Formation of the superdeep South Caspian basin: subsidence driven by phase change in continental crust

The large hydrocarbon basin of South Caspian is filled with sediments reaching a thickness of 20–25 km. The sediments overlie a 10–18 km thick high-velocity basement which is often interpreted as oceanic crust. This interpretation is, however, inconsistent with rapid major subsidence in Pliocene-Pleistocene time and deposition of 10 km of sediments because the subsidence of crust produced in spreading ridges normally occurs at decreasing rates. Furthermore, filling a basin upon a 10–18 km thick oceanic crust would require twice less sediments. Subsidence as in the South Caspian, of ≥20 km, can be provided by phase change of gabbro to dense eclogite in a 25–30 km thick lower crust. Eclogites which are denser than the mantle and have nearly mantle P velocities but a chemistry of continental crust may occur beneath the Moho in the South Caspian where consolidated crust totals a thickness of 40–50 km. The high subsidence rates in the Pliocene-Pleistocene may be attributed to the effect of active fluids infiltrated from the asthenosphere to catalyze the gabbro-eclogite transition. Subsidence of this kind is typical of large petroleum provinces. According to some interpretations, historic seismicity with 30–70 km focal depths in a 100 km wide zone (beneath the Apsheron-Balkhan sill and north of it) has been associated with the initiation of subduction under the Middle Caspian. The consolidated lithosphere of deep continental sedimentary basins being denser than the asthenosphere, can, in principle, subduct into the latter, while the overlying sediments can be delaminated and folded. Yet, subduction in the South Caspian basin is incompatible with the only 5–10 km shortening of sediments in the Apsheron-Balkhan sill and south of it and with the patterns of earthquake foci that show no alignment like in a Benioff zone and have mostly extension mechanisms.     

Alpine and Pacific styles of Phanerozoic mountain building: subduction-zone petrogenesis of continental crust

A broad continuum exists between two distinct end-member types of mountain building. Alpine-type orogenic belts develop during subduction of an ocean basin between two continental blocks, resulting in collision. They are characterized by an imbricate sequence of oceanward verging nappes; some Alpine belts exhibit superimposed late-stage backthrusting. Sediments are chiefly platform carbonates and siliciclastics, in some cases associated with minor amounts of bimodal volcanics; pre-existing granitic gneisses and related continental rocks constitute an autochthonous–parautochthonous basement. Metamorphism of deeply subducted portions of the orogen ranges from relatively high-pressure (HP) to ultrahigh-pressure (UHP). Calcalkaline volcanic–plutonic rocks are rare, and have peraluminous, S-type bulk compositions. In contrast, Pacific-type orogens develop within and landward from long-sustained oceanic subduction zones. They consist of an outboard oceanic trench–accretionary prism, and an inboard continental margin–island arc. The oceanic assemblage consists of first-cycle, in-part mélanged volcaniclastics, and minor but widespread cherts ± deep-water carbonates, intimately mixed with disaggregated ophiolites. The section recrystallized under HP conditions. Recumbent fold vergence is oceanward. A massive, slightly older to coeval calcalkaline arc is sited landward from the trench complex on the stable, non-subducted plate. It consists of abundant, dominantly intermediate, metaluminous, I-type volcanics resting on old crust; both assemblages are thrown into open folds, intruded by comagmatic I-type granitoids, and metamorphosed locally to regionally under high-T, low-P conditions. In the subduction channel of collisional and outboard Circumpacific terranes, combined extension above and subduction below allows buoyancy-driven ascent of ductile, thin-aspect ratio slices of HP–UHP complexes to midcrustal levels, where most closely approached neutral buoyancy; exposure of rising sheets caused by erosion and gravitational collapse results in moderate amounts of sedimentary debris because exhumed sialic slivers are of modest volume. At massive sialic buildups associated with convergent plate cuSPS (syntaxes), tectonic aneurysms may help transport HP–UHP complexes from mid- to upper-crustal levels. The closure of relatively small ocean basins that typify many intracratonic suture zones provides only limited production of intermediate and silicic melts, so volcanic–plutonic belts are poorly developed in Alpine orogens compared with Circumpacific convergent plate junctions. Generation of a calcalkaline arc mainly depends on volatile evolution at the depth of magma generation. Phase equilibrium studies show that, under typical subduction-zone P–T trajectories, clinoamphibole ± Ca–Al hydrous silicates constitute the major hydroxyl-bearing phases in deep-seated metamorphic rocks of MORB composition; other hydrous minerals are of minor abundance. Ca and Na clinoamphiboles dehydrate at pressures of above approximately 2 GPa, but low-temperature devolatilization may be delayed by pressure overstepping; thus metabasaltic blueschists and amphibolites expel H₂O at melt-generation depths, and commonly achieve stable eclogitic assemblages. Partly serpentinized mantle beneath the oceanic crust dehydrates at roughly comparable conditions. For reasonable subduction-zone geothermal gradients however, white micas ± biotites remain stable to pressures >3 GPa. Accordingly, attending descent to depths of >100 km, mica-rich quartzofeldspathic lithologies that constitute much of the continental crust fail to evolve substantial amounts of H₂O, and transform incompletely to stable eclogite-facies assemblages. Underflow of amphibolitized oceanic lithosphere thus generates most of the deep-seated volatile flux, and the consequent partial melting to produce the calcalkaline suite, along and above a subduction zone; where large volumes of micaceous intermediate and felsic crustal materials are carried down to great depths, volatile flux severely diminishes. Thus, continental collision in general does not produce a volcanic–plutonic arc whereas in contrast, the long-continued contemporaneous underflow of oceanic lithosphere does.     

