1 00:00:00,790 --> 00:00:07,320 [Music] 2 00:00:11,720 --> 00:00:09,129 [Applause] 3 00:00:13,459 --> 00:00:11,730 hi everyone I'm Elizabeth had a meal I'm 4 00:00:15,410 --> 00:00:13,469 gonna present the work that's being done 5 00:00:18,499 --> 00:00:15,420 on Micah which is a microfluidic I see 6 00:00:22,010 --> 00:00:18,509 world chemistry analyzer this is a 7 00:00:23,510 --> 00:00:22,020 collaboration between a couple of 8 00:00:25,729 --> 00:00:23,520 different NASA centers NASA aims to 9 00:00:30,200 --> 00:00:25,739 propulsion labs Tufts University Tony 10 00:00:32,690 --> 00:00:30,210 Rico is the PI on it and so mica is 11 00:00:34,880 --> 00:00:32,700 basically a combination between the 12 00:00:37,790 --> 00:00:34,890 heritage of the Phoenix wet chemistry 13 00:00:40,430 --> 00:00:37,800 labs which flew and and did some 14 00:00:41,930 --> 00:00:40,440 experiments on Mars back in 2008 and the 15 00:00:43,880 --> 00:00:41,940 work that's been done with micro 16 00:00:45,880 --> 00:00:43,890 fluidics on small satellites through 17 00:00:50,330 --> 00:00:45,890 Ames and together we're combining these 18 00:00:52,400 --> 00:00:50,340 ya into a basically a smaller version of 19 00:00:54,920 --> 00:00:52,410 the Phoenix wet chemistry labs that 20 00:00:59,139 --> 00:00:54,930 would might be useful on Europa Lander 21 00:01:01,580 --> 00:00:59,149 potential mission so the Europa Lander 22 00:01:04,160 --> 00:01:01,590 science definition team report came out 23 00:01:05,359 --> 00:01:04,170 with of course several different key 24 00:01:08,840 --> 00:01:05,369 science goals that they were interested 25 00:01:10,999 --> 00:01:08,850 in and we believe that the the mic 26 00:01:14,899 --> 00:01:11,009 instrument that we're building well not 27 00:01:16,879 --> 00:01:14,909 necessarily obviously going to address 28 00:01:20,809 --> 00:01:16,889 these it does have a very important role 29 00:01:22,489 --> 00:01:20,819 in them in it and the primary 30 00:01:23,899 --> 00:01:22,499 measurements that Myka is going to make 31 00:01:25,010 --> 00:01:23,909 our inorganic measurements just a little 32 00:01:26,419 --> 00:01:25,020 bit different from what a lot of other 33 00:01:29,840 --> 00:01:26,429 people are talking about here today 34 00:01:31,940 --> 00:01:29,850 it's an electro chemistry array that 35 00:01:33,800 --> 00:01:31,950 uses ion selective electrodes cyclical 36 00:01:36,379 --> 00:01:33,810 cemetry and chrono potentiometry and 37 00:01:38,739 --> 00:01:36,389 where it fits in in this this science 38 00:01:41,300 --> 00:01:38,749 definition team report is looking at 39 00:01:43,429 --> 00:01:41,310 characterizing the inorganic environment 40 00:01:45,879 --> 00:01:43,439 characterizing the sort of sources for 41 00:01:48,499 --> 00:01:45,889 energy that might be fueling these 42 00:01:50,840 --> 00:01:48,509 potential life forms looking at the 43 00:01:53,239 --> 00:01:50,850 habitability of the surface and just 44 00:01:57,289 --> 00:01:53,249 characterizing the chemical matrix in 45 00:01:59,209 --> 00:01:57,299 which the measurements will be taken and 46 00:02:00,769 --> 00:01:59,219 so all of this sort of stems from the 47 00:02:02,870 --> 00:02:00,779 Phoenix lander and so for those of you 48 00:02:05,089 --> 00:02:02,880 who maybe don't think about the Phoenix 49 00:02:06,499 --> 00:02:05,099 lander as often as some of us do I want 50 00:02:08,210 --> 00:02:06,509 to remind you exactly what the wet 51 00:02:10,070 --> 00:02:08,220 chemistry labs are and why they're 52 00:02:14,540 --> 00:02:10,080 actually a really great stepping stone 53 00:02:16,250 --> 00:02:14,550 for the Europa Lander so in 2008 the 54 00:02:17,839 --> 00:02:16,260 Phoenix lander landed on the northern 55 00:02:20,119 --> 00:02:17,849 plains