1 00:00:03,909 --> 00:00:02,070 ever since we've been pointing 2 00:00:05,590 --> 00:00:03,919 spacecraft at the sun 3 00:00:08,310 --> 00:00:05,600 two regions on our star have been 4 00:00:10,310 --> 00:00:08,320 missing from satellite images 5 00:00:12,549 --> 00:00:10,320 the sun's two poles have never been 6 00:00:14,150 --> 00:00:12,559 mapped because all the solar images 7 00:00:15,589 --> 00:00:14,160 we've built have remained in the 8 00:00:17,750 --> 00:00:15,599 ecliptic plane 9 00:00:19,830 --> 00:00:17,760 the swath of space roughly aligned with 10 00:00:21,109 --> 00:00:19,840 the sun's equator where all the planets 11 00:00:23,269 --> 00:00:21,119 orbit 12 00:00:25,990 --> 00:00:23,279 a new mission from the european space 13 00:00:27,990 --> 00:00:26,000 agency and nasa called solar orbiter 14 00:00:31,269 --> 00:00:28,000 aims to escape this plane and take the 15 00:00:33,270 --> 00:00:31,279 very first images of the poles 16 00:00:34,790 --> 00:00:33,280 the planets are all moving and circling 17 00:00:37,110 --> 00:00:34,800 the sun and so we already have some 18 00:00:38,869 --> 00:00:37,120 velocity going one way if we want to 19 00:00:40,549 --> 00:00:38,879 launch up out of the ecliptic it 20 00:00:43,270 --> 00:00:40,559 requires more energy 21 00:00:45,990 --> 00:00:43,280 to get outside the ecliptic plane solar 22 00:00:47,990 --> 00:00:46,000 orbiter uses earth's and venus's gravity 23 00:00:49,110 --> 00:00:48,000 to slingshot itself into a view of the 24 00:00:51,029 --> 00:00:49,120 poles 25 00:00:53,990 --> 00:00:51,039 the only other satellite to fly over the 26 00:00:56,150 --> 00:00:54,000 poles was ulysses which launched in 1990 27 00:00:58,150 --> 00:00:56,160 to study the solar atmosphere 28 00:01:00,549 --> 00:00:58,160 but solar orbiter will be the first 29 00:01:02,950 --> 00:01:00,559 mission to capture actual images of this 30 00:01:04,549 --> 00:01:02,960 hard to reach region 31 00:01:06,230 --> 00:01:04,559 scientists think the poles could be the 32 00:01:09,109 --> 00:01:06,240 missing piece to understanding what 33 00:01:11,830 --> 00:01:09,119 drives the sun's activity 34 00:01:15,270 --> 00:01:11,840 every 11 years the sun's magnetic field 35 00:01:17,749 --> 00:01:15,280 flips north becomes south and vice versa 36 00:01:20,469 --> 00:01:17,759 this mysterious process has direct 37 00:01:22,950 --> 00:01:20,479 effects on earth before the poles flip 38 00:01:25,109 --> 00:01:22,960 solar activity reaches its peak the 39 00:01:27,270 --> 00:01:25,119 number of eruptions increases sending 40 00:01:29,510 --> 00:01:27,280 powerful bursts of solar material that 41 00:01:32,630 --> 00:01:29,520 can potentially harm our astronauts and 42 00:01:35,350 --> 00:01:32,640 satellites we don't really have a good 43 00:01:37,590 --> 00:01:35,360 understanding of the global solar 44 00:01:40,149 --> 00:01:37,600 behavior another one of the missions 45 00:01:43,670 --> 00:01:40,159 goals is to monitor how these eruptions 46 00:01:46,469 --> 00:01:43,680 and solar material travel through space 47 00:01:48,550 --> 00:01:46,479 using a suite of 10 instruments solar 48 00:01:51,270 --> 00:01:48,560 orbiter observes an active region on the 49 00:01:52,950 --> 00:01:51,280 surface as it explodes and then also 50 00:01:54,710 --> 00:01:52,960 takes measurements as the escaping 51 00:01:56,149 --> 00:01:54,720 material passes directly by the 52 00:01:58,550 --> 00:01:56,159 spacecraft 53 00:02:01,429 --> 00:01:58,560 solar orbiter will give us a 54 00:02:02,310 --> 00:02:01,439 comprehensive full view of the entire 55 00:02:06,709 --> 00:02:02,320 sun 56 00:02:09,029 --> 00:02:06,719 the entire solar system at closest 57 00:02:11,589 --> 00:02:09,039 approach solar orbiter will be closer to 58 00:02:13,990 --> 00:02:11,599 the sun than mercury at a mere distance 59 00:02:15,589 --> 00:02:14,000 of 26 million miles away 60 00:02:17,750 --> 00:02:15,599 the ideal distance to get a 61 00:02:19,350 --> 00:02:17,760 comprehensive view of the sun and its 62 00:02:21,350 --> 00:02:19,360 surrounding atmosphere 63 00:02:23,190 --> 00:02:21,360 it will fly close to the sun every six 64 00:02:25,190 --> 00:02:23,200 months and endure temperatures more than 65 00:02:27,670 --> 00:02:25,200 900 degrees fahrenheit 66 00:02:30,150 --> 00:02:27,680 to survive the intense radiation a large 67 00:02:32,470 --> 00:02:30,160 titanium shield protects the instruments 68 00:02:34,150 --> 00:02:32,480 while a carefully orchestrated dance of 69 00:02:36,309 --> 00:02:34,160 opening and closing eye holes in the 70 00:02:37,910 --> 00:02:36,319 shield allows the instruments to peep 71 00:02:39,750 --> 00:02:37,920 out at the right time 72 00:02:42,229 --> 00:02:39,760 other instruments will directly measure 73 00:02:43,350 --> 00:02:42,239 solar material from behind the shadow of 74 00:02:45,430 --> 00:02:43,360 the shield 75 00:02:47,509 --> 00:02:45,440 all of these observations will tell us 76 00:02:48,550 --> 00:02:47,519 more about the sun than we've ever known 77 00:02:51,190 --> 00:02:48,560 before 78 00:02:52,949 --> 00:02:51,200 and by the end of the seven year mission 79 00:02:55,030 --> 00:02:52,959 we will have seen our star in a 80 00:02:58,710 --> 00:02:55,040 completely new way 81 00:03:00,070 --> 00:02:58,720 our understanding of the sun will change 82 00:03:02,630 --> 00:03:00,080 dramatically