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What is the magnitude of the free-fall acceleration of a ball (mass \(m\) ) due to the Earth's gravity at an altitude of \(2 R\), where \(R\) is the radius of the Earth?

Short Answer

Expert verified
Answer: The magnitude of the free-fall acceleration is given by the expression \(a = G\frac{M}{(3R)^2}\), where \(G\) is the gravitational constant, \(M\) is the mass of the Earth, and \(R\) is the radius of the Earth.

Step by step solution

01

Gravitational force formula

We start by recalling the formula for the force between two objects due to gravity: \(F = G\frac{Mm}{r^2}\) where \(F\) is the gravitational force, \(G\) is the gravitational constant, \(M\) is the mass of the Earth, \(m\) is the mass of the ball, and \(r\) is the distance between the centers of the two objects. In this case, the distance \(r\) is equal to the sum of the Earth's radius and the altitude of the ball, so \(r = R + 2R = 3R\). We can now rewrite the formula as: \(F = G\frac{Mm}{(3R)^2}\)
02

Equate gravitational force to mass times acceleration

The gravitational force acting on the ball is also equal to its mass times its free-fall acceleration, which we'll denote as \(a\). So we can write: \(F = ma\)
03

Solve for acceleration

Now we can equate the expressions from steps 1 and 2, and solve for the acceleration: \(ma = G\frac{Mm}{(3R)^2}\) Divide both sides by the mass of the ball, \(m\): \(a = G\frac{M}{(3R)^2}\) That's the expression for the magnitude of the free-fall acceleration of the ball at an altitude of \(2R\).

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Key Concepts

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

Gravitational Force
Gravitational force is the attraction between two objects with mass. This force keeps planets in orbit and governs how objects fall on earth. Newton's law of universal gravitation quantifies this force. It says that any two objects attract each other with a force that is proportional to the product of their masses. This force is also inversely proportional to the square of the distance between their centers. The formula is \( F = G\frac{Mm}{r^2} \):
  • \( F \) stands for gravitational force.
  • \( G \) is the gravitational constant, a number that tells us about the strength of gravity. It's about \( 6.674 \times 10^{-11} \, \text{Nm}^2/\text{kg}^2 \).
  • \( M \) and \( m \) are the masses of the objects.
  • \( r \) is the distance between the centers of the two masses.
As the distance increases, the gravitational force becomes weaker. Thus, if you double the distance, the gravitational force is reduced to a quarter of the original strength.
Free-Fall Acceleration
Free-fall acceleration is the acceleration of an object caused solely by gravity. On Earth, this acceleration is denoted by \( g \) and is approximately \( 9.81 \, \text{m/s}^2 \) at the surface. When an object is in free-fall, it seems weightless because gravity is the only force acting on it. For an object at altitude, like the ball in the problem, the free-fall acceleration changes due to the increased distance to the center of the Earth.In the exercise, we found the expression for free-fall acceleration at an altitude of \( 2R \):
  • At that distance, the acceleration \( a \) is \( G\frac{M}{(3R)^2} \).
  • This formula helps us understand that acceleration reduces as we go further from the Earth's surface.
By plugging in the values for \( G \) and the Earth's mass \( M \), and calculating, you can find the acceleration value in \( \text{m/s}^2 \). This shows how gravity's pull becomes weaker with height.
Altitude
Altitude refers to the height above the Earth's surface. In the context of this exercise, altitude impacts how strongly gravity pulls on an object. Here's why altitude matters:
  • The gravitational force decreases with increased altitude.
  • Higher altitudes mean a larger distance \( r \) in the force equation \( F = G\frac{Mm}{r^2} \).
  • If you are closer to the Earth's surface, gravity's pull is stronger.
  • At \( 2R \) above Earth's surface where our ball is, the free-fall acceleration is not the same as \( g \).
Understanding altitude's impact on gravity helps in many areas like space travel, engineering, and even enjoying a day on a mountaintop. Altitude changes how forces interact, affecting how objects move and experience gravity.

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Most popular questions from this chapter

Satellites in low orbit around the Earth lose energy from colliding with the gases of the upper atmosphere, causing them to slowly spiral inward. What happens to their kinetic energy as they fall inward?

An asteroid is discovered to have a tiny moon that orbits it in a circular path at a distance of \(100 . \mathrm{km}\) and with a period of \(40.0 \mathrm{~h}\). The asteroid is roughly spherical (unusual for such a small body) with a radius of \(20.0 \mathrm{~km} .\) a) Find the acceleration of gravity at the surface of the asteroid. b) Find the escape velocity from the asteroid.

A space shuttle is initially in a circular orbit at a radius of \(r=6.60 \cdot 10^{6} \mathrm{~m}\) from the center of the Earth. A retrorocket is fired forward, reducing the total energy of the space shuttle by \(10 \%\) (that is, increasing the magnitude of the negative total energy by \(10 \%\) ), and the space shuttle moves to a new circular orbit with a radius that is smaller than \(r\). Find the speed of the space shuttle (a) before and (b) after the retrorocket is fired.

Can the expression for gravitational potential energy \(U_{\mathrm{g}}(y)=m g y\) be used to analyze high-altitude motion? Why or why not?

Careful measurements of local variations in the acceleration due to gravity can reveal the locations of oil deposits. Assume that the Earth is a uniform sphere of radius \(6370 \mathrm{~km}\) and density \(5500 . \mathrm{kg} / \mathrm{m}^{3},\) except that there is a spherical region of radius \(1.00 \mathrm{~km}\) and density \(900 . \mathrm{kg} / \mathrm{m}^{3}\) whose center is at a depth of \(2.00 \mathrm{~km} .\) Suppose you are standing on the surface of the Earth directly above the anomaly with an instrument capable of measuring the acceleration due to gravity with great precision. What is the ratio of the acceleration due to gravity that you measure compared to what you would have measured had the density been \(5500 . \mathrm{kg} / \mathrm{m}^{3}\) everywhere? (Hint: Think of this as a superposition problem involving two uniform spherical masses, one with a negative density.)

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