of Mars and its mission was to 56 00:02:21,470 --> 00:02:20,129 assess the habitability of that site and 57 00:02:23,300 --> 00:02:21,480 it did that with 58 00:02:24,710 --> 00:02:23,310 different tools one of this was this 59 00:02:27,110 --> 00:02:24,720 microscopy electrochemistry and 60 00:02:29,479 --> 00:02:27,120 conductivity analyzer Mecca and what 61 00:02:31,970 --> 00:02:29,489 Mecca did was it had as part of it a 62 00:02:33,440 --> 00:02:31,980 series of four cells which were the wet 63 00:02:35,300 --> 00:02:33,450 chemistry labs and they were these 64 00:02:37,100 --> 00:02:35,310 electrochemical sensor arrays they 65 00:02:38,900 --> 00:02:37,110 included a suite of ion selective 66 00:02:41,530 --> 00:02:38,910 electrodes conductivity probes they 67 00:02:44,240 --> 00:02:41,540 sensed pH oxidation reduction potential 68 00:02:46,130 --> 00:02:44,250 and different oxidants in the soil and 69 00:02:48,289 --> 00:02:46,140 this was really the first time that on 70 00:02:51,020 --> 00:02:48,299 Mars we were able to characterize the 71 00:02:54,110 --> 00:02:51,030 the regul if in terms of these soluble 72 00:02:55,550 --> 00:02:54,120 species which was very important and in 73 00:02:57,289 --> 00:02:55,560 addition to having the success of 74 00:02:58,580 --> 00:02:57,299 actually measuring the primary cations 75 00:03:00,680 --> 00:02:58,590 that were in the soil and really giving 76 00:03:03,259 --> 00:03:00,690 us a context for that in measure pH for 77 00:03:05,809 --> 00:03:03,269 the first time and it detected 78 00:03:07,309 --> 00:03:05,819 perchlorate in the surface for the first 79 00:03:09,199 --> 00:03:07,319 time and this was a really really really 80 00:03:12,199 --> 00:03:09,209 important contribution to how we 81 00:03:13,339 --> 00:03:12,209 understand Mars so before this you know 82 00:03:15,020 --> 00:03:13,349 we had always expected there to be 83 00:03:16,250 --> 00:03:15,030 organic molecules and we'd go and we'd 84 00:03:19,190 --> 00:03:16,260 measure and they weren't there and we 85 00:03:20,809 --> 00:03:19,200 were all like what is happening and so 86 00:03:22,759 --> 00:03:20,819 when when Phoenix showed up and they 87 00:03:24,349 --> 00:03:22,769 actually measured what was in the soil 88 00:03:25,610 --> 00:03:24,359 they measured what was in the matrix of 89 00:03:27,800 --> 00:03:25,620 the sample that they were trying to 90 00:03:29,740 --> 00:03:27,810 detect these organics in they found this 91 00:03:31,729 --> 00:03:29,750 molecule called perchlorate and 92 00:03:32,900 --> 00:03:31,739 perchlorate is interesting because if 93 00:03:34,250 --> 00:03:32,910 you heat it up in the presence of 94 00:03:35,569 --> 00:03:34,260 organics which you get are a bunch of 95 00:03:37,809 --> 00:03:35,579 combusted organics and you don't 96 00:03:40,640 --> 00:03:37,819 actually see what you wanted to see so 97 00:03:42,530 --> 00:03:40,650 you know since then curiosity is then 98 00:03:44,629 --> 00:03:42,540 confirmed the presence of organic with 99 00:03:46,339 --> 00:03:44,639 this oxygen evolution peak so when 100 00:03:48,440 --> 00:03:46,349 perchlorate degrades when you heat it up 101 00:03:50,180 --> 00:03:48,450 it has this oxygen evolution peak and it 102 00:03:51,650 --> 00:03:50,190 explains why we were really for a long 103 00:03:53,300 --> 00:03:51,660 time only getting these very small 104 00:03:54,890 --> 00:03:53,310 chlorinated organics and it wasn't until 105 00:03:56,990 --> 00:03:54,900 very recently that we started to detect 106 00:03:58,430 --> 00:03:57,000 other things where we could search in 107 00:04:00,199 --> 00:03:58,440 environments that maybe perchlorate 108 00:04:01,759 --> 00:04:00,209 wasn't as abundant and what I'm trying 109 00:04:03,920 --> 00:04:01,769 