The Role of Partial Melting and Extensional Strain Rates in the Development of Metamorphic Core Complexes
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
The Segregation and Emplacement of Granitic Magmas
Journal of the Geological society, London, Vol. 144, 1987, pp. 281-297, 13 figs. Printed in Northern Ireland The segregation and emplacement of granitic magmas S. M. WICKHAM Division of Geological and Planetary Sciences California Institute of Technology, Pasadena, California 91125 USA Abstract: The segregation of granitic magma from residual crystals at low melt-fraction is strongly dependent on the viscosity of the melt. Theoretical considerations imply that for the typical range of granitic meltviscosities (104Pa S to 10” Pa S) only verylimited separation will bepossible by a compaction mechanism over the typical duration of a crustal melting event (c. 106years). Small-scale segregations (millimetre to metre) of the type observed in migmatite terranes may be generated by compaction (possiblyassisted by -continuousdeformation), or byflow of melt into extensional fractures, but low melt-fraction liquids are unlikely to be extracted to form large (kilometre-size) granitic plutons because of the limited separation efficiency. At higher melt-fractions (>30%) the rapid decrease in strengthand effectiveviscosity during partial meltingallows other segregation processes tooperate. Calculations and experiments indicate that in granitic systems the effective viscosity of partially melted rocks,having a very narrow melt fraction range of 30-50% will fall rapidly to levels at which convective overturn of kilometre-thick zones can occur. Convective motion within anatectic regionsis capable of generating large (kilometre-size) homogeneous, highcrystal- fraction, crustally-derived magma bodies, which are orders of magnitude greater insize than low melt-fraction segregates. Before convective instability is reached, small (centimetre- to metre-sized) pods of granitic liquid may rise buoyantly through, and pond at the top of such partly molten zones; such a process is consistent with the observation that some granulites appear to be residue rocks, chemically depleted in a minimum melt component. -
Full-Text PDF (Final Published Version)
Pritchard, M. E., de Silva, S. L., Michelfelder, G., Zandt, G., McNutt, S. R., Gottsmann, J., West, M. E., Blundy, J., Christensen, D. H., Finnegan, N. J., Minaya, E., Sparks, R. S. J., Sunagua, M., Unsworth, M. J., Alvizuri, C., Comeau, M. J., del Potro, R., Díaz, D., Diez, M., ... Ward, K. M. (2018). Synthesis: PLUTONS: Investigating the relationship between pluton growth and volcanism in the Central Andes. Geosphere, 14(3), 954-982. https://doi.org/10.1130/GES01578.1 Publisher's PDF, also known as Version of record License (if available): CC BY-NC Link to published version (if available): 10.1130/GES01578.1 Link to publication record in Explore Bristol Research PDF-document This is the final published version of the article (version of record). It first appeared online via Geo Science World at https://doi.org/10.1130/GES01578.1 . Please refer to any applicable terms of use of the publisher. University of Bristol - Explore Bristol Research General rights This document is made available in accordance with publisher policies. Please cite only the published version using the reference above. Full terms of use are available: http://www.bristol.ac.uk/red/research-policy/pure/user-guides/ebr-terms/ Research Paper THEMED ISSUE: PLUTONS: Investigating the Relationship between Pluton Growth and Volcanism in the Central Andes GEOSPHERE Synthesis: PLUTONS: Investigating the relationship between pluton growth and volcanism in the Central Andes GEOSPHERE; v. 14, no. 3 M.E. Pritchard1,2, S.L. de Silva3, G. Michelfelder4, G. Zandt5, S.R. McNutt6, J. Gottsmann2, M.E. West7, J. Blundy2, D.H. -
Geochemical Behaviour of Trace Elements During Fractional
