Economic Geology; January 2005; v. 100; no. 1;
p. 63-86; DOI: 10.2113/100.1.0063
© 2005 Society of Economic Geologists
Ore-Forming Processes in Irish-Type Carbonate-Hosted Zn-Pb Deposits: Evidence from Mineralogy, Chemistry, and Isotopic Composition of Sulfides at the Lisheen Mine
J. J. Wilkinson
and
S. L. Eyre*
Department of Earth Science and Engineering, Royal School of Mines, Imperial
College London, Exhibition Road, London SW7 2AZ, United Kingdom
A. J. Boyce
Scottish Universities Environmental Research Centre, East Kilbride, Glasgow
G75 0QF, Scotland
Corresponding author: e-mail, j.wilkinson{at}imperial.ac.uk
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Abstract
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Lisheen is a strata-bound zinc-lead deposit formed during the Mississippian
by replacement of hydrothermally dolomitized, grossly stratiform breccia bodies
located near the base of the Carboniferous Waulsortian Limestone. It represents
one of a number of carbonate-hosted massive sulfide ore deposits in the Irish
ore field that, due to several unique features, have been classified as Irish
type.
Disseminated pyrite occurs in preore dolomite and around the margins of
preore dolomite clasts within dolomite breccias. Early fine-grained sphalerite-pyrite
mineralization occurs as infill of intergranular dolomite porosity. Locally,
massive to semimassive iron sulfide is observed, mainly comprising pyrite with
lesser marcasite. A complex polymetallic sulfide assemblage typifies the main
ore stage, dominated by fine-grained disseminated, massive or colloform
sphalerite and galena, with minor pyrite, chalcopyrite, arsenopyrite, tennantite,
nickel- and cobalt-bearing minerals. Silver occurs in solid solution in
tennantite, galena, and sphalerite. Dolomite and barite dominate the gangue,
with lesser calcite. Main-stage mineralization involved the progressive
replacement of preexisting iron sulfides and the dolomite breccias, initially by
replacement of the breccia matrix and ultimately by replacement of clasts.
Coarse crystalline sphalerite and euhedral galena crystals are generally
restricted to fracture-fill mineralization or vugs within main ore-stage
assemblages where they occur with euhedral dolomite and calcite.
Barite intergrown with main ore-stage sulfides has
34S
values of 14.3 to 18.1 per mil, consistent with the derivation of sulfate from
coeval Carboniferous seawater. The
34S values for
sulfides range from 44.1 to +11.8 per mil, with a mean value of 13.7 per
mil, typical of the Irish ore deposits. The dominant low
34S
signature is considered to be the result of bacterial reduction of coeval
seawater sulfate. Extremely low
34S values, in the
range of 38 to 44 per mil, are only observed in preore disseminated
pyrite; such extreme fractionations are thought to be due to low bacterial
sulfate reduction rates coupled with oxidative cycles in near-sea floor pore
waters. Main ore-stage sulfides have
34S values in
the range of 4 to 18 per mil, with a mode of 10 per mil, consistent
with a typical bacterial fractionation from coeval seawater sulfate. Isotopic
equilibrium between cogenetic sulfides is not observed. The bacteriogenic sulfur
component was probably transported from bacterial colonies fringing the ore
system by low-temperature brines.
The
34S values of late ore-stage sulfides mainly
range from 20.2 to +12.0 per mil, with the majority having relatively high
values (mean = 3.0 ± 8.5
, 1
) interpreted as being due
to the presence of a hydrothermal sulfur component, leached from the lower
Paleozoic basement. For galena and sphalerite there is a general increase in
34S
values with depth in the system, with time, and with proximity to east-west
and northwest-trending faults. These relationships suggest that input of
hydrothermal sulfur from depth via fractures became increasingly important.
Hydrothermal sulfur appears to be more important at Lisheen than the other major
Irish deposits.
Galena lead isotope analyses gave average 206Pb/204Pb, 207Pb/204Pb,
and 208Pb/204Pb values of 18.183, 15.594, and 38.080,
respectively. These data do not correlate with ore-stage, galena texture or
34S.
The results are comparable to previous data from Lisheen and from Silvermines,
35 km to the west, implying a common lead source in the lower Paleozoic
basement.
The textural, mineral, chemical, and isotopic evidence suggests that
main-stage ore was precipitated as a consequence of rapid supersaturation,
caused by fluid mixing within the permeable dolomite breccias. This process
involved relatively high temperature (ca. 240°C), metal-bearing solutions
derived from a basement-equilibrated fluid reservoir (carrying Zn, Pb, Fe, Cd)
and shallow, saline (ca. 25 wt % NaCl equiv) formation waters rich in
bacteriogenic H2S. Minor metals (Cu, As, Ni, Co) are thought to have
been stripped from the footwall Old Red Sandstone during hydrothermal alteration
around fault conduits. The availability of abundant seawater sulfate, operation
of open-system bacterial sulfate reduction, and episodic availability of free
oxygen imply that ore formation cannot have occurred at significant depth below
the paleosea floor. Cessation of mineralization was due to a cut-off of the
sulfur-rich brine supply, possibly by deposition of impermeable hanging-wall
sediments. This process of ore formation is consistent with evidence from the
other economic Irish-type deposits in the ore field.
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Introduction
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The Lisheen deposit, situated in County Tipperary, Ireland (Fig. 1), is the
most recent of six carbonate-hosted Zn-Pb deposits to have been discovered in
the Irish ore field in the last 35 yr. Found in 1990 by a Chevron Mineral
Corporation-Ivernia West joint venture, the deposit began production in late
1999. It contained a total premining resource (undiluted) of 16.7 million metric
tons (Mt) of ore, grading 14.1 percent Zn and 2.4 percent Pb (weighted average
calculated from Fusciardi et al., 2003), together with approximately 16 percent
Fe and 26 g/t Ag (Elmes et al., 2000). The ore is hosted principally by
carbonate breccias near the base of the Mississippian (Courceyan) Waulsortian
Limestone. The deposit is the most significant of a number of mineralized
occurrences in the Rathdowney trend of the southern Midlands (Fig. 1) that
include the Galmoy deposit (Doyle et al., 1992), 10 km to the northeast.
Lisheen, together with the deposits of Galmoy, Navan, Tynagh, and Silvermines,
represents the deposit class known as "Irish-type" as redefined by
Wilkinson (2003).
Early studies at Lisheen (Hitzman et al., 1992; Earls, 1994; Shearley et al.,
1995, 1996) provided the initial geologic framework for the deposit. This work
showed that Lisheen has geologic affinities with the other Waulsortian-hosted
deposits of Galmoy and Silvermines (B and G zones). Mineralization in all three
deposits is hosted primarily by dolomite breccias, the so-called "black
matrix" or "rock matrix" breccias. Recently, Hitzman et al.
