The Origin and Evolution of the Marine Environment (MSCI*112)

The Earth's Interior: Layered Structure

  • Structure and key terms

    • Lithosphere: rigid, cool, brittle outer shell including the crust and the uppermost part of the mantle; typically about 100 km thick (locally varies 5–200 km). Brittle and can be broken into tectonic plates.

    • Asthenosphere: the rest of the upper mantle beneath the lithosphere; partially molten and behaves plastically (ductile, "jello-like").

    • Mesosphere: the hotter but stronger region of the mantle due to high pressures; lies below the asthenosphere.

    • Crust (outermost shell):

    • Oceanic crust: very thin, about 5–10 km thick; basaltic rocks enriched in Fe and Mg.

    • Continental crust: thicker, typically 30–85 km thick; granitic rocks enriched in Si and Al; lighter than oceanic crust.

    • Mantle: extends from beneath the crust down to about the outer core boundary; composition mainly peridotite; density and temperature increase with depth.

    • Core: divided into a liquid outer core and a solid inner core; composition dominated by Fe and Ni.

  • Boundaries and terminology

    • Moho discontinuity: boundary between crust and mantle; identified in 1909 by Andrija Mohorovičić. Oceanic crust thickness ~5–10 km; Continental crust thickness ~30–85 km.

    • Core–Mantle Boundary (CMB): also called the Gutenberg discontinuity; depth to ~2891 km; boundary between the mantle and the liquid outer core; discovery linked to Beno Gutenberg in 1914.

    • Peridotite: the mantle rock type rich in Fe and Mg and low in Al and Si.

    • Mantle convection: movement in the mantle expressed at the surface as tectonic plate motion.

  • Layered structure summary (depth ranges and composition)

    • Crust: 0–30/85 km depending on oceanic vs continental; oceanic crust thinner, continental crust thicker.

    • Upper mantle (part of the lithosphere): solid rock; part of the rigid shell with the crust.

    • Lower mantle: extends down to ~2890 km.

    • Outer core: liquid metal; depth ~2891–5150 km.

    • Inner core: solid metal; depth ~5150–6371 km.

  • Seismic interpretation of the interior

    • Seismic waves reveal internal structure; convection and boundaries inferred from wave behavior.

    • Tomographic images show hot (high-velocity anomalies) and cool (low-velocity anomalies) regions in the mantle, e.g., superplumes beneath Africa and descending remnants of subducted slabs under North America.

  • Lithosphere vs. asthenosphere (physical properties)

    • Lithosphere: cool, rigid, brittle; behaves elastically; ~100 km thickness but varies.

    • Asthenosphere: hot, weak, plastic; partially melted; ductile.

    • Mesosphere: hot but stronger due to increased pressure.

  • Earth’s interior temperatures (geotherm)

    • Temperature generally rises with depth; typical gradient: rac{dT}{dz} \,\approx\, 20\text{--}40\ \frac{^ ext{°C}}{\text{km}}

    • Base of the lithosphere: T \approx 1200\text{--}1400\ ^{\circ}\text{C}

    • Core temperatures: T_{\text{core}} \approx 3000\text{--}6000\ ^{\circ}\text{C}

  • Radius and scale example from the slides

    • Radius of the Earth: R_{\oplus} \approx 6400\ \text{km}

    • Largest surface height difference: about \Delta h = 20\ \text{km} (9 km up to highest mountain + 11 km down to deepest ocean).

  • Take-away from the scale exercise (Question 2 on the slides)

    • If the Earth is shrunk proportionally to a golf-ball size with radius R' = 20\ \text{mm} starting from R = 6400\text{km}, the largest surface height difference becomes:

    • Scale factor: s = \dfrac{R'}{R} = \dfrac{20\ \text{mm}}{6400\ \text{km}} = \dfrac{0.02\ \text{m}}{6.4\times 10^{6}\ \text{m}} = 3.125\times 10^{-9}

    • Scaled height difference: \Delta h' = \Delta h \times s = (2.0\times 10^{4}\ \text{m}) \times (3.125\times 10^{-9}) \approx 6.25\times 10^{-5}\ \text{m} = 0.0625\ \text{mm}

  • The Earth’s magnetic field and the geodynamo

    • Core composition drives the geodynamo; field lines in the mantle resemble a dipole at the core–mantle boundary but are entangled due to convective motions in the core.

    • Magnetic field lines plotted in 3D show complexities caused by fluid motions in the outer core.

    • Reversals: the Earth’s magnetic field reverses on timescales of a few 10^4 to 10^6 years (occurs irregularly).