to emphasize here is the importance of 110 00:04:05,569 --> 00:04:03,930 measuring even this inorganic matrix 111 00:04:07,220 --> 00:04:05,579 before you start doing these incredibly 112 00:04:09,140 --> 00:04:07,230 complicated awesome techniques that can 113 00:04:10,490 --> 00:04:09,150 maybe detect really low levels of 114 00:04:12,559 --> 00:04:10,500 organics and all of that but if you 115 00:04:14,990 --> 00:04:12,569 don't understand your chemical matrix at 116 00:04:16,759 --> 00:04:15,000 the base level then you could be missing 117 00:04:20,199 --> 00:04:16,769 something very obvious and now you've 118 00:04:23,629 --> 00:04:20,209 wasted all of this time and energy - and 119 00:04:25,370 --> 00:04:23,639 - because you just simply didn't test 120 00:04:27,770 --> 00:04:25,380 your your your matrix and this is really 121 00:04:30,050 --> 00:04:27,780 a first step in any basic laboratory 122 00:04:34,110 --> 00:04:30,060 analysis you know test your pH test 123 00:04:36,240 --> 00:04:34,120 what's in there and so we know that we 124 00:04:38,129 --> 00:04:36,250 did a really excellent job on Mars but 125 00:04:39,780 --> 00:04:38,139 there are different challenges for going 126 00:04:42,900 --> 00:04:39,790 forward on Europa and so we've been 127 00:04:43,980 --> 00:04:42,910 developing these sensors to test them to 128 00:04:45,870 --> 00:04:43,990 make sure that they will be robust 129 00:04:47,670 --> 00:04:45,880 enough to handle the environments that 130 00:04:49,950 --> 00:04:47,680 we expect on Europa and the first of 131 00:04:51,960 --> 00:04:49,960 those tests was the radiation dose so 132 00:04:53,460 --> 00:04:51,970 the radiation on Europa is much larger 133 00:04:55,020 --> 00:04:53,470 than the radiation on Mars and so we've 134 00:04:58,260 --> 00:04:55,030 been testing at this 300 killer ad 135 00:05:00,900 --> 00:04:58,270 totalized an ionization dose because the 136 00:05:02,670 --> 00:05:00,910 molecules that do sort of the heavy 137 00:05:04,500 --> 00:05:02,680 lifting and ion selective electrode are 138 00:05:06,180 --> 00:05:04,510 actually small organic molecules and so 139 00:05:07,260 --> 00:05:06,190 one of our concerns was that if they 140 00:05:09,200 --> 00:05:07,270 couldn't handle the higher radiation 141 00:05:11,730 --> 00:05:09,210 that there would be a problem and so we 142 00:05:14,189 --> 00:05:11,740 did some measurements we calibrated them 143 00:05:16,080 --> 00:05:14,199 and we compared them before and after 144 00:05:17,400 --> 00:05:16,090 this 300 kilo rad total radiation dose 145 00:05:19,529 --> 00:05:17,410 and we found that at least for the ones 146 00:05:20,760 --> 00:05:19,539 that we've tested so far there doesn't 147 00:05:22,890 --> 00:05:20,770 really seem to be a loss of performance 148 00:05:26,700 --> 00:05:22,900 so it looks like that high radiation 149 00:05:28,140 --> 00:05:26,710 environment doesn't seem to be going to 150 00:05:30,900 --> 00:05:28,150 be too much of a problem for at least 151 00:05:32,070 --> 00:05:30,910 these potentially these organic 152 00:05:34,770 --> 00:05:32,080 molecules that we put in our our 153 00:05:36,870 --> 00:05:34,780 membranes the second is the lifetime so 154 00:05:38,790 --> 00:05:36,880 Mars is a lot closer than Europa and so 155 00:05:41,430 --> 00:05:38,800 if we're looking at a 10-year flight 156 00:05:42,839 --> 00:05:41,440 mission we just wanted to make sure that 157 00:05:44,520 --> 00:05:42,849 these electrodes would still function 158 00:05:46,050 --> 00:05:44,530 when we got there and this was one of 159 00:05:47,610 --> 00:05:46,060 the great things about using a heritage 160 00:05:49,890 --> 00:05:47,620 technology is we actually had an 161 00:05:52,350 --> 00:05:49,900 original flight spare beaker