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©2013 Society of Economic Geologists, Inc.
Economic Geology, v. 108, pp. 45–58
Sulfide Saturation in Mafic Magmas: Is External Sulfur Required for
Magmatic Ni-Cu-(PGE) Ore Genesis?
EDWARD M. RIPLEY† AND CHUSI LI
Department of Geological Sciences, Indiana University, Bloomington, Indiana 47405
Abstract
The importance of externally derived sulfur in the genesis of sulfide-rich, magmatic Ni-Cu-(platinum group
element [PGE]) deposits remains a key, yet unresolved, issue. Calculations utilizing a variety of mafic magma
types indicate that, in general, sulfide saturation by fractional crystallization occurs after Ni has been depleted
due to olivine crystallization. Cu- and PGE-rich layers may form during relatively later stages of closed-system
crystallization, but unless the collection of the cotectic proportion of immiscible sulfide is extremely efficient,
the mass of sulfide is too small to produce an economic deposit. We show that there are numerous processes
that may lead to early sulfide saturation in mafic/ultramafic magmas. Contamination of mantle-derived magmas by siliceous country rocks or their partial melts will lower the sulfur content needed to induce sulfide liquid saturation, typically by amounts ranging from 200 to 700 ppm. The mixing of magmas, particularly if the
result is to lower the liquidus temperature of the mixed magma, may also lower the sulfur content needed to
attain sulfide saturation by similar amounts. An increase in magma fO2 related to the addition of volatiles such
as H2O and CO2 is less effective in decreasing the sulfur concentration needed to achieve sulfide liquid saturation. Contamination processes that lead to an increase in the activity of SiO2 in the melt, and hence may promote orthopyroxene rather than olivine crystallization, aid in generating relative Ni enrichment in remaining
liquid as a result of the lower DNi (mineral – melt) value of orthopyroxene relative to olivine. Although contamination and magma mixing may produce early sulfide saturation without the addition of externally derived
sulfur, Ni-rich sulfide deposits can form in such cases only from large-volume, open systems, where the efficiency of sulfide collection is high. No matter what the liquidus minerals may be, without the addition of country rock-derived sulfur, the mass of sulfide necessary to generate economic Ni-Cu-(PGE) concentrations
requires efficient sulfide collection from large, but not necessarily unrealistic, volumes of magma. Small
deposits (4–30 Mt of sulfide) may form from the collection of cotectic proportions of sulfide from less than 50
km3 of magma. Larger deposits such as those at Noril’sk could involve more than 200 km3 of magma; this volume of magma is not unreasonable, particularly in rift/plume-related settings. Despite such possibilities, sulfur
isotope data clearly indicate that externally derived sulfur has been involved in the formation of many large deposits, and that collection of mantle-derived sulfide in sufficient quantities to produce orebodies is a rare
process. We propose that magmatic Ni-Cu-(PGE) sulfide ore formation normally requires significant sulfide
supersaturation, and that the addition of sulfur derived from xenoliths is the most viable mechanism for producing sulfide well above the cotectic proportion in mafic/ultramafic magmas.
Introduction
THE ATTAINMENT of sulfide saturation of a magma and the
separation of immiscible sulfide liquid, together with the
presence of an appropriate physical environment for the collection and concentration of the metal-rich sulfide liquid, are
key ingredients for the formation of magmatic Ni-Cu-(platinum group element [PGE]) deposits. Experimental studies
of the solubility of sulfur in mafic magmas (e.g., Haughton et
al., 1974; Shima and Naldrett, 1975; Buchanan and Nolan,
1979; Danckworth et al., 1979; Wendlandt, 1982; Mavrogenes
and O’Neill, 1999; Holzheid and Grove, 2002; O’Neill and
Mavrogenes, 2002; Clemente et al., 2004; Jugo et al., 2005;
Scaillet and Macdonald, 2006; Liu et al., 2007; Moune et al.,
2009) have shown that several processes can lead to the attainment of sulfide saturation in a mafic magma. Mavrogenes
and O’Neill (1999) showed that the solubility of sulfide in a
mafic magma increases with decreasing pressure, and therefore concluded that mafic magmas that are emplaced at relatively shallow depths are unlikely to be sulfide saturated.
They noted that, in order for sulfide saturation to be achieved
in the low-pressure environment, either extensive fractional
† Corresponding
crystallization or the introduction of external sulfur must
occur. The experimental data on sulfide and sulfate solubility
in mafic magmas that are now available can be used to illustrate that several processes of contamination of mafic magma,
or mixing of magma types, can lead to the saturation of a
mafic magma with sulfide or sulfate liquid. However, one of
the major questions still posed with respect to magmatic NiCu-(PGE) ore deposition is if externally derived sulfur is an essential ingredient in the process. Recent articles illustrate the
strongly contrasting points of view. For example, Keays and
Lightfoot (2010) state that crustal sulfur must be added to
mantle-derived magmas to promote ore genesis, whereas Seat
et al. (2009) provide evidence from the Nebo-Babel deposit
that mantle S can be sufficient to promote ore formation.
The only process for the attainment of sulfide saturation in
a mafic magma that does not require some type of interaction
with country rocks, or mixing of magmas, is fractional crystallization. The increase in S concentration of a melt as a result
of crystallization of olivine, pyroxene, feldspar, etc., may lead
to the separation of what is known as “cotectic” proportions of
sulfide liquid. Sulfide-poor but PGE-enriched layers such as
that found in the Sonju Lake intrusion (e.g., Miller, 1999; Park
et al., 2004) are thought to result from fractional crystallization
author: e-mail, [email protected]
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Submitted: February 27, 2012
Accepted: May 16, 2012
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RIPLEY AND LI
of a tholeiitic melt. Tao et al. (2007) proposed that sulfide saturation was achieved due to olivine and chromite crystallization in magma that gave rise to PGE-enriched disseminated
sulfide zones in the Jinbaoshan intrusion in China.
Most, but perhaps not all, of the world’s large Cu-Ni-(PGE)
deposits exhibit evidence for mixing processes in their evolution, either involving a compositionally distinct mantle-derived
magma or a crustal contaminant. Chemical mixing of magmas
has been proposed as an integral process in the formation of
high-grade PGE deposits, such as those of the Merensky Reef
in the Bushveld Complex and the JM Reef in the Stillwater
Complex (e.g., Campbell et al., 1983; Naldrett and von
Gruenewaldt, 1989), and has recently been proposed by
Godel et al. (2011) as a key process in the generation of the
Nebo-Babel deposits. Li and Ripley (2009) showed that mixing of two magmas could lead to the attainment of sulfide saturation in the mixed magma. However, the degree of sulfide
saturation is critically dependent on the sulfur contents of the
end-member magmas, and the amount of sulfide liquid that
may form will typically be small. Sulfide-poor but PGE-rich
deposits could result, but it is not clear whether sulfide-rich,
large tonnage Cu-Ni-(PGE) deposits could be produced.
