by Wayne Goodfellow and John Lydon
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There are 132 SEDEX (including Irish and BHT subtypes) deposits worldwide with known grade and tonnage, and of these, 50 have geological resources equal to or greater than 20 Mt. In Canada, there are 35 deposits, seven with measured geological resources of more than 20 Mt, including the Sullivan deposit with 162 Mt. Twelve Canadian deposits are past producers, the largest of which is the Sullivan deposit, which produced 149 Mt of 5.33 percent Zn and 5.64 percent Pb.
The morphology of SEDEX deposits is highly variable and includes mounds, lenses, and tabular or sheet-like bodies. Their internal architecture is controlled by the proximity of seafl oor sulphides to fl uid discharge vents. Vent-proximal deposits typically formed from buoyant hydrothermal fl uids, whereas vent-distal deposits formed from fl uids that are denser than seawater and pooled in bathymetric depressions that may be remote from seafl oor vents.
Most SEDEX deposits are hosted by organic-rich sedimentary rocks that were deposited in basins during periods in the Earth’s history when the oceans were stratifi ed with a lower anoxic and H2S-rich water column. In the Paleozoic Selwyn Basin, for example, there is a close temporal relationship between upward-increasing δ34S secular trends in sedimentary pyrite, anoxic laminated carbonaceous shales and cherts, and three major SEDEX forming events in the Late Cambrian, Early Silurian, and Late Devonian.
The typical basinal architecture of most SEDEX deposits is a continental rift basin with at least 2 to 5 km of syn-rift, coarse-grained, permeable clastics and related volcanic rocks and/or volcaniclastics overlain by post-rift relatively impermeable basinal shales or carbonates. Hydrothermal discharge to the seafl oor was commonly focused at the intersection of extensional and transform faults. There is close temporal and, in many cases, spatial association of SEDEX deposits with basaltic volcanic rocks, dykes, and sills. The low rigidity, permeability, and thermal conductivity of host sediments served to focus and prolong hydrothermal discharge at a restricted number of vent sites, thereby generating deposits that are an order of magnitude larger on average than VMS deposits.
SEDEX deposits most likely formed from oxidized and therefore H2S-poor fl uids generated in geopressured hydrothermal reservoirs within syn-rift clastic (and evaporitic) sediments sealed by fi ne-grained marine sediments. The large variability in the temperature, salinity, metal content, and redox conditions of SEDEX fl uids was controlled by a number of parameters including the local thermal regime, the redox state of the reservoir sediments, and the presence or absence of evaporates. Because most of the fl uids that formed SEDEX deposits were probably depleted in reduced S, an essential requirement for this deposit type is a suffi cient supply of reduced S at the site of deposition. In the case of well-bedded deposits that formed at the seafl oor, the most likely S source is bacteriogenic H2S generated in an ambient anoxic water column.
This synthesis of SEDEX deposits is intended as a synopsis of the major economic, geological, geochemical and genetic attributes of SEDEX deposits, with an emphasis on those that are considered important in mineral exploration. A great deal of the key attributes are based on research undertaken in the Selwyn Basin, Canada (e.g., Goodfellow, 2004; Goodfellow, 2007) and the Sullivan district, southeast B.C. (Höy et al., 2000; Lydon et al., 2000a; Lydon et al., 2007). This was augmented by major research programs on SEDEX deposits of the Northern Territories, Australia, by the Centre for Ore Deposits Research (CODES; e.g., Large et al., 1998; Bull and Rawlings, 1999) and on the Red Dog deposits, Brooks Range, Alaska by the U.S. Geological Survey (e.g., Kelley and Jennings, 2004; Young, 2004).
For a comprehensive analysis of this economically important deposit type, the reader is referred to reviews by Large (1981b), Goodfellow et al. (1993) and Leach et al. (2005).
Mineral Deposit Type
Sedimentary exhalative (SEDEX) deposits are typically tabular bodies composed predominantly of Zn, Pb, and Ag bound in sphalerite and galena that occur interbedded with iron sulphides and basinal sedimentary rocks, and that were deposited on the seafl oor and in associated sub-seafl oor vent complexes from hydrothermal fl uids vented into mostly reduced sedimentary basins in continental rifts.
