1 00:00:04,309 --> 00:00:02,230 welcome to nasa's jet propulsion 2 00:00:06,470 --> 00:00:04,319 laboratory in pasadena california i'm 3 00:00:08,470 --> 00:00:06,480 veronica mcgregor we had a date with a 4 00:00:10,230 --> 00:00:08,480 comet last night and things went 5 00:00:12,070 --> 00:00:10,240 exceptionally well 6 00:00:13,830 --> 00:00:12,080 we did have to wait a long time for 7 00:00:15,430 --> 00:00:13,840 those images to come down this morning 8 00:00:17,029 --> 00:00:15,440 though and that is why we are starting a 9 00:00:18,870 --> 00:00:17,039 little bit late and 10 00:00:21,109 --> 00:00:18,880 please accept our apologies for that so 11 00:00:24,070 --> 00:00:21,119 we are bringing you the latest images 12 00:00:25,830 --> 00:00:24,080 that are hitting the ground as we speak 13 00:00:27,269 --> 00:00:25,840 let me introduce the panelists for you 14 00:00:30,630 --> 00:00:27,279 now 15 00:00:32,709 --> 00:00:30,640 first we'll have dr ed weiler he is 16 00:00:34,630 --> 00:00:32,719 nasa's associate administrator the 17 00:00:37,990 --> 00:00:34,640 science mission directorate at nasa 18 00:00:41,990 --> 00:00:39,510 tim larson 19 00:00:47,029 --> 00:00:42,000 the stardust next project manager from 20 00:00:51,510 --> 00:00:49,590 dr joe viverka the stardust next 21 00:00:56,950 --> 00:00:51,520 principal investigator from cornell 22 00:01:01,990 --> 00:00:59,750 dr don brownlee the stardust next 23 00:01:06,230 --> 00:01:02,000 co-investigator from the university of 24 00:01:11,190 --> 00:01:08,789 and dr pete schultz another stardust 25 00:01:13,670 --> 00:01:11,200 next co-investigator and he's from brown 26 00:01:16,230 --> 00:01:13,680 university in providence rhode island 27 00:01:18,310 --> 00:01:16,240 and we will begin with dr weiler 28 00:01:20,550 --> 00:01:18,320 thank you veronica 29 00:01:22,789 --> 00:01:20,560 five and a half years ago a spacecraft 30 00:01:25,190 --> 00:01:22,799 named deep impact had a close encounter 31 00:01:27,030 --> 00:01:25,200 with a comet named temple one 32 00:01:30,149 --> 00:01:27,040 the mission was designed to drop off an 33 00:01:32,390 --> 00:01:30,159 800 pound metal slug which would impact 34 00:01:34,550 --> 00:01:32,400 the comet at a high velocity and throw 35 00:01:36,230 --> 00:01:34,560 up a bunch of comet material 36 00:01:38,469 --> 00:01:36,240 the spacecraft's instruments would then 37 00:01:40,710 --> 00:01:38,479 look at that material and eject it to 38 00:01:43,510 --> 00:01:40,720 better understand the chemical makeup of 39 00:01:45,429 --> 00:01:43,520 these primordial bodies called comets in 40 00:01:47,830 --> 00:01:45,439 fact the principal scientist of that 41 00:01:49,030 --> 00:01:47,840 mission um my dr mike rahern from 42 00:01:50,630 --> 00:01:49,040 university of maryland is in the 43 00:01:53,030 --> 00:01:50,640 audience today 44 00:01:56,310 --> 00:01:53,040 but that was yesterday's news 45 00:01:58,789 --> 00:01:56,320 in 2006 dr joe vaverka from cornell sent 46 00:02:00,709 --> 00:01:58,799 a proposal to nasa with a rather novel 47 00:02:02,870 --> 00:02:00,719 idea to re-target 48 00:02:05,350 --> 00:02:02,880 a different spacecraft called stardust 49 00:02:07,429 --> 00:02:05,360 to revisit temple one 50 00:02:09,190 --> 00:02:07,439 stardust is a twelve-year-old spacecraft 51 00:02:10,389 --> 00:02:09,200 having completed its prime mission many 52 00:02:11,990 --> 00:02:10,399 years ago 53 00:02:14,150 --> 00:02:12,000 this was the second time actually that 54 00:02:17,350 --> 00:02:14,160 nasa would take advantage of an old 55 00:02:19,670 --> 00:02:17,360 mission for new science and exploration 56 00:02:21,830 --> 00:02:19,680 the first was comet hartley encounter 57 00:02:25,350 --> 00:02:21,840 with a reused deep impact spacecraft 58 00:02:27,190 --> 00:02:25,360 renamed epoxy just last fall 59 00:02:30,229 --> 00:02:27,200 thanks to a great effort by the science 60 00:02:32,390 --> 00:02:30,239 team engineers navigators lockheed jpl 61 00:02:35,110 --> 00:02:32,400 and nasa we are here today to show you 62 00:02:37,430 --> 00:02:35,120 the results of humanity's first revisit 63 00:02:39,270 --> 00:02:37,440 to a comment to study how these objects 64 00:02:40,949 --> 00:02:39,280 evolve over time 65 00:02:43,190 --> 00:02:40,959 and i might add the results you will see 66 00:02:45,270 --> 00:02:43,200 in a few minutes were achieved for less 67 00:02:47,270 --> 00:02:45,280 than 10 percent 68 00:02:48,949 --> 00:02:47,280 of the cost of a new discovery class 69 00:02:50,630 --> 00:02:48,959 mission 70 00:02:52,949 --> 00:02:50,640 before i turn over to tim i have a 71 00:02:55,190 --> 00:02:52,959 message for any school kids out there 72 00:02:57,830 --> 00:02:55,200 who might be wondering how nasa can send 73 00:03:00,470 --> 00:02:57,840 a spacecraft billions of miles through 74 00:03:03,190 --> 00:03:00,480 the solar system and somehow wind up 75 00:03:05,670 --> 00:03:03,200 flying so close to a tiny comet only a 76 00:03:09,910 --> 00:03:05,680 few kilometers in diameter 77 00:03:14,470 --> 00:03:12,149 so pay attention in math class if you 78 00:03:16,550 --> 00:03:14,480 ever dreamed of being involved in this 79 00:03:18,630 --> 00:03:16,560 kind of real science discovery and 80 00:03:20,390 --> 00:03:18,640 exploration tim 81 00:03:21,830 --> 00:03:20,400 thank you ed 82 00:03:23,110 --> 00:03:21,840 again i'd like to reiterate this is 83 00:03:24,470 --> 00:03:23,120 exciting for us because it's the first 84 00:03:26,070 --> 00:03:24,480 time we've ever had the opportunity to 85 00:03:28,949 --> 00:03:26,080 visit a comet twice 86 00:03:30,309 --> 00:03:28,959 if you roll the animation that we have 87 00:03:32,149 --> 00:03:30,319 you'll see that temple one is a 88 00:03:34,390 --> 00:03:32,159 jupiter-class comet that goes its orbit 89 00:03:35,910 --> 00:03:34,400 goes out as far as jupiter and in this 90 00:03:38,630 --> 00:03:35,920 case comes in 91 00:03:40,630 --> 00:03:38,640 as close to the sun as the orbit of mars 92 00:03:43,670 --> 00:03:40,640 and that's about where we met it last 93 00:03:44,869 --> 00:03:43,680 night with the spacecraft 94 00:03:46,229 --> 00:03:44,879 based on the data that we brought down 95 00:03:49,110 --> 00:03:46,239 from the spacecraft we've been able to 96 00:03:51,270 --> 00:03:49,120 confirm that our flyby distance from the 97 00:03:52,710 --> 00:03:51,280 comet was 178 kilometers that's about 98 00:03:54,710 --> 00:03:52,720 110 miles 99 00:03:56,869 --> 00:03:54,720 uh we went past the comet at the 100 00:03:59,110 --> 00:03:56,879 velocity of 10.9 kilometers