Geochemistry and Mineralogy of Basalts from the South Mid-Atlantic
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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. -
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 Surface Reactions of Silicate Minerals
RESEARCH BULLETIN 614 SEPTEMBER, 1956 UNIVERSITY OF MISSOURI COLLEGE OF AGRICULTURE AGRICULTURAL EXPERIMENT STATION J. H. Longwell, Director The Surface Reactions Of Silicate Minerals PART II. REACTIONS OF FELDSPAR SURFACES WITH SALT SOLUTIONS. V. E. NASH AND C. E. MARSHALL (Publication authorized September 5, 1956) COLUMBIA, MISSOURI TABLE OF CONTENTS Introduction .......... .. 3 The Interaction of Albite with Salt Solutions . .. 4 The Interaction of Anorthite with Salt Solutions ........ .. 7 Relative Effectiveness of Ammonium Chloride and Magnesium Chloride on the Release of Sodium from Albite . .. 9 Surface Interaction of Albite with Salt Solutions in Methanol . .. 13 Experiments on Cationic Fixation ............................... 16 Detailed Exchange and Activity Studies with Individual Feldspars .......... .. 19 Procedure .. .. 20 Microcline . .. 21 Albite .................................................... 22 Oligoclase . .. 23 Andesine . .. 24 Labradori te . .. 25 Bytownite ................................................. 25 Anorthite . .. 27 Discussion ........ .. 28 Summary ..................................................... 35 References .. .. 36 Most of the experimental material of this and the preceding Research Bulletin is taken from the Ph.D. Thesis of Victor Nash, University of Missouri, June 1955. The experiments on cation fixation were carried our with the aid of a research grant from the Potash Rock Company of America, Lithonia, Georgia, for which the authors wish to record their appreciation. The work was part of Department of Soils Research Project No.6, entitled, "Heavy Clays." The Surface Reactions of Silicate Minerals PART II. REACTIONS OF FELDSPAR SURFACES WITH SALT SOLUTIONS. v. E. NASH AND C. E. MARSHALL INTRODUCTION The review of literature cited in Part I of this series indicates that little is known of the interaction of feldspar surfaces with salt solutions. The work of Breazeale and Magistad (1) clearly demonstrated that ex change reactions between potassium and calcium occur in the case of or thoclase surfaces. -
Noritic Anorthosite Bodies in the Sierra Nevada Batholith
MINERALOGICAL SOCIETY OF AMERICA, SPECIAL PAPER 1, 1963 INTERNATIONALMINERALOGICAL ASSOCIATION,PAPERS, THIRD GENERAL MEETING NORITIC ANORTHOSITE BODIES IN THE SIERRA NEVADA BATHOLITH ALDEN A. LOOMISl Department of Geology, Stanford University, Stanford, California ABSTRACT A group of small noritic plutons were intruded prior to the immediately surrounding granitic rocks in a part of the composite Sierra Nevada batholith near Lake Tahoe. Iron was more strongly concentrated in the late fluids of individual bodies than during the intrusive sequence as a whole. Pyroxenes are more ferrous in rocks late in the sequence, although most of the iron is in late magnetite which replaces pyroxenes. Both Willow Lake type and normal cumulative layering are present. Cumulative layering is rare; Willi ow Lake layering is common and was formed early in individual bodies. Willow Lake layers require a compositional uniqueness providing high ionic mobility to explain observed relations. The Sierran norites differ from those in large stratiform plutons in that (1) the average bulk composition is neritic anorthosite in which typical rocks contain over 20% AbO" and (2) differentiation of both orthopyroxene and plagioclase produced a smooth progressive sequence of mineral compositions. A plot of modal An vs. En for all the rocks in the sequence from early Willow Lake-type layers to late no rite dikes defines a smooth non-linear trend from Anss-En76 to An,,-En54. TLe ratio An/ Ab decreased faster than En/Of until the assemblage Anso-En65 was reached and En/Of began to decrease more rapidly. Similar plots for large stratiform bodies show too much scatter to define single curves. -
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. -
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. -
And