(2002) and Fusciardi et al. (2003) presented geologic descriptions of the
deposit and preliminary genetic models. Here we report the results of a detailed
petrological and geochemical study of the deposit, carried out as part of a
Ph.D. research project between 1994 and 1998 (Eyre, 1998). This study builds on
previous work and provides new insights into ore-forming processes at Lisheen.
In this paper, we concentrate on the mineralogy and chemistry of the sulfide
ore, together with sulfur and lead isotope evidence for the sources of metals
and sulfur in the deposit. The nature and causes of spatial and temporal
variations in mineral chemistry and isotopic systematics are considered and
compared with data from other deposits in the ore field. The geochemical, fluid
inclusion, and isotopic studies of carbonate alteration and fluid evolution in
the deposit will be presented elsewhere.
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Geologic Setting
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The Irish deposits are hosted by a Lower Carboniferous marine transgressive
sequence that conformably overlies a terrigenous clastic red-bed succession (Old
Red Sandstone) of Devonian-Carboniferous age. This lies unconformably on a
peneplained basement of Silurian graywackes, siltstones, shales, and volcanic
rocks that were deformed and weakly metamorphosed in the Caledonian orogeny.
Mineralization is hosted by a variety of carbonate facies, primarily shallow
marine deposits of the Navan Group and the deeper water mud mounds of the
Waulsortian Limestone (Hitzman and Large, 1986; Phillips and Sevastopulo, 1986; Andrew, 1993; Hitzman, 1995; Hitzman and Beaty, 1996).
At Lisheen, the lower part of the Carboniferous marine sequence includes
carbonate-rich shales, siliciclastic sedimentary rocks, and argillaceous
bioclastic limestones (Lower Limestone Shale and Ballysteen Limestone; Philcox,
1983). The deposit is hosted by the Courceyan to early Chadian Waulsortian
Limestone, which comprises coalesced wackestone or packstone mud mounds flanked
by argillaceous bioclastic limestone (Philcox, 1983; Phillips and Sevastopulo,
1986). Growth fault control of sedimentation in the Courceyan-Chadian
(immediately prior to and during deposition of the Waulsortian Limestone) is
indicated by thickness variations across structures (Boyce et al., 1983; Hitzman
et al., 2002; Carboni et al., 2003; Fusciardi et al., 2003).
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Geology of the Lisheen Deposit
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Stratigraphy
The local stratigraphy in the Lisheen area is described by Hitzman et al.
(2002) and is summarized in Figure 2. The main host to mineralization is the
Waulsortian Limestone, dominantly comprising massive, pale-gray biomicrite,
together with green-gray and gray argillites, wavy laminated and stylonodular
micrites. The Waulsortian is commonly brecciated, particularly toward its base,
and it is these breccias that host the bulk of the ore. Although there is still
debate over the relative importance of sedimentary and hydrothermal controls on
the genesis of Waulsortian breccias (Hitzman and Beaty, 1996; Lee, 2002; Lee and
Wilkinson, 2002; Reed and Wallace, 2003; Wilkinson and Lee, 2003), their
significance is clear as the primary host rocks to ore in the south and west
Midlands. At Lisheen, synsedimentary breccias are present locally in the hanging
wall of normal faults (Hitzman et al., 2002; Carboni et al., 2003; Fusciardi et
al., 2003), but it is not clear whether these are always precursors for the
hydrothermally overprinted and mineralized dolomite breccias as has been
documented at Silvermines (Lee and Wilkinson, 2002).
Structure
The Lisheen deposit is localized by a left-stepping extensional fault array
(Hitzman et al., 1992, 2002; Shearley et al., 1995, 1996; Carboni et al., 2003;
Fusciardi et al., 2003) with three main east-northeasttrending strands: the
Killoran, Derryville, and Bog faults (Fig. 3). This fault zone continues across
the Tipperary-Kilkenny border to the northeast and is an important control on
mineralization at Galmoy (G fault).

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FIG. 3. Simplified structural map of the Lisheen deposit, showing main ore
zones and locations of drill holes sampled in the present study (Lisheen mine,
1998).
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A series of subordinate hanging-wall accommodation structures have also been
described. Hitzman et al. (1992) stated that west-northwesttrending
structures may have played a role in controlling mineralization in the Main
zone, although these faults are not shown in maps produced subsequent to more
extensive drilling (e.g., Hitzman and Beaty, 1996). Underground observations
have not identified the north-south structures shown in Hitzman et al. (2002) but the presence of numerous early east-northeast and northwest-trending
normal faults and late northwest-trending structures, important in controlling
present-day ground-water flow and also believed to control mineralization, has
been confirmed (Carboni et al., 2003; Fusciardi et al., 2003; see Fig. 3).
Facies variations across these structures indicate that fault activity began
during deposition of the Ballysteen Limestone in the Courceyan (J. Güven, pers.
commun., 2004).
Regional dolomitization
Several phases of dolomitization occur in the Lisheen area, the origin of
which are still debated (e.g., Wilkinson, 2003). The earliest is a fine- to
medium-grained, subhedral to euhedral gray dolomite that preferentially replaces
micritic components of the precursor Waulsortian Limestone (D1a).
This is partially recrystallized to and/or postdated by a coarse white planar to
weakly nonplanar dolomite (D1b) that preferentially replaces coarser
crystalline components of the Waulsortian, such as early marine calcite cements
in stromatactis cavities and bioclasts. Together, these phases form what has
been described as the "regional dolomite" that occurs throughout much
of the Waulsortian in southeast Ireland (Hitzman et al., 1998).
In the Lisheen area, the entire Waulsortian Complex, as well as relatively
nonargillaceous beds within the lowermost part of the overlying Crosspatrick
Formation, are dolomitized (Shearley et al., 1996). Regional dolomite occurs on
both the hanging-wall and footwall sides of the main Killoran and Derryville
faults (Hitzman and Shearley, 1991, unpub. technical report for Chevron Mineral
Corporation of Ireland, Intercompany Technical Group on Carbonates Seminar
LN91000514). In the northern part of the Rathdowney trend and along the margin
of the Leinster massif, dolomitization of this type has been observed locally to
extend higher in the stratigraphy, into the Aghmacart Formation. However,
dolomite has not been observed in the Arundian-age upper portion of the
Aghmacart Formation (Sheridan, 1977). The Rathdowney trend essentially marks the
northwest limit of pervasively dolomitized Waulsortian, with the Lisheen and
Galmoy deposits located just to the southeast of the dolomite front (Hitzman and
Beaty, 1996).
The most recent studies conclude that D1a formed during early
seawater diagenesis but later underwent neomorphic recrystallization (Wright et
al., 1999, 2000; Gregg et al., 2001). D1b is thought to have
developed in response to the onset of extensive fault-controlled hydrothermal
circulation in the late Courceyan-Chadian (Wilkinson, 2003). The regional
dolomite plays a pivotal role in arguments concerning deposit genesis because it
is considered to predate ore formation at Lisheen and Galmoy (Doyle et al.,
1992; Shearley et al., 1995; Eyre, 1998; Hitzman et al., 2002; Wilkinson et al.,
2003), thereby providing a maximum limit for the age of mineralization.
