PROF. DANIEL ARIZTEGUI (Orcid ID : 0000-0001-7775-5127)
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Article type
: Original Research Article
Banded Iron Travertines at the Ilia Hot Spring (Greece): An interplay of biotic and
abiotic factors leading to a modern Banded Iron Formation analog?
Christos Kanellopoulos1,2, Camille Thomas2, Nikolaos Xirokostas3 and Daniel Ariztegui2,*
1
National and Kapodistrian University of Athens, Department of Geology and
Geoenvironment, Panepistimioupolis, Ano Ilissia, 15784 Athens, Greece, e-mail:
ckanellopoulos@gmail.com
2
Department of Earth Sciences, University of Geneva, Rue des Maraîchers 13, 1205 Genève,
GE, Switzerland, e-mail: Camille.Thomas@unige.ch , daniel.ariztegui@unige.ch
3
Institute of Geology and Mineral Exploration (I.G.M.E.), 1st Spirou Louis St., Olympic
Village, 13677, Acharnae, Greece, e-mail: nikosxirokostas@yahoo.com
* Correspondent author: daniel.ariztegui@unige.ch
Abstract
A hot spring at Ilia in the Greek Island of Euboea precipitates iron-rich travertine at an oregrade concentration (up to 35.3 wt% Fe). This hydrothermal chemical sediment system
deposits bands of iron oxihydroxides (ferrihydrite), millimetres to centimetres thick,
alternating with calcium carbonate dominated layers, creating “Banded Iron Travertine”
(BIT). The ferrihydrite laminae display a dendritic texture formed of spherical nodules often
covering filaments identified as bacterial stalks of Zetaproteobacteria. These microaerophilic
iron-oxidizing bacteria were identified by their 16S rRNA gene sequences in ferrihydrite-
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doi: 10.1002/dep2.55
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enriched samples from areas under high water flow. They were missing in the
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aragonite/calcite-dominated samples exhibiting features of aerial exposure and cyanobacteria
instead. These characteristics, and the relative depletion in Fe-rich layers of redox sensitive
elements like Mn and Ce, as well as the presence of halite in Ca-rich layers, suggest that the
bands form by successive changes in hydrothermal flow. This allowed microaerophilic iron
oxidation to form Fe-rich layers, while Ca-rich bands precipitated when the hydrothermal
water had time to equilibrate with the atmosphere. This seawater-dominated hydrothermal
system is enriched in reduced iron and rapidly precipitating carbonates and ferrihydrite in the
form of bands, having similarities to “Banded Iron Formation” (BIF). BIF represent archives
of Earth’s primitive biogeochemistry although the combined abiotic and biotic processes that
have likely led to their formation are not fully resolved. Diagenesis and metamorphism have
a strong imprint on BIF. Thus, continuous efforts are pursued to identify modern analogues
that could help unravel their formation. Although carbonate is not a common feature of BIFs,
Ilia system provides an interesting analog for their depositional processes and potential
microbial-mineral associations they may have hosted. It also presents pre-diagenesis facies
association and mineralogy that could bring new clues for unraveling BIF modes of
formation and the salient biogeochemical conditions characteristic of their original
depositional environment.
Keywords Calcium carbonates, ferrihydrite, hydrothermal springs iron-rich thermogenic
travertines, Zetaproteobacteria.
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INTRODUCTION
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Among the most important iron ore deposits on Earth are the spectacular and enigmatic
Banded Iron Formations (BIFs). Despite extensive studies, their modes of depositions have
not been fully resolved; although one of the prevalent models is that BIFs are thought to be
the result of the reaction between hydrothermal reduced iron, and photosynthetically
produced oxygen. Microbes are generally recognized as important contributors to the specific
sedimentological conditions of these deposits, both regarding the processes of primary iron
oxidation and secondary iron reduction (Posth et al., 2013). Since BIFs likely hold
information on some of the earliest forms of life on Earth, they are extensively investigated
and analogs for their mode of formation are thoroughly searched for.
Active hydrothermal iron-rich deposits are among the targets of this search. They can be
found in terrestrial environments i.e. iron-rich thermogenic travertines (Takashima & Kano,
2005; Takashima et al., 2011; Kanellopoulos et al., 2017) and in submarine hydrothermal
environments (Pichler & Veizer, 1999; Kilias et al., 2013; Bortoluzzi et al., 2017). In these
systems, the presence of microbial activity is most often identified at redox interfaces and has
been suggested to play an active role in the formation of iron minerals such as iron oxides
(Widdel et al., 1993; Konhauser, 1998; Kappler & Newman, 2004). Hot springs are ideal
environments for iron oxidation, since the hydrothermal fluid is often enriched in Fe(II) and
free of oxygen. In such conditions, a steep redox gradient develops in the water immediately
adjacent to the spring vent through uptake of atmospheric O2 (Takashima et al., 2008). In
near-neutral pH hydrothermal springs, the Fe-rich deposits consist primarily of ferric
hydroxides (commonly as ferrihydrite). These ferric hydroxides precipitate readily abiotically
in oxygenated environments or their precipitation can be microbially mediated and influenced
(Konhauser, 1998; Chan et al., 2011). When microbes are involved, rates of iron
mineralization can increase four-fold (Kasama & Murakami, 2001). These processes
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generally occur at redox interfaces, where iron-oxidizing bacteria are commonly found and
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where microaerophilic conditions dominate (Konhauser, 1998). Such conditions have been
suggested in the formation of BIFs, and iron-oxidizing bacteria as associated with the
formation of iron bands in Precambrian BIFs (Holm, 1987, Chaudhuri et al. 2001; Konhauser
et al. 2002). However, the study of iron mineralization in hydrothermal systems is often
hampered by the poor accessibility of active sites, and the instable characteristics of
ferrihydrite therein.
This study characterizes the iron-rich thermogenic travertines of Ilia, on the Greek island
of Euboea. The depositional system hosts almost pure ferrihydrite lamina which, together
with fast precipitation rates, high iron enrichment and specific hydrothermal chemistry
(Kanellopoulos et al., 2017) provides a unique setting for the study of laminated iron
chemical sediments. The purpose of the work presented in this paper is to understand the
depositional processes leading to the formation of laminated iron-rich deposits in Ilia and to
further link them to BIF depositional models. This study documents the geochemistry of the
Fe-rich hydrothermal fluids from the Ilia area, the macro-facies and micro-facies, the
petrographical characteristics, mineralogical and geochemical composition of the newly
formed iron-rich thermogenic travertine, and the microbial communities associated with the
different facies of this deposit. The Fe-rich travertine is compared with active hydrothermal
systems elsewhere and all of the available data synthesized to propose a model for Banded
Iron Travertine (BIT) deposition, with possible analogy to the formation of BIFs. The goal is
to provide a depositional model associated to an easily accessible and dynamic system
precipitating banded iron-rich chemical sediments.
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GEOLOGICAL SETTING
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Ilia is located in the north-western part of Euboea Island, Greece (Fig. 1). The geological
setting of the region is unique since it is located at the western extremity of the North
Anatolian Fault and is in a back-arc position with respect to the South Aegean Active
Volcanic Arc (Pe-Piper & Piper, 2002; Vött, 2007; Ring et al., 2010). It is one of the most
neo-tectonically active areas in Greece dominated by extensional tectonics similarly to the
rest of the Aegean Sea.
Ilia’s hot spring i.e. artesian borehole (38o 51΄ 07΄΄N, 23o 07΄ 44΄΄E) is one surface
manifestation of a large geothermal system with other surface manifestations of hot springs in
northern Euboea island and the neighboring area of Sperchios (mainland; Kanellopoulos,
2011; Kanellopoulos et al., 2017). This hydrothermal system is controlled by active tectonics
and supplied with heat by a deep magma chamber (Kanellopoulos et al., 2017), identified at
depths of 7-8 km under the Northern Euboean Gulf (Karastathis et al., 2011), which has the
Plio-Pleistocene trachyandesitic volcanic center of Lichades as a surface manifestation. A
salient feature of Euboea`s hot springs is the dominance of thermogenic travertine deposition
(Kanellopoulos, 2011, 2012, 2013) including the Fe±As -rich ore-bearing travertines of Ilia
(Kanellopoulos, 2011, 2012; Kanellopoulos et al., 2017).
