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introduce the subject prior to the field guides. Many studies have presented the overall
characteristics of the geology and mineral deposits of the IPB (e.g. Carvalho et al., 1976; Strauss
et al., 1977; Carvalho, 1979; Routhier et al., 1980; Barriga, 1990). Very recently, Carvalho et al.
(1997) have summarized rather thoroughly the present state of the art concerning the IPB geology
and
SEG Neves Corvo Field Conference 1997 Introduction to the IPB
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quartz are the most common phenocryst phases.Typical specimens are composed of small grains
(devitrified glass, quartz and feldspar) within a very fine-grained volcanic matrix.
4.
Regionalpyrite equivalent). The deposits can be divided into three main groups (Figure 5): l)
autochthonous (rooted or proximal), 2) transitional, and 3) allochthonous (redeposited or distal).
Most deposits have footwall stockworks, and are included in the autochthonous (proximal) and
transitional sub-type deposits (Carvalho, 1979; Barriga, 1990). Stockwork mineralization is
composed of anastomosing veinlets and vein networks (feeder channels) and disseminations of
Introduction to the IPB SEG Neves Corvo Field Conference 1997
12
sulfides that grade into massive sulfide lenses by coalescense of veins and replacements.
Stockworks occur principally in highly silicified and chloritized footwall volcanic rocks - the socalled
stockwork rock (Barriga and Carvalho, 1983). Examples of well-developed stockworks are
those of Rio Tinto, Aznallcóllar, La Zarza, Concepción, Aljustrel (Feitais) and Neves-Corvo.
Some deposits (e.g. some bodies of Lousal, Sotiel and Tharsis) that have neither stockwork nor
hydrothermal alteration are considered allochthonous due to either distal deposition or to synvolcanic
tectonism displacement and redeposition. Barite is commonly present in almost all
proximal deposits. The IPB volcanogenic sulfide deposits have many features in common with
equivalent deposits associated with felsic volcanic rocks of other world famous
the IPB is the single largest VMS district in the world (see Leistel et al., 1994; Carvalho et al.,
1997). The average composition of known resources and reserves is: Cu - 1.3%; Zn - 2.0%; Pb -
Figure 5.
Types of VMS deposits, geologic setting and ore-zone alteration in the IPB (after Carvalho 1979; Barriga1990). A: Felsic volcanic rocks; B: Predominantly chloritic alteration and cupriferous stockwork; C: Predominantly
sericitic alteration; D: Massive polimetallic sulfides; 1: Autochthonous subtype; 2: Transitional subtype; 3:
Allochthonous subtype; J: Jaspers with Mn.
SEG Neves Corvo Field Conference 1997 Introduction to the IPB
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0.7%; Au - 0.5 g/t; Ag - 26 g/t; S - 45%; Fe - 40%. Concentrations ranging from tens to hundreds
of ppm of minor metals such as: Sn, Co, Cd, Hg, Bi, Sr, In are commonly present.
About 90 individual massive sulfide deposits are known in the IPB and most of them occur in
clusters. These clusters may represent multiple hydrotherrnal vent fields within the same volcanic
center, or bodies or lenses dismembered and displaced from larger, pre-existing accumulations
due to syn-depositional slumping or to post-depositional slivering by faults and thrusts, or both.
The spectrum of ore lens distribution ranges from S. Domingos (mined out), which is a singular
orebody, to Neves-Corvo, where at least five interconnected bodies have been delineated (see JT
Oliveira et al., this volume); to Lousal (mined out), with 18 separate ore lenses from 100,000 tons
to >3 million tons (Strauss and Madel, 1974). The S. Domingos case is unique, and the reason for
this singular deposit may be due to erosion of other deposits, or because additional lenses remain
to be discovered. An additional, small syn-sedimentary displacement or tectonic deformation on
the big Neves-Corvo sulfide accumulation could have led to the spatial separation of five or more
Figure 6
. Size and grade characteristics of selected copper deposits (after Jansen and Bateman, 1981 andCarvalho et al., 1997).
Introduction to the IPB SEG Neves Corvo Field Conference 1997
14
completely separated bodies. Almodovar et al. and Silva et al (this volume) present detailed
accounts of the various deposits at Aznallcóllar, Tio Tinto, Tharsis and Aljustrel.
