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  • 1
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 93, No. S2 ( 2019-05), p. 6-6
    Abstract: The Kazdağı metaophiolite crops out in the Kazdağı (Ida) Mountains in the Biga Peninsula in northwestern Turkey. It is in stratigraphic contact with the high–grade metamorphic rocks of the Kazdağı Massif. Metaophiolitic and high–grade metamorphic rocks are tectonically overlain by low–grade metamorphic units of the Permo‐Triassic Karakaya Complex of the Sakarya Zone. Late Oligocene‐Early Miocene granites intruded these tectonic units (Okay and Satır, 2000; Duru et al. 2012). In the Kazdağı metaophiolitic sequence, upper mantle peridotites are represented by metaharzburgite and metadunite, whereas the mantle transition zone metaperidotites are composed of metadunite, metapyroxenite and minor plagioclase‐bearing metalherzolite. The upper part of the metadunites in the mantle transition zone show intercalation with metagabbros. Gabbros of oceanic crust experienced amphibolite facies metamorphism and are transformed into amphibolite, garnet amphibolite and migmatitic gabbros. The metagabbros and amphibolites display MORB‐ and IAT‐like geochemical features. The Kazdağı metaophiolite is conformably overline by basal conglomerates and hemi‐pelagic carbonate rocks continuing upward into forearc‐type flysch–like detrital sedimentary rocks interspersed with mafic volcanic intervals. These cover units underwent high–grade metamorphism into gneisses, migmatites, amphibolites and marbles in a compressional regime during the Alpine orogeny. New U–Pb zircon data from the metagabbros show two crystallization peaks at ∼52 Ma and ∼73 Ma. This has implications for the age of subduction of the Izmir–Ankara–Erzincan Ocean, generally assumed to be northward under the Sakarya Zone. During the Triassic to Middle Eocene, progressive overthrusting of the Sakarya Zone via a N–S compresional regime created by the Alpine orogeny onto subduction–accretion‐ and forearc‐units resulted in high–grade metamorphic conditions in the Biga Peninsula.
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    ISSN: 1000-9515 , 1755-6724
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    Publisher: Wiley
    Publication Date: 2019
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  • 2
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 89, No. s2 ( 2015-12), p. 98-98
    Type of Medium: Online Resource
    ISSN: 1000-9515 , 1755-6724
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    Publisher: Wiley
    Publication Date: 2015
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  • 3
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 91, No. s1 ( 2017-05), p. 16-17
    Abstract: The ophiolites that crop out discontinuously along the ∼2000 km Yarlung Zangbo Suture zone (YZSZ) between the Nanga Parbat and Namche Barwa syntaxes in southern Tibet represent the remnants of Neotethyan oceanic lithosphere (Fig. 1a). We have investigated the internal structure and the geochemical makeup of mafic‐ultramafic rock assemblages that are exposed in the westernmost segment of the YZSZ where the suture zone architecture displays two distinct sub‐belts of ophiolitic and mélange units separated by a continental Zhongba terrane (Fig. 1b). These two sub‐belts include the Daba – Xiugugabu in the south (Southern sub‐belt, SSB) and the Dajiweng – Saga in the north (Northern sub‐belt, NSB). We present new structural, geochemical, geochronological data from upper mantle peridotites and mafic dike intrusions occurring in these two sub‐belts and discuss their tectonomagmatic origin. In‐situ analysis of zircon grains obtained from mafic dikes within the Baer, Cuobuzha and Jianabeng massifs in the NSB, and within the Dongbo, Purang, Xiugugabu, Zhaga and Zhongba in the SSB have yielded crystallization ages ranging between130 and 122 Ma. Dike rocks in both sub‐belts show N‐MORB REE patterns and negative Nb, Ta and Ti anomalies, reminiscent of those documented from SSZ ophiolites. Harzburgitic host rocks of the mafic dike intrusions mainly display geochemical compositions of abyssal peridotites (Fig. 2), with the exception of the Dajiweng harzburgites, which show the geochemical signatures of forearc peridotites (Lian et al., 2016). Extrusive rocks that are spatially associated with these peridotite massifs in both sub‐belts also have varying compositional and geochemical features. Tithonian to Valanginian (150 – 135 Ma) basaltic rocks in the Dongbo massif have OIB‐like geochemistry and 138 Ma basaltic lavas in the Purang massif have EMORB‐like geochemistry (Liu et al., 2015). Tuffaceous rocks in the Dajiweng massif are 140 Ma in age and show OIB‐like geochemistry. We interpret these age and geochemical data to reflect a rifted continental margin origin of the extrusive rock units in both sub‐belts. These data and structural observations show that the western Yarluang Zangbo ophiolites represent fragments of an Ocean‐Continent Transition (OCT) peridotites altered by fluids in an initial supersubduction setting. We infer that mafic‐ultramafic rock assemblages exposed in the SSB and NSB initially formed in an ocean – continent transition zone (OCTZ) during the late Jurassic, and that they were subsequently emplaced in the forearc setting of an intraoceanic subduction zone within a Neotethyan seaway during 130 to 122 Ma. The NSB and SSB are hence part of a single, S‐directed nappe sheet derived from a Neotethyan seaway located north of the Zhongba terrane.
