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Article

New Insight into Geochemistry and Mineralogy of Deep Caves in Croatian Karst and Its Implications for Environmental Impacts

by
Dalibor Paar
1,
Stanislav Frančišković-Bilinski
2,*,
Nenad Buzjak
3 and
Krešimir Maldini
4
1
Department of Physics, Faculty of Science, University of Zagreb, Bijenička cesta 32, 10000 Zagreb, Croatia
2
Division for Marine and Environmental Research, Ruđer Bošković Institute, Bijenička cesta 54, 10000 Zagreb, Croatia
3
Department of Geography, Faculty of Science, University of Zagreb, Trg Marka Marulića 19, 10000 Zagreb, Croatia
4
Main Water Laboratory (MWL), Department of Monitoring, Josip Juraj Strossmayer Water Institute, Ulica Grada Vukovara 220, 10000 Zagreb, Croatia
*
Author to whom correspondence should be addressed.
Water 2025, 17(7), 1001; https://doi.org/10.3390/w17071001
Submission received: 20 February 2025 / Revised: 26 March 2025 / Accepted: 26 March 2025 / Published: 28 March 2025
(This article belongs to the Special Issue Recent Advances in Karstic Hydrogeology, 2nd Edition)

Abstract

:
This study examines speleothems, sediments, rock, and water to assess geochemical and mineralogical processes in deep karst systems. Focusing on Slovačka jama cave (−1320 m deep) and the Velebita cave system (−1026 m deep), we identify elemental and mineralogical anomalies that provide valuable records of element transport, mineral formation, and paleoenvironmental changes. Heavy metal anomalies (Al, B, Co, Mn, Na, Tl, Ba, Be, Cr, Cu, Fe, K, Pb, Rb, Ti, U, Zn) at 300–400 m of depth in Slovačka jama indicate a complex interplay of geological conditions, geomorphological processes, atmospheric deposition, and potential anthropogenic influences. Factor analysis reveals two elemental associations: (1) Fe, Pb, Cu, and Zn, linked to terrigenous aluminosilicates, and (2) Cd, Cr, Mo, and Ni, suggesting airborne or geological sources. Mineralogical analysis confirms the dominance of calcite, with quartz, clay minerals, feldspars, magnetite, and goethite also detected. High magnetic susceptibility values in sediment-rich samples suggest Fe-rich mineral inputs from weathering, biogenic activity, or industrial sources. Ba anomalies in feldspar-rich samples and Sr accumulation at depth indicate distinct geochemical processes. These findings enhance our understanding of deep karst geochemistry, crucial for paleoenvironmental reconstructions and groundwater protection.

1. Introduction

The Croatian karst is primarily situated in the Dinaric karst, globally recognized as the locus typicus of Classical Karst, with a smaller portion extending into isolated karst areas of the Pannonian Basin [1]. Karst landscapes are among the most complex and hydrologically dynamic environments on Earth, characterized by high permeability, rapid water flow, and intricate interactions between surface and underground processes [2,3]. Despite its significance, the geochemistry and mineralogy of Croatian caves remained largely unexplored until recent years.
To address this research gap, a study was launched in 2016 with the aim of identifying speleothem proxies suitable for paleoenvironmental reconstructions [4]. The primary focus was to analyze the elemental composition and mineralogy of speleothems from various Croatian karst sites and assess how distinct climatic, geological, geomorphological, and hydrological conditions influence their characteristics. A total of 37 speleothem samples from 32 caves across different geomorphological and climatic zones were analyzed. The elemental composition of 30 elements was determined using ICP-MS, while mineral phases—including calcite, quartz, dolomite, muscovite/illite, chlorite, and plagioclase—were identified via XRD. Among the most abundant elements, in addition to calcium, those exceeding 500 mg/kg included Al, Fe, Si, and Mg. Statistical analysis using boxplot methods revealed significant anomalies in the deep caves of Northern Velebit, particularly in Lukina jama, where extreme values were recorded for Pb, Cu, Zn, Mn, Ni, Cr, Co, Ba, K, Mg, Li, Be, Al, U, Si, Ti, W, Fe, and As. These findings align with previous studies indicating that deep karst environments often record significant geochemical anomalies due to their complex hydrological and tectonic histories [4,5].
Given that the most pronounced anomalies among 32 studied caves in different parts of Croatia were identified in our earlier study [4] in the deep caves of Velebit Mountain, a new study was initiated to investigate geochemical and mineralogical variations at depths of up to 1320 m in Slovačka jama cave and 1026 m in the Velebita cave system. These caves, which contain the highest anomalies of heavy metals and other chemical elements among all 32 studied caves from different parts of Croatia, are located within a geologically complex karst terrain shaped by intensive tectonics, particularly during the Neotectonic period, which, in conjunction with prolonged karstification, has resulted in intricate subsurface structures (Figure 1). Recent research suggests that such deep cave environments provide valuable records of past climatic and geochemical conditions, making them critical sites for paleoenvironmental studies [6,7]. Sample 107 from Slovačka jama cave, the most anomalous site, showed elemental anomalies consistent with those found in our previous research [4], where this cave was analyzed along with other Croatian caves. Since both caves are situated within the same geological units and are only about 2 km apart, their geochemical profiles—reflected in speleothems, rocks, and sediments—are expected to be highly similar. Therefore, paleodata obtained from one cave should be applicable to the other, justifying our approach of evaluating both caves together in this study.
The Velebita and Slovačka jama caves are located in the strictly protected Northern Velebit National Park and are difficult to access due to the absence of nearby roads. Velebita lies approximately 6 km from the village of Krasno, while Slovačka is about 8 km from Krasno and a similar distance from the nearest coastal settlement. Both caves are predominantly vertical (Figure 2), making them unsuitable for tourism and accessible only to skilled speleologists and researchers. Consequently, entry is rare, occurring only during occasional speleological expeditions, typically a few times per decade.
The study of karst systems is not only important for understanding past environmental changes, but also has direct implications for water resource management. Karst aquifers are highly vulnerable to contamination due to their rapid recharge and direct connectivity between surface and groundwater systems [8]. It is estimated that approximately 25% of the world’s population relies on groundwater extracted from karst aquifers [9]. Understanding the hydrogeochemical dynamics of these systems is particularly challenging due to their extreme heterogeneity [10,11]. Investigations in deep caves offer a unique opportunity for in situ sampling, measuring, and analyses of karst processes in deep karst (>1.000 m), shedding light on the mechanisms controlling element mobility, mineral formation, and potential anthropogenic impacts [12] influencing epiphreatic and phreatic zones important for regional aquifer characteristics.
In our study, we expand upon previous research by analyzing multiple sampling media—including speleothems, cave clastic sediments, and water chemistry—to assess their geochemical and mineralogical properties and identify potential interactions. Such multi-proxy approaches remain relatively rare in karst research, particularly concerning cave sediments and water chemistry. However, several relevant studies provide useful comparisons. For instance, Rozkowski et al. [13] examined the migration and concentration of heavy metals in infiltration waters within a carbonate massif, linking these variations to both natural mobility and anthropogenic influences. Similarly, Pons-Branchu et al. [14] utilized urban speleothems to reconstruct heavy metal pollution histories in shallow groundwater systems, demonstrating how speleothem chemistry can serve as a long-term record of environmental changes. Other studies have explored the role of cave sediments and particulate matter in element transport, with Allan et al. [15] analyzing lead concentrations and isotopic compositions in Belgian caves to distinguish between anthropogenic and natural sources. More recently, Xu and Zeng [16,17] investigated heavy metal contamination in cave water and suspended particulate matter, respectively, underscoring the importance of geochemical monitoring in karst systems.
The primary aim of this study is to systematically investigate geochemical and mineralogical variations in deep karst cave environments, assess the potential interactions between different sampling media, and evaluate their implications for paleoenvironmental reconstructions and pollution monitoring.