Another type of mixing involves mafic magmas and partial
melt derived from assimilated, siliceous wall rocks. Irvine
(1975) deduced that the addition of SiO2 to a mafic magma
could decrease sulfide solubility and promote the formation
of an immiscible sulfide liquid. Magma silicification or felsification has been proposed as a mechanism to induce sulfide
saturation in mafic magmas by Irvine (1975), Li and Naldrett
(2000), Lightfoot and Hawkesworth (1997), and Seat et al.
(2009). Li and Ripley (2005) also showed that silicification of
a mafic magma can lead to sulfide saturation, but questions
similar to those for magma mixing remained, in terms of the
mass of sulfide that could be sequestered as a result of such a
process.
Lehmann et al. (2007) and Holwell et al. (2007) have called
upon the assimilation of carbonate to increase magma fO2 and
decrease the sulfide solubility of magmas related to the NiCu–rich ores of the Jinchuan deposit and the PGE-rich occurrences in the Platreef of the Bushveld Complex, respectively.
Changes in magma fO2 are related to changes in key compositional values such as the FeO/Fe2O3 ratio. Experimental
results suggest that at relatively low fO2 conditions, where sulfide is the predominant sulfur species, small increases in fO2
of a magma coupled with decreased amounts of FeO will decrease the S concentration needed to attain sulfide saturation.
However, whether this process can account for the large
amounts of sulfide in systems such as Jinchuan remains unclear. Perhaps the most obvious contaminant to induce sulfide
saturation in magmas is S itself. This was pointed out by
Mavrogenes and O’Neill (1999) as a result of their experimental work on the effect of pressure on sulfide solubility,
and has been proposed by many researchers based on physical parameters such as the spatial proximity of S-rich country
rocks or S isotope results. Sulfur isotope results have provided
strong evidence for the introduction of S in komatiite-related
deposits (e.g., Naldrett, 1966; Lesher and Groves, 1986; Bekker
et al., 2009), the deposits at Noril’sk (Grinenko, 1985; Gorbachev and Grinenko, 1973; Li et al., 2003b), sulfide deposits
in the Duluth Complex (e.g., Ripley, 1981; Ripley and Al-Jassar,
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1987; Lee and Ripley, 1995; Arcuri et al., 1998; Ripley et al.,
2007), Voisey’s Bay (Ripley et al., 1999, 2002), Uitkomst (Li et
al., 2002), and the recent discoveries of Kabanga in southern
Africa (Maier et al., 2011). In fact, it is often the absence of
compelling S isotope evidence that has led researchers to
seek alternatives to external S addition to promote sulfide saturation in mafic magmas (e.g., Seat et al., 2009). There are at
least two reasons why δ34S values of sulfide ores that fall in
the range generally considered to be normal for S in the upper
mantle (~0 to 2‰, Ripley, 1999, and references therein)
should not necessarily be taken as an indicator that S contamination has not occurred. One is the situation discussed by
Ripley et al. (2002) for the Voisey’s Bay deposit. At Voisey’s
Bay, only the ores in the Reid Brook zone show δ34S values
that are different from those of mantle S. However, when
examined in detail, it is clear that the Proterozoic Tasiuyak
Gneiss, a locally sulfidic/graphitic pelite that is a likely source
of externally derived S, is characterized by a wide range of
δ34S values (~ –17 to +18‰; Ripley et al., 2002). These values are not unusual for sulfide found in sedimentary rocks,
and of particular significance is the fact that the weighted average δ34S of the Tasiuyak Gneiss is –1.4‰. Clearly, if homogenization occurred in the magma, anomalous δ34S values
should not be expected. This example holds for any situation
where the δ34S value of country-rock S is near 0‰. A second
possibility is that if sulfides accumulated in a chamber where
additional uncontaminated magma passed, isotopic exchange
reactions (Ripley and Li, 2003) could result in δ34S values that
approach those of mantle values. This process would be
expected in conduit systems where magma passage may have
led to increases in the tenor of accumulated sulfide. In
Archean systems, where sedimentary sulfides may be characterized by δ34S values that depart only slightly from those of
mantle values, the use of multiple S isotopes (e.g., δ33S as well
as δ34S) has proven valuable in the determination of externally
derived S from Archean rocks. Archean sedimentary sulfides
often record anomalous Δ33S values (deviation from the terrestrial fractionation line), thought to be linked to low oxygen
values in the Archean atmosphere (e.g., Farquhar and Wing,
2003). Anomalous Δ33S values have been utilized by Bekker
et al. (2009) to confirm the importance of crustal S in komatiiterelated deposits. For magmatic deposits where Archean rocks
are unlikely to have supplied S to the magma, Δ33S will be of
little value as an indicator of external S addition where δ34S
values are near 0‰. There can be little argument that crustal
S has played a significant role in ore genesis in those deposits
where S isotope values are strongly anomalous. In their
recent paper, Keays and Lightfoot (2010) used chalcophile
element geochemistry of basaltic rocks at Noril’sk compared
to those of the Deccan to arrive at their conclusion that crustal
S is essential for the genesis of magmatic Ni-Cu deposits.
Others (e.g., Lehmann et al., 2007; Seat et al., 2009) refute
such a claim, and the question remains if other mechanisms
which can promote sulfide saturation in a magma can lead to
the generation of magmatic Ni-Cu sulfide orebodies. In this
paper we review many of the processes that can lead to the attainment of sulfide saturation in a mafic magma and attempt
to constrain some key parameters that are of importance in
situations where the addition of externally derived S to a
magma is not indicated, and hence may not be of significance
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SULFIDE SATURATION IN MAFIC MAGMAS: IS EXTERNAL SULFUR REQUIRED FOR MAGMATIC Ni-Cu-(PGE) ORE GENESIS?
for Ni-Cu-(PGE) ore formation. We utilize the equation of Li
and Ripley (2009) to estimate the concentration of sulfur at
sulfide saturation (SCSS) in a mafic magma; the equation is
based on experimental results from a variety of sulfide-saturated and compositionally variable systems (see above) and
gives results that are similar to the equation of Liu et al.
(2007). We use the equation in conjunction with the MELTS
routine of Ghiroso and Sack (1995) to evaluate how processes
such as fractional crystallization, compositional variations related to contamination, and changes in intensive parameters
such as fO2 affect the attainment of sulfide saturation in magmas. We also evaluate the importance of the mass of magma
involved in potential ore-forming systems where the introduction of externally derived S may not have occurred.
