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Metallogenic model of the Eocene Santa María and Antares Zn-Pb(-Ag) skarn deposits, Velardeña Mining District, Durango, Mexico.

Authors :
Cano, Néstor
Camprubí, Antoni
González-Partida, Eduardo
González-Ambrocio, Ana K.
Alfonso, Pura
Miggins, Daniel P.
Fuentes-Guzmán, Edith
Cienfuegos-Alvarado, Edith
Iriondo, Alexander
Source :
Mineralium Deposita; Apr2024, Vol. 59 Issue 4, p671-698, 28p
Publication Year :
2024

Abstract

The Santa María and Antares Zn-Pb(-Ag) skarn deposits in the Velardeña Mining District are located in central–NW Mexico. They lie 470 m apart along the contact between Oligocene felsic intrusions and Cretaceous limestones, and were developed during prograde, retrograde, post-ore (Santa María), and late stages. Firstly, the prograde stage was formed by fluids at ~ 600 °C and 15 wt% NaCl equiv., and consists of garnet + wollastonite ± clinopyroxene and biotite ± K-feldspar assemblages. Secondly, the retrograde/ore stage was formed by fluids at 300–500 °C with salinities of 20–30 wt% CaCl<subscript>2</subscript> (Santa María) and > 40 wt% NaCl equiv. (Antares). It comprises assemblages of chlorite, amphibole, epidote, calcite, scapolite, quartz, sericite, adularia, fluorite, and muscovite associated with sphalerite, pyrite, galena, pyrrhotite, arsenopyrite, chalcopyrite, and Pb-Bi-Sb sulfosalts. Thirdly, the post-ore stage was formed by fluids at ~ 400 °C and 20–30 wt.% CaCl<subscript>2</subscript> and comprises poorly mineralized calcite veins. Fourthly, the late stage was formed by fluids at < 300 °C and 20–30 wt.% CaCl<subscript>2</subscript> (Santa María) and ~ 15 wt% NaCl equiv. (Antares), and crystallized tetrahedrite-group minerals and pyrite + marcasite. δ<superscript>18</superscript>O<subscript>fluid</subscript> between ~ 14‰ and 23‰ at Santa María and between ~ 12‰ and 17‰ at Antares show a less-modified magmatic affinity for mineralizing fluids at Antares; δ<superscript>13</superscript>C<subscript>fluid</subscript> between 0‰ and –6‰ register recycling of sedimentary C. Moreover, sulfides with δ<superscript>34</superscript>S<subscript>VCDT</subscript> between –3‰ and 2‰ reveal a magmatic source for S. Altogether, these data suggest that, at Santa María, magmatic-derived fluids actively interacted with the wall rocks, whereas at Antares the fluid-rock interaction was milder. In both deposits, metal deposition was triggered by the cooling and neutralization of ore-bearing fluids with carbonate rocks. Our <superscript>40</superscript>Ar/<superscript>39</superscript>Ar dates for adularia of ca. 37.5 Ma place the deposits within the Eocene–early Miocene metallogenetic epoch of central–NW Mexico, during which other world-class skarn-epithermal systems were emplaced (e.g., Concepción del Oro and Mazapil-Peñasquito). [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00264598
Volume :
59
Issue :
4
Database :
Complementary Index
Journal :
Mineralium Deposita
Publication Type :
Academic Journal
Accession number :
176033354
Full Text :
https://doi.org/10.1007/s00126-023-01225-4