Chromian spinel exsolution in ilmenite from the Premier Mine,Transvaal, South Africa

Exsolution intergrowths of a chrome rich spinel are reported for the first time in terrestrial ilmenite. The ilmenite in which this phenomenon has been observed occurs in the Premier Diamond Mine kimberlite. The occurrence is also noteworthy for the reasons that exsolution textures of any nature are extremely rare in ilmenite derived from kimberlite, and because the exsolved spinel has no known terrestrial counterpart, but is remarkably similar in chemical composition to certain lunar chromian ulvöspinels.     

Abundance and Partitioning of OH in a High-pressure Magmatic System: Megacrysts from the Monastery Kimberlite, South Africa

Concentrations of OH, and major and trace elements were determinedin a suite of mantle-derived megacrysts that represent the crystallizationproducts of a kimberlite-like magma at     

Multiply exsolved clinopyroxene megacrysts from the Frank Smith Mine,Cape Province,South Africa

Two clinopyroxene megacrysts from the Frank Smith kimberlite show multiple exsolution of garnet, orthopyroxene and oxide phases. In one of the megacrysts the lamellar texture has partly recrystallized to a granular one. The chemical compositions of the exsolved phases are similar to those of discrete nodules and of granular pyroxenites found in the same kimberlite. Conditions of formation of the original homogeneous clinopyroxene solid solution are estimated to be ～1500°C and 37 kb, whereas the re-equilibration conditions are closer to 900°C and 35 kb. The megacrysts may have belonged to the Karroo age magnetism which predated kimberlite activity and have been brought to the surface as accidental xenocrysts by the Frank Smith kimberlite.     

The petrogenesis of group 2 ultrapotassic kimberlites from Finsch Mine, South Africa

Major, trace element and radiogenic isotope results are presented for a suite of hypabyssal kimberlites from a single pipe, at the Finsch Mine, South Africa. These are Group 2 kimberlites characterised by abundant phlogopite ± serpentine ± diopside; they are ultrabasic (SiO₂ < 42 wt.%%) and ultrapotassic (K₂O/Na₂O > 6.9) igneous rocks, they exhibit a wide range in major element chemistry with SiO₂ = 27.6−41.9 wt. % and MgO = 10.4−33.4 wt. %. (⁸⁷Sr/⁸⁶Sr)_i=0.7089 to 0.7106, ε_{Nd is} −6.2 to −9.7 and they have unradiogenic (²⁰⁷Pb/²⁰⁴Pb)_i contents which ensure that they plot below the Pb-ore growth curve. They have high incompatible and compatible element contents, a striking positive array between Y and Nb which indicates that garnet was not involved in the within suite differentiation processes, and a negative trend between K/Nb and Nb contents which suggests that phlogopite was involved. In addition, some elements exhibit an unexpected order of relative incompatibility for different trace elements which suggests that the intra-kimberlite variations are not primarily due to variations in the degree of partial melting. The effects of fractional crystallization are difficult to establish because for the most part they have been masked by the entrainment of 50–60% mantle peridotite. Thus, the Finsch kimberlites are interpreted as mixtures of a melt component and entrained garnet peridotite, with no evidence for significant contamination with crustal material. The melt component was characterised by high incompatible element contents, which require both very small degrees of partial melting, and source regions with higher incompatible element contents than depleted or primitive mantle. Since the melt component was the principal source of incompatible elements in the kimberlite magma, the enriched Nd, Sr and Pb isotope ratios of the kimberlite are characteristic of the melt source region. The melt fractions were therefore derived from ancient, trace elements enriched portions of the upper mantle, most probably situated within the sub-continental mantle lithosphere, and different from the low ⁸⁷Sr/⁸⁶Sr garnet peridotite xenoliths found at Finsch. Within the sub-continental mantle lithosphere old, incompatible element enriched source regions for the kimberlite melt fraction are inferred to have been overlain by depleted mantle material which became entrained in the kimberlite magma.     

