Isolation and characterization of a manganese oxidizing bacterium from the Mediterranean marine sponge Suberites domuncula

In the present study of sponge-bacterial association, the presence of a marine bacterium which has not seen to be associated previously with the Mediterranean sponge Suberites domuncula was investigated. The marine sponge S. domuncula was chosen as the subject of investigation, for the identification of potential symbiotic microorganisms, since it can be kept under controlled laboratory conditions for over five years. By the use of specialized media assisting in the growth of a metal oxidizing bacterium, the manganese oxidizing bacterium was isolated from the surface of the marine sponge. The bacterium so isolated was characterized for its growth characteristics by microbiological and biochemical techniques, a detailed analysis of which showed that the bacterium followed a life cycle where the culture showed the presence of spore forming bacteria. This was correlated to the manganese oxidation activity of the bacteria and it was found that both stages are interdependent.The action of the protein responsible for carrying out the manganese (Mn) oxidation was studied by an in-gel oxidation assay, and the presence of a multi copper oxidase was confirmed by the use of copper chelators in the buffer. In parallel the effect of addition of copper was observed on the manganese oxidation by the bacteria thus supporting the observations. The manganese oxidation reaction by the bacteria was determined in the culture medium and on the surface of the cells, and it could be concluded that the oxidation was facilitated by the presence of the polysaccharides and proteins on the surface of the cells.Thus the presence of a bacterium capable of oxidizing the manganese from the surroundings was confirmed to be symbiotically associated with the marine sponge S. domuncula by monitoring its growth in axenic cultures. The reasons behind this association were studied.This bacterium displays a crucial role in the physiology/metabolism of the sponge by acting as a reversible Mn store in S. domuncula. According to this view, the presence of SubDo-03 bacteria is required as a protection against higher, toxic concentrations of Mn in the environment; manganese (II) after undergoing oxidation to manganese (IV), becomes an insoluble ion. Since only minute levels of manganese exist in the surrounding seawater a substantial accumulation of manganese has to arise, or a release by the bacterial-precipitated manganese (IV) is implicated to maintain the reversible balance. The other possible benefits provided by the bacterial association to the sponge could be in preventing cellular oxygen toxicity, help in nutrient scavenging and detoxification.

Stable isotope composition of atmospheric carbon monoxide : a modelling study

Stable isotope composition of atmospheric carbon monoxide: A modelling study.rnrnThis study aims at an improved understanding of the stable carbon and oxygen isotope composition of the carbon monoxide (CO) in the global atmosphere by means of numerical simulations. At first, a new kinetic chemistry tagging technique for the most complete parameterisation of isotope effects has been introduced into the Modular Earth Submodel System (MESSy) framework. Incorporated into the ECHAM/MESSy Atmospheric Chemistry (EMAC) general circulation model, an explicit treatment of the isotope effects on the global scale is now possible. The expanded model system has been applied to simulate the chemical system containing up to five isotopologues of all carbon- and oxygen-bearing species, which ultimately determine the δ13C, δ18O and Δ17O isotopic signatures of atmospheric CO. As model input, a new stable isotope-inclusive emission inventory for the relevant trace gases has been compiled. The uncertainties of the emission estimates and of the resulting simulated mixing and isotope ratios have been analysed. The simulated CO mixing and stable isotope ratios have been compared to in-situ measurements from ground-based observatories and from the civil-aircraft-mounted CARIBIC−1 measurement platform.rnrnThe systematically underestimated 13CO/12CO ratios of earlier, simplified modelling studies can now be partly explained. The EMAC simulations do not support the inferences of those studies, which suggest for CO a reduced input of the highly depleted in 13C methane oxidation source. In particular, a high average yield of 0.94 CO per reacted methane (CH4) molecule is simulated in the troposphere, to a large extent due to the competition between the deposition and convective transport processes affecting the CH4 to CO reaction chain intermediates. None of the other factors, assumed or disregarded in previous studies, however hypothesised to have the potential in enriching tropospheric CO in 13C, were found significant when explicitly simulated. The inaccurate surface emissions, likely underestimated over East Asia, are responsible for roughly half of the discrepancies between the simulated and observed 13CO in the northern hemisphere (NH), whereas the remote southern hemisphere (SH) compositions suggest an underestimated fractionation during the oxidation of CO by the hydroxyl radical (OH). A reanalysis of the kinetic isotope effect (KIE) in this reaction contrasts the conventional assumption of a mere pressure dependence, and instead suggests an additional temperature dependence of the 13C KIE, which is driven by changes in the partitioning of the reaction exit channels. This result is yet to be confirmed in the laboratory.rnrnApart from 13CO, for the first time the atmospheric distribution of the oxygen mass-independent fractionation (MIF) in CO, Δ17O, has been consistently simulated on the global scale with EMAC. The applicability of Δ17O(CO) observations to unravelling changes in the tropospheric CH4-CO-OH system has been scrutinised, as well as the implications of the ozone (O3) input to the CO isotope oxygen budget. The Δ17O(CO) is confirmed to be the principal signal for the CO photochemical age, thus providing a measure for the OH chiefly involved in the sink of CO. The highly mass-independently fractionated O3 oxygen is estimated to comprise around 2% of the overall tropospheric CO source, which has implications for the δ18O, but less likely for the Δ17O CO budgets. Finally, additional sensitivity simulations with EMAC corroborate the nearly equal net effects of the present-day CH4 and CO burdens in removing tropospheric OH, as well as the large turnover and stability of the abundance of the latter. The simulated CO isotopologues nonetheless hint at a likely insufficient OH regeneration in the NH high latitudes and the upper troposphere / lower stratosphere (UTLS).rn