Iron–silica-rich low-temperature hydrothermal precipitates were collected from the CDE hydrothermal field located at the East Lau Spreading Center. Phylogenetic analysis showed that the precipitates were dominated by the members of α-proteobacteria and marine group I archaea. Ultrastructural analysis suggested the bacteriogenic origin of the iron–silica-rich deposits. Distinctive biosignatures detected included straight filaments, helical stalks and curved irregular filaments, which were similar in appearance to those structures excreted by the known iron-oxidizing genera Leptothrix spp., Gallionella spp. and Mariprofundus spp. 16S rRNA gene analysis confirmed the presence of neutrophilic iron-oxidizing bacteria with the detection of phylotypes clustering with Gallionella spp. and the proposed ζ-proteobacteria class. Mineralogy and bulk geochemical analyses showed that the precipitates were dominated by amorphous silica with low amounts of iron. Based on microbiological, geochemical and mineralogical analyses, we conclude that silicification was a common process and microbial cells and related ultrastructures likely acted as nucleation templates for silica precipitation in the CDE hydrothermal field.
Iron–silica-rich precipitates, generally formed in association with low-temperature hydrothermal fluids, have been commonly found in hydrothermal fields along mid-ocean ridges and back-arc spreading centres (Alt, 1988; Emerson & Moyer, 2002; Kennedy et al., 2003; Davis et al., 2009; Hodges & Olson, 2009; Peng et al., 2011). Morphological evidence indicates that microorganisms play important roles in the formation of these mineral deposits (Juniper & Fouquet, 1988; Langley et al., 2009 and references cited therein). Iron–silica precipitates usually exhibit unique micro-textures that are remarkably similar to microbial forms and are regarded as apparent bacterial origin. Ultrastructure analyses reveal that amorphous silica or Fe-oxyhydroxides aggregate on the outer surface of microorganism-like structures or completely replace original microbial cells by intracellular mineralization (Fortin et al., 1998; Peng et al., 2007). Particularly, putative Fe-oxidizing bacteria (FeOB) biosignature remains, such as filaments, sheaths and helical stalk-like morphologies are widely identified from these iron–silica deposits (Hrischeva & Scott, 2007; Templeton et al., 2009; Edwards et al., 2011).
However, direct evidence from microbial and molecular analyses in association with microbial mineralization has been limited. Although previous investigations using cultivation and molecular techniques to assess microbial communities have been carried out and novel FeOBs have been isolated (Emerson & Moyer, 2002; Emerson et al., 2007), most of the studies focused primarily on dense iron-rich flocculent microbial mats at Loihi Seamount, Hawaii (Moyer et al., 1995; Emerson & Moyer, 2002; Rassa et al., 2009; Edwards et al., 2011), Cleft Segment of Juan de Fuca Ridge (Davis et al., 2009), Tonga-Kermadec Arc(Hodges & Olson, 2009; Forget et al., 2010) and Southern Mariana Trough (Kato et al., 2009). In contrast, direct microbiological and mineralogical evidence is still lacking for low-temperature hydrothermal deposits that are composed mostly of amorphous silica with minute amounts of iron, where the putative Fe oxidizers may contribute significantly to the formation of these deposits. Furthermore, features of microbial communities inhabited in these deposits such as diversity, abundance and composition have not been fully illustrated (Al-Hanbali et al., 2001; Peng et al., 2007, 2010).
The Lau Basin is a back-arc spreading centre in the south-west Pacific. The Eastern Lau Spreading Center (ELSC), located within the basin from 19°20′S to 22°45′S, includes six known hydrothermal fields. According to previous studies, their deep lavas, vent fluid chemistry, mineralogy, geochemistry of hydrothermal deposits and microbial ecology vary considerably within the basin and are different from other well-studied hydrothermal vent sites in the Pacific Ocean (Reno, 2006; Hsu-Kim et al., 2008). In this study, we present results of microbiological, geochemical and mineralogical analyses and discuss microbial diversity and abundance and the role microorganisms have played in mineral precipitation in the recently discovered ‘CDE’ hydrothermal field in ESLC (Zhou et al., 2008).
