Constraints imposed by experimental petrology on possible and impossible magma sources and products

Experimental petrology can be used in forward and inverse approaches. The forward approach defines the compositions of liquids generated by partial melting of possible source rocks at various depths. The inverse approach determines conditions for multiple-mineral saturation at the liquidus of primitive magmas, correlates them with residual minerals of possible source rocks, and thus provides estimates of depths and temperatures required for their derivation. Review of a selection of forward and inverse results is followed by evaluation of petrological and geophysical processes in layered mantle and in subduction zones. Physical constraints imposed by solidus curves and geotherms present problems for models that derive basalts from deep mantle reservoirs, separated from overlying convecting layers. Magmas from mantle are limited to compositions less siliceous than basaltic andesite, with rare exceptions. Granite liquids cannot be generated from normal peridotite, nor from oceanic crust at mantle pressures in subduction zones. In continental crust, hydrous granite liquid is generated at depths of less than 30 km. Basaltic andesite and picritic basalt are parental magmas for the calc-alkaline series. Andesite is not primary from subcontinental depths, and can be generated as liquid in continental crust only if temperatures exceed about 1100°C. Calc-alkaline magmas may contain components from mantle peridotite, subducted oceanic crust, and continental crust.

2008 ◽  
Vol 145 (4) ◽  
pp. 463-474 ◽  
Author(s):  
SHEN LIU ◽  
RUI-ZHONG HU ◽  
CAI-XIA FENG ◽  
HAI-BO ZOU ◽  
CAI LI ◽  
...  

AbstractGeochemical and Sr–Nd–Pb isotopic data are presented for volcanic rocks from Zougouyouchaco (30.5 Ma) and Dogai Coring (39.7 Ma) of the southern and middle Qiangtang block in northern Tibet. The volcanic rocks are high-K calc-alkaline trachyandesites and dacites, with SiO2 contents ranging from 58.5 to 67.1 wt % The rocks are enriched in light REE (LREE) and contain high Sr (649 to 986 ppm) and relatively low Yb (0.8 to 1.2 ppm) and Y (9.5 to 16.6 ppm) contents, resulting in high La/Yb (29–58) and Sr/Y (43–92) ratios, as well as relatively high MgO contents and Mg no., similar to the compositions of adakites formed by slab melting in subduction zones. However, the adakitic rocks in the Qiangtang block are characterized by relatively low εNd(t) values (−3.8 to −5.0) and highly radiogenic Sr ((87Sr/86Sr)i=0.706–0.708), which are inconsistent with an origin by slab melting. The geochemistry and tectonics indicate that the adakitic volcanic rocks were most likely derived from partial melting of delaminated lower continental crust. As the pristine adakitic melts rose, they interacted with the surrounding mantle peridotite, elevating their MgO values and Mg numbers.


Geology ◽  
2019 ◽  
Vol 48 (3) ◽  
pp. 216-220 ◽  
Author(s):  
David Hernández-Uribe ◽  
Juan David Hernández-Montenegro ◽  
Kim A. Cone ◽  
Richard M. Palin

Abstract Arc volcanism and trace-element recycling are controlled by the devolatilization of oceanic crust during subduction. The type of fluid—either aqueous fluids or hydrous melts—released during subduction is controlled by the thermal structure of the subduction zone. Recent thermomechanical models and results from experimental petrology argue that slab melting occurs in almost all subduction zones, although this is not completely supported by the rock record. Here we show via phase equilibrium modeling that melting of either fresh or hydrothermally altered basalt rarely occurs during subduction, even at water-saturated conditions. Melting occurs only along the hottest slab-top geotherms, with aqueous fluids being released in the forearc region and anatexis restricted to subarc depths, leading to high-SiO2 adakitic magmatism. We posit that aqueous fluids and hydrous melts preferentially enhance chemical recycling in “hot” subduction zones. Our models show that subducted hydrothermally altered basalt is more fertile than pristine basaltic crust, enhancing fluid and melt production during subduction and leading to a greater degree of chemical recycling. In this contribution, we put forward a petrological model to explain (the lack of) melting during the subduction of oceanic crust and suggest that many large-scale models of mass transfer between Earth’s surface and interior may require revision.


