Renelle Dubosq, Alfredo Camacho, Anna Rogowitz, Siyuan Zhang, Baptiste Gault
Garnet is a common rock-forming mineral that occurs in a variety of rock types and over a wide range of pressure (P)–temperature (T) conditions in the Earth's lithosphere. Because garnet is considered a high-strength mineral stable across an extensive range of conditions (1–25 GPa, <300–2000°C), it is generally accepted that garnets can retain their microstructures and chemical composition during deformation and metamorphism. Therefore, garnet is commonly used as a geothermobarometer and geochronometer to provide P–T and timing constraints on tectonic events. Herein, we study garnet from an eclogite facies mylonite (central Australia) to investigate the mechanisms of element mobility during high-strain deformation under relatively dry, lower crustal conditions. Electron backscatter diffraction (EBSD) and electron channelling contrast imaging (ECCI) reveal evidence of crystal plasticity associated with brittle deformation in the form of heterogeneous misorientation patterns and low-angle grain boundaries developed over length scales of 20–50 μm in the rims of garnet porphyroclasts. Atom probe tomography (APT) analysis of a low-angle grain boundary within a highly strained portion of a clast shows Ca enrichment and Mg depletion along dislocations, whereas APT data along the rim of a mostly undeformed clast reveal a homogeneous distribution of garnet major components in the specimen matrix with the exception of Ca, Fe and Mg enrichment within a healed microfracture. The above-mentioned results suggest that under relatively dry conditions, crystal plasticity enhances bulk element mobility via pipe diffusion, highlighting the importance of deformation-induced microstructures on element mobility, with important implications for the robust and reliable use of garnet as a petrological tool.
{"title":"Influence of high-strain deformation on major element mobility in garnet: Nanoscale evidence from atom probe tomography","authors":"Renelle Dubosq, Alfredo Camacho, Anna Rogowitz, Siyuan Zhang, Baptiste Gault","doi":"10.1111/jmg.12758","DOIUrl":"10.1111/jmg.12758","url":null,"abstract":"<p>Garnet is a common rock-forming mineral that occurs in a variety of rock types and over a wide range of pressure (P)–temperature (T) conditions in the Earth's lithosphere. Because garnet is considered a high-strength mineral stable across an extensive range of conditions (1–25 GPa, <300–2000°C), it is generally accepted that garnets can retain their microstructures and chemical composition during deformation and metamorphism. Therefore, garnet is commonly used as a geothermobarometer and geochronometer to provide P–T and timing constraints on tectonic events. Herein, we study garnet from an eclogite facies mylonite (central Australia) to investigate the mechanisms of element mobility during high-strain deformation under relatively dry, lower crustal conditions. Electron backscatter diffraction (EBSD) and electron channelling contrast imaging (ECCI) reveal evidence of crystal plasticity associated with brittle deformation in the form of heterogeneous misorientation patterns and low-angle grain boundaries developed over length scales of 20–50 μm in the rims of garnet porphyroclasts. Atom probe tomography (APT) analysis of a low-angle grain boundary within a highly strained portion of a clast shows Ca enrichment and Mg depletion along dislocations, whereas APT data along the rim of a mostly undeformed clast reveal a homogeneous distribution of garnet major components in the specimen matrix with the exception of Ca, Fe and Mg enrichment within a healed microfracture. The above-mentioned results suggest that under relatively dry conditions, crystal plasticity enhances bulk element mobility via pipe diffusion, highlighting the importance of deformation-induced microstructures on element mobility, with important implications for the robust and reliable use of garnet as a petrological tool.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 3","pages":"355-372"},"PeriodicalIF":3.4,"publicationDate":"2024-01-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12758","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139589180","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
An eclogite from the Early Palaeozoic Fleur-de-Lys Supergroup in Newfoundland was studied because of its biotite porphyroblasts, which very rarely occur in this rock type. Thermodynamic modelling suggests that eclogitic biotite in common metabasite (former basalt–gabbro) is limited to (1) bulk-rock compositions, which are relatively rich in Fe2+ and K and poor in Fe3+, and (2) the low-pressure range of the eclogite facies. The latter reason is supported by the determination of the pressure–temperature (P–T) path of the Newfoundland eclogite. Chemical zonation of garnet, presence of phengite with Si contents of ~3.4 per formula unit, Zr contents in rutile and petrographic observations resulted in a P–T trajectory starting at medium-pressure conditions. Nearly isothermal burial led to a peak pressure of 18–19 kbar at ~575°C, followed by exhumation and slight heating. Deformation occurred at or close to the peak pressure. Subsequent introduction of hydrous fluids caused the formation of porphyroblasts of biotite and Ca–amphibole in the pressure range of 12–17 kbar at peak temperatures of 625–640°C. Retrogression led to very fine-grained symplectites around omphacite and phengite and marginal replacement of biotite porphyroblasts by plagioclase and titanite. Geodynamic scenarios invoking either a flat subduction of oceanic crust followed by continent–continent collision or intracontinental subduction along a transpressional fault system might best explain the formation of eclogite with biotite porphyroblasts in general. For the Newfoundland eclogite, the latter scenario is preferred.
{"title":"Eclogite with biotite porphyroblasts—Which conditions are responsible for their formation? An example from the northern Fleur-de-Lys Supergroup, Newfoundland, Canada","authors":"Hans-Joachim Massonne","doi":"10.1111/jmg.12755","DOIUrl":"10.1111/jmg.12755","url":null,"abstract":"<p>An eclogite from the Early Palaeozoic Fleur-de-Lys Supergroup in Newfoundland was studied because of its biotite porphyroblasts, which very rarely occur in this rock type. Thermodynamic modelling suggests that eclogitic biotite in common metabasite (former basalt–gabbro) is limited to (1) bulk-rock compositions, which are relatively rich in Fe<sup>2+</sup> and K and poor in Fe<sup>3+</sup>, and (2) the low-pressure range of the eclogite facies. The latter reason is supported by the determination of the pressure–temperature (P–T) path of the Newfoundland eclogite. Chemical zonation of garnet, presence of phengite with Si contents of ~3.4 per formula unit, Zr contents in rutile and petrographic observations resulted in a P–T trajectory starting at medium-pressure conditions. Nearly isothermal burial led to a peak pressure of 18–19 kbar at ~575°C, followed by exhumation and slight heating. Deformation occurred at or close to the peak pressure. Subsequent introduction of hydrous fluids caused the formation of porphyroblasts of biotite and Ca–amphibole in the pressure range of 12–17 kbar at peak temperatures of 625–640°C. Retrogression led to very fine-grained symplectites around omphacite and phengite and marginal replacement of biotite porphyroblasts by plagioclase and titanite. Geodynamic scenarios invoking either a flat subduction of oceanic crust followed by continent–continent collision or intracontinental subduction along a transpressional fault system might best explain the formation of eclogite with biotite porphyroblasts in general. For the Newfoundland eclogite, the latter scenario is preferred.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 3","pages":"291-318"},"PeriodicalIF":3.4,"publicationDate":"2024-01-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12755","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139517275","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Charlotte Möller, Yue Cai, Hannes K. Brueckner, Kristoffer Szilas, Martin J. Whitehouse
The Western Gneiss Region (WGR) is a Precambrian basement domain in the Scandinavian Caledonides and one of the world's largest high- and ultrahigh-pressure terranes. The south–central WGR underwent regional eclogite facies metamorphism 415–400 Ma ago when Baltica subducted beneath Laurentia, during the Scandian orogeny. Eclogites in the WGR group into two traditional types: (1) Precambrian mafic intrusions metamorphosed in situ during Scandian continental subduction and (2) eclogites, garnet peridotites and garnet pyroxenites within ultramafic complexes derived from the subcontinental mantle beneath Laurentia. We document, using field relations, petrography, whole-rock geochemistry and secondary ion mass spectrometry (SIMS) zircon geochronology, a hitherto unrecognized third type of eclogite in the WGR that places new constraints on its tectonic architecture: an eclogitized fragment of oceanic crust from the Iapetus Ocean. The Kråkfjord eclogite complex is a km2-sized body with an interior consisting of kyanite eclogite (meta-troctolite) and subordinate layers and lenses of garnet peridotite, garnet websterite and kyanite–garnet leucotonalite. This interior is capped by Fe–Ti-rich eclogite, which locally contains subordinate pockets of migmatitic aluminous gneiss. The elemental abundances and isotopic compositions of the Fe–Ti-rich eclogites resemble those of mid-ocean ridge basalt (MORB). In contrast, the interior kyanite eclogites, peridotites and pyroxenites have compositions similar to the gabbroic cumulates in the lower oceanic crust of slow-spreading ridges. U–Pb SIMS dating of igneous zircon cores from a leucotonalite pod in the interior of the Kråkfjord complex yields Cambro-Ordovician igneous ages of 500–440 Ma, with the ~500 Ma age interpreted as the isotopically undisturbed age. This age matches those of Iapetan oceanic rocks exposed elsewhere in the mountain belt. Metamorphic zircon from an Fe–Ti-rich eclogite in the carapace of the Kråkfjord complex dates the eclogite facies metamorphism at 421.9 ± 2.2 Ma, synchronous with the continental collision. Zircon from a leucosome in Fe–Ti-rich retro-eclogite indicates an age of 408.5 ± 2 Ma for the crystallization of partial melt following the decompression. Detrital zircon core ages from a pocket of aluminous migmatitic gneiss in the carapace indicate derivation of sediment from the Baltic crust. Collectively, the data show that the eclogite complex (1) originated at an Iapetus spreading centre near the continent Baltica, (2) subducted to eclogite conditions during Scandian continental collision and (3) was tectonically intercalated with the Precambrian Baltica basement of the WGR.
西部片麻岩地区(WGR)是斯堪的纳维亚喀里多尼亚山系的前寒武纪基底区域,也是世界上最大的高压和超高压地层之一。在 415-400 Ma 前的斯堪的纳维亚造山运动期间,当波罗的海俯冲到劳伦西亚之下时,WGR 中南部经历了区域性的蚀变岩面变质作用。西太平洋地区的斜长岩分为两种传统类型:(1) 前寒武纪黑云母侵入体在斯堪的纳维亚大陆俯冲过程中就地变质;(2) 来自劳伦提亚地下次大陆地幔的超基性复合体中的斜长岩、石榴石橄榄岩和石榴石辉石。我们利用现场关系、岩相学、全岩地球化学和二次离子质谱(SIMS)锆石地质年代学,记录了迄今为止尚未认识到的世界地质公园内的第三类蚀变岩,为其构造结构提供了新的制约因素:来自伊阿佩托斯洋的大洋地壳蚀变碎片。Kråkfjord斜长岩复合体是一个平方公里大小的岩体,其内部由闪长岩斜长岩(元直长岩)以及石榴石橄榄岩、石榴石网纹岩和闪长岩-石榴石白云母的附属层和透镜体组成。内部被富含铁钛的辉绿岩所覆盖,局部含有从属的偏闪铝片麻岩。富钛铁闪长岩的元素丰度和同位素组成与大洋中脊玄武岩(MORB)相似。相比之下,内部的辉长岩、橄榄岩和辉绿岩的成分与慢展海脊下洋壳中的辉长岩累积岩相似。对克拉科峡湾岩群内部白云母岩荚中的火成岩锆石岩心进行 U-Pb SIMS 测定,得出了 500-440 Ma 的寒武-奥陶纪火成岩年龄,其中约 500 Ma 的年龄被解释为同位素未扰动年龄。这一年龄与山脉带其他地方出露的伊阿佩坦洋岩的年龄相吻合。从克拉科夫峡湾复合地壳中一块富含铁钛的斜长岩中提取的变质锆石,将斜长岩面变质的年代定为 421.9 ± 2.2 Ma,与大陆碰撞同步。富含铁钛的后夕长岩中的白云母中的锆石表明,减压后部分熔体结晶的年龄为 408.5 ± 2 Ma。从躯壳中的一袋铝辉长片麻岩中提取的锆石岩芯年龄表明,沉积物来自波罗的海地壳。总之,这些数据表明夕卡岩复合体(1)起源于波罗的海大陆附近的伊阿佩图斯扩张中心,(2)在斯堪的纳维亚大陆碰撞过程中俯冲至夕卡岩条件,(3)在构造上与波罗的海前寒武纪波罗的海基底相互交错。
{"title":"An Iapetus origin for a layered eclogite complex in the northern Western Gneiss Region, Scandinavian Caledonides","authors":"Charlotte Möller, Yue Cai, Hannes K. Brueckner, Kristoffer Szilas, Martin J. Whitehouse","doi":"10.1111/jmg.12757","DOIUrl":"10.1111/jmg.12757","url":null,"abstract":"<p>The Western Gneiss Region (WGR) is a Precambrian basement domain in the Scandinavian Caledonides and one of the world's largest high- and ultrahigh-pressure terranes. The south–central WGR underwent regional eclogite facies metamorphism 415–400 Ma ago when Baltica subducted beneath Laurentia, during the Scandian orogeny. Eclogites in the WGR group into two traditional types: (1) Precambrian mafic intrusions metamorphosed in situ during Scandian continental subduction and (2) eclogites, garnet peridotites and garnet pyroxenites within ultramafic complexes derived from the subcontinental mantle beneath Laurentia. We document, using field relations, petrography, whole-rock geochemistry and secondary ion mass spectrometry (SIMS) zircon geochronology, a hitherto unrecognized third type of eclogite in the WGR that places new constraints on its tectonic architecture: an eclogitized fragment of oceanic crust from the Iapetus Ocean. The Kråkfjord eclogite complex is a km<sup>2</sup>-sized body with an interior consisting of kyanite eclogite (meta-troctolite) and subordinate layers and lenses of garnet peridotite, garnet websterite and kyanite–garnet leucotonalite. This interior is capped by Fe–Ti-rich eclogite, which locally contains subordinate pockets of migmatitic aluminous gneiss. The elemental abundances and isotopic compositions of the Fe–Ti-rich eclogites resemble those of mid-ocean ridge basalt (MORB). In contrast, the interior kyanite eclogites, peridotites and pyroxenites have compositions similar to the gabbroic cumulates in the lower oceanic crust of slow-spreading ridges. U–Pb SIMS dating of igneous zircon cores from a leucotonalite pod in the interior of the Kråkfjord complex yields Cambro-Ordovician igneous ages of 500–440 Ma, with the ~500 Ma age interpreted as the isotopically undisturbed age. This age matches those of Iapetan oceanic rocks exposed elsewhere in the mountain belt. Metamorphic zircon from an Fe–Ti-rich eclogite in the carapace of the Kråkfjord complex dates the eclogite facies metamorphism at 421.9 ± 2.2 Ma, synchronous with the continental collision. Zircon from a leucosome in Fe–Ti-rich retro-eclogite indicates an age of 408.5 ± 2 Ma for the crystallization of partial melt following the decompression. Detrital zircon core ages from a pocket of aluminous migmatitic gneiss in the carapace indicate derivation of sediment from the Baltic crust. Collectively, the data show that the eclogite complex (1) originated at an Iapetus spreading centre near the continent Baltica, (2) subducted to eclogite conditions during Scandian continental collision and (3) was tectonically intercalated with the Precambrian Baltica basement of the WGR.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 3","pages":"319-354"},"PeriodicalIF":3.4,"publicationDate":"2024-01-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12757","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139496096","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Alexandre Peillod, Clifford G. C. Patten, Kirsten Drüppel, Aratz Beranoaguirre, Armin Zeh, Dominik Gudelius, Simon Hector, Jarosław Majka, Barbara I. Kleine-Marshall, Andreas Karlson, Axel Gerdes, Jochen Kolb
Reconstructing the original geometry of a high-pressure tectonic unit is challenging but important to understand the mechanisms of mountain building. While a single nappe is subducted and exhumed, nappe-internal thrusts may disrupt it into several subunits. The Middle-CBU nappe of the Cycladic Blueschist Unit (Hellenide subduction orogen, Greece) shows evidence of such disruption along a Trans-Cycladic-Thrust (TCT), however, the timing of this thrusting is unknown. Here, we report multi-petrological and geochronological data from the Middle-CBU nappe from the Thera and Ios islands (Greece). Using Zr-in-rutile thermometry coupled with quartz-in-garnet elastic barometry, average P–T and phase equilibrium thermodynamic modelling, we show that garnet growth in Ios occurred during prograde metamorphism at 6.7 ± 1.4 kbar to 13.0 ± 1.6 kbar and 326 ± 20°C to 506 ± 13°C (2σ uncertainty) followed by early exhumation to 10.1 ± 0.6 kbar and 484 ± 14°C and a greenschist facies overprint at 5.7 ± 1.2 kbar and 416 ± 14°C. For Thera, we constrain peak HP conditions of 7.6 ± 1.8 kbar and 331 ± 18°C, followed by exhumation and equilibration at ~2 kbar and ~275°C using average P–T and phase equilibrium thermodynamic modelling. For Ios, Uranium-Pb garnet geochronology provides ages of 55.7 ± 5.0 Ma (2σ uncertainties) for prograde and 40.1 ± 1.4 Ma for peak HP metamorphism. Combining our new P–T–t data from Thera and Ios islands with existing data from Naxos island, we conclude that the studied nappe segments represent remnants of a former coherent nappe. The P–T–t data define an Eocene subduction rate of 2.1 ± 1.0 km/Ma, which is distinctly slower than the current subduction rate of 40–45 km/Ma. After subduction, the exhumation of the Middle-CBU nappe occurred during the Oligocene at different rates for different localities. The Middle-CBU nappe of Naxos was exhumed at a rate of ~6 km/Ma, contrasting with the exhumation rate of ~3 km/Ma calculated for Ios. This result suggests that the Middle-CBU nappe of Naxos rocks was thrust on the Ios one during the Oligocene. Using P–T–t data and assuming realistic subduction angles during the Eocene and the Oligocene, we present a 2D structural reconstruction of the Middle-CBU nappe of these islands. This reconstruction helps to understand the mechanisms of subduction of a continental margin and its disruption during exhumation.
重建高压构造单元的原始几何形状具有挑战性,但对于了解造山机制非常重要。虽然一个单一的岩层经过俯冲和隆起,但岩层内部的推力可能会将其破坏成几个子单元。基克拉泽斯蓝晶岩单元(希腊海伦内德俯冲造山带)的中基克拉泽斯蓝晶岩岩脉显示了沿跨基克拉泽斯推力(TCT)发生这种破坏的证据,但是,这种推力发生的时间尚不清楚。在此,我们报告了来自希腊泰拉岛和伊奥斯岛的中CBU岩层的多岩石学和地质年代学数据。通过使用Zr-in-rutile热量测定法、石英-in-石榴石弹性气压测定法、平均P-T和相平衡热力学建模,我们表明伊奥斯岛的石榴石生长发生在6.7 ± 1.4千巴至13.0±1.6千巴、326±20°C至506±13°C(不确定性为2σ),随后是早期掘起至10.1±0.6千巴和484±14°C,以及5.7±1.2千巴和416±14°C的绿泥石面叠加。对于Thera,我们利用平均P-T和相平衡热力学建模,将峰值HP条件约束在7.6 ± 1.8千巴和331 ± 18°C,然后在~2千巴和~275°C进行出露和平衡。对于 Ios,铀铅石榴石地质年代学提供了 55.7 ± 5.0 Ma 的顺行年龄(不确定性为 2σ)和 40.1 ± 1.4 Ma 的峰值 HP 变质作用年龄。结合特雷拉岛和伊奥斯岛的新 P-T-t 数据以及纳克索斯岛的现有数据,我们得出结论,所研究的岩层片段代表了以前连贯岩层的残余。P-T-t数据确定始新世的俯冲速率为2.1 ± 1.0 km/Ma,明显慢于目前40-45 km/Ma的俯冲速率。在俯冲作用之后,中CBU岩浆岩在渐新世以不同的速度在不同的地方发生了隆起。纳克索斯的中-CBU岩层以大约6 km/Ma的速度被掘出,与伊奥斯计算出的大约3 km/Ma的掘出速度形成鲜明对比。这一结果表明,在渐新世时期,纳克索斯岩石的中CBU岩层被推到了伊奥斯岩层上。利用P-T-t数据,并假设始新世和渐新世期间的俯冲角度符合实际情况,我们提出了这些岛屿的中CBU岩层的二维结构重建。这种重建有助于理解大陆边缘的俯冲机制及其在掘起过程中的破坏。
{"title":"Disruption of a high-pressure unit during exhumation: Example of the Cycladic Blueschist unit (Thera, Ios and Naxos islands, Greece)","authors":"Alexandre Peillod, Clifford G. C. Patten, Kirsten Drüppel, Aratz Beranoaguirre, Armin Zeh, Dominik Gudelius, Simon Hector, Jarosław Majka, Barbara I. Kleine-Marshall, Andreas Karlson, Axel Gerdes, Jochen Kolb","doi":"10.1111/jmg.12753","DOIUrl":"10.1111/jmg.12753","url":null,"abstract":"<p>Reconstructing the original geometry of a high-pressure tectonic unit is challenging but important to understand the mechanisms of mountain building. While a single nappe is subducted and exhumed, nappe-internal thrusts may disrupt it into several subunits. The Middle-CBU nappe of the Cycladic Blueschist Unit (Hellenide subduction orogen, Greece) shows evidence of such disruption along a Trans-Cycladic-Thrust (TCT), however, the timing of this thrusting is unknown. Here, we report multi-petrological and geochronological data from the Middle-CBU nappe from the Thera and Ios islands (Greece). Using Zr-in-rutile thermometry coupled with quartz-in-garnet elastic barometry, average P–T and phase equilibrium thermodynamic modelling, we show that garnet growth in Ios occurred during prograde metamorphism at 6.7 ± 1.4 kbar to 13.0 ± 1.6 kbar and 326 ± 20°C to 506 ± 13°C (2σ uncertainty) followed by early exhumation to 10.1 ± 0.6 kbar and 484 ± 14°C and a greenschist facies overprint at 5.7 ± 1.2 kbar and 416 ± 14°C. For Thera, we constrain peak HP conditions of 7.6 ± 1.8 kbar and 331 ± 18°C, followed by exhumation and equilibration at ~2 kbar and ~275°C using average P–T and phase equilibrium thermodynamic modelling. For Ios, Uranium-Pb garnet geochronology provides ages of 55.7 ± 5.0 Ma (2σ uncertainties) for prograde and 40.1 ± 1.4 Ma for peak HP metamorphism. Combining our new P–T–t data from Thera and Ios islands with existing data from Naxos island, we conclude that the studied nappe segments represent remnants of a former coherent nappe. The P–T–t data define an Eocene subduction rate of 2.1 ± 1.0 km/Ma, which is distinctly slower than the current subduction rate of 40–45 km/Ma. After subduction, the exhumation of the Middle-CBU nappe occurred during the Oligocene at different rates for different localities. The Middle-CBU nappe of Naxos was exhumed at a rate of ~6 km/Ma, contrasting with the exhumation rate of ~3 km/Ma calculated for Ios. This result suggests that the Middle-CBU nappe of Naxos rocks was thrust on the Ios one during the Oligocene. Using P–T–t data and assuming realistic subduction angles during the Eocene and the Oligocene, we present a 2D structural reconstruction of the Middle-CBU nappe of these islands. This reconstruction helps to understand the mechanisms of subduction of a continental margin and its disruption during exhumation.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 2","pages":"225-255"},"PeriodicalIF":3.4,"publicationDate":"2023-12-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12753","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138949346","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Samantha March, Martin Hand, Laura Morrissey, David Kelsey
U–Pb zircon and monazite geochronology are considered to be among the most efficient and reliable methods for constraining the timing of high-temperature (HT) metamorphic events. However, the reliability of these chronometers is coupled to their ability to participate in reactions. A case study examining the responsiveness of zircon and monazite has been conducted using granulite facies metapelitic and metamafic lithologies in the Warumpi Province, central Australia. In some instances, metapelitic granulites from this locality are polymetamorphic, with an early M1 assemblage containing orthopyroxene, cordierite, biotite, quartz, ilmenite and magnetite, and an M2 assemblage represented by garnet, sillimanite, orthopyroxene, cordierite, biotite, sapphirine, ilmenite and magnetite. M2 metamorphism is linked to HT peak conditions of 8–10 kbar and 850–915°C. Detrital and metamorphic zircon and monazite from these rocks dominantly record U–Pb dates of 1670–1610 Ma and have trace element compositions suggesting they grew prior to peak M2 garnet in the rock. Lu–Hf geochronology from M2 garnet gives ages of c. 1150 Ma. Zircon and monazite are therefore suggested to have remained largely inert during HT metamorphism. We attribute the relatively minor response of zircon and monazite during high-temperature Mesoproterozoic metamorphism to the localized development of refractory bulk compositions at c. 1630 Ma during M1 metamorphism. This created refractory Mg–Al-rich bulk compositions that were unable to undergo significant partial melting, despite experiencing subsequent temperatures of ~900°C at c. 1150 Ma. In contrast, metapelitic and metamafic rocks in the area that did not develop refractory bulk compositions during M1 metamorphism were able to partially melt and record c. 1150 Ma accessory mineral U–Pb ages. These results contribute to a small, but growing number of case studies investigating the systematics of the U–Pb system in zircon and monazite in polymetamorphic HT terranes and their apparent resistance to isotopic resetting. Where disequilibrium is apparent, garnet Lu–Hf geochronology can form an important tool to interrogate the significance of accessory U–Pb ages. In the Warumpi Province in central Australia, c. 1640 Ma zircon U–Pb ages had previously been interpreted to reflect the formation of HT garnet-bearing granulites during a collisional event. Instead, the garnet-bearing assemblages formed at c. 1150 Ma during the Mesoproterozoic, calling into question the existence of a late Palaeoproterozoic collisional system in central Australia.
{"title":"The inhibited response of accessory minerals during high-temperature reworking","authors":"Samantha March, Martin Hand, Laura Morrissey, David Kelsey","doi":"10.1111/jmg.12754","DOIUrl":"10.1111/jmg.12754","url":null,"abstract":"<p>U–Pb zircon and monazite geochronology are considered to be among the most efficient and reliable methods for constraining the timing of high-temperature (<i>HT</i>) metamorphic events. However, the reliability of these chronometers is coupled to their ability to participate in reactions. A case study examining the responsiveness of zircon and monazite has been conducted using granulite facies metapelitic and metamafic lithologies in the Warumpi Province, central Australia. In some instances, metapelitic granulites from this locality are polymetamorphic, with an early M1 assemblage containing orthopyroxene, cordierite, biotite, quartz, ilmenite and magnetite, and an M2 assemblage represented by garnet, sillimanite, orthopyroxene, cordierite, biotite, sapphirine, ilmenite and magnetite. M2 metamorphism is linked to <i>HT</i> peak conditions of 8–10 kbar and 850–915°C. Detrital and metamorphic zircon and monazite from these rocks dominantly record U–Pb dates of 1670–1610 Ma and have trace element compositions suggesting they grew prior to peak M2 garnet in the rock. Lu–Hf geochronology from M2 garnet gives ages of c. 1150 Ma. Zircon and monazite are therefore suggested to have remained largely inert during <i>HT</i> metamorphism. We attribute the relatively minor response of zircon and monazite during high-temperature Mesoproterozoic metamorphism to the localized development of refractory bulk compositions at c. 1630 Ma during M1 metamorphism. This created refractory Mg–Al-rich bulk compositions that were unable to undergo significant partial melting, despite experiencing subsequent temperatures of ~900°C at c. 1150 Ma. In contrast, metapelitic and metamafic rocks in the area that did not develop refractory bulk compositions during M1 metamorphism were able to partially melt and record c. 1150 Ma accessory mineral U–Pb ages. These results contribute to a small, but growing number of case studies investigating the systematics of the U–Pb system in zircon and monazite in polymetamorphic <i>HT</i> terranes and their apparent resistance to isotopic resetting. Where disequilibrium is apparent, garnet Lu–Hf geochronology can form an important tool to interrogate the significance of accessory U–Pb ages. In the Warumpi Province in central Australia, c. 1640 Ma zircon U–Pb ages had previously been interpreted to reflect the formation of <i>HT</i> garnet-bearing granulites during a collisional event. Instead, the garnet-bearing assemblages formed at c. 1150 Ma during the Mesoproterozoic, calling into question the existence of a late Palaeoproterozoic collisional system in central Australia.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 2","pages":"257-289"},"PeriodicalIF":3.4,"publicationDate":"2023-12-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12754","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138949232","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Carson Kinney, Jillian Kendrick, Manuel Duguet, Chris Yakymchuk
Heat generated from the decay of K, Th, and U plays a fundamental role in the differentiation and stabilization of Earth's continental crust. This is particularly important in the construction of Archean cratons that form the nuclei of Earth's continents. The Kapuskasing uplift is a rare exposure of an Archean-age crustal cross-section that provides a snapshot of crustal melting, differentiation, and compositional stratification. We integrate field observations, whole-rock compositions, thermodynamic equilibrium and accessory mineral modelling with heat production and latency time modelling to provide insights into the partitioning of heat-producing elements between residue and melt during anatexis of metabasites as well as the resulting effects on metamorphic timescales and the production of tonalite–trondhjemite–granodiorite (TTG) suites. We model six metabasite compositions ranging from relatively fertile greenschist facies metabasites to melt-depleted residual mafic (upper-)amphibolites to granulites. Heat-producing elements are modelled to be partitioned between melt and residue; the dominant minerals in the residue that host these elements are apatite, hornblende, K-feldspar, and epidote. At 800–850°C epidote is no longer stable, and the melt fraction is predicted to contain roughly half of the heat production capacity for the system. Apatite and melt are expected to be the dominant repositories for Th and U during anatexis; zircon is predicted to be completely consumed by 850°C, whereas apatite persists to higher temperatures and allanite is expected only in minor modal abundances at high-P, low-T conditions. The partitioning of heat-producing elements into relatively low-density melt decreases the heat production of the residual system during anatexis. Due to their high density and affinity for U and Th, epidote and apatite retain heat production capacity in the residue during metabasite melting. Thermal latency modelling of metamorphism suggests that enriched metabasite compositions require 38–46 My to increase the temperature from ~650 to 850°C (solidus temperature to peak metamorphic temperature of the Kapuskasing uplift), whereas estimates are considerably shorter for depleted compositions (7–25 My). Four of the six samples modelled require 60–70 My to reach 1000°C from the solidus. Our modelling of heat-producing element partitioning and predicted proportions of melt suggest that enriched basaltic compositions are the most reasonable source of TTG magmas and our heating time modelling indicates the mantle as an equal to dominant source of heat for metabasite anatexis compared with radiogenic heat production.
钾、钍和铀衰变产生的热量在地球大陆地壳的分化和稳定过程中起着根本性的作用。这对于形成地球大陆核心的阿新世陨石坑的构造尤为重要。卡普斯卡辛隆起是阿基坦时代地壳横截面的罕见露头,提供了地壳熔化、分化和成分分层的快照。我们将野外观测、全岩成分、热力学平衡和附属矿物建模与产热和潜伏时间建模结合起来,深入研究了在偏闪长岩的安山过程中,产热元素在残余物和熔体之间的分配,以及由此对变质时间尺度和碳酸盐岩-特长闪长岩-花岗闪长岩(TTG)岩套的生成所产生的影响。我们模拟了六种偏闪长岩成分,从相对肥沃的绿辉石面偏闪长岩到熔体贫化的残余黑云母(上)闪长岩再到花岗岩。产热元素被模拟为在熔体和残余物之间分配;残余物中容纳这些元素的主要矿物是磷灰石、角闪石、K长石和闪长岩。在摄氏 800-850 度时,表土不再稳定,预计熔体部分将包含该系统大约一半的产热能力。预计磷灰石和熔体将成为安山期 Th 和 U 的主要储存地;预计锆石在 850°C 时将被完全消耗,而磷灰石将持续到更高的温度,预计在高 P、低 T 条件下,阳起石仅以较小的模态丰度存在。产热元素被分割到密度相对较低的熔体中,降低了残余体系在安氏过程中的产热量。由于表土和磷灰石的高密度和对铀和钍的亲和性,它们在偏闪石熔融过程中保留了残余物的产热能力。变质作用的热潜伏期模拟表明,富集偏闪长岩成分需要38-46 My才能将温度从大约650°C提高到850°C(卡普斯卡辛隆起的固结温度到变质峰值温度),而贫化成分的估计值要短得多(7-25 My)。在模拟的六个样品中,有四个需要 60-70 My 才能从固结温度达到 1000°C。我们的产热元素分配模型和预测的熔体比例表明,富集玄武岩成分是TTG岩浆最合理的来源,我们的加热时间模型表明,与放射源产热相比,地幔是变质岩厌氧作用的同等或主要热源。
{"title":"Redistribution of heat-producing elements during melting of Archean crust","authors":"Carson Kinney, Jillian Kendrick, Manuel Duguet, Chris Yakymchuk","doi":"10.1111/jmg.12751","DOIUrl":"10.1111/jmg.12751","url":null,"abstract":"<p>Heat generated from the decay of K, Th, and U plays a fundamental role in the differentiation and stabilization of Earth's continental crust. This is particularly important in the construction of Archean cratons that form the nuclei of Earth's continents. The Kapuskasing uplift is a rare exposure of an Archean-age crustal cross-section that provides a snapshot of crustal melting, differentiation, and compositional stratification. We integrate field observations, whole-rock compositions, thermodynamic equilibrium and accessory mineral modelling with heat production and latency time modelling to provide insights into the partitioning of heat-producing elements between residue and melt during anatexis of metabasites as well as the resulting effects on metamorphic timescales and the production of tonalite–trondhjemite–granodiorite (TTG) suites. We model six metabasite compositions ranging from relatively fertile greenschist facies metabasites to melt-depleted residual mafic (upper-)amphibolites to granulites. Heat-producing elements are modelled to be partitioned between melt and residue; the dominant minerals in the residue that host these elements are apatite, hornblende, K-feldspar, and epidote. At 800–850°C epidote is no longer stable, and the melt fraction is predicted to contain roughly half of the heat production capacity for the system. Apatite and melt are expected to be the dominant repositories for Th and U during anatexis; zircon is predicted to be completely consumed by 850°C, whereas apatite persists to higher temperatures and allanite is expected only in minor modal abundances at high-P, low-T conditions. The partitioning of heat-producing elements into relatively low-density melt decreases the heat production of the residual system during anatexis. Due to their high density and affinity for U and Th, epidote and apatite retain heat production capacity in the residue during metabasite melting. Thermal latency modelling of metamorphism suggests that enriched metabasite compositions require 38–46 My to increase the temperature from ~650 to 850°C (solidus temperature to peak metamorphic temperature of the Kapuskasing uplift), whereas estimates are considerably shorter for depleted compositions (7–25 My). Four of the six samples modelled require 60–70 My to reach 1000°C from the solidus. Our modelling of heat-producing element partitioning and predicted proportions of melt suggest that enriched basaltic compositions are the most reasonable source of TTG magmas and our heating time modelling indicates the mantle as an equal to dominant source of heat for metabasite anatexis compared with radiogenic heat production.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 2","pages":"197-224"},"PeriodicalIF":3.4,"publicationDate":"2023-12-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12751","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138573731","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Sara Nerone, Alessandro Petroccia, Fabiola Caso, Davide Dana, Andrea Maffeis
Metamorphic reactions are commonly driven to completion within shear zones thanks to fluid circulation, making the re-equilibration of the mineral assemblage one of the dominant processes. Despite the important role of H2O in such processes, forward thermodynamic modelling calculations commonly assume either H2O-saturated conditions or only fluid loss during prograde evolution to peak conditions. These assumptions influence the understanding of shear zones during the retrograde evolution. Here, we investigate the P–T–MH2O retrograde evolution of the Mt. Bracco Shear Zone (MBSZ), an Alpine ductile tectonic contact which marks the boundary between two HP units in the Dora-Maira Massif (Western Alps, Italy). After the eclogite-facies peak (at 500–520°C and 1.8–2.2 GPa), the subsequent mylonitic event is constrained at amphibolite-facies conditions, continuing its evolution at decreasing pressure and temperature during rock exhumation, from ~590°C, 1.0 GPa down to ~520°C, 0.7 GPa. The P/T–MH2O forward modelling highlights different behaviour for the two analysed samples. After reaching a minimum H2O content at the transition from eclogite- to amphibolite-facies conditions, a significant fluid gain is modelled for only one of the two analysed samples just before the mylonitic event. The MBSZ then evolves towards H2O-undersaturated conditions. This work thus underlines the necessity of investigating the H2O evolution within shear zones, as the H2O content is susceptible to change through the P–T path, due to dehydration reactions or fluid infiltration events. Furthermore, lithological heterogeneities influence possible different fluid circulation regimes in shear zones, resulting in externally or internally derived fluid gain.
{"title":"Assessing the importance of H2O content in the tectono-metamorphic evolution of shear zones: A case study from the Dora-Maira Massif (Western Alps)","authors":"Sara Nerone, Alessandro Petroccia, Fabiola Caso, Davide Dana, Andrea Maffeis","doi":"10.1111/jmg.12750","DOIUrl":"10.1111/jmg.12750","url":null,"abstract":"<p>Metamorphic reactions are commonly driven to completion within shear zones thanks to fluid circulation, making the re-equilibration of the mineral assemblage one of the dominant processes. Despite the important role of H<sub>2</sub>O in such processes, forward thermodynamic modelling calculations commonly assume either H<sub>2</sub>O-saturated conditions or only fluid loss during prograde evolution to peak conditions. These assumptions influence the understanding of shear zones during the retrograde evolution. Here, we investigate the <i>P–T–M</i>H<sub>2</sub>O retrograde evolution of the Mt. Bracco Shear Zone (MBSZ), an Alpine ductile tectonic contact which marks the boundary between two H<i>P</i> units in the Dora-Maira Massif (Western Alps, Italy). After the eclogite-facies peak (at 500–520°C and 1.8–2.2 GPa), the subsequent mylonitic event is constrained at amphibolite-facies conditions, continuing its evolution at decreasing pressure and temperature during rock exhumation, from ~590°C, 1.0 GPa down to ~520°C, 0.7 GPa. The <i>P</i>/<i>T</i>–<i>M</i>H<sub>2</sub>O forward modelling highlights different behaviour for the two analysed samples. After reaching a minimum H<sub>2</sub>O content at the transition from eclogite- to amphibolite-facies conditions, a significant fluid gain is modelled for only one of the two analysed samples just before the mylonitic event. The MBSZ then evolves towards H<sub>2</sub>O-undersaturated conditions. This work thus underlines the necessity of investigating the H<sub>2</sub>O evolution within shear zones, as the H<sub>2</sub>O content is susceptible to change through the <i>P–T</i> path, due to dehydration reactions or fluid infiltration events. Furthermore, lithological heterogeneities influence possible different fluid circulation regimes in shear zones, resulting in externally or internally derived fluid gain.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 2","pages":"171-196"},"PeriodicalIF":3.4,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12750","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138515091","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Anastasia O. Mikhno, Anton F. Shatskiy, Andrey V. Korsakov, Yulia G. Vinogradova, Jasper Berndt, Stephan Klemme, Sergey V. Rashchenko
Understanding calcite genesis in ultrahigh-pressure crustal rocks is a key to the reconstruction of the evolution of ultrahigh-pressure metacarbonate rocks. Here, we present new data and a new model on the genesis and the P–T conditions of the formation of calcite found in the ultrahigh-pressure calc-silicate rocks from the Kokchetav massif. In the studied sample aragonite inclusions coexist with Type A calcite inclusions (previously interpreted as mineral inclusions) and the inclusions of Type B calcite (previously interpreted as derived from the crystallization of carbonatitic melt) in cores of garnet porphyroblasts. The most Mg-rich calcite from Type A inclusions coexisting with aragonite inclusions in one garnet growth zone shows XCa = 0.935 implying their crystallization during a retrograde metamorphic stage at P ~ 2.3 GPa and T ~ 870°C along the P–T path. Type A calcite and aragonite inclusions were also found coexisting in one growth zone with K-bearing clinopyroxene inclusion (ω[K2O] = 0.5 wt.%). Such a high K2O-content in clinopyroxene testify that the pressure of inclusion capture exceeded 3.5 GPa, which contradicts the P–T conditions estimated by XCa in magnesian calcite. Thus, Type A calcite inclusions were initially captured as an aggregate of aragonite+ magnesian calcite at ultrahigh pressure metamorphic stage (P ≥ 3.5 GPa, T = 900–1,000°C) and then re-equilibrated at lower conditions (P ≤ 2.3 GPa and T ≤ 870°C). The trace element composition of aragonite and Type A and Type B calcite from inclusions was also studied to clarify calcite genesis in these inclusions. Aragonite shows high LREE (5–57 ppm) and Sr-content (600–800 ppm). Calcite from Type A inclusions shows low LREE (2.9–19.8 ppm) and Sr-content (490–670 ppm). Calcite from Type B inclusions forms two groups according to the LREE and Sr content distribution (Type B1 and Type B2). Trace element distribution in Type B1 calcite is identical to that of Type A calcite, while Type B2 calcite shows high LREE (6.8–64.9 ppm) concentrations along with low Sr-content (180–340 ppm). Type A and Type B1 calcite is interpreted to have been re-equilibrated. Type B2 calcite inclusions crystallized from the hydrous carbonatitic melt.
了解超高压地壳岩石中方解石的成因是重建超高压偏碳酸盐岩演化的关键。在这里,我们展示了关于来自科克切塔夫丘陵的超高压钙硅酸盐岩中方解石形成的成因和P-T条件的新数据和新模型。在所研究的样本中,文石包裹体与石榴石斑岩岩芯中的 A 型方解石包裹体(以前被解释为矿物包裹体)和 B 型方解石包裹体(以前被解释为碳酸盐岩熔体结晶)共存。在一个石榴石生长带中与文石包裹体共存的 A 型包裹体中镁含量最高的方解石显示 XCa = 0.935,这意味着它们是在 P ~ 2.3 GPa 和 T ~ 870°C 的逆变质阶段沿 P-T 路径结晶的。在一个生长带中还发现了A型方解石和文石包裹体与含K的挛辉石包裹体(ω[K2O] = 0.5 wt.%)共存。霞石中如此高的 K2O 含量证明包裹体的捕获压力超过了 3.5 GPa,这与镁方解石中 XCa 估算的 P-T 条件相矛盾。因此,A 型方解石包裹体最初是在超高压变质阶段(P ≥ 3.5 GPa,T = 900-1,000°C)作为文石+菱镁方解石的集合体被捕获的,然后在较低的条件下(P ≤ 2.3 GPa,T ≤ 870°C)重新平衡。为了弄清包裹体中方解石的成因,还研究了包裹体中文石以及 A 型和 B 型方解石的微量元素组成。文石显示出较高的 LREE(5-57 ppm)和 Sr-含量(600-800 ppm)。A 型包裹体中的方解石显示出较低的 LREE(2.9-19.8 ppm)和 Sr-含量(490-670 ppm)。根据 LREE 和 Sr 含量的分布,B 型包裹体中的方解石分为两组(B1 型和 B2 型)。B1 型方解石的微量元素分布与 A 型方解石相同,而 B2 型方解石的 LREE 含量高(6.8-64.9 ppm),Sr 含量低(180-340 ppm)。据解释,A 型和 B1 型方解石已经过再钙化。B2型方解石包裹体由含水碳酸盐岩熔体结晶而成。
{"title":"The origin of calcite in calc-silicate rocks from the Kokchetav ultrahigh-pressure metamorphic complex","authors":"Anastasia O. Mikhno, Anton F. Shatskiy, Andrey V. Korsakov, Yulia G. Vinogradova, Jasper Berndt, Stephan Klemme, Sergey V. Rashchenko","doi":"10.1111/jmg.12749","DOIUrl":"10.1111/jmg.12749","url":null,"abstract":"<p>Understanding calcite genesis in ultrahigh-pressure crustal rocks is a key to the reconstruction of the evolution of ultrahigh-pressure metacarbonate rocks. Here, we present new data and a new model on the genesis and the <i>P–T</i> conditions of the formation of calcite found in the ultrahigh-pressure calc-silicate rocks from the Kokchetav massif. In the studied sample aragonite inclusions coexist with Type A calcite inclusions (previously interpreted as mineral inclusions) and the inclusions of Type B calcite (previously interpreted as derived from the crystallization of carbonatitic melt) in cores of garnet porphyroblasts. The most Mg-rich calcite from Type A inclusions coexisting with aragonite inclusions in one garnet growth zone shows X<sub>Ca</sub> = 0.935 implying their crystallization during a retrograde metamorphic stage at <i>P</i> ~ 2.3 GPa and <i>T</i> ~ 870°C along the <i>P–T</i> path. Type A calcite and aragonite inclusions were also found coexisting in one growth zone with K-bearing clinopyroxene inclusion (ω[K<sub>2</sub>O] = 0.5 wt.%). Such a high K<sub>2</sub>O-content in clinopyroxene testify that the pressure of inclusion capture exceeded 3.5 GPa, which contradicts the <i>P–T</i> conditions estimated by X<sub>Ca</sub> in magnesian calcite. Thus, Type A calcite inclusions were initially captured as an aggregate of aragonite+ magnesian calcite at ultrahigh pressure metamorphic stage (<i>P</i> ≥ 3.5 GPa, <i>T</i> = 900–1,000°C) and then re-equilibrated at lower conditions (<i>P</i> ≤ 2.3 GPa and <i>T</i> ≤ 870°C). The trace element composition of aragonite and Type A and Type B calcite from inclusions was also studied to clarify calcite genesis in these inclusions. Aragonite shows high LREE (5–57 ppm) and Sr-content (600–800 ppm). Calcite from Type A inclusions shows low LREE (2.9–19.8 ppm) and Sr-content (490–670 ppm). Calcite from Type B inclusions forms two groups according to the LREE and Sr content distribution (Type B1 and Type B2). Trace element distribution in Type B1 calcite is identical to that of Type A calcite, while Type B2 calcite shows high LREE (6.8–64.9 ppm) concentrations along with low Sr-content (180–340 ppm). Type A and Type B1 calcite is interpreted to have been re-equilibrated. Type B2 calcite inclusions crystallized from the hydrous carbonatitic melt.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 2","pages":"143-170"},"PeriodicalIF":3.4,"publicationDate":"2023-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"135272098","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
David Hernández-Uribe, Robert M. Holder, Juan D. Hernández-Montenegro
<p>Eclogite thermobarometry is crucial for constraining the depths and temperatures to which oceanic and continental crust subduct. However, obtaining the pressure and temperature (<i>P–T</i>) conditions of eclogites is complex as they commonly display high-variance mineral assemblages, and the mineral compositions only vary slightly with <i>P–T</i>. In this contribution, we present a comparison between two independent and commonly used thermobarometric approaches for eclogites: conventional thermobarometry and forward phase-equilibrium modelling. We assess how consistent the thermobarometric calculations are using the garnet–clinopyroxene–phengite barometer and garnet–clinopyroxene thermometer with predictions from forward modelling (i.e. comparing the relative differences between approaches). Our results show that the overall mismatch in methods is typically ±0.2–0.3 GPa and ±29–42°C although differences as large as 80°C and 0.7 GPa are possible for a few narrow ranges of <i>P–T</i> conditions in the forward models. Such mismatch is interpreted as the relative differences among methods, and not as absolute uncertainties or accuracies for either method. For most of the investigated <i>P–T</i> conditions, the relatively minor differences between methods means that the choice in thermobarometric method itself is less important for geological interpretation than careful sample characterization and petrographic interpretation for deriving <i>P–T</i> from eclogites. Although thermobarometry is known to be sensitive to the assumed <i>X</i><sub>Fe</sub><sup>3+</sup> of a rock (or mineral), the <i>relative</i> differences between methods are not particularly sensitive to the choice of bulk-rock <i>X</i><sub>Fe</sub><sup>3+</sup>, except at high temperatures (>650°C, amphibole absent) and for very large differences in assumed <i>X</i><sub>Fe</sub><sup>3+</sup> (0–0.5). We find that the most important difference between approaches is the activity–composition (<i>a–x</i>) relations, as opposed to the end-member thermodynamic data or other aspects of experimental calibration. When equivalent <i>a–x</i> relations are used in the conventional barometer, <i>P</i> calculations are nearly identical to phase-equilibrium models (Δ<i>P</i> < 0.1). To further assess the implications of these results for real rocks, we also evaluate common mathematical optimizations of reaction constants used for obtaining the maximum <i>P–T</i> with conventional thermobarometric approaches (e.g. using the highest <i>a</i>Grs<sup>2</sup> × <i>a</i>Prp in garnet and Si content in phengite, and the lowest <i>a</i>Di in clinopyroxene). These approaches should be used with caution, because they may not represent the compositions of equilibrium mineral assemblages at eclogite facies conditions and therefore systematically bias <i>P–T</i> calculations. Assuming method accuracy, geological meaningful <i>P</i><sub>max</sub> at a typical eclogite facies temperature of ~660°C will be obtained
{"title":"Eclogite thermobarometry: The consistency between conventional thermobarometry and forward phase-equilibrium modelling","authors":"David Hernández-Uribe, Robert M. Holder, Juan D. Hernández-Montenegro","doi":"10.1111/jmg.12747","DOIUrl":"10.1111/jmg.12747","url":null,"abstract":"<p>Eclogite thermobarometry is crucial for constraining the depths and temperatures to which oceanic and continental crust subduct. However, obtaining the pressure and temperature (<i>P–T</i>) conditions of eclogites is complex as they commonly display high-variance mineral assemblages, and the mineral compositions only vary slightly with <i>P–T</i>. In this contribution, we present a comparison between two independent and commonly used thermobarometric approaches for eclogites: conventional thermobarometry and forward phase-equilibrium modelling. We assess how consistent the thermobarometric calculations are using the garnet–clinopyroxene–phengite barometer and garnet–clinopyroxene thermometer with predictions from forward modelling (i.e. comparing the relative differences between approaches). Our results show that the overall mismatch in methods is typically ±0.2–0.3 GPa and ±29–42°C although differences as large as 80°C and 0.7 GPa are possible for a few narrow ranges of <i>P–T</i> conditions in the forward models. Such mismatch is interpreted as the relative differences among methods, and not as absolute uncertainties or accuracies for either method. For most of the investigated <i>P–T</i> conditions, the relatively minor differences between methods means that the choice in thermobarometric method itself is less important for geological interpretation than careful sample characterization and petrographic interpretation for deriving <i>P–T</i> from eclogites. Although thermobarometry is known to be sensitive to the assumed <i>X</i><sub>Fe</sub><sup>3+</sup> of a rock (or mineral), the <i>relative</i> differences between methods are not particularly sensitive to the choice of bulk-rock <i>X</i><sub>Fe</sub><sup>3+</sup>, except at high temperatures (>650°C, amphibole absent) and for very large differences in assumed <i>X</i><sub>Fe</sub><sup>3+</sup> (0–0.5). We find that the most important difference between approaches is the activity–composition (<i>a–x</i>) relations, as opposed to the end-member thermodynamic data or other aspects of experimental calibration. When equivalent <i>a–x</i> relations are used in the conventional barometer, <i>P</i> calculations are nearly identical to phase-equilibrium models (Δ<i>P</i> < 0.1). To further assess the implications of these results for real rocks, we also evaluate common mathematical optimizations of reaction constants used for obtaining the maximum <i>P–T</i> with conventional thermobarometric approaches (e.g. using the highest <i>a</i>Grs<sup>2</sup> × <i>a</i>Prp in garnet and Si content in phengite, and the lowest <i>a</i>Di in clinopyroxene). These approaches should be used with caution, because they may not represent the compositions of equilibrium mineral assemblages at eclogite facies conditions and therefore systematically bias <i>P–T</i> calculations. Assuming method accuracy, geological meaningful <i>P</i><sub>max</sub> at a typical eclogite facies temperature of ~660°C will be obtained ","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 1","pages":"89-108"},"PeriodicalIF":3.4,"publicationDate":"2023-10-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12747","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"135779815","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Silvia Volante, Annika Dziggel, Jesse B. Walters, Noreen J. Evans, Maximilian Herbst, Richard Albert Roper
Despite extensive investigation, the tectono-thermal evolution of the Archean crust in the Lewisian Gneiss Complex in NW Scotland (LGC) is debated. Most U–Pb zircon geochronological and metamorphic studies have focused on rocks from the central region of the mainland LGC, where granulite facies assemblages associated with the oldest (Badcallian) tectono-metamorphic event at c. 2.75 Ga are overprinted by younger amphibolite facies assemblages related to the Inverian (c. 2.5 Ga) and subsequent Laxfordian (c. 1.9–1.65 Ga) tectono-thermal events. In the southern and northern regions of the mainland LGC, deformation and metamorphism associated with the Laxfordian event are pervasive, although the timing and conditions are poorly constrained. Here, we present new field, petrographic and structural data, U–Pb zircon and titanite geochronology and phase equilibrium modelling of amphibolite samples from the northern and southern regions. Our field observations show that in both regions, pre-Laxfordian structures are significantly reworked by steep NW-striking fabrics that are themselves pervasively overprinted by co-axial deformation and amphibolite facies metamorphism related to the Laxfordian event. In situ U–Pb titanite geochronology yields Laxfordian ages of 1853 ± 20 Ma in the southern region (P = 6–8 kbar and T = 640–690°C) and 1750 ± 20 Ma and 1776 ± 10 Ma in the northern region (P = 6–7.5 kbar and T = 740–760°C). While U–Pb dating of zircon rims from felsic gneisses in the central region shows a dominant Inverian metamorphic overprint at c. 2500 Ma, zircon rims in felsic gneisses from the northern and southern regions commonly yield Laxfordian dates as young as c. 1800 Ma. Combined, the results support the idea that, during the Palaeoproterozoic, the central region of the LGC acted as low-strain domain, in which intense deformation and metamorphism were restricted to crustal-scale shear zones. By contrast, in the southern and northern regions, early (c. 1.85 Ga) and late (c. 1.75 Ga) Laxfordian deformation and fluid-mediated metamorphism were much more pervasive and at higher P–T conditions than previously proposed. The diachronous Laxfordian evolution of the southern and northern regions indicate that they reflect early and late snapshots of collisional to transpressional tectonics in the mainland LGC. The long-lasting Laxfordian evolution documents the collision of the Rae and North Atlantic cratons during the Palaeoproterozoic amalgamation of the supercontinent Nuna, with implications for the palaeogeographic configuration of NW Scotland during Palaeoproterozoic Nuna.
{"title":"Constraints on the Palaeoproterozoic tectono-metamorphic evolution of the Lewisian Gneiss Complex, NW Scotland: Implications for Nuna assembly","authors":"Silvia Volante, Annika Dziggel, Jesse B. Walters, Noreen J. Evans, Maximilian Herbst, Richard Albert Roper","doi":"10.1111/jmg.12748","DOIUrl":"10.1111/jmg.12748","url":null,"abstract":"<p>Despite extensive investigation, the tectono-thermal evolution of the Archean crust in the Lewisian Gneiss Complex in NW Scotland (LGC) is debated. Most U–Pb zircon geochronological and metamorphic studies have focused on rocks from the central region of the mainland LGC, where granulite facies assemblages associated with the oldest (Badcallian) tectono-metamorphic event at c. 2.75 Ga are overprinted by younger amphibolite facies assemblages related to the Inverian (c. 2.5 Ga) and subsequent Laxfordian (c. 1.9–1.65 Ga) tectono-thermal events. In the southern and northern regions of the mainland LGC, deformation and metamorphism associated with the Laxfordian event are pervasive, although the timing and conditions are poorly constrained. Here, we present new field, petrographic and structural data, U–Pb zircon and titanite geochronology and phase equilibrium modelling of amphibolite samples from the northern and southern regions. Our field observations show that in both regions, pre-Laxfordian structures are significantly reworked by steep NW-striking fabrics that are themselves pervasively overprinted by co-axial deformation and amphibolite facies metamorphism related to the Laxfordian event. In situ U–Pb titanite geochronology yields Laxfordian ages of 1853 ± 20 Ma in the southern region (P = 6–8 kbar and T = 640–690°C) and 1750 ± 20 Ma and 1776 ± 10 Ma in the northern region (P = 6–7.5 kbar and T = 740–760°C). While U–Pb dating of zircon rims from felsic gneisses in the central region shows a dominant Inverian metamorphic overprint at c. 2500 Ma, zircon rims in felsic gneisses from the northern and southern regions commonly yield Laxfordian dates as young as c. 1800 Ma. Combined, the results support the idea that, during the Palaeoproterozoic, the central region of the LGC acted as low-strain domain, in which intense deformation and metamorphism were restricted to crustal-scale shear zones. By contrast, in the southern and northern regions, early (c. 1.85 Ga) and late (c. 1.75 Ga) Laxfordian deformation and fluid-mediated metamorphism were much more pervasive and at higher P–T conditions than previously proposed. The diachronous Laxfordian evolution of the southern and northern regions indicate that they reflect early and late snapshots of collisional to transpressional tectonics in the mainland LGC. The long-lasting Laxfordian evolution documents the collision of the Rae and North Atlantic cratons during the Palaeoproterozoic amalgamation of the supercontinent Nuna, with implications for the palaeogeographic configuration of NW Scotland during Palaeoproterozoic Nuna.</p>","PeriodicalId":16472,"journal":{"name":"Journal of Metamorphic Geology","volume":"42 1","pages":"109-142"},"PeriodicalIF":3.4,"publicationDate":"2023-10-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1111/jmg.12748","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"135779948","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}