1 00:00:00,790 --> 00:00:07,320 [Music] 2 00:00:12,920 --> 00:00:09,580 [Applause] 3 00:00:15,410 --> 00:00:12,930 time and again we have been bowled over 4 00:00:17,900 --> 00:00:15,420 by the indescribable foreignness of 5 00:00:19,430 --> 00:00:17,910 other worlds and I wanted to take a few 6 00:00:22,609 --> 00:00:19,440 minutes this morning just to talk about 7 00:00:26,359 --> 00:00:22,619 the idea of looking for life as we don't 8 00:00:28,819 --> 00:00:26,369 know it so picking up where Dave left 9 00:00:30,700 --> 00:00:28,829 off I would argue that looking for life 10 00:00:33,140 --> 00:00:30,710 as we do know it has been a terrific 11 00:00:36,050 --> 00:00:33,150 starting point as we've gotten our feet 12 00:00:38,030 --> 00:00:36,060 wet with astrobiology especially for a 13 00:00:40,250 --> 00:00:38,040 planet like Mars we're never gonna find 14 00:00:42,349 --> 00:00:40,260 another planet more similar to earth in 15 00:00:44,510 --> 00:00:42,359 the solar system Mars and Earth had 16 00:00:46,819 --> 00:00:44,520 these thick carbon dioxide atmospheres 17 00:00:49,819 --> 00:00:46,829 protective magnetic fields silicate 18 00:00:51,830 --> 00:00:49,829 crust at least some episodic water early 19 00:00:54,410 --> 00:00:51,840 in their histories around the time life 20 00:00:56,779 --> 00:00:54,420 was getting started here on earth and we 21 00:00:59,000 --> 00:00:56,789 know that up to a billion tons of rocks 22 00:01:00,619 --> 00:00:59,010 were likely exchanged early in the 23 00:01:02,060 --> 00:01:00,629 histories and there's a possibility that 24 00:01:04,610 --> 00:01:02,070 we could have just kind of caught life 25 00:01:06,520 --> 00:01:04,620 from the next planet over that life on 26 00:01:10,640 --> 00:01:06,530 earth and life on Mars might be 27 00:01:12,740 --> 00:01:10,650 ancestrally related and we've developed 28 00:01:15,200 --> 00:01:12,750 as Dave mentioned these really robust 29 00:01:16,249 --> 00:01:15,210 approaches for Terran life detection we 30 00:01:18,880 --> 00:01:16,259 know how to look for these 31 00:01:21,679 --> 00:01:18,890 well-established widely accepted 32 00:01:23,870 --> 00:01:21,689 identified NT fires of biologic 33 00:01:26,179 --> 00:01:23,880 processes and because we're starting 34 00:01:28,580 --> 00:01:26,189 with what we know it's a lot easier to 35 00:01:31,010 --> 00:01:28,590 interpret the data we've got signals 36 00:01:32,780 --> 00:01:31,020 that can be very rich and information 37 00:01:34,999 --> 00:01:32,790 and importantly I think we have much 38 00:01:37,850 --> 00:01:35,009 stronger understanding of taphonomy what 39 00:01:39,590 --> 00:01:37,860 happens when an organism dies you know 40 00:01:41,030 --> 00:01:39,600 we might not find a dinosaur in the 41 00:01:43,580 --> 00:01:41,040 rocky mountains but we don't have to 42 00:01:45,730 --> 00:01:43,590 because we can find a dinosaur bone and 43 00:01:48,260 --> 00:01:45,740 the same thing is true with molecular 44 00:01:50,359 --> 00:01:48,270 fossilization we can even if we lose a 45 00:01:55,039 --> 00:01:50,369 bunch of functional groups we can still 46 00:01:58,100 --> 00:01:55,049 identify what was once there but as we 47 00:01:59,569 --> 00:01:58,110 expand deeper into the solar system I 48 00:02:01,819 --> 00:01:59,579 think it's really important that we're 49 00:02:04,100 --> 00:02:01,829 thinking about these new targets and the 50 00:02:06,289 --> 00:02:04,110 possibilities