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Assume that the continental crust and lithosphere have been stretched by a factor \(\alpha=2\). Taking \(h_{c c}=35 \mathrm{~km}, y_{L 0}=125 \mathrm{~km}, \rho_{m}=3300\) \(\begin{array}{lllll}\mathrm{kg} \mathrm{m}^{-3}, & \rho_{c c}=2750 & \mathrm{~kg} \mathrm{~m}^{-3}, & \rho_{s}=2550 & \mathrm{~kg} \mathrm{~m}^{-3}\end{array}\) \(\alpha_{v}=3 \times 10^{-5} \mathrm{~K}^{-1}\), and \(T_{1}-T_{0}=1300 \mathrm{~K},\) deter- mine the depth of the sedimentary basin. What is the depth of the sedimentary basin when the thermal lithosphere has thickened to its original thickness?

Short Answer

Expert verified
The sedimentary basin depth is approximately 12.83 km.

Step by step solution

01

Calculate Initial Thermal Lithosphere Thickness

To calculate the thermal lithosphere thickness before stretching, use the formula \( y_{L} = \frac{y_{L0}}{\alpha} \). Here, \( y_{L0} = 125\, \text{km} \) and \( \alpha = 2 \). Thus, \( y_L = \frac{125}{2} = 62.5\, \text{km} \).
02

Determine Initial Crustal Thickness After Stretching

The continental crust thickness after stretching by a factor of \( \alpha \) can be calculated using \( h_c = \frac{h_{cc}}{\alpha} \). Given \( h_{cc} = 35\, \text{km} \), so, \( h_c = \frac{35}{2} = 17.5\, \text{km} \).
03

Calculate the Subsidence Due to Density Differences

Using the formula for sedimentary basin depth, \( D = (\rho_{m} - \rho_{c c})\,(h_{c c} - h_c) / (\rho_{m} - \rho_{s}) \), substitute the values: \( \rho_{m} = 3300\, \text{kg/m}^{3} \), \( \rho_{cc} = 2750\, \text{kg/m}^{3} \), \( \rho_{s} = 2550\, \text{kg/m}^{3} \), \( h_{c c} = 35\, \text{km} \), \( h_c = 17.5\, \text{km} \). \[ D = \frac{(3300 - 2750) \times (35 - 17.5)}{3300 - 2550} = \frac{550 \times 17.5}{750} = \frac{9625}{750} \approx 12.83\, \text{km} \]
04

Consider Thermal Lithosphere Expansion

Calculate the change in lithosphere due to thermal expansion using \( \Delta_y = \alpha_v (T_1 - T_0) y_L \), where \( \alpha_v = 3 \times 10^{-5}\, \text{K}^{-1} \), \( T_1 - T_0 = 1300\, \text{K} \), and \( y_L = 62.5\, \text{km} \). \[ \Delta_y = 3 \times 10^{-5} \times 1300 \times 62.5 = 2.4375\, \text{km} \].
05

Determine Total Lithosphere Thickness

The total thickness after thermal expansion is calculated as: \[ y_{LTotal} = y_L + \Delta_y = 62.5\, \text{km} + 2.4375\, \text{km} = 64.9375\, \text{km} \]
06

Recalculate Sedimentary Basin Depth

If the thermal lithosphere returns to its original thickness, the sedimentary basin depth will again be \( h_{s0} \), or 0, as no stretching occurred. Otherwise, with stretching, re-calculate as in Step 3. Here, continue assuming the aforementioned expansions.

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Key Concepts

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

Continental Crust Stretching
Stretching of the continental crust is a fascinating geodynamic process that plays a key role in forming sedimentary basins. When the crust is stretched by a factor, often denoted as \( \alpha \), it leads to thinning of the crust. In our example, with \( \alpha = 2 \), the original crust thickness \( h_{cc} \) of 35 km is halved, resulting in a new thickness \( h_c \) of 17.5 km.
This process is crucial as it results in extended areas where sediment can accumulate, shaping the topography significantly.
  • The amount of stretching determines the amount of thinning.
  • Stretched regions are prone to subsidences, leading to basin formation.
  • This mechanism is a primary driver for subsidence and subsequent sedimentation.
Understanding the factors involved in crustal stretching helps geologists predict geological formations and natural resource deposits.
Thermal Lithosphere Thickness
The lithosphere, comprising the crust and the upper part of the mantle, changes thickness due to temperature variations. Initially, its thickness can be calculated by adjusting for stretching using the formula \( y_{L} = \frac{y_{L0}}{\alpha} \). In this context, before stretching, with \( y_{L0} = 125 \) km and \( \alpha = 2 \), its thickness becomes 62.5 km.
Thermal lithosphere thickness is important because:
  • It influences the mechanical behavior of the crust.
  • Thicker lithospheres are typically more rigid, impacting tectonic activity.
  • The thickness affects heat flow and, consequently, the surface heat gradient.
In scenarios where the lithosphere thickness returns to its original value, it indicates the absence of thermal or mechanical changes.
Density Differences in Lithosphere
Density variations within the lithosphere mainly result from compositional differences between its layers. The mantle \( \rho_m \) is usually denser than the continental crust \( \rho_{cc} \) or sediments \( \rho_{s} \). This density contrast creates differential buoyancy, which leads to subsidence or uplift. In our example, these values are \( 3300 \), \( 2750 \), and \( 2550 \) kg/m³, respectively.
The differences in density are fundamentally responsible for the formation of sedimentary basins, aiding in:
  • Increasing the potential for oil and gas reserves.
  • Enhancing the understanding of basin dynamics.
  • Providing critical insights into past geological transformations.
Calculating the subsidence depths with these densities allows for predictions of basin evolutions over geological timescales.
Thermal Expansion in Geodynamics
Thermal expansion is a critical concept in geodynamics, describing how materials expand when heated. In the lithosphere, this entails the change in thickness due to temperature changes. Using the thermal expansion coefficient \( \alpha_v = 3 \times 10^{-5} \) K⁻¹, along with a temperature differential \( T_1 - T_0 = 1300 \) K, the change in lithospheric thickness can be calculated. For instance, with a pre-stretch thickness \( y_L = 62.5 \) km, thermal expansion adds an additional 2.4375 km.
This phenomenon impacts:
  • The stress distribution within tectonic plates.
  • Temperature-induced deformational processes.
  • Long-term stability of the crust during temperature fluctuations.
Recognizing thermal expansion's influence is key to understanding past and present geodynamic behavior.

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Most popular questions from this chapter

The exponential depth dependence of heat production is preferred because it is self-preserving upon erosion. However, many alternative models can be prescribed. Consider a two-layer model with \(H=\) \(H_{1}\) and \(k=k_{1}\) for \(0 \leq y \leq h_{1},\) and \(H=H_{2}\) and \(k=k_{2}\) for \(h_{1} \leq y \leq h_{2} .\) For \(y>h_{2}, H=0\) and the upward heat flux is \(q_{m} .\) Determine the surface heat flow and temperature at \(y=h_{2}\) for \(\rho_{1}=2600 \mathrm{~kg} \mathrm{~m}^{-3}\), \(\rho_{2}=3000 \mathrm{~kg} \mathrm{~m}^{-3}, k_{1}=k_{2}=2.4 \mathrm{~W} \mathrm{~m}^{-1} \mathrm{~K}^{-1}\) \(h_{1}=8 \mathrm{~km}, h_{2}=40 \mathrm{~km}, \rho_{1} H_{1}=2 \mu W \mathrm{~m}^{-3}, \rho_{2} H_{2}=\) \(0.36 \mu W \mathrm{~m}^{-3}, T_{0}=0^{\circ} \mathrm{C},\) and \(q_{m}=28 \mathrm{~mW} \mathrm{~m}^{-2}\).

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 \(r=b\).

Suppose that upon entering the Earth's atmosphere, the surface of a meteorite has been heated to the melting point and the molten material is carried away by the flow. It is of interest to calculate the rate at which melting removes material from the meteorite. For this purpose, consider the following problem. The surface of a semi-infinite half-space moves downward into the half-space with constant velocity \(V\), as indicated in Figure \(4.39 .\) The surface is always at the melting temperature \(T_{m},\) and melted material above the instantaneous surface is removed from the problem. Assume that the surface of the half-space is melted by a constant heat flux \(q_{m}\) into the half-space from above the surface. Assume also that far from the melting surface the temperature is \(T_{0}\); that is, \(T \rightarrow T_{0}\) as \(\zeta \rightarrow \infty\). Find the temperature distribution in the half-space as a function of time \(T(\zeta, t),\) and determine \(V\) in terms of \(q_{m}\) and the thermodynamic properties of the rock. Account for the latent heat \(L\) required to melt the material.

Assume that the continental lithosphere satisfies the half-space cooling model. If a continental region has an age of \(1.5 \times 10^{9}\) years, how much subsidence would have been expected to occur in the last 300 Ma? Take \(\rho_{m}=3300 \mathrm{~kg} \mathrm{~m}^{-3}, \kappa=1 \mathrm{~mm}^{2} \mathrm{~s}^{-1}\), \(T_{m}-T_{0}=1300 \mathrm{~K},\) and \(\alpha_{v}=3 \times 10^{-5} \mathrm{~K}^{-1}\). Assume that the subsiding lithosphere is being covered to sea level with sediments of density \(\rho_{s}=2500 \mathrm{~kg} \mathrm{~m}^{-3}\).

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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