1 00:00:00,790 --> 00:00:08,560 [Music] 2 00:00:13,970 --> 00:00:11,000 hello everyone so I'm going to sort of 3 00:00:15,530 --> 00:00:13,980 completely switch gears so I'm a 4 00:00:18,080 --> 00:00:15,540 master's student at Johns Hopkins 5 00:00:20,810 --> 00:00:18,090 studying bio informatics and I also work 6 00:00:23,840 --> 00:00:20,820 at Jet Propulsion lab under the 7 00:00:24,980 --> 00:00:23,850 planetary protection group and today I'm 8 00:00:28,130 --> 00:00:24,990 sort of not going to talk about either 9 00:00:30,620 --> 00:00:28,140 those things so we're going to talk 10 00:00:32,840 --> 00:00:30,630 about the organic detection in evaporite 11 00:00:37,729 --> 00:00:32,850 minerals and what that tells us about 12 00:00:40,340 --> 00:00:37,739 our search for biosignatures on Mars so 13 00:00:43,459 --> 00:00:40,350 sort of the purpose to track the 14 00:00:45,410 --> 00:00:43,469 microbiological changes that occur when 15 00:00:48,470 --> 00:00:45,420 going from an active biological system 16 00:00:52,119 --> 00:00:48,480 into these evaporite minerals prior to 17 00:00:55,430 --> 00:00:52,129 during and after evaporite of formation 18 00:00:58,010 --> 00:00:55,440 so the methods we employed so we extract 19 00:01:00,410 --> 00:00:58,020 the DNA from multiple samples and 20 00:01:03,799 --> 00:01:00,420 developed in-house validation techniques 21 00:01:06,800 --> 00:01:03,809 to confirm the extraction from hyper 22 00:01:08,780 --> 00:01:06,810 saline fluids as some of you may know 23 00:01:10,820 --> 00:01:08,790 that this might be difficult due to 24 00:01:13,700 --> 00:01:10,830 inhibitors that are present within the 25 00:01:16,370 --> 00:01:13,710 fluids and the minerals we also utilized 26 00:01:18,830 --> 00:01:16,380 Rahman datasets to compare the active 27 00:01:20,120 --> 00:01:18,840 biological information into the 28 00:01:23,060 --> 00:01:20,130 evaporite minerals and what we're 29 00:01:24,499 --> 00:01:23,070 detecting they're sort of the goals we 30 00:01:27,800 --> 00:01:24,509 want to quantify the preservation 31 00:01:30,109 --> 00:01:27,810 potential when going from an active 32 00:01:32,420 --> 00:01:30,119 system into evaporite minerals which may 33 00:01:35,120 --> 00:01:32,430 be Sol which may support active 34 00:01:37,910 --> 00:01:35,130 biological life or may sort of form 35 00:01:39,920 --> 00:01:37,920 dormant versions of the microorganisms 36 00:01:42,319 --> 00:01:39,930 that are present we also wanted to 37 00:01:44,300 --> 00:01:42,329 compare the sensitivity of these bio 38 00:01:48,410 --> 00:01:44,310 signatures and comparing multiple 39 00:01:49,880 --> 00:01:48,420 detection techniques within modern 40 00:01:54,200 --> 00:01:49,890 evaporites and what that looks like 41 00:01:55,399 --> 00:01:54,210 across a larger time scale so the three 42 00:01:57,440 --> 00:01:55,409 main questions that we looked at what 43 00:01:59,749 --> 00:01:57,450 would be the threshold of detection for 44 00:02:01,280 --> 00:01:59,759 both the bio signatures what the 45 00:02:03,440 --> 00:02:01,290 preservation looks like and what that 46 00:02:05,899 --> 00:02:03,450 looks like over a larger geological time 47 00:02:08,419 --> 00:02:05,909 scale so how much biology would you need 48 00:02:10,910 --> 00:02:08,429 in the active system to constitute a 49 00:02:13,680 --> 00:02:10,920 viable and detectable signal within the 50 00:02:15,810 --> 00:02:13,690 evaporite minerals sort of what what 51 00:02:19,170 --> 00:02:15,820 can get preserved from the active system 52 00:02:21,060 --> 00:02:19,180 and if there's any selection as to what 53 00:02:22,500 --> 00:02:21,070 is being selected and what is being 54 00:02:26,400 --> 00:02:22,510 preserved within the evaporite minerals 55 00:02:27,960 --> 00:02:26,410 for a longer time scale so the 56 00:02:30,540 --> 00:02:27,970 motivation behind this study this is 57 00:02:33,240 --> 00:02:30,550 chrism data from the Mars Reconnaissance 58 00:02:36,090 --> 00:02:33,250 Orbiter which is an orbiter on Mars that 59 00:02:38,610 --> 00:02:36,100 got there in 2006 so as you can see 60 00:02:41,370 --> 00:02:38,620 we've detected phyllosilicates silica 61 00:02:42,960 --> 00:02:41,380 chlorides carbonates and sulfates which 62 00:02:44,580 --> 00:02:42,970 is what we're what which is what I'm 63 00:02:49,050 --> 00:02:44,590 going to talk about so particularly 64 00:02:51,120 --> 00:02:49,060 gypsum and halite so this is the 65 00:02:52,800 --> 00:02:51,130 analogue site that we used to study 66 00:02:55,650 --> 00:02:52,810 these evaporite minerals to the north 67 00:02:58,260 --> 00:02:55,660 arm of the Great Salt Lake in Utah this 68 00:03:01,470 --> 00:02:58,270 is an active system supports a variety 69 00:03:03,240 --> 00:03:01,480 of microbial organisms and it is cut off 70 00:03:07,110 --> 00:03:03,250 from the south arm so it is a closed 71 00:03:09,120 --> 00:03:07,120 system and sort of the analogous site on 72 00:03:11,910 --> 00:03:09,130 Mars would be the Jazira crater where 73 00:03:13,460 --> 00:03:11,920 we've detected the presence of clays and 74 00:03:16,260 --> 00:03:13,470 sulfates 75 00:03:18,300 --> 00:03:16,270 again another analogous environment 76 00:03:20,010 --> 00:03:18,310 between what we studied and Mars so the 77 00:03:22,710 --> 00:03:20,020 gypsum crystals that we looked at and 78 00:03:24,900 --> 00:03:22,720 sort of the sulfate veins which are 79 00:03:27,180 --> 00:03:24,910 hydrated minerals that are present 80 00:03:32,640 --> 00:03:27,190 within Gale Crater on Mars and this is 81 00:03:35,190 --> 00:03:32,650 an image from MSL so sort of going 82 00:03:37,560 --> 00:03:35,200 through the various samples that we 83 00:03:40,550 --> 00:03:37,570 looked at so we focused on the hey light 84 00:03:42,930 --> 00:03:40,560 hopper crystals that are found here and 85 00:03:45,210 --> 00:03:42,940 particularly within these crystals we 86 00:03:47,699 --> 00:03:45,220 wanted to focus on the fluid inclusions 87 00:03:50,040 --> 00:03:47,709 within them so these may serve as sort 88 00:03:52,290 --> 00:03:50,050 of micro environments within the crystal 89 00:03:54,750 --> 00:03:52,300 that may support maybe even active 90 00:03:58,440 --> 00:03:54,760 metabolic some of these organisms that 91 00:04:00,060 --> 00:03:58,450 are being preserved here on the bottom 92 00:04:02,310 --> 00:04:00,070 these are the hey light terraces that 93 00:04:05,130 --> 00:04:02,320 were sampled so on the top you can see a 94 00:04:06,720 --> 00:04:05,140 much clearer white in comparison to the 95 00:04:09,390 --> 00:04:06,730 bottom that has sort of a pinkish color 96 00:04:11,760 --> 00:04:09,400 to it so the top we believe I mean you 97 00:04:13,920 --> 00:04:11,770 have the same sort of biology that's 98 00:04:16,349 --> 00:04:13,930 present within these two however the top 99 00:04:19,409 --> 00:04:16,359 is being irradiated by UV radiation and 100 00:04:22,020 --> 00:04:19,419 and we believe that that pigmentation 101 00:04:23,250 --> 00:04:22,030 loss is due to that although you can't 102 00:04:27,330 --> 00:04:23,260 see it in this image but underneath 103 00:04:27,930 --> 00:04:27,340 these pink crystal or the pink hey light 104 00:04:30,420 --> 00:04:27,940 Terrace 