1 00:00:13,190 --> 00:00:11,270 the deep impact mission was a mission to 2 00:00:14,910 --> 00:00:13,200 come at temple one to deliver an 3 00:00:18,150 --> 00:00:14,920 impactor in 4 00:00:20,470 --> 00:00:18,160 2005 the instruments on the deep impact 5 00:00:24,230 --> 00:00:20,480 spacecraft were designed to be 6 00:00:25,910 --> 00:00:24,240 diagnostic in a flyby of a comet 7 00:00:28,230 --> 00:00:25,920 we got some fascinating results from 8 00:00:29,910 --> 00:00:28,240 comet tempo one but once we got past 9 00:00:31,669 --> 00:00:29,920 temple one we had plenty of fuel left 10 00:00:33,510 --> 00:00:31,679 the spacecraft was healthy then 11 00:00:35,110 --> 00:00:33,520 immediately everybody set to work on 12 00:00:37,510 --> 00:00:35,120 figuring out what new bodies we could 13 00:00:40,069 --> 00:00:37,520 get to that's what led to the proposal 14 00:00:42,150 --> 00:00:40,079 to come go to comet hartley 2. it's 15 00:00:44,389 --> 00:00:42,160 really a good deal for for nasa and for 16 00:00:45,110 --> 00:00:44,399 the american public to send a spacecraft 17 00:00:47,830 --> 00:00:45,120 to 18 00:00:50,549 --> 00:00:47,840 a whole new mission for maybe uh a small 19 00:00:52,389 --> 00:00:50,559 fraction of what the a new mission cost 20 00:00:54,389 --> 00:00:52,399 we were able to re-target the spacecraft 21 00:00:55,990 --> 00:00:54,399 using a few flybys of earth take 22 00:00:57,590 --> 00:00:56,000 advantage of the gravity assist from 23 00:00:59,349 --> 00:00:57,600 earth to re-target ourselves change our 24 00:01:00,950 --> 00:00:59,359 trajectory just enough so that now we're 25 00:01:01,990 --> 00:01:00,960 able to get to comet hartley 2 in 26 00:01:03,910 --> 00:01:02,000 november 27 00:01:05,509 --> 00:01:03,920 because this wasn't what the spacecraft 28 00:01:06,310 --> 00:01:05,519 was planned for there's challenges and 29 00:01:08,149 --> 00:01:06,320 there's 30 00:01:10,550 --> 00:01:08,159 inevitably going to be surprises the 31 00:01:12,149 --> 00:01:10,560 geometry of the temple one flyby was 32 00:01:13,910 --> 00:01:12,159 such that we could look at the comet and 33 00:01:15,990 --> 00:01:13,920 take images at the same time that our 34 00:01:18,469 --> 00:01:16,000 high gain antenna was pointed at earth 35 00:01:20,950 --> 00:01:18,479 because of the geometry of the hartley 2 36 00:01:22,950 --> 00:01:20,960 flyby when we're pointed at the comet on 37 00:01:25,910 --> 00:01:22,960 approach our high gain antenna cannot 38 00:01:27,910 --> 00:01:25,920 see the earth so we cannot downlink data 39 00:01:29,350 --> 00:01:27,920 in real time so we have to design 40 00:01:31,190 --> 00:01:29,360 everything to 41 00:01:33,109 --> 00:01:31,200 for one thing protect that imaging 42 00:01:35,429 --> 00:01:33,119 sequence to make sure no matter what 43 00:01:38,230 --> 00:01:35,439 happens we're able to recover and keep 44 00:01:41,190 --> 00:01:38,240 taking images the things we will be 45 00:01:43,190 --> 00:01:41,200 looking for will be how different is the 46 00:01:45,190 --> 00:01:43,200 nucleus compared to the other comets 47 00:01:47,030 --> 00:01:45,200 that we've been to what does the nucleus 48 00:01:49,190 --> 00:01:47,040 look like that makes it so active can we 49 00:01:51,190 --> 00:01:49,200 see which parts of the comet are 50 00:01:53,109 --> 00:01:51,200 emitting so much gas and what's the 51 00:01:54,550 --> 00:01:53,119 nature of the chemicals the compounds 52 00:01:56,310 --> 00:01:54,560 that are coming off the comet the 53 00:01:57,910 --> 00:01:56,320 excitement about studying comets is 54 00:01:59,590 --> 00:01:57,920 really driven by getting a better 55 00:02:01,990 --> 00:01:59,600 understanding of the early phases and 56 00:02:03,350 --> 00:02:02,000 early formation of our solar system 57 00:02:05,030 --> 00:02:03,360 comets essentially have been in the 58 00:02:06,789 --> 00:02:05,040 refrigerator since the beginning of the 59 00:02:08,229 --> 00:02:06,799 solar system and so when we explore 60 00:02:10,150 --> 00:02:08,239 these objects and we find out what 61 00:02:12,150 --> 00:02:10,160 they're made of we get a look back at to 62 00:02:14,470 --> 00:02:12,160 the beginning of the formation of the 63 00:02:16,070 --> 00:02:14,480 solar system this mission is very 64 00:02:17,830 --> 00:02:16,080 economical and we're going to get