


Vol 57, No 6 (2019)
- Year: 2019
- Articles: 11
- URL: https://journals.rcsi.science/0016-7029/issue/view/9468
Article
Effect of Thermal State on the Mantle Composition and Core Sizes of the Moon
Abstract
Based on the joint inversion of seismic and gravity data in combination with phase equilibrium calculations within the Na2O–TiO2–CaO–FeO–MgO–Al2O3–SiO2 system using the method of Gibbs free energy minimization, we estimated the influence of the thermal state on the model chemical composition of the lunar mantle and the size of the Fe–S lunar core. Models based on the Apollo seismic data and mass and moment of inertia estimates from the data of the GRAIL mission were used as boundary conditions. The solution of the inverse problem provided constraints on the chemical composition (major oxide abundances) and mineralogy of the three-layer mantle. It was shown that, independent of temperature distribution, the FeO contents (~11–14 wt %) and MG# values (80–83) of the upper, middle, and lower mantle of the Moon are approximately equal and strongly different from those of the bulk silicate Earth (BSE): FeO ~ 8% and MG# ~ 89. In contrast, the estimates of Al2O3 content in the mantle are sensitive to temperature distribution. The analysis of thermal state models with temperature differences of 100–200°C at different depths showed that the Al2O3 content increases from 1–5 wt % in the upper and middle mantle to 4–7 wt % in the lower mantle containing up to 20 wt % garnet. The lunar abundance of Al2O3 is ~(1.0–1.2) × BSE for “cold” models and may be as high as (1.3–1.7) × BSE for “hot” models. The abundance of SiO2 is less sensitive to temperature distribution and is 50–55 wt % in the upper mantle and 45–50 wt % in the lower mantle. Orthopyroxene rather than olivine is the dominant mineral of the upper mantle. Based on the modeling of Fe–S melt density at high P and T, the size of the lunar core was estimated. The radius of the Fe–S core having a mean density of 7.1 g/cm3 and a sulfur content of 3.5–6.0 wt % lies within the range 50–350 km with the most probable value of approximately 300 km and depends weakly on the thermal regime of the Moon. The results of modeling imply that the lunar mantle is chemically stratified and the compositions of the Earth and its satellite are significantly different.



Geochemistry and Catagenetic Transformations of Kerogen from the Bazhenov Horizon
Abstract
A representative suite of 276 samples was used to study the isotopic and elemental geochemistry of kerogens from the Bazhenov horizon (Bazhenov Formation and its age equivalents) of the western Siberian sedimentary basin and to map the variations in the elemental composition of kerogen in the area. The elemental composition of the kerogen was used to determine the types of organic matter (H and C contents), the initial components of the living matter that were the source of the kerogen (H and N contents), the diagenetic history of organic matter (S content), and the level of catagenetic transformation of the kerogen (C and O contents). Kerogen from the central, western, and southern parts of the western Siberian basin, up to the pinch-out boundary of the Bazhenov horizon, shows strong enrichment in hydrogen (up to 8–9%) and 12С (δ13С‰ from –35 to –29), suggesting its derivation from polymer lipids of aquatic origin. Kerogen from the Bazhenov horizon (catagenetic grade MC1) in the northeast of the basin contains much lower hydrogen concentrations (2–4%). A map of the types of organic matter in the Bazhenov horizon is constructed.



Anoxia in the Photic Layer of the Sedimentation Basin: Markers in the Oils of Tatarstan
Abstract
The source rocks of the oils in Tatarstan were determined to be formed under similar conditions, at anoxia in the photic layer of the sedimentation basin, with anoxia continuing throughout the whole time when the initial organic matter was accumulated, at a significant thickness of the H2S-infected layer. For some of the oils, disturbances in the anoxia may have occurred, or the thickness of the H2S-infected layer may have been reduced, and this resulted in a decrease in the content of anoxia markers in these oils. Biocenoses of microflora in the sedimentation layer contaminated with H2S show evidence of high stability. Transformation conditions of the buried organic matter in the course of diagenesis and catagenesis were uniform, as follows from the merely insignificantly varying relations between the depth of the complete hydrogenation and cyclization of the initial polyene aromatic carotenoids, the similarity in the molecular mass distributions of the destruction products of the C–C bond in C40 components, and the relatively small differences in ratios of the total concentration of monoaromatic compounds to the totals of hydrogenated analogues of the initial aromatic carotenoids. The source rocks of oils in Tatarstan can be identified based on analysis for concentrations of components that are anoxia markers in all of the Devonian rocks.