2. Materials and Methods

2.1. Sample Preparation and Analysis

The speleothems for this study were collected with minimal disturbance to the cave environment, ensuring that natural formations remained intact. The sampling locations in the Velebita cave system and Slovačka jama cave are shown in Figure 2 and Table 1. Samples were collected from sites where carbonate precipitation and karst drainage networks facilitate speleothem growth [18,19,20,21]. These locations were carefully selected to ensure representative data on geochemical and mineralogical processes within the deep karst environment.
Samples were carefully handled to prevent contamination, washed with distilled water, air-dried, and then homogenized using a Retsch RM 200 mortar grinder (Retsch, Haan, Germany). Whole speleothems were crushed to obtain representative powders incorporating all growth layers. From these, 1 g of material was used for ICP-MS and XRD analysis.
For the elemental analysis of solid samples, 0.1 g of powdered sample was digested in a mixture of suprapur nitric and puriss hydrochloric acid, and heated in an Anton Paar Multiwave 3000 Oven (Anton Paar, Graz, Austria) following ISO 11466 standards. ICP-MS (Elan 9000, Perkin Elmer, Shelton, CT, USA) was used to determine elemental concentrations, employing internal standards (Ge, Rh, In, Re) according to ISO 17294-1 and ISO 17294-2. Precision (RSD) was within 10%, and accuracy was verified using reference material (RTC CNS392-050), with results aligning within 15% of certified values. Only two samples (64, 70) had values below the quantification limit for Tl (5.4%).
Mineralogical composition was identified using X-ray diffraction (XRD) with a Philips PW3040/60 X’Pert PRO diffractometer (Philips Analytical, Almelo, The Netherlands) and analyzed via Powder Diffraction File (1997) and X’Pert HighScore software (version 5.2). Semi-quantitative mineralogy followed [22].
Magnetic susceptibility (MS) was measured using an SM30 (ZH Instruments, Brno, Czech Republic) susceptibility meter, capable of detecting low-magnetic and diamagnetic materials such as limestone and quartz. Measurements were performed three times per sample, with the mean value recorded to ensure accuracy.
Electroconductivity and pH were measured using a SevenMulti instrument (Mettler Toledo, Schwerzenbach, Switzerland) in accordance with standards HRN EN ISO 10523:2012 and HRN EN 27888:2008. Turbidity was analyzed with a 2100 N turbidimeter (Hach, Loveland, CO, USA) following the standard method SM:1995-2130 B.
Anions and cations were quantified via ion chromatography using an ICS 3000 system (Dionex, Sunnyvale, CA, USA) according to standards HRN EN ISO 10304-1:2009 and HRN EN ISO 14911:2001. Alkalinity was determined using a Mantech PC-Titrate system (Guelph, ON, Canada) following standard HRN EN ISO 9963-1:1998. Total dissolved solids and HCO3 concentrations were calculated as per [23,24].
Orthophosphates were analyzed with a Lambda 25 spectrophotometer (PerkinElmer, Shelton, CT, USA) in accordance with standard HRN EN ISO 6878:2008. Total organic carbon (TOC) and total nitrogen (TN) were measured using a TOC-VCPH analyzer with a TNM-1 unit (Shimadzu Corporation, Kyoto, Japan) following standards HRN EN 1484:2002 and HRN EN 12260:2008. Chemical oxygen demand (COD) was determined using the titrimetric method in compliance with standard HRN EN 8467:2001.
Total phosphorus (TP) was measured via inductively coupled plasma mass spectrometry (ICP-MS, Elan 9000, PerkinElmer, USA), utilizing a 20 µg L−1 In solution as an internal standard, according to HRN ISO 17294-2:2003.
To define hydrochemical facies, a Piper diagram was used (generated with USGS software GW Chart, version 1.24.0.0), which illustrates the relationships among major anions and cations (Ca2+, Mg2+, Na+, K⁺, HCO3, CO32−, SO42−, and Cl).

2.2. Statistical Analysis

Statistical analyses were conducted using Statistica 6.0 [25] and included the following:
(a)
Descriptive Statistics: Basic parameters (mean, median, standard deviation, skewness, kurtosis) were calculated to summarize the dataset. Pearson’s correlation coefficients were determined to assess relationships between elements (p < 0.05).
(b)
Boxplot Analysis: Used to identify anomalies in sediment samples based on interquartile range, with outliers and extreme values defined according to Tukey [26] and Reimann et al. [27].
(c)
Cluster Analysis (Q-mode): Performed to group similar samples using a hierarchical method, distinguishing sample clusters rather than elemental correlations [28].
(d)
Factor Analysis: Applied to reduce variable complexity and identify key natural or anthropogenic influences, assuming correlations between multiple elements are driven by a smaller set of main factors [29,30].

3. Results

3.1. Mineralogical Analysis Using X-Ray Diffraction

Mineralogical analysis using X-ray diffraction (XRD) identified 10 minerals across the samples: carbonates (calcite, dolomite), silicates (quartz, clay minerals—kaolinite, muscovite, chlorite, montmorillonite, and feldspar—plagioclase), spinels (magnetite), and oxihydroxides (goethite). This method is qualitative, with a detection limit of ~5%.
As expected, calcite was present in all samples due to the karstic environment, where speleothems form through limestone dissolution and carbonate precipitation (Table A1). Dolomite appeared in only three rock samples from Slovačka jama (samples 118, 122, 123), suggesting localized geochemical variations. In eight samples, only calcite was detected (e.g., 101, 111, 113).
Quartz, the second most abundant mineral, was found in 36 of 45 samples, likely originating from fine-grained clastic sediments introduced into the cave system [4]. Similar findings were reported in karstic river sediments [31].
Among clay minerals, muscovite and chlorite were most common, followed by kaolinite and montmorillonite. Samples containing at least two clay minerals (e.g., 105, 107, 110) often coincided with geochemical anomalies and high magnetic susceptibility (MS). Notably, samples 105 and 107, from the same vertical channel of Slovačka jama, displayed strong similarities despite a 145 m elevation difference. The abundance of clay minerals suggests a potential paragenetic relationship between quartz and kaolinite. This observation is consistent with the findings of Chen et al. [32], who proposed that quartz cementation likely resulted from feldspar dissolution, the illitization of smectite and kaolinite, and the pressure solution of quartz grains.
Feldspars (plagioclase) were detected in only four samples (112, 126, 130, 133), all from channel-bottom sediments in Slovačka jama and the Velebita cave system. Among Fe-bearing minerals, magnetite and goethite were identified in samples from Slovačka jama, with sample 110 being the only one containing both. These minerals may indicate past hydrothermal influences or iron mobilization within the cave system.
The relationships between mineralogical composition, ICP-MS element concentrations, and magnetic susceptibility will be further explored in the discussion.

