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The mantle rocks of the asthenosphere from which the lithosphere forms are expected to contain a small amount of magma. If the mass fraction of magma is 0.05 , determine the depth of the lithosphere-asthenosphere boundary for oceanic lithosphere with an age of 60 Ma. Assume \(L=400 \mathrm{~kJ}\) \(\mathrm{kg}^{-1}, c=1 \mathrm{~kJ} \mathrm{~kg}^{-1} \mathrm{~K}^{-1}, T_{m}=1600 \mathrm{~K}, T_{0}=275 \mathrm{~K},\) and \(\kappa=1 \mathrm{~mm}^{2} \mathrm{~s}^{-1}\).

Short Answer

Expert verified
The depth of the lithosphere-asthenosphere boundary is approximately 100 km.

Step by step solution

01

Understanding the Problem

We are tasked with determining the depth of the lithosphere-asthenosphere boundary. The variables given include the mass fraction of magma (0.05), latent heat \( L \), specific heat capacity \( c \), melting temperature \( T_m \), surface temperature \( T_0 \), and thermal diffusivity \( \kappa \). The lithosphere age is 60 million years (Ma).
02

Convert Age from Millions of Years to Seconds

Convert the lithosphere age from millions of years to seconds to match the units of thermal diffusivity. Since 1 Ma = \( 10^6 \) years and 1 year = approximately 31.536 million seconds, the age in seconds is:\[ t = 60 \times 10^6 \times 31.536 \times 10^6 \text{ seconds}\]
03

Apply the Diffusion Equation for Depth

The depth \( z \) of the lithosphere-asthenosphere boundary can be calculated using the diffusion equation:\[ z = 2 \sqrt{\kappa t} \]Substitute \( \kappa = 1 \times 10^{-6} \text{ m}^2/\text{s} \) and the calculated value for \( t \).
04

Calculate the Depth

Plug the values into the equation and solve: \[ z = 2 \sqrt{1 \times 10^{-6} \times 60 \times 10^6 \times 31.536 \times 10^6} \]Simplify and calculate the numerical value of \( z \).
05

Verify Considerations

Ensure that all assumptions, such as ignoring heat production in the lithosphere or frictional heating, are acceptable for this approximation of the lithosphere-asthenosphere boundary depth calculation.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Lithosphere-Asthenosphere Boundary
The lithosphere-asthenosphere boundary (LAB) is the zone separating the rigid, cooling lithosphere from the hotter, more ductile asthenosphere beneath. This boundary is not fixed but varies with factors like temperature and pressure, impacting tectonic processes. It is crucial in geodynamics as it influences the convection currents driving plate movements. In an oceanic context, where the lithosphere is thinner than its continental counterpart, the LAB can be determined by understanding the thermal evolution of the oceanic plate over time. With cooling, the lithosphere thickens. Its depth is often calculated using thermal diffusion equations to model how heat disperses through rocks.
Mantle Dynamics
Mantle dynamics refer to the movements within Earth's mantle caused by internal heat dissipation. These dynamics are characterized by convection currents, crucial for driving plate tectonics. The mantle's movement is a slow but continuous process, circulating heat from Earth's core to the crust. This circulation helps in understanding how continents drift and ocean basins expand. - Mantle convection influences the creation and subduction of lithospheric plates. - The lithosphere sits on the asthenosphere, a part of the mantle that allows it to drift. - Gravitational forces and varying temperatures affect the mantle flow, thus impacting the surface geology.
Thermal Properties of Rocks
The thermal properties of rocks involve understanding how heat is transported through and stored within Earth's materials. Key properties include: - **Thermal Conductivity**: The ability of rocks to conduct heat. Higher conductivity means heat moves more easily through the material. - **Specific Heat Capacity**: The amount of heat required to change the temperature of a rock by one degree. Rocks with high specific heat capacity can store more thermal energy. - **Thermal Diffusivity**: A measure of how quickly a rock can conduct thermal energy relative to its ability to store it. This value is crucial in calculating depth boundaries like the LAB. These properties are essential in modeling Earth's thermal structure and help explain phenomena like volcanic activity and geothermal gradients.
Oceanic Lithosphere Age
The age of the oceanic lithosphere plays a significant role in determining its properties and behavior. As the oceanic lithosphere ages, it undergoes cooling, becoming denser and thicker. Older oceanic lithosphere shows distinct characteristics compared to newer formations: - **Thermal State**: Older lithosphere is generally cooler, affecting its density and buoyancy. - **Thickness**: With age, the lithosphere thickens due to ongoing thermal contractions and sediment accumulation. - **Strength and Rigidity**: Increasing age enhances the lithosphere's mechanical strength making it more brittle. Age is a vital parameter in calculating the lithosphere-asthenosphere boundary depth, as thermal diffusion over millions of years affects the LAB's positioning.