per second 101 00:04:02,229 --> 00:03:59,120 which is on the order of 24 000 miles 102 00:04:04,949 --> 00:04:02,239 per hour and our closest approach was 103 00:04:08,229 --> 00:04:04,959 right before 8 40 p.m uh here in on the 104 00:04:10,149 --> 00:04:08,239 west coast on valentine's evening 105 00:04:12,630 --> 00:04:10,159 our spacecraft telemetry shows that all 106 00:04:14,390 --> 00:04:12,640 of our subsystems operating exactly as 107 00:04:16,229 --> 00:04:14,400 we expected during the flyby 108 00:04:18,789 --> 00:04:16,239 the autonav software which is the 109 00:04:20,390 --> 00:04:18,799 autopilot software that controls the the 110 00:04:22,629 --> 00:04:20,400 motion of the mirror that keeps the 111 00:04:24,710 --> 00:04:22,639 comet in the image of field in the field 112 00:04:26,710 --> 00:04:24,720 of view of the camera worked exactly as 113 00:04:27,909 --> 00:04:26,720 planned and kept the comet exactly where 114 00:04:29,510 --> 00:04:27,919 it was supposed to be all the way 115 00:04:31,430 --> 00:04:29,520 through the flyby 116 00:04:33,030 --> 00:04:31,440 all the desired data that we wanted to 117 00:04:35,350 --> 00:04:33,040 collect was all collected and stored on 118 00:04:37,830 --> 00:04:35,360 board that's 72 images 119 00:04:39,909 --> 00:04:37,840 and approximately three megabytes of 120 00:04:41,590 --> 00:04:39,919 dust data for a total of about 78 121 00:04:43,110 --> 00:04:41,600 megabytes of data that doesn't sound 122 00:04:44,950 --> 00:04:43,120 like a lot to you but this is an old 123 00:04:49,030 --> 00:04:44,960 spacecraft 124 00:04:51,350 --> 00:04:49,040 after the flyby we were able to confirm 125 00:04:53,270 --> 00:04:51,360 that there is no noticeable degradation 126 00:04:55,189 --> 00:04:53,280 to the spacecraft to the health or 127 00:04:57,110 --> 00:04:55,199 function of the spacecraft despite the 128 00:04:58,629 --> 00:04:57,120 fact that we have detected several dust 129 00:05:01,110 --> 00:04:58,639 hits through the flyby and you'll hear a 130 00:05:02,710 --> 00:05:01,120 little bit more about that later 131 00:05:05,830 --> 00:05:02,720 so after the flyby we turned the hygiene 132 00:05:09,270 --> 00:05:05,840 antenna back to earth and began to uh 133 00:05:11,749 --> 00:05:09,280 downlink uh our our data as planned 134 00:05:14,070 --> 00:05:11,759 at that point since the spacecraft was 135 00:05:16,230 --> 00:05:14,080 healthy and we really wanted to gain a 136 00:05:17,909 --> 00:05:16,240 little bit more margin in our downlink 137 00:05:20,790 --> 00:05:17,919 to make sure that we protected this data 138 00:05:22,310 --> 00:05:20,800 and got it down in one pass safely 139 00:05:24,070 --> 00:05:22,320 we decided to delay our downlink by 140 00:05:25,830 --> 00:05:24,080 about 45 minutes so that we could 141 00:05:27,830 --> 00:05:25,840 reconfigure both the spacecraft and the 142 00:05:29,670 --> 00:05:27,840 deep space network station uh to 143 00:05:31,189 --> 00:05:29,680 accommodate that 144 00:05:33,110 --> 00:05:31,199 so that was that was accomplished and 145 00:05:35,189 --> 00:05:33,120 that went very well 146 00:05:37,990 --> 00:05:35,199 next we had our plan 147 00:05:39,830 --> 00:05:38,000 on the playback was to send five images 148 00:05:41,189 --> 00:05:39,840 that bracketed the closest approach 149 00:05:43,510 --> 00:05:41,199 period of 150 00:05:44,950 --> 00:05:43,520 of the flyby we wanted those five images 151 00:05:46,390 --> 00:05:44,960 to come down first in the queue when we 152 00:05:47,510 --> 00:05:46,400 started sending images back down to 153 00:05:49,510 --> 00:05:47,520 earth 154 00:05:50,870 --> 00:05:49,520 when we commanded that it turns out due 155 00:05:53,029 --> 00:05:50,880 to a software glitch that we had on 156 00:05:54,629 --> 00:05:53,039 board the images started coming down in 157 00:05:56,390 --> 00:05:54,639 the order they were taken 158 00:05:58,070 --> 00:05:56,400 so this did not jeopardize any of the 159 00:06:00,550 --> 00:05:58,080 data that we had on board all the data 160 00:06:02,390 --> 00:06:00,560 was safely stored in memory and was it 161 00:06:04,070 --> 00:06:02,400 was ready to be sent down we just had to 162 00:06:05,749 --> 00:06:04,080 wait a little bit longer for those 163 00:06:07,909 --> 00:06:05,759 images that all of us were really ready 164 00:06:09,590 --> 00:06:07,919 to see at that time so those images got 165 00:06:11,670 --> 00:06:09,600 down to the ground about between six and 166 00:06:12,870 --> 00:06:11,680 seven o'clock this morning uh you've 167 00:06:15,110 --> 00:06:12,880 already probably seen them out on the 168 00:06:17,590 --> 00:06:15,120 web and some very exciting findings 169 00:06:19,430 --> 00:06:17,600 coming out of those 170 00:06:21,189 --> 00:06:19,440 the spacecraft is continuing to send 171 00:06:23,430 --> 00:06:21,199 images down to earth we're at this point 172 00:06:24,870 --> 00:06:23,440 where approximately 60 out of the 72 173 00:06:27,029 --> 00:06:24,880 images are down on the ground we'll 174 00:06:29,110 --> 00:06:27,039 continue doing this until mid afternoon 175 00:06:31,270 --> 00:06:29,120 once we've confirmed that all the images 176 00:06:32,710 --> 00:06:31,280 and all the data is on the ground and 177 00:06:34,230 --> 00:06:32,720 all the packets are complete no 178 00:06:36,309 --> 00:06:34,240 corruption to any of the data that would 179 00:06:38,230 --> 00:06:36,319 require re-transmit at that point we'll 180 00:06:40,150 --> 00:06:38,240 be able to reconfigure the spacecraft 181 00:06:41,670 --> 00:06:40,160 and get ready for our outbound imaging 182 00:06:43,590 --> 00:06:41,680 when we do that we'll spend one to two 183 00:06:46,230 --> 00:06:43,600 weeks at least of looking back at the 184 00:06:47,749 --> 00:06:46,240 comet as we go away from it and as long 185 00:06:48,950 --> 00:06:47,759 as the scientists can get useful 186 00:06:51,029 --> 00:06:48,960 information out of the data we'll 187 00:06:52,230 --> 00:06:51,039 continue that process 188 00:06:54,070 --> 00:06:52,240 joel i'll leave it to you to tell us 189 00:06:56,070 --> 00:06:54,080 what we found all right well let's see 190 00:06:57,830 --> 00:06:56,080 tim a few minutes ago said that he was 191 00:06:59,189 --> 00:06:57,840 excited let me just say i mean more 192 00:07:02,629 --> 00:06:59,199 excited 193 00:07:05,909 --> 00:07:02,639 there is a great science and if we could 194 00:07:09,510 --> 00:07:05,919 have the first slide 195 00:07:11,670 --> 00:07:09,520 this shows us selected four images 196 00:07:14,390 --> 00:07:11,680 taken around closest