Vanadium,nickel and cobalt variations in eclogites from Roberts Victor Mine,South Africa

The V-Ni-Co variation trend of Roberts Victor eclogites is toward the enrichment of vanadium at the expense of nickel with relatively little change of cobalt. The systematic V-Ni-Co variation together with petrographic evidences suggest that Group I and Group II eclogites from Roberts Victor Mine were most probably formed by fractional crystallization.     

Thaumasite from the Tschwinning mine,South Africa

Summary Thaumasite from the manganese mine of Tschwinning, South Africa, has the formula Ca_3.097 Si_1.062OH_6.372(CO₃)_0.994(SO₄)_1.000·11.596 H₂O. Unit cell parameters (a=11.013(2) Å,c=10.379(5) Å,V=1090.1(6) ų) and refraction indices (n_e=1.458(2),n _o=1.498(2)) compare well with the best ones available in the literature. The IR spectrum and DT-TG profiles are given. Contradictions between the IR spectrum, a recent structural refinement and the DT-TG are discussed, but cannot be explained satisfactorily.

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Thaumasit aus der Mangan-Mine von Tschwinning, Süd-Afrika

Zusammenfassung Thaumasit aus der Mangan-Mine von Tschwinning, Süd-Afrika, besitzt die Formel Ca_3.097 Si_1.062OH_6.372(CO₃)_0.994(SO₄)_1.000·11.596 H₂O. Die Parameter der Elementarzelle (a=11.013(2) Å,c=10.379(5) Å,V=1090.1(6) ų) und die Brechungsindizes (n _e=1.458(2),n _o=1.498(2)) zeigen gute Übereinstimmung mit verfügbaren Literaturdaten. Es werden ein IR-Spektrum und DT-TG-Profile präsentiert. Gegensätze zwischen dem IR-Spektrum, einer neueren Strukturverfeinerung und dem DT-TG werden diskutiert, können jedoch nicht zufriedenstellend erklärt werden.

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With 2 Figures     

Thrust-controlled gold mineralisation at the Elandshoogte Mine,Sabie-Pilgrim's Rest goldfield,South Africa

Stratiform quartz-sulphide-gold veins, locally termed reefs are hosted within the Proterozoic Transvaal Sequence sedimentary succession, in the Sabie-Pilgrim's Rest goldfield, eastern Transvaal. These deposits have produced about 180 tonnes of gold and share many characteristics with those of Telfer, Western Australia. Detailed examination of the Elandshoogte Mine shows that gold deposition occurred in two stages, both linked to bedding-parallel thrust faulting within the sedimentary pile. Deformation being concentrated within incompetent shale beds, interlayered within more competent units. The majority of gold was introduced in the second stage of mineralisation and occurs within fractures in early-formed sulphide minerals. Deposition of competent quartz veins accompanying early sulphide and gold mineralisation resulted in a change in deformation style within the reef zone, from early shearing in shales to later duplex faulting of the quartz-reef. Fluids accompanying faulting are implied to have transported gold, and a magmatic source of mineralisation is suggested.     

A late quaternary pollen record from the Transvaal bushveld, South Africa

Pollen spectra from cores of organic spring deposits from the Transvaal provide evidence for the climatic evolution of the province during the last 35,000 yr B.P. or more. The past climatic phases are derived from palynological reconstructions of past vegetation types by comparison of fossil pollen data with modern surface pollen spectra from various localities. Evidence is provided for an early moist, cool phase with relatively mesic bushveld and expanded montane forest in the central Transvaal, followed by a drier period with drier bushveld which probably lasted until approximately 25,000 yr B.P. During the next phase, which at the latest ended about 11,000 yr B.P., the temperatures were probably 5°–6°C cooler than at present. At that time bushveld vegetation in the central Transvaal was replaced by open grassland with macchia elements. Climatic amelioration came and semiarid savanna returned to the plains, at first gradually and then developing into a warm Kalahari thornveld-type vegetation. After 6000 yr B.P. it apparently became slightly wetter and a more broad-leafed bushveld developed. About 4000 yr B.P. it again became cooler and slightly wetter and the bushveld vegetation on the central and northern plains was comparable to present open upland types. After 2000 yr B.P. conditions gradually became warner until about 1000 yr B.P., when the modern climate of the central Transvaal bushveld originated.     