The hydrothermal fluids of northern Euboea’s hot springs have near neutral pH and a
sodium-chloride composition. They are similar in their chemical characteristics and are
classified as deep geothermal fluids, with volcanic origin affinities (Kanellopoulos et al.,
2017). Based on geochemical and isotopic studies (Shimizu et al., 2005; Kanellopoulos et al.,
2011; Dotsika, 2015; Kanellopoulos et al., 2017) their chemistry is controlled mainly by
contribution of three components: i) high seawater participation, ii) deeper magmatic fluids,
and iii) the local bedrock. The chemical composition of the thermogenic travertine, together
with drilling data (Gkioni-Stavropoulou, 1998; Hatzis et al., 2008; Kanellopoulos et al.,
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2017), strongly suggest that the source of calcium for the extensive travertine deposits of
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Euboea is the dissolution by geothermal fluids of marble/limestone located below the
metamorphic sequence of Aedipsos and Ilia.
MATERIAL AND METHODS
Hot water samples
Hydrothermal fluid samples from the hot spring/artesian borehole were collected from the
mouth of the pipe (Fig. 2A through D). Physicochemical parameters such as temperature, pH,
electrical conductivity (E.C.) and total dissolved solids (T.D.S.) were measured in-situ, using
portable probes. The pH-meter was calibrated with standard buffer solutions of pH 4.0 and
7.0 before any measurements were taken. The pH measurement error, including accuracy and
reproducibility, is better than ±0.05 pH units. Temperature was measured with the probe
connected to the pH-meter and the error is estimated to be less than ±0.3 °C. Moreover, a
thermal imaging camera was used in order to present through thermal images the temperature
changes at the sampling site. Thermal imaging camera is a type of thermographic camera,
which is reading infrared radiation as visible light and allow us to see areas of heat through
water or solid rock.
Water was collected in polyethylene bottles for laboratory analyses. Aliquots of 250 mL
intended for the determination of trace elements were acidified to pH < 2 with analytical
grade HNO3 (Suprapur 65%). All samples were stored in a portable cooler containing ice
packs, transported to the laboratory and refrigerated at 4 °C until analysis. One-liter aliquots
(non-acidified) were filtered in the laboratory before major ion determinations.
The major ion concentrations were measured using spectrophotometry, titration and
Inductively Coupled Plasma-Optical Emission Spectrometry (ICP-OES; Perkin Elmer
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Optima 5300 DV). The trace element concentrations were measured using Inductively
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Coupled Plasma-Mass Spectrometry (ICP-MS; Perkin Elmer Sciex Elan 6100).
Travertine samples
The hydrothermal spring of Ilia vents from an artesian borehole accessible from the road
that run along the beach. The water then flows along a 3-5 m long pipe and out onto the
beach (Fig. 2). Samples of thermogenic travertine were collected from the top part of the
borehole, from the venting point of the pipe and from the deposits at the beach (Fig. 2). The
mineralogical composition of the main mineral phases in these travertines was identified with
X-Ray Diffraction (XRD) using a Siemens Model 5005 X-ray diffractometer, Cu Ka
radiation at 40 kV, 40 nA, 0.020o step size, and 1.0 sec step time. The XRD patterns were
evaluated using the EVA program of the Siemens DIFFRACplus and the D5005 software
package. The minor mineral phases were identified by Scanning Electron Microscopy (SEM)
and Energy Dispersive Spectroscopy (EDS). The SEM-EDS analyses were carried out using
a Jeol JSM 5600 SEM instrument, equipped with an Oxford ISIS 300 micro analytical device.
The travertine samples were analysed for whole rock geochemistry after drying and
pulverizing in an agate mortar and mill to less than 0.075 mm. The samples were digested
with a mixture of HCl-HNO3-HF acids and analysed with Inductively Coupled Plasma–
Optical Emission Spectroscopy method (ICP-OES; Perkin Elmer Optima 5300 DV) for Ca,
Na, P, S, Si, and by Inductively Coupled Plasma-Mass Spectrometry method (ICP-MS;
Perkin Elmer Sciex Elan 6100) for a series of trace elements, including rare earth elements
(REE). Analytical data quality was test with internal standards, certified and in-house
reference materials in random positions within the analytical batch and by blank analysis and
duplicate analysis of a proportion of the samples (Ramsey et al., 1987).
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Molecular Biology
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Samples for microbiological studies were collected at the vent of the artesian borehole
(Ilia Drill for ID-labelled samples, Fig. 3A and B) and at the pipe outlet (Ilia Pipe for IPlabelled samples, Fig. 3C and D). They experienced different environmental conditions at
time of sampling, which are detailed in Table 1.
Hard rock samples were taken using a chisel and a hammer cleaned and sterilized with
ethanol. Soft material was sampled using a sterile scalpel. All samples were stored in 50 mL
falcon tubes or zip-lock bags and kept at -20°C until further processing. Hard rock samples
were then crushed under clean conditions in a sterilized agate mortar. Two grams of
processed sample were used for DNA extraction using the MOBIO power soil kit. Triplicate
DNA amplification was realized with a total of ~10 ng of DNA per triplicate using universal
primer
515F
(5′-GTGYCAGCMGCCGCGGTA-3′)
and
909R
(5′-
CCCCGYCAATTCMTTTRAGT-3′) for the V4-V5 hypervariable region of the 16S rRNA
gene (Wang & Qian, 2009), with indexes integrated following the dual-indexing procedure
described by Kozich et al. (2013). Product triplicates were then pooled, quantified using
Picogreen assay (Life Technologies, Carlsbad, USA) and pooled equimolarly. The final pool
was concentrated using a SpeedVac Plus SC110A Savant and purified with CleanNA beads
(Moka science).
Sequencing was performed by Fasteris (Geneva, Switzerland) on an Illumina Miseq with
2x250 cycles, with settings of 7.5 Gb yield (including PhiX), an error rate of 2.5% and Q30 at
75%. The analysis yielded 5.3 Gb of sequences with an error rate within quality
specifications. Adapters were removed using trimmomatic (Bolger et al., 2014), paired-ends
reads were joined using ea-utils (Aronesty, 2011) quality checks were performed using
FastQC, and samples were demultiplexed using the Fasteris in-house script. Fasteris also did
all the downstream work described above.
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DNA-derived 16S rRNA gene sequences were processed using Mothur (Schloss et al.,
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2009). Samples were dereplicated, aligned, and filtered by length. Chimeras were removed
using uchime (Edgar et al., 2011), and taxonomic affiliation was then realized using the
method of Wang et al. (2007) at a cutoff of 80% against the Silva SSU database 123 (Quast
et al., 2013). Operational Taxonomic Units (OTU) were then defined at a 97% similarity and
used for similarity analysis. Random subsampling was realized based on the smallest number
of obtained sequences in one sample after singleton removal (see Tables S1 and S2 for more
details). A matrix was built at the phylum level (excluding phyla that accounted for less than
1 % of the total community) and Principal Component Analysis (PCA) was performed using
Past (Hammer et al., 2001). Sequences were submitted to NCBI and can be found under the
accession number MH385389 - MH388018.
RESULTS
Water Chemistry
Based on repeated measurements conducted over the sampling period and the previous
years (Kanellopoulos et al., 2017), the physicochemical parameters of the hydrothermal fluid
have only limited variation, with temperature varying from 60.9 to 63.7 °C and acidic pH
values varying from 5.88 to 6.45 (Table 2, Fig. 2).
