Influence of oxygen pressure on defect concentrations in olivine with a fixed cationic ratio     

R.L. Stocker 《Physics of the Earth and Planetary Interiors》1978,17(2):118-129

The variation of the point-defect concentrations with oxygen partial pressure, P_O2, and temperature are derived for forsterite, Mg₂SiO₄, and Mg-rich olivine (Mg,Fe)₂SiO₄ assuming the cation/cation ratios are fixed. These dependencies differ from the open-system situation in which matter is easily transferable between forsterite or olivine and other solid phases. The details depend on whether the cation/cation ratio is exactly stoichiometric, or, if non-stoichiometric, the nature of the majority defects at precise oxygen stoichiometry. One generality which emerges is that regardless of the cation/cation stoichiometry the dominant defects in forsterite at low P_O2 are free electrons, Mg and Si interstitials; at high P_O2 the majority defects are holes, Mg and Si vacancies. In Mg-rich olivine the same defect species exist at the extremes of oxygen partial pressure with the exception of trivalent Fe on Mg sites replacing holes. At low P_O2, therefore, both behave as n-type conductors. The models also suggest that in the P_O2 range around precise oxygen stoichiometry the electrical conductivity in both materials can be a complex function of P_O2.  相似文献   

Effect of oxygen partial pressure on the dislocation recovery in olivine: a new constraint on creep mechanisms     

Shun-ichiro Karato  Hiroki Sato 《Physics of the Earth and Planetary Interiors》1982,28(4):312-319

The dislocation annihilation rate in experimentally deformed olivine single crystals was measured as a function of oxygen partial pressure (P_O2). It was shown that the dislocation annihilation rate decreased with increasing P_O2. This result is inconsistent with the reported P_O2 dependence of creep rate () in single olivine crystals, thus indicating that the creep in single olivine crystals is not rate-controlled by recovery, under the experimentally investigated conditions.  相似文献   

Ion microprobe studies of water in silicate melts: Temperature-dependent water diffusion in obsidian     

J.L. Karsten  J.R. Holloway  J.R. Delaney 《Earth and Planetary Science Letters》1982,59(2):420-428

The temperature dependence of water diffusivity in rhyolite melts over the range 650–950°C and [P_T(H₂O] = 700 bars is evaluated from water concentration-distance profiles measured in glass with an ion microprobe. Diffusivities are exponentially dependent on concentration over this temperature range and vary from about 10^?8 cm²/s at 650°C to about 10^?7 cm²/s at 950°C at 2 wt.% water. Water solubility also varies with temperature at a rate of ?0.14 wt. per 100°C increase. The avtivation energy (E_a) appears to be constant at 19 ± 1kal/mole for 1, 2,and 3 wt.% H₂O. Comparison of these data with results for cation diffusion indicates that this value is a minimum E_a for diffusion of any species in a rhyolite melt.Compensation plots of log₁₀D₀ (the frequency factor) versus E_a indicate that hydrous rhyolite melts follow the same trend as anhydrous basalts. D₀ increases for H₂O and Ca²⁺ [1] as E_a decreases. This suggests that these molecules may diffuse by different mechanisms than do monovalent cations, and that hydration of the melt affects diffusion of Ca²⁺ and H₂O differently than it does monovalent cation diffusion. The results imply that dramatic increases in cation diffusivities by hydration [1] may occur with additions of less than 1 wt.% H₂O.  相似文献   

Studies in diffusion,II. Oxygen in phlogopite mica     

B.J. Giletti  T.F. Anderson 《Earth and Planetary Science Letters》1975,28(2):225-233