Aspects of diamond mineralisation and distribution at the Helam Mine, South Africa

The diamonds from the Swartruggens dyke swarm are mainly tetrahexahedra, with subsidiary octahedral and cuboid crystals. They are predominantly colourless, with subordinate yellows, browns, and greens. The existence of discrete cores and oscillatory growth structures within the diamonds, together with the recognition of harzburgite, lherzolite, at least two eclogitic and a websteritic diamond paragenesis, variable nitrogen contents, and both Type IaAB and Type Ib–IaA diamonds provides evidence for episodic diamond growth in at least six different environments. The predominance of plastic deformation in the diamonds, the state of nitrogen aggregation, and the suite of inclusion minerals recovered are all consistent with a xenocrystic origin for the diamonds, with the Type Ib–IaA diamonds being much younger than the rest. Mantle storage at a time-averaged temperature of ±1100 °C is inferred for the Type IaAB diamonds. The distribution of mantle xenocrysts of garnet and chromite within the high-grade Main kimberlite dyke compared to the low-grade Changehouse kimberlite dyke strongly suggests that the difference in diamond content is due to an increased eclogitic component of diamonds in the Main kimberlite dyke.     

Recent advances in the geology of Koffiefontein Mine, Free State Province, South Africa

The complex internal geology of the Koffiefontein pipe has contributed to the marginal nature of the mine. The key to this is the presence of a large zone dominated by down-rafted country rock Karoo sediment and dolerite xenoliths. Recent work indicates that the kimberlite pipe at Koffiefontein consists of precursor dykes (the West and East Fissures), and the main pipe, in which two main eruptive phases have been recognized. Groundmass spinel compositions have been used to provide a chemical fingerprint of each lithology. There is evidence for at least three magma batches, each with its own chemical signature. Cross-cutting contact relationships were used to determine the emplacement sequence. The characterization of the different internal geological units permitted the development of a three-dimensional (3D) model of the pipe. Both main eruptive phases, viz., the Speckled west kimberlite and the Speckled east kimberlite comprise volcaniclastic kimberlite. They are separated by a large irregular mass of kimberlite that contains abundant country rock xenoliths comprising varying proportions of Karoo mudstone and dolerite, as well as probable bedded crater–facies fragments. This zone of contamination dilutes the grade of the kimberlites, affects the geotechnical stability and adversely affects the economics of the mine.     

A palaeoenvironmental interpretation of the Early Proterozoic Malmani dolomite from Zwartkops,South Africa

The Malmani Subgroup northwest of Johannesburg consists of dolomite and chert with only minor clastic sediments.A precise upper intertidal to marginal supratidal analogy and the associated relationship of varied structures suggest that much of the succession represents a tidal flat to intertidal complex formed within differing semiprotected to protected conditions. The dolomites from these environments are recrystallized, reflecting a meteoric influence, and the cherts which are commonly developed within them are also related to prevailing lower pH's. This dolomitization is considered to have been enhanced by the influx of meteoric waters which however resulted in the dolomites having undersaturated iron-manganese ratios. Rare colour-banded dolomites containing columnar stromatolites are thought to represent more steeply shelving intertidal conditions than are normally encountered in the epeiric sea. These dolomites contain quartz crystals rather than chert, suggestive of a lower concentration of silica in the original alkaline solutions. The exposure is part of a very widespread carbonate unit, dated at ca. 2.250 m.y.Subtidal conditions in which large elongate stromatolitic domes developed can be related to a marine transgression across a basal clastic beach sand; and secondly to a progradational tidal flat seawards of which a talus breccia developed on a steepened slope leading down to the subtidal regime. These dolomites formed by interaction with marine waters saturated with respect to iron and manganese, while the absence of chert reflects persisting alkaline conditions.A dark chert-free dolomitic facies with high iron and manganese contents of saturated ratios is considered to have developed in an alkaline lagoonal environment behind a subaqueous bar that is now represented by an overlying thick oolitic unit.The succession contains numerous chert breccias with which shales are associated. The breccias represent subaerial exposure phenomena related to regressions which were followed by periods of short-lived terrigenous influx.     