Materials and methods
Study site and sample collection
The CDE hydrothermal field is located on the Eastern Lau Spreading Center (ELSC) at 176°11′W, 20°40′S. It was discovered by R/V DaYang YiHao (Ocean One) in May 2007 and is about four miles south of the ABE hydrothermal field (Fig. 1) (Zhou et al., 2008). Chemosynthetic communities (anemones and crabs) and white microbial mats attached to pillar chimneys with heights from < 1 m to more than 5 m were found at the site using a deep tow camera system. Abnormity of turbidity (ΔNTU = 0.07), temperature (0.03 °C) and CH4 (5.36 nM) were detected at the water column above the CDE hydrothermal field, by deep-water surveys using MAPR, CTD and onboard GC analysis of water samples, respectively. Low-temperature hydrothermal Fe–Si-rich precipitates were collected by a TV-grab (station No.19IV-TVG13) near hydrothermal chimneys at a depth of 2200 m. In situ temperatures of these precipitates were not measured because of the sampling technique limitations. Immediately after retrieval, samples were frozen and stored until further analyses.
Mineralogy and chemical analysis
Iron–silica-rich precipitates were dried at approximately 50 °C and thoroughly ground using a mortar and pestle. X-ray diffraction (XRD) pattern analysis was then performed by a Rint 2000 X-ray diffractometer (Rigaku Corporation, Tokyo, Japan) using Cu Kα radiation at 40 kV and 30 mA. Diffraction angles (referred to as ‘2θ’) corresponding to the atomic structure unique to each mineral were measured. Bulk chemical analyses were carried out using X-ray fluorescence (XRF) and ICP-MS at the Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, China.
Morphological observation and ultrastructure analysis
Samples were examined using FEI Quant 400 environmental scanning electron microscopy (ESEM, the Netherlands). Gold coating on sample surfaces was not required for wet samples using environmental SEM, which avoided pretreatments on spectral analysis. In addition, we examined the ultrastructure of the hydrothermal precipitates with transmission electron microscopy (TEM). Small fragments fixed in 4% glutaraldehyde were prepared by washing three times with 0.1 M phosphate buffer (pH 7.4), further fixed with osmium tetroxide at 4 °C for 2 h and dehydrated through a series of ethanol solutions (10%, 20%, 30%, 40%, 50%, 60%, 70%, 80%, 90% and 100%, 10 min each). Dehydrated samples were then washed twice in propylene oxide, followed by overnight stand in a 50/50 mixture of propylene oxide and Agar100 resin. Samples were then allowed to stand in 100% resin for 24 h and then transferred into fresh embedding tubes where they were set in fresh resin and polymerized at 60 °C for 24 h. The samples were then sectioned on an ultramicrotome, mounted on copper grids and stained with uranyl acetate and lead citrate to improve contrast. Micro-area chemical composition of mineral surfaces was analysed on a Genesis energy dispersive spectrometer (EDAX).
DNA extraction, amplification and cloning
The DNA was extracted by SDS-based extraction with some modification (Zhou et al., 1996). In brief, about 5 g of samples was mixed with 13.5 mL of DNA extraction buffer (100 mM Tris–HCl, 100 mM sodium EDTA, 100 mM sodium phosphate, 1.5 M NaCl, 1% CTAB) and 100 μL of proteinase K (10 mg mL−1; Sigma) in tubes by horizontal shaking at 225 r.p.m. for 30 min at 37 °C. After shaking, 1.5 mL of 20% (w/v) SDS was added and samples were incubated in a 65 °C water bath for 2 h. The supernatants were collected after centrifugation at 6000 g for 10 min and transferred into 50-ml centrifuge tubes. The supernatants were mixed with an equal volume of chloroform isoamyl alcohol (24 : 1, v/v). The aqueous phase was recovered by centrifugation and precipitated with 0.6 volume of isopropanol for about 1 h. Crude nucleic acids were obtained by centrifugation at 16 000 g for 20 min at room temperature, washed with 70% ethanol and resuspended in sterile deionized water. The crude nucleic acids were purified with a cycle-pure kit (Omega).