It should be noted that the equation for SCSS by Li and
Ripley (2009) does not take into account chalcophile elements such as Ni and Cu. Ariskin et al. (2010) and Evans et
al. (2008) have shown that chalcophile elements, in addition
to Fe, may exert a significant control on the solubility of S in
mafic to ultramafic magmas. The potential influence of Ni
and Cu on sulfur solubility is particularly important when
assessing the role of mantle-derived S in ore genesis. As S is
held primarily within Ni, Cu, and Fe sulfide minerals in the
mantle, complexing with these metals is to be expected. This
will be true for high-degree or second-stage mantle melts,
where immiscible sulfide liquid may ultimately dissolve in
silicate liquids. There is no reason for the breaking of S-Cu
or S-Ni bonds in favor of S-Fe, and both Ni and Cu must
exert a control on the capacity of a mafic magma to dissolve
sulfide. If S is introduced into a mafic/ultramafic melt in a
form that does not involve metal complexing, such as H2S,
the mass action effect will strongly favor the formation of FeS complexes. O’Neill and Mavrogenes (2002) have stated
that the sulfide capacity of a melt with ~10% FeO is controlled mostly by the Fe content. Until additional experimental data that treat the effects of chalcophile element
concentration on sulfide solubility over a broad range of
compositions are available, we are unable to update our regression equation.
Fractional Crystallization and Sulfide Saturation
In Figure 1 we illustrate the sulfide saturation curves for a
high-Al olivine tholeiite (HAOT—Table 1) liquid thought to
be a reasonable parental magma for troctolitic rocks (e.g.,
Duluth Complex and, potentially, Voisey’s Bay; Ripley et al.,
2007; Scoates and Mitchell, 2000), a high-FeO picritic liquid
thought to be a potential parental magma for rocks that host
the Eagle deposit (Ding et al., 2010), and a high-FeO,
siliceous high-MgO basalt liquid similar to the B1 magma
type proposed by Barnes at al. (2010) as a potential parental
magma to the Lower and lower Critical zones of the Bushveld
Complex. In this discussion the magmas are assumed to be
anhydrous; the effect of H2O on the sulfide saturation curve
is discussed below. For the high-Al olivine tholeiite (Fig. 1a)
the sulfide saturation value rises slightly from that of the 1-kb
liquidus due largely to iron enrichment in the liquid related
to crystallization of plagioclase and olivine in a ratio of 3:1
(Table 2). It is not until later in the sequence, and particularly
when spinel becomes a liquidus mineral, that the sulfide saturation value begins to decrease. In the case of a picritic
parental magma, the S content required for saturation at the
liquidus is considerably higher than that required to saturate
the HAOT liquid, but the saturation value decreases as
olivine initially crystallizes, followed by olivine plus clinopyroxene (Fig. 1b; Table 2). Where clinopyroxene and plagioclase begin to crystallize, the FeO content of the residual
magma rises, and the S content required for sulfide liquid
saturation increases as well. In the case of the FeO-rich,
siliceous high-MgO basalt, the SCSS progressively declines,
as initial olivine crystallization is quickly followed by orthopyroxene (~3.5% crystallization), and then clinopyroxene and
plagioclase. These three examples illustrate the types of variations in the SCSS trajectories that may characterize mafic
magmas.
Treating S as a perfectly incompatible element during silicate crystallization, we indicate when fractional crystallization
should induce sulfide saturation in the HAOT and picritic
magmas. A value of 1,000 ppm S is representative of a melt
TABLE 1. Composition of Magmas Used to Assess SCSS (values in wt %)
SiO2
TiO2
Al2O3
Fe2O3
FeO
MgO
CaO
Na2O
K2O
H2O
1
2
3
4
5
6
7
8
47.77
1.29
19.90
0.71
10.37
7.10
9.69
2.67
0.50
0.00
46.56
1.25
19.40
1.62
10.74
6.92
9.44
2.60
0.49
1.00
48.95
2.84
12.82
2.05
10.06
7.73
12.52
2.51
0.51
0.00
52.30
1.17
12.70
1.17
5.87
13.08
9.56
3.73
0.43
0.00
55.37
0.38
11.53
1.32
8.16
13.79
6.58
1.85
1.02
0.00
48.00
1.81
11.69
1.84
10.91
13.67
9.83
1.75
0.48
0.00
47.26
0.27
6.55
1.27
8.83
30.23
5.04
0.45
0.10
0.00
71.42
Columns: 1) High-Al olivine tholeiite; Ripley et al., 2007; liquidus T = 1,229°C
2) High-Al olivine tholeiite, 1 wt % H2O; Ripley et al., 2007; liquidus T = 1,169°C
3) Ocean island tholeiite; Kent et al., 1999; liquidus T = 1,205°C
4) Siliceous high-MgO basalt; e.g., Barnes, 1989; liquidus T = 1,347°C
5) High-FeO, siliceous high-MgO basalt; e.g., Barnes et al., 2010; liquidus T = 1,382°C
6) High-FeO picrite; Ding et al., 2009; liquidus T = 1,337°C
7) Komatiite; Barnes, 2007; liquidus T = 1,617°C
8) Partial melt from pelite; Hoffer and Grant, 1980
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13.70
1.20
0.28
5.40
4.03
4.00
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RIPLEY AND LI
a
b
c
FIG. 1. Sulfur content at sulfide liquid saturation versus wt % of magma crystallization. The sulfur axis refers either to the
sulfur content at sulfide liquid saturation or, in the case of fractional crystallization, to the sulfur content of the remaining
liquid. Fractionating assemblages are given in Table 2. All calculations were done using a pressure of 1 kbar. Note the relatively small differences between the HAOT at QFM and QFM-2 (a), and a similar relationship for the high-FeO picrite (b).
Trends for the contaminated magmas, and the hydrous HAOT, are similar, with much lower SCSS values than their anhydrous and uncontaminated counterparts. Sulfur enrichment due to fractional crystallization is illustrated for initial concentrations of 800, 1,000, and 1,500 ppm. Sulfide saturation is attained at less than ~20% crystallization in contaminated magmas with 1,000 ppm S. Of particular note is the fact that orthopyroxene is the fractionating phase rather than olivine and
plagioclase in the HAOT magma contaminated with 15% SiO2 (Table 2). Although the S content of the magma contaminated
with SiO2 only would drop to 850 ppm, saturation would still be attained at ~10% crystallization. Orthopyroxene is the fractionating phase at ~3.5% crystallization for the high-FeO, siliceous high-MgO basalt (c). Because DNi(mineral-melt) values
are lower for orthopyroxene relative to olivine, the crystallization of orthopyroxene may be relevant for the formation of Nirich sulfide orebodies where sulfide saturation was attained after significant magma crystallization.
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SULFIDE SATURATION IN MAFIC MAGMAS: IS EXTERNAL SULFUR REQUIRED FOR MAGMATIC Ni-Cu-(PGE) ORE GENESIS?
troctolitic rocks from the Duluth Complex that show no evidence for crustal contamination contain from 500 to 600 ppm
S and suggest that the parental HAOT contained far less than
1,000 ppm S (Ripley et al., 2007). For comparative purposes,
we show S trajectories as a result of fractional crystallization
for initial concentrations of 800, 1,000, and 1,500 ppm. In the
case of the picritic magma, saturation at 1 kb is reached at
~40% crystallization for a starting magma with 1,000 ppm S.