Mineral Deposit Subtypes
Subtypes of SEDEX deposits include the Broken Hill type (BHT) and those that formed below but near the seafl oor (e.g., Irish-type deposits). The Irish type of SEDEX deposits (e.g., Hitzman and Beaty, 1997) is hosted predominantly by carbonate rocks and these deposits, either individually or collectively (district-wide), may show characteristics of both seafl oor deposition and epigenetic features typical of Mississippi Valley-type (MVT) deposits (e.g., Sangster, 1990; Paradis et al., 2007). Irish-type deposits are considered to have formed by ore-forming processes similar to those of SEDEX deposits, but because carbonate platforms are highly soluble in mildly acidic ore fl uids, the ores were also deposited in open space that commonly formed by hydrothermal karsting (e.g., dissolution voids, collapse breccias). BHT deposits (Beeson, 1991; Parr and Plimer, 1993; Walters, 1998) are characterized by high metamorphic grade, elevated base metal to S ratios, a spatial and temporal association with Fe-Si-Mn oxide exhalites, and bimodal felsic-mafi c volcanic/intrusive and fi ne- to coarse-grained, mostly clastic sedimentary host rocks.
It is generally recognized that, especially at the deposit scale, no matter the criteria used to defi ne a SEDEX deposit, there is a continuum of characteristics between SEDEX and VMS (volcanogenic massive sulphide) deposits on the one hand, and SEDEX and MVT deposits on the other hand. The distinction between the three classes of deposits is based not only on the typical physical, chemical, and geological attributes of member deposits and their respective geological environments, but also on genetic models for the class. Both SEDEX and MVT deposits occur within marine platforms of thick sedimentary basins and are thought to result from the migration of basinal metalliferous saline fl uids, whereas VMS deposits occur in submarine volcanic-sedimentary sequences and are formed from convective hydrothermal fl uids driven by, and/or magmatic fl uids from, a subvolcanic magma body. Both SEDEX and VMS deposits were formed by hydrothermal systems that vented fl uids onto the sea fl oor, so that the age difference between the ores and the immediate host rocks is by defi nition small. In contrast, MVT deposits formed in the subsurface and so the age difference between ores and host rocks can be much larger than for SEDEX deposits (Leach et al., 2001; Leach et al., 2005).
Associated Mineral Deposit-Types
SEDEX-associated deposits include MVT (Paradis et al., 2007) and stratiform barite deposits (Goodfellow, 2004). The MVT deposits occur in platformal carbonate sequences that are the shallow-water facies equivalent of basinal, typically fi ne-grained sediments that host SEDEX deposits. Although there is debate regarding the genetic link between SEDEX and MVT deposits, the overlap in timing and the compositional similarities suggests that these deposits formed from similar basinal metalliferous fl uids (Goodfellow, 1987; Sangster, 1990). The only major difference is that ore-forming fl uids vented at the seafl oor in the case of SEDEX deposits whereas most of the sulphide precipitation took place subsurface in the case of MVT deposits. The source of most of the reduced S in both deposit types is most likely bacterial reduced seawater sulphate (Goodfellow, 1987).
Summary
SEDEX deposits are an important resource for Zn and Pb (Table 1). In 2004, SEDEX deposits accounted for 38.8% and 65.1% of the western world’s Zn reserves and resources, respectively (Fig. 1; Hunt, 2006). By comparison, VMS and MVT deposits accounted for 30.2% and 15.3%, and 4.2% and 1.4%, of Zn reserves and resources, respectively. In addition, the percentage of SEDEX Zn reserves has shown a consistent increase over the past two decades. In 2004, SEDEX deposits also accounted for 32% of Zn production that was followed by VMS at 27%, Zn oxide at 12%, and MVT at 6%. The size (in tonnes of Pb + Zn metal) of SEDEX deposits is on average about an order of magnitude greater than that of VMS deposits (Goodfellow et al., 1993).
The bulk of the mineralization in most SEDEX deposits resides in the bedded ore facies. The ore minerals in this facies are commonly fi ne-grained and intergrown, which leads to low metal recoveries during ore benefi ciation. Although recrystallization of fi ne-grained sedimentary sulphides by metamorphism and/or by hydrothermal reworking in the vent complex produces coarser-grained ores from which higher recovery rates are obtained, these rates for SEDEX deposits are, on average, much lower than for VMS, MVT, and BHT deposits, the other major sources of Zn and Pb (Goodfellow et al., 1993).
Grade and tonnage Characteristics
There are 132 SEDEX including Irish and BHT deposits world wide with grade and tonnage fi gures (Fig,. 2 and Appendix 2, DVD), and of these, 50 have geological resources greater than 20 Mt (Table 1). In Canada, there are 35 deposits with known geological resources (Appendix 1, DVD), of which seven contain more than 20 Mt, including the Sullivan deposit with 161 Mt and the Howards Pass deposits estimated at 120 Mt (Table 2 and Fig. 2). Of the 35 Canadian deposits, 12 are past producers, the largest of which is the Sullivan deposit that produced 149 Mt of 5.33% Zn and 5.64% Pb (Table 3). The Howards Pass deposit is currently not economic, although it is currently undergoing major exploration and evaluation. Most SEDEX deposits in Canada occur in the Anvil, MacMillan Pass, and Howards Pass districts, Selwyn Basin; the Gataga district, Kechika Trough; the Sullivan district, Belt-Purcell; and the Duncan district, southern British Columbia (Fig. 3).