Table 2 shows the physicochemical and chemical parameters analyzed in situ and in the
laboratory. Chloride is the dominant anion of the Ilia fluid (1.28% Cl). Based on the
hydrochemical analyses (Table 2), the fluid is characterized by Na-Cl hydrochemical type.
Specific enrichment exists in major elements such as Fe (13.3 mg.L-1) and Ca (1570 mg.L-1)
and in trace elements such as As (up to 250 μg.L-1), Mn (500 μg.L-1), Ni (up to 80 μg.L-1) and
ammonium cation (up to 1.9 mg.L-1 ΝΗ4+, Table 2). It also shows concentrations of Sr of 24
mg.L-1, B of 9.7 mg.L-1, F of 3.8 mg.L-1, and Li of 3.4 mg.L-1.
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Morphology of the travertine deposit
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Ilia’s hot water artesian borehole deposits thermogenic travertine at the discharge point,
along the pipe, at the mouth of the pipe and at its outflow on the beach, building up the sides
of a keel that slowly rises in height with time (Figs 2 and 3). Precipitation also occurs below
the pipe as the water flows on the wall and onto the beach (Figs 2E, F and 3D) although
deposition practically stops only a few metres from the pipe. Travertine deposition is also
taking place inside the borehole (Fig. 3A). Periodic intervention of the local authorities to
remove the deposits prevents the borehole and pipes from becoming completely clogged.
The thermogenic travertine (Fig. 4) at the discharge point consists of separate Fe-rich
(brownish-metallic colour) and Ca-rich (orange-yellowish colour) laminae/bands up to a few
centimetres thick (Fig. 4B through D). The travertine macro-facies consists of laminated
specular, knob-like and botryoid shapes (Fig. 4) which evolves into a dense layered
crystalline travertine crust at the pipe mouth (Figs 2A, B, E, F and 4A, B) forming bands
(Fig. 4C and DF) or thin layers (Fig. 4E and F) usually botryoidal in shape. A vertical cross
section through several samples revealed a well-developed laminated texture in all of them
(Fig. 4C through F), with band thickness ranging from submillimetre (Fig. 4F) to centimetre
scale (Fig. 4C and D).
Based on field observations, Ilia deposition is mainly orange in colour, suggesting Ca-rich
component dominates. This colour expands along the hot water flow, until it reaches the sea.
Dark-brown to black coloured surfaces (Fe-rich component) are observed where the hot water
with a high flow-rate reaches the ground; in the top part of the borehole where water-level
changes due to degassing (Fig. 3A); and inside the pipe, especially at water level, which
changes depending on the water flow (Fig. 2C through F).
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Mineralogical Study and microfacies of the travertine deposit
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Samples from Fe-rich and Ca-rich components were separated and analyzed by XRD
(Fig. 5A). Based on these analyses, the Fe-rich component is composed mainly of two-line
ferrihydrite and to a lesser extent of aragonite and calcite (Fig. 5B), as previously described
by Kanellopoulos (2012) and Kanellopoulos et al. (2017). The Ca-rich component is
composed mainly of aragonite and calcite with a minor contribution from ferrihydrite and
halite (Fig. 5C).
Under the optical microscope, the Fe-rich and Ca-rich bands are markedly distinct (Fig.
6A). The Ca-rich bands are mainly laminated (Fig. 6B), consisting of needle-like crystals of
aragonite, growing normal to the substrate (Fig. 6C). The crystals are elongated parallel to the
c-axis, exhibiting straight extinction. The substrate is usually a thin lamina of silt-sized
micritic aggregates (Fig. 6C) or another Fe-rich lamina. In several cases, parallelogramshaped areas of aragonite, with rounded edges, are observed developing within Fe-rich
masses (Fig. 6D), suggesting the complex 3-D spatial spreading of the two main components
(i.e. Fe-rich and Ca-rich components).
Under the optical microscope the Fe-rich components mainly consist of dark red to brown
ferrihydrite. Combined optical microscope observations and SEM images show two
ferrihydrite facies. The first type consists of laterally aligned shrub-like structures extending
and branching upwards and forming laminae (Figs 6E through G and 7A, B). Typically, they
are elongated, dense masses consisting of ferrihydrite micritic clumps, usually with spherical
nodules creating “branches” and dendritic fabric (Figs 6E, F and 7F through H). Based on the
classification scheme of Chafetz and Guidry (1999), they could be characterized as woody
shrub or bush (i.e. bacterial shrubs). These shrubs are usually developed above aragonitic
laminae (Fig. 6E). In some cases, dark-tinted axes (filament-like), potentially consisting of
organic matter, can be observed encased within the ferrihydrite shrubs (Fig. 6G). The
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filaments extend and branch upwards, over a distance corresponding to the thickness of the
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lamina. Revealed under SEM, the iron-rich components of the studied samples are commonly
composed of fine-scale laminae of the iron-rich mineral phase (ferrihydrite) alternating with
calcium-rich (aragonite) laminae over a few tens of micrometres (Fig 7A). Ferrihydrite has
been observed in several cases to fill empty space between ferrihydrite shrubs, or between
aragonite crystals (Fig. 7E) creating very dense laminae. However, in several cases empty
spaces between the dendrite aggregate was observed inside the laminae (Fig. 7B).
Additionally, ferrihydrite was identified in a second type of facies consisting of dense
laminae, with very limited porosity (Figs 6D, H and 7C through E). In this case, no
crystalline habit or microfacies of the ferrihydrite could be identified. Although, the
ferrihydrite laminae followed the geometry dictated by the substrate (i.e. Ca-rich laminae or
bedrock).
Minor amounts of sulphides such as pyrite, As-rich pyrite, arsenopyrite, stibnite, galena,
Fe-rich sphalerite, chalcopyrite and oxides, and non-metallic mineral phases such as barite,
fluorite, and some REE-bearing phases, can be found in the studied samples. All of these
minerals occur as very small crystals (few μm in size), in accordance to Kanellopoulos et al.
(2017).
Travertine geochemistry
Samples from Fe-rich and Ca-rich components were separated to analyze their bulk
geochemical composition (Table 3). The Fe-rich component of the Ilia travertine is enriched
compared to the Ca-component (and typical travertines) in Fe (35.3%), As (2.6%), and Na
(4%) for major elements and in Y (323 mg/Kg), Nd (96 mg/Kg), Dy (63 mg/Kg) for trace and
rare earth elements (REE). In contrast, the Ca-rich components of the Ilia travertine is less
enriched in all of these elements (11% Fe, 931 mg/Kg As, 0.08% Na, inc. all the REE), but
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has higher concentrations of certain elements like Mn (330 mg/Kg), S (0.27 %) and other
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metals such as Co (0.24%), Cr (2.68%) and Ni (1.58%). Both components are presenting
comparable concentrations to elements such as Cu (Fe-rich component: 6 mg/Kg and Ca-rich
component: 8.4 mg/Kg), Mg (Fe-rich component: 1915 mg/Kg and Ca-rich component: 1650
mg/Kg), Pb (Fe-rich component: 4.7 mg/Kg and Ca-rich component: 2.9 mg/Kg), U (Fe-rich
component: 240 μg/Kg and Ca-rich component: 290 μg/Kg), Zn (Fe-rich component: 63
mg/Kg and Ca-rich component: 48 mg/Kg).
Normalization of the whole rock chemical data to the average composition of Upper
Continental Crust (UCC, Rudnick & Gao, 2003) and Post-Archaean Australian Shale (PAAS,
Taylor & McLennan, 1985; Fig. 8) indicates that both laminae are enriched in elements such
as As, Fe and S. The Fe-rich component in particular is enriched 5440 times in As, compared
to UCC abundances and almost 10 times in Fe, compared to UCC and PAAS abundances.
Additionally, the Fe-rich component shows a clear enrichment in REE compared to UCC and
PAAS, by more than 10 times (Fig. 8). The two studied components show similarities with
respect to light REE depletion, but the Ca-rich component has small positive anomalies in Ce
and Y, which are not present in the Fe-rich component.