For the HAOT, ~40% crystallization is also required to induce sulfide liquid saturation. Of additional note is that, due
to the shallow trend of the SCSS curve where plagioclase and
clinopyroxene are liquidus minerals (Table 2), and the positive slope where Fe enrichment accompanies the cessation of
olivine crystallization, only small amounts of immiscible sulfide
liquid can be generated as a result of fractional crystallization
until late stages of the process. In strong contrast, sulfide saturation is attained in the high-FeO, siliceous high-MgO basalt
at ~17% fractional crystallization for a magma with an initial
S concentration of 1,000 ppm.
Concentrations of platinum group elements and Cu are
expected to increase during fractional crystallization due to
their high degree of incompatibility. This is not the case for
Ni, which is readily accepted into the olivine structure. Distribution coefficients for Ni between olivine and liquid in sulfide-undersaturated conditions are a strong function of MgO
contents and range between 4 and 20 at MgO concentrations
from 22 to 4 wt % (see summary in Li et al., 2003a). For the
picritic parental magma (assuming an initial concentration of
Ni = 300 ppm), where the ratio of olivine crystallized to plagioclase plus clinopyroxene at the point of sulfide saturation
is ~1.7, the concentration of Ni in the residual liquid drops to
127 ppm using an olivine/liquid D value of 7. The drop in Ni
concentration for the HAOT at the 40% crystallized point,
where sulfide saturation is predicted, is similar (139 ppm) due
in part to an olivine/liquid D value of 15. The drop in Ni concentration is far less extreme for the high-FeO, siliceous highMgO basalt, where orthopyroxene replaces olivine as a liquidus phase before sulfide saturation is attained. Because the
DiNi (orthopyroxene-liquid) value for orthopyroxene (~1–3,
Hashizume and Hariya, 1992; Frei et al., 2009) is considerably lower than the DiNi (olivine-liquid) value, higher concentrations of Ni will be available for partitioning into sulfide
liquid. Of obvious concern is whether sulfide-saturated magmas where prior crystallization of olivine is indicated and that
contain less than 140 ppm Ni can produce Ni sulfide-rich orebodies. We will return to this point below, but end the current
discussion with an example where fractional crystallization
appears to have played a strong role in the distribution of S
and metals in an intrusion.
The Sonju Lake intrusion is a relatively small (~1,200 m
thick) layered body in the Beaver Bay Complex associated
with the ~1.1 Ga Duluth Complex (Miller and Ripley, 1996).
Miller (1999) and Park et al. (2004) have described the presence of Cu- and PGE-enriched zones in the layered sequence
at the level of Fe oxide-rich gabbro (Fig. 2). Miller (1999)
suggested that the “reef” represents the level at which sulfide
saturation was achieved in the crystallizing magma. Li and
Ripley (2005) confirmed that sulfide saturation should have
been achieved at the time that spinel became a liquidus mineral using an equation which is the predecessor to that used
TABLE 2. Fractionating Minerals from the Magmas Illustrated in Figure 1
T°C
(first appearance)
Minerals1
QFM-2
1,233
1,198
1,118
1,078
pl
pl,ol
pl,ol,sp
pl,cpx,sp
HAOT
QFM
1,229
1,209
1,140
1,120
1,100
ol
pl,ol
pl,ol,opx,cpx
pl,ol,cpx
pl,cpx,sp
HAOT, 1% H2O
QFM
1,169
1,161
1,079
1,069
ol
pl,ol
pl,ol,sp
pl,ol,sp,cpx
HAOT + 10% pelite melt
QFM-2
1,187
1,060
1,040
pl,ol
pl,ol,sp
pl,cpx,sp
HAOT + 30% SiO2 melt
QFM-2
1,207
1,180
1,060
opx
pl,opx
pl,opx,sp
High-FeO picrite
QFM-2
1,337
1,175
1,150
ol
ol,pl,cpx
pl,cpx
High-FeO picrite
QFM
1,337
1,200
1,175
ol
ol,cpx
cpx,pl
High-FeO picrite + 10%
pelite melt
QFM
1,321
1,170
1,140
1,000
ol
cpx
cpx,pl
cpx,pl,sp
High-FeO, siliceous
high-MgO basalt
QFM
1,382
1,356
1,191
1,183
ol
opx
cpx
cpx,pl
High-FeO, siliceous
high-MgO basalt, 1% H2O
QFM
1,361
1,240
1,110
1,090
990
ol
opx
cpx
cpx,pl
cpx,pl,sp
High-FeO, siliceous
high-MgO basalt +
10% pelite melt
QFM
1,363
1,322
1,132
1,032
ol
opx
cpx,pl
cpx,pl,sp
Magma
fO2
HAOT
1 cpx = clinopyroxene, ol = olivine, opx = orthopyroxene, pl = plagioclase,
sp = spinel
derived from 20% melting of a mantle with 200 ppm S (Palme
and O’Neill, 2004). Lower degrees of melting may produce
melts with higher S concentrations, but, if sulfide saturation
is attained, immiscible sulfide may be retained in the mantle
(e.g., Keays, 1995; Naldrett, 2011). In the case of a magma
such as a HAOT, which may be itself derived from fractional
crystallization of a more primitive liquid, the S concentration
of the derivative liquid may be more elevated. However,
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RIPLEY AND LI
FIG. 2. Stratigraphic column from the Sonju Lake intrusion, showing the depletion of Ni upward, and the enrichment in
Pt and Pd in the ferrogabbro (modified from Miller, 1999, and Park et al., 2004). Abbreviations: Units in the Sonju Lake
intrusion are preceded by the abbreviation “sl”: Sonju Lake apatite diorite (slad), dunite (sld), ferrogabbro (slfg), gabbro
(slg), monzodiorite (slmd), melatroctolite (slmt), and troctolite (slt). Country rocks are the Finland quartz monzodiorite
(fqmd) and Finland granite (flg).
in this manuscript (Li and Ripley, 2009). What is particularly
important is the fact that at the level of the Cu and PGE
enrichment, the concentration of Ni has dropped to values of
less than 20 ppm. The field and geochemical evidence
strongly suggests that Ni was sequestered by olivine prior to
the attainment of sulfide saturation in the magma. The Sonju
Lake intrusion perhaps represents an end-member case
where extensive Ni depletion occurred prior to the arrival of
sulfide saturation in the magma by fractional crystallization.
H2O + 2 FeO = Fe2O3 + H2. However, Carmichael (1991) and
Righter et al. (2008) have discussed the uncertainty of H2O
addition to a magma resulting in an increase of magma fO2.
