Unknown

Dataset Information

0

Sulfur cycling and methanogenesis primarily drive microbial colonization of the highly sulfidic Urania deep hypersaline basin.


ABSTRACT: Urania basin in the deep Mediterranean Sea houses a lake that is >100 m deep, devoid of oxygen, 6 times more saline than seawater, and has very high levels of methane and particularly sulfide (up to 16 mM), making it among the most sulfidic water bodies on Earth. Along the depth profile there are 2 chemoclines, a steep one with the overlying oxic seawater, and another between anoxic brines of different density, where gradients of salinity, electron donors and acceptors occur. To identify and differentiate the microbes and processes contributing to the turnover of organic matter and sulfide along the water column, these chemoclines were sampled at a high resolution. Bacterial cell numbers increased up to a hundredfold in the chemoclines as a consequence of elevated nutrient availability, with higher numbers in the upper interface where redox gradient was steeper. Bacterial and archaeal communities, analyzed by DNA fingerprinting, 16S rRNA gene libraries, activity measurements, and cultivation, were highly stratified and metabolically more active along the chemoclines compared with seawater or the uniformly hypersaline brines. Detailed analysis of 16S rRNA gene sequences revealed that in both chemoclines delta- and epsilon-Proteobacteria, predominantly sulfate reducers and sulfur oxidizers, respectively, were the dominant bacteria. In the deepest layers of the basin MSBL1, putatively responsible for methanogenesis, dominated among archaea. The data suggest that the complex microbial community is adapted to the basin's extreme chemistry, and the elevated biomass is driven largely by sulfur cycling and methanogenesis.

SUBMITTER: Borin S 

PROVIDER: S-EPMC2685740 | biostudies-literature | 2009 Jun

REPOSITORIES: biostudies-literature

altmetric image

Publications

Sulfur cycling and methanogenesis primarily drive microbial colonization of the highly sulfidic Urania deep hypersaline basin.

Borin Sara S   Brusetti Lorenzo L   Mapelli Francesca F   D'Auria Giuseppe G   Brusa Tullio T   Marzorati Massimo M   Rizzi Aurora A   Yakimov Michail M   Marty Danielle D   De Lange Gert J GJ   Van der Wielen Paul P   Bolhuis Henk H   McGenity Terry J TJ   Polymenakou Paraskevi N PN   Malinverno Elisa E   Giuliano Laura L   Corselli Cesare C   Daffonchio Daniele D  

Proceedings of the National Academy of Sciences of the United States of America 20090522 23


Urania basin in the deep Mediterranean Sea houses a lake that is >100 m deep, devoid of oxygen, 6 times more saline than seawater, and has very high levels of methane and particularly sulfide (up to 16 mM), making it among the most sulfidic water bodies on Earth. Along the depth profile there are 2 chemoclines, a steep one with the overlying oxic seawater, and another between anoxic brines of different density, where gradients of salinity, electron donors and acceptors occur. To identify and dif  ...[more]

Similar Datasets

| S-EPMC10494364 | biostudies-literature
| S-EPMC6606867 | biostudies-literature
| S-EPMC7173876 | biostudies-literature
| S-EPMC93321 | biostudies-literature
| S-EPMC9635834 | biostudies-literature
| S-EPMC9812581 | biostudies-literature
| S-EPMC4649258 | biostudies-literature
| S-EPMC4260694 | biostudies-literature
| S-EPMC7415356 | biostudies-literature
| S-EPMC3996697 | biostudies-literature