The bulk of the mineralogy in massive sulfide bodies comprises fine to medium grained pyrite,
with variable amounts of sphalerite, chalcopyrite, galena (and cassiterite at Neves Corvo).
Tetrahedrite-tennantite, arsenopyrite, bournonite and pyrrhotite are common, and many other
minerals have been identified in small and trace amounts. Tin minerals, cassiterite and Cu-Zn-Sn
sulfides (stannite-kesterite, mawsonite and stannoidite) are present in most deposits, and reach
extremely high concentrations in the tin and copper-tin ores at Neves-Corvo. The tin ores at
Neves Corvo are unique among VMS deposits globally in this respect (see JT Oliveira et al., this
volume).
Sedimentary structures such as graded bedding, cross-bedding, sedimentary breccias and slump
structures are common in massive, laminated ores. Primary colloform and framboidal textures are
present in pyrite in most deposits. Gaspar (1991, 1995c) described textures in ores at Aljustrel,
Neves-Corvo and Lagoa-Salgada as similar to those in sulfide chimneys of black smokers from
hydrothermal fields of the East Pacific Rise. In a broad sense, mineralogical and chemical
zonation within IPB deposits is similar to that found in VMS from other areas.
6.1
Manganese deposits and other metalliferous sedimentsHundreds of small manganese deposits are known from within the Volcanic-Sedimentary
Complex of the IPB, and have been object of minor mining operations. They occur within various
lithologies, namely tuffites, siliceous slates (often red or purple, hematitic) and cherts and jaspers.
The ensemble of the Mn concentrations and their immediate host lithologies constitute mappable
units, and lie invariably on volcanic rocks, both mafic and felsic, or on their lateral equivalents.
They constitute good field evidence of a late- to post-volcanic environment, but cannot be
considered true "marker horizons" in exploration for massive sulphide deposits, because they
occur associated with both productive and non productive volcanic episodes Jaspers are
particularly significant, and are perhaps the most typical rocks of the IPB (Carvalho, 1979).
The cherts, jaspers and manganese ores related to felsic volcanism are almost exclusively
chemical hydrothermal sea floor precipitates (Barriga and Oliveira, 1986).
A similar, but much more detailed study of the Aljustrel siliceous and metalliferous
sediments (Barriga, 1983; Barriga and Fyfe, 1988) indicates a hydrothermal origin for these
SEG Neves Corvo Field Conference 1997 Introduction to the IPB
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15
rocks, and unveils an intimate relationship with the genesis of the associated sulphide ores (see
Silva et al, this volume).
7.
Hydrothermal alterationHydrothermal alteration is a prominent feature of several lithologies of the VS Complex,
notably igneous rocks in general and essentially all host rocks to autochthonous massive sulphide
deposits. Two main types can be considered: regional and ore zone alteration.
7.1
Regional alterationMost, if not all volcanic and hypabissal rocks in the IPB have been affected by (sea water)
hydrothermal metamorphism (Munhá and Kerrich, 1981; Barriga, 1983, 1990). The rocks are
spilitized (propylitized), often with nearly total replacement of the igneous minerals.
Alteration of the igneous rocks on a regional scale has importance on metallogenetic studies
and on mineral exploration. In some instances it has been possible to document metal leaching
from volcanic rocks, implying that mineralized solutions may have originated from such
processes (Barriga, 1983; Barriga and Fyfe, 1997).
7.2
Ore zone hydrothermal alterationOre zone hydrothermal alteration includes stockworks, their peripheral haloes, and in some
instances additional alteration types, particularly hanging wall alteration. The core of stockworks
(Type 1 ore-zone alteration) is invariably constituted by stockwork rock (chlorite-quartz-pyritechalcopyrite).
At Lagoa Salgada, the paragenesis includes pyrophyllite (Relvas et al., 1994). A
peripheral halo of sericite + quartz + pyrite ± sphalerite is frequently found (Type 2 ore-zone
alteration). In some cases (e.g. Aljustrel and Gavião), a third type of ultraperipheral alteration has
been found (Type 3), characterized, among other features, by weak, Na-sericite bearing alteration
(Relvas et al., 1990; Relvas, 1991). Minor amounts of carbonate are often present. Locally, these
may become abundant.