This is particularly true if H2O dissolution is via molecular
H2O rather than an OH– complex. Even without a substantial
change in fO2, the SCSS of an H2O-bearing mafic magma may
be much lower relative to the anhydrous counterpart. In Figure 1a the SCSS curve for an HAOT with 1 wt % H2O at
QFM is shown to be lower than that of the anhydrous variety
by ~280 ppm at liquidus temperatures. Ripley et al. (2007)
have shown that a value of 1 wt % H2O is reasonable for many
of the magmas that produced sulfide-bearing intrusions in the
Duluth Complex. A large part of the H2O may have been derived via assimilation of fluid produced as country rocks were
dehydrated. In the case of the high-FeO, siliceous high-MgO
basalt, the addition of 1 wt % H2O lowers the SCSS by ~135
ppm at the liquidus, and by greater values throughout the
course of crystallization. The effect is very similar to that produced by the assimilation of a pelite-derived partial melt (see
below). Although additional study of the effect of H2O addition on the solubility of S in mafic magmas is warranted, it appears that hydrous magmas may attain sulfide liquid saturation much sooner than low-H2O magmas.
A similar uncertainty in terms of increases of magma fO2 is
associated with assimilation of CO2. Dissolution mechanisms
Contamination and Sulfide Saturation
Assimilation of volatiles
The addition of volatile species such as H2O, CO2, CH4,
and H2S to a magma may occur without melting or dissolution
of major minerals. We will treat the potential for the addition
of volatile S species to a magma below. The role of H2O in the
solubility of S in mafic magmas has received only minor
attention (e.g., Liu et al., 2007; Gorbachev and Bezman, 2011;
Moune et al., 2009), and further experimental study is required to assess the importance of species such as H2S and
HS– in sulfide dissolution within mafic magmas. The addition
of H2O to a magma is frequently linked to an increase in fO2
and decrease in FeO content (and hence the capacity of a
magma to dissolve sulfide) via a reaction such as the following:
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SULFIDE SATURATION IN MAFIC MAGMAS: IS EXTERNAL SULFUR REQUIRED FOR MAGMATIC Ni-Cu-(PGE) ORE GENESIS?
of carbonic species in a magma are important in evaluating
potential magma fO2 increases. At relatively high pressure,
CO2 dissolves as CO2–
3 (e.g., Blank and Brooker, 1994) with
relatively little variation in magma fO2. Stanley et al. (2011)
found no correlation between CO2 concentration and the
ratio of Fe3+ to total Fe in a basaltic liquid. In contrast, Wenzel et al. (2002) proposed that CO2-rich fluids released during
the decomposition of dolomitic xenoliths in the Ioko-Dovyren
intrusion resulted in locally elevated magma fO2 values. Mollo
et al. (2010) suggested the opposite—that carbonate assimilation involving magma-H2O-CO2 interaction may lead to a
decrease in magma fO2 values. Methane may be a component
of fluids produced by dehydration of carbonaceous pelites
(e.g., Ohmoto and Kerrick, 1977; Andrews and Ripley, 1989).
The assimilation of CH4 is expected to reduce the fO2 of the
magma and may be of significance in the reduction of sulfate
in magmas with oxidation states that permit sulfate plus sulfide coexistence or the presence of sulfate only (e.g., Jugo et
al., 2005; Jugo, 2009). The assimilation of graphite, perhaps
accompanied by CH4, by relatively oxidized, sulfate-bearing
magmas has also been proposed as an important process for
decreasing magma fO2 and causing the reduction of sulfate in
the magma to sulfide (e.g., Nixon, 1998; Jugo and Lesher,
2005; Thakurta et al., 2008a, b). Tomkins et al. (2012) have
also suggested the assimilation of graphite-bearing felsic magmas by oxidized arc basalts as a mechanism to promote
magma reduction and the formation of immiscible sulfide
liquid.
The assessment of sulfur-free volatile assimilation on sulfide solubility in mafic magmas remains difficult because fO2
changes in natural magmas are often linked with assimilation
processes that alter magma compositions other than Fe2+/Fe3+
ratios. Li and Ripley (2005) showed that fO2 /fS2 ratios in many
of the experiments listed above can be expressed as a function
of melt composition. The effect of crystallization at QFM
rather than QFM-2 on sulfide saturation in the HAOT and
high-Fe picritic liquids is shown in Figure 1a and b. Saturation
values at QFM are lower than those at QFM-2, as expected,
but the effect is small compared to variations in sulfide saturation values related to assimilation of nonvolatile elements
(see below). Jugo (2010) also noted that changes in fO2 below
~QFM resulted in little change in the magma Fe2+/∑Fe ratio,
and hence little change in the SCSS. Increases in the magma
fO2 above QFM result in decreases in the Fe2+/∑Fe ratio, as
well as oxidation of sulfide to sulfate. Due to the increase in S
solubility within oxidized magmas, the concentration of S
needed to obtain sulfide liquid saturation also rises (e.g.,
Jugo, 2009).
so the potential effect of H2O on sulfide saturation is included
in the assessment.
In Figure 3, we have compared the sulfide saturation value
at the liquidus temperature (1 kb) for a variety of mafic magmas and the corresponding values at the liquidus for the same
magmas after 10% assimilation of the Hoffer and Grant (1980)
partial melt. All sulfide saturation values decreased from a
high (in terms of differences between contaminated and uncontaminated liquids) of 681 ppm S in a komatiitic liquid to a
low of 246 ppm in a siliceous, high-MgO basalt liquid. As expected, the more siliceous the initial magma, the less decrease
recorded by the addition of the partial melt. Starting basaltic
compositions with 47 to 48 wt % SiO2 showed decreases in
sulfide saturation values from 365 to 488 ppm. The computations illustrate the exceptionally strong effect that assimilation
may have on komatiitic and picritic magmas, but, in all cases,
the assimilation of a granitic contaminant by a mafic magma
lowers the SCSS and may lead to early generation of a sulfide
liquid.
We utilize the SiO2-only contaminant with the HAOT to
illustrate a potentially important change in the mineralogy of
fractionating phases in the contaminated magma (Table 2).