for life there and the 51 00:02:08,600 --> 00:02:06,299 ideas of developing tools and techniques 52 00:02:09,740 --> 00:02:08,610 that that go beyond just life as we know 53 00:02:12,620 --> 00:02:09,750 it I think are gonna be especially 54 00:02:14,660 --> 00:02:12,630 important we've got a whole bevy of new 55 00:02:16,610 --> 00:02:14,670 moons that we are suddenly able to 56 00:02:19,040 --> 00:02:16,620 target much more sophisticated ly with 57 00:02:20,220 --> 00:02:19,050 these new solar propulsion technologies 58 00:02:23,400 --> 00:02:20,230 huge rockets 59 00:02:25,949 --> 00:02:23,410 the SLS and when we think about you know 60 00:02:28,320 --> 00:02:25,959 what might the same molecular building 61 00:02:30,509 --> 00:02:28,330 blocks of life in a world like Titan 62 00:02:31,860 --> 00:02:30,519 look like where water's not even your 63 00:02:33,839 --> 00:02:31,870 solvent you know you've got these 64 00:02:37,410 --> 00:02:33,849 hydrocarbon lakes as seen in this 65 00:02:41,220 --> 00:02:37,420 Cassini radar image we just need to 66 00:02:43,380 --> 00:02:41,230 think broader so NASA is recently funded 67 00:02:45,509 --> 00:02:43,390 through its astrobiology program a team 68 00:02:48,600 --> 00:02:45,519 of investigators called the laboratory 69 00:02:50,190 --> 00:02:48,610 for agnostic bio signatures or a lab and 70 00:02:52,110 --> 00:02:50,200 I just wanted to talk through a few 71 00:02:55,440 --> 00:02:52,120 examples of the things that we're 72 00:02:57,780 --> 00:02:55,450 working on to target these agnostic bio 73 00:02:59,309 --> 00:02:57,790 signatures and just to be clear when I 74 00:03:00,839 --> 00:02:59,319 say agnostic what what I'm really 75 00:03:04,979 --> 00:03:00,849 talking about is without presupposing 76 00:03:07,559 --> 00:03:04,989 any underlying biochemistry any 77 00:03:08,789 --> 00:03:07,569 particular molecular framework so not 78 00:03:11,009 --> 00:03:08,799 necessarily life that's even 79 00:03:14,130 --> 00:03:11,019 carbon-based just thinking as broadly as 80 00:03:16,170 --> 00:03:14,140 possible and and it comes at an exciting 81 00:03:18,449 --> 00:03:16,180 time this is a report from the NASA 82 00:03:19,860 --> 00:03:18,459 Astrobiology strategy was out a few 83 00:03:22,289 --> 00:03:19,870 months ago saying you know this is a 84 00:03:25,770 --> 00:03:22,299 great time to think about research on 85 00:03:27,720 --> 00:03:25,780 novel and agnostic bio signatures kind 86 00:03:29,970 --> 00:03:27,730 of how it is we look for life as we 87 00:03:33,559 --> 00:03:29,980 don't know it how we can contend with 88 00:03:36,780 --> 00:03:33,569 the truly alien so just the doctor a few 89 00:03:40,050 --> 00:03:36,790 examples so so one idea is the safety of 90 00:03:42,300 --> 00:03:40,060 chemical complexity and as my colleague 91 00:03:44,970 --> 00:03:42,310 and lab Kelly Cronin likes to say if you 92 00:03:46,710 --> 00:03:44,980 find a 747 on the surface of Mars you 93 00:03:49,860 --> 00:03:46,720 may not know how I got there but it 94 00:03:51,660 --> 00:03:49,870 probably wasn't random and so a neat 95 00:03:53,430 --> 00:03:51,670 paper then you put out I have about a 96 00:03:55,860 --> 00:03:53,440 year and a half ago was really asking 97 00:03:58,379 --> 00:03:55,870 what's the simplest way we can instruct 98 00:04:00,569 --> 00:03:58,389 a molecule from its parts taking with 99 00:04:02,009 --> 00:04:00,579 the simplifying feature