Hydrothermal dolomitization
A weakly developed, dark-gray dolomite of uncertain genesis forms the first
localized alteration phase at Lisheen (Hitzman et al., 1992). The first
well-developed dolomite of inferred hydrothermal origin (D2) forms
the matrix of the grossly stratiform, wedge-shaped breccia bodies ("black
matrix breccias") that occur near the base of the Waulsortian Limestone
(Fig. 4). The term "matrix" is used here in a general sense to mean
the material surrounding breccia clasts, rather than implying a specific origin
for this material since its origin is uncertain. At Lisheen, it is not clear
whether the matrix dolomite is (1) merely a replacement of the precursor
dolomitized limestone, (2) a true cement to breccia clasts, or (3) predominantly
a replacement of an earlier (synsedimentary) breccia matrix, as has been shown
to be the case in the Silvermines district (Lee and Wilkinson, 2002). It could
have formed from a combination of these processes (Hitzman et al., 2002). Fluid
inclusion data from the Tynagh basin have shown that the black dolomite commonly
observed associated with mineralization in the Irish ore field is likely to be a
characteristic product of fluid mixing (Wilkinson and Earls, 2000), probably
forming ahead of sulfides in a prograding reaction front (Hitzman et al., 2002; Lee and Wilkinson, 2002; Wilkinson et al., 2003).

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FIG. 4. North-south cross section through the Derryville zone, showing major
lithological units and location of main ore lens (Lisheen mine, 1998).
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The matrix dolomite is extremely fine grained, with planar subhedral to
euhedral morphology. Under the microscope, unmineralized and weakly mineralized
examples display high intergranular porosity (>5 vol %) and clast margins are
diffuse, showing clear evidence of recrystallization. The clasts are angular to
subrounded and range from tens of centimeters (though this may be an
underestimate due to the limitation imposed by core observations) down to
microscopic size. In the latter case, it becomes difficult to distinguish
precursor regional dolomite clast material from the later hydrothermal matrix
dolomite. Although polymictic breccia intervals occur from the lower half of the
Waulsortian to the lower Crosspatrick Formation at Lisheen (Hitzman et al.,
2002; Carboni et al., 2003; see Fig. 2), the breccias are normally dominated by
regionally dolomitized Waulsortian micrite. Preore sulfides either occupy
intergranular porosity or replace the matrix dolomite (Hitzman et al., 1992,
2002; Eyre, 1998). Ore-stage sulfides replace both the matrix and, ultimately,
also the clasts in the breccias (Shearley et al., 1996; Eyre, 1998). The matrix
dolomite at Lisheen is nonstoichiometric (being markedly enriched in Ca over Mg;
Eyre, 1998), making it much more susceptible to recrystallization and
replacement (Tucker and Wright, 1990).
Crackle breccias and stockworks cemented by medium- to coarse-grained white,
planar or weakly nonplanar variably ferroan dolomite (D3), commonly
referred to as "white matrix breccias," form a broad halo to the D2
dolomite breccias and are developed through much of the thickness of the
Waulsortian. These are comparable to the "crystalline dolomite
breccias" at Galmoy (Doyle et al., 1992). The relative timing of these
breccias is uncertain as they tend to occur above and/or lateral to D2
dolomite breccias (Hitzman et al., 2002), such that crosscutting relationships
are rarely observed. Shearley et al. (1996) inferred a post-D2
timing, but the local presence of both crystalline white dolomite in D2
breccia clasts and black dolomite in D3 dolomite breccias (also
observed at Silvermines; Lee et al., 2001; Lee and Wilkinson, 2002) implies a
broadly contemporaneous origin (also see Fusciardi et al., 2003). The textural
differences are believed to result from the mode of formation; black dolomite
precipitated rapidly during fluid mixing, whereas white dolomite crystallized
from a single hydrothermal fluid (Earls and Wilkinson, 2000; Wilkinson, 2003).
The dolomite breccias are crosscut by generally steeply dipping veins of
ferroan dolomite, dolomite (D4), and calcite (C4). These
phases also fill residual vuggy porosity within earlier dolomite generations.
The veins typically display symmetrical drusy crystal growth and may be
composite. They also commonly contain sulfides.
A late-stage, distinctive pink dolomite (D5) crosscuts and
aggressively dissolves all previous dolomite and/or sulfide generations and is
often coprecipitated with minor pyrite and/or chalcopyrite (Eyre, 1998; Hitzman
et al., 2002; Fusciardi et al., 2003). This is similar to late pink dolomite
observed elsewhere in the Midlands (e.g., Boast et al., 1981; Wilkinson, 2003).
Sometimes, residual porosity in this dolomite is filled by a white, blocky
calcite (C6).
Mineralization
Mineralization at Lisheen occurs within 30 m of the base of the Waulsortian,
forming single and locally multiple, generally stratiform, sulfide lenses
separated by D2 dolomite breccias (Fig. 4). The orebodies comprise
texturally complex, polymetallic massive sulfide, displaying both gradational
and sharp, planar or undulating contacts with the enclosing breccias. Sometimes,
postore stylolites are developed along these contacts. Sulfides are also present
in the Lisduff Oolite Member (Fig. 2), predominantly in the footwall but also in
the hanging wall of the Killoran and Derryville faults (Eyre, 1998; Hitzman et
al., 2002; Fusciardi et al., 2003). The Lisduff Oolite is much less extensively
mineralized than the basal Waulsortian and only comprises a minor proportion of
the total resource.
Four main ore zones have been defined: Main, North, Derryville, and Bog (Fig.
3). The Main zone forms the largest orebody, followed by Derryville, North, and
the Bog zone. Detail on metal zoning patterns in the four zones is available in
Hitzman et al. (2002) and Fusciardi et al. (2003).
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Methodology
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Textural and petrographic relationships of sulfides were determined by the
detailed study of more than 200 polished blocks and thin sections in reflected
light and under the scanning electron microscope (SEM). This work was based only
on drill core samples collected between 1994 and 1997, prior to underground
exposures becoming available for study. Representative drill core samples
covering the spectrum of ore stages, mineralization styles, and a range of
lateral and vertical positions within the four main ore zones (Fig. 3) were
collected in order to evaluate temporal and spatial variations in sulfide
mineralogy and sulfur isotope composition. Quantitative analysis of sulfides
using the microprobe was carried out mainly on the ore-stage mineralization to
determine the temporal and spatial distribution of trace elements, particularly
in relation to putative hydrothermal feeder structures. Analyses were performed
using a Cameca SX50 wavelength dispersive electron microprobe at the Natural
History Museum, London. A summary of results is presented in Table 1 and full
results are available from the author on request.
