Distribution of trace elements during breakdown of mantle garnet: an example from Zabargad

Ion probe investigations on mineral phases forming the Al-Di pyroxenites from the Zabargad peridotite body indicate that porphyroclastic pyroxenes in composite mafic layers record an unusual HREE, Zr, Sc enrichment not registered by pyroxenes in spinel websterites. Orthopyroxene in the opx+sp clusters forming the inner, cpx-free zone of layered pyroxenites shows strongly fractionated REE patterns (HREE_N/LREE_N>1000; Yb>100xch) and very high Zr, Sc and Y abundances (up to 30,672 and 60ppm, respectively). In the outer, cpx-rich zone porphyroclastic clinopyroxene is strongly HREE enriched (HREE_N/LREE_N29; Yb 269xch) and displays very high Sc and Zr abundances (up to 819 and 164 ppm, respectively). It is suggested that the unusual trace element abundances are inherited from a precursor garnet. Composite pyroxenite layers are interpreted as former garnet clinopyroxenites characterized by gnt/cpx modal zoning. The sp+opx(cpx-free) assemblage in the inner part is a product of the break-down reaction of garnet upon decompression, with Ca of the original garnet completely entering the enstatite solid solution. The temperature at which the breakdown reaction occurred is estimated to be higher than 1000°C (P in the range 20–30 kbar). In the outer part, decompression caused the garnet to form a sp+opx assemblage; however, the grossularite component participated in the formation of new clinopyroxene which reacted with the clinopyroxene present in the original mode before the decompression reaction, thus forming a cpx₂+sp+opx assemblage. As a result of garnet breakdown, pyroxenes have peculiar HFSE anomalies. Progressive upwelling during the Red Sea rifting produced incomplete reaction under pl-facies conditions. The geochemical signatures of precursor garnet in pyroxenes were partially crased during the recrystallization from granular spincl-bearing to granoblastic plagioclase-bearing assemblages, being preserved only in a few porphyroclast relies. The finding of pyroxenes with trace element characteristics of precursor garnet has important geodynamic and geochemical implications. Al-Di pyroxenite layers had a long history within the mantle, before the continental lithosphere rifting and thinning took place in the region. It is suggested that Al-Di pyroxenites were formed by deep-seated tholeiitic magmatism unrelated to the Red Sea evolution, thus representing the earliest event in the Zabargad upper mantle. Garnet breakdown significantly preceded the metasomatism induced by hydrous fluids (crystallization of Ti-rich pargasite) and the later intrusion of hydrous (Cr-Di) pyroxenite dykes. During the stages of mantle evolution, the HFSE anomalies in pyroxenes varied significantly. We note that the study of HFSE anomalies in mineral phases reveals complex geochemical histories which are not recorded by the whole-rock system.     

Les péridotites et pyroxénolites à grenat du Bois des feuilles (Monts du lyonnais) (France)

The author describes a new occurrence of garnet peridotite and garnet pyroxenite interlayered in the biotite-sillimanite-garnet gneisses at the top of the granulitic serie of the Monts du Lyonnais (Massif Central français). Its dimensions are rather significant for a crustal gisement (500×100 m). It is only composed of forsterite, enstatite, chromiferous diopside, pyrope and spinel peridotites with their products of retrograde transformations as kelyphites, amphiboles, chlorites, lizardite, ores, etc. The petrographic studies show the heterogeneity of the massif and the anteriority of the red spinel upon the garnet which always forms a corona around the spinel. The peridotites are intermingled with numerous streched and dislocated layers of garnet websterites with rare centimetric levels. These pyroxenites would be derived of particular magmatic processes (partial anatectic melting followed by cristallisation) developped from an upper mantle level in a primary pyrolitic lherzolitic (s. l) or garnet peridotitic material. The garnet peridotite of “Le Bois des Feuilles” would be, in fact, a “secondary garnet lherzolite” derived: - either from a spinel lherzolite intermingled with garnet websterite layers and their “dunitic” remnants, to form a “pseudo-garnet lherzolite” like this of Beni Bouchera described by Kornprobst; - or from a spinel lherzolite associated with garnet websterites and submitted temporarily, at the time of its diapiric rising movement from the mantle towards the crust to the conditions of the spinel garnet lherzolite facies. The plastic deformations and intense laminations form blastomylonites of mixed rocks recristallised ultimately under granulitic facies conditions. These rocks are, pro parte, not very different from the other crustal garnet peridotites, in spite of the frequency of the spinel inclusions in garnet. In corollary, it seems that numerous crustal garnet peridotites would have the same origin.     

