copper-gold ore from west papua, indonesia
TRANSCRIPT
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Ore Geology Reviews 2
A Re–Os isotope study of sedimentary rocks and copper–gold ores
from the Ertsberg District, West Papua, Indonesia
Ryan Mathura,b,T, Spencer Titleya, Joaquin Ruiza, Stacie Gibbinsa, Kurt Friehauf c
aDepartment of Geosciences, University of Arizona, Tucson, AZ 85721, USAbDepartment of Geology, Juniata College, Huntingdon, PA, 16652, USA
cDepartment of Physical Sciences, Kutztown University, Kutztown, PA 19530, USA
Received 1 November 2003; accepted 21 July 2004
Available online 17 March 2005
Abstract
The ores of the Ertsberg district consist of both porphyry stockwork and contact controlled mineralization related to the
Grasberg and Ertsberg intrusion centers. High-grade copper mineralization with gold occurs in skarns on the periphery of each
of the intrusion centers. The periphery mineralization includes the Kucing Liar skarn-related ores, the massive sulfide lenses on
the borders of the Grasberg Intrusive Complex, and the giant skarn bodies of the Deep and Intermediate Ore Zones, together
with the ores of the Dom complex on the margin of the Ertsberg diorite. The Ertsberg orebody, the basis of discovery of the
district, is a copper–gold, roof-pendant of sedimentary strata in the diorite. In order to clarify genetic and geochronologic links
between the peripheral sediment-hosted ore bodies and the intrusion-hosted ore bodies, Re–Os isotopes of the ores and
subjacent Precambrian and Phanerozoic crust were analyzed. Re–Os geochronology of molybdenites was used to resolve the
age relationships of the ore bodies. The Grasberg and Kucing Liar molybdenites have older molybdenite mineralization ages of
2.88F0.02 Ma, and 3.01F0.02 Ma, respectively, whereas the Ertsberg molybdenite has a younger age of 2.54F0.02 Ma.
These data agree with Ar chronologies of the alteration associated with mineralization (Pollard and Taylor, 2000 [Pollard, P.J.,
Taylor, R., 2000. Geochronology of intrusive rocks and Cu–Au mineralization in the Ertsberg District. In: Proceedings of
Freeport-Institut Teknologi Bandung (ITB) Geological Symposium, Bandung, Java, pp. 17–19.]), and also indicate that the
Grasberg and Kucing Liar molybdenites are closely similar in age, and older than the Ertsberg Intrusive System.
Re–Os data from pyrite, chalcopyrite, magnetite, gold, and the surrounding sedimentary rocks from the district define a
mixing relationship between samples from the initial stockwork mineralization and peripheral ores of each intrusion center.
Sulfide and oxide minerals from primary stockwork mineralization are isotopically homogeneous and define trends on isochron
diagrams with distinct Os initial ratios, whereas sulfides and oxides taken from peripheral ores are isotopically heterogeneous
and define trends on mixing diagrams. One possible end member for the mixing is sedimentary rock surrounding the
porphyries. The measured Os ratios of the sedimentary rocks range from 0.52 to 2.21, and overlap the Os initial ratios of the
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6 (2005) 207–226
ee front matter D 2005 Elsevier B.V. All rights reserved.
egeorev.2004.07.001
ng author. Department of Geology, Juniata College, Huntingdon, PA 16652, USA. Tel.: +1 814 641 3725; fax: +1 814 641
ess: [email protected] (R. Mathur).
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226208
sulfides and oxides sampled from both stockwork and contact mineralization. The data suggest a model in which the continental
crust supplied some of the Os (and by inference other metals) during magma genesis in the lower crust and the remainder came
from sedimentary rocks near the intrusion centers.
D 2005 Elsevier B.V. All rights reserved.
Keywords: Re–Os; Porphyry copper deposit; Gold; Ertsberg
1. Introduction
The origin of gold in various types of epigenetic
mineral deposits remains enigmatic; consequently,
their origin has been a major question in economic
geology and in mass balance considerations con-
cerning the role of the crust and mantle as metal
sources in ore genesis. Two possible sources have
been suggested for metals in most ore deposits.
The most commonly suggested possibility is that
metals are derived directly from the magma.
Possible sources for metals in magmas include an
enriched mantle wedge, the subducted slab, and
assimilation of continental crust (Burnham, 1959;
Krauskopf, 1967; Noble, 1970; Sillitoe, 1972;
Zartman, 1974; Titley, 1991; Goldfarb et al.,
2001). In the simplest case, such as porphyry-
related deposits, the metals are thought to be
concentrated in a fluid exsolved from a cooling
magma and deposited in metal-rich minerals. A
second possible source for metals is wall rocks
surrounding the magma and ore deposit. In this
case, as the intrusion cools, exsolved fluid leaches
metals from the surrounding crust. Few studies
have provided evidence for the source of Au and
other metals in ores (McInnes et al., 1999; Mathur
et al., 2000; Kesler et al., 2002; Kirk et al., 2002).
In this study, we consider both the magma and the
surrounding crust as a source for metals by use of
Re and Os isotopic compositions of sulfide ore
minerals and wallrocks in the Ertsberg district.
Mathur et al. (2000) presented the first Re–Os
evidence demonstrating that both sources might be
important in the Ertsberg district. This study examined
two distinctly different kinds of mineralization asso-
ciated with the porphyry stock, typical primary
stockwork porphyry copper mineralization and mas-
sive sulfide ores that border the deposit. The Os
isotopic composition of the sulfide minerals suggested
two distinct crustal sources of Cu–Au for the two
types of ore:
1. Os in stockwork mineralization, which is isotopi-
cally homogeneous, was interpreted to come from
magmas generated from both mantle and crust and
mixed at depth.
2. Os in massive sulfide mineralization, which is
isotopically complex and heterogeneous, was
interpreted to have been scavenged from adjacent
wall rocks by circulating hydrothermal fluids.
The results and ideas presented in this earlier study
have been tested further here by examination of
different parts of the ore-forming system and analyses
of samples from other parts of the Ertsberg district.
Our new results reveal clear isotopic signatures typical
of a crustal source in ore minerals of the district.
Consequently, we propose that consideration be given
to the continental crust as a source for Os in this and
other ore systems.
1.1. Rationale and objectives
Re–Os isotope analyses are carried out on ore
minerals and therefore provide data that are more
directly related to the source of ore metals than other
isotopic analyses carried out on alteration minerals
(Luck and Allegre, 1980; Shirey and Walker, 1998).187Os is derived from the decay of 187Re that has a
half-life of 41.6 billion years. Because Re is orders of
magnitude more incompatible than Os in the rocks
and minerals of the mantle (Walker et al., 1989,
Righter and Hauri, 1998, Burton et al., 2002, Brenan
et al., 2003), any crustal material derived from the
mantle has a greater Re/Os ratio than the mantle and
will evolve greater 187Os/188Os ratios than the mantle.
For the purposes of this study, the presence of187Os/188Os initial ratios significantly greater (N0.15)
Fig. 1. Location map of the Ertsberg area (after Rubin and
Kyle, 1997).