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TABLE 1 TABLE 1. Summary of Sulfide Compositions (wt %) from the Lisheen Deposit Determined by Microprobe Analysis
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Sulfur isotope analysis
Standard techniques were employed for determining sulfur isotope compositions
of both sulfides and barite. Samples of individual mineral grains (510 mg)
representing different stages of the paragenesis were drilled from split core
using a fine diamond-tipped drill. Separation of individual (submillimeter)
growth zones within sulfides was not possible so the data record the average
sulfur isotope composition of specific sulfide generations.
Sulfur was extracted as SO2 from sulfides by fusing samples under
vacuum at 1,076°C in a Cu2O (200-mg) matrix (Robinson and Kusakabe,
1975). Sulfur was extracted as SO2 from sulfates following the method
of Coleman and Moore (1978) and analyzed on a VG SIRA II mass spectrometer to
obtain values of
66SO2, which were
converted to
34S. Standard correction factors were
then applied (e.g., Craig, 1957). Results are given in conventional
34S
notation relative to the Vienna Cañon Diablo troilite standard (V-CDT) and are
summarized in Table 2 and given in full in the Appendix. Reproducibility based
on full replicate analyses of internal laboratory standards was ±0.2 per mil (1
).
Repeat analyses on duplicate splits were carried out for some samples (see
Appendix), with all but three replicates being within 1 per mil.
Lead isotope analysis
Galena samples for lead isotope analysis were drilled from core specimens.
Approximately 2 to 5µg of galena was dissolved in an excess of 6M
HCl. These solutions were pipetted directly onto a single rhenium filament using
a standard lead loading technique with phosphoric acid and silica gel. The 206Pb/204Pb,
207Pb/204Pb, and 208Pb/204Pb ratios
were measured on a VG 54E mass spectrometer. The results were normalized to the
NBS 981 international standard and corrected for instrumental mass fractionation
(see Table 3).
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Ore Mineralogy and Paragenesis
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Sphalerite and galena are the principal ore minerals in a relatively simple
mineral assemblage that also contains abundant iron sulfides, including both
marcasite and pyrite. Chalcopyrite, arsenopyrite, bornite, and
tetrahedrite-tennantite, Pb-Sb sulfosalts, such as boulangerite (Pb5Sb4S11),
and Pb-As sulfosalts including jordanite (Pb14As6S23)
are present in minor amounts. Hitzman et al. (2002) also reported the presence
of gratonite, seligmannite, and gersdorffite, and Fusciardi et al. (2003) noted
the local presence of cobaltite, niccolite, pararammelsbergite, bournonite, and
ullmannite.
Based on the broad textural and mineralogical associations observed within
the deposit, mineralization has been classified into four stages: (1) preore
stage, (2) main ore stage, (3) late ore stage, and (4) postore stage (Fig. 5).

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FIG. 5. Summary paragenesis for the Lisheen deposit (after Eyre, 1998). Width
of bar corresponds to relative abundance; bars for sulfides are shown hatched
for clarity.
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Preore stage
Minor disseminated pyrite occurs in preore D1a dolomite and around
the margins of preore D1a/D1b dolomite clasts within the D2
dolomite breccias (Fig. 6a). This pyrite contains up to 0.79 wt percent As.
There is intergranular porosity infilling in D2 dolomite by early,
fine-grained sphalerite and pyrite, with pyrite occurring interstitial to
sphalerite. The pyrite is granular in appearance and is composed of
polycrystalline aggregates of anhedral to euhedral crystals a few microns in
size. This is overgrown by large, euhedral, equant pyrite grains with
approximately 120° interfacial angles, often enclosing aggregates of early,
fine-grained, noncolloform sphalerite. The first significant zinc mineralization
comprises a very fine crystalline, locally colloform, pale pink-brown sphalerite
(Fig. 6b). This sphalerite occurs mainly in the D2 dolomite matrix,
primarily within intergranular porosity but also as a replacement of matrix
crystals where it is better developed.

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FIG. 6. Core photographs and reflected light photomicrographs of preore-stage
samples. (a). Preore-stage pyrite preferentially replacing the matrix of typical
black dolomite matrix breccia. Sample LK262/153.6m, Derryville zone. (b).
Pale-brown early sphalerite preferentially replacing matrix of dolomite breccia.
Sample LK121-189.3m, Main zone. (c). Preore-stage colloform pyrite with minor
carbonate and sphalerite inclusions overgrown by subhedral pyrite (py) and
marcasite (ma). Sample LK420/190.7m, Derryville zone. (d). Fine-grained granular
pyrite (py) pseudomorphous after barite laths. Timing of euhedral pyrite
uncertain. Subhedral-anhedral sphalerite (sp) overgrows and replaces pyrite.
Sample LK262/162.1m, Derryville zone. (e). Massive sulfide sample showing
colloform banding. Preore-stage fine-grained pyrite-marcasite (py-ma) with
sphalerite-rich outer zone is overgrown by pyrite-marcasite band, itself
succeeded and partly replaced by ore-stage sphalerite (sp), dolomite (dol), and
euhedral galena (gn). Sample LK394/164.3m, Derryville zone (Derryville fault).
(f). Preore-stage massive pyrite (py) and marcasite (ma) that has undergone
cataclasis and cementation by dolomite (dol) and sphalerite (sp). Sample
LK262/159.1m, Derryville zone.
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The most extensive iron sulfide mineralization postdates the earliest
noncolloform and weakly colloform pink-brown sphalerite but predates the main
sphalerite-galena ore stage. Pyrite is the earliest and dominant iron sulfide
and is overgrown by pyrite-marcasite growth bands, with marcasite becoming more
abundant through time (also observed by Hitzman et al., 2002; Fig. 6c). Small
pyrite spheroids (110 µm diam) probably acted as nuclei for
pyrite growth, leading to the development of colloform banded pyrite, a
significant textural component of the massive iron sulfide. Pyrite framboids are
observed locally and tend to occur in isolation or in small clusters,
particularly in samples close to the major east-westtrending faults. They are
commonly overgrown by massive pyrite. Good examples of pyrite replacement
textures exist, such as the pseudomorphous replacement of elongate laths of
barite by fine-grained granular pyrite and subhedral pyrite-marcasite
intergrowths (Fig. 6d). Pyrite also locally replaces ooids in the Lisduff Oolite
Member, with the preservation of relict ooid textures.
Marcasite occurs in colloform masses, elongate radiating laths intergrown
with pyrite, and as coarse subhedral grains. Sphalerite, galena, and dolomite
locally occur as inclusions within the banded iron sulfides, either in discrete
layers or as isolated crystals along particular iron sulfide growth bands (Fig.
6e). Galena commonly occurs as small spheres within massive iron sulfide.
Sulfides displaying radial coxcomb textures are generally uncommon but are well
developed in the Lisduff Oolite Member adjacent to the main fault zone.