approach 197 00:07:16,710 --> 00:07:14,400 and what i want to emphasize is 198 00:07:19,589 --> 00:07:16,720 that we achieved all of our science 199 00:07:21,350 --> 00:07:19,599 objectives we had four major science 200 00:07:23,270 --> 00:07:21,360 objectives three 201 00:07:26,230 --> 00:07:23,280 dealing with imaging and one with the 202 00:07:28,390 --> 00:07:26,240 dust experiments that we have on board 203 00:07:30,469 --> 00:07:28,400 the three imaging 204 00:07:31,749 --> 00:07:30,479 goals were first of all 205 00:07:33,270 --> 00:07:31,759 to 206 00:07:35,909 --> 00:07:33,280 look again 207 00:07:39,270 --> 00:07:35,919 at areas on temple that we had seen 208 00:07:42,950 --> 00:07:39,280 before in 2005 with deep impact to for 209 00:07:45,270 --> 00:07:42,960 the first time see what changes occur on 210 00:07:47,990 --> 00:07:45,280 a comet when it comes close to the sun 211 00:07:49,430 --> 00:07:48,000 and where those changes occur 212 00:07:51,430 --> 00:07:49,440 we also 213 00:07:53,749 --> 00:07:51,440 wanted to take the opportunity to look 214 00:07:56,070 --> 00:07:53,759 at the deep impact site where 215 00:07:58,469 --> 00:07:56,080 the deep impact impactor 216 00:08:00,070 --> 00:07:58,479 collided with the comet 217 00:08:02,629 --> 00:08:00,080 and finally we wanted to take the 218 00:08:05,189 --> 00:08:02,639 opportunity to 219 00:08:07,670 --> 00:08:05,199 extend our exploration and see areas on 220 00:08:11,029 --> 00:08:07,680 temple that we have not seen before so 221 00:08:13,510 --> 00:08:11,039 we had three imaging objectives and one 222 00:08:15,670 --> 00:08:13,520 objective having to do with analyzing 223 00:08:18,070 --> 00:08:15,680 collecting dust the dr brownlee will 224 00:08:20,710 --> 00:08:18,080 talk about dust i'll talk about imaging 225 00:08:25,350 --> 00:08:22,710 if you ask me 226 00:08:28,070 --> 00:08:25,360 was this mission a hundred percent 227 00:08:30,390 --> 00:08:28,080 successful in terms of the science 228 00:08:32,469 --> 00:08:30,400 i would have to say no it was a thousand 229 00:08:34,389 --> 00:08:32,479 percent successful 230 00:08:36,709 --> 00:08:34,399 and so i would like to just very quickly 231 00:08:38,389 --> 00:08:36,719 go over some of the highlights uh 232 00:08:39,990 --> 00:08:38,399 what we're looking at here are four 233 00:08:42,550 --> 00:08:40,000 images around closest approach and the 234 00:08:44,949 --> 00:08:42,560 way we planned this encounter was on the 235 00:08:47,350 --> 00:08:44,959 way in to see some of the old territory 236 00:08:49,030 --> 00:08:47,360 that we had seen before in 2005 237 00:08:52,070 --> 00:08:49,040 including the 238 00:08:54,710 --> 00:08:52,080 crater site and then on 239 00:08:57,750 --> 00:08:54,720 after close approach to see new parts of 240 00:08:59,509 --> 00:08:57,760 the comet so behind me here we have the 241 00:09:02,070 --> 00:08:59,519 approach images i just point out to 242 00:09:03,509 --> 00:09:02,080 craters this is the area where the deep 243 00:09:09,509 --> 00:09:03,519 impact 244 00:09:10,630 --> 00:09:09,519 can barely see in this image is a region 245 00:09:13,190 --> 00:09:10,640 that 246 00:09:15,750 --> 00:09:13,200 was intriguing to us because we expected 247 00:09:17,269 --> 00:09:15,760 that region to change significantly in 248 00:09:19,350 --> 00:09:17,279 the five and a half years between the 249 00:09:21,190 --> 00:09:19,360 encounters so let me first of all show 250 00:09:22,550 --> 00:09:21,200 you one example of the changes in the 251 00:09:24,710 --> 00:09:22,560 next slide 252 00:09:25,829 --> 00:09:24,720 which is that area that i pointed out 253 00:09:27,590 --> 00:09:25,839 before 254 00:09:29,590 --> 00:09:27,600 the smooth right this is a deep impact 255 00:09:30,870 --> 00:09:29,600 image up here 256 00:09:32,070 --> 00:09:30,880 you see 257 00:09:35,509 --> 00:09:32,080 the 258 00:09:37,829 --> 00:09:35,519 region in 2005 this is about 2 or three 259 00:09:40,230 --> 00:09:37,839 kilometers in extend this is maybe three 260 00:09:43,910 --> 00:09:40,240 or four hundred uh i'm sorry uh meters 261 00:09:46,790 --> 00:09:43,920 across here uh this is 2005 this is 262 00:09:48,470 --> 00:09:46,800 2011. this is the current situation and 263 00:09:51,509 --> 00:09:48,480 let me just point out a few things for 264 00:09:54,230 --> 00:09:51,519 example up here you see three pits 265 00:09:57,350 --> 00:09:54,240 here you see one contiguous pit 266 00:09:59,829 --> 00:09:57,360 erosion on a scale of 20 30 meters of 267 00:10:00,870 --> 00:09:59,839 material has occurred in a five or six 268 00:10:02,870 --> 00:10:00,880 years 269 00:10:04,550 --> 00:10:02,880 since we took this picture also if you 270 00:10:06,230 --> 00:10:04,560 follow the outline of this of this 271 00:10:08,150 --> 00:10:06,240 boundary and compare it to what we see 272 00:10:10,069 --> 00:10:08,160 today you will again see significant 273 00:10:12,550 --> 00:10:10,079 changes so we were successful in that 274 00:10:14,389 --> 00:10:12,560 objective we we are seeing 275 00:10:16,470 --> 00:10:14,399 changes we have to spend time and 276 00:10:19,030 --> 00:10:16,480 quantifying those changes and 277 00:10:19,829 --> 00:10:19,040 understanding what they mean our second 278 00:10:22,389 --> 00:10:19,839 uh 279 00:10:24,230 --> 00:10:22,399 goal if i could have the next slide 280 00:10:26,710 --> 00:10:24,240 uh okay 281 00:10:28,710 --> 00:10:26,720 this is just uh uh shows us the two 282 00:10:29,670 --> 00:10:28,720 areas uh the uh 283 00:10:31,190 --> 00:10:29,680 the uh 284 00:10:33,269 --> 00:10:31,200 the area outlined here where the changes 285 00:10:37,269 --> 00:10:33,279 occurred and also the boundary but what 286 00:10:38,790 --> 00:10:37,279 we're looking for is the following slide 287 00:10:40,230 --> 00:10:38,800 that is not the following slide but how 288 00:10:43,910 --> 00:10:40,240 about the one what have you got after 289 00:10:49,430 --> 00:10:47,829 you have anything after this one 290 00:10:50,230 --> 00:10:49,440 yep that's that's the one they have for 291 00:10:53,670 --> 00:10:50,240 you 292 00:10:58,069 --> 00:10:55,190 not at this time 293 00:11:00,550 --> 00:10:58,079 okay well then folks uh the way this is 294 00:11:03,269 --> 00:11:00,560 going to work is that 295 00:11:04,710 --> 00:11:03,279 we do in fact have a comparison of the 296 00:11:05,670 --> 00:11:04,720 deep impact 297 00:11:08,949 --> 00:11:05,680 area 298 00:11:10,870 --> 00:11:08,959 in 2005 and 2011 299 00:11:12,710 --> 00:11:10,880 and it in fact does show an impact 300 00:11:15,030 --> 00:11:12,720 