Reinaldo Sáez

Prof. Dr. Reinaldo Sáez

Earth Science Department, University of Huelva, Avenida de las Fuerzas Armadas, S/N, 21071 Huelva, Spain

Research Focus & Metrics

Academic Career Length

30Years (1997-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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7 July 1999 in Mineralium Deposita
Verified
Journal Article
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RSReinaldo Sáez
Reinaldo Sáez
EPE. Pascual
E. Pascual
Manuel ToscanoManuel Toscano
Manuel Toscano
ALAlmodóvar
Almodóvar
GRG. R.
G. R.

14 October 2010 in Mineralium Deposita
Verified
Journal Article
Closed access
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RSReinaldo Sáez
Reinaldo Sáez
CMCarmen Moreno
Carmen Moreno
FGFelipe Gonzalez
Felipe Gonzalez
GAGabriel R. Almodóvar
Gabriel R. Almodóvar

24 October 2019 in Minerals
Verified
Journal Article
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GSGabriel Ruiz de Almodovar Sel
Gabriel Ruiz de Almodovar Sel
LYLola Yesares
Lola Yesares
RSReinaldo Sáez
Reinaldo Sáez
Manuel ToscanoManuel Toscano
Manuel Toscano
FGFelipe Gonzalez
Felipe Gonzalez
JPJuan Manuel Pons
Juan Manuel Pons
The Iberian Pyrite Belt (IPB) is recognized as having one of the major concentrations of volcanogenic massive sulfide (VMS) deposits on Earth. Original resources of about 2000 Mt of massive sulfides have been reported in the province. Recent classifications have considered the IPB deposits as the bimodal siliciclastic subtype, although major differences can be recognized among them. The main ones concern the hosting rocks. To the north, volcanic and volcaniclastic depositional environments predominate, whereas to the south, black shale-hosted VMS prevail. The mineral composition is quite simple, with pyrite as the main mineral phase, and sphalerite, galena, and chalcopyrite as major components. A suite of minor minerals is also present, including arsenopyrite, tetrahedrite–tennantite, cobaltite, Sb–As–Bi sulfosalts, gold, and electrum. Common oxidized phases include magnetite, hematite, cassiterite, and barite. The spatial relationship between all these minerals provides a very rich textural framework. A careful textural analysis reported here leads to a general model for the genetic evolution of the IPB massive sulfides, including four main stages: (1) Sedimentary/diagenetic replacement process on hosting rocks; (2) sulfides recrystallization at rising temperature; (3) metal distillation and sulfides maturation related to late Sb-bearing hydrothermal fluids; and (4) metal remobilization associated with the Variscan tectonism. The proposed model can provide new tools for mineral exploration as well as for mining and metallurgy.

2 December 1997 in Mineralium Deposita
Verified
Journal Article
Closed access
PDF file
GSGabriel Ruiz de Almodovar Sel
Gabriel Ruiz de Almodovar Sel
RSReinaldo Sáez
Reinaldo Sáez
JPJ. M. Pons
J. M. Pons
AMA. Maestre
A. Maestre
Manuel ToscanoManuel Toscano
Manuel Toscano
EMEmilio Pascual Martínez
Emilio Pascual Martínez

24 August 2024 in Minerals
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Journal Article
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RSReinaldo Sáez
Reinaldo Sáez
FGFelipe Gonzalez
Felipe Gonzalez
TDTeodosio Donaire
Teodosio Donaire
Manuel ToscanoManuel Toscano
Manuel Toscano
LYLola Yesares
Lola Yesares
CMCarmen Moreno
Carmen Moreno
The Iberian Pyrite Belt (IPB) represents one of the largest districts of volcanogenic massive sulfide (VMS) deposits in the world, and is a critical source of base metals (Cu, Pb, and Zn) for Europe. Confirmed resources exceed 1700 Mt of massive sulfides with grades of around 1.2% Cu, 1% Pb, and 3% Zn as well as more than 300 Mt of stockwork-type copper mineralization. Significant resources of Sn, precious metals (Au and Ag), and critical metals (Co, Bi, Sb, In, and Se) have also been evaluated. The genesis of these deposits is related to a complex geological evolution during the late Devonian and Mississippian periods. The geological record of such evolution is represented by three main lithological units: Phyllite–Quartzite Group, the volcano–sedimentary Complex (VSC), and the so-called Culm Group. The sulfide deposits are located in the VSC, associated with felsic volcanic rocks or sedimentary rocks such as black shales. The massive sulfide deposits occur as tabular bodies and replacement masses associated with both volcanic and sedimentary rocks. Their mineralogical composition is relatively simple, dominated by pyrite, chalcopyrite, sphalerite, and galena. Their origin is related to three evolutionary stages at increasing temperatures, and a subsequent stage associated with the Variscan deformation. The present paper summarizes the latest developments in the IPB and revises research areas requiring further investigation.

14 January 2019 in Minerals
Verified
Journal Article
Open access
PDF file
CMCarmen Moreno
Carmen Moreno
FGFelipe Gonzalez
Felipe Gonzalez
RSReinaldo Sáez
Reinaldo Sáez
The Rammelsberg sulfide deposit is classically considered as a SEDEX-type deposit. The origin of SEDEX-type massive sulfides links with the evolution of their hosting basins. They frequently constitute the source for the metal-enriched basinal brines transported afterwards as mineralizing hydrothermal fluids. This study revisits previous data concerning the analysis of the basin that hosts the Rammelsberg deposit, the Goslar basin, updating its subsidence analysis and providing new tectonic and total subsidence curves from two different paleogeographic locations: the depocenter and the basin margin. The basin evolution is defined by five stages depicting different subsidence intensity and mechanisms for each of these locations. The stratigraphic position of Rammelsberg coincides with a drastic change in the basin evolution. A rapid tectonic subsidence event is proposed as a trigger mechanism for hydrothermal activity. The paleogeographic location and the relation between supply of mineralizing fluids and sedimentation rate were critical for the concentration or dissemination of sulfides.