Cataclastic textures in pyrite and marcasite are common near to major faults
in the Main and Derryville zones. There is infilling and partial replacement of
pyrite along fractures by sphalerite and dolomite (Fig. 6f) and also by
ore-stage galena.
Main ore stage
A complex polymetallic sulfide assemblage characterizes the main ore stage,
dominated by sphalerite and galena, with minor pyrite, chalcopyrite,
arsenopyrite, tennantite, dolomite, and barite. Coprecipitation of some phases
is suggested by the presence of mutual growth boundaries, although replacement
of one sulfide by another is also common. No consistent paragenetic sequence can
be defined and the assemblage appears to be the product of multiple overprinting
and recrystallization events. Sulfides of the main ore stage often replace early
iron sulfides (Fig. 7a) and overprint the dolomite breccias, preferentially
replacing the D2 dolomite matrix and ultimately also D1a
clasts (Fig. 7b). This sequence of progressive replacement can be clearly traced
laterally into the ore from essentially pristine, unmineralized breccias.
Apparently brecciated massive sulfide pseudomorphs may in fact represent
preexisting dolomite breccia textures (Fig. 7b), although rebrecciation in situ
during intense mineralization close to the main fault zones is also likely.

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FIG. 7. Core photographs and reflected light photomicrographs of main
ore-stage samples. (a). Massive fine-grained pyrite in gray Waulsortian micrite
(m), crosscut and replaced by sphalerite (sp) and galena (gn) in white dolomite
stockwork. Sample LK121/190.2m, Main zone. (b). Complex massive sulfide with
pyrite (py) intergrown with and replaced by galena (gn) and pale-brown
sphalerite (sp). Note apparent breccia texture (replaced dolomite breccia?).
Sample LK262/159.85m, Derryville zone. (c). Colloform sphalerite containing thin
bands of fine-grained pyrite and occasional botryoidal pyrite intergrown with
dolomite and fine-grained, zinc-rich (?geopetal) carbonate. Sample
LK262/159.85m, Derryville zone. (d). Pyrite (py) and sphalerite (sp)
incorporated in dolomite (dol) euhedra along growth surfaces and overgrown by
apparently homogeneous colloform sphalerite. Sample LK416/193.6m, Derryville
zone. (e). Selective replacement of foraminifera (Endothyrid). Sphalerite (sp)
preferentially replaces chamber walls with chambers filled by galena (gn) and
carbonate gangue (c), the whole surrounded by pyrite (py). An unidentified Fe-As
sulfide (u) with minor Ni, Co, and In forms a thin layer inside the microfossil.
Sample LK137/134.9m, Derryville zone (sub-Waulsortian, footwall of Derryville
fault). (f). Mixed ore-stage sulfide assemblage comprising intergrown euhedral
pyrite (py) and galena (gn), together with sphalerite (sp), probably
pseudomorphous after barite laths. Sample LK325/146.2m, Derryville zone. (g).
Selective replacement of ooid by galena (gn), surrounded and partly replaced by
sphalerite (sp) and minor pyrite (py). Galena replacement may postdate plastic
deformation of ooid reflected by oval shape and curviplanar contacts that
parallel distorted laminae (upper right). No replaced stylolites truncating
laminae, or fractured, or spalled laminae are observed indicating replacement
preceded mechanical compaction, or that mechanical compaction did not occur.
Sample LK394/164.3m, Derryville zone (Derryville fault). (h). Symmetrical
vug-fill sulfides comprising sphalerite (sp) intergrown with laminated and/or
colloform pyrite (py), with both being replaced from the margins inward by
subhedral galena (gn). Carbonate infilling in remaining space (c), with minor
dissolution of sphalerite along contact. Sample LK420/196.0m, Derryville zone.
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Main ore-stage sphalerite (Fig. 7c) is dominated by colloform aggregates
within mixed massive sulfides that display pale-cream to dark-brown color
banding. Galena and pyrite are common in the form of interbands or as discrete
crystals distributed along colloform layers in the sphalerite. Rhombic dolomite
with inclusions of early pyrite and sphalerite in growth zones also occurs in
colloform sphalerite (Fig. 7d), together with granular Zn-rich carbonate (Fig.
7c). Locally, the colloform sphalerite is broken and rotated.
Colloform sphalerite displays marked compositional variation (Table 1).
Individual samples may contain up to 40 distinct zones with significant
variations in Cd, Fe, and As concentrations (Fig. 8a). Cu (up to 0.11 wt %) is
also observed in some zones. The color of colloform sphalerite generally
correlates with mineral chemistry. For example, in a sample from the North zone,
gray-yellow bands contain up to 0.12 wt percent Fe (avg 0.06 wt % Fe), yellow
sphalerite contains up to 1.95 wt percent Fe (avg 0.37 wt % Fe), and
orange-brown layers contain up to 2.84 wt percent Fe (avg 0.63 wt % Fe). Other
elements may also be present such as Ag (up to 0.24 wt %), Cd (up to 0.47 wt %),
and As (up to 0.60 wt %). In two samples analyzed for Tl, highly variable
concentrations of up to 0.54 wt percent were found. However, there are no
statistically significant correlations between major or trace elements within
any of the colloform sphalerite analyzed.

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FIG. 8. Examples of variations in chemical composition of sphalerite as
determined by microprobe analyses (supplementary information on detection limits
and full data available from author on request). (a). Traverse across main
ore-stage color-banded colloform sphalerite (sample 262/159.1m, Derryville
zone). Note lack of correlation between element concentrations in individual
bands and occasional detectable Cu. (b). Traverse across late ore-stage finely
crystalline, red-amber color-zoned sphalerite (sample 471/210.4m, Main zone).
This sample is unusual in that it shows elevated Cd and Fe and shows a rare
correlation between Cd and Fe concentrations.
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Massive, fine-grained sphalerite is the second most common textural variety
after colloform sphalerite. This sphalerite is unzoned and is commonly
intergrown with pyrite and galena. Fe and Cd concentrations in this type of
sphalerite are lower than in colloform sphalerite, generally less than 0.5 wt
percent. Fine-grained, pale-gray sphalerite is nearly pure, with less than 0.5
wt percent impurities. Concentrations of up to 1.09 wt percent Cu are observed
in massive sphalerite in samples containing chalcopyrite from the footwall of
the Killoran fault in the Main zone, and low concentrations of Cu in crystalline
and colloform sphalerite are found in samples within 200 m of the main faults in
the Main, Derryville, and Bog zones. Elsewhere in Ireland, Cu-bearing sphalerite
has only been noted in the 3-1 lens at Navan (T. Thorpe, pers. commun., 2001)
and from the Lower G zone at Silvermines (Rhoden, 1960). Backscattered electron
imaging of Navan samples showed that Cu was present in solid solution, varied
significantly between adjacent growth zones (up to 1.30 wt %), and covaried with
Sb.