crater 301 00:11:16,949 --> 00:11:15,040 and uh unfortunately i can't show it to 302 00:11:19,269 --> 00:11:16,959 you but pete schultz in a few minutes 303 00:11:22,230 --> 00:11:19,279 apparently if we are lucky he might 304 00:11:24,069 --> 00:11:22,240 actually have that comparison so we were 305 00:11:26,389 --> 00:11:24,079 again successful we achieved our 306 00:11:28,949 --> 00:11:26,399 objective we not only imaged the area of 307 00:11:31,190 --> 00:11:28,959 the deep impact event but we have an 308 00:11:32,949 --> 00:11:31,200 image of the crater that was produced 309 00:11:35,829 --> 00:11:32,959 and finally the slide that we have here 310 00:11:38,310 --> 00:11:35,839 is to exemplify our third goal which was 311 00:11:40,470 --> 00:11:38,320 to extend the exploration of temple to 312 00:11:43,590 --> 00:11:40,480 areas we have not seen before so this is 313 00:11:45,750 --> 00:11:43,600 a part of in this picture the parts that 314 00:11:48,470 --> 00:11:45,760 we have seen before are sort of behind 315 00:11:49,509 --> 00:11:48,480 up here and this is all new territory on 316 00:11:52,710 --> 00:11:49,519 the comet 317 00:11:55,509 --> 00:11:52,720 and it is simply amazing uh there are 318 00:11:58,230 --> 00:11:55,519 extensive areas of layering 319 00:12:00,310 --> 00:11:58,240 layers that have been deposited each 320 00:12:01,190 --> 00:12:00,320 layer a few meters thick maybe 10 meters 321 00:12:03,990 --> 00:12:01,200 thick 322 00:12:05,430 --> 00:12:04,000 we have to puzzle how does this happen 323 00:12:07,190 --> 00:12:05,440 we have large 324 00:12:09,110 --> 00:12:07,200 regions this is about a kilometer across 325 00:12:11,030 --> 00:12:09,120 where material has apparently been 326 00:12:14,150 --> 00:12:11,040 sublimated from the surface 327 00:12:16,150 --> 00:12:14,160 and removed there are areas on here 328 00:12:17,829 --> 00:12:16,160 which look like they're heavily pitted 329 00:12:19,269 --> 00:12:17,839 or heavily cratered 330 00:12:21,430 --> 00:12:19,279 again 331 00:12:23,750 --> 00:12:21,440 geology that we did not see on the outer 332 00:12:25,030 --> 00:12:23,760 space of temple and to understand how 333 00:12:27,110 --> 00:12:25,040 this comet works we have to put 334 00:12:29,910 --> 00:12:27,120 everything together in closing i want to 335 00:12:32,230 --> 00:12:29,920 emphasize that to achieve these three 336 00:12:34,550 --> 00:12:32,240 imaging objectives we had to arrive at 337 00:12:36,389 --> 00:12:34,560 the comet at precisely the right time as 338 00:12:38,230 --> 00:12:36,399 i mentioned we planned it so that on 339 00:12:40,710 --> 00:12:38,240 approach we would see the deep impact 340 00:12:43,430 --> 00:12:40,720 area and then after close approach we've 341 00:12:44,710 --> 00:12:43,440 seen you terrain that meant arriving 342 00:12:47,190 --> 00:12:44,720 precisely 343 00:12:48,310 --> 00:12:47,200 at the right time at the right place 344 00:12:50,710 --> 00:12:48,320 and 345 00:12:52,949 --> 00:12:50,720 to achieve that not only did we need 346 00:12:54,710 --> 00:12:52,959 first class navigation but we needed 347 00:12:55,829 --> 00:12:54,720 information on the rotation state of the 348 00:12:57,430 --> 00:12:55,839 comet 349 00:12:59,910 --> 00:12:57,440 we had an international effort over 350 00:13:02,550 --> 00:12:59,920 several years of monitoring the comet's 351 00:13:05,509 --> 00:13:02,560 rotation and and predicting what the 352 00:13:06,470 --> 00:13:05,519 state would be at encounter time 353 00:13:08,550 --> 00:13:06,480 uh 354 00:13:09,350 --> 00:13:08,560 how well did we do 355 00:13:11,670 --> 00:13:09,360 uh 356 00:13:14,069 --> 00:13:11,680 we got the longitude 357 00:13:16,790 --> 00:13:14,079 uh over which wanted to fly 358 00:13:19,030 --> 00:13:16,800 to plus or minus one or two degrees out 359 00:13:22,470 --> 00:13:19,040 of 360 degrees so that was a great 360 00:13:25,670 --> 00:13:22,480 achievement by our scientists so we're 361 00:13:28,310 --> 00:13:25,680 tremendously happy and i will now pass 362 00:13:30,069 --> 00:13:28,320 the discussion on to dr schultz who 363 00:13:31,430 --> 00:13:30,079 hopefully does have a picture of the 364 00:13:39,990 --> 00:13:31,440 crater 365 00:13:43,030 --> 00:13:40,000 but i've never had to wait five and a 366 00:13:45,110 --> 00:13:43,040 half years to see the results 367 00:13:47,110 --> 00:13:45,120 so if we can we have that first time 368 00:13:48,949 --> 00:13:47,120 step up there and you can actually see 369 00:13:51,829 --> 00:13:48,959 what deep impact saw and one of the 370 00:13:53,990 --> 00:13:51,839 close-up views that showed from the 371 00:13:56,550 --> 00:13:54,000 probe's perspective as it was zooming in 372 00:13:57,350 --> 00:13:56,560 to the surface and where it was going to 373 00:13:59,269 --> 00:13:57,360 hit 374 00:14:01,750 --> 00:13:59,279 around nine feet tempo one 375 00:14:03,829 --> 00:14:01,760 if we go to the next time step 376 00:14:06,870 --> 00:14:03,839 this is why we needed to go back on the 377 00:14:09,269 --> 00:14:06,880 left hand side is an image 378 00:14:11,750 --> 00:14:09,279 from one of the hri images and on the 379 00:14:14,389 --> 00:14:11,760 right is an image that deep impact saw 380 00:14:16,310 --> 00:14:14,399 about 700 seconds afterwards you notice 381 00:14:18,069 --> 00:14:16,320 we can't see the crater it's it's 382 00:14:20,069 --> 00:14:18,079 obscured by all the ejecta that was 383 00:14:22,230 --> 00:14:20,079 tossed up by the impact 384 00:14:23,590 --> 00:14:22,240 we never saw the craters went by is 385 00:14:25,189 --> 00:14:23,600 there somewhere 386 00:14:27,509 --> 00:14:25,199 um you know that created a lot of 387 00:14:28,629 --> 00:14:27,519 mystery it also created help to create 388 00:14:29,590 --> 00:14:28,639 this mission 389 00:14:31,590 --> 00:14:29,600 uh 390 00:14:32,550 --> 00:14:31,600 um let's take a look at the next time 391 00:14:34,949 --> 00:14:32,560 step 392 00:14:37,030 --> 00:14:34,959 i just want to show you how well we can 393 00:14:40,069 --> 00:14:37,040 correlate the different features on the 394 00:14:42,150 --> 00:14:40,079 left is an image of from deep impact on 395 00:14:44,150 --> 00:14:42,160 the right is stardust next and you can 396 00:14:46,150 --> 00:14:44,160 see those two craters those two 397 00:14:49,030 --> 00:14:46,160 crater-like features each one of them 398 00:14:51,189 --> 00:14:49,040 about 300 meters across 399 00:14:52,790 --> 00:14:51,199 almost a thousand feet 400 00:14:54,389 --> 00:14:52,800 where we were aiming was right in 401 00:14:55,910 --> 00:14:54,399 between