


Vol 61, No 4 (2019)
- Year: 2019
- Articles: 6
- URL: https://journal-vniispk.ru/1075-7015/issue/view/13419
Article
Scale Effect in a Fluid-Conducting Fault Network
Abstract
This paper successively reports on a methodology for investigating the orientation and morphogenetic characteristics of fault systems at four scale levels: kilometers, meters, centimeters, and millimeters. The research object is the Urtui granite massif in southeastern Transbaikalia west of the Streltsovska caldera, incorporating unique uranium deposits. The massif is composed of Late Riphean granites and granite gneisses variably affected by dynamometamorphic and hydrothermal–metasomatic alterations and is crosscut by numerous faults with traces of fluid activity from various tectogenesis episodes. The relationship between the geometric parameters of the fault systems, such as specific density and specific length, has been established. It is advisable to use these geostructural data for conceptual and numerical modeling of fluid filtration and radionuclide transport processes in the three-dimensional fractured–pore space of crystalline rocks, for reconstructing and modeling uranium ore formation, and using the geological space for the isolation of radioactive materials.



Anorthosites of the Low-sulfide Platiniferous Horizon (Reef I) in the Upper Riphean Yoko–Dovyren Massif (Northern Cisbaikalia): New Data on the Composition, PGE–Cu–Ni Mineralization, Fluid Regime, and Formation Conditions
Abstract
Recent investigations have made it possible to update the mineralogical, petrochemical, and geochemical characteristics of anorthosites, which are considered the main link and main PGE and Au concentrator in low-sulfide PGM mineralization localized in a specific taxitic horizon (Reef I) of the Yoko–Dovyren massif. The recognized compositional and structural features of this horizon suggest that the anorthosites formed as a result of not only magmatic processes proper, but also late magmatic and postmagmatic processes with extremely high volatile-component activity. The origin of this horizon can be explained by the “compaction” hypothesis and thermal shrinking phenomenon. Zones of weakness up to fractures and cavities formed at the interface of rocks with contrasting compositions and properties while they cooled. Due to the decompression effect, these zones “sucked in” the interstitial leucocratic melt and the volatiles squeezed out of the massif’s deeper horizons. The established trends of variation in mineral composition—Pl (82–88% An); Ol (78–81% Fo); Cpx (40–44% En, 9–18% Fs, and 41–47% Wo); and Opx (74–78% En, 16–24% Fs, and 2–5% Wo)—suggest fractional crystallization of the residual liquor. Fluid–magma interaction processes led to the significant heterogeneity of anorthosites and other rocks, the formation of nonequilibrium mineral assemblages, and the concentration of ore-bearing components. The sulfide assemblages were viewed as products of the subsolidus transformation of solid solutions (mss and iss + poss) that formed during the crystallization of a Cu-rich immiscible sulfide fluid. It was demonstrated that noble metals were associated not only with the limited volume of the sulfide fluid. The bulk of the noble metals with “crustal” components (Sn, Pb, Hg, Bi, As, Sb, Te, S, etc.) were supplied to anorthosite cavities together with volatile components and chlorine, and this accounts for the abundance of platinoid minerals among the other forms of platinoid occurrence. The leading role of reduced gases (H2, CH4, and CO), H2O, and Cl has been established in the genesis of noble metal minerals.



Magmatic Control of Gold Mineralization in Western Primorye
Abstract
The article analyzes the regional gravitational field of northeastern China, Korea, and Western Primorye. The distribution of gold deposits is compared with the development of Mesozoic magmatism and negative gravitational field anomalies. Based on an analysis of geological, minerogenic, petrophysical, and geophysical materials, geological and geophysical zoning of the western part of the Khanka massif was carried out and a scheme was compiled for interpreting geological and geophysical data with minerogenic elements. The authors have determined the relationship between magnetic and gravitational field anomalies and the position of prospective gold-bearing ore districts and clusters in the junction zone of the North China Triassic–Jurassic volcanoplutonic belt with Proterozoic substrates of the Khanka massif. Based on geophysical data, early Jurassic intrusions were identified, which controlled the location of gold ore clusters. A conclusion is drawn about the relationship between gold mineralization and Jurassic magmatism, which increases the prospects for discovering gold mineralization in the Prikhankaysky region of Western Primorye.



Ore Potential of Granitic Rocks of the Gargan Block, East Sayan
Abstract
An algorithm for identifying derivatives of potentially ore-bearing magmas among Precambrian rocks of tonalite–trondhjemite–granodiorite associations (TTGAs) is elaborated and tested using current genetic models. The algorithm is a succession of geochemical criteria for identifying the genesis of source of matters and, as a result, the melt products of geochemical reservoirs enriched in Au and other ore elements. This algorithm (a set of geochemical criteria of the ore potential) can be used for metallogenic zoning of the territories composed of TTGA rocks within ancient cratons.



Mineral Associations and Mo–W Ore Types of the Slepaya Zalezh’ Orebody at the Tyrnyauz Deposit
Abstract
Slepaya Zalezh’, the largest orebody of the Tyrnyauz Mo–W deposit, is considered a first-priority object should mining operations at the deposit be resumed. Molybdoscheelite, scheelite, and molybdenite impregnation in mineable concentrations is genetically related to metasomatites of the productive stage overprinted on skarns, periskarn rocks, hornfelses, and marble. Ore types have been recognized based on the relative amounts of different ore-bearing metasomatite facies and protoliths acting as a diluting mass. Seven ore types have been recognized and mapped in cross section. Types I and II are characterized by predominant (70–90%) aposkarn ores after endo- and exoskarns, accordingly. Type III is characterized by approximately equal proportions of ores after endoskarns and periskarn rocks; type IV differs from type III by a decrease in periskarn rocks replenished by an increase in hornfels. Type V is dominated by ores after exoskarns and, to a lower extent (up to 25%), after marble. Type VI is intermediate between types III and IV. Type VII represents all protoliths in approximately equal proportions. Each type exhibits a stable mineral and chemical composition inherited from the protolith. The ores of each particular type have simple distinguishing features, convenient for logging and mapping, which can be used for manual picking of grab and bulk samples and preliminary ore separation. The ores exhibit narrow ranges of variation in sizes and shapes of ore mineral grains and intergrowths and concentrations of minerals harmful to flotation. The subtle differences in ore mineral concentrations between ore types enable their selective mining and blending. Maps and cross sections contain data on the spatial distribution of the associated components such as garnet and wollastonite in skarns and productive metasomatites, pyroxene–plagioclase periskarn rocks, and hydrothermally altered rocks with Cu, Au, and other mineralization.



The New Massadou Diamondiferous Kimberlite Field in Guinea
Abstract
A new Massadou kimberlite field, was discovered in southeastern Guinea, near the town of Macenta. It consists of 16 poorly diamondiferous kimberlite dikes, ~1 m thick on average. The ore-controlling zone has a width of around 600 m, its orientation corresponds to the K-4 trend after S. Haggerty, and it is quite well detectable in satellite images. A thick laterite weathering profile has developed on the kimberlites. The main indicator minerals are pyrope, chromite, and ilmenite. Ilmenite grains have a zoned structure with a high-Fe core (hemoilmenite) overgrown by a parallel-columnar aggregate of Mg-ilmente rim resulting from interaction of the core phase with kimberlitic melt. The age of kimberlites is estimated as 140–145 Ma by analogy with those in adjacent areas. Dikes occur as an independent form of kimberlite magmatism in the Guinean–Liberian shield, rather than being roots of kimberlite pipes; therefore, the erosion cutout is relatively small and large-scale diamond placers should not be expected.