  • Seismic waves: types and behavior

    • Types of seismic waves:

    • P-waves (primary, compressional): propagate in solids, liquids, and gases; particle motion parallel to the direction of travel; faster speeds.

    • S-waves (secondary, shear): propagate only through solids; particle motion perpendicular to the direction of travel; slower than P-waves; cannot travel through the liquid outer core.

    • Rayleigh waves (surface): retrograde elliptical motion; involve both vertical and horizontal components.

    • Love waves (surface): horizontal shear waves; slower propagation than P-waves but can cause significant surface shaking.

    • Wave paths and boundaries

    • P and S waves are reflected and refracted at boundaries such as the Moho and the CMB.

    • Shadow zones exist because S-waves do not travel through the liquid outer core, creating S-wave shadows, and P-waves refract at the mantle–core boundary creating P-wave shadow zones.

    • Practical seismology: seismographs record arrival times of different wave types; relative arrivals help determine depths to interfaces and the properties of interior layers.

  • Isostasy: floating crust and compensation of topography

    • Physical idea: the crust floats on a viscous mantle. Archimedes principle governs the buoyant force: Fb = \rho{\text{fluid}} g V_{\text{displaced}}

    • The crust adjusts its height to restore isostatic equilibrium when mass distribution changes (isostatic adjustment).

    • Models of isostasy

    • Airy model: thicker crust corresponds to higher topography, compensated by a deeper, denser crustal root.

    • Pratt model: topography compensated by lateral variations in crustal density rather than thickness.

    • Evidence: gravity measurements (plumb bob analogy) show mass deficiencies beneath mountainous regions, supporting isostasy.

    • Isostatic adjustment scenarios

    • Ice-sheet growth: crust is depressed under the load; after melting, rebound (isostatic uplift) occurs over thousands of years.

    • The Himalayas, large river deltas, and parts of northern North America show ongoing isostatic adjustments.

    • Ice-sheet history example

    • Canada was covered by an ice sheet ~3–5 km thick about 20,000 years ago; melting completed ~7,000 years ago. The crust responds with uplift (isostatic rebound) after unloading; rebound continues long after the ice has melted.

    • Practical timeline (illustrative):

    • TIME 1: Ice load forms and thickens.

    • TIME 2: Crust bends downward to provide buoyant support.

    • TIME 3: Ice melts and warming begins.

    • TIME 4: Crust rebounds toward pre-ice elevations; raised beaches form due to uplift.

  • Quick practice questions (from the slides)

    • Question 3: Which layer has the largest thickness within the Earth? Answer: Mantle.

    • Question 4: Which layer has the largest volume within the Earth? Answer: Mantle.

    • Question 5: The speed of seismic waves beneath Hawaii is lower than beneath the continental US. The most plausible cause is

    • Answer: A. Hawaii is a volcanic island underlain by hot molten rocks. (Lower wave speeds indicate hotter rocks.)

    • Question 6: Isostatic response of crust beneath Canada after melting an ~3–5 km thick ice sheet ~20,000 years ago? Answer: A. The crust rises first and sinks subsequently (initial rebound followed by continued adjustments).

    • Question 7: Himalayan crust vs Appalachian crust thickness. Correct statement: B. Crust is thicker underneath the Himalaya.

  • Take-home takeaways

    • Earth consists of multiple concentric layers: crust, mantle, outer core, inner core.

    • Oceanic crust is thin (~5–10 km); continental crust is thicker (~30–85 km).

    • The mantle extends from beneath the crust to the outer core; the upper mantle includes the asthenosphere, which is ductile and partially molten.

    • The outer core is liquid; the inner core is solid; the geodynamo arising from core convection generates Earth’s magnetic field.

    • Seismic P- and S-waves reveal interior structure; P-waves can travel through solids and liquids, S-waves only through solids; their behavior explains shadow zones and boundary depths.

    • Isostasy explains the relationship between surface topography and subsurface density structure; crust thickening increases elevation, while thick roots balance massif topography in the Airy model, and density variation balances topography in the Pratt model.

    • Temperature and geotherm control material properties and phase states inside Earth; gradients indicate hotter, weaker regions at depth and solid/liquid state transitions at boundaries.

