1 00:00:02,140 --> 00:00:06,630 [Music] 2 00:00:12,310 --> 00:00:08,629 thank you my name is hannah miller i am 3 00:00:13,350 --> 00:00:12,320 here at cu working with alexis templeton 4 00:00:14,789 --> 00:00:13,360 so we've already talked about 5 00:00:16,070 --> 00:00:14,799 serpentinization a little bit but i'm 6 00:00:18,710 --> 00:00:16,080 going to go into a little bit more 7 00:00:20,950 --> 00:00:18,720 detail to the actual 8 00:00:24,070 --> 00:00:20,960 geochemical reaction right here 9 00:00:26,710 --> 00:00:24,080 so serpentinization is a water rock 10 00:00:27,509 --> 00:00:26,720 reaction in which you get the oxidation 11 00:00:28,470 --> 00:00:27,519 of 12 00:00:30,870 --> 00:00:28,480 mantle 13 00:00:33,510 --> 00:00:30,880 rocks and minerals such as olivine which 14 00:00:35,350 --> 00:00:33,520 i show in this equation so olivine has 15 00:00:38,229 --> 00:00:35,360 this iron two in it when it reacts with 16 00:00:40,069 --> 00:00:38,239 water in an anoxic environment it 17 00:00:42,869 --> 00:00:40,079 generates magnesium bearing minerals 18 00:00:44,069 --> 00:00:42,879 such as serpentine and brucite along 19 00:00:46,950 --> 00:00:44,079 with 20 00:00:49,510 --> 00:00:46,960 oxidized minerals like magnetite here 21 00:00:51,029 --> 00:00:49,520 and hydrogen gas 22 00:00:52,549 --> 00:00:51,039 and this reaction has been very well 23 00:00:54,630 --> 00:00:52,559 studied at high temperatures that 24 00:00:56,869 --> 00:00:54,640 hydrothermal vents are spreading ocean 25 00:00:58,630 --> 00:00:56,879 or spreading ridges under the ocean but 26 00:00:59,910 --> 00:00:58,640 it hasn't been well characterized at low 27 00:01:03,910 --> 00:00:59,920 temperatures 28 00:01:05,830 --> 00:01:03,920 celsius where life can actually be 29 00:01:08,070 --> 00:01:05,840 actively harnessing that hydrogen being 30 00:01:10,230 --> 00:01:08,080 generated from these reactions 31 00:01:12,230 --> 00:01:10,240 this is an image of what a partially 32 00:01:13,910 --> 00:01:12,240 serpentized rock looks like so you can 33 00:01:16,070 --> 00:01:13,920 see why it's called serpentine because 34 00:01:19,030 --> 00:01:16,080 it generates these veins that look kind 35 00:01:23,510 --> 00:01:20,710 so what we always talk about how does 36 00:01:24,390 --> 00:01:23,520 this relate back to astrobiology 37 00:01:26,469 --> 00:01:24,400 both 38 00:01:28,469 --> 00:01:26,479 well mars we definitely know has olivine 39 00:01:30,390 --> 00:01:28,479 mineral olivine minerals on it as well 40 00:01:31,990 --> 00:01:30,400 as serpentine minerals so there's 41 00:01:33,749 --> 00:01:32,000 potential that these 42 00:01:36,149 --> 00:01:33,759 water rock reactions could be occurring 43 00:01:37,910 --> 00:01:36,159 on mars making hydrogen gas which is an 44 00:01:39,030 --> 00:01:37,920 electron donor for organisms to be 45 00:01:41,270 --> 00:01:39,040 utilizing 46 00:01:42,870 --> 00:01:41,280 additionally europa might also contain 47 00:01:46,710 --> 00:01:42,880 some of these 48 00:01:48,870 --> 00:01:46,720 rocks that could be subpoenaizing and 49 00:01:50,710 --> 00:01:48,880 also studies have been done on enceladus 50 00:01:52,469 --> 00:01:50,720 and how there might be high ph fluids 51 00:01:53,990 --> 00:01:52,479 there that indicate serpentinization is 52 00:01:55,910 --> 00:01:54,000 occurring 53 00:01:57,510 --> 00:01:55,920 so there are several metabolisms that 54 00:02:00,389 --> 00:01:57,520 could be supported by these water rock 55 00:02:03,190 --> 00:02:00,399 reactions one that is oftentimes invoked 56 00:02:05,030 --> 00:02:03,200 is methanogenesis because if you have 57 00:02:06,469 --> 00:02:05,040 all this hydrogen around if you if 58 00:02:08,869 --> 