1976 ◽  
Vol 13 (8) ◽  
pp. 1007-1019 ◽  
Author(s):  
Peter J. Wyllie ◽  
Wuu-Liang Huang ◽  
Charles R. Stern ◽  
Sven Maaløe

The calc-alkalic rocks of batholiths or their precursors may be generated in deep continental crust, in subducted oceanic crust, in the mantle wedge above, or in processes involving material from all three sources. For the series gabbro–tonalite–granite, we have phase relationships with excess H2O to 35 kbar (3500 MPa), and the H2O-undersaturated liquidus surfaces mapped with contours for H2O contents and with fields for near-liquidus minerals. Isobaric diagrams with low H2O contents provide grids potentially useful in defining limits for the H2O content of magmas, based on the sequence of crystallization. Conclusions from the experimental framework include: (1) The H2O content of large granitic bodies is less than 1.5%. (2) Primary granite magmas can not be derived from the mantle or subducted ocean crust. (3) Primary granite magmas with low H2O content are generated in the crust, and erupted as rhyolites. (4) Primary tonalite and andesite are not generated from mantle peridotite; the H2O contents required are unrealistically high. (5) Primary tonalite and andesite are not generated in the crust unless temperatures are significantly higher than those of regional metamorphism. (6) Subducted ocean crust yields magmas with intermediate SiO2 content, but not primary tonalite and andesite. (7) Batholiths are produced from crustal rocks as a normal consequence of regional metamorphism, with the formation of H2O-undersaturated granite liquid and mobilized migmatites. Some batholiths receive in addition contributions of material and heat from mantle and subducted ocean crust.


2020 ◽  
Vol 61 (2) ◽  
Author(s):  
Gong-Jian Tang ◽  
Qiang Wang ◽  
Derek A Wyman ◽  
Wei Dan ◽  
Lin Ma ◽  
...  

Abstract Accretionary orogens are characterized by voluminous juvenile components (recently derived from the mantle) and knowing the origin(s) of such components is vital for understanding crustal generation. Here we present field and petrological observations, along with mineral chemistry, zircon U–Pb age and Hf–O isotope data, and whole rock geochemical and Sr–Nd isotopic data for the c.320 Ma Ulungur intrusive complex from the Central Asian Orogenic Belt. The complex consists of two different magmatic series: one is characterized by medium- to high-K calc-alkaline gabbro to monzogranite; the other is defined by peralkaline aegirine–arfvedsonite granitoids. The calc-alkaline and peralkaline series granitoids have similar depleted mantle-like Sr–Nd–Hf isotopic compositions, but they have different zircon δ18O values: the calc-alkaline series have mantle-like δ18O values with mean compositions ranging from 5·2 ± 0·5‰ to 6·0 ± 0·9‰ (2SD), and the peralkaline granitoids have low δ18O values ranging from 3·3 ± 0·5‰ to 3·9 ± 0·4‰ (2SD). The calc-alkaline series were derived from a hydrous sub-arc mantle wedge, based on the isotope and geochemical compositions, under garnet peridotite facies conditions. This study suggests that the magmas underwent substantial differentiation, ranging from high pressure crystallization of ultramafic cumulates in the lower crust to lower pressure crystallization dominated by amphibole, plagioclase and minor biotite in the upper crust. The peralkaline series rocks are characterized by δ18O values lower than the mantle and enrichment of high field strength elements (HFSEs) and heavy rare earth elements (HREEs). They likely originated from melting of preexisting hydrothermally altered residual oceanic crust in the lower crust of the Junggar intra-oceanic arc. Early crystallization of clinopyroxene and amphibole was inhibited owing to their low melting temperature, leading to HFSEs and HREEs enrichment in residual peralkaline melts during crystallization of a feldspar-dominated mineral assemblage. Thus, the calc-alkaline and peralkaline series represent episodes of crust generation and reworking, respectively, demonstrating that the juvenile isotopic signature in accretionary orogens can be derived from diverse source rocks. Our results show that reworking of residual oceanic crust also plays an important role in continental crust formation for accretionary orogens, which has not previously been widely recognized.


