1. Introduction
The Salar de Atacama, located in the Antofagasta Region in northern Chile, is an extensive evaporitic basin covering approximately 2900 km
2, making it the second-largest salt flat in the world after the Uyuni salt flat in Bolivia. This salt flat lies between the Domeyko Range to the west and the Andean Altiplano to the east, forming what has been geographically termed one of the pre-Andean basins. This area is characterized by an extremely arid climate, with the annual precipitation typically barely reaching 16 mm in the flattest part of the salt flat [
1]. The geological and hydrogeological structure of the salt flat is complex, featuring a central nucleus primarily composed of halite containing interstitial brine (halite nucleus), surrounded by various evaporitic units that include gypsum and carbonates, as well as fine detrital units (
Figure 1).
The Salar de Atacama has been extensively studied, including aspects such as its isotopic composition [
2,
3,
4,
5,
6], stratigraphy of evaporite deposits [
7,
8,
9], and underground flow dynamics [
1,
10,
11,
12,
13,
14]. However, uncertainties persist regarding some important hydrogeological and hydrogeochemical processes that control its hydrodynamics, such as the recharge mechanisms in the nucleus and surrounding areas, the relationship between the upper and lower aquifers, the impact of brine extraction on the salt wedge, and the ecosystems on the edge of the salt flat, among others.
Figure 1.
Geography of the study area in Chile: (
A) location of the Salar de Atacama and (
B) geological map of the study area (modified from [
9]). The maps are georeferenced in UTM coordinates.
Figure 1.
Geography of the study area in Chile: (
A) location of the Salar de Atacama and (
B) geological map of the study area (modified from [
9]). The maps are georeferenced in UTM coordinates.
The brine from the halite nucleus of the Salar de Atacama is a hypersaline solution resulting from the concentration of surface and groundwater subjected to intense evaporation in a closed basin environment [
2]. These brines can have conductivity values exceeding 200,000 µS/cm, indicating extreme salinity. Their chemical composition is dominated by high concentrations of sodium and chloride, with significant amounts of lithium, potassium, magnesium, sulfate, and calcium [
6]. The chloride concentrations can exceed 240,000 mg/L, and the sodium concentrations can surpass 120,000 mg/L. The unique chemical composition reflects the interaction of complex hydrogeological and geochemical processes that have occurred over long periods of time [
15]. Additionally, the
87Sr/
86Sr ratios in the waters of the nucleus also indicate complex processes of the dissolution, mixing and evaporation of evaporites [
6]. A detailed analysis of the chemistry of the nucleus brine can be reviewed in Munk [
6].
In this regard, the hydrogeology of the salar is determined by the interaction between the surface and groundwater. The main current source of recharge has been identified as lateral groundwater flows from the peripheral sub-basins, mainly from the north and southeast [
12,
15,
16,
17,
18]. This aligns with other interpretations that have also determined that the recharge of the salar’s aquifer occurs primarily at the edge of the salar, although they have also mentioned a mechanism of infiltration from lagoons fed by groundwater that discharges into the springs in the Soncor area [
3].
Furthermore, a gap between the brine extraction and estimated recharge has been recognized [
5]. Between 2000 and 2010, an average brine level decrease of 0.3 m was recorded in the southern sector of the salt flat. However, considering the amount of brine extracted and the estimated recharge from local precipitation, evaporation, and shallow groundwater flow, various calculations have suggested that the level should have decreased by about 2.0 m [
5]. This difference between the expected and observed decline indicates that there are additional water sources that have not been fully accounted for in the water balance of the salt flat nucleus and require further analysis [
19]. In this respect, it has been proposed that these sources may include deep groundwater flows or the migration of the freshwater–brine interface [
5,
17].
The isotopic determination of δ2H and δ18O in the brine of the halite nucleus shows significant variations that are difficult to explain in a steady state. In the central part of the nucleus, slightly depleted isotopic values have been identified compared to the brines from the margins. These isotopic values allow for the identification of various recharge sources, distinguishing between meteoric waters, surface waters affected by extreme evaporation, and deep groundwater recharge.
The extraction of brine in the Salar de Atacama has previously been studied, but it is still unknown how this activity impacts the isotopic composition of groundwater and the mixing zone between freshwater and brine that occurs at the edge of the salt flat. The rapid recharge of fresh water into the brine aquifer after significant precipitation events has also been documented [
5]. However, this recharge is limited, due to the low frequency of significant rainfall events in the basin. Furthermore, recent research has suggested that the recharge of the upper aquifer might be decoupled from modern inputs and dominated by fossil water, although they did not evaluate the waters of the saline nucleus [
17]. The study of the evaporites of the nucleus of the Salar de Atacama has revealed the presence of lacustrine deposits indicating periods of greater humidity in the past [
8,
9,
20], suggesting significant changes in the recharge over time.