Replacement textures are common, such as the replacement of dolomite rhombs
by sphalerite and/or galena. Selective replacement of microfossils by sphalerite
and other sulfides is also observed locally (Fig. 7e), as has been reported at
Navan (Anderson et al., 1998). Sphalerite bow-tie textures in pyrite and
elongate laths of sphalerite in a mixed assemblage of pyrite and galena are
probably pseudomorphs after early barite or gypsum (Fig. 7f). Sphalerite also
occurs in small veinlets crosscutting and replacing pyrite (Fig. 7a) and galena.
Galena locally forms skeletal and dendritic growths, similar to those
described from Navan (Anderson et al., 1998). However, ore-stage galena is
predominantly coarsely crystalline or massive and replacive, as indicated by
caries textures, where galena replaces D2 dolomite, and by the
selective replacement of microfossils, early marine cements, and ooids (Fig.
7g). Galena is particularly abundant in zones proximal to the Killoran and
Derryville faults where it commonly contains inclusions of tennantite,
especially in the Main zone. Galena inclusions are also found within tennantite.
Boulangerite is commonly associated with galena.
Galena generally does not contain detectable concentrations of trace elements
(Table 1). Massive Waulsortian-hosted ore-stage galena locally contains elevated
Te (up to 0.27 wt %). Ag concentrations are usually below detection with the
exception of a few samples located proximal to faults that contain up to 0.19 wt
percent Ag. The phase that contains the highest concentrations of Ag in the
deposit is tennantite (see below).
Tennantite, chalcopyrite, arsenopyrite, and barite are most abundant near the
Killoran and Derryville faults, especially within the footwall Lisduff Oolite
Member. In this unit, tennantite commonly occurs as irregular inclusions in
galena, chalcopyrite, and sphalerite and is characterized by up to 3.91 wt
percent Zn, 5.63 wt percent Fe, and 0.32 wt percent Ag (Table 1). This contrasts
with tennantite in galena from the Waulsortian, which contains up to 8.55 wt
percent Zn, less Fe (<1.72 wt %), and less Ag (<0.24 wt %).
Short intervals of massive chalcopyrite are observed in drill core from the
footwall Lisduff Oolite of the Main zone and this contains up to 0.73 wt percent
As (avg 0.16 wt %). Minor chalcopyrite in the Bog zone Lisduff Oolite also
contains As, up to 0.11 wt percent (avg 0.07 wt %). Minor disseminated
arsenopyrite rhombs commonly occur in ore-stage galena, proximal to faults in
the Main and Derryville zones.
Main ore-stage pyrite generally comprises fine- to coarse-grained euhedra
intergrown with and locally interstitial to sphalerite and galena (e.g., Fig.
7f). Trace element concentrations in ore-stage pyrite are quite variable (Table
1). Arsenic concentrations range up to 5.21 wt percent and are significantly
higher than in preore pyrite. In As-rich samples, As correlates with Cu with
both showing a strong antipathetic relationship with Fe. Co and Ni are usually
below detection, with the notable exception of pyrite hosted by the Lisduff
Oolite Member in the footwall of the Killoran fault (up to 0.44 wt % Co and 1.92
wt % Ni). This pyrite also contains up to 3.34 wt percent As, which is strongly
correlated with Ni content. Elevated levels of Co and Ni are also observed in
the Ballysteen Limestone close to a secondary fault (F-291) in the hanging wall
of the Derryville fault (Fig. 3).
Barite was probably deposited both prior to and during the main period of
sulfide mineralization. Early sulfides, in particular pyrite and sphalerite, and
ore-stage sulfides (Fig. 7f) both replace barite. Later barite, associated with
complex mixed sulfide assemblages, crosscuts early pyrite-sphalerite
assemblages.
Late ore stage
Coarse (17 mm) crystalline sphalerite and euhedral galena crystals are
restricted to fracture-fill mineralization that crosscuts the main ore-stage
assemblages and to vugs within main-stage ore. These phases commonly predate or
were coprecipitated with D4 dolomite and C4 calcite veins
and vug-filling cements (Fig. 7h). Sphalerite was generally the last sulfide to
precipitate, commonly as rims on galena. Concentrically zoned pyrite grains
locally occur within these sphalerite rims and late, euhedral, fracture-filling
galena is sometimes observed.
Although texturally late, there is no evidence to suggest that these phases
are unrelated to the main ore stage and are therefore regarded as representing
waning hydrothermal activity, precipitated within residual porosity and tectonic
fractures.

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FIG. 9. Variation of cadmium and iron concentrations in sphalerite as a
function of textural type and location. Note that the vast majority of samples
are enriched in either cadmium or sphalerite, but not both, suggesting
substitution of one or other element into the same lattice site. Darker brown
sphalerite may be either Cd or Fe rich. The most Cd rich sphalerites are hosted
by the Lisduff Oolite; Fe-rich sphalerites are generally from within the main
fault zones. Most sphalerite in the main orebodies (within thick hatched line)
contains variable Fe and low Cd.
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The color of late-stage crystalline sphalerite is extremely variable, ranging
from pale yellow, through amber and red, to dark brown. The darkest sphalerite
is observed within the main fault zones (Fig. 9) and is dominant in
sub-Waulsortian veins, whereas yellow-amber sphalerite is prevalent in the
Waulsortian Limestone. In general, the crystalline sphalerite is richer in Fe
and contains less As (usually <1.0 wt %) than the main ore-stage colloform
sphalerite. Dark-brown crystalline sphalerite is usually more Fe rich (up to
4.96 wt % Fe) than yellow and amber sphalerite (generally <0.50 wt % Fe) and
is spatially associated with the main faults in the Derryville and Bog zones.
Cadmium concentrations are mainly uniform (0.20.4 wt %) within individual
crystalline sphalerite samples, in contrast to the colloform sphalerite.
However, Lisduff Oolite-hosted brown sphalerite from the Bog zone and pink
dolomite-hosted amber sphalerite from the west Main zone are anomalous with
elevated and variable Cd (0.652.48 and 0.261.14 wt %, respectively; Fig.
9). There is an antipathetic relationship between Fe and Cd in brown sphalerite,
whereas pale sphalerite is characterized by low concentrations of both elements
(Fig. 9). In a rare example of red sphalerite from the Main zone, Fe and Cd are
positively correlated (Fig. 8b). Silver concentrations in dark-brown sphalerite
are below detection but in the amber-yellow Waulsortian-hosted sphalerite Ag
concentrations up to 0.24 wt percent were recorded (avg 0.13 wt %). This
sphalerite is an important host for silver in the deposit.
Postore stage
Sulfides that occur in veins that clearly crosscut all previous stages are
defined as postore stage. At Lisheen, these sulfides are commonly associated
with pink saddle dolomite (D5), which is associated with extensive
dissolution of earlier carbonates and sulfides. This often leaves extensive
vuggy porosity and abundant pink dolomite typically correlates with poor ore
grades. Chalcopyrite and pyrite are the dominant sulfides, typically forming
encrustations on saddle dolomite crystals together with minor sphalerite and
galena. There is white blocky calcite (C6) infilling of residual
porosity in some samples.
