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University of Cambridge > Talks.cam > Institute of Astronomy Seminars > Murdin Prize Ceremony -- Proposed energy-metabolisms cannot explain the atmospheric chemistry of Venus
Murdin Prize Ceremony -- Proposed energy-metabolisms cannot explain the atmospheric chemistry of VenusAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Hannah Uebler. The clouds of Venus have been proposed as a potential abode for life. Life, if present in sufficiently high abundance, must be interacting with the atmospheric chemistry via its metabolism. Three possible sulfur-based metabolisms have been previously suggested which Venusian life could use to obtain energy from its environment. These metabolisms raise the possibility of Venus’s enigmatic cloud-layer SO2 -depletion being caused by life. We perform a test for the possiblity of abundant Venusian life by coupling each proposed energy-metabolism to a photochemical-kinetics code and predicting the composition of Venus’s atmosphere under the scenario that life produces the observed SO2 -depletion. Using this coupled photo-bio-chemical kinetics code, we show that all three metabolisms can produce SO2 -depletions, but do so by violating other observational constraints on Venus’s atmospheric chemistry. We therefore calculate an upper limit on the possible biomass of sulfur-metabolising life in the clouds of Venus before violating observational constraints. This talk is part of the Institute of Astronomy Seminars series. This talk is included in these lists:
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