Analysis of microbial communities based on 16S rRNA gene sequences.
Microbial communities differ from each other based on sample lithology and exposure to
water/air (Fig. 9A). Bacteria-associated reads are dominant in all samples, but samples ID1
and ID4 have 19% and 26% of archaeal reads respectively, and IP2 and IP3 reach 44% and
28% (Fig. 9A).
Principal component analysis shows the relationship between samples and the main phyla
that characterize their relative composition (Fig. 9B). Samples IP2 and ID2 are marked by a
high number of Aquificae of the Hydrogenotherma genus (40% and 65% respectively). They
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also share Zetaproteobacteria of the Mariprofundales genus with IP3 and ID3 (11% for IP2,
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5% for ID2, 3% for ID3 and 7% for IP3). IP3 and ID3, together with IP1 and ID5, are clearly
characterized by Alphaproteobacteria and Cyanobacteria. Alphaproteobacteria are generally
represented by unclassified members as well as Rhodobacterales, Rhodospiralles,
Erythrobarcteraceae and Rhizobiales. ID1 and ID4 are both characterized by a large number
of Thaumarchaeota (15% and 10%, respectively), Planctomycetes (34% and 17%,
respectively), Chloroflexi (28% and 26%), Deltaproteobacteria (9% and 10%) and finally
Deferribacteres (5% and 8%). Nitrospira are found in ID4, ID3 (13%) and form a significant
portion of the Thermodesulfovibrio associated sequences. Sample ID2, however, is
dominated by unclassified Nitrospira sequences (11% of the total relative abundance).
Clades involved in iron reduction and oxidation are abundantly represented in the samples
of the Ilia travertine. Members of the iron-oxidizing Zetaproteobacteria represent 3% of the
community in ID2 and ID3. This clade is even more abundant in the Ilia pipe samples, where
they correspond to 10% and 7% of IP2 and IP3 microbial communities, respectively. The
presence of unclassified Rhodobacteracea may also be related to phototrophic iron oxidation,
but this is not certain.
DISCUSSION
Hydrothermal fluid
The hot spring/artesian borehole of Ilia degases mainly CO2 (D`Alessandro et al., 2014)
and deposits Fe±As -rich thermogenic travertine (Kanellopoulos, 2011; 2012; Kanellopoulos
et al., 2017). It is part of a large single hydrothermal system, which occurs at the
northwestern part of Euboea island, and at the neighboring area of mainland i.e. Sperchios
area (Kanellopoulos et al., 2017, Fig. 1). The hydrothermal fluids of NW Euboea`s hot
springs are near neutral pH, sodium-chloride, with very close chemical relation between them
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(Kanellopoulos et al., 2017). Ilia’s hydrochemical fluid type is Na-Cl (Table 2), with chloride
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concentrations (i.e. 1.28% Cl) comparable to Aegean Sea seawater (2.2% Cl, Athanasoulis et
al., 2016). However, Ilia’s hydrothermal fluid has higher concentration of Sr (24 mg.L-1) and
similar concertation of Li (3.4 mg.L-1) comparable to Aegean Sea seawater (5.8 mg.L-1 for Sr;
and 3.4 mg.L-1 for Li; Athanasoulis et al., 2016). The Ilia hot spring/artesian borehole is
located only few metres from the seashore. The dominant anion and cation in Ilia’s
hydrothermal fluid are chloride (up to 1.28%) and sodium (up to 0.7%). Additionally, the
fluid shows high concentrations of a series of ions and trace elements (conservative
constituents), typically associated with seawater or/ and are likely to be of deep geothermal
origin such as F, SiO2, and Li. In accordance with the findings of previous studies
(D`Alessandro et al., 2014; Dotsika, 2015; Vakalopoulos et al., 2016; Kanellopoulos et al.,
2017) these enrichments suggest high seawater participation and a magmatic contribution.
Moreover, hydrothermal fluid from the Ilia area shows the highest concentrations of Fe (up to
13300 μg.L-1) and As (250 μg.L-1) compared to any of the other hot springs on NW Euboea
island (Kanellopoulos et al., 2017, Table 1). Kanellopoulos et al. (2017, 2018) based on
mineralogical and geochemical observations such as i) the presence of elements in their
native form, such as Fe, Pb, Cu, ii) the presence of native alloys such as Au±Cu-Ag and the
enrichment of metalloids such as As, Sb and iii) the abundance of REE, suggested that the
system has a magmatic contribution. As a result, metals and metalloids were mainly derived
from magmatic fluids, which after mixing with heated sea waters deposited native elements,
sulphide mineralization at depth, and As-Fe-rich travertines in the surface (Kanellopoulos et
al., 2017; 2018). The repeated measurements conducted during the last years (including wet
and dry seasons, Kanellopoulos et al., 2017) have shown that the physicochemical parameters
of the hydrothermal fluid are relatively stable with temperatures varying only from 60.9 to
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63.7 °C and pH values from 5.9 to 6.45 (Table 1, Fig. 2). The results reported here are in line
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with previously published values.
Terrestrial thermogenic Fe-rich travertines with ferrihydrite have been reported in
Shionaha (Takashima & Kano, 2005) and Okuoku-Hachikurou, Japan (Takashima et al.,
2008, 2011). Additionally, the presence of ferrihydrite in hydrothermal environments has also
commonly been reported in submarine vents (chimneys and hydrothermal sediments) such as
the Basiluzzo Islet, Italy (Bortoluzzi et al., 2017), Kolumbo, Greece (Kilias et al., 2013) and
Tutum Bay in Papua New Guinea (Pichler & Veizer, 1999). By comparing Ilia’s
hydrothermal fluid with these occurrences (Table 2), the studied fluids show similar pH
values (slightly acidic: 5-6.6). The temperatures of the other known terrestrial ferrihydrite
depositing hot springs in Japan are 20-35oC lower, potentially allowing the development of
non-thermophilic organisms. Regarding iron, Ilia’s hydrothermal fluid shows higher
concentrations than the terrestrial hot springs of Japan (Takashima & Kano, 2005; Takashima
et al., 2008) and the hydrothermal vent from Tutum Bay (Papua New Guinea; Pichler &
Veizer, 2004). However, iron concentrations are lower when compared to the Basiluzzo Islet
(Italy; Bortoluzzi et al., 2017) and Kolumbo (Greece; Kilias et al., 2013) submarine vents.
Hence, Ilia hot spring shares some similar physicochemical characteristics with the fluids of
the above-mentioned areas. Additionally, based on these characteristics Ilia can be ranked
among the most iron enriched terrestrial hot springs worldwide, with near neutral pH.
Iron-rich travertine composition
Based on their strong differences such as their color and also their facies and chemical
composition, it is clear that the Fe-rich and Ca-rich laminae of the travertine are formed under
very different conditions. In particular, spatial discrimination of Fe-deposits from Ca-deposits
is observed, with a dark colour (representative of iron oxides of the Fe-rich laminae) only
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present when there is hot water flowing at a relatively high speed. When the flow rate
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decreases (away from the vent) or where the is no water flow (on the sides of the pipe for
example), the orange colour, representative of the Ca-rich component, dominates. These
observations strongly suggest that the differential deposits of the Fe-rich and Ca-rich
component are controlled by variations in the flow rate of hot water venting from the spring.
As a result, it is expected that the laminae are controlled by these changes.
The elements As, Sc, and Y are clearly enriched in the Fe-rich component compared to
the Ca-rich component. The strong binding potential of metal oxides towards arsenic could
explain this difference in the ferrihydrite-rich component (Smedley & Kinniburgh, 2002). In
contrast, the Ca-rich component of the Ilia travertine clearly has higher concentrations of Mn
(330 mg.Kg-1) compared to the Fe-rich component. This may be related to the fast oxidation
of Mn2+ in changing redox conditions, which may have varied between the two different
phases. Metals such as Co and Ni follow the same trend. Similarly, the positive Ce anomaly
observed in the Ca-rich component could be linked to the sensitivity of Ce to oxidative
conditions (Bau & Koschinky, 2009). Hence, enrichment is observed in elements that become
insoluble when oxidized in the Ca-rich component, potentially pointing towards changes in
redox conditions during the precipitation of this phase.
