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As a first approximation, Earth's continents may be thought of as granite blocks floating in a denser rock (called peridotite) in the same way that ice floats in water. (a) Show that a formula describing this phenomenon is $$ \rho_{g} t=\rho_{p} d $$ where \(\rho_{g}\) is the density of granite \(\left(2.8 \times 10^{3} \mathrm{~kg} / \mathrm{m}^{3}\right), \rho_{p}\) is the density of peridotite \(\left(3.3 \times 10^{3} \mathrm{~kg} / \mathrm{m}^{3}\right), t\) is the thickness of a continent, and \(d\) is the depth to which a continent floats in the peridotite. (b) If a continent sinks \(5.0 \mathrm{~km}\) into the peridotite layer (this surface may be thought of as the ocean floor), what is the thickness of the continent?

Short Answer

Expert verified
The thickness of the continent is approximately 5.9 km.

Step by step solution

01

Understand and Express the Law

Firstly, we need to express the fundamental principle that underpins this exercise, which is Archimedes' principle of buoyancy: the upward force (buoyant force) that opposes the weight of an immersed object is equal to the weight of the fluid that the object displaces. Symbolically, this principle can be expressed as \( F_{up} = F_{disp} \). However, here we don't talk about forces, but about densities, which are mass divided by volume. If the volumes are the same, we can divide both forces by the common volume and get \( \rho_{obj} g = \rho_{fluid} g \), where \( \rho_{obj} \) is the density of the object (in this case, the block of granite), \( \rho_{fluid} \) is the density of the fluid (here, the peridotite), and \( g \) is the gravitational acceleration. Because the \( g \) is the same on both sides, we can ignore it. We then get: \( \rho_{obj} = \rho_{fluid} \). As the block is partially submerged, it displaces a volume of peridotite equal to the submerged volume, not the total volume of the block. So instead of equal densities, we multiply each side by appropriate distances to express volumes, and get the needed equation: \( \rho_{g} t = \rho_{p} d \), where \( \rho_{g} \) is the density of granite, \( \rho_{p} \) is the density of peridotite, \( t \) is the thickness of a continent, and \( d \) is the depth to which a continent floats in the peridotite.
02

Calculating Thickness

To calculate the thickness of the continent, we'll re-arrange the equation for \( t \): \( t = \frac{\rho_{p} d}{\rho_{g}} \). We can now substitute the given values: \( t = \frac{3.3 \times 10^{3} kg/m^{3} \times 5.0 km }{2.8 \times 10^{3} kg/m^{3}} \). The units \( kg/m^{3} \) cancel out and with the fact that \( 1 km = 1000 m \), we are left with \( t = 5.0 km \times \frac{3.3}{2.8} \)
03

Final Calculation

Calculate \( 5.0 km \times \frac{3.3}{2.8} \) using a calculator. Remember that the result will be in kilometers due to the remaining units.

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Key Concepts

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

Density of Granite
Understanding the density of granite is crucial when studying Earth's geology and the principles of buoyancy. Granite is a common type of felsic intrusive igneous rock that is granular in texture. Its density plays a significant role in how continents 'float' on the denser mantle layer below, much like icebergs float in water.

The density of granite is typically around \(2.8 \times 10^3 \text{{kg/m}}^3\). This number represents how much a cubic meter of granite weighs and is influenced by several factors including mineral composition and porosity. In the context of continental buoyancy, this lower density compared to the underlying mantle allows continents to rest on the mantle without sinking completely, akin to how a less dense material floats in a more dense fluid.
Density of Peridotite
Peridotite is a dense, coarse-grained igneous rock composed primarily of the minerals olivine and pyroxene. It is typically found in the Earth's mantle and plays a significant role in the concept of isostasy, which explains the equilibrium between Earth's crust and mantle.

The density of peridotite is about \(3.3 \times 10^3 \text{{kg/m}}^3\), making it denser than granite. This density differential is at the core of how continents can be envisioned as 'blocks' of granite floating within a 'sea' of denser peridotite. The higher density of peridotite provides a buoyant force that supports the continents above it, just as water supports less dense objects that float on its surface.
Continental Thickness Calculation
Calculating the thickness of Earth's continents involves understanding the balance of forces and densities between the continental crust (primarily granite) and the mantle (represented by peridotite in this model). When a continent is in equilibrium, the mass of the granite above the level of the peridotite is balanced by the mass of the displaced peridotite.

The equilibrium condition can be mathematically expressed as \( \rho_{g} t = \rho_{p} d \), where \( \rho_{g} \) is the density of granite, \( \rho_{p} \) is the density of peridotite, \( t \) is the thickness of the continent, and \( d \) is the depth the continent sinks into the peridotite. By re-arranging this formula to solve for \( t \), we obtain the continental thickness calculation which allows geologists and earth scientists to estimate the thickness of Earth's crust at various locations.
Buoyant Force
The buoyant force is a fundamental concept in fluid dynamics and is based on Archimedes' principle. It can be described as the upward force exerted by a fluid that opposes the weight of an object submerged in it. This force is equal to the weight of the fluid that the object displaces.

In our continental model, the peridotite exerts a buoyant force on the granite 'block' of the continent. The denser the fluid (or peridotite, in this case), the greater the buoyant force it can exert. Since granite is less dense than peridotite, it is buoyed up by this force, maintaining the 'floatation' of continents atop the mantle. Understanding the interplay between the buoyant force and the densities of both granite and peridotite is essential in explaining the concept of isostasy and the dynamic stability of continental and oceanic crust on Earth's mantle.

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Most popular questions from this chapter

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