High-pressure Partial Melting of Mafic Lithologies in the Mantle

We review experimental phase equilibria associated with partialmelting of mafic lithologies (pyroxenites) at high pressuresto reveal systematic relationships between bulk compositionsof pyroxenite and their melting relations. An important aspectof pyroxenite phase equilibria is the existence of the garnet–pyroxenethermal divide, defined by the enstatite–Ca-Tschermakspyroxene–diopside plane in CaO–MgO–Al₂O₃–SiO₂projections. This divide appears at pressures above 2 GPa inthe natural system where garnet and pyroxenes are the principalresidual phases in pyroxenites. Bulk compositions that resideon either side of the divide have distinct phase assemblagesfrom subsolidus to liquidus and produce distinct types of partialmelt ranging from strongly nepheline-normative to quartz-normativecompositions. Solidus and liquidus locations are little affectedby the location of natural pyroxenite compositions relativeto the thermal divide and are instead controlled chiefly bybulk alkali contents and Mg-numbers. Changes in phase volumesof residual minerals also influence partial melt compositions.If olivine is absent during partial melting, expansion of thephase volume of garnet relative to clinopyroxene with increasingpressure produces liquids with high Ca/Al and low MgO comparedwith garnet peridotite-derived partial melts. KEY WORDS: experimental petrology; mantle heterogeneity; partial melting; phase equilibrium; pyroxenite     

Incomplete high P–T metamorphic transitions within the Kvamsøy pyroxenite complex, west Norway: a case study of disequilibrium

Abstract The Kvamsøy pyroxenite complex consists of olivine websterite, olivine gabbro and leucogabbro-norite which have been subjected to regional high P-T (HPT) metamorphism. The metamorphism has resulted in a range of disequilibrium textures with the development of coronas and pseudomorphism of the igneous phases. Reactions between felsic and mafic mineral domains have been controlled by variable and selective diffusion of elements, resulting in a variety of local plagioclase-breakdown reactions and in significant compositional variations for the product garnet. Restricted diffusion favours transient reaction stages with garnet ± spinel ± corundum ± zoisite after calcic plagioclase in olivine gabbro and olivine websterite and garnet ± spinel ± kyanite ± quartz + sodic plagioclase in leucogabbro-norite. Complete HPT reaction has produced garnet pyroxenite which consists of garnet + diopside + hornblende + zoisite in gabbroic rocks, while amphibolitization continued during the cooling and uplift history. Grt + Ky + Pl + Qtz geobarometry suggests pressures in the range 13-16 kbar for T = 750°C, comparable with the regional eclogite-forming metamorphism.     

Melts of garnet lherzolite: experiments, models and comparison to melts of pyroxenite and carbonated lherzolite

Phase equilibrium experiments on a compositionally modified olivine leucitite from the Tibetan plateau have been carried out from 2.2 to 2.8 GPa and 1,380–1,480 °C. The experiments-produced liquids multiply saturated with spinel and garnet lherzolite phase assemblages (olivine, orthopyroxene, clinopyroxene and spinel ± garnet) under nominally anhydrous conditions. These SiO₂-undersaturated liquids and published experimental data are utilized to develop a predictive model for garnet lherzolite melting of compositionally variable mantle under anhydrous conditions over the pressure range of 1.9–6 GPa. The model estimates the major element compositions of garnet-saturated melts for a range of mantle lherzolite compositions and predicts the conditions of the spinel to garnet lherzolite phase transition for natural peridotite compositions at above-solidus temperatures and pressures. We compare our predicted garnet lherzolite melts to those of pyroxenite and carbonated lherzolite and develop criteria for distinguishing among melts of these different source types. We also use the model in conjunction with a published predictive model for plagioclase and spinel lherzolite to characterize the differences in major element composition for melts in the plagioclase, spinel and garnet facies and develop tests to distinguish between melts of these three lherzolite facies based on major elements. The model is applied to understand the source materials and conditions of melting for high-K lavas erupted in the Tibetan plateau, basanite–nephelinite lavas erupted early in the evolution of Kilauea volcano, Hawaii, as well as younger tholeiitic to alkali lavas from Kilauea.     