  • Key numerical references and boundaries (for quick recall)

    • Oceanic crust thickness: 5$-$10\ \text{km}

    • Continental crust thickness: 30$-$85\ \text{km}

    • Moho depth (crust–mantle boundary): oceanic ~5$-$10\ \text{km}; continental ~30$-$85\ \text{km}

    • Core–Mantle Boundary (Gutenberg discontinuity) depth: \approx 2891\ \text{km}

    • Outer core: 2891\ \text{km} \le r \le 5150\ \text{km} (liquid)

    • Inner core: 5150\ \text{km} \le r \le 6371\ \text{km} (solid)

    • Geotherm gradient: \dfrac{dT}{dz} \approx 20\text{--}40\ \frac{^{\circ}\text{C}}{\text{km}}

    • Base of lithosphere temperature: T \approx 1200\text{--}1400\ ^{\circ}\text{C}

    • Core temperatures: T \approx 3000\text{--}6000\ ^{\circ}\text{C}

    • Scale example for Earth shrinking to golf-ball size: scale factor s = \dfrac{R'}{R} = \dfrac{20\ \text{mm}}{6400\ \text{km}} = 3.125\times 10^{-9} and scaled surface relief \Delta h' = \Delta h \times s = (2.0\times 10^{4}\ \text{m}) \times (3.125\times 10^{-9}) \approx 6.25\times 10^{-5}\ \text{m} = 0.0625\ \text{mm}

  • Connections to broader concepts

    • Plate tectonics and mantle convection explain continental drift, mountain building, ocean basin formation, and seismic activity.

    • The geodynamo links deep Earth processes to the observable magnetic field, affecting navigation and shielding from cosmic radiation.

    • Isostasy links surface processes (glaciation, sedimentation) to subsurface density and crustal architecture, explaining long-term topographic evolution.

  • Real-world relevance and implications

    • Seismic studies inform earthquake hazard assessment and the depths of faults.

    • Understanding the geotherm helps model magma generation, volcanic activity, and tectonic movement.

    • Knowledge of crust thickness and mantle properties underpins resource exploration (minerals, hydrocarbons) and geothermal energy.

  • References to lecture content

    • Moho (1909) Mohorovičić; Gutenberg (1914) core–mantle boundary; Lehmann (1936) inner core discovery.

    • Mantle tomography and geophysical cross-sections show heterogeneity in the mantle with hot plumes and subducted slabs.

    • Isostasy evidenced by gravity measurements and the need for a buoyant crust–mantle system to balance topography.

  • Glossary of terms to remember

    • Lithosphere, Asthenosphere, Mesosphere, Moho, Gutenberg discontinuity, Peridotite, Geodynamo, P-waves, S-waves, Rayleigh waves, Love waves, Isostasy, Airy model, Pratt model, Tomography

Take-Home Messages (concise)

  • Earth’s interior is layered: crust, mantle, outer core (liquid), inner core (solid).

  • Oceanic crust is thinner and basaltic; continental crust is thicker and granitic.

  • The lithosphere is rigid; the asthenosphere is ductile; mantle convection drives plate tectonics.

  • The outer core is liquid and generates Earth’s magnetic field via the geodynamo; the inner core is solid.

  • Seismic waves (P and S) reveal interior structure; S-waves do not traverse the liquid outer core, leading to shadow zones.

  • Isostasy explains topography through buoyancy: Airy (thickness-based) and Pratt (density-based) models; crust adjusts height after loading/unloading (e.g., ice sheets).

  • Global temperature increases with depth (geotherm): typical gradient ~dT/dz \approx 20\text{--}40\ \dfrac{\circ C}{\text{km}}; base of lithosphere ~1200\text{--}1400\ \circ C; core ~3000\text{--}6000\ \circ C.

Practice and quick review questions

  • Which layer has the largest thickness and largest volume within the Earth? Mantle.

  • Why do Hawaii and the continental US have different seismic velocities beneath them? Hotter mantle beneath Hawaii due to volcanic activity lowers wave speeds.

  • What is the fate of the crust after melting an ice sheet? Initial rebound (uplift) followed by continued isostatic adjustment.

  • Where is crust thicker, Himalaya or Appalachian region? Himalaya (thicker crust).

Quick references to the figures and boundaries mentioned in the slides

  • Moho discontinuity: crust–mantle boundary; oceanic crust ~5–10 km, continental ~30–85 km.

  • Core–Mantle Boundary (Gutenberg): boundary at ~2891 km depth; outer core is liquid; inner core is solid.

  • Mantle structure: upper mantle + lithosphere vs. asthenosphere; tomographic images show hot plumes and cool slabs.

  • Seismic wave behavior: P-waves and S-waves; shadow zones due to core properties; seismic data collected by seismographs.