The 16S rRNA genes were amplified by universal bacterial and archaeal primers (Lane, 1991; Delong, 1992). Bacterial 16S rRNA gene was amplified using Eubac27f (5′-AGA GTT TGA TCC TGG CTC AG-3′)/Eubac1492r (5′-GGT TAC CTT GTT ACG ACT T-3′); and Arch21f (5′-TTC CGG TTG ATC CYG CCG GA-3′)/Arch958r (5′-YCC GGC GTT GAM TCC AAT T-3′) were used for archaea with products of 1500 and 900 bp, respectively. Amplification conditions were as follows: an initial denaturalization step of 94 °C for 4min and then denaturation at 94 °C for 60 s, annealing at 55 °C for 45 s, and extension at 72 °C for 60 s for a total of 30 cycles, followed by a final extension of 72 °C for 10 min. All the PCR products were purified with a Gel-extraction kit (Omega) following the manufacturer's instructions. Purified PCR products were cloned into the pMD18-T vectors (Takara, Japan) and transformed to competent Escherichia coli DH5α cells (Takara). The PCR of the bacterial colonies was used to screen the presence of the correct-size inserts with the vector-specific primers M13f (5′-GTA AAA CGA CGG CCA G-3′) and M13r (5′-CAG GAA ACA GCT ATG AC-3′). Clones containing target 16S rRNA gene were subjected to restriction fragment length polymorphism (RFLP) analysis. Representative clones of archaea and bacteria with unique RFLP banding patterns were chosen for sequencing.
Quantification of 16S rRNA gene
Quantification of the microbial 16S rRNA gene was performed by fluorescence quantitative real-time PCR. Amplification was performed on the 7500 real-time PCR system (Applied Biosystems) in 20-μL reaction mixture, which consisted of 1 μL of template DNA (10 ng), a 0.15 μM concentration of each primer and 10 μL of Power SYBR green PCR master mix (Applied Biosystems) with ROX and SYBR green I. Melting curve analysis was performed after amplification, and the cycle threshold was set automatically using system 7500 software (1.3). Primers used to amplify the 16S rRNA gene were selected according to previous research (Treusch et al., 2005; Nunoura & Takai, 2009).
Sequencing and phylogenetic analysis
Representative clones were directly sequenced by dideoxynucleotide chain termination using an ABI 3730 capillary electrophoresis sequencer (Applied Biosystems) with T-vector universal primers, M13f and M13r. The whole insert sequences were spliced by dnaman software (version 6.0), and the vector sequences were deleted. Archaeal and bacterial 16S rRNA gene sequences were obtained with lengths of about 900 and 1500 bp, respectively. Chimeric sequences were checked using Bellerophon (3.0) at www.greengenes.lbl.gov (Huber et al., 2004; DeSantis et al., 2006). The program dotur was used to determine the operation taxonomic units (OTUs) for each sequence using a 97% similarity cut-off. Nonchimeric sequences were submitted to the Advanced blast search programme (available through the National Center for Biotechnology Information) to find closely related sequences in GenBank and EMBL databases for phylogenetic analysis. All clones sequences and matched sequences were aligned using the software ClustalX 1.83, and alignment positions with gaps were removed. Phylogenetic trees were constructed by neighbour-joining (NJ) using Mega (5.05) with default parameters (Tamura et al., 2011). Bootstrap analysis was used to provide confidence estimates of tree topologies.
Nucleotide sequence accession numbers
The sequences reported in this study were deposited in the GenBank database. Bacterial sequences have GenBank accession numbers GU220728–GU220769 and archaeal sequences GU207312–GU207319, respectively.
Mineralogy and bulk chemistry
The Fe–Si-rich hydrothermal precipitates had a yellow interior with black to orange coatings. X-ray diffractometry (XRD) was used to identify different mineral phases. Results indicate that our samples were poorly crystallized. According to the XRD traces, the samples were composed mainly of amorphous silica, with a scattering broad band of maximum intensity centred at about 4 Å (22° 2θ), similar to opal-A (Rodgers et al., 2004). The proportion of opal-A was > 90%, forming the dominant phase present in the precipitates. However, we did not detect any iron oxyhydroxides such as the two-line ferrihydrite and goethite.