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Sulfur and Lead Isotopes
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Sulfur Isotopes
A total of 119 analyses were carried out on 53 samples of sulfides (mainly
pyrite, sphalerite, and galena) and barite from the four main ore zones and from
all stages of the paragenesis (Table 2, Appendix).
The
34S values show a very wide range from 44.1
to +11.8 per mil, with a mean value of 13.7 per mil (Fig. 10a). Extremely low
34S values in the range of 38 to 44 per mil
are only observed in preore-stage disseminated pyrite (Fig. 10b), and pyrite in
general has lower values than the other sulfides, a feature typical of the
Irish-type deposits (e.g., Boyce, 1990; Anderson et al., 1998; Fallick et al.,
2001; Blakeman et al., 2002). Sphalerite and galena have similar ranges in
isotopic composition.
Main ore-stage sulfides always have negative
34S
values and fall dominantly within the range of 4 to 18 per mil, with a
mode of 10 per mil (Fig. 10b). Although the different ore zones have broadly
the same range in sulfur isotope compositions, there appears to be a slight
trend toward lower
34S values in the Derryville
zone compared to the Main zone (see below). Late ore-stage, vein-hosted, and
vug-filling sulfides have
34S values of 20.2 to
+12 per mil (excluding three anomalously low values in pyrite, sphalerite, and
galena in sample 451/139.1 m from the Bog zone; see Appendix) with the majority
having higher values (avg 3.0 ± 8.5
, 1
). Postore-stage
sulfides have
34S values mainly between 24 and
27 per mil, with one very low value at 37.9 per mil.

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FIG. 11. Variations in sulfur isotope composition of (a) sphalerite, (b)
galena, and (c) pyrite with depth and textural type. Outliers: BZ = Bog zone, DZ
= Derryville zone, MZ = Main zone, NZ = North zone. Samples from sub-Waulsortian
units are indicated. Sphalerite and galena show trends toward higher 34S
values with depth in the main ore zones and in sub-Waulsortian sulfides
consistent with input of an 34S-enriched sulfur component from depth.
Pyrite does not show such a trend in the main ore zones, suggesting that much of
it formed relatively early when the flux of hydrothermal sulfur from depth was
minor or absent.
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Sphalerite:
34S values of sphalerite (n =
41) fall within the range of 31.5 to +8.6 per mil (avg 7.9 ± 8.5
, 1
;
Fig. 10a). Ore-stage sphalerite (n = 25) has a narrow range of
34S
with a mean of 11.1 ± 3.8 per mil. There is a relationship between
sphalerite texture and
34S, with main ore-stage
colloform sphalerite having values consistently around 11 per mil, fine
crystalline sphalerite having a markedly wider range, and late ore-stage
crystalline sphalerite being the most heterogeneous of all (Fig. 11a).
Sphalerite shows a broad correlation between sulfur isotope composition and
sample depth. More negative
34S values occur in
shallower, Waulsortian-hosted sulfides, and higher
34S
values occur lower in the stratigraphy at the base of the Waulsortian and in the
Ballysteen Limestone Formation, including the Lisduff Oolite Member (Fig. 11a).
Variation in the sulfur isotope composition of sphalerite between the ore zones
is also observed. Sphalerite in the Main zone is relatively homogeneous in
sulfur isotope composition (Fig. 11a).
34S values
for sphalerite from the Derryville zone are slightly more negative and have a
wider range, and sphalerite from the Bog zone has the widest range of isotopic
compositions, albeit based on only four analyses (Fig. 11a).
Galena:
34S values of galena (n = 34) fall
within the range of 26.8 to +3.2 per mil (avg 11.7 ± 7.5 per mil, 1
;
Fig. 10a). Main ore-stage galena (n = 22), like sphalerite, has a narrow
range of
34S values with an average of 11.2 ±
3.3 per mil. Galena hosted by the Lisduff Oolite Member and intergrown with
fine-grained sphalerite has the highest
34S value
of +3.2 per mil. The lowest
34S value, 26.8 per
mil, was obtained from late- to postore-stage, vein-hosted galena associated
with tennantite at the base of Waulsortian-hosted massive sulfide in the
Derryville zone. Galena shows a clearly defined increase in
34S
values with depth and increasing heterogeneity from the Main to Derryville to
Bog zones (Fig. 11b), similar to sphalerite.
Pyrite:
34S values in pyrite (n = 37) range
from 44.1 to +11.8 per mil (avg 22.4 ± 13.3 per mil, 1
;
Fig. 10a). Disseminated preore-stage pyrite hosted by well-developed
hydrothermal D2 dolomite has the lowest
34S
values of 44.1 to 38.1 per mil. Main ore-stage pyrite (n = 24) has
a restricted range of sulfur isotope compositions but is still more variable
than sphalerite and galena and also has markedly lower values than the other
sulfides, with a mean of 20.1 ± 7.1 per mil. In the Waulsortian, no
correlation with depth is apparent (Fig. 11c). However, the highest
34S
value of +11.8 per mil is from relatively deep in the system, from a vein within
the upper calcarenite member of the Ballysteen Limestone Formation. Pyrite from
the Main zone has a more uniform isotopic composition than in the Derryville
zone, similar to the other main sulfides. Only two data from one drill hole in
the Bog zone were analyzed, and these are rather similar.
Chalcopyrite: Chalcopyrite samples, all from the Main zone and
representing the main ore stage, have typical ore-stage
34S
values ranging from 6.6 to 8.3 per mil (n = 3; Fig. 10a).
Barite: Barite intergrown with main ore-stage sulfides in the Derryville
zone (n = 2) has
34S values of +18.1 and
+17.2 per mil (repeat analyses on splits of a single sample, Fig. 10a). Barite
associated with main ore-stage sulfides in the Main zone (n = 2) has
lower values (although possibly sulfide contaminated) of +14.3 and +14.5 per
mil.
Lead isotopes
A preliminary study of four galena samples was carried out to provide
supplementary data on the lead isotope character of the deposit and to compare
the results with existing data from the Irish ore field. The samples analyzed
were from massive ore-stage galena and from vein-hosted, late- to postore-stage
galena (Table 3). The results are compared to data from other deposits in the
ore field in Figure 12.

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FIG. 12. 207Pb/204Pb vs. 206Pb/204Pb
plot, showing lead isotope compositions of galena from Lisheen (this study) with
error bars, compared to deposit array (encompasses average values for all Irish
deposits and prospects) and average Silvermines value (see Table 3). Lisheen
data fall close to the Silvermines average, implying a common lead source from
local lower Paleozoic rocks. Pb growth curve of Stacey and Kramers (1975) is
marked in 250 Ma increments for reference.