Geochemical dispersion from the Gamsberg Orebody, northwestern Cape, South Africa

The geochemical dispersion, in an arid environment, of Pb and Zn in stream sediments is examined with respect to size fractions and depth of sampling in a stream draining the Gamsberg Zn orebody.Sampling results indicate that there is a well-developed drainage train for approximately 8 km from the orebody for both Pb and Zn. The length of the drainage train is similar for both the minus 80 and minus 200-mesh size fractions but it is less for the minus 10, plus 40-mesh fraction.Higher metal values were obtained from samples taken from the surface of the stream bed. Metal values are generally lower in samples collected below the surface of the stream bed. The sampling position within the stream channel is not important.Sampling of the magnetite fraction from the stream sediments produced a well-defined Zn train for a distance of 14 km from the orebody. This train is more significant than the train found by normal sediment sampling.     

Accessory mineralogy of orangeite from Swartruggens, South Africa

Summary ?Orangeite occurring as a complex series of dikes at Swartruggens (South Africa), is host to a diversity of accessory minerals, the most common of which are apatite, barite and calcite. Less common, but important phases are perovskite, wadeite, an unidentified Ca–Ti–Fe-silicate, strontianite, unidentified Ca-REE phosphate, zircon, rutile, titaniferous magnetite, quartz and diverse sulphides. The accessory minerals show wide variations in their mode in different segments of the dike suite as a consequence of crystal sorting during flow differentiation. Compositional data are given for apatite, barite, calcite, perovskite, wadeite and the unidentified Ca–Ti–Fe-silicate. The accessory mineral suite is similar to that found in lamproites but is sufficiently distinct in composition and paragenesis to preclude inclusion with that clan. Differences include the common presence of groundmass calcite, barite and serpentine in the orangeite and the absence of typomorphic minerals (leucite, sanidine, richterite) of the lamproite clan. Received January 15, 2001; revised version accepted October 15, 2001     

Two diamond-bearing peridotite xenoliths from the finsch kimberlite,South Africa

Two diamond bearing xenoliths found at Finsch Mine are coarse garnet lherzolites, texturally and chemically similar to the dominant mantle xenoliths in that kimberlite. A total of 46 diamonds weighing 0.053 carats have been recovered from one and 53 diamonds weighing 0.332 carats from the other. The diamonds are less corroded than diamonds recovered from the kimberlite. Geothermobarometric calculations indicate that the xenoliths equilibrated at 1,130° C and pressures 50 kb which is within the diamond stability field; this corresponds to depths of 160 km and would place the rocks on a shield geotherm at slightly greater depths than most coarse garnet lherzolites from kimberlite. The primary minerals in the two rocks are very similar to each other but distinctly different to the majority of mineral inclusions in Finsch diamonds. This suggests a different origin for the diamonds in the kimberlite and the diamonds in the xenoliths although the equilibration conditions for both suites are approximately coincident and close to the wet peridotite solidus.     

A TEM investigation of shock metamorphism in quartz from the Vredefort dome, South Africa

The origin of the Vredefort structure in South Africa is still debated. Several causes have been discussed, namely asteroid impact, internal gas explosion or tectonic processes. Evidence of dynamic rock deformation is pervasive in the form of planar features in quartz grains, shatter cones, veins of pseudotachylite and occurrence of coesite and stishovite (high-pressure quartz polymorphs). A number of these characteristics is widely believed to support an impact origin. However, the planar features in quartz, which are generally considered as one of the strongest indicators of impact, are in the Vredefort case considered as anomalous when compared with those from accepted impact structures.