Anais da Academia Brasileira de Ciências (2015) 87(4): 1959-1979 (Annals of the Brazilian Academy of Sciences) Printed version ISSN 0001-3765 / Online version ISSN 1678-2690 http://dx.doi.org/10.1590/0001-3765201520130385 www.scielo.br/aabc Geochemical behaviour of trace elements during fractional crystallization and crustal assimilation of the felsic alkaline magmas of the state of Rio de Janeiro, Brazil AKIHISA Motoki1*, SUSANNA E. SICHEL2, THAIS Vargas1, DEAN P. MELO3 and KENJI F. Motoki2 1Departamento de Mineralogia e Petrologia Ígnea, Universidade do Estado do Rio de Janeiro, Rua São Francisco Xavier, 524, Sala A-4023, Maracanã, 20550-990 Rio de Janeiro, RJ, Brasil 2Departamento de Geologia, Universidade Federal Fluminense, Av. General Milton Cardoso, s/n, 4° Andar, Gragoatá, 24210-340 Niterói, RJ, Brasil 3PETROBRAS, CENPES, Av. Horácio Macedo, 950, Cidade Universitária, 21941-915 Rio de Janeiro, RJ, Brasil Manuscript received on September 24, 2013; accepted for publication on June 10, 2015 ABSTRACT This paper presents geochemical behaviour of trace elements of the felsic alkaline rocks of the state of Rio de Janeiro, Brazil, with special attention of fractional crystallization and continental crust assimilation. Fractionation of leucite and K-feldspar increases Rb/K and decreases K2O/(K2O+Na2O). Primitive nepheline syenite magmas have low Zr/TiO2, Sr, and Ba. On the Nb/Y vs. Zr/TiO2 diagram, these rocks are projected on the field of alkaline basalt, basanite, and nephelinite, instead of phonolite. Well-fractionated peralkaline nepheline syenite has high Zr/TiO2 but there are no zircon. The diagrams of silica saturation index (SSI) distinguish the trends originated form fractional crystallization and crustal assimilation. -
Chapter 10: Mantle Melting and the Generation of Basaltic Magma 2 Principal Types of Basalt in the Ocean Basins Tholeiitic Basalt and Alkaline Basalt
Chapter 10: Mantle Melting and the Generation of Basaltic Magma 2 principal types of basalt in the ocean basins Tholeiitic Basalt and Alkaline Basalt Table 10.1 Common petrographic differences between tholeiitic and alkaline basalts Tholeiitic Basalt Alkaline Basalt Usually fine-grained, intergranular Usually fairly coarse, intergranular to ophitic Groundmass No olivine Olivine common Clinopyroxene = augite (plus possibly pigeonite) Titaniferous augite (reddish) Orthopyroxene (hypersthene) common, may rim ol. Orthopyroxene absent No alkali feldspar Interstitial alkali feldspar or feldspathoid may occur Interstitial glass and/or quartz common Interstitial glass rare, and quartz absent Olivine rare, unzoned, and may be partially resorbed Olivine common and zoned Phenocrysts or show reaction rims of orthopyroxene Orthopyroxene uncommon Orthopyroxene absent Early plagioclase common Plagioclase less common, and later in sequence Clinopyroxene is pale brown augite Clinopyroxene is titaniferous augite, reddish rims after Hughes (1982) and McBirney (1993). Each is chemically distinct Evolve via FX as separate series along different paths Tholeiites are generated at mid-ocean ridges Also generated at oceanic islands, subduction zones Alkaline basalts generated at ocean islands Also at subduction zones Sources of mantle material Ophiolites Slabs of oceanic crust and upper mantle Thrust at subduction zones onto edge of continent Dredge samples from oceanic crust Nodules and xenoliths in some basalts Kimberlite xenoliths Diamond-bearing pipes blasted up from the mantle carrying numerous xenoliths from depth Lherzolite is probably fertile unaltered mantle Dunite and harzburgite are refractory residuum after basalt has been extracted by partial melting 15 Tholeiitic basalt 10 5 Figure 10-1 Brown and Mussett, A. E. (1993), The Inaccessible Earth: An Integrated View of Its Lherzolite Structure and Composition. -
Partial Melting - Simple Process, Huge Global Impact How Partial Melting, Coupled with Plate Tectonics, Has Changed the Chemistry of Our Planet
Earthlearningidea - http://www.earthlearningidea.com/ Partial melting - simple process, huge global impact How partial melting, coupled with plate tectonics, has changed the chemistry of our planet Demonstrating partial melting Explaining the planetary effects of partial melting Prepare two small beakers as described in the Each time that partial melting takes place during different resources section below. stages of the plate tectonic cycle, materials with different chemical and physical makeup are formed. Pre- prepared The starting point for these processes is the mantle, beakers where the most abundant elements are oxygen, silicon, magnesium and iron in that order. However the Earth’s crust contains much more silicon and oxygen and much less magnesium and iron than the mantle, and is formed through these stages: Photo: C. King. Stage 1: the mantle partially melts beneath oceanic ridges; the melt formed is richer in oxygen/silicon (and poorer in iron/magnesium) than the original mantle rock. This rises and then cools to form new oceanic crust and Show the pupils the beaker containing the mixture of ocean ridge volcanoes, as plates move apart. gravel and chopped candlewax before heating; ask what will happen if the beaker is heated until the wax Stage 2: the oceanic crust subducted beneath melts. Most will realise that the gravel will sink to the oceanic plates partially melts; the melt is still richer in bottom to form a mixed gravel/wax layer, whilst pure oxygen/silicon (and poorer in iron/ magnesium) than the wax will flow to the top to form another layer. Then original oceanic crust rock. -
