Titlebook: Halophilic Microorganisms; Antonio Ventosa Book 2004 Springer-Verlag Berlin Heidelberg 2004 Evolution.Polysaccharid.archaea.biodiversity.e

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Understanding Archaeal Protein Translocation: , as a Model System,ser examination also reveals the existence of archaeal-specific properties. These could be related to the unique chemical composition of the archaeal membrane or to the extreme conditions in which Archaea can exist, including highly saline environments.

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Extremely Halophilic Archaea: Insights into Their Response to Environmental Conditions,re extremely high and precipitation of different salts is commonly taking place. In these environments, both solar irradiation and salt concentration contribute to heat accumulation, and temperatures of 55 °C or higher can be frequently reached (Rodríguez-Valera et al.1985).

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Trophic Ecology of Solar Salterns,mes even further. The two extremes provide one of the most common habitats in the world (seawater) and one of the most extreme habitats in the world (calcium and magnesium chloride saturated brines). This is particularly interesting for microbial ecology, since large organisms disappear early in the

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Microbial Molecular and Physiological Diversity in Hypersaline Environments, 10–15 years these same innovative techniques have also changed our concepts of the microbial communities in hypersaline environments.We now recognize that such specialized environments also have very complex communities that have received relatively little attention. This chapter will describe the

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Red, Extremely Halophilic, but not Archaeal: The Physiology and Ecology of ,, a Bacterium Isolated for the study of microbial processes at high salt concentrations.In multi-pond saltern environments a broad range of salt concentrations is found, increasing from seawater (around 35 g dissolved salts per liter) to brines with salt concentrations exceeding 350 g l. (see, e.g., Rodriguez-Valera et al

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,From Intraterrestrials to Extraterrestrials — Viable Haloarchaea in Ancient Salt Deposits,1.3 million cubic kilometers of salt were deposited in the late Permian and early Triassic periods alone (ca. 240 to 280 million years ago; Zharkov 1981). The continental land masses were concentrated around the paleoequator and formed the supercontinent Pangaea (Fig. 5.1). Salt sediments developed

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