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J. SE Asian Appl. Geol., Jan–Jun 2012, Vol. 4(1), pp. 1–14

ORE AND CHEMISTRY OF , , AND AT SORIPESA PROSPECT AREA, SUMBAWA ISLAND, INDONESIA

Win Kant∗1,2, I Wayan Warmada1, Arifudin Idrus1, Lucas Donny Setijadji1, and Koichiro Watanabe3

1Department of Geological Engineering, Gadjah Mada University, Yogyakarta, Indonesia 2Department of , Banmaw University, Myanmar 3Department of Resource Engineering, Kyushu University,

Abstract rite inclusion/disease also occurred. Ga and Ge con- tents are also high in sphalerite. Co>Ni in pyrite, The Soripesa prospect area is located at Maria vil- low content of Ag in Galena, low content of Fe and lage, Wawo district, Bima region in the East Sum- mole % FeS in sphalerite, high content of Ga and bawa Island, Indonesia. Lithology is dominantly Ge, and log (Ga/Ge) in sphalerite, show that pyrite, composed of a lithic- tuff of andesitic and galena, and sphalerite from Soripesa prospect area dacitic composition and bedded . The poly- were formed under low temperature condition of hy- metallic epithermal veins are hosted by an- drothermal fluid. desitic volcaniclastic rocks. Within these veins, mul- Keywords: textures, paragenesis, deposition, tiphases, colloform-crustiform, bedding to massive hydrothermal fluid, low temperature textures with pyrite, sphalerite, galena, chalcopy- rite, , , and are observed. 1 Introduction Selected samples were analyzed by using ore mi- croscopy and SEM-EDX. Ore show re- The Soripesa prospect area is located in Maria placement, ex-solution, colloform, and zonal tex- village, Wawo district, Bima regency, West tures. The paragenesis diagram was made from a Nusa Tenggara Province. The prospect area careful study of polished sections and thin sections. is previously owned by PT Bima Baruna Raya Textures of ore minerals such as banded, exsolution, (BBRM) and PT Sumbawa Timur Min- replacement, and zone, have been interpreted to cor- ing. These companies have observed Au-Ag respond to the order of deposition. In pyrite, the av- deposit and base mineralization. At erage content of Co (0.45 wt.%) is higher than Ni present, PT Bima Putera Minerals (Indomin- content (0.14 wt.%) and it means that their origin ing Group) has a Mining Permit (exploration may be hydrothermal origin. Average content ratio, stage) for those deposits. The prospect area Co:Ni is 2.81. Galena shows a low Ag content of is mainly composed of andesitic and dacitic 0.07 % in average. But they show a high Au content volcaniclastic host rocks and small amount of 1.48 % in average. Sphalerite shows a low Fe con- of Tertiary bedded . There have tent of 1.04 % in average and occasionally chalcopy- five main veins in the Soripesa prospect area, trending nearly north-south. Those veins are ∗Corresponding author: W. KANT, Department of Geological Engineering, Faculty of Engineering, Gadjah hosted in andesitic volcaniclastic rocks (lower Mada University, Jl. Grafika 2 Yogyakarta, 55281, Indone- Miocene in age). The common ore minerals sia. E-mail: [email protected]

