Geology: Deep Structure, Composition, and Magnetic Fields of Earth

Introduction to Earth’s Interior

  • Studying the interior of the Earth presents a significant challenge because humans lack direct access to it.
  • Despite this lack of access, understanding the interior is essential because processes observed at the Earth’s surface are driven by heat generated within the Earth.
  • Results of internal processes include:
    • Volcanism.
    • Earthquakes.
    • Many of the Earth’s surface features.
  • Knowledge of the interior is primarily gathered through indirect means, primarily by using seismic data to determine internal structure.
  • Early 1900s Discovery: Scientists discovered that seismic waves generated by earthquakes help distinguish the properties of the internal layers.
  • Seismic Wave Properties:
    • The velocity of these waves (Primary and Secondary waves, or P and S waves) changes based on the density of the materials they travel through.
    • Seismic waves do not travel in straight lines; they are reflected and refracted, indicating the Earth is not homogeneous throughout.

Seismic Waves and Internal Detection

  • Seismic waves are energy waves generated during earthquakes that propagate through the Earth as wave fronts from their point of origin.
  • Primary Waves (P-waves): These are compressional waves that move back and forth like an accordion.
  • Secondary Waves (S-waves): These are shear waves that move material in a direction perpendicular to the direction of travel, similar to snapping a rope.
  • Wave Velocity and Density: The velocity of both P and S waves increases as the density of the material they travel through increases (vρv \propto \rho).
  • Behavior in Liquids:
    • Most liquids are less dense than their solid counterparts.
    • Seismic velocity is dependent on density; therefore, the presence of liquid phases affects wave behavior.
    • S-waves cannot travel through liquids because the side-to-side (shear) motion cannot be maintained in fluids. This absence of S-waves in certain areas indicates that the outer core is liquid.
  • Refraction and Shadow Zones:
    • If the Earth were completely homogeneous, waves would travel in straight lines. Instead, they are refracted (bent) as their direction and velocity alter when entering materials of different densities.
    • Shadow Zones: Areas along the Earth where no seismic waves are detected due to refraction.
    • P-wave Shadow Zone: Exists from 103o103^o to 143o143^o from the earthquake focus (origination point).
    • S-wave Shadow Zone: Exists in areas greater than 103o103^o from the earthquake focus.

Density and Chemical Composition

  • Bulk Earth Density: Based on the Earth's travel through space, the average density is determined to be 5.52g/cm35.52\,\text{g/cm}^3.
  • Crustal Density: Rocks analyzed at the surface typically have densities between 2.5g/cm32.5\,\text{g/cm}^3 and 3g/cm33\,\text{g/cm}^3.
  • Core Density: Because the surface density is lower than the average, the interior must be denser. The core region is estimated to have a density of 9g/cm39\,\text{g/cm}^3 to 13g/cm313\,\text{g/cm}^3.
  • Chemical Makeup of the Bulk Earth:
    • Iron (FeFe): 32%\sim 32\%
    • Oxygen (OO): 30%\sim 30\%
    • Silicon (SiSi): 16%\sim 16\%
    • Magnesium (MgMg): 15%15\%
  • Chemical Makeup of the Surface (Crust):
    • Oxygen (OO): 47%\sim 47\%
    • Silicon (SiSi): 28%\sim 28\%
    • Aluminum (AlAl): 8%\sim 8\%
    • Lesser amounts of Iron (FeFe), Calcium (CaCa), Sodium (NaNa), Potassium (KK), and Magnesium (MgMg).
  • Silicates: Minerals composed of silicon and oxygen; these are the most important minerals in the crust.
  • Iron Distribution: Much of the Earth's iron has migrated to the core, which explains the major increase in density in that region compared to the crust.

Detailed Breakdown of Earth’s Layers

  • Continental Crust:
    • Density: 2.72.9g/cm3\sim 2.7 - 2.9\,\text{g/cm}^3
    • Thickness: 2070km\sim 20 - 70\,\text{km}
    • Composition: Felsic rocks.
  • Oceanic Crust:
    • Density: 3.0g/cm3\sim 3.0\,\text{g/cm}^3
    • Thickness: 810km\sim 8 - 10\,\text{km}
    • Composition: Mafic rocks.
  • Mantle:
    • Density: 3.45.6g/cm3\sim 3.4 - 5.6\,\text{g/cm}^3
    • Thickness: 2,885km\sim 2,885\,\text{km}
    • Composition: Ultramafic rocks.
  • Outer Core:
    • Density: 9.912.2g/cm3\sim 9.9 - 12.2\,\text{g/cm}^3
    • Thickness: 2,200km\sim 2,200\,\text{km}
    • Composition: Iron, some sulfur, nickel, oxygen, silicon.
  • Inner Core:
    • Density: 12.813.1g/cm3\sim 12.8 - 13.1\,\text{g/cm}^3
    • Thickness: 1,220km\sim 1,220\,\text{km}
    • Composition: Iron, some sulfur, and nickel.
  • Lithosphere: The outer, rigid part of the Earth, consisting of the upper mantle, oceanic crust, and continental crust.
  • Asthenosphere: Located just beneath the lithosphere; it behaves plastically and flows rather than remaining rigid.

Seismic Tomography

  • Definition: A relatively recent imaging technology used to generate detailed 3D models of the Earth’s interior.
  • CAT Scan Metaphor: Similar to medical CAT scans where X-rays rotate to create cross-sectional images, seismic tomography stacks repeated scans of seismic waves to produce a three-dimensional image.
  • Applications: Used for petroleum exploration near the surface and for imaging the planet as a whole.
  • Thermal Convection Models: Tomography models depict mantle temperature variations:
    • Blue areas: Represent cool mantle material.
    • Red areas: Represent warm mantle material.
    • Thin red areas: Represent rising plumes.

Earth’s Magnetic Field

  • Generation: Produced by electrical currents created by thermal and compositional currents moving within the liquid outer core, coupled with the Earth’s rotation.
  • Structure: Similar in shape to a large bar magnet.
  • Magnetic vs. Geographic Poles: The ends of the magnetic field are close to, but not exactly at, the geographic poles. Consequently, a compass points to magnetic north, not geographic north.
  • Protective Role: The magnetic field deflects most solar wind (hot gases called plasma). Without this protection, these damaging rays would harm life on Earth.
  • Magnetic Field Distortion: As solar wind approaches, the side of the field closest to the Sun is pushed in, while the opposite side stretches out.
  • Aurora Borealis (Northern Lights): Magnificent light displays created by solar storms causing disturbances within the magnetic field.
  • Magnetic Reversals: The field changes constantly and has undergone numerous polarity reversals in the past; the exact reasons for these are not well understood.

Paleomagnetism and Polar Wandering

  • Paleomagnetism: The study of the record of remnant magnetism preserved within certain rock types.
  • Iron-bearing Minerals: Minerals forming from lava align with Earth's magnetic field, acting as a record of the field at the time of formation.
  • Curie Point: The specific temperature above which minerals lose their magnetism. If minerals remain below this point, iron atoms "lock" into position, pointing to the magnetic pole.
  • Normal Polarity: Our current state, where the north arrow on a compass aligns closely with the geographic North Pole.
  • Apparent Polar Wander: The perceived movement of the Earth’s paleomagnetic poles relative to a fixed continent.
  • Evidence for Plate Tectonics:
    • Polar wandering curves show the migration of poles across the Earth’s surface over time.
    • Curves for different continents do not agree on magnetic pole locations for the past, but all converge on the current pole location today.
    • This disagreement provides evidence that the continents themselves have moved (drifted) while the pole remained relatively fixed.