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 209
than the mantle (~0.13, Meisel et al., 2001) indicates a
crustal source for Os. The mantle from which the
magmas that are responsible for mineralization in the
Ertsberg district came may have a slightly greater187Os/188Os (perhaps 0.15) because the exact187Os/188Os of the mantle wedge in subduction zone
environments is most likely not constant. There is
some evidence that the mantle wedge in arc environ-
ments does have 187Os/188Os values greater than
~0.13. For instance, McInnes et al. (1999) and Widom
et al. (2003) suggested that metasomatized portions of
the mantle have measured 187Os/188Os of up to 0.17,
although Chesley et al. (2004) demonstrated through
the used of chemical mixing diagrams that the187Os/188Os value of metasomatized mantle is no
greater than 0.15.
Questions remain regarding the utility of Re and
Os as a geochemical tracer for the source of base
metals. Goldschmidt originally defined Re and Os as
chalcophile and siderophile elements, thus their
general behavior during magma generation and ascent
to the surface is similar to the behavior of other base
metals. Roy-Barman et al. (1998) confirmed this
relationship by finding that the sulfide blebs in
MORB contained more Re and Os than the surround-
ing matrix. Experimental studies by Sattari et al.
(2002), Peach and Mathez (1996), and Barnes et al.
(1985) further demonstrate that Re and Os readily
partition into immiscible sulfur-rich melts in mafic
magmas. No information is available on the partition-
ing of rhenium and osmium between magmas and
coexisting hydrothermal solutions, but Xiong and
Wood (2000, 2001) have demonstrated that Os can be
transported in hydrothermal solutions associated with
porphyry copper deposits. Their experiments were run
at a pH of 5 and temperatures between 400 and 500
8C. Their results suggest that Os is transported and/or
present as a chloride complex and that fluids
associated with porphyry copper deposits are capable
of transporting enough PGE to produce a mid-sized
PGE deposit, and they identified several deposits that
contained the predicted amount of PGE. However,
they recognized that Re and Os in mantle sulfides may
not be completely soluble in the magma thus explain-
ing some of the variations in PGE concentrations
measured in porphyry copper deposits. Xiong and
Wood (1999) also found that Re is highly soluble in
Cl-rich fluids and can be transported in solutions
similar to those associated with porphyry copper
deposits. They noted that the behavior of Re would
most likely change with the addition of sulfur causing
most of the Re and Os to be associated with the sulfur
rich fluid. Suzuki et al. (2000) noted that both
elements can be leached from molybdenite and they
suggested low temperature, saline fluids could also
transport Re and Os. These observations show that the
behavior of Re and Os in magmatic and hydrothermal
systems is sufficiently similar to that of base and
precious metals for it to be used as a tracer for these
elements in efforts to define metal sources.
Molybdenite contains orders of magnitude more
Re than the common sulfides and effectively no initial
radiogenic 187Os (Luck and Allegre, 1983). Therefore,
it can be used as a precise geochronometer (e.g.,
McCandless and Ruiz, 1993; Stein et al., 1998; Selby
et al., 2002).
2. The Ertsberg/Grasberg system
Ore deposits of the Ertsberg district (Figs. 1 and 2)
compose one of the largest and richest porphyry and
skarn copper–gold systems on earth (Van Nort et al.,
1991; Freeport McMoRan, 1997, 1998; Meinert et al.,
1997) and formed due to a series of complex tectonic
events. New Guinea resulted from the collision,
during Oligocene time, between the northward mov-
ing Australian continental plate and an island arc
within the southward moving Pacific-Indo Plate (e.g.,
Dewey and Bird, 1970; Van Nort et al., 1991;
MacDonald et al., 1995). Accretion of this island arc
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226210
created a suture zone that attached slices of ophiolite
and oceanic sedimentary units from the Pacific Plate
to the northeastern margin of the Australian continent
(Hamilton, 1979). Compressional stress continued and
rapid uplift ensued (Weiland and Cloos, 1996),
creating the Papuan Fold and Thrust Belt (Central
Mobile Fold and Thrust Belt), south of the suture. The
over-thickened crust contributed to the formation of
partial melts, probably through anatexis (MacDonald
et al., 1995; Housh and McMahon, 2000), which
resulted in substantial calc-alkaline to alkaline igneous
activity along the Lagaip Fault Zone during the
Pliocene (e.g., McMahon, 1994; Rubin and Kyle,
1997). Both the Grasberg Intrusive Center and the
Ertsberg Intrusive System are products of this activity.
The magmas associated with mineralization
intruded highly deformed Paleozoic and Mesozoic
sedimentary rocks. Housh and McMahon (2000)
used U–Pb and Sm–Nd geochemistry to determine
that Proterozoic to Archean crust were significant
contributors to the source of magmas related to
mineralization.
Styles of mineralization in the two centers contrast
in significant ways. The Grasberg Intrusive Center
comprises three distinct stages of intrusions, from
monzodioritic to monzonitic in composition. The
oldest and largest intrusive mass of the Grasberg
Intrusive Center is the Dalam Fragmental, a funnel-
shaped body in the sedimentary host rocks. The
Dalam Fragmental unit is a clast-supported breccia
unit with dioritic matrix and clasts. The center of the
Dalam Fragmental is cut by the Main Grasberg
Intrusion, a monzonite (MacDonald and Arnold,
1994). The Kali dike swarm is the youngest intrusive
event in the Grasberg Intrusive Center. Ore reserves
and resources in the Grasberg Intrusive Center are
approximately 2000 Mt @ 1% Cu and 1.2 g/t Au.
Both the porphyry and surrounding breccia masses
host stockwork mineralization. This mineralization is
characterized by chalcopyrite in an assemblage with a
high chalcopyrite: pyrite ratio (N5) with iron occur-
ring mostly in magnetite. The dominant silicate
alteration phase found in the system is orthoclase.
Adjacent to the Grasberg Intrusive Center is the
Kucing Liar ore body, located between the southern
contact of the Grasberg Intrusive Center and the
Idenberg No.1 fault, approximately 1000 to 1500 m
below the present surface. Kucing Liar is an Mg-skarn
hosted in the Cretaceous Kembelangan Ekmai lime-
stone, and limestones/dolomites of the Tertiary New
Guinea Group Carbonates, and has a resource and
reserve of 320 Mt @ 1.4% Cu and 1.4 g/t Au.
Although the Kucing Liar is not in direct contact with
the Grasberg Intrusive Center unit, its proximity
(~200 m) to the Grasberg Intrusive Center is a
compelling argument for a genetic relationship.
The Ertsberg Intrusive System, in contrast, is a mass
of holocrystalline pyroxene-diorite with wall rocks
containing forsterite–monticellite–diopside skarns
with copper and gold (Rubin and Kyle, 1998). The
original Ertsberg Orebody, which was rooted in the
Ertsberg Intrusive System, consists of the Ertsberg
diorite, an equigranular, phaneritic intrusion that
constitutes most of the Ertsberg Intrusive System, and
a series of 1108 trending porphyritic dikes of diorite to
monzodiorite composition that parallel its northeastern
boundary (Friehauf et al., 2000). Within the diorite
mass, stockwork fractures are mineralized mostly by
bornite and magnetite in magnetite–chlorite altered
rocks. The Ertsberg stockwork zone is proximal to the
series of porphyry dikes, and has reserves and
resources of 100Mt@ 1%Cu and 1 g/t Au. Proximally
associated with the Ertsberg Intrusive System are calcic
and magnesium skarns, occurring as either roof
pendants or at the wall rock-intrusion contact. Exam-
ples of these skarns are the Gunung Bijih, Dom, West
Hanging Valley, and massive skarns along its north-
eastern contact (Fig. 2). The Dom is located on the
southern periphery of the Ertsberg Intrusive System.
