Pre‐Oxfordian (>163 Ma) Ophiolite Obduction in Central Tibet
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Ophiolite in Southeast Asia
Ophiolite in Southeast Asia CHARLES S. HUTCHISON Department of Geology, University of Malaya, Kuala Lumpur, Malaysia ABSTRACT semblages are classified into definite ophiolite, tentatively identified ophiolite, and associations that have previously been named No fewer than 20 belts of mafic-ultramafic assemblages have ophiolite but that are not. Each of the ophiolite or other been named "ophiolite" in the complex Southeast Asia region of mafic-ultramafic associations is listed in Table 1, with brief reasons Sundaland. Fewer than half of these can be confidently classified as for its classification, particularly in regard to the petrography of the ophiolite. The only well-documented complete ophiolite, with con- rock suite and the nature of its sedimentary envelope. The basis for tinuous conformable sections from mantle harzburgite through identification (or rejection) of these rock associations as ophiolite is gabbro to spilite, occurs in northeast Borneo and the neighboring discussed in the following section. Philippine Islands. It contains a record of oceanic lithospheric his- tory from Jurassic to Tertiary and has a Miocene emplacement age. OPHIOLITE FORMATION All other ophiolite belts of the region are either incomplete or dis- membered. The Sundaland region probably has examples of several The oceanic lithosphere, with its thin oceanic crust formed along types of emplacement mechanism and emplacement ages ranging the spreading axes of divergent plate junctures, is thought to be from early Paleozoic to Cenozoic. Key words: Sundaland, plate consumed at arc-trench systems of convergent plate junctures (Fig. tectonics. 2). Minor subtractions of crustal and mantle material from de- scending slabs of oceanic lithosphere are thought to be added to INTRODUCTION belts of mélange, and imbricate slices are caught in crustal subduc- tion zones at the trenches (Dickinson, 1972). -
Hydrothermal Alteration of a Supra-Subduction Zone Ophiolite Analog, Tonga
AN ABSTRACT OF THE THESIS OF Melanie C. Kelman for the degree of Master of Science in Geology presented on May 29, 1998. Title: Hydrothermal Alteration of a Supra-Subduction Zone Ophiolite Analog, Tonga. Southwest Pacific. Abstract approved: Redacted for Privacy Sherman Bloomer The basement of the Tonga intraoceanic forearc comprises Eocene arc volcanic crust formed during the earliest phases of subduction. Volcanic rocks recovered from the forearc include boninites and arc tholeiites, apparently erupted into and upon older mid- oceanic ridge tholeiites. Rock assemblages suggest that the forearc basement is a likely analog for large supra-subduction zone (SSZ) ophiolites not only in structure and Ethology, but also in the style of hydrothermal alteration. Dredged volcanic samples from the central Tonga forearc (20-24° S) exhibit the effects of seafloor weathering, low (<200°C, principally <100°C) alteration, and high temperature (>200°C) alteration. Tholeiites and arc tholeiites are significantly more altered than boninites. Seafloor weathering is due to extensive interaction with cold oxidizing seawater, and is characterized by red-brown staining and the presence of Fe- oxyhydroxides. Low temperature alteration is due to circulation of evolving seawater- derived fluids through the volcanic section until fluid pathways were closed by secondary mineral precipitation. Low temperature alteration is characterized by smectites, celadonite, phillipsite, mixed-layer smectite/chlorite, carbonates, and silica. All phases fill veins and cavities; clay minerals and silica also replace the mesostasis and groundmass phases. Low temperature alteration enriches the bulk rock in K, Ba, and Na, and mobilizes other elements to varying extents. The few high temperature samples are characterized by mobilizes other elements to varying extents. -
Two Contrasting Phanerozoic Orogenic Systems Revealed by Hafnium Isotope Data William J