An alternative model for the Damara Mobile Belt: Ocean crust subduction and continental convergence

The Pan-African Damara Mobile Belt has previously been described as ensialic, possibly resulting from a modified aulacogen.Three features of the Damara Mobile Belt are difficult to reconcile with ensialic models. Firstly, the complex asymmetrical structural pattern of linear zones, with up to 80% shortening across the belt. Secondly, the markedly asymmetric metamorphic pattern broadly follows the structural pattern forming two distinct, parallel metamorphic belts of relatively high (northern belt) and low (southern belt) geothermal gradients, respectively. Abundant granitic intrusions occur in the high-grade metamorphic belt. Thirdly, the evolution of the Damara igneous rocks; the early (Nosib) igneous rocks are alkali; mid-Damara (Matchless Member) amphibolites resemble oceanic-floor basalts. Depleted upper-mantle material representing oceanic lithosphere was tectonically emplaced into the Damara metasediments during early tectonism. An extensive calc-alkali suite (the Salem Suite) intruded the high-grade metamorphic belt during a long period spanning most of the Damara tectonism.A model invoking the formation of alkali rocks, followed by the development of oceanic crust, initiation of northwestward subduction and ocean closure terminating in continental collision is considered to explain the major features.     

Pseudotachylytes in the Balmuccia peridotite (Ivrea Zone) as markers of the exhumation of the southern Alpine continental crust

Two types of pseudotachylytes are observed in the Balmuccia peridotite of the Ivrea zone (Southern Alps, Italy). A-type pseudotachylytes correspond to previously studied occurrences and were formed under temperatures comprising between 550 and 900 °C and pressures comprising between 0.6 and 1.2 GPa. These conditions were met in the Ivrea crust between 350 and 270 Ma, suggesting that A-type pseudotachylytes were formed during Variscan tectonics or Permian transtensional tectonics. B-type pseudotachylytes post-date A-type pseudotachylytes. Textural characteristics of B-type veins suggest a formation in the upper continental crust, at depths of about 5–10 km or less. Petrological constraints indicate that the exhumation of the Ivrea crust at such shallow depths was achieved later than c.  70 Ma, thus providing a maximum age of 70 Ma for B-type veins. Pseudotachylytes appear as markers of the poly-orogenic evolution of the Alpine belt.     

Relation between alternations of uplift and subsidence revealed by Late Cenozoic fluvial sequences and physical properties of the continental crust

Reversals in vertical crustal motion, alternations between uplift and subsidence over time scales of hundreds of thousands of years or more, have been identified in Late Cenozoic fluvial sequences in many regions worldwide. They form a class of fluvial archive that is distinct from the extreme stability observed in Archaean cratons and the monotonic uplift or subsidence that is widely observed in other regions. Such alternations between uplift and subsidence are characteristic of regions of Early or Middle Proterozoic crust, where the initial crustal consolidation included the development of a thick ‘root’ of mafic material at the base of the crust; the present study focuses on localities with this crustal type in the USA and eastern Europe. It has previously been suggested on the basis of uplift modelling that this style of crustal behaviour occurs only in regions where the mobile lower‐crustal layer is relatively thin. This study supports this conclusion on the basis of independent geothermal calculations, which indicate that such alternations between uplift and subsidence occur where the mobile lower‐crustal layer is ≤～7 km thick. An understanding of this phenomenon, in relation to the understanding of vertical crustal motions induced by surface processes (and thus by climate change) in general, therefore requires analysis of the properties and dynamics of the mobile lower‐crustal layer; detailed analysis of fluvial sequences thus contributes unique information in this area.     