that back 162 00:05:54,540 --> 00:05:52,360 in 2007 they sealed up put in a freezer 163 00:05:56,159 --> 00:05:54,550 and forgot about for 10 years and then 164 00:05:58,529 --> 00:05:56,169 we said well would this work if we got 165 00:06:00,210 --> 00:05:58,539 to Europa in 10 years it was very easy 166 00:06:01,920 --> 00:06:00,220 to test we just opened up the beaker and 167 00:06:03,960 --> 00:06:01,930 we did the calibration again and you can 168 00:06:05,939 --> 00:06:03,970 see before and after the the calibration 169 00:06:07,439 --> 00:06:05,949 the sensitivity hasn't really changed 170 00:06:09,210 --> 00:06:07,449 over time so they definitely do have a 171 00:06:11,909 --> 00:06:09,220 demonstrated actual 10-year 172 00:06:15,659 --> 00:06:11,919 survivability which was pretty exciting 173 00:06:17,400 --> 00:06:15,669 for us to learn and then the next thing 174 00:06:19,230 --> 00:06:17,410 that we wanted to know is you know the 175 00:06:21,750 --> 00:06:19,240 original wickel beakers use 25 176 00:06:24,150 --> 00:06:21,760 milliliters of water and that's a that's 177 00:06:25,350 --> 00:06:24,160 a lot of water for Europa and so we 178 00:06:27,270 --> 00:06:25,360 wanted to make sure that these would 179 00:06:29,850 --> 00:06:27,280 still function if we reduce that sample 180 00:06:31,950 --> 00:06:29,860 volume down to the micro liter level so 181 00:06:34,230 --> 00:06:31,960 we took the original form factor of the 182 00:06:36,629 --> 00:06:34,240 Wicklow electrodes and we put them into 183 00:06:40,409 --> 00:06:36,639 a sort of microfluidic channel so this 184 00:06:43,560 --> 00:06:40,419 is 14 electrodes in a total channel 185 00:06:44,700 --> 00:06:43,570 volume of 100 microliters and we tested 186 00:06:46,620 --> 00:06:44,710 to see whether or not the performance 187 00:06:47,480 --> 00:06:46,630 change going from a beaker with a large 188 00:06:48,950 --> 00:06:47,490 volume to 189 00:06:51,020 --> 00:06:48,960 this manifold with a small volume and as 190 00:06:53,480 --> 00:06:51,030 you can tell the performance actually 191 00:06:56,390 --> 00:06:53,490 stays pretty good and novita had a 192 00:06:57,830 --> 00:06:56,400 poster on what was that Monday about 193 00:06:59,659 --> 00:06:57,840 that I'm sure it's still up if you are 194 00:07:00,950 --> 00:06:59,669 interested or you can find her and chat 195 00:07:03,290 --> 00:07:00,960 about it and she's been doing more work 196 00:07:05,420 --> 00:07:03,300 testing the different components to make 197 00:07:09,320 --> 00:07:05,430 sure that these manifolds still still 198 00:07:10,520 --> 00:07:09,330 hold up and there were you know going 199 00:07:13,249 --> 00:07:10,530 forward it's nice to know that these 200 00:07:14,689 --> 00:07:13,259 heritage kind of electrodes actually do 201 00:07:16,100 --> 00:07:14,699 function and they would be useful on 202 00:07:17,480 --> 00:07:16,110 Europe and we could still get the same 203 00:07:19,730 --> 00:07:17,490 kind of excellent science return that we 204 00:07:20,960 --> 00:07:19,740 got from Phoenix using them but we 205 00:07:22,640 --> 00:07:20,970 wanted to make sure that we weren't 206 00:07:23,570 --> 00:07:22,650 missing anything so it's been a while 207 00:07:25,790 --> 00:07:23,580 since Phoenix and there have been 208 00:07:27,499 --> 00:07:25,800 amazing technology advances since then 209 00:07:29,390 --> 00:07:27,509 and so we sort of started looking at 210 00:07:30,920 --> 00:07:29,400 what the next generation of these ion 211 00:07:32,570 --> 00:07:30,930 selective electrodes looks like and so 212 00:07:35,059 --> 00:07:32,580 we started comparing the heritage local 213 00:07:36,860 --> 00:07:35,069 ones which are here to the Salt contact 214 00:07:38,659 --> 00:07:36,870 ones to see if