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1 University of Ottawa, Ottawa, Canada
2 99 Fifth Avenue, Suite 122, Ottawa, Canada
3 Geological Survey of Finland, Espoo, Finland
4 US Geological Survey, Spokane, USA
* E-mail: khattori{at}uottawa.ca
| ABSTRACT |
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All grains examined are solid solutions of Ru and Os with Ir (2.7111.76 wt.%) and Pd (0.310.66 wt.%). Their compositions are similar to laurite from ophiolitic rocks. The compositions show broad negative correlations between Os and Ir, between As and Ir, and between As (0.40.74 wt.%) and Se (140 to 240 ppm). Laurite with higher Os contains more Se and less Ir and As. The negative correlations between Se and As may be attributed to their occupancy of the S site, but the compositional variations of Os, Ir and As probably reflect the compositional variation of rocks where the crystals grew.
Ratios of S/Se in laurite show a narrow spread from 1380 to 2300, which are similar to ratios for sulphides from the refractory sub-arc mantle. Sulphur isotopic compositions of laurite are independent of chemical compositions and morphologies and are similar to the chondritic value of 0
. The data suggest that S in laurite has not undergone redox changes and originated from the refractory mantle. The data support the formation of laurite in the residual mantle or in a magma generated from such a refractory mantle, followed by erosion after the obduction of the host ultramafic rocks.
KEYWORDS: PGM, nugget, alluvial placer, placer deposit, electron-microprobe, stable-isotopes, osmium, SEM data, Kalimantan, trace-element geochemistry
| Introduction |
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Osmium isotopic data have contributed to the discussion. A relatively narrow spread of 187Os/188Os is used to support the mechanical derivation of PGM from Alpine-type and Alaskan-type intrusions (Hattori and Cabri, 1992; Cabri et al., 1996), and a considerable isotopic variation from PGM associated with large intrusions, such as those in Freetown Complex (Hattori et al., 1991), is explained by the isotopic heterogeneity of host igneous rocks (Hattori, 2002). However, in contrast, Bowles et al. (2000) attributed the variation of 187Os/188Os in PGM associated with the Freetown Complex to surface processes and crystallization of PGM in placers. Bird et al. (1999) found elevated concentrations of 186Os in leachates during acid extractions of Os from placer PGM associated with Josephine ophiolite, Oregon, and suggested their crystallization near the core-mantle boundary. In contrast, Meibom et al. (2002) attributed the variation of 186Os to heterogeneity of the upper mantle.
In order to constrain the origin of coarse-grained PGM, we determined the concentrations of As and Se and the S isotopic compositions, because these values are susceptible to hydrothermal and low-temperature processes.
| Sample locations |
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At the Tambanio locality, the laurite grains were collected from sediments in the main channel of the river, upstream from the junction with the westward-flowing Buluhembok River (Fig. 1a,b
). No other PGM were recovered at this site. Metasedimentary and metavolcanic rocks, tonalitic gneiss, and schist occur in the watershed immediately upstream of the laurite occurrence (Zientek and Page, 1990), but small northwest-flowing tributaries drain from ophiolite complexes of the Meratus Range to the site. The laurite is believed to have been derived from the ophiolitic rocks. The laurite locality is ~4 km upstream from the gold-PGE placers and lode occurrences described by Zientek et al. (1992). Burgath and Mohr (1986) and Burgath (1988) described the PGM-bearing ophiolites in the area.
Hattori et al.(1992) reported the occurrence of laurite grains and their Os isotopic compositions in chromitites of the Meratus Range ophiolite at Sungai Kalaan and compared the data with placer laurite grains collected from the streams draining from these ophiolitic rocks in the same area.
| Analytical procedure |
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, Ru-L
, Rh-L
, Pt-L
, Pd-Lß, As-Lß, Ni-K
. Standards are pure metals and alloys except for a pyrite standard for S-K
. Raw X-ray data were converted to wt.% using the Cameca PAP matrix correction program.