The Dom ore body is a monticellite–forsterite–garnet
skarn, with retrograde alteration of specular hematite–
calcite–anhydrite–chalcopyrite. Dom is a 31 Mt
resource and reserve with 1.67% Cu and 0.47g/t Au
(Freeport Mining Report, 1998).
2.1. Mineralogical setting of Au and Cu
In the Grasberg Complex, copper mineralogy is
dominated by chalcopyrite whereas in the Ertsberg
Complex, copper is mostly in bornite. In the district,
gold is most frequently observed as inclusions in or on
the rims of chalcopyrite, bornite, and to a lesser extent
pyrite (Rubin and Kyle, 1997). Gold occurs with
bornite and chalcopyrite in the Ertsberg skarns. In the
Grasberg ore body, some Au occurs in veins and
fillings. Our petrographic observations of the samples
Fig. 2. Geologic map of the Ertsberg area. Numbers on the map indicate sample locations. Dark black line represents location where the drill
core samples for the study by Mathur et al. (2000) were taken.
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 211
analyzed in this study confirm that most of the Au is
included in or associated with sulfide phases. In order
to further understand the Os signature in gold, we
analyzed a pure gold separate. The gold sample
consisted of very fine-grained fragments that were
separated from fine-grained copper rich ores by
gravitational and centrifugal methods.
3. Sampling and analytical techniques
All ore samples were taken from drill core or hand
specimens collected underground and in the active pit.
Fig. 2 and Tables 1 and 2 provide sample location and
mineral/rock descriptions. There are both high and
low concentrations of Re and Os in the mineral suites
analyzed.
Molybdenite is not a common phase in this district
and its relative scarcity limited this study to only three
samples. The ages obtained from these molybdenite
samples will be compared with crystallization and
alteration ages taken from the literature to further
understand the timing of mineralization and alteration.
A debate surrounds ways to determine whether the
Re–Os isotope system in molybdenite has been altered
since it was deposited. This is an important point
when looking at complex hydrothermal systems (such
as porphyry copper deposits) where multiple miner-
alization and alteration events overprint one another.
McCandless et al. (1993) suggested several ways to
detect alteration of the Re–Os system in molybdenite.
McCandless et al. (1993) also argued that samples
with Re rich clay overgrowths produced geologically
unreasonable ages. Suzuki et al. (2000) investigated
the suggestions of McCandless et al. (1993) by
conducting laboratory experiments using low temper-
ature, saline fluids to alter molybdenites. Their results
did not indicate that changes in crystallography
accompanied the alteration of the Re–Os system in
molybdenite. Therefore, they strongly suggested that
Table 1
Description of analyzed ore and sedimentary rocks samples, from a suite of 25, collected along the GBMA Road, West Papua, Indonesia
Sample names Description
MGI Grasberg cpy Main Grasberg Intrusion cpy: Irregular 1–2 cm wide chalcopyrite lens within quartz vein.
Host rock is quartz–biotite-altered Main Grasberg Intrusive rock.
Erts cpy 1 Underground sample of cpy–py–mo mineralization from a quartz vein in the Ertsberg Diorite.
Vein selvage is principally quartz–sericite and wall rock is K-altered Diorite.
Erts cpy 2 Ore sample (10 cm�10 cm) of high-grade skarn ore from the original Ertsberg
orebody-provided by Frank Nelson. The sample is that of a magnetite–chalcopyrite
pseudo-breccia or an original mass of replaced magnetite. Mineralization associated with
marginal bands of forsterite and magnetite.
Erts cpy 3 Sample of mineralization from the Ertsberg orebody-provided by Frank Nelson. The sample
represents skarn associated chalcopyrite blebs in a mass of magnetite. The host was within the
sedimentary strata of the Kembalagan Group.
Erts cpy 4 Underground sample of quartz–vein mass of chalcopyrite and bornite from the stockwork zone
of the Ertsberg Diorite Wallrock alteration of the diorite appears feldspar-stable.
KL 36-7 332 Massive magnetite replacement of probable carbonate beds in Tertiary strata bordering lenses
of serpentinized carbonate and clay-altered sandstone. NQ Drill core.
KL 36-7 302 Chalcopyrite and pyrite (replacement) in magnetite–serpentine-altered Tertiary strata. NQ Drill core
KL 36-7 300 Mixed lenses or veins of pyrite and chalcopyrite in massive magnetite rock within serpentine-altered
sedimentary strata, below KL36-7 300 NQ Drill core.
DOM Massive sulfide replacement of tertiary clastic in contact with magnetite lens. Alternating layers
of mixed pyrite and chalcopyrite.
GBMA-1 Kariem Formation, A Member (Proterozoic–Cambrian). Thinly-laminated grey to black mudstone
(Phyllite) ~20 m above basal contact with Awatagon Formation.
GBMA-7 Kariem Formation, B Member. (Proterozoic–Cambrian). Compact to thinly-laminated black
mudstone from 20 m thick layer between fine-grained sandstone units. Near center of mapped
unit, ~1000 m above base.
GBMA-10 Tuaba Formation. Possibly Ordovician, mapped by Quarles van Ufford as Proterozoic–Cambrian.
Sample is medium-grained cross-bedded sandstone from lower third of section.
GBMA-12 Modio Formation. (Devonian–Silurian). Sample is from Quarles van Ufford’s A member, a black weathering,
white, algal dolostone. Collected at Tunnel entrance.
GBMA-20 Tipuma Formation. (Triassic–Jurassic). Sample is massive red, green-mottled siltstone, collected
from ~200 m below the top of the 2400 m thick formation.
GBMA-21 Kopai Formation (Basal Formation of the Kembalangen Group) Cretaceous to Jurassic age. Sample
is weakly calcareous, black mudstone.
GBMA-22 Kopai Formation. Sample is black mudstone to shale. Collected ~100 m up-section from GBMA-22.
GBMA-23 Kopai Formation. Sample is calcareous black shale 1000 m above GBMA-22, 23.
Analytical data are shown in Tables 2 and 3 and locations in Fig. 4. Nomenclature and ages of the sedimentary strata are extracted from and
adapted from Quarles van Ufford (1996). cpy=chalcopyrite.
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226212
repeat analyses of molybdenite samples are necessary
to indicate that samples have not experienced alter-
ation of the Re–Os system.
Stein et al. (2001, 2003) and others pointed out that
Re and Os can be decoupled and indicate that all
molybdenite samples that are ground to become
homogenized produce the most geologically reason-
able ages. They suggest multiple analyses of the
sample to ensure reliable age determinations. Further
discussion of this topic can be found in McCandless et
al. (1993), Stein et al. (1998, 2001), Xiong and Wood
(1999), Suzuki et al. (2000), Selby and Creaser
(2001), and Barra et al. (2003).
Rock and ore samples for this study were
wrapped in paper, crushed, and handpicked to
obtain a pure sample of molybdenite. Pure molyb-
denite samples were powdered for analysis. Microp-
robe analyses of the samples did not reveal any Re
rich clay overgrowths, and the samples have the 2H
crystal structure. Replicate samples were run for the
Kucing Liar sample to demonstrate reproducibility
of the technique and homogeneity of the sample.