In order of endowment of SEDEX deposits globally, the major basins are: Mt. Isa-McArthur Basin (seven deposits totaling 112 Mt of Zn + Pb metal), Curnamona Craton (one deposit of 75 Mt Zn+Pb), Selwyn Basin (17 deposits totaling 55 Mt Zn+Pb), Brooks Range (three deposits totaling 40 Mt Zn+Pb), Namaqualand (four deposits totaling 30 Mt Zn+Pb), Rajasthan (fi ve deposits totaling 20 Mt Zn+Pb), Belt-Purcell Basin (one deposit totaling 19 Mt Zn+Pb), Irish Midlands (fi ve deposits totaling 15 Mt Zn+Pb), and Rhenish Basin (two deposits totaling 11 Mt Zn+Pb; Sangster and Hillary, 2000).
Singer (1995) defi ned giant deposits as the top 10 percentile and super-giants as the top one percentile in terms of metal content. Using these criteria, giant deposits contain more than 8 Mt of Pb+Zn metal. If the criteria are extended to total geological size, giant and super-giant SEDEX deposits contain more than 100 and 300 Mt of ore, respectively. Some obvious conclusions from Table 1 and Figure 4 are:
Metal grades are highly variable, with a mean of 0.97 wt. % Cu, 3.28 wt. % Pb, 6.76 wt. % Zn and 63 g/t Ag. Average geological resources are 34.78 Mt of sulphide and 3.165 Mt of Zn + Pb metal Fig. 5. Most of the production from SEDEX deposits in Canada came from the world-class Sullivan deposit in the Belt-Purcell basin, southeastern British Columbia, the Faro, Grum, and Vangorda deposits in the Selwyn Basin, Yukon, and the H.B. and Reeves-MacDonald deposits, southern British Columbia (Table 3).
Deposit morphology
The bulk of the ore is contained in a stratiform sulphide body that typically has a high aspect ratio (i.e., the ratio of the lateral extent of the body to its maximum stratigraphic thickness). Because most SEDEX deposits have an aspect ratio of 20 or more, the most common morphology is represented by sheets or tabular lenses of stratiform sulphides up to a few tens of metres in thickness and more than a km in length (Large, 1983). The Sullivan deposit in southern B.C.(Fig. 6), and the Tom and Jason deposits at MacMillan Pass, Yukon, are wedge-shaped and have a moderately high aspect ratio. The Howards Pass (Fig. 7) and Anniv deposits in the Howards Pass district, on the other hand, are saucer-shaped and taper gradually laterally for distances of several km. Unlike the vent-proximal Tom and Jason deposits (e.g.,Fig. 8A), the Howards Pass deposits (XY, Anniv, and OP) are probably not spatially associated with a hydrothermal seafl oor vent (e.g., Fig. 8B). The geometry of distal deposits is controlled by the basin morphology within which hydrothermal metalliferous fl uids formed brine pools similar to Atlantis II and Discovery deeps in the Red Sea (Zierenberg, 1990).
Deposit Architecture
Vent-proximal deposits are characterized by four distinct facies: 1. bedded sulphides, 2. vent complex, 3. sulphide stringer zone, and 4. distal hydrothermal sediments. Near the center of fl uid up-fl ow represented by the stringer zone, the bedded sulphides are characteristically infi lled, veined, and variable replaced by a higher-temperature mineral assemblage, producing the vent complex (Goodfellow et al., 1993). The distal hydrothermal sediments probably represent plume fallout that has been dispersed by bottom currents or alternatively clastic sulphides shed from sulphide mounds. Examples of deposits with zone-refi ned vent complexes include the Sullivan, Tom, Jason, and Rammelsberg deposits.
Vent-distal deposits, however, are typically weakly zoned, well bedded, and conform to the basin morphology (e.g., Fig. 8B). There is no evidence of the type of zone refi ning that accompanies veining, infi lling, and replacement of bedded sulphides by a typically higher-temperature assemblage and that characterizes vent-proximal deposits.