Self-diffusion of oxygen in a natural phlogopite mica (annite 4%) has been measured under hydrothermal conditions at 2000 bars pressure and from 500 to 800°C using water enriched in¹⁸O. Diffusional transport is dominantly parallel to the c crystallographic axis. A linear Arrhenius plot was obtained with a pre-exponential term = (1.03 ± 0.38) × 10^?9cm²sec^?1 a and an activation energy of 29 ± 2kcal/g-atom O. The difference in transport rate between oxygens in the OH groups and those in tetrahedral sites is small to non-existent unless the OH oxygens diffuse much more slowly than the other oxygens, which we consider unlikely. A typical phlogopite crystal, 0.2 mm thick by 1 mm across will lose radiogenic argon faster than it will exchange oxygen at temperatures above 435°C, but the reverse holds at lower temperatures if the diffusion mechanism can be extrapolated to temperatures below 500°C. Such a crystal will lose only 5% of its argon if held at 380°C for 1 m.y., but could exchange 27% of its oxygen in that time. The rate at which phlogopite will undergo deformation by diffusional creep does not appear to be controlled by oxygen diffusion.  相似文献   

Transient and steady-state creep of pure forsterite at low stress     

W.B. Durham  C. Froidevaux  O. Jaoul 《Physics of the Earth and Planetary Interiors》1979,19(3):263-274

Thirty-one single crystals of synthetic forsterite, Fo₁₀₀, were deformed in 69 compressional creep tests in a 0.1-MPa confining atmosphere of H₂ + Ar. Temperature ranged from 1753 to 2023 K and stress σ (= σ₁ - σ₃) from 1.5 to 37.8 MPa. Steady-state creep under these conditions follows an empirical law of the form: strain rate $\text{?}\text{?}\text{= A}{}_{\mathrm{zigma;}}{}^{\mathrm{n}}\text{exp}\text{(}\text{?Q}\text{RT}\text{)}$ where A, n, and Q are constants. General characteristics of Fo₁₀₀ creep — uniformity of strain, shape change as a function of orientation of σ, relative deformation resistance of different orientations — match those of natural olivine single crystals of composition Fo₉₂. Specific constants in the flow law, however, are distinctly new: for σ oriented along [111]_c (equidistant from the three principal crystallographic axes), values for Fo₁₀₀ are n = 2.9 ± 0.2 and Q = 0.67 ± 0.03 MJ/mol (160 ± 7 kcal/mol). A single law covers the range 3 < σ < 30 MPa and 1753 < T < 1953 K. Steady-state deformation is preceded by a transient period of strain softening. High strain rates at σ ? 10 MPa render the transient barely resolvable; it apparently displaces the steady-state flow law by approximately ?0.5% in strain. At σ ? 7.8 MPa, the amount of strain imparted to a sample of the [101]_c orientation is typically <0.1% after one hour.  相似文献   

Experimental investigation of reaction coronas on olivine in Apollo 14 high-grade breccias     

S.E. Kesson 《Earth and Planetary Science Letters》1975,28(1):65-68

Reaction coronas of pyroxene ± ilmenite occur around clasts of olivine in Apollo 14 high-grade metamorphic breccias. In experiments of several months duration, there was no evidence of corona formation at 1000°C, but at 1050°, withfO₂ at or above Ilm-Ru-Fe and below Fe-Fe₁?x O, incipient coronas formed around Fo_50–70 in synthetic 14311 matrix. In addition, withfO₂ controlled by Ilm-Ru-Fe at 1050°C, the olivines reduced to Fo₆₈, En₆₉ + Fe. Reduction of olivine under these conditions is inconsistent with the calculated stability relations and is attributed to uncertainties in the activity coefficient for olivine or pyroxene. The experiments also suggest that vesicularity in the Apollo 14 high-grade breccias may correlate with the amount of glassy material in their unmetamorphosed precursors. The metamorphic event is attributed to burial in a hot ejecta blanket, such as that of the Imbrium event.  相似文献   

Ion microprobe studies of water in silicate melts. Concentration-dependent water diffusion in obsidian     

J.R. Delaney  J.L. Karsten 《Earth and Planetary Science Letters》1981,52(1):191-202