1 KANT et al of those veins are , galena, spha- minerals and their textures. Ore textures and lerite, pyrite, chalcocite, , azurite, and ore mineral assemblages are analysed under ore malachite, which are forming as polymetallic microscopy at Earth Resource Engineering De- epithermal quartz veins. partment, Kyushu University. An Energy Dis- The purpose of this paper is to identify the persive X-Ray Analyser (EDX or EDA) is also ore mineral paragenesis and ore forming pro- used to provide elemental identification and cesses, and mineral chemistry of some sul- quantitative compositional information. For fide minerals, especially for pyrite, galena, and SEM-EDX analyses, 15 polished sections and 3 sphalerite from polymetallic epithermal quartz thin sections were used to identify the mineral veins at Soripesa prospect area, East Sumbawa, chemistry by using a SHIMADZU SS-550 SEM Indonesia. with a Genesis 2000 energy dispersive spec- trometer (EDX) at the Center of Advanced In- 2 Regional Geology strumental Analysis, Kyushu University. Semi- quantitative analyses were performed at an ac- The Sumbawa Island forms as a part of the celerating potential of 15 kV, with a beam cur- Cenozoic calc-alkaline volcanic inner Banda- rent of about 6.0×10−10 A, and a beam diam- Sunda Arc which is still active up to present. eter of 3µm. All the data were corrected with Sunda-Banda island arc is a volcanic arc formed a ZAF matrix-correction program. The low- by the interaction of plate subduction slab in est detection limit is 100 ppm. Ore minerals the form of Indo- with Asian plate such as sphalerite, galena, pyrite, chalcopyrite, (Carlile and Mitchell, 1994). Sunda-Banda arc is chalcocite, azurite, malachite, minerals, the longest in Indonesia, extending from north and some unknown minerals were analyzed by Sumatra through Java, Bali, Lombok, and Sum- SEM-EDX for elemental identification and com- bawa, to east Damar. The shape of the is- positional information. Based on the elemen- land arc is now being modified in the east due tal compositions, ore minerals can be estimated to collision with the Australian–New Guinea and identified their , and ore form- continental margin, including East Sumbawa ing processes. (Hamilton, 1974). The Sumbawa Island is mainly composed 4 Results and Discussions by andesitic to basaltic lava and of the Lower Miocene, with intercalations of tuff 4.1 Ore Minerals Assemblages and Their and limestone, fresh pyroclastic sequences and Textural Characteristics shoshonite. This sequence is overlain in parts by dacitic tuff and bedded limestone of the Common ore minerals of the polymetallic ep- Mid Miocene. These units have been intruded ithermal quartz veins at Soripesa prospect area by numerous small to medium bodies (several are chalcopyrite [CuFeS2], galena [PbS], spha- km’s) in the Middle to Upper Miocene includ- lerite [ZnS], azurite, malachite, chalcocite, cov- ing andesite, dacite, , trachyte and syen- ellite, pyrite [FeS2], , and other - ite (Figures 1 and 2). Sumbawa Island, re- oxide minerals. gionally, is intersected by NW-SE and NE-SW trending structures. However, the formation of Chalcopyrite. chalcopyrite is one of abundant quartz veining, alteration and mineralization at ore minerals and also occurs within sphalerite Soripesa Prospect are related to the N-S faulting as chalcopyrite disease/inclusion (Figure 3e). (Noya et al, 2009). This texture is called as ex-solution texture. Some chalcopyrite replace in pyrite (Figure 3g). The cracking of some chalcopyrite are also re- 3 Sampling and Analytical Methods placed by Fe oxide minerals such as colloform Eighteen selected samples were made thin sec- and hematite. inclusions are also tions and polished sections to identify the ore occurred in chalcopyrite.

2 c 2012 Department of Geological Engineering, Gadjah Mada University ORE MINERALOGY AND MINERAL CHEMISTRY OF PYRITE, GALENA, AND SPHALERITE

Figure 1: Simplified geologic map and chronology of map units for Sumbawa island, Indonesia including Soripesa prospect area (Source: Garwin, 2002)

c 2012 Department of Geological Engineering, Gadjah Mada University 3 KANT et al

Figure 2: Geological map of around Soripesa prospect area with epithermal quartz veins (modified after Noya et al, 2009)

4 c 2012 Department of Geological Engineering, Gadjah Mada University ORE MINERALOGY AND MINERAL CHEMISTRY OF PYRITE, GALENA, AND SPHALERITE