105 00:04:32,850 --> 00:04:30,430 there is sort of a pool of the lake 106 00:04:34,680 --> 00:04:32,860 water that is providing continual inputs 107 00:04:37,080 --> 00:04:34,690 into the formation of these evaporites 108 00:04:38,730 --> 00:04:37,090 so sort of looking at the microbiology 109 00:04:41,340 --> 00:04:38,740 that's present within the liquid and 110 00:04:44,700 --> 00:04:41,350 what we can extract from the evaporites 111 00:04:47,160 --> 00:04:44,710 can tell us what is being preserved the 112 00:04:50,550 --> 00:04:47,170 gypsum crystals on the right we also 113 00:04:52,350 --> 00:04:50,560 extracted DNA from these and again 114 00:04:54,270 --> 00:04:52,360 similar to the hey light hopper crystals 115 00:04:56,730 --> 00:04:54,280 we wanted to understand whether those 116 00:04:59,820 --> 00:04:56,740 clays which are being entombed within 117 00:05:02,850 --> 00:04:59,830 the gypsum crystals again provide a sort 118 00:05:04,770 --> 00:05:02,860 of safe haven for the microbial life 119 00:05:08,130 --> 00:05:04,780 that's being preserved within these as 120 00:05:10,230 --> 00:05:08,140 well as the potential bio signatures and 121 00:05:11,970 --> 00:05:10,240 then comparing that with in the 122 00:05:13,920 --> 00:05:11,980 unfiltered lake water as well as the 123 00:05:18,810 --> 00:05:13,930 environmental controls so the unfiltered 124 00:05:20,610 --> 00:05:18,820 lake water is home to active life and so 125 00:05:22,110 --> 00:05:20,620 looking at the sort of diversity and 126 00:05:25,500 --> 00:05:22,120 abundance that's present there in 127 00:05:27,680 --> 00:05:25,510 comparison to the crystals will allow us 128 00:05:30,420 --> 00:05:27,690 to understand what that preservation 129 00:05:34,080 --> 00:05:30,430 potential looks like the environmental 130 00:05:37,140 --> 00:05:34,090 controls sort of served as a baseline to 131 00:05:39,030 --> 00:05:37,150 understand whether or not any any of the 132 00:05:41,700 --> 00:05:39,040 surrounding sediment that's within the 133 00:05:45,300 --> 00:05:41,710 vicinity of these crystals had any 134 00:05:49,320 --> 00:05:45,310 inputs in terms of the microbial life 135 00:05:51,470 --> 00:05:49,330 that we're detecting so this is an 136 00:05:54,120 --> 00:05:51,480 overall map of sort of some of the most 137 00:05:58,170 --> 00:05:54,130 relevant biomolecules that we've looked 138 00:06:00,420 --> 00:05:58,180 at so DNA of course provides the most 139 00:06:02,040 --> 00:06:00,430 relevant information you can extract out 140 00:06:04,950 --> 00:06:02,050 the resistances that are present with 141 00:06:07,170 --> 00:06:04,960 indeed within these microorganisms their 142 00:06:09,500 --> 00:06:07,180 metabolic pathways you get down to 143 00:06:12,090 --> 00:06:09,510 species even strain level information 144 00:06:14,130 --> 00:06:12,100 however it is fairly a short-lived 145 00:06:16,470 --> 00:06:14,140 molecule in comparison to some of these 146 00:06:21,530 --> 00:06:16,480 others proteins which would be the 147 00:06:24,240 --> 00:06:21,540 active workers of the cell although 148 00:06:26,550 --> 00:06:24,250 those are that they do provide relevant 149 00:06:28,260 --> 00:06:26,560 information it is quite difficult to 150 00:06:30,810 --> 00:06:28,270 extract them and sort of relate them 151 00:06:32,960 --> 00:06:30,820 back to what species they came from 152 00:06:35,730 --> 00:06:32,970 within a mixed environmental sample 153 00:06:39,210 --> 00:06:35,740 similar to lipids where you have that 154 00:06:41,700 --> 00:06:39,220 limitation however these are viable over 155 00:06:43,980 --> 00:06:41,710 