Textures and Mineralogy
The bedded facies in both distal and proximal deposits is composed of sulphide minerals, other hydrothermal products such as carbonates, chert, barite, and apatite, and non-hydrothermal clastic, chemical, and biogenic sedimentary rocks. The dominant sulphide mineral in most deposits is pyrite, although in some deposits (e.g., Sullivan and Mt. Isa), pyrrhotite is predominant. The main economic minerals are sphalerite and galena (e.g., Fig. 9A, Howards Pass deposit), although chalcopyrite is an economically important mineral in a few deposits (e.g., Rammelsberg; Hannak, 1981). The ratio of iron sulphides to base metal sulphides ranges from less than 1:1 (e.g., Red Dog; Moore et al., 1986) to greater than 5:1 (e.g., Sullivan; Hamilton et al., 1982). The relative proportion of non-sulphide hydrothermal components is similarly variable. Barite, when present, occurs in major amounts (i.e., more than 25% of the hydrothermal product) and is present in about 25% of Proterozoic and about 75% of Phanerozoic SEDEX deposits (Goodfellow et al., 1993). Silica, usually as chert, is ubiquitous in most stratiform ores and is in part hydrothermally derived.
The outer margins of the stratiform body, referred to as the distal facies, usually consist of bedded hydrothermal products that have no economic value, due to a decrease in the relative proportion of base metal sulphides with distance from the center of hydrothermal discharge (e.g., Sullivan horizon, Fig. 9C). The distal facies includes laminated pyrite and pyrrhotite, manganese, iron and calcium carbonates, iron oxides, barite, and phosphate. The contact between the bedded ore facies and the distal sedimentary facies is in most cases gradational and economically defined.
In contrast to the regularly layered appearance of the bedded ore facies, the vent complex is heterogeneous in nature and is typically composed of massive zones, replacement patches, irregular veins and/or disseminations of sulphides, carbonates, and silicates (mostly quartz; e.g., Fig. 9B, Tom vent complex). The mineral assemblage is dominated by pyrite, pyrrhotite, galena, sphalerite, ferroan carbonate, dolomite, quartz, tourmaline, and lesser muscovite, chlorite, chalcopyrite, arsenopyrite, and sulphosalt minerals. In deposits in which the vent complex has been well documented (e.g., Tom, Jason, and Sullivan), the contact between the stratabound vent complex and adjacent sedimentary-hydrothermal facies is a discordant replacement contact. The vent complex is formed by the reaction of upfl owing hydrothermal fl uids with hydrothermal and host sediment, which causes the replacement of the lower-temperature sedimentary minerals by higher-temperature vent assemblages (Turner, 1990; Kelley et al., 2004).
The feeder zone underlying vent complexes is discordant and composed of sulphide, carbonate, and silica veins, impregnations, and replacements that intersects the footwall sedimentary sequence (e.g., Fig. 9D, Sullivan deposit; Fig. 9E, Red Dog deposit). The feeder zone at many deposits appears to be rooted in a synsedimentary fault zone, and fault-scarp breccias, debris flows, and abrupt facies changes associated with SEDEX deposits indicate that the fault was active before, during, and/or after sulphide formation (e.g., Jason and HYC deposits; Turner, 1990; Large and McGoldrick, 1998).
Host Rocks
Most SEDEX deposits are hosted by basinal marine, reduced facies, fi ne-grained sedimentary rocks that consist mostly of carbonaceous chert and shale. These sedimentary rocks generally represent pelagic and hemipelagic sediments. In some deposits (e.g., Sullivan), pelagic and/or hemipelagic sedimentary rocks are interbedded with basinwide turbiditic siltstones and sandstones, and locally derived coarse-grained clastic sediments shed off uplifted blocks during extensional tectonism. In the case of the Irish-type deposits, the dominant lithologies are limestone and dolomite. BHT deposits are hosted by a bimodal volcanic and clastic sedimentary sequence that is commonly metamorphosed to amphibolite-granulite facies, as at Broken Hill, Australia.
Ore Composition
The main economic constituents of SEDEX ores are Zn, Pb, and Ag that occur primarily in sphalerite and galena in both the bedded ores and vent complex. Grades of Pb + Zn are commonly highest near the transition between the zone-refi ned vent complex and the laterally extensive bedded ore facies (e.g., Tom and Sullivan, Goodfellow and Rhodes, 1990; Lydon et al., 2000a). This increase in base metals and ore-associated elements (e.g., Hg, As, Sb) is caused by the leaching of these elements from the vent complex and reprecipitation in bedded facies adjacent to the vent complex. In a few deposits, such as Rammelsberg in Germany and Mount Isa in Australia, Cu is an important economic resource and is concentrated in what has been interpreted as the vent facies (Goodfellow et al., 1993). Other economically recoverable elements include Sn in the Sullivan deposit (Hauser and Hutchinson, 1983) and Au in deposits of the Anvil district (Jennings and Jilson, 1986) and Sullivan (Conly et al., 2000), although the Au content of SEDEX deposits is typically low (Emsbo, 2000).
