1 00:00:08,629 --> 00:00:06,150 just like scientific discoveries happen 2 00:00:10,790 --> 00:00:08,639 every day in today's laboratories so 3 00:00:12,789 --> 00:00:10,800 planetary spacecraft over the last 4 00:00:15,030 --> 00:00:12,799 several decades have made startling 5 00:00:17,269 --> 00:00:15,040 discoveries concerning the solar system 6 00:00:19,349 --> 00:00:17,279 we live in 7 00:00:21,189 --> 00:00:19,359 in the quest for better understanding of 8 00:00:29,349 --> 00:00:21,199 the world and universe 9 00:00:34,229 --> 00:00:31,830 the spectacular achievements of voyager 10 00:00:36,229 --> 00:00:34,239 1 and 2 as they flew past jupiter and 11 00:00:41,350 --> 00:00:36,239 its satellites far exceed the 12 00:00:45,670 --> 00:00:43,910 new discoveries heighten our awareness 13 00:00:47,750 --> 00:00:45,680 raising new questions 14 00:00:50,150 --> 00:00:47,760 what part do earth and its inhabitants 15 00:00:51,750 --> 00:00:50,160 play in this universal scene 16 00:00:53,990 --> 00:00:51,760 how is earth different from other 17 00:00:56,069 --> 00:00:54,000 planets in our solar system 18 00:00:58,630 --> 00:00:56,079 how are we the same 19 00:01:00,630 --> 00:00:58,640 as voyager past jupiter it discovered a 20 00:01:03,670 --> 00:01:00,640 thin ring about the planet 21 00:01:05,910 --> 00:01:03,680 what is its composition 22 00:01:08,310 --> 00:01:05,920 we know there are 16 moons are there 23 00:01:12,710 --> 00:01:10,149 several of the satellites are composed 24 00:01:15,190 --> 00:01:12,720 partially of water ice 25 00:01:17,429 --> 00:01:15,200 one is violently volcanic 26 00:01:19,749 --> 00:01:17,439 how did these bodies form and what is 27 00:01:22,070 --> 00:01:19,759 their history 28 00:01:24,469 --> 00:01:22,080 what can this giant planet tell us about 29 00:01:27,030 --> 00:01:24,479 the history of our solar system 30 00:01:29,190 --> 00:01:27,040 dr torrance johnson project scientist 31 00:01:31,350 --> 00:01:29,200 well jupiter itself of course we believe 32 00:01:33,590 --> 00:01:31,360 to be composed primarily of material 33 00:01:35,670 --> 00:01:33,600 that's very similar and virtually 34 00:01:37,350 --> 00:01:35,680 unchanged uh 35 00:01:39,510 --> 00:01:37,360 in the last four billion years to the 36 00:01:41,830 --> 00:01:39,520 material that formed all of the planets 37 00:01:43,749 --> 00:01:41,840 the fundamental solar nebula if you will 38 00:01:46,069 --> 00:01:43,759 the gas and dust from which all the 39 00:01:47,830 --> 00:01:46,079 planets formed in addition to which the 40 00:01:49,590 --> 00:01:47,840 satellite systems surrounding its 41 00:01:51,270 --> 00:01:49,600 magnetic field 42 00:01:53,429 --> 00:01:51,280 environment make it virtually a 43 00:01:56,069 --> 00:01:53,439 miniature solar system so by studying 44 00:01:58,550 --> 00:01:56,079 this system we can learn a lot about how 45 00:02:01,910 --> 00:01:58,560 the solar system as a whole formed and 46 00:02:04,950 --> 00:02:01,920 something about our own origins 47 00:02:07,109 --> 00:02:04,960 galileo the new generation spacecraft is 48 00:02:13,589 --> 00:02:07,119 designed to spend an extended period of 49 00:02:21,270 --> 00:02:15,910 the spacecraft will release a probe to 50 00:02:26,550 --> 00:02:23,270 the orbiter is then targeted to its 51 00:02:32,070 --> 00:02:26,560 first encounter io a moon known to have 52 00:02:35,750 --> 00:02:33,830 then the orbiter points its relay 53 00:02:45,670 --> 00:02:35,760 antenna toward the probe which begins 54 00:02:50,070 --> 00:02:47,589 once there it will investigate the 55 00:02:52,630 --> 00:02:50,080 composition temperatures and pressures 56 00:02:54,070 --> 00:02:52,640 at varying levels and send data back to 57 00:03:05,350 --> 00:02:54,080 the orbiter 58 00:03:07,990 --> 00:03:05,360 system measuring and observing the giant 59 00:03:10,550 --> 00:03:08,000 magnetic field and plasma as well as the 60 