a larger geological time scale 156 00:06:45,540 --> 00:06:43,990 and then the total organic carbon which 157 00:06:48,720 --> 00:06:45,550 is the longest-lived and sort of 158 00:06:51,620 --> 00:06:48,730 comparing that as a robust bio signature 159 00:06:57,390 --> 00:06:51,630 back to DNA which would be our more 160 00:07:00,270 --> 00:06:57,400 relevant and highest resolution this is 161 00:07:02,430 --> 00:07:00,280 some of the preliminary data so we did 162 00:07:04,710 --> 00:07:02,440 extract DNA from these samples and we 163 00:07:06,450 --> 00:07:04,720 have sent them for sequencing to look at 164 00:07:09,930 --> 00:07:06,460 sort of the microbiome that's present 165 00:07:13,590 --> 00:07:09,940 across but we were able to extract DNA 166 00:07:16,230 --> 00:07:13,600 from all the samples so one thing to 167 00:07:18,330 --> 00:07:16,240 note is that this gypsum both the clay 168 00:07:21,270 --> 00:07:18,340 and non clay so we were able to target 169 00:07:23,850 --> 00:07:21,280 and take a core of just the clay and 170 00:07:25,980 --> 00:07:23,860 compare that back to the gypsum portions 171 00:07:30,300 --> 00:07:25,990 that didn't have that sediment entombed 172 00:07:31,890 --> 00:07:30,310 within them they do have much more DNA 173 00:07:34,530 --> 00:07:31,900 in comparison to some of these other 174 00:07:37,590 --> 00:07:34,540 samples including the active system and 175 00:07:41,070 --> 00:07:37,600 this is normalized down to a per gram or 176 00:07:43,740 --> 00:07:41,080 per ml of the material that we extracted 177 00:07:46,170 --> 00:07:43,750 from so although we know there's life 178 00:07:50,630 --> 00:07:46,180 here this is sort of a much more 179 00:07:53,010 --> 00:07:50,640 concentrated version of that lake water 180 00:07:56,250 --> 00:07:53,020 when you compare that to the sediment 181 00:07:58,290 --> 00:07:56,260 that's present the sediment is much more 182 00:08:01,440 --> 00:07:58,300 abundant in microbial life and and that 183 00:08:05,360 --> 00:08:01,450 makes sense because soil houses a great 184 00:08:07,410 --> 00:08:05,370 diversity of microbes and so 185 00:08:09,690 --> 00:08:07,420 understanding the microbial abundance 186 00:08:12,300 --> 00:08:09,700 present here we are able to track and 187 00:08:14,400 --> 00:08:12,310 parse out whether these had any inputs 188 00:08:17,630 --> 00:08:14,410 into the formation of the minerals and 189 00:08:20,900 --> 00:08:17,640 whether there's any crosstalk across 190 00:08:24,150 --> 00:08:20,910 this sort of the merged data of our 191 00:08:25,980 --> 00:08:24,160 various sample categories so we did 192 00:08:28,590 --> 00:08:25,990 sample multiple sites and replicates 193 00:08:30,780 --> 00:08:28,600 within those sites so you are again able 194 00:08:32,580 --> 00:08:30,790 to see that the lake water in comparison 195 00:08:35,520 --> 00:08:32,590 to the gypsum gypsum we're able to get 196 00:08:39,080 --> 00:08:35,530 much more DNA and environmental controls 197 00:08:42,660 --> 00:08:39,090 are still way above the evaporites 198 00:08:46,140 --> 00:08:42,670 system of the preliminary raman data we 199 00:08:48,810 --> 00:08:46,150 looked at so the main thing to note here 200 00:08:51,660 --> 00:08:48,820 is that the reference halo bacteria that 201 00:08:54,690 --> 00:08:51,670 we used this was a pure culture we did 202 00:08:55,260 --> 00:08:54,700 get similar peaks within that in 203 00:08:57,540 --> 00:08:55,270 comparison 204 00:08:59,640 --> 00:08:57,550 to the mixed environmental samples which 205 00:09:02,060 --> 00:08:59,650 tells us whatever we're detecting is 206 00:09:04,800 --> 00:09:02,070 sort of ubiquitously found across 207 00:09:06,990 --> 00:09:04,810 various different species because these 208 00:09:09,000 --> 00:09:07,000 may have multiple different species and 209 00:09:11,040 --> 00:09:09,010 this is a pure culture and we sort of 210 00:09:13,770 --> 00:09:11,050 trace that back to beta-carotene which 211 00:09:15,890 --> 00:09:13,780 was mentioned as something that comes up 212 00:09:18,290 --> 00:09:15,900 within Rahman data it's a carotenoid 213 00:09:24,120 --> 00:09:18,300 that some of these extreme affiliate 214 00:09:26,610 --> 00:09:24,130 organisms produce so in conclusion these 215 00:09:29,700 --> 00:09:26,620 evaporite minerals halite and gypsum do 216 00:09:31,920 --> 00:09:29,710 absolutely retain and preserve some of 217 00:09:36,990 --> 00:09:31,930 the biological material that's present 218 00:09:38,940 --> 00:09:37,000 within the lake system and in particular 219 00:09:41,040 --> 00:09:38,950 we wanted to focus on the fluid 220 00:09:43,860 --> 00:09:41,050 inclusions within the halite and the 221 00:09:47,130 --> 00:09:43,870 clay within the gypsum to see whether or 222 00:09:50,820 --> 00:09:47,140 not those have any selection as to what 223 00:09:53,840 --> 00:09:50,830 is being preserved within them on the 224 00:09:55,890 --> 00:09:53,850 right you see an image of using an FTIR 225 00:09:58,290 --> 00:09:55,900 spectrometer and this sort of the heat 226 00:10:00,780 --> 00:09:58,300 map that's overlaid onto the gypsum 227 00:10:02,190 --> 00:10:00,790 fluid inclusion which is here and this 228 00:10:05,250 --> 00:10:02,200 is sort of what the clay looks like 229 00:10:07,200 --> 00:10:05,260 that's entombed within the gypsum and so 230 00:10:09,420 --> 00:10:07,210 in the red here we're able to pinpoint 231 00:10:11,250 --> 00:10:09,430 the presence of the beta-carotene within 232 00:10:15,900 --> 00:10:11,260 that and start everythings radiating 233 00:10:17,490 --> 00:10:15,910 away from the beta-carotene the so the 234 00:10:19,410 --> 00:10:17,500 raman signature peaks from the halo 235 00:10:21,510 --> 00:10:19,420 bacteria in comparison to the mixed 236 00:10:25,290 --> 00:10:21,520 environmental samples where you have 237 00:10:27,270 --> 00:10:25,300 multiple organisms present do lead us to 238 00:10:29,370 --> 00:10:27,280 believe that we are detecting beta 239 00:10:31,890 --> 00:10:29,380 carotene within the environmental 240 00:10:33,660 --> 00:10:31,900 samples and this could be a diagnostic 241 00:10:35,940 --> 00:10:33,670 peak that could be used as a bio 242 00:10:39,120 --> 00:10:35,950 signature in the future and we may be 243 00:10:42,120 --> 00:10:39,130 able to use Kwan or this may be parsed 244 00:10:44,610 --> 00:10:42,130 out and and a quantitative data could be 245 00:10:46,860 --> 00:10:44,620 used within the Raman signatures to 246 00:10:48,750 --> 00:10:46,870 understand the abundance of the beta 247 00:10:51,630 --> 00:10:48,760 carotene and trace that back to sort of 248 00:10:55,920 --> 00:10:51,640 what we're seeing from the microbiome 249 00:10:57,360 --> 00:10:55,930 data and similarly same Raman so we're 250 00:10:59,910 --> 00:10:57,370 looking at the fluid inclusions again 251 00:11:03,720 --> 00:10:59,920 and pinpointing the presence of beta 252 00:11:05,760 --> 00:11:03,730 carotene these are the corona crystals 253 00:11:07,890 --> 00:11:05,770 that we looked at and these are hey 254 00:11:08,430 --> 00:11:07,900 light hopper crystals within this is 255 00:11:12,270 --> 00:11:08,440 about 256 00:11:14,490 --> 00:11:12,280 micron scale is a submicron using again 257 