Microbial communities of the travertine deposits of Ilia
Communities of the thermogenic travertines of Ilia vary with changes in water flow,
distance to the vent, aerial exposure and natural redox conditions (Table 1, Fig. 9A). The two
samples that experienced the highest water flow (ID2 and IP2) are marked by an abundance
of thermophilic organism of the Aquificae phylum. Sequences of this phylum are uniquely
attributed to the family Hydrogenothermaceae, which consists of chemolithoautotrophic
microaerophilic thermophiles (Takai & Nakagawa, 2014). The other phyla consist mainly of
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unclassified sequences, except for Zetaproteobacteria, which are attributed to the Fe-
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oxidizers of Mariprofundaceae family (Emerson et al., 2010). Interestingly, these Feoxidizers are characteristic of marine environments like the Loihi seamount (Emerson &
Moyer, 2012), Santorini marine hydrothermal springs (Handley et al., 2010) or of Basiluzzo
Islet in the Aeolian islands (Bortoluzzi et al., 2017). Communities obtained from IP3 and ID3
share similarities allowing a continuum to be drawn between the environments of ID2 and
IP2. Aquificae and Zetaproteobacteria sequences are still present (3.3% and 7.2%).
Additionally, species richness is higher, with photosynthetic Cyanobacteria in IP3 and a large
number of Bacteroidetes and Alphaproteobacteria. These are widespread clades for which
metabolic styles are hard to distinguish at the phylum to family level. However, the
coexistence of Cytophagia, Erythrobacteraceae, Rhodospirillaceae, and Rhodobacteraceae
clades suggests a dynamic environment in photic zone (Table 1), with different sources of
carbon vis autotrophy and heterotrophy under microaerophilic to aerobic conditions.
Sequences obtained from samples ID5 and IP1 show a clear dominance of aerobic
metabolisms. No iron-related clade was obtained and visual examination clearly showed
photosynthetic activity (green-pigmented travertine interpreted as containing Cyanobacteria)
for these two samples (Figs 3A, C), as well as in other areas of the Ilia system where water
flow was slow or nonexistent (because of daily to monthly flow variations). It is suggested
that the high-water temperature prevents the development of Cyanobacteria in other light
exposed systems. This would differentiate this system from the Okuoku-Hachikurou hot
spring (Takashima et al., 2011). But as soon as the water flow rate drops or diverges,
Cyanobacteria take over and dominate the travertine assemblage. Samples ID1 and ID4 show
completely different communities (Fig. 9B) marked by anaerobic clades. Sequences are
attributed to members of the Planctomycetes, Chloroflexi unclassified or attributed to the
Anaerolinae class, which consists only of strict anaerobes commonly found in hot spring
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microbial mats (Hanada & Pierson, 2006), Defferibacter and Deltaproteobacteria. From the
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latter class, sequences that could be assigned to an order were either related to
Desulfobacterales, Desulfoarculales or Syntrophobacterales, which all point towards
organisms involved in sulphate reduction. Defferibacter-associated sequences could only be
assigned to the thermophilic anaerobic Caldithrix genus that consists of fermenters
potentially using nitrate as an electron acceptor (Alauzet & Jumas-Bilak, 2014). Overall, this
environment is likely anaerobic and its microbial assemblage relies mainly on the anaerobic
degradation of organic carbon, potentially involving sulphate and nitrate reduction.
The 16S rRNA gene analysis revealed the presence of diverse microbial communities,
which could be associated with the deposition of ferrihydrite. The compositional variability
of the microbial community is indicative of the heterogeneity and dynamic nature of the
studied system. Microaerophilic conditions dominate at the vent, where water starts to
equilibrate with the ambient oxygen. When the water flow decreases, oxygen content
increases and microaerophilic organisms are replaced by aerobic autotrophs and heterotrophs.
In buried settings fermenters and other sulphate reducers degrade the organic matter
previously deposited by runoff or past microbial production.
Biologically induced ferrihydrite precipitation
Ferrihydrite precipitates from oxidation of Fe2+ to Fe3+ and from rapid hydrolysis of Fe3+
in abiotic or biologically aided processes (Jambor et al., 1998; Konhauser, 1998). In the case
of the Ilia travertine, several lines of evidence suggest that ferrihydrite is mainly precipitated
by bacterial activity in microaerophilic conditions. This conclusion is supported by the
presence of fabrics showing a close association of ferrihydrite with filamentous textures
resembling sheaths formed by Zetaproteobacteria (Figs 6G and 7G, H). They are covered
with ferrihydrite particles, and are strikingly similar to the structures described in other
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settings exhibiting the same organisms (Takashima et al., 2008; Handley et al., 2010;
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Bortoluzzi et al., 2017). In submarine or continental hydrothermal systems, ferrihydrite is
interpreted as precipitated by sheathed or stalked iron oxidizers. These sheathed or stalked
iron oxidizers are generally encountered in loose sediments without any textural
characteristics. Until now, only Takashima et al. (2008) have identified well-preserved
erected filaments encased in dendritic structures, in their case in the Shionoha iron-rich
travertine deposits although these were preserved in calcite. Encased-filaments from Ilia are
visually similar to the Shionoha structures and could possibly be formed by analogous
microbe-mineral interactions. In Shionoha spring (Takashima et al., 2011) the central, darker
part of the dendritic fabric of the ferrihydrite spherical aggregates has been interpreted as
microbially encrusted filaments. Zetaproteobacteria Mariprofundaceae, identified in the Ilia
travertine 16S rRNA gene library, is known to form these ferrihydrite-covered stalks
(Emerson et al., 2007; Handley et al., 2010). In Ilia deposits, they were found in
environments of high water flow, which experienced moderate oxygenation that could have
allowed their development under microaerophilic conditions (Konhauser, 1998; Takashima et
al., 2008). All of the Ilia system data thus suggests microbially aided deposition of
ferrihydrite by Zetaproteobacteria under microaerophilic conditions.
The second type of ferrihydrite facies, described as dense laminae with limited porosity
and no crystalline habit, has been attributed to abiotic precipitation by Kanellopoulos et al.
(2017). The findings presented here cannot rule out this hypothesis, and it is possible that
ferrihydrite precipitation continues to occur once it has been initiated by the iron-oxidizing
bacteria community, potentially evolving from the shrub ferrihydrite facies to porosity-filling
by small ferrihydrite spherulites. A geomicrobiological investigation at the lamina scale will
be necessary to untangle these processes.
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Proposed model for the precipitation of Banded Iron Travertine (BIT)
Accepted Article
The two types of bands (i.e. Fe-rich and Ca-rich) observed in the BIT display different
mineralogical, morphological, chemical and microbiological features, all related to the
distinct processes of deposition. Fe-rich bands show relative depletion in elements that are the
most sensitive to redox conditions (Mn and Ce), implying more reduced conditions during
their precipitation than for the Ca-rich bands. Microbiological analyses of organisms living
under these conditions support this kind of redox process, all displaying a significant fraction
of iron-oxidizing bacteria from the Zetaproteobacteria class. Hence, it is suggested that these
microorganisms only develop where microaerophilic conditions prevail, and that they are
responsible for most of the primary ferrihydrite precipitation within the iron bands. Due to
the significant variations in water flux at the spring, these microaerophilic environments may
develop at different levels of the borehole and pipe system. During periods of higher flow,
the upcoming reduced spring water will be oxidized further away from the vent, and the site
where microaerophilic Fe-oxidizers can develop and precipitate ferrihydrite will move away
as well. In conditions of lower flow, fully oxidized conditions may develop in areas that used
to be microaerophilic. In such conditions, biologically induced ferrihydrite precipitation
would not occur and the CaCO3 precipitation takes over as exposure to the atmosphere allows
degassing and travertine formation (Fig. 10). Potentially, the development of Cyanobacteria
in such settings would enhance this CaCO3 formation. Areas of standing water will most
likely develop such conditions and evaporative processes accompanying the travertine
deposition will allow co-precipitation of halite, as observed in the XRD data (Fig. 5).