Pyrite. most of pyrite occurs as euhedral form from the mutual relationships among the min- and some are replaced by chalcopyrite. Pyrite erals and assemblages (Misra, 1999). The inter- occurs in both host rock samples and sam- pretation of microscopic textures of ore miner- ples. Some are replaced by Fe oxide minerals als is very useful to prepare the paragenesis di- such as goethite and hematite which are show agrams of those ore minerals. The paragene- in concentric texture (Figure 3a). Some pyrite sis was made from a careful study of polished minerals show ribbon texture. sections and thin sections. Textures of ore min- erals such as banded, exsolution, replacement, Galena. galena is one of common ore miner- and zone, have been interpreted to correspond als in this research. Some of galena shows a typ- to the order of deposition. Pyrite and quartz ical texture of triangular pits (Figure 3c). Most minerals show their euhedral crystal form. It of the crystal outlines of galena are generally re- is clear that sphalerite is younger than quartz placed by chalcocite (Figures 3c and 3e). in order of deposition (Figure 3d). In Figure 3e, it can be seen clear that covellite replace chal- Sphalerite. sphalerite is also a common ore cocite, and chalcocite commonly coats and re- mineral of polymetallic epithermal quartz veins places the margins of galena and sphalerite, and in this research area. Most of sphalerite show sphalerite replace galena. Chalcopyrite inclu- intergrowth texture with oriented an unori- sions also occur as exsolution textures in crys- ented inclusions of chalcopyrite (the so-called tallographic direction of sphalerite (Figure 3e). “chalcopyrite disease”; Barton, 1978). Tradi- Fe oxide minerals replace in the cracks of chal- tionally, the texture has been described as an ex- copyrite and pyrite (Figures 3a and 3f). Azurite solution of chalcopyrite from sphalerite. How- and malachite occurs as later phase minerals. ever Barton (1970, 1978) and Kalogeropoulos Based on the textural characteristics, order of (1982) have convincing evidence that “chal- deposition can be divided in to two phases as copyrite disease” is a cancerous replacement early phases and later phases. Quartz, galena, produced by Cu in aqueous solution reacting pyrite, sphalerite, and chalcopyrite are formed with FeS in sphalerite. In some case, the out- in early stage of deposition. Chalcocite, cov- lines of sphalerite minerals are in general con- ellite, azurite, malachite, and Fe oxide miner- cave toward quartz minerals (Figure 3d). It als are formed later phase of ore deposition. means that sphalerite is younger than quartz The paragenesis of a mineral deposit can pro- in order of deposition. Sphalerite shows a lot vide a record of the local changes in geochemi- of cracks which are replaced by chalcocite and cal parameters (T, P, fluid composition, etc.) in covellite the course of mineralization (Bastin, 1955). The paragenesis diagrams of ore and min- Chalcocite. they are found as replacement erals from polymetallic epithermal quartz veins minerals and replace sphalerite, chalcopyrite, at Soripesa prospect area are shown in Figure 4. and galena (Figures 3b-e). In some case, they show colloform textures. 4.3 Mineral Chemistry of Pyrite, Galena, and Sphalerite Covellite. they also occur as replacement Minor Elements in Pyrite minerals and replaced mainly in chalcocite. Azurite and malachite are found as hydrother- Pyrite is one of the most abundant miner- mal alteration minerals. Some azurite shows als in the polymetallic epithermal at Soripesa zonal texture under ore microscopy (Figure 3e). prospect area. 21 pyrite minerals are detected by SEM-EDX to know the elemental composi- tion. Average contents (wt.%) of some minor 4.2 Ore-gangue Minerals Paragenesis elements of pyrite are Cd (0.2), Co (0.45), Ni The paragenesis for a mineral deposit or a ge- (0.14), Ag (0.24), Au (1.42), and As (0.75) (Table netically related group of deposits is inferred 1). Some pyrite minerals under SEM-EDX show

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Figure 3: Photomicrographs showing ore mineral assemblages of polymetallic epithermal quartz veins at Soripesa prospect area (qtz = quartz, ccp = chalcopyrite, gn = galena, Ag = silver, py = pyrite, cc = chalcocite, mal = malachite, and goe = goethite).

6 c 2012 Department of Geological Engineering, Gadjah Mada University ORE MINERALOGY AND MINERAL CHEMISTRY OF PYRITE, GALENA, AND SPHALERITE

Figure 4: Paragenetic diagram of ore-gangue minerals assemblage of polymetallic epithermal quartz veins at Soripesa prospect area.

Figure 5: Elemental composition and peak intensity of some pyrite minerals detected by SEM-EDX analyses.

Table 1: SEM-EDX analyses of element composition (wt.%) of Pyrite minerals. Element composition (normalized wt.%) of Pyrite minerals.

