Elsevier

Chemical Geology

Volume 371, 15 April 2014, Pages 96-114
Chemical Geology

Fluid geochemistry and geothermometry in the unexploited geothermal field of the Vicano–Cimino Volcanic District (Central Italy)

https://doi.org/10.1016/j.chemgeo.2014.02.005Get rights and content

Highlights

  • We studied the geochemical features of fluids emerging around the Lake Vico (Italy).

  • Waters emerge from both shallow (cold) and deep (thermal and CO2-rich) reservoirs.

  • Gas phase is dominated by CO2 which is mainly originated by decarbonation reactions.

  • The structural framework plays a key role in the upraise of deep-originated fluid.

  • Secondary processes significantly affect the chemistry of the uprising deep fluids.

Abstract

The Vicano–Cimino Volcanic District (VCVD) is related to the post-orogenic magmatic activity of the peri-Tyrrhenian sector of Central Italy. The chemical and isotopic compositions of 333 water discharges and 25 gas emissions indicate the occurrence of two main sources: 1) cold Ca-HCO3 to Ca(Na, K)-HCO3 type waters from relatively shallow aquifers hosted in volcanic and sedimentary formations; and 2) thermal Ca-SO4(HCO3) type waters located in a deep CO2-pressurized reservoir, hosted in carbonate–evaporite rocks and separated from the shallow aquifers by thick sequences of low-permeability formations. Carbon dioxide is mainly produced by thermal metamorphic decarbonation within the deepest and hottest parts of the carbonate–evaporite reservoir (δ13C–CO2 from − 3.1 to + 2.2‰ vs. VPDB), likely affected by a mantle-rooted CO2. Release of CO2-rich gases from the deep aquifer into the overlying shallow aquifers produces high-CO2 springs and bubbling pools. The spatial distribution of thermal waters and CO2-rich cold discharges is strongly controlled by fractures and faults located in correspondence with buried structural highs. Stable isotopes (δD and δ18O) suggest that meteoric water feeds both the shallow and deep reservoirs. The relatively low R/Ra values (0.27–1.19) indicate that He is mainly deriving from a crustal source, with minor component from the mantle affected by crustal contamination related to the subduction of the Adriatic plate. Consistently, relatively high N2/Ar and N2/3He ratios and positive δ15N–N2 values (from 0.91 to 5.7‰ vs. air) characterize the VCVD gas discharges, suggesting the occurrence of a significant “excess” nitrogen. Isotopic compositions of CH413C–CH4 and δD–CH4 values from − 28.9 to − 22.1‰ vs. VPDB and from − 176 to − 138‰ vs. VSMOW, respectively), and composition of light alkanes are indicative of prevalent thermogenic CH4, although the occurrence of abiogenic CH4 production cannot be excluded. The δ34S–H2S values (from + 9.3 to + 11.4‰ vs. VCDT) are consistent with the hypothesis of H2S production from thermogenic reduction of Triassic anhydrites. Gas geothermometry in the H2O–H2–Ar–H2S system suggests that the VCVD gases equilibrated in a liquid phase at redox conditions controlled by interactions of fluids with the local mineral assemblage at temperatures lower (< 200 °C) than that and measured in deep (> 2000 m) geothermal wells. This confirms that secondary processes, i.e. steam condensation, gas dissolution in shallow aquifers, re-equilibration at lower temperature, and microbial activity, significantly affect the chemistry of the uprising fluids. Thermal water chemistry supports the occurrence in this area of an anomalous heat flow that, coupled with the recent demographic growth, makes this site suitable for direct and indirect exploitation of the geothermal resource, in agreement with the preliminary surveys carried out in the 1970's–1990's for geothermal exploration purposes.

Introduction

The Vicano–Cimino Volcanic District (VCVD) is part of a thermally anomalous area that extends from southern Tuscany down to the Campanian volcanic areas of the Phlegrean Fields and Vesuvius, where CO2-pressurized reservoirs developed in a complex geodynamic setting (Barberi et al., 1994, and references therein). Thermal emissions and mineral springs, as well as areas characterized by an anomalously high CO2 diffuse degassing from the soil, are spatially controlled by fractures and faults related to an extensional tectonic regime (Minissale, 2004, and references therein). Most VCVD thermal manifestations are located W of the town of Viterbo along a N10°E tectonic alignment (Fig. 1). Here, the thermal activity is known since Etruscan and Roman times and acknowledged by Dante in the Divina Commedia (Dante Alighieri, Inferno XIV, 76–84). Thermal discharges are currently used as spa thermal resorts for health therapies and public pools (Chiocchini et al., 2001). A thermal spa near Nepi (Terme dei Gracchi), constructed in Roman times (Fig. 1), exploits sulfur-rich and sparkling waters that are currently bottled for commercial use. The VCVD, as well as the whole region between southern Tuscany and northern Latium, was intensively investigated for evaluating geothermal potential (Conforto, 1954, Cataldi and Rendina, 1973, Calamai et al., 1976, Cataldi et al., 1978, Borghetti et al., 1983, Bertrami et al., 1984, Cavarretta and Tecce, 1987, Cataldi et al., 1995, Barelli et al., 2000). Starting from the early 1950's, 9 deep wells and 76 test-holes (Fig. 1) were drilled by Terni Company (Conforto, 1954) and then, by the Italian energy provider (ENEL) and the national oil company (ENI-AGIP). A maximum temperature of 218 °C was measured in the Cimino 1 well, at the depth of 2153 m. Despite the significant potential highlighted by these preliminary explorations, the geothermal resources at VCVD have not yet been exploited.

