Fluid inclusion and stable isotope study of the Cobre–Babilonia polymetallic epithermal vein system, Taxco district, Guerrero, Mexico
Introduction
The Taxco district is found in the northern part of Guerrero state in southern Mexico (Fig. 1), close to the boundaries with Morelos and México states. The district lies in the southeastern part of a broad north–northwest trending belt of polymetallic epithermal deposits (Damon et al., 1981, Clark et al., 1982, Camprubí et al., 2003a), which includes the Guanajuato, Pachuca-Real del Monte, Zacatecas, Sombrerete and Fresnillo districts. In neighboring areas such as Temascaltepec, Sultepec, Amatepec and Miahuatlán-Ixtapan del Oro, other vein deposits are hosted in similar stratigraphic sections. Although Taxco is one of the oldest mining districts in the Americas, it still lacks detailed studies. This district includes Ag–Zn–Pb producing mines (namely the San Antonio, Guerrero, Babilonia, Guadalupe, Golondrina, Pedregal and Hueyapa mines) presently mined or explored by Industrial Minera México SA de CV (IMMSA). The first geologic descriptions of the district by Fowler et al. (1948) and Osborne (1956), and later work by Pérez-Segura (1973), Gómez-Fragoso (1973), and Leija-Vázquez (1973) partially describe some of the mineralized structures. In this paper we provide fluid inclusion and stable isotope data from the Cobre–Babilonia vein system and from the nearby Esperanza Vieja and Guadalupe mantos.
Section snippets
Regional geology
The epithermal deposits in Taxco are related to hydrothermal activity associated with the latest volcanic activity of the Sierra Madre del Sur (SMS). The epithermal veins have not been directly dated, but are attributed an age of 38–36 Ma (Alaniz-Álvarez et al., 2002, Camprubí et al., 2003a). Paleozoic Taxco Schists form the basement, and are unconformably overlain by the propilitized Late Triassic–Early Jurassic Taxco Viejo Greenstone, that consists mainly of propylitized andesitic flows.
Structure and stratigraphy of the veins
There are more than 50 individual veins in the Taxco district, most of them striking NW (30° to 50°), that are associated with large replacement mantos, especially south of the veins. The veins are hosted by all the rocks described above, although the Tertiary pyroclastic rocks show only limited development of the veins, and this is true for the Cobre–Babilonia vein system within a mechanically incompetent rock where veins split in a horse-tail structure. The mantos formed preferentially at the
Fluid inclusions
A fluid inclusion microthermometry study was performed on 130 samples that are distributed in a 3200-m long and 900-m deep section (Fig. 2). The analyzed minerals were sphalerite, quartz and calcite. We analyzed only inclusions hosted by minerals lacking evidence for recrystallization. Primary, secondary, and pseudosecondary inclusions were found, which are liquid-rich or vapor-rich with no daughter minerals. The fluid inclusions are mostly 5 to 15 μm in size, but range up to 50 μm, and are
Stable isotopes
δ18O and δ13C values in calcite were measured using the CO2 obtained using the conventional method of McCrea (1950). The analyses were carried out with a Finnigan Delta Plus XL mass spectrometer at the Instituto de Geología of the UNAM. Oxygen and carbon isotopes are reported in using the delta permil notation with respect to the V-SMOW and V-PDB standards, respectively. Calcite samples show δ13C of − 10.4 for the Guadalupe vein, − 7.5 for the Esperanza Vieja manto, and between − 5.4‰ and − 9‰ for
Discussion and conclusions
The mineralogy of veins and mantos, the dominance of the Zn–Pb–Cu associations over Ag–Au, plus the characteristics of associated mineralizing fluids and stable isotopes, indicate that the Cobre–Babilonia vein system is an epithermal deposit that belongs to the intermediate sulfidation type, though mineralizing fluids are less saline in late mineral associations and thus suggest an evolution towards the low sulfidation field (see Sillitoe and Hedenquist, 2003, Camprubí and Albinson, in press).
Acknowledgements
This work was partially funded with the Conacyt research projects 46473 and 42642. Special thanks are devoted to IMMSA and the staff at Taxco for their assistance. The stable isotope analyses were carried out by Edith Cienfuegos at the Instituto de Geología of the UNAM and Clemente Recio at the Universidad de Salamanca. We also thank Caridad Hernández, Anastasio Lozano, and Francisco Otero for their assistance in isotopic analyses. We also gratefully acknowledge the critical reviews of G.
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