00:02:06,479 there's some carbon available you can 59 00:02:10,469 --> 00:02:08,879 make methane gas and methane is a 60 00:02:13,190 --> 00:02:10,479 prevalent gas to be found in these 61 00:02:15,190 --> 00:02:13,200 serpentinizing environments is source is 62 00:02:17,350 --> 00:02:15,200 oftentimes debated it may be biotic 63 00:02:19,110 --> 00:02:17,360 abiotic a mixture of the two but it's 64 00:02:21,510 --> 00:02:19,120 definitely a relevant gas along with 65 00:02:23,750 --> 00:02:21,520 hydrogen in these environments 66 00:02:25,910 --> 00:02:23,760 additionally we know we have all we have 67 00:02:27,510 --> 00:02:25,920 this electron donor hydrogen around but 68 00:02:31,110 --> 00:02:27,520 you need electron acceptors two for 69 00:02:32,630 --> 00:02:31,120 organisms oftentimes nitrate and sulfate 70 00:02:34,710 --> 00:02:32,640 are found in these environments so you 71 00:02:36,869 --> 00:02:34,720 can also have various metabolisms that 72 00:02:39,030 --> 00:02:36,879 utilize those 73 00:02:41,110 --> 00:02:39,040 one potential exciting metabolism would 74 00:02:42,949 --> 00:02:41,120 be anaerobic methane oxidation occurring 75 00:02:45,030 --> 00:02:42,959 in these environments 76 00:02:47,830 --> 00:02:45,040 so you can see that serpentinization can 77 00:02:50,070 --> 00:02:47,840 fuel a variety of life and that's kind 78 00:02:52,070 --> 00:02:50,080 of the theme of the rock powered life 79 00:02:54,470 --> 00:02:52,080 nasa astrobiology institute which alexis 80 00:02:55,910 --> 00:02:54,480 templeton heads up here at cu so we are 81 00:02:57,270 --> 00:02:55,920 really investigating this and a lot of 82 00:02:59,509 --> 00:02:57,280 different people at the conference have 83 00:03:01,830 --> 00:02:59,519 been talking about various things that 84 00:03:04,790 --> 00:03:01,840 rpl is working on 85 00:03:05,830 --> 00:03:04,800 so i'm specifically working in oman 86 00:03:08,390 --> 00:03:05,840 which is 87 00:03:10,390 --> 00:03:08,400 located right here on the eastern edge 88 00:03:11,509 --> 00:03:10,400 of the arabian peninsula 89 00:03:13,350 --> 00:03:11,519 and 90 00:03:14,630 --> 00:03:13,360 oman is a great place to study 91 00:03:16,229 --> 00:03:14,640 serpentinization because it's the 92 00:03:18,550 --> 00:03:16,239 world's largest and best exposed 93 00:03:20,710 --> 00:03:18,560 ophelite sequence and for you 94 00:03:24,149 --> 00:03:20,720 non-geologists out there an ophiolite 95 00:03:25,430 --> 00:03:24,159 sequence contains layers of upper mantle 96 00:03:26,790 --> 00:03:25,440 so if you think about the earth as an 97 00:03:28,949 --> 00:03:26,800 avocado 98 00:03:30,710 --> 00:03:28,959 you have your mantle right here so an 99 00:03:31,910 --> 00:03:30,720 ophelite would be this upper mantle 100 00:03:33,270 --> 00:03:31,920 which is the green fleshy part of the 101 00:03:34,550 --> 00:03:33,280 avocado which is actually very 102 00:03:36,070 --> 00:03:34,560 appropriate because peridotite is a 103 00:03:37,830 --> 00:03:36,080 beautiful green color because of all 104 00:03:41,030 --> 00:03:37,840 this reduced iron 105 00:03:43,110 --> 00:03:41,040 and then you have layered gabbros and 106 00:03:44,789 --> 00:03:43,120 pillar basalts on top 107 00:03:47,670 --> 00:03:44,799 but i'm really interested in this 108 00:03:50,470 --> 00:03:47,680 peridotite right here in oman and 109 00:03:52,309 --> 00:03:50,480 the opioid was originally 110 00:03:53,910 --> 00:03:52,319 at a spreading ridge on the ocean floor 111 00:03:55,509 --> 00:03:53,920 so it's already partially altered by the 112 00:03:57,350 --> 00:03:55,519 time we study it in oman it's already 113 00:03:59,830 --> 00:03:57,360 partially sepanized some of that