We have investigated by optical and transmission electron microscopy (TEM) the defect microstructures in quartz grains from different lithologies sampled at various places at the Vredefort structure. Whatever the locality, only thin mechanical Brazil twin lamellae in the basal plane are observed by TEM. So far, such defects have only been found in quartz from impact sites, but always associated with sets of thin glass lamellae in rhombohedral planes 10−1n with n = 1, 2, 3, and 4. At the scale of the optical microscope, Brazil twins in (0001) are easily detected in Vredefort quartz grains because of the numerous tiny fluid inclusions which decorate them. Similar alignments of tiny fluid inclusions parallel to other planes are also detected optically, but at the TEM scale no specific shock defects are detected along their traces. If these inclusion alignments initially were shock features, they are now so severely weathered that they can no longer be recognized as unambiguous shock lamellae. Fine-grained coesite was detected in the vicinity of narrow pseudotachylite veinlets in a quartzite specimen, but stishovite was not found, even in areas where its occurrence was previously reported. Finally, definite evidence of high-temperature annealing was observed in all the samples. These observations lead us to the conclusion that our findings regarding microdeformation in quartz are consistent with an impact origin for the Vredefort structure. Most of the original shock defects are now overprinted by an intense post-shock annealing episode. Only the thin mechanical twin lamellae in the basal plane have survived.     

Diamondiferous garnet harzburgites from the Finsch kimberlite,Northern Cape,South Africa

Two xenoliths of garnet harzburgite from the Finsch kimberlite, South Africa, have been found to contain diamond. One of the xenoliths has mineral compositions typical of low-T coarse textured garned peridotites, whereas minerals in the other are similar but not identical to most peridotite-suite minerals included in diamonds, especially in the low-CaO content of garnet. Geothermobarometric calculations show both xenoliths equilibrated at temperatures above 1,100°C and pressures>55 kbar, which is near the low-pressure end of the range of equilibration conditions for diamond-free garnet lherzolites and garnet harzburgites from Finsch. The chemistries of the minerals in the two rocks are distinctly different to most of the mineral inclusions in Finsch diamonds. This, as well as the different ¹³C compositions between xenolith diamonds (-2.8 to-4.6) and diamonds in the kimberlite (generally<-4.3) suggest different origins or sources for the diamonds.     

A sand budget for the Alexandria coastal dunefield, South Africa

The sand in the Alexandria coastal dunefield is derived from the sandy beach which forms the seaward boundary of the dunefield. Sand is blown off the beach onto the dunefield by the high-energy onshore-directed dominant wind. The dunefield has been forming over the past 6500 years. Sand transport rates calculated from dune movement rates and wind data range from 15 to 30 m³ m ^-1 yr^-1 in an ENE direction. The sand transport rate decreases with increasing distance from the sea due to a reduction in wind speed resulting from the higher drag imposed upon the wind by the land surface. Aeolian sand movement rates of this order are typical of dunefields around the world. The total volume of sand blown into the dunefield is 375 000 m³ yr^-1. Sand is being lost to the sea by wave erosion along the eastern third of the dunefield at a rate of 45 000 m³ yr ^-1. The dunefield thus gains 330 000 m³ of sand per year. This results in dunefield growth by vertical accretion at about 1.5 mm yr^-1 and landward movement at about 0.25 m yr^-1. The dunefield is a significant sand sink in the coastal sand transport system. The rate of deposition in coastal dunefields can be 10 times as high as rates of deposition in continental sand seas. The higher rate of deposition may result from the abundant sand supply on sandy beaches, and the higher energy of coastal winds. Wind transport is slow and steady compared to fluvial or longshore drift transport of sediment, and catastrophic aeolian events do not seem to be significant in wind-laid deposits.     