The ion microprobe at Johnson Space Center has been calibrated for in situ water determinations on a 10-μm scale over the range 0.2 wt.% H₂O to 1.8, 6.8, and 3.7 wt.%, for basaltic, albitic, and rhyolitic glasses, respectively. The basalt glass calibration curve differs substantially from those of albite and rhyolite glasses, indicating a need to carefully match composition and/or melt structure between H₂O standards and unknowns.A value for the diffusivity of water as a function of concentration and time has been calculated from water diffusion profiles measured in rhyolite glasses prepared at 850°C and 700 barsP_t(H₂O) [1]. Transient diffusion into a semi-infinite medium is described by the equation:?(φ/2)?¸/?φ=?(D_w?¸/?φ)/?φ #x003B8;=1, φ=0, θ→ 0, θ→∞, wherex =distance from the cylinder edge,t =time,C₀ =initial concentration,C_s =concentration at the edge,C =concentration at x,θ = C ? C₀/C_s ? C₀,φ = x/t^1/2, andD_w =diffusivity of water. An iterative technique has been used to calculate solutions to the diffusion equation as a function ofD_w [2]. Comparison of these solutions with the ion probe data indicate that, for0.2wt.% ≤ C ≤ 3.7wt.%H₂O,D_w can be described by an exponential function of θ, of the formD_w = D₀exp(bθ), withD₀ (i.e.,D_w at 0.2%) = (0.8?2.2) × 10^?8 cm²/s and2 ≤ b ≤ 4.  相似文献   

Oxygen isotope constraints on the origin and differentiation of the Moon     

《Earth and Planetary Science Letters》2007,253(1-2):254-265

We report new high-precision laser fluorination three-isotope oxygen data for lunar materials. Terrestrial silicates with a range of δ¹⁸O values (− 0.5 to 22.9‰) were analyzed to independently determine the slope of the terrestrial fractionation line (TFL; λ = 0.5259 ± 0.0008; 95% confidence level). This new TFL determination allows direct comparison of lunar oxygen isotope systematics with those of Earth. Values of Δ¹⁷O for Apollo 12, 15, and 17 basalts and Luna 24 soil samples average 0.01‰ and are indistinguishable from the TFL. The δ¹⁸O values of high- and low-Ti lunar basalts are distinct. Average whole-rock δ¹⁸O values for low-Ti lunar basalts from the Apollo 12 (5.72 ± 0.06‰) and Apollo 15 landing sites (5.65 ± 0.12‰) are identical within error and are markedly higher than Apollo 17 high-Ti basalts (5.46 ± 0.11‰). Evolved low-Ti LaPaz mare-basalt meteorite δ¹⁸O values (5.67 ± 0.05‰) are in close agreement with more primitive low-Ti Apollo 12 and 15 mare basalts. Modeling of lunar mare-basalt source composition indicates that the high- and low-Ti mare-basalt mantle reservoirs were in oxygen isotope equilibrium and that variations in δ¹⁸O do not result from fractional crystallization. Instead, these differences are consistent with mineralogically heterogeneous mantle sources for mare basalts, and with lunar magma ocean differentiation models that result in a thick feldspathic crust, an olivine–pyroxene-rich mantle, and late-stage ilmenite-rich zones that were convectively mixed into deeper portions of the lunar mantle. Higher average δ¹⁸O (WR) values of low-Ti basalts compared to terrestrial mid ocean ridge basalts (Δ=0.18‰) suggest a possible oxygen isotopic difference between the terrestrial and lunar mantles. However, calculations of the δ¹⁸O of lunar mantle olivine in this study are only 0.05‰ higher than terrestrial mantle olivine. These observations may have important implications for understanding the formation of the Earth–Moon system.  相似文献   

Origin of iron-rich olivine in the matrices of type 3 ordinary chondrites: an experimental study     

Hiroko Nagahara  Ikuo Kushiro 《Earth and Planetary Science Letters》1987,85(4)