大陆边缘弧岩浆成因与大陆地壳形成

大陆地壳如何形成是国际学术界长期关注并正在持续攻关的一个重大基础科学问题。活动陆缘弧的岩浆成因和密度分选过程是理解大陆地壳形成机制和演化过程的关键。北美白垩纪Cordilleran大陆边缘弧的形成可能经历了与底侵幔源岩浆有关的下地壳部分熔融和岩浆混合,或幔源初始玄武质岩浆的两阶段成分分异过程,以花岗质成分为主的北美内华达地区垂向地壳成分剖面结构可能与榴辉岩相残留体或堆晶岩的拆沉作用密切相关。目前并不清楚亚洲大陆南部以约200 Ma和约90 Ma两个时间断面为代表的中生代冈底斯弧,为何出现大量角闪石岩并具有玄武安山质的平均成分。探究中生代冈底斯弧的岩浆成因、地壳垂向成分结构和地壳形成机制可能有助于或多或少地解决这一问题。     

Sm／Nd Evolution of Upper Mantle and Continental Crust：Constraints on Gowth Rates of the Continental Crust

A new approach to the investigation of the Sm/Nd evolution of the upper mantle directly from the data on lherzolite xenoliths is described in this paper.It is demonstrated that the model age TCHUR of an unmetasomatic iherzolite zenolith ca represent the mean depletion age of its mantle source, thus presenting a correlation trend between f^Sm/Nd and the mean depletion age of the upper mantle from the data on xenoliths.This correlation trend can also be derived from the data on river suspended loads as well as from granitoids.Based on the correlation trend mentioned above and mean depletion ages of the upper mantle at various geological times, an evolution curve for the mean f^Sm/Nd value of the upper mantle through geological time has been established.It is suggested that the upwilling of lower mantle material into the upper mantle and the recycling of continental crust material during the Archean were more active ,thus maintaining fairly constantf^Sm/Nd and εNd values during this time period. Similarly ,an evolution curve for the mean f^Sm/Nd value of the continental crust through geological time has also been established from the data of continental crust material.In the light of both evolution curves for the upper mantle and continental crust ,a growth curve for the continental crust has been worked out ,suggesting that :(1)about 30%(in volume )of the present crust was present as the continental crust at 3.8 Ga ago ;(2)the growth rate was much lower during the Archean ;and (3)the Proterozoic is another major period of time during which the continental crust wsa built up .     

Chemical composition and fractionation of the continental crust

A new estimate of the bulk continental crust is reported consisting of 57 percent lower crust (60% felsic and 40% mafic granulites) and 43 percent upper crust. The proportions of crustal units are based on petrological observations (Bohlen &Mezger, 1989). The estimate of a bulk composition is intermediate between andesite and tonalite and is higher in Si, K, Rb, Sr, Zr, Nb, Ba, LREE, Pb, Th concentrations and lower in Mg, Ca, Sc, Mn, Fe than the crustal abundances reported byTaylor &McLennan (1985). Equal chemical composition between the upper crust and the felsic part of the lower crust is attained in balance computations if one restores a fraction of 12.5 percent S-type granite from the upper into the lower crust. An example of water-undersaturated partial melting and separation of a fraction of about 35 percent granitic magma at the conversion from amphibolite-into granulite-facies metasediments has been balanced bySchnetger (1988) in the Ivrea area (N. Italy). The worldwide observed discrepancy between a larger negative Eu anomaly in the upper crust compared with the half as large positive anomaly of the lower crust increasing from the early Precambrian to present has been explained by recycling of Ca-rich restite into the upper mantle. The composition of the Archean crust (example: Greenland) does not differ systematically from the post-Archean crust.

