Evolution of Calc-Alkaline to Alkaline Magmatism Through Carboniferous
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And Post-Collision Calc-Alkaline Magmatism in the Qinling Orogenic Belt, Central China, As Documented by Zircon Ages on Granitoid Rocks
Journal of the Geological Societv. London, Vol. 153, 1996, pp. 409-417. Palaeozoic pre- and post-collision calc-alkaline magmatism in the Qinling orogenic belt, central China, as documented by zircon ages on granitoid rocks F. XUE'.*,',A. KRONER', T. REISCHMANN' & F. LERCH' 'Institut fiir Geowissenschaften, Universitat Mainz, 55099 Mainz, Germany 'Department of Geology, Northwest University, 710069 Xi'an, China .'Present address: Department of Geophysical Sciences, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA Abstract: Basedon large-scale reconnaissance mapping, we identifiedtwo calc-alkaline plutonic assemblagesfrom the northern Qinling orogenic belt.central China. The older assemblage of intrusions. closely associated and deformed coevally with their host volcanic arc sequences, seems to represent the fractionation product of basaltic arc magma. It therefore predates the collision of the North China Block with the Central Qinling island-arc system that developed in a SW Pacific-type oceanic domain south of the North China Block. Single-zircon zo7Pb/2'"Pb evaporation dating yielded early to middle Ordovician ages for this assemblage. with a relatively small range from 487.2 f 1.1 to 470.2 f 1.3 Ma. Intrusions of the younger assemblage are largely undeformed and truncate structures shown in rocks of theolder assemblage. They are interpreted as post-collisional calc-alkaline granitoids.Single zircon dating provided an age of 401.8 f 0.8 Mafor the younger assemblage. consistentwith earlier work that defines an age range from c. 420 to 395Ma. Our datafavour a tectonicmodel involving formation and amalgamation of islandarc and microcontinent terranes between ca. 490 and 470 Ma ago to create the Central Qinling Zone which subsequently collided with theNorth China Block prior to c. -
Neoproterozoic Glaciations in a Revised Global Palaeogeography from the Breakup of Rodinia to the Assembly of Gondwanaland
Sedimentary Geology 294 (2013) 219–232 Contents lists available at SciVerse ScienceDirect Sedimentary Geology journal homepage: www.elsevier.com/locate/sedgeo Invited review Neoproterozoic glaciations in a revised global palaeogeography from the breakup of Rodinia to the assembly of Gondwanaland Zheng-Xiang Li a,b,⁎, David A.D. Evans b, Galen P. Halverson c,d a ARC Centre of Excellence for Core to Crust Fluid Systems (CCFS) and The Institute for Geoscience Research (TIGeR), Department of Applied Geology, Curtin University, GPO Box U1987, Perth, WA 6845, Australia b Department of Geology and Geophysics, Yale University, New Haven, CT 06520-8109, USA c Earth & Planetary Sciences/GEOTOP, McGill University, 3450 University St., Montreal, Quebec H3A0E8, Canada d Tectonics, Resources and Exploration (TRaX), School of Earth and Environmental Sciences, University of Adelaide, SA 5005, Australia article info abstract Article history: This review paper presents a set of revised global palaeogeographic maps for the 825–540 Ma interval using Received 6 January 2013 the latest palaeomagnetic data, along with lithological information for Neoproterozoic sedimentary basins. Received in revised form 24 May 2013 These maps form the basis for an examination of the relationships between known glacial deposits, Accepted 28 May 2013 palaeolatitude, positions of continental rifting, relative sea-level changes, and major global tectonic events Available online 5 June 2013 such as supercontinent assembly, breakup and superplume events. This analysis reveals several fundamental ’ Editor: J. Knight palaeogeographic features that will help inform and constrain models for Earth s climatic and geodynamic evolution during the Neoproterozoic. First, glacial deposits at or near sea level appear to extend from high Keywords: latitudes into the deep tropics for all three Neoproterozoic ice ages (Sturtian, Marinoan and Gaskiers), al- Neoproterozoic though the Gaskiers interval remains very poorly constrained in both palaeomagnetic data and global Rodinia lithostratigraphic correlations. -
Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets
EPSC Abstracts Vol. 11, EPSC2017-945, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets D. Lourenco, P. J. Tackley, A. Rozel and M. Ballmer Institute of Geophysics, Department of Earth Sciences, ETH Zurich, Switzerland ([email protected] / Fax: +41 44 633 1065) Abstract reported in [3], we use thermo-chemical global mantle convection numerical simulations to Plate tectonics on Earth-like planets is typically systematically investigate the effect of plutonism, in modelling using a strongly temperature-dependent conjugation with eruptive volcanism. Results visco-plastic rheology. Previous analyses have reproduce the three common tectonic/convective generally focussed on purely thermal convection. regimes usually obtained in simulations using a However, we have shown that the influence of visco-plastic rheology: stagnant-lid (a one-plate compositional heterogeneity in the form of planet), episodic (where the lithosphere is unstable continental [1] or oceanic [2] crust can greatly and frequently overturns into the mantle), and influence plate tectonics by making it easier (i.e. it mobile-lid (similar to plate tectonics). At high occurs at a lower yield stress or friction coefficient). intrusion efficiencies, we observe and characterise a Here we present detailed results on this topic, in new additional regime called “plutonic-squishy lid”. particular focussing on the influence of intrusive vs. This regime is characterised by a set of strong plates extrusive magmatism on the tectonic mode. separated by warm and weak regions generated by plutonism. Eclogitic drippings and lithospheric delaminations often occur around these weak regions. -
The Western Amazonia Igneous Belt
Journal of South American Earth Sciences 96 (2019) 102326 Contents lists available at ScienceDirect Journal of South American Earth Sciences journal homepage: www.elsevier.com/locate/jsames The Western Amazonia Igneous Belt T ∗ Gilmar José Rizzottoa, , Cléber Ladeira Alvesa, Francisco Sene Riosa, Márcia Aparecida de Sant’Ana Barrosb a Geological Survey of Brazil (CPRM), Rua 148, nº 485, 74170-110, Goiânia, Goiás, Brazil b Institute of Geosciences of the Federal University of Mato Grosso, Rua 44, No. 41, CEP 78.068-505, Cuiabá, Mato Grosso, Brazil ARTICLE INFO ABSTRACT Keywords: The Western Amazonia Igneous Belt (WAIB) occupies the northern part of South American continent, and a total Amazonian craton area close to 125,000 km2. The belt is composed dominantly by volcano-plutonic felsic rocks (Juruena super- Bimodal magmatism suite, Teles Pires suite and Colíder group) and has dominant alkali-calcic, metaluminous to peraluminous, fer- Underplating rous, geochemical characteristics, similar to A-type granites. The Silicic members are represented by granites and Teles pires suite rhyolitic-rhyodacitic volcanic rocks, mafic members by gabbroic rocks and diabase dykes. Intermediate rocks are rare. Local magma mingling and hybridization are present in several areas. The assemblage of silicic and basic rocks of WAIB was formed between c. 1825 and 1757 Ma. The presence of inherited zircons, from 1875 to 2050 Ma, as well as some Archean ages in the granitic and volcanic rocks from the WAIB, are suggestive of derivation by melting of pre-existing crustal basement (Ventuari-Tapajós Province). This hypothesis is also corroborated by bimodal magmatism and by several model-ages of granites, felsic volcanic rocks and mafic plutonic rocks, with TDM ranging from 2.0 to 2.3 Ga, and εNd value, varying from −3.90 to +2.52. -
Volcanism in a Plate Tectonics Perspective
Appendix I Volcanism in a Plate Tectonics Perspective 1 APPENDIX I VOLCANISM IN A PLATE TECTONICS PERSPECTIVE Contributed by Tom Sisson Volcanoes and Earth’s Interior Structure (See Surrounded by Volcanoes and Magma Mash for relevant illustrations and activities.) To understand how volcanoes form, it is necessary to know something about the inner structure and dynamics of the Earth. The speed at which earthquake waves travel indicates that Earth contains a dense core composed chiefly of iron. The inner part of the core is solid metal, but the outer part is melted and can flow. Circulation (movement) of the liquid outer core probably creates Earth’s magnetic field that causes compass needles to point north and helps some animals migrate. The outer core is surrounded by hot, dense rock known as the mantle. Although the mantle is nearly everywhere completely solid, the rock is hot enough that it is soft and pliable. It flows very slowly, at speeds of inches-to-feet each year, in much the same way as solid ice flows in a glacier. Earth’s interior is hot both because of heat left over from its formation 4.56 billion years ago by meteorites crashing together (accreting due to gravity), and because of traces of natural radioactivity in rocks. As radioactive elements break down into other elements, they release heat, which warms the inside of the Earth. The outermost part of the solid Earth is the crust, which is colder and about ten percent less dense than the mantle, both because it has a different chemical composition and because of lower pressures that favor low-density minerals. -