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    ISSN: 1000-9515 , 1755-6724
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  • 4
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    Wiley ; 2017
    In:  Acta Geologica Sinica - English Edition Vol. 91, No. s1 ( 2017-05), p. 49-49
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 91, No. s1 ( 2017-05), p. 49-49
    Abstract: Deeply subducted lithospheric slabs may reach to the mantle transition zone (MTZ, 410–660 km depth) or even to the core – mantle boundary (CMB) at depths of ∼2900 km. Our knowledge of the fate of subducted surface material at the MTZ or near the CMB is poor and based mainly on the tomography data and laboratory experiments through indirect methods. Limited data come from the samples of deep mantle diamonds and their mineral inclusions obtained from kimberlites and associated rock assemblages in old cratons. We report in this presentation new data and observations from diamonds and other UHP minerals recovered from ophiolites that we consider as a new window into the life cycle of deeply subducted oceanic and continental crust. Ophiolites are fragments of ancient oceanic lithosphere tectonically accreted into continental margins, and many contain significant podiform chromitites. Our research team has investigated over the last 10 years ultrahigh‐pressure and super‐reducing mineral groups discovered in peridotites and/or chromitites of ophiolites around the world, including the Luobusa (Tibet), Ray‐Iz (Polar Urals‐Russia), and 12 other ophiolites from 8 orogenic belts in 5 different countries (Albania, China, Myanmar, Russia, and Turkey). High‐pressure minerals include diamond, coesite, pseudomorphic stishovite, qingsongite (BN) and Ca‐Si perovskite, and the most important native and highly reduced minerals recovered to date include moissanite (SiC), Ni‐Mn‐Co alloys, Fe‐Si and Fe‐C phases. These mineral groups collectively confirm extremely high‐¬ pressures (300 km to ≥660 km) and super‐reducing conditions in their environment of formation in the mantle. All of the analyzed diamonds have unusually light carbon isotope compositions (δ 13 C = −28.7 to −18.3‰) and variable trace element contents that distinguish them from most kimberlitic and UHP metamorphic varieties. The presence of exsolution lamellae of diopside and coesite in some chromite grains suggests chromite crystallization depths around 〉 380 km, near the mantle transition zone. The carbon isotopes and other features of the high‐pressure and super‐reduced mineral groups point to previously subducted surface material as their source of origin. Recycling of subducted crust in the deep mantle may proceed in three stages: Stage 1 – Carbon‐bearing fluids and melts may have been formed in the MTZ, in the lower mantle or even near the CMB. Stage 2 – Fluids or melts may rise along with deep plumes through the lower mantle and reach the MTZ. Some minerals, such as diamond, stishovite, qingsongite and Ca‐silicate perovskite can precipitate from these fluids or melts in the lower mantle during their ascent. Material transported to the MTZ would be mixed with highly reduced and UHP phases, presumably derived from zones with extremely low fO 2 , as required for the formation of moissanite and other native elements. Stage 3 – Continued ascent above the transition of peridotites containing chromite and ultrahigh‐pressure minerals transports them to shallow mantle depths, where they participate in decompressional partial melting and oceanic lithosphere formation. The widespread occurrence of ophiolite‐hosted diamonds and associated UHP mineral groups suggests that they may be a common feature of in‐situ oceanic mantle. Because mid‐ocean ridge spreading environments are plate boundaries widely distributed around the globe, and because the magmatic accretion of oceanic plates occurs mainly along these ridges, the on‐land remnants of ancient oceanic lithosphere produced at former mid‐ocean ridges provide an important window into the Earth's recycling system and a great opportunity to probe the nature of deeply recycled crustal material residing in the deep mantle
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  • 5