In order to understand the origin of iron-rich olivine in the matrices of type 3 ordinary chondrites, the reaction of metallic iron and enstatite, with and without forsterite and SiO₂, has been experimentally reproduced at temperatures between 1150° and 800°C and P_O2 between 10⁻¹¹ and 10⁻¹⁶ atm (between the IQF and MW buffers). The olivine produced ranges from Fo₅₈ to Fo₃₄ and this composition does not change significantly with temperature and time of the runs. The magnesian olivine which forms does become more magnesian with increasing forsterite/enstatite ratio of the starting materials. Iron-rich olivine (Fo< 35) cannot be formed by the reaction of enstatite and metallic iron, with or without forsterite as starting materials but it can be formed in the presence of free silica. The composition of olivine becomes more iron-rich with increasing silica/enstatite ratio. The compositional range of olivine formed from each mixture is 25–30 mole% Fo regardless of the temperature, composition, mineral assemblage, and run duration.From these experimental results, two possibilities suggested for the origin of the iron-rich olivine in the matrices of type 3 ordinary chondrites: (1) free silica must have been present if the iron-rich olivine was formed by solid-state reactions under oxidizing condition in the solar nebula; (2) reaction of silicon-rich gas with metallic iron took place under oxidizing condition in the solar nebula. Though it is difficult to define which alternative was dominant, the formation of free silica or silicon-rich gas may be a result of fractional condensation. This is possible if there is a reaction relation between forsterite and gas to produce enstatite. The suggested fractional condensation is supported by the fact that the compositions of the fine-grained matrices of type 3 ordinary chondrites are more silica-rich than the bulk compositions of the chondrites. Though it is not known whether such conditions were established all over the nebula or locally in the nebula, both fractionation and more oxidizing conditions than the average solar nebula are required for the formation of matrix olivine.  相似文献   

Ni₂SiO₄-enthalphy of the olivine-spinel transition by solution calorimetry at 713°C     

Alexandra Navrotsky 《Earth and Planetary Science Letters》1973,19(4):471-475

The high pressure spinel polymorph of Ni₂SiO₄ persists metastably at 713°C and atmospheric pressure. The enthalpy of the olivine-spinel transition was obtained by measuring the heats of solution of both polymorphs in a molten oxide solvent, 2PbO · B₂O₃, at that temperature. For Ni₂SiO₄(ol)→Ni₂SiO₄, ΔH₉₈₆⁰ = +1.4 ± 0.7kcal/mol. The heat content increments, H₉₈₆ ? H₂₉₇, were found to be: olivine, 25.73 ± 0.42kcal/mol, and spinel, 25.39 ± 0.20kcal/mol. The measured enthalpy of the transformation is consistent with the low slope of the phase boundary, ?P/?T = ～ 12b/deg, observed by Akimoto and others. The entropy of the olivine-spinel transition in Ni₂SiO₄ is accordingly about a factor of three smaller in magnitude (ΔS = ～ ?1cal/deg mol) than that for Co₂SiO₄,Fe₂SiO₄,Mg₂SiO₄or Mg₂GeO₄ (ΔS = ?3to?3.5cal/deg mol).  相似文献   