Environmental Effects of Large Igneous Province Magmatism: a Siberian Perspective Benjamin A
20 Environmental effects of large igneous province magmatism: a Siberian perspective benjamin a. black, jean-franc¸ois lamarque, christine shields, linda t. elkins-tanton and jeffrey t. kiehl 20.1 Introduction Even relatively small volcanic eruptions can have significant impacts on global climate. The eruption of El Chichón in 1982 involved only 0.38 km3 of magma (Varekamp et al., 1984); the eruption of Mount Pinatubo in 1993 involved 3–5km3 of magma (Westrich and Gerlach, 1992). Both these eruptions produced statistically significant climate signals lasting months to years. Over Earth’s his- tory, magmatism has occurred on vastly larger scales than those of the Pinatubo and El Chichón eruptions. Super-eruptions often expel thousands of cubic kilo- metres of material; large igneous provinces (LIPs) can encompass millions of cubic kilometres of magma. The environmental impact of such extraordinarily large volcanic events is controversial. In this work, we explore the unique aspects of LIP eruptions (with particular attention to the Siberian Traps), and the significance of these traits for climate and atmospheric chemistry during eruptive episodes. As defined by Bryan and Ernst (2008), LIPs host voluminous (> 100,000 km3) intraplate magmatism where the majority of the magmas are emplaced during short igneous pulses. The close temporal correlation between some LIP eruptions and mass extinction events has been taken as evidence supporting a causal relationship (Courtillot, 1994; Rampino and Stothers, 1988; Wignall, 2001); as geochronological data become increasingly precise, they have continued to indicate that this temporal association may rise above the level of coincidence (Blackburn et al., 2013). Several obstacles obscure the mechanisms that might link LIP magmatism with the degree of global environmental change sufficient to trigger mass extinction. -
Geochemistry and Tectonic Significance of Late Paleoproterozoic A-Type Granites Along the Southern Margin of the North China
www.nature.com/scientificreports OPEN Geochemistry and tectonic signifcance of late Paleoproterozoic A-type granites along the southern margin of the North China Craton Yan Wang1, Yi-Zeng Yang1*, Wolfgang Siebel2, He Zhang1, Yuan-Shuo Zhang1 & Fukun Chen1 The Longwangzhuang pluton is a typical example of Paleoproterozoic A-type granite intrusions at the southern margin of the North China Craton. This pluton is composed of arfvedsonite granite and minor aegirine–augite granites. Samples from both granite types display similar zircon U-Pb ages with 207U-206Pb ages of 1612 ± 19 Ma [mean square weighted deviation (MSWD) = 0.66] and 1609 ± 24 Ma (MSWD = 0.5), respectively. The granites exhibit similar high silica (SiO2 = 71.1–73.4 wt.%), high alkaline (Na2O + K2O = 8.10–9.26 wt.%, K2O/Na2O > 1), and low Al2O3 (11.8–12.8 wt. %) contents and metaluminous to weakly peraluminous bulk chemistry. The chemical variations of the Longwangzhuang pluton suggest the efects of mineral fractionation. In addition, all samples show typical characteristics of A-type granites, such as high 10000Ga/Al ratios (4.10–7.28), high FeOtot/(FeOtot + MgO) ratios (0.88– 0.99), and high Zr (484–1082 ppm), Ce (201–560 ppm), and Y (78–156 ppm) contents. The εNd(t) values 206 204 207 204 208 204 and the ( Pb/ Pb)t, ( Pb/ Pb)t, and ( Pb/ Pb)t ratios of the arfvedsonite granite samples vary from −4.6 to –5.3, 15.021 to 17.349, 15.241 to 15.472, and 33.206 to 36.905, respectively, and those for the aegirine–augite granite sample amount at −0.2, 14.421, 15.175, and 33.706. -
Provenance and Implication of Carboniferous–Permian Detrital