A ferrotantalite-ferrotapiolite intergrowth from Spittal a.d. Drau,Carinthia, Austria

Summary Intimate intergrowths of ferrotantalite and ferrotapiolite occur in a pegmatite in Spittal a.d. Drau, Carinthia. They are associated with muscovite, albite, smoky quartz, cassiterite, and microscopic uranmicrolite, zircon and uraninite. An assemblage of secondary uranium minerals is also present, generated by extensive alteration and leaching of the uranmicrolite and zircon. Textures of the ferrotantalite-ferrotapiolite intergrowths suggest considerable recrystallization that obliterated most of their primary features; neither coprecipitation nor exsolution can be recognized with certainty. Despite intersecting tielines indicating disequilibrium, the ferrotantalite and ferrotapiolite compositions show very restricted ranges (Mn/(Mn + Fe) 0.08–0.11, Ta/(Ta + Nb) 0.53–0.57 for ferrotantalite, and 0.01–0.04, 0.84–0.89 for ferrotapiolite, respectively), particularly in comparison with compositions from other localities featuring primary textures. A degree of compositional equilibration could have been attained during recrystallization. This process may also explain the high level of structural order characterizing both minerals; they are considerably disordered in other localities. Extensive deformation typical of pegmatites in the southern Ostalpen in general, and specifically of the Spittal pegmatite, is probably responsible for the recrystallization phenomena in the Ta, Nb, Sn-bearing mineral assemblage.

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Eine Ferrotantalit-Ferrotapiolit Verwachsung von Spittal a.d. Drau, Kärnten, österreich

Zusammenfassung In einem Pegmatit von Spittal a.d. Drau, Kärnten, treten enge Verwachsungen von Ferrotantalit und Ferrotapiolit auf. Diese werden von Muskovit, Albit, Rauchquarz, Zinnstein sowie-in mikroskopischem Masstab-von Uranmikrolith und Zirkon begleitet. Die Textur der Verwachsungen lässt Rekristallisation erheblichen Ausmasses erkennen, die die primären Merkmale weitgehend auslöscht. Weder eine gemeinsame Auskristallisation der beiden Mineralphasen noch eine Bildung durch Entmischung kann mit Sicherheit erkannt werden. Trotz einander kreuzender Verbindungslinien, die einen Hinweis auf Ungleichgewicht darstellen, zeigen die Zusammensetzungen des Ferrotantalits und des Ferrotapiolits lediglich geringe Schwankungsbreiten: Mn/(Mn + Fe) 0,08–0,11, Ta/(Ta + Nb) 0,53–0,57 für den Ferrotantalit beziehungsweise 0,01–0,04 und 0,84–0,89 für den Ferrotapiolit. Dies gilt insbesondere für den Vergleich mit Zusammensetzungen solcher Mineralphasen mit jenen von Fundarten, die primäre Verwachsungstrukturen aufweisen. Bis zu einem gewissen Ausmass ist diese homogene Zusammensetzung möglicherweise auf die Rekristallisation zurück zuführen. Diese Rekristallisation könnte auch den hohen strukturellen Ordnungsgrad der beiden Mineralphasen erklären. An anderen Fundorten zeigen diese Minerale strukturell merklich geringeren Ordnungsgrad. Intensive metamorphe überprägung, wie sie für die Pegmatite in den südlichen Ostalpen und insbesondere für jenen von Spittal typisch sind, kann wahrscheinlich als Ursache der Rekristallisationsphänomene der Ta-Nb-Sn Mineralparagenese angenommen werden.

     

一种新型南非紫色玉石的矿物学特征研究

为探究南非最近产出的一种新型紫色玉石的矿物学特征及颜色成因,对其进行了常规宝石学特征测试,并采用X射线粉末衍射仪（XRD）、扫描电子显微镜（SEM）及紫外-可见分光光度计（UV-Vis）等仪器对其矿物组成、结构特征、化学成分和致色元素进行了研究。常规宝石学测试结果表明,该玉石折射率为1．54（点测）,相对密度为2．1-2．2,摩氏硬度为1-2。XRD分析结果表明样品主要矿物组成为鳞镁铁矿,呈紫色,次要矿物成分为利蛇纹石,呈褐绿色;SEM分析结果显示鳞镁铁矿大多为集合体,主要以鳞片状和纤维状两种集合体形式存在,能谱分析（EDS）结果显示紫色部分主要化学成分为Mg,O,C,Fe,Cr等,佐证了紫色部分为鳞镁铁矿;UV-Vis结合EDS分析结果显示,鳞镁铁矿的紫色可能由Cr致色引起。