In addition to the ore-forming elements, SEDEX deposits are enriched in a large suite of ore-associate elements that may include Fe, Mn, P, Ba, Ca, Mg, Hg, Cd, As, Sb, Se, Sn, In, Ga, Bi, Co, Ni, and Tl (e.g., Goodfellow, 1984; Goodfellow and Rhodes, 1990; Slack et al., 2004).
Textural, Mineralogical and Chemical Zonation
One of the most characteristic features of many SEDEX deposits is the radial zonation of hydrothermal textures, minerals, and elements about centers of hydrothermal fl uid discharge. This lateral zonation away from the center of fluid discharge is controlled mostly by zone refining in the vent complex and is typically accompanied by a decrease in the thickness of the stratiform body and the number and/ or thickness of individual beds of hydrothermal minerals (Goodfellow et al., 1993).
An increase in the Zn:Pb ratio away from the vent complex is the most pronounced and consistent feature of SEDEX deposits, and has been well documented for the Tom (Goodfellow and Rhodes, 1990), Jason (Turner, 1990), Cirque (Jefferson et al., 1983), Sullivan (Hamilton et al., 1982), and Red Dog (Moore et al., 1986) deposits. Other chemical zonation patterns include increases in Pb:Ag, Cu:Zn+Pb, Fe:Zn, Ba:Zn, and SiO2:Zn ratios away from the vent complex (e.g., Sullivan and Tom, Hamilton et al., 1982; Goodfellow, 2004).
The Tom deposit is a good example of a deposit that is highly zoned. The bedded ore facies sediments that overlie the fl uid discharge conduit are brecciated, veined, and variably replaced by silica, ferroan carbonate, and sulphides. The subsurface replacement processes have produced a marked textural, mineralogical, and chemical zonation from the core of the vent complex to the distal fringes (Goodfellow and Rhodes, 1990). At the margins of the vent complex, fi ne-grained low-temperature phases of the bedded ore facies (i.e., Fe-poor, cream sphalerite, galena, framboidal pyrite, barite, and chert) are replaced by coarser-grained, higher-temperature assemblages (i.e., coarsely crystalline, Fe-rich black sphalerite, and Hg-rich pink sphalerite, galena, siderite, quartz, pyrrhotite, chalcopyrite, arsenopyrite, and tetrahedrite). These mineralogical changes are refl ected by the systematic zonation of Zn, Pb, Cu, Cd, Hg, As, Sb, Ba, Fe, Mn, Ca, and CO2 within and about the vent complex, and an increase in Pb/Pb+Zn ratios towards the center of hydrothermal fl uid discharge (Goodfellow and Rhodes, 1990). Near the core of the vent complex, sedimentary barite has been completely replaced by ferroan carbonate minerals.
Alteration Textures, Mineralogy and Chemistry
Although many SEDEX deposits are closely associated with an underlying hydrothermal feeder zone, hydrothermal alteration has not been well documented and mapped at most deposits. Alteration minerals that have been reported for SEDEX deposits include quartz, muscovite, chlorite, ankerite, siderite, tourmaline, and sulphides. The sulphide content of alteration zones is typically low, but pyrite, pyrrhotite, galena, sphalerite, chalcopyrite, tetrahedrite, and arsenopyrite may be present.
Hydrothermal alteration associated with SEDEX deposits is commonly widespread and extends for hundreds of metres into the pre- and post-ore sedimentary sequence and up to several kilometres laterally from the deposit. For example, sericite alteration at Sullivan extends more than 200 m below the ore, approximately 4 km in an east–west direction along the Kimberley Fault, and about 6 km south along the Sullivan-North Star corridor (Fig. 10 from Turner et al., 2000). Large et al. (2000) have described a widespread Zn, Pb, and Tl halo that extends laterally from the McArthur River deposit along the pyritic black shale facies of the Barney Creek Formation for at least 15 km to the west, and hundreds of metres above and below the mineralized zone.
Hydrothermal alteration of the hangingwall sedimentary sequence has not been documented for most SEDEX deposits. Although post-ore hydrothermal sediments clearly show that hydrothermal fl uids continued to vent well after SEDEX formation, the paucity of post-ore hydrothermal alteration described in the literature may indicate that it is too subtle in most cases to be readily recognized. Perhaps the best documented example of post-ore hydrothermal alteration is the albite-chlorite-pyrite alteration of turbiditic sedimentary rocks overlying the Sullivan deposit (Hamilton et al., 1982; Turner et al., 2000). The late albitization of the vent complex and feeder zone is clear evidence that post-ore hydrothermal fl uids utilized the same conduits as the ore-forming fluids.