3.2. ICP-MS Analysis, Magnetic Susceptibility, and Elemental Anomalies

The ICP-MS analysis results for speleothems and water samples are presented in Table A2 and Table A3. While elemental concentrations in speleothems will be statistically analyzed in later sections, water sample data were not statistically evaluated due to the limited number of results (n = 3).
The results of physico-chemical parameters, nutrients, ions, total nitrogen (TN), total phosphorus (TP), chemical oxygen demand (COD), and total organic carbon (TOC) in the three water samples are presented in Table A4.
Magnetic susceptibility (MS) values, expressed in 10−3 SI units, range from 0.000 to 0.168, with the highest value recorded in sample 107 (Table A5). MS variations will be discussed in relation to elemental composition in later sections.
Elemental anomalies identified using the boxplot statistical method (Figure 3) indicate that sample 107 has the highest number of anomalies, followed by 127.
Outliers and extremes were observed for multiple elements, suggesting localized geochemical or environmental influences. These patterns will be further explored in the discussion.

3.3. Q-Modality Cluster Analysis

The Q-mode cluster analysis results are presented in Table A6 and Table A7. Three clusters were identified:
  • Cluster 1 (deepest, avg. depth 664.25 m): Composed of eight sediments, four speleothems, and four rock samples, showing a moderate concentration of heavy metals.
  • Cluster 2 (intermediate, avg. depth 440.25 m): Contains 10 rocks, nine speleothems, and one sediment sample, with the lowest heavy metal concentrations.
  • Cluster 3 (shallowest, avg. depth 323.89 m): Includes eight sediments and one rock sample, exhibiting the highest heavy metal concentrations (except for Ni), suggesting accumulation near the surface due to airborne pollution, soil leaching, and surface runoff.
Both caves are formed within massive Velebit limestone breccias (previously referred to as Jelar deposits) down to a depth of approximately 250 m, where they transition gradually into intensely fractured to layered Upper Jurassic dolomitic limestones [33]. Between depths of 400 and 980 m, limestone breccias once again dominate, but they occur in irregular alternations with layered limestones of a normal stratigraphic sequence. The presence of breccias at depths of up to 980 m below the surface is explained by a model of tectonized zones filled with Velebit breccias, which intersect Jurassic limestones in a normal sequence.
Comparing the available literature data with the average depth of our clusters reveals that the shallowest, Cluster 3, is located within fractured to layered Upper Jurassic dolomitic limestones. The intermediate Cluster 2 and the deepest Cluster 1 are positioned within limestone breccias that alternate irregularly with layered limestones. Thus, the cave’s rock composition is unlikely to have a significant influence on heavy metal concentrations, while the other processes mentioned are more likely to play a dominant role.
Heavy metals appear to migrate downward, accumulating first in shallow cave sections before being rinsed and redeposited in deeper zones. These transport mechanisms require further investigation.
Strontium concentrations notably increase in the deepest sections, but current data are insufficient to draw firm conclusions, warranting further research. Additionally, calcium concentrations in speleothems are lowest in shallow sections, nearly four times lower than in the middle depth, where they peak.

3.4. Factor Analysis

Factor analysis was performed on 16 variables, including sample depth and elemental concentrations (Al, Be, Ca, Cd, Co, Cr, Cu, Fe, Li, Mn, Ni, Pb, Si, Sr, Zn). The results explained 83.7% of the total variability, indicating a strong statistical model. Factor scores (Table A9) indicate the degree of influence of each factor on individual samples, while factor loadings (Table A8) reveal relationships between variables.

Interpretation of Factors

Factor 1: Dominated by the aluminosilicate component, indicating high influence from soil and non-carbonate rocks. Ca shows a strong negative correlation, while Fe and Mn likely originate from natural aluminosilicates. Zn, Pb, and Co may have either natural or anthropogenic sources, but strongly correlate with this factor.
Factor 2: Primarily associated with Cd, Cr, and Ni, forming a distinct elemental group. Their origin could be either atmospheric deposition from distant pollution sources or natural geological processes, differing from elements in Factor 1.
Factor 3: Shows negative correlations with depth and Sr, consistent with Q-mode cluster analysis, which indicates that Sr concentrations increase with depth.
These factors offer valuable insights into the geochemical processes influencing element distribution within the studied cave system. However, a more detailed characterization of mineral associations related to specific factors is not possible due to the limitations of the available XRD method, which has a detection limit of >3–5%.

4. Discussion

This section integrates mineralogical, geochemical, and geophysical data to explain the origin of detected elements and minerals, their distribution, and interactions within the cave system.

4.1. Mineralogy and Magnetic Susceptibility (MS) Relationships

Samples containing only calcite (or calcite + dolomite) exhibited very low MS values (≤0.002 × 10−3 SI units) and showed few or no elemental anomalies. A notable exception was sample 123, where an Mg anomaly coincided with the presence of dolomite, confirming its natural origin. This sample, collected from a horizontal channel at the bottom of Slovačka jama, suggests the presence of dolomitic bedrock at depth, though current geological maps lack subsurface detail.
In contrast, samples containing clay minerals displayed higher MS values and numerous elemental anomalies. The most abundant clay minerals were chlorite and muscovite, with kaolinite and montmorillonite present in smaller amounts. Chlorite, commonly found in metamorphic and volcanic environments, is known to contain Fe and Mn, which may explain the observed high MS values. It is likely formed through low-grade metamorphism or the weathering of mafic minerals (e.g., pyroxenes, amphiboles, biotite).

4.2. Elements and Magnetic Susceptibility (MS) Relationships

Table A10 presents the correlations between magnetic susceptibility (MS) and chemical elements in the studied samples. MS exhibits strong to excellent correlations with Al, Ba, Be, Bi, Ca, Co, Cu, Fe, Li, Mn, Pb, Rb, Ti, Tl, and Zn, suggesting that MS can serve as a reliable proxy for detecting locations with elevated concentrations of these elements. The use of MS in environmental research as a promising, fast, and cost-effective method for detecting heavy metal anomalies is relatively new. It was only recently applied for the first time in Croatia [34]. Therefore, the correlations between MS and elemental concentrations in this study represent a significant step toward the routine application of this method in karst research.