iron 114 00:04:02,550 --> 00:03:59,840 has already been oxidized 115 00:04:04,550 --> 00:04:02,560 so i i work on water rock reactions to 116 00:04:06,630 --> 00:04:04,560 actually characterize how hydrogen is 117 00:04:08,789 --> 00:04:06,640 being produced in these low temperature 118 00:04:10,710 --> 00:04:08,799 reactions so first of all we take some 119 00:04:12,550 --> 00:04:10,720 rock from oman you can see it has a 120 00:04:14,470 --> 00:04:12,560 beautiful oxidized weathering rind on 121 00:04:17,110 --> 00:04:14,480 the outside we cut that off because 122 00:04:20,069 --> 00:04:17,120 we're just interested in looking at this 123 00:04:22,069 --> 00:04:20,079 relatively unoxidized iron and then we 124 00:04:23,990 --> 00:04:22,079 go through this arduous process of 125 00:04:25,749 --> 00:04:24,000 grinding it up into really small pieces 126 00:04:27,510 --> 00:04:25,759 so there's higher surface area and these 127 00:04:29,670 --> 00:04:27,520 reactions actually proceed on the level 128 00:04:31,270 --> 00:04:29,680 of a phd time scale 129 00:04:36,390 --> 00:04:31,280 and 130 00:04:38,390 --> 00:04:36,400 into these anaerobic vials we add some 131 00:04:39,990 --> 00:04:38,400 water of various compositions some that 132 00:04:42,790 --> 00:04:40,000 simulate seawater or simulate the 133 00:04:45,350 --> 00:04:42,800 groundwater in the area and then we 134 00:04:48,629 --> 00:04:45,360 purge the headspace with a nitrogen and 135 00:04:50,710 --> 00:04:48,639 co2 gas mixture so that there's no 136 00:04:51,909 --> 00:04:50,720 oxygen in there and these the iron can 137 00:04:53,749 --> 00:04:51,919 oxidize 138 00:04:55,909 --> 00:04:53,759 without oxygen around 139 00:04:57,110 --> 00:04:55,919 and the results we see so i did these 140 00:04:58,870 --> 00:04:57,120 reactions with this partially 141 00:05:00,230 --> 00:04:58,880 subpoenaized rock from oman at 100 142 00:05:02,230 --> 00:05:00,240 degrees celsius 143 00:05:03,990 --> 00:05:02,240 and this is showing hydrogen production 144 00:05:05,270 --> 00:05:04,000 right here the two different colors 145 00:05:07,830 --> 00:05:05,280 indicate 146 00:05:09,430 --> 00:05:07,840 the rock was reacting with two different 147 00:05:11,270 --> 00:05:09,440 see what with two different water 148 00:05:13,110 --> 00:05:11,280 compositions i'm not really going to go 149 00:05:15,590 --> 00:05:13,120 into that but you get different hydrogen 150 00:05:16,950 --> 00:05:15,600 production based off of the media 151 00:05:19,110 --> 00:05:16,960 composition you're reacting the rock 152 00:05:21,510 --> 00:05:19,120 with but you can see that we generate 153 00:05:23,510 --> 00:05:21,520 hydrogen up to about 500 animals per 154 00:05:25,110 --> 00:05:23,520 gram of mineral reactant which is 155 00:05:26,950 --> 00:05:25,120 actually quite significant for a 156 00:05:29,029 --> 00:05:26,960 temperature of 100 degrees celsius it's 157 00:05:30,390 --> 00:05:29,039 one of the highest rate highest 158 00:05:31,590 --> 00:05:30,400 concentrations reported in the 159 00:05:33,110 --> 00:05:31,600 literature 160 00:05:34,950 --> 00:05:33,120 and it's also important to note that 161 00:05:37,029 --> 00:05:34,960 it's sustained hydrogen production it 162 00:05:39,270 --> 00:05:37,039 doesn't make hydrogen for one day and 163 00:05:41,189 --> 00:05:39,280 then just stop it's actually sustained 164 00:05:43,670 --> 00:05:41,199 so there's a chance a microbe could 165 00:05:44,950 --> 00:05:43,680 actually be using that hydrogen over 166 00:05:46,550 --> 00:05:44,960 time 167 00:05:48,550 --> 00:05:46,560 additionally we look at the aqueous 168 00:05:50,550 --> 00:05:48,560 chemistry during these reactions and we 169 00:05:53,270 --> 00:05:50,560 can see that there's an increase in ph 170 00:05:54,469 --> 00:05:53,280 to about ph 9 after just 24 hours of 171 00:05:56,870 --> 00:05:54,479 reaction 172 00:05:58,469 --> 00:05:56,880 and that aligns with what you see in 173 00:06:02,150 --> 00:05:58,479 serpentinizing environments they have 174 00:06:04,070 --> 00:06:02,160 high ph's usually they go up to ph 11. 