with deep impact that's where 402 00:14:57,590 --> 00:14:55,920 that probe went in 403 00:14:58,870 --> 00:14:57,600 and if we take a look at the next time 404 00:15:06,870 --> 00:14:58,880 step 405 00:15:09,269 --> 00:15:06,880 huh that's the next picture that's a 406 00:15:10,949 --> 00:15:09,279 nice picture yeah very nice picture 407 00:15:13,350 --> 00:15:10,959 um i i don't know yeah we're going to 408 00:15:14,949 --> 00:15:13,360 put that last one up 409 00:15:16,790 --> 00:15:14,959 okay is there another one after this no 410 00:15:20,069 --> 00:15:16,800 there is not there is no hey joe guess 411 00:15:23,590 --> 00:15:22,150 it's it's clearly well done let me just 412 00:15:27,110 --> 00:15:23,600 let me just tell them 413 00:15:29,430 --> 00:15:27,120 hey we saw the crater 414 00:15:30,470 --> 00:15:29,440 yeah really we really did see we saw the 415 00:15:33,110 --> 00:15:30,480 crater 416 00:15:35,829 --> 00:15:33,120 and i tell you what i'll give you 417 00:15:36,870 --> 00:15:35,839 stay with me here okay we saw this 418 00:15:38,310 --> 00:15:36,880 crater 419 00:15:40,870 --> 00:15:38,320 it's subdued 420 00:15:43,430 --> 00:15:40,880 it's about 150 meters across and has a 421 00:15:45,430 --> 00:15:43,440 small central mound in the center it 422 00:15:47,430 --> 00:15:45,440 looks as if from the impact the stuff 423 00:15:50,069 --> 00:15:47,440 went up and came back down 424 00:15:52,069 --> 00:15:50,079 so we did get it there's no doubt and i 425 00:15:54,310 --> 00:15:52,079 think one of the bottom uh bottom line 426 00:15:56,790 --> 00:15:54,320 messages is that this surface of the 427 00:15:59,509 --> 00:15:56,800 comet where we hit is very weak 428 00:16:00,870 --> 00:15:59,519 uh it's fragile so the crater partly 429 00:16:02,710 --> 00:16:00,880 healed itself 430 00:16:04,629 --> 00:16:02,720 so let's let me turn this over to don 431 00:16:07,030 --> 00:16:04,639 brownlee and see if he can give them 432 00:16:08,870 --> 00:16:07,040 some data 433 00:16:11,590 --> 00:16:08,880 do do you have the picture of the crater 434 00:16:17,269 --> 00:16:14,069 we had a lot we had thousands of craters 435 00:16:19,189 --> 00:16:17,279 the uh uh comets unlike any other body 436 00:16:20,470 --> 00:16:19,199 in the solar system are unique because 437 00:16:22,310 --> 00:16:20,480 when they're in the inner part of the 438 00:16:25,110 --> 00:16:22,320 solar system where the earth is they're 439 00:16:27,749 --> 00:16:25,120 literally coming apart and sending tons 440 00:16:29,030 --> 00:16:27,759 and tons of gas and rocks and dust out 441 00:16:30,629 --> 00:16:29,040 in space 442 00:16:32,790 --> 00:16:30,639 so last night 443 00:16:34,949 --> 00:16:32,800 this spacecraft stardust 444 00:16:36,949 --> 00:16:34,959 went through this cloud of dust and 445 00:16:38,710 --> 00:16:36,959 rocks coming off the comet the second 446 00:16:41,509 --> 00:16:38,720 time it survived this 447 00:16:43,189 --> 00:16:41,519 it actually had a dozen impacts on the 448 00:16:45,590 --> 00:16:43,199 front leading edge of the spacecraft 449 00:16:48,069 --> 00:16:45,600 here called the whipple bumper that went 450 00:16:50,870 --> 00:16:48,079 through the front that's a it's a 451 00:16:52,629 --> 00:16:50,880 graphite cyanate honeycomb 452 00:16:53,590 --> 00:16:52,639 sheet that's about as thick as your 453 00:16:56,470 --> 00:16:53,600 finger 454 00:16:58,790 --> 00:16:56,480 and a dozen of those were big enough 455 00:17:00,710 --> 00:16:58,800 about almost a millimeter size they went 456 00:17:04,069 --> 00:17:00,720 punctured into it and went into the 457 00:17:06,309 --> 00:17:04,079 inside of the whipple shield from behind 458 00:17:07,270 --> 00:17:06,319 in addition to that we have uh the 459 00:17:10,630 --> 00:17:07,280 instrument 460 00:17:12,309 --> 00:17:10,640 spacecraft called dust flux monitor 461 00:17:14,230 --> 00:17:12,319 instrument and this was made by a 462 00:17:16,630 --> 00:17:14,240 collaboration of the university of 463 00:17:19,270 --> 00:17:16,640 chicago and university of kent 464 00:17:22,470 --> 00:17:19,280 in england and they have sensor to 465 00:17:24,390 --> 00:17:22,480 detect these impacts they detected 5 000 466 00:17:26,309 --> 00:17:24,400 smaller particles 467 00:17:29,190 --> 00:17:26,319 but one of the really interesting things 468 00:17:30,870 --> 00:17:29,200 about just the impact rate and i hope we 469 00:17:33,350 --> 00:17:30,880 can hear the impact rate in just a 470 00:17:35,750 --> 00:17:33,360 second was the nature of the impact rate 471 00:17:37,110 --> 00:17:35,760 when we flew past the previous comet 472 00:17:39,270 --> 00:17:37,120 bill 2 473 00:17:41,990 --> 00:17:39,280 years ago we were stunned 474 00:17:43,909 --> 00:17:42,000 that instead of having a slow rise in 475 00:17:46,630 --> 00:17:43,919 the impact rate and then peaking out 476 00:17:49,190 --> 00:17:46,640 when we got closest and then dropping 477 00:17:51,669 --> 00:17:49,200 off it came in sputters and starts never 478 00:17:53,830 --> 00:17:51,679 thought what on earth is going on what's 479 00:17:56,310 --> 00:17:53,840 going on this is the way comets 480 00:17:58,789 --> 00:17:56,320 act they don't just spew off things in a 481 00:18:01,029 --> 00:17:58,799 uniform way they send it out in bursts 482 00:18:02,070 --> 00:18:01,039 and puffs and even more than that they 483 00:18:05,190 --> 00:18:02,080 send out 484 00:18:06,390 --> 00:18:05,200 clods of dirt and ice and rock that come 485 00:18:08,870 --> 00:18:06,400 apart 486 00:18:11,909 --> 00:18:08,880 and so a good analogy of thinking of 487 00:18:13,510 --> 00:18:11,919 like a b17 in world war ii flying 488 00:18:15,590 --> 00:18:13,520 through flack 489 00:18:17,270 --> 00:18:15,600 and so instead of being big bing bing 490 00:18:19,270 --> 00:18:17,280 bing like that it's just burst of things 491 00:18:21,110 --> 00:18:19,280 we had sometimes a large number of 492 00:18:23,190 --> 00:18:21,120 impacts in less than a tenth 493 00:18:26,150 --> 00:18:23,200 of a second so it's a very dramatic 494 00:18:30,070 --> 00:18:26,160 environment do we have the audio tape on 495 00:18:31,110 --> 00:18:30,080 on on that we'll have a little 496 00:18:37,110 --> 00:18:31,120 okay 497 00:18:37,120 --> 00:18:46,150 that's it 498 00:18:49,510 --> 00:18:47,830 so weren't you glad you weren't on the 499 00:18:51,990 --> 00:18:49,520 spacecraft 500 00:18:54,470 --> 00:18:52,000 and this went on and on and on and the 501 00:18:56,230 --> 00:18:54,480 first impacts are several minutes be 502 00:18:58,950 --> 00:18:56,240 before the closest approach and