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in the range of 2–3 (Xuexin, 1984). It means Table 2: Geometric means of (Co) and that from Soripesa prospect area may (Ni) contents (in ppm) and Co:Ni ratios be formed under the hydrothermal condition. of , hydrothermal, and massive sul- There is a correlation between As and S, and phide pyrite minerals (Xuexin, 1984). no correlation between As and Fe in pyrite of this research (Figures 7a-b). These relations indicate substitution of As for S in the pyrite structure, as would be expected for pyrite con- taining As1− (Deditius et al, 2009). There is also a correlation between Au and Ag but no corre- lation between Au and As (Figures 6a-b).

Minor Elements in Galena Galena is also common ore minerals of epither- mal quartz veins in this research area. 16 galena their image, result of element composition (nor- minerals were detected by SEM-EDX for their malized wt.%) and peaks of elements (Figure 4). mineral chemistry. Some detected minor ele- Xuexin (1984) mentioned a statistically signif- ments of galena from this research are Fe (1.4 icant difference among sedimentary, hydrother- wt.%), Hg (1.92 wt.%), Ag (0.07 wt.%), Au (1.48 mal (replacement veins), and massive sulfide wt.%), Sb (0.39 wt.%), and Se (1.05 wt.%) (Table pyrites (Table 2). According to his study, the 3). SEM image, peaks of elements, and results massive sulfide pyrites are characterized by a of element composition (normalized wt.%) of Co:Ni ratio between 5 and 50; hydrothermal some Galena analysed by SEM-EDX are shown pyrites by a variable Co:Ni ratio (often less than in Figure 8. 5); and sedimentary pyrites by a much lower Tischendorf (1955) found that the Co:Ni ratio (typically <1). Pyrite from sul- content (present at least in part as ) fide ore deposits generally contains appreciable decreased with decreasing temperature of for- amounts of cobalt and has Co>Ni. mation. Schroll (1955) considers the presence According to Carstens (1942), pyrite of sed- of in galena to be a mark of high- imentary origin is characterized by contain- temperature -near deposits. Galena in ing less than 100 ppm cobalt and CoNi. Pyrite from silver varied directly with those of antimony high-temperature deposits is generally high in and bismuth and inversely with content of ar- cobalt, but noted exceptions and considered senic. Fleischer (1956) reported that the content that the effect of temperature was slight. In this of silver, bismuth, and antimony are decreased research, average content of Co (0.45 wt.%) is with decreasing temperature of formation. Sil- higher than Ni content (0.14 wt.%) and it means ver content (0.07) is very low and it means that that their origin may be hydrothermal origin. galena from this research may be formed in de- Pyrite of high-temperature and hydrothermal creasing temperature of formation. sulfide deposits has only a slightly higher av- erage nickel content than pyrite of sedimentary Minor Elements in Sphalerite origin and the ranges of concentration overlap. Sphalerite is one of the most useful indicators Hawley (1952) found that Ni content was a little of the environment of ore deposition because of higher in high-temperature samples. Average its refractory nature, wide distribution in nat- ratio for Co/Ni is 2.81. The Co/Ni ratios for environments, and wide range of compo- -hydrothermal, metamorphosed vol- sition resulting from substitution of Zn by Fe canogenic and -hydrothermal pyrites are (Misra, 1999). Detected minor elements in spha-

8 c 2012 Department of Geological Engineering, Gadjah Mada University ORE MINERALOGY AND MINERAL CHEMISTRY OF PYRITE, GALENA, AND SPHALERITE

Figure 6: Plots showing correlation diagrams of Au, Ag, and As concentration in pyrite.

Figure 7: Plots showing correlation diagrams of As, S, and Fe concentration in pyrite.

Figure 8: Elemental composition and peak intensity of some detected by SEM-EDX analy- ses.

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Table 3: SEM-EDX analyses of element composition (wt.%) of galena. Element composition (nor- malized wt.%) of Galena minerals.