Major chemical analysis by X-ray fluorescence (XRF) revealed that the hydrothermal deposits were rich in Si (74.2 wt%, SiO2). Although no iron oxyhydroxides appeared according to XRD results, relatively high concentrations of Fe2O3 (about 9.8 wt%) were detected. Concentrations of other major elements (Al, Ca, K, Mg, Mn, Na, Sr, Cr, P) ranged from 0.1 to 1.3 wt% (Supporting Information, Table S1).
Morphological observation and description
The microscale morphologies of the hydrothermal precipitants were examined using environmental scanning electron microscopy (ESEM). Delicate structures such as filaments, stalks, rods, spheres and their aggregates were observed. Filament morphology was particularly variable and ranged from short simple-branching filaments to complex filament networks. Some were remarkably similar to bacterial-like structures.
Straight filaments were abundant and frequently entwined with each other, with dense arrays throughout the precipitates (Fig. 2a–c). The filaments or long bacilliforms were tens to near a hundred micrometre long, with external diameters between 0.5 and 1.5 μm. Occasionally, irregular-shaped grains with diameters of 0.5–2.0 μm occurred on the surface of filaments (Fig. 2b). These rod-like structures resembled the sheath of Leptothrix ochracea, a well-known iron-oxidizing bacterium (FeOB). EDS analyses confirmed that the surfaces of these structures were mainly encrusted by amorphous silica (SiO2). In addition, although the surfaces of these nonbranching silicified bacterial-like structures seemed smooth, many ringed grooves were observed after magnification (Fig. 2c,d). Uneven precipitation of amorphous silica may be responsible for the occurrence of these ringed grooves mentioned above.
Ribbon-like helical stalks
The distinctive filamentous ribbon-like helical stalks were recognized from the iron–silica precipitates (Fig. 2h). These special structures closely resembled those biogenic Fe-rich oxides produced by neutrophilic Fe-oxidizing bacteria such as Gallionella ferruginea and Mariprofundus ferrooxydans. EDS analysis showed that the distinctive filamentous ribbon-like helical stalk was mainly composed of Si (28.77 wt%), Fe (21.22 wt%) and O (48.76 wt%). The unique features of these stalks included the ribbon-like regular helical or twisted morphologies generally present in iron-rich microbial mats from deep-sea hydrothermal fields or subterranean environments (Ferris et al., 1999; Emerson & Moyer, 2002; Edwards et al., 2004). As products of FeOBs metabolic activity, their occurrences were used as direct evidence of bacteriogenic mineralization (Chan et al., 2011).
Curved filaments and branching filaments
Commonly occurring, curved filamentous structures were also observed (Fig. 2f,g). These structures varied from several to tens micrometre, occasionally up to a 100 μm in length. Some were also bifurcated and formed branching filaments (Fig. 2g). Based on the observed morphologies, the curved filaments and stalk-like fragments resembled the extracellular filamentous material produced by M. ferrooxydans PV-1 strain (Emerson & Moyer, 2002; Emerson et al., 2007). SEM–EDS analyses indicated that all these filaments appeared to be heavily encrusted with siliceous precipitates (SiO2).
In addition to those distinctive morphologies described above, colloid particles with irregular spherical shapes were also abundant and dominated the analysed deposits (Fig. 2e). Usually, they agglomerated upon suitable substrates and formed globular aggregates with diameters varying from 0.5 to 20 μm. Occasionally, these microspheres coagulated and became loosely interwoven, which helped cement various microbe-like structures. Chemical analyses indicated that these aggregates were composed of a gel-like material rich in SiO2. From morphologies, composition and mineralogy, we conclude that these structures were likely the first-phase silica deposits, that is, opal-A (Rodgers et al., 2004).