4.3. Potential Sources of Clay Minerals and Heavy Metals

The clay minerals in the samples studied may originate from multiple sources:
  • Terra rossa contribution: Similar to findings from Istria [35], terra rossa in karst regions often forms from insoluble residues of limestone and dolomite, but can also contain aeolian dust, volcanic debris, and transported sedimentary particles. These external sources may have introduced heavy metals over geological timescales.
  • Aeolian and volcanic inputs: Past atmospheric processes could have deposited metal-rich dust and volcanic ash, leading to localized heavy metal anomalies.
  • Hydrothermal activity: Though not confirmed, hydrothermal processes might have contributed to mineral transformations and heavy metal enrichment in deeper cave sediments.

4.4. Feldspars and Their Geochemical Significance

Feldspars (plagioclase) were detected in only four samples, often alongside clay minerals. While no major anomalies were associated with feldspar-rich samples, Ba anomalies were identified in samples 130 and 133. Since alkaline barium feldspars can form through Ba substitution for K in feldspar structures, it might be possible that crystallization processes in igneous or metamorphic rocks played a role in Ba enrichment, but to confirm this, additional research is needed. With the available XRD method, it is not possible to characterize minor minerals present in amounts below 3–5%. Therefore, it remains uncertain whether Ba originates from barite or is present in adsorbed forms.

4.5. Iron Minerals and Their Origins

Two Fe-rich minerals were detected:
  • Magnetite (spinels)—Found in cave sediments, with the following possible origins:
    (a)
    Natural sources, such as weathering of bauxites (known to occur in Velebit Mt.).
    (b)
    Biogenic activity, as some microorganisms can precipitate magnetite.
    (c)
    Anthropogenic pollution, transported via airborne deposition.
  • Goethite (oxyhydroxides)—Typically forms through lateritic weathering and was found in samples where Fe anomalies were detected.
Samples 107 and 127, both from Slovačka jama, exhibited Fe anomalies and contained magnetite, suggesting an unusual geochemical environment in these sediments.

4.6. An Unusual Geochemical Outlier

Sample 107 (285 m depth, Slovačka jama) displayed the following:
  • The highest MS value (0.168 × 10−3 SI units).
  • A complex mineralogical composition (calcite, quartz, all four clay minerals, magnetite).
  • Multiple elemental anomalies, including extremes for Al, B, Co, Mn, Na, Tl and outliers for Ba, Be, Cr, Cu, Fe, K, Pb, Rb, Ti, U, Zn.
These anomalies suggest a unique depositional or geochemical process, potentially involving multiple metal sources (natural and anthropogenic), deep sediment accumulation, and prolonged geochemical transformations. Further geochemical and isotopic studies are needed to fully understand its formation.

4.7. Factor Analysis and Elemental Associations

Factor analysis revealed a distinct grouping of Cd, Cr, and Ni, separate from other heavy metals. This suggests the following:
  • Different sources or transport mechanisms compared to Zn, Pb, and Co.
  • Possible atmospheric deposition (long-range transport of industrial pollutants).
  • Alternatively, a unique natural geological source distinct from the aluminosilicate fraction.
Our results indicate that heavy metal anomalies in cave sediments and speleothems can be attributed to a combination of natural geochemical processes and potential atmospheric deposition. Similar findings were reported by Rozkowski et al. [13], who examined heavy metal transport within the unsaturated and saturated zones of a carbonate massif in Poland. Their study highlighted the influence of infiltration processes on metal migration, which aligns with our observations of metal transport from shallow to deep cave sections in Slovačka jama and the Velebita cave system. The accumulation of elements like Pb, Zn, and Cu in cave sediments suggests both allochthonous input (surface-derived material) and internal redistribution within the karst system.
Moreover, our analysis supports the idea that speleothems can serve as long-term environmental archives, recording changes in metal concentrations over time. Pons-Branchu et al. [36] demonstrated that speleothems in urban settings provide valuable records of historical heavy metal pollution, showing enrichment in Pb, Mn, V, Cu, Cd, and Al due to anthropogenic contamination. While our study is focused on deep karst environments rather than urban speleothems, the detection of Cd, Cr, and Ni as a distinct elemental association (factor analysis) raises the possibility of airborne metal deposition from distant pollution sources, a hypothesis also considered in their research.
While Pb anomalies in our samples could originate from natural sources (aluminosilicate components), the presence of additional metals associated with industrial activity suggests that long-range atmospheric transport may also contribute. The role of lead in karst environments has been extensively studied, with Allan et al. [15] demonstrating how Pb concentrations and isotopic ratios in speleothems can be used to trace atmospheric pollution since the Industrial revolution. Further isotopic analysis could help differentiate between these sources.

4.8. Geochemical Characterization of Three Water Samples

Dissolved anions and cations in water samples from Slovačka jama cave indicate that the groundwater belongs to the calcium–bicarbonate type (Ca–HCO3) (Figure 4). Since the water samples have nearly identical compositions in terms of anions and cations, all three points are closely aligned in almost the same position on the Piper diagram. The measurement results for physico-chemical parameters, nutrients, ions, total organic carbon (TOC), and chemical oxygen demand (COD) at the three sampling sites are presented in Table A4. Since water in karst areas is buffered by carbonate, all three analyzed water samples are of a slightly alkaline type, with pH values ranging between 7.7 and 7.9. The dominant cation in all three water samples is Ca, with low concentrations of Mg, Na, and K. Low concentrations of ammonium, nitrates, nitrites, orthophosphates, TN, TP, and TOC indicate that the water in the Slovačka jama cave is not significantly impacted by pollution.
The solubility and transport of elements from speleothems are influenced by pH values and redox conditions. The relatively low concentrations of elements in the water samples suggest oxidative conditions, favoring their deposition in speleothems. This deposition is further supported by the relatively low concentrations of total organic carbon (TOC).
The mean values of pH, nitrates, total nitrogen, and all measured elements—except for Ba and Sr—were higher than the average values reported for Biokovo Mt. springs by [37]. This difference can be attributed to variations in geological composition, as the Velebit region contains both carbonate and non-carbonate rocks, such as clastic formations. Importantly, all measured indicators in the three water samples remained below the maximum permitted values.
Overall, the combined use of mineralogical, geochemical, and statistical methods provided a comprehensive understanding of element distribution in deep karst environments, highlighting both natural and anthropogenic influences on cave sediments.