Petrology and Geochemistry of Acid Volcano-Plutonic Rocks from Riwasa and Nigana Areas of Neoproterozoic Malani Igneous Suite, Northwestern Peninsular India: An Understanding Approach to Magmatic Evolution
Abstract
This paper discusses the geochemical and petrological characteristics of acid volcano-plutonic suite of rocks exposed in Riwasa and Nigana areas of Malani Igneous Suite (MIS), Northwestern India. Geochemically, these acidic rocks having peraluminous and alkalic to alkali-calcic nature and classified as volcanic phase (Riwasa rhyolites), plutonic phase (Nigana granites) and dyke phase (micro-granites). Petrographically, rhyolites show porphyritic, granophyric, glomeroporphyritic, aphyritic, spherulitic and perlitic textures whereas granites show hypidomorphic, granophyric and microgranophyric textures. They are high in silica, A/CNK, total alkalis, Fe/Mg, Ga/Al, Zr, Rb, U, Th, Cu, REEs (except Eu) and low in CaO, MgO, Sc, Cr, Ni, Sr and Eu abundances, which have affinity with A-type granitoids. Their chemistry also support that they are high heat production (HHP) granitoids and their crustal origin. The enrichment of trace elements indicates a genetic link between fractional crystallization of silicate minerals and post magmatic fluid alterations in magmatic chamber. Negative anomalies of Ti, P, Sr and Eu in the multi-element spider diagrams indicate that the emplacement of these granites and associated acid volcanics were controlled by fractionation of feldspar (alkali and plagioclase) and crustal contamination in the magmatic melt arise upward. Normative values of silicate oxides further suggests that these rocks are formed between 2–7 kb pressure ranges and may be emplaced from shallow to greater depth ranges (15–30 km and 450–900°C). Furthermore, geochemical features in acidic rocks such as strong linear positive correlation between LREE, Zr, Nb, Ga, Y and Rb emphasize that the behavior and enrichment of these elements are largely controlled by post-magmatic processes in plume related associations. Hence, the geochemical data presented here, are therefore consistent with an intraplate, co-magmatic and A2-subtype granite field emplaced in extensional tectonic regime of MIS.



Geochemistry of Sillimanite–Magnetite–Kaolinite Metasomatic Rocks on Great Tyuters Island, Gulf of Finland, Russia
Abstract
Secondary quartzites on Tyuters Island in the Gulf of Finland host long linear zones, up to 3 m thick, that are easily discernible in detailed satellite imagery. The zones consist of sillimanite–magnetite–kaolinite metasomatites, rocks that were first found in these zones. The metasomatites were produced at shattering of the quartzites and subsequent fluid introduction of material enriched in various components. The metasomatites are enriched in Al2O3 (16–23 wt %, as compared to 2–5 wt % in the quartzites). In contrast to the quartzites, iron in the metasomatic is contained mostly in the form of ferric oxide (whereas it occurs dominantly as ferrous oxide in the quartzites). The metasomatites contain practically no alkalis and alkali-earth elements and are enriched in Zn (146–199 ppm) and some other trace elements, including REE, first of all Ce (34 ppm) and La (17 ppm). Both the metasomatites and the quartzites show similar and insignificant REE fractionation: (La/Yb)n = 6.55 and 6.17. The metasomatites consist of the same minerals as the quartzites, but the proportions of these minerals and their composition in these rock types are different. It is worth mentioning magnetite of the metasomatites: it hosts abundant quartz inclusions with kaolinite rims. The quartz inclusions host, in turn, inclusions of magnetite crystallites. The metasomatites were produced in a number of stages of a metasomatic process, with changes in the fluid composition and its pH. The development of the metasomatites in the linear zones, the disintegration of their protolithic quartzites, and the high kaolinite contents in the rocks make these metasomatites similar, in a sense, to weathering crusts. However, the facts that the metasomatites and their protolithic quartzites consist of the same minerals, that the metasomatites contain absolutely no sulfides and sulfur but contain magnetite with complicated mineral inclusions make these rocks different from classic weathering crusts.



Syn-rift Clayey Rocks: Bulk Chemical Composition and Position on Discriminant Paleogeodynamic Diagrams
Abstract
The paper analyzes the bulk chemical composition and distribution of the fields of syn-rift clayey rocks on a number of discriminant paleogeodynamic diagrams. It is shown that the syn-rift clayey rocks, in general, demonstrate significant variations in the bulk chemical composition. For example, the average SiO2 content varies from 44.74 to 66.42 wt %, the average Al2O3 content varies from 16.62 to 29.92 wt %, and the K2Oaver is in the range 0.24 … 5.77 wt %. Based on the distribution of the data points of syn-rift clayey rocks from various objects in the F1–F2 diagram, it can be assumed that the sources of fine aluminosiliciclastic material were magmatic and sedimentary rocks of a wide composition range. The substantial overlap of the fields of various objects in the classification diagrams [(Na2O + K2O)/Al2O3]–[(Fe2O3tot + MgO)/SiO2] and K/Al–Mg/Al indicates, in general, the similar composition of syn-rift fine-grained clastic rocks of various types of riftogenic structures. The localization of the composition fields of the clayey rocks of different riftogenic structures in such discriminant paleogeodynamic diagrams as K2O/Na2O–SiO2/Al2O3 and SiO2–K2O/Na2O suggests that they cannot be used to discriminate reliably between syn-rift clayey rocks and fine-grained clastic rocks of other geodynamic environments. The position of the syn-rift clayey rocks fields from our database in the diagram DF1–DF2 has its own characteristics. In most cases, they occupy a particular position in the areas characterizing collision and rifting environments, and a number of fields are located in all three classification areas of this diagram. A significant part of the midpoints of the syn-rift clayey rocks is localized in the collision field in the DF1–DF2 diagram. All these facts indicate that the DF1–DF2 diagram also cannot determine the geodynamic nature of terrigenous associations.