The nature and extent of the hydrothermal alteration and mineralization in the feeder zone depends to a large degree on the mineralogy and physical properties of footwall sediments, the temperature and chemical composition of the hydrothermal fl uids, and hydrostatic pressure or water depth (Goodfellow et al., 1993). As a result, compared to VMS deposits, feeder pipes and associated alteration underlying SEDEX deposits are relatively inconspicuous due to low sulphide contents, less reactive siliciclastic sediments compared to glassy volcanic rocks, and limited seawater recharge through the low-permeability hemipelagic mud that hosts most deposits. Furthermore, subtle but diagnostic hydrothermal assemblages such as clay minerals are obscured by later metamorphism.
Distal and Post-ore Hydrothermal Sediments
Hydrothermal systems that form SEDEX deposits are typically long-lived and highly focused at discrete vent sites. Furthermore, hydrothermal activity commonly continues after sulphide formation, forming post-ore hydrothermal sediments and alteration that extend for hundreds of metres into the stratigraphic hanging-wall sequence. In most SEDEX deposits, the basal contact between the stratiform sulphides and underlying sedimentary rocks is sharp, whereas the top of the sulphide zone grades into an overlying sequence of host sedimentary pelagic and/or clastic sedimentary rocks.
Hydrothermal products that extend for hundreds of meters into the post-ore sequence and provide an important target for mineral exploration include:
Most SEDEX deposits are also surrounded by hydrothermal sediments that extend for up to several km from the sulphide zone. In deposits containing barite (e.g., Tom and Meggen), these distal sediments typically consist of interlayered barite, chert, carbonate and host lithologies. In other deposits, this facies is represented by iron sulphides and/or chert interbedded with host lithologies (e.g., Sullivan, Hamilton et al., 1982). At Howards Pass in the Yukon, the distal fringe of the ore zone consists of a laminated phosphatic chert and pyritic shale (Goodfellow, 2004). A manganese-rich halo has been noted to surround several SEDEX deposits, including the Tom (Large, 1981a) and Meggen (Gwosdz and Krebs, 1977). Widespread lithogeochemical halos have also been documented at the Lady Loretta (Large and McGoldrick, 1998) and McArthur River (HYC; Large et al., 2000) deposits.
Tectonic Settings
SEDEX, Irish, and BHT deposits occur in intra-cratonic and epicratonic sedimentary basins (Large, 1980). The tectonic settings include intra-cratonic rifts driven by mantle plumes (e.g., Belt-Purcell basin; Anderson and Goodfellow, 2000), reactivated rifted margins (e.g., Howards Pass; Goodfellow et al., 1986), and far-fi eld back-arc rifting (e.g., MacMillan Pass-Gataga (Fig. 11) and Mount Isa-McArthur districts; Nelson et al., 2002; Betts et al., 2003). Although there is considerable debate on BHT deposits, our interpretation is that the association of the Broken Hill deposit with coeval bimodal igneous rocks in a sedimentary basinal sequence suggests that this deposit type is similar to less-deformed and metamorphosed VSHMS (volcanic-sediment- hosted massive sulphide) deposits in sedimented backarc continental rifts (e.g., Bathurst Mining Camp, Finlayson Lake, Iberian Pyrite Belt).
Most SEDEX deposits formed during periods of tectonism which is typically manifested by fault reactivation, intrabasin clastic sedimentation, and in many cases magmatism represented by volcanism and/or sill emplacement. Most deposits occur in reduced marine basins that formed during the sag phase of basin history, adjacent to deeply penetrating faults.
Secular variations and the sulphur cycle
SEDEX, Irish, and BHT deposits formed during several discrete episodes from Paleoproterozoic (about 2000 Ma) to Cretaceous (Fig. 12). The number and size of SEDEX per 50 million years are greatest in the Middle Paleoproterozoic and Paleoproterozoic, respectively. Lead and Ag grades are highest in the Early Mesoproterozoic, due to the infl uence of the giant Sullivan deposit, and Au grades reach a maximum in Paleoproterozoic and Early Mesoproterozoic deposits although the database of Au grades is very limited (see Table 1 and Appendix 1, DVD).
