Book contents
- Frontmatter
- Contents
- Foreword to the English edition
- Foreword to the French edition
- Acknowledgments
- Introduction
- 1 The properties of elements
- 2 Mass conservation – elemental and isotopic fractionation
- 3 Geochronology and radiogenic tracers
- 4 Element transport
- 5 Geochemical systems
- 6 Waters present and past
- 7 Mineral reactions
- 8 The solid Earth
- 9 The Earth in the Solar System
- 10 The geochemical behavior of selected elements
- Appendix A Composition of the major geological units
- Appendix B The mixing equation for ratios
- Appendix C A refresher on thermodynamics
- Appendix D The Rayleigh distillation equation
- Appendix E The geological time scale
- Appendix F An overview of analytical methods
- Appendix G Physical and geophysical constants
- Appendix H Some equations relative to residence time
- Further reading
- Index
8 - The solid Earth
- Frontmatter
- Contents
- Foreword to the English edition
- Foreword to the French edition
- Acknowledgments
- Introduction
- 1 The properties of elements
- 2 Mass conservation – elemental and isotopic fractionation
- 3 Geochronology and radiogenic tracers
- 4 Element transport
- 5 Geochemical systems
- 6 Waters present and past
- 7 Mineral reactions
- 8 The solid Earth
- 9 The Earth in the Solar System
- 10 The geochemical behavior of selected elements
- Appendix A Composition of the major geological units
- Appendix B The mixing equation for ratios
- Appendix C A refresher on thermodynamics
- Appendix D The Rayleigh distillation equation
- Appendix E The geological time scale
- Appendix F An overview of analytical methods
- Appendix G Physical and geophysical constants
- Appendix H Some equations relative to residence time
- Further reading
- Index
Summary
Before discussing the formation of the major geological units of the solid Earth, we should review the internal structure of our planet as described by seismic wave studies (Fig. 8.1). The most important discontinuities observed by seismologists down to the base of the mantle are:
The base of the crust (called the Mohorovičić discontinuity or Moho), 40 km below the continents, but only 5–7 km beneath the oceans.
The base of the lithosphere, on average 80 km below the oceans, and deeper still beneath the continents. This is the lower boundary of the rigid tectonic plates. The softer part of the upper mantle underneath the lithosphere is called the asthenosphere.
The 440 km discontinuity corresponding to a change in olivine structure (spinel or ringwoodite phase).
The 660 km discontinuity corresponding to the transformation of all minerals into perovskite and minor Fe-Mg oxide (magnesio-wüstite). This is the base of the upper mantle.
The mantle–core boundary at about 2900 km. Above this boundary is a seismically abnormal layer some 200 km thick, known as the D″ layer.
The core is divided into a liquid outer core, responsible for the Earth's magnetic field, and a solid inner core. The core is metallic and composed mostly of iron and nickel.
Plate tectonics is a powerful theory that unifies the geological expression of crustal and upper mantle geodynamics (Fig. 8.2).
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- Information
- GeochemistryAn Introduction, pp. 137 - 164Publisher: Cambridge University PressPrint publication year: 2003