Table 2
Sample descriptions and Re–Os data
Sample name Location Phase Re (ppt) Os (ppt) 187Re/188Os 187Os/188Os 187Os/188Osi Au (ppb) 187Os/188Osi age
MGI Grasberg
cpy
Fig. 1 #1 cpy 74 60 6.64F1 0.872F0.008 0.87
Grasberg Au Composite
Au sample
Au 578 873 3.65F0.13 1.237F0.003 1.23
Erts cpy 1 Fig. 2 #2 cpy 2206 4 7955F1500 0.68F0.15 0.26F0.13
Erts 2 mg+cpy Fig. 2 #3 mg 3384 6 2781F255 0.48F0.03 0.36
Erts 2 mg+cpy Fig. 2 #3 cpy 11,308 5 10,893F950 0.66F0.04 0.22
Erts 3 cpy+mg-2 Fig. 2 #3 mg 1516 8 945F71 0.41F0.02 0.37
Erts 3 cpy+mg-2 Fig. 2 #3 cpy 1038 8 676F51 0.46F0.02 0.44
Erts 4 cpy-1 Fig. 2 #3 cpy 11,185 9 7662F590 0.69F0.04 0.26F0.13
Erts 4 cpy-1 Fig. 2 #3 cpy 8802 8 5492F412 0.56F0.03 0.26F0.13
KL 36-7 332 Fig. 2 #4 mg 1657 33 254F5 0.59F0.01 0.58F0.01
KL 36-7 302 Fig. 2 #4 cpy+py 16,905 183 492F2 0.945F0.005 0.922F0.005
KL 36-7 300 Fig. 2 #4 cpy+py 18,011 65 1474F15 0.88F0.01 0.81F0.01
KL 36-7 332 Fig. 2 #4 cpy 2119 40 275F5 0.71F0.01 0.77F0.01
KL 36-7 332 Fig. 2 #4 mg 2619 51 264F4 0.59F0.01 0.58F0.01
DOM Fig. 2 #5 mg 28,167 341 424.4F0.9 0.627F0.002 0.606F0.002
BS Karim-1 Fig. 4 mdst 20 18 7.2F1 1.56F0.1 1.63 5
BS Karim-7 Fig. 4 mdst 7 1.44F0.21 58
BS Kem-22 Fig. 4 bs 173 263 3.38F0.1 0.528F0.001 5
BS Kem-22-2 Fig. 4 bs 201 0.532F0.002 5
BS Kem-23-2 Fig. 4 bs 468 0.831F0.001
BS Kem-23-1 Fig. 4 bs 399 0.804F0.002
Arkose Tri 20-1 Fig. 4 ark 10 2.21F0.18 5
Dev LS 12 Fig. 4 ls 5 3.79F0.71
BS 20-1 Fig. 4 bs 30 1.58F0.04 12
Error treatment is discussed in the article. Gold analyses were completed by Skyline Labs, Tucson AZ. Abbreviations: cpy=chalcopyrite,
mg=magnetite, py=pyrite, mdst=mudstone, bs=black shale, ark=arkose, ls=limestone, mly=molybdenite. Column labeled 187Os/188Osi=Os
initial ratio calculated from isochron plots, 187Os/188Osi age=Os initial ratio calculated for the Ertsberg skarn ores using the molybdenite age of
2.54 Ma.
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 213
We used the carius tube method (Shirey andWalker,
1995) for sample digestion, and distillation for extrac-
tion of Re and Os from all ores and sedimentary rocks
(Frei et al., 1998; Mathur, 2001). Concentrations were
determined by isotope dilution, and we used two non-
3.63.43.23.02.82.62.42.2
GrasberKucing Liar
Age
(M
a)
Fig. 3. Comparison of KAr, 40Ar39Ar, and Re–Os geochronologic informati
5 =Average age of 40Ar–39Ar analyses from Pollard and Taylor (2001); x
mixed spikes, 185Re enriched spike (161.58 ppm) and190Os enriched spike (99.84 ppb) for molybdenite
separates and 185Re enriched spike (6.72 ppb) and190Os enriched spike (1.11 ppb) for lower concen-
tration samples. Samples were measured on a Negative
g Ertsberg
on. o =Average age of K–Ar analyses from McDowell et al. (1996);
=molybdenite ages from this contribution.
0 5
kilometers
2Km
4
pCkt
TnTnTnTnTn
A A'
A
A'
Rock Types:
Ds Pa JtiaKk
PintpCka pCkb
pCka- Kariem Fm. A Member
pCkb- Kariem Fm. B Member
pCt- Tuaba Fm.
Ds- Modio Fm.
Pa- Aiduna Fm.
Jtia- Tipuma Fm. Kk- Kopia Fm. Pint- Grasberg Igneous Intr.
Tn- Tertiary Ls.
137° 00' E 137° 02' E
137° 04' E 137° 06' E 137° 08' E 137° 10' E
137° 04' E
4° 04' S
4° 10' S
4° 12' S
4° 08' S
4° 10' S
4° 12' S
4° 14' S
4° 16' S
Kopai Fm. (Jur.-Cret.) Tipuma Fm. (Tr.Jur.)Aiduna Fm. (Perm)Modio Fm, B member (Sil.-Dev.)Modio Fm, A member(Sil.-Dev.)Tuaba Fm.(Precamb.-early Palazoic)Kariem Fm, B member(Precamb.-early Palazoic)Kariem Fm, A member(Precamb.-early Palazoic)
KJkoJTtPaDSmb
DSma
pCt
pCkb
pCka
Kembalangan (J-K)and New GuineaLimestone (Tert.)Groups, Undivided
Enlarged area
GBMA 23
GBMA 22
GBMA 21
GBMA 20
GBMA 7
GBMA 1
GBMA 10
GBMA 12
35
KJko
JTt
JTt
Pa
DSmb
DSmapCt
pCkb
pCka
Fig. 4. Sketch map showing generalized geologic section and location of sedimentary rocks that were collected. Enlarged area of the map is
shown in detail in Fig. 2.
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226214
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 215
Thermal Ionization Mass Spectrometer, using loading
and instrument procedures that are described in Creaser
et al. (1991).
Molybdenite ages are calculated by assuming no
initial 187Os (these are reported in Table 3; Fig. 3),
similar to McCandless and Ruiz (1993). Fig. 3
summarizes the different types of geochronologic
information taken from all the deposits in the district.
The plot compares molybdenite ages to 40Ar/39Ar and
K–Ar ages from silicate alteration minerals from the
respective deposits. The decay constant we used for187Re is 1.666�10�11 yr�1 F1% (Smoliar et al.,
1996). Errors are calculated based on the calibration
of the spike (0.22–0.4%), and the uncertainty of the
decay constant of Re. Replicate analyses indicate an
error on analysis of F0.5% for each element.
We analyzed materials with lower Re and Os
concentrations than the molybdenites, including sedi-
mentary rocks, pyrite, gold, magnetite, and chalcopyr-
ite. Sedimentary rocks were collected on the Gunung
BijihMine Access Road (GBMA; Fig. 4) a mining road
leading to the ore deposit. The road bisects the limb of a
syncline that exposes a relatively complete section of
the northward-dipping, late Precambrian through Cen-
ozoic sedimentary rocks. The down-dip projection of
this section lies beneath the mining district and was
crossed by magmas that formed the porphyry copper
deposits. We sampled shales, arkoses, limestones, and
mudstones across this thick succession of sedimentary
strata (Fig. 4). The pure Au sample was provided by
Freeport McMoRan Inc. (labeled Grasberg Au in Table
2) and is a composite metallurgical concentrate of many
ores from the Ertsberg district. According to esti-
mates based on proportions of ores taken from the
district, probably 95% of the Au in this concentrate
originated from the Grasberg Intrusive Center. The
other sulfide and oxide samples were collected
underground from drill core, or taken directly from
the operating pit.