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Most popular questions from this chapter

Derive an expression for the temperature at the center of a planet of radius \(a\) with uniform density \(\rho\) and internal heat generation \(H\). Heat transfer in the planet is by conduction only in the lithosphere, which extends from \(r=b\) to \(r=a\). For \(0 \leq r \leq b\) heat transfer is by convection, which maintains the temperature gradient \(d T / d r\) constant at the adiabatic value \(-\Gamma\). The surface temperature is \(T_{0}\). To solve for \(T(r)\), you need to assume that \(T\) and the heat flux are continuous at \(r=b\).

It is assumed that a constant density planetary body of radius \(a\) has a core of radius \(b\). There is uniform heat production in the core but no heat production outside the core. Determine the temperature at the center of the body in terms of \(a, b, k, T_{0}\) (the surface temperature), and \(q_{0}\) (the surface heat flow).

Estimate the effects of variations in bottom water temperature on measurements of oceanic heat flow by using the model of a semi-infinite half-space subjected to periodic surface temperature fluctuations. Such water temperature variations at a specific location on the ocean floor can be due to, for example, the transport of water with variable temperature past the site by deep ocean currents. Find the amplitude of water temperature variations that cause surface heat flux variations of \(40 \mathrm{~mW} \mathrm{~m}^{-2}\) above and below the mean on a time scale of 1 day. Assume that the thermal conductivity of sediments is \(0.8 \mathrm{~W} \mathrm{~m}^{-1} \mathrm{~K}^{-1}\) and the sediment thermal diffusivity is \(0.2 \mathrm{~mm}^{2} \mathrm{~s}^{-1}\).

Scientists believe that early in its evolution, the Moon was covered by a magma ocean with a depth of \(50 \mathrm{~km}\). Assuming that the magma was at its melt temperature of \(1500 \mathrm{~K}\) and that the surface of the Moon was maintained at \(500 \mathrm{~K}\), how long did it take for the magma ocean to solidify if it was cooled from the surface? Take \(L=320 \mathrm{~kJ} \mathrm{~kg}^{-1}, \kappa=1 \mathrm{~mm}^{2}\) \(\mathrm{s}^{-1}\), and \(c=1 \mathrm{~kJ} \mathrm{~kg}^{-1} \mathrm{~K}^{-1}\).

A body of water at \(0^{\circ} \mathrm{C}\) is subjected to a constant surface temperature of \(-10^{\circ} \mathrm{C}\) for 10 days. How thick is the surface layer of ice? Use \(L=320 \mathrm{~kJ}\) \(\mathrm{kg}^{-1}, k=2 \mathrm{~J} \mathrm{~m}^{-1} \mathrm{~s}^{-1} \mathrm{~K}^{-1}, c=4 \mathrm{~kJ} \mathrm{~kg}^{-1} \mathrm{~K}^{-1}, \rho=\) \(1000 \mathrm{~kg} \mathrm{~m}^{-3}\).

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