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The investigation of key mineral phases such as zircon, apatite, titanite, rutile, monazite, xenotime, allanite, baddeleyite and garnet, explored in this book, has provided breakthroughs in our understanding of continental crust composition and evolution, as well as the timing, conditions, petrogenetic and geodynamic processes related to its growth and reworking. Therefore, the continuing development of analytical techniques, improvement of tools, data handling, processing, and interpretation allow us to extract and better understand these complex geological processes. This special publication aims at showcasing contributions reviewing the tools and applications of these key minerals, recent technique developments, and new applications using focused case studies investigating igneous, metamorphic and/or detrital rocks that help us put together the continental crust evolution puzzle. This volume highlights the progress made in studies using these key minerals and their future potential.
Methods and Applications of Geochronology provides a comprehensive, practical guide to the rapidly developing field of geochronology. Chapters are written by leading experts in their specific field of geochronology and discuss practical information and ‘rules of thumb’ for establishing laboratories and using analytical equipment. Methods and Applications of Geochronology is an authoritative guide not only for the foundational principles of geochronological research, but also descriptions of analytical methods, guidance for sample selection, all the way to data reduction and presentation. Features the latest techniques and recommended tools for each of the most common geochronological methods Includes perspectives from a variety of well-respected researchers in the field, each representing different specialties of geochronology Bridges the gap between theory and application, offering best practices and relevant case studies throughout
This book presents the first overview of the composition and structure of the Earth’s lower mantle. The first part focuses on the study of lower-mantle minerals, identified as inclusions in diamonds from different regions of the world. Three associations are established among the lower-mantle minerals: ultramafic, mafic, and carbonatic. The carbonatic association is of particular interest because it characterizes the media of natural diamond formation. In turn, the second part analyzes the structure of the lower mantle, revealing its heterogeneous composition. It is based on the results of experiments demonstrating phase transitions in lower-mantle minerals, and on seismological data. Deep-seated earthquakes point to the presence within the lower mantle of numerous seismic boundaries caused by mineral structure transitions. In closing, the last part of the book compares observed data with experimental data, highlighting several discrepancies that indicate Earth may have a more complex planetary history than previously assumed, and examining its primarily non-chondritic composition.
This dissertation, "Experimental Approach to the Direct Interaction Between the Proto-atmosphere and Rocky Crust of the Early Earth and Its Implications to the Early Evolution of Earth-like Planets" by Xiluo, Hao, 郝锡荦, was obtained from The University of Hong Kong (Pokfulam, Hong Kong) and is being sold pursuant to Creative Commons: Attribution 3.0 Hong Kong License. The content of this dissertation has not been altered in any way. We have altered the formatting in order to facilitate the ease of printing and reading of the dissertation. All rights not granted by the above license are retained by the author. Abstract: The first eon of the Earth, Hadean, is no doubt critical for the evolution of Earth towards a habitable planet and the origin of life. However, there is almost no petrologic record preserved for this piece of history because of the long-term geological reworking. In this study, batch experiments simulating the interaction between the early Earth's ultramafic crust and H2O-CO2 atmosphere were performed in order to gain some new insights into the direct interaction and its influence on the evolution of mineral, atmosphere, ocean and the prebiotic chemistry on the early Earth. Electron microscopic observations (including SEM and TEM) show that the secondary minerals produced in the experiments mainly include phyllosilicates, carbonates and Fe-oxide. Phyllosilicates which are essential for biomonomer synthesis can be found in each of our experiments. Different rock-water-H2O systems result in different clay minerals with varied crystal habits. Carbonates can be found in experiments carried out at temperature below 400 C. With the experimental temperature decrease from 400 C to 200 C, the formed carbonates change from calcite, dolomite and magnesite accordingly. Energy dispersive spectroscopy reveals the incorporation of iron in all kinds of carbonates. Hexagonal