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Discussion
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Timing of mineralization
Mineralization within the D2 dolomite breccias postdates the
regional dolomite, which provides a potential maximum age limit for ore
formation. Assuming that formation of the regional dolomite is not diachronous
and is not an early diagenetic product, ore formation occurred no earlier than
the late Chadian (Shearley et al., 1995, 1996; Sevastopulo and Redmond, 1999;
Hitzman et al., 2002). However, if models of early seawater dolomitization are
correct (Gregg et al., 2001) then crosscutting relationships do not provide a
useful constraint on the timing of mineralization (Wilkinson, 2003; Wilkinson et
al., 2003).
Since there is good evidence that mineralization is localized by the Lisheen
fault array, the timing of fault movement provides some constraints on the
timing of mineralization. We consider that it is highly unlikely for extensive
fluid flow to exploit these potential fluid conduits except during periods of
active tectonism, since any fault-related permeability would be rapidly sealed
by hydrothermal precipitates in times of quiescence. Sediment thickness
variations imply that fault-controlled sedimentation in the area initiated
immediately prior to Waulsortian deposition, significantly earlier than
previously thought (Carboni et al., 2003; Fusciardi et al., 2003). Thus,
mineralization could have begun as early as the Courceyan (cf. Lee and
Wilkinson, 2002). The frequent observation of cataclastically deformed preore
sulfides in the Main and Derryville zones overprinted by main ore-stage
mineralization (e.g., Fig. 6f) indicates that ore formation did not entirely
postdate fault movements, as suggested by Sevastopulo and Redmond (1999),
Hitzman et al. (2002), and Carboni et al. (2003). Synsedimentary faulting
continued during deposition of the Crosspatrick Formation, suggesting that
mineralization could have persisted into, or initiated in, the Chadian
(Fusciardi et al., 2003).
The fact that ore-stage sulfides at Lisheen replace early marine cements and
regional dolomite indicates that the main phase of mineralization must have
occurred subsea-floor during or subsequent to early diagenesis of the
Waulsortian Limestone. However, it is probable that ore formation occurred close
in time and space to the oxic and/or suboxic transition in the connate
porewaters (Wilkinson et al., 2003). Furthermore, the sulfur isotope data
indicate that this must have occurred at a depth where the ore-forming system
remained open to seawater sulfate. These features, coupled with the evidence for
near-sea floor and exhalative mineralization in other Irish-type deposits
(Wilkinson et al., 2003), suggest that mineralization probably occurred within a
few tens of meters, and at most a few hundred meters below the sea floor, much
sooner during burial than suggested by Hitzman et al. (2002).
Source of lead
The limited new lead isotope data from Lisheen show no obvious correlation
between ore stage or galena texture and lead isotope composition and there is no
indication of a covariance between lead isotopes and
34S
values in galenas (Table 3), as has been observed in some Mississippi
Valley-type deposits (Sverjensky, 1981). This lead isotope homogeneity is
consistent with results from the other Irish deposits and suggests a
well-homogenized crustal reservoir. The data are comparable with those reported
for Lisheen by Hitzman et al. (1992) and are similar to results from
Silvermines, 35 km to the west (OKeeffe, 1986; Fig. 12). The similarity
between Lisheen and Silvermines implies a common lead source; the match between
deposit galenas and estimated composition of the lower Paleozoic sequence in the
southwest Midlands at the time of mineralization (Dixon et al., 1990) implicates
Silurian graywackes, siltstones, and grits of the Hollyford Formation. The lead
isotope data therefore support fluid-flow models involving deep basement
circulation and are inconsistent with fluid flow through and derivation of lead
from the Old Red Sandstone, as summarized by Everett et al. (2003).
Distribution and source of other metals
Petrographic and mineral chemical studies show that Cu-, As-, Co-, and
Ni-bearing phases are abundant close to the major faults and in sub-Waulsortian
mineralization, particularly within the Lisduff Oolite (also see Fusciardi et
al., 2003). Similarly, these elements are enriched (and covary) in other main
ore-stage phases (sphalerite, pyrite, chalcopyrite) in proximity to the major
structures. The co-occurrence of these elements in a range of phases, both as
major and minor constituents, suggests that they were enriched in the
hydrothermal fluids active during the main ore stage. The clear spatial
association with major east-west faults implies that these structures were
important conduits for fluids transporting these elements from depth. Intense
bleaching of the Old Red Sandstone is observed close to the main fault zones at
Lisheen (Mallon, 1997; Everett, 1999; Hitzman et al., 2002; Everett et al.,
2003), and results of acid leaching experiments on unaltered Old Red Sandstone
samples show that Ni and Co are readily liberated (C. Everett, pers. commun.,
2000). Therefore, it is suggested that Cu, As, Co, and Ni were stripped during
early, localized alteration of the sandstone footwall around fault conduits and
redeposited in ore-stage minerals at higher levels by buoyant hydrothermal
fluids.
Trace element substitutions in sphalerite appear to have been controlled by
different processes. Fe is generally enriched in vein sphalerite from close to
faults, particularly in the Derryville and Bog zones and in the sub-Waulsortian
stratigraphy. There is no obvious correlation with fluid inclusion
homogenization temperatures (Eyre, 1998), suggesting that temperature is not a
primary control on Fe content. Given the probability of high sulfur fugacity in
the upper parts of the system during ore formation (see below), it is suggested
that the Fe content of sphalerite is controlled by sulfur fugacity in an inverse
relationship (cf. Czamanske, 1974).
Cd concentrations in sphalerite are generally decoupled from Fe and show no
obvious systematic pattern in space or time. A weak correlation with sulfur
isotope composition (Fig. 13) suggests that Cd may be cotransported with
isotopically heavy sulfur (derived from depth; see below) and is favorably
partitioned into the first sphalerite precipitated in fluid conduits. There is
no evidence for liberation of Cd during alteration of the Old Red Sandstone,
therefore it is suggested that Cd is sourced, with Pb, from the lower Paleozoic
basement.

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FIG. 13. Range of cadmium concentrations in sphalerite samples (determined by
microprobe analysis) plotted against sulfur isotope composition. A weak positive
correlation exists, suggesting that cadmium is associated with the hydrothermal
sulfur component, both being derived from the lower Paleozoic basement.
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Sources of sulfur
Barite
34S values are comparable to results
reported by Hitzman and Beaty (1996) and are identical to Lower Carboniferous
seawater sulfate (Claypool et al., 1980). This suggests that barite
precipitation at Lisheen involved essentially unmodified Carboniferous marine
sulfate, as inferred for barite in all the other Irish deposits (
34S
= 1523
; Graham, 1970; Greig et al., 1971; Coomer and Robinson, 1976; Boast
et al., 1981; Caulfield et al., 1986; Anderson et al., 1998). The very low
solubility of barium in seawater excludes this as a source for Ba. Given that
barium is not present as a significant constituent of the host rocks, it can be