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Zusammenfassung Die chemische Zusammensetzung der gesamten kontinentalen Kruste, die zu 57% aus der Unterkruste (60% felsische und 40% mafische Granulite) und zu 43% aus Oberkruste besteht, wurde neu ermittelt. Die Proportionen der Krusteneinheiten beruhen auf petrologischen Beobachtungen (Bohlen &Mezger, 1989). Die geschätzte Zusammensetzung der Gesamtkruste liegt zwischen Andesit und Tonalit. Sie ist höher in den Gehalten an Si, K, Rb, Sr, Zr, Nb, Ba, LREE, Pb, Th und niedriger im Mg, Ca, Sc, Mn, Fe als die vonTaylor &McLennan (1985) mitgeteilten mittleren Krustenwerte. Die chemischen Unterschiede zwischen Ober- und Unterkruste werden ausgeglichen, wenn man die Substanz von 12,5% S-Typ-Granit von der Oberkruste abzieht und zur Unterkruste hinzufügt. Als typisches Beispiel der Abtrennung granitischer Partialschmelzen im wasseruntersättigten System wird das der variskischen Metamorphose von Metasedimenten in der Ivreazone (Nord-Italien) angesehen.Schnetger (1988) konnte hier mit einer chemischen Bilanz zeigen, daß die Umwandlung von amphibolitfaziellen zu granulitfaziellen Gesteinen mit dem Verlust von etwa 35% granitischer Schmelze verbunden war. Die negative Eu-Anomalie der Oberkruste ist weltweit doppelt so groß wie die positive Anomalie der Unterkruste. Diese in der Zeit vom Archaikum bis heute vergrößerte Diskrepanz läßt sich nur mit dem Verlust von Ca-reichen Restiten aus der Kruste an den Mantel erklären. Die chemische Zusammensetzung der kontinentalen Kruste hat sich sonst seit dem Archaikum nicht systematisch geändert, wie am Beispiel Grönlands gezeigt wird.

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Résumé Cette note propose une nouvelle estimation de la composition chimique d'ensemble de la croûte continentale, constituée pour 57% de croûte inférieure (60% de granulites felsiques et 40% de granulites mafiques) et pour 43% de croûte supérieure. Les proportions de ces unités crustales sont basées sur les observations pétrologiques (Bohlen etMezger 1989). La composition d'ensemble proposée est intermédiaire entre celles d'une andésite et d'une tonalite; par rapport aux abondances crustales données parTaylor etMcLennan (1985), les teneurs sont plus élevées en Si, K, Rb, Sr, Zr, Nb, Ba, LEE, Pb, Th et moins élevées en Mg, Ca, Sc, Mn, Fe. Si on tranfère de la croûte supérieure à la croûte inférieure la matière correspondant à 12,5% de granite de type S, la différence de composition entre ces deux croûtes disparaît. Un exemple typique de fusion partielle granitique en système sous-saturé en eau est fourni par le métamorphisme varisque de métasédiments dans la zone d'Ivrée (Italie du Nord). D'après ce bilan chimique établi parSchnetger (1988), le passage des roches du faciès des amphibolites à celui des granulites s'accompagne de la production d'environ 35% de magma granitique. L'anomalie négative en Eu de la croûte supérieure est partout le double de l'anomalie positive de la coûte inférieure. Cette différence, qui s'est accrue depuis l'Archéen jusqu'aujourd'hui, s'explique par le passage de restites riches en Ca dans le manteau supérieur. La composition d'ensemble de la croûte continentale ne s'est toutefois pas modifiée depuis l'Archéen, comme le montre l'exemple du Groenland.

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, 57% (60% 40% ), -43%. , (Bohlen & Mezger, 1989). . Taylor & McLennan (1985) Si, K, Rb, Sr, Zr, Nb, Ba, LREE, Pb, Th Mg, Ca, Sc, Mn, Fe. , 12,5% S, , . — , , . Schnetger (1988) , 35%. , . , , , , , . , .

     

Element Abundances of China‘s Continental Crust and Its Sedimentary Layer and Upper Continental Crust

China’s continental crust (CCC) has an average thickness of 47km, with the upper continental crust (CUCC) being 31 km and the sedimentary layer(CSL) 5 km in thickness. The CCC, CUCC and CSL measure 12.437 × 10⁻¹⁷, 8.005 × 10⁻¹⁷ and 1.146 × 10¹⁷ metric tons in mass, respectively. The mass ratio of the upper continental crust to the lower one is 1.8:1. The element abundances were calculated for the CCC, CUCC and CSL respectively in terms of the chemical compositions of 2246 samples of various types and some complementary trace element data. The total abundance of 13 major elements accounts for 99.6% of the CCC mass while the other minor elements only account for 0.4%. REE characteristics, the abundance ratios of element pairs and the amounts of ore-forming elements are also discussed in the present paper.     