lerite are Fe (1.04 wt.%), Ga (0.7 wt.%), Ge (0.54 trate from a pyritic ore may contain 61-63 wt.% wt.%), Cd (0.7 wt.%), and Ag (0.2 wt.%). Au Zn, but a concentrate from a pyrite-pyrhotite content is below detection limit in all sphalerite ore will often contain only 51-58 wt.% (Table 4). Figure 9 show the result of some spha- and be considerably less valuable. The aver- lerite minerals analysed by SEM-EDX. The re- age content of Zn (63.48 wt.%) in sphalerite of sults show SEM image, peaks of elements, and this research may be related with pyritic ore elemental composition in wt.%. condition. Jonasson and Sangster (1978) investigated the Zn/Cd ratios of from some sul- Sphalerite Geothermometry and Geobarometry phide in and concluded that the Cd contents and Zn/Cd ratios in sphalerites A very interesting recent development is vary with the genetic types of deposit. The the Ga/Ge geothermometer using sphalerite Zn/Cd ratios (average 93.34) in sphalerite from (Moller, 1985). Ga/Ge can be used to deter- the Soripesa prospect area are close to Zn/Cd mine temperatures in the source regions of ore ratios (104–214) of sphalerites from hydrother- solutions and to estimate the degree of mixing mal deposits and skarn-hydrothermal deposits. of hot parental ore fluids with cool, near sur- Stoiber (1940) and Schroll, (1955) considered face waters (Evans, 1993). Ten samples were that the content is most likely to be high simultaneously detected levels for these two in sphalerites from low-temperature deposits elements. The application of these geother- such as those of Mississippi Valley type and in mometer results of calculating the logarithm those from low-temperature quartz veins. follows: In this research, average Ga content (0.7 %) in sphalerites is very high and it means that log[(Ga/Ge) flog[(Ga/Ge) sph] (1) they may be formed under low temperature Note that: f = mineraliser fluid; sph = spha- condition. Many investigators agree that spha- lerite. lerite from low-temperature deposits to be Determining the values of log (Ga/Ge) for higher in content than those from the analyzes of sphalerite minerals, we obtain mesothermal or high-temperature deposits the values in the ranges between -0.4 to 1.15. (Stoiber, 1940; Warren and Thompson, 1945, These values are applied to the chart geother- Fleischer, 1999). In this research, average con- mometer Ga/Ge, based on geothermometer tent of Ge (0.54%) is also very high. Vaughan of Al/Si, and in this case that of muscovite- and Craig (1997) suggested that a zinc concen- chlorite-quartz, given the degree of metamor-

10 c 2012 Department of Geological Engineering, Gadjah Mada University ORE MINERALOGY AND MINERAL CHEMISTRY OF PYRITE, GALENA, AND SPHALERITE

Figure 9: Elemental composition and peak intensity of some sphalerites detected by SEM-EDX analyses.

Table 4: Chemical SEM-EDX analyses of element composition (wt.%) of sphalerites.