Table 3
Molybdenite ages
Sample name Location 187Re (ppm) 187Os (pp
Grasberg Fig. 2 #6 1405.5 (4) 67.55 (3)
Kucing Liar Fig. 2 #4 98.91 (4) 4.981 (2)
Kucing Liar Fig. 2 #4 98.41 (4) 4.991 (2)
Ertsberg Fig. 2 #3 121.16 (6) 5.245 (2)
Sample preparation for all of the low-concentration
samples required crushing of the material. The
crushed sedimentary rocks were powdered and
directly loaded into the carius tubes. The sulfide
samples were handpicked after the initial crushing,
and powdered for analysis. Some of the sulfide
samples contained magnetite, which was separated
magnetically.
Internal reproducibility for the measurements of the
isotopic ratios is always better than F0.2% (2j).However this value is an underestimate of the error for
the whole procedure because the concentration of the
Os blank varies. Procedural chemical blanks during
this study varied from 1 to 2 pg for Os and 20 to 40 pg
for Re. Because the greatest source of error in the
analysis is the variation in the concentration of the Os
blank, errors for the magnetite, sulfide, and sedimen-
tary rock samples are calculated by varying the blank
concentration between 1 and 2 pg. Thus, the ratios
reported assume a concentration of the Os blank of 1.5
pg and the errors record the variation of the ratio with
the change in Os blank concentration. The 187Os/188Os
of the blank remained constant (0.175F0.008)
throughout this study.
4. Results
Concentrations of Re and Os for the molybdenites
vary between 156 and 2235 (ppm) and between 4 and
66 (ppb), respectively (Tables 2 and 3). The ages
calculated assuming no initial 187Os for the molyb-
denites sampled are: 2.88 MaF0.02 for the Grasberg,
3.01F0.02 Ma (and 3.03F0.02 Ma for a repeat
analysis) for the Kucing Liar, and 2.54F0.01 Ma for
the Ertsberg sample.
For the sedimentary rocks, the concentration of Os
varies from 5 to 468 ppt, and the measured 187Os/188Os
ratios range from 0.54 to 3.8. Skyline Actlab in Tucson,
b) Age Associated minerals
2.88F0.02 Quartz–sericite vein with cpy
3.01F0.02 Covellite–pyrite in ls host
3.03F0.02 Covellite–pyrite in limestone host
2.54F0.02 Quartz–sericite vein with cpy
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226216
AZ measured gold concentrations for the sedimentary
rocks. The Au values reported in Table 2 are averages
for 3 different measurements on each sample.
Samples from Ertsberg stockwork mineralization
have Re and Os concentrations and ratios similar to
those found in Grasberg stockwork mineralization.
The concentration of Os varies from 4 to 9 ppt and
Re from 1 to 11 ppb in the sulfides and oxides.
The 187Os/188Os measured ratios range from 0.41 to
0.68, and the 187Re/188Os measured ratios range
from 676 to 10893. Splits of two samples from the
stockwork mineralization of the Ertsberg (Erts-1
and Erts-3 and replicate) form a two sample, 3-
point isochron (MSWD=0.61) with an age of 3.3F1.2
Ma and Os initial value equal to 0.26F0.13 (Fig. 5).
If the samples from the skarn mineralization are
plotted along with the stockwork samples of the
Ertsberg, the isochron statistics yield an imprecise
age (MSWD=6.2) of 1.62F0.72 Ma, 187Os/188Os=
0.42F0.07. Because Erts-2 and Erts-3 are genet-
ically different and yield a less precise isochron, we
also solve for the 187Os/188Os initial ratio using the
molybdenite age (2.54 Ma; Table 2) for time (t) in
the age equation:
ð187Os=188OsÞm ¼ ð187Os=188OsÞI
þ ð187Re=188OsÞmekt � 1 ð1Þ
where (187Os/188Os)m=measured ratio, =(187Os/188O-
s)I=initial Os ratio, (187Re/188Os)m=measured ratio,
and k=decay constant of Re (1.666�10�11). Age
and initial 187Os/188Os ratios for the isochron
0.00
0.10
0.20
0.30
0.40
0.50
0.60
0.70
0 1000 2000 3000 4000187Re/
187 O
s/18
8 Os
Age = 3.3 ±Initial 187Os/188O
MSWD =
Fig. 5. Isochron plot of the low concentration
calculations were calculated with the computer
program developed by Ludwig (2001).
It is important to note that we analyzed the
molybdenite and chalcopyrite (Erts-1) from the same
hand-sized sample in which both sulfide phases are
intergrown. There has been debate surrounding the
use of Os initial ratios from low concentration sulfide
minerals calculated by the isochron method. For
example, Stein et al. (2003) stated that bRe–Osanalysis of sulfides in contact or direct association
with molybdenite is highly inadvisable, and can lead
to ages that are too old and, in the case of Re–Os
isochrons, can provide initial 187Os/188Os ratios that
are too high, leading to errant geologic inter-
pretationsQ. It is relevant to note that the Erts-1
chalcopyrite has an Os initial ratio less than all of
the observed Os initial ratios calculated for the sulfide
minerals and sedimentary rocks in this data set. This
observation holds true regardless of how the Os initial
ratio is calculated; by the isochron method or by
substituting age information to derive Os initial ratios.
Therefore, for the samples analyzed in this study,
migration (diffusion) of either element after the
precipitation of these two phases and the calculated
Os initial ratios does not appear to have caused binitial187Os/188Os ratios that are too high. . .Q Perhaps a
plausible explanation for these results is that the
diffusion rate of Os is too slow to have predicted the
migration of Os atoms across these minerals interface,
therefore when considering that Os isotopic ratios can
be disturbed, a time frame for the diffusion should be
considered.
5000 6000 7000 8000 9000188Os
1.2 Ma
s =0.26 ± 0.13 0.61
samples from the Ertsberg stockwork.
A.)
Au ppm Cu %
Length of drill core (m)
1
2
3
100 200 300 400 500 700
AuCu
Os ppt
10
50
100
Os
1
6
3
187Os/188Os = 0.56
187Os/188Os initial > 0.56
B.)
1/Os (ppt)
187 O
s/18
8 Os
initi
al
0 0.01 0.02 0.03 0.04 0.05
0.5
1
1.5
0
Grasberg Stockwork
Grasberg Massive sulfide
C.)
0 2000 4000 6000 8000 10000 12000 140000
0.5
1.0
1.5
2.0
187 O
s/18
8 Os
Initial187Os/188Os = 0.56+/-0.02
Age= 2.9+/-0.3Ma
187Re/188Os
Fig. 6. (A) Isochron diagram of the stockwork ores taken from the Grasberg, isochron statistics calculated by a program developed by Clark, if
the data are reduced using Ludwig (2001), the age=2.8F0.5 Ma, MSWD=4.5, the initial 187Os/188Os=0.56F0.05. (B) Distribution of metals
along drill core segment (dark black line in Fig. 2), note that the Os concentration along with Cu, Au, and Os initial ratio increases in the
massive sulfide. (C) Mixing diagram with the stockwork mineralization (n) and massive sulfide (.) minerals of the Grasberg (use of symbols
remains constant through next three figures).
