ISSN:
1420-9136
Source:
Springer Online Journal Archives 1860-2000
Topics:
Geosciences
,
Physics
Notes:
Summary Photosynthesis (assimilation) is currently understood as a photoreduction of CO2 by water into carbohydrates; reoxidation by O2 (dissimilation) closes the biological carbon cycle. If, originally, there was a surplus of H2, thermodynamical equilibrium would require that C, Fe, Mn, S and N exist as CH4, Fe++, Mn++, S−− and NH3. The redox equilibrium is believed to have been shifted gradually as a result of the escape of H2 formed photochemically in the atmosphere. However, in a system containing H2, CO2 is an energy-rich compound affording 31.2 kcal on reduction to CH4; it should be so rare that even CaCO3 would dissolve. How, then, could photoreduction evolve, lacking CO2 and a thermodynamical advantage? Also H2 escape, governed by diffusion, does not account for so much H2 during geological time (Miller andUrey [19]). The hypothesis of areductive primeval carbon cycle between biomass (C(H2O)) and methane involvinginverse assimilation and dissimilation (Decker [6]), as presented in the following scheme, would evercome these difficulties. The present oxidative carbon cycle requires 114 kcal supplied by two consecutive photoreactions: regular: $$CO_2 + H_2 OC(H_2 O) + O_2 + 114 kcal.$$ A reductive carbon cycle involving inverse assimilation and dissimilation would require only 32 kcal, i.e. only one photoreaction: inverse: $$CH_4 + H_2 OC(H_2 O) + 2H_2 + 32 kcal.$$ It could actively support an elevated H2 level necessary to explain the observed escape rate, until all CH4 was consumed and burried as elemental C or carbonate, the latter resulting from fermentations in ‘anaerobic’ environments. All enzymatic steps of such a cycle are present in contemporary organisms except a photochemical CH4 assimilation in a CO2-free atmosphere, which, however, has apparently never seriously been looked for. Further facts pro and contra should be available in the geological record, e.g. in Precambrian ‘anaerobic’ Fe3+ and CaCO3 deposits.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00881492
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