To determine the effects of Saharan dust on the abundance, biomass, community structure, and metabolic activity of oceanic microbial plankton, we conducted eight bioassay experiments between ca. 30uN and 30uS in the central Atlantic Ocean. We found that, although bulk abundance and biomass tended to remain unchanged, different groups of phytoplankton and bacterioplankton responded differently to Saharan dust addition. The predominant type of metabolic response depended on the ecosystem's degree of oligotrophy and was modulated by competition for nutrients between phytoplankton and heterotrophic bacteria. The relative increase in bacterial production, which was the dominant response to dust addition in ultraoligotrophic environments, became larger with increasing oligotrophy. In contrast, primary production, which was stimulated only in the least oligotrophic waters, became less responsive to dust as the ecosystem's degree of oligotrophy increased. Given the divergent consequences of a predominantly bacterial vs. phytoplanktonic response, dust inputs can, depending on the ecosystem's degree of oligotrophy, stimulate or weaken biological CO 2 drawdown. Thus, the biogeochemical implications of changing dust fluxes might not be universal, but variable through both space and time.

The distribution and activity of the bulk picoplankton community and, using microautoradiography combined with catalysed reported deposition fluorescence in situ hybridization (MICRO-CARD-FISH), of the major prokaryotic groups (Bacteria, marine Crenarchaeota Group I and marine Euryarchaeota Group II) were determined in the water masses of the subtropical North Atlantic. The bacterial contribution to total picoplankton abundance was fairly constant, comprising approximately 50% of DAPI-stainable cells. Marine Euryarchaeota Group II accounted always for < 5% of DAPI-stainable cells. The percentage of total picoplankton identified as marine Crenarchaeota Group I was approximately 5% in subsurface waters (100 m depth) and between 10% and 20% in the oxygen minimum layer (250-500 m) and deep waters [North East Atlantic Deep Water (NEADW) and Lower Deep Water (LDW), 2750-4800 m depth]. Single-cell activity, determined via a quantitative MICRO-CARD-FISH approach and taking only substrate-positive cells into account, ranged from 0.05 to 0.5 amol D-aspartic acid (Asp) cell(-1) day(-1) and 0.1-2 amol L-Asp cell(-1) day(-1), slightly decreasing with depth. In contrast, the D-Asp:L-Asp cell-specific uptake ratio increased with depth. By combining data reported previously using the same method as applied here and data reported here, we found a decreasing relative abundance of marine Crenarchaeota Group I throughout the meso- and bathypelagic water column from 65 degrees N to 5 degrees N in the eastern basin of the North Atlantic. Thus, the relative contribution of marine Crenarchaeota Group I to deep-water prokaryotic communities might be more variable than previous studies have suggested. This apparent variability in the contribution of marine Crenarchaeota Group I to total picoplankton abundance might be related to successions and ageing of deep-water masses in the large-scale meridional ocean circulation and possibly, the appearance of crenarchaeotal clusters other than the marine Crenarchaeota Group I in the (sub)tropical North Atlantic.

The dark ocean is one of the largest biomes on Earth, with critical roles in organic matter remineralization and global carbon sequestration. Despite its recognized importance, little is known about some key microbial players, such as the community of heterotrophic protists (HP), which are likely the main consumers of prokaryotic biomass. To investigate this microbial component at a global scale, we determined their abundance and biomass in deepwater column samples from the Malaspina 2010 circumnavigation using a combination of epifluorescence microscopy and flow cytometry. HP were ubiquitously found at all depths investigated down to 4000 m. HP abundances decreased with depth, from an average of 72 ± 19 cells ml À 1 in mesopelagic waters down to 11 ± 1 cells ml À 1 in bathypelagic waters, whereas their total biomass decreased from 280±46 to 50±14 pg C ml À 1 . The parameters that better explained the variance of HP abundance were depth and prokaryote abundance, and to lesser extent oxygen concentration. The generally good correlation with prokaryotic abundance suggested active grazing of HP on prokaryotes. On a finer scale, the prokaryote:HP abundance ratio varied at a regional scale, and sites with the highest ratios exhibited a larger contribution of fungi molecular signal. Our study is a step forward towards determining the relationship between HP and their environment, unveiling their importance as players in the dark ocean's microbial food web.