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 217
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226218
Concentrations of Re and Os in the contact ores
from the Kucing Liar and Dom are much greater than
the stockwork mineralization, and range from 2 to 28
ppb and 40 to 341 ppt, respectively. The 187Os/188Os
measured ratios range from 0.59 to 0.94 and the187Re/188Os measured ratios range from 254 to1474.
None of the data from the peripheral ore deposits
(Kucing Liar and Dom) lie on the isochrons devel-
oped for the Grasberg or Ertsberg stockwork miner-
alization. Instead, data from the Kucing Liar are
isotopically heterogeneous. The Os initial ratios
presented for these samples are calculated by using
Eq. (1). By assuming a mineralization age of 3Ma for
the Kucing Liar samples and 2.5Ma for the Dom
sample, the calculated Os initial ratios range from
0.58 to 0.92. The samples from the Kucing Liar lie on
the mixing trend between the Grasberg intrusion
sulfides and the massive sulfide mineralization
peripheral to the Grasberg ore deposit (Mathur et al.,
2000). Figs. 6 and 7 illustrate this relationship. The
Dom sample, spatially associated with the Ertsberg
mineralization, does not lie on this trend or the
errorchron plot of the Ertsberg stockwork samples.
The composite gold sample has 578 ppt Re and
873 Os, and has measured 187Os/188Os of 1.23 and187Re/188Os of 3.6. This datum point does not plot on
isochron diagrams. The calculated Os is 1.23 if a
mineralization age of 2.9Ma is assumed. The Os
initial ratio for this sample lies near the apex of the
187 O
s/18
8 Os
initi
al
0 0.01 0.02
0.5
1
1.5
0
*
Kucing Liar
Au concentrate
1/Os (
Fig. 7. Mixing diagram of samples from the Grasberg ore body, data from M
composite gold sample. Note the general trend exists and suggests a geneti
mixing trend demonstrated for the Grasberg peripheral
ores (Fig. 7).
5. Discussion
5.1. Geochronology of the district
In order to examine the relationship between the
Ertsberg and the Grasberg systems, we analyzed both
sulfides with low concentrations of Re–Os (pyrite,
chalcopyrite) and molybdenites with high Re concen-
trations. The two low concentration/conventional
isochron plots of stockwork mineralization from the
Ertsberg (isochron in Fig. 5; with an age of 3.3F1.2
Ma), and the Grasberg (isochron; 2.9F0.3 Ma;
Mathur et al., 2000) yield ages that are the same
within the error of the analysis.
In order to develop a more accurate and precise
chronology for the area, we analyzed molybdenite
samples from each of the deposits. Each of the
molybdenite samples from different parts of the
district yields a different age. We interpret the
molybdenite ages to represent mineralization ages.
Therefore, these molybdenite ages reveal that there
have been at least three distinct mineralization events
in the Ertsberg district.
Fig. 3 compares K–Ar, 40Ar/39Ar, and our new Re–
Os molybdenite ages for the district. The K–Ar and
0.03 0.04 0.05
Grasberg Stockwork
Massive Sulfide
ppt)
athur et al. (2000) and the present study. o=Kucing Liar, and *=thec link between the Kucing Liar ore body and the Grasberg ore body.
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 219
40Ar/39Ar ages come from two sources. McDowell et
al. (1996) illustrated that the K–Ar alteration and
intrusion ages for the Ertsberg are slightly younger
than those present in the Grasberg. Pollard and Taylor
(2000) continued exploring the geochronologic rela-
tionships of the area by examining the 40Ar/39Ar
systematics of biotite, muscovite, and phlogopite from
each of the alteration sequences in the Kucing Liar ore
body, Kali intrusion (Grasberg Intrusive Complex),
and the Ertsberg diorite. They also found that the
Grasberg and Kucing Liar alteration/cooling ages are
older than the Ertsberg.
The Re–Os molybdenite ages (Fig. 3) are in accord
with the K–Ar and Ar–Ar ages defined by Pollard and
Taylor (2000) and McDowell et al. (1996). The
Kucing Liar and Grasberg molybdenites are distinctly
older than the Ertsberg molybdenite (according to the
statistical analysis derived by Dalrymple and Lan-
phere (1969) errors of the molybdenite ages are small
enough to indicate different events). Further geologic
evidence that supports the notion that the Grasberg
Intrusive Center is older than the Ertsberg Intrusive
System comes from paragenetic crosscutting relation-
ships defined by the following studies (Katchan,
1982; Meinert et al., 1997; Predenergast et al., 2001).
5.2. Deposit scale geochronology
5.2.1. Re–Os evidence for links between the massive
sulfide, Kucing Liar, and the Grasberg stockwork
mineralizations
Mathur et al. (2000) examined two mineralization
events in the Grasberg. Re–Os results from sulfide
stockwork related to porphyry copper gold mineral-
ization in the Grasberg Intrusive Center were
sampled from different silicate alteration assemblages
and host rocks and plotted on an isochron with an
initial 187Os/188Os of 0.56F0.02 (Fig. 6A). The
initial 187Os/188Os of this isochron is highly radio-
genic compared to the present mantle 187Os/188Os of
0.1296 (Meisel et al., 2001). This indicates that the
source of Os and, by inference, the associated metals
have a significant crustal component. A younger
mineralization event, characterized by massive pyr-
ite, crosscuts the typical stockwork mineralization
and borders the intrusive complex. The samples do
not plot on the isochron developed for the stockwork
mineralization of the Grasberg, thus the Os initial
ratios calculated for these samples were determined
by substituting in a mineralization of 2.9 Ma. These
samples have evolved heterogeneous initial Os
isotopic ratios that are greater than the stockwork
mineralization (labeled N0.5 on Fig. 6B), ranging
from 0.61 to 1.23. The samples with the highest and
most radiogenic signatures (Os isotope ratios) also
have higher Au concentration than stockwork min-
eralization of the Grasberg system.
The mixing diagram in Fig. 6C illustrates a
relationship between massive sulfide and the stock-
work mineralization. The data suggest that the stock-
work mineralization event began as isotopically
homogeneous, and as the hydrothermal system
evolved, it became isotopically heterogeneous as the
fluids mixed with a highly radiogenic source that is
mirrored in the minerals of the massive sulfide
orebody. A reasonable end member for this mixing
trend is black shale, and evidence linking the ores to
sedimentary rocks is presented below.
In order to test the relationship between the
Kucing Liar skarn and the Grasberg stockwork
orebody mineralization, we analyzed five samples
from drill core that sampled skarn and stockwork.
Magnetite, chalcopyrite, and pyrite samples from this
skarn do not define a trend on an isochron diagram
with age significance. They plot on the mixing trend
developed along with samples from massive sulfide
and stockwork mineralization of the Grasberg ore-
body (Fig. 7). Included in the graph is the composite
gold separate from the Ertsberg district. The approx-
imate trend of the data suggests that there is a
relationship between these three ore bodies. The
addition of the Kucing Liar data further demonstrates
the isotopically heterogeneous nature of the fluids
that precipitated the peripheral Kucing Liar and the
massive sulfide ore bodies and that some Os was
acquired from the surrounding crust. The data
support a model in which the primary, isotopically
homogenous, copper–gold rich fluid had its source
presumably associated with the igneous intrusion and
while this intrusion cooled by convection; the
hydrothermal fluids leached metals from the sur-
rounding host sedimentary rocks and deposited them
in the mineralization center.