The environmental impact assessment of brine extraction on the various ecosystems of the Salar de Atacama is a critical aspect that requires further research. Moreover, most of the previous studies have focused on the current state of the system, limiting the evaluation of the long-term sustainability of the water resources and the prediction of the future impacts of lithium extraction and climate change on the salt flat [
17]. The growing concern among the communities in the Salar de Atacama basin about the high extraction of lithium-rich brine in the central part of the Salar de Atacama motivated the conducting of various hydrogeological investigations and monitoring, both public and private, to evaluate the natural environment and, especially, the marginal lagoons of the salt flat. Since the 1990s, these investigations have generated a large amount of data, now available from various public agencies responsible for managing water resources and the environment. From these more than two-decades-long monitoring activities, the changes in groundwater levels, as well as the chemical and isotopic composition of the surface and groundwater, have been recorded. The study of δ
18O and δ
2H isotopes in this research is possible thanks to the more than 12 years of systematic sampling of various water points, conducted by the Sociedad Química y Minera de Chile (SQM) throughout the Salar de Atacama basin [
21,
22]. The data stored in this extensive database include water samples from rivers, lagoons, shallow wells, and deep wells from across the basin. The isotopic data from various studies conducted by the company Albemarle and published in various scientific articles and technical reports have also been used in this research. This study specifically focuses on the isotopic variation in δ
18O and δ
2H in the waters of the halite nucleus.
The objective of this research is to characterize the water flow in the halite nucleus of the Salar de Atacama through a study of the spatial and temporal variations in the isotopic composition of δ18O and δ2H, in order to determine possible recharge sources. In this sense, the application of δ18O and δ2H isotopes to trace groundwater flow is essential, considering that the paleoclimate of the Salar de Atacama basin has been variable from the Late Pleistocene to the present, as evidenced by the alternation of arid periods dominated by the formation of evaporites, and more humid periods where lakes were formed.
2. Climate
The Salar de Atacama is located in an arid–hyperarid climatic zone, characterized by very low precipitation and a high potential evaporation rate [
7]. This hyperarid climate is influenced by several climatic factors, including the cold Humboldt Current and the Andes Mountains. The Humboldt Current, which flows parallel to the coast of Chile [
18], lowers the air temperature and limits evaporation, thereby reducing the atmospheric humidity available for precipitation formation. Additionally, the Andes Mountains act as a significant orographic barrier, preventing the passage of moist air masses from the east and further intensifying the region’s aridity [
1,
23].
Precipitation in the Salar de Atacama is scarce and shows marked spatial and temporal variability. Most of the precipitation occurs during the austral summer, mainly between January and March, due to the influence of moisture from the Amazon Basin [
24]. Lesser amounts of precipitation are recorded between April and August due to the passage of cold fronts from the Pacific Ocean [
1]. The average annual precipitation on the surface of the salt flat is approximately 16 mm [
25]. Additionally, the precipitation in the basin exhibits a decreasing gradient, from approximately 300 mm/year in the Andes Mountains to about 5 mm/year in the Domeyko Range [
1].
The evaporation rate in the Salar de Atacama is extremely high, with an annual potential value of approximately 2130 mm [
13,
26]. This high evaporation rate is attributed to a combination of factors, such as the high temperatures, the intense solar radiation reaching the surface, the wind speed, and the low relative humidity in the region [
25,
27]. During the summer, when temperatures are higher, evaporation reaches its peak [
1,
3]. The average annual temperature in the Salar de Atacama is approximately 14.1 °C. The average maximum temperatures reach around 24 °C, while the minimum temperatures average around 4 °C. These temperatures can vary significantly between day and night due to the nature of the desert climate [
1,
28].
3. Geology of the Salar de Atacama
The general structure of the Salar de Atacama can be divided into three main zones: the saline nucleus, the marginal zone, and the alluvial fan zone [
9]. The halite nucleus constitutes the central part of the salt flat and is characterized mainly by halite, with some intercalations of sulfates and carbonates (
Figure 1).
The halite nucleus, which covers nearly 50% of the surface area of the Salar de Atacama, is characterized by very homogeneous crusts composed almost exclusively of sodium chloride, with a smaller proportion of fine detrital material [
29]. This evaporitic unit represents the most superficial manifestation of growth associated with the ascent of groundwater near the surface, which increases in salinity due to evaporation and halite precipitation
The marginal zone of the Salar de Atacama is composed mainly of evaporitic deposits of carbonates and sulfates, intercalated with fine-grained detrital deposits, such as clays and silts [
5,
6].
The alluvial system, located on the eastern edge of the salt flat, consists of fans formed by the accumulation of sediments transported by ephemeral streams descending from the surrounding Andes. These cone-shaped fans extend over the flat surface of the salt flat. The alluvial fans in this region are composed mainly of unconsolidated sediments, such as gravels, sands, and silts [
3]. These materials are transported by water during infrequent precipitation events, resulting in episodic sedimentation. The fans exhibit a variety of slopes that decrease from the apex near the mountains to the distal edges, where they merge with the surface of the salt flat [
30].
