21,930 --> 00:07:19,690 rock as well as the spacecraft the day 176 00:07:23,850 --> 00:07:21,940 before launch technicians will roll the 177 00:07:25,950 --> 00:07:23,860 rocket out of his protective service 178 00:07:28,409 --> 00:07:25,960 structure they'll fuel the first stage 179 00:07:31,170 --> 00:07:28,419 and the Centaur upper stage as the Atlas 180 00:07:32,940 --> 00:07:31,180 stands on the pad the spacecraft was 181 00:07:35,490 --> 00:07:32,950 built in Maryland at NASA's Goddard 182 00:07:39,090 --> 00:07:35,500 Space Flight Center and it arrived in 183 00:07:40,830 --> 00:07:39,100 florida in august two thousand nine it 184 00:07:43,320 --> 00:07:40,840 went through a number of comprehensive 185 00:07:46,860 --> 00:07:43,330 tests including deploying the spacecraft 186 00:07:48,930 --> 00:07:46,870 solar arrays technicians install stos 187 00:07:51,000 --> 00:07:48,940 batteries and loaded fuel into the 188 00:07:53,880 --> 00:07:51,010 spacecraft before it was trucked to the 189 00:07:55,409 --> 00:07:53,890 launch complex spacecraft typically 190 00:07:57,630 --> 00:07:55,419 spend several months in launch 191 00:07:59,310 --> 00:07:57,640 integration and testing because the 192 00:08:01,590 --> 00:07:59,320 machines are designed to work in such a 193 00:08:03,659 --> 00:08:01,600 harsh place that technicians and 194 00:08:06,570 --> 00:08:03,669 scientists want to make sure everything 195 00:08:08,790 --> 00:08:06,580 is just right before launch the Sun is 196 00:08:11,250 --> 00:08:08,800 our Astrophysical laboratory this is the 197 00:08:13,260 --> 00:08:11,260 place where we look at the Sun and stop 198 00:08:16,350 --> 00:08:13,270 calling it the Sun when we look at the 199 00:08:17,940 --> 00:08:16,360 Sun it's just an average star when we 200 00:08:20,430 --> 00:08:17,950 look out in the universe and we plot 201 00:08:23,040 --> 00:08:20,440 star stuff up the sun's always right in 202 00:08:26,520 --> 00:08:23,050 the middle it's like the perfect average 203 00:08:28,190 --> 00:08:26,530 star and if our average star has solar 204 00:08:33,350 --> 00:08:28,200 activity 205 00:08:35,270 --> 00:08:33,360 and indeed we do you know we need to 206 00:08:38,930 --> 00:08:35,280 know when a solar event is going to 207 00:08:41,510 --> 00:08:38,940 happen we can save a life a day before 208 00:08:43,700 --> 00:08:41,520 the Solar Dynamics Observatory begins 209 00:08:46,580 --> 00:08:43,710 its mission the excitement is reaching a 210 00:08:49,130 --> 00:08:46,590 crescendo here at NASA's Kennedy Space 211 00:08:50,990 --> 00:08:49,140 Center we hope you've enjoyed this look 212 00:08:53,680 --> 00:08:51,000 at the mission and found out a little 213 00:08:56,240 --> 00:08:53,690 more about our closest star the Sun