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Автор(ы):SchUtfort E.G.
Издание:2001 г., 149 стр.
Язык(и)Английский
The genesis of the San Vicente lead zinc rhythmite deposit, Peru - a petrologic, geochemical, and sulfur isotope study / Генезис свинцово-цинкового ритмитового месторождения Сан-Висенте, Перу - петрологическое, геохимическое и изотопное исследование серы

The purpose of this research has been to determine the origin of the San Vicente zinc-lead deposit based on textural, mineralogical and geochemical studies of the sulfide ores and carbonate host rock. The relatively simple and uncomplicated mineralogy of the ores and host rock permits the application of standard petrographic techniques as well as specialized methods such as cathodoluminescence, electron microprobe analysis, and detailed sulfur isotope geochemistry. <...>

Редактор(ы):Cubitt J.M., England W.A.
Издание:The Geological Society of London, 1995 г., 316 стр., ISBN: 1-897799-26-8
Язык(и)Английский
The geochemistry of reservoirs / Геохимия резервуаров

We believe this is the first collection of papers to be devoted entirely to reservoir geochemistry, which is an area of growing scientific and economic importance. The main aim of reservoir geochemistry is to understand the distributions and origin(s) of the petroleums, waters and minerals in the reservoir and account for their possible spatial and compositional variation. This is ideally related to basin history and location of source-rock kitchens and migration pathways.

Автор(ы):Porter T.M., Sterling S.Cook
Издание:PGS Publishing, Linden Park, 2005 г., 34 стр.
Язык(и)Английский
The Geologic History of Oxidation and Supergene Enrichment in the Porphyry Copper Deposits of Southwestern North America

More than fifty significant porphyry copper deposits are distributed over a 2000 km interval within the U.S. and Mexico, following a trend subparallel to the southwestern margin of North America. These include giant supergene enriched deposits such as those at Morenci in Arizona (4.7 Gt @ 0.52% Cu) and Cananea (7.1 Gt @ 0.42% Cu) in Sonora, Mexico.

The porphyry copper deposits of southwestern North America were developed in a continental margin cratonic setting, above a subduction zone that was active largely from the Early Mesozoic to the Late-Tertiary. While significant ore deposits of Jurassic to Mid-Tertiary age are known, the majority were emplaced between 72 and 55 Ma, during the peak of magmatic activity along the Laramide Arc. Laramide magmatism and crustal shortening ceased by around 50 Ma, in the mid Eocene, to be followed by a 15 m.y. period of magmatic quiescence, erosion and localised continental sedimentation, the Eocene Epeirogeny. This was succeeded from around 35 Ma by the Mid-Tertiary Orogeny, which persisted through the Oligocene to the Early Miocene and resulted in renewed, widespread volcanism, and by crustal extension. Extension was characterised by the development of listric, detachment and strike-slip faults, associated listric tilting of up to 60° or more, and the uplift and exposure of metamorphic core complexes. During the Mid- to Late-Miocene, between 18 and 10 Ma, the nature of tectonism in the region changed through a period of transition, from an extensional to a block faulted 'basin and range' regime which persists locally to the present. The typical basins are grabens or half grabens, with structural relief between the base of sediment filled basins and the crests of the adjacent ranges of from 2 to 4 km, and sometimes more than 6 km.

Автор(ы):Wilhelms D.E.
Издание:United States Government Printing Office, 1987 г., 328 стр.
Язык(и)Английский
The geologic history of the moon / Геологическая история луны

The Moon held little interest for most scientists after its basic astronomic properties had been determined and before direct exploration appeared likely (Wright and others, 1963; Baldwin, 1978). Speculations about its internal structure, composition, and origin were only broadly constrained by cosmochemical data from meteorites and solar spectra, and by astronomic data about its size, shape, motions, and surficial properties (Urey, 1951, 1952; Kuiper, 1954). Most investigators who were active before the space age began in 1957 believed that significant new advances in lunar knowledge required acquisition of additional data.

Том 1-2
Редактор(ы):Gradstein F.M., Ogg G.M., Ogg J.G., Schmitz M.D.
Издание:Elsevier, 2012 г., 1138 стр., ISBN: 978-0-44-459390-0
Язык(и)Английский
The geologic time scale / Геологическая временная шкала

This study presents the science community and schools with a new geologic timescale for circa four billion years of Earth history. A chapter is also devoted to time scales for our moon and neighboring planets. This book details many recent advances in stratigraphy, the science of the layering of strata and its content, in radiogenic and stable isotopes chronology, and in age and duration calculations using orbital tuning models.

