Earth's Interior
Earth's Interior
Probing Earth’s Interior
- Most knowledge of Earth's interior comes from seismology.
- Travel times of seismic waves vary depending on the rock type.
- Travel paths are complex, enabling the identification of resources like oil.
Seismic Wave Properties
- Important characteristics of seismic waves:
- S waves only travel through solids.
- P waves travel faster than S waves.
- Seismic waves travel faster through stiffer rock.
- Waves can reflect and refract at boundaries between different materials.
Earth's Layer Structure
- By analyzing changes in wave behavior, scientists locate boundaries within the Earth.
- Types of layers by composition:
- Crust
- Mantle
- Core
- Types of layers by physical properties:
- Lithosphere
- Asthenosphere
- Transition Zone
- Mesosphere
- D” Layer
- Outer Core
- Inner Core
Layers by Composition
Crust:
- Thin outer layer of the Earth.
- Oceanic Crust:
- Averages 7 km thick; typically younger and denser.
- Continental Crust:
- Averages 40 km thick; can reach up to 70 km.
The Moho (Mohorovicic discontinuity):
- The boundary between the crust and the mantle, where P waves are refracted.
Mantle:
- A solid rocky shell made primarily of peridotite, extending to a depth of approximately 2900 km.
Layers by Physical Properties
Upper Mantle:
- Extends to 660 km depth.
- Lithosphere:
- Comprises the crust and upper mantle, ranging from a few to about 200 km deep.
Asthenosphere:
- Extends up to 410 km; noted for its weaker properties.
Transition Zone:
- Ranges from 410 km to 660 km with a rapid increase in density and phase changes in olivine.
Lower Mantle (Mesosphere):
- Extends from 660 km to ~2800 km.
- D” Layer:
- Boundary between core and mantle, with variable composition and temperature.
Core-mantle boundary:
- P waves die out around 100°, reappearing around 140° creating a P-wave shadow zone.
Core Composition
Core:
- Primarily made of iron, some nickel, with trace amounts of other elements.
- Radius is approximately 3500 km.
Outer Core:
- Liquid layer about 2300 km thick, responsible for Earth's magnetic field.
Inner Core:
- Solid, with a diameter of roughly 1200 km. It will grow as Earth cools.
Inner-core / outer-core boundary:
- P waves passing through the inner core are faster, demonstrating refraction.
Earth's Temperature
- Earth remains hot due to:
- Collisions during formation.
- Impact events that led to the formation of the Moon.
- Radiogenic Heat: Caused by short-lived radioactive atoms and long-lived isotopes effecting decay.
Heat Transfer Mechanisms
Convection:
- Movement of material in fluid-like manner.
Conduction:
- Collisions of atoms; transmission of energy through electron flow.
Radiation:
- Transfer of energy via waves, predominantly occurring in the atmosphere.
Geothermal Gradient
- The geothermal gradient fluctuates significantly across the surface and varies with depth.
Earth's Structure Characteristics
- Earth is not perfectly spherical; it is larger at the equator, leading to gravity anomalies.
Earth's Magnetic Field
- The magnetic field has a similar structure to that of a bar magnet and is thought to form like an electromagnet via a process known as geodynamo.
Requirements for Magnetic Field Production
- An electrically conducting, fluid interior is essential.
- Convection within the fluid layer is necessary.
- Some minimum rotation of the Earth is needed.
Polar Wandering and Field Reversal
- The inner core rotates faster than the Earth’s surface, contributing to polar wandering.
- The magnetic field not only wanders but can also reverse, a process still under investigation.
Seismic Tomography
- Utilizes signals from numerous earthquakes and seismograph stations to create a comprehensive image of the Earth’s interior, akin to a CT scan.
Summary Notes
- Understanding the internal structure of Earth.
- Methods of studying Earth's interior.
- Specifics of different geological layers.
- Internal temperature dynamics.
- Gravitational variations and implications of seismic tomography.
- Characteristics of Earth's magnetic field.