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Volcn Ollage (2117'S) is a large stratovolcano that liesslightly east of the main axis of Quaternary Volcanoes in theAndean Central Volcanic Zone (CVZ). Euptive products range frombasaltic andesite to dacite and define a high-K, calc-alkalinesuite. This compositional range is similar to the collectivecompositional range of the other stratovolcanoes in the CVZ,and it provides a record of both early and late-stage differentiationprocesses operating at the stratovolcanoes. The volumetrically dominant andesitic and dacitic lavas aredivided into four eruptive series on the basis of vent locationsand petrography. In ascending stratigraphic order they are:the Vinta Loma, Chasca Orkho, post-collapse, and La Celosa series.Whole-rock compositions of the lavas are remarkably similarregardless of eruptive series. Variations in phenocryst assemblagesand magmatic fo2 however, suggest differences in subliquidusvolatile contents for magma chambers developed beneath the summitof the volcano versus those developed beneath the flanks. Basalticandesite magmas are principally preserved as quenched inclusionswithin the andesitic and dacitie lava flows. Large ranges inisotopic ratios over a narrow compositional range indicate thatthe basaltic andesites were derived by crystal fractionationcoupled with large amounts of crustal assimilation. IncreasingCe/Yb ratios with decreasing Yb contents further suggest thatthis initial stage of differentiation occurred at deep crustallevels where garnet was stable. Additional supporting evidencefor differentiation in the deep crust includes isotopic andtrace element compositions that indicate assimilation by thebasaltic andesite magmas of a crust different from upper-crustalrocks exposed at present in the region. Whole-rock major and trace element trends of the dacitic lavascan be simulated largely by fractional crystallization of parentalandesitic magma. The fractionating assemblages for the differenteruptive series are consistent with the observed modes of theparent magmas. Small increases in Sr isotope ratios with increasingRb contents indicate that the fractionating magmas also assimilatedsmall amounts of wall rocks similar in composition to the upper-crustalbasement to the volcano. Consideration of the chemical trends, mineral compositions,and eruptive history of Ollage rocks permits construction ofa model for the evolution of shallow crustal magma chambersbeneath the stratovolcanoes in the CVZ. At a relatively maturestage, the magma chambers may be compositionally, thermally,and density stratified. Temperatures estimated from Fe-Ti oxideand pyroxene thermometry for the chambers beneath Ollage rangefrom 1000 to 790C with increasing SiO2 from 59 to 67 wt.% inthe upper reaches, and from 1150 to 1020C with increasing SiO2from 53 to 59 wt.% in the lower reaches. The occurrence of basalticandesite magmatic inclusions within the intermediate lavas andthe repeated eruption of monotonous composition andesitic magmasindicate that the shallow chambers are periodically replenishedwith parental basaltic andesite magmas. Ubiquitous, reversely zoned plagioclase and pyroxene phenocrystsin the lavas at Ollage suggest that convective cooling of thebasaltic andesite releases buoyant derivative liquid that mixeswith the overlying intermediate-composition body of the chambers.Further crystallization and differentiation of the intermediatemagmas may take place in solidification zones at the boundariesof the magma chambers. If so, the return of residual liquidfrom the crystallizing margins and mixing with the interiorare highly efficient such that magma differentiation can bemodeled as a simple, homogeneous, fractional crystallizationprocess. 相似文献
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Dry deposition of particles 总被引：5，自引：0，他引：5
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DAVIDSON BLACK 《地质学报》1926,(Z1)
A rich fossiliferous deposit at Chou Kou Tien 70 li to the south west of Peking was first discovered in the summer of 1921 by Dr. J. G. Andersson and later surveyed and partially excavated by Dr. O Zdansky. A preliminary roport on the site was published by Dr. Andersson in March 1923 (Mem. Geol. 相似文献
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The island of St Martin lies inthe inactive part of the northernLesser Antilles island arc. The island consists of volcaniclasticsediments overlain and intruded by volcanic and plutonic rocks,which are in turn overlain by Miocene limestones. The extrusiveand intrusive rock suites are closely spaced in time (around27 Ma) although field relations suggest that the volcanic rockswere intruded by the plutons. Pluton emplacement gave rise tothermal metamorphism of the volcanic and volcaniclastic carapace,and to widespread hydrothermal alteration throughout the island. Geochemically, the igneous rocks of St Martin form a mildlytholeiitic to calc-alkaline typical subduction-related suite.The extrusive rocks are basalts to andesites, and the magmasappear to have differentiated largely through fractional crystallizationof plagioclase, clinopyroxene, and olivine. The REE displayflat chondrite-normalized patterns, with no significant Eu anomalydespite convincing evidence for plagioclase fractionation. Theplutonic rocks are more silica-rich diorites to granites, containingplagioclase, amphibole, and, less commonly, K-feldspar, sphene,zircon, and pyroxene. REE patterns are slightly LREE enrichedbut display distinct negative Eu anomalies. The fractionationof amphibole and accessory phases may have been important inthe evolution of the plutonic suite, as REE contents do notincrease overall with differentiation. Sr and Nd isotopic ratios of the St Martin suite form restrictedranges which vary little with differentiation, or between theextrusive and intrusive suiteSi 87Sr/86Sr ratios are slightlyhigher and 143Nd/l44Nd slightly lower than for volcanic rocksuites from the currently active northern Lesser Antilles volcanicarc. Some of the high 87Sr/86Sr ratios are explained in termsof hydrothermal alteration involving a high 87Sr/86Sr fluid,associated with pluton emplacement. Pb isotope ratios are similarto those of the currently active northern Lesser Antilles arc,and correlate with SiO2. Such correlations, together with largeranges of incompatible (and immobile) trace element ratios suggestthat open-system differentiation occurred during the evolutionof the St Martin suite. The composition of magma sources in the northern Lesser Antillesarc apparently has not changed significantly over the last 30Ma, despite a westward shift in the locus of arc magmatism.Addition of a slab-derived fluid to the mantle wedge is responsiblefor the high relative abundances of large ion lithophile elements(LILE) and enrichment in radiogenic Pb and Sr relative to mid-oceanridge basalt (MORB). Subsequent differentiation may involveassimilation of the arc basement in St Martin, which is believedto consist of Cretaceous to early Tertiary arc material, similarto that encountered in the Greater Antilles.