Some subcalcic clinopyroxenites from Salt Lake Crater,Oahu, and their petrogenetic significance

Some inclusions from Salt Lake Crater are essentially single-phase subcalcic clinopyroxenites whose original clinopyroxenes, prior to extensive unmixing, were tschermakitic subcalcic varieties with compositions close to Ca₃₄Mg₅₄Fe₁₂. In addition to copious amounts of orthopyroxene, very minor garnet and spinel also were exsolved from the subcalcic clinopyroxenes.The genesis of the garnet pyroxenite suite at Salt Lake Crater has been examined in terms of three models, namely: (i) cumulates from alkali basaltic magmas; (ii) fractional fusion of basanitic garnet clinopyroxenite; and (iii) anatexis of upper mantle lherzolites. Field, mineralogical, chemical and experimental data collectively favour model (iii) and indicate that the nodules are genetically unrelated to their nephelinitic hosts. The Salt Lake garnet pyroxenites can be closely equated with the garnet pyroxenites in magmatictype layers in certain alpine-type ultramafic massifs and they are also similar to many garnet pyroxenite xenoliths in alkaline volcanics from other localities.Liquids produced by anhydrous partial melting of spinel Iherzolite at pressures of approximately 20 kb commonly have picritic chemistries. The crystallization behaviour of picritic liquids at elevated pressures ( 20 kb) indicates that the initial crystallization products may be either essentially single-phase subcalcic clinopyroxenites (with minimal high pressure fractionation) or a range of olivine-aluminous orthopyroxene-aluminous subcalcic clinopyroxene-garnet-(spinel) assemblages with variable 100 Mg/(Mg+Fe) ratios (when fractionation has been operative). All these assemblages may be subsequently modified by subsolidus exsolution and recrystallization.     

大别山北麓尖晶石橄榄岩中石榴辉石岩包体的成因矿物学信息

大别山北坡霍山饶拔寨等地的超基性岩中含有石榴辉石岩的包体。石榴辉石岩为草绿色致密块状 ,呈分米级的块体出现于蛇纹石化强烈的橄榄岩中。运用成因矿物学的方法 ,研究对比了石榴辉石岩的主要矿物组成石榴子石 ( Prp2 5— 3 5 )和钠质普通辉石 ( Jd1 0— 2 5 )等。岩石结构显示退变质作用有两期 :榴辉岩相退变形成的麻粒岩相矿物组合明显地被角闪岩相所切割。石榴辉石岩的寄主岩是尖晶石橄榄岩类 ,包括尖晶石方辉橄榄岩和尖晶石二辉橄榄岩。由于强烈的蛇纹石化 ,残余的橄榄石 ( Fo92— 93 )仅占 5%～ 4 0 % ,斜方辉石富镁 ( En87— 93)并有解理弯曲等韧性变形现象。采用 Ellisand Green的石榴子石单斜辉石 Fe-Mg交换平衡温度计 ,可计算出石榴辉石岩的 Fe-Mg分配系数 ( KD)为 4 .0 6～ 5.2 8。变质温度 t=84 1～ 94 3℃ ,估算压力 p=1 .5GPa,可以推测该橄榄岩体是从深度约 60 km的地幔 ,固态侵位于下地壳 ,而后与之一起隆升到地表。显然 ,此种石榴辉石岩应属 Coleman所划分的 A型榴辉岩 ,它与地幔岩浆作用有密切关系。石榴辉石岩和橄榄岩的岩石化学特征和稀土配分形式 ,说明它们的化学性质相当于地幔部分熔融所形成的玄武岩熔体及其残留体。在侧重探讨石榴辉石岩及其有关岩石中主要造岩矿物的成因矿物?     

Amphibole pyroxenite xenoliths: Cumulate or replacement phenomena from the upper mantle,Nunivak Island,Alaska

Interstitial to poikilitic amphibole found in garnet pyroxenite xenoliths has been interpreted, in the past, to represent a critically silica undersaturated, residual intercumulus melt trapped by its cumulate assemblage of anhydrous phases. The textural features of such amphibole in pyroxenite xenoliths from Nunivak Island, Alaska, however, are more compatible with an origin by replacement of the anhydrous phases of the pyroxenite, following a period of cooling and sub-solidus recrystallization in the upper mantle. The reaction of amphibole and olivine to give orthopyroxene, observed in two specimens, requires that the associated fluid phase was not critically silica undersaturated. The amphibole is therefore thought to reflect the interaction of an alkali-bearing, migratory, aqueous fluid and an upper mantle consisting of spinel lherzolite cut by veins of spinel and garnet pyroxenite.     