they 503 00:19:01,350 --> 00:18:58,960 continued on but thousands of impacts 504 00:19:03,590 --> 00:19:01,360 including you know firecracker size uh 505 00:19:05,430 --> 00:19:03,600 burst so that was really exciting and 506 00:19:07,270 --> 00:19:05,440 and from the comet science is very 507 00:19:09,350 --> 00:19:07,280 interesting so there's two comets we've 508 00:19:11,190 --> 00:19:09,360 seen that behave this way 509 00:19:13,029 --> 00:19:11,200 but even more you know we've been to 510 00:19:15,270 --> 00:19:13,039 several comets now 511 00:19:17,110 --> 00:19:15,280 and comet harley didn't have a dust 512 00:19:18,710 --> 00:19:17,120 detector on it but it took these 513 00:19:21,350 --> 00:19:18,720 marvelous pictures 514 00:19:22,470 --> 00:19:21,360 of these snow and dirt balls coming 515 00:19:24,950 --> 00:19:22,480 apart 516 00:19:27,430 --> 00:19:24,960 in space after they're admitted for from 517 00:19:30,470 --> 00:19:27,440 the comets so these clods come off 518 00:19:32,230 --> 00:19:30,480 disintegrate and then the spacecraft uh 519 00:19:33,830 --> 00:19:32,240 goes through them 520 00:19:37,350 --> 00:19:33,840 the 521 00:19:39,510 --> 00:19:37,360 massage is detecting dust we also had an 522 00:19:42,230 --> 00:19:39,520 instrument on the side of the spacecraft 523 00:19:44,150 --> 00:19:42,240 called cita made by max blanc institute 524 00:19:46,710 --> 00:19:44,160 in germany and this measures the 525 00:19:48,950 --> 00:19:46,720 chemical composition of dust 526 00:19:52,549 --> 00:19:48,960 and there are several dozen particles 527 00:19:54,630 --> 00:19:52,559 that were analyzed last night 528 00:19:57,510 --> 00:19:54,640 during the flyby and 529 00:20:00,230 --> 00:19:57,520 this time the instrument was carefully 530 00:20:03,029 --> 00:20:00,240 tuned to be very sensitive to very small 531 00:20:05,270 --> 00:20:03,039 particles and also to measure organics 532 00:20:06,710 --> 00:20:05,280 and the first spectra i saw was very 533 00:20:07,750 --> 00:20:06,720 exciting because it showed peaks for 534 00:20:13,510 --> 00:20:07,760 carbon 535 00:20:16,310 --> 00:20:13,520 anyway it was a real thrill to do this 536 00:20:18,470 --> 00:20:16,320 the whole mission was was a real thrill 537 00:20:20,950 --> 00:20:18,480 and it's it's great to use one 538 00:20:24,950 --> 00:20:20,960 spacecraft to go to multiple targets 539 00:20:28,149 --> 00:20:26,789 okay we are going to open it up to 540 00:20:31,750 --> 00:20:28,159 questions in the meantime they are 541 00:20:34,710 --> 00:20:31,760 trying to find uh the images um 542 00:20:36,149 --> 00:20:34,720 they're they were 543 00:20:37,669 --> 00:20:36,159 and we're hoping also to have a flicker 544 00:20:39,430 --> 00:20:37,679 movie of the 545 00:20:41,029 --> 00:20:39,440 images altogether all the images that we 546 00:20:42,549 --> 00:20:41,039 have so far but in the meantime let me 547 00:20:44,549 --> 00:20:42,559 go ahead and open it up to questions 548 00:20:46,390 --> 00:20:44,559 we'll start in the room first if there 549 00:20:48,549 --> 00:20:46,400 are any questions if not we do have some 550 00:20:55,430 --> 00:20:48,559 people on the phone uh are there any 551 00:20:59,110 --> 00:20:57,270 yes go ahead and give us your name and 552 00:21:02,390 --> 00:20:59,120 affiliation sure stand in totten with 553 00:21:03,510 --> 00:21:02,400 kpcc uh you pointed to an image of uh 554 00:21:05,029 --> 00:21:03,520 i'm not sure what it was but it was a 555 00:21:07,350 --> 00:21:05,039 shape that you said had changed it had 556 00:21:08,950 --> 00:21:07,360 eroded over time uh can you explain a 557 00:21:10,630 --> 00:21:08,960 little bit more what that what caused 558 00:21:11,909 --> 00:21:10,640 that shape and what caused the changes 559 00:21:13,669 --> 00:21:11,919 how did that happen when we were well 560 00:21:17,510 --> 00:21:13,679 what caused the changes the surface of 561 00:21:19,350 --> 00:21:17,520 the comet is uh in part made of water 562 00:21:20,149 --> 00:21:19,360 ice when the comet comes close to the 563 00:21:20,950 --> 00:21:20,159 sun 564 00:21:28,070 --> 00:21:20,960 the 565 00:21:31,830 --> 00:21:28,080 that's why we see gases and dust coming 566 00:21:34,230 --> 00:21:31,840 from a comet and so 567 00:21:38,230 --> 00:21:34,240 what you saw are places where during the 568 00:21:40,870 --> 00:21:38,240 last five years ice has evaporated and 569 00:21:45,270 --> 00:21:40,880 carried with a dust into space 570 00:21:45,280 --> 00:21:50,870 sorry about that 571 00:21:55,750 --> 00:21:52,390 any other questions from news media in 572 00:21:58,870 --> 00:21:55,760 the room uh yes alicia chang 573 00:22:00,470 --> 00:21:58,880 alicia chang from ap um tim the reason 574 00:22:02,549 --> 00:22:00,480 why it took so long to download the 575 00:22:04,549 --> 00:22:02,559 pictures was it a result of commands 576 00:22:07,750 --> 00:22:04,559 that were already sent up disgrace 577 00:22:10,390 --> 00:22:07,760 spacecraft before or 578 00:22:12,630 --> 00:22:10,400 when you had to do the reconfiguration 579 00:22:14,630 --> 00:22:12,640 during the mission oh that was yeah the 580 00:22:16,390 --> 00:22:14,640 initial reconfiguration we did that that 581 00:22:17,830 --> 00:22:16,400 configuration was planned ahead of time 582 00:22:19,510 --> 00:22:17,840 we designed that as part of the 583 00:22:20,630 --> 00:22:19,520 encounter but we wanted to make sure 584 00:22:22,070 --> 00:22:20,640 that no matter what kind of 585 00:22:23,990 --> 00:22:22,080 contingencies happened during the 586 00:22:25,909 --> 00:22:24,000 encounter we came on out on the other 587 00:22:27,830 --> 00:22:25,919 side of it in a known configuration that 588 00:22:29,909 --> 00:22:27,840 we could support with telecom that's why 589 00:22:32,390 --> 00:22:29,919 we had that particular configuration 590 00:22:34,789 --> 00:22:32,400 selected once we knew we were healthy 591 00:22:36,630 --> 00:22:34,799 and could support a different decoder at 592 00:22:37,830 --> 00:22:36,640 the station we went ahead and asked for 593 00:22:39,990 --> 00:22:37,840 that because that gave us a little bit 594 00:22:41,750 --> 00:22:40,000 more margin on our on our down like just 595 00:22:44,070 --> 00:22:41,760 to make sure we had uh 596 00:22:45,669 --> 00:22:44,080 more safety net above above the signal 597 00:22:47,029 --> 00:22:45,679 that we had 598 00:22:48,310 --> 00:22:47,039 but the fact that it took so long for 599 00:22:50,470 --> 00:22:48,320 the pictures to download was it a 600 00:22:52,950 --> 00:22:50,480 mistake in the commands that were sent 601 