With 10% contamination by the Hoffer and Grant (1980)
melt, all resultant magma compositions retained olivine as an
early crystallizing mineral. With the addition of 15% SiO2 to
the HAOT composition, not only is the sulfide saturation
value decreased by 569 ppm, but the liquidus phase changes
to orthopyroxene. In the case of the high-FeO, siliceous highMgO basalt, the elevated initial SiO2 concentration drives the
early crystallization of orthopyroxene, without assimilation of
a siliceous contaminant (although such assimilation may have
been responsible for the elevated SiO2 content initially). As
noted above, because of the lower DiNi (orthopyroxene-liquid)
value for orthopyroxene relative to olivine (Hashizume and
Hariya, 1992; Frei et al., 2009), increased concentrations of
Ni will be available to sulfide liquids where similar percentages of orthopyroxene crystallize rather than olivine. We suggest that such a process may be significant for norite-hosted,
Ni-rich orebodies. In this case, not only does assimilation
reduce the capacity of the magma to dissolve sulfide, but Ni
availability is also enhanced relative to magmas from which
olivine is the primary early crystallizing ferro-magnesian mineral. Figure 3 also illustrates that very little, if any, fractional
crystallization is required to promote sulfide saturation in
contaminated siliceous magma. To summarize, analysis of sulfide solubility systematics of mafic magmas clearly shows that
assimilation of siliceous contaminants will cause a significant
drop in the S concentration needed for the attainment of sulfide saturation. In most cases, little, if any, fractional crystallization of the contaminated magma is required to achieve
sulfide saturation. Where the aSiO2 is sufficiently elevated, orthopyroxene, rather than olivine, is an early crystallizing mineral
and, because of the lower DNi value of orthopyroxene relative
to olivine, additional Ni is available for incorporation into a
sulfide liquid. Fractional crystallization of most low-SiO2 mafic
magmas will not promote sulfide saturation until 20 to 40%
crystallization. Although PGE and Cu contents may continue
to rise with crystallization, significant Ni will be sequestered
in olivine. Assimilation of volatiles such as H2O and CO2 may
or may not result in fO2 increases of the crystallizing magma,
Assimilation of siliceous country rocks
We utilize two compositions of contaminants to illustrate
the effect of the assimilation of siliceous country rocks on the
sulfide saturation state of a mafic magma. One composition is
the granitic partial melt produced from a pelite in the experiments of Hoffer and Grant (1980; Table 1). The second is
simply addition of SiO2 only, as may result from magma interaction with an SiO2-rich sedimentary or metamorphic rock, or
as may result from disequilibrium and polystage melting of
pelitic rocks (e.g., Ripley and Alawi, 1988; Mariga et al.,
2006). The Hoffer and Grant (1980) melt contains 4% H2O,
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RIPLEY AND LI
FIG. 3. Comparison of the SCSS from uncontaminated magmas and those contaminated with 10% of the partial melt derived from a pelite (Table 1; Hoffer and Grant, 1980). Number 7 is a mixture of 30% HAOT with 1 wt % H2O and 70% highFeO picrite. The SCSS of the mixed magma is somewhat less than that caused by contamination of the high-FeO picrite by
10% of the pelite-derived melt. Calculations performed using a pressure of 1 kbar.
but, in any case, the drop in the sulfide saturation value
caused by fO2 increase (up to ~QFM) alone is minor compared to that caused by assimilation of Si-rich contaminants.
shown in Figure 4. The degree of sulfide supersaturation (defined as the difference in the sulfur concentration and that of
the SCSS, which is the minimum necessary to promote the
formation of sulfide liquid droplets) that may be attained as a
result of mixing is a strong function of the shape (concavity)
of the SCSS curve. Figure 4a illustrates that the concavity of
the high-FeO picrite-HAOT mixture is so slight that only mixtures of magmas very near the end-member saturation values
will attain sulfide saturation upon mixing. In contrast, where
variations in SCSS values of mixtures are more strongly concave (e.g., Li and Ripley, 2005) or vary as shown in Figure 4b
for an ocean island tholeiite-HAOT mixture, mixing of mafic
magmas can be a mechanism to produce sulfide supersaturation. Figure 4b illustrates that even in this case the mixing
process will be effective only if the end-members are within
~100 ppm of their sulfide saturation values. Tomkins et al.
(2012) have shown how the mixing of an S-bearing oxidized
arc basalt with a reduced graphite-bearing felsic melt could
result in reduction of sulfate and sulfide supersaturation in
the mixed magma.
Mixing of magmas
Li and Ripley (2005) confirmed that mixing of two magmas
may induce sulfide saturation of the resultant magma. We will
not dwell on this point as the systematics are much the same
as contamination involving country rock. We illustrate that
the SCSS for a mixture of 70% high-Fe picrite with 30% of
HAOT containing 1 wt % H2O is lower than that of the uncontaminated picrite by ~300 ppm. This amount is slightly
less than that produced by assimilation by the HAOT of 10%
of the melt produced by pelite partial melting (Fig. 3), but
illustrates that mixing of chemically distinct magmas is a viable
mechanism to reduce the sulfur concentration necessary to
saturate a resultant magma in sulfide liquid. In the case of the
picrite-HAOT mixture, the FeO content of the mixed magma
differs only slightly from either of the end-members; the principal control on the lowering of the saturation value is the
drop in the liquidus temperature of the mixed magma.
Although a lower SCSS value may result relative to that of
fractional crystallization by any of the processes mentioned
above, the mixing of mafic magmas alone will be unlikely to
produce sulfide saturation unless both end-members are
close to their saturation values. This feature has been pointed
out by Naldrett (2011) and is illustrated in what is essentially
an end-member case for the high-FeO picrite-HAOT mixture
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Addition of externally derived sulfur
Perhaps the most efficient means of causing prolonged sulfide supersaturation in a mafic magma is through the addition
of S derived from country rocks. As outlined above, in many
localities the combination of isotopic (e.g., Ripley and Li,
2003) and geochemical (e.g., Keays and Lightfoot, 2010) data
strongly points to the involvement of externally derived S in
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SULFIDE SATURATION IN MAFIC MAGMAS: IS EXTERNAL SULFUR REQUIRED FOR MAGMATIC Ni-Cu-(PGE) ORE GENESIS?
are clearly of potential significance in the generation of magmatic, sulfide-rich Ni-Cu-PGE deposits. However, as we have
illustrated above, many processes that do not involve the incorporation of external S may promote sulfide saturation of a
mafic magma. Whether an economic accumulation of sulfide
may result is a function of the size of the magmatic system,
rate and duration of magma emplacement, and efficiency of
sulfide collection.
a
The Importance of Magma Volume and Chamber Shape
Given that mafic magma may reach sulfide saturation as a
result of fractional crystallization, and much sooner via contamination involving a siliceous end-member or by magma
mixing, the question remains whether an economic sulfide
accumulation may be produced without the addition of external S. In all cases described above, except those of xenolith
digestion or thermomechanical erosion, the amount of sulfide
liquid produced is that of, or very near, the cotectic proportion (Barnes, 2007; Li and Ripley, 2009). Both Barnes (2007)
and Li and Ripley (2009) describe methods to calculate the
cotectic proportion of sulfide. The amount of sulfide liquid
produced per crystallization increment is small (generally
<1.5 wt %), and very efficient collection is required to produce horizons with more than ~2 vol % sulfide. In the case of
a magma with a sulfide saturation value that has been decreased
due to contamination and mixing, the mass of collectible sulfide is constrained by the initial concentration of sulfide in the
system. This is an obvious point, but one of extreme importance when considering ore-forming systems. For example,
for the Sonju Lake intrusion the parental magma is estimated
to have contained no more than 1,000 ppm S. Miller and Ripley (1996) estimate that the intrusion is considerably larger
than its exposed area of 9 km2, with a strike length of ~20 km.