Facies Structure and Quantitative Parameters of Pleistocene Sediments from the East Australian Continental Margin
Abstract
Abstract—Lithological and facies zonality of Neopleistocene and Eopleistocene sediments of the Australian seas is described for the first time. Processing of these maps and isopach schemes by A.B. Ronov volumetric method gave us an opportunity to calculate the quantitative parameters of sedimentation for different types of the Pleistocene sediments. It was revealed that carbonate sediments predominate over other sediment groups. The Neopleistocene was characterized by more intense accumulation of carbonate planktic sediments and lithogenic sediments than Eopleistocene.



Biogenic Factors of Formation of Geochemical Uranium Anomalies near the Sludge Storage of the Novosibirsk Chemical Concentrate Plant
Abstract
This paper presents evidence on the possible impact of aerobic and anaerobic microbiological processes on uranium migration in upper aquifers polluted by sulfates and nitrates at the Novosibirsk chemical concentrate plant (PAO NCCP). Uranium can be immobilized in local areas with high contents of organic substances, and the most important microbiological process is a decrease in redox potential owing to aerobic respiration, which can be followed under anaerobic conditions by redox-dependent uranium reduction in areas with negative Eh values. Moreover, in the presence of sufficient amounts of sulfate ions, further anaerobic processes of microbial sulfate and iron reduction result in the formation of iron sulfide, which serves as an antioxidant buffer in the case of oxygen infiltration into the sediment and transforms to molecular sulfur or sulfate preventing uranium oxidation.



Short Communications
Natural Kaersutite: FTIR, Raman, Thermal, and Thermochemical Studies
Abstract
The paper reports original thermochemical data obtained on natural oxo-amphibole kaersutite Na0.4K0.3(Ca1.6Na0.4)(Mg2.9\({\text{Fe}}_{{0.8}}^{{2 + }}\)Al0.7Ti0.6\({\text{Fe}}_{{0.5}}^{{3 + }}\))[Si6.1Al1.9O22](OH)0.2O1.8 from alkaline basalt in Mongolia. The data were obtained using a Tian–Calvet microcalorimeter. The enthalpy of formation from elements Δf\(H_{{{\text{el}}}}^{{\text{0}}}\)(298.15 K) = –12102 ± 16 kJ/mol) was obtained by high-temperature melt solution calorimetry. The entropy, enthalpy, and Gibbs energy of formation of the end members of the isomorphic series kaersutite NaCa2Mg3TiAl[Si6Al2O22]O2–ferrikaersutite NaCa2Mg3TiFe3+[Si6Al2O22]O2 were estimated.



Experimental Study of Silicate Phosphatization under Supergene Zone Conditions: Hornblende, Orthoclase, and Labradorite
Abstract
The hypothesis of silicate phosphatization under supergene zone conditions was experimentally tested. To extend our previous experimental work on clay minerals (kaolinite and montmorillonite), we studied the phosphatization of aluminosilicates of other structural types (hornblende, orthoclase, and labradorite) interacting for nine months with 1.2–6.0 mM orthophosphate solutions over a wide range of solution acidity. Nearly linear dependence common for all minerals was found between variations in phosphorus and silicon concentrations in the solution: Δ[Si] ≈ –Δ[P]. It was demonstrated that aluminosilicates can be replaced by phosphate minerals at relatively minor concentrations of dissolved phosphorus corresponding to phosphate abundances in soil solutions.



New Isotope-Hydrogeochemical Data on the Bang Spring (Kuang Binh Province, Central Vietnam)
Abstract
Abstract—New isotope hydrogeochemical data on two types of thermal water from the Bang spring (Kuang Binh province, central Vietnam) are reported in the work. The first type includes HCO3–Cl–Na–Mg water with extremely low mineralization (44–87 mg/dm3) and pH variations from weakly acidic to weakly alkaline values (5.71–7.84). The second type includes HCO3–Na water with mineralization up to 256–659 mg/dm3 and pH 8.03 to 8.51. The studied types differ significantly in temperature: 24.3–34.5°C in the first type and 62.1–97.1°C in the second type. The analysis of the distribution of oxygen (δ18O) and hydrogen (δD) isotopes carried out for the first time confirms different genetic nature of these hydrogeochemical water types. The first type has an atmospheric genesis (δ18O = –7.3…–6.2‰ and δD = –51.4…–39.3‰), while the second type restricted to the Kien Giang–Bang intersection zone has a deeper source (δ18O = –1.6…–1.3‰ and δD = –22.2…–21.4‰). The tritium (3H) data also point to different circulation times of these waters. The formation time of the HCO3–Cl–Na–Mg waters does not exceed 50 years (3H = 4.3–11.1 ТЕ), while that of HCO3–Na water may reach more than 1000 years (3H = 0.5 ТЕ).