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 94, No. S1 ( 2020-10), p. 13-13
    Abstract: The Zhangguangcai Range in the Xing'an(Hinggan) Mongolian Orogenic Belt, NE China, contains Early Jurassic (c. 188 Ma) Dabaizigou (DBZG) porphyritic dolerite. Compared with other island‐arc mafic rocks, the DBZG dolerite is characterized by high trace‐element contents, relatively weak Nb and Ta enrichments, and no Zr, Hf or Ti depletions, similar to OIB‐type rocks. Analysed rocks have ( 87 Sr/ 86 Sr) i ratios of 0.7033–0.7044, relatively uniform positive ∊ Nd ( t ) values of 2.3–3.2 and positive ∊ Hf ( t ) values of 8.5–17.1. Trace‐element and isotopic modelling indicates that the DBZG mafic rocks were generated by partial melting of asthenospheric mantle under garnet‐to spinel‐facies conditions. The occurrence of OIB‐like mafic intrusion suggests significant upwelling of the asthenosphere in response to lithospheric attenuation caused by continental rifting. These processes occurred in an incipient continental back‐arc environment in the upper plate of a palaeo‐Pacific slab subducting W–NW beneath East Asia.
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    ISSN: 1000-9515 , 1755-6724
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    Publisher: Wiley
    Publication Date: 2020
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  • 6
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    Wiley ; 2017
    In:  Acta Geologica Sinica - English Edition Vol. 91, No. s1 ( 2017-05), p. 24-25
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 91, No. s1 ( 2017-05), p. 24-25
    Abstract: Mesozoic ophiolites crop out discontinuously in the Indo‐Myanmar Ranges in NE India and Myanmar, and represent the remnants of the Neotethyan oceanic lithosphere (Sengupta et al., 1990; Mitchell, 1993). These ophiolites in the Indo‐Myanmar Ranges are the southern continuation of the Neotethyan ophiolites occurring along the Yarlung Zangbo Suture Zone (YZSZ) in southern Tibet farther northwest (Mitchell, 1993; Fareeduddin and Dilek, 2015), as indicated by their coeval crystallization ages and geochemical compositions (Yang et al., 2012; Liu et al., 2016). The Kalaymyo ophiolite is located in the central part of the eastern Indo‐Myanmar Ranges (Fig. 1). composition of these ophiolites from the central Tibetan Plateau (CTP) is dominated by MORBs and minor OIBs and a distinct lack of IATs and BONs, which is inconsistent with most ophiolites worldwide (Robinson and Zhou, 2008; Zhang et al., 2008). But the generation and tectonic nature of these ophiolites are still controversial. The Kalaymyo peridotites consist mainly of harzburgites, which show typical porphyroclastic or coarse‐grained equigranular textures. They are composed of olivine (Fo = 89.8–90.5), orthopyroxene (En86‐91Wo1‐4Fs8‐10; Mg# = 89.6–91.9), clinopyroxene (En46‐49Wo47‐50Fs3‐5; Mg# = 90.9–93.6) and spinel (Mg# = 67.1–78.9; Cr# = 13.5–31.5), and have relatively homogeneous whole‐rock compositions with Mg#s of 90.1–90.8 and SiO 2 (41.5–43.65 wt.%), Al 2 O 3 (1.66–2.66 wt.%) and CaO (1.45–2.67 wt.%) contents. They display Light Rare Earth Element (LREE)‐depleted chondrite‐normalized REE patterns with (La/Yb) CN = 0.04–0.21 and (Gd/Yb) CN = 0.40–0.84, and show a slight enrichment from Pr to La with (La/Pr)CN in the range of 0.98–2.36. The Kalaymyo peridotites are characterized by Pd‐enriched chondrite‐normalized PGE patterns with superchondritic (Pd/Ir)CN ratios (1.15–2.36). Their calculated oxygen fugacities range between QFM–0.57 and QFM+0.90. These mineralogical and geochemical features collectively suggest that the Kalaymyo peridotites represent residual upper mantle rocks after low to moderate degrees (5–15%) of partial melting at a mid‐ocean‐ridge (MOR) environment. The observed enrichment in LREE and Pd was a result of their reactions with enriched MORB‐like melts, percolating through these already depleted, residual peridotites. The Kalaymyo and other ophiolites in the Indo‐Myanmar Ranges hence represent mid‐ocean ridge (MOR)–type Tethyan oceanic lithosphere derived from a downgoing plate and accreted into a westward migrating subduction–accretion system along the eastern margin of India.
    Type of Medium: Online Resource
    ISSN: 1000-9515 , 1755-6724
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    Publication Date: 2017
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  • 7
    Online Resource
    Online Resource
    Wiley ; 2019
    In:  Acta Geologica Sinica - English Edition Vol. 93, No. S2 ( 2019-05), p. 23-23
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 93, No. S2 ( 2019-05), p. 23-23
    Abstract: Mesozoic ophiolites crop out discontinuously in the Indo‐Myanmar Ranges in NE India and Myanmar, and represent the remnants of the Neotethyan oceanic lithosphere. These ophiolites in the Indo‐Myanmar Ranges are the southern continuation of the Neotethyan ophiolites occurring along the Yarlung Zangbo Suture Zone in southern Tibet farther northwes, as indicated by their coeval crystallization ages and geochemical compositions. The Kalaymyo ophiolite is located in the central part of the Indo‐Myanmar Ranges (Myanmar). The Kalaymyo ophiolite are composed of olivine (Fo = 89.8–90.5), orthopyroxene (En86‐91Wo1‐4Fs8‐10; Mg#=89.6–91.9), clinopyroxene (En46‐49Wo47‐50Fs3‐5; Mg# = 90.9–93.6) and spinel (Mg# = 67.1–78.9; Cr# = 13.5–31.5), and have relatively homogeneous whole‐rock compositions with Mg# of 90.1–90.8 and SiO2 (41.5–43.65 wt.%), Al 2 O 3 (1.66–2.66 wt.%) and CaO (1.45–2.67 wt.%) contents. They display Light Rare Earth Element (LREE)‐depleted chondrite‐normalized REE patterns and show a slight enrichment from Pr to La. The Kalaymyo peridotites are characterized by Pd‐enriched chondrite‐normalized PGE patterns with superchondritic (Pd/Ir) CN ratios (1.15–2.36). Their calculated oxygen fugacities range between QFM–0.57 and QFM+0.90. These features collectively suggest that the Kalaymyo peridotites represent residual upper mantle rocks after low to moderate degrees (5–15%) of partial melting at a mid‐ocean‐ridge environment. The observed enrichment in LREE and Pd was a result of their reactions with enriched MORB‐like melts, percolating through these already depleted, residual peridotites. The Kalaymyo and other ophiolites in the Indo‐Myanmar Ranges hence represent mid‐ocean ridge–type Tethyan oceanic lithosphere derived from a downgoing plate and accreted into a westward migrating subduction–accretion system along the eastern margin of India.
    Type of Medium: Online Resource
    ISSN: 1000-9515 , 1755-6724
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    Publication Date: 2019
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  • 8
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    Wiley ; 2019
    In:  Acta Geologica Sinica - English Edition Vol. 93, No. S2 ( 2019-05), p. 8-8
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 93, No. S2 ( 2019-05), p. 8-8
    Abstract: The Yarlung Zangbo suture zone (YZSZ) in southern Tibet includes the remnants of Neo‐Tethyan oceanic lithosphere and marks a major suture between the Indian plate to the south and the Lhasa terrane of Tibet to the north. The upper mantle section of the Cuobuzha ophiolite in the northern subbelt of the western YZSZ comprises mainly clinopyroxene (cpx)‐rich and depleted harzburgites. Spinels in the cpx‐harzburgites show lower Cr # values (12.6–15.1) than the spinels in the harzburgites (26.1–34.5), and the cpx‐harzburgites display higher heavy rare earth element concentrations than the depleted harzburgites. The harzburgites have subchondritic Os isotopic compositions (0.11624–0.11699), yielding Re‐depletion model ages (TRD) ages from 1.8 to 1.7 Ga, indicating that the Cubuzha mantle underwent at least one ancient melt extraction event ca. 1.8‐1.7Ga; whereas the cpx‐harzburgites have suprachondritic 187 Os/ 188 Os ratios (0.12831–0.13125) with higher Re concentrations (0.380–0.575 ppb), indicating subsequent addition of Re following the last partial melting event that occurred during mid‐ocean ridge melt evolution processes. Although these geochemical and isotopic signatures suggest that both peridotite types in the ophiolite represent mid‐oceanic ridge–type upper mantle units, their melt evolution trends reflect different mantle processes. The cpx‐harzburgites formed from low‐degree partial melting of a primitive mantle source, and they were subsequently modified by melt‐rock interactions in a mid‐oceanic ridge environment. The depleted harzburgites, however, were produced by remelting of the cpx‐harzburgites, which later interacted with mid‐oceanic ridge basalt– or island‐arc tholeiite–like melts, possibly in a trench–distal backarc spreading center. Our new isotopic and geochemical data from the Cuobuzha peridotites confirm that the Neo‐Tethyan upper mantle had highly heterogeneous Os isotopic compositions as a result of multiple melt production and melt extraction events during its seafloor spreading evolution.
    Type of Medium: Online Resource
    ISSN: 1000-9515 , 1755-6724
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  • 9
    Online Resource
    Online Resource
    Wiley ; 2017
    In:  Acta Geologica Sinica - English Edition Vol. 91, No. s1 ( 2017-05), p. 8-9
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 91, No. s1 ( 2017-05), p. 8-9
    Abstract: Ophiolites consist predominantly of mafic‐ultramafic rocks but also contain in subordinate amounts intermediate to silicic intrusive – extrusive rocks in them. These rocks, although not in large volumes in comparison to mafic–ultramafic units, reveal significant clues about melt evolution, magmatic accretion processes, and partial melting of pre‐existing oceanic crust during ophiolite evolution. They also yield ample accessory minerals, such as zircon and monazite, which are widely used to date the timing of oceanic crust generation. We present a global synthesis of the occurrence of such leucocratic, intrusive and volcanic rocks from 150 Phanerozoic to Archean ophiolites, and evaluate models for their genesis during the development of oceanic crust in different tectonic environments. In the ophiolite complexes we have investigated, intrusive and extrusive rocks show a wide range in composition. Intermediate rocks (with SiO 2 between 52 and 63 wt.%) include andesite and diorite, whereas the silicic rocks (with SiO 2 more than 63 wt.%) include dacite, trondhjemite, tonalite and granite. For subduction‐related and subduction‐unrelated MORB‐type ophiolites in the Phanerozoic orogenic belts, the most commonly reported intermediate to silicic intrusive rocks, independent of their original tectonic setting, are trondhjemite, plagiogranite and tonalite, and less commonly quartz‐diorite and diorite. These rock types have been documented from 80 percent of the 104 ophiolites included in this study. Intermediate to silicic lavas and/or pyroclastic rocks (basaltic andesite, andesite, dacite and rhyolite) are less abundant, and have been reported from only 35 percent of the 104 ophiolites. Trachyte occurs in some of the Rift/Continental Margin type, subduction‐unrelated ophiolites Evolved rocks in subduction‐unrelated, Rift/Continental Margin ophiolites are predominantly basaltic andesite and andesite, whereas MOR type (mid‐ocean ridge) ophiolites exhibit nearly equal proportions of basaltic andesite/andesite and rhyodacite and Plume/MOR type ophiolites are characterized by rhyolites. Intermediate to silicic volcanic uints in the Backarc sub‐group of subduction‐related ophiolites are characterized by similar amounts of basaltic andesite/andesite and rhyodacite, whereas in the Backarc to Forearc, Forearc, and Volcanic Arc sub‐groups they are mainly basaltic andesite/andesite. Intermediate to silicic rocks in Rift/Continental Margin and Plume/MOR type ophiolites are generally LREE‐enriched, whereas those in the MOR type vary from LREE‐depleted to LREE‐enriched. The Backarc and Backarc to Forearc types are similar to the MOR type; silicic rocks of the Forearc and Volcanic Arc types are generally LREE‐enriched. The main process in the formation of the majority of the intermediate to silicic rocks in both subduction‐unrelated and subduction‐related ophiolites is partial melting of basaltic and/or gabbroic rocks beneath the spreading centers, whereas a minor volume in subduction‐related ophiolites are adakites that were produced from partial melting of a subducting slab. Silcic to intermediate rocks in Plume/MOR type ophiolites are generated by fractional crystallization of basaltic melt. The incompatible, non‐conservative elements, such as Ba and Th, are weakly to strongly enriched in subduction‐related ophiolites as a result of shallow to deep enrichment associated with subduction zone processes. The field occurrence and the geochemical character of leucocratic rocks in ophiolites show considerable variations, providing additional constraints on the petrogenesis of ophiolites in different tectonic settings. Fractional crystallization appears to have been an important process in the formation of the intermediate to silicic rocks in Rift/CM and P/MOR ophiolites in the subduction‐unrelated class, as well as VA ophiolites in the subduction‐related class. In these types of ophiolites magma chambers might have operated as closed‐systems for a sufficient amount of time for fractionation and compositional zoning of the magma to take place (Fig. 1C1). Fractional crystallization was of subordinate importance during the igneous construction of the MOR, BA, FA, and BA‐FA ophiolites. Instead, partial melting of hydrothermally altered crust was the most common process resulting in the majority of the intermediate to felsic rocks of the Rift/CM (estimated to 60%), MOR (estimated to 95%), and the BA, FA and BA‐FA (estimated to 75%) ophiolites, as well as a high proportion of the VA ophiolites (∼ 40%) (Fig. 1C2). Slab‐generated melts that result in the production of intermediate to silicic rocks of adakitic character represent a relatively small fraction (∼15% in Phanerozoic ophiolites) of subduction‐related ophiolites (Fig. 1C3). Some adakites are very low in incompatible elements (e.g., La), suggesting that these melts were generated from highly depleted MORB. Precambrian ophiolites contain a higher percentage of adakites (ca. 35%), indicating that physical conditions were more favorable for slab melting during the Precambrian than in the Phanerozoic. This phenomenon may have resulted from higher geothermal gradient along relatively shallow‐dipping subduction zones during the Precambrian.
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    ISSN: 1000-9515 , 1755-6724
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  • 10
    In: Acta Geologica Sinica - English Edition, Wiley, Vol. 93, No. S2 ( 2019-05), p. 16-16
    Abstract: He Pozanti‐Karsanti ophiolite (PKO) is one of the largest oceanic remnants in the Tauride belt, Turkey. Micro‐diamonds were recovered from the podiform chromitites, and these were investigated based on morphology, color, cathodoluminescence, nitrogen content, carbon and nitrogen isotopes, internal structure and inclusions. The diamonds recovered from the PKO are mainly mixed‐habit diamonds with sectors of different brightness under the cathodoluminescence images. The total δ 13 C range of the PKO diamonds ranges between −18.8 ‰ and −28.4 ‰, with a principle δ 13 C mode at −25 ‰. Nitrogen contents of the diamonds range from 7 to 541 μg/g with a mean value of 171 μg/g, and the δ 15 N values range from −19.1 ‰ to 16.6 ‰, with a δ 15 N mode of −9 ‰. Stacking faults and partial dislocations are commonly observed in the Transmission Electron Microscopy foils whereas inclusions are rather rare. Combinations of (Ca 0.81 Mn 0.19 )SiO 3 , NiMnCo‐alloy and nano‐size, quenched fluid phases were observed as inclusions in the PKO diamonds, confirming a natural origin of these diamonds. We believe that the δ 13 C‐depleted carbon signature of the PKO diamonds is a remnant of previously subducted crustal matter. These diamonds may have crystallized in metal‐rich melts in the asthenospheric mantle at depth below 250 km which were subsequently carried rapidly upward by asthenospheric melts/fliuds. We concluded that diamond‐bearing asthenospheric melts were likely involved in the formation of the Pozanti‐Karsanti podiform chromitite.
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    ISSN: 1000-9515 , 1755-6724
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    Publisher: Wiley
    Publication Date: 2019
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