We estimate a potential volume of ~30 km3 of magma, but of
particular significance is the fact that, even with the improbable collection of all available sulfide, only a ~2-m-thick massive sulfide horizon could be produced in the intrusion. As
stated above, Ni concentration dropped to extremely low values prior to sulfide saturation. When sulfide saturation was
attained in the intrusion as a result of fractional crystallization, the R-factor would have been ~260, assuming sulfide
saturation affected all portions of the remaining 60% liquid.
A 2-m-thick massive sulfide would grade ~3 wt % Cu (100
ppm Cu in the parent magma) and 1.3 ppm Pt (3.5 ppb Pt in
initial liquid). A 2-m-thick massive sulfide would be an unlikely candidate for a Cu ore, but a PGE reef could be produced. In the Sonju Lake intrusion, the zone of PGE and Cu
enrichment is dispersed over ~100 m rather than 1 or 2 m,
with grades of ~0.06% Cu and 30 ppb Pt, but less than 70
ppm Ni. These are expected values for dispersion of the
immiscible liquid with the composition described above.
Without the addition of external S, most magmas that crystallize as closed systems (whether uncontaminated or after
contamination involving S-poor country rocks) are unlikely to
produce sufficient quantities of sulfide to form economic
deposits, unless the volume of magma from which sulfide is
derived is large. Barnes (2007) evaluated whether cotectic
amounts of sulfide were sufficient to account for the large,
disseminated sulfide orebody at Mt. Keith. Large, disseminated sulfide-bearing intrusions are logical candidates where
b
FIG. 4. Comparison of SCSS trajectories for mixed magmas: (a) high-FeO
picrite and HAOT, and (b) ocean island tholeiite and HAOT. Mixing of mafic
magmas is potentially important for the attainment of sulfide supersaturation
where end-member S concentrations are close to those required for sulfide
saturation and the shape of the SCSS curve for the mixture is strongly concave or has a pronounced inflection.
ore genesis. The importance of external S in magmatic NiCu-(PGE) ore genesis has been highlighted, and debated, by
many authors, and it is not the purpose of this manuscript to
further review the premise. However, two points regarding
external sulfur addition to mafic magmas deserve further
mention. One is that the addition of H2S- or HS–-bearing fluids from country rocks in a contact aureole is unlikely to produce sulfide in excess of the cotectic proportion. This is
largely due to the fact that external fluids will be added to
magmas only up to their solubility limits. In many cases, fluid
in country rocks will be channeled either by layer-parallel
flow or away from the magmatic heat source. Where sulfide is
derived from xenoliths, the concentration of S in the contaminated magma may far exceed saturation values for the prevailing temperature. In the case of komatiites, the process of
thermomechanical erosion described by Lesher and coworkers (e.g., Lesher and Keays, 2002; Houlé et al., 2012) also provides a mechanism for the incorporation of sulfide (whether
derived via devolatilization, sulfide dissolution, or sulfide melting) that greatly exceeds saturation values. Processes such as
these that promote sulfide supersaturation in a mafic magma
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RIPLEY AND LI
crystallization of cotectic proportions of sulfide may have
been responsible for ore generation. Barnes (2007) concluded that sulfide in excess of cotectic amounts was required
to produce the Mt. Keith orebody and proposed the mechanical deposition of transported sulfide, formed in response to
the introduction of sulfur from country rocks.
In a very large volume system such as the impact melt sheet
at Sudbury, concentrations of 600 to 1,000 ppm S (as estimated by Keays and Lightfoot, 1999; Lightfoot et al., 2001)
are consistent with the estimated mass of sulfide in the Sudbury ores (Lesher and Thurston, 2002; Keays and Lightfoot,
2004; Fig. 5). For a system such as Noril’sk (sulfide content
between 275 and 750 Mt; Lightfoot and Hawkesworth, 1997;
Naldrett, 2011), the amount of sulfide present far exceeds
that which could be collected from closed-system crystallization of magma that produced tabular, ~1,000-m-thick (or less)
sills. If contamination not involving S addition is a key process
for the attainment of saturation, then open-system processes
are likely to have been operative to result in the concentration
of sufficient quantities of sulfide. The mass and grade of sulfide at Noril’sk have been the focus of many studies, virtually
all of which focus on sulfide collection from passing magmas
in a conduit system, followed by some type of metal upgrading (e.g., Brügmann et al., 1993; Naldrett and Lightfoot,
1999; Arndt et al., 2003; Kerr and Leitch, 2005; Lightfoot and
Keays, 2005; Li et al., 2009). Figure 5 illustrates that for the
Noril’sk ores, the estimated sulfide mass, if collected from
magma with ~1,000 ppm S available as immiscible sulfide,
would require between ~34 and 100 km3 of magma. For comparison, the 30-Mt Ovoid orebody at Voisey’s Bay (Lightfoot
et al., 2012) would have required sulfide collection from ~3.7
km3 of magma. For both of these systems the required
amounts of magma may not be unreasonable; the involvement of 100 km3 in an ore-forming system represents only a
small fraction of that which generated the Siberian Traps
(e.g., Reichow et al., 2009). For the small but high-grade
(~3.5% Ni) Eagle deposit, the 4-Mt sulfide orebody could
have been generated from as little as 0.5 km3 of magma containing 1,000 ppm S. A more realistic estimate for the Eagle
deposit also serves to illustrate that Ni contents in parental
magmas of ~150 ppm may give rise to sulfide assemblages
with tenors similar to those found in many deposits. Figure 1b
shows that sulfide saturation of a picritic magma contaminated with a partial melt from a pelite may occur at ~15%
crystallization. The Ni content of the liquid at this time would
be ~155 ppm. Crystallization of an additional 10% involves
clinopyroxene and results in the Ni content of the liquid
falling to no less than 140 ppm. The computed mass of
immiscible sulfide available for collection from the residual
liquid over this interval is ~0.3 wt %, resulting in an R-factor
of ~335. With Ni contents in the residual liquid of 140 to 150
ppm, R-factors of 200 to 350 will produce Ni tenors in the sulfide liquid of 2 to 3 wt %. Hence, collection of this sulfide
could generate an orebody similar in grade to many of the
world’s large deposits. For the small, 4-Mt orebody at Eagle,
the amount of silicate magma needed based on the above calculation is ~2 km3 .These values would appear to be very reasonable quantities of magma to be delivered in a developing
rift system. The example from the Sonju Lake intrusion also
serves to emphasize that if the amount of mantle-derived sulfide present in a moderate-sized, sheet-type intrusion were
to have been collected in a restricted magmatic conduit, an
FIG. 5. Plot of tonnes of sulfide in ore versus S concentration in a source magma. Cubic kilometers of magma are shown
assuming that all the sulfur in magma is collected to generate the ore. For example, if only 200 ppm S is available as immiscible sulfide during magma crystallization, deposits similar in size to those at Noril’sk (between 275 and 750 Mt) can be generated from between 200 and 300 km3 of magma. Small orebodies such as Eagle can be formed by collection of immiscible
sulfide from less than 10 km3 of magma.
