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Some of the deepest mines in the world are in South Africa and are roughly \(3.5 \mathrm{~km}\) deep. Consider the Earth to be a uniform sphere of radius \(6370 \mathrm{~km}\). a) How deep would a mine shaft have to be for the gravitational acceleration at the bottom to be reduced by a factor of 2 from its value on the Earth's surface? b) What is the percentage difference in the gravitational acceleration at the bottom of the \(3.5-\mathrm{km}\) -deep shaft relative to that at the Earth's mean radius? That is, what is the value of \(\left(a_{\text {surf }}-a_{3,5 \mathrm{~km}}\right) / a_{\text {surf }} ?\)

Short Answer

Expert verified
Answer: To find the depth at which the gravitational acceleration is reduced by half, first calculate the surface acceleration using the formula \(g_{surf} = -\frac{4}{3} \pi G \rho R\). Then, set up an equation to solve for the depth \(D\) such that \(g(R - D) = \frac{1}{2} g_{surf}\). Calculate the value of \(D\). To find the percentage difference in acceleration between the surface and a 3.5 km deep mine shaft, first calculate the gravitational acceleration at 3.5 km depth using \(g_{3.5 \text{ km}} = -\frac{4}{3} \pi G \rho (R - 3.5)\). Then, compute the percentage difference using the formula \(\frac{g_{surf} - g_{3.5 \text{ km}}}{g_{surf}}\). Express the result as a percentage.

Step by step solution

01

Gravitational Acceleration Formula

To calculate the gravitational acceleration inside a uniform sphere, we can use the formula: \(g(r) = - \frac{4}{3} \pi G \rho r\), where \(g(r)\) is the gravitational acceleration at radius \(r\), \(G\) is the gravitational constant, and \(\rho\) is the density of the Earth.
02

Find the Gravitational Acceleration at the Surface

Calculate the surface acceleration \(g_{surf}\) by using the radius of the Earth, \(R = 6370 \text{ km}\). We will also need the Earth's density \(\rho\). We can estimate \(\rho = 5500 \text{ kg/m}^3\). So, \(g_{surf} = -\frac{4}{3} \pi G \rho R\)
03

Determine the Depth for Half Gravitational Acceleration

We want to find the depth \(D\) such that the gravitational acceleration is half its surface value, i.e., \(g(R - D) = \frac{1}{2} g_{surf}\). To solve for \(D\), set up the equation as follows: \(\frac{1}{2} g_{surf} = -\frac{4}{3} \pi G \rho (R - D)\) Solve for \(D\) and calculate its value.
04

Calculate the Gravitational Acceleration at 3.5 km Depth

Next, we need to find the gravitational acceleration at the bottom of the 3.5 km deep mine shaft. Calculate \(g_{3.5 \text{ km}}\) using the formula: \(g_{3.5 \text{ km}} = -\frac{4}{3} \pi G \rho (R - 3.5)\)
05

Calculate the Percentage Difference in Gravitational Acceleration

Finally, we can calculate the percentage difference between the surface and 3.5 km depth accelerations as follows: \(\frac{a_{\text {surf }}-a_{3,5 \mathrm{~km}}}{a_{\text {surf }}} = \frac{g_{surf} - g_{3.5 \text{ km}}}{g_{surf}}\) Compute the value and express it as a percentage.

