1 00:00:04,710 --> 00:00:02,470 hi i'd like to tell you about some 2 00:00:07,749 --> 00:00:04,720 recent numerical modeling work examining 3 00:00:09,910 --> 00:00:07,759 stable isotopes on enceladus 4 00:00:12,470 --> 00:00:09,920 as water vapor and other gases erupt 5 00:00:14,470 --> 00:00:12,480 from the ocean light isotopes erupt more 6 00:00:16,710 --> 00:00:14,480 easily which should make the plume 7 00:00:19,029 --> 00:00:16,720 isotopically lighter than the ocean and 8 00:00:20,790 --> 00:00:19,039 make the ocean isotopically heavier over 9 00:00:23,750 --> 00:00:20,800 time 10 00:00:26,150 --> 00:00:23,760 for carbon and co2 the ocean is probably 11 00:00:27,990 --> 00:00:26,160 only slightly heavier than the plume but 12 00:00:30,150 --> 00:00:28,000 if the current plume eruption rates have 13 00:00:32,069 --> 00:00:30,160 persisted over long time scales then the 14 00:00:35,270 --> 00:00:32,079 co2 in the ocean may have been 15 00:00:37,350 --> 00:00:35,280 isotopically lighter in the past 16 00:00:40,069 --> 00:00:37,360 if we assume methane started with the 17 00:00:41,990 --> 00:00:40,079 same isotopic ratio as co2 then a 18 00:00:45,029 --> 00:00:42,000 fractionation between these gases in the 19 00:00:47,350 --> 00:00:45,039 ocean can emerge over long time scales 20 00:00:49,270 --> 00:00:47,360 however the maximum we see here around 21 00:00:52,150 --> 00:00:49,280 two and a half per ml is still much 22 00:00:54,709 --> 00:00:52,160 smaller than biological fractionation 23 00:00:58,150 --> 00:00:54,719 so this process alone should not create 24 00:01:00,150 --> 00:00:58,160 false positive biosignatures 25 00:01:02,310 --> 00:01:00,160 the d to h ratio of water may have 26 00:01:04,710 --> 00:01:02,320 evolved similarly but even with 27 00:01:06,550 --> 00:01:04,720 persistent long-term eruption the d-h 28 00:01:08,310 --> 00:01:06,560 ratio of enceladus still seems 29 00:01:11,270 --> 00:01:08,320 consistent with an origin from