FIGURE CP13.71 shows a particle of mass m at distance 𝓍 from the center of a very thin cylinder of mass M and length L. The particle is outside the cylinder, so 𝓍 > L/2 . Calculate the gravitational potential energy of these two masses.
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Gravitational Potential Energy
Problem 46a
Textbook Question
A rogue band of colonists on the moon declares war and prepares to use a catapult to launch large boulders at the earth. Assume that the boulders are launched from the point on the moon nearest the earth. For this problem you can ignore the rotation of the two bodies and the orbiting of the moon. What is the minimum speed with which a boulder must be launched to reach the earth? Hint: The minimum speed is not the escape speed. You need to analyze a three-body system.

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Step 1: Identify the key forces and energies involved in the problem. The boulder must overcome the gravitational pull of both the moon and the earth. This is a three-body system, so we need to consider the gravitational potential energy due to both the moon and the earth.
Step 2: Write the total energy equation for the boulder. The total energy consists of the kinetic energy and the gravitational potential energy. The kinetic energy is given by \( KE = \frac{1}{2}mv^2 \), and the gravitational potential energy is \( U = -\frac{GMm}{r} \), where \( G \) is the gravitational constant, \( M \) is the mass of the celestial body, \( m \) is the mass of the boulder, and \( r \) is the distance from the center of the celestial body.
Step 3: Set up the energy conservation equation. At the launch point on the moon, the boulder has an initial kinetic energy \( KE_{initial} \) and gravitational potential energy due to both the moon and the earth. At the earth's surface, the boulder will have zero velocity (minimum speed condition) and gravitational potential energy due to the earth. Write the equation: \( KE_{initial} + U_{moon} + U_{earth} = U_{earth,final} \).
Step 4: Substitute the expressions for gravitational potential energy. For the moon, \( U_{moon} = -\frac{G M_{moon} m}{R_{moon}} \), where \( M_{moon} \) is the mass of the moon and \( R_{moon} \) is the radius of the moon. For the earth, \( U_{earth} = -\frac{G M_{earth} m}{d} \), where \( M_{earth} \) is the mass of the earth and \( d \) is the distance between the moon and the earth. At the earth's surface, \( U_{earth,final} = -\frac{G M_{earth} m}{R_{earth}} \), where \( R_{earth} \) is the radius of the earth.
Step 5: Solve for the minimum initial velocity \( v \). Rearrange the energy conservation equation to isolate \( v \): \( \frac{1}{2}mv^2 = \left( -\frac{G M_{earth} m}{R_{earth}} \right) - \left( -\frac{G M_{moon} m}{R_{moon}} - \frac{G M_{earth} m}{d} \right) \). Simplify the terms and solve for \( v \). Note that the mass of the boulder \( m \) cancels out, leaving an expression for \( v \) in terms of \( G \), \( M_{moon} \), \( M_{earth} \), \( R_{moon} \), \( R_{earth} \), and \( d \).

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Gravitational Potential Energy
Gravitational potential energy is the energy an object possesses due to its position in a gravitational field. In the context of launching a boulder from the moon to the Earth, this energy is crucial as it determines how much energy is needed to overcome the gravitational pull of the moon and reach the Earth. The potential energy can be calculated using the formula U = -G(m1*m2)/r, where G is the gravitational constant, m1 and m2 are the masses of the two bodies, and r is the distance between their centers.
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Kinematics of Projectile Motion
Kinematics of projectile motion describes the motion of an object that is launched into the air and is subject to gravitational forces. In this scenario, understanding the initial velocity required for the boulder to reach Earth involves analyzing its trajectory, which is influenced by the gravitational forces of both the moon and the Earth. The equations of motion can be applied to determine the necessary launch angle and speed to ensure the boulder travels the required distance.
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Introduction to Projectile Motion
Three-Body Problem
The three-body problem refers to the challenge of predicting the motion of three celestial bodies interacting with each other through gravitational forces. In this case, the moon, Earth, and the boulder represent a three-body