minerals Article Provenance and Implication of Carboniferous–Permian Detrital Zircons from the Upper Paleozoic, Southern Ordos Basin, China: Evidence from U-Pb Geochronology and Hf Isotopes Ziwen Jiang 1, Jinglan Luo 1,*, Xinshe Liu 2,3, Xinyou Hu 2,3, Shangwei Ma 4, Yundong Hou 2,3, Liyong Fan 2,3 and Yuhua Hu 1 1 State Key Laboratory of Continental Dynamics, Department of Geology, Northwest University, Xi’an 710069, China; [email protected] (Z.J.); [email protected] (Y.H.) 2 State Engineering Laboratory of Exploration and Development for Low Permeability Oil and Gas Fields, Xi’an 710018, China; [email protected] (X.L.); [email protected] (X.H.); [email protected] (Y.H.); [email protected] (L.F.) 3 Research Institute of Petroleum Exploration and Development, PetroChina Changqing Oilfield Company, Xi’an 710018, China 4 Shaanxi Mineral Resources and Geological Survey, Xi’an 710068, China; [email protected] * Correspondence: [email protected] Received: 9 February 2020; Accepted: 13 March 2020; Published: 15 March 2020 Abstract: Carboniferous–Permian detrital zircons are recognized in the Upper Paleozoic of the whole Ordos Basin. Previous studies revealed that these Carboniferous–Permian zircons occurred in the Northern Ordos Basin mainly originated from the Yinshan Block. What has not been well documented until now is where this period’s zircons in the Southern Ordos Basin came from, and very little discussion about their provenance. To identify the provenance of the detrital zircons dating from ~350 to 260 Ma, five sandstone samples from the Shan 1 Member of Shanxi Formation and eight sandstone samples from the He 8 Member of Shihezi Formation were analyzed for detrital zircon U-Pb age dating and in situ Lu-Hf isotopic compositions. -
Fifth International Dyke Conference
FIFTH INTERNATIONAL DYKE CONFERENCE Abstracts and Programme NAL DYKE TIO C A O N N R F E E T R N I E N H C T F E I F 5 IDC F D I N L A N 31 July - 3 August 2005, Pohtimolampi Wilderness Hotel - Polar Circle - Rovaniemi - Finland FIFTH INTERNATIONAL DYKE CONFERENCE 31.7 – 3.8.2005 – ROVANIEMI, FINLAND FIFTH INTERNATIONAL DYKE CONFERENCE "Dyke swarms - time markers of crustal evolution" Pohtimolampi Wilderness Hotel - Polar Circle - Rovaniemi - Finland 31 June – 3 August 2005 ABSTRACTS AND PROGRAMME edited by Jouni Vuollo Geological Survey of Finland P.O. Box 77, FIN-96101 Rovaniemi Satu Mertanen Geological Survey of Finland P.O. Box 96, FIN-02151 Espoo ISBN 951-690-926-4 i FIFTH INTERNATIONAL DYKE CONFERENCE 31.7 – 3.8.2005 – ROVANIEMI, FINLAND Reference (an example): Alaabed S., 2005. Intrusion types of the mantle sequence of the northern Semail ophiolite (UAE Section). In: Vuollo, J. and Mertanen, S. (eds.), 5th International Dyke Conference, 31 July – 3 August 2005, Rovaniemi, Finland, Abstracts and Programme, p. 1. ii FIFTH INTERNATIONAL DYKE CONFERENCE 31.7 – 3.8.2005 – ROVANIEMI, FINLAND Welcome from the Organising Committee Welcome to Rovaniemi! We are very pleased to host you here as a participant of the Fifth International Dyke Conference (IDC- 5). The conference will bring together specialists in volcanology, tectonics, structural geology, petrology, geochemistry, geochronology, and geophysics to present progress made in the last years in various subjects related to dykes and other sheeted intrusions. An important part of the meeting are the pre- and post-conference excursions to the southern and eastern Finland and to the Kola Peninsula, Russia. -
Magma Genesis, Plate Tectonics, and Chemical Differentiation of the Earth
REVIEWS OF GEOPHYSICS, VOL. 26, NO. 3, PAGES 370-404, AUGUST 1988 Magma Genesis, Plate Tectonics, and Chemical Differentiation of the Earth PETER J. WYLLIE Division of Geolo•7icaland Planetary Sciences,California Institute of Technolo•Ty,Pasadena Magma genesis,migration, and eruption have played prominent roles in the chemical differentiation of the Earth. Plate tectonics has provided the framework of tectonic environments for different suites of igneousrocks and the dynamic mechanismsfor moving massesof rock into melting regions.Petrology is rooted in geophysics.Petrological and geophysicalprocesses are calibrated by the phase equilibria of the materials. The geochemistry of basalts and mantle xenoliths demonstrates that the mantle is hetero- geneous.The geochemical reservoirs are related to mantle convection, with interpretation of a mantle layered or stratified or peppered with blobs. Seismic tomography is beginning to reveal the density distribution of the mantle in three dimensions,and together with fluid mechanical models and interpreta- tion of the geoid, closer limits are being placed on mantle convection. Petrological cross sectionscon- structed for various tectonic environments by transferring phase boundaries for source rocks onto assumedthermal structuresprovide physical frameworks for consideration of magmatic and metasoma- tic events,with examplesbeing given for basalts,andesites, and granites at ocean-continentconvergent plate boundaries, basalts and nephelinitesfrom a thermal plume beneath Hawaii, kimberlites in cratons, -