Minor element concentrations were determined using a Cameca SX 50 equipped with four wavelength-energy dispersive spectrometers. Se-L
on TAP As-Kß on LiF. As-K
was used for base metal sulphides, but not used for laurite because of overlaps with Os-Lß2. Instead, As-Kß was measured with LiF. Analytical conditions were 35 kV and beam current of 500 nA. Measuring time was 300 s for peak and 300 s for backgrounds. The minimum detection limits are defined as 3
Bx
t, where B is background count on either side of the peak and t the counting time. Under the analytical conditions above, the detection limits for Se are 15 ppm for laurite and 8 ppm for other sulphides, those for As are 370 ppm for laurite and 30 ppm for other sulphides. The proximity of Os-Kß to the As-Lß2 line and of the Os-Lß8 line to the Se-L
line raised the detection limit of As and Se in laurite. Standards used are pure metallic Se and cobaltite for As (45.2 wt.% As). Replicate analyses of 12 spots on different dates during the period between July, 2002, and May, 2003, show a reproducibility of <9% for Se and <5% for As. The detailed analytical procedure is essentially the same as that described by Robinson et al. (1998).
For S isotope analysis, laurite grains from Tambanio River were examined with a SEM-EDS without carbon coating and each grain (0.6 to 1.2 mg) was ground in an agate mortar together with V2O5 (1:3 weight ratio). The mixture containing ~0.050.59 mg of laurite was placed in tin foil and injected into a CE Elemental Analyzer. The samples were combusted at ~1700°C to release SO2. The SO2 gas was introduced to a Finnigan-Mat Delta Plus mass spectrometer for the isotope analysis after passing through 7 ml of silica at ~1000°C and Cu at ~600°C to buffer O isotopes and reduce SO3. Duplicate or triplicate analyses of all samples show a reproducibility of 30.2
. The standards used were: IAEA-S1 (0.3
) and IAES-S2 (+21.7
).
The XRD analyses were carried out on crushed grains and analysed using a Rigaku position-sensitive detector microdiffraction goniometer (PSD-MDG) at 50 kV, 180 mA, scanned over the range 570°2
.
| Results |
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One grain contains a spherical inclusion of a mixture of chalcopyrite, bornite, pentlandite and heazlewoodite (Fig. 4
). The texture between sulphide phases and the spherical outer shape (Fig. 4d
) suggests that the inclusion was once homogeneous Fe-Cu-Ni sulphide and exsolved into monosulphide solid solution (mss) and intermediate sulphide solid solution (iss). Further crystallization formed pentlandite and heazlewoodite from mss and bornite and chalcopyrite from iss. Another grain contains several inclusions of Ca amphibole (Fig. 2d
).
The crushed material from three grains gave a clean XRD pattern ascribed to laurite, with a cell edge a = 5.6117 Å. Taking an average composition of all laurites analysed (Table 1
) gives (Ru0.66Os0.28Ir0.06Pd0.01)1.01S2.00, which may be compared to 5.6089 Å, reported for laurite from Senduma Chrome Mines, Sierra Leone, with a more Ru-rich composition of (Ru0.84Os0.04Ir0.04)0.95S1.05 (Bowles et al., 1983).
Arsenic and selenium
All grains contain considerable amounts of Se and As, far greater than the detection limits of 15 and 370 ppm, respectively. The concentrations of Ir show a broad negative correlation with As (r = 0.77; Fig. 6a
) and positive correlation with Os (r = 0.83; Fig. 6b
). The As and Se contents show a broad negative correlation (r = 0.57; Fig. 6c
). Grains with greater Os contain less Ir (Fig. 6b
) and Se (Fig. 6a,c
) and more As (r = 0.94; Fig. 6d
). As mentioned above, the samples from Tambanio plot close to the end-member composition with high Ir and Se, and low Os and As.
The S/Se ratios of laurite show a narrow spread between 1380 and 2300 (Table 1
). The concentrations of Se in the sulphide inclusion show a considerable variation among different phases, with S/Se ratios varying from 3500 to 6560, but the concentrations are overall lower than the host laurite (Table 2
). The weighted ratio of As/S of the sulphide inclusion is 38x105, which is far lower than those of the host laurite, >1000x105. The data suggest that laurite incorporates As and Se in preference to base metal sulphides.