Activity of iron and olivine solubility in basaltic liquids     

P.L. Roeder 《Earth and Planetary Science Letters》1974,23(3):397-410

Some of the factors which control the solubility of ferrous iron and olivine in basaltic liquids have been determined from experiments conducted in equilibrium with metallic iron at temperatures of 1150° to 1306°C and oxygen fugacities of log?O₂ = ?12.5to?14.5atm. In order to insure that the samples were in equilibrium with metallic iron and the gas atmosphere during the experiment, the samples were continuously mixed (60 r.p.m.) for at least 90 hours with a metallic iron mixing rod.The solubility of ferrous iron and olivine in basaltic liquid was found to decrease as the alkali and alumina content of the liquid increased. The activity coefficient of ferrous iron in the liquid was calculated from the oxygen fugacity and mole fraction of ferrous oxide in the liquid and varied from 0.79 to 2.00. The ferrous iron/magnesium ratio in the liquid relative to olivine was insensitive to the changing alkali content as measured by the constant distribution coefficient of0.30 ± 0.03 (SD). The calculated silica activity of these liquids varied from 0.11 to 0.50 and the distribution coefficient of ferrous iron-manganese between olivine and liquid was found to be1.4 ± 0.2 (SD). It was found that the major element content of olivine does not exert a strong structural control on the manganese content of olivine.The magnitude of depletion in the liquid of the metal oxides by the crystallization of olivine is in the order Ni > Mg > Co > Fe > Mn, which reflects the relative octahedral site preference of these elements. The composition of the crystallizing olivine reflects the ratio of the above elements in the liquid and is relatively insensitive to temperature, variation of the other elements in the liquid or to the changing magnesium/ferrous iron ratio in the olivine.  相似文献   

The influence of oxidation state on the electrical conductivity of olivine     

Al Duba  I.A. Nicholls 《Earth and Planetary Science Letters》1973,18(1):59-64

The electrical conductivity of a single crystal of San Carlos olivine (Fo₉₂, 0.16 wt.% Fe₂O₃) has been measured as a function of temperature and oxygen fugacity (fO₂). After heating to 1338°C at fO₂ = 10^?12 atm., the conductivity at 950°C was 10^?5 (ohm-m)^?1, almost 3 orders of magnitude less than that measured in air. This decrease is due to the reduction of Fe³⁺ to Fe²⁺. Further heating to 1500°C at fO₂ = 10^?14 atm., decreased the electrical conductivity at 950°C to 10^?6 (ohm-m)^?1. When recovered at room temperature, the speciment had Fo₉₆ composition and contained small, opaque blebs distributed throughout the crystal. Derivations of temperature profiles for the earth's mantle from conductivity-depth models must take account of the important role played by iron oxidation state in the electrical conductivity of olivine.  相似文献   

Radon-222 as a tracer for mixing in the water column and benthic exchange in the southern California borderland     

W.M. Berelson  D.E. Hammond  C. Fuller 《Earth and Planetary Science Letters》1982,61(1):41-54

The concentrations of²²²Rn and²²⁶Ra in the water column and in the sediments of Santa Barbara and San Nicolas Basins have been measured semi-annually over the last four years. Approximately one-third of excess radon profiles obtained in the water column in these basins can be adequately fit with a one-dimensional eddy diffusion-decay model. Exponential profiles in the center of San Nicolas Basin yield a vertical eddy diffusivity of 26±16 cm²/s and 3.4±1.0 cm²/s for Santa Barbara Basin. The application of a two-dimensional eddy diffusion-decay model to profiles obtained in the center and on the margins of San Nicolas Basin produces a better fit than is found using a one-dimensional vertical eddy diffusivity. The two-dimensional model for San Nicolas Basin predicts a vertical eddy diffusivity of 17 cm²/s and a horizontal eddy diffusivity of 10⁵ cm²/s. These values are in reasonable agreement with those predicted from the vertical buoyancy gradient and the horizontal length scale.The vertically integrated radon excess (standing crop) in the water column of Santa Barbara Basin averages 53±23 atoms/m² s. This is in good agreement with the flux across the sediment-water interface of 60±15 atoms/m² s, calculated by measuring radon emanation in the sediments as a function of depth and applying a molecular diffusion-reaction model. Hence, one-dimensional molecular diffusion accurately predicts the flux of radon from the laminated Santa Barbara Basin sediments. In San Nicolas Basin the integrated radon excess in the water column is 376±143 atoms/m² s, but the diffusive randon flux from San Nicolas Basin sediments averages only 190±53 atoms/m² s. This descrepancy indicates that a non-diffusive process, probably macrofaunal irrigation, supplies much of the flux of radon from San Nicolas Basin sediments.  相似文献   

Pressure dependence of nickel partitioning between forsterite and aluminous silicate melts     