there would be a benefit 215 00:07:40,820 --> 00:07:38,669 and maybe sacrificing a little TRL to 216 00:07:42,980 --> 00:07:40,830 get some benefit later on or whether or 217 00:07:44,420 --> 00:07:42,990 not it's it's better just to stick with 218 00:07:46,399 --> 00:07:44,430 the Heritage and so what we're mainly 219 00:07:49,700 --> 00:07:46,409 comparing here is the original heritage 220 00:07:51,050 --> 00:07:49,710 design it uses a hydrogel inner filling 221 00:07:53,180 --> 00:07:51,060 solution in order to do its main 222 00:07:55,100 --> 00:07:53,190 transduction from an ionic signal to an 223 00:07:57,170 --> 00:07:55,110 electronic one and while we know it can 224 00:07:58,909 --> 00:07:57,180 survive ten years of storage and we've 225 00:08:00,529 --> 00:07:58,919 done some dry storage testing which also 226 00:08:02,450 --> 00:08:00,539 kind of confirms that we can bring them 227 00:08:03,589 --> 00:08:02,460 back to life after drawing them out we 228 00:08:05,689 --> 00:08:03,599 wanted to know whether or not there 229 00:08:06,830 --> 00:08:05,699 would be benefit in eliminating that one 230 00:08:08,810 --> 00:08:06,840 of the benefits to eliminating that 231 00:08:10,370 --> 00:08:08,820 aside from just potentially adding a 232 00:08:12,260 --> 00:08:10,380 stability and survivability would be 233 00:08:14,300 --> 00:08:12,270 that we can reduce the size so this six 234 00:08:16,760 --> 00:08:14,310 millimeter size is kind of the limit if 235 00:08:17,839 --> 00:08:16,770 you're using that hydrogel but with by 236 00:08:19,700 --> 00:08:17,849 getting rid of it and using a 237 00:08:23,120 --> 00:08:19,710 carbon-based material which uses a 238 00:08:24,499 --> 00:08:23,130 capacitive transduction mechanism 239 00:08:26,390 --> 00:08:24,509 instead of a redox based one we're able 240 00:08:28,010 --> 00:08:26,400 to get it down to two millimeters so we 241 00:08:30,230 --> 00:08:28,020 could possibly fit more of them into a 242 00:08:32,839 --> 00:08:30,240 smaller array and we've been developing 243 00:08:34,430 --> 00:08:32,849 these well really there's been a lot of 244 00:08:36,889 --> 00:08:34,440 iterations of developing these solid 245 00:08:38,389 --> 00:08:36,899 contact ones since since the original 246 00:08:39,829 --> 00:08:38,399 Phoenix mission and this is sort of the 247 00:08:43,010 --> 00:08:39,839 most recent one so we have this two 248 00:08:46,160 --> 00:08:43,020 millimeter diameter using a graphene 249 00:08:47,930 --> 00:08:46,170 oxide carbon nanotube based transduction 250 00:08:50,120 --> 00:08:47,940 level and we've sort of are currently 251 00:08:52,850 --> 00:08:50,130 testing it in this small form-factor 252 00:08:54,889 --> 00:08:52,860 microfluidic array that includes 253 00:08:57,079 --> 00:08:54,899 calibration reservoirs and things of 254 00:08:58,579 --> 00:08:57,089 that nature and conductivity in testing 255 00:09:01,140 --> 00:08:58,589 it in this manner to see how it performs 256 00:09:03,120 --> 00:09:01,150 and so far it's performing just as well 257 00:09:04,890 --> 00:09:03,130 the original heritage ones which is 258 00:09:07,710 --> 00:09:04,900 which is excellent 259 00:09:09,990 --> 00:09:07,720 we were also wanted to address some of 260 00:09:11,730 --> 00:09:10,000 the some of the ions that we didn't 261 00:09:16,230 --> 00:09:11,740 actually measure when we were on Phoenix 262 00:09:18,150 --> 00:09:16,240 so ICS are really excellent at cations 263 00:09:20,490 --> 00:09:18,160 and then things get a little fuzzier 264 00:09:21,780 --> 00:09:20,500 when you go to anions and so what we 265 00:09:23,550 --> 00:09:21,790 were able to tech perchlorate to there 266 00:09:24,960 --> 00:09:23,560 are interferences and detecting becau 267 00:09:26,220 --> 00:09:24,970 