Anhydrous partial melting of an iron-rich mantle I: subsolidus phase assemblages and partial melting phase relations at 10 to 30 kbar

Anhydrous partial melting experiments, at 10 to 30 kbar from solidus to near liquidus temperature, have been performed on an iron-rich martian mantle composition, DW. The DW subsolidus assemblage from 5 kbar to at least 24 kbar is a spinel lherzolite. At 25 kbar garnet is stable at the solidus along with spinel. The clinopyroxene stable on the DW solidus at and above 10 kbar is a pigeonitic clinopyroxene. Pigeonitic clinopyroxene is the first phase to melt out of the spinel lherzolite assemblage at less than 20°C above the solidus. Spinel melts out of the assemblage about 50°C above the solidus followed by a 150° to 200°C temperature interval where melts are in equilibrium with orthopyroxene and olivine. The temperature interval over which pigeonitic clinopyroxene melts out of an iron-rich spinel lherzolite assemblage is smaller than the temperature interval over which augite melts out of an iron-poor spinel lherzolite assemblage. The dominant solidus assemblage in the source regions of the Tharsis plateau, and for a large percentage of the martian mantle, is a spinel lherzolite.     

A possible role for garnet pyroxenite in the origin of the “garnet signature” in MORB

 Geochemical data have been interpreted as requiring that a significant fraction of the melting in MORB source regions takes place in the garnet peridotite field, an inference that places the onset of melting at ≥80 km. However, if melting begins at such great depths, most models for melting of the suboceanic mantle predict substantially more melting than that required to produce the 7±1 km thickness of crust at normal ridges. One possible resolution of this conflict is that MORBs are produced by melting of mixed garnet pyroxenite/spinel peridotite sources and that some or all of the “garnet signature” in MORB is contributed by partial melting of garnet pyroxenite layers or veins, rather than from partial melting of garnet peridotite. Pyroxenite layers or veins in peridotite will contribute disproportionately to melt production relative to their abundance, because partial melts of pyroxenite will be extracted from a larger part of the source region than peridotite partial melts (because the solidus of pyroxenite is at lower temperature than that of peridotite and is encountered along an adiabat 15–25 km deeper than the solidus of peridotite), and because melt productivity from pyroxenite during upwelling is expected to be greater than that from peridotite (pyroxenite melt productivity will be particularly high in the region before peridotite begins melting, owing to heating from the enclosing peridotite). For reasonable estimates of pyroxenite and peridotite melt productivities, 15–20% of the melt derived from a source region composed of 5% pyroxenite and 95% peridotite will come from the pyroxenite. Most significantly, garnet persists on the solidus of pyroxenite to much lower pressures than those at which it is present on the solidus of peridotite, so if pyroxenite is present in MORB source regions, it will probably contribute a garnet signature to MORB even if melting only occurs at pressures at which the peridotite is in the spinel stability field. Partial melting of a mixed spinel peridotite/garnet pyroxenite mantle containing a few to several percent pyroxenite can explain quantitatively many of the geochemical features of MORB that have been attributed to the onset of melting in the stability field of garnet lherzolite, provided that the pyroxenite compositions are similar to the average composition of mantle-derived pyroxene-rich rocks worldwide or to reasonable estimates of the composition of subducted oceanic crust. Sm/Yb ratios of average MORB from regions of typical crustal thickness are difficult to reconcile with derivation by melting of spinel peridotite only, but can be explained if MORB sources contain ∼5% garnet pyroxenite. Relative to melting of spinel peridotite alone, participation of model pyroxenite in melting lowers aggregate melt Lu/Hf without changing Sm/Nd ratios appreciably. Lu/Hf-Sm/Nd systematics of most MORB can be accounted for by melting of a spinel peridotite/garnet pyroxenite mantle provided that the source region contains 3–6% pyroxenite with ≥20% modal garnet. However, Lu/Hf-Sm/Nd systematics of some MORB appear to require more complex melting regimes and/or significant isotopic heterogeneity in the source. Another feature of the MORB garnet signature, (²³⁰Th)/(²³⁸U)>1, can also be produced under these conditions, although the magnitude of (²³⁰Th)/(²³⁸U) enrichment will depend on the rate of melt production when the pyroxenite first encounters the solidus, which is not well-constrained. Preservation of high (²³⁰Th)/(²³⁸U) in aggregated melts of mixed spinel peridotite/garnet pyroxenite MORB sources is most likely if the pyroxenites have U concentrations similar to that expected in subducted oceanic crust or to pyroxenite from alpine massifs and xenoliths. The abundances of pyroxenite in a mixed source that are required to explain MORB Sm/Yb, Lu/Hf, and (²³⁰Th)/(²³⁸U) are all similar. If pyroxenite is an important source of garnet signatures in MORB, then geochemical indicators of pyroxenite in MORB source regions, such as increased trace element and isotopic variability or more radiogenic Pb or Os, should correlate with the strength of the garnet signature. Garnet signatures originating from melts of the garnet pyroxenite components of mixed spinel peridotite/garnet pyroxenite sources would also be expected to be stronger in regions of thin crust. Received: 15 February 1995/Accepted: 7 February 1996     