ARTICLES PUBLISHED ONLINE: 17 APRIL 2011 | DOI: 10.1038/NGEO1127 Two contrasting Phanerozoic orogenic systems revealed by hafnium isotope data William J. Collins1*(, Elena A. Belousova2, Anthony I. S. Kemp1 and J. Brendan Murphy3 Two fundamentally different orogenic systems have existed on Earth throughout the Phanerozoic. Circum-Pacific accretionary orogens are the external orogenic system formed around the Pacific rim, where oceanic lithosphere semicontinuously subducts beneath continental lithosphere. In contrast, the internal orogenic system is found in Europe and Asia as the collage of collisional mountain belts, formed during the collision between continental crustal fragments. External orogenic systems form at the boundary of large underlying mantle convection cells, whereas internal orogens form within one supercell. Here we present a compilation of hafnium isotope data from zircon minerals collected from orogens worldwide. We find that the range of hafnium isotope signatures for the external orogenic system narrows and trends towards more radiogenic compositions since 550 Myr ago. By contrast, the range of signatures from the internal orogenic system broadens since 550 Myr ago. We suggest that for the external system, the lower crust and lithospheric mantle beneath the overriding continent is removed during subduction and replaced by newly formed crust, which generates the radiogenic hafnium signature when remelted. For the internal orogenic system, the lower crust and lithospheric mantle is instead eventually replaced by more continental lithosphere from a collided continental fragment. Our suggested model provides a simple basis for unravelling the global geodynamic evolution of the ancient Earth. resent-day orogens of contrasting character can be reduced to which probably began by the Early Ordovician12, and the Early two types on Earth, dominantly accretionary or dominantly Paleozoic accretionary orogens in the easternmost Altaids of Pcollisional, because only the latter are associated with Wilson Asia13. -
Initial Growth of the Northern Lhasaplano, Tibetan Plateau in the Early Late Cretaceous (Ca
hu-B35124.1 2nd pages / 1 of 14 Initial growth of the Northern Lhasaplano in the early Late Cretaceous Initial growth of the Northern Lhasaplano, Tibetan Plateau in the early Late Cretaceous (ca. 92 Ma) Wen Lai1, Xiumian Hu1,†, Eduardo Garzanti2, Gaoyuan Sun1,3, Carmala N. Garzione4, Marcelle BouDagher Fadel5, and Anlin Ma1 1State Key Laboratory of Mineral Deposits Research, School of Earth Sciences and Engineering, Nanjing University, Nanjing 210023, China 2Department of Earth and Environmental Sciences, Università di Milano-Bicocca, Milano 20126, Italy 3College of Oceanography, Hohai University, Nanjing 210098, China 4Department of Earth and Environmental Sciences, University of Rochester, Rochester, New York 14627, USA 5Department of Geological Sciences, University College London, London WC1E6BT, UK ABSTRACT INTRODUCTION Stable isotopes in lacustrine carbonates suggest that the basins surrounding the Gangdese Moun Constraining the growth of the Tibetan The Tibetan Plateau, with an average ele tains in the southern Lhasa terrane had reached Plateau in time and space is critical for test- vation of ~5000 m, is the world’s highest and an elevation >4500 m since IndiaAsia collision ing geodynamic models and climatic changes widest orogenic plateau, and exerts a major in (Ding et al., 2014). Lowtemperature thermo at the regional and global scale. The Lhasa fluence on the Asian monsoon, global climate chronology reveal that the central and northern block is a key region for unraveling the early change, and regional distribution of living spe Lhasa terranes experienced rapid to moderate history of the Tibetan Plateau. Distinct from cies (Raymo and Ruddiman, 1992; Molnar et al., cooling and exhumation between 85 and 45 Ma the underlying shallow-marine limestones, 1993; An et al., 2001; DupontNivet et al., 2007; (Hetzel et al., 2011; Rohrmann et al., 2012). -
Kinematic Reconstruction of the Caribbean Region Since the Early Jurassic
Earth-Science Reviews 138 (2014) 102–136 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev Kinematic reconstruction of the Caribbean region since the Early Jurassic Lydian M. Boschman a,⁎, Douwe J.J. van Hinsbergen a, Trond H. Torsvik b,c,d, Wim Spakman a,b, James L. Pindell e,f a Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands b Center for Earth Evolution and Dynamics (CEED), University of Oslo, Sem Sælands vei 24, NO-0316 Oslo, Norway c Center for Geodynamics, Geological Survey of Norway (NGU), Leiv Eirikssons vei 39, 7491 Trondheim, Norway d School of Geosciences, University of the Witwatersrand, WITS 2050 Johannesburg, South Africa e Tectonic Analysis Ltd., Chestnut House, Duncton, West Sussex, GU28 OLH, England, UK f School of Earth and Ocean Sciences, Cardiff University, Park Place, Cardiff CF10 3YE, UK article info abstract Article history: The Caribbean oceanic crust was formed west of the North and South American continents, probably from Late Received 4 December 2013 Jurassic through Early Cretaceous time. Its subsequent evolution has resulted from a complex tectonic history Accepted 9 August 2014 governed by the interplay of the North American, South American and (Paleo-)Pacific plates. During its entire Available online 23 August 2014 tectonic evolution, the Caribbean plate was largely surrounded by subduction and transform boundaries, and the oceanic crust has been overlain by the Caribbean Large Igneous Province (CLIP) since ~90 Ma. The consequent Keywords: absence of passive margins and measurable marine magnetic anomalies hampers a quantitative integration into GPlates Apparent Polar Wander Path the global circuit of plate motions. -