On Charnockites ⁎ B
Available online at www.sciencedirect.com Gondwana Research 13 (2008) 30–44 www.elsevier.com/locate/gr GR Focus On charnockites ⁎ B. Ronald Frost , Carol D. Frost Department of Geology and Geophysics, University of Wyoming, Laramie, WY 82071, USA Received 4 June 2007; received in revised form 20 July 2007; accepted 24 July 2007 Available online 7 August 2007 Abstract Charnockitic rocks form extensive orthogneiss plutons in many granulite terranes and are less commonly found in unmetamorphosed plutons, which have formed in various tectonic regimes. Geochemically, clearly igneous charnockites cover nearly the whole range of granite chemistry, from magnesian to ferroan and from calcic to alkalic. Pyroxenes from unmetamorphosed charnockitic rocks have compositions ranging from magnesian to very iron-rich and record temperatures as high as 1000 °C. Oxygen fugacities for these plutons range from below FMQ to Δ log FMQN+2, values that cover nearly the whole range found in other granitic rocks. This range in bulk chemistry and intensive parameters is a reflection of the many mechanisms that produce charnockites. They may form in rifting environments, where they are ferroan, alkali-calcic to alkalic and metaluminous. Many of these ferroan charnockites are isotopically primitive, suggesting that they have been derived largely or entirely from differentiation or melting of tholeiitic melts. Charnockites are also found in deeply eroded arcs, where they are magnesian, calcic to calc-alkalic and metaluminous. Some charnockitic magmas may form by crustal melting or have incorporated a large component of crustal melt; these plutons tend to be weakly to moderately peraluminous and to have intermediate values of FeO/(FeO+MgO). -
Petrogenesis of Slab-Derived Trondhjemite-Tonalite-Dacite/ Adakite Magmas M
Transactions of the Royal Society of Edinburgh: Earth Sciences, 87, 205-215, 1996 Petrogenesis of slab-derived trondhjemite-tonalite-dacite/ adakite magmas M. S. Drummond, M. J. Defant and P. K. Kepezhinskas ABSTRACT: The prospect of partial melting of the subducted oceanic crust to produce arc magmatism has been debated for over 30 years. Debate has centred on the physical conditions of slab melting and the lack of a definitive, unambiguous geochemical signature and petrogenetic process. Experimental partial melting data for basalt over a wide range of pressures (1-32 kbar) and temperatures (700-1150=C) have shown that melt compositions are primarily trondhjemite- tonalite-dacite (TTD). High-Al (> 15% A12O3 at the 70% SiO2 level) TTD melts are produced by high-pressure 015 kbar) partial melting of basalt, leaving a restite assemblage of garnet + clinopyroxe'ne ± hornblende. A specific Cenozoic high-Al TTD (adakite) contains lower Y, Yb and Sc and higher Sr, Sr/Y, La'/Yb and.Zr/Sm relative to other TTD types and is interpreted to represent a slab melt under garnet amphibolite to eclogite conditions. High-Al TTD with an adakite-like geochemical character is prevalent in the Archean as the result of a higher geotherm that facilitated slab melting. Cenozoic adakite localities are commonly associated with the subduction of young (<25Ma), hot oceanic crust, which may provide a slab geotherm (*9-10=C km"1) conducive for slab dehydration melting. Viable alternative or supporting tectonic effects that may enhance slab melting include highly oblique convergence and resultant high shear stresses and incipient subduction into a pristine hot mantle wedge. -
Shallow-Crustal Metamorphism During Late Cretaceous Anatexis in the Sevier Hinterland Plateau: Peak Temperature Conditions from the Grant Range, Eastern Nevada, U.S.A