Sarah Lambart - 2016 Recap Lecture 16: Isotopes 101 • Radioactive (parent) vs. radiogenic (daugher) isotopes • Unstable (radioactive) vs stable isotopes • Uses: for dating (geochronology) and as tracers (source composition) Recap Lecture 16: Isotopes 101 • As tracers: • Ex.: 87Sr/86Sr: DMM < co < cc High Rb/Sr c.c. Crust evolution o.c. 87Sr 86Sr melting event DMM Low Rb/Sr Mantle Primitive Mantle/BSE Depleted mantle evolution € 4.55 b.y. Time -> today Recap Lecture 16: Isotopes 101 • As tracers: • Ex.: 87Sr/86Sr: DMM < co < cc • Isotopes do not fractionate during partial melting and crystallization processes!!! ⇒ 87Sr/86Sr (source) = 87Sr/86Sr (magma) ⇒ if 87Sr/86Sr (magma) ≠ constant ⇒ several source components (subducted oc, subducted sediments, subcontinental lithosphere, ect…) or crustal contamination (AFC) Mid-Ocean Ridges Basalt (MORB) • Facts: • Oceanic floors: 60% of Earth’s surface • Most of the rocks produced at ridges are MORB • Large compositional variability 3) Source composition 2) Melting conditions (Pressure, Temperature) 4) Melt segregation and transport 1) Magma differentiation/crystallization Structure of Mid-Ocean Ridges • Ridges: submarine (most of the time) mountain chains ≈ 3000m Slow-spreading ridge: Fast-spreading ridge: Ex.: Mid-Atltantic ridge : 2cm/yr Ex.: EPR: 10 cm/yr Fig. 13-15 in Winters Structure of Mid-Ocean Ridges • Ridges: submarine (most of the time) mountain chains ≈ 3000m Slow-spreading ridge: Fast-spreading ridge: Ex.: Mid-Atltantic ridge : 2cm/yr Ex.: EPR: 10 cm/yr - Spreading rate: 8-10 cm/yr - Spreading rate: <5 cm/yr - Axial uplift = horst - Axial valley = rift (relief = 300m) - Bigger magma reservoir ⇒ more differentiation - Numerous normal faults: active seismic zone - Small multiple magma reservoirs? The oceanic lithosphere • Maturation d(m) = 2500 + 350 T1/2 (Ma) Fig. -
A Database of Plagioclase Crystal Preferred Orientations (CPO)
Solid Earth, 4, 511–542, 2013 Open Access www.solid-earth.net/4/511/2013/ doi:10.5194/se-4-511-2013 Solid Earth © Author(s) 2013. CC Attribution 3.0 License. A database of plagioclase crystal preferred orientations (CPO) and microstructures – implications for CPO origin, strength, symmetry and seismic anisotropy in gabbroic rocks T. Satsukawa1,2,*, B. Ildefonse2, D. Mainprice2, L. F. G. Morales3, K. Michibayashi1,4, and F. Barou2 1Graduate School of Science and Technology, Shizuoka University, Ohya 836, Shizuoka 422-8529, Japan 2Géosciences Montpellier, Université Montpellier 2 and CNRS, CC 060, 34095 Montpellier cedex 5, France 3Helmholtz Zentrum Potsdam, Deutsches GeoForschungsZentrum (GFZ), Telegrafenberg, 14473 Potsdam, Germany 4Institute of Geosciences, Shizuoka University, Ohya 836, Shizuoka 422-8529, Japan *present address: ARC Center of Excellence for Core to Crust Fluid Systems (CCFS) and GEMOC National Key Centre, Department of Earth and Planetary Sciences, Macquarie University, Sydney, NSW 2109, Australia Correspondence to: T. Satsukawa ([email protected]) Received: 3 August 2013 – Published in Solid Earth Discuss.: 14 August 2013 Revised: 14 November 2013 – Accepted: 19 November 2013 – Published: 18 December 2013 Abstract. This study presents a unique database of 172 pla- ture compared with magmatic flow, and the large number gioclase Crystallographic Preferred Orientations (CPO) of of possible slip-systems in plagioclase probably account for variously deformed gabbroic rocks. The CPO characteris- these differences. Calculated seismic properties (P wave and tics as a function of the deformation regime (magmatic or S wave velocities and anisotropies) of plagioclase aggregates crystal-plastic) are outlined and discussed. The studied sam- show that anisotropy (up to 12 % for P wave and 14 % for ples are dominantly from slow- and fast-spread present-day S wave) tends to increase as a function of ODF J index. -
Paleomagnetic Reconstruction in the Troodos Ophiolite Gabbro
The oceanic crust in 3D: Paleomagnetic reconstruction in the Troodos ophiolite gabbro Abstract The Troodos complex, Cyprus, provides an opportunity to study the structural configuration along a fossil intersection of a spreading axis and a transform fault. We complement studies at Troodos that have reconstructed the brittle deformation of the upper crust by new paleomagnetic data from the gabbro suite. The gabbro suite is exposed at the extinct spreading axis continuing the Solea graben toward the intersection with the fossil Arakapas oceanic transform. This is a unique exposure of deep crustal rocks formed at both an inside-corner and an outside-corner