Bjørn O. Mysen  Ikuo Kushiro 《Earth and Planetary Science Letters》1979,42(3):383-388

Nickel partitioning between forsterite and aluminosilicate melt of fixed bulk composition has been determined at 1300°C to 20 kbar pressure. The value of the forsterite-liquid nickel partition coefficient is lowered from >20 at pressures equal to or less than 15 kbar to <10 at pressures above 15 kbar.Published data indicate that melts on the join Na₂O-Al₂O₃-SiO₂ become depolymerized in the pressure range 10–20 kbar as a result of Al shifting from four-coordination at low pressure to higher coordination as the pressure is increased. This coordination shift results in a decreasing number of bridging oxygens in the melt. It is suggested that the activity coefficient of nickel decreases with this decrease in the number of bridging oxygens. As a result, the nickel partition coefficient for olivine and liquid is lowered.Magma genesis in the upper mantle occurs in the pressure range where the suggested change in aluminum coordination occurs in silicate melts. It is suggested, therefore, that data on nickel partitioning obtained at low pressure are not applicable to calculation of the nickel distribution between crystals and melts during partial melting in the upper mantle. Application of high-pressure experimental data determined here for Al-rich melts to the partial melting process indicates that the melts would contain about twice as much nickel as indicated by the data for the low-pressure experiments. If, as suggested here, the polymerization with pressure is related to the Al content of the melt, the difference in the crystal-liquid partition coefficient for nickel at low and high pressure is reduced with decreasing Al content of the melt. Consequently, the change ofD_Ni^{ol-andesite melt} is greater than that ofD_Ni^{ol-basalt melt}, for example.  相似文献   

Petrogenesis of basalts from the project FAMOUS area: experimental study from 0 to 15 kbars   总被引：1，自引：0，他引：1  

J.F. Bender  F.N. Hodges  A.E. Bence 《Earth and Planetary Science Letters》1978,41(3):277-302

Tholeiitic basalt glasses from the FAMOUS area of the Mid-Atlantic Ridge are among the most primitive basaltic liquids reported from the ocean basins. One of the more primitive of these[Mg/(Mg+Fe²⁺) = 0.68;Ni= 232ppm;TiO₂ = 0.61] glasses (572-1-1) was selected for an experimental investigation. This study found olivine to be the liquidus phase from 1 atm to 10.5 kbar where it is replaced by clinopyroxene. The sequence of appearance of phases at 1 atm pressure is olivine (1268°C), plagioclase (1235°C) and clinopyroxene (1135°C). The sample is multiply saturated at 10.5 kbar with olivine (Fo₈₈), clinopyroxene (Wo₃₂En₆₀Fs₉), and orthopyroxene (Wo₅En₈₃Fs₁₂). From the 1-atm data we have measured (FeO/MgO) olivine/(FeO*/MgO) liquid (K′_D) for olivine-melt pairs equilibrated at 12 temperatures in the range 1268–1205°C.K′_D varies from 0.30 at 1205°C to 0.27 at 1268°C. Analysis of high-pressure olivine melt pairs indicates a systematic increase inK′_D with pressure.Evaluation of the 1-atm experiments reveals that fractionation of olivine followed by olivine + plagioclase can generate much of the variation in major element chemistry observed in the FAMOUS basalt glasses. However, it cannot account for the entire spectrum of glass compositions — particularly with respect to TiO₂ and Na₂O. The variations in these components are such as to require different primary liquids.Comparison of clinopyroxene microphenocrysts/xenocrysts found in oceanic tholeiites with experimental clinopyroxenes reveal that the majority of those in the tholeiites may have crystallized from the magma at pressures greater than ～ 10 kbar and are not accidental xenocrysts. Clinopyroxene fractionation at high pressures may be a viable mechanism for fractionating basaltic magmas.The major and minor element mineral/meltK′_d's from our experiments have been used to model the source region residual mineralogy for given percentages of partial melting. These data suggest that ～20% partial melting of a lherzolite source containing 0–10% clinopyroxene can generate the major and minor element concentrations in the parental magmas of the Project FAMOUS basalt glasses.  相似文献   