00:03:12,390 --> 00:03:10,560 intense radiation that surrounds jupiter 61 00:03:17,110 --> 00:03:12,400 while performing closer studies of the 62 00:03:21,589 --> 00:03:19,430 the combination of closer encounters and 63 00:03:24,070 --> 00:03:21,599 advanced instrument technologies carried 64 00:03:29,270 --> 00:03:24,080 on board galileo will give much better 65 00:03:33,270 --> 00:03:31,830 specific major advances that we've made 66 00:03:35,350 --> 00:03:33,280 is in the camera system where we're 67 00:03:37,670 --> 00:03:35,360 using the same optical system same 68 00:03:40,149 --> 00:03:37,680 telescope if you will that voyager did 69 00:03:43,270 --> 00:03:40,159 but instead of having a relatively slow 70 00:03:45,670 --> 00:03:43,280 and insensitive vidicon tube 71 00:03:47,589 --> 00:03:45,680 such as was used in tv cameras in the 72 00:03:50,309 --> 00:03:47,599 50s and 60s 73 00:03:52,710 --> 00:03:50,319 instead of that at the focus of the the 74 00:03:55,350 --> 00:03:52,720 telescope we now have a silicon based 75 00:03:57,589 --> 00:03:55,360 device a charged couple device 76 00:04:00,949 --> 00:03:57,599 camera system which gives us a 77 00:04:03,350 --> 00:04:00,959 increase in speed or sensitivity of the 78 00:04:04,710 --> 00:04:03,360 instrument of between 300 and a thousand 79 00:04:06,229 --> 00:04:04,720 times 80 00:04:09,110 --> 00:04:06,239 that allows us to take much higher 81 00:04:11,190 --> 00:04:09,120 resolution pictures much closer 82 00:04:12,789 --> 00:04:11,200 without blurring and it also gives us 83 00:04:14,390 --> 00:04:12,799 access to a little bit of the infrared 84 00:04:16,949 --> 00:04:14,400 part of the spectrum that was totally 85 00:04:18,789 --> 00:04:16,959 inaccessible to the voyager cameras 86 00:04:20,789 --> 00:04:18,799 now in addition to that in the infrared 87 00:04:23,430 --> 00:04:20,799 we have an entirely new device called 88 00:04:25,110 --> 00:04:23,440 the near-infrared mapping spectrometer 89 00:04:27,110 --> 00:04:25,120 which if you will is a little bit like a 90 00:04:28,790 --> 00:04:27,120 landsat type device 91 00:04:31,749 --> 00:04:28,800 giving us images in many different 92 00:04:33,670 --> 00:04:31,759 spectral bands and we'll have about 300 93 00:04:36,469 --> 00:04:33,680 different spectral bands what this means 94 00:04:38,550 --> 00:04:36,479 is we'll have from this device pictures 95 00:04:41,030 --> 00:04:38,560 with relatively modest resolution 96 00:04:43,270 --> 00:04:41,040 spatially but with where each pixel 97 00:04:45,189 --> 00:04:43,280 element within the picture will have a 98 00:04:46,870 --> 00:04:45,199 300 channel spectrum attached we're 99 00:04:49,830 --> 00:04:46,880 going to be using this in both jupiter 100 00:04:51,670 --> 00:04:49,840 and the satellites to map composition on 101 00:04:54,230 --> 00:04:51,680 their surfaces study the characteristics 102 00:04:56,310 --> 00:04:54,240 of jovian clouds find out where ices are 103 00:04:58,070 --> 00:04:56,320 on the surface try to identify the 104 00:05:01,430 --> 00:04:58,080 materials frozen out on the surface of 105 00:05:06,870 --> 00:05:04,150 enroute to jupiter galileo will pick up 106 00:05:09,430 --> 00:05:06,880 energy by utilizing gravity assists 107 00:05:10,710 --> 00:05:09,440 while traveling once by venus and twice 108 00:05:12,710 --> 00:05:10,720 by earth 109 00:05:15,189 --> 00:05:12,720 in addition to the bonus of studying 110 00:05:17,990 --> 00:05:15,199 these two planets and earth's moon 111 00:05:20,390 --> 00:05:18,000 galileo will perform close flybys on one 112 00:05:25,029 --> 00:05:20,400 or two asteroids never before closely 113 00:05:31,990 --> 00:05:26,790 then galileo will rendezvous with 114 00:05:36,550 --> 00:05:33,990 this unique trajectory will allow 115 00:05:38,710 --> 00:05:36,560 galileo to reach its ultimate goal 116 00:05:40,870 --> 00:05:38,720 returning a bonanza of scientific