duplication 100 00:04:04,129 --> 00:04:02,019 because you can get high molecular 101 00:04:06,390 --> 00:04:04,139 weight polymers that aren't necessarily 102 00:04:08,550 --> 00:04:06,400 complex they're just repeating small 103 00:04:13,199 --> 00:04:08,560 subunits and so as you can see with this 104 00:04:15,030 --> 00:04:13,209 example biphenyl you could simplify that 105 00:04:17,129 --> 00:04:15,040 into a construction process that just 106 00:04:19,199 --> 00:04:17,139 requires six steps and you can start to 107 00:04:21,509 --> 00:04:19,209 explore chemical space and you can see 108 00:04:23,850 --> 00:04:21,519 that simple molecules like glycine can 109 00:04:26,430 --> 00:04:23,860 be assigned an index of four much more 110 00:04:28,710 --> 00:04:26,440 complicated molecules like ATP can be 111 00:04:30,300 --> 00:04:28,720 assigned an index of 21 so this is 112 00:04:32,390 --> 00:04:30,310 adding a new element or a new type of 113 00:04:34,730 --> 00:04:32,400 bond a new feature 114 00:04:36,530 --> 00:04:34,740 um and what leads found is that there 115 00:04:39,370 --> 00:04:36,540 appears to be this threshold above which 116 00:04:42,020 --> 00:04:39,380 it's very unlikely that you don't have 117 00:04:44,150 --> 00:04:42,030 machinery biological machinery 118 00:04:46,279 --> 00:04:44,160 associated with creating that molecule 119 00:04:48,620 --> 00:04:46,289 and so that's not taking into account 120 00:04:50,810 --> 00:04:48,630 anything about what the actual chemical 121 00:04:52,189 --> 00:04:50,820 constituents of that molecule are so 122 00:04:54,529 --> 00:04:52,199 Lee's got a terrific talk about this 123 00:04:56,420 --> 00:04:54,539 Thursday morning at 11:30 for folks that 124 00:05:00,650 --> 00:04:56,430 are interested in how his algorithms are 125 00:05:03,040 --> 00:05:00,660 coming along along similar lines we're 126 00:05:05,330 --> 00:05:03,050 also working on this idea of molecular 127 00:05:06,890 --> 00:05:05,340 complementarity so one of the most 128 00:05:08,680 --> 00:05:06,900 exciting things I think that's happened 129 00:05:10,670 --> 00:05:08,690 in the world of genomics is we've had 130 00:05:12,140 --> 00:05:10,680 miniaturization and sequencing 131 00:05:14,450 --> 00:05:12,150 technologies so now we have these 132 00:05:17,360 --> 00:05:14,460 handheld sequencers that can only wait 133 00:05:19,010 --> 00:05:17,370 85 grams and draw a lot of power and you 134 00:05:20,750 --> 00:05:19,020 know for folks that create instruments 135 00:05:22,909 --> 00:05:20,760 for spacecraft this is half the battle 136 00:05:25,700 --> 00:05:22,919 just getting something down this small 137 00:05:28,129 --> 00:05:25,710 so NASA is currently funding two teams 138 00:05:30,529 --> 00:05:28,139 through matisse and cold tech to develop 139 00:05:32,659 --> 00:05:30,539 nanopore sequencers to send into space 140 00:05:34,700 --> 00:05:32,669 they've been tested in extreme 141 00:05:36,860 --> 00:05:34,710 environments down here in Antarctica as 142 00:05:37,730 --> 00:05:36,870 well as off at the International Space 143 00:05:40,670 --> 00:05:37,740 Station 144 00:05:42,320 --> 00:05:40,680 and one thing you might say well 145 00:05:44,659 --> 00:05:42,330 sequencing that's looking for nucleic 146 00:05:45,950 --> 00:05:44,669 acids that's not agnostic you know and 147 00:05:47,540 --> 00:05:45,960 and so even though these kinds of 148 00:05:49,939 --> 00:05:47,550 technologies