Most SEDEX deposits coincide with periods in Earth history when the oceans were episodically stratifi ed with a lower anoxic and H2S-rich water column (Fig. 13A). In the Paleozoic Selwyn Basin, for example, there is a close relationship between upward increasing d34S secular trends in sedimentary pyrite, anoxic laminated carbonaceous shales and cherts, and three major SEDEX forming events in the Late Cambrian, Early Silurian, and Late Devonian (Fig. 13B). In the Selwyn Basin, episodes of ocean stratifi cation with reduced bottom waters coincide with global cycles of black shale deposition during the Paleozoic (Arthur and Sageman, 1994), indicating that the Selwyn Basin anoxic episodes refl ect global processes. The secular variation of pyrite d34S values has been attributed to Rayleigh fractionation of S isotopes under closed or partly closed anoxic conditions, and accompanying increased rates of isotopically light S deposition as sedimentary sulphides causing an increase in d34S values for H2S in the reduced water column (Goodfellow, 1987).
The transition from a ferrous Fe-dominated Archean ocean to a reduced S-dominated stratifi ed Proterozoic and Phanerozoic oceans followed the oxidation and precipitation of Fe in Superior-type iron formations (Fig. 13A). This major change in ocean chemistry was accompanied by the build-up of sulphate, which was essential for bacterial sulphate reduction, and the establishment of H2S-rich anoxic water columns. The absence of Archean and Early Paleoproterozoic SEDEX deposits is probably controlled, therefore, by the limiting effect of high contents of reduced Fe on the activity of H2S in anoxic oceans. Under these conditions, metals in S-depleted saline hydrothermal fl uids vented into seawater would be expected to be lost to the water column because of a lack of reduced S to precipitate them (Goodfellow et al., 1993).
Basin architecture
The ideal basinal architecture for the formation of SEDEX deposits (Fig. 14) is a continental rift basin with at least 2 to 5 km of coarse-grained permeable clastics and related volcanics and/or volcaniclastics that form the syn-rift phase overlain by an impermeable cap or seal of basinal shales and/or carbonates (Lydon, 1983; Large, 1986). The source for Zn and Pb is syn-rift dominantly clastic sedimentary rocks (Lydon et al., 2000b). The ideal traps for the metals are reduced subbasins with an adequate supply of bacteriogenic H2S in the ambient water column (Fig. 14). Although an association with magmatism is not indicated for all SEDEX deposits, mafi c volcanic rocks and sills are spatially and temporally associated with many deposits (e.g., Selwyn Basin and Belt- Purcell basin) and bimodal volcanic rocks host most BHT deposits (e.g., Broken Hill; Parr and Plimer, 1993)
Two of the best understood continental basins hosting SEDEX deposits in Canada are the Paleozoic Selwyn Basin that extends from Alaska border through Canada into the U.S. south of the British Columbia (Fig. 15 from Goodfellow et al., 1995), and the Middle Proterozoic Belt- Purcell basin that extends from southeastern British Columbia to Montana and Idaho in the U.S. The Bathurst Mining Camp in northern New Brunswick (Goodfellow and McCutcheon, 2003) and the Finlayson district in the Yukon are two possible examples of BHT deposits (Piercey et al., 2001; Peter et al., 2007).
District scale (Canada)
At the district scale, SEDEX deposits commonly occur in clusters and formed during several hydrothermal events within local second- order basins adjacent to extensional structures (e.g., Fig. 16, Sullivan deposit) separating basinal facies fi ne-grained sediments from platformal carbonates sequences. Some deposits are spatially and temporally associated with volcanic and intrusive rocks. Most deposits are hosted by marine basinal sedimentary rocks that include black shales and cherts, carbonates, and intrabasinal clastic sedimentary rocks.
Deposit scale
SEDEX, Irish, and BHT deposits typically occur in local third-order sedimentary basins. Vent-proximal deposits are associated with active faults that commonly defi ne the margins of local basins (Fig. 8A), whereas vent-distal deposits occupy bathymetric depressions on the seafl oor (Fig. 8B). The most recognized control on the siting of vents and associated ores is cross-stratal faults that served as conduits for transporting metalliferous fl uids from the hydrothermal reaction zone to the seafl oor. Other factors that infl uenced the location of vents are: 1. basement highs where the thickness of soft sediment is at a minimum, 2. the hydrology of the reaction zone which is partly controlled by the thermal structure, 3. the basement geometry, and 4. the position of recharge zones. In the case of vent-distal deposits, the predominant control other than proximity to vents on the location of deposits is fl uid density and local seafl oor bathymetry.