c 2012 Department of Geological Engineering, Gadjah Mada University 11 KANT et al phism. The chart shows the values of tempera- sis diagram was drawn from a study of pol- tures between 180 to 240◦C. Figure 10 presents ished sections and thin sections under micro- the projection of the respective analysis chart scope. Ore mineral textures have been inter- that correlates the race Ga/Ge with the temper- preted to identify the order of deposition and ature. This graph is based on geothermometers to made paragenesis diagram. Quartz, pyrite, known systems of Al/Si and published data for galena, sphalerite and chalcopyrite are formed reasons of Ga/Ge in many geological systems in early stage and chalcocite, covelite, azurite, (M¨oller, 1985; 1987). malachite, and Fe oxide minerals are formed in Neiva (1956) considers that the presence of late stage of order of deposition. Ge is higher in sphalerites that are formed at Pyrite, galena, and sphalerite are analysed low temperature. Based on the fluid inclusion by SEM-EDX to know the elemental compo- data from quartz (host minerals), ranges of ho- sitions. Average contents (wt.%) of some mi- mogenization temperature for quartz veins is nor elements of pyrite are Cd (0.2), Co (0.45), between 180 and 300◦C (Khant et al, 2012a). The Ni (0.14), Ag (0.24), Au (1.42), and As (0.75). temperature differences observed between the Some detected minor elements of galena from two geothermometers can be related to the mix- this research are Fe (1.4 wt.%), Hg (1.92 wt.%), ing and circulation of fluids late and/or pre- Ag (0.07 wt.%), Au (1.48 wt.%), Sb (0.39 wt.%), fluid surface (M¨oller, 1985; 1987). and Se (1.05 wt.%). Detected minor elements in Kullerud (1953) suggested that the FeS con- sphalerite are Fe (1.04 wt.%), Ga (0.7 wt.%), Ge tent of sphalerite gave a direct measurement (0.54 wt.%), Cd (0.7 wt.%), and Ag (0.2 wt.%). of its temperature of deposition. Average Fe Average content of Co (0.45) is higher than Ni content (1.04 %) of sphalerite in this research content (0.14) and average ratio for Co/Ni is is very low. Mole % FeS in sphalerite is also 2.81 in pyrite from this research. It means that very low and between 1–2 %. In Zn-Fe-S of origin of pyrite from this research may be hy- low pressure system, this value (1–2 %) falls in drothermal origin. Based on the low contents pyrite field (Figure 11). Within the pyrite field of Sb, Bi, and Ag in average, we can conclude the decrease in FeS content of sphalerite with that galena from this research are formed in de- increasing aS2 ( activity) is much greater creasing temperature of formation. resulting in a close spacing of isopleths near The Zn/Cd ratios (average 93.34) in spha- the pyrite- buffer and in very low lerite from the Soripesa prospect area are close −10 FeS contents in sphalerite at high, aS2 (10 to Zn/Cd ratios (104–214) of sphalerites from to 10−11). It is commonly found that spha- hydrothermal deposits. Low content of Fe, and lerites formed at high aS2 have a honey yellow high content of Ga and Ge, also indicate that to light brown colour with their low FeS con- sphalerites from this research are formed in low tents whereas sphalerites formed at low aS2 and temperature quartz veins. Based on Ga/Ge within the pyrrhotite field are dark brown to geothermometer, the formation temperatures of black (Scott, 1983). Those factors mean they sphalerites can be estimated and they may be may be formed in low temperature condition. formed at between 180 and 240◦C.1to2Mole% FeS in sphalerite indicate that ore deposition −10 −11 5 Conclusion formed under high aS2 (10 to 10 ) and as- sociated with pyrite field. Common ore minerals of the polymetallic ep- ithermal quartz veins at Soripesa prospect area Acknowledgement are chalcopyrite (CuFeS2), galena (PbS), spha- lerite (ZnS), azurite, malachite, chalcocite, cov- The authors want to express deep thanks to alite, pyrite (FeS2), hematite, and other Fe oxide AUN/SEED-Net and JICA program for their fi- minerals. Common textures of ore minerals are nancial supporting to do this research. And replacemnent, exsolution, banded (colloform- then, thankful acknowledgements are due to crustifom), and zone textures. The paragene- Indo mining group for their kind helps and per-

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Figure 10: Graph showing the dependence between Ga/Ge ratios in sphalerite and formation tem- perature. This graph is based on existing Al/Si geothermometers. The musc-clo-qtz line is the chlorite geothermometer in the Si/Al system (M¨oller, 1985; 1987).

Figure 11: Phase relationships for the Fe-Zn-S system at 1 bar compiled from Barton and Toulmin (1966), Scott and Barnes (1971) and Czamanske (1974). Red line represents the sulfur activity of sphalerite in this research. Abbreviations: bn = ; cpy = chalcopyrite po = pyrhotite; py = pyrite; Sl = liquid sulphur; Sv = sulphur vapour.