magnetite nanoplates are observed in komatiite-H2O-CO2 experiment carried out at 450 C. The mineralogical compositions imply that the interaction between the early Earth's ultramafic crust and H2O-CO2 atmosphere were able to produce clay minerals, carbonates and oxides on the rocky planets such as Earth, which was corroborated by the recent discovery of layered clay minerals and carbonates assemblages on Mars. More importantly, these secondary minerals are effective in catalyzing the inorganic molecular to biomolecules that are essential in prebiotic chemical evolution. The GC measurement of the gaseous phases trapped in the capsule after experiments show that abiogenetic methane, ethane and propane as well as hydrogen were detected in most our experiments. The relative concentrations of these gases are higher in high temperature experiments, which indicate high productivity of CH4 and H2 during the interaction between the early Earth's ultramafic crust and H2O-CO2 atmosphere. The abiotic formation and accumulation of H2, methane, and short hydrocarbon would not only provide material basis for the chemical evolution towards life but also play essential roles in preventing the surface of the Earth from freezing in the Hadean eon while the Earth was suffering from extensive precipitation of atmospheric CO2 and the faint young sun. Generally, the earliest interaction between the Earth's ultramafic crust and H2O-CO2 atmosphere could have changed the physicochemical condition of the Earth's surface that favored the prebiotic chemical evolution towards life. DOI: 10.5353/th_b5570776 Subjects: Atmosphere
Volume 57 of Reviews in Mineralogy and Geochemistry highlights the present knowledge on micro- and mesoporous mineral phases, with focus on their crystal-chemical aspects, occurrence and porous activity in nature and experiments. As zeolites are the matter of numerous ad hoc meetings and books - including two volumes in this series - they do not specifically appear in the present volume. The phases of the sodalite and cancrinite-davyne groups, which mineralogists consider distinct from zeolites, are instead considered (in the order, chapter 7 by W. Depmeier and part of chapter 8 by E. Bonaccorsi and S. Merlino, respectively).
Mineral deposits are not only primary sources of wealth generation, but also act as windows through which to view the evolution and interrelationships of the Earth system. Deposits formed throughout the last 3.8 billion years of the Earth's history preserve key evidence with which to test fundamental questions about the evolution of the Earth. These include: the nature of early magmatic and tectonic processes, supercontinent reconstructions, the state of the atmosphere and hydrosphere with time, and the emergence and development of life. The interlinking processes that form mineral deposits have always sat at the heart of the Earth system and the potential for using deposits as tools to understand that evolving system over geological time is increasingly recognized. This volume contains research aimed both at understanding the origins of mineral deposits and at using mineral deposits as tools to explore different long-term Earth processes.
Mineral Systems, Earth Evolution, and Global Metallogeny provides insights into the critical parameters of Earth’s evolution, particularly in terms of thermal state, tectonics, and the atmosphere-hydrosphere-biosphere system, that control the metallogeny of the planet. World-class to giant mineral systems are described and interpreted in terms of their relationship to critical periods of change in tectonic regimes within the supercontinent cycle and evolution of the mantle lithosphere. Specific times of formation of highly anomalous giant mineral systems, such as the so-called Boring Billion, are discussed together with specific tectonic environments, such as craton edges and thick lithosphere margins. Mineral Systems, Earth Evolution, and Global Metallogeny provides an overview of how the evolution of Earth has dictated the nature and distribution of its mineral resources that are the foundation of our modern industries and provides insights into critical parameters for conceptual exploration targeting. Researchers, academicians, undergraduate and graduate students, and geologists in the fields of economic geology, geologic exploration, mineral systems, and earth evolution will find this to be a helpful textbook in understanding the timing and distribution of the world’s major mineral deposits are related to critical parameters controlling earth evolution. Draws together aspects of each book section through summary tables Synthesizes data in each book section using summary diagrams/figures Provides continuity between related sections of the book by providing end-of-chapter bullet-point conclusions
Reviews in Mineralogy & Geochemistry (RiMG) volumes contain concise advances in theoretical and/or applied mineralogy, crystallography, petrology, and geochemistry.