4. Hydrogeology of the Nucleus of the Salar de Atacama
The nucleus of the Salar de Atacama, with a surface area of approximately 2900 km
2, presents a geological composition that is key to understanding groundwater flow. This hydrogeological unit is mainly composed of halite, although it shows some variability in its evaporitic and detrital facies vertically, leading to significant heterogeneity [
2]. The entire halite nucleus is also intersected by the salar fault system, which plays an important role in its hydrogeological structure. This fault, which traverses the halite nucleus, has caused significant vertical displacements, creating an uplifted block on the western side and a subsided block on the eastern side [
20]. These differences in thickness and associated fault structures have influenced hydraulic connectivity within the halite nucleus [
14]. Thus, for the hydrogeological description and interpretation of the halite nucleus in this study, the nucleus is subdivided based on this fault, defining a Western Domain and an Eastern Domain of the nucleus (
Figure 1).
From a hydrostratigraphic perspective, the shallowest part of the halite nucleus can be divided into three main units. The upper part of the aquifer system is predominantly composed of halite, forming an upper aquifer with variable thickness across the nucleus. In the Western Domain, this aquifer has a thickness of approximately 15 to 20 m, while in the Eastern Domain, it reaches up to 30 m. The thickness variation in the upper aquifer is likely controlled by the active tectonics of the main north–south fault that crosses the salar nucleus (Salar Fault). This fault, with active tectonics, has played a fundamental role in the formation of ancient paleo-lakes in different periods [
20]. This upper halite aquifer is characterized by a high hydraulic conductivity, with values ranging from 101 to 103 m/day [
11]. The high heterogeneity of its hydraulic properties is largely controlled by structures of preferential connectivity, such as karst conduits and fault zones [
14].
Immediately below this upper aquifer, a thin layer of sulfate and organic matter has been identified, with a thickness varying from 0.2 to 4 m [
29]. Due to the hydraulic characteristics of this unit, it is considered to act as an aquitard in the halite nucleus [
12].
Figure 2 presents an isopach map of the aquitard, clearly showing that in the Western Domain, the thickness of this unit varies between 0.20 m and 1 m, while in the Eastern Domain, the thicknesses are greater, varying between 0.2 and 2 m [
29]. In general, the greatest thickness of the aquitard occurs in the northern part of the halite nucleus, where it can reach up to 4 m in thickness.
Immediately below the aquitard, another halite aquifer is recognized which, although similar in composition to the upper aquifer, exhibits lower permeabilities, with values ranging from 1 to 40 m/day, thereby limiting water circulation compared to the upper aquifer [
11]. The top of this lower aquifer is defined by the base of the aquitard. The base of the aquifer is not clearly defined due to the variability in the detrital and evaporitic facies existing in different parts of the Salar de Atacama. In the Western Domain, the base of the lower halite aquifer consists of gypsum levels identified at a depth of 50 m. In this case, the thickness of the lower aquifer is 20 to 30 m. In the Eastern Domain, the base of the lower aquifer is not clearly defined, due to the greater thickness of the evaporitic facies, mainly composed of halite. In the northern part of the nucleus, the gypsiferous facies are more abundant and thicker than in the southern part [
29]. Various hydraulic studies conducted in the lower aquifer have classified it as semi-confined [
11,
12].
5. Paleoclimate in the Salar de Atacama Basin
Various paleoclimatic studies conducted in the Atacama Desert in northern Chile have provided valuable information on climate variability from the Late Pleistocene to the present [
31]. Specifically, paleoenvironmental studies have identified significant fluctuations in the climatic conditions in the Atacama Desert, resulting in periods of increased or decreased precipitation, which are reflected in the formation and expansion of paleolakes and paleowetlands during the Late Pleistocene and, to a lesser extent, during the Holocene [
32]. For the Altiplano, most of these studies have agreed that during the Last Glacial Maximum (approximately 16,000 years ago), arid conditions prevailed [
32,
33,
34,
35]. These studies have also indicated a wetter period at the end of the Last Glacial Maximum (LGM), between 14,000 and 9000 years BP. It was during this period that many of the current salt flats in the Altiplano constituted various permanent Andean lakes and reached their maximum extent. Radiocarbon dating has established that the expansion of most of the ancient Altiplanic lakes began approximately 14,000 to 12,000 years BP, reaching their maximum levels between 10,800 and 9200 years BP [
32,
33,
36,
37]. From their maximum extent, reached 9200 years ago, there was a decline in lake levels, until many of these water bodies disappeared or had a significant reduction in their surface area between 8400 and 8000 years BP [
33]. However, studies of the age of the aquifer recharge in the coastal range of northern Chile have identified a third, less intense wet period [
38,
39]. This period of increased recharge associated with moisture from the Pacific Ocean has also been recognized in the Domeyko Range, south of the study area [
40].
