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Cover image for Archean and Proterozoic Earth Infancy and Adolescence of the Planet Earth.
Title:
Archean and Proterozoic Earth Infancy and Adolescence of the Planet Earth.
Author:
Philippot, Pascal.
ISBN:
9781394417841

9781394417865
Publication Information:
Newark : John Wiley & Sons, Incorporated, 2025.
Physical Description:
1 online resource (381 p.).
General Note:
Description based upon print version of record.

5.3. Ocean temperature during the Precambrian
Contents:
1.6. Conclusion -- 1.7. References -- Chapter 2. Dynamics of the Mantle, Lithosphere, and Crust in the Archean -- 2.1. Introduction -- 2.2. Change in the composition of the upper continental crust: plate tectonics or denudation? -- 2.2.1. A crustal perspective on continental growth -- 2.2.2. A mantle perspective on continental growth -- 2.3. Archean tectonics -- 2.3.1. Beyond observations: numerical geodynamics -- 2.4. Conclusions -- 2.5. References -- Chapter 3. Precambrian Magnetic Field and Paleogeographic Reconstructions -- 3.1. Introductory overview of Earth's magnetic field

3.1.1. The magnetic field in the Ediacaran -- 3.1.2. The Proterozoic: tracing back to the Archean (from 635 to 2,500 Ma) -- 3.1.3. In the Archean (and before) -- 3.1.4. Life under an unstable and weak magnetic field -- 3.2. Using the Earth's magnetic field record to build paleogeographic reconstructions -- 3.2.1. Insights from paleogeographic reconstructions -- 3.2.2. Reconstructing the paleopositions of cratonic blocks and paleogeographies: paleomagnetism -- 3.3. Precambrian paleogeographic models -- 3.3.1. Supercratons/supercontinents -- 3.3.2. The Archean and paleoproterozoic

3.3.3. From the Paleoproterozoic to the Mesoproterozoic: Nuna supercontinent -- 3.3.4. From the Mesoproterozoic to the Neoproterozoic: the Rodinia supercontinent -- 3.3.5. The end of the Precambrian: toward the formation of Gondwana -- 3.4. References -- Chapter 4. Archean Magmatism -- 4.1. Introduction -- 4.2. The lavas of the greenstone belts -- 4.2.1. Basic and ultrabasic lavas -- 4.2.2. Basic and intermediate lavas with "arc" affinity -- 4.2.3. Acidic lavas and pyroclastic rocks -- 4.3. Granitoids -- 4.3.1. Granitoids derived from the melting of crustal lithologies

4.3.2. Granitoids associated with a differentiation lineage: a mantle origin -- 4.4. Gray gneisses -- 4.5. Geodynamic considerations -- 4.5.1. The magmas of the present-day Earth and their geodynamic significance -- 4.5.2. Archean magmas and the dynamics of the ancient Earth -- 4.5.3. On "subduction" -- 4.5.4. The temporal evolution of Archean magmas -- 4.6. References -- Chapter 5. Temperature and Chemical Composition of Precambrian Oceans -- 5.1. Introduction -- 5.2. Very ancient oceans -- 5.2.1. Liquid water on Earth since the Hadean -- 5.2.2. The origin of water
Abstract:
It took nearly four billion years for the Earth to become a hospitable planet. Archean and Proterozoic Earth traces the geodynamic, biological, climatic and environmental upheavals that accompanied this evolution. This book looks at the planet's secular cooling and its implications for the dynamics of the Earth's mantle and the development of plate tectonics, as well as the evolution of magma composition and the formation of a differentiated continental crust. It shows how variations in the intensity of the Earth's magnetic field have proved useful in reconstructing the movement of continents across the surface of the globe. The book also documents the origin of the oceans and the appearance of the first traces of life, and describes the evolution of the major biogeochemical cycles that led to the oxygenation of the atmosphere, the diversification of living organisms and the concentration of substances of economic interest, particularly metals.
Local Note:
John Wiley and Sons
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