00:22:54,870 --> 00:22:52,960 up no uh that that initial one was 602 00:22:56,549 --> 00:22:54,880 driven purely by physics because it 603 00:22:58,470 --> 00:22:56,559 required a command to the spacecraft and 604 00:22:59,350 --> 00:22:58,480 the round-trip light time is around 40 605 00:23:01,669 --> 00:22:59,360 minutes 606 00:23:04,070 --> 00:23:01,679 um the second downlink uh issue that i 607 00:23:06,549 --> 00:23:04,080 talked about that was that is a software 608 00:23:09,590 --> 00:23:06,559 issue that we're looking into uh it was 609 00:23:12,070 --> 00:23:09,600 supposed to have put the uh 610 00:23:13,909 --> 00:23:12,080 the five pre-selected images uh into the 611 00:23:16,390 --> 00:23:13,919 downlink queue first and we don't know 612 00:23:18,630 --> 00:23:16,400 yet why it didn't 613 00:23:20,149 --> 00:23:18,640 also 200 million miles away but those 614 00:23:23,669 --> 00:23:20,159 images are on the ground they're all on 615 00:23:27,270 --> 00:23:24,870 all right we're going to take a question 616 00:23:29,510 --> 00:23:27,280 next from the phone lines uh the la 617 00:23:31,750 --> 00:23:29,520 times is on the line amina khan please 618 00:23:33,510 --> 00:23:31,760 go ahead with your question 619 00:23:35,990 --> 00:23:33,520 hi and thank you for taking my call i 620 00:23:38,710 --> 00:23:36,000 have a couple of questions uh you 621 00:23:40,870 --> 00:23:38,720 mentioned that the cost would be about 622 00:23:43,029 --> 00:23:40,880 10 percent of a new discovery type 623 00:23:45,669 --> 00:23:43,039 mission how much is the actual cost of 624 00:23:47,750 --> 00:23:45,679 this mission um the second question 625 00:23:51,190 --> 00:23:47,760 is related to 626 00:23:53,430 --> 00:23:51,200 the surface of the comet um yeah i heard 627 00:23:55,430 --> 00:23:53,440 yesterday that there were some smooth 628 00:23:57,590 --> 00:23:55,440 areas that seemed to suggest there had 629 00:23:59,110 --> 00:23:57,600 been flows along the surface could you 630 00:24:00,710 --> 00:23:59,120 um talk a little bit about that and what 631 00:24:02,390 --> 00:24:00,720 might have caused that 632 00:24:05,669 --> 00:24:02,400 okay i'll take this is ed weiler from 633 00:24:08,149 --> 00:24:05,679 nasa the uh i'll take the first question 634 00:24:10,310 --> 00:24:08,159 the cost of a new discovery mission to 635 00:24:12,149 --> 00:24:10,320 do this kind of sciences in the range 636 00:24:14,070 --> 00:24:12,159 counting the launch vehicle of perhaps 637 00:24:15,430 --> 00:24:14,080 three to four to five hundred million 638 00:24:18,390 --> 00:24:15,440 dollars 639 00:24:20,070 --> 00:24:18,400 uh this mission cost nasa exactly 29 640 00:24:22,310 --> 00:24:20,080 million dollars so i was being 641 00:24:25,590 --> 00:24:22,320 conservative when i said 10 it may be as 642 00:24:30,149 --> 00:24:27,430 uh the smooth flaws that you're 643 00:24:33,990 --> 00:24:30,159 referring to were discovered on temple 644 00:24:37,029 --> 00:24:34,000 uh in 2005 by deep impact and they came 645 00:24:38,149 --> 00:24:37,039 as a surprise to comet scientists 646 00:24:40,789 --> 00:24:38,159 uh 647 00:24:43,909 --> 00:24:40,799 they have been interpreted as places 648 00:24:46,710 --> 00:24:43,919 where uh very volatile gas 649 00:24:49,669 --> 00:24:46,720 from below the surface 650 00:24:53,510 --> 00:24:49,679 has erupted carrying with it 651 00:24:55,590 --> 00:24:53,520 small particles of ice and dust and 652 00:24:56,470 --> 00:24:55,600 while some of this stuff leaves into 653 00:24:58,549 --> 00:24:56,480 space 654 00:25:01,430 --> 00:24:58,559 some of it just 655 00:25:03,669 --> 00:25:01,440 flows downhill because the comet does 656 00:25:05,510 --> 00:25:03,679 have a little bit of gravity 657 00:25:07,190 --> 00:25:05,520 so what is surprising about those 658 00:25:08,230 --> 00:25:07,200 features is that they seem to be fairly 659 00:25:09,590 --> 00:25:08,240 recent 660 00:25:11,830 --> 00:25:09,600 and 661 00:25:13,990 --> 00:25:11,840 apparently they also change 662 00:25:16,070 --> 00:25:14,000 with time readily because that's where 663 00:25:20,149 --> 00:25:16,080 we have seen the most obvious changes in 664 00:25:21,510 --> 00:25:20,159 the comparison between 2005 and 2011. 665 00:25:22,950 --> 00:25:21,520 but uh 666 00:25:24,549 --> 00:25:22,960 in short i mean they are they are 667 00:25:26,549 --> 00:25:24,559 parental places where material from the 668 00:25:31,110 --> 00:25:26,559 subsurface is erupted onto the surface 669 00:25:34,549 --> 00:25:32,390 we'll take another question from the 670 00:25:36,470 --> 00:25:34,559 phone lines we have denise chao with 671 00:25:37,909 --> 00:25:36,480 space.com please go ahead with your 672 00:25:43,269 --> 00:25:37,919 question 673 00:25:45,830 --> 00:25:43,279 crash site um when you were looking at 674 00:25:48,070 --> 00:25:45,840 the the comparison images um i think it 675 00:25:50,549 --> 00:25:48,080 was maybe dr larson that said that um 676 00:25:51,909 --> 00:25:50,559 when the impactor had had hit the comet 677 00:25:54,870 --> 00:25:51,919 that it had all this material that sort 678 00:25:56,149 --> 00:25:54,880 of obscured the view in 2005 679 00:25:57,190 --> 00:25:56,159 when you're looking at the images from 680 00:26:00,710 --> 00:25:57,200 last night was there anything that 681 00:26:03,110 --> 00:26:00,720 surprised you about the impact site 682 00:26:05,190 --> 00:26:03,120 yeah i'll take that um yeah there was a 683 00:26:06,549 --> 00:26:05,200 surprise in the sense that you know you 684 00:26:08,230 --> 00:26:06,559 could have expected a crater that was 685 00:26:10,310 --> 00:26:08,240 very very well defined 686 00:26:11,830 --> 00:26:10,320 and the creator was more subdued than i 687 00:26:15,590 --> 00:26:11,840 think some of us thought 688 00:26:18,230 --> 00:26:15,600 but it was still uh basically what the 689 00:26:21,110 --> 00:26:18,240 the kind of the size that we expected 690 00:26:23,430 --> 00:26:21,120 um and i think the real point is is that 691 00:26:25,430 --> 00:26:23,440 it's consistent with what we saw in 2005 692 00:26:27,430 --> 00:26:25,440 with the ejector going up and then a 693 00:26:29,830 --> 00:26:27,440 component coming down 694 00:26:32,149 --> 00:26:29,840 and so in a way it partly buried itself 695 00:26:36,549 --> 00:26:32,159 and i think we saw that very clearly in 696 00:26:36,559 --> 00:26:40,710 trust us 697 00:26:43,750 --> 00:26:41,510 okay 698 00:26:45,029 --> 00:26:43,760 we're going to put up an image um it is 699 00:26:46,950 --> 00:26:45,039 the image that we do have in our 700 00:26:47,990 --> 00:26:46,960 broadcast system you can tell us if it's 701 00:26:49,590 --> 00:26:48,000 the image you want and just so 702 00:26:52,230 --> 00:26:49,600 everyone's clear the image that they 703 00:26:53,430 --> 00:26:52,240 wanted will be posted to the internet no 704 00:26:55,909 --> 00:26:53,440 matter what so you'll all see it does 705 00:26:59,029 --> 00:26:55,919 this one work for you yeah great okay 706 00:27:00,470 --> 00:26:59,039 i'll talk to the speed please 707 00:27:02,390 --> 00:27:00,480 there's several things in this image i 708 00:27:04,149 --> 00:27:02,400 wanted to point out one of them 709 00:27:06,310 --> 00:27:04,159 is that these are the two craters we're 710 00:27:09,029 --> 00:27:06,320 talking about the other thing is notice 711 00:27:10,950 --> 00:27:09,039 this feature that's here if you notice 712 00:27:12,470 --> 00:27:10,960 over here that feature is gone even 713 00:27:14,950 --> 00:27:12,480 though many other features you can 714 00:27:16,549 --> 00:27:14,960 identify you can easily identify 715 00:27:18,870 --> 00:27:16,559 the interesting thing is that these 716 00:27:21,350 --> 00:27:18,880 concentric circles represent 717 00:27:23,350 --> 00:27:21,360 our estimate of the crater rim and then 718 00:27:24,710 --> 00:27:23,360 the inner circle is an estimate of the 719 00:27:26,230 --> 00:27:24,720 crater floor 720 00:27:29,029 --> 00:27:26,240 you can barely see this but there's a 721 00:27:30,950 --> 00:27:29,039 little lit area on that side and a dark 722 00:27:33,110 --> 00:27:30,960 area on the other and that's the central 723 00:27:34,870 --> 00:27:33,120 mound where we think the material came 724 00:27:37,350 --> 00:27:34,880 down so 725 00:27:38,149 --> 00:27:37,360 we think we see the crater with a sunlit 726 00:27:40,389 --> 00:27:38,159 rim 727 00:27:42,630 --> 00:27:40,399 on that side or some wall on that side a 728 00:27:44,789 --> 00:27:42,640 small little bit of a shadow there and 729 00:27:46,070 --> 00:27:44,799 we see the mound on the floor this is 730 00:27:48,950 --> 00:27:46,080 kind of what you would expect for an 731 00:27:50,389 --> 00:27:48,960 oblique impact at an angle of 30 degrees 732 00:27:52,710 --> 00:27:50,399 with a lot of material that went up and 733 00:27:55,190 --> 00:27:52,720 came back down 734 00:27:57,430 --> 00:27:55,200 so the picture on the on one side is a 735 00:27:59,269 --> 00:27:57,440 deep impact yeah that's the deep impact 736 00:28:00,149 --> 00:27:59,279 view over here and that's the stardust 737 00:28:03,029 --> 00:28:00,159 next 738 00:28:05,110 --> 00:28:03,039 it's about 150 meters across 739 00:28:09,430 --> 00:28:05,120 is what the current estimate um but you 740 00:28:11,990 --> 00:28:10,549 all right we're going to go to another 741 00:28:14,310 --> 00:28:12,000 question on the phone line sky and 742 00:28:15,990 --> 00:28:14,320 telescope kelly beatty please go ahead 743 00:28:17,590 --> 00:28:16,000 okay thank you very much uh this is for 744 00:28:20,630 --> 00:28:17,600 pete schultz i guess pete i'm sure glad 745 00:28:22,470 --> 00:28:20,640 you're convinced um is the muted nature 746 00:28:24,230 --> 00:28:22,480 of this crater 747 00:28:26,470 --> 00:28:24,240 more muted than when you would have 748 00:28:29,510 --> 00:28:26,480 expected and are you anticipating 749 00:28:31,510 --> 00:28:29,520 finding a kind of mantling all over uh 750 00:28:33,590 --> 00:28:31,520 the comet's nucleus due to all the dust 751 00:28:35,029 --> 00:28:33,600 and debris that was ejected 752 00:28:36,870 --> 00:28:35,039 well two you know the two questions 753 00:28:37,750 --> 00:28:36,880 first is that 754 00:28:39,269 --> 00:28:37,760 you know 755 00:28:40,630 --> 00:28:39,279 one of the reasons for going back to see 756 00:28:42,149 --> 00:28:40,640 what the crater looked like you know 757 00:28:45,190 --> 00:28:42,159 there were some thoughts that maybe the 758 00:28:47,430 --> 00:28:45,200 creator would simply bury itself or that 759 00:28:49,990 --> 00:28:47,440 it would sort of collapse 760 00:28:51,990 --> 00:28:50,000 because of its formation 761 00:28:53,510 --> 00:28:52,000 in terms of the ejecta 762 00:28:55,590 --> 00:28:53,520 if that was all ice that could have 763 00:28:58,789 --> 00:28:55,600 sublimated away very quickly and 764 00:29:01,029 --> 00:28:58,799 completely by the time we got back to it 765 00:29:02,870 --> 00:29:01,039 so i think when we look at the stereo we 766 00:29:05,269 --> 00:29:02,880 can see this feature 767 00:29:07,190 --> 00:29:05,279 and we can see it in multiple images and 768 00:29:14,549 --> 00:29:07,200 so i think i feel very confident that we 769 00:29:19,029 --> 00:29:16,870 okay thanks um we have one more question 770 00:29:21,190 --> 00:29:19,039 on the phone lines leo enright from 771 00:29:23,590 --> 00:29:21,200 irish television please go ahead 772 00:29:25,590 --> 00:29:23,600 thanks very much uh i was just wondering 773 00:29:26,789 --> 00:29:25,600 about this low bait feature that has 774 00:29:28,950 --> 00:29:26,799 been 775 00:29:31,029 --> 00:29:28,960 mentioned several times is this 776 00:29:33,029 --> 00:29:31,039 advancing or retreating i think that was 777 00:29:35,029 --> 00:29:33,039 one of the questions that you wanted to 778 00:29:36,389 --> 00:29:35,039 answer 779 00:29:38,230 --> 00:29:36,399 that's an excellent question the 780 00:29:41,190 --> 00:29:38,240 question is about the bait feature we 781 00:29:43,669 --> 00:29:41,200 talked about is it eroding or increasing 782 00:29:45,510 --> 00:29:43,679 at the present time it is eroding so it 783 00:29:51,029 --> 00:29:45,520 was formed at some time past and since 784 00:29:56,870 --> 00:29:52,470 do we have any more questions from the 785 00:30:00,389 --> 00:29:58,470 no i'm going to do one last check to see 786 00:30:02,630 --> 00:30:00,399 if we have any new images if the control 787 00:30:04,950 --> 00:30:02,640 room can tell me no we are done those 788 00:30:06,950 --> 00:30:04,960 are all the images that we have but we 789 00:30:08,710 --> 00:30:06,960 will be posting new images and new 790 00:30:10,549 --> 00:30:08,720 products to the web all day long as 791 00:30:12,590 --> 00:30:10,559 those become available so please do 792 00:30:15,430 --> 00:30:12,600 visit 793 00:30:17,750 --> 00:30:15,440 www.nasa.gov you'll find links there to 794 00:30:19,590 --> 00:30:17,760 all of the images from this comment 795 00:30:21,350 --> 00:30:19,600 encounter we want to thank all of you 796 00:30:54,870 --> 00:30:21,360 for joining us today 797 00:30:54,880 --> 00:31:08,870 oh 798 00:31:08,880 --> 00:31:34,470 uh