Elementverteilung im Liegenden des Kupferschiefers

The leached zone below the Kupferschiefer was investigated in two drillholes (drillhole Drevenack: Zechsteinconglomerate, drillhole Rannungen: grey sandstone) using sedimentpetrographical and geochemical methods. Samples were taken from the uppermost red coloured Rotliegend up to directly below the Kupferschiefer. No big differences concerning the mineral composition and the distribution of elements between the red coloured and the leached rocks have been found. The border between the two is no boundary for the changes which took place during diagenesis.The trace element concentrations in both profiles are higher than the average values. The higher concentrations of elements in the whole leached zone must be interpreted as due to mobilisation from the underground. Besides, there is a clear zone of additional enrichment just below the Kupferschiefer which is a result of impregnation from it.The elements were set free during recrystallisation of haematite. Cu, Ni and Pb are present possibily as sulfides whereas Mn and Zn are in the carbonates.

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Herrn Prof. Dr. Dr. h.c. C. W. Correns und Herrn Prof. Dr. K. H. Wedepohl danke ich für zahlreiche Diskussionen und Anregungen. Herrn Prof. Dr. H. Harder danke ich für die Arbeitsmöglichkeit im Sedimentpetrographischen Institut.

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Der Gewerkschaft Brigitta danke ich für die Überlassung der Bohrproben Rannungen, der Hamborner Bergbau AG für die Proben der Bohrung Drevenack.

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Der Deutschen Forschungsgemeinschaft bin ich für finanzielle Unterstützung zu Dank verpflichtet.     

Experimental melting of a modally heterogeneous mantle

Summary Melting of a spinel lherzolite with a spinel clinopyroxenite layer was investigated experimentally from 3.5 to 20 kbar and from 1200 to 1450 °C. The melt fraction in the spinel pyroxenite layer increases rapidly, and clinopyroxene disappears leaving olivine-spinel residua according to the reaction Cpx + Sp = Ol + Liq. The melt in the pyroxenite layer reacts with the surrounding lherzolite resulting in the formation of an essentially monomineral (olivine) zone with interstitial melt near the former pyroxenite. Melt compositions in the central melt pool are similar to those produced by other authors in melting experiments with peridotites similar to the bulk compositions of our samples. It is suggested that similar small-scale mantle heterogeneities (i.e. thin pyroxenite layers in lherzolite) may exert significant influence on mantle rheology and melt segregation, whereas melt compositions are not strongly affected and controlled by the dominating lherzolite lithology. Received October 10, 2000; revised version accepted August 31, 2001     

Wege in die Tiefen

Zusammenfassung Die Vorstellungen über Natur und Bewegungen der tiefen, nicht aufgeschlossenen Krustenteile hängen weitgehend von der Wahl der Deutungsprinzipien und Leitbilder für die Erscheinungen der sichtbaren Krustenteile ab.Einführungsvortrag zum Kapitel Der Tiefbau der Orogene der 50. Jahrestagung der Geologischen Vereinigung im März 1960 in Würzburg.     

Garnet-spinel-pyroxenite xenoliths from hyblean plateau (South-eastern Sicily, Italy)

Summary Rare garnet-spinel pyroxenite xenoliths occur in some basaltic tuff-breccia levels of Miocene age from the Valle Guffari (Hyblean Plateau, Sicily), together with a number of spinel-bearing mantle xenoliths. The garnet-bearing pyroxenites may be divided into two groups (a and b) on textural and mineralogical bases. Garnet-bearing spinel websterites with a fully recrystallized texture represent the first group (a). Here the garnet (Py_54.5 A1m₃₂ Gr_13.5), with a diffuse kelyphitic alteration, forms a reaction corona between coarse spinel grains and the in contact pyroxenes. The transition from the spinel-pyroxenite to the garnet-pyroxenite field may depend on isobaric cooling from higher (magmatic?) temperatures. Garnet-pyroxene geothermometry indicates that the last equilibration most probably occurred at P = 1.0 GPa (ca.), T = 750 °C (ca).The second lithotype (b) is an orthopyroxene-bearing garnet-spinel clinopyroxenite, exhibiting a complex texture. It consists of zones of coarse clinopyroxene grains enclosing euhedral spinel passing to zones where tiny rounded crystals of the same pyroxene and spinel are enclosed in relatively large patches of extensively kelyphitisized garnet (Py_64.8 Alm_25.6 Gr_9.6). Garnet also occurs as inclusion-free grains up to 4 mm in diameter. P-T calculations give significantly higher values than for the former case (a). The origin of the b-type garnet may also depend on subsolidus reaction of spinel and pyroxenes after an isobaric cooling from still higher temperatures, but a primary magrnatic origin might also be possible, especially for the granular garnets.P-T estimates for both the pyroxenite types closely match a steady geotherm for 100 mW/m² surface heat flow. Such a relatively intense heat flow may suggest the occurrence of huge masses of hot magma intruding the Hyblean lithospheric mantle and lower crust at different levels.