175 00:06:05,670 --> 00:06:04,080 so we don't see that in the time scales 176 00:06:06,710 --> 00:06:05,680 of our reactions but it's probably just 177 00:06:08,469 --> 00:06:06,720 because 178 00:06:10,710 --> 00:06:08,479 this low temperature reaction isn't 179 00:06:12,150 --> 00:06:10,720 actually in equilibrium right now 180 00:06:15,029 --> 00:06:12,160 additionally we see the loss of 181 00:06:17,270 --> 00:06:15,039 magnesium iron and manganese ions 182 00:06:19,350 --> 00:06:17,280 initially during the reaction 183 00:06:21,430 --> 00:06:19,360 so there must be some mineral phase 184 00:06:24,150 --> 00:06:21,440 that's dissolving 185 00:06:26,150 --> 00:06:24,160 and we add co2 to the head space as i 186 00:06:27,350 --> 00:06:26,160 noted that also gets drawn down pretty 187 00:06:30,230 --> 00:06:27,360 immediately 188 00:06:32,070 --> 00:06:30,240 and when we see that co2 get drawn down 189 00:06:33,430 --> 00:06:32,080 we also see a formation of formate and 190 00:06:34,469 --> 00:06:33,440 acetate 191 00:06:38,309 --> 00:06:34,479 these 192 00:06:40,550 --> 00:06:38,319 see just what their formulas are right 193 00:06:42,070 --> 00:06:40,560 here but this likely forms through this 194 00:06:43,830 --> 00:06:42,080 reaction right here you have hydrogen 195 00:06:46,390 --> 00:06:43,840 combining with some of that co2 that's 196 00:06:47,670 --> 00:06:46,400 dissolved in the fluid to make formate 197 00:06:48,629 --> 00:06:47,680 the fact that we have acetate is a 198 00:06:50,309 --> 00:06:48,639 little bit 199 00:06:51,990 --> 00:06:50,319 interesting and enigmatic because it's a 200 00:06:53,189 --> 00:06:52,000 lot more complicated to form acetate 201 00:06:55,510 --> 00:06:53,199 than formate 202 00:06:56,950 --> 00:06:55,520 but this is still an interesting result 203 00:06:58,469 --> 00:06:56,960 that we found through these water rock 204 00:06:59,909 --> 00:06:58,479 reactions 205 00:07:01,589 --> 00:06:59,919 additionally we also really want to 206 00:07:03,990 --> 00:07:01,599 characterize the mineralogy during these 207 00:07:05,749 --> 00:07:04,000 water rock reactions to see how the iron 208 00:07:07,270 --> 00:07:05,759 is actually oxidizing and what are the 209 00:07:09,110 --> 00:07:07,280 different reservoirs 210 00:07:11,510 --> 00:07:09,120 of iron in the system 211 00:07:13,029 --> 00:07:11,520 so first this is a 212 00:07:15,110 --> 00:07:13,039 picture of a thin section from ramen 213 00:07:18,469 --> 00:07:15,120 micro microscopy 214 00:07:20,309 --> 00:07:18,479 and these yellow blobs here olivine and 215 00:07:22,150 --> 00:07:20,319 then the light blue in the background is 216 00:07:24,710 --> 00:07:22,160 all serpentine and this is just a big 217 00:07:25,670 --> 00:07:24,720 like chromite diopside thing 218 00:07:28,150 --> 00:07:25,680 but 219 00:07:30,469 --> 00:07:28,160 we can see that before this rock reacts 220 00:07:31,830 --> 00:07:30,479 we have serpentine so this rock is 221 00:07:34,070 --> 00:07:31,840 already reacted we can see it's a 222 00:07:35,670 --> 00:07:34,080 partially subpoenaized rock but when we 223 00:07:37,430 --> 00:07:35,680 look at the serpentine right here this 224 00:07:38,950 --> 00:07:37,440 is the fingerprint region in raman so 225 00:07:41,749 --> 00:07:38,960 these are the characteristic serpentine 