Published August 16, 2011 | Version Published
Journal Article Open

Microaerobic steroid biosynthesis and the molecular fossil record of Archean life

  • 1. ROR icon Massachusetts Institute of Technology
  • 2. ROR icon Howard Hughes Medical Institute

Abstract

The power of molecular oxygen to drive many crucial biogeochemical processes, from cellular respiration to rock weathering, makes reconstructing the history of its production and accumulation a first-order question for understanding Earth's evolution. Among the various geochemical proxies for the presence of O_2 in the environment, molecular fossils offer a unique record of O_2 where it was first produced and consumed by biology: in sunlit aquatic habitats. As steroid biosynthesis requires molecular oxygen, fossil steranes have been used to draw inferences about aerobiosis in the early Precambrian. However, better quantitative constraints on the O_2 requirement of this biochemistry would clarify the implications of these molecular fossils for environmental conditions at the time of their production. Here we demonstrate that steroid biosynthesis is a microaerobic process, enabled by dissolved O_2 concentrations in the nanomolar range. We present evidence that microaerobic marine environments (where steroid biosynthesis was possible) could have been widespread and persistent for long periods of time prior to the earliest geologic and isotopic evidence for atmospheric O_2. In the late Archean, molecular oxygen likely cycled as a biogenic trace gas, much as compounds such as dimethylsulfide do today.

Additional Information

© 2011 National Academy of Sciences. Edited by John M. Hayes, Woods Hole Oceanographic Institution, Berkeley, CA, and approved July 5, 2011 (received for review March 19, 2011). Published online before print August 8, 2011. We are grateful to Alexa Price-Whelan and Paula Welander for guidance with anaerobic culturing techniques, to Lars Dietrich for assistance with microelectrode measurements, and to Maureen Coleman for comments, discussion, and help with model visualization. We also acknowledge helpful comments by Lee Kump and two anonymous reviewers that improved the manuscript. This work was supported by grants from the National Aeronautics and Space Administration Astrobiology Institute and the Agouron Institute (to R.E.S. and D.K.N.), by the Howard Hughes Medical Institute (HHMI), and by an Office of Naval Research National Defense Science and Engineering Graduate Fellowship and an National Science Foundation Graduate Research Fellowship (to J.R.W.). D.K.N. is an HHMI Investigator. Author contributions: J.R.W., D.K.N., and R.E.S. designed research; J.R.W. performed research; J.R.W. and R.E.S. analyzed data; and J.R.W., D.K.N., and R.E.S. wrote the paper.

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Identifiers

PMCID
PMC3158215
Eprint ID
37752
Resolver ID
CaltechAUTHORS:20130403-162415003

Funding

NASA
Agouron Institute
Howard Hughes Medical Institute (HHMI)
Office of Naval Research (ONR)
NSF Graduate Research Fellowship
National Defense Science and Engineering Graduate (NDSEG) Fellowship

Dates

Created
2013-04-04
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Updated
2021-11-09
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