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Granat-Spinell-Pyroxenit-Xenolithe aus dem Iblei-Plateau (Südost-Sizilien, Italien)

Zusammenfassung Seltene Granat-Spinell-Pyroxenit-Xenolithe kommen in einigen basaltischen Tuff-Breckzien Horizonten miozänen Alters aus dem Valle Guffari (lblei-Plateau, Sizilien) zusammen mit einer Anzahl von Spinell-führenden Mantel-Xenolithen vor. Aufgrund textureller und mineralogischer Kriterien können die Granat-führenden Pyroxenite in zwei Gruppen (a und b) unterteilt werden. Granat-führende Spinell-Websterite mit vollkommen rekristallisierter Textur repräsentieren die erste Gruppe (a). Hier bildet Granat (Py_54.5 Alm₃₂ Gr_13.5) mit einer diffusen kelyphitischen Umwandlung, einen Reaktionssaum zwischen grobkörnigem Spinell und Pyroxenen, mit denen er in Kontakt ist. Der übergang vom Spinell-Pyroxenit- zum Granat-Pyroxenit-Feld kann auf isobarische Abkühlung von höheren (magmatischen ?) Temperaturen zurückgehen. Granat-Pyroxen-Geothermometrie zeigt, dass die letzte Equilibrierung sehr wahrscheinlich bei P = 1.0 GPa (ca.), T = 750°C (ca.) erfolgte.Der zweite Typ von Granat-führenden Pyroxeniten ist ein (b) Orthopyroxenführender Granat-Spinell-Klinopyroxenit, der komplexe Texturen zeigt. Er besteht aus Zonen von grobkörnigem Klinopyroxen mit Einschlüssen von idiomorphem Spinell, der in Zonen übergeht, wo kleine gerundete Kristalle des gleichen Pyroxens und Spinells in relativ große Bereiche von extensiv kelyphitisiertem Granat (Py_64,8 Alm_25,6 Gr_9,6) eingeschlossen sind. Granat kommt auch als einschlußfreie Körner mit bis zu 4 mm Durchmesser vor. P-T Berechnungen geben wesentlich höhere Werte als für die Gesteine des Types (a). Die Entstehung der b-Typ-Granaten kann auch durch Subsolidus-Reaktion von Spinell und Pyroxen nach isobarischer Abkühlung von noch höheren Temperaturen beeinflußt sein; ein primärer magmatischer Ursprung könnte auch möglich sein, besonders für die körnigen Granate.P-T Abschätzungen für beide Pyroxenit-Typen sind gut einer Geotherme für 100 mW/m² Wärmefluß an der Oberfläche zuzuordnen. Ein solcher, relativ intensiver Wärmefluß könnte auf das Vorkommen von großen heißen Magmenkörpern hinweisen, die den lithosphärischen Mantel unter dem Iblei-Plateau und die untere Kruste in verschiedenen Niveaus intrudierten.

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With 4 Figures     

Petrologische Untersuchungen der mineralfaziellen Zustandsbedingungen im SW-Teil der Münchberger Gneismasse

Ohne ZusammenfassungMit 37 TextabbildungenVorliegende Arbeit wurde im Jahre 1955 als Dissertation beim Mineralogisch-Geologischen Institut der Universität Würzburg eingereicht.     

