Geochemical Constraints on Mantle Melting and Magma Genesis at Pohnpei Island, Micronesia
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Geochemistry of Sideromelane and Felsic Glass Shards in Pleistocene Ash Layers at Sites 953, 954, and 9561
Weaver, P.P.E., Schmincke, H.-U., Firth, J.V., and Duffield, W. (Eds.), 1998 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 157 25. GEOCHEMISTRY OF SIDEROMELANE AND FELSIC GLASS SHARDS IN PLEISTOCENE ASH LAYERS AT SITES 953, 954, AND 9561 Andrey A. Gurenko2 and Hans-Ulrich Schmincke2 ABSTRACT Sideromelane and felsic glass shards from unconsolidated Pleistocene volcaniclastic sediments drilled at Sites 953, 954, and 956 are thought to have derived from submarine and subaerial volcanic eruptions on Gran Canaria (Sites 953 and 954) and Tenerife (Sites 954 and 956). We analyzed these glasses by electron microprobe for major elements and sulfur, chlorine, and fluorine. Sideromelane glasses represent a spectrum from alkali basalt through basanite, hawaiite, mugearite, and tephrite to nephelinite. Felsic glasses have compositions similar to benmoreite, trachyte, and phonolite. Vesiculated mafic and felsic glass shards, which are characterized by low S and Cl concentrations (0.01−0.06 wt% S and 0.01–0.04 wt% Cl), are interpreted to have formed by pyroclastic activity on land or in shallow water and appeared to have been strongly degassed. Vesicle-free blocky glass shards having 0.05−0.13 wt% S are likely to have resulted from submarine eruptions at moderate water depths and represent undegassed or slightly degassed magmas. Cl concentrations range from 0.01 to 0.33 wt% and increase with increasing MgO, suggesting that Cl behaves as an incompatible element during magma crystallization. Concentrations of fluorine (0.04− 0.34 wt% F) are likely to represent undegassed values, and the variations in F/K ratios between 0.02 and 0.24 are believed to reflect those of parental magmas and of the mantle source. -
Chemical Composition of Earth's Primitive Mantle and Its Variance: 2
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, B03212, doi:10.1029/2005JB004224, 2007 Click Here for Full Article Chemical composition of Earth’s primitive mantle and its variance: 2. Implications for global geodynamics Tanya Lyubetskaya1 and Jun Korenaga1 Received 16 December 2005; revised 17 June 2006; accepted 20 November 2006; published 29 March 2007. [1] The global budgets of argon and heat-producing elements have traditionally been used to argue for layered-mantle convection because they require a large fraction of Earth’s mantle to remain isolated from mantle convection. We revise these mass balance arguments using our new composition model of the primitive mantle and show that the global budgets of argon, heat-producing elements, and rare earth elements are consistent with Earth’s mantle almost entirely composed of the mid-ocean ridge basalt source mantle, supporting the notion of whole mantle convection. Combined with a recent theory on the thermal evolution of Earth, our revised thermal budget implies inefficient mixing and processing in the past, explaining the survival of long-lived geochemical heterogeneities in convecting mantle. Citation: Lyubetskaya, T., and J. Korenaga (2007), Chemical composition of Earth’s primitive mantle and its variance: 2. Implications for global geodynamics, J. Geophys. Res., 112, B03212, doi:10.1029/2005JB004224. 1. Introduction arguments do not provide a robust constraint on the size of such a hidden reservoir, because the interpretation of [2] The structure of mantle convection has been one of geochemical data is often model-dependent. For example, the most controversial subjects in modern geodynamics and observed geochemical differences between mantle-derived geochemistry. -
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. -
Complex Basalt-Mugearite Sill in Piton Des Neiges Volcano, Reunion
THE AMERICAN MINERALOGIST. VOL. 52, SEPTEMBER-OCTOBER, 1967 COMPLEX BASALT-MUGEARITE SILL IN PITON DES NEIGES VOLCANO, REUNION B. G. J. UetoN, Grant Institute oJ Geology,Uniaersi,ty oJ Ed.inburgh, Edinbwrgh, Scotland, AND W. J. WaoswoRru, Deportmentof Geology,The Un'it;ersity, Manchester,England.. ABsrRAcr An extensive suite of minor intrusions, contempcraneous with the late-stage differenti- ated lavas of Piton des Neiges volcano, occurs within an old agglomeratic complex. An 8-m sill within this suite is strongly difierentiated with a basaltic centre (Thorton Tuttle Index 27.6), residual veins of benmoreite (T. T. Index 75.2), and still more extreme veinlets of quartz trachyte. Although gravitative settling of olivine, augite and ore irz silzr is believed to be responsible for some of the observed variation, the over-all composition of the sill is con- siderably more basic than the mugearite which forms the chilled contacts. It is therefore concluded that considerable magmatic