2014 GSA Annual Meeting in Vancouver, British Columbia (19–22 October 2014)

Paper No. 281-10
Presentation Time: 10:15 AM

RECONSTRUCTION OF LIMNOLOGY AND MICROBIALITE FORMATION CONDITIONS FROM CARBONATE CLUMPED ISOTOPE PALEOTHERMOMETRY: A TEST CASE FROM PAVILION AND KELLY LAKES


PETRYSHYN, Victoria A., Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90095, LIM, Darlene S.S., Space Science and Astrobiology, NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000, LAVAL, Bernard, Civil Engineering, University of British Columbia, Vancouver, BC V6T 1Z4, Canada, BRADY, Allyson L., School of Geography and Earth Sciences, McMaster University, 1280 Main Street West, Hamilon, ON L8S4K1, SLATER, Gregory F., School of Geography and Earth Sciences, McMaster University, Hamilton, ON L8S 4K1, Canada and TRIPATI, Aradhna, Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, 595 Charles Young Drive East, Box 951567, Los Angeles, CA CA 90095-156

Quantitative tools for deciphering the environment of microbialite formation are relatively limited. For example, the carbonate-water geothermometer requires assumptions about the isotopic composition of the water of formation. This study explores the utility of using “clumped” isotope thermometry to study microbialite formation conditions. We measured freshwater microbialites from Pavilion and Kelly Lake (British Columbia) in order to determine the temperature of precipitation and the 18O/16O ratio of the waters of formation. Microbialites span the thermocline in both lakes, ranging from depths of 10-55 m in Pavilion Lake, and 10-25 m in Kelly Lake. Isotopic ratios were determined for each sample, and used to reconstruct limnology. Results were then compared to current limnological data from the lake in order to reconstruct the history of microbialite formation. Microbialites collected at shallow depths (~10 m) in Pavilion Lake and Kelly Lake yield clumped isotope-based temperature of formation of 20.8 ±2.8°C and 15.9 ±2.5 °C (1 s.e.) respectively. Similar temperatures are also found for microbialites collected from deeper parts of both lakes. The data for the shallower depths match the current measured temperature profiles, however the clumped isotope-based temperature estimates from the deeper microbialites do not match the present limnological characteristics. The deepest microbialites (~50 m) yield radioisotope ages indicating they primarily formed earlier in the Holocene, when pollen data and our reconstructed water 18O/16O ratios indicate a period of aridity, with lower lake levels. Given the deepest microbialites are receiving <1% of photosynthetically active radiation (PAR), it is likely that the deepest microbialites primarily formed when lower lake levels resulting in these microbialites being located higher in the photic zone.