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Key Concepts

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

Uniform Sphere Model
When we talk about Earth as a uniform sphere, we mean imagining Earth as a large, perfect ball that has the same density throughout. Think of it like a solid rubber ball. When simplified this way, calculations for gravitational effects, like how gravity changes underground, become easier.
This model assumes that:
  • Earth's mass is evenly distributed.
  • There's no variation in density from the surface to the core.
  • The radius of Earth remains constant.
This simplification helps in deriving formulas. In our case, it helps estimate gravitational acceleration at different depths inside Earth based on radius and density.
Earth's Density
Density, denoted as \(\rho\), is essential for calculating gravitational acceleration. It tells us how much mass is in a certain volume. For Earth, the average density used is about \(5500 \text{ kg/m}^3\).
This value helps in determining the gravitational force felt at any point inside Earth. An even distribution is assumed in the uniform sphere model, meaning each chunk of Earth has the same density.
If you were to descend into a mine, the density remains constant, simplifying calculations based on Earth's geometry and mass.
Gravitational Constant
The gravitational constant, symbolized by \(G\), is a key figure in physics, necessary to calculate gravitational forces. Its approximate value is \(6.674 \times 10^{-11} \text{ N(m/kg)}^2\).
This constant appears in Newton's law of gravitation and is vital for understanding the gravitational attraction between masses. In our formula \(g(r) = - \frac{4}{3} \pi G \rho r\), \(G\) is used alongside density and radius, determining the gravity experienced at different Earth layers.
No matter where in the universe physics is applied, \(G\) remains a consistent value, making it foundational for both terrestrial and celestial calculations.
Depth and Gravitational Variation
As we go deeper into Earth, gravitational force changes. Interestingly, inside the Earth, gravity decreases as you go lower. Using the formula \(g(r) = -\frac{4}{3} \pi G \rho r\), gravity is calculated for a given depth based on Earth's density and radius.
For a mine shaft that reaches 3.5 km, gravity slightly reduces because less mass exists below you pulling downwards. The deeper you go, the less mass is beneath, causing a decrease in felt gravity.
The exercise specifically looks at how much gravity diminishes by half at a certain depth or changes at 3.5 km deep, spotlighting how variations aren't always apparent at a surface glance but are significant in scientific undertakings.

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Most popular questions from this chapter

You have been sent in a small spacecraft to rendezvous with a space station that is in a circular orbit of radius \(2.5000 \cdot 10^{4} \mathrm{~km}\) from the Earth's center. Due to a mishandling of units by a technician, you find yourself in the same orbit as the station but exactly halfway around the orbit from it! You do not apply forward thrust in an attempt to chase the station; that would be fatal folly. Instead, you apply a brief braking force against the direction of your motion, to put you into an elliptical orbit, whose highest point is your present position, and whose period is half that of your present orbit. Thus, you will return to your present position when the space station has come halfway around the circle to meet you. Is the minimum radius from the Earth's center-the low point \(-\) of your new elliptical orbit greater than the radius of the Earth \((6370 \mathrm{~km})\), or have you botched your last physics problem?

Newton's Law of Gravity specifies the magnitude of the interaction force between two point masses, \(m_{1}\) and \(m_{2}\), separated by a distance \(r\) as \(F(r)=G m_{1} m_{2} / r^{2} .\) The gravitational constant \(G\) can be determined by directly measuring the interaction force (gravitational attraction) between two sets of spheres by using the apparatus constructed in the late 18th century by the English scientist Henry Cavendish. This apparatus was a torsion balance consisting of a 6.00 -ft wooden rod suspended from a torsion wire, with a lead sphere having a diameter of 2.00 in and a weight of 1.61 lb attached to each end. Two 12.0 -in, 348 -lb lead balls were located near the smaller balls, about 9.00 in away, and held in place with a separate suspension system. Today's accepted value for \(G\) is \(6.674 \cdot 10^{-11} \mathrm{~m}^{3} \mathrm{~kg}^{-1} \mathrm{~s}^{-2}\) Determine the force of attraction between the larger and smaller balls that had to be measured by this balance. Compare this force to the weight of the small balls.

For two identical satellites in circular motion around the Earth, which statement is true? a) The one in the lower orbit has less total energy. b) The one in the higher orbit has more kinetic energy. c) The one in the lower orbit has more total energy. d) Both have the same total energy.

The distances from the Sun at perihelion and aphelion for Pluto are \(4410 \cdot 10^{6} \mathrm{~km}\) and \(7360 \cdot 10^{6} \mathrm{~km},\) respectively. What is the ratio of Pluto's orbital speed around the Sun at perihelion to that at aphelion?

For the satellite in Solved Problem 12.2, orbiting the Earth at a distance of \(3.75 R_{\mathrm{E}}\) with a speed of \(4.08 \mathrm{~km} / \mathrm{s}\) with what speed would the satellite hit the Earth's surface if somehow it suddenly stopped and fell to Earth? Ignore air resistance.

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