0.0(0)
study
Generate Practice test
study
Chat with Kai
study
View the linked pdf

9a_InternalStructure

Earth’s Changing Landscape Systems

Earth’s Internal Energy and Structure

  • Earth’s Internal Heat Engine

    • Major processes contributing to Earth's internal heat:

      • Heat from colliding particles during Earth's formation.

      • Heat released from gravitational contraction of the early Earth.

      • Heat from radioactive decay of unstable isotopes within Earth.

      • Early impact with a Mars-sized object which caused significant heating.

      • Heat released as iron crystallized to form the solid inner core.

Formation of Earth

  • Planetesimals Aggregated to Form Larger Bodies

    • Formed approximately 4.6 billion years ago, leading to planetary formation.

    • Earth was struck by a large Mars-sized body around 4.5 billion years ago.

      • This collision resulted in extensive heating and melting of both the Earth and the impactor.

      • Formation of the Moon from ejected material into space.

  • Global Chemical Differentiation

    • Began about 4.5 billion years ago, setting the stage for Earth’s internal structure.

The Earth 4.5 Billion Years Ago

  • Magma Ocean

    • Initial magma ocean was hundreds of kilometers deep.

    • Cooled and crystallized from the bottom-up to form a solid mantle capped by primitive crust composed of basalt and komatiite.

  • Radioactive Isotopes

    • Short-lived radioactive isotopes with a few million years half-lives have long since decayed.

    • Long-lived isotopes continue to warm the planet.

  • Internal Layers of Earth Today

    • Iron sank during differentiation to form outer and inner core.

    • The mantle and crust were formed after cooling of the magma ocean.

    • Studying Earth’s interior is challenging due to:

      • Limited depth of drilling (few kilometers into the crust).

      • Rocks sampled may not represent deeper layers.

Exploring the Subsurface

Physical Samples

  • Magma brings up pieces of deeper rocks through:

    • Mines, drilling, and deep, uplifted rock exposures.

Geophysical Surveys

  • Techniques for subsurface exploration include:

    • Magnetic data.

    • Gravity data and models.

    • Electrical surveys.

    • Seismic-reflection data.

Investigating Deep Processes

  • Utilize computers to model Earth’s interior using seismic refraction data.

  • Study rocks originating from deep within the Earth.

  • Replicate deep conditions in laboratory settings.

Seismic Waves

  • Definition and Behavior

    • Tectonic forces cause Earth’s crust to deform and break along faults, releasing energy as seismic waves.

    • Seismic waves travel through Earth in all directions, contributing to our understanding of earthquakes.

    • The point of initial fault slippage is known as the focus, with the point directly above it on the surface referred to as the epicenter.

  • Seismographs

    • Instruments measuring ground vibrations, capturing three components of motion:

      • Vertical up-down motion.

      • Horizontal east-west motion.

      • Horizontal north-south motion.

Types of Seismic Waves

  • P-waves (Primary Waves)

    • Fastest seismic waves, arriving first at a station.

    • Travel through solids, liquids, and gases at an average speed of ~5 km/sec.

    • Push or pull particles of matter in the direction of travel.

  • S-waves (Secondary Waves)

    • Arrive second; half the speed of P-waves.

    • Can only travel through solid rock; shear waves that push material at right angles.

  • Surface Waves

    • Slowest waves, confined to surface and outer layers of the Earth.

    • Cause most earthquake destruction, similar in motion to ocean waves.

Seismic Wave Behavior at Boundaries

  • When seismic waves encounter boundaries (different materials), they split into reflected and refracted waves:

    • If the waves speed up, they bend upward; if they slow down, they bend downward.

Crustal Composition

  • Oceanic Crust

    • Ranges from 3 to 15 km thick, primarily composed of basalt and gabbro.

  • Continental Crust

    • ~40 to 65 km thick, average composition of granite, more buoyant than oceanic crust.

Lithosphere and Asthenosphere

  • Lithosphere

    • Cool, rigid layer averages about 100 km thick but can be up to 250 km beneath older continental regions.

    • Comprised of the crust and solid upper portion of the mantle.

  • Asthenosphere

    • Lies just below the lithosphere, a weaker zone of partially melted peridotite.

    • Seismic velocities slow down in the upper portion.

Transition Zones

  • Upper Transition Zone

    • Marks the change from olivine to spinel crystal structure (400 km depth).

  • Lower Transition Zone

    • Marks the transition from spinel to perovskite crystal structure (670 km depth).

    • Seismic waves bend outward in the deep mantle due to increasing velocities.

The Mesosphere (Lower Mantle)

  • P- and S-wave velocities increase with depth in the mesosphere.

  • Rocks are solid but extremely hot and capable of flow.

Study of the Outer and Inner Core

  • Outer Core

    • Composed of liquid iron, where P-waves slow down and S-waves cannot pass through.

    • P-wave shadow zone created due to bending of seismic waves.

  • Inner Core

    • Consists of solid iron and nickel, where P-waves speed up again.

Earth’s Magnetic Field

  • Generated by circulation of liquid iron in the outer core due to convection driven by internal heat.

  • Electric currents from this motion create Earth’s magnetic field.

Earth’s Internal Heat Engine

  • Earth’s temperature increases with depth, known as the geothermal gradient:

    • Averages between 20°C and 30°C per km in the crust, less in other layers.

    • Variations can occur in heat flow across different regions.

Modern Heat Flow

  • Heat continues to escape from the Earth's interior:

    • High heat flow in mid-ocean ridges and volcanically active areas.

    • Lower heat flow within stable continental interiors.

Heat Transfer Mechanisms

  • Heat flow in the crust: conduction, generally inefficient at transferring heat.

  • Heat flow in the mantle: moderate temperature increase with depth, effective heat transfer likely through convection.

Theories of Mantle Convection

  • Two-Layer Mantle Convection

    • Separate convection cells for upper and lower mantle, defined by the 670 km transition zone.

  • Whole-Mantle Convection

    • Upper and lower mantle form one system with large convection cells originating at the core-mantle boundary.

Seismic Tomography

  • Creates 3D models of Earth's interior based on seismic wave data.

  • Requires extensive seismic records from various earthquakes, revealing regions with varying wave speeds, attributed to temperature and material differences.

0.0(0)
study
Chat with Kai
study
View the linked pdf
robot