Until recently, ammonia oxidation, a key process in the global nitrogen cycle, was thought to be mediated exclusively by a few bacterial groups. It has been shown now, that also Crenarchaeota are capable to perform this initial nitrification step. The abundance of ammonia oxidizing Bacteria and Archaea was determined using the bacterial and archaeal ammonia monooxygenase-a subunit (amoA) gene as functional markers in a quantitative PCR approach and related to the abundance of Bacteria and Archaea in the Eastern Mediterranean Sea. Archaeal amoA copy numbers decreased from 4000-5000 copies ml À1 seawater from the 200-500 m depth layer to 20 copies ml À1 at 1000 m depth. b-Proteobacterial amoA genes were below the detection limit in all the samples. The archaeal amoA copy numbers were correlated with NO 2 À concentrations, suggesting that ammonia-oxidizing Archaea may play a significant role in the nitrification in the mesopelagic waters of the Eastern Mediterranean Sea. In the bathypelagic waters, however, archaeal amoA gene abundance was rather low although Crenarchaeota were abundant, indicating that Crenarchaeota might largely lack the amoA gene in these deep waters. Terminal restriction fragment length polymorphism analysis of the archaeal community revealed a distinct clustering with the mesopelagic community distinctly different from the archaeal communities of both, the surface waters and the 3000-4000 m layers. Hence, the archaeal community in the Eastern Mediterranean Sea appears to be highly stratified despite the absence of major temperature and density gradients between the meso-and bathypelagic waters of the Mediterranean Sea.

The contribution of Chloroflexi-type SAR202 cells to total picoplankton and bacterial abundance and uptake of D- and L-aspartic acids (Asp) was determined in the different meso- and bathypelagic water masses of the (sub)tropical Atlantic (from 35 degrees N to 5 degrees S). Fluorescence in situ hybridization (FISH) revealed that the overall abundance of SAR202 was < or = 1 x 10(3) cells ml(-1) in subsurface waters (100 m layer), increasing in the mesopelagic zone to 3 x 10(3) cells ml(-1) and remaining fairly constant down to 4000 m depth. Overall, the percentage of total picoplankton identified as SAR202 increased from < 1% in subsurface waters to 10-20% in the bathypelagic waters. On average, members of the SAR202 cluster accounted for about 30% of the Bacteria in the bathypelagic waters, whereas in the mesopelagic and subsurface waters, SAR202 cells contributed < 5% to total bacterial abundance. The ratio of D-Asp : L-Asp uptake by the bulk picoplankton community increased from the subsurface layer (D-Asp : L-Asp uptake ratio approximately 0.03) to the deeper layers reaching a ratio of approximately 1 at 4000 m depth. Combining FISH with microautoradiography to determine the proportion of SAR202 cells taking up D-Asp versus L-Asp, we found that approximately 30% of the SAR202 cells were taking up L-Asp throughout the water column while D-Asp was essentially not taken up by SAR202. This D-Asp : L-Asp uptake pattern of SAR202 cells is in contrast to that of the bulk bacterial and crenarchaeal community in the bathypelagic ocean, both sustaining a higher fraction of D-Asp-positive cells than L-Asp-positive cells. Thus, although the Chloroflexi-type SAR202 constitutes a major bathypelagic bacterial cluster, it does not contribute to the large fraction of d-Asp utilizing prokaryotic community in the meso- and bathypelagic waters of the North Atlantic, but rather utilizes preferentially L-amino acids.