P-T history of a mantle diapir: the Horoman peridotite complex,Hokkaido, northern Japan

The Horoman peridotite complex, Hokkaido, Japan is divided into Lower and Upper zones on the basis of contrasting geological features. The complex recorded a consecutive decompression history in chemical zoning of pyroxenes and plagioclase in plagioclase lherzolite, which is interpreted to have been derived from garnet lherzolite by subsolidus decompression reactions. In the Lower Zone, and earlier decompression history is clearly preserved in large pyroxene porphyroclasts, which show marked M-shaped Al zoning characterized by low Al concentration at the core (Al=0.12/6 oxygens), gradual increase toward the marginal region, and rapid decrease toward the rim. The Ca content in the core is nearly constant (Ca=0.03/6 oxygens) with slight increase toward the margin followed by abrupt decrease toward the rim. The Al and Ca contents in the core of orthopyroxene in plagioclase lherzolite from the Upper Zone (Al=0.22, Ca=0.055/6 oxygens) are much higher than those for the Lower Zone, and the Al content typically decreases monotonously from the core to the rim with several exceptions that show poorly developed M-shaped zoning profiles. The earliest P-T conditions, inferable from the core compositions of pyroxenes are 900–950°C and 20 kbar for the Lower Zone and 1100–1150°C and 20 kbar for the Upper Zone. The increase of Al from the core to the margin is inferred to have resulted from nearly adiabatic decompression from these conditions into spinel peridotite facies. The complex experienced further decompression from the spinel stability field into the plagioclase stability field, which is inferred from plagioclase zoning in fine-grained aggregates composed mostly of plagioclase, chromite spinel, and olivine with minor pyroxenes. The Na-Ca ratio of each plagioclase grain decreases from the core to the rim, suggesting continuous decompression reaction producing olivine and plagioclase from pyroxenes and spinel. The sharp increase in Ca content toward the rim indicates that fairly rapid cooling associated with decompression is necessary to form and preserve the marked zoning. The sharp decrease in Al and Ca contents toward the rim of orthopyroxene was also formed during this final ascent of the complex. The systematic changes of the mineralogic and petrographic features that are gradational between the Lower and Upper zones suggest that the Horoman complex retains a temperature variation from the upper mantle. The Upper Zone is interpreted to have followed a higher temperature decompression path than the Lower Zone and probably represents a relatively hotter portion of a mantle diapir ascending from a depth greater than 60 km in the upper mantle.     

Les pyroxénolites à amphibole et les amphibololites associées aux lherzolites du gisement de Lherz (Ariège,France): un exemple du rôle de l'eau au cours de la cristallisation fractionnée des liquides issus de la fusion partielle de lherzolites

Amphibole pyroxenites with or without garnet and amphibolites (hydrous facies) which occur in the Lherz outcrop form monofacies or composite dykes cutting the primary schistosity of the spinel lherzolite. They coexist with monofacies or composite dykes of amphibole — free pyroxenites, with or without garnet (anhydrous facies), which are folded with the peridotite. The range of compositions, from olivine tholeiite (anhydrous facies only) to olivine basanites and nephelinites (hydrous facies) signifies a peculiar differenciation which could result from 1) fractionations closely controled by variation of the PH₂O/Pt in liquids derived from partial melting of a peridotite originally containing a small amount of water. 2) tectonic features of the emplacement of the ultrabasic body up to the lower levels of the crust, during which residual liquids, increasingly undersatured and enriched in alkalies and titanium, have been segregated. The result of such a process is the formation of rocks (amphibolites) having a chemical composition close to that of some olivine melilitic nephelinites flows.     

Petrological constraints on the cooling history of high-temperature garnet peridotite massifs in lower Austria

High-temperature peridotite massifs occur as lensoid bodies with high-pressure granulites in the southern Bohemian massif. In lower Austria the peridotites comprise garnet lherzolites lacking primary spinel, rare garnet and garnet-spinel harzburgites, and harzburgites containing Cr-rich primary spinel instead of garnet. These phase assemblages suggest initial high-pressure equilibration and are consistent with results from garnet-orthopyroxene geobarometry indicating equilibration at around 3–3.5 GPa. Maximum temperature estimates obtained on core compositions of coexisting minerals from the peridotites are not higher than ca. 1100 °C. In contrast, pyroxene megacryst compositions, garnet exsolution textures in the garnet pyroxenites, and results from geothermometry indicate much higher original equilibration temperatures in most of the pyroxenites (up to 1400 °C). High temperatures, modal zoning, the occasional presence of Mg-rich garnetites and chemical evidence suggest that the pyroxenites are cumulates which crystallized from low-degree melts derived from the sub-lithospheric mantle. Isothermal interpolation of the high temperatures to an upper mantle adiabat suggests that the melts were derived from a minimum depth of 180–200 km. The formation of small garnet II grains and garnet exsolution lamellae in the pyroxenites and pyroxene megacrysts may reflect isobaric cooling of the cumulates from temperatures above 1400 °C to ca. 1100–1200 °C (at 3–3.5 GPa) to approach the ambient lithospheric isotherm. This model differs from other models in which the formation of garnet II was explained by an increase in pressure during cooling in a subduction zone. Isobaric cooling was followed by near-isothermal decompression from 3–3.5 GPa to 1.5–2 GPa at 1000–1200 °C, as indicated by the increase of Al in pyroxenes near garnet. Further cooling in the spinel lherzolite stability field is indicated by spinel exsolution lamellae in pyroxenes from lherzolites. The formation of symplectites and kelyphites indicate sub-millimetre scale re-equilibration during exhumation in the course of the Carboniferous collision in the Bohemian massif. The peridotite massifs represent fragments of normal (non-cratonic) lithospheric mantle from a Paleozoic convergent plate margin. Received: 22 July 1996 / Accepted 28 February 1997     