difierentiation must have preceded the emplacement of the sill. This probably took place in a dykeJike magma body with a compositional gra- dient from mugearite at the top to olivine basalt in the lower parts. INrnonucrroN The island of Reunion, in the western Indian Ocean, has the form of a volcanic doublet overlying a great volcanic complex rising from the deep ocean floor. The southeastern component of this doublet is still highly active and erupts relatively undifierentiated, olivine-rich basalts of mildly alkaline or transitional type (Coombs, 1963; Upton and Wads- worth, 1966). The northwestern volcano however has been inactive a sufficient time for erosionalprocesses to have hollowed out amphitheatre- headed valleys up to 2500 meters deep in the volcanic pile. -
Nonexplosive and Explosive Magma/Wet-Sediment Interaction
Journal of Volcanology and Geothermal Research 181 (2009) 155–172 Contents lists available at ScienceDirect Journal of Volcanology and Geothermal Research journal homepage: www.elsevier.com/locate/jvolgeores Nonexplosive and explosive magma/wet-sediment interaction during emplacement of Eocene intrusions into Cretaceous to Eocene strata, Trans-Pecos igneous province, West Texas Kenneth S. Befus a,⁎, Richard E. Hanson a, Daniel P. Miggins b, John A. Breyer a, Arthur B. Busbey a a Department of Geology, Texas Christian University, Box 298830, Fort Worth, TX 76129, USA b U.S. Geological Survey, Denver Federal Center, Box 25046, Denver, CO 80225, USA article info abstract Article history: Eocene intrusion of alkaline basaltic to trachyandesitic magmas into unlithified, Upper Cretaceous Received 16 June 2008 (Maastrichtian) to Eocene fluvial strata in part of the Trans-Pecos igneous province in West Texas produced Accepted 22 December 2008 an array of features recording both nonexplosive and explosive magma/wet-sediment interaction. Intrusive Available online 13 January 2009 complexes with 40Ar/39Ar dates of ~47–46 Ma consist of coherent basalt, peperite, and disrupted sediment. Two of the complexes cutting Cretaceous strata contain masses of conglomerate derived from Eocene fluvial Keywords: deposits that, at the onset of intrusive activity, would have been N400–500 m above the present level of phreatomagmatism peperite exposure. These intrusive complexes are inferred to be remnants of diatremes that fed maar volcanoes during diatreme an early stage of magmatism in this part of the Trans-Pecos province. Disrupted Cretaceous strata along Trans-Pecos Texas diatreme margins record collapse of conduit walls during and after subsurface phreatomagmatic explosions. -
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. -
Alkalic-Type Epithermal Gold Deposit Model
Alkalic-Type Epithermal Gold Deposit Model Chapter R of Mineral Deposit Models for Resource Assessment Scientific Investigations Report 2010–5070–R U.S. Department of the Interior U.S. Geological Survey Cover. Photographs of alkalic-type epithermal gold deposits and ores. Upper left: Cripple Creek, Colorado—One of the largest alkalic-type epithermal gold deposits in the world showing the Cresson open pit looking southwest. Note the green funnel-shaped area along the pit wall is lamprophyre of the Cresson Pipe, a common alkaline rock type in these deposits. The Cresson Pipe was mined by historic underground methods and produced some of the richest ores in the district. The holes that are visible along several benches in the pit (bottom portion of photograph) are historic underground mine levels. (Photograph by Karen Kelley, USGS, April, 2002). Upper right: High-grade gold ore from the Porgera deposit in Papua New Guinea showing native gold intergrown with gold-silver telluride minerals (silvery) and pyrite. (Photograph by Jeremy Richards, University of Alberta, Canada, 2013, used with permission). Lower left: Mayflower Mine, Montana—High-grade hessite, petzite, benleonardite, and coloradoite in limestone. (Photograph by Paul Spry, Iowa State University, 1995, used with permission). Lower right: View of north rim of Navilawa Caldera, which hosts the Banana Creek prospect, Fiji, from the portal of the Tuvatu prospect. (Photograph by Paul Spry, Iowa State University, 2007, used with permission). Alkalic-Type Epithermal Gold Deposit Model By Karen D. Kelley, Paul G. Spry, Virginia T. McLemore, David L. Fey, and Eric D. Anderson Chapter R of Mineral Deposit Models for Resource Assessment Scientific Investigations Report 2010–5070–R U.S. -
Mantle Plumes