5. Conclusions and Future Research

This study highlights the complex geochemical interactions in deep karst environments, with speleothems and sediments serving as important archives of elemental transport and potential pollution pathways. Our results align with findings by Rozkowski et al. [13], Pons-Branchu et al. [36], and Allan et al. [15], all of whom investigated metal migration and accumulation in carbonate environments. The detection of heavy metal anomalies in sediments and speleothems suggests that karst systems are influenced by both natural geochemical processes and possible anthropogenic inputs.
Mineralogical analysis confirmed that calcite is the dominant mineral in all samples, as expected in a karst environment, while quartz was present in most samples, likely introduced via fine-grained clastic sediments. Clay minerals, including muscovite, chlorite, kaolinite, and montmorillonite, were found to be associated with higher magnetic susceptibility (MS) and heavy metal anomalies, indicating their role in metal transport. The presence of iron minerals such as magnetite and goethite, particularly in cave sediments, points to multiple possible origins, including natural sources such as bauxites, biogenic activity, or even airborne pollution.
Geochemical and statistical analyses provided additional insights into element distribution and transport within the cave system. Samples composed solely of calcite or calcite with dolomite exhibited the lowest MS values, indicating minimal influence from non-carbonate materials, whereas samples containing clay minerals displayed elevated MS values and a high number of elemental anomalies, supporting the hypothesis that clays play a significant role in metal retention. Boxplot analysis identified the highest number of anomalies in samples 107 and 127, suggesting a complex geochemical environment. Q-mode cluster analysis revealed that heavy metals are more concentrated in shallow cave sections, likely due to airborne deposition or surface leaching, with subsequent transport and accumulation in deeper parts of the cave system. Factor analysis identified cadmium, chromium, and nickel as a distinct group, indicating a different origin from other heavy metals, potentially related to atmospheric deposition or specific geological sources.
This research has advanced the understanding of deep cave geochemistry, particularly since such data are lacking in both the Dinaric karst and karst worldwide. Given the Dinaric karst’s significance, the studied region provides key insights into karst processes and supports remarkable geological and biological diversity. However, several aspects still require further investigation.
Future research should focus on the stable isotope analysis of heavy metals, particularly Pb, to better identify the sources of these anomalies. A detailed examination of element transport to and within the caves, including more detailed geological mapping at depth and seismic profiling, is essential. Additionally, continued monitoring of atmospheric deposition and the identification of distant pollution sources could provide insights into the long-range transport of pollutants. Expanding both the spatial and depth range of sampling will improve our understanding of metal transport mechanisms and their implications for karst hydrology and groundwater protection in anthropogenically impacted areas. Investigating the role of aeolian dust and past volcanic activity in mineral deposition would also help to better understand the origins of clay minerals and associated elements. However, since the study sites are located within the Northern Velebit National Park and a strict nature reserve, with no nearby human settlements or roads, the designation of new protection zones is unnecessary.

Author Contributions

Conceptualization, D.P., S.F.-B. and N.B.; methodology, K.M., S.F.-B., D.P. and N.B.; software, S.F.-B. and D.P.; analysis, S.F.-B., N.B., D.P. and K.M.; investigation, D.P., S.F.-B. and N.B.; collection data in the field, D.P.; writing—original draft preparation, D.P., S.F.-B. and N.B.; writing—review and editing, supervision, D.P., S.F.-B. and N.B. All authors have read and agreed to the published version of the manuscript.

Funding

This research was partially supported by the Northern Velebit National Park, Croatia (2020–2025), and research funding from the Department of Geography in the Faculty of Science, University of Zagreb (2024).

Data Availability Statement

The data will be made available on request.

Acknowledgments

The authors thank Nenad Tomašić for assistance with the mineralogical analysis. We acknowledge the support provided by the Josip Juraj Strossmayer Water Institute, Main Water Laboratory (MWL), especially Simana Milović. We thank the members of the Speleological Society Velebit and Speleological Committee of CMA, Zagreb, for their assistance in field work. We also appreciate the journal’s reviewers for taking their precious time to review the manuscript.

Conflicts of Interest

The authors declare no conflicts of interest.