Stockwork zonation is present at two scales: megascopically it is clear that stockwork rock
(chloritic) predominates largely in the core of the alteration pipe, and is enveloped by a relatively
well defined halo of outer stockwork rocks (sericitic) before feldspar-bearing rocks are found
(Type 3, or no ore-zone alteration). At the scale of individual sulfide-rich veins chlorite-quartz
selvedges are surrounded by sericite-quartz rock which sometimes grades into rock unaffected by
Introduction to the IPB SEG Neves Corvo Field Conference 1997
16
ore zone alteration. When this happens, regional alteration types are found, clearly as relics in the
stockwork, implying that regional alteration predates stockwork formation. From the periphery to
the core of the stockwork, original volcanic textures are progressively obliterated by corrosion of
the original minerals and comcomitant precipitation of alteration phases. Stockwork alteration
extends laterally beyond the limits of the sulfide orebodies, and thus can be used as an ore guide
in exploration.
In some instances, hanging wall alteration has been described, such as above the Salgadinho
deposit (Plimer and Carvalho, 1982), and above Feitais (Barriga, 1983; Barriga & Fyfe, 1988; see
Silva et al., this volume). The presence of this type of alteration indicates that hydrothermal
activity persisted after deposition of the immediate hanging wall rocks. These may include not
only volcanic rocks but also shales, phyllites, tuffites, cherts and jaspers. Hanging wall alteration
may be mineralogically similar to stockwork alteration (especially in volcanic rocks), but can also
consist of manganese enrichment (oxides or carbonates).
8.
Isotope geochemistryMany isotopic studies have been carried out in relation with the IPB mineral deposits.
Sulphur isotopic studies (e.g. Arnold et al., 1977; Munhá and Kerrich, 1981; Mitsuno et al., 1988;
Kase et al., 1990; Yamamoto et al., 1993) have been recently summarized by Carvalho et al.
(1997), who have showed that these data fit the trend of sulfur isotope ratios in massive sulfide
deposits and coeval marine sulfate deposits noted on a global scale by Sangster (1968).
Furthermore, the data also suggest variable degrees if involvement of bacteriogenic sulfur in the
generation of the sulfides.
Oxygen and hydrogen isotopic studies have been undertaken in several areas and deposits in
Portugal, and in the Cerro Colorado stockwork in Spain (Barriga and Kerrich, 1984; Munhá et al.,
1986). These data are interpreted as meaning that mineralizing fluids in the IPB were mostly
derived from sea water, perhaps with small contributions of fluids derived from other reservoirs
(magmatic, metamorphic), although these are not required by the isotopic data. Massive sulfide
formation temperatures may have spanned 200-270ºC.
Lead isotope composition studies on massive sulfides have been reported by Marcoux et al.
(1992), Leistel et al. (1994) and Marcoux (1997). These authors concluded that the isotopic
compositions of massive and stockwork ores, excluding Neves Corvo, are fairly similar and very
SEG Neves Corvo Field Conference 1997 Introduction to the IPB
17
17
homogeneous along the belt, indicating that most of the ore lead was derived from the same
continental crust environment as the accompanying volcanic rocks. Neves Corvo is the only IPB
orebody that has a heterogeneous isotopic composition, including highly radiogenic stanniferous
ore with
206Pb/204Pb>18.40 in cassiterites, implying either a more complex ore forming process orthe inclusion of traces of U in the cassiterite crystal structure.
9.
Concluding StatementThe sea water convective model for massive sulfide generation is firmly established in the
IPB. In some deposits containing exceptional ores, especially Neves Corvo, a significant
magmatic fluid contribution may be indicated. Several lines of evidence also suggest that variable
proportions of the massive sulfides may have precipitated slightly below the paleo sea floor,
protected from direct contact with basinal, unmodified sea water. Carvalho et al. (1997) have
recently summarized these and other genetic aspects of the IPB ores. Some of the models are
controversial, especially in detail, but there can be no question that the IPB is a province where
the variables conducive to VMS generation were matched with very unusual efficiency. As
proposed by those authors, the IPB deserves recognition as the type-reference VMS province for
deposits hosted in bimodal siliciclastic settings.
Acknowledgments
We wish to thank all the authors who participated in the Guidebook for their efforts to
comply with the requests of the reviewers and/or editors. The reviewers are also deeply thanked
for their hard work with the manuscripts. Very special thanks to Prof. António Mateus
(GeoFCUL), whose technical assistance and nearly unlimited availability were essential for the
preparation of most of the figures, including redrafting many of them, as well as for assembling
the text in its final version.
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