2020 ◽  
Author(s):  
Gong-Jian Tang ◽  
Qiang Wang ◽  
Derek Wyman ◽  
Wei Dan ◽  
Lin Ma ◽  
...  

<p>Accretionary orogens are characterized by voluminous juvenile components (recently derived from the mantle) and knowing the origin(s) of such components is vital for understanding crustal generation. Here we present field and petrological observations, along with mineral chemistry, zircon U–Pb age and Hf-O isotope data, and whole rock geochemical and Sr-Nd isotopic data for the c. 320 Ma Ulungur intrusive complex from the Central Asian Orogenic Belt. The complex consists of two different magmatic series: one is characterized by medium-K to high-K calc-alkaline gabbro to monzogranite; the other is defined by peralkaline aegirine-arfvedsonite granitoids. The calc-alkaline and peralkaline series granitoids have similar depleted mantle-like Sr-Nd-Hf isotopic compositions, but they have different zircon δ<sup>18</sup>O values: the calc-alkaline series have mantle-like δ<sup>18</sup>O values with mean compositions ranging from 5.2 ± 0.5‰ to 6.0 ± 0.9‰ (2SD), and the peralkaline granitoids have low δ<sup>18</sup>O values ranging from 3.3 ± 0.5‰ to 3.9 ± 0.4‰ (2SD). The calc-alkaline series were derived from a hydrous sub-arc mantle wedge, based on the isotope and geochemical compositions, under garnet peridotite facies conditions. This study suggests that the magmas underwent substantial differentiation, ranging from high pressure crystallization of ultramafic cumulates in the lower crust to lower pressure crystallization dominated by amphibole, plagioclase and minor biotite in the upper crust. The peralkaline series rocks are characterized by δ<sup>18</sup>O values lower than the mantle and enrichment of high field strength elements (HFSEs) and heavy rare earth elements (HREEs). They likely originated from melting of preexisting hydrothermally altered residual oceanic crust in the lower crust of the Junggar intra-oceanic arc. Early crystallization of clinopyroxene and amphibole was inhibited owing to their low melting temperature, leading to HFSEs and HREEs enrichment in residual peralkaline melts during crystallization of a feldspar-dominated mineral assemblage. Thus, the calc-alkaline and peralkaline series represent episodes of crust generation and reworking, respectively, demonstrating that the juvenile isotopic signature in accretionary orogens can be derived from diverse source rocks. Our results show that reworking of residual oceanic crust also plays an important role in continental crust formation for accretionary orogens, which has not previously been widely recognized.</p>


2001 ◽  
Vol 172 (3) ◽  
pp. 319-332 ◽  
Author(s):  
Gaelle Prouteau ◽  
Rene C. Maury ◽  
Manuel Pubellier ◽  
Joseph Cotten ◽  
Herve Bellon