Paleomagnetic Constraints on the Mesozoic Drift of the Lhasa Terrane (Tibet) from Gondwana to Eurasia
Paleomagnetic constraints on the Mesozoic drift of the Lhasa terrane (Tibet) from Gondwana to Eurasia Zhenyu Li1, Lin Ding1,2*, Peter C. Lippert3, Peiping Song1, Yahui Yue1, and Douwe J.J. van Hinsbergen4 1Key Laboratory of Continental Collision and Plateau Uplift (LCPU), Institute of Tibetan Plateau Research, Chinese Academy of Sciences (ITPCAS), Beijing 100101, China 2Center for Excellence in Tibetan Plateau Earth Sciences, Chinese Academy of Sciences, Beijing 100101, China 3Department of Geology and Geophysics, University of Utah, Salt Lake City, Utah 84112-9057, USA 4Department of Earth Sciences, Utrecht University, Heidelberglaan 2, 3584 CS Utrecht, Netherlands ABSTRACT Himalaya (the northernmost continental rocks The Mesozoic plate tectonic history of Gondwana-derived crustal blocks of the Tibetan derived from the Indian plate) that collided with Plateau is hotly debated, but so far, paleomagnetic constraints quantifying their paleolati- Lhasa in the Eocene along the Indus-Yarlung tude drift history remain sparse. Here, we compile existing data published mainly in Chinese suture zone (Yin and Harrison, 2000; Hu et al., literature and provide a new, high-quality, well-dated paleomagnetic pole from the ca. 180 2015; Huang et al., 2015). Ma Sangri Group volcanic rocks of the Lhasa terrane that yields a paleolatitude of 3.7°S Most authors describe an ideal Wilson-cycle ± 3.4°. This new pole confirms a trend in the data that suggests that Lhasa drifted away scenario, wherein the blocks of the Tibetan Pla- from Gondwana in Late Triassic time, instead of Permian time as widely perceived. A total teau all drifted from India in Paleozoic to Meso- northward drift of ~4500 km between ca. -
Introduction to Himalayan Tectonics: a Modern Synthesis
Downloaded from http://sp.lyellcollection.org/ at Kingston University on January 3, 2020 Introduction to Himalayan tectonics: a modern synthesis MICHAEL P. SEARLE1* & PETER J. TRELOAR2 1Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, UK 2School of the Natural and Built Environment, Kingston University, Penrhyn Road, Kingston-upon-Thames, Surrey KT1 2EE, UK MPS, 0000-0001-6904-6398 *Correspondence: [email protected] The Himalaya resulted from collision of the Indian widespread migmatization and mid-crustal melting plate with Asia and are well known as the highest, during the Oligocene–Mid-Miocene. The age of the youngest and one of the best studied continental col- abundant leucogranite sills and dykes along the top lision orogenic belts. They are frequently used as the of the GHS, beneath the STD, is concomitant with type example of a continental collision orogenic belt the sillimanite-grade metamorphic event. The GHS in studies of older Phanerozoic orogenic belts. The metamorphism is all part of one continuum of crustal beauty of the Himalaya is that, on a broad scale they thickening and shortening, increasing pressure and form a relatively simple orogenic belt. The major temperature following a standard clockwise Pressure- structural divisions, the Indus–(Yarlung Tsangpo) Temperature-Time (PTt) path. Decompression suture zone, the Tethyan Himalaya sedimentary melting peaked with widespread partial melting and units, Greater Himalaya Sequence (GHS) metamor- formation of migmatites and leucogranites along the phic rocks, the Lesser Himalaya fold-and-thrust highest peaks of the Himalaya. Structural mapping belt and the Sub-Himalaya Siwalik molasse basin and timing constraints suggest the large-scale are present along the entire 2000 km length of the southward extrusion of a partially melted layer of Himalaya (Figs 1 & 2). -
Mid-Cretaceous Thick Carbonate Accumulation in Northern Lhasa (Tibet): Eustatic Vs