In the Salar de Atacama, the wetter periods that occurred from the end of the Pleistocene to the Holocene are also recorded in the stratigraphy of the halite nucleus. In a study of three cores in the evaporitic deposits, pristine chevron halite facies were identified [
9]. This type of evaporitic halite facies is associated with saline lakes, according to the classification by Lowenstein and Hardie [
41]. Several paleolake periods with these types of evaporitic facies were identified in the upper 200 m of the eastern sector of the salt flat, which were dated using the
230Th/
234U disequilibrium method in halite formed during the lake stages, particularly trapped clay minerals rich in U [
8,
9]. The thickest layer identified in the halite nucleus reaches 23 m in thickness and terminates at a 42 m depth. In the western block of the halite nucleus, this layer is thinner, with a thickness of 17 m, terminating at a 14 m depth [
9]. This primary halite layer shows some dissolution features in its base, indicating increasingly wetter conditions and the existence of a permanent paleolake that existed in the Salar de Atacama [
2,
8,
9,
20]. Dating has determined that the formation of this paleolake started around 60 to 30 ka, and terminated 16.5 ± 3.6 ka [
8,
9]. The lake was at its deepest during the LGM and its termination, an age that approximately coincides with the period of expansion of the Andean lakes during the wetter period at the end of the LGM, although the
230Th/
234U dates obtained have a high standard deviation.
In the halite nucleus, two other levels of pristine chevron halite evaporites have also been identified at 10 and 5 m depths, but are much thinner, indicating the shorter duration of these paleolakes [
2]. For these last two wetter periods, only the upper layer has been dated, giving an approximate age of 5.4 ± 2.7 ka. Both evaporitic layers have been interpreted as the result of the formation of ephemeral lakes that existed approximately 10? ka and 5.4 ka, respectively [
2,
9]. These ages of wetter periods coincide with the results of paleowetland studies conducted in the Salar de Atacama basin and nearby areas, which have defined two significant wet periods since the end of the Pleistocene [
42]. The first period ranged from 12,800 to 8100 years BP, recorded only in the eastern part of the Salar de Atacama (in Tilomonte), and a second, more active period from 7400 to 3000 years BP, recorded in the Tilomonte area, Loa River, Salado River, and Puripica Ravine. The stable isotope data of the paleolake water trapped in the chevron halite fluid inclusions indicate that the weather patterns and moisture sources were similar to those of today [
2].
6. Methodology
The communities of the Salar de Atacama basin, particularly those located near the salar, are interested in preserving the lagoons and wetlands on the eastern edge of the salar, which host ecosystems rich in flora and fauna. Since the 1990s, various hydrogeological research and monitoring efforts, both public and private, have been carried out to assess the impact of brine extraction on the nucleus of the Salar de Atacama. These efforts have generated a significant amount of data, which have been made partially available through public and private organizations responsible for water resource management and environmental protection.
This analysis of δ
18O and δ
2H isotopes was conducted using an extensive database that includes water samples collected by SQM at various points across the Salar de Atacama basin [
21,
22]. The samples encompass water from rivers, lagoons, shallow wells, and deep wells, collected between 2008 and 2020. Although some of the data series are incomplete and, in certain cases, only three data points are available, in general, the isotopic records offer data at an annual or biennial frequency.
The samples utilized in this study were analyzed for their isotopic composition at the University of Waterloo (Ontario, Canada) [
21,
22]. The δ
18O values were determined through CO₂ equilibration following the method of Epstein and Mayeda (1953), employing a Gilson Autosampler, GVI MultiFlow system, and an Iso-Prime CF-IRMS, with a precision of ±0.2‰ [
21]. For the δ
2H analysis, water reduction to hydrogen gas on hot chromium was conducted using a CTC AS200 Autosampler, Eurovector Euro 3000 Elemental Analyzer, and a Micromass IsoPrime mass spectrometer, achieving a precision of ±0.8‰. The saline samples with conductivities greater than 10,000 μS/cm were pre-treated by distillation. The results were standardized using the international reference materials VSMOW (Vienna Standard Mean Ocean Water) and VSLAP (Vienna Standard Light Antarctic Precipitation) from the International Atomic Energy Agency (IAEA) [
21,
22].
Our research focused on analyzing the spatial and temporal variations in the isotopic composition of δ
18O and δ
2H in the water from wells located in the upper aquifer of the halite nucleus. For this analysis, three transects (W-E) in the halite nucleus, located in the northern, central, and southern parts, were examined (
Figure 1). A total of 82 δ
18O and δ
2H isotopic data points were used (
Table S1, Supplementary Material). Some of the wells had up to eleven measurements of δ
18O and δ
2H taken over different time periods, while other wells had only two data points. To characterize the isotopic composition of the lower aquifer, four wells were selected, with a single sample from each (
Table S2, Supplementary Material). In this case, a smaller number of wells were selected (only four) to ensure that the waters from these wells were representative of the lower aquifer [
22].