Appendix A

Table A1. Mineral (phase) composition of speleothem samples. Sign “+” means that sample contains this mineral.
Table A1. Mineral (phase) composition of speleothem samples. Sign “+” means that sample contains this mineral.
SampleCalciteQuartzKaoliniteMuscoviteChloriteMontmorill.MagnetiteGoethitePlagioclaseDolomite
100++
101+
102++
103++
104+++
105++ +++
106++
107+++++++
108++
109++
110++ +++++
111+
112++ +++ +
113+
114++ + +
115++++ +
116++ ++
118++ +
119++++ +
120++
121++ ++
122++ + +
123+ +
124++ ++
125++
126++ + +
127+++ + +
128+++++ +
129++
130++ +++ +
131++
132+
133++ ++ +
134++ ++
135+++
136++
138++
139++
140+
141+
142++
143++
144A+
144B++
145+
Table A2. Results of ICP-MS analysis of 30 chemical elements in solid samples.
Table A2. Results of ICP-MS analysis of 30 chemical elements in solid samples.
SampleAl
mg/kg
B
mg/kg
Ba
mg/kg
Be
mg/kg
Bi
mg/kg
Ca
mg/kg
Cd
mg/kg
Co
mg/kg
Cr
mg/kg
Cs
mg/kg
Cu
mg/kg
Fe
mg/kg
K
mg/kg
Li
mg/kg
Mg
mg/kg
1004730.6796.950.0330.23681,8550.0540.3913.780.4361.6216181292.66101
1012510.5963.200.0150.07192,4650.0400.2874.930.5320.66055894.25.18156
1024720.7608.210.0360.21374,6200.0470.4702.950.5531.2013871362.75200
1033750.2533.600.0200.09886,8360.0440.3503.521.00.83179356.82.7292.6
10435022.1935.30.1561.3649,2490.0761.2910.96.795.76987673114.1377
10541139.9661.50.1750.66490,2030.1531.9812.42.074.20557011435.56507
1064091.734.850.0150.103128,2130.0430.5873.800.2520.5905172693.77300
10713,73713.11120.4522.037320.3745.6431.94.569.3026,293192322.2738
1083200.3635.630.0120.053114,4210.0310.5313.580.1700.54550076.70.61845.2
1091800.1457.820.0160.07287,3550.0860.4502.680.1400.75066427.50.844105
11061714.9071.20.2731.1226,9500.4433.4420.2.3.324.6216,48085323.9321
11130.80.1450.845<0.0050.023106,6000.0170.2932.34<0.0300.37365.612.80.085520
11217190.69446.40.0910.48164,4090.0691.096.551.122.1548985693.06389
1131220.1442.120.0100.04488,8240.0450.4082.410.1070.53942422.60.619209
11419620.60210.50.1050.32375,6380.3841.287.381.472.085203289.94190
11519830.66711.40.0900.36440,6780.2320.9597.611.192.1266643275.01125
11639383.4040.70.1952.9535,9850.3941.6239.94.136.9214,30176218.1534
1181250.2032.710.0110.04582,3590.0180.3231.730.1680.496361.42.21.11274
11927791.2615.50.1751.1855,2980.3662.2325.62.584.0312,32631714.8213
12019.5<0.10013.1<0.005<0.03079,1820.0670.31911.6<0.0300.44184.28.280.047634
12118510.80431.80.1050.88472,3330.1471.156.501.692.1044543233.89712
1229232.07.470.0350.16966,8250.0900.6006.280.8152.2338457671.09396
1231050.2051.570.0110.04469,1730.0200.3092.700.0640.46245963.50.1006630
12423962.1321.00.1380.71554,1260.5051.378.491.253.5887337014.70329
12511.3<0.1000.545<0.0050.154113,7340.0720.26412.0<0.0300.29877.54.670.06810.3
12615050.66023.30.0780.50571,4450.0581.026.311.053.6742414613.23379
12711,2027.1876.10.5032.4615,9500.3235.8435.86.557.6828,640116741.8500
12873883.7463.50.3701.7128,0580.2133.6917.85.566.6520,436133829.5504
12985.9<0.1000.917<0.005<0.03094,9220.0470.3192.520.0690.46025714.60.30019.4
13047332.051380.3021.5613,3200.1052.6214.83.465.9817,600150215.21069
13112.08.3540.512.55.404.120.19854.21.8672.868.20.0890.6851834.44
1323.7017.79.6825.60.7792.450.49532.71.0319132.60.0470.6041231.24
13312.54.5222.16.333.044.140.27257.51.3612580.30.1151.031003.41
1345.665.5514.59.711.402.160.31844.21.1984.849.60.0610.5011141.53
13547.67.0726.516.213.024.90.5031481.7952.03860.7002.231479.66
1361152.801326.107.8513.00.1861081.5026.83420.6220.91277.39.14
1387.913.4082.17.441.051.400.08122.20.87010736.80.0751.0681.51.07
1395607.6711621.731.943.70.78298.52.4530.710681.624.2921224.5
14011.03.9816.06.850.7301.640.25020.40.52311.338.30.0790.29269.60.892
14173.35.0711.76.831.430.8980.15018.71.1947.040.20.1310.6001131.27
1424778.2436.018.020.222.90.65680.71.6338.74961.182.2598.114.0
1430.7675.029.67.350.2510.1760.3592.761.351165.410.0090.9751370.711
144A70.63.5831.06.145.5011.60.09876.50.83085.52870.2640.90068.44.10
144B16.15.0815.27.200.8270.6500.03915.01.2293.429.00.0380.8701040.739
1451265.4517.37.506.767.660.2021060.77218.12140.3080.92076.75.08
SampleMn
mg/kg
Mo
mg/kg
Na
mg/kg
Ni
mg/kg
Pb
mg/kg
Rb
mg/kg
Sb
mg/kg
Si
mg/kg
Sn
mg/kg
Sr
mg/kg
Ti
mg/kg
Tl
mg/kg
U
mg/kg
V
mg/kg
Zn
mg/kg
10012.08.3540.512.55.404.120.19854.21.8672.868.20.0890.6851834.44
1013.7017.79.6825.60.7792.450.49532.71.0319132.60.0470.6041231.24
10212.54.5222.16.333.044.140.27257.51.3612580.30.1151.031003.41
1035.665.5514.59.711.402.160.31844.21.1984.849.60.0610.5011141.53
10447.67.0726.516.213.024.90.5031481.7952.03860.7002.231479.66
1051152.801326.107.8513.00.1861081.5026.83420.6220.91277.39.14
1067.913.4082.17.441.051.400.08122.20.87010736.80.0751.0681.51.07
1075607.6711621.731.943.70.78298.52.4530.710681.624.2921224.5
10811.03.9816.06.850.7301.640.25020.40.52311.338.30.0790.29269.60.892
10973.35.0711.76.831.430.8980.15018.71.1947.040.20.1310.6001131.27
1104778.2436.018.020.222.90.65680.71.6338.74961.182.2598.114.0
1110.7675.029.67.350.2510.1760.3592.761.351165.410.0090.9751370.711
11270.63.5831.06.145.5011.60.09876.50.83085.52870.2640.90068.44.10
11316.15.0815.27.200.8270.6500.03915.01.2293.429.00.0380.8701040.739
1141265.4517.37.506.767.660.2021060.77218.12140.3080.92076.75.08
1151084.6219.98.036.377.230.1801130.93911.13510.3130.91589.64.55
11611112632.820475.035.80.4742012.7668.75300.6032.1916218.6
1182.783.6111.75.200.6451.081.0320.61.3913125.80.0530.83382.30.772
11925170.716.710718.014.80.5311571.8732.55250.4142.3913811.2
1200.98237.111.551.00.2030.1800.3832.900.84743426.650.0103.5275.20.444
12152.94.7220.18.348.011.00.4751000.93911272040.4251.1878.63.53
1229.3316.417.022.02.7810.60.1911350.8881031620.0411.311081.64
1236.357.9313.29.140.2650.8380.20513.91.0565.410.70.0221.131110.755
12485.59.8920.716.310.116.70.3831271.6638.54610.2472.01117.58
1250.23454.34.321070.2430.0760.2261.430.68910.22.980.0450.17092.80.535
12643.63.3026.17.465.619.100.2011191.0376.52040.2600.94086.03.57
1272159.4744.622.929.738.40.8111042.4044.57541.913.2612425.0
1283125.4684.717.024.933.80.5071122.2850.56581.273.0911818.4
1292.286.467.2213.60.4330.4480.0358.520.8128.4418.60.0280.2391610.851
1301453.552049.5517.637.70.3801221.7945.44860.6021.3410712.7
1318.4946118.66581.102.230.10848.90.92128.965.00.0950.36594.51.77
1321.6246.612.663.80.6000.9030.28414.51.080.616.20.0151.431220.848
1331686.0770.310.923.731.50.3601192.1473.86130.420 2.0212412.3
1341362.8538.67.2518.431.80.26371.31.6059.24350.7212.1976.514.1
1351049.9222.321.711.324.70.4191121.3878.83980.9312.6211511.2
13630.37.2915.312.84.428.160.4601261.2976.32050.2611.111494.36
1380.7618.0634.010.70.4620.4010.1767.411.0814.311.00.0210.1131631.13
1392.234.8120.37.340.6210.8380.03914.20.78614.725.80.0230.1261400.734
1406.5518813.42921.080.5760.61418.21.6883.033.90.0210.8551731.40
1412.422.806.134.940.7810.8690.15720.50.41358.633.80.0210.62467.01.10
1423.2597.410.11480.6020.6320.10813.01.3943.121.50.0200.3071650.966
1430.2549.6140.513.00.2360.0910.1001.341.4227.93.860.0430.1441940.777
144A0.3855.8410.59.430.2220.1130.0841.980.83322.52.170.0400.0561220.660
144B1.6140013.45960.1780.1530.3364.330.8501467.10<0.0031.431570.530
1451.087.6717610.90.3240.2300.3136.451.731139.880.0052.531681.17