Untersuchungen mit der Elektronenstrahlmikrosonde an natürlichen Skutteruditen

Quantitative electronprobe microanalyses of natural skutterudites from various localities have shown that the formula (Co, Fe, Ni), (As, S)₃ is valid for this mineral.The area of solid solution in the ternary diagram of the natural Co-Fe-Ni-skutterudites is nearly congruent with the area determined for synthetic skutterudites by Roseboom (1962). However, the range of solid solution may be enlarged in the diagram to the Ni-corner.Furthermore, the metal/arsenic ratio was found to conform to 13.00. Arsenic can be replaced by sulfur up to 4.5 weight-%. In addition, published analysis of skutterudites are discussed.

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Teil einer von der Fakultät für Bergbau und Hüttenwesen der TH Aachen angenommenen Dissertationsschrift.

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Danksagung. Der Verf. möchte Frau Prof. D. Schachner herzlich danken für die Förderung dieser Arbeit, die im Rahmen einer Dissertation entstand, ferner für die Erlaubnis, Sammlungsmaterial des Institutes zu benutzen. Herrn Priv.-Doz. Dr. G. Springer gilt mein Dank für die Einführung in die Mikrosondentechnik. Herrn Priv.-Doz. Dr. D. D. Klemm am Institut für allgemeine und angewandte Geologie und Mineralogie der Universität München bin ich für die freundliche Überlassung einiger Anschliffe dankbar. Der Deutschen Forschungsgemeinschaft bin ich zu Dank verpflichtet für die Erlaubnis, die von ihr zur Verfügung gestellte Elektronenstrahl-Mikrosonde benutzen zu dürfen.     

Partial melting of secondary pyroxenite at 1 and 1.5 GPa,and its role in upwelling heterogeneous mantle

We performed partial melting experiments at 1 and 1.5 GPa, and 1180–1400 °C, to investigate the melting under mantle conditions of an olivine-websterite (GV10), which represents a natural proxy of secondary (or stage 2) pyroxenite. Its subsolidus mineralogy consists of clinopyroxene, orthopyroxene, olivine and spinel (+garnet at 1.5 GPa). Solidus temperature is located between 1180 and 1200 °C at 1 GPa, and between 1230 and 1250 °C at 1.5 GPa. Orthopyroxene (±garnet), spinel and clinopyroxene are progressively consumed by melting reactions to produce olivine and melt. High coefficient of orthopyroxene in the melting reaction results in relatively high SiO₂ content of low melt fractions. After orthopyroxene exhaustion, melt composition is controlled by the composition of coexisting clinopyroxene. At increasing melt fraction, CaO content of melt increases, whereas Na₂O, Al₂O₃ and TiO₂ behave as incompatible elements. Low Na₂O contents reflect high partition coefficient of Na between clinopyroxene and melt (\(D_{{{\text{Na}}_{ 2} {\text{O}}}}^{{{\text{cpx}}/{\text{liquid}}}}\)). Melting of GV10 produces Quartz- to Hyperstene-normative basaltic melts that differ from peridotitic melts only in terms of lower Na₂O and higher CaO contents. We model the partial melting of mantle sources made of different mixing of secondary pyroxenite and fertile lherzolite in the context of adiabatic oceanic mantle upwelling. At low potential temperatures (T _P < 1310 °C), low-degree melt fractions from secondary pyroxenite react with surrounding peridotite producing orthopyroxene-rich reaction zones (or refertilized peridotite) and refractory clinopyroxene-rich residues. At higher T _P (1310–1430 °C), simultaneous melting of pyroxenite and peridotite produces mixed melts with major element compositions matching those of primitive MORBs. This reinforces the notion that secondary pyroxenite may be potential hidden components in MORB mantle source.