might be able to be used 149 00:05:52,189 --> 00:05:49,949 for non-standard bases prints you'll 150 00:05:54,589 --> 00:05:52,199 even informational polymers what we've 151 00:05:56,950 --> 00:05:54,599 been most excited on my team is about 152 00:06:00,070 --> 00:05:56,960 this idea of harnessing the power of 153 00:06:03,290 --> 00:06:00,080 sequencing to explore complexity of 154 00:06:05,420 --> 00:06:03,300 surfaces and so this is not necessarily 155 00:06:08,000 --> 00:06:05,430 looking for any life that has nucleic 156 00:06:11,149 --> 00:06:08,010 acids involved but the idea is that you 157 00:06:13,550 --> 00:06:11,159 could take libraries of millions of 158 00:06:15,529 --> 00:06:13,560 randomly generated short oligos so 159 00:06:18,170 --> 00:06:15,539 strands of DNA and RNA there were just 160 00:06:20,450 --> 00:06:18,180 3050 base pairs in length and they'll 161 00:06:22,670 --> 00:06:20,460 naturally curl up and have secondary and 162 00:06:26,600 --> 00:06:22,680 tertiary structures and they'll bind to 163 00:06:28,159 --> 00:06:26,610 a wide variety of analytes and so we're 164 00:06:31,460 --> 00:06:28,169 talking about peptides and proteins 165 00:06:33,469 --> 00:06:31,470 small organics inorganics like mineral 166 00:06:35,480 --> 00:06:33,479 surfaces of course from the RNA world we 167 00:06:38,330 --> 00:06:35,490 know RNAi sticks to montmorillonite and 168 00:06:39,830 --> 00:06:38,340 even metals and they'll bind with the 169 00:06:43,670 --> 00:06:39,840 same sort of specificities and 170 00:06:45,110 --> 00:06:43,680 affinities as antibodies and so the idea 171 00:06:48,140 --> 00:06:45,120 if you can just imagine 172 00:06:50,840 --> 00:06:48,150 simple sort of end member say you have a 173 00:06:53,150 --> 00:06:50,850 simple little mineral grain versus a 174 00:06:54,980 --> 00:06:53,160 cell and even the most primitive cell on 175 00:06:57,409 --> 00:06:54,990 earth contains a vast amount of 176 00:06:59,570 --> 00:06:57,419 information patterned on its surface if 177 00:07:02,090 --> 00:06:59,580 you were to incubate with libraries of 178 00:07:04,730 --> 00:07:02,100 millions randomly generated oligos some 179 00:07:07,250 --> 00:07:04,740 very very small proportion of those 180 00:07:09,290 --> 00:07:07,260 would bind and they bind again with 181 00:07:11,270 --> 00:07:09,300 these very high specificities and and 182 00:07:12,920 --> 00:07:11,280 affinities and if you've got a surface 183 00:07:14,659 --> 00:07:12,930 with a lot of binding sites a lot of 184 00:07:17,270 --> 00:07:14,669 different analytes they could bind to 185 00:07:19,430 --> 00:07:17,280 you'll have many more diverse sequences 186 00:07:21,490 --> 00:07:19,440 detected versus something simple like a 187 00:07:24,260 --> 00:07:21,500 repeating crystalline structure and 188 00:07:26,060 --> 00:07:24,270 because these reporters that we'd be 189 00:07:28,100 --> 00:07:26,070 using are nucleic acids instead of 190 00:07:31,159 --> 00:07:28,110 proteins we could amplify them up using 191 00:07:32,810 --> 00:07:31,169 the PCR polymerase chain reaction and we 192 00:07:35,480 --> 00:07:32,820 think this could have a lot of potential 193 00:07:37,909 --> 00:07:35,490 especially for ocean worlds where key 194 00:07:40,340 --> 00:07:37,919 Melissa trophic life might be much much 195 00:07:41,750 --> 00:07:40,350 lower biomass than we're expecting here 196 00:07:45,290 --> 00:07:41,760 on earth where we have