of a ridge- transform intersection. Remanence directions from gabbros (24 sites) were used as indicators for rigid body rotation. The spatial distribution of rotation axes allow recognition of three regions to which deformation is partitioned: 1) a western region (outside corner) that experienced primarily tilt about horizontal axis 2) a central region with minor rotation and, 3) an eastern area (inside corner) where vertical axis rotations are dominant. The absence of significant rotation in the 6 km-wide central domain together with its location between the inside- and the outside corner uncover the root of a fossil axial volcanic zone, a zone sufficiently hot so the upper crust can decouple from the substrate. Clockwise rotation in the gabbro increases from the axial zone eastward, similar to that in the overlying dikes, indicating coupling of the lower crust with the brittle upper oceanic crust. The transition from the decoupled layers of sheeted dikes and gabbro in the axial-zone to the dikes- gabbro coupling in the inside corner is in keeping with deepening of the brittle-ductile transition from the dike-gabbro boundary into the lower crust away from the axial zone. -
Optical Properties of Common Rock-Forming Minerals
AppendixA __________ Optical Properties of Common Rock-Forming Minerals 325 Optical Properties of Common Rock-Forming Minerals J. B. Lyons, S. A. Morse, and R. E. Stoiber Distinguishing Characteristics Chemical XI. System and Indices Birefringence "Characteristically parallel, but Mineral Composition Best Cleavage Sign,2V and Relief and Color see Fig. 13-3. A. High Positive Relief Zircon ZrSiO. Tet. (+) 111=1.940 High biref. Small euhedral grains show (.055) parallel" extinction; may cause pleochroic haloes if enclosed in other minerals Sphene CaTiSiOs Mon. (110) (+) 30-50 13=1.895 High biref. Wedge-shaped grains; may (Titanite) to 1.935 (0.108-.135) show (110) cleavage or (100) Often or (221) parting; ZI\c=51 0; brownish in very high relief; r>v extreme. color CtJI\) 0) Gamet AsB2(SiO.la where Iso. High Grandite often Very pale pink commonest A = R2+ and B = RS + 1.7-1.9 weakly color; inclusions common. birefracting. Indices vary widely with composition. Crystals often euhedraL Uvarovite green, very rare. Staurolite H2FeAI.Si2O'2 Orth. (010) (+) 2V = 87 13=1.750 Low biref. Pleochroic colorless to golden (approximately) (.012) yellow; one good cleavage; twins cruciform or oblique; metamorphic. Olivine Series Mg2SiO. Orth. (+) 2V=85 13=1.651 High biref. Colorless (Fo) to yellow or pale to to (.035) brown (Fa); high relief. Fe2SiO. Orth. (-) 2V=47 13=1.865 High biref. Shagreen (mottled) surface; (.051) often cracked and altered to %II - serpentine. Poor (010) and (100) cleavages. Extinction par- ~ ~ alleL" l~4~ Tourmaline Na(Mg,Fe,Mn,Li,Alk Hex. (-) 111=1.636 Mod. biref. -
29. Sulfur Isotope Ratios of Leg 126 Igneous Rocks1
Taylor, B., Fujioka, K., et al., 1992 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 126 29. SULFUR ISOTOPE RATIOS OF LEG 126 IGNEOUS ROCKS1 Peter Torssander2 ABSTRACT Sulfur isotope ratios have been determined in 19 selected igneous rocks from Leg 126. The δ34S of the analyzed rocks ranges from -0.1 o/00 to +19.60 o/oo. The overall variation in sulfur isotope composition of the rocks is caused by varying degrees of seawater alteration. Most of the samples are altered by seawater and only five of them are considered to have maintained their magmatic sulfur isotope composition. These samples are all from the backarc sites and have δ34S values varying from +0.2 o/oo to +1.6 o/oo , of which the high δ34S values suggest that the earliest magmas in the rift are more arc-like in their sulfur isotope composition than the later magmas. The δ34S values from the forearc sites are similar to or heavier than the sulfur isotope composition of the present arc. INTRODUCTION from 0 o/oo to +9 o/00 (Ueda and Sakai, 1984), which could arise from inhomogeneities in the mantle but are more likely a result of contami- Sulfur is a volatile element that can be degassed during the ascent nation from the subducting slab (A. Ueda, pers. comm., 1988). of basaltic magma. Degassing causes sulfur isotope fractionation; the Leg 126 of the Ocean Drilling Program (ODP) drilled seven sites isotopic composition of sulfur in rocks can vary with the concentra- in the backarc and forearc of the Izu-Bonin Arc (Fig.