Transmission electron microscopy
Examination of the samples by TEM and EDS revealed two different types of mineralization. The first type was silicification, mainly related to siliceous precipitation (Fig. 3b,c), while the second was chiefly involved in the formation of iron oxyhydroxide (Fig. 3a). Amorphous siliceous precipitation was common and often formed various spheres, irregular morphologies and their aggregates (as shown in Fig. 3b). The cross-sections of some filaments exhibited hollow structures with relatively rough walls. Noticeably, the walls of different hollow structures had different chemical components, which were mainly composed of either silica (Fig. 3c) or iron oxyhydroxide (Fig. 3a). Cross-sections showed that some filaments were filled with an iron-rich matrix surrounded by amorphous silica (Fig. 3e). TEM revealed a linear chain of Fe-rich oxyhydroxides in the centre of the filaments encrusted by a siliceous matrix (Fig. 3f,g). In addition, TEM observations of thin cross-sections found that some cells were undergoing intracellular mineralization, with the cytoplasm being replaced by amorphous materials in the lysed bacterial cells (Fig. 3d). Energy dispersive X-ray spectroscopy indicated that the cell walls had higher iron and silicon content (18.61 and 3.93 wt%) than the inner materials (3.72 and 1.37 wt%, respectively). TEM–EDS analysis suggested that microbe-like structures were generally encrusted by amorphous silica, indicating their role as nucleation site for the silica precipitation.
Quantitative PCR of the small subunit (SSU) 16S rRNA gene and biomass estimation
The results of the qPCR indicated that the number of archaeal 16S rRNA genes were about 6.21 × 107 copies per gram of hydrothermal precipitates, while the bacterial 16S rRNA genes were about 1.22 × 108 copies per gram. Based on the qPCR results and assuming an average 16S rRNA gene copy number of 4.17 and 1.71 per cell for bacteria and archaea (Lee et al., 2009), we estimated that the cell densities of bacteria and archaea inhabited in our precipitates were 2.93 × 107 and 3.63 × 107 cells g−1, respectively.
Diversity of 16S rRNA genes
Phylogenetic analyses of PCR-amplified 16S rRNA gene from the hydrothermal precipitates were carried out to investigate the microbial communities in the precipitates.
Archaeal SSU rRNA gene clone analysis
Eight unique archaeal 16S rRNA gene phylotypes were identified from a total of 76 representative clones. Five of the phylotypes (including 68 clones) were primarily affiliated with the marine group I (MGI) Crenarchaeota group. Members of this group are almost ubiquitous in various oceanic environments, and sequences related to our phylotypes have been detected mainly in deep-sea sediments on the Pacific Nodule Province, Japan Trench, Nankai Trough, and the Antarctic and Aegean Seas (Fig. 4). Noticeably, sequences similar to phylotype TVG13-A8 and A66 included the only pure culture of MGI, Nitrosopumilus maritimus (identity = 97–98%), an autotrophic ammonia-oxidizing marine archaea that grows chemolithoautotrophically by aerobically oxidizing ammonia to nitrite (Konneke et al., 2005). In the present study, 25 clones were closely related to phylotypes TVG13-A8 and A66, accounting for 33% of the archaeal library. In addition, three residual phylotypes (representing eight clones) were of archaeal lineage and classified as Euryarchaeota (Fig. 4 and Table S2).
Bacterial SSU rRNA gene clone analysis
A total of 78 positive clones from the bacterial 16S library were analysed, with 41 phylotypes identified for phylogenetic analysis. These sequences mainly fell within Proteobacteria (α-, β-, γ-, δ-, ε- and ζ-), Verrucomicrobia and Planctomycetes (Fig. 5, Fig. S1 and Table S3).