The collected data underwent a rigorous analysis process to identify patterns in the isotopic variation in δ18O and δ2H. Specialized software was used for the data processing, allowing for comparison between the different sampling points and the identification of the potential influences of brine extraction on the marginal areas of the halite nucleus. The expectation was that in these zones, farther from the areas of intensive extraction, the mixing of waters from different sources induced by pumping would be less significant, providing a clear baseline for impact assessment.
Additionally, the research was complemented with isotopic data provided by the company Albemarle, which also conducts brine extraction in the southern part of the halite nucleus [
43].
7. Results
7.1. Isotopic Composition of δ18O and δ2H in the Salar de Atacama Basin
To provide an overview of the isotopic composition of the waters in the Salar de Atacama, a general characterization of the isotopic composition of δ
18O and δ
2H in the waters from the main hydrogeological units of the Salar de Atacama basin is presented.
Figure 3 shows a δ
18O vs. δ
2H plot summarizing the isotopic compositions of the precipitation, water from deep wells within the alluvial aquifer, and water from wells located in the marginal and central parts of the Salar de Atacama.
The data used for the isotopic characterization of the precipitation in this research were obtained from the southern part of the Salar de Atacama. However, there is extensive work on the isotopic characterization of δ
18O and δ
2H in the precipitation of the Salar de Atacama basin [
24]. Samples corresponding to the accumulated rainfall were collected at three monitoring stations located at different altitudes in the southern part of the Salar de Atacama basin. The samples obtained correspond to the accumulated rainfall during the months of January, February, and March 2017. Snow samples were also collected in June 2017. The location of the snow sampling points was the same as that of the rainwater collectors. These analyses also include some specific data collected by the authors during other sampling campaigns in the Altiplano (near Laguna Tuyajto) [
44,
45].
In contrast, the isotopic composition of the groundwater in the eastern alluvial aquifer of the Salar de Atacama was obtained from [
46]. The recharge of the peripheral aquifers of the Salar de Atacama mainly comes from local precipitation and the infiltration of surface waters generated within the hydrographic basin of the salar itself [
24]. The isotopic values of δ
18O vs. δ
2H in the alluvial aquifer fall within a narrow range, varying between −7‰ and −9‰ for δ
18O and between −50‰ and −68‰ for δ
2H (
Figure 3). This narrow range of isotopic composition in an extensive alluvial aquifer may result from good water mixing within the aquifer. Based on this consideration, it has also been assumed that these waters have had a long residence time in the aquifer [
2]. These isotopic values also coincide with those obtained for the volcanic aquifer in the southern part of the Salar de Atacama basin, in the Monturaqui sub-basin [
15] (
Figure 3).
The isotopic composition of the waters in the Salar de Atacama is more complex to characterize due to the different sources contributing to it. To provide an initial characterization of the isotopic composition of δ
18O and δ
2H in the waters of the halite nucleus and the marginal zone of the Salar de Atacama, the isotopic values obtained from various previous investigations were used. In the northern and eastern marginal zones of the Salar de Atacama, the waters emerging from various springs are channeled into surface flows that circulate within the salar, forming different lagoons (
Figure 3). The isotopic signature of these spring waters originates from the waters of the alluvial aquifer, which discharge at the edge of the salar. One of the most notable lagoon systems is Soncor [
3,
4,
47]. Most of the waters near the spring emergence points (Laguna Puilar) have an isotopic composition of δ
18O and δ
2H similar to that of the wells in the alluvial aquifer. However, as the waters flow through small streams into the interior of the salar, they progressively show greater fractionation due to evaporation, as observed in the waters of Laguna Chaxa and Laguna Barros Negros. In
Figure 3, only some of these waters, which show some degree of evaporation fractionation, are plotted [
47].
In the southern marginal zone, the isotopic compositions of the waters are strongly influenced by the groundwater input from the Monturaqui sub-basin [
15]. The transect used to evaluate the isotopic composition of the waters from the alluvial aquifer to the nucleus of the salar showed progressive isotopic enrichment due to evaporation [
5]. This transect revealed that the greatest evaporation fractionation occurred in the waters of the various lagoons located in the marginal zone. It was also observed, for the first time, that the isotopic composition of the groundwater located further inside the halite nucleus had a less enriched isotopic composition than the waters of the lagoons in the marginal zone, explained by the direct groundwater input from the Cordón de Lila, which mixes with the brine of the halite nucleus [
5].
Figure 3.
Isotopic composition of δ
18O and δ
2H of rain water, lagoons, and groundwater of Salar de Atacama basin. GMWL = global meteoric water line; δ
2H = 8δ
18O + 10‰ [
2,
5,
15,
46,
47,
48].
Figure 3.
Isotopic composition of δ
18O and δ
2H of rain water, lagoons, and groundwater of Salar de Atacama basin. GMWL = global meteoric water line; δ
2H = 8δ
18O + 10‰ [
2,
5,
15,
46,
47,
48].