c 2012 Department of Geological Engineering, Gadjah Mada University 13 KANT et al mission during the field work. Finally, the au- Kalogeropoulos, S.I. (1982) Chemical in thors wish to thank Earth Resources Engineer- the hanging wall of volcanogenic massive sulfide ing Department, Kyushu University for per- deposits. Ph.D. thesis, Univ. Toronto, 488 p. Khant, W., Warmada, I W., Idrus, A., Satijadji, forming laboratory works and analyses. L.D., and Watanabe, K. (2012) Fluid Inclusion Study on Polymetallic Epithermal Quartz Veins References at Soripesa Prospect Area, Sumbawa Island, In- donesia. Journal of Southeast Asian Applied Ge- ology (in preparation). Barton, P.B., Jr. (1978) Some ore textures involving Kullerud, G. (1953) The FeS–ZnS system: a geologi- sphalerite from the Furutobe Mine, Akita Prefec- cal thermometer. Nor. Geol. Tiddskr. 32: 61–147. ture, Japan, 28: 293–300. Misra, K.C. (1999) Understanding Mineral Deposits, Barton, P.B., Jr. (1970) Mineral Society of America, Kluwer Academic Publisher, 758p. Special Paper 3: 187–198. M¨oller, P. (1985) Development and application of the Barton, P.B., Jr. and Toulmin, P. III. (1966) Economic Ga/Ge-Geothermometer for sphalerite from sed- Geology 61: 815–849. iment hosted deposits, In Germann K. (ed.), Geo- Bastin, E.S. (1955) Interpretations of ore textures, chemical aspects for Ore Formation in Recent and The Geological Society of America, Memoir 45, Sedimentary Environments, p. 15–30. 101p. M¨oller, P. (1987) Correlation of Homogeniza- Carlile, J.C. and Mitchell, A.H.G. (1994) Magmatic tion Temperatures of Acessory Minerals from arcs and associated and mineraliza- Sphalerite-bearing Deposits and Ga/Ge Model tion in Indonesia, Journal of Geochemical Explo- Temperatures, Chemical Geology 61: 153–159. ration 50: 91–145. Noya, Y., Effendhy, O., Hamdan Abidin, Z., and Carstens, C.W. (1942) Uber den Co-Ni-Gehalt Pakaya, Y. (2009) Geological background and eco- norwegischer Schwefelkies-vorkommen: Kgl. nomic prospect of the Soripesa deposit, eastern Norske Videnskabs, Selgkabs, Forh. 15: 165–168. Sumbawa, Proceeding pit IAGI Semarang, 2009. Deditius, A.P., Utsunomiya, S., Kesler, S.E., Ewing, The 38th IAGI annual Convention and Exhibition R.C., and Walshe, J. (2009) Behaviour of trace ele- Semarang, 13-14, October. ments in arsenian pyrite in ore deposits, The 10th Scott, S.D. (1983) Chemical behavior of sphalerite Biannual Meeting of SGA, Townsville, 17–20 Au- and in hydrothermal and metamor- gust. Smart Science for Exploration and Mining phic environments. Mineralogical Magazine 47: 1–2, p. 710–712. 427–435. Evans, A.M. (1993) Ore Geology and Industrial Min- Schroll, E. (1955) Uber das Vorkommen einiger erals: An Introduction, Blackwell scientific publi- Spurenmetalle in Blei-Zink-Erzen der ostalpinen cations, 3rd Ed., 390p. Metallprovinz, Tshermaks Mineralog, Petrog, Fleischer, M. (1956) Minor Elements in Some Sulfide Mitt. 5: 183–208. Minerals? , 50th Anniversary Stoiber, R.E. (1940) Minor elements in Sphalerite, Volume, p. 970–1024. Economic Geology 35: 501–519. Garwin, S. (2002) The Geologic Setting of Intrusion- Tischendorf, G. (1955) Paragenetische und tek- Related Hydrothermal Systems near the Batu Hi- tonische Untersuchungen auf Gangen des fluo- jau Copper-Gold Deposit, Sumbawa, rbarytischen bleiformation Freibergs, Freiberger Indonesia. Global Exploration 2002: Integrated Forschungshefte, C18: 1–129. Methods for Discovery, , USA, 9, p. 333– Vaughan, D.J. and Craig, J.R. (1997) Sulfide Ore Min- 366. eral Stabilities, Morphologies, and Intergrowth Texture, In Barnes H.L. (ed.) Geochemistry of Hy- Hamilton, W. (1974) Tectonics of the Indonesian re- drothermal Ore Deposits, John Wiley & Sons, p. gion. U.S. Geol. Surv., Prof. Pap. 1078p. 367–434. Hawley, J.E. (1952) Spectrographic studies of pyrite Warren, H.V. and Thompson, R.M. (1945) Spha- in some Eastern Canadian mines, Economic Geol- lerites from western Canada. Economic Geology ogy 47: 260–304. 40: 309–335. Jonasson, I.R. and Sangster, D.F. (1978) Zn:Cd ra- Xuexin, S. (1984) Minor Elements and Ore Genesis tios for sphalerites separated from some Cana- dian sulphide ore samples, Paper Geol. Surv. of the Fankou -Zinc Deposit, . Mineral Canada 78-1B: 195–201. Deposita 19: 95–104.

14 c 2012 Department of Geological Engineering, Gadjah Mada University