Members of α-Proteobacteria contained 20 phylotypes (representing 36 clones) and dominated the bacterial communities, accounting for 46% of the total clones. Within α-Proteobacteria, bacterial populations were diverse and covered various subclasses such as Rhizobiales, Rhodobacterales, Kordiimonadales and Rhodospirillales (Fig. S1). Five phylotypes (seven clones) were assigned to Rhizobiales and were most closely related to sequences from uncultivated organisms in various sea floor hydrothermal environments, such as sediments, lavas and submarine hot spring. Bacteria belonging to Rhodospirillales included three phylotypes representing three clones. Together with several pure cultures, this phylogenetic clade was formed from the clones and environmental sequences of the Pacific Ocean, Sargasso Sea, eastern Mediterranean Sea, Loi′hi Seamount and Antarctic Booney. Sequences affiliated to Rhodobacterales and Kordiimonadales constituted 17% (four phylotypes, nine clones) and 4% (one phylotype, four clones) of the bacterial sequences, respectively. Other sequences within α-Proteobacteria showed high similarity to uncultivated organisms and low similarity to cultured species (generally < 91%).
Six phylotypes, including 13 clones with a proportion of 16.7%, were identical to the members of ε-Proteobacteria. Most of the phylotypes were related to clones or isolates from different marine environments such as hydrothermal chimney, cold-seep and sediments (Fig. 5). The distributions of other groups were as follows: β-Proteobacteria (one phylotype, one clones), γ-Proteobacteria (three phylotypes, five clones), δ-Proteobacteria (four phylotypes, eight clones), candidate ζ-Proteobacteria (two phylotypes, eight clones), Verrucomicrobia (one phylotype, two clones) and Planctomycetes (three phylotypes, four clones). In addition, one phylotypes (TVG13-B7) branched into unclassified groups owing to their low similarity to known sequences.
Notably, several phylotypes aligned well with those well-known Fe-oxidizing bacteria. Phylotype TVG13-B96 (representing one clone) fell into β-Proteobacteria and shared highest (97%) sequence similarity with the Gallionella phylotype YS18Uc25 obtained from Fe–Si-rich microbial mats at the hydrothermal field of the Southern Mariana Trough (Kato et al., 2009). We also detected another important group involved in Fe-oxidation, specifically, a new Candidatus class of Proteobacteria (ζ-proteobacteria) widely distributed in deep-sea environments (Emerson et al., 2007). Two phylotypes, TVG13-B2 and B40, were aligned with the cultivated iron-oxidizing organism M. ferrooxydans and environmental clones within this group obtained from various hydrothermal vents systems.
The dominance of amorphous opal-A and low concentrations of metals suggest that Fe–Si-rich precipitates studied in this paper belong to typical low-temperature hydrothermal deposits, which were probably precipitated from low-temperature hydrothermal fluids (Boyd & Scott, 2001). Although some abiological processes could result in microorganism-like micro-textures (Garcia-Ruiz, 1998), morphological characteristics observed in our samples afford further support of their bacteriogenic origin. Typical morphologies observed in our study include filamentous and stalk-like forms. These filamentous structures were abundant and geometrically consistent with the size, form and aggregation of microorganisms, suggesting that microorganisms probably have played an important role in the mineralization.
Biomineralization related to neutrophilic iron oxidizers
Tubular sheaths, helical or twisted stalks and slender or irregular filaments, which are characteristic and distinguishable biosignatures, are generally considered as reliable indicators of biomineralization involving the FeOBs (Juniper & Fouquet, 1988; Emerson & Moyer, 2002; Emerson et al., 2007; Chan et al., 2011). Previous studies have established the corresponding relationship between those distinctive morphologies and certain species of the known FeOBs (Emerson & Moyer, 2002; Emerson et al., 2010; McAllister et al., 2011). In this study, the samples contained numerous filamentous structures whose morphologies were similar to those produced by known FeOBs. Among these characteristic structures, helical stalks shown in Fig. 2 are the most commonly observed structures, offering supporting evidence for a biological origin of these structures, which were likely formed by G. ferruginea or M. ferrooxydans. Generally, these FeOBs obtain energy from Fe-oxidation (Fe2+→Fe3+) and form Fe-rich stalks to eliminate the ferric waste product (Chan et al., 2011; Suzuki et al., 2011). Emerson et al. (2007) demonstrated that iron-oxidizing bacteria M. ferrooxydans produced filamentous stalk-like structures composed of Fe oxyhydroxide during chemolithotrophic growth. Our SEM–EDS results showed that the stalk-like microstructures in our samples were mainly composed of iron-rich materials. Phylogenetic analyses confirm the presence of the FeOBs known for their direct involvement in the formation of Fe-rich precipitates. The two phylotypes (TVG13-B2, B40) detected in the precipitates aligned well with M. ferrooxydans and other sequences within the ζ-proteobacteria group (Fig. 5). One phylotype, TVG13-B96, showed high identity to Gallionella. spp. Thus, on the basis of ultrastructural and phylogenetic analyses, we tentatively conclude that the tubular sheaths, filaments, helical and twisted stalks observed in the CDE hydrothermal field are of bacteriogenic origin, formed probably with the involvement of FeOBs.
