ISSN:
1573-0875
Source:
Springer Online Journal Archives 1860-2000
Topics:
Biology
,
Geosciences
Notes:
Abstract From the Archean geological record, one can infer that photoautotrophy evolved early in earth history; however, the nature of this photosynthesis — whether it was predominantly bacterial or cyanobacterial — is less clearly understood. General agreement that the earth's atmosphere did not become oxygen rich before the Early Proterozoic era places constraints on theories concerning more ancient biotas. Accommodating this limitation in various ways, different workers have hypothesized (1) that blue-green algae first evolved in the Early Proterozoic; (2) that oxygen producing proto-cyanobacteria existed in the Archean but had no biochemical mechanism for coping with ambient O2; and (3) that true cyanobacteria flourished in the Archean, but did not oxygenate the atmosphere because of high rates of oxygen consumption caused, in part, by the emanation of reduced gases from widespread Archean volcanoes. Inversion of hypothesis three leads to another, as yet unexplored, alternative. It is possible that physiologically modern blue-green algae existed in Archean times, but had low productivity. Increased rates of primary production in the Early Proterozoic era resulted in the atmospheric transition documented in strata a this age. An answer to the question of wht productivity should have changed from the Archean to the Proterozoic may lie in the differing tectonic frameworks of the two areas. The earliest evidence of widespread, stable, shallow marine platforms is found in Lower Proterozoic sedimentary sequences. In such environments, productivity was, and is, high. In contrast, Archean shallow water environments are often characterized by rapid rates of clastic and pyroclastic influx —conditions that reduced rates of benthonic primary production. This hypothesis suggests that the temporal correlation of major shifts in tectonic mode and at mospheric composition may not be fortuitous. It also suggests that sedimentary environments may have constituted a significant limit to the abundance and diversity of early life.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00926824
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