Solubility of gold in the SiO2-NaCl-H2O system at 300°C and50 MPa     

Yishan Zeng  Fengzhen Wang  Ruiying Ai 《中国科学D辑(英文版)》1997,40(5):485-490

The solubility of gold and quartz in 0.01, 0.10 and 1. 00 mol/kg NaCl solutions with various pH was determined in the presence of the NNO oxygen buffer at 300°C and 50 MPa using a flexible gold cell hydrothermal apparatus. The Au speciation in the SiO₂-NaCI-H₂O system was inferred and the equilibrium constants for the following dissolution reactions were obtained: Au+H₂O = AuOH⁰+1/2H₂, logK(AuOH⁰) = -7.92 ± 0.25; Au+Cl^-+H₂O = AuOHCl^-+1/2H₂, logK(AuOHCl^-) = - 7. 56 ± 0.65. The present study suggests that Au as AUOH⁰ and AuOHCl^- is basically transported in ore-forming solutions under geologically realistic conditions of acidity, chloride molality and oxygen fugacity. The reason for the common association of Au with SiO₂ in hydrothermal gold deposits is discussed. Project supported hy the National Natural Science Foundation of China.  相似文献   

Fractional crystallization trends in the system Mg2SiO4-CaAl2Si2O8-FeO-Fe2O3-SiO2 over the range of oxygen partial pressures of 10−11 to 10−0.7 atm     

P. L. Roeder  E. F. Osborn 《Bulletin of Volcanology》1966,29(1):659-668

A brief report is made of current laboratory investigations on phase relations among olivine, pyroxene, anorthite, magnetite, tridymite, liquid and gas in the system Mg₂SiO₄-CaAl₂Si₂O₈-FeO-Fe₂O₂-SiO₂ over a wide range of oxygen partial pressures. Courses of fractional crystallization under various conditions of oxygen partial pressure are depicted using an anorthite saturation diagram. Starting with a basalt-like composition in the system, fractional crystallization at a moderate oxygen partial pressure (10 atm.) results in an andesite-like residual liquid of composition 55 SiO₂, 14 iron oxide, 6 MgO, 9 CaO, 16 Al₂O₃ at a temperature of 1155°C. With fractional crystallization in a closed system, the end liquid approaches the composition of 45 SiO₂, 38 iron oxide, 6 CaO and 11 Al₂O₃, at a temperature of 1050°C and oxygen partial pressure of about 10^?12 atm. The andesitic final liquid in this system would be expected to further differentiate toward dacitic and rhyolitic compositions if alkalies and water were present in the system. On the basis of these studies, the derivation of liquids of andesitic, dacitic or rhyolitic composition from primary basalts by fractional crystallization seems entirely possible if the oxygen partial pressure is maintained at a moderate or high level.  相似文献   

High-pressure recovery of olivine: implications for creep mechanisms and creep activation volume     