photosynthetic 197 00:07:47,300 --> 00:07:45,300 life so related talks exciting ones just 198 00:07:49,730 --> 00:07:47,310 following this session in the agnostic 199 00:07:51,830 --> 00:07:49,740 bio signatures session by M lab coli 200 00:07:53,300 --> 00:07:51,840 sandy Ellington and Eric Hanson at UT 201 00:07:57,590 --> 00:07:53,310 those are going to be in the Cedar 202 00:07:59,990 --> 00:07:57,600 Ballroom this morning we also have just 203 00:08:02,240 --> 00:08:00,000 this idea of compartmentalization and 204 00:08:04,490 --> 00:08:02,250 chemical fractionation can we find 205 00:08:07,279 --> 00:08:04,500 separation from an environment as an 206 00:08:09,650 --> 00:08:07,289 agnostic bio signature so here are just 207 00:08:12,770 --> 00:08:09,660 some nano Sims images or you can see 208 00:08:14,719 --> 00:08:12,780 really different compartments can can 209 00:08:16,190 --> 00:08:14,729 light up and we might be able to look at 210 00:08:18,170 --> 00:08:16,200 this and these are the kinds of things 211 00:08:20,089 --> 00:08:18,180 that Chris house has been working on in 212 00:08:22,640 --> 00:08:20,099 his laboratory at Penn State but we have 213 00:08:26,659 --> 00:08:22,650 lots of excitement about where this 214 00:08:29,120 --> 00:08:26,669 might take us and then also energy 215 00:08:30,980 --> 00:08:29,130 transfer for extant life this is this 216 00:08:33,380 --> 00:08:30,990 wonderful quote life is nothing but an 217 00:08:35,719 --> 00:08:33,390 electron looking for a place to rest 218 00:08:38,060 --> 00:08:35,729 so we've long known that microbes can 219 00:08:40,730 --> 00:08:38,070 utilize minerals as electron acceptors 220 00:08:43,490 --> 00:08:40,740 you can use insoluble ferric oxide for 221 00:08:45,829 --> 00:08:43,500 example and what turns out is that the 222 00:08:48,230 --> 00:08:45,839 electrochemical properties of abiotic 223 00:08:50,030 --> 00:08:48,240 and biotic oxidation actually look 224 00:08:52,160 --> 00:08:50,040 different and it's apparent and even the 225 00:08:54,829 --> 00:08:52,170 simplest of setups as shown here you get 226 00:08:56,540 --> 00:08:54,839 this market and sustained increase in 227 00:08:58,290 --> 00:08:56,550 voltage and these little reactors that 228 00:09:00,450 --> 00:08:58,300 have microbial communities that 229 00:09:02,400 --> 00:09:00,460 been inoculated this is every time iron 230 00:09:04,530 --> 00:09:02,410 sulfide tailings are added in this 231 00:09:06,120 --> 00:09:04,540 simple setup so this is something Pete 232 00:09:09,030 --> 00:09:06,130 Girgis has been working on and we'll be 233 00:09:10,920 --> 00:09:09,040 talking more about Friday morning and in 234 00:09:13,590 --> 00:09:10,930 collaboration with Jana DOE and other co 235 00:09:16,020 --> 00:09:13,600 I on our team also this possibility of 236 00:09:18,960 --> 00:09:16,030 setting these specific potentials so 237 00:09:21,750 --> 00:09:18,970 this last image is it's these glass 238 00:09:23,220 --> 00:09:21,760 lithographically etched glass slides and 239 00:09:25,410 --> 00:09:23,230 you can look at these chips and you can 240 00:09:26,970 --> 00:09:25,420 set these very specific potentials and 241 00:09:30,050 --> 00:09:26,980 you could cycle through looking to 242 00:09:33,750 --> 00:09:30,060 discover possible energetic niches for 243 00:09:36,660 --> 00:09:33,760 extraterrestrial microbes so now some of 244 00:09:38,790 --> 00:09:36,670 these techniques