Paleoproterozoic sterol biosynthesis and the rise of oxygen
Abstract
Natural products preserved in the geological record can function as 'molecular fossils', providing insight into organisms and physiologies that existed in the deep past. One important group of molecular fossils is the steroidal hydrocarbons (steranes), which are the diagenetic remains of sterol lipids. Complex sterols with modified side chains are unique to eukaryotes, although simpler sterols can also be synthesized by a few bacteria. Sterol biosynthesis is an oxygen-intensive process; thus, the presence of complex steranes in ancient rocks not only signals the presence of eukaryotes, but also aerobic metabolic processes. In 1999, steranes were reported in 2.7 billion year (Gyr)-old rocks from the Pilbara Craton in Australia, suggesting a long delay between photosynthetic oxygen production and its accumulation in the atmosphere (also known as the Great Oxidation Event) 2.45–2.32 Gyr ago. However, the recent reappraisal and rejection of these steranes as contaminants pushes the oldest reported steranes forward to around 1.64 Gyr ago (ref. 6). Here we use a molecular clock approach to improve constraints on the evolution of sterol biosynthesis. We infer that stem eukaryotes shared functionally modern sterol biosynthesis genes with bacteria via horizontal gene transfer. Comparing multiple molecular clock analyses, we find that the maximum marginal probability for the divergence time of bacterial and eukaryal sterol biosynthesis genes is around 2.31 Gyr ago, concurrent with the most recent geochemical evidence for the Great Oxidation Event. Our results therefore indicate that simple sterol biosynthesis existed well before the diversification of living eukaryotes, substantially predating the oldest detected sterane biomarkers (approximately 1.64 Gyr ago), and furthermore, that the evolutionary history of sterol biosynthesis is tied to the first widespread availability of molecular oxygen in the ocean–atmosphere system.
Additional Information
© 2017 Macmillan Publishers Limited. received 21 May 2016; accepted 19 January 2017. Published online 6 March 2017. We gratefully acknowledge funding from the Agouron Institute Geobiology Fellowship to D.A.G. and the Simons Foundation Collaboration on the Origins of Life to R.E.S. and G.P.F. Additional support was provided by the National Science Foundation programme 'Frontiers of Earth System Dynamics' (EAR-1338810) to R.E.S., and the National Science Foundation programme 'Integrated Earth Systems' (IES-1615426) to G.P.F. Author Contributions: R.E.S. and D.A.G. designed the experiment. D.A.G. and A.C. performed the data analysis. All authors were involved in interpreting the data and drafting the manuscript. The authors declare no competing financial interests.Attached Files
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Supplemental Material - nature21412-sf6.jpg
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Additional details
- Eprint ID
- 75824
- Resolver ID
- CaltechAUTHORS:20170407-083556533
- Agouron Institute
- Simons Foundation
- NSF
- EAR-1338810
- NSF
- IES-1615426
- Created
-
2017-04-07Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field