S. Karato  M. Ogawa 《Physics of the Earth and Planetary Interiors》1982,28(2):102-117

High-temperature and high-pressure recovery experiments were made on experimentally deformed olivines at temperatures of 1613–1788 K and pressures of 0.1 MPa to 2.0 GPa. In the high-pressure experiments, a piston cylinder apparatus was used with BN and NaCl powder as the pressure medium, and the hydrostatic condition of the pressure was checked by test runs with low dislocation density samples. No dislocation multiplication was observed. The kinetics of the dislocation annihilation process were examined by different initial dislocation density runs and shown to be of second order, i.e. where ρ is the dislocation density, k₀ is a constant, $\text{E}{}^1\text{and}\text{V}{}^1$ are the activation energy and volume respectively, and P, R and T are pressure, gas constant and temperature, respectively. Activation energy and volume were estimated from the temperature and pressure dependence of the dislocation annihilation rate as $\text{E}{}^1\text{=389±59}\text{kJ mol}{}^{\mathrm{?1}}$ and $\text{V}{}^1\text{=14±2}\text{cm}{}^3\text{mol}{}^{\mathrm{?1}}$, respectively.The diffusion constants relevant to the dislocation annihilation process were estimated from a theoretical relation k=αD where $\text{k=k}{}_0\text{exp}\text{[?(E}{}^1\text{+ PV}{}^1\text{)/RT], D}$ is the diffusion constant and α is a non-dimensional constant of ca. 300. The results agree well with the self-diffusion constant of oxygen in olivine. This suggests that the dislocation annihilation is rate-controlled by the (oxygen) diffusion-controlled dislocation climb.The mechanisms of creep in olivine and dry dunite are examined by using the experimental data of static recovery. It is suggested that the creep of dry dunite is rate-controlled by recovery at cell walls or at grain boundaries which is rate-controlled by oxygen diffusion. Creep activation volume is estimated to be 16±3 cm³ mol^?1.  相似文献   

Shear modulus and Q of forsterite and dunite near partial melting from forced-oscillation experiments     

H. Berckhemer  W. Kampfmann  E. Aulbach  H. Schmeling 《Physics of the Earth and Planetary Interiors》1982,29(1):30-41

An apparatus designed to determine the complex shear modulus of rock samples by forced torsion oscillations at high temperature and in the seismic frequency band 0.003–30 Hz is briefly described. Measurements were performed on natural dunite from Åheim (Norway) up to 1400°C and on polycrystalline forsterite up to 1500°C at 1 atm pressure. The two materials were chosen to study, by comparison, the effect of melt on the elasticity and anelasticity of mantle rocks.Between 1000 and 1200°C the absolute values of the shear modulus G are almost equal for both materials. Above 1200°C G for natural dunite decreases progressively with temperature and at 1400°C and 1 Hz reaches $\text{～}\text{1}\text{3}$ of its value at 1100°C. In contrast, G of pure forsterite depends little on temperature. For petrological reasons, supported by simultaneous measurements of the electric resistivity, there is strong evidence that the decrease of G in dunite above 1200°C is due to melt from the lower melting components of the dunite. Based on different models estimates of the melt fraction are made.At high temperature, in both materials Q^?1 is characterized by a monotonic decrease with frequency according to ω^?α, with α ≈ 0.25. An apparent activation energy of 38±5 kcal mol^?1 for forsterite and 48±8 kcal mol^?1 for dunite was found with no significant change in the regime of partial melting. From this it is concluded that Q^?1, even at partial melting, is dominated by solid state high temperature background absorption. There is no indication from these experiments for a constant-Q-band at low seismic frequencies or an increase of Q proportional to frequency as suggested by some seismologists. The present results are in good qualitative agreement with those for Young's modulus obtained previously by strain retardation experiments.  相似文献   

Hydrogarnet substitution in pyrope: a possible location for “water” in the mantle     

L. Ackermann  L. Cemič  K. Langer 《Earth and Planetary Science Letters》1983,62(2):208-214

Single-crystal spectra of pyropes, synthesized on the 3:1:3 composition of the system MgO-Al₂O₃-SiO₂ atp_H2O = p_total = 25kbar and 1000°C, show a broad band centered at around 3400 cm^?1 due toν_H2O of (H₂O)_n aggregates in fluid inclusions and a sharp intense band near 3600 cm^?1 due toν_OH of (HO)₄^4? clusters introduced by the hydrogarnet substitutionSi⁴⁺ = 4H⁺. The water contents in the synthetic pyrope, due to (HO)₄^4? clusters are estimated near 0.05 wt.% H₂O from spectroscopic data. Si deficits in microprobe analyses of the pyropes studied support the hydrogarnet substitution. These results show that the hydrogarnet substitution in pyrope may contribute to water contents in the mantle.  相似文献