Редактор(ы):Gradstein F.M., Ogg G.M., Ogg J.G., Schmitz M.D.
Издание:Cambridge University Press, 2004 г., 610 стр., ISBN: 978-0-511-07405-9
Язык(и)Английский
The geologic time scale / Геологическая временная шкала

This study presents the science community with a new geologic time scale for circa 3850 million years of Earth history. The scale encompasses many recent advances in stratigraphy, the science of the layering of strata on Earth. The new scale closely links radiometric and astronomical age dating, and provides comprehensive error analysis on the age of boundaries for a majority of the geologic divisions of time. Much advantage in time scale construction is gained by the concept of stage boundary definition, developed and actively pursued under the auspices of the International Commission on Stratigraphy (ICS), that co-sponsors this study. <...>

Редактор(ы):Gradstein F.M., Ogg G.M., Ogg J.G., Schmitz M.D.
Издание:Elsevier, 2020 г., 1366 стр., ISBN: 978-0-12-824360-2
Язык(и)Английский
The geologic time scale / Геологическая временная шкала
Издание:PGS Publishing, Linden Park, 2002 г., 21 стр.
Язык(и)Английский
The Geological Framework, Distribution and Controls of Fe-Oxide Cu-Au Mineralisation in the Gawler Craton, South Australia: Part I - Geological and Tectonic Framework / Геологическая структура, распределение и контроль железооксидно-медно-золотой минер...

Геологическая структура, распределение и контроль железооксидно-медно-золотой минерализации в кратоне Гоулер, Южная Австралия: Часть I - Геологическая и тектоническая структура

 

The Archaean to Mesoproterozoic Gawler Craton hosts a range of economic mineral commodities, including Au (central Craton), Ag-Pb-Zn (eastern Eyre Peninsula) and iron ore of the Middleback Ranges. A major iron-oxide copper-gold province containing the world class Olympic Dam Cu-U-Au-Ag-REE deposits extends ~ 500 km along the eastern margin of the Craton, from the Mount Woods Inlier in the north to the Moonta-Wallaroo district in the south. This paper presents new advances in our understanding of the structure, deformation history and tectonic evolution of the Gawler Craton, which may lead to a better understanding of the distribution of these mineral systems. The Craton is subdivided into tectonic domains, each encompassing an area of crust containing similar lithological and structural associations. New tectonic events have been defined within the three major orogenic cycles of the Gawler Craton (the Sleaford, Kimban and Kararan Orogenies). The recent discovery that much of the craton comprises relatively juvenile Proterozoic crust has improved our understanding of cratonic evolution. We propose growth through accretion in magmatic arc settings along the eastern margin of an arcuate Archaean core at ~ 1850 Ma (Donington Suite), and along the southwestern margin at ~ 1680 Ma (Tunkillia Suite) and 1620 Ma (St Peters Suite). We suggest an alternative model to a largely anorogenic setting for emplacement of the Hiltaba Suite, an intracontinental, extensional back-arc, located behind a northeast dipping subduction zone, south of the Nuyts Domain, which produced the arc-related magmatism of the St Peters Suite.

The Hiltaba Suite magmatic event was widespread across the Gawler Craton, and is broadly associated, both temporally and in places spatially with a major mineralising event. At the Olympic Dam deposit, a close spatial and temporal association is recognised between its host rock, the Roxby Downs Granite, and iron-oxide copper-gold mineralisation. Other mineral prospects related to Hiltaba Suite magmatism include Tarcoola, Tunkillia, Myall, Sheoak, Barns, and possibly Weednana, and Menninnie Dam. The presence of Hiltaba Suite granites is an important factor for exploration companies in tenement selection.

Издание:PGS Publishing, Linden Park, 2002 г., 15 стр.
Язык(и)Английский
The Geological Framework, Distribution and Controls of Fe-Oxide Cu-Au Mineralisation in the Gawler Craton, South Australia: Part II - Alteration and Mineralisation

The Olympic Cu-Au province on the eastern margin of the Gawler Craton includes three major regions of hydrothermal alteration and mineralisation: Stuart Shelf basement (including the Olympic Dam Cu-U-Au deposit), Mount Woods lnlier and the Moonta-Wallaroo-Roopena region. Each of these regions contains high-, moderate- and low-temperature Fe-oxide rich alteration, Cu-Au+U mineralisation, and felsic to mafic Mesoproterozoic (-1590 Ma) intrusions of the Hiltaba Suite with or without coeval Gawler Range Volcanics. The three regions are interpreted to represent the 'footprints' of separate crustal-scale thermal anomalies. Three key hydrothermal alteration and ore mineral assemblages are recognised in the metallogenic province: (1) CAM: calcsilicate - alkali feldspar ± magnetite ± Fe-Cu sulphides (generally minor); (2) MB: magnetite-biotite + Fe-Cu sulphides; and (3) HSCC: hematite-sericite-chlorite-carbonate ± Fe-Cu sulphides ± U, REE minerals. Ore grade Cu-U-Au mineralisation is generally associated with the HSCC assemblage, which is paragenetically later than the CAM and MB assemblages in most deposits and prospects. The crustal level of exposure of the hydrothermal systems may vary significantly between and within the three mineralised regions. The CAM, MB and HSCC assemblages and associated Cu-Au mineralisation represent a possible spectrum of settings from deeper, higher temperature, shear-hosted environments to near-surface, low-temperature breccia and fault settings.

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