*Present address: Department of Geosciences, University of Arizona, Tucson, Arizona 85721 相似文献
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Geochronology and geological evolution of metamorphic rocks in the Field Islands area, East Antarctica 总被引：2，自引：0，他引：2
Detailed geochronological, structural and petrological studies reveal that the geological evolution of the Field Islands area, East Antarctica, was substantially similar to that of the adjacent Archaean Napier Complex, though with notable differences in late and post Archaean times. These differences reflect the area's proximity to the Proterozoic Rayner Complex and consequent vulnerability to tectonic process involved in the formation of the latter. Distinctive structural features of the Field Islands are (1) consistent development of a discordant, pervasive S3 axial-plane foliation; (2) re-orientation of S3 axial planes to approximate to the subsequent E-W tectonic trend of the nearby Rayner Complex; (3) selective retrogression by a post-D3 static thermal overprint; and (4) relatively common development of retrogressive, E-W-trending, mylonitic shear zones. Peak metamorphic conditions in excess of 800°C at 900 ± 100 M Pa (9 kbar) were attained at one locality following, but probably close to the time of D2 folding. D3 took place in late Archaean times when metamorphic temperatures were about 650°C and pressures were about 600 MPa (6 kbar). Later, temperatures of 600 ± 50°C and pressures of 700 MPa (7kbar) were attained in an amphibolite-facies event, presumably associated with the widespread granulite to amphibolite-facies metamorphism and intense deformation involved in the formation of the Rayner Complex at about 1100 Ma. The area was subsequently subjected to near-isothermal uplift. Rb-Sr isotopic data indicate that the pervasive D3 fabric developed at about 2400–2500 Ma, and this age can be further refined to 2456+8-5 Ma by concordant zircon analyses from a syn-D3 pegmatite. All zircons were affected by only minor (<7–10%) Pb loss and/or new zircon growth during the Rayner event at about 1100Ma. Thus the 450–850 μg/gU concentrations of these zircons were too low to cause sufficient lattice damage over the 1350 Ma (from 2450 Ma) for excessive Pb to be lost during the 1100 Ma event. The emplacement of pegmatite at 522 ± 10 Ma substantially changed the Rb-Sr systematics of the only analysed rock that developed a penetrative fabric during the 1100 Ma event. Monazite in this pegmatite contains an inherited Pb component, which probably resides in small opaque inclusions. A good correlation is found between Rb-Sr total-rock ages and rock fabric. U-Pb zircon intercepts with concordia also mostly correspond to known events. However, in one example a near perfect alignment of zircon analyses, probably developed by mixing of unrelated components, produced concordia intercepts that appear to have no direct geochronological significance. 相似文献
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Jemma DAVIDSON Henner BUSEMANN Ian A. FRANCHI 《Meteoritics & planetary science》2012,47(11):1748-1771
Abstract– Interplanetary dust particles (IDPs) are the most primitive extraterrestrial material available for laboratory studies and may, being likely of cometary origin, sample or represent the unaltered starting material of the solar system. Here we compare IDPs from a “targeted” collection, acquired when the Earth passed through the dust stream of comet 26P/Grigg‐Skjellerup (GSC), with IDPs from nontargeted collections (i.e., of nonspecific origin). We examine both sets to further our understanding of abundances and character of their isotopically anomalous phases to constrain the nature of their parent bodies. We identified ten presolar silicates, two oxides, one SiC, and three isotopically anomalous C‐rich grains. One of seven non‐GSC IDPs contains a wealth of unaltered nebula material, including two presolar silicates, one oxide, and one SiC, as well as numerous δD and δ15N hotspots, demonstrating its very pristine character and suggesting a cometary origin. One of these presolar silicates is the most 17O‐rich discovered in an IDP and has been identified as a possible GEMS (glass with embedded metal and sulfides). Organic matter in an anhydrous GSC IDP is extremely disordered and, based on Raman spectral analyses, appears to be the most primitive IDP analyzed in this study, albeit only one presolar silicate was identified. No defining difference was seen between the GSC and non‐GSC IDPs studied here. However, the GSC collectors are expected to contain IDPs of nonspecific origin. One measure alone, such as presolar grain abundances, isotopic anomalies, or Raman spectroscopy cannot distinguish targeted cometary from unspecified IDPs, and therefore combined studies are required. Whilst targeted IDP populations as a whole may not show distinguishable parameters from unspecified populations (due to statistics, heterogeneity, sampling bias, mixing from other cometary sources), particular IDPs in a targeted collection may well indicate special properties and a fresh origin from a known source. 相似文献
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