Shallow-crustal metamorphism during Late Cretaceous anatexis in the Sevier hinterland plateau: Peak temperature conditions from the Grant Range, eastern Nevada, U.S.A. Sean P. Long1*, Emmanuel Soignard2 1SCHOOL OF THE ENVIRONMENT, WASHINGTON STATE UNIVERSITY, PULLMAN, WASHINGTON 99164, USA 2LEROY EYRING CENTER FOR SOLID STATE SCIENCE, ARIZONA STATE UNIVERSITY, TEMPE, ARIZONA 85287, USA ABSTRACT Documenting spatio-temporal relationships between the thermal and deformation histories of orogenic systems can elucidate their evolu- tion. In the Sevier hinterland plateau in eastern Nevada, an episode of Late Cretaceous magmatism and metamorphism affected mid- and upper-crustal levels, concurrent with late-stage shortening in the Sevier thrust belt. Here, we present quantitative peak temperature data from the Grant Range, a site of localized, Late Cretaceous granitic magmatism and greenschist facies metamorphism. Twenty-two samples of Cambrian to Pennsylvanian metasedimentary and sedimentary rocks were analyzed, utilizing Raman spectroscopy on carbonaceous material, vitrinite reflectance, and Rock-Eval pyrolysis thermometry. A published reconstruction of Cenozoic extension indicates that the samples span pre-extensional depths of 2.5–9 km. Peak temperatures systematically increase with depth, from ~100 to 300 °C between 2.5 and 4.5 km, ~400 to 500 °C between 5 and 8 km, and ~550 °C at 9 km. The data define a metamorphic field gradient of ~60 °C/km, and are corroborated by quartz recrystallization microstructure and published conodont alteration indices. Metamorphism in the Grant Range is correlated with contemporary, upper-crustal metamorphism and magmatism documented farther east in Nevada, where metamorphic field gradients as high as ~50 °C/km are estimated. -
End of Chapter Question Answers Chapter 4 Review Questions 1
End of Chapter Question Answers Chapter 4 Review Questions 1. Describe the three processes that are responsible for the formation of magma. Answer: Magmas form from melting within the Earth. There are three types of melting: decompression melting, where magmas form when hot rock from deep in the mantle rises to shallower depths without undergoing cooling (the decrease in pressure facilitates the melting process); flux melting, where melting occurs due to the addition of volatiles such as CO2 and H2O; and heat transfer melting, where melting results from the transfer of heat from a hotter material to a cooler one. 2. Why are there so many different compositions of magma? Does partial melting produce magma with the same composition as the magma source from which it was derived? Answer: Magmas are formed from many different chemical constituents. Partial melting of rock yields magma that is more felsic (silicic) than the magma source because a higher proportion of chemicals needed to form felsic minerals diffuse into the melt at lower temperatures. Magma may incorporate chemicals dissolved from the solid rock through which it rises or from blocks of rock that fall into the magma. This process is called assimilation. Finally, fractional crystallization can modify magma composition as minerals crystallize out of a melt during the cooling process, causing the residual liquid to become progressively more felsic. 3. Why does magma rise from depth to the surface of the Earth? Answer: Magma rises toward the surface of the Earth because it is less dense than solid rock and buoyant relative to its surroundings. -
The Archean Geology of Montana
THE ARCHEAN GEOLOGY OF MONTANA David W. Mogk,1 Paul A. Mueller,2 and Darrell J. Henry3 1Department of Earth Sciences, Montana State University, Bozeman, Montana 2Department of Geological Sciences, University of Florida, Gainesville, Florida 3Department of Geology and Geophysics, Louisiana State University, Baton Rouge, Louisiana ABSTRACT in a subduction tectonic setting. Jackson (2005) char- acterized cratons as areas of thick, stable continental The Archean rocks in the northern Wyoming crust that have experienced little deformation over Province of Montana provide fundamental evidence long (Ga) periods of time. In the Wyoming Province, related to the evolution of the early Earth. This exten- the process of cratonization included the establishment sive record provides insight into some of the major, of a thick tectosphere (subcontinental mantle litho- unanswered questions of Earth history and Earth-sys- sphere). The thick, stable crust–lithosphere system tem processes: Crustal genesis—when and how did permitted deposition of mature, passive-margin-type the continental crust separate from the mantle? Crustal sediments immediately prior to and during a period of evolution—to what extent are Earth materials cycled tectonic quiescence from 3.1 to 2.9 Ga. These compo- from mantle to crust and back again? Continental sitionally mature sediments, together with subordinate growth—how do continents grow, vertically through mafi c rocks that could have been basaltic fl ows, char- magmatic accretion of plutons and volcanic rocks, acterize this period. A second major magmatic event laterally through tectonic accretion of crustal blocks generated the Beartooth–Bighorn magmatic zone assembled at continental margins, or both? Structural at ~2.9–2.8 Ga. -