Volcanic and Magmatic Rocks - J
EARTH SYSTEM: HISTORY AND NATURAL VARIABILITY - Vol. I - Volcanic and Magmatic Rocks - J. Ulrych and V. Cajz VOLCANIC AND MAGMATIC ROCKS J. Ulrych and V. Cajz Institute of Geology, Academy of Sciences of the Czech Republic, Prague, Czech Republic Keywords: Magma, lava, petrology, magmatism, plutonism, volcanism, classification, igneous rocks, plutonic, dyke and volcanic rocks, pyroclastic rocks, structure and texture of rocks, volcanology, landforms of volcanic products, intrusive and extrusive (effusive) products, utilization of rocks, zeolites Contents 1. State of the Art 2. Origin of Igneous Rocks 3. Forms of Plutonic and Subvolcanic Bodies 3.1 Abyssal Bodies 3.2 Subvolcanic Bodies 4. Landforms of Surface Volcanic Products 5. Classification and Characteristics of Principal Igneous Rocks 5.1 Plutonic Rocks 5.1.1. Granites and Granitoids (Alkali-Feldspar Granites, Granodiorites and Quartz Diorites) and Syenites 5.1.2 Gabbros and Diorites 5.1.3 Anorthosites 5.1.4 Ultramafic Plutonic Rocks (Peridotites, Pyroxenites, Hornblendites) 5.1.5 Carbonatites 5.1.6 Charnockites 5.2 Dyke Rocks 5.2.1 Porphyry 5.2.2 Lamprophyric Rocks (Lamprophyres, Lamproites, Kimberlites) 5.3 Volcanic Rocks 5.3.1 Basalts and Basaltoids (including Trachybasalt, Tephrite, Basanite, Olivine Foidite) 5.3.2 TrachytesUNESCO and Phonolites – EOLSS 5.3.3 Andesites and Dacites 5.3.4 Rhyolites 6. Importance and Utilization of Igneous Rocks Glossary SAMPLE CHAPTERS Bibliography Biographical Sketches Summary The Earth‘s internal regime is associated with heat derived from the radioactivity of U, Th, and K, and from the early thermal history of the planet. This internal heat causes plate motions, earthquakes, orogenic movements, and volcanic activity on the surface of the Earth. -
The Rhyacian El Cortijo Suture Zone: Aeromagnetic Signature and Insights for the Geodynamic Evolution of the Southwestern Rio De La Plata Craton, Argentina
Geoscience Frontiers 5 (2014) 43e52 Contents lists available at SciVerse ScienceDirect China University of Geosciences (Beijing) Geoscience Frontiers journal homepage: www.elsevier.com/locate/gsf Research paper The Rhyacian El Cortijo suture zone: Aeromagnetic signature and insights for the geodynamic evolution of the southwestern Rio de la Plata craton, Argentina Carlos J. Chernicoff a,b,*, Eduardo O. Zappettini b, Javier Peroni b a Council for Scientific and Technical Research (CONICET), Argentina b Argentine Geological-Mining Survey (SEGEMAR), Argentina article info abstract Article history: The amalgamation of the southern Río de la Plata craton involves two possibly coeval Rhyacian sutures Received 21 September 2012 associated with the Transamazonian orogeny, rather than a single one as previously envisaged, i.e. the El Received in revised form Cortijo suture zone and the Salado suture. We circumscribe the Tandilia terrane to the region between 20 March 2013 these two sutures. Accepted 15 April 2013 The El Cortijo suture zone runs along a roughly WNW oriented magnetic low aligned along the Available online 7 May 2013 southern boundary of the Tandilia terrane, i.e. boundary between the Tandilia and Balcarce terranes. This extensive magnetic low, ca. 300 km long, and ca. 90 km wide, would be caused by demagnetization Keywords: El Cortijo suture zone associated with shearing. At a more local scale, the trend of the El Cortijo suture zone often turns e Rhyacian toward the E W. At this scale, WNW trending tholeiitic dykes of Statherian age are seen to cut the Río de la Plata craton Rhyacian El Cortijo suture zone. Spatially associated with the El Cortijo suture zone, there are small Aeromagnetics magnetic highs interpreted to be related to unexposed basic bodies of ophiolitic nature related to those forming part of the El Cortijo Formation.