Table A3. Results of ICP-MS and ion chromatography analysis of 30 chemical elements in three water samples.
Table A3. Results of ICP-MS and ion chromatography analysis of 30 chemical elements in three water samples.
SampleAl
µg/L
As
µg/L
B
µg/L
Ba
µg/L
Be
µg/L
Ca
mg/L
Cd
µg/L
Co
µg/L
Cr
µg/L
Cs
µg/L
Cu
µg/L
Fe
µg/L
K
mg/L
Li
µg/L
Mg
mg/L
W330.30.4412.855.45<0.00537.10.0200.0970.260<0.0301.7238.40.9000.226<0.500
W119.70.3802.493.93<0.00534.8<0.0100.0850.127<0.0302.3313.70.2000.227<0.500
W264.10.3552.853.70<0.00535.1<0.0100.0900.162<0.0301.0614.30.2500.157<0.500
MAC *200101500700n.a.n.a.5n.a.25n.a.200020012n.a.n.a.
SampleMn
µg/L
Mo
µg/L
Na
mg/L
Ni
µg/L
Pb
µg/L
Rb
µg/L
Sb
µg/L
Si
mg/L
Sn
µg/L
Sr
µg/L
Ti
µg/L
Tl
µg/L
U
µg/L
V
µg/L
Zn
µg/L
W31.220.0880.8600.5570.4110.4750.2071.300.06029.00.7320.0040.2120.4431.58
W10.5090.0430.6202.900.1900.2160.0361.16<0.02030.10.579<0.0030.1530.3161.38
W20.6070.0650.6100.649<0.0100.2370.0811.04<0.02027.80.534<0.0030.1410.2831.28
MAC *50n.a.200205n.a.10n.a.n.a.n.a.n.a.n.a.3053000
Notes: * Ordinance on compliance parameters, methods of analysis, monitoring, and water safety plans for human consumption and method of keeping a register of legal entities performing the activity of public water supply (OG 64/2023). n.a.—Not analysed.
Table A4. Results of physico-chemical parameters, nutrients, ions, TN, TP, COD, and TOC in three water samples.
Table A4. Results of physico-chemical parameters, nutrients, ions, TN, TP, COD, and TOC in three water samples.
W3W1W2MAC *
pH7.77.87.96.5–9.5
Conductivity
(µScm−1)
1821671702500
TDS122112114n.a.
Alkalinity (mgCaCO3L−1)908487n.a.
Total Hardness (mgCaCO3L−1)94.488.589n.a.
HCO3 (mgL−1)110102106n.a.
Turbidity (NTU)16.20.750.874
Ammonium
(mgNL−1)
0.017<0.008<0.0080.5
Nitrates (mgNL−1)0.810.740.7750
Nitrites (mgNL−1)<0.002<0.002<0.0020.5
Orthophosphates
(mgPL−1)
0.007<0.0050.0050.3
Sulphates (mgL−1)1.72.11.7250
Chlorides (mgL−1)1.821.01.07250
Fluorides (mgL−1)<0.025<0.025<0.0251.5
TP (mgPL−1)0.008<0.0030.016n.a.
TN (mgNL−1)1.080.830.95n.a.
COD (mgL−1)1.3<0.7<0.75
TOC (mgL−1)2.210.450.58n.a.
Notes: * Ordinance on compliance parameters, methods of analysis, monitoring, and water safety plans for human consumption and method of keeping a register of legal entities performing the activity of public water supply (OG 64/2023). n.a.—Not analysed.
Table A5. Magnetic susceptibility measured in cave samples from Velebit Mt.
Table A5. Magnetic susceptibility measured in cave samples from Velebit Mt.
Sample100101102103104105106107108109110
MS (10−3 SI units)0.0080.0000.0140.0000.0470.0430.0020.1680.0020.0010.064
Sample111112113114115116118119120121122
MS (10−3 SI units)0.0000.0940.0000.0260.0090.0700.0000.0380.0000.0330.005
Sample124125126127128129130131132133134
MS (10−3 SI units)0.0150.0010.0990.0240.0690.0020.1520.0030.0020.0890.060
Sample135136138139140141142143144A 144B 145
MS (10−3 SI units)0.0420.0080.0020.0050.0010.0000.0030.0000.002*0.001*0.000
* p < 0.05.
Table A6. Members of obtained clusters and distances from respective cluster centers.
Table A6. Members of obtained clusters and distances from respective cluster centers.
Cluster Number 1Cluster Number 2 Cluster Number 3
Distance Distance Distance
100 2296.907101 986.315107 3840.709
102 1160.563103 1949.649110 707.108
104 3505.504105 1746.685115 3650.59
112 780.491106 5148.341116 2335.307
114 1327.349108 2782.85127 2383.742
118 2442.552109 1859.763128 995.872
119 2682.862111 1447.447130 1696.761
120 2068.802113 1608.54133 630.79
121 615.082125 2667.503134 857.839
122 428.126129 568.616
123 1283.476131 1669.34
124 2634.997132 1892.675
126 454.429138 241.428
135 3506.321139 113.224
136 979.731140 851.933
141 2363.343142 923.613
143 1501.29
144A1315.248
144B 1271.849
145 274.117
Table A7. Mean values of 10 elements and two other parameters for 3 obtained clusters. Elements’ contents are given in mg/kg, elevation in m.
Table A7. Mean values of 10 elements and two other parameters for 3 obtained clusters. Elements’ contents are given in mg/kg, elevation in m.
Cluster—No. 1Cluster—No. 2Cluster—No. 3
Depth664.25440.25323.89
Al1402.22352.466420.78
B1.040.864.40
Ba17.685.5579.56
Be0.080.020.32
Bi0.480.101.72
Ca68,916.3198,196.2523,043.11
Cd0.130.130.26
Co0.910.463.06
Cr7.5023.3330.18
Cs1.475.564.00
Cu2.240.755.82
Fe4795.51644.8517,686.45
K353.35101.231105.11
Li4.901.2420.72
Mg725.63153.69608.00
Mn53.6213.11248.00
Mo12.6666.9219.33
Na19.8833.5971.88
Ni19.66100.3435.48
Pb5.991.0227.53
Rb9.401.4531.43
Sb0.360.220.49
Si86.0120.21113.50
Sn1.211.102.00
Sr405.1963.5046.96
Ti204.4739.59599.00
Tl0.260.070.96
U1.460.682.39
V106.01128.59123.47
Zn4.551.4016.02
Table A8. Factor loadings (varimax normalized; marked loadings are >0.7).
Table A8. Factor loadings (varimax normalized; marked loadings are >0.7).
Factor—1Factor—2Factor—3
Depth−0.124302−0.023993−0.819019
Al0.9548210.0405760.065068
Be0.9646410.0133760.052559
Ca−0.910654−0.0354860.071048
Cd0.3678320.8704090.002824
Co0.9435610.0883190.060373
Cr0.0970570.9566660.030635
Cu0.9658420.0435180.106860
Fe0.9877100.0450080.063385
Li0.9288420.0595400.121091
Mn0.8607860.1074960.059534
Ni−0.1834420.9408520.034932
Pb0.7922680.1174710.138042
Si0.7225760.0237010.062805
Sr−0.060724−0.024627−0.804648
Zn0.9796500.0572480.111071
Expl.Var9.3809622.6067501.405087
Prp.Totl0.5863100.1629220.087818
Table A9. Factor scores for analyzed samples.
Table A9. Factor scores for analyzed samples.
Factor—1Factor—2Factor—3
100−0.44969−0.4683350.91344
101−0.66168−0.4234530.83505
102−0.44930−0.5071570.74082
103−0.61171−0.4811940.81870
1040.65183−0.4692770.74884
1050.34543−0.2806470.72149
106−0.77655−0.4555620.83723
1072.916830.2204520.07686
108−0.76396−0.4771400.54742
109−0.59976−0.3899110.39858
1101.572511.2307460.06671
111−0.80161−0.5013580.12572
112−0.03876−0.442072−0.02598
113−0.68940−0.4683410.36007
1140.181790.1385920.29450
1150.16931−0.1512570.20318
1161.484450.9831930.95783
118−0.70573−0.5505350.84204
1190.885860.5311370.26291
120−0.34931−0.095727−4.94046
1210.13086−0.249879−2.03191
122−0.13940−0.339670−1.09632
123−0.56206−0.484421−1.03985
1240.479500.399545−1.17644
125−0.87972−0.0121480.13909
126−0.01168−0.4836150.24995
1272.753710.1266280.10225
1281.96719−0.1951670.15930
129−0.76242−0.4431310.47835
1301.28806−0.4394840.58186
131−0.824804.817560−0.06662
132−0.727760.1546020.02479
1331.22900−0.462031−0.21315
1341.10399−0.353444−0.18035
1350.67268−0.338948−0.41738
136−0.08725−0.449788−0.31604
138−0.71929−0.485320−0.28463
139−0.70896−0.517329−0.27965
140−0.741951.245226−0.42709
141−0.59604−0.507463−0.55998
142−0.723490.332592−0.55415
143−0.86040−0.4864550.96571
144A−0.85409−0.5145460.99775
144B−1.023193.1841890.74276
145−0.71303−0.439658−0.58319
Table A10. Correlations between MS and determined chemical elements. Correlations are significant at p < 0.05000. N = 45—marked in red.
Table A10. Correlations between MS and determined chemical elements. Correlations are significant at p < 0.05000. N = 45—marked in red.
AlBBaBeBiCaCdCoCrCsCuFeKLiMg
MS0.730.590.870.750.71−0.750.190.690−0.010.80.740.840.570.09
MnMoNaNiPbRbSbSiSnSrTiTlUVZn
MS0.7−0.150.56−0.140.60.810.310.590.53−0.10.780.640.510.040.72