we need some time these 245 00:09:40,500 --> 00:09:38,800 are very low TRL some of them are more 246 00:09:43,920 --> 00:09:40,510 at the concept stage that needs to be 247 00:09:46,350 --> 00:09:43,930 developed but others are higher heritage 248 00:09:48,510 --> 00:09:46,360 and so trying to think about how we can 249 00:09:50,100 --> 00:09:48,520 translate these concepts to actual 250 00:09:53,130 --> 00:09:50,110 missions I think is where the rubber 251 00:09:54,540 --> 00:09:53,140 hits the road the one opportunity that I 252 00:09:57,570 --> 00:09:54,550 wanted to talk about that's pretty 253 00:09:59,850 --> 00:09:57,580 immediate is this idea of translating to 254 00:10:03,930 --> 00:09:59,860 say Mars mission so MoMA the Mars 255 00:10:05,670 --> 00:10:03,940 organic molecule analyzer is um is an 256 00:10:08,010 --> 00:10:05,680 instrument that's gonna be sent on the 257 00:10:10,890 --> 00:10:08,020 ExoMars Rover that launches next summer 258 00:10:13,290 --> 00:10:10,900 will land the following spring MoMA is a 259 00:10:14,790 --> 00:10:13,300 really fantastic instrument it's a grass 260 00:10:16,800 --> 00:10:14,800 come out of grass mass spectrometer 261 00:10:18,750 --> 00:10:16,810 coupled to a laser desorption mass 262 00:10:20,940 --> 00:10:18,760 spectrometer it's got this incredible 263 00:10:22,770 --> 00:10:20,950 range not only for high molecular weight 264 00:10:27,540 --> 00:10:22,780 stuff but also things that aren't easily 265 00:10:29,610 --> 00:10:27,550 volatilized to big advantage is moma and 266 00:10:31,680 --> 00:10:29,620 LDL smoking actually detect these heavy 267 00:10:34,020 --> 00:10:31,690 organic compounds even in the presence 268 00:10:36,480 --> 00:10:34,030 of perchlorates which has been really 269 00:10:38,820 --> 00:10:36,490 steaming every time we heat samples 270 00:10:40,890 --> 00:10:38,830 above 200 degrees celsius with pyrolysis 271 00:10:43,470 --> 00:10:40,900 perchlorates released these reactive 272 00:10:45,840 --> 00:10:43,480 gases that make it hard to that obscure 273 00:10:48,210 --> 00:10:45,850 the signals but MoMA can avoid this 274 00:10:51,210 --> 00:10:48,220 problem and it also can analyze 275 00:10:53,370 --> 00:10:51,220 structure using its ms/ms mode so if 276 00:10:55,230 --> 00:10:53,380 you've got a peak that's of interest a 277 00:10:57,770 --> 00:10:55,240 particularly interesting peak you can 278 00:11:01,620 --> 00:10:57,780 zoom in on it and create its own 279 00:11:03,930 --> 00:11:01,630 fragmentation pattern and so we've been 280 00:11:05,190 --> 00:11:03,940 doing ongoing work at Goddard Space 281 00:11:07,980 --> 00:11:05,200 Flight Center which has been responsible 282 00:11:10,530 --> 00:11:07,990 for building MoMA building this whole 283 00:11:12,280 --> 00:11:10,540 training set using these flight capable 284 00:11:14,319 --> 00:11:12,290 instrument bed boards and flight 285 00:11:16,629 --> 00:11:14,329 prototypes see if we can start pulling 286 00:11:18,730 --> 00:11:16,639 out complexity information working in 287 00:11:21,310 --> 00:11:18,740 close collaboration with lea and his 288 00:11:23,110 --> 00:11:21,320 complexity work as well but um this is 289 00:11:25,840 --> 00:11:23,120 just one example say here's this really 290 00:11:27,910 --> 00:11:25,850 interesting peak at 825 Dalton's we 291 00:11:30,340 --> 00:11:27,920 isolate it and we look at the ms/ms 292 00:11:32,410 --> 00:11:30,350 pattern we see