In the case of the Okuoku-Hachikurou hot spring, a symbiotic relationship between
Cyanobacteria and Fe-OB was suggested to explain the laminated texture of iron-rich
deposits. These laminations were thought to reflect changes in photosynthetic intensity
(Takashima et al., 2011). In the Ilia travertines, co-occurrence of Zetaproteobacteria and
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Cyanobacteria was not observed, likely because of the more dynamic with higher
Accepted Article
temperature. The interlayering change of Fe-rich and Ca-rich bands is explained by changes
in water flow coming from the vent. It allowed the biologically driven precipitation of the
iron bands to alternate with mainly abiotically driven precipitation of the CaCO3 bands in the
same location. These changes may be link to tide cycles as seawater fuels the hydrothermal
spring system, or by magmatic pulses. Pulses have been observed on a daily basis in the
Euboea hydrothermal system (unpublished results). While cyanobacteria may contribute to
the carbonate precipitation in this system, the high precipitation rates suggest that it is
unlikely that they play the major role in carbonate precipitation.
Iron-rich travertines as analogs to BIF
The Ilia travertines are mainly the result of seawater circulation within a hydrothermal
system that subsequently leads to the formation of iron-rich deposits, when interacting with
oxidative environments, at a geologically fast rate. It leads to deposition of almost pure
ferrihydrite laminae alternating with another chemically precipitated facies (here calcium
carbonate) that resemble BIF characteristics. In particular, the Ilia travertines have iron
enrichment of up to 35 wt%, only comparable with systems like Tutum Bay in Papua New
Guinea (Pichler & Veizer, 1999) and the Endeavour Segment Main Field (Hannington et al.,
2005). Even the Ca-rich bands exhibit higher iron concentrations than many active submarine
hydrothermal deposits (Table 3), which emphasizes the enormous iron enrichment exhibited
by the Ilia travertine and corroborates its resemblance to BIF. As an example, Algoma-type
BIF ore grade varies from 15 to 45 wt% (Bekker et al., 2010, 2014; Posth et al., 2010). Other
similarities with the general geological setting of Algoma-type BIFs (Cannon, 1986; Bekker
et al., 2010, 2014) are apparent in the Ilia case. The Ilia travertine forms in a back-arc region,
after circulation within deeper bedrock including ophiolitic-ultramaphic rocks. Algoma-type
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BIFs were likely deposited in island arc/back arc basins (Veizer, 1983; Bekker et al., 2010,
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2014) associated with similar (ultra)mafic volcanics (Gourcerol et al., 2016).
The entangling of biogenic and abiotic processes is also a salient feature of BIF
deposition. Several hypotheses have been suggested concerning the biological influence on
BIF deposition (Bekker et al., 2010, 2014): the anoxygenic phototrophic iron-oxidizing
bacteria, which can couple Fe(II) oxidation to the reduction of CO2 (Widdel et al., 1993;
Ehrenreich & Widdel, 1994), the cyanobacterial model for BIF formation (Cloud, 1973) or
the chemolithoautotrophic iron-oxidizing bacteria living in a neutral pH environment (Holm,
1989). In the case of the BIT of Ilia, the latter model likely explains the process of iron
precipitation in the Fe-rich bands. This process however relies on the existence of suboxic
conditions (incomplete oxygenation of the spring water at the Ilia vent). Similar suboxic
conditions could have been encountered during the time of BIF deposition, when oxygen
production fueled by ancestral cyanobacterial activity was only being initiated.
Although, there are some BIF with carbonate bands such as the Cauê Iron Formation in
Brazil (Spier et al., 2007; Teixeira et al., 2017), BIFs do not typically contain carbonate
bands. The mineralogy of BIF generally consists of silica as chert, magnetite, hematite, Ferich silicate minerals such as stilpnomelane, minnesotaite, greenalite, and riebeckite,
carbonate minerals such as siderite, ankerite, calcite, and dolomite, and in some cases sulfides
such as pyrite and pyrrhotite (Barrett et al., 2010, 2014; Koeksoy et al., 2016). The silica
considered to have been originated either from the sediment–water interface in colloidal
form, by absorption on iron oxyhydroxides from seawater and scavenged with organic matter
(Krapez et al., 2003; Grenne & Slack, 2005 Fischer & Knoll, 2009; Bekker et al., 2010;
2014), or from replacement of the original sediment, formed beneath the sediment–water
interface (Krapez et al., 2003; Bekker et al., 2014). However, all BIFs have undertaken
significant modifications either during diagenesis, or during metamorphism. So, their
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mineralogy is the results of a series of factors, including the bulk composition of the original
Accepted Article
sediment, the diagenetic conditions, the metamorphic conditions, and the post-depositional
fluid flow. Especially, the effects of temperature and pressure have led to mineralogy
replacement, recrystallization, and from change to deletion of primary textures (Klein, 2005;
Barrett et al., 2014).
The BIT of Ilia interestingly present poorly diagenetically transformed structures and
chemical components that could help untangle the primary features of BIFs. For example, the
presence of both, ferric and ferrous minerals in BIFs suggests an average oxidation state of
Fe2.4+ (Klein & Beukes, 1992), which means that 60% of the Fe in BIFs is made up of Fe(II).
The BIF mineralogical composition reflects significant post-depositional alteration under
diagenetic and metamorphic conditions. The Fe-rich bands, which consist of magnetite and
hematite, are most likely to have formed from an initial Fe(III) oxyhydroxide phase such as
ferrihydrite (Klein, 2005; Posth et al., 2008; Bekker et al., 2010, 2014; Gauger et al., 2015).
The BIT of Ilia have an almost pure ferrihydrite composition in their Fe-rich bands, which
could represent the primary composition of Fe-rich bands in BIFs and therefore may provide
a model of BIF depositional characteristics.
Moreover, the BIT of Ilia also procures a model for potential diagenetic processes in
precursor bands. The existence of fermenters and sulphate reducers for example, in these Ferich reducing environments (Fig. 9) attests of organic matter recycling already taking place
within sites of actively forming iron bands. The Ilia spring is therefore an interesting and
easily accessible laboratory to investigate the initiation of iron mineral precipitation, micro to
macro-banding formation and iron and carbon early syn-sedimentary recycling. Overall, the
Ilia BIT shares many textural, mineralogical, chemical, and depositional similarities with
Algoma-type BIFs. Given its intense precipitation rates, strong iron enrichment and easy
access, it is suggested that a thorough investigation of the biotic and abiotic processes
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involved in this dynamic small-scale system will help in understanding the suite of complex
Accepted Article
processes that have led to BIFs as we know them today.
Acknowledgments
CK would like to thank the Institute of Geology and Mineral Exploration (I.G.M.E.) -
Division of geothermal energy and thermo-metallic waters for the support and collaboration.
CT and DA acknowledge the technical and funding support of the University of Geneva as
well as the Swiss National Science Foundation (project N° 200021_166308/1).
Conflict of Interest
All authors declare no conflict of interest.
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Accepted Article
Table 1: Microbiological sample description and characteristics
Site
Water
flow
light exposure
air
exposure
composition
commentaire
ID1
Borehole
no
no
burried
black mat
black unconsolidated material, EPS like
ID2
Borehole
high
no
no
ferrihydrite
crust
black crust
ID3
Borehole
moderate
moderate
no
ferrihydrite
crust
black crust on leaf
ID4
Borehole
no
no
burried
black crust
underneath black crust
ID5
Borehole
low
yes
yes
mixed mat
black crust cyano mat in contact with
black
IP1
Pipe mouth
low
yes
yes
CaCO3 crust
cyano mat in pipe
IP2
Pipe mouth
high
moderate
no
mixed crust
below pipe
IP3
Pipe mouth
moderate
moderate
no
mixed crust
below pipe off light little flow
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Table 2. Physiochemical parameters, major ions and trace elements concentrations from the
Accepted Article
studied hot spring and others terrestrial hot springs and hydrothermal submarine vents
depositing ferrihydrite.