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Figure 1. Position of Velebita cave system and Slovačka jama cave on the geological map of Velebit Mt. Lithostratigraphical legend: J1—limestones and dolomites (Lower Jurassic), J3—limestones and dolomites (Upper Jurassic), Pg, Ng—carbonate breccia (Paleogene, Neogene). Map: Croatian Geological Survey (2009): Geological map of the Republic of Croatia M 1:300,000, Zagreb.
Figure 1. Position of Velebita cave system and Slovačka jama cave on the geological map of Velebit Mt. Lithostratigraphical legend: J1—limestones and dolomites (Lower Jurassic), J3—limestones and dolomites (Upper Jurassic), Pg, Ng—carbonate breccia (Paleogene, Neogene). Map: Croatian Geological Survey (2009): Geological map of the Republic of Croatia M 1:300,000, Zagreb.
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Figure 2. Sampling locations in Slovačka jama and Velebita cave system, Velebit Mt., Croatia. Red numbers refer to samples. Map: Speleological Committee of CMA (1995–2017).
Figure 2. Sampling locations in Slovačka jama and Velebita cave system, Velebit Mt., Croatia. Red numbers refer to samples. Map: Speleological Committee of CMA (1995–2017).
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Figure 3. Anomalies determined by boxplot method (E: extremes—presented in red color, O: outliers—presented in blue color).
Figure 3. Anomalies determined by boxplot method (E: extremes—presented in red color, O: outliers—presented in blue color).
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Figure 4. Piper diagram of three water samples from Slovačka jama cave. Data for construction of Piper diagram are taken from Table A3 (ICP-MS and ion chromatography results of water samples) for Ca2+, Mg2+, Na+, and K+, while data for all other ions are taken from Table A4, which presents results of physico-chemical parameters, nutrients, ions, TN, TP, COD, and TOC.
Figure 4. Piper diagram of three water samples from Slovačka jama cave. Data for construction of Piper diagram are taken from Table A3 (ICP-MS and ion chromatography results of water samples) for Ca2+, Mg2+, Na+, and K+, while data for all other ions are taken from Table A4, which presents results of physico-chemical parameters, nutrients, ions, TN, TP, COD, and TOC.
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Table 1. List of samples, types, and locations in Slovačka jama cave (S) and Velebita cave system (V).
Table 1. List of samples, types, and locations in Slovačka jama cave (S) and Velebita cave system (V).
CaveDepth (m)SpeleothemSedimentRockWater
S0 116
S10 100101, 118
S65 102, 104103
S140 105106
S285 107
S350108, 119, 129110, 127109
S360114128113, 115W1
S405 126
S550 112111W2
S620125 W3
S1250 124
S1254120, 121 122, 123
V30144A 144B
V50143130
V580131133, 134132
V786 135, 136
V860138, 139
V880 140
V975 141
V1000142, 145
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Paar, D.; Frančišković-Bilinski, S.; Buzjak, N.; Maldini, K. New Insight into Geochemistry and Mineralogy of Deep Caves in Croatian Karst and Its Implications for Environmental Impacts. Water 2025, 17, 1001. https://doi.org/10.3390/w17071001

AMA Style

Paar D, Frančišković-Bilinski S, Buzjak N, Maldini K. New Insight into Geochemistry and Mineralogy of Deep Caves in Croatian Karst and Its Implications for Environmental Impacts. Water. 2025; 17(7):1001. https://doi.org/10.3390/w17071001

Chicago/Turabian Style

Paar, Dalibor, Stanislav Frančišković-Bilinski, Nenad Buzjak, and Krešimir Maldini. 2025. "New Insight into Geochemistry and Mineralogy of Deep Caves in Croatian Karst and Its Implications for Environmental Impacts" Water 17, no. 7: 1001. https://doi.org/10.3390/w17071001

APA Style

Paar, D., Frančišković-Bilinski, S., Buzjak, N., & Maldini, K. (2025). New Insight into Geochemistry and Mineralogy of Deep Caves in Croatian Karst and Its Implications for Environmental Impacts. Water, 17(7), 1001. https://doi.org/10.3390/w17071001

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