The Origin of Himalayan Anatexis and Inverted Metamorphism: Models and Constraints
Journal of Asian Earth Sciences 17 (1999) 755±772 The origin of Himalayan anatexis and inverted metamorphism: Models and constraints T. Mark Harrison*, Marty Grove, Oscar M. Lovera, E.J. Catlos, Jessica D'Andrea Department of Earth and Space Sciences and Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095-1567, USA Abstract The key to comprehending the tectonic evolution of the Himalaya is to understand the relationships between large-scale faulting, anatexis, and inverted metamorphism. The great number and variety of mechanisms that have been proposed to explain some or all of these features re¯ects the fact that fundamental constraints on such models have been slow in coming. Recent developments, most notably in geophysical imaging and geochronology, have been key to coalescing the results of varied Himalayan investigations into constraints with which to test proposed evolutionary models. These models fall into four general types: (1) the inverted metamorphic sequences within the footwall of the Himalayan thrust and adjacent hanging wall anatexis are spatially and temporally related by thrusting; (2) thrusting results from anatexis; (3) anatexis results from normal faulting; and (4) apparent inverted metamorphism in the footwall of the Himalayan thrust is produced by underplating of right-way-up metamorphic sequences. We review a number of models and ®nd that many are inconsistent with available constraints, most notably the recognition that the exposed crustal melts and inverted metamorphic sequences not temporally related. The generalization that appears to best explain the observed distribution of crustal melts and inverted metamorphic sequences is that, due to speci®c petrological and tectonic controls, episodic magmatism and out-of-sequence thrusting developed during continuous convergence juxtaposing allochthonous igneous and metamorphic rocks. -
Mineralogical Evidence for Partial Melting and Melt-Rock Interaction Processes in the Mantle Peridotites of Edessa Ophiolite (North Greece)
minerals Article Mineralogical Evidence for Partial Melting and Melt-Rock Interaction Processes in the Mantle Peridotites of Edessa Ophiolite (North Greece) Aikaterini Rogkala 1,* , Petros Petrounias 1 , Basilios Tsikouras 2 , Panagiota P. Giannakopoulou 1 and Konstantin Hatzipanagiotou 1 1 Section of Earth Materials, Department of Geology, University of Patras, 265 04 Patras, Greece; [email protected] (P.P.); [email protected] (P.P.G.); [email protected] (K.H.) 2 Physical and Geological Sciences, Faculty of Science, Universiti Brunei Darussalam, Jalan Tungku Link, Gadong BE1410, Bandar Seri Begawan, Brunei Darussalam; [email protected] * Correspondence: [email protected]; Tel.: +30-2610996288 Received: 10 December 2018; Accepted: 14 February 2019; Published: 17 February 2019 Abstract: The Edessa ophiolite complex of northern Greece consists of remnants of oceanic lithosphere emplaced during the Upper Jurassic-Lower Cretaceous onto the Palaeozoic-Mesozoic continental margin of Eurasia. This study presents new data on mineral compositions of mantle peridotites from this ophiolite, especially serpentinised harzburgite and minor lherzolite. Lherzolite formed by low to moderate degrees of partial melting and subsequent melt-rock reaction in an oceanic spreading setting. On the other hand, refractory harzburgite formed by high degrees of partial melting in a supra-subduction zone (SSZ) setting. These SSZ mantle peridotites contain Cr-rich spinel residual after partial melting of more fertile (abyssal) lherzolite with Al-rich spinel. Chromite with Cr# > 60 in harzburgite resulted from chemical modification of residual Cr-spinel and, along with the presence of euhedral chromite, is indicative of late melt-peridotite interaction in the mantle wedge. Mineral compositions suggest that the Edessa oceanic mantle evolved from a typical mid-ocean ridge (MOR) oceanic basin to the mantle wedge of a SSZ.