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The Younger Andesites and Dacites of Iztacc?huatl volcano, Mexico,constitute a medium-K calcalkaline rock suite (58–66 wt.per cent SiO2) characterized by high Mg-numbers (100Mg/(Mg+0?85Fe2+=55–66) and relatively high abundances of MgO (2?5–6?6wt. per cent), Ni(17–158 p.p.m.), and Cr (42–224p.p.m.). Chemical stratigraphy plots of eruptive sequences indicatethe existence of a plexus of long-lived dacite magma chambersperiodically replenished by influxes of basaltic magma ascendingfrom depth. Short-term geochemical evolution after batch influxwas dictated by magma mixing and eventual dilution of the basalticcomponent by ‘quasi-steady state’ hornblende dacitemagma. The chemical data support textural and mineralogicalevidence for rapid homogenization of originally diverse magmasby convective blending of residual liquids accompanied by dynamicfractional crystallization (Nixon, 1988). Internally-consistent mixing calculations used to derive thecomposition of basaltic magma influx incorporate analyticaluncertainties and the observed range of salic end-member compositions.Mafic end-members are basalts to basaltic andesites (52–54wt. per cent SiO2) with Mg-numbers (73–76), MgO (9–11wt. per cent), Ni (250 p.p.m.), and Cr (340–510 p.p.m.)concentrations, and liquidus olivine compositions (Fo90–88),appropriate for unfractionated partial melts of mantle peridotite.The majority of model compositions are Ol-Hy-normative, similarto those of primitive basaltic lavas on the flanks of Iztacc?huatland in the Valley of Mexico. However, calculated magma batchesrange from weakly Qz-normative to strongly Ne-normative. Bothcalculated and analyzed basaltic compositions are distinguishedby highly variable abundances of alkalies and incompatible traceelements, notably Rb, Ba, Sr, P, Zr, and Y. Initial 87Sr/86Sr ratios for Iztacc?huatl lavas (0?7040–0?7046;n=24) are comparable to those for primitive basaltic rocks (0?7037–0?7045;?=4) and indicate that (1) mantle source regions are isotopicallyheterogeneous; and (2) contamination of iztacc?huatl magma chambersby radiogenic crustal rocks was not a significant factor inthe evolution of calc-alkaline andesites and dacites. The replenishment of Iztacc?huatl dacite reservoirs by Ne-normativemagmas late in the history of cone growth precludes exhaustionof mantle source regions by progressive partial melting. Thewaning stages of volcanic activity at Iztacc?huatl appear toreflect the inability of dense basaltic influxes to successfullypenetrate a large high-level chamber of low density hornblendedacite magma. 相似文献
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A Non-cognate Origin for the Gibeon Kimberlite Megacryst Suite, Namibia: Implications for the Origin of Namibian Kimberlites 总被引：7，自引：4，他引：3
Trace element and Sr–Nd–Pb isotope analyses arepresented on unaltered kimberlites and clinopyroxenes and garnetsof the low-Cr megacryst suite from the Gibeon Province, Namibia.Significant Sr and Pb isotope disequilibrium between the kimberlitesand megacrysts establishes that the megacrysts are not cognatematerial. Calculated equilibrium melts for the megacrysts haverare earth element contents comparable with those of alkalibasalts. Rb–Sr mica ages, 相似文献
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Geochemical Constraints on the Petrogenesis of Diamond Facies Pyroxenites from the Beni Bousera Peridotite Massif, North Morocco 总被引：10，自引：4，他引：6
The petrogenesis of pyroxenite layers within the Beni Bouseraperidotite massif is investigated by means of elemental andNd-Sr-Pb-O-S isotope analyses. The light rare earth element(LREE) depleted nature of many of the pyroxenites, their widevariation in composition, and lack of correlation between incompatibleelements and fractionation indices preclude them from representingcrystallized melts from a peridotitic source. The physical characteristicsof the pyroxenites and their large (greater than a factor of20) range in Ni rule out partial melting as the cause of theirpetrological and geochemical diversity. Major and compatibletrace element geochemistry is consistent with formation of mostof the pyroxenite suite via high-pressure crystal segregationin magma conduits intruding the peridotites. These magmas crystallizedclinopyroxene, orthopyroxene, and garnet. The pressure of crystallizationis constrained to be above {small tilde}45 kbar from the presenceof graphitized diamonds in pyroxenite layers. Lack of correlationbetween fractionation indices and highly incompatible elementsand the wide variation in incompatible element abundances suggestthat the suite did not form from genetically related magmas.The presence of positive and negative Eu anomalies (Eu/Eu* =0•54–2•0) in pyroxenites which crystallizedat pressures much greater than the plagioclase stability field({small tilde} 45 kbar) suggests that the parental magmas originatedfrom precursors which formed in the crust. Oxygen isotope compositionsof coexisting minerals in the pyroxenites indicate high-temperatureequilibration but 18O values vary from +4•9 to + 9•3,ruling out their derivation from the host peridotites or othernormal mantle sources. The extreme O-isotope variation, togetherwith 34S values of up to + 13 in sulphides included within CPXstrongly suggests that the melts from which the pyroxenitescrystallized were derived from hydrothermally altered, subductedoceanic lithosphere. Extreme initial radiogenic isotope variationin the pyroxenites (Nd + 26 to –9 , 87Sr/86Sr 0•7025–0•7110,206Pb/204Pb 18•21–19•90) support such an originbut also require a component with ancient, high U/Pb and Th/Pbin their source to explain the high 7/4 and 8/4 values of somepyroxenites. This component may be subducted hemi-pelagic sediment.Further evidence for a sediment component in the pyroxenitesis provided by isotopically light carbon in the graphite pyroxenites(13C–16 to – 28). Parentdaughter isotopes in thepyroxenites are strongly decoupled, making estimation of formationages speculative. The decoupling occurred recently (<200Ma), probably as a result of partial melting associated withdiapiric upwelling and emplacement of the massif into the crustfrom the diamond stability field. This late partial meltingevent further depleted the pyroxenites in incompatible elements.The variably altered nature of the subducted protolith and complexhistory of trace element fractionation of the pyroxenites haslargely obscured geochemical mixing trends. However, Nd–Pbisotope systematics indicate that incorporation of the componentwith high U/Pb–Th/Pb occurred relatively recently (<200Ma) for some pyroxenites. Other pyroxenites do not show evidencefor incorporation of such a component and may be substantiallyolder. Tectonic, geophysical, and isotopic constraints indicateformation of the pyroxenites in the mantle wedge above a subductingslab during the Cretaceous. Physical and chemical evidence forhigh-pressure fractionation seen in most of the pyroxenitesprecludes them from simply representing ancient subducted oceaniclithosphere, thinned by diffusion. However, the petrologicaland isotopic diversity of the massif support the concept ofa ‘marble cake’ mantle capable of producing theobserved geochemical diversity seen in oceanic magmas.