Nd-Sr isotopic characteristics of the Lugano volcanic rocks and constraints on the continental crust formation in the South Alpine domain (N-Italy-Switzerland)

The Rb-Sr and Sm-Nd isotope data emphasize the importance of mantle crust interaction, wall-rock assimilation and fractional crystallization for the generation of the Lugano volcanic rocks. It is suggested that the parental magma generation occurs in hot upwelling asthenosphere in the wedge above a subducting slab. In the lower crust the rising mantle derived melts became strongly modified by crust assimilation and formed andesitic melts. These andesitic melts, rising from this lower crustal region, became additionally modified by fractional crystallization and further assimilation of lower and upper crustal components to form the dacites, rhyolites, granophyres and Mt. OrfanoBaveno granites. The best fit lines to the Rb-Sr and Sm-Nd isotope whole rock data points correspond to ages of 346+/– 2 m.y. and 341+/–40 m.y., respectively. These lines are considered to be pseudo-isochrons and the result of simultaneously running fractional crystallization and wallrock assimilation. The best age estimate of the investigated volcanites is given by a Rb-Sr mineral isochron of 262+/–I m.y.. It dates a single volcanic event of the Permo-Carboniferous magmatism. Since it is suggested, that the calc-alkaline rock sequence has been generated in an Andean type subduction environment, synchronous with the final phase of convergence of Gondwana and Laurasia, the Rb-Sr mineral isochron indicates, that parts of the Proto-Tethys closed later than 262 m.y. ago. The crustal source material of the Irvea and Strona-Ceneri paragneisses, Lugano volcanites and Mt. Orfano-Baveno intrusive rocks may not necessarily be derived from a shield area in Northern Europe or Africa but may come from a Proterozoic European continental lithosphere.     

Field,petrophysical and carbon isotope studies on the Lapland Granulite Belt: implications for deep continental crust

The Palaeoproterozoic Lapland Granulite Belt is a seismically reflective and electrically conductive sequence of deep crustal (6–9 kbar) rocks in the northern Fennoscandian Shield. It is composed of garnet-sillimanite gneisses (khondalites) and pyroxene granulites (enderbites) which in certain thrust sheets form about 500 m thick interlayers. The structure was formed by the intrusion of intermediate to basic magmas into turbiditic sedimentary rocks under granulite facies metamorphism accompanied by shearing of the deep crust about 1.93–1.90 Gyr ago (Gal. Granulites were upthrust 1.90–1.87 Ga and the belt was divided by crustal scale duplexing into four structural units whose layered structure was preserved. The thrust structures are recognized by the repetition of lithological ensembles and by discordant structural patterns well distinguishable in airborne magnetic and electromagnetic data. Thrusting gave rise to clockwise pressure-temperature evolution of the belt. However, some basic rocks possibly record an isobaric cooling path. The low bulk resistivity of the belt (200–1000 Ωm) is caused by interconnected graphite and subordinate sulphides in shear zones. On the basis of carbon isotope ratios this graphite is derived mostly from sedimentary organic carbon. The seismic reflectivity of the belt may be caused by velocity and density differences between pyroxene granulites and khondalites, as well as by shear zones.     

Mechanisms of continental crust formation in the Central Asian Foldbelt

Geological and isotopic study of rocks occurring in the Early and Late Baikalian, Caledonian, Hercynian, and Indosinian fold regions of Central Asia is carried out. The juvenile crust formation occurred in these fold regions have determined the systematic differences in isotopic compositions of the crust. In the course of the subsequent (postaccretion) evolution, the crust of these domains underwent multiple reworking. These processes were accompanied by variations in the Nd isotopic compositions of the crust, which, in turn, are recorded in the isotopic compositions of granites and felsic volcanics as products of crust melting. Three types of crust differing in Nd isotopic composition and structure and, as a consequence, in formation mechanisms, are distinguished. The isotopically homogeneous crust is a source of igneous rocks with constant model Nd isotopic age (T_Nd(DM2st)) irrespective of the age of the crustal igneous rocks. These are the isotopic provinces, the crust of which remained isolated from addition of alien materials during postaccretion evolution. The axial zone of the Hercynides in the Central Asian Foldbelt is an example. The isotopically heterogeneous layered crust consists of fragments differing in isotopic composition. The products of its melting are characterized by widely scattered ɛ_Nd(T) and (T_Nd(DM2st). The appearance of alien sources of melt is considered in terms of underplating. This mechanism develops either due to subduction of the juvenile oceanic lithosphere beneath the mature continental lithosphere at convergent boundaries or as a result of plume-lithosphere interaction. The first mechanism operated during the formation of granitoids pertaining to the Tuva-Mongolia microcontinent. The second mechanism was responsible for the formation of batholiths in the zonal Hangay, Barguzin, and Mongolia-Transbaikalia magmatic fields. The isotopically heterogeneous mixed crust is composed of fragments differing in isotopic composition, which are tectonically mixed, resulting in the formation of an isotopically uniform reservoir in the domain of magma generation. As a result, the products of melting acquire isotopic parameters substantially distinct from the juvenile rocks of the corresponding structural zone. The formation of such a crust is related to the tectonic delamination, which provides for juxtaposition and a high degree of tectonic mingling of heterogeneous fragments at deep levels. The Caledonides of the Central Asian Foldbelt are characterized by such a mechanism of crust formation.     

