The Adavosertib molecular weight carbon isotopic signature of photosynthesis Spurred by the pioneering studies of Park and Epstein (1963) and Hoering (1967), data have been amassed from thousands of analyses of the carbon isotopic compositions of inorganic carbonate minerals and carbonaceous kerogens coexisting in Precambrian sediments (e.g., Strauss and Moore 1992). Such data show a consistent difference between the inorganic and organic carbon analyzed in the relative abundances of the two stable isotopes of carbon, 12C and 13C, which extends from the present to ~3,500 Ma ago (Fig. 8). The enrichment of the fossil organic matter in the lighter isotope, 12C, relative to coexisting

carbonate click here (a proxy for the seawater-dissolved CO2 required for its precipitation) and the magnitude of the isotopic difference (expressed as δ13CPDB values) between the inorganic and organic carbon reservoirs, invariably falling within a range of 25 ± 10‰, are consistent with the carbon isotopic fractionation that occurs as a result of Rubisco-(ribulose bisphospate carboxylase/oxygenase-) mediated CO2-fixation in O2-producing cyanobacteria (e.g., Hayes et al. 1992;

House et al. 2000, 2003). Such evidence of carbon isotopic fractionation is well documented in rocks ~3,200 to ~3,500 Ma in age, the oldest fossil-bearing deposits now known (Fig. 9). Fig. 8 Carbon isotopic values of coexisting carbonate and organic carbon measured in bulk samples of Phanerozoic and Precambrian sedimentary rocks, for the Precambrian represented by data from 100 fossiliferous cherts and shales shown as average values for groups of samples from 50-Ma-long intervals (Strauss and Moore 1992; PF-2341066 Schopf Metalloexopeptidase 1994b) Fig. 9 Carbon isotopic values of carbonate and organic carbon measured in bulk samples of the oldest microfossiliferous units now known (Schopf 2006) Although this carbon isotopic signature of photosynthesis seems certain to evidence the continuous existence of photoautotrophs over the past 3,500 Ma, it does not necessarily reflect the presence of oxygenic photoautotrophy. Owing to the mixing of carbonaceous matter from diverse biological sources

which occurs as sediments are deposited, and the alteration of carbon isotopic compositions that can occur during geological metamorphism, the δ13CPDB values of the analyzed kerogen range broadly (±10‰) and, thus, are consistent not only with primary production by cyanobacteria but by non-O2-producing photosynthetic bacteria and, perhaps, anaerobic chemosynthetic bacteria. Archean kerogens may have been derived from some or all of these sources, and interpretation of the data is further complicated by the presence in Archean sediments of carbonaceous matter so enriched in 12C as to be plausibly derived only from CH4-metabolizing methanotrophs, indicating that methane-producing Archaea played a significant role in the ancient ecosystem (Hayes 1983; Schopf 1994b).