Taurine, an amino acid-like compound, acts as an osmostress protectant in many marine metazoans and algae and is released via various processes into the oceanic dissolved organic matter pool. Taurine transporters are widespread among members of the marine prokaryotic community, tentatively indicating that taurine might be an important substrate for prokaryotes in the ocean. In this study, we determined prokaryotic taurine assimilation and respiration throughout the water column along two transects in the North Atlantic off the Iberian Peninsula. Taurine assimilation efficiency decreased from the epipelagic waters from 55 ± 14% to 27 ± 20% in the bathypelagic layers (means of both transects). Members of the ubiquitous alphaproteobacterial SAR11 clade accounted for a large fraction of cells taking up taurine, especially in surface waters. Archaea (Thaumarchaeota + Euryarchaeota) were also able to take up taurine in the upper water column, but to a lower extent than Bacteria. The contribution of taurine assimilation to the heterotrophic prokaryotic carbon biomass production ranged from 21% in the epipelagic layer to 16% in the bathypelagic layer. Hence, we conclude that dissolved free taurine is a significant carbon and energy source for prokaryotes throughout the oceanic water column being utilized with similar efficiencies as dissolved free amino acids. Electronic supplementary material The online version of this article (10.1007/s00248-019-01320-y) contains supplementary material, which is available to authorized users.

Prokaryotic abundance, activity and community composition were studied in the euphotic, intermediate and deep waters off the Galician coast (NW Iberian margin) in relation to the optical characterization of dissolved organic matter (DOM). Microbial (archaeal and bacterial) community structure was vertically stratified. Among the Archaea, Euryarchaeota, especially Thermoplasmata, was dominant in the intermediate waters and decreased with depth, whereas marine Thaumarchaeota, especially Marine Group I, was the most abundant archaeal phylum in the deeper layers. The bacterial community was dominated by Proteobacteria through the whole water column. However, Cyanobacteria and Bacteroidetes occurrence was considerable in the upper layer and SAR202 was dominant in deep waters. Microbial composition and abundance were not shaped by the quantity of dissolved organic carbon, but instead they revealed a strong connection with the DOM quality. Archaeal communities were mainly related to the fluorescence of DOM (which indicates respiration of labile DOM and generation of refractory subproducts), while bacterial communities were mainly linked to the aromaticity/age of the DOM produced along the water column. Taken together, our results indicate that the microbial community composition is associated with the DOM composition of the water masses, suggesting that distinct microbial taxa have the potential to use and/or produce specific DOM compounds.

Taurine (Tau), an amino acid‐like compound, is present in almost all marine metazoans including crustacean zooplankton. It plays an important physiological role in these organisms and is released into the ambient water throughout their life cycle. However, limited information is available on the release rates by marine organisms, the concentrations and turnover of Tau in the ocean. We determined dissolved free Tau concentrations throughout the water column and its release by abundant crustacean mesozooplankton at two open ocean sites (Gulf of Alaska and North Atlantic). At both locations, the concentrations of dissolved free Tau were in the low nM range (up to 15.7 nM) in epipelagic waters, declining sharply in the mesopelagic to about 0.2 nM and remaining fairly stable throughout the bathypelagic waters. Pacific amphipod–copepod assemblages exhibited lower dissolved free Tau release rates per unit biomass (0.8 ± 0.4 μmol g−1 C‐biomass h−1) than Atlantic copepods (ranging between 1.3 ± 0.4 μmol g−1 C‐biomass h−1 and 9.5 ± 2.1 μmol g−1 C‐biomass h−1), in agreement with the well‐documented inverse relationship between biomass‐normalized excretion rates and body size. Our results indicate that crustacean zooplankton might contribute significantly to the dissolved organic matter flux in marine ecosystems via dissolved free Tau release. Based on the release rates and assuming steady state dissolved free Tau concentrations, turnover times of dissolved free Tau range from 0.05 d to 2.3 d in the upper water column and are therefore similar to those of dissolved free amino acids. This rapid turnover indicates that dissolved free Tau is efficiently consumed in oceanic waters, most likely by heterotrophic bacteria.