Vertical variation of heat flow density in the continental crust

Terrestrial heat flow density is a key parameter in understanding the past, present and future development of our planet. Most phenomena studied in deep crustal geophysics are temperature dependent and therefore reliable assesments of deep temperatures are necessary. Most heat flow measurements have been made in drill holes which are shallow (< 1 km) in comparison to the thicknesses of the crust and lithosphere. The recent findings in deep drilling projects (e.g. the Kola deep hole in Russia and the KTB hole in Germany) have yielded results which suggest that there is a distinct contrast between heat flow densities measured in the uppermost 1 km and values measured at deeper levels. The factors contributing to the vertical variation in the uppermost few kilometres are discussed with special emphasis on palaeoclimatic ground surface temperature changes and groundwater circulation in the bedrock.     

Creation and destruction of lower continental crust

Bulk continental crustal composition results from the net mass exchange between crust and mantle. Crustal addition is mainly by the rise of mantle-derived melts into and through the crust at convergent plate margins and (at a lower rate) within plate interiors. Crustal subtraction occurs by subduction of uppermost crust (sediment, continent-derived elements in hydrothermally altered oceanic crust), by subcrustal erosion at convergent margins and by delamination of lowermost crust following densifying gabbro-eclogite phase transformations that result in a crust-mantle density inversion. As the phase transformations only occur at high pressure, tectonic overthickening of the crust (to > 50 km) is required. The lowermost crust at continent-ocean and continent-continent convergent plate margins is more likely to experience these transient overthickening events (compressional orogenies) than is intraplate crust. Correspondingly, the preservation probability of mafic lower crust is greater for intraplate than for plate margin localities. Delamination of mafic lower crust is the main process for removing basic composition rocks from the crust, thereby creating »andesitic« crustal composition. Evidence for lower crustal delamination comes from »geochemically balanced« cross section of compressional belts, and from the high La/Yb ratios, lack of Eu anomalies, and high Sr contents in deep crustallyderived magmas from the base of tectonically over-thickened crust. These crustal magmas are often accompanied by mantle-derived basalts associated with crustal uplift and extension, both related to the coincident delamination of underlying mantle lithosphere.

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Zusammenfassung Die Gesamtzusammenfassung der Kontinentalen Kruste resultiert aus dem Massenaustausch zwischen Kruste und Mantel. Krustenzuwachs erfolgt hauptsächlich beim Aufstieg in und durch die Kruste von aus dem Mantel abstammenden Basalt an konvergierenden Plattengrenzen und zum geringeren Teil Plattenintern. Der Krustenabbau wird erreicht per Subduktion der obersten Kruste, durch subkrustale Erosion an konvergierenden Plattengrenzen (Sedimente, Elemente kontinentaler Herkunft von hydrothermal veränderter ozeanischer Kruste). Dies wird hervorgerufen von der Schichtspaltung der untersten Kruste nach der Verdichtung durch die Gabbro-Eklogit-Phasentransformation, welche in der Krusten-Mantel-Dichte-Inversion resultiert. Da die Phasentransformation nur unter hohen Drücken stattfindet, werden tektonische Mächtigkeitszunahmen der Kruste (> 50 km) benötigt. Die unterste Kruste in Bereichen von konvergierenden Kontinent-Ozean und Kontinent-Kontinent Plattengrenzen unterliegt einer größeren Wahrscheinlichkeit vorübergehende Mächtigkeitszunahmen zu erfahren als platteninterne Kruste. Dementsprechend ist die Erhaltungswahrscheinlichkeit von mafischer unterer Kruste für platteninterne Bereiche größer als für Plattengrenzen. Schichtspaltung von mafischer unterer Kruste ist der Hauptprozeß basisch zusammengesetzte Gesteine aus der Kruste zu entfernen, hierbei wird die Kruste in Richtung »andesitische« Zusammensetzung verändert. Hinweise für Schichtspaltung der unteren Kruste stammen von »geochemisch bilanzierten« Profilen aus druckhaft deformierten Zonen. Weiterhin sprechen dafür hohe La/Yb-Werte, das Fehlen von Eu-Anomalien und hohe Sr-Gehalte, wie sie an der Basis tektonisch verdickter Kruste in Magmen, die aus der tiefen Kruste stammen, gefunden werden. Diese krustalen Magmen werden häufig von Mantelbasalten begleitet, die zu Krustenhebung und Dehnung in Verbindung stehen; beides im Zusammenhang stehend zu der gleichzeitig stattfindenden Schichtspaltung der unterlagernden Mantellithosphäre.

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Résumé La composition d'ensemble de la croûte continentale résulte des échanges entre la croûte et le manteau. L'apport dans la croûte provient en ordre principal de la montée de basalte d'origine mantélique qui s'opère aux bordures des plaques convergentes et, dans une moindre mesure, à l'intérieur des plaques. Le départ hors de la croûte se produit par la subduction de la croûte supérieure (sédiments, éléments dérivés des continents dans la croûte océanique affectée d'altération hydrothermale), par érosion subcrustale le long des marges convergentes et par délamination à la base de la croûte, les transformations de phase gabbro-éclogitiques entraînant une augmentation de densité et une inversion de densité entre croûte et manteau. Comme ces transformations de phases ne se produisent qu'à haute pression, elles impliquent un épaississement tectonique de la croûte (jusqu'à plus de 50 Km). Le domaine probable de tels épaississement est la partie inférieure de la croûte en bordure des plaques convergentes continentocéan ou continent-continent (orogènes de compression), plutôt que la croûte intra-plaque. Inversement, la probabilité de conversion d'une croûte inférieure mafique est plus élevée au milieu des plaques que sur leurs bordures. La délamination de la croûte inférieure est le processus courant d'appauvrissement de la croûte en roches mafiques, avec création d'une composition crustale »andésitique«. Les arguments en faveur de cette delamination sub-crustale sont tirés de profils »géochimiquement équilibrés« dans les ceintures en compression, ainsi que des rapports La/Yb élevés, de l'absence d'anomalie de l'Eu et des hautes teneurs en Sr dans les magmas dérivés de la partie profonde des croûtes tectoniquement épaissies. Ces magmas crustaux sont souvent accompagnés de basaltes d'origine mantélique associés à un soulèvement et à une extension crustale, ces deux processus étant liés à la délamination concommittante de la lithosphère mantélique sousjacente.

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Heterogeneous magnesium isotopic composition of the upper continental crust

High-precision Mg isotopic data are reported for ∼100 well-characterized samples (granites, loess, shales and upper crustal composites) that were previously used to estimate the upper continental crust composition. Magnesium isotopic compositions display limited variation in eight I-type granites from southeastern Australia (δ²⁶Mg = −0.25 to −0.15) and in 15 granitoid composites from eastern China (δ²⁶Mg = −0.35 to −0.16) and do not correlate with SiO₂ contents, indicating the absence of significant Mg isotope fractionation during differentiation of granitic magma. Similarly, the two S-type granites, which represent the two end-members of the S-type granite spectrum from southeastern Australia, have Mg isotopic composition (δ²⁶Mg = −0.23 and −0.14) within the range of their potential source rocks (δ²⁶Mg = −0.20 and +0.15) and I-type granites, suggesting that Mg isotope fractionation during crustal anatexis is also insignificant. By contrast, δ²⁶Mg varies significantly in 19 A-type granites from northeastern China (−0.28 to +0.34) and may reflect source heterogeneity.Compared to I-type and S-type granites, sedimentary rocks have highly heterogeneous and, in most cases, heavier Mg isotopic compositions, with δ²⁶Mg ranging from −0.32 to +0.05 in nine loess from New Zealand and the USA, from −0.27 to +0.49 in 20 post-Archean Australian shales (PAAS), and from −0.52 to +0.92 in 20 sedimentary composites from eastern China. With increasing chemical weathering, as measured by the chemical index of alternation (CIA), δ²⁶Mg values show a larger dispersion in shales than loess. Furthermore, δ²⁶Mg correlates negatively with δ⁷Li in loess. These characteristics suggest that chemical weathering significantly fractionates Mg isotopes and plays an important role in producing the highly variable Mg isotopic composition of sedimentary rocks.Based on the estimated proportions of major rock units within the upper continental crust and their average MgO contents, a weighted average δ²⁶Mg value of −0.22 is derived for the average upper continental crust. Our studies indicate that Mg isotopic composition of the upper crust is, on average, mantle-like but highly heterogeneous, with δ²⁶Mg ranging from −0.52 to +0.92. Such large isotopic variation mainly results from chemical weathering, during which light Mg isotopes are lost to the hydrosphere, leaving weathered products (e.g., sedimentary rocks) with heavy Mg isotopes.     

