F4.1 Earth Structure

Introduction

  • Recap of the internal structure of the Earth.

  • Understand how geologists gather evidence about Earth's interior.

Page 1: Understanding the Internal Structure of Earth

  • Objective to deepen understanding of Earth's internal structure.

  • Overview of geologists' methods to investigate the Earth's interior.

Page 2: The Hypsographic Curve

  • Mountain heights: Mt. Everest = 8850 meters.

  • Land comprises 29.2% of Earth's surface; oceans cover 70.8%.

  • Average elevation of land is approximately 840 meters.

  • Average depth of oceans is about 3729 meters.

  • Deep ocean regions and trenches, like the Mariana Trench (11,022 meters), are highlighted.

Page 3: Distribution of Elevations

  • Hypsographic curve visualizes cumulative elevations of Earth's surface.

  • Key elevation groupings:

    • Continents: typically hundreds of meters above sea level.

    • Oceanic abyssal plains: approximately 4300 meters below sea level.

  • Differences in oceanic and continental crust structure confirmed by research.

  • Dynamic Earth processes prevent erosion and sediment accumulation over long periods.

Page 4: Interest in Other Planets

  • Exploration of surfaces of Venus, Mars, and the Moon compared to Earth.

  • Characterization of planetary elevations through Gaussian distribution.

Page 5: Major Features of Earth's Surface

  • Major geological features discussed:

    • Oceanic Crust (20-65 Ma, 65 Ma).

    • Geological provinces such as shields, platforms, orogens, basins, and large igneous provinces.

Page 7: Structure of Earth

  • Illustrates Earth’s structure:

    • Crust: outer layer, contains continents, mountains, and oceans.

    • Mantle: extends beneath the crust.

    • Core: innermost part consisting of inner and outer cores.

Page 9: Tectonic Plate Interaction

  • Description of crust and mantle interactions due to tectonic activity.

  • Explains magma movement and tectonic currents.

Page 10: Earth's Structure

  • Overview of Earth's layers:

    • Crust (oceanic and continental): granitic and basaltic rocks.

    • Lithosphere: rigid outer shell.

    • Asthenosphere: softer layer beneath the lithosphere.

    • Mesosphere: lower mantle features.

    • Outer core: liquid; inner core: solid.

Page 11: Oceanic Crust Details

  • Oceanic crust characteristics:

    • Solid rock: up to 35km thick.

    • Composed mainly of basalt.

    • Higher density (3 g/cm³), therefore young in geological terms (rarely older than 200 million years).

Page 13: Continental Crust Overview

  • Continental crust properties:

    • Thicker than oceanic crust (average 40km).

    • Composed of various rocks, primarily granitic (felsic materials).

    • Lower density (2.7 g/cm³); older history (up to 3.7 billion years).

Page 15: Discontinuities in Earth's Layers

  • Explanation of discontinuities, signifying changes in physical or chemical properties of rocks:

    • Conrad Discontinuity, Moho Discontinuity, Repetti Discontinuity, Gutenberg Discontinuity, and Lehmann Discontinuity.

Page 18: Asthenosphere Characteristics

  • Lithosphere and asthenosphere:

    • Lithosphere: rigid layer of the crust and upper mantle.

    • Asthenosphere: semi-fluid layer allowing for tectonic movement.

    • Low-velocity zone signifies mantle properties where rocks begin to partially melt.

Page 21: Upper Mantle Composition

  • Upper mantle:

    • Consists of solid silicates, primarily peridotite.

    • Radioactive decay contributes to Earth's heat source.

Page 22: Lower Mantle Properties

  • Lower mantle:

    • Remains solid due to intense pressure.

    • Contains heavier silicates, resembling stony meteorites.

Page 24: Understanding the Outer Core

  • Characteristics of the outer core:

    • Composed mainly of liquid iron and nickel, creating reduced rigidity.

    • Temperature and pressure conditions result in its liquid state.

Page 26: Inner Core Description

  • Inner core:

    • Solid state, composed primarily of iron (with some nickel).

    • Experiences extreme pressure (3.6 million times Earth’s surface pressure).

    • Density approximately 12 g/cm³.

Conclusion

  • Understanding the internal structure is key to grasping Earth's geological activity.

  • Discontinuities and the differences between crust types provide insights into tectonic processes.