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34S values (+1.16±0.36
) and minor enrichment of 34S, but they are very close to the meteorite standard value of 0
. The values are independent of the morphology and the composition of the grains (Table 3
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| Discussion |
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Sulphur isotopic compositions
Sulphide formation in surface environments requires the reduction of dissolved sulphate. This reduction of sulphate, either by a kinetic or equilibrium process, at low temperature is accompanied by large isotopic fractionation and the product, S2, has low
34S, as much as 60
less than SO42values (e.g. Hoefs, 1997). In addition, dissimilatory sulphate-reducing bacteria, which probably participate in sulphate reduction in surface environments, produce S2 with variable isotopic compositions because bacterial reduction is affected by many factors, such as nutrient for bacteria, sulphate concentrations and bacterial population. Hence, sulphides formed near the surface show a large variation in
34S, as shown in many sedimentary rocks (Table 4
). Our data thus rule out laurite formation in near-surface environments, including "element agglutination" (Augustithis, 1965) or "accretion" of fine particles (Cousins, 1973; Cousins and Kinloch, 1976) during weathering and deposition of placers (Bowles, 1986, 1988; Barker and Lamal, 1989).
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34S is <2
, even after extensive degassing at magmatic temperatures. Therefore, the consistent S isotopic compositions, near meteoritic sulphur values of 0
, from the laurite samples studied indicate that their formation did not involve any oxidation-reduction of sulphide sulphur. Thus, the laurite formed under reduced conditions at deep levels in the crust or mantle (Table 4
Compositional variations
Laurite belongs to the isometric diploidal system, similar to pyrite. Pyrite and laurite contain divalent metals (Fe2+, Ru2+, Os2+, Ir2+) and two covalently bonded sulphur atoms as a dianion. Pyrite can accommodate significant amounts of As, and most of the As replaces S, forming (As-S)2 (Fleet et al., 1993). Pyrite with high concentrations of As may contain thin, 10 to 15 Å, layers of arsenopyrite-like structure (Simon et al., 1999). Irarsite (IrAsS) and ruarsite (RuAsS) belong to this arsenopyrite group with a crystal configuration similar to that of arsenopyrite.
The correlation between As and Se is, therefore, easily understood, considering that both elements occupy the S site, forming (As-S)2 and (Se-S)2. There are fewer S atoms in As-rich laurite. In addition, anion pairs of (Se-As)2 may not be easily formed in the structure.
The laurite samples studied also display correlations among metal ions. The atomic ratio of Os to Ir is 1.2, which suggests the two heavy atoms are nearly substituting for each other. However, the atomic ratios of Ir/As and As/Se are 18 and 71, respectively. This means that the loss of 18 atoms of Ir corresponds to an increase of 1 atom of As and 71 atoms of As to 1 atom of Se. The observed compositional variations may be attributed to either crystallographic effects or compositional control of the environment for crystal growth.
We suggest the latter. First, the correlations between Os and Ir and between Ir and As are not easily explained by the crystallographic configuration, because these three metals form divalent cations. In addition, Ru and Os should be interchangeable in the crystal considering that the two have very similar ionic radii and electro-negativities. Thus, high Ir concentrations in low-Os laurite are attributed to an external cause, the compositional variation of rocks where the laurite grains crystallized. Our proposed interpretation is further supported by the compositions of laurite from other locations (Figs 7
and 8
). For example, laurite from the Bushveld Complex shows a wide range of Ir almost independent of Os content (Fig. 7
), but a broad positive correlation between Ir and As (Fig. 8
). Considerable compositional variation in a single sample is also noted in the western Bushveld Complex (Maier et al., 1999). Laurite grains from other ophiolitic rocks also show a wide scatter without any apparent correlations on the diagrams of Os vs. Ir and Ir vs. As (Fig. 8
).