right meant we couldn't detect a nitrate 268 00:09:29,610 --> 00:09:26,230 and so we've been developing techniques 269 00:09:31,170 --> 00:09:29,620 using the same types of electronics and 270 00:09:32,430 --> 00:09:31,180 electrodes that were in the original one 271 00:09:33,780 --> 00:09:32,440 we've been just sort of developing 272 00:09:35,760 --> 00:09:33,790 methods that would allow us to tailor 273 00:09:38,190 --> 00:09:35,770 that to detect other things and so 274 00:09:39,990 --> 00:09:38,200 here's an example of some CV which was 275 00:09:42,300 --> 00:09:40,000 on board the original Phoenix I'm using 276 00:09:44,280 --> 00:09:42,310 a silver electrode to detect nitrate you 277 00:09:45,570 --> 00:09:44,290 can see that the peak here varies with 278 00:09:47,940 --> 00:09:45,580 concentration and you can actually 279 00:09:49,620 --> 00:09:47,950 measure your nitrate based on that and 280 00:09:51,810 --> 00:09:49,630 we did a similar thing with sulfate and 281 00:09:54,150 --> 00:09:51,820 the led electrode where you can see that 282 00:09:56,460 --> 00:09:54,160 we can vary the concentration and get 283 00:09:58,470 --> 00:09:56,470 some potentially quantifying information 284 00:10:02,390 --> 00:09:58,480 about these these anions that might be 285 00:10:04,440 --> 00:10:02,400 swamped by other signals in the IOC's 286 00:10:05,790 --> 00:10:04,450 and so we've taken all of these 287 00:10:09,240 --> 00:10:05,800 wonderful developments for the the 288 00:10:10,650 --> 00:10:09,250 wickel heritage electrochemistry array 289 00:10:12,150 --> 00:10:10,660 and we're sort of coupling it with the 290 00:10:13,580 --> 00:10:12,160 knowledge at NASA Ames with their 291 00:10:17,610 --> 00:10:13,590 microfluidic so they've been doing these 292 00:10:20,130 --> 00:10:17,620 small satellite microfluidic devices for 293 00:10:22,800 --> 00:10:20,140 years and I'm not going to talk too much 294 00:10:25,410 --> 00:10:22,810 about that because someone else can talk 295 00:10:27,510 --> 00:10:25,420 about it later if they feel like it but 296 00:10:29,670 --> 00:10:27,520 we sort of brought these together and 297 00:10:31,620 --> 00:10:29,680 and put it in this splice which was 298 00:10:33,180 --> 00:10:31,630 talked about I was funded under cold 299 00:10:36,660 --> 00:10:33,190 tech funding I think Leslie talked about 300 00:10:37,560 --> 00:10:36,670 it on Tuesday I believe and this was 301 00:10:38,880 --> 00:10:37,570 sort of built and it has these 302 00:10:42,930 --> 00:10:38,890 connections where I can integrate with 303 00:10:44,460 --> 00:10:42,940 this this these at this M wickel are 304 00:10:45,720 --> 00:10:44,470 these these sort of microfluidic wickel 305 00:10:47,390 --> 00:10:45,730 devices that we've been building so 306 00:10:49,950 --> 00:10:47,400 we've been sort of testing it like that 307 00:10:51,270 --> 00:10:49,960 for a while and then this all comes 308 00:10:52,830 --> 00:10:51,280 together eventually in all of this 309 00:10:54,930 --> 00:10:52,840 knowledge and experience in this sort of 310 00:10:56,220 --> 00:10:54,940 heritage and high TRL work that we've 311 00:10:58,410 --> 00:10:56,230 been doing comes together in these 312 00:11:00,960 --> 00:10:58,420 actual proposed mica systems so we have 313 00:11:02,520 --> 00:11:00,970 a sealing door and a sample handling 314 00:11:06,030 --> 00:11:02,530 that's being developed by honeybee 315 00:11:07,320 --> 00:11:06,040 that'll allow us to have the meet the 316 00:11:08,850 --> 00:11:07,330 requirements that we need for that we 317 00:11:10,800 --> 00:11:08,860 have our calibrations our water 318 00:11:12,329 --> 00:11:10,810 reservoir our electrochemical sensor 319 00:11:14,129 --> 00:11:12,339 right here if here is Siri 320 00:11:16,170 --> 