K. M. Towe has been a long-standing advocate of the idea of a generally oxidizing Archean environment (1, 2), a point of view for which there has recently been a resurgence of enthusiasm (3, 4). However, we stand by our arguments that the Mount McRae Shale nitrogen isotopic results and other geochemical data presented in companion papers (5, 6) point toward a generally anoxic environment with a brief interruption of somewhat more oxidizing conditions.
We note that the scarcity of Mo and Re through most of the section, despite high (>1%) sulfide levels indicating the potential for thiol-organic scavenging (7), suggest low marine concentrations of these elements that are largely supplied by oxidative weathering (6). Moreover, the occurrence of large Δ33S mass-independently fractionated isotope anomalies, even in rocks with low organic carbon concentrations (5), implies that this signature was imparted by photolysis of sulfurous gases in an oxygen-deficient atmosphere and not by thermochemical sulfate reduction by organic compounds (4). The near-zero δ15N values through much of the section indicate low dissolved nitrate concentrations inhibiting heavy-isotope enrichment during denitrification (2). If Towe's oxic scenario were correct, we would expect persistent δ15N values above +5 per mil as in the modern oxygen- and nitrate-rich ocean, along with high Mo and Re abundances and negligible Δ33S. Instead, we find such features restricted to a narrow stratigraphic interval, most consistent with the temporary development of slightly oxygenic conditions in a persistently low-oxygen environment.
Regarding Towe’s points:
(i) Nitrogen fixation now allows the accumulation of substantial concentrations of dissolved nitrate in the ocean, despite the high energetic cost. This is because there is a leak of nitrogen from the bioavailable pool back to the atmosphere as N2 and N2O after denitrification, as well as to sediments as organic nitrogen. Thus, the system is close to a steady state, in which the leaks to the system encourage the continuation of nitrogen fixation in defiance of oxygenic inhibition and high energy cost. In an anoxic Archean world, ammonification would not inhibit nitrogen fixation as NH3 diffusion back to the atmosphere and organic nitrogen loss to sediments would serve as a similar stimulus to the maintenance of nitrogen fixation.
(ii) Oxygen levels of 10-6 to 10-5 PAL should not, according to recent studies (8, 9), prohibit aerobic respiration given that the critical minimum level is approximately 10-7 atm (9). Thus, organic carbon would have been available for aerobic respiration and thus for oxygen consumption. Nitrogen-fixing microbes have many alternative strategies other than heterocysts to avoid oxygenic inhibition, such as temporal separation of N-fixation from O2 production, intracellular segregation of N-fixing from oxidative processes, and consortial living. So even if the TOC in Archean sedimentary rocks were all produced by oxygenic photosynthesis (a moot point for such ancient times when anoxygenic photosynthesis using Fe2+ and H2S may have been more significant), oxygen production need not have inhibited N-fixation.
(iii) The 10-5 PAL figure refers to atmospheric levels of oxygen, not to those in the marine photic zone where dissolved O2 can be locally enhanced by oxygenic photosynthesis to levels supportive of nitrification, regardless of oxygen levels in the overlying atmosphere.
(iv) Inhabitants of the photic zone are shielded from UV radiation even in the absence of an ozone shield by water attenuation of UV at all depths below the immediate surface layer.
We see no compelling reason to adapt the data to fit an oxygenated atmosphere or to radically alter our perception of a generally anoxic Archean environment, albeit one in which temporary or localized oxygenic conditions could occur.
Jessica Garvin, Roger Buick
Department of Earth and Space Sciences and Astrobiology Program, University of Washington, Seattle, WA 98195-1310, USA.
Ariel D. Anbar
School of Earth and Space Exploration, and Department of Chemistry and Biochemistry, Arizona State University, Tempe, AZ 85287, USA.
Gail L. Arnold
School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.
Alan J. Kaufman
Department of Geology, University of Maryland, College Park, MD 20742, USA.
References
1. K. M. Towe, Precambrian Res. 16, 1 (1981).
2. K. M. Towe, Palaeogeogr. Palaeoecol. 97, 113 (1991).
3. Y. Kato et al., Earth Planet. Sci. Lett. 278, 40 (2009).
4. Y. Watanabe, J. Farquhar, H. Ohmoto, Science 324, 370 (2009).
5. A. J. Kaufman et al., Science 317, 1900 (2007).
6. A. D. Anbar et al., Science 317, 1903 (2007).
7. N. Tribovillard, A. Riboulleau, T. Lyons, F. Baudin, Chem. Geol. 213, 385 (2004).
8. Q. Jin, C. M. Bethke, Geochim. Cosmochim. Acta. 69, 1133 (2005).
9. Q. Guo et al., Geology 37, 399 (2009).