these mass units that are 293 00:11:34,030 --> 00:11:32,420 repeating they're separated by the same 294 00:11:36,340 --> 00:11:34,040 mass units and so what this actually is 295 00:11:38,139 --> 00:11:36,350 indicative indicating is that this is a 296 00:11:40,150 --> 00:11:38,149 polymer which indeed it is and if you 297 00:11:42,670 --> 00:11:40,160 saw a pattern like this you would not 298 00:11:44,710 --> 00:11:42,680 think this is a complex molecule but 299 00:11:46,389 --> 00:11:44,720 we're trying to explore chemical space 300 00:11:48,670 --> 00:11:46,399 and do this for lots of different things 301 00:11:50,499 --> 00:11:48,680 to build this training set so that we 302 00:11:52,449 --> 00:11:50,509 can work with colleagues at the Santa Fe 303 00:11:53,970 --> 00:11:52,459 Institute on our project trying to 304 00:11:56,410 --> 00:11:53,980 develop these machine learning 305 00:11:59,470 --> 00:11:56,420 capabilities where we can take this data 306 00:12:03,189 --> 00:11:59,480 and translate it into to you know data 307 00:12:05,379 --> 00:12:03,199 processing techniques so one thing I 308 00:12:07,449 --> 00:12:05,389 will say that's important to note is 309 00:12:10,620 --> 00:12:07,459 that these agnostic techniques are gonna 310 00:12:13,059 --> 00:12:10,630 trade definitiveness for inclusivity 311 00:12:14,949 --> 00:12:13,069 it's never going to be as definitive as 312 00:12:17,470 --> 00:12:14,959 say finding a whole pane or a DNA 313 00:12:19,689 --> 00:12:17,480 sequence but one thing that we're 314 00:12:21,129 --> 00:12:19,699 fortunate is when we send missions off 315 00:12:22,920 --> 00:12:21,139 into space we usually get to send a 316 00:12:25,569 --> 00:12:22,930 package of instruments not just one 317 00:12:27,759 --> 00:12:25,579 instrument and so we've got a whole wing 318 00:12:29,439 --> 00:12:27,769 of our project thinking along the lines 319 00:12:31,389 --> 00:12:29,449 of computation and theoretical 320 00:12:34,600 --> 00:12:31,399 approaches how we can start combining 321 00:12:36,790 --> 00:12:34,610 multiple techniques data streams from 322 00:12:38,889 --> 00:12:36,800 that maybe lots of different bio hints 323 00:12:40,540 --> 00:12:38,899 together and using Bayesian networks 324 00:12:43,090 --> 00:12:40,550 trying to convert these measurements 325 00:12:44,559 --> 00:12:43,100 into thresholds and likelihoods trying 326 00:12:47,439 --> 00:12:44,569 to push away from this life for a 327 00:12:49,629 --> 00:12:47,449 no-life binary into okay this is three 328 00:12:52,180 --> 00:12:49,639 sigma away from what we might expect 329 00:12:53,290 --> 00:12:52,190 with abiotic processes and I think 330 00:12:55,240 --> 00:12:53,300 Sarah's going to touch on some of these 331 00:12:57,790 --> 00:12:55,250 cool data interpretation strategies as 332 00:12:59,350 --> 00:12:57,800 well so I'll leave it there but I just 333 00:13:01,509 --> 00:12:59,360 want to say thank you so much to NASA 334 00:13:04,000 --> 00:13:01,519 for this tremendous opportunity and and 335 00:13:06,759 --> 00:13:04,010 we're proud of net enfold the network 336 00:13:08,050 --> 00:13:06,769 for life detection which is um you know 337 00:13:09,579 --> 00:13:08,060 I think Nikki's gonna tell you about 338 00:13:11,650 --> 00:13:09,589 some events we have within fold this 339 00:13:14,090 --> 00:13:11,660 week that you're all welcome to join for 340 00:13:15,290 --> 00:13:14,100 and so I'll leave it there