T
(oC)
pH
E.C. (mS/cm)
T.D.S. (mg/L)
Ca2+
(mg/L)
Mg2+ (mg/L)
Na+
(mg/L)
K+
(mg/L)
HCO3- (mg/L)
Cl(mg/L)
SO42- (mg/L)
NO3(mg/L)
NH4+ (mg/L)
NO2(mg/L)
F(mg/L)
SiO2- (mg/L)
Ag
(μg/L)
Al
(μg/L)
As
(μg/L)
B
(μg/L)
Ba
(μg/L)
Be
(μg/L)
Br
(μg/L)
Cd
(μg/L)
Co
(μg/L)
Cr
(μg/L)
Cu
(μg/L)
Fe
(μg/L)
Hg
(μg/L)
I
(μg/L)
Li
(μg/L)
Mn
(μg/L)
Mo
(μg/L)
Ni
(μg/L)
Pb
(μg/L)
Rb
(μg/L)
Sb
(μg/L)
Se
(μg/L)
Sr
(μg/L)
U
(μg/L)
V
(μg/L)
Zn
(μg/L)
Terrestrial
Ilia,
EuboeaGreece*1
63.5
5.9
34150
23200
1420
190
6940
180
640
12550
810
bdl
1.9
bdl
3.6
100
bdl
bdl
250
9700
190
bdl
40300
bdl
bdl
bdl
70
11300
bdl
560
1900
380
bdl
75
bdl
220
bdl
310
18000
bdl
80
bdl
Ilia,
EuboeaGreece*1
63.7
6.1
34400
22700
1570
230
6760
210
640
12800
800
bdl
0.6
bdl
3.8
50
bdl
bdl
150
9200
210
bdl
38100
bdl
bdl
bdl
130
13300
bdl
500
3360
500
bdl
80
20
190
bdl
220
24000
bdl
70
bdl
ShionahaJapan*2
37.8
6.38
350
34.2
534
90
712
82.1
12100
-
Submarine
OkuokuhachikurouJapan*3
43.3
6.6
790
150
510
25
1270
770
bdl
51279.021
6800
-
Basiluzzo
Islet- Italy*4
KolumboGreece*5
5.7
33300
2770
3690
21780
1790
31530
660
53696.43
5
191000
3240000
0.29 (%)
1510
24.2 (%)
0.1 (%)
2.88 (%)
-
320000
520000
100000
0.1 (%)
23500
314500
170000
173000
20000
39000
408000
30000
0.57 (%)
0.26 (%)
Sea water
Tutum BayPapua New
Guinea*6
6.1
201
bdl
650
76
840
295
930
231
820
8400
6800
1720
1020
495
350
8.2
6790
-
SW, Aegean
Sea-Greece*7
25.9
8.18
56350
40900
475
1160
13240
423
168
22270
3257
<5
<0.05
<0.05
2.45
5
105
<10
13800
<10
87300
120
52
3360
<10
30
5800
<30
*1 = Vakalopoulous et al., 2016, *2 = Takashima and Kano, 2005, *3 = Takashima et al., 2008, *4 = Bortoluzzi et al., 2017 (DFS1), *5 =
Kilias et al., 2013 (NA014-027 Champagne active mound-2), *6 = Pichler and Veizer, 2004 (Vents 1-3), *7 = Athanasoulis et al., 2016
(seawater analyses from Aegean Sea)
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ccepted Articl
Table 3. Whole-rock travertine chemistry of the studied travertines as determined by ICP-MS and ICP-AES analysis and comparison with Ferich travertines elsewhere and submarine Fe-rich hydrothermal depositions.
Ilia (Ca-rich part)Greece
AedipsosGreece 1
IliaGreece 1
N. CaucassusRussia 2
Savo VolacanoSolomon Islands 3
Tutum Bay (submarine
hydrothermal aragonite)Papua New Guinea 4
Tutum Bay (submarine
hydroth. Fe (III).
Oxyhydroxide dep.)Papua New Guinea 6
KolumboGreece 7
Brothers
(Volcanic arcs) 8
Lake Taupo
massive sulphides
(Volcanic arcs) 9
S. Explorer Ridge
(Mid-ocean ridge) 8
Endeavour Segment
Main Field
(Mid-ocean ridge) 8
Average JADE site1
(Back arc rifts) 10
Izena cauldron
(Back arc rifts) 8
Tyrrhenian Sea Panarea
(Back arc basins) 8
Tyrrhenian Sea Palinuro
(Back arc basins) 8
Submarine
Ilia (Fe-rich part)Greece
Terrestrial
Ca %
Fe %
35.3
11
(n=23)
3.2 – 62
0.0049-2.395
(n=3)
10.3-21.9
13.1-28.9
(n=56)
0.4 – 49.3
0.0114-6.83
(n=5)
32-37
0.06-2.29
(n=4)
37.2-38.5
0.049 – 0.126
(up to 29.7)5
(n=7)
1.2-5
31-37.8
(n=14)
16.6
(n=9)
7.4
(n=1)
25.3
(n=51)
25.2
(n=83)
30.1
6.2251
(n=40)
6.2
(n=5)
10.5
(n=15)
15.1
Al mg/Kg
As mg/Kg
1340
26120
1850
930
6-1150
66-230
54-150
4895-18300
9 – 7475
-
0.6-626
bdl-5500
4.9-6.2 (%)
3810
2155
588
575
356
17500
17500
505
3400
Ba mg/Kg
Cd mg/Kg
Co μg/Kg
Cr μg/Kg
Cu mg/Kg
K mg/Kg
Li μg/Kg
Mg mg/Kg
Mn mg/Kg
Na mg/Kg
Ni μg/Kg
Pb mg/Kg
Rb μg/Kg
S mg/Kg
Sc μg/Kg
Si mg/Kg
Th μg/Kg
U μg/Kg
V μg/Kg
Y μg/Kg
Zn mg/Kg
117
1.1
705
16830
6
9960
6640
1915
98
40480
7635
4.7
1460
897
73445
720
240
3970
322790
63
88
bdl
2450
26800
8.4
10750
8565
1650
330
810
15860
2.9
1290
2720
4985
30350
450
290
19700
48
3-145
0.001-0.025
bdl
bdl
3.6-14.7
36-1090
140-3900
87-2990
1-1984.
700-33100
bdl
0.348-10.6
417-690
230-67800
130-630
12-950
bdl-150
10-91.
140-2560
80-7980
2.52-25.9
80-90
0.015-0.018
bdl
bdl
bdl
335-510
1530-1940
545-690
74-195
3280-4960
bdl
0.72-2.21
520-790
650-2740
2560-8870
86-340
9-41.
75-200
1040-2610
71100-258900
16-24.3
4-10890
bdl -48200
bdl-29000
bdl - 58.5
bdl - 1270
bdl - 88600
bld-41800
5 - 18000
bdl-6870
bdl – 48200
bdl – 34.6
16 - 12400
30 – 6650
27 – 8140
bdl - 3700
bdl - 6500
bdl - 28800
61-86000
bdl -162
23-167
0.05-0.36
100-2900
1700
0.150-0.780
bdl-100
900-4300
1260-7065
140-630
1500-4000
0.03-1.25
530-1800
(up to 33200) 5
bdl-47
bdl -0.4
bdl
bdl
bdl-18
bdl
240-540
77-540
bdl-590
bdl
7-24.