Mid-Cretaceous thick carbonate accumulation in Northern Lhasa (Tibet): eustatic vs. tectonic control? Yiwei Xu1, Xiumian Hu1,†, Eduardo Garzanti2, Marcelle BouDagher-Fadel3, Gaoyuan Sun4, Wen Lai1, and Shijie Zhang5 1 State Key Laboratory of Mineral Deposits Research, School of Earth Sciences and Engineering, Nanjing University, Nanjing 210023, China 2 Department of Earth and Environmental Sciences, Università di Milano-Bicocca, Milano 20126, Italy 3 Department of Earth Sciences, University College London, Gower Street, London, WC1E 6BT, UK 4 College of Oceanography, Hohai University, Nanjing 210098, China 5 School of Tourism, Henan Normal University, Xinxiang 453007, China ABSTRACT INTRODUCTION Moreover, their thickness does not exceed a few hundreds of meters, because carbonate Widespread accumulation of thick car- The Lhasa terrane, lying between the In- production is hampered in orogenic settings bonates is not typical of orogenic settings. dus–Yarlung suture to the south and the Ban- where tectonic uplift and erosion produce During the mid-Cretaceous, near the Ban- gong suture to the north (Fig. 1A), is the latest abundant terrigenous detritus (Wilson, 1975; gong suture in the northern Lhasa terrane, microcontinent accreted to Asia before colli- Dorobek, 1995). However, in a few cases (e.g., the shallow-marine carbonates of the Lang- sion between the Indian and Asian continental the Papua–New Guinea foreland basin) car- shan Formation, reaching a thickness up to margins. The timing of collision between the bonate thickness may reach 1.2 km (Sinclair, ∼1 km, accumulated in an epicontinental Qiangtang and Lhasa terranes along the Ban- 1997). Finally, carbonates generally occur only seaway over a modern area of 132 × 103 km2, gong suture (Fig. -
GEOLOGIC FRAMEWORK, TECTONIC EVOLUTION, and DISPLACEMENT HISTORY of the ALEXANDER TERRANE Georgee
TECTONICS, VOL. 6, NO. 2, PAGES 151-173, APRIL 1987 GEOLOGIC FRAMEWORK, TECTONIC EVOLUTION, AND DISPLACEMENT HISTORY OF THE ALEXANDER TERRANE GeorgeE. Gehrels1 and Jason B. Saleeby Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena Abstract. The Alexander terrane consists of Devonian (Klakas orogeny). The second phase is upper Proterozoic(?)-Cambrian through marked by Middle Devonian through Lower Middle(?) Jurassic rocks that underlie much of Permian strata which accumulated in southeastern (SE) Alaska and parts of eastern tectonically stable marine environments. Alaska, western British Columbia, and Devonian and Lower Permian volcanic rocks and southwestern Yukon Territory. A variety of upper Pennsylvanian-Lower Permian syenitic to geologic, paleomagnetic, and paleontologic dioritic intrusive bodies occur locally but do not evidence indicates that these rocks have been appear to represent major magmatic systems. displaced considerable distances from their The third phase is marked by Triassic volcanic sites of origin and were not accreted to western and sedimentary rocks which are interpreted to North America until Late Cretaceous-early have formed in a rift environment. Previous Tertiary time. Our geologic and U-Pb syntheses of the displacement history of the geochronologic studies in southern SE Alaska terrane emphasized apparent similarities with and the work of others to the north indicate rocks in the Sierra-Klamath region and that the terrane evolved through three distinct suggested that the Alexander terrane evolved in tectonic phases. During the initial phase, from proximity to the California continental margin late Proterozoic(?)-Cambrian through Early during Paleozoic time. Our studies indicate, Devonian time, the terrane probably evolved however, that the geologic record of the along a convergent plate margin. -
Himalaya - Southern-Tibet: the Typical Continent-Continent Collision Orogen
237 Himalaya - Southern-Tibet: the typical continent-continent collision orogen When an oceanic plate is subducted beneath a continental lithosphere, an Andean mountain range develops on the edge of the continent. If the subducting plate also contains some continental lithosphere, plate convergence eventually brings both continents into juxtaposition. While the oceanic lithosphere is relatively dense and sinks into the asthenosphere, the greater sialic content of the continental lithosphere ascribes positive buoyancy in the asthenosphere, which hinders the continental lithosphere to be subducted any great distance. Consequently, a continental lithosphere arriving at a trench will confront the overriding continent. Rapid relative convergence is halted and crustal shortening forms a collision mountain range. The plane marking the locus of collision is a suture, which usually preserves slivers of the oceanic lithosphere that formerly separated the continents, known as ophiolites. The collision between the Indian subcontinent and what is now Tibet began in the Eocene. It