Interestingly, we detected one clone related to Gallionella in the β-proteobacteria class. Phylotype TVG13-B96 showed high identity (97%) to clone YS18Uc25, which is the only Gallionella phylotype detected from deep-sea hydrothermal environments (Kato et al., 2009). As discussed in early reports (e.g. Kennedy et al., 2003), it was initially assumed that ribbon-like helical stalks were produced by freshwater Gallionella spp., almost no sequence data or convincing microbial evidence exist to confirm the occurrence of Gallionella in marine environments. With the isolation of M. ferrooxydans (Emerson & Moyer, 2002; Emerson et al., 2007), which could produce strikingly similar Fe-rich stalks but is phylogenetically distant from Gallionella, it was proposed that those stalks should be ascribed to ζ-proteobacteria because it has been widely detected in diverse hydrothermal habitats around the world. Together with YS18Uc25, our results suggest that members related to Gallionella indeed exist in deep-sea hydrothermal vents and probably contribute to biomineralization of iron.
The role of microorganisms in silicification
Results of morphological observation and chemical analysis indicate that silicification was a common mineralizing phenomenon in our CDE hydrothermal precipitates. SEM- and TEM–EDS analyses showed that many microstructures were heavily encrusted by amorphous silica and those siliceous spherules, strumae and irregular forms could aggregate on the surfaces of structures (Figs 2 and 3). Although the role of microorganisms in mediating silicification remains debated, it has been suggested that microbial cell surfaces and their extracellular polymers can act as excellent nucleation sites for silica precipitation (Urrutia & Beveridge, 1993; Fein et al., 2002; Phoenix et al., 2003; Konhauser et al., 2004). When hydrothermal fluids with high concentrations of dissolved silica are mixed with ambient low-temperature fluids, amorphous silica rapidly precipitates on the surface of multifarious materials for the reduced solubility and then forms amorphous opal-A. Once the encrusted core (microbial cell or their organic affiliates) decomposes, the siliceous crusts would remain and cause the observed central hollow canals as shown in Fig. 3c.
Biogenic ultrastructures related to FeOBs, including stalks and various filaments, probably also served as the scaffolding for silica accumulation and precipitation and thus contributed significantly to silicification in our samples. Simulation experiments suggest that Fe plays an important role in the precipitation of silica (Fein et al., 2002) and can significantly accelerate the rate and extent of Si removal from solutions (Yee et al., 2003). Therefore, filamentous structures typically are heavily encrusted by amorphous silica (Fig. 2). Among the TEM micrographs, we observed an iron-rich filamentous core surrounded by a matrix of silica (Fig. 3f,g). Even the fresh-looking ribbon-like helical stalk was also coated by the SiO2 (Fig. 2h), suggesting that biogenic filamentous structure may have served as templates for silica precipitation.
