/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 27 The earth is divided into solid ... [FREE SOLUTION] | 91Ó°ÊÓ

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The earth is divided into solid inner core, a liquid outer core, and a plastic mantle. Physical properties such as density change discontinuously at the boundaries between one layer and the next. Although the density is not completely constant within each region, we will approximate it as being so for the purposes of this problem. (We neglect the crust as well.) Let \(R\) be the radius of the earth as a whole and \(M\) its mass. The following table gives a model of some properties of the three layers, as determined by methods such as the observation of earthquake waves that have propagated from one side of the planet to the other. $$ \begin{array}{lll} \text { region } & \text { outer radius } / R & \text { mass } / M \\ \text { mantle } & 1 & 0.69 \\ \text { outer core } & 0.55 & 0.29 \\ \text { inner core } & 0.19 & 0.017 \end{array} $$ The boundary between the mantle and the outer core is referred to as the Gutenberg discontinuity. Let \(g_{s}\) be the strength of the earth's gravitational field at its surface and \(g_{G}\) its value at the Gutenberg discontinuity. Find \(g_{G} / g_{s}\)

Short Answer

Expert verified
\(g_G / g_s \approx 1.015\)

Step by step solution

01

Understand the problem

We need to find the ratio of the gravitational field strength at the Gutenberg discontinuity, denoted as \(g_G\), to the gravitational field strength at the Earth's surface, denoted as \(g_s\). The gravitational field strength \(g\) at a radius \(r\) within a spherically symmetric mass distribution is given by \(g = \frac{G M_r}{r^2}\), where \(M_r\) is the mass contained within radius \(r\) and \(G\) is the gravitational constant.
02

Calculate gravitational field at the Earth's surface

At the surface, \(r = R\), the total mass \(M\) contributes to the gravitational field. Therefore, \(g_s = \frac{G M}{R^2}\).
03

Calculate gravitational field at the Gutenberg discontinuity

The Gutenberg discontinuity is at the boundary between the mantle and the outer core, which has an outer radius of \(0.55R\). The mass contributing to gravity at this radius includes the inner core and outer core, totaling \(0.017M + 0.29M = 0.307M\). Therefore, \(g_G = \frac{G \cdot 0.307M}{(0.55R)^2}\).
04

Find the ratio \(g_G / g_s\)

Substitute the expressions for \(g_s\) and \(g_G\) into \(g_G / g_s\) to get:\[\frac{g_G}{g_s} = \frac{\frac{G \cdot 0.307M}{(0.55R)^2}}{\frac{G M}{R^2}} = \frac{0.307}{0.55^2}\].
05

Calculate the numerical value

Calculate \(0.55^2\) which equals \(0.3025\). Then compute the ratio:\[\frac{0.307}{0.3025} \approx 1.015\].

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Key Concepts

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

Gravitational Field
The gravitational field is a force field that surrounds the Earth, exerting a force on objects that have mass. This force is what keeps you grounded and gives objects weight. The strength of this field, often denoted as \( g \), depends on two main factors: the total mass of the Earth and the distance from the center of the Earth to the point where the field is measured.
The formula used to calculate the gravitational field strength at any point inside or outside the Earth is given by:
  • \( g = \frac{G M_r}{r^2} \)
Here, \( G \) is the gravitational constant, \( M_r \) is the mass within radius \( r \), and \( r \) is the distance from the center of the Earth to the point of interest.
At the Earth's surface, the gravitational field strength, \( g_s \), can be calculated using the surface radius \( R \) and total mass \( M \). This tells us exactly how strong Earth's pull is on objects at its surface, with typical values being around 9.8 m/s².
Gutenberg Discontinuity
The Gutenberg Discontinuity is a crucial boundary within the Earth's interior, located between the mantle and the outer core. Named after seismologist Beno Gutenberg, this boundary is situated at a depth where the physical properties of Earth's layers change significantly.
One notable change at the Gutenberg Discontinuity is the shift from solid to liquid in terms of state. The mantle, composed primarily of solid rock, gives way to the outer core that is liquid. This transition influences how seismic waves travel through the Earth. Seismic waves slow down as they encounter the liquid outer core due to its less rigid structure.
The gravitational field strength also experiences a change at the Gutenberg Discontinuity. Since it marks the transition between layers with different densities and mass distributions, the gravitational field at this level, \( g_G \), can be different than at the Earth's surface, \( g_s \). This boundary is essential for understanding how the Earth’s internal layers are structured and how they impact phenomena such as magnetic fields and seismic activities.
Seismic Waves
Seismic waves are vibrations that travel through the Earth's interior and surface. They are the result of energy released during an earthquake or any other significant ground-shaking event. There are two primary types of seismic waves: body waves and surface waves. Body waves include two sub-types: P-waves (primary or pressure waves) and S-waves (secondary or shear waves).
- **P-waves**: These are the fastest seismic waves and can travel through both solid and liquid layers of the Earth. They compress and expand the ground in the direction of wave propagation, similar to how sound waves move through air.
- **S-waves**: These waves travel slower than P-waves and can only move through solid materials. They move the ground perpendicular to the direction of wave travel, like waves on a string.
When seismic waves encounter the Gutenberg Discontinuity, they behave differently. P-waves slow down upon entering the less rigid, liquid outer core, while S-waves cannot pass through the liquid directly, causing them to be absent in certain regions of a seismograph, leading to shadow zones. Understanding seismic wave behavior helps scientists map the Earth's internal structure.
Mass Distribution in Earth
The Earth's mass is not evenly distributed across its layers. Instead, it varies significantly depending on the material composition and density of each layer. This distribution affects the gravitational field and how Earth's interior functions.
- **Mantle**: The mantle comprises the bulk of Earth's volume and holds about 69% of Earth's mass. It consists of silicate rocks that are in a solid yet plastic state, allowing for slow motion and flow within the layer.
- **Outer Core**: This layer contains about 29% of Earth's mass and is composed of liquid metals, primarily iron and nickel. Its fluid nature is crucial for the Earth's magnetic field generation through the process of convection and rotation.
- **Inner Core**: Although it makes up only about 1.7% of Earth's mass, the inner core is solid due to intense pressure. It is composed mainly of iron and nickel as well.
Understanding how mass is distributed helps scientists predict how the Earth's interior affects its dynamics, including the behavior of the gravitational field at different depths. Areas like the Gutenberg Discontinuity play a key role in such studies by acting as significant boundaries within this framework.

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Most popular questions from this chapter

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