Abstract Magmatic activity linked to syn- or post-collisional zones leads to the emplacement of remarkably heterogeneous rocks: calc-alkaline, high-K calc-alkaline or shoshonitic series variably contaminated by continental crust; anatectic granites and ignimbrites derived from the latter; and finally alkali potassic to ultrapotassic basalts [Harris et al., 1990; Pearce et al., 1984, 1990; Arnaud et al., 1992; Benito et al., 1999]. The main sources of these magmas are either the upper mantle (sub-oceanic or subcontinental) frequently metasomatized by hydrous fluid originating from the subducted slab; or the continental crust, which can act as a contaminant [Benito et al., 1999; Miller et al., 1999] or melt directly [Harris et al., 1990; Zingg et al., 1990]. The purpose of the present paper is to document the role of a third source: the subducted oceanic crust, as evidenced by the occurrence of Miocene adakites in Sarawak (NW Borneo). The studied rocks have been sampled from western Sarawak (fig. 1), and their location is shown on the geological map [Tan, 1982] of figure 2. They mostly occur as stocks, dykes and sills which crosscut the Paleozoic to Miocene sedimentary units. Two kinds of intrusions can be distinguished. High-K calc-alkaline to medium-K calc-alkaline diorites and microdiorites occur in the northern part of the studied area, in Salak Island and Santubong Peninsula. Microtonalites and dacites occur near Kuching and in the southern part of Sarawak (Kuap and Bau areas). Whole-rock K-Ar data (table I) demonstrate that these two associations are of different ages: high-K calc-alkaline diorites were emplaced during the Lower Miocene (22.3 to 23.7 Ma), whereas the microtonalites and dacites are younger by ca. 8 Ma or more (Middle to Upper Miocene, 14.6 to 6.4 Ma). Major and trace element data (table II) show that the Lower Miocene diorites display all the usual characteristics of subduction-related magmas. The Middle to Upper Miocene microtonalites and dacites share some of these characteristics, but in addition they display typical adakitic features: SiO 2 -rich (65.5-70%) and sodic (Na 2 O/K 2 O>2) character (table II and figure 3); lack or rare occurrence of pyroxenes, usually replaced by early-crystallized (near-liquidus) amphiboles (table III); very low Y and HREE contents, consistent with the presence of residual garnet in their source, and leading to characteristically high La/Yb and Sr/Y ratios (fig. 4, 5). Their titanomagnetite-hemoilmenite associations reflect equilibrium features [Bacon and Hirschman, 1988] indicating moderate temperatures (<900 degrees C) and highly oxidizing (NNO+1) crystallization conditions [Ghiorso and Sack, 1991]. The Lower Miocene Sarawak diorites are typically subduction-related from a geochemical point of view. They likely derive from the evolution of island-arc basaltic magmas, which themselves originated from the partial melting of upper mantle peridotites previously metasomatized by hydrous fluids expelled from the subducting oceanic slab [Tatsumi et al., 1986; Tatsumi, 1989]. The origin of the Middle-Upper Miocene adakitic microtonalites and dacites is different. According to previous studies, they likely derive from the partial melting of metabasalts (garnet amphibolites or eclogites) from subducted oceanic crust [Defant and Drummond, 1990; Defant et al., 1991, 1992; Drummond et al., 1996; Maury et al., 1996; Martin, 1993, 1999]. Their position in the hybrid tonalite+peridotite system [Caroll and Wyllie, 1989] shows that they crystallized within the garnet stability field and likely interacted with the upper mantle during their ascent (fig. 7). This feature is not consistent with their genesis through melting of metabasalts accreted at the base of the Borneo continental crust. In addition, the less evolved Sarawak adakites display mineralogical and geochemical features remarkably similar to those of the 1991 Mt Pinatubo dacite, the experimental petrology of which has been extensively studied at low [2 kbar; Scaillet and Evans, 1999; Rutherford and Devine, 1996] to medium pressures [4 to 20 kbar; Prouteau et al., 1999]. Such dacitic magmas are not in equilibrium with garnet at pressures lower than or equal to 20 kbar, which rules out their derivation from metabasalts tectonically or magmatically accreted to the base of the North Borneo continental crust. We propose, instead, that they originated from the partial melting of basalts from a fragment of oceanic lithosphere within the upper mantle. Like the adakites of Central Mindanao, Philippines [Sajona et al., 1994, 1997 and 2000; Maury et al., 1996] and those from Aird Hills, Papua-New Guinea [Smith et al., 1979; Defant and Drummond, 1990] the Sarawak adakites represent potential markers of the occurrence at depth of oceanic crust slivers, which could be much more common in collision zones than previously thought.