Microbial diversity inhabited in the Fe–Si-rich precipitates of the CDE Field
Up to date, numerous molecular analyses have been carried out to investigate bacterial communities related to low-temperature hydrothermal Fe–Si-rich precipitates (Emerson & Moyer, 2002; Davis et al., 2009; Hodges & Olson, 2009; Kato et al., 2009; Rassa et al., 2009; Forget et al., 2010; Edwards et al., 2011; McAllister et al., 2011). Most of the studies showed that ζ-proteobacteria, including the only isolate M. ferrooxydans and related uncultured clones, are abundant and predominant. However, our molecular analysis revealed obviously different and diverse bacterial communities. A variety of bacterial 16S rRNA gene phylotypes were recovered from the Fe–Si-rich precipitate samples. Members of α-proteobacteria instead of FeOBs-related groups dominated the bacterial clone library (46.0% of the clone library). Although α-proteobacteria are widely distributed in various marine environments such as surface seawater, water column, sediments and hydrothermal environments, sequences closely related to our phylotypes mainly come from sediments (as shown in Table S3). The ε-proteobacteria were the next largest group accounting for 16.7% of the clone library. Phylotypes within this group were closely related to the known Sulphurimonas spp. and Sulphurospirillum spp. (Fig. 5), which are sulphur cycle-related bacteria (Inagaki et al., 2003). In addition, members of γ- and δ-proteobacteria also occurred with low proportions. Members of the known FeOBs such as Gallinella and ζ-proteobacteria were relatively low in abundance. Generally, the abundance of FeOBs is closely related to the concentrations of ferrous iron in the hydrothermal fluids and the low abundance of FeOBs means that the supply of Fe2+ was probably limited. So most of biosignatures detected in this study probably are the remnants of earlier activities of FeOBs. With the decreasing ferric iron concentrations, the majority of FeOBs probably died off and disappeared.
In contrast to the extensive eubacteria investigations, archaeal community composition has been rarely reported in such environments (Moyer et al., 1995; Kato et al., 2009). Representatives of the MGI were the largest group and dominated in the archaeal library (accounting for 90%) in our samples. Moreover, nearly 33% of the clones within MGI showed high sequence similarity (97–98%) to N. maritimus, a chemolithoautotrophic ammonia oxidizer (Konneke et al., 2005). This strongly suggests that ammonia oxidation was common and the related microorganisms likely contributed to the carbon and nitrogen cycle in the CDE hydrothermal field. Data from the amoA functional gene analysis also supported this conclusion (data not shown). In addition, phylotypes fallen into the DHVE group were also detected (TVG13-A6 and TVG13-A79, representing seven clones). As the DHVE group are generally considered to be restricted to high-temperature hydrothermal environments (Hoek et al., 2003; Reysenbach et al., 2006), the detection of the DHVE groups in low-temperature hydrothermal niches implies that these phylotypes probably come from the vicinal high-temperature vents.
In conclusion, this study revealed the occurrence of microbial mineralization and microbial communities in the low-temperature hydrothermal precipitates of the CDE field located at ESLC. We described distinct ultrastructures produced by unique microorganisms and characterized biomineralization involving the FeOBs and silicification. Special morphological characteristics are good indicators for recognizing biological signatures in modern and fossil hydrothermal vent environments. Although morphological characteristics are similar to what was observed in other hydrothermal environments, microbial diversity, abundance and component inhabited in these precipitates are distinctive. However, because of the limitations in our sampling procedures, the lack of basic environmental parameters hinders our interpretation for the possible reasons of the differences. It is important to note that our samples, mainly composed of amorphous silica (SiO2, 74.2 wt%) with much less iron (Fe2O3, 9.8 wt%) are obviously different from those Fe-rich flocculent mats consisting dominantly of iron oxides/oxyhydroxides with variable amounts of silica. The difference in mineralogy and chemical composition indicates the different venting fluid characteristics and precipitating stage (Halbach et al., 2002), which could have significantly influenced the microbial composition in our Fe–Si-rich precipitates present here. Nevertheless, the present study provides valuable insights into microbial mineralization and microbiology of Fe–Si-rich precipitates in deep-sea low-temperature hydrothermal environments.
We are grateful to Christian Griebler and two anonymous reviewers whose insightful comments and suggestions greatly improved the manuscript. We thank all crew members of R/V DaYang YiHao for retrieving the samples studied. The authors would like to warmly thank Dr David Emerson for information regarding iron-oxidizing bacteria. This work was financially supported by the National Natural Science Foundation of China (NSFC, No. 41002122) and National Basic Research Program of China (973 Program, No. 2012CB417300).
Additional Supporting Information may be found in the online version of this article: