ORCID Profile
0000-0003-1200-3826
Current Organisation
Monash University
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Geology | Geochronology And Isotope Geochemistry | Geomagnetism | Isotope Geochemistry | Geochronology | Geophysics | Structural Geology | Geotectonics | Tectonics | Ore Deposit Petrology | Geochemistry | Artificial Intelligence and Image Processing | Earth Sciences Not Elsewhere Classified | Information Systems | Chemical Oceanography | Igneous And Metamorphic Petrology | Petroleum Geology | Geochronology | Ore Deposit Petrology | Extraterrestrial Geology | Data Structures | Software Engineering | Information Systems Organisation | Conservation and Biodiversity | Geology Not Elsewhere Classified | Glaciology | Geochemistry Not Elsewhere Classified | Global Information Systems | Simulation And Modelling | Environmental Science and Management | Geodynamics | Mathematical Sciences Not Elsewhere Classified | Materials Engineering Not Elsewhere Classified | Environmental Sciences Not Elsewhere Classified | Structural Geology | Geophysics Not Elsewhere Classified | Atmospheric Sciences Not Elsewhere Classified |
Earth sciences | Information processing services | Climate change | Expanding Knowledge in the Earth Sciences | Application packages | Energy Exploration not elsewhere classified | Mineral Exploration not elsewhere classified | Estuarine and lagoon areas | Chemical sciences | Physical sciences | Climate variability | Living resources (incl. impacts of fishing on non-target species) | Alumina production | Physical and chemical conditions | Integrated (ecosystem) assessment and management | Oceanic processes (excl. climate related) | Other | Technological and organisational innovation | Oil and gas | Oil and gas | Marine protected areas | Exploration | Living resources (flora and fauna) | Land and water management | Precious (Noble) Metal Ore Exploration | Other
Publisher: Geological Society of London
Date: 2008
DOI: 10.1144/SP294.2
Publisher: Research Square Platform LLC
Date: 21-03-2023
DOI: 10.21203/RS.3.RS-2594860/V1
Abstract: When modern-style plate tectonics commenced on Earth remains one of fundamental questions in unravelling the evolution of our planet, due to the apparent lack of low-thermal gradients in old metamorphic rocks ( 350 °C/GPa)—a key indicator of modern plate subduction—during the Archaean and Palaeoproterozoic Era. Here we present 2.0 Gyr lawsonite eclogites and associated eclogite-facies garnet-kyanite-chloritoid schists with low-thermal gradients of 265-290°C/GPa from the Kongling Complex in South China through integrated thermodynamic modelling and zircon in situ U-Pb dating. More importantly, a temporally equivalent mafic granulites with high-thermal gradients of ~720 °C/GPa has been also recognized spatially adjacent to those low dT/dP eclogite-facies rocks, integrated as a classic paired metamorphic belt. The results show a new discovery of Paleoproterozoic classic paired metamorphic belts driven by cold deep subduction in South China, indicating that the modern-style plate tectonics was already operative on Earth by the Palaeoproterozoic.
Publisher: Springer Science and Business Media LLC
Date: 23-09-2019
Publisher: Elsevier BV
Date: 10-2012
Publisher: Geological Society of America
Date: 18-04-2014
DOI: 10.1130/B30884.1
Publisher: Elsevier BV
Date: 08-2000
Publisher: American Geophysical Union (AGU)
Date: 08-2022
DOI: 10.1029/2022TC007240
Abstract: Long‐standing debates exist over the mechanism of continental lithospheric extension and, more specifically, over the strain distribution across the lithosphere in intraplate settings. The Cretaceous extensional system in South China extends up to ∼800 km inboard of the Paleo‐Pacific convergent margin and enables investigation of the mechanism(s) of intraplate lithospheric extension. Here we use high‐resolution seismic reflection data to image the crustal and upper‐mantle architecture of the central segment of the extensional system. We identify a compositionally stratified upper lithosphere that has undergone depth‐dependent extension, expressed by heterogeneous normal faulting in the upper crust, widely distributed ductile stretching in the lower crust, mantle influx into the crust, a broadly smooth Moho with localized uplift, and mantle shear‐zone generation. We detect, beneath the center of the Ganzhou Rift, the thinnest crust (28–30 km thick) in South China. It spatially correlates with the locus of strong lithospheric thinning and asthenospheric upwelling. We suggest that the generation of the thinnest crust was assisted by lower‐crustal ductile stretching, mantle shearing, and exhumation during depth‐dependent extension. Our study provides insights into the partitioning of depth‐dependent extensional strain into an intraplate stratified lithosphere and the feedback between crustal and mantle processes that shaped the thinnest crust at a position ∼300 km inboard of the convergent margin during continental extension.
Publisher: Elsevier BV
Date: 10-2023
Publisher: Elsevier BV
Date: 04-2022
Publisher: Wiley
Date: 08-09-2022
DOI: 10.1111/JMG.12689
Publisher: Geological Society of London
Date: 1990
Publisher: Elsevier BV
Date: 07-2023
Publisher: Elsevier BV
Date: 2023
Publisher: Elsevier BV
Date: 07-2023
Publisher: Geological Society of America
Date: 1988
Publisher: American Geophysical Union (AGU)
Date: 12-2022
DOI: 10.1029/2022RG000789
Abstract: Understanding of secular evolution of the Earth system is based largely on the rock and mineral archive preserved in the continental lithosphere. Based on the frequency and range of accessible data preserved in this record, we ide the secular evolution into seven phases: (a) “ Proto‐Earth ” (ca. 4.57–4.45 Ga) (b) “ Primordial Earth ” (ca. 4.45–3.80 Ga) (c) “ Primitive Earth ” (ca. 3.8–3.2 Ga) (d) “Juvenile Earth ” (ca. 3.2–2.5 Ga) (e) “ Youthful Earth ” (ca. 2.5–1.8 Ga) (f) “ Middle Earth ” (ca. 1.8–0.8 Ga) and (g) “ Contemporary Earth ” (since ca. 0.8 Ga). Integrating this record with knowledge of secular cooling of the mantle and lithospheric rheology constrains the changes in the tectonic modes that operated through Earth history. Initial accretion and the Moon forming impact during the Proto‐Earth phase likely resulted in a magma ocean. The solidification of this magma ocean produced the Primordial Earth lithosphere, which preserves evidence for intra‐lithospheric reworking of a rigid lid, but which also likely experienced partial recycling through mantle overturn and meteorite impacts. Evidence for craton formation and stabilization from ca. 3.8 to 2.5 Ga, during the Primitive and Juvenile Earth phases, likely reflects some degree of coupling between the convecting mantle and a lithosphere initially weak enough to favor an internally deformable, squishy‐lid behavior, which led to a transition to more rigid, plate like, behavior by the end of the early Earth phases. The Youthful to Contemporary phases of Earth, all occurred within a plate tectonic framework with changes between phases linked to lithospheric behavior and the supercontinent cycle.
Publisher: Elsevier BV
Date: 12-2019
Publisher: Elsevier BV
Date: 10-2014
Publisher: Geological Society of America
Date: 02-2013
DOI: 10.1130/G33594.1
Publisher: Elsevier BV
Date: 09-1991
Publisher: Geological Society of London
Date: 09-2006
Publisher: Elsevier BV
Date: 12-2018
Publisher: Informa UK Limited
Date: 1987
Publisher: Elsevier BV
Date: 12-2016
Publisher: Elsevier BV
Date: 09-2022
Publisher: Elsevier BV
Date: 10-2008
Publisher: Elsevier BV
Date: 12-2020
Publisher: Elsevier BV
Date: 12-2022
Publisher: Annual Reviews
Date: 30-08-2017
DOI: 10.1146/ANNUREV-EARTH-063016-020525
Abstract: The record of the continental lithosphere is patchy and incomplete no known rock is older than 4.02 Ga, and less than 5% of the rocks preserved are older than 3 Ga. In addition, there is no recognizable mantle lithosphere from before 3 Ga. We infer that there was lithosphere before 3 Ga and that ∼3 Ga marks the stabilization of blocks of continental lithosphere that have since survived. This was linked to plate tectonics emerging as the dominant tectonic regime in response to thermal cooling, the development of a more rigid lithosphere, and the recycling of water, which may in turn have facilitated plate tectonics. A number of models, using different approaches, suggest that at 3 Ga the volume of continental crust was ∼70% of its present-day volume and that this may be a minimum value. The continental crust before 3 Ga was on average more mafic than that generated subsequently, and this pre-3 Ga mafic new crust had fractionated Lu/Hf and Sm/Nd ratios as inferred for the sources of tonalite-trondhjemite-granodiorite and later granites. The more intermediate composition of new crust generated since 3 Ga is indicated by its higher Rb/Sr ratios. This change in composition was associated with an increase in crustal thickness, which resulted in more emergent crust available for weathering and erosion. This in turn led to an increase in the Sr isotope ratios of seawater and in the drawdown of CO 2 . Since 3 Ga, the preserved record of the continental crust is marked by global cycles of peaks and troughs of U-Pb crystallization ages, with the peaks of ages appearing to match periods of supercontinent assembly. There is increasing evidence that the peaks of ages represent enhanced preservation of magmatic rocks in periods leading up to and including continental collision in the assembly of supercontinents. These are times of increased crustal growth because more of the crust that is generated is retained within the crust. The rates of generation of continental crust and mantle lithosphere may have remained relatively constant at least since 3 Ga, yet the rates of destruction of continental crust have changed with time. Only relatively small volumes of rock are preserved from before 3 Ga, and so it remains difficult to establish which of these are representative of global processes and the extent to which the rock record before 3 Ga is distorted by particular biases.
Publisher: Geological Society of London
Date: 03-2003
Publisher: Geological Society of America
Date: 20-12-2017
DOI: 10.1130/B31588.1
Publisher: Canadian Science Publishing
Date: 02-1996
DOI: 10.1139/E96-017
Abstract: The Corner Brook–Glover Island region records the development of the internal domain of the Humber Zone and its relationship to the adjoining external domain and Dunnage Zone. The region preserves both the Laurentian margin basement–cover contact and the siliciclastic–carbonate transition within the cover sequence. Precambrian Grenville basement of the Corner Brook Lake Complex is the oldest lithostratigraphic unit and yielded a U/Pb zircon age of 1510 ± 6 Ma. Three main lithostratigraphic assemblages overlie basement: silicic and mafic igneous rocks of the Lady Slipper Pluton which yielded a U/Pb zircon age of [Formula: see text] Ma siliciclastic lithologies which include the South Brook and Summerside formations and carbonate-dominated sequences with clastic incursions which include the Port au Port, St. George, and Table Head groups, and the Breeches Pond, Irishtown, and Pinchgut formations. Dunnage Zone units include plutonic ultramafic to mafic rocks of the Grand Lake Complex, dated by U/Pb zircon from trondhjemite at 490 ± 4 Ma, volcanic and epiclastic rocks of the Glover Island Formation, and the Matthews Brook Serpentinite, the latter restricted to fault slivers within the Humber Zone sequence. The deformed Glover Island Granodiorite intrudes the Dunnage Zone rocks on Glover Island and is dated by U/Pb zircon and titanite at 440 ± 2 Ma. Little deformed Carboniferous sedimentary rocks unconformably overlie both Humber Zone and Dunnage Zone rock units. Timing of regional deformation and peak hibolite-facies metamorphism in the eastern Humber Zone is constrained by isotopic data to the Early Silurian. In the Dunnage Zone, shear zones and foliation development both pre- and postdate the age of the Glover Island Granodiorite, with the later possibly temporally equivalent to deformation in the Humber Zone. Final juxtaposition of the two zones occurred during Carboniferous movement of the Cabot Fault.
Publisher: Elsevier BV
Date: 2023
Publisher: Wiley
Date: 25-09-2020
Publisher: Elsevier BV
Date: 10-2008
Publisher: American Geophysical Union (AGU)
Date: 04-2022
DOI: 10.1029/2021JB023911
Abstract: How the geological record of cratons reconciles with the tectonic environments in which they formed has remained debated. We use 2D Cartesian geometry numerical models of mantle convection varying temperatures from present day to Archaean‐inferred values, to address the formation of cratons, accounting for melt depletion‐dependent rheological stiffening. For mantle temperatures comparable to present day, melting is negligible and the convective regime depends on the strength of the thermal lithosphere. For mantle potential temperatures higher than present day, high depletion degree and large depleted mantle volumes are formed at low lithospheric strength and high surface mobility, whereas these are negligible beneath a poorly mobile lithosphere. When compared to the models, the record of tectonics and large volumes of high‐degree depleted mantle in Archaean cratons is best explained by a lithosphere initially prone to yielding and mobility. At high mobility, large depletion favors the progressive differentiation of the thermochemical lithosphere, which stiffens and thickens with increasing mantle temperatures. The ensuing reduced heat flow atop a hotter mantle is in agreement with the inferred Archaean thermal evolution, and may rule out the viability of a stagnant lid for the early Earth. Large‐scale depletion stiffening resists plate margin formation and this wanes as heat production decreases, thus may hold the key for the establishment of plate tectonics during secular cooling.
Publisher: Elsevier BV
Date: 05-2018
Publisher: American Journal of Science (AJS)
Date: 2021
DOI: 10.2475/01.2021.02
Publisher: Elsevier BV
Date: 09-2022
Publisher: Geological Society of London
Date: 13-03-2023
Abstract: Continental arcs are key sites of granitic magmatism, yet details of the origins of these magmas, including the role and contribution of mafic magma, the timing and location of initial zircon formation and how zircon isotopic signatures relate to granite formation, remain as challenges. Here we use U–Pb dating, trace elements and Hf isotopic systematics of zircon in mafic microgranular enclaves (MMEs), from the convergent plate margin Satkatbong diorite (SKD) in Korea to understand lower arc magmatism and zircon production. The host granitic body and MMEs display similar major element evolutionary trends and similar ranges of Sr, Nd and Hf isotopes, implying a cognatic relationship. Zircons show a large variability in ε Hf ( t ) ( c. 6 units) and age ( Ma). We propose that the SKD and MMEs originated from the same, long-lasting, lower crustal mush reservoir, enabling long and variable residence times for zircons. Prolonged zircon ages, combined with the Hf isotope variability within a single pluton (SKD and its MME), indicate that not all zircons were instantaneously crystallized in a rapidly cooling shallow magma chamber but were continuously formed in a long-lasting hot source. A low-melt-fraction mush type reservoir in a deep crustal hot zone provides a viable model for the source setting. Continuous replenishment of mafic magmas acts as the main re-activator of the reservoir, and provide a critical role in spawning zircons that record a long age span, because (1) the magma adds Zr into the reservoir, enabling it to reach zircon saturation and (2) the generated zircon grains are transported upward as antecrysts by flow inside of the reservoir. This means that antecrysts with different ages may mix with each other in the ascending magma body. The significance of this model is that a conclusive time of intrusion cannot be constrained by such zircon ages, as these antecrysts constitute inherited grains.
Publisher: Canadian Science Publishing
Date: 05-1995
DOI: 10.1139/E95-045
Abstract: Displacement of the Early Ordovician ophiolitic Bay of Islands Complex was accompanied by the development of a metamorphic sole in underlying accreted gabbro, mafic pillow lava, pelite, and psammite. The metamorphic sole contains up to 130 m of hibolite, underlain by up to 80 m of mafic and pelitic–psammitic schist, which, in turn, overlies chlorite-bearing rocks that overlie mudstone-matrix mélange. A major foliation, locally mylonitic and (or) isoclinally folded, is pervasively developed in the greenschists and hibolites. An extension lineation is widely developed and plunges north in hibolite and trends east–west in greenschist, consistent with a changing direction of thrust transport from northerly to westerly as the mantle wedge cooled over time. Shear sense criteria in greenschist facies pelitic–psammitic schist indicate thrusting towards the west. In the southwestern Blow-Me-Down massif, two sets of folds postdate development of accretion-related S-L fabrics and resulted in a substantial widening of the metamorphic sole. Late disruption by foliation-parallel, low-angle extensional and steep faults have excised parts of the metamorphic sole, resulting in a marked discontinuity of units along strike. Extensional faults were induced by gravitational spreading as the Coulomb thrust wedge, containing the ophiolite, metamorphic sole, and underlying mélange unit, became supercritical. This was probably due to a combination of two factors: (1) development of a substantially weakened basal mélange layer and (2) lowering of the basal slope of the wedge as it was thrust over the Ordovician slope onto the shelf.
Publisher: Society for Sedimentary Geology
Date: 1987
Publisher: Elsevier BV
Date: 04-2019
Publisher: Elsevier BV
Date: 02-2019
Publisher: Elsevier BV
Date: 06-2012
Publisher: Oxford University Press (OUP)
Date: 28-12-2021
Publisher: Elsevier BV
Date: 06-2019
Publisher: Elsevier BV
Date: 09-2020
Publisher: Elsevier BV
Date: 03-2017
Publisher: Geological Society of America
Date: 09-2001
Publisher: Wiley
Date: 24-11-2021
DOI: 10.1111/JMG.12641
Abstract: Deciphering the tectono‐metamorphic evolution of Precambrian terranes can be difficult due to reworking by later superimposed events. Whole‐rock elemental and isotopic geochemistry and zircon U–Pb geochronology are often employed in those studies, but these approaches are often not sensitive to the presence of multiple events and medium‐grade metamorphic episodes. The Rio Apa Terrane (RAT), an allochthonous fragment of the Amazonian Craton, is a crustal block with a well‐characterized crustal evolution but with no detailed thermal constraints for its tectono‐metamorphic evolution. In contrast to previous studies, we show the existence of four tectono‐metamorphic events at c . 1,780, c . 1,625, c . 1,420–1,340, and c . 1,300–1,200 Ma on the basis of apatite, titanite, and rutile U–Pb, in situ white‐mica Rb–Sr, and in situ garnet Lu–Hf geochronology combined with mineral chemistry and phase‐equilibria modelling. The c . 1,780 Ma event is recorded in the basement of the Western domain, representing an extensional event coeval with the development of its Eastern domain in response to the retreat stage of the accretionary system. This is followed by juxtaposition of the Western and Eastern domains along a major crustal boundary at c . 1,625 Ma, which is defined by the magnetic profiles and zircon U–Pb–Hf data across the boundary. The third and fourth events correspond to progressive high‐pressure/medium‐temperature (HP/MT) metamorphism, characterized by an anticlockwise P–T path, suggesting a convergent‐to‐collisional tectonic setting. The RAT was accreted to the adjoining Paraguá Terrane at c . 1,420–1,340 Ma under an isobaric P–T evolution spanning ~530°C to 600°C and ~10.0 kbar. Subsequently, the combined Rio Apa and Paraguá terranes collided with the SW Amazonian Craton at c . 1,300–1,200 Ma, reaching P–T conditions of ~560–580°C and ~10.9–11.7 kbar during crustal thickening. This study reveals for the first time the existence of a HP/MT metamorphic evolution related to the growth of the SW Amazonian Craton as part of an accretionary orogenic system during Rodinia assembly in the Palaeoproterozoic to Mesoproterozoic.
Publisher: Geological Society of America
Date: 24-06-2011
DOI: 10.1130/B30415.1
Publisher: Geological Society of America
Date: 22-12-2016
DOI: 10.1130/G37399.1
Publisher: Geological Society of America
Date: 08-2013
DOI: 10.1130/G34395.1
Publisher: American Journal of Science (AJS)
Date: 10-1991
Publisher: Elsevier BV
Date: 2018
Publisher: Elsevier BV
Date: 02-2022
Publisher: Elsevier BV
Date: 02-2021
Publisher: Geological Society of America
Date: 09-11-2022
DOI: 10.1130/G49418.1
Publisher: Elsevier BV
Date: 09-2019
Publisher: Elsevier BV
Date: 12-2012
Publisher: Elsevier BV
Date: 12-2012
Publisher: Geological Society of America
Date: 24-02-2021
DOI: 10.1130/B35859.1
Publisher: Geological Society of America
Date: 1993
DOI: 10.1130/SPE275-P135
Publisher: Informa UK Limited
Date: 04-1986
Publisher: American Geophysical Union (AGU)
Date: 2017
DOI: 10.1002/2016JB013508
Publisher: University of Chicago Press
Date: 2012
DOI: 10.1086/662717
Publisher: Oxford University Press (OUP)
Date: 26-11-2022
DOI: 10.1093/NSR/NWAB211
Publisher: Wiley
Date: 02-2002
Publisher: Elsevier BV
Date: 06-2012
Publisher: Elsevier BV
Date: 05-2016
Publisher: American Geophysical Union (AGU)
Date: 28-10-2017
DOI: 10.1002/2017GL074717
Publisher: Elsevier BV
Date: 08-2015
Publisher: Elsevier BV
Date: 12-2013
Publisher: Elsevier BV
Date: 05-2014
Publisher: Elsevier BV
Date: 2021
Publisher: Oxford University Press (OUP)
Date: 06-2001
Publisher: American Journal of Science (AJS)
Date: 12-2018
DOI: 10.2475/10.2018.01
Publisher: Geological Society of America
Date: 04-2001
Publisher: Canadian Science Publishing
Date: 11-1998
DOI: 10.1139/E98-053
Abstract: The Humber Zone of the western Newfoundland Appalachians represents the early Paleozoic Laurentian margin established by Neoproterozoic rifting. After a period of passive margin thermal subsidence, Taconian deformation began in the Early Ordovician with westward thrusting. Subsequently, an extensive foreland basin developed beneath the Gulf of St. Lawrence. It records rapid Late Ordovician to Early Silurian subsidence mid-Silurian erosion and renewed Late Silurian to Devonian subsidence. The Humber Zone was traversed by Lithoprobe seismic reflection profiles. Within the external part of the orogen, seismic reflections in the upper crustal section appear more coherent where seismic lines are parallel to fold hinges. Some subhorizontal reflectors are interpreted as thrust sheets of shelf limestone, but others probably represent intrabasement structures. A group of moderately northwest-dipping reflections probably represents late extensional shear zones. On the Baie Verte Peninsula, low-angle reflections passing beneath the Baie Verte Line are probably also late extensional shears, possibly reactivating earlier thrusts. Tectonism in the Humber Zone probably began with attempted eastward subduction of the Laurentian margin. Deep burial of the margin, accompanied by eclogite-facies metamorphism, probably coincided with rapid subsidence in the foreland basin. Later Barrovian metamorphism was associated with cleavage development and east-directed shear, and with dextral oblique slip, in Baie Verte Peninsula. Later Silurian sinistral transpression with thrusting east of the Baie Verte Line was followed by dextral transpression to transtension. "Acadian" thrusting dominated the western margin of the orogen in the Devonian and possibly earliest Carboniferous.
Publisher: Elsevier BV
Date: 09-08-2005
Publisher: Elsevier BV
Date: 04-2022
Publisher: Wiley
Date: 30-12-2012
Publisher: Elsevier BV
Date: 09-2016
Publisher: Elsevier BV
Date: 02-2016
Publisher: Geological Society of America
Date: 2006
DOI: 10.1130/GSAT01607.1
Publisher: Geological Society of London
Date: 03-2010
Publisher: Elsevier BV
Date: 08-2016
Publisher: Elsevier BV
Date: 2022
Publisher: Society for Sedimentary Geology
Date: 02-2012
DOI: 10.2110/JSR.2012.6
Publisher: Cambridge University Press (CUP)
Date: 03-2002
DOI: 10.1017/S0016756801006276
Abstract: Ion microprobe analyses of detrital zircons in the Te Akatarawa Terrane, New Zealand, reveal that the age of unfossiliferous turbidites overlying a fusuline- and coral-bearing limestone block olistostromal mélange is no older than 255±4 Ma (Late Permian). This is approximately 15 m.y. younger than the Kungurian age of the fusulinid limestone. We interpret this to indicate collapse of a Permian oceanic seamount as it entered a subduction zone along the Pacific margin of Gondwana. These turbidites differ markedly in composition from adjoining Permian to Middle Triassic sand-stones of the Torlesse Terrane. Detrital zircon age data indicate predominantly Permian and Carboniferous ages for source rocks supplying the Te Akatarawa turbidites, but also reveal significant earlier Palaeozoic and Proterozoic components, ranging back to 1.9 Ga. The warm-water setting of limestone blocks and the short 15 m.y. time period between sedimentation and accretion onto a continental margin require the limestone to have formed in a low-latitude position probably off the northeast Australian (New Guinea) margin of Gondwana. Zircons within the s le underwent re-crystallization at around 230±11 Ma which may be related to alteration during accretion in a subduction zone environment. Over a period of 100 to 150 m.y. from 255 Ma the terrane underwent more than 5000 km translation along the continental margin southward to its current location as an exotic mini-terrane enclosed within the New Zealand Torlesse Terrane.
Publisher: American Geophysical Union (AGU)
Date: 27-09-2021
DOI: 10.1029/2021TC006806
Abstract: Sedimentary successions deposited within arc‐trench gaps (forearcs) record topographic oscillations related to subduction tectonism. The collision of oceanic plateaus can inhibit normal subduction and induce detachment of the subducted oceanic lithosphere (slab), leading to subduction translation or shut‐down. Such second‐order subduction processes complicate the stratigraphic record making discrete events difficult to resolve, as preserved ex les are rare and typically overprinted by deformation. We compiled and averaged (stacked) top subduction wedge (Pahau Terrane) subsidence and paleo‐water depth curves from 30 locations containing mid‐Cretaceous forearc successions in Marlborough, New Zealand. Subsidence curve stacking proved effective in removing deformation due to normal subduction, allowing for resolution of higher order plate‐margin events. The stacked curves reveal a synchronous topographic oscillation affecting over 100 km of the paleo‐coastline between 110 and 95 Ma, which penetrated almost 250 km into the forearc hinterland and created up to 3 km of accommodation space. Topographic drawdown and highstand deposition from 110 Ma were followed by rebound and volcanism by 98 Ma, a response to regional tectonism that was compared to theoretical predictions for ridge and plateau collision. We conclude that plate flexure, and slab extension and tearing reasonably account for the synchronous topographic oscillation observed, which we attribute to Hikurangi Plateau collision. We postulate that collision began east of Marlborough along the present day Chatham Rise from 110 Ma, producing topographic upheaval and disruption of adjacent sedimentary systems. Sediments deposited contemporaneously along the margin preserve a record of these events and provide a rare insight into evolving mid‐Cretaceous plate dynamics.
Publisher: Springer Science and Business Media LLC
Date: 10-06-2021
DOI: 10.1038/S41467-021-23805-6
Abstract: The formation of stable, evolved (silica-rich) crust was essential in constructing Earth’s first cratons, the ancient nuclei of continents. Eoarchaean (4000–3600 million years ago, Ma) evolved crust occurs on most continents, yet evidence for older, Hadean evolved crust is mostly limited to rare Hadean zircons recycled into younger rocks. Resolving why the preserved volume of evolved crust increased in the Eoarchaean is key to understanding how the first cratons stabilised. Here we report new zircon uranium-lead and hafnium isotope data from the Yilgarn Craton, Australia, which provides an extensive record of Hadean–Eoarchaean evolved magmatism. These data reveal that the first stable, evolved rocks in the Yilgarn Craton formed during an influx of juvenile (recently extracted from the mantle) magmatic source material into the craton. The concurrent shift to juvenile sources and onset of crustal preservation links craton stabilisation to the accumulation of enduring rafts of buoyant, melt-depleted mantle.
Publisher: Elsevier BV
Date: 03-2012
Publisher: Elsevier BV
Date: 11-2020
Publisher: Elsevier BV
Date: 09-2020
Publisher: Geological Society of America
Date: 09-11-2022
DOI: 10.1130/G49416.1
Publisher: Geological Society of America
Date: 05-2020
Publisher: Research Square Platform LLC
Date: 10-03-2021
DOI: 10.21203/RS.3.RS-287716/V1
Abstract: Initiation of stable Mariana type one-sided oceanic subduction zones requires rheologically strong oceanic lithosphere, which developed through secular cooling of Earth mantle. This enabled the development of focused high stress zones resulting in narrow weak zones of convergence with resultant oceanic subduction leading to mantle hydration and arc magmatism. Based on detailed study and identification of the oldest (518 Ma) Mariana type oceanic subduction initiation ophiolite (Munabulake ophiolite) on Earth from northern Tibet, along with compilation of oceanic subduction initiation ophiolites through Earth history, we argue for the initiation of modern plate tectonic regime by at least the early Cambrian. The mantle and crust members of the Munabulake ophiolite preserve a complete ophiolite stratigraphy. Blocks of layered marble and siliceous rocks interlayered with meta-basalt indicate a marine environment. Zircons from an olivine gabbro s le yield a concordant age of 518 Ma, along with mantle derived low δ 18 O (2.69‰ – 5.7‰) and high εHf(t) (11.1–13.6) values. The zircons also have varied H 2 O contents ranging from 109–1339 ppm with peaks at 260 and 520 ppm, indicative of hydration of mantle derived magma. The highly depleted peridotites display U–shaped REE patterns and varied Zr/Hf ratios, whereas spinel and olivine compositions within the peridotites indicate that they are residues of various degrees of melt extraction and evolved from abyssal to fore-arc peridotites. The crustal members of the ophiolite are mostly tholeiitic, display flat REE patterns and lower HFSEs, comparable to transitional lavas associated with Mariana subduction initiation ophiolite. Some rocks from the crustal section of the ophiolite display NMORB-like compositions but are also characterized by depletion in HSFEs. Therefore, the Munabulake ophiolite displays a chemical duality and progressively evolved from MORB (mid-ocean ridge basalt) to SSZ (supra-subduction zone) compositions, consistent with observations from zircon Hf-O isotopes and H 2 O contents. Furthermore, the ophiolite was formed during subduction initiation of the Proto-Tethys Ocean at the northern Gondwana margin, and coincided with an inferred slab roll back event in the southern Gondwana margin at ca. 530 − 520 Ma, indicative of a time of global tectonic re-organization. The early Cambrian Munabulake ophiolite indicates comparable slab strength and conditions to those that characterize modern plate tectonics. Such a tectonic regime coincided with final Gondwana assembly, and was associated with ca. 530 − 520 Ma global tectonic re-organization.
Publisher: Springer Science and Business Media LLC
Date: 20-05-2023
Publisher: Elsevier BV
Date: 08-2012
Publisher: Elsevier BV
Date: 12-2021
Publisher: Elsevier BV
Date: 05-2023
Publisher: Geological Society of America
Date: 08-2001
Publisher: Geological Society of London
Date: 2001
Publisher: American Geophysical Union (AGU)
Date: 09-2017
DOI: 10.1002/2017TC004600
Publisher: Springer Science and Business Media LLC
Date: 21-09-2023
Publisher: Elsevier BV
Date: 2004
Publisher: Elsevier BV
Date: 12-2009
Publisher: Institute of Earth's Crust, Siberian Branch of the Russian Academy of Sciences
Date: 2017
Publisher: Elsevier BV
Date: 2004
Publisher: Informa UK Limited
Date: 09-1991
Publisher: Elsevier BV
Date: 2016
Publisher: Research Square Platform LLC
Date: 18-08-2021
DOI: 10.21203/RS.3.RS-733095/V1
Abstract: Geological and geophysical data coupled with numerical simulations have shown that lithospheric extension at passive margins may be classified into three end-member scenarios of pure shear, simple shear, and depth-dependent deformation. However, how lithospheric extension evolves in an intraplate setting remains enigmatic due to lack of reliable constraints on the deep lithospheric architecture. Here we use a seismic reflection profile across the ~800-km-wide Cretaceous intraplate extensional system of South China to illustrate depth-dependent kinematic decoupling of extension in a mechanically stratified lithosphere. The extension was initially distributed in magma-poor conditions as expressed by normal faulting in the upper crust and lower-crustal flow toward the rift axis. Necking of the crust and Moho uplift led to mantle shear-zone formation, lower-crustal flow toward the rift flanks, and deep mantle flow. We demonstrate that the extensional modes vary with decreasing mantle strength from magma-poor to magma-rich domains, as reflected in decreasing crust-mantle decoupling with increased Moho temperatures (TM), and the replacement of a two-layer (brittle vs ductile) mantle by a fully ductile mantle. These findings reveal a first-order lithospheric configuration of intraplate depth-dependent extension driven by far-field stresses attributable to slab retreat.
Publisher: Elsevier BV
Date: 04-2018
Publisher: Springer Science and Business Media LLC
Date: 27-11-2019
DOI: 10.1038/S41598-019-54230-X
Abstract: Despite being the largest accretionary orogen on Earth, the record of crustal growth and reworking of in idual microcontinental massifs within the Central Asian Orogenic Belt (CAOB) remain poorly constrained. Here, we focus on zircon records from granitoids in the Erguna Massif to discuss its crustal evolution through time. Proterozoic–Mesozoic granitoids are widespread in the Erguna Massif, and spatiotemporal variations in their zircon ε Hf (t) values and T DM2 (Hf) ages reveal the crustal heterogeneity of the massif. Crustal growth curve demonstrates that the initial crust formed in the Mesoarchean, and shows a step-like pattern with three growth periods: 2.9–2.7, 2.1–1.9, and 1.7–0.5 Ga. This suggests that microcontinental massifs in the eastern CAOB have Precambrian basement, contradicting the hypothesis of significant crustal growth during the Phanerozoic. Phases of growth are constrained by multiple tectonic settings related to supercontinent development. Calculated reworked crustal proportions and the reworking curve indicate four reworking periods at 1.86–1.78 Ga, 860–720 Ma, 500–440 Ma, and 300–120 Ma, which limited the growth rate. These periods of reworking account for the crustal heterogeneity of the Erguna Massif.
Publisher: American Association for the Advancement of Science (AAAS)
Date: 16-03-2012
Abstract: The appearance and persistence of continents through geologic time has influenced most processes on Earth, from the evolution of new species to the climate. The relative proportion of newly formed crust compared to reworked, or destroyed, older crust reveals which processes controlled continental growth. Based on the combined analyses of Hf-Pb and O isotopes in zircon minerals, Dhuime et al. (p. 1334 ) measured continuous but variable rates of new crustal production throughout Earth's history. Increased rates of crustal destruction starting around 3 billion years ago coincide with the onset of subduction-drive plate tectonics, slowing down the overall rate of crustal growth.
Publisher: Informa UK Limited
Date: 08-1998
Publisher: Elsevier BV
Date: 10-2023
Publisher: Elsevier BV
Date: 08-2023
Publisher: Elsevier BV
Date: 12-2010
Publisher: Elsevier BV
Date: 10-2013
Publisher: Elsevier BV
Date: 02-2020
Publisher: American Geophysical Union (AGU)
Date: 04-2012
DOI: 10.1029/2011TC002937
Publisher: American Geophysical Union (AGU)
Date: 09-2020
DOI: 10.1029/2019TC005988
Publisher: American Geophysical Union (AGU)
Date: 08-2021
DOI: 10.1029/2021GL094236
Abstract: The widespread Tibetan Permo‐Carboniferous glaciogenic diamictites (PCGDs) are conventionally thought to be sourced from Indian Gondwana during glacier transport and deglaciation. However, the Lhasa PCGDs differ in detrital zircon U‐Pb age spectra and ε Hf ( t ) values from those in Southern Qiangtang and Tethyan Himalaya. The similarities in ε Hf ( t ) values for similar‐age detrital zircons, the development of glacier transport pathways, and the large volumes of the Tibetan PCGDs indicate an Australian source for the Lhasa PCDGs, and an Indian source for the Southern Qiangtang and Tethyan Himalayan PCDGs. We conclude that the Southern Qiangtang and Tethyan Himalayan are paleographically linked to northern India, whereas Lhasa is positioned adjacent to NW Australia during the Paleozoic. Magmatic and metamorphic records further indicate that eastern Lhasa (E90°–E95°) represents the outboard extension of events recorded in northern Central Australia, whereas western Lhasa (E80°–E90°) was located outboard of the West Australian Craton.
Publisher: American Geophysical Union (AGU)
Date: 12-2013
DOI: 10.1002/TECT.20099
Publisher: Elsevier BV
Date: 06-2023
Publisher: Elsevier BV
Date: 09-2021
Publisher: Geological Society of America
Date: 22-08-2022
DOI: 10.1130/B36395.1
Publisher: Elsevier BV
Date: 02-2021
Publisher: Geological Society of America
Date: 07-2007
DOI: 10.1130/B26152.1
Publisher: Informa UK Limited
Date: 06-1999
Publisher: American Journal of Science (AJS)
Date: 04-2019
DOI: 10.2475/04.2016.02
Publisher: Geological Society of America
Date: 30-08-2019
DOI: 10.1130/G46855.1
Abstract: Plume-modified orogeny involves the interaction between a mantle plume and subducting oceanic lithosphere at accretionary margins. We propose that a plume can also be involved in collisional orogeny and accounts for the late Paleozoic geological relations in Central Asia. Continental collision between the Tarim and Central Tianshan–Yili blocks at the end Carboniferous resulted in an orogeny lacking continental-type (ultra)high-pressure [(U)HP] rocks and significant syncollision surface erosion and uplift, features normally characteristic of continent-continent interactions. Their absence from the Tianshan region corresponded with the arrival of a mantle plume beneath the northern Tarim. Elemental and isotopic data reveal an increasing influence of the mantle plume on magmatic petrogenesis from ca. 300 to 280 Ma, immediately after collision at 310–300 Ma. The rising mantle plume interrupted the normal succession of collisional orogenic events, destroying the deeply subducted continental crust and hence preventing slab break-off–induced continental rebound. Plume-modified continental collision thus limited continental (U)HP rock exhumation and associated surface uplift.
Publisher: Geological Society of America
Date: 10-2014
DOI: 10.1130/G35892.1
Publisher: Society of Economic Geologists
Date: 03-2020
Publisher: Geological Society of America
Date: 15-04-2019
DOI: 10.1130/G45915.1
Publisher: Geological Society of London
Date: 27-08-2020
Publisher: Geological Society of London
Date: 03-2007
Publisher: Elsevier BV
Date: 2001
Publisher: Elsevier BV
Date: 11-2017
Publisher: American Geophysical Union (AGU)
Date: 12-08-2022
DOI: 10.1029/2021GL097515
Abstract: The compositional similarity between high‐Mg andesite‐dacite from accretionary orogens and bulk continental crust (CC) provides an opportunity to unravel the CC formation paradox. Compositional data from a global compilation of Quaternary magmatic arcs indicate the presence of low‐Mg series (LMS) and high‐Mg series (HMS). The LMS show trends of crystal fractionation and can be sub ided into high Ba/Th and high La/Sm groups, which likely originate from fluid‐ and sediment melt‐modified mantle wedge, respectively. In contrast, the HMS have variably mixed compositions (e.g., high Mg#, Ba/Th, and La/Sm) and can be explained by partial melting of mélange diapirs rising into the mantle wedge, which are mixtures of subducted sediment, eroded arc crust or CC, buoyant oceanic crust, and peridotite. We, therefore, propose a two‐step process for creating CC involving extraction of LMS from the mantle followed by re‐melting of recycled LMS in the mantle to generate HMS and thus CC.
Publisher: Research Square Platform LLC
Date: 06-06-2023
DOI: 10.21203/RS.3.RS-2986195/V1
Abstract: Tonalite-trondhjemite-granodiorite (TTG) gneisses, the major components of Archean continental crust, show a broad compositional range. Most were viewed as crust-derived, and the inferred melting P-T conditions shaped our knowledge about the origin of early continental crust. While one single basaltic source (e.g., median of Archean tholeiites) was commonly invoked for different TTG gneisses, the potential influences of wide-ranging basaltic sources remain not well constrained. Late Neoarchean tonalitic to trondhjemitic gneisses, covering the compositional spectrum of global database, were identified from the Jiaobei terrane, North China Craton. Thermodynamic and trace element modeling demonstrates that (1) their chemical ersity is primarily determined by different basaltic sources with variable TiO2 and heavy rare earth element (HREE) contents and (2) the inferred melting pressures of most tonalitic to trondhjemitic gneisses would reduce dramatically if a different basaltic source with slightly lower TiO2 and HREE contents was assumed. Integrated with synchronous chemical changes of global Archean TTG and basaltic rocks, a source-based twofold classification of TTG gneisses (i.e., low- and high-Ti-HREE types) is put forward. The low-Ti-HREE TTG gneisses necessitate both low-Ti-HREE basaltic sources and high melting pressures (~1.8 GPa), and their outburst after ~3.2 Ga may mark the development of thickened continental crust globally.
Publisher: Elsevier BV
Date: 09-2018
Publisher: Elsevier BV
Date: 08-2021
Publisher: Elsevier BV
Date: 07-2017
Publisher: Proceedings of the National Academy of Sciences
Date: 08-11-2021
Abstract: Understanding when and how subaerial continental crust first formed is crucial, as it likely played a critical role in establishing Earth’s habitability. Although debated, the broad consensus is that the subaerial rise of continents began ∼2.5 billion years ago and was driven by plate tectonics. Here, we integrate the igneous and sedimentary history of Archean cratons to demonstrate that stable continental landmasses started to emerge above sea level 3.3 to 3.2 billion years ago (i.e., over 700 million years earlier than most models predict). We also demonstrate that these initial episodes of continental emersion were driven by voluminous granitoid magmatism in non–plate tectonic settings that formed ∼50-km-thick, silica-rich crust, which rose above the oceans due to isostasy.
Publisher: Informa UK Limited
Date: 08-07-2021
Publisher: Informa UK Limited
Date: 06-1999
Publisher: American Geophysical Union (AGU)
Date: 11-2017
DOI: 10.1002/2017GC006977
Publisher: American Journal of Science (AJS)
Date: 2000
DOI: 10.2475/AJS.300.1.60
Publisher: Geological Society of London
Date: 2001
Publisher: Elsevier BV
Date: 11-2018
Publisher: American Geophysical Union (AGU)
Date: 05-2021
DOI: 10.1029/2020GC009622
Abstract: New geochronological and geochemical data document a new and widely distributed succession of igneous and sedimentary rocks within the Sibumasu that extend from SW Yunnan through SE Asia as far as Sumatra. Our data revealed the presence of an Ordovician‐Silurian (mainly ∼490–430 Ma) igneous zone. The early Paleozoic granites in the zone display similar elemental and Sr–Nd–Pb–Hf isotopic compositions. They were derived from a common mixed source of ancient crustal materials with a juvenile component and formed in a subduction‐related setting. Detrital‐zircon U‐Pb apparent ages from the previously defined Precambrian Lancang and Ximeng units in the SW Yunnan portion of the Sibumasu are in the range of 3,306–428 Ma and 3,316–512 Ma, with the youngest age‐peaks of 505 Ma and 447 Ma, respectively, indicating the lower Paleozoic (Cambrian‐Silurian) sedimentary sequences. The Tarutao Unit and its equivalents in the SE Asia portion of the Sibumasu yield the U‐Pb apparent ages of 3,177–510 Ma, suggesting the maximum deposited time being Cambrian‐Ordovician. All these detrital zircon U‐Pb ages define two main peaks of ∼554–528 Ma and 964–905 Ma with ε Hf (t) values similar to those in the Qiangtang, Tethyan Himalaya, and eastern Indochina. The lower Paleozoic detritus in the Sibumasu were likely derived from the India‐Antarctica region of East Gondwana. We propose that the late Cambrian‐Silurian units formed in an outward‐propagating accretionary orogen in response to the consumption of the Prototethyan Ocean in SW Yunnan and SE Asia. Sibumasu might represent a part of the easterly migrating accretionary orogen along the northern margin of East Gondwana in the late Cambrian‐late Silurian.
Publisher: Elsevier BV
Date: 03-2020
Publisher: GeoScienceWorld
Date: 10-02-2022
DOI: 10.2113/2022/2103213
Abstract: Shear zones are zones of localized high strain accommodating differential motion in the lithosphere and impacting the crustal rheology and deformational history of orogenic belts. Although terrane bounding shear zones are widely studied, intraterrane shear zones and their tectonic significance, especially in association with supercontinent assembly, is a largely unexplored topic. The Ribeira Belt (SE Brazil), a Neoproterozoic-Cambrian orogenic belt from West Gondwana, is dissected by a crustal-scale NE-trending transcurrent shear zone system that juxtaposes composite terranes. Despite its extensive coverage and complexity, this shear zone system remains poorly investigated. In this paper, we explore the thermal and deformational regimes, and timing of ductile shearing using a multiscale approach combining structural analysis derived from remote sensing and field-based structural data, microstructures, quantitative structural analysis, and multimineral U–Pb geochronology (zircon, titanite, monazite, and xenotime). Our data, combined with previously published data, indicate a transitional northeastward increase in metamorphic conditions from lower greenschist to granulite facies conditions (from 250–300 to 750–800°C), reflecting the different crustal levels that are exposed. Vorticity and finite strain data indicate a complex strain regime with varied contributions of pure and simple shear and oblate-shape ellipsoids in strike-slip shear zones and prolate-shaped ellipsoids in dip-slip reverse shear zones. The strain set suggests that all shear zones were developed under subsimple shear deformational regimes involving thrusting and folding followed by wrench tectonics. The pure shear component of deformation was accommodated in folded domains between shear zones. Geochronological data suggest intermittent ductile shear zone activations from ca. 900–830 to 530 Ma, partially coeval with at least two major episodes of terrane accretion at 850–760 Ma and 610–585 Ma. The spatial and temporal record of shear zones within the Ribeira Belt indicates that some relate to assembly of the belt and represent either terrane bounding structures (e.g., Itapirapuã shear zone) or intraterrane structures (e.g., Ribeira, Figueira, and Agudos Grandes shear zones), whereas others are terrane bounding, postcollisional shear zones (e.g., Taxaquara shear zone) reactivated in an intracontinental setting (560–535 Ma).
Publisher: Elsevier BV
Date: 09-2000
Publisher: Cambridge University Press (CUP)
Date: 17-05-2019
DOI: 10.1017/S001675681900027X
Abstract: The Neoproterozoic Jiangnan orogenic belt records the accretion and collision between the Yangtze and Cathaysia blocks in South China. The orogen is isible into three units: a northeastern domain (also referred to as the Huaiyu or Shuangxiwu domain), a central domain (Jiuling domain) and an undifferentiated southwestern domain. Detrital zircons from the oldest sequences (Shuangqiaoshan, Lengjiaxi, Fanjingshan and Sibao groups) in the central and southwest domains yield similar age spectra with major age populations at c . 875–820 Ma, along with minor Palaeo- to Mesoproterozoic and Archaean ages. The dominance of detrital ages close to the deposition ages of the units, along with juvenile zircon Hf isotopic compositions and arc-like whole-rock compositional data, indicate the sedimentary units accumulated adjacent to a convergent plate margin magmatic arc. The presence of Mesoproterozoic and older zircons, both as detritus in the units and as xenocrysts within igneous rocks displaying a subduction-related signature, along with the compositional data, place the magmatic arc along a continental margin. In the northeastern domain, the oldest coeval sequence (Shuangxiwu and Qigong groups) and arc igneous suites are dated at c . 970–850 Ma, and lack older detritus and xenocrysts, indicating they represent an accreted oceanic arc system.
Publisher: University of Chicago Press
Date: 09-2016
DOI: 10.1086/687396
Publisher: Elsevier BV
Date: 12-2020
Publisher: Elsevier BV
Date: 09-2020
Publisher: Geological Society of America
Date: 10-02-2017
DOI: 10.1130/B31604.1
Publisher: Geological Society of London
Date: 21-03-2017
DOI: 10.1144/JGS2016-080
Publisher: Elsevier BV
Date: 11-2016
Publisher: Elsevier BV
Date: 06-2009
Publisher: Elsevier BV
Date: 09-2012
Publisher: Elsevier BV
Date: 05-2015
Publisher: Geological Society of America
Date: 11-10-2019
DOI: 10.1130/B35027.1
Publisher: Elsevier BV
Date: 05-2019
Publisher: Elsevier BV
Date: 11-2023
Publisher: Research Square Platform LLC
Date: 02-05-2023
DOI: 10.21203/RS.3.RS-2820807/V1
Abstract: Subduction of oceanic lithosphere is widely invoked for the Neoarchean but the thermal and geometrical configurations of the inferred subduction zones remain poorly constrained. Two Neoarchean subduction-related tectonic belts (A and B) with contrasting lithotectonic evolutions are preserved in the North China Craton. In Belt A, the oxygen fugacity of ca. 2.6-2.5 Ga modified mantle from crustal recycling-related basalts is coincident with modern arc mantle, but that of Belt B is more reducing. Based on the relationship between mantle redox state and slab dip from contemporary arcs, the dip of subducting oceanic lithosphere in Belt A was in a relatively steep dip (~50°), whereas Belt B had a low angle dip (~15°). These belts represent contrasting styles of Neoarchean subduction with significant differences in mantle temperature and redox state, lithosphere thickness and slab dip.These discoveries further refine our insights into Archean slab subduction and the early Earth’s geodynamic evolution.
Publisher: Elsevier BV
Date: 02-1984
Publisher: Geological Society of America
Date: 16-09-2014
DOI: 10.1130/B31068.1
Publisher: Elsevier BV
Date: 10-2021
Publisher: Elsevier BV
Date: 11-2019
Publisher: Annual Reviews
Date: 31-05-2023
Publisher: Geological Society of London
Date: 27-02-2009
Publisher: American Journal of Science (AJS)
Date: 02-2013
DOI: 10.2475/02.2013.02
Publisher: American Geophysical Union (AGU)
Date: 02-2020
DOI: 10.1029/2019TC005951
Publisher: Elsevier BV
Date: 12-2017
Publisher: Elsevier BV
Date: 11-2022
Publisher: Elsevier BV
Date: 06-1989
Publisher: American Journal of Science (AJS)
Date: 11-2010
DOI: 10.2475/09.2010.11
Publisher: Elsevier BV
Date: 09-2019
Publisher: Geological Society of America
Date: 11-02-2020
DOI: 10.1130/B35370.1
Abstract: Hainan Island may have lain at the boundary between the Tethyan and Pacific domains since the late Paleozoic. Permo–Triassic granitoids outcropped on the island provide insight into Mesozoic tectonic evolution and potential dynamics. Based on analyses of zircon U-Pb geochronological and Hf-O isotopic data, along with whole-rock elemental and Sr-Nd isotopic data, the Permo–Triassic granitoids are ided into three groups: Late Permian (256–252 Ma) gneissic granitoids (Group 1), Early–Middle Triassic (247–244 Ma) massive granitoids (Group 2), and Middle-Late Triassic (242–225 Ma) massive granitoids (Group 3). Groups 1 and 2 exhibit similar elemental and Sr-Nd isotopic compositions with εNd(t) values ranging from –6.71 to –3.25. Group 1 is characterized by gneissic foliation and calc-alkaline I-type geochemical affinities with negative Nb-Ta and Ti anomalies it has low εHf(t) (–4.2∼+0.2) and high δ18O values (9.35–10.46‰), possibly related to derivation of a metabasite source in a continental arc setting. The Group 2 s les are peraluminous massive granitoids with slightly high A/CNK ratios of 1.00–1.31, δ18O values (8.85–11.75‰), and high Sr/Y ratios but low εHf(t) (–8.7∼+1.6) values. They may have originated from the mixed source of greywacke and metabasite, indicating a compressive tectonic setting. The Group 3 high-K calc–alkaline granitoids have high zircon temperatures (842–867 °C) and show the geochemical signatures of A-type granites. They are featured by slightly low whole-rock εNd(t) and zircon εHf(t) values, suggestive of the derivation from a metabasite–greywacke source in an extensional setting. In combination with other geochronological and geochemical data from Hainan Island, it is proposed that the Permian–Triassic igneous magmatism in Hainan Island reflects a continuous amalgamation process from back-arc consumption (272–252 Ma) to orogenic assembly (251–243 Ma) and orogenic collapse (242–225 Ma) between the South China and Indochina Blocks. Such a temporal–spatial pattern for the Hainan granitoids is consistent with that along the Truong Son, Jinshajiang–Ailaoshan–Song Ma tectonic zone, suggesting dominant control of Paleotethyan domain instead of Paleopacific tectonics.
Publisher: Copernicus GmbH
Date: 15-05-2023
DOI: 10.5194/EGUSPHERE-EGU23-4566
Abstract: The Earth has evolved into a habitable planet through ongoing and complex cycling. Decades of field studies, geochemical analyses and computational approaches to integrate data into feasible geodynamic models reveal that Earth& #8217 s evolution was not linear but evolved in discrete phases. The timing of changes between these phases, their loci within Earth& #8217 s crust or between discrete cratonic terranes, and most importantly the drivers or tipping point for these changes, remain elusive.Integrating the record from the continental archive with knowledge of the ongoing cooling of the mantle and lithospheric rheology (parametrized for its evolving thermal state) allows us to determine that a number of different tectonic modes operated through the early history of the Earth. The temporal boundaries between these proposed different phases in tectonic mode are approximate, transitional, and correspond with the first recording of a key feature of that phase.Initial accretion and the moon forming impact resulted in a proto-Earth phase (ca. 4.57-4.45 Ga) likely characterized by a magma ocean. Its solidification produced the primitive Earth lithosphere that extended from ca. 4.45-3.80 Ga, which based on the very minor fragments preserved in younger cratons provides evidence for intra-lithospheric reworking, but which also likely involved intermittent and partial recycling of the lid through mantle overturn and meteoritic impacts. Evidence for craton formation and stabilization during the primitive (ca. 3.8 Ga to 3.2 Ga), and juvenile (ca. 3.2 Ga to 2.5 Ga) phases of Earth evolution likely reflects some degree of coupling between the convecting mantle and a lithosphere initially weak enough to favour an internally deformable, squishy-lid behaviour. These regions of deformable lithosphere likely oscillated spatially and temporally with regions of more rigid, plate like, behaviour leading to a transition to global plate tectonics by the end of the Archean (ca. 2.5 Ga). Evidence for assembly of rigid cratonic blocks in the late Archean along with their subsequent rifting and breakup followed by their reassembly along major linear orogenic belts in the Paleoproterozoic marks the clear inception of the supercontinent cycle in response to a plate tectonic framework of oceans opening and closing.Since solidification of the magma ocean early in Earth history, the available record suggests some degree of mantle-lithosphere coupling. The development and stabilization of cratons from 3.8-2.5 Ga provides evidence for the progressive development of rigid lithosphere and represents the inexorable precursor to the development of plate tectonics.
Publisher: Springer Science and Business Media LLC
Date: 07-06-2022
DOI: 10.1038/S41467-022-30886-4
Abstract: The redox evolution of Archean upper mantle impacted mantle melting and the nature of chemical equilibrium between mantle, ocean and atmosphere of the early Earth. Yet, the origin of these variations in redox remain controversial. Here we show that a global compilation of ∼3.8-2.5 Ga basalts can be sub ided into group B-1, showing modern mid-ocean ridge basalt-like features ((Nb/La) PM ≥ 0.75), and B-2, which are similar to contemporary island arc-related basalts ((Nb/La) PM 0.75). Our V-Ti redox proxy indicates a more reducing upper mantle, and the results of both ambient and modified mantle obtained from B-1 and B-2 s les, respectively, exhibit a ∼1.0 log unit increase in their temporal evolution for most cratons. Increases in mantle oxygen fugacity are coincident with the changes in basalt Th/Nb ratios and Nd isotope ratios, indicating that crustal recycling played a crucial role, and this likely occurred either via plate subduction or lithospheric drips.
Publisher: Elsevier BV
Date: 2019
Publisher: Geological Society of America
Date: 1994
Publisher: Elsevier BV
Date: 05-2003
Publisher: Oxford University Press (OUP)
Date: 21-06-2023
Publisher: Geological Society of London
Date: 24-10-2018
DOI: 10.1144/SP483.14
Publisher: Elsevier BV
Date: 03-2014
Publisher: Elsevier BV
Date: 11-2021
Publisher: Elsevier BV
Date: 08-2020
Publisher: Elsevier BV
Date: 04-2022
Publisher: Wiley
Date: 18-04-2013
DOI: 10.1111/TER.12043
Publisher: Elsevier BV
Date: 04-2022
Publisher: Geological Society of America
Date: 1983
Publisher: Springer Science and Business Media LLC
Date: 06-03-2023
DOI: 10.1038/S43247-023-00731-7
Abstract: The composition and origin of Earth’s earliest continental crust remains enigmatic due to the absence of Hadean ( Ga) age rocks. Here we address this question by using machine learning to examine the provenance of the 4.4–3.3 Ga Jack Hills zircons, which constitute the best archive of Earth’s earliest continental crust. Our results reveal that although some Jack Hills zircons may be derived from trondhjemite-tonalite-granodiorite series rocks, which were common during the Archean (4–2.5 Ga), most (as high as ~70%) are sourced from igneous (I-) and sedimentary (S-) type granites. This finding provides clear evidence for rocks other than the trondhjemite-tonalite-granodiorite suite in the Earth’s earliest continental crust. Considering that I- and S-type granites are typical of modern convergent plate margins, the presence of a high proportion of Jack Hills zircons from these rocks supports the operation of a horizontal, mobile-lid tectonic regime in the early Earth.
Publisher: Geological Society of America
Date: 21-06-2022
DOI: 10.1130/G50183.1
Publisher: Elsevier BV
Date: 05-2012
Publisher: Geological Society of America
Date: 08-01-2016
DOI: 10.1130/B31371.1
Publisher: Springer Science and Business Media LLC
Date: 23-09-2015
DOI: 10.1038/SREP14289
Abstract: New geochronological and geochemical data on magmatic activity from the India-Asia collision zone enables recognition of a distinct magmatic flare-up event that we ascribe to slab breakoff. This tie-point in the collisional record can be used to back-date to the time of initial impingement of the Indian continent with the Asian margin. Continental arc magmatism in southern Tibet during 80–40 Ma migrated from south to north and then back to south with significant mantle input at 70–43 Ma. A pronounced flare up in magmatic intensity (including ignimbrite and mafic rock) at ca. 52–51 Ma corresponds to a sudden decrease in the India-Asia convergence rate. Geological and geochemical data are consistent with mantle input controlled by slab rollback from ca. 70 Ma and slab breakoff at ca. 53 Ma. We propose that the slowdown of the Indian plate at ca. 51 Ma is largely the consequence of slab breakoff of the subducting Neo-Tethyan oceanic lithosphere, rather than the onset of the India-Asia collision as traditionally interpreted, implying that the initial India-Asia collision commenced earlier, likely at ca. 55 Ma.
Publisher: Elsevier BV
Date: 12-2015
Publisher: Wiley
Date: 17-02-2022
DOI: 10.1002/ECY.3614
Abstract: Seventy five percent of the world's food crops benefit from insect pollination. Hence, there has been increased interest in how global change drivers impact this critical ecosystem service. Because standardized data on crop pollination are rarely available, we are limited in our capacity to understand the variation in pollination benefits to crop yield, as well as to anticipate changes in this service, develop predictions, and inform management actions. Here, we present CropPol, a dynamic, open, and global database on crop pollination. It contains measurements recorded from 202 crop studies, covering 3,394 field observations, 2,552 yield measurements (i.e., berry mass, number of fruits, and fruit density [kg/ha], among others), and 47,752 insect records from 48 commercial crops distributed around the globe. CropPol comprises 32 of the 87 leading global crops and commodities that are pollinator dependent. Malus domestica is the most represented crop (32 studies), followed by Brassica napus (22 studies), Vaccinium corymbosum (13 studies), and Citrullus lanatus (12 studies). The most abundant pollinator guilds recorded are honey bees (34.22% counts), bumblebees (19.19%), flies other than Syrphidae and Bombyliidae (13.18%), other wild bees (13.13%), beetles (10.97%), Syrphidae (4.87%), and Bombyliidae (0.05%). Locations comprise 34 countries distributed among Europe (76 studies), North America (60), Latin America and the Caribbean (29), Asia (20), Oceania (10), and Africa (7). S ling spans three decades and is concentrated on 2001–2005 (21 studies), 2006–2010 (40), 2011–2015 (88), and 2016–2020 (50). This is the most comprehensive open global data set on measurements of crop flower visitors, crop pollinators and pollination to date, and we encourage researchers to add more datasets to this database in the future. This data set is released for non‐commercial use only. Credits should be given to this paper (i.e., proper citation), and the products generated with this database should be shared under the same license terms (CC BY‐NC‐SA).
Publisher: The Royal Society
Date: 10-2018
Abstract: The secular evolution of the Earth's crust is marked by a profound change in average crustal chemistry between 3.2 and 2.5 Ga. A key marker for this change is the transition from Archaean sodic granitoid intrusions of the tonalite–trondhjemite–granodiorite (TTG) series to potassic (K) granitic suites, akin (but not identical) to I-type granites that today are associated with subduction zones. It remains poorly constrained as to how and why this change was initiated and if it holds clues about the geodynamic transition from a pre-plate tectonic mode, often referred to as stagnant lid, to mobile plate tectonics. Here, we combine a series of proposed mechanisms for Archaean crustal geodynamics in a single model to explain the observed change in granitoid chemistry. Numeric modelling indicates that upper mantle convection drives crustal flow and subsidence, leading to profound ersity in lithospheric thickness with thin versus thick proto-plates. When convecting asthenospheric mantle interacts with lower lithosphere, scattered crustal drips are created. Under increasing P-T conditions, partial melting of hydrated meta-basalt within these drips produces felsic melts that intrude the overlying crust to form TTG. Dome structures, in which these melts can be preserved, are a positive diapiric expression of these negative drips. Transitional TTG with elevated K mark a second evolutionary stage, and are blends of subsided and remelted older TTG forming K-rich melts and new TTG melts. Ascending TTG-derived melts from asymmetric drips interact with the asthenospheric mantle to form hot, high-Mg sanukitoid. These melts are small in volume, predominantly underplated, and their heat triggered melting of lower crustal successions to form higher-K granites. Importantly, this evolution operates as a disseminated process in space and time over hundreds of millions of years (greater than 200 Ma) in all cratons. This focused ageing of the crust implies that compiled geochemical data can only broadly reflect geodynamic changes on a global or even craton-wide scale. The observed change in crustal chemistry does mark the lead up to but not the initiation of modern-style subduction. This article is part of a discussion meeting issue ‘Earth dynamics and the development of plate tectonics’.
Publisher: Elsevier BV
Date: 03-2020
Publisher: Oxford University Press (OUP)
Date: 30-08-2022
DOI: 10.1093/PETROLOGY/EGAC084
Abstract: The trace element contents of zircon can provide unique insights into tectonothermal events, however, interpreting these data and identifying correlations with specific magmatic/metamorphic events can be challenging. This limits our ability to construct temporally constrained petrogenetic histories of complex metamorphic terranes. Unlocking the information that the rare earth element (REE) patterns of zircon contain is difficult because of the need to quantify differences. We have parametrised the shape of zircon REE patterns in terms of three independent parameters: average abundance, slope, and curvature. Quantifying REE patterns using independent shape parameters is similar to the use of REE ratios but is an improvement as (1) it uses information from all 14 REE rather than just two (2) the use of two independent parameters (e.g. slope and curvature) is a more robust discriminant than the use of a single ratio and (3) subtle variations in shape are easily distinguished enabling trends in the REE patterns of large datasets to be identified. Quantitative models were constructed showing how the shapes of the REE patterns of zircon change due to the co-crystallisation of other metamorphic minerals (monazite, apatite, and garnet). Diagnostic changes in shape enable the REE contents of zircon crystals or crystal zones to be accurately related to the growth of specific minerals and hence metamorphic events. The results were used to interpret the REE patterns of zircons from high-grade metamorphic terranes, which have experienced multiple deformation events (Val Malenco, Italy Betic Cordillera, Spain Seram, Indonesia Lewisian Gneiss Complex, Scotland Napier Complex, East Antarctica) and clearly identified zircon that crystallised in the presence of garnet. Quantitative comparison enabled zircon that crystallised prior to, synchronously with, or after garnet to be identified. Similar models can be used to interpret the REE patterns of monazite. This allows the relative timing of the growth of these minerals to be accurately constrained, which given the importance of zircon for geochronology and garnet for geobarometry has the potential to provide insights into the evolution of a metamorphic event.
Publisher: The Royal Society
Date: 10-2018
Abstract: Less than 25% of the volume of the juvenile continental crust preserved today is older than 3 Ga, there are no known rocks older than approximately 4 Ga, and yet a number of recent models of continental growth suggest that at least 60–80% of the present volume of the continental crust had been generated by 3 Ga. Such models require that large volumes of pre-3 Ga crust were destroyed and replaced by younger crust since the late Archaean. To address this issue, we evaluate the influence on the rock record of changing the rates of generation and destruction of the continental crust at different times in Earth's history. We adopted a box model approach in a numerical model constrained by the estimated volumes of continental crust at 3 Ga and the present day, and by the distribution of crust formation ages in the present-day crust. The data generated by the model suggest that new continental crust was generated continuously, but with a marked decrease in the net growth rate at approximately 3 Ga resulting in a temporary reduction in the volume of continental crust at that time. Destruction rates increased dramatically around 3 billion years ago, which may be linked to the widespread development of subduction zones. The volume of continental crust may have exceeded its present value by the mid/late Proterozoic. In this model, about 2.6–2.3 times of the present volume of continental crust has been generated since Earth's formation, and approximately 1.6–1.3 times of this volume has been destroyed and recycled back into the mantle. This article is part of a discussion meeting issue ‘Earth dynamics and the development of plate tectonics'.
Publisher: Elsevier BV
Date: 10-1994
Publisher: The Royal Society
Date: 10-2018
Abstract: Plate tectonics, involving a globally linked system of lateral motion of rigid surface plates, is a characteristic feature of our planet, but estimates of how long it has been the modus operandi of lithospheric formation and interactions range from the Hadean to the Neoproterozoic. In this paper, we review sedimentary, igneous and metamorphic proxies along with palaeomagnetic data to infer both the development of rigid lithospheric plates and their independent relative motion, and conclude that significant changes in Earth behaviour occurred in the mid- to late Archaean, between 3.2 Ga and 2.5 Ga. These data include: sedimentary rock associations inferred to have accumulated in passive continental margin settings, marking the onset of sea-floor spreading the oldest foreland basin deposits associated with lithospheric convergence a change from thin, new continental crust of mafic composition to thicker crust of intermediate composition, increased crustal reworking and the emplacement of potassic and peraluminous granites, indicating stabilization of the lithosphere replacement of dome and keel structures in granite-greenstone terranes, which relate to vertical tectonics, by linear thrust imbricated belts the commencement of temporally paired systems of intermediate and high dT/dP gradients, with the former interpreted to represent subduction to collisional settings and the latter representing possible hinterland back-arc settings or ocean plateau environments. Palaeomagnetic data from the Kaapvaal and Pilbara cratons for the interval 2780–2710 Ma and from the Superior, Kaapvaal and Kola-Karelia cratons for 2700–2440 Ma suggest significant relative movements. We consider these changes in the behaviour and character of the lithosphere to be consistent with a gestational transition from a non-plate tectonic mode, arguably with localized subduction, to the onset of sustained plate tectonics. This article is part of a discussion meeting issue ‘Earth dynamics and the development of plate tectonics'.
Publisher: Elsevier BV
Date: 2021
Publisher: Elsevier BV
Date: 04-2023
Publisher: Elsevier BV
Date: 08-2000
Publisher: Elsevier BV
Date: 11-2020
Publisher: Elsevier BV
Date: 02-2021
Publisher: Geological Society of London
Date: 16-10-2019
DOI: 10.1144/JGS2019-051
Publisher: Elsevier BV
Date: 12-2016
Publisher: Geological Society of London
Date: 09-2012
Publisher: Geological Society of America
Date: 25-02-2021
DOI: 10.1130/B35778.1
Publisher: American Geophysical Union (AGU)
Date: 27-07-2010
DOI: 10.1029/2009TC002600
Publisher: Society of Economic Geologists
Date: 30-09-2013
Publisher: Elsevier BV
Date: 08-2018
Publisher: Elsevier BV
Date: 06-2021
Publisher: Geological Society of America
Date: 08-10-2021
DOI: 10.1130/G49238.1
Publisher: Elsevier BV
Date: 05-2017
Publisher: Elsevier BV
Date: 05-2017
Publisher: Elsevier BV
Date: 07-2019
Publisher: Elsevier BV
Date: 09-2009
Publisher: Informa UK Limited
Date: 06-1989
Publisher: Research Square Platform LLC
Date: 16-05-2023
DOI: 10.21203/RS.3.RS-2881098/V1
Abstract: How Earth switched from any earlier regimes such as plume-lid tectonics to plate tectonics remains an unresolved issue in Earth sciences. We report early Neoarchean (~ 2.77–2.68 Ga) metavolcanic rocks, including older calc-alkaline basaltic-andesitic rocks in the southwest but younger tholeiitic rocks in the northeast, from Jiaobei terrane, North China Craton. Genetic studies and thermodynamic and trace element modeling demonstrate that the tholeiitic magmas originated from deeper and unmodified mantle sources (~ 1600 ℃ and ~ 3.5 GPa), relative to the shallower and metasomatized mantle sources (~ 1450 ℃ and ~ 2.2 GPa) of calc-alkaline magmas. Geochemical changes indicate that the mantle sources became isotopically enriched but less metasomatized from southwest to northeast. These data suggest an early Neoarchean plate subduction-induced deep mantle upwelling regime. We further depict a potential geodynamic framework for the early Neoarchean Earth involving active interaction of plate subduction and deep mantle upwelling, which possibly changed the thermal evolutionary trajectory of the Earth and accelerated the arrival of global plate tectonics.
Publisher: Elsevier BV
Date: 2021
Publisher: Geological Society of London
Date: 11-1995
Publisher: American Geophysical Union (AGU)
Date: 12-2018
DOI: 10.1029/2018JB016353
Publisher: Elsevier BV
Date: 06-2008
Publisher: Elsevier BV
Date: 03-2007
Publisher: American Geophysical Union (AGU)
Date: 15-09-2011
DOI: 10.1029/2011TC002864
Publisher: Elsevier BV
Date: 03-2016
Publisher: Springer Science and Business Media LLC
Date: 21-12-2016
Publisher: Geological Society of London
Date: 09-2004
Publisher: Elsevier BV
Date: 08-2019
Publisher: American Geophysical Union (AGU)
Date: 04-08-2022
DOI: 10.1029/2021GL096817
Abstract: The geological evolution of orogens is the sum of events related to both their cycle of generation as well as features inherited from their basement units. The Himalayan Orogen provides a well‐constrained Cenozoic history of active plate convergence and orogenic processes overprinting an early Paleozoic orogen. A total of 1,627 Himalayan leucogranite zircons were depth‐profiled showing high resolution (0.6 μm) internal age structures. Zircon rim ages record a detailed and complex history of melting and deformation, postdating the North Indo‐Australie Orogen (ca. 490–460 Ma) documented by the zircon core age data. An interesting finding is the inconsistency of age groups between detrital zircons in the Himalaya and inherited cores of leucogranite zircons, re‐evaluating the argument that leucogranites are purely derived from melting of metasedimentary rocks. Variations in the thickness of zircon rims corresponds with changing Cenozoic orogenic stages with rims thicker than 4 μm indicating the extensional regime.
Publisher: Elsevier BV
Date: 03-2001
Publisher: Elsevier BV
Date: 12-2005
Publisher: Oxford University Press (OUP)
Date: 15-03-2013
Publisher: Geological Society of America
Date: 12-10-2020
DOI: 10.1130/G48308.1
Abstract: Late Tonian to Cambrian sedimentary sequences in northwestern India and South China provide vital evidence for modeling their paleogeographic linkage, including their juxtaposition and subsequent separation during the transition from the Rodinia to the Gondwana supercontinents. Similarities in lithostratigraphy and detrital zircon U-Pb-Hf-O isotopic characteristics in the late Tonian sedimentary units from both regions underline a common provenance. A substantial decrease in zircon δ18O values from super- to sub-mantle compositions and simultaneous increase in the zircon εHf(t) values in South China and northwestern India for the 800–700 Ma time window suggest a common Neoproterozoic extensional magmatic event, corresponding with the Rodinia breakup. A distinct change in sedimentary provenance is noted during the Cryogenian period. Sedimentation along the northwestern margin of India for the remainder of the Neoproterozoic encompasses large volumes of clastic detritus dominated by old zircon ages, derived inboard from the Indian craton. In contrast, contemporaneous sedimentary units in the Yangtze region of South China are dominated by Neoproterozoic zircons. The detrital zircon age data underline a close paleogeographic linkage between northwestern India and South China (Yangtze and Cathaysia regions) in the Rodinia supercontinent configuration and argue for their separation through continental rifting during the Cryogenian. Northwestern India developed into a passive margin, whereas the South China block partially rifted, rotated, and migrated dextrally along the Gondwana margin toward northeastern India and Western Australia, such that the Cathaysia block continued to receive detritus from Gondwana continental regions.
Publisher: Elsevier BV
Date: 2022
Publisher: Wiley
Date: 07-2000
Publisher: Elsevier BV
Date: 05-2022
Publisher: Geological Society of America
Date: 05-11-2020
DOI: 10.1130/B35380.1
Abstract: New age data for the Baoban Complex, South China establishes that it lay outboard of western Laurentia in the early Mesoproterozoic but was not part of the Cathaysia Block, with which it is traditional linked, until the mid-Paleozoic. Our geochronology data for detrital zircon and authigenic monazite grains from metasedimentary rocks indicate accumulation between ca. 1.55 Ga and 1.45 Ga for the Gezhencun succession of the Baoban Complex and ca. 1.45 Ga and 1.30 Ga for the Ewenling succession. The former unit is dominated by detrital zircon populations between 1900 Ma and 1500 Ma with two peaks at 1780 Ma and 1580 Ma. The Ewenling succession has detrital zircon peaks at 1720 Ma and 1450 Ma. Newly discovered gneissic granites were emplaced at 1550 Ma and intruded by 1450 Ma leucogranite dykes that are coeval with 1460–1430 Ma bimodal magmatism. The whole Baoban Complex was metamorphosed over the range of 1.3–0.9 Ga based on ages of authigenic zircon and monazite. Depositional ages of metasedimentary rocks are coeval with successions of the Belt-Purcell Basin, western Laurentia. Detrital zircon from the two regions have similar age populations and Lu-Hf compositions, and display a synchronous provenance shift at ca. 1.45 Ga. Basement lithologies on Hainan Island range in age from ca. 1.55–1.43 Ga and underwent metamorphism during 1.3–0.9 Ga. This is younger than basement rocks on the mainland of the Cathaysia Block in South China, suggesting the two regions are spatially unrelated at this time and hence the Mesoproterozoic record of the island cannot constrain the location of the Cathaysia Block in the Nuna and Rodinia supercontinents.
Publisher: Elsevier BV
Date: 11-2002
Publisher: Elsevier BV
Date: 12-2021
Publisher: Elsevier BV
Date: 09-2015
Publisher: Informa UK Limited
Date: 12-1999
Publisher: Geological Society of America
Date: 08-1999
Publisher: Elsevier BV
Date: 2019
Publisher: Elsevier BV
Date: 10-2001
Publisher: Elsevier BV
Date: 04-2022
Publisher: American Geophysical Union (AGU)
Date: 07-2020
DOI: 10.1029/2019JB019260
Abstract: Numerous late Paleoproterozoic to early Mesoproterozoic mafic magmatic rocks are exposed in the southwestern Yangtze Block, corresponding to early breakup of the Nuna supercontinent. Geochronological data reveal three episodes of mafic magmatism at ~1,740, 1,700, and 1,500 Ma. The two older generations have MORB‐like Nb/Ta ratios and superchondritic Nd‐Hf isotopes, indicating that they were likely derived from partial melting of asthenospheric mantle. In contrast, the ~1,500 Ma mafic rocks possess OIB‐like Nb/Ta (16.7–19.1) and Zr/Hf (41.0–45.1) ratios, ε Nd ( t ) values (−0.8 to +0.1), and ε Hf ( t ) values (−3.3 to +8.4), suggesting that they originated from a mantle plume. These three pulses of mafic magmatic activity in the Yangtze Block have geochemical features (such as TiO 2 contents, Nb/Y, and La/Yb values), similar to coeval mafic rocks in Siberia and Laurentia, consistent with detrital zircon provenance studies, which show a spatial linkage of the Yangtze Block with northern Laurentia in the Nuna configuration. Taking all synchronous mafic magmatism into account, a mantle plume beneath southern Siberia was considered to be initiated at ~1,750 Ma forming a broad region of mafic magmatism that extended into the Yangtze Block as well as beneath northern Laurentia and resulted in lithospheric extension. The Yangtze Block was possibly the nearest neighbor to northwestern Siberia at ~1,500 Ma and subsequently drifted from the Nuna supercontinent induced by the ~1,500 Ma Kuonamka mantle plume, heralding a period of limited magmatic activity and tectonic quiescence in the Yangtze Block that extended throughout the remainder of the Mesoproterozoic.
Publisher: Elsevier BV
Date: 08-2023
Publisher: Geological Society of London
Date: 09-2004
Publisher: Elsevier BV
Date: 11-2007
Publisher: Springer Science and Business Media LLC
Date: 15-07-2014
Publisher: Elsevier BV
Date: 04-1990
Publisher: American Geophysical Union (AGU)
Date: 07-2021
DOI: 10.1029/2020JB021217
Abstract: The magmatic differentiation of cooling arc lavas on their way to the surface is dominated by fractional crystallization, which predominantly occurs at lower crustal arc levels (25–40 km) at continental margins. The magmatic storage in the deep crust is complex and remote, and rarely studied compared to shallow magma fractionation, but carries key information for the formation and evolution of the lower continental crust. At convergent continental margins, mantle‐derived melts must pass through a complex system of rocks in the lower arc crust. In particular, melts inevitably transition through deep “hot” (melt‐rich) or “cold” (i.e., water‐rich) zones, collectively termed here lower crustal arc zones (LoCAZ) to account for both scenarios. Their role in driving melt modification, including formation and oxidation of calc‐alkaline suites, remains unclear. Here we report stable Fe isotope compositions of 40 well‐characterized Neoproterozoic mafic dikes from the northwestern margin of the Yangtze Block, representing three stages of continental arc evolution. Rocks from the Tongde dikes display strong correlations between δ 57 Fe values and trace element indices of garnet fractionation (e.g., high La/Yb and depleted heavy REE patterns). An increase in heavy Fe isotopes with garnet fractionation indicates a redox‐filtering of melts through LoCAZ. We thus propose that retention of Fe 2+ in deep crustal garnet is one driver for elevated f O 2 and the calc‐alkaline trend in continental margin rocks. With continental arc rocks being on average more oxidized than intra‐oceanic arc lavas, garnet redox‐filtering may be an additive oxidizer in thicker arc crust. The Tongde dike swarms may represent a rare, volumetrically small, direct ex le of melts ejected out of the lower arc crust. The complex mixing and mingling of melts reported for most arcs and their plutons may obscure this redox process contributing to continental crust growth.
Publisher: Geological Society of London
Date: 25-11-2014
DOI: 10.1144/JGS2012-143
Publisher: Elsevier BV
Date: 03-2017
Publisher: Elsevier BV
Date: 12-2008
Publisher: Elsevier BV
Date: 07-2023
Publisher: Elsevier BV
Date: 09-2023
Publisher: Elsevier BV
Date: 03-2023
Publisher: Elsevier BV
Date: 1999
Publisher: Elsevier BV
Date: 05-2022
Publisher: Geological Society of America
Date: 21-03-2014
DOI: 10.1130/G35363.1
Publisher: American Journal of Science (AJS)
Date: 04-1999
Publisher: Geological Society of America
Date: 06-06-2013
DOI: 10.1130/G34520.1
Publisher: Elsevier BV
Date: 06-2019
Publisher: Elsevier BV
Date: 11-2018
Publisher: Elsevier BV
Date: 08-2015
Publisher: Geological Society of America
Date: 16-08-2016
DOI: 10.1130/GSATG272A.1
Publisher: Elsevier BV
Date: 10-2016
Publisher: Elsevier BV
Date: 04-2022
Publisher: Elsevier BV
Date: 09-2015
Publisher: Springer Science and Business Media LLC
Date: 25-11-2022
DOI: 10.1038/S41597-022-01730-7
Abstract: This article presents a resource for automated search, extraction and collation of geochemical and geochronological data from the Figshare repository using web scraping code. To answer fundamental questions about the Earth’s evolution, such as spatial and temporal evolution and interrelationships between the planet’s solid and surficial reservoirs, researchers must utilize global geochemical datasets. Due to the volume of data being published, these datasets become quickly outdated. We present a resource that allows researchers to rapidly curate and update their own databases from existing published data. We use open-source Python code to web scrape the Figshare repository for journal supplementary files using the application programming interface, allowing for the collection and download of hundreds of supplementary files and metadata in minutes. Use of this web scraping tool is demonstrated here by collation of a zircon geochronology and chemistry database of ,000 analyses. The database is consistent in reproducing trends in other published zircon compilations. Providing a resource for automated collection of Figshare data files will encourage data sharing and reuse.
Publisher: Elsevier BV
Date: 03-2020
Publisher: Elsevier BV
Date: 07-2012
Publisher: Springer Science and Business Media LLC
Date: 23-06-2021
DOI: 10.1038/S41467-021-24139-Z
Abstract: Constraining thickness and geothermal gradient of Archean continental crust are crucial to understanding geodynamic regimes of the early Earth. Archean crust-sourced tonalitic–trondhjemitic–granodioritic gneisses are ideal lithologies for reconstructing the thermal state of early continental crust. Integrating experimental results with petrochemical data from the Eastern Block of the North China Craton allows us to establish temporal–spatial variations in thickness, geothermal gradient and basal heat flow across the block, which we relate to cooling mantle potential temperature and resultant changing geodynamic regimes from vertical tectonics in the late Mesoarchean (~2.9 Ga) to plate tectonics with hot subduction in the early to late Neoarchean (~2.7–2.5 Ga). Here, we show the transition to a plate tectonic regime plays an important role in the rapid cooling of the mantle, and thickening and strengthening of the lithosphere, which in turn prompted stabilization of the cratonic lithosphere at the end of the Archean.
Publisher: Elsevier BV
Date: 06-2007
Publisher: Springer Science and Business Media LLC
Date: 07-07-2021
DOI: 10.1038/S41467-021-24422-Z
Abstract: Initiation of Mariana-type oceanic subduction zones requires rheologically strong oceanic lithosphere, which developed through secular cooling of Earth’s mantle. Here, we report a 518 Ma Mariana-type subduction initiation ophiolite from northern Tibet, which, along with compilation of similar ophiolites through Earth history, argues for the establishment of the modern plate tectonic regime by the early Cambrian. The ophiolite was formed during the subduction initiation of the Proto-Tethys Ocean that coincided with slab roll-back along the southern and western Gondwana margins at ca. 530-520 Ma. This global tectonic re-organization and the establishment of modern plate tectonic regime was likely controlled by secular cooling of the Earth, and facilitated by enhanced lubrication of subduction zones by sediments derived from widespread surface erosion of the extensive mountain ranges formed during Gondwana assembly. This time also corresponds to extreme events recorded in climate and surface proxies that herald formation of the contemporary Earth.
Publisher: Geological Society of America
Date: 03-1993
Publisher: Elsevier BV
Date: 10-2013
Publisher: American Geophysical Union (AGU)
Date: 12-2014
DOI: 10.1002/2014TC003748
Publisher: Elsevier BV
Date: 02-2015
Publisher: Elsevier BV
Date: 07-2019
Publisher: Elsevier BV
Date: 04-2021
Publisher: Virtual Explorer Pty Ltd.
Date: 2006
Publisher: Elsevier BV
Date: 06-2018
Publisher: Elsevier BV
Date: 02-2000
Publisher: Elsevier BV
Date: 08-2018
Publisher: American Association for the Advancement of Science (AAAS)
Date: 30-10-2020
Abstract: Ocean floor lavas from an active spreading ridge keep a geochemical memory of an Early Cretaceous subduction zone.
Publisher: Elsevier BV
Date: 12-2015
Publisher: Elsevier BV
Date: 04-2015
Publisher: Elsevier BV
Date: 10-2023
Publisher: Elsevier BV
Date: 10-2017
Publisher: American Geophysical Union (AGU)
Date: 07-03-2023
DOI: 10.1029/2023GL102979
Abstract: Paleogeographic reconstruction of Precambrian terranes reworked by Phanerozoic orogens (e.g., the Tibetan Plateau) results in complex lithotectonic relations due to intracrustal reworking by tectonothermal events. Detrital zircon rare earth element (REE) databases at global (global major river sands) and regional (the Gangdese Mountains, southern Tibet) scales reveal trends in and Eu/Eu* that effectively record the crustal evolution of the source, including crustal thickness and redox state of the magma that generated the zircons. Regional comparisons of these chemical markers provide a new approach for paleogeographic reconstructions that we apply to study the origin of the Lhasa terrane, southern Tibet. Using Precambrian to early Paleozoic sedimentary and igneous rocks in the Lhasa terrane and compiling detrital zircon analyses from the northern margin of Gondwana, we show that the Lhasa terrane had an African affinity in the Rodinia–Gondwana supercontinent cycles (ca. 1.4–0.4 Ga).
Publisher: Elsevier BV
Date: 09-1999
Publisher: Geological Society of America
Date: 02-2010
DOI: 10.1130/G30450.1
Publisher: Elsevier BV
Date: 05-2023
Publisher: Elsevier BV
Date: 09-2018
Publisher: Elsevier BV
Date: 10-2010
Publisher: Elsevier BV
Date: 05-2020
Publisher: Frontiers Media SA
Date: 06-08-2020
Publisher: Geological Society of America
Date: 20-08-2019
DOI: 10.1130/G46239.1
Abstract: Thermomechanical models of mantle convection and melting in an inferred hotter Archean Earth show the emergence of pressure-temperature (P-T) regimes that resemble present-day plate tectonic environments yet developed within a non–plate tectonics regime. The models’ P-T gradients are compatible with those inferred from evolving tonalite-trondhjemite-granodiorite series rocks and the paired metamorphic belt record, supporting the feasibility of ergent and convergent tectonics within a mobilized, yet laterally continuous, lithospheric lid. “Hot” P-T gradients of 10–20 °C km–1 form along asymmetric lithospheric drips, then migrate to areas of deep lithospheric downwelling within ∼300–500 m.y., where they are overprinted by high-pressure warm and, later, cold geothermal signatures, up to ∼8 °C km–1. Comparisons with the crustal production and reworking record suggest that this regime emerged in the Hadean.
Publisher: Research Square Platform LLC
Date: 10-2021
DOI: 10.21203/RS.3.RS-948127/V1
Abstract: The redox evolution of Archean mantle impacted Earth differentiation, mantle melting and the nature of chemical equilibrium between mantle, ocean and atmosphere of the early Earth. However, how and why it varies with time remain controversial. Archean mantle-derived volcanic rocks, especially basalts are ideal lithologies for reconstructing the mantle redox state. Here we show that the ~3.8-2.5 Ga basalts from fourteen cratons are sub ided geochemically into two groups, B-1, showing incompatible element depleted and modern mid-ocean ridge basalt-like features ((Nb/La)PM ≥ 0.75) and B-2 ((Nb/La)PM 0.75), characterized by modern island arc basalt-like features. Our updated V-Ti redox proxy indicates the Archean upper mantle was more reducing than today, and that there was a significant redox heterogeneity between ambient and modified mantle presumably related to crustal recycling, perhaps via plate subduction, as shown by B-1 and B-2 magmas, respectively. The oxygen fugacity of modified mantle exhibits a ~1.5-2.0 log units increase over ~3.8-2.5 Ga, whereas the ambient mantle becomes more and more heterogeneous with respect to redox, apart from a significant increase at ~2.7 Ga. These findings are coincident with the increase in the proportions of crustal recycling-related lithologies with associated enrichment of associated incompatible elements (e.g., Th/Nb), indicating that increasing recycling played a crucial role on the secular oxidation of Archean upper mantle.
Publisher: American Geophysical Union (AGU)
Date: 08-2020
DOI: 10.1029/2020TC006071
Publisher: American Association for the Advancement of Science (AAAS)
Date: 14-01-2011
Abstract: Island arc rocks provide a better constraint on when the continental crust was generated.
Publisher: Elsevier BV
Date: 10-2021
Publisher: Elsevier BV
Date: 04-2022
Publisher: Elsevier BV
Date: 11-2014
Publisher: Springer Science and Business Media LLC
Date: 02-12-2020
Publisher: Elsevier BV
Date: 04-2016
Publisher: Elsevier BV
Date: 12-2016
Publisher: American Geophysical Union (AGU)
Date: 05-2018
DOI: 10.1002/2018JB015582
Publisher: Elsevier BV
Date: 03-2017
Publisher: Elsevier BV
Date: 03-2021
Publisher: Elsevier BV
Date: 12-2013
Publisher: Elsevier BV
Date: 03-2021
Publisher: Elsevier BV
Date: 09-2022
Publisher: Geological Society of America
Date: 1994
Publisher: American Geophysical Union (AGU)
Date: 15-11-2021
DOI: 10.1029/2021GL095192
Abstract: The evolution of the western Kunlun‐Pamir region involved the opening and closing of several branches of the Paleo‐Tethys Ocean, although the specific timing of these events is poorly constrained. Here, we present a synthesis of sedimentary, magmatic, and metamorphic records associated from the Mazar‐Kangxiwa suture zone in the western Kunlun‐Pamir that is generally regarded as the main Paleo‐Tethys Ocean suture. These data show that the Paleo‐Tethyan oceanic basin opened at ca. 340 Ma and closed by ca. 250 Ma, and there is no record of a magmatic arc between ca. 300–250 Ma. The absence of a magmatic arc was a result of oceanic crust underthrusting, rather than oceanic subduction, which is consistent with a narrow back‐arc basin. Our study provides an important ex le of how an oceanic basin opened and closed without oceanic subduction, and highlights a potential mechanism to account for the absence of a magmatic arc.
Publisher: Elsevier BV
Date: 05-2023
Publisher: Elsevier BV
Date: 07-2022
Publisher: Elsevier BV
Date: 11-2017
Publisher: Elsevier BV
Date: 10-2014
Publisher: Elsevier BV
Date: 07-2013
Publisher: Frontiers Media SA
Date: 24-09-2020
Publisher: Elsevier BV
Date: 04-2017
Publisher: American Geophysical Union (AGU)
Date: 08-2018
DOI: 10.1029/2018TC005130
Publisher: Geological Society of America
Date: 31-10-2013
DOI: 10.1130/B30722.1
Publisher: Geological Society of America
Date: 06-2014
DOI: 10.1130/G35402.1
Publisher: Elsevier BV
Date: 05-2022
Publisher: American Geophysical Union (AGU)
Date: 08-2015
DOI: 10.1002/2015TC003835
Publisher: Elsevier BV
Date: 04-2019
Publisher: Elsevier BV
Date: 05-2022
Publisher: Elsevier BV
Date: 2019
Publisher: American Geophysical Union (AGU)
Date: 08-1992
DOI: 10.1029/92TC00471
Publisher: Springer Science and Business Media LLC
Date: 14-12-2017
Publisher: Springer Science and Business Media LLC
Date: 21-11-2022
DOI: 10.1038/S41467-022-34826-0
Abstract: Generation of continental crust in collision zones reflect the interplay between oceanic subduction and continental collision. The Gangdese continental crust in southern Tibet developed during subduction of the Neo-Tethyan oceanic slab in the Mesozoic prior to reworking during the India-Asia collision in the Cenozoic. Here we show that continental arc magmatism started with fractional crystallization to form cumulates and associated medium-K calc-alkaline suites. This was followed by a period commencing at ~70 Ma dominated by remelting of pre-existing lower crust, producing more potassic compositions. The increased importance of remelting coincides with an acceleration in the convergence rate between India and Asia leading to higher basaltic flow into the Asian lithosphere, followed by convergence deceleration due to slab breakoff, enabling high heat flow and melting of the base of the arc. This two-stage process of accumulation and remelting leads to the chemical maturation of juvenile continental crust in collision zones, strengthening crustal stratification.
Publisher: Geological Society of America
Date: 1989
Publisher: Elsevier BV
Date: 03-2022
Publisher: Elsevier BV
Date: 2019
Publisher: Elsevier BV
Date: 05-2020
Publisher: Elsevier BV
Date: 03-2021
Publisher: Elsevier BV
Date: 09-2021
Publisher: American Journal of Science (AJS)
Date: 03-2002
Publisher: Elsevier BV
Date: 12-2020
Publisher: Geological Society of America
Date: 10-2012
DOI: 10.1130/G32945.1
Publisher: Geological Society of London
Date: 2004
Publisher: International Union of Geological Sciences
Date: 12-2019
Publisher: Elsevier BV
Date: 02-2020
Publisher: Springer Science and Business Media LLC
Date: 02-2003
Publisher: Elsevier BV
Date: 08-2023
Publisher: Elsevier BV
Date: 03-2010
Publisher: American Geophysical Union (AGU)
Date: 12-2007
DOI: 10.1029/2007TC002099
Publisher: Springer Science and Business Media LLC
Date: 18-12-2015
DOI: 10.1038/SREP17236
Abstract: New geochronological and geochemical data on magmatic activity from the India-Asia collision zone enables recognition of a distinct magmatic flare-up event that we ascribe to slab breakoff. This tie-point in the collisional record can be used to back-date to the time of initial impingement of the Indian continent with the Asian margin. Continental arc magmatism in southern Tibet during 80–40 Ma migrated from south to north and then back to south with significant mantle input at 70–43 Ma. A pronounced flare up in magmatic intensity (including ignimbrite and mafic rock) at ca. 52–51 Ma corresponds to a sudden decrease in the India-Asia convergence rate. Geological and geochemical data are consistent with mantle input controlled by slab rollback from ca. 70 Ma and slab breakoff at ca. 53 Ma. We propose that the slowdown of the Indian plate at ca. 51 Ma is largely the consequence of slab breakoff of the subducting Neo-Tethyan oceanic lithosphere, rather than the onset of the India-Asia collision as traditionally interpreted, implying that the initial India-Asia collision commenced earlier, likely at ca. 55 Ma.
Publisher: Elsevier BV
Date: 02-2010
Publisher: Elsevier BV
Date: 2021
Publisher: American Geophysical Union (AGU)
Date: 10-1984
Publisher: Elsevier BV
Date: 2022
Publisher: Elsevier BV
Date: 2023
Publisher: Geological Society of London
Date: 2009
DOI: 10.1144/SP318.1
Publisher: Geological Society of London
Date: 1991
Publisher: Elsevier BV
Date: 10-2021
Publisher: Elsevier BV
Date: 06-2017
Publisher: American Geophysical Union (AGU)
Date: 05-2015
DOI: 10.1002/2014TC003803
Publisher: Elsevier BV
Date: 02-2020
Publisher: Elsevier BV
Date: 03-2005
Publisher: Geological Society of America
Date: 04-2011
DOI: 10.1130/G31785.1
Publisher: Cambridge University Press (CUP)
Date: 05-1999
DOI: 10.1017/S001675689900254X
Abstract: Mafic granulites from the North China craton can be ided into two textural types, referred to as A- and B-types. A-type mafic granulites display garnet+quartz symplectic coronas, and outcrop in the eastern and western zones of the craton, whereas B-type mafic granulites exhibit orthopyroxene+plagioclase±clinopyroxene symplectites or coronas, and are mainly exposed in the central zone of the craton. Most A-type mafic granulites preserve the prograde (M 1 ), peak (M 2 ) and post-peak near-isobaric cooling (M 3 ) assemblages, which are represented respectively by inclusions of hornblende+plagioclase+quartz, a peak mineralogy of orthopyroxene+clinopyroxene+plagioclase+quartz+garnet, and overprinted by garnet+quartz symplectic coronas. These mineral assemblages and their P–T (pressure-temperature) estimates define anticlockwise P–T evolutionary paths. The B-type mafic granulites preserve the peak (M 1 ), post-peak near-isothermal decompression (M 2 ) and cooling (M 3 ) assemblages, which are represented by the peak assemblage of orthopyroxene+clinopyroxene+plagioclase+quartz+garnet±hornblende, post-peak orthopyroxene+plagioclase±clinopyroxene symplectites or coronas, and later hornblende+plagioclase+magnetite symplectites, respectively. These mineral assemblages and their P–T estimates define clockwise P–T paths. The anticlockwise P–T paths of the A-type mafic granulites in the eastern and western zones of the North China craton are consistent with a model of underplating and intrusion of mantle-derived magmas. In combination with lithological, structural and geochronological data, the eastern and western zones of the North China craton are considered to represent two continental blocks that developed through the interaction of mantle plumes with the lithosphere from the Palaeoarchaean to the Neoarchaean era. The B-type mafic granulites and associated rocks in the central zone represent a magmatic arc that was metamorphosed and deformed during amalgamation of the eastern and western continental blocks in the late Palaeoproterozoic era. The mineral reaction relations and clockwise P–T paths of the B-type mafic granulites from the central zone record the tectonothermal history of the collision that resulted in the final assembly of the North China craton at c . 1800 Ma.
Publisher: Wiley
Date: 10-01-2022
DOI: 10.1111/BRE.12650
Publisher: Elsevier BV
Date: 07-2019
Publisher: Elsevier BV
Date: 02-2005
Publisher: University of Chicago Press
Date: 07-1982
DOI: 10.1086/628692
Publisher: American Association for the Advancement of Science (AAAS)
Date: 02-01-2009
Publisher: Elsevier BV
Date: 08-2020
Publisher: Elsevier BV
Date: 2023
Publisher: Geological Society of America
Date: 26-02-2019
DOI: 10.1130/G45745.1
Publisher: CSIRO Publishing
Date: 2008
DOI: 10.1071/PC080231
Abstract: Most would agree that it is much better to be warned about an impending tsunami when it is many kilometres offshore ? and have time to take life-saving action ? than to find out about it once it looms large on the horizon.
Publisher: Elsevier BV
Date: 06-1987
Publisher: Elsevier BV
Date: 06-2020
Publisher: Geological Society of America
Date: 1991
Publisher: American Geophysical Union (AGU)
Date: 12-2010
DOI: 10.1029/2010TC002750
Publisher: Geological Society of London
Date: 24-10-2015
DOI: 10.1144/SP393.1
Publisher: Elsevier BV
Date: 10-2022
Publisher: Elsevier BV
Date: 02-2023
Publisher: Elsevier BV
Date: 1980
Publisher: Elsevier BV
Date: 04-2020
Publisher: Oxford University Press (OUP)
Date: 23-12-2009
Publisher: The Royal Society
Date: 02-2021
Publisher: Elsevier BV
Date: 02-2022
Publisher: Geological Society of America
Date: 17-08-2016
DOI: 10.1130/G38117.1
Publisher: GeoScienceWorld
Date: 27-03-2022
DOI: 10.2113/2022/6253194
Abstract: The Ortosuu and Uchkuduk regions of the Tianshan orogen contain a volumetrically small series of basaltic rocks erupted primarily during the late Mesozoic-Paleogene. Petrology, chemical composition, and P-T geotherm data from xenoliths within the basalts characterize the nature of the lithospheric mantle beneath this orogenic belt. Two groups of clinopyroxene can be identified from the studied xenoliths based on their Mg# and trace element patterns. Group 1, primitive clinopyroxenes, has lower Mg# (86–90) and LREE-depleted patterns than group 2, depleted clinopyroxenes, which are characterized by a relatively high Mg#, 91–92, and LREE-enriched patterns. The REE distribution in group 1 clinopyroxenes suggests that they were controlled by partial melting, whereas group 2 clinopyroxenes are far more complex involving partial melting degrees of 6–11%, and later metasomatism by carbonatite and/or silicate melts. Coupled P-T estimations from geothermobarometry indicate that the more fertile group 1 xenoliths were probably derived from the uppermost mantle, and the more depleted group 2 xenoliths were likely derived from a depth close to the crust mantle boundary.
Publisher: University of Chicago Press
Date: 09-2017
DOI: 10.1086/693036
Start Date: 06-2002
End Date: 06-2005
Amount: $227,718.00
Funder: Australian Research Council
View Funded ActivityStart Date: 07-2005
End Date: 03-2009
Amount: $300,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 06-2009
End Date: 12-2012
Amount: $580,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 04-2009
End Date: 07-2010
Amount: $800,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 03-2017
End Date: 03-2024
Amount: $2,851,557.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2006
End Date: 12-2006
Amount: $246,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2002
End Date: 12-2002
Amount: $770,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 05-2010
End Date: 12-2013
Amount: $510,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 10-2005
End Date: 10-2006
Amount: $220,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2010
End Date: 12-2010
Amount: $700,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2004
End Date: 12-2004
Amount: $10,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2003
End Date: 12-2004
Amount: $10,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 05-2021
End Date: 06-2023
Amount: $905,654.00
Funder: Australian Research Council
View Funded ActivityStart Date: 03-2011
End Date: 12-2015
Amount: $550,000.00
Funder: Australian Research Council
View Funded Activity