2016 ◽  
Vol 12 (3) ◽  
pp. 125
Author(s):  
Ediar Usman ◽  
Udaya Kamiludin

Pengeplotan data unsur kimia pada diagram SiO2 vs K2O untuk sampel sedimen dasar laut cenderung terjadi kenaikan SiO2 dan penurunan K2O, sehingga arah evolusi berkembang dari kalk-alkalin sedang ke kalk-alkalin rendah (toleitik). Pada sampel batuan beku dan sedimen hasil pemboran memperlihatkan pola evolusi magma sebaliknya, terjadi kenaikan SiO2 dan K2O dalam seri magma yang sama (toleitik). Kondisi ini diperkuat oleh diagram segitiga AFM (A = Na2O+K2O; F = FeOtotal ; M = MgO) yang menunjukkan sebagian besar sampel yang diplot berada antara toleitik dan kalk-alkalin sedang. Hasil ini memberi kesimpulan bahwa batuan ini bersifat transisi antara toleitik dan kalk-alkalin sedang, dan condong ke arah seri toleitik sebagai indikasi batuan berasal dari daerah samudera. Berdasarlan pengeplotan pada diagram segitiga TiO2 – 10MnO – P2O5, lingkungan tektonik batuan beku di pantai Cibobos, sedimen dasar laut dan sedimen pemboran pada umumnya berada pada lingkungan tektonik andesit kepulauan samudera dan sebagian busur benua. Hasil tersebut, maka dapat disimpulkan bahwa sedimen di daerah Bayah berhubungan dengan seri magma dengan afinitas rendah mulai toleitik hingga kalk-alkalin sedang dan batuan samudera yang menyusup ke busur kepulauan atau busur benua. Hasil ini dapat mengetahui lingkungan dan evolusi batuan sumber sehingga diharapkan bermanfaat dalam kegiatan ekplorasi sumber daya mineral dan energi di masa mendatang. Kata kunci: unsur kimia utama, lingkungan tektonik, evolusi, kerak samudera dan kontinen, perairan Bayah Plotting of major elements data of the seafloor sediment samples on diagram of SiO2 vs K2O tends to increase the SiO2 and decrease the K2O, therefore the direction of evolution develop from medium to low calc-alkaline (tholeitic). From igneous rocks and drilling sediment samples shows that the evolution magma has the opposite pattern, increasing of SiO2 and K2O in the same magma series ( tholeitic). This condition is confirmed by the triangular diagram of AFM (A = Na2O+K2O; F = FeOtotal ; M = MgO) that shows the most of plotted samples are between medium calc-alkaline and tholeitic. This result give a conclusion that these rocks are at transitional area between tholeitic and medium calc-alkaline, and tend towards tholeitic series as an indication of rocks from oceanic zone. Based on plotting on the triangular diagram of TiO2 - 10MnO - P2O5, tectonic environment of igneous rocks in the coast of Cibobos, surface and drilling sediment samples, in general these samples are in the tectonic environment of oceanic islands andesite and partial of continental arc. From this study, it can be concluded that the sediment in the Bayah area is associated with affinity magma series from low kalk-alkaline (tholeitic) to medium calc-alkaline, and oceanic crust is being subducting to continental arc. This result could recognize the environment and the evolution of source rocks, therefore it may useful in the exploration activities of mineral and energy resources in the future. Keywords: major elements, tectonic environment, evolution, continental and oceanic crust, Bayah waters.


1984 ◽  
Vol 21 (12) ◽  
pp. 1426-1441 ◽  
Author(s):  
E. G. Nisbet

Simple isostatic models of the development of selected Archaean basins and greenstone belts can be used to constrain models of the Archaean lithosphere. Geophysical, geochemical, and thermal data imply that in southern Africa the late Archaean crust was probably comparable in thickness to the modern continental crust, and the whole lithosphere was perhaps over 80–100 km thick. Two Archaean belts studied may have developed by stretching of the order of 1.3–1.6:1. Isostatic and thermal data and petrological assumptions allow the construction of simple models of the Archaean oceanic lithosphere. Oceans were probably deep: mid-ocean ridges were probably subaqueous and fed by komatiitic liquids. Calc-alkaline volcanism in the Archaean may have been produced as a consequence of the subduction of hydrated komatiitic oceanic crust into a hot, low-viscosity asthensophere.


2021 ◽  
Vol 292 ◽  
pp. 452-467
Author(s):  
Rachel Bezard ◽  
Simon Turner ◽  
Bruce Schaefer ◽  
Gene Yogodzinski ◽  
Kaj Hoernle

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