*Present Address: Department of Terrestrial Magnetism, 5241 Broad Branch Road, N.W., Washington, DC 20015 Present address: Department of Geological Sciences, 1066 C.C. Little Building, University of Michigan, Ann Arbor, Michigan 48109 相似文献
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Adam NIXON Mark J. BURCHELL Mark C. PRICE Anton T. KEARSLEY Steven JONES 《Meteoritics & planetary science》2012,47(4):623-633
Abstract– Impacts of small particles of soda‐lime glass and glycine onto low density aerogel are reported. The aerogel had a quality similar to the flight aerogels carried by the NASA Stardust mission that collected cometary dust during a flyby of comet 81P/Wild 2 in 2004. The types of track formed in the aerogel by the impacts of the soda‐lime glass and glycine are shown to be different, both qualitatively and quantitatively. For example, the soda‐lime glass tracks have a carrot‐like appearance and are relatively long and slender (width to length ratio <0.11), whereas the glycine tracks consist of bulbous cavities (width to length ratio >0.26). In consequence, the glycine particles would be underestimated in diameter by a factor of 1.7–3.2, if the glycine tracks were analyzed using the soda‐lime glass calibration and density. This implies that a single calibration for impacting particle size based on track properties, as previously used by Stardust to obtain cometary dust particle size, is inappropriate. 相似文献
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Disequilibrium phenocryst assemblages in the Younger Andesitesand Dacites of Iztacc?huatl, a major Quaternary volcano in theTrans-Mexican Volcanic Belt, provide an excellent record ofepisodic replenishment, magma mixing, and crystallization processesin calc-alkaline magma chambers. Phenocryst compositions andtextures in ‘mixed’ lavas, produced by binary mixingof primitive olivine-phyric basalt and evolved hornblende dacitemagmas, are used to evaluate the mineralogical and thermal characteristicsof end-members and the physical and chemical interactions thatattend mixing. Basaltic end-members crystallized olivine (FO90–88) andminor chrome spinel during ascent into crustal magma chambers.Resident dacite magma contained phenocrysts of andesine (An45–35),hypersthene (En67–61), edenitic-pargasitic hornblende,biotite, quartz, .titanomagnetite, and ilmenite. On reachinghigh-level reservoirs, basaltic magmas were near their liquidiat temperatures of about 1250–1200?C according to theolivine-liquid geothermometer. Application of the Fe-Ti-oxidegeothermometer-oxygen barometer indicates that hornblende dacitemagma, comprising phenocrysts (<30 vol. per cent) and coexistingrhyolitic liquid, had an ambient temperature between 940 and820?C at fO2s approximately 0?3 log units above the nickel-nickeloxide buffer assemblage. Mixing induced undercooling of hybridliquids and rapid crystallization of skeletal olivine (Fo88–73),strongly-zoned clinopyroxene (endiopside-augite), calcic plagioclase(An65–60); and orthopyroxene (bronzite), whereas low-temperaturephenocrysts derived from hornblende dacite were resorbed ordecomposed by hybrid melts. Quartz reacted to form coronas ofacicular augite and hydroxylated silicates were heated to temperaturesabove their thermal stability limit ({small tilde}940?C foramphibole, according to clinopyroxene-orthopyroxene geothermometry,and {small tilde}880?C for biotite). Calculations of phenocrystresidence times in hybrid liquids based on reaction rates suggestthat the time lapse between magma chamber recharge and eruptionwas extremely short (hours to days). It is inferred that mixing of magmas of diverse compositionis driven by convective turbulence generated by large differencesin temperature between end-members. The mixing mechanism involves:(1)rapid homogenization of contrasting residual liquid compositionsby thermal erosion and diffusive transfer (liquid blending);(2) assimilation of phenocrysts derived from the low-temperatureend-member; and (3) dynamic fractional crystallization of rapidlyevolving hybrid liquids in a turbulent boundary layer separatingbasaltic and dacitic magmas. The mixed lavas of lztacc?huatlrepresent samples of this boundary layer quenched by eruption. 相似文献
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