Geochemical data of some fluid discharges from VCVD were reported in studies carried out at regional scale (Baldi et al., 1973, Arnone, 1979, Duchi et al., 1985, Chiodini et al., 1995, Chiodini et al., 1999, Minissale et al., 1997a, Minissale, 2004), whereas recent investigations have dealt with the reconstruction of a hydrogeological conceptual model of the Viterbo thermal area (Piscopo et al., 2006, Baiocchi et al., 2012) and VCVD (Baiocchi et al., 2006, Angelone et al., 2009, Chiocchini et al., 2010).

This study presents an original and detailed dataset of chemical and isotopic analyses of 333 fluid discharges (cold and thermal waters) and 25 gas emissions collected from VCVD. The main goals are to: 1) evaluate the fluid contributions from different source regions and their relationship with the tectonic assessment, 2) constrain the chemical–physical conditions controlling the chemistry of the fluid reservoirs, and 3) investigate the effects of secondary processes occurring during the uprising of deep-originated fluids toward the surface. Geochemical data were integrated with the available information concerning the stratigraphical, geophysical, hydrogeological and structural setting aimed to define a detailed conceptual model for fluid circulation and provide insights into the most promising areas for geothermal exploitation.

Section snippets

Geological and hydrological setting

VCVD is located along the peri-Tyrrhenian sector of Central Italy and covers a surface area of approximately 1400 km2. This sector has undergone a post-collisional Plio-Quaternary extension that has led to the development of NW–SE and NE–SW-trending fault sets (Barberi et al., 1994). The former fault set is dominantly extensional, while the transverse NE–SW-trending faults are transtensive/transfer structures accommodating differential extension (Borghetti et al., 1981, Acocella and Funiciello,

Role of structural framework in the upraise of deep-originated fluids

The fluids in the study area mostly discharge in correspondence with the buried structural highs, which are schematically interpreted as horst structures on the basis of residual gravity anomalies (see the regional cross-section AB of Fig. 2). However, some of the structural highs likely refer to thrust folds later affected by the Plio-Quaternary extensional tectonics. Fold anticlines are privileged locus of fluid trapping and thus, they might represent important elements in the reconstruction

Water analysis

Complete results of field and laboratory analysis for almost all cold waters are provided as supplementary material (SM 1, 2). Temperature, pH, Eh, electrical conductivity and alkalinity (titration with 0.05 N HCl) concentrations were determined in the field. Water samples for laboratory analysis were filtered at 0.45 μm and stored in high-density polyethylene bottles. Two aliquots were acidified with HCl and ultra-pure HNO3, respectively. Ion-chromatography (F, Cl, Br, SO42  and NO3) on

Chemical and isotopic composition of waters

Cold waters located in both the volcanic and sedimentary domains (Fig. 1) have total dissolved solids (TDS) generally lower than 1000 mg/L, slightly acidic to slightly alkaline pH and Ca-HCO3 to Ca(Na,K)-HCO3 composition (Fig. 3). The pCO2 values, computed by using the PHREEQC code v. 2.12 (Parkhurst and Appelo, 1999), are lower than 0.07 bars. Exceptions are some cold waters, locally known as acque acetose (samples 38, 62, 79, 83, 84, 87, 91, 109, 122, 123, 150, 167, 170, 174, 179, 191, 192,

Processes governing the chemical and isotopic composition of waters

As shown in the δD vs. δ18O diagram (Fig. 5a), where the Global Meteoric Water Line (GMWL; Craig, 1961) and the Mediterranean Meteoric Water Line (MMWL; Gat and Carmi, 1970) are reported, the isotopic signature of most waters from VCVD is consistent with that of meteoric water. The negative 18O-shift shown by most of bubbling pools (samples 37, 80, 81, 308, 316, 324) is likely produced by isotopic exchange between water and CO2 (Negrel et al., 1999, Cartwright et al., 2002). In contrast, water

Temperature and redox conditions controlling uprising fluids

Chiodini and Marini (1998) demonstrated that chemical–physical conditions controlling the source regions of hydrothermal fluids are successfully predicted by applying geothermometric techniques in the H2O–CO2–CH4–H2–CO system. Unfortunately, the VCVD gas discharges lack of necessary prerequisites for this theoretical approach, since they are characterized by the presence of liquid water with T  63 °C at the gas emergences, which causes condensation of water vapor and dissolution of soluble

Conclusions

The VCVD hosts a water-dominated reservoir fluid having a sulfate-bicarbonate-type composition at T ~ 220 °C, whose surface emergence occurs along extensional fractures and faults affecting the buried structural highs (Fig. 17). Thermal waters seep out at temperatures ranging from 21 to 63 °C, indicating a strong cooling during the fluid uprising and mixing between deep fluids and shallow aquifers. A CO2-dominated gas phase is commonly associated with the thermal springs of the area, although

Acknowledgments

This work has benefitted by the financial support of the project Ricerca compilativa delle caratteristiche geologico-strutturali, idrologiche e geochimiche dei M. della Tolfa (Resp. D. Cinti), the Fluid Geochemistry, Geological Storage and Geothermics unit of INGV (Resp. F. Quattrocchi) and the Laboratory of Fluid and Rock Geochemistry of University of Florence (Resp. F. Tassi). All the municipalities of the VCVD are warmly thanked for their help during the extensive field work. A special

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