In the Ertsberg district, there is widespread
evidence of fluid and thermal activity extending for
at least 2 km beyond the intrusive centers. Gammons
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226220
and Williams-Jones (1997) proposed a mechanism in
which cool solutions in the periphery of such systems
could derive gold through leaching in an environment
of high H2S activity. We suggest that heating of these
fluids during the convective process would reduce
gold solubility and precipitate the metal in the
mineralization center.
5.2.2. Comparison of Os initial ratios of stockwork
and skarn minerals in the Ertsberg and Grasberg
systems
These two intrusion-centered ore bodies occur
within a 6 km radius of each other. The similarities
or differences among the Re–Os isotope systematics
seen within the ores can be used to interpret possible
genetic relationships among the ore stockwork type
mineralization present in each ore body and the
surrounding wall-rock mineralization. In other words,
the isotopic signatures present in the ores can be used
to link the complex, crosscutting mineralization
events present in this intensely fractured portion of
crust.
The Os initial ratios calculated for the stockwork
mineralization from these two intrusion centers are
different. As stated above, the Re–Os data from
stockwork mineralization from the Grasberg con-
strain an Os initial ratio of 0.54F0.02 (Fig. 6A). In
contrast, chalcopyrite and magnetite from the stock-
work mineralization of the Ertsberg form a 3 point
isochron that has an initial 187Os/188Os of 0.26F0.13
(MSWD=0.61; Fig. 5). The two analyses from skarn
sulfide mineralization taken from within the mine
also plot on the isochron diagram and yield an age
of 1.62F0.72 Ma (MSWD=6.3). Because these
skarn samples are paragenetically different from
the stockwork samples and they reduce the stat-
istical significance of the Ertsberg stockwork min-
eralization isochron plot, we also used the age
calculated by the molybdenite from the Ertsberg
(2.54 Ma) and solved for the Os initial ratio (Table
2). Both the isochron plot method and solution for
the Os initial ratios by substituting the molybdenite
ages indicate that the ranges of initial Os values for
the Ertsberg samples are different than those
calculated for the Grasberg stockwork samples.
Importantly, Os initial values calculated by both
methods constrain Os initial values that are greater
than the mantle. Nonetheless, the concentrations of
Re and Os for both of the Grasberg and Ertsberg
stockwork samples are roughly similar. The single
sample from the Dom (peripheral skarn of the
Ertsberg) does not plot on the isochron trends. This
sample has elevated Re and Os concentrations in
comparison to the stockwork mineralization from
both intrusions.
Figs. 7 and 8 are mixing diagrams with data from
the district. The Grasberg and Kucing Liar mixing
relationship lies to the left of the diagram on Fig.
8A. The distinctly different Os initial ratio of the
Ertsberg Intrusive System stockwork mineralization
does not plot on the mixing trend seen in the
Grasberg and Kucing Liar deposits. The diagram
demonstrates that there is no district scale genetic
correlation among the Os isotopic signatures for the
ores and could be indicating several possible
scenarios. For instance, the magmas responsible for
stockwork mineralization could be related to a
dparentT batholith at great depths (N5 km) and as
these dapotheosesT intruded, they assimilated differ-
ent amounts of crust or these magmas have no
relationship at depth. Most importantly, the Os data
indicate that the stockwork of the Grasberg and
Ertsberg ore bodies are relics of two unique hydro-
thermal systems that developed independently and
are not related to the same stock.
Interestingly, the Dom and Ertsberg skarn samples
can be related to the Ertsberg stockwork in a fashion
similar to that suggested for the relationship of the
massive sulfide and Kucing Liar samples, to those of
the Grasberg stockwork. The Dom sample has higher
concentrations of Os and more radiogenic Os initial
ratios, which are comparable to those seen in the
surrounding continental crust. Thus, the Os present in
the Dom skarn could also originate from the
surrounding crust via a process of crustal leaching
similar to that discussed above for the Kucing Liar
and massive sulfide of the Grasberg.
5.3. Genetic link to the sedimentary rocks and the ores
present throughout the Ertsberg district
Os evidence from the ores presented above
suggests that there are two distinct crustal sources
for Os. To develop more insight into where the crustal
metals could have originated and how much of the
metals were derived from sedimentary sources, we
0
0.2
0.4
0.6
0.8
1
1.2
1.4
0 0.05 0.1 0.15 0.2 0.25
1/Os (ppt)
187 O
s/18
8 Os
initi
al
0
0.2
0.4
0.6
0.8
1
1.2
1.4
0 0.05 0.1 0.15 0.2 0.25
1/Os (ppt)
187 O
s/18
8 Os
initi
al
A.)
B.)
Grasberg/ K
ucing Liar
Ertsberg/DOM
Stockwork Grasberg
Stockwork Ertsberg
Sedimentary Rocks Analyzed
Fig. 8. (A) Mixing diagram plot of the all the data from the sulfide ore samples. x=Kucing Liar and massive sulfides; .=Ertsberg skarns;
E=Dom. Dashed line is the mixing line among the massive sulfide, Kucing Liar, and the Grasberg stockwork, and the solid line is the mixing
line for the Ertsberg stockwork, skarns, and Dom. (B) The outlined area represents measured Os ratios and concentrations of the sedimentary
rocks analyzed in this study. The open squares in this figure are sedimentary rock analyses (some sedimentary rocks do not fit in the plotted area,
therefore the arrows indicate that there are higher Os ratios measured within the cross hatched area). Note the overlap of the crust field with the
peripheral ore bodies (e.g., Kucing Liar, massive sulfide, and Dom) and stockwork mineralization of the Grasberg.
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 221
analyzed the Os isotopic composition and concen-
tration of gold in selected sedimentary rocks. Figs. 4
and 8B illustrate the variation of Os isotope ratios and
concentrations present in the selected samples from
the stratigraphic section. We measured Os ratios and
concentrations to use for comparison on mixing
diagrams because the 187Re/188Os ratios for these
sediments are low (e.g., GBMA1, 22-1) and ore
formation occurred recently in the geologic past
(correction for 2 Ma would insignificantly shift the
measured ratios).
Interpretation of the mixing diagrams proposed as
evidence for crustal leaching in the Grasberg system
by Mathur et al. (2000) invoked shale as a possible
end member. This study presents Re–Os results from
Mesozoic shale units that the hydrothermal system
could have interacted. These rocks have higher
concentrations of Os (between 200 and 400 ppt) and
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226222
radiogenic ratios roughly similar to or slightly greater
(0.52 to 0.89) than the stockwork mineralization of
the Grasberg and Ertsberg ores (0.56 and 0.26,
respectively). In comparison, the limestone, arkose,
and mudstone have considerably less Os (5 to 25 ppt)
and radiogenic 187Os/188Os ratios greater (between 1.4
to 3.7) than the stockwork mineralization. These
differences in concentrations are in accord with
previous observations showing that, on the average,
black shales contain relatively larger concentrations of
Os and Re than do other sedimentary lithologies
(Ravizza and Turekian, 1992; Esser and Turekian,
1993; Horan et al., 1994; Singh et al., 1999). The187Os/188Os measured in the sedimentary rocks of this
study is reasonable because the measured 187Os/188Os
of the shale units is identical to the Os isotopic
signature of fluvial systems draining from the
mountains of Irian Jaya found by Martin et al. (2000).