Geol. 655 Isotope Geochemistry Lecture 21 Spring 2007 ISOTOPIC EVOLUTION OF THE MANTLE IV THE ORIGIN OF MANTLE PLUMES AND THE COMMON COMPONENT IN PLUMES Determining how the various geochemical reservoirs of the mantle have evolved is among the most vexing problems in geochemistry. The principal observation to be explained is that mantle plumes in- variably have less depleted isotopic signatures than MORB, and the isotopic compositions of some in- dicate net enrichment in incompatible elements. As we saw in the previous lecture, mantle plumes were initially thought to consist of primitive mantle (e.g., Schilling, 1973). As we found, mixing be- tween primitive and depleted mantle can explain the Sr and Nd isotopic compositions of some plumes, but virtually none of the Pb isotope data can be explained this way, nor are the trace element composi- tions of OIB consistent with plumes being composed of primitive mantle. Indeed, although ‘primitive mantle’ has proved to be a useful hypothetical concept, no mantle-derived basalts or xenoliths have appropriate compositions to be ‘primitive mantle’ or derived from it. It is possible that no part of the mantle retains its original, primitive, composition (on the other hand, to have survived, primitive man- tle must not participate in volcanism and other such processes, so the absence of evidence for a primi- tive mantle reservoir is not evidence of its absence). Hofmann and White (1982) suggested mantle plumes obtain their unique geochemical signature through deep recycling of oceanic crust (Figure 21.1). Partial melting at mid-ocean ridges creates oce- anic crust that is less depleted in incompatible elements than the depleted upper mantle. -
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. -
THE PETROCHEMISTRY of JAKE M: a MARTIAN MUGEARITE. Stolper
44th Lunar and Planetary Science Conference (2013) 1685.pdf THE PETROCHEMISTRY OF JAKE_M: A MARTIAN MUGEARITE. Stolper, E.M.1, Baker, M.B.1, Fisk, M.2, Gellert, R.3, King, P.L.4, McLennan, S.M.5, Minitti, M.6, Newcombe, M.1, Schmidt, M.E. 7, Treiman, A.H.8, and the MSL Science Team. 1Caltech, Pasadena, CA 91125, 2Oregon State Univ., 3Univ. Guelph, 4Res. School Earth Sci., ANU, 5SUNY, Stony Brook, 6Applied Phys. Lab., Johns Hopkins Univ., 7Brock Univ., 8Lunar & Planet. Inst. Introduction: Rock “Jake_M” (JM; named for JPL The surface of JM was not brushed or abraded prior engineer Jake Matijevic) was the first sample analyzed to analysis, so the APXS analyses probably include by the Alpha Particle X-ray Spectrometer (APXS) in- contributions from surface coatings, including adhering strument on MSL [1]. Although it is an isolated frag- dust, and these are the probable source of the S and Cl ment lacking field context, its dark color and apparently in JM. Experience with MER, however, indicates that fine-grained texture suggested it was a relatively homo- the characteristics of rock compositions are typically geneous igneous rock and thus an appropriate sample to not obscured by surface components, and the levels of S initiate the APXS analytical program. We report here and Cl in JM are lower than virtually all unbrushed the preliminary APXS analyses of JM and a plausible analyses from the Spirit rover and lower than many of interpretation of their significance for petrogenesis. the brushed analyses, so the level of surface contamina- Results: Three spots on JM were analyzed with the tion and alteration are likely relatively minor [5]. -
Chemical Composition of Earth's Primitive Mantle and Its Variance
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, B03211, doi:10.1029/2005JB004223, 2007 Click Here for Full Article Chemical composition of Earth’s primitive mantle and its variance: 1. Method and results Tanya Lyubetskaya1 and Jun Korenaga1 Received 16 December 2005; revised 17 June 2006; accepted 20 November 2006; published 29 March 2007. [1] We present a new statistical method to construct a model for the chemical composition of Earth’s primitive mantle along with its variance. Earth’s primitive mantle is located on the melting trend exhibited by the global compilation of mantle peridotites, using cosmochemical constraints on the relative abundances of refractory lithophile elements (RLE). This so-called pyrolite approach involves the least amount of assumptions, thereby being probably most satisfactory compared to other approaches. Its previous implementations, however, suffer from questionable statistical treatment of noisy geochemical data, leaving the uncertainty of model composition poorly quantified. In order to properly take into account how scatters in peridotite data affect this geochemical inference, we combine the following statistical techniques: (1) modeling a nonlinear melting trend in the multidimensional compositional space through the principal component analysis, (2) determining the primitive mantle composition on the melting trend by simultaneously imposing all of cosmochemical constraints with least squares, and (3) mapping scatters in original data into the variance of the final model through the bootstrap resampling technique. Whereas our model is similar to previous models in terms of Mg, Si, and Fe abundances, the RLE contents are at 2.16 ± 0.37 times the CI chondrite concentration, which is lower than most of previous estimates.