430-49000
bdl
bdl
bdl
bdl-970
30-1100
bdl
18000-90000
bdl
70-220
bld
16000-45000
13-160
996-2739
4400-7720
542-851
3560-8080
80-550
14-49
3800-13000
bdl
5.7-9.77 (%)
340-920
bdl-80000
8100-21000
24-56
276
1640
35000
14100
10200
105
28000
2000
33000
4.2
8.2
62.5
200
32000
1000
44409
54000
250
27000
5000
42539
64000
794
33000
110800
19634
200200
820
33000
118000
47214
202000
255
500
28000
118735
62000
4000
86000
179000
1500-10500
100-400
bdl-200
0.3-21
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ccepted Articl
Zr μg/Kg
-
-
29-2080
290-1070
bdl - 338000
-
700-49000
-
-
-
-
-
-
-
-
-
-
La μg/Kg
Ce μg/Kg
Pr μg/Kg
Nd μg/Kg
Sm μg/Kg
Eu μg/Kg
Gd μg/Kg
Tb μg/Kg
Dy μg/Kg
Ho μg/Kg
Er μg/Kg
Tm μg/Kg
Yb μg/Kg
Lu μg/Kg
54760
157070
21030
96070
30520
10290
49910
9450
62920
13330
35700
4310
24160
2960
470
3920
500
2120
620
205
1035
220
1565
380
1190
160
875
130
180-1100
19-1660
2-220
6-1110
3-390
1-150
6-770
bdl-140
1-950
bdl-190
7-1140
bdl-60
2-300
bdl-38
14300-57300
27500-119300
3640-16900
16700-76500
5280-24400
1850-8300
8830-38400
1750-7580
12700-51300
2710-10800
7570-29700
940-3760
5230-19800
650-2410
bdl-32100
60-78200
7-8400.
57-31000
bdl-7200
bdl-1700
22-8700
bdl-1600
bdl-11900
bdl-2800
10-9800.
bdl-1700
bdl – 11000
bdl-1800
700-2700
-
-
bdl-18000
-
-
-
-
-
-
-
-
-
-
1=Kanellopoulos et al., 2017, 2=Lavrushin et al., 2006, 3=Smith, 2008. 4=hydrothermal aragonite, Pichler and Veizer, 2004, 5=sediment cores, Price and Pichler, 2005, 6=hydrothermal Fe III. oxyhydroxide
precipitates, Pichler and Veizer, 1999, 7=Kilias et al., 2013, 8=Hannington et al., 2005, 9=De Ronde et al., 2002, 10=Glasby et al., 2008, bdl=below detection limit.
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Figure Legends
Accepted Article
Figure 1. Simplified geological Map of Northern Euboea Island, Greece (after Kanellopoulos
et al., 2018).
Figure 2. Paired views of Ilia’s hot spring pictures and corresponding thermal images of the
same area. In the right side of each thermal picture, a color column shows the temperature
scale corresponding to the colors. (A and B) General view of the hot water venting out from
the pipe. (C and D) Close view of the pipe end point. (E) Venting point of the hot water and
associated deposition. Orange-yellowish color component is Ca-rich and brownish-metallic
color component is Fe-rich. At close-up image (F) could be observed that inside the Ca-rich
component are developing Fe-rich bands (see red arrows).
Figure 3. Position of the different samples used for microbiological study. (A) Artesian
borehole and locations of the ID samples. (B) Ferrihydrite encrusted leaf, from the borehole.
(C) Pipe outflow where IP samples were taken. (D) Localization of IP2 and IP3 underneath
the pipe opening.
Figure 4. Different macro- and microfacies of Ila Fe-rich travertine deposit. (A) Spicular,
knob-like Fe-rich thermogenic travertine deposition from inside the borehole (upper part).
(B) Dense Fe-rich travertine deposition. (E-F) Fe-rich laminae/bands with varying thickness
from few mm up to few cm, alternating with Ca-rich laminae/bands.
Figure 5. XRD pattern of Fe-travertine from Ilia. (A) Combined XRD patterns of selected
material from pure Fe-rich (with black color) and Ca-rich (with blue color) bands. It is
distinct the presence of the two characteristic broad peaks at around 35o and 62o in 2θ, which
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are typical of poorly crystalline two-line ferrihydrite and the sharp peaks corresponding to the
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other mineral phases. (B) XRD pattern of selected material from pure Fe-rich bands (red
color = aragonite). (C) XRD pattern of selected material from pure Ca-rich bands (red color =
aragonite, blue color = calcite, green color = halite).
Figure 6. Microscopic features of the travertines, under transmitted-light microscope, with
parallel nicols. (A) Well developed and separated Ca- and Fe-rich components. (B) Close-up
of the Ca-rich component composed of numerous growth laminae. (C) Ca-rich laminas
separated by laminae of silt-sized micritic aggregates. (D) Ca-rich component develops
isolated in a Fe-rich- component. Fe-rich component, even if no crystalline shape could be
identified under the optical microscope, it seems that it is also developing in layers/ laminas.
(E and F) Laterally aligned shrub-like structures creating dendritic fabric extending and
branching upwards. At (G) aragonitic laminas has filled up the empty spaces between the Ferich shrub-like structures and at the centers of the shrubs could be distinguished filaments
often show dark-tinted axes, likely consisting of organic substances, and are encased in
ferrihydrite. (H) Fe-rich band consisted of ferrihydrite, even if no crystalline shape could be
identified under the optical microscope, it seems that it is also developing in layers/ laminas.
Figure 7. Back-scattered electron images (BSEI: A-D) of laminated travertines from Ilia.
Light areas have a higher average atomic weight (Fe-rich) than the dark areas (Ca-rich). And
SEM photomicrograph (E-H) of Fe-rich travertines fragments from Ilia (Arg = Aragonite and
Fh = Ferrihydrite). (A-B). Numerous growth laminae which have different average atomic
weights (Fe-rich and Ca-rich). At image (B) could be seem laterally aligned Fe-rich shrublike structures extending and branching upwards, creating dendritic fabric and composed by
spherical nodules aggregates of about 250 nm. (C) Dense, well developed and separated
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laminas of the two phases. Only, the Fe-rich area present some empty spaces. Additionally,
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(C) is presenting the transition from one lamina to the other. The Fe-rich lamina expands
(shrubs) in to the Ca-rich lamina. (D) Close-up of image. (E) Transition from ferrihydrite
laminae to aragonite laminae. The aragonite laminae are composed by needle-like crystals
(radiating arrays). The crystals are elongated parallel to the c-axis, exhibiting straight
extinction and creating dense laminae. The ferrihydrite have been developed filling the empty
spaces of the top part of the aragonite crystals, no empty space could be observed. The
ferrihydrite laminae are usually also very dense, without any crystallographic habit.
Although, in some cases empty spaces between the dendrite aggregations were observed
inside the laminas (see arrows). (F) Spherical nodules aggregates of ferrihydrite co-existing
with aragonite crystals at the surface of a sample. The aragonite crystals have been
developing by following -covering the empty spaces of the ferrihydrite aggregates shrubs (see
arrows). (G) Encrusted filaments and EPS with spherical nodules aggregates of ferrihydrite.
The aragonite crystals are developing in a way to fill up the empty spaces. (H) Dendritic
branches of encrusted filaments with spherical nodules aggregates of ferrihydrite.
Figure 8. Bulk geochemical analysis of travertine normalized against average Upper
Continental Crust (Rudnick & Gao, 2003) and Post-Archaean Australian Shale (PAAS,
Taylor and McLennan, 1985). (A and B) Major and trace elements. (C and D) REE.
Figure 9. Microbial assemblages (16S rRNA gene sequences) of the Ilia travertine. (A)
Composition of the different samples at the phylum level as a function of the water flow
exposure. (B) Principal component analysis of the microbial community composition at the
phylum level.
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Figure 10. Model for the formation of banded iron travertine of Ilia. Switching from one
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mode to another might be controlled by variations in the flow of venting water, potentially
controlled by volcanic pulses and whatever controls the fluid circulation in the hydrothermal
system.
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