involved and still involves north-south convergence throughout southern Tibet and the Himalayas. This youthful mountain area is the type example for studies of continental collision processes. The Himalayas Location The Himalayas form a nearly 3000 km long, 250-350 km wide range between India to the south and the huge Tibetan plateau, with a mean elevation of 5000 m, to the north. The Himalayan mountain belt has a relatively simple, arcuate, and cylindrical geometry over most of its length and terminates at both ends in nearly transverse syntaxes, i.e. areas where orogenic structures turn sharply about a vertical axis. Both syntaxes are named after the main peaks that tower above them, the Namche Barwa (7756 m) to the east and the Nanga Parbat (8138 m) to the west, in Pakistan. -
Unraveling the Geologic History of the Avalon Terrane in MA Erin Nevens
Undergraduate Review Volume 2 Article 12 2006 Unraveling the Geologic History of the Avalon Terrane in MA Erin Nevens Follow this and additional works at: http://vc.bridgew.edu/undergrad_rev Part of the Geology Commons Recommended Citation Nevens, Erin (2006). Unraveling the Geologic History of the Avalon Terrane in MA. Undergraduate Review, 2, 56-66. Available at: http://vc.bridgew.edu/undergrad_rev/vol2/iss1/12 This item is available as part of Virtual Commons, the open-access institutional repository of Bridgewater State University, Bridgewater, Massachusetts. Copyright © 2006 Erin Nevens 56 Unraveling the Geologic History ofthe Avalon Terrane in MA BY ERIN NEYENS Erin Nevens wrote this piece under the Abstract mentorship of Dr. Michael Krol. "PO-. ield and petrographic analysis of rocks at Black Rock Beach in Co 10_.. hasset, MA record at least two phases of metamorphism and mag matic activity and three episodes ofdeformation. The earliest phase of metamorphism and deformation are recorded by mafic gneiss xenoliths. These xenoliths preserve a mylonitic texture, which represents de velopment in a ductile deformation environment. The xenoliths occur as large blocks that were later incorporated into the intruding magma of the Dedham granodiorite. Following crystallization, the Dedham granodiorite experienced an episode of plastic deformation. This event resulted in the development of a weak foliation defined by aligned feldspar porphyroclasts. Quartz and feldspar microstructures indicate deformation occurred between 350-450"C. A second phase of magmatic activity was associated with the intrusion ofseveral 1·2 me· ter wide porphyritic basalt dikes that cross-cut both the xenoliths and grano diorite,.and resulted in the brittle cataclasis of the Dedham granodiorite, The basalt dikes were emplaced during a time ofcrustal extension and subsequently experienced a late-stage hydrothermal alteration. -
Pan-African Orogeny 1
Encyclopedia 0f Geology (2004), vol. 1, Elsevier, Amsterdam AFRICA/Pan-African Orogeny 1 Contents Pan-African Orogeny North African Phanerozoic Rift Valley Within the Pan-African domains, two broad types of Pan-African Orogeny orogenic or mobile belts can be distinguished. One type consists predominantly of Neoproterozoic supracrustal and magmatic assemblages, many of juvenile (mantle- A Kröner, Universität Mainz, Mainz, Germany R J Stern, University of Texas-Dallas, Richardson derived) origin, with structural and metamorphic his- TX, USA tories that are similar to those in Phanerozoic collision and accretion belts. These belts expose upper to middle O 2005, Elsevier Ltd. All Rights Reserved. crustal levels and contain diagnostic features such as ophiolites, subduction- or collision-related granitoids, lntroduction island-arc or passive continental margin assemblages as well as exotic terranes that permit reconstruction of The term 'Pan-African' was coined by WQ Kennedy in their evolution in Phanerozoic-style plate tectonic scen- 1964 on the basis of an assessment of available Rb-Sr arios. Such belts include the Arabian-Nubian shield of and K-Ar ages in Africa. The Pan-African was inter- Arabia and north-east Africa (Figure 2), the Damara- preted as a tectono-thermal event, some 500 Ma ago, Kaoko-Gariep Belt and Lufilian Arc of south-central during which a number of mobile belts formed, sur- and south-western Africa, the West Congo Belt of rounding older cratons. The concept was then extended Angola and Congo Republic, the Trans-Sahara Belt of to the Gondwana continents (Figure 1) although West Africa, and the Rokelide and Mauretanian belts regional names were proposed such as Brasiliano along the western Part of the West African Craton for South America, Adelaidean for Australia, and (Figure 1).