Major metallogenetic districts that host SEDEX deposits (Fig. 3) are:
The Selwyn Basin occupies the Paleozoic margin of western North America and has been subdivided into fi ve spatially distinct mining districts representing three ages of mineralization: 1. Late Cambrian Anvil, 2. Late Cambrian Duncan, 3. Early Silurian Howards Pass, 4. Late Devonian MacMillan Pass, and 5. Late Devonian Gataga districts. The Middle Proterozoic Belt-Purcell is an intracratonic basin (Price and Sears, 2000) that hosts the Sullivan district (Höy et al., 2000). Other SEDEX districts include the highly metamorphosed Neoproterozoic Shuswap district in southern British Columbia, and the Mesoproterozoic Maniwaki-Gracefi eld district in the Grenville Province of Quebec. In the Appalachian orogen, the Carboniferous Walton district of Nova Scotia hosts the pastproducing Walton deposit.
Conventional models
SEDEX deposits most likely formed from oxidized and therefore H2S-poor fl uids generated in geopressured hydrothermal reservoirs within syn-rift clastic (and evaporitic) sediments sealed by fi ne-grained marine sediment or carbonates (Goodfellow et al., 1993; Cooke et al., 2000). During the post-rift or sag phase of basin formation, which is typically long-lived and spans over 200 million years in the case of the Selwyn Basin, Zn and Pb were probably leached from iron oxides coating detrital minerals and homogenized by convecting fl uids in the hydrothermal reservoir. The large variability in the temperature, salinity, metal content, and redox conditions of SEDEX fl uids was controlled by a number of parameters including the local thermal regime, the redox state of the reservoir sediments, and the presence or absence of evaporates. Ancient SEDEX fl uids are similar to metalliferous fl uids in modern sedimentary basins, which are characterized by temperatures up to 305°C (e.g., Salton Sea brines; McKibben et al., 1988), high salinities, and very low total S(reduced):total metal ratios.
A mineralizing episode is triggered by tectonic events that re-activate major rift faults that generate rapidly subsiding grabens or half-grabens. The reactivated rift faults can breach the sediment cap, causing the discharge of metal-rich saline fl uids (enriched in Fe, Zn, Pb as chloride complexes, and variable SO4 2-) along the faults to the basin fl oor. For most SEDEX deposits, metal sulphides are precipitated at or the sulphate has been reduced to sulphide, barium carried by hydrothermal fl uids will be lost to the water column because of a lack of sulphate to precipitate barite.
Recent advances in genetic/exploration models
Major advances in the genetic and exploration models are listed and discussed briefl y below:
Continental scale
At the continental or basin-wide scale, criteria indicating a high potential for SEDEX and BHT Zn-Pb deposits include:
District and deposit scale
At the district scale, the criteria for evaluating the potential to host SEDEX and BHT Zn-Pb deposits are:
Surficial geochemical anomalies: sediment and water samples that are locally anomalous in deposit-forming and ore-associated elements.
Key knowledge gaps are summarized below.
Using the criteria outlined above for identifying productive basins, major sedimentary basins in Canada are rated for their potential to host SEDEX, Irish-type and BHT sulphide deposits. It should be noted that the confi dence level varies with the quality and comprehensiveness of geoscientifi c data, and the level of exploration by the mining industry.
Basins Hosting SEDEX Deposits
The following basins host SEDEX and VSHMS deposits and are therefore highly prospective for additional new deposits within existing districts and new districts.
Highly Prospective Sedimentary Basins
The following basins do not contain SEDEX deposits but exhibit all or most of the key attributes of productive basins.
Moderately Prospective Sedimentary Basins
The following basins do not contain SEDEX deposits and exhibit most of the key attributes of productive basins but are defi cient in at least one fundamental attribute. The Richardson Trough in not underlain by a syn-rift clastic sequence and therefore does not exhibit the classic architecture of productive sedimentary basins. All the remaining sedimentary basins listed below are older than the oldest SEDEX deposits and may be defi cient in bacteriogenic S that is considered essential for precipitating base metals vented by H2S-poor hydrothermal fl uids into ambient seawater.
This synthesis is based largely on previous reviews of SEDEX deposits and research emanating from Geological Survey of Canada research projects on SEDEX deposits of the Selwyn Basin, Yukon, and Sullivan mining district, southern British Columbia. It is intended to have a global perspective but a national focus on SEDEX deposits and sedimentary basins considered to have SEDEX potential. We thank C. Allen and S. Paradis for reviewing the manuscript and offering many excellent suggestions, and I. Kjarsgaard for checking and editing an earlier version of the manuscript and accompanying Canadian and global SEDEX databases. P. Smith of Brook Hunt is thanked for making recent data on global Zn and Pb production, reserves and resources available for plotting in Figure 1.
[Click on an image thumbnail to view a larger image, notice]
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