Chapter 8 Earth as a Planet

Earth: Overview and Significance

  • Earth exhibits few craters due to a thick atmosphere and active surface, unlike airless bodies which show numerous craters.

  • Historic images from space, particularly from the 1968 Moon missions, marked a shift to a global perspective on Earth.

  • Exploration of Earth’s composition, structure, atmosphere, and oceans aids in understanding its history.

The Global Perspective

Learning Objectives

  • Describe Earth's interior components and the methods used to ascertain its structure.

  • Specify the origin, size, and extent of Earth's magnetic field.

Basic Properties of Earth

  • Diameter: Approximately 12,756 km.

  • Composition: Primarily heavy elements like iron, silicon, and oxygen.

  • Orbit: Nearly circular, allowing for liquid water to exist on its surface

  • Conditions for Life: Earth is uniquely situated to support life due to its temperature range.

Comparison with Other Celestial Bodies

  • Inner planets (terrestrial) differ from stars (hydrogen and helium-dominant).

Earth’s Interior

Challenges in Study

  • Most direct experiences limited to the outer crust (few kilometers deep), making deeper studies challenging.

  • Seismic waves from earthquakes provide insight into Earth's inner structure.

Seismic Studies and Layers

  • Earth's interior comprises several layers determined through seismic wave transmission studies:

    • Crust: The outermost layer.

    • Mantle: Extends down to about 2,900 km; mostly solid but can flow under pressure.

    • Core: Composed mainly of iron (liquid outer core, solid inner core).

    • Density Variation: Density increases with depth, illustrating differentiation.

Earth’s Exterior

Structure of Earth’s Crust

  • Oceanic Crust: Covers 55% of Earth’s surface, composed mainly of basalt, about 6 km thick.

  • Continental Crust: Covers 45%, with thickness between 20-70 km, predominantly made of granite.

  • Density Comparison: Rocks are denser than water (3 g/cm3 versus 1 g/cm3).

Plate Tectonics

  • Geologically, Earth is dynamic with a history of volcanism, erosion, and tectonic movements.

  • Plate Tectonics Theory: Explains the slow movement and interactions of crustal plates leading to continental drift, volcanic activity, and earthquakes.

  • Alfred Wegener proposed continental drift, later corroborated by plate tectonics theory.

    • Rift Zones: Points where crusts pull apart, generating new crust (e.g., Mid-Atlantic ridge).

    • Subduction Zones: Areas where plates collide, often forming ocean trenches and volcanic activity.

Volcanoes

  • Types of Volcanic Activity: Associated with mid-ocean ridges, subduction zones, and hot spots (e.g., Hawaiian Islands).

  • Volcanoes can act as windows into the inner Earth.

Earth’s Atmosphere

Composition and Structure

  • Atmosphere consists mainly of:

    • **78% Nitrogen (N2)

    • 21% Oxygen (O2)

    • Trace amounts of other gases including CO2 and water vapor.**

  • Layers: Troposphere (weather occurs), stratosphere (contains ozone layer), mesosphere, and ionosphere.

Atmospheric Changes Over Time

  • Initially dominated by CO2, atmosphere transformed largely by photosynthesis leading to the oxygen-rich atmosphere of today.

  • Industrialization and human activity increased CO2 levels causing climate change.

Life and Evolution

The Origin of Life

  • Life forms date back over 3.5 billion years, with evidence primarily in the form of stromatolites from microbial life.

  • The evolution of life influenced the stable composition of Earth’s atmosphere.

Human Impact

  • Human activities have markedly influenced climate change, biodiversity, and the composition of the atmosphere.

  • Anthropocene Epoch: Proposed term indicating the profound impact humans have on Earth.

Cosmic Influences on Earth's History

Impact Events

  • Earth has experienced multiple impact events influencing geological and biological evolution.

  • Large impacts can lead to mass extinctions (e.g., 65 million years ago impacting dinosaurs).

Current Threats

  • Ongoing research aims to identify and mitigate the risk of potential future impacts on Earth (e.g., NASA's efforts to track nearby asteroids).

Summary of Key Concepts

  • Earth’s composition, active geology, and atmosphere distinguish it from other celestial bodies.

  • The processes of plate tectonics and volcanic activity shape the surface and history of Earth.

  • Life began early in Earth's timeline and has significantly altered its atmosphere over geological time.