Microscopic sulfides with low 34S/32S ratios in marine sulfate deposits from the 3490-million-year old Dresser Formation, Australia, have been interpreted as evidence for the presence of early sulfate-reducing organisms on Earth. We show that these microscopic sulfides have a mass-independently fractionated sulfur isotopic anomaly (Delta33S) that differs from that of their host sulfate (barite). These microscopic sulfides could not have been produced by sulfate-reducing microbes, nor by abiologic processes that involve reduction of sulfate. Instead, we interpret the combined negative delta34S and positive Delta33S signature of these microscopic sulfides as evidence for the early existence of organisms that disproportionate elemental sulfur.

No abstract

Summary We report here a molecular survey based on 16S rRNA genes of the bacterial diversity found in two deep‐sea vent niches at the Mid‐Atlantic Ridge: hydrothermal sediment (Rainbow site), and microcolonizers made of three different substrates (organic‐rich, iron‐rich and pumice) that were exposed for 15 days to a vent emission. Bacterial diversity in sediment samples was scattered through many bacterial divisions. The most abundant and diverse environmental sequences (phylotypes) in our libraries corresponded to the Gammaproteobacteria, followed by the Acidobacteria. We detected members of all the subdivisions within the Proteobacteria. Myxobacterial lineages were the most represented within the delta subdivision. Phylotypes ascribing to the Cytophaga‐Flavobacterium‐Bacteroides, Planctomycetales, high and low G + C Gram‐positives, Nitrospirae, and the candidate division TM7 were also identified. Compared to this broad taxonomic coverage, microcolonizers were almost exclusively colonized by epsilonproteobacteria, although these exhibited considerable morphological and phylogenetic in‐group diversity. No specificity for any of the substrates tested was seen. This observation further supports the idea of the ecological dominance of epsilonproteobacteria in the fluid–seawater interface environment. Because oxidation of reduced S species and/or sulphur‐reduction is thought to be essential for their energetic metabolism in these areas, we mapped different oxidation states of S in individual bacterial filaments from the iron‐rich microcolonizer. For this, we used high‐resolution, non‐destructive synchrotron micro‐X‐ray Absorption Near‐Edge Spectroscopy (micro‐XANES), which revealed the co‐existence of different S oxidation states, from sulphide to sulphate, at the level of individual cells. This suggests that these cells were metabolizing sulphur in situ.

Post-orogenic extension in the Aegean Sea has produced several metamorphic domes. Some domes ("b-type") are elongated perpendicular to the main N-S direction of extension, and they correspond to the exhumation of the middle crust along northdipping detachments. The example of Tinos shows the progressive localization of deformation from the initial boudinage at all scales to the formation of brittle structures at the tips of boudins and the selection of one of those, which becomes the main detachment. The progressive deformation leading to strain localization is described alongside the P-T-t evolution and the role of fl uid circulation. The second type of domes ("a-type") has a long axis parallel to the direction of extension. Extension is accommodated by a detachment that exhumes high-temperature gneisses issued from deeper parts of the Hellenic edifi ce. Shortening perpendicular to stretching has produced the extension-parallel folds that are also observed in b-type domes but to a lesser extent. The formation of b-type and then a-type domes during extension is discussed in terms of crustal collapse during slab retreat.

No abstract

No abstract

No abstract

Understanding the atmosphere's composition during the Archean eon is a fundamental issue to unravel ancient environmental conditions. We show from the analysis of nitrogen and argon isotopes in fluid inclusions trapped in 3.0-3.5 Ga hydrothermal quartz that the PN2 of the Archean atmosphere was lower than 1.1 bar, possibly as low as 0.5 bar, and had a nitrogen isotopic composition comparable to the present-day one. These results imply that dinitrogen did not play a significant role in the thermal budget of the ancient Earth and that the Archean PCO2 was probably lower than 0.7 bar