226 00:07:44,150 --> 00:07:41,759 peaks but when we look at the oh the od 227 00:07:45,990 --> 00:07:44,160 the oh stretch of the serpentine we see 228 00:07:48,309 --> 00:07:46,000 this bump right here that corresponds to 229 00:07:49,670 --> 00:07:48,319 brucite so we can see that bruceite is 230 00:07:52,070 --> 00:07:49,680 intimately intermixed with this 231 00:07:53,350 --> 00:07:52,080 serpentine and based off of the peak of 232 00:07:55,110 --> 00:07:53,360 this bruce site 233 00:07:57,110 --> 00:07:55,120 we've calibrated how much iron is 234 00:07:59,670 --> 00:07:57,120 present in the brew site so we can see 235 00:08:01,189 --> 00:07:59,680 there's 15 weight percent iron present 236 00:08:02,710 --> 00:08:01,199 and that's important because this could 237 00:08:04,070 --> 00:08:02,720 be an important source of iron that 238 00:08:06,550 --> 00:08:04,080 could be oxidizing and leading to 239 00:08:09,029 --> 00:08:06,560 hydrogen generation 240 00:08:10,950 --> 00:08:09,039 so when we look at the 241 00:08:13,510 --> 00:08:10,960 the grains that have reacted and formed 242 00:08:16,790 --> 00:08:13,520 hydrogen these are some powder xod 243 00:08:19,189 --> 00:08:16,800 spectrum spectra and you can see 244 00:08:21,189 --> 00:08:19,199 that right here red 245 00:08:22,950 --> 00:08:21,199 is the unreacted rock and there's a 246 00:08:24,790 --> 00:08:22,960 bunch of olivine and serpentine peaks 247 00:08:26,790 --> 00:08:24,800 but the peak i'm going to focus on this 248 00:08:28,869 --> 00:08:26,800 one right here this black bump right 249 00:08:30,710 --> 00:08:28,879 here is bruceite so you can see in the 250 00:08:32,790 --> 00:08:30,720 unreacted rock there's a fair amount of 251 00:08:35,589 --> 00:08:32,800 bruceite but then when we act when we 252 00:08:36,949 --> 00:08:35,599 react the rock with various medias we 253 00:08:39,350 --> 00:08:36,959 can see that that brewsight peak 254 00:08:41,350 --> 00:08:39,360 disappears so bruceite is being consumed 255 00:08:42,790 --> 00:08:41,360 during these water rock reactions 256 00:08:45,350 --> 00:08:42,800 and that's likely why we saw that 257 00:08:47,509 --> 00:08:45,360 release of magnesium manganese and iron 258 00:08:48,949 --> 00:08:47,519 in the aqueous chemistry 259 00:08:50,790 --> 00:08:48,959 and we also know that brucite contains 260 00:08:52,310 --> 00:08:50,800 iron so that's a very likely source of 261 00:08:55,430 --> 00:08:52,320 the iron ii that's been leading to 262 00:08:57,269 --> 00:08:55,440 hydrogen generation as it gets oxidized 263 00:08:59,269 --> 00:08:57,279 additionally we've seen 264 00:09:01,110 --> 00:08:59,279 these are some images of just the thin 265 00:09:03,269 --> 00:09:01,120 sections of the rock before and after 266 00:09:05,670 --> 00:09:03,279 reaction so you can see all these little 267 00:09:07,430 --> 00:09:05,680 splotches of mineral that are forming 268 00:09:09,030 --> 00:09:07,440 there's definitely serpentine formation 269 00:09:10,790 --> 00:09:09,040 during these reactions it's very 270 00:09:11,910 --> 00:09:10,800 amorphous and white and there's not that 271 00:09:13,590 --> 00:09:11,920 much of it 272 00:09:15,350 --> 00:09:13,600 but that is important because we know 273 00:09:17,190 --> 00:09:15,360 from that initial reaction i showed you 274 00:09:18,630 --> 00:09:17,200 serpentine should be forming 275 00:09:20,470 --> 00:09:18,640 at these high temperatures we know it 276 00:09:21,750 --> 00:09:20,480 definitely does but it also does at low 277 00:09:23,590 --> 00:09:21,760 temperatures 278 00:09:25,829 --> 00:09:23,600 additionally we use magnetic 279 00:09:27,990 --> 00:09:25,839 susceptibility methods to show that 280 00:09:30,070 --> 00:09:28,000 magnetite forms and that's also 281 00:09:31,990 --> 00:09:30,080 important to note because at these high 282 00:09:34,630 --> 00:09:32,000 temperatures magnetite is 283 00:09:35,990 --> 00:09:34,640 thermodynamically expected to form but 284 00:09:38,070 --> 00:09:36,000 at lower temperatures it hasn't been 285 00:09:40,230 --> 00:09:38,080 observed as much but we definitely see 286 00:09:42,150 --> 00:09:40,240 that magnetite is forming and likely 287 00:09:45,030 --> 00:09:42,160 that's what's accommodating this iron 288 00:09:48,630 --> 00:09:46,070 okay 289 00:09:50,790 --> 00:09:48,640 so overall why we think we want to 290 00:09:53,030 --> 00:09:50,800 propose some sort of reaction for this 291 00:09:54,870 --> 00:09:53,040 low temperature serpentinization and we 292 00:09:56,310 --> 00:09:54,880 believe that the dissolution of iron ii 293 00:09:57,910 --> 00:09:56,320 bearing bruce site is leading to 294 00:10:00,230 --> 00:09:57,920 hydrogen generation at these low 295 00:10:02,550 --> 00:10:00,240 temperatures so because this rock was 296 00:10:03,990 --> 00:10:02,560 already partially sepantonized 297 00:10:06,150 --> 00:10:04,000 there are some thoughts well is it even 298 00:10:08,710 --> 00:10:06,160 still reacted is it reactive is there 299 00:10:10,550 --> 00:10:08,720 still iron two available for oxidation 300 00:10:14,230 --> 00:10:10,560 and yes there is and we think a lot of 301 00:10:16,069 --> 00:10:14,240 that iron too is coming out of brucite 302 00:10:19,670 --> 00:10:16,079 additionally these reactions can make up 303 00:10:21,030 --> 00:10:19,680 to 37 nanomoles of hydrogen so this is 304 00:10:22,230 --> 00:10:21,040 the hydrogen that's dissolved in the 305 00:10:24,069 --> 00:10:22,240 fluid the hydrogen that's more 306 00:10:26,870 --> 00:10:24,079 biologically available 307 00:10:28,630 --> 00:10:26,880 and that's more than enough to support 308 00:10:31,430 --> 00:10:28,640 some sort of microorganism because 309 00:10:32,550 --> 00:10:31,440 methanogens require much lower levels 310 00:10:34,069 --> 00:10:32,560 than that 311 00:10:36,310 --> 00:10:34,079 additionally these reactions make 312 00:10:38,389 --> 00:10:36,320 reduced energy sources such as formating 313 00:10:40,790 --> 00:10:38,399 acetate which can support support 314 00:10:44,150 --> 00:10:40,800 fermenters living in the 315 00:10:49,030 --> 00:10:47,110 so overall that's how we think that low 316 00:10:50,790 --> 00:10:49,040 temperature hydrogen generation is 317 00:10:53,829 --> 00:10:50,800 happening in oman of course it's very 318 00:10:55,910 --> 00:10:53,839 site-specific because these minerals had 319 00:10:57,430 --> 00:10:55,920 a lot of brewside in them 320 00:10:59,190 --> 00:10:57,440 i would like to thank everyone in my lab 321 00:11:00,770 --> 00:10:59,200 and our collaborators and i would like 322 00:11:06,389 --> 00:11:00,780 to take any questions 323 00:11:22,630 --> 00:11:06,399 [Applause] 324 00:11:26,710 --> 00:11:24,230 i was just curious what the average 325 00:11:28,790 --> 00:11:26,720 ratio of supreme tonight to prototype 326 00:11:31,190 --> 00:11:28,800 that you had for your samples 327 00:11:34,470 --> 00:11:31,200 it started off as about 50 serpentine 328 00:11:35,750 --> 00:11:34,480 and 50 um olivine 329 00:11:37,910 --> 00:11:35,760 was that your question like the mineral 330 00:11:41,030 --> 00:11:37,920 proportions and 331 00:11:42,630 --> 00:11:41,040 during the reaction it barely changes 332 00:11:44,470 --> 00:11:42,640 so just a little bit of blue site we 333 00:11:46,470 --> 00:11:44,480 think it's about five percent by mass 334 00:11:50,470 --> 00:11:46,480 brucite reacted to generate the hydrogen