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SULFIDE SATURATION IN MAFIC MAGMAS: IS EXTERNAL SULFUR REQUIRED FOR MAGMATIC Ni-Cu-(PGE) ORE GENESIS?
economic ore accumulation could have resulted. The conduit
environment provides a physical setting where small amounts
of sulfide from large volumes of magma may collect; in addition, subsequent upgrading may occur as sulfide-undersaturated magmas utilize the conduit and partially dissolve the
accumulated sulfide (e.g., Kerr and Leitch, 2005; Li et al.,
2009). Ni enrichment of a low-Ni sulfide that initially formed
from a system where Ni was sequestered by olivine could also
occur. Maier et al. (2001) pointed out the importance of conduits in the formation of magmatic Ni-Cu-PGE sulfide
deposits, as well as the lack of such deposits in large layered
intrusions. The point here is that geochemical data are consistent with the mineralization that is found in intrusions such
as Sonju Lake being related to processes that did not involve
the introduction of external S (or even significant contamination of any type). Had this sulfide been able to accumulate in
a conduit setting, there appears to be little reason to suspect
that an orebody could not have resulted. Barnes et al. (2011)
have recently described an Ni-rich disseminated sulfide orebody that occurs as a stratiform layer in the Fazenda Mirabela
intrusion of Brazil. The authors note that this is a very unusual
occurrence produced as a result of mixing of two compositionally distinct magmas, one of which contained suspended
sulfide droplets. δ34S values of sulfide minerals (–1.0–0.5‰)
are consistent with the premise that sulfur is of mantle origin
(Almeida Lazarin, 2011).
Isotopic data from Noril’sk (e.g., Gorbachev and Grinenko, 1973; Grinenko, 1985; Arndt et al., 2003; Li et al.,
2003b), Voisey’s Bay (Ripley et al., 1999, 2002), and Eagle
(Ding et al., 2012) indicate that externally derived S has
been involved in ore genesis in each of these systems. Sulfur
isotope data (e.g., Ripley et al., 2010) suggest that as much
as 50% of the S contained in the Noril’sk deposits is of country-rock origin; this permits the speculation that, considering the size of the Noril’sk deposits, economic deposits
could have formed even without the addition of external S.
Recent evaluations suggest that this is an unlikely scenario
(Keays and Lightfoot, 2010). However, it is clear that extremely efficient collection of mantle-derived sulfide from
appropriate volumes of magma will reduce the importance
of externally derived S in the formation of magmatic ore deposits. The fact that many large Ni-Cu-(PGE) deposits show
evidence for external S addition suggests that such efficient
collection of immiscible sulfide derived solely from mantle
S is a rare process. Early attainment of sulfide saturation
may be pivotal not only for Ni availability but also for potential sulfide collection in conduits prior to dissemination
within sheet- or sill-like intrusions. The external addition of
S to a mafic/ultramafic magma may not only supply additional sulfide mass, but also trigger early sulfide saturation
and, potentially, more rapid collection of immiscible sulfide
liquid. Given that early attainment of sulfide saturation is
possible in contaminated magma as we have shown above,
the mechanisms of collection of immiscible sulfide liquid remain as important topics for researchers concerned with the
genesis of magmatic Ni-Cu-(PGE) deposits. Mungall and Su
(2005), Chung and Mungall (2009), and de Bremond d’Ars
et al. (2001) have provided constraints on physical properties related to the collection of immiscible sulfide liquid
droplets. Additional research of this type is vital to enhance
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our understanding of all processes that may lead to the formation of magmatic Ni-Cu-(PGE) deposits.
Conclusions
An assessment of mechanisms that can promote sulfide saturation in mafic magmas indicates that externally derived S
may not be required for Ni-Cu-(PGE) ore formation in open
systems where the volume of magma involved is large and an
efficient process of sulfide collection is operative. Conduits
provide a physical environment where sulfide collection and
upgrading may occur, related in part to the passage of multiple pulses of magma. The fact that many large Ni-Cu-(PGE)
sulfide deposits show strong evidence for the incorporation of
crustally derived S suggests that efficient collection of mantle-derived sulfide is a rare process, and that sulfide supersaturation is often required. Sulfide supersaturation in magmas
is accomplished via the liberation of sulfur from xenoliths in
intrusions or via similar transport due to thermomechanical
erosion near the base of komatiite lava flows.
Closed-system fractional crystallization of mantle-derived
magmas will be unlikely to produce sulfide accumulations of
sufficient size for economic exploitation. Sulfide saturation in
most uncontaminated mantle-derived magmas will not occur
via fractional crystallization until ~20 to 40% crystallization.
Sulfide accumulations that may form will be Ni poor because
of sequestration of Ni by early crystallizing olivine. Systems
with sufficient volume have the potential to generate Cu-rich
PGE reefs. The contamination of mafic magmas by siliceous
country rocks, or mixing of magma types, will cause a reduction in the S concentration necessary for the attainment of
early sulfide saturation of between ~ 200 and 700 ppm. This
facilitates sulfide saturation but does not necessarily trigger it.
Where the aSiO2 is sufficiently elevated to cause orthopyroxene rather than olivine crystallization, more Ni is available for
incorporation into sulfide. Ni sulfide-rich ores could form
preferentially in orthopyroxene-bearing rocks, but only from
large-volume systems.
Addition of volatiles such as H2O and CO2 to mafic magmas
is frequently linked to an increase in magma fO2 and a lowering of the SCSS. Assimilation of oxygen-bearing volatiles does
not necessarily result in an increase of magma fO2; in addition,
at QFM and below an increase in fO2 results in only small
changes in the SCSS of the magma. Assimilation of siliceous,
and potentially hydrous, partial melts derived from country
rocks and mixing of chemically distinct magmas are more
viable processes for decreasing the SCSS of a mafic magma,
relative to increased fO2 alone. Methane, as well as graphite,
may serve as a reductant in high fO2 magmas where sulfate is
predominant and the solubility of S is considerably higher
than in reduced magmas.
Acknowledgments
Discussions with A.J. Naldrett, C.M. Lesher, R.R. Keays,
Jon Hronsky, P.C. Lightfoot, W.D. Maier, S.-J. Barnes, M.
Fiorentini, and S.J. Barnes regarding S saturation in mafic
magmas are appreciated and helped to stimulate the writing
of this manuscript. Reviews by Wolf Maier and Alexey Ariskin
improved the manuscript presentation. We thank Steve Barnes,
who served as associate editor for the manuscript, and Editor
Larry Meinert, for their comments and supervision. Research
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on magmatic ore deposits at Indiana University has been supported by NSF Grant EAR 1016031 to E.M. Ripley and C.
Li. A gift to the Indiana University Economic Geology program from Rio Tinto is gratefully acknowledged.
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