Rates of generation and growth of the continental crust

Models for when and how the continental crust was formed are constrained by estimates in the rates o crustal growth. The record of events preserved in the continental crust is heterogeneous in time with distinctive peaks and troughs of ages for igneous crystallisation, metamorphism, continental margin and mineralisation. For the most part these are global signatures, and the peaks of ages tend to b associated with periods of increased reworking of pre-existing crust, reflected in the Hf isotope ratios o zircons and their elevated oxygen isotope ratios. Increased crustal reworking is attributed to periods o crustal thickening associated with compressional tectonics and the development of supercontinents Magma types similar to those from recent within-plate and subduction related settings appear to hav been generated in different areas at broadly similar times before ~3.0 Ga. It can be difficult to put th results of such detailed case studies into a more global context, but one approach is to consider when plate tectonics became the dominant mechanism involved in the generation of juvenile continental crust The development of crustal growth models for the continental crust are discussed, and a number o models based on different data sets indicate that 65%-70% of the present volume of the continental crus was generated by 3 Ga. Such estimates may represent minimum values, but since ~3 Ga there has been reduction in the rates of growth of the continental crust. This reduction is linked to an increase in th rates at which continental crust is recycled back into the mantle, and not to a reduction in the rates a which continental crust was generated. Plate tectonics results in both the generation of new crust and it destruction along destructive plate margins. Thus, the reduction in the rate of continental crustal growth at ~3 Ga is taken to reflect the period in which plate tectonics became the dominant mechanism b which new continental crust was generated.     

Exhumation of subducted continental crust along the arc region

The Kutná Hora crystalline complex (KHCC) in the Bohemian Massif is a HP/HT complex adjacent to the magmatic arc. It is dominated by migmatite, orthogneiss and granulite with bodies of eclogite and peridotite. The KHCC migmatite consists of K-feldspar, plagioclase, quartz, phengite, biotite, garnet and kyanite. Melting conditions were estimated at 780 °C and >16 kbar and inferred melt volume varies between 1 and 4 vol%. Peak temperature is 865 °C at 18–19 kbar followed by decompression in the presence of melt to 12–13 kbar and 770–800 °C. U-Pb monazite geochronology reveals a spread of ages between 550 Ma and 330 Ma. REE patterns show low Yb/Gd for 550–500 Ma, high Yb/Gd for ages at ~480 Ma, and decreasing Yb/Gd towards ~340 Ma. First monazite in equilibrium with garnet constrains the HP metamorphism to ~350 Ma, which is followed by recrystallization of monazite down to 325 Ma. U-Pb zircon geochronology displays an age range from ~670 Ma to ~430 Ma. The broad age range records a span of protolith crystallization and/or old metamorphism. The presence of HP ky + mu migmatite, their P–T path, protolith zircon and monazite metamorphic ages and whole-rock geochemistry are similar to HP migmatites in the Eger crystalline complex (ECC) in the Saxothuringian domain further in the west. We propose the following geodynamic scenario for subduction-relamination-exhumation mechanism: (i) subduction of the Saxothuringian continental lithosphere at 360 Ma related to early stage of trans-lithospheric diapirism triggered by arc-related magma weakening; (ii) large-scale emplacement of relaminant into the upper plate lithosphere at 350–340 Ma; and (iii) return flow of the relaminant along the subduction interface (the ECC) and emplacement of relaminant in the upper–middle crust in the rear part of the arc system (the KHCC) at 340–330 Ma.     

Genesis of high Mg# andesites and the continental crust

The continental crust has an andesitic composition with high Mg/(Mg+Fe) and Ni contents which may be too high to have formed by differentiation of basaltic magmas. Instead, mantle-derived, high Mg# andesites (HMA) may form a substantial component of the crust. HMA may be produced by partial melting of previously depleted, subsequently metasomatised mantle peridotite. However, they are more likely produced by reaction between ascending melts and mantle peridotite. HMA are less common than basalts among lavas in modern island arcs, but may have been more common in the past, may be produced in specific environments (such as ridge subduction), may be more common among plutonic rocks in the lower and middle crust than among lavas at the surface, and may be selectively preserved during later erosion and subduction processes.