7.2. Isotopic Composition of δ18O and δ2H in the Halite Nucleus
As discussed in the section on the hydrogeology of the halite nucleus, the aquifer system can be divided into a Western Domain and an Eastern Domain, separated by a regional fault oriented approximately north–south [
20]. The majority of the brine extraction wells (pumping wells) operated by various companies are located in the Western Domain, with extraction primarily from the upper aquifer. Conversely, in the Eastern Domain there are no pumping wells for brine extraction, but there are a large number of monitoring wells. This distinction is relevant when interpreting the isotopic values of the groundwater, as the flow induced by the numerous brine extraction wells in the Western Domain is slower, thereby reducing the possibility of mixing water from different aquifers, which is associated with more chaotic groundwater flow lines near brine extraction sites.
The isotopic composition of the upper aquifer was characterized using monitoring wells located mainly in the eastern edge of the halite nucleus (
Table S1). In most cases, shallow wells not exceeding 30 m in depth were used. Generally, in the Eastern Domain, the upper aquifer can reach depths of up to 30 m [
11]. Since the wells in this area are farthest from the brine pumping area, their isotopic composition was assumed to be less affected by the flow induced by pumping, thus avoiding the potential mixing effects associated with these flows. Additionally, since 1996, brine reinjection into the upper aquifer has been practiced, and the isotopic composition of the reinjected brine is unknown, potentially altering the isotopic interpretation of the waters closer to the extraction field.
Special attention is given to the initial isotopic data obtained at the start of monitoring around 2008, when the brine extraction rates were still lower than the current ones, and the drawdowns were not as significant. The isotopic data used in this characterization are from determinations made between 2008 and 2020, although many of the data series are incomplete.
To characterize the isotopic composition of δ
18O and δ
2H in the lower aquifer, data were selected from the SQM database from wells for which the well construction details and the location of the screened intervals are clearly indicated [
21]. Several wells labeled as “deep nucleus” in the database show screen openings throughout their depth or do not specify their location, potentially resulting in mixed water and a distinct isotopic composition, which could mischaracterize the lower aquifer. Therefore, the isotopic data from these monitoring wells were excluded from this analysis. The only samples likely to have a representative composition of the lower aquifer were obtained from four wells: KINT-04, KINT-08, KINT-33, and KINT-35 (
Table S2). Although these wells are located in the Western Domain of the nucleus, their screen positions between 23 and 40 m depths suggest the absence of mixing with water from the upper aquifer. The isotopic values of δ
18O and δ
2H in the waters of the lower aquifer fall within a narrow range, varying from −0.87‰ to −2.49‰ for δ
18O and from −26.04‰ to −33.25‰ for δ
2H. These isotopic values are considerably depleted compared to the isotopic composition of the upper aquifer waters.
To achieve a spatial and temporal characterization of the isotopic variation in δ
18O in the waters of each analyzed sector, three transects were delineated, including wells located near the marginal zone and extending toward the interior of the halite nucleus (
Figure 4). A northern, central, and southern transect were analyzed to evaluate whether the changes in the isotopic composition of δ
18O over time were local or associated with a general change within the halite nucleus.
Figure 1 and
Figure 2 show the location of the various wells used in these transects. To assess the relationship between the isotopic variation in δ
18O in the brine and in the drawdowns caused by brine pumping in the extraction field, drawdown measurements, obtained from the same wells that were sampled for the isotopic analysis, were also plotted alongside the δ
18O values.
An initial interpretation of the isotopic values of δ
18O and δ
2H for the eastern edge of the halite nucleus allows us to recognize that there was an isotopic evolution of these values, from highly enriched isotopic values to lighter values, in a short period of time. The most enriched δ
18O and δ
2H isotopic values occurred between the years 2008 and 2012, and the lightest isotopic values occurred between the years 2013 and 2020, identified in the initial interpretations of [
22]. The explanation for the progressive isotopic lightening of the waters is associated with the recharge due to more the frequent rainfall that has occurred since 2013. This hypothesis is only plausible if the changes in the isotopic composition of the groundwater begin from the eastern edge of the halite nucleus, where the waters enter from various springs and, through small streams, reach the lagoon systems in the nucleus and infiltrate them. On the other hand, to produce such significant changes in the isotopic composition of the upper aquifer water, the recharge from precipitation would have to be very high, which does not seem to be the case. In this research, an analysis is attempted using the different transects, starting from the eastern edge of the halite nucleus toward the center of the salar, to evaluate the spatial and temporal isotopic changes shown by the waters of the upper aquifer.
7.3. Northern Transect
In the northern transect, the wells considered ranged from those located very close to the marginal zone to those toward the interior of the nucleus. These wells included SOPM-14 (located 3 km from Laguna Barros Negros), L2-14 (located 6 km from the marginal zone), SOPM-4 (located 9 km from the marginal zone), and MSW-268 (located 15 km from the marginal zone and 3 km from the pumping well field) (
Figure 1 and
Figure 2).