00:11:17,070 --> 00:11:14,500 FTIR imaging and looking at the fluid 258 00:11:22,090 --> 00:11:17,080 inclusions within these as well as well 259 00:11:33,740 --> 00:11:22,100 as the halide hopper crystals that's it 260 00:11:39,810 --> 00:11:37,500 hey thanks um great talk I have one 261 00:11:43,740 --> 00:11:39,820 comment actually opened up the north arm 262 00:11:46,770 --> 00:11:43,750 of the salt lake now um oh okay 263 00:11:48,090 --> 00:11:46,780 hi it was just recently last fall um but 264 00:11:50,640 --> 00:11:48,100 I was also wondering you might have 265 00:11:52,890 --> 00:11:50,650 grazed by this were you extracting DNA 266 00:11:54,420 --> 00:11:52,900 from your fluid inclusions to try to get 267 00:11:57,660 --> 00:11:54,430 microbial life inside of that fluid 268 00:11:59,820 --> 00:11:57,670 inclusion yeah so the the Clay's and non 269 00:12:01,320 --> 00:11:59,830 clays we were able to separate those and 270 00:12:02,880 --> 00:12:01,330 understand that differently but the 271 00:12:04,590 --> 00:12:02,890 fluid inclusions within the hey light is 272 00:12:07,440 --> 00:12:04,600 sort of something we're still developing 273 00:12:09,390 --> 00:12:07,450 as to how we can separate the fluid 274 00:12:11,220 --> 00:12:09,400 inclusions look at that separately from 275 00:12:13,260 --> 00:12:11,230 the halide crystals so we weren't able 276 00:12:15,510 --> 00:12:13,270 to do that okay so you haven't found a 277 00:12:16,110 --> 00:12:15,520 way to sterilize the outside yeah 278 00:12:20,520 --> 00:12:16,120 exactly 279 00:12:28,540 --> 00:12:20,530 okay yeah yep we have any other 280 00:12:32,300 --> 00:12:30,590 this is really awesome study I was 281 00:12:33,800 --> 00:12:32,310 wondering kind of are you gonna plan to 282 00:12:35,930 --> 00:12:33,810 look at these kind of with ExoMars or 283 00:12:37,730 --> 00:12:35,940 MSL as good technique because you've got 284 00:12:39,800 --> 00:12:37,740 a kind of Mars 2020 raman spectroscopy 285 00:12:41,060 --> 00:12:39,810 would like laser desorption all kind of 286 00:12:44,360 --> 00:12:41,070 pyrolysis so you plan to do those 287 00:12:47,360 --> 00:12:44,370 experiments yeah we are we are trying to 288 00:12:50,000 --> 00:12:47,370 look at multiple methods to sort of 289 00:12:52,400 --> 00:12:50,010 trace back what we can see our primary 290 00:12:55,580 --> 00:12:52,410 focus is looking at wet micro lab 291 00:12:57,800 --> 00:12:55,590 techniques so the DNA extraction can be 292 00:13:00,860 --> 00:12:57,810 done and within a lab setting and sort 293 00:13:02,330 --> 00:13:00,870 of mapping that onto the data that we 294 00:13:04,880 --> 00:13:02,340 can receive from an instrument that 295 00:13:07,310 --> 00:13:04,890 could be easily mounted onto a rover or 296 00:13:08,600 --> 00:13:07,320 an orbiter so that that's our primary 297 00:13:14,060 --> 00:13:08,610 focus but yeah that's something we're 298 00:13:17,300 --> 00:13:14,070 definitely looking at thanks cool if you 299 00:13:19,970 --> 00:13:17,310 have user so field Raman or just a lab 300 00:13:22,820 --> 00:13:19,980 laboratory rapid instruments it was a 301 00:13:24,140 --> 00:13:22,830 lab rahman okay yeah you plan to do you 302 00:13:26,360 --> 00:13:24,150 plan to go to the field to do that 303 00:13:29,090 --> 00:13:26,370 directly there to see how much you can 304 00:13:30,890 --> 00:13:29,100 detect or yeah the field round we are 305 00:13:33,050 --> 00:13:30,900 we're definitely looking at field Raman 306 00:13:38,210 --> 00:13:33,060 as well to see if there are any 307 00:13:40,460 --> 00:13:38,220 differences okay well with that let's