The fundamental purpose of this study has been to
examine and if possible quantify the role of con-
tinental crust and igneous intrusions as sources of
some metals of the ores of the Ertsberg district. We
believe that the Re and Os data demonstrate a link
between the ores and the sedimentary rocks of the
surrounding crust. Of the several sedimentary rock
samples analyzed here, none provide the exact Os
characteristics for doneT stratigraphic unit-source to
account for the observed mixing trend. However, a
mixture of the Os concentrations and isotopic
compositions from these sedimentary sources could
easily account for the mixing trends present at the
district scale of the Ertsberg and Grasberg intrusive
complexes. Fig. 8B demonstrates this point by high-
lighting the concentrations and measured ratios of the
sedimentary rocks on the mixing diagram plot. Since
the hydrothermal aureole affects all of the surrounding
Cenozoic and Mesozoic strata, leaching of a specific
stratigraphic unit probably did not occur. Rather, the
hydrothermal system’s acquisition of metals included
a mixture of Os from all of the sedimentary units and
the resulting product of this process is illustrated in
the isotopic heterogeneity of the massive sulfide,
Kucing Liar, and the Dom.
These data provide an explanation for aspects of
metallization in peripheral skarns, but do not explain
the extent to which, nor the means by which, initial
magmas were enriched in copper and gold before the
mixing process took place in the upper crust. Conven-
tional views would propose that sources of possible
magma (and radiogenic) components of the igneous/
hydrothermal system evolve at depths where the
progenitors could be each, or combinations of, the
lower crust, the subducted slab, or metasomatized
mantle. The data and interpretations of magma and
possible metal sources interpreted here are consistent
with the model of crustal assimilation and fractional
crystallization proposed for Neogene magmatism in
New Guinea by Housh and McMahon (2000) and for
some porphyry related intrusions in North American
by Anthony and Titley (1988) and Lang and Titley
(1998). A two-end member geochemical mixing
calculation that assumes the average lower continental
crust of Australia (187Os/188Os=0.85, Os=50 ppt; Saal
et al., 1998) and a mantle (187Os/188Os=0.1296, Os=2
ppb; Meisel et al., 2001) indicates that about 40% of
the lower crust may have been assimilated to generate
an Os initial ratio of 0.56 present in the Grasberg
stockwork ores. If the Kariem Os datum from this
study is used, then the percentage of dKariem-likeTlower crust necessary to generate the Grasberg stock-
work Os (initial value of 0.56) reduces slightly to
30%. If the Ertsberg Os initial ratio of 0.26 is
considered, the amount of continental crust (either
from Saal et al. (1998) or the Kariem crust of this
study) is reduced to approximately 15 to 20%.
Although sample quality precluded the collection
of dunalteredT samples (sedimentary rocks near the
intrusion that did not display low grade hydrothermal
metamorphic mineralization) in the district, we under-
score the possibility of hydrothermal interaction with
strata of the Cretaceous and Tertiary sections that
compose the wall rock at the deposit level of the
Ertsberg and Grasberg systems. The geologic evi-
dence of widespread development of marble, a broad
(km-scale) aureole of weak metamorphism, and
scattered exposures of altered strata are indicators, at
mineralization levels, of the effects of intrusion and
wall rock interaction during the intrusion and miner-
alizing process.
Several studies have explored this concept. Brim-
hall (1979, 1980) has addressed deep hypogene
leaching of plutonic hosts and porphyries to develop
ore grade assemblages at Butte Montana. Norton
(1982) has modeled the nature of fluid flow around
cooling plutons of the North American craton and has
shown the nature and habits of source regions and
R. Mathur et al. / Ore Geology Reviews 26 (2005) 207–226 223
pathlines for fluids involved in the process. Kendrick
et al. (2001) have identified the provenance of ore
fluids in this same North American province; Gerlach
et al. (1975) and Norton (1979) report the results of
studies of chemical mass transfer between plutons and
wall rocks. In the studies of concern here, we see
many of the same physical properties of altered
fractures and intrusion and carbonate hosts present
in the Grasberg and Ertsberg intrusive systems. These
observations allow us to consider hydrothermal
leaching as a possible mechanism to explain the
chemical mixing relationships seen throughout the
deposits.
We have demonstrated that the continental crust
has a profound influence on the source of Os in the
ore minerals from the Erstberg district. Given that
the Os data from the selected units in the surround-
ing crust reveal a direct genetic relationship, the Os
signatures in the stockwork mineralization quite
likely represent the result of a mixing process that
involved igneous and hydrothermal interaction with
multiple crustal sources during the igneous and
hydrothermal processes. Further evidence from the
concentration of gold in the sedimentary rocks
adjacent to the hydrothermal system provides support
that there are sources of radiogenic elements and
gold within the crust that the mineralizing processes
interacted.
6. Conclusions
A combination of the molybdenite chronology of
the area, and the Os initial ratio data from the ores
points to a model in which two adjacent intrusions
and hydrothermal systems evolved independently in
the epicrustal environment. The highly radiogenic
and concentrated Os values from the surrounding
rocks demonstrate that the continental crust is a
likely source for Os, whether by leaching and/or
assimilation. The radiogenic initial Os initial values
from stockwork ores present in both systems indicate
that the metals originated from a crustal source. The
contribution of at least some Os (and by inference
other metals) from the continental crust was further
amplified during the cooling process, when the fluids
responsible for precipitating the periphery ores
apparently mixed with and acquired Os (and by
inference other metals) from the surrounding con-
tinental crust. The relevance of these observations is
that there are two distinct crustal sources present in
the ores, one related to lower crustal magmatic origin
and another found in the middle to upper crust of
these deposits that reside in the thick Australian
continental crust.
Acknowledgements
We wish to thank Freeport McMoRan, Cu and Au
Inc., and P.T. Freeport Indonesia for their support of
the geological studies, during the several field
seasons on which this report is based and for
permission to publish this work. Analytical work
was supported by the National Science Foundation
Grants EAR 9708361, and EAR 9628150, and an
instrumentation grant from the W. M. Keck Founda-
tion. We also thank Brian New for providing the
molybdenite sample from the Kucing Liar deposit.
Dave Potter and Steve Van Nort encouraged this
work in the district. Keith Parris and George
MacDonald sustained liaison. Chuck Brannon, Al
Edwards, Wahyu Sunyoto. Sugeng Widodo, Norris
Beluz, Lasito Soebari, Larry Segerstrom, together
with numerous Freeport geologists were instrumental
in facilitating field support and providing access to
pit and underground sample sites, and core. We
acknowledge with thanks the productive discussions
of precious metal geology with Imants Kavalieris
and Jay Pennington. Frank Nelson provided samples
of Ertsberg orebody mineralization. Paul Warren’s
help and knowledge of regional stratigraphy were
crucial to those aspects of the field study. Finally, we
would like to thank two anonymous reviewers and
Associate Editor Stephen Kesler for their insightful
comments to improve this presentation.
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