00:11:14,139 pumps and valves all of them and all of 321 00:11:19,410 --> 00:11:16,180 these are meant to fit into a design 322 00:11:22,350 --> 00:11:19,420 that is about you know 10 centimeters by 323 00:11:23,639 --> 00:11:22,360 17 by 11 and a half and it's basically 324 00:11:27,329 --> 00:11:23,649 going to fit into one of these smaller 325 00:11:30,329 --> 00:11:27,339 sections of the the proposed Europa 326 00:11:32,519 --> 00:11:30,339 Lander and so this is the current CAD 327 00:11:34,049 --> 00:11:32,529 design that we're working up and we're 328 00:11:35,519 --> 00:11:34,059 actually getting printed a I don't want 329 00:11:37,710 --> 00:11:35,529 to say as we speak but sometime in the 330 00:11:39,929 --> 00:11:37,720 not-too-distant future for integration 331 00:11:41,429 --> 00:11:39,939 and testing of all of these final are 332 00:11:43,829 --> 00:11:41,439 these these initial designs that we've 333 00:11:44,910 --> 00:11:43,839 been we've been doing and so with that I 334 00:11:46,379 --> 00:11:44,920 just want to run through these 335 00:11:48,360 --> 00:11:46,389 conclusions real quick so we have these 336 00:11:50,309 --> 00:11:48,370 electrochemistry measurements that are 337 00:11:52,199 --> 00:11:50,319 really well-suited to to address things 338 00:11:53,699 --> 00:11:52,209 like habitability and sample site 339 00:11:55,049 --> 00:11:53,709 characterization which is incredibly 340 00:11:56,730 --> 00:11:55,059 important when you're going to a place 341 00:11:58,679 --> 00:11:56,740 for the first time to do sort of 342 00:12:00,660 --> 00:11:58,689 complicated measurements and it really 343 00:12:04,379 --> 00:12:00,670 incorporates a lot of really high TRL 344 00:12:05,549 --> 00:12:04,389 Flight heritage devices which makes it 345 00:12:07,350 --> 00:12:05,559 what makes it a really promising 346 00:12:09,210 --> 00:12:07,360 technology and has been built off of 347 00:12:10,530 --> 00:12:09,220 funding from cold techs and things like 348 00:12:11,639 --> 00:12:10,540 that that have been basically bringing 349 00:12:14,340 --> 00:12:11,649 all of this together 350 00:12:15,840 --> 00:12:14,350 since the start of it and that we're at 351 00:12:17,549 --> 00:12:15,850 the stage where we're about to actually 352 00:12:36,569 --> 00:12:17,559 integrate all of these things and test 353 00:12:41,090 --> 00:12:36,579 them finally so in question I was really 354 00:12:42,210 --> 00:12:41,100 intrigued by your use of the the Phoenix 355 00:12:43,319 --> 00:12:42,220 parts 356 00:12:47,150 --> 00:12:43,329 was there anything else that you 357 00:12:49,679 --> 00:12:47,160 cannibalized that stood the test of time 358 00:12:51,269 --> 00:12:49,689 well yeah so the spare flake because you 359 00:12:52,710 --> 00:12:51,279 know it's it's funny that box sits in 360 00:12:53,939 --> 00:12:52,720 the freezer for a while and it takes up 361 00:12:55,679 --> 00:12:53,949 a lot of space and then it comes very 362 00:12:57,439 --> 00:12:55,689 useful I'm in that respect if there's 363 00:12:59,460 --> 00:12:57,449 anything else from them that we're using 364 00:13:01,559 --> 00:12:59,470 specifically from Phoenix I'm not sure 365 00:13:03,239 --> 00:13:01,569 because that was really optimized for 366 00:13:04,889 --> 00:13:03,249 taking soil and mixing it with water 367 00:13:06,360 --> 00:13:04,899 right and here we're expecting to be 368 00:13:07,919 --> 00:13:06,370 able to sort of maybe melt our sample 369 00:13:10,499 --> 00:13:07,929 and we don't need to do as much in the 370 00:13:12,030 --> 00:13:10,509 mixing so from there we have a few a few 371 00:13:16,390 --> 00:13:12,040 tweaks which is a micro fluidics part of 372 00:13:18,319 --> 00:13:16,400 it but yeah cool nice work 373 00:13:18,520 --> 00:13:18,329 [Music]