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The apparent distribution coefficient for Se, KSe, is ~3.0. The value is large, probably due to low-temperature re-equilibration, considering the rapid diffusion of Se in sulphides (e.g. Bethke and Barton, 1971). Nevertheless, the data suggest that laurite preferentially incorporates Se compared to base metal sulphides.
Variations of S/Se ratios
Surface waters contain very low Se (i.e. high S/Se ratios) because of the sluggish oxidation of Se. This is reflected by low Se in sulphides in most clastic sedimentary rocks, evaporites and seawater, S/Se > 100,000 (Measures and Burton, 1980; Fig. 9
). Selenium may be enriched in Fe-oxide chemical sediments due to strong adsorption of SeO32 on an oxide surface and may also be enriched in organic-rich black shales formed in anoxic basins (e.g. Stanton, 1972; Howard, 1977), but these cases are not applicable to the studied samples. Thus, the S/Se data from the laurite grains studied are not consistent with their formation in surface environments (Table 4
).
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(1) Selenium and S are fractionated in solutions near the redox boundary of S. When S is oxidized to form SO42 and HSO4, Se remains as H2Se, Hse and Se2. Thus, the S2/Se2 ratios in solutions near the redox boundary of sulphur vary widely due to oxidation of S. Sulphides formed from such solutions show a large variation in S/Se ratio. This is not applicable for the studied samples because the sulphur isotopic data indicate no redox change of S.
(2) Incursion of surface waters may cause a large variation of S/Se ratios because surface waters show very high S/Se ratios due to sluggish oxidation of Se. For example, seawater shows ratios > 4x108 (e.g. Measures and Burton, 1980).
(3) The remaining possibility is the removal of different sulphide phases and melt. Laurite preferentially incorporates Se compared to base-metal sulphides, as shown in the fractionation of Se among sulphide grains. Ruthenium and Os are considered to be refractory metals, retained in the mantle during partial melting. In contrast, Cu and Fe are incompatible with mantle minerals and are preferentially removed from the mantle during partial melting. Thus, partial melting and removal of base metal sulphides would lead to the enrichment of Se (lower S/Se) in the mantle. This is further supported by low S/Se ratios of sulphides found in refractory mantle underlying arcs (Hattori et al., 2002). Low S/Se ratios of the studied laurite samples, therefore, probably reflect the origin of S in laurite from a refractory mantle. We, therefore, suggest that the laurite grains crystallized either in the upper refractory mantle or in the cumulates of mafic magmas that were derived from such a refractory mantle.
The proposed interpretation implies high-temperature crystallization of laurite and this is consistent with experimental data on the stability of laurite (Andrews and Brenan, 2002).
| Conclusions |
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Values of
34S for all PGM studied are similar, near 0
. The consistent S isotopic values near chondritic composition discount their crystallization at moderate to low temperatures at shallow crustal levels. Instead, they formed at depth where S has not undergone redox changes.
| Acknowledgements |
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We thank Alan Hart, Natural History Museum, London, for the laurite grains from the type locality (Pontyn River), Monika Wilke-Alemany for sample preparation in the laboratory, Paul Middlestead and Wendy Abdi, the University of Ottawa, for maintenance of the mass spectrometry laboratory, and Peter Jones and Lew Ling, Carleton University, for assisting with the SEM and electron probe analysis, and to John Wilson, CANMET/MMSL for the XRD analysis. We are also grateful to Ernst A.J. Burke of Vrije University for the information on the occurrence of the Pontyn laurite, Chris Stanley, Natural History Museum, London, for sending us a polished section containing PGM from Rio Pilpe, Colombia, that he and Alan Criddle had studied, even though it was not used in this study. LJC acknowledges the technical support provided by CANMET during his tenure as Emeritus Research Scientist. This project was funded by a NSERC grant to KHH. Comments by A. Bookstrom and S. Box, USGS, and by journal reviewers Baruch Spiro and Adrian Boyce helped to improve the manuscript.
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[Manuscript received 4 August 2003: revised 13 January 2004]
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