As shown in
Figure 4, the waters from well SOPM-14, situated very close to the marginal zone, exhibit the most enriched isotopic values, with δ
18O values ranging from +9.6‰ to +9.9‰. These more enriched values correspond to the samples obtained at the beginning of isotopic monitoring, in 2008 and 2012. Subsequently, from 2016 to 2020, more depleted isotopic values are observed, reaching +2.92‰ for δ
18O in 2020. Unfortunately, there are no data available for between 2013 and 2015 to infer when the most significant isotopic change occurred. In 2019, there is a slight rise in water levels, possibly related to reduced pumping. Coincidentally, the δ
18O value of the water shows a slight increase in isotopic enrichment, with values of +3.9 and +4.2‰.
In the case of well L2-14, located slightly further inside the nucleus in the northern transect, the initial isotopic value of δ18O measured in 2008 is +3.47‰. In subsequent years, the general trend shows a progressive depletion in isotopic composition until 2016, when the value reaches +0.46‰.
Finally, wells SOPM-4 and MSW-268, situated further inside the halite nucleus, generally show little variation in their isotopic composition from 2008 to 2020. The isotopic composition of both wells is more depleted, generally corresponding to the isotopic composition of the lower aquifer.
7.4. Central Transect
In the central transect of the halite nucleus, there are few wells with extensive δ18O data series that allow for a comprehensive analysis of the isotopic trends. In this analysis, wells L4-16 (located 0.5 km from the marginal zone) and L4-6 (located 3.6 km from the marginal zone) are considered. Both wells have extensive isotopic data series from 2008 to 2020. The data from some wells closer to the pumping well field are also used, but these wells generally have very few data points to establish clear trends in the isotopic evolution. Additionally, these latter data should be considered cautiously due to the potential for mixing and other previously described considerations. This group includes wells MSW-275 (located 7.3 km from the marginal zone) and MSW-246 (located 12.6 km from the marginal zone).
In this transect, similar to the northern transect, the wells closest to the marginal zone show a trend towards less enriched δ18O isotopic values, synchronized with greater drawdowns. The changes in the δ18O isotopic composition are first observed in well L4-6, located further inside the halite nucleus compared to well L4-16, which is situated closer to the marginal zone. Additionally, well L4-6 shows some stability in its isotopic composition value around +7.5‰ until 2012, after which there is a general trend towards lighter δ18O isotopic values, reaching −5.81‰. This isotopic value is the lightest recorded and falls outside the defined range for the lower aquifer. In the case of well L4-16, located farther from the pumping well field, changes in the δ18O isotopic composition begin in 2015 and are less pronounced than in well L4-6. Generally, the latest δ18O isotopic determinations from 2018 to 2019 tend to stabilize around a value of 4.61‰. It is interesting to note that in well L4-16, the change in composition to lighter values begins in 2012, while in the well closer to the marginal zone, where most of the recharge is assumed to occur, the change only begins in 2015.
Unlike the general trend in the northern transect, where the isotopic values of the wells closer to the pumping well field generally showed a trend towards lighter δ
18O values, this trend is not present in the central transect, and the observed values tend towards enriched δ
18O values. It is difficult to explain the observed isotopic values in wells MSW-275 and MSW-246. The data on the thickness of the aquitard in this sector indicate that it reaches its greatest thickness here [
29]. One possible way to explain the more enriched δ
18O isotopic values relates to the increased thickness of the aquitard in this sector. The increase in aquitard thickness could hinder the upward vertical flow from the lower aquifer to the upper aquifer. However, since this sector is closer to the pumping well field, this scenario should be viewed with caution.
7.5. Southern Transect
The southern transect of the nucleus of the salar was characterized using wells 1028 (located 0.6 km from the marginal zone), TPB-5 (located 1.7 km from the marginal zone), L10-11 (located 2.5 km from the marginal zone), and L10-12 (located 4.5 km from the marginal zone). The isotopic composition data from well MSW-253 (located 11 km from the marginal zone) were also used in this characterization, although with the caution of the previously mentioned considerations.
Figure 4 presents a graph of the time series of the drawdowns and the δ
18O isotopic values of the analyzed well waters.
In the case of well L10-11, located 3 km from the marginal zone, there is a marked lightening of the δ18O isotopic composition observed between 2018 and 2020, ranging from 4.17‰ to −2.4‰. This change coincides well with a significant piezometric level drop of nearly 1 m recorded in the same well. Unfortunately, there are no isotopic data available for the years 2019 and 2020 for well L10-12.
Finally, in the case of well MSW-253, it is observed that the δ
18O value is around −2.9‰, and varies very little over the course of 10 years. This value is quite close to the lightest value found in the lower aquifer. This well is located near the SQM well field and also the Albemarle well field, so high contributions from the water from the lower aquifer are expected. Additionally, in this sector, the thickness of the aquitard is thinner, reaching approximately between 20 and 40 cm in thickness (
Figure 2).
Some wells in the southern part of the nucleus of the Salar de Atacama were sampled almost monthly during 2013 [
43]. This was the case for well TPB-5, which was monitored eight times during 2013, allowing for an analysis of the general trend in the isotopic evolution of δ
18O and δ
2H during this period, which also coincided with a year of significant precipitation in the salar [
5].
Figure 5 shows the evolution of the δ
18O and δ
2H isotopic values over time, with the major precipitation events of 2013, obtained from the Paine meteorological station, added to the graphs [
49]. This figure clearly shows the general trend toward lighter δ
18O and δ
2H isotopic values, as observed in the different transects analyzed. However, slightly enriched δ
18O and δ
2H isotopic values can also be seen shortly after precipitation events. This observation may be due to the direct recharge of rainwater over the nucleus of the salar, as suggested by previous studies [
5]. It is highly likely that this precipitation infiltrated through cracks in the salt crusts of the salt flat and underwent isotopic fractionation due to evaporation as it descended. However, due to the limited amount of precipitation and its infrequent occurrence, the recharge is expected to be not very significant.
Figure 5.
Isotopic composition of δ
18O y δ
2H from well PTPB-05 monitored during the year 2013 (red rhombus) and precipitation (mm) events recorded at the Paine station [
49].
Figure 5.
Isotopic composition of δ
18O y δ
2H from well PTPB-05 monitored during the year 2013 (red rhombus) and precipitation (mm) events recorded at the Paine station [
49].
Figure 6 presents the δ
18O and δ
2H graph of the samples used in the previously presented transects. This graph also includes the isotopic composition of the waters from the lower aquifer. Additionally, samples from the alluvial aquifer are included to analyze their relationship with the waters of the upper and lower aquifers. As observed in
Figure 6, the waters from the various transects show more enriched isotopic compositions of δ
18O and δ
2H when monitoring began in 2008, and progressively, over the course of a decade, their composition tends toward the isotopic composition of the waters from the lower aquifer. Although almost all the water samples from the upper aquifer have an isotopic composition that tends toward the composition of the lower aquifer, there are two samples that exhibit a lighter isotopic composition of δ
18O and δ
2H. These correspond to the water from wells L4-6 and 1028p, located in the central and southern parts of the eastern edge of the halite nucleus. In the case of the sample from well 1028p, the isotopic value of δ
18O and δ
2H falls within the isotopic composition range of the waters from the alluvial aquifer and the Vilama River, while the sample from well L4-6 is slightly more enriched. The composition of these waters with lighter isotopic values may have several explanations that will be addressed in the Discussion.
9. Conclusions
The isotopic composition of δ18O and δ2H in the waters at the upper part of the halite nucleus are not homogeneous and show some isotopic stratification, with less enriched isotopic values at depth. The preliminary results of this research suggest that the waters less enriched in δ18O and δ2H are located in the lower aquifer immediately below the aquitard.
This analysis of the isotopic composition of δ
18O and δ
2H in the halite nucleus of the Salar de Atacama shows significant spatial and temporal variations between 2008 and 2020, which can be attributed to the flows induced by intensive brine extraction and the mixing of waters from aquifers with very different isotopic compositions. Brine extraction has created a hydraulic imbalance, causing upward vertical flows from the confined lower aquifer to the unconfined upper aquifer, as evidenced by the isotopic changes observed in the monitoring wells. This also coincides with recent research conducted using SAR interferometry (InSAR) based on SAOCOM-1, ALOS-2, and Sentinel-1 data, which concluded that a 2.5 cm subsidence is occurring in the halite nucleus associated with brine extraction [
58].
The more depleted δ18O and δ2H isotopic values in the lower aquifer suggest significant historical recharge from ephemeral paleolakes formed during the wet periods of the Holocene. This implies that a significant portion of the water stored in the lower aquifer may have been trapped for thousands of years. The wetter climatic conditions of the past would have played a crucial role in the recharge of the aquifers, and the identification of three periods of paleolake formation supports the hypothesis of significant historical recharges, favored by higher hydraulic gradients and infiltration processes. The waters recharged from the ancient paleolakes would have mixed with waters coming mainly from the northern and southern parts of the Salar de Atacama, through contributions from the confined aquifers.
The results of our research also highlight the role that thin layers of low permeability, interlayered between permeable units, can play in potentially modifying vertical flow and causing changes in brine flow.
For the sustainable management of the water resources in the Salar de Atacama, it is essential to continue the isotopic monitoring of δ18O and δ2H, assessing the future evolution of the flow and the impact of brine extraction. The application of this methodology in future projects for extracting the lithium-rich brines in the other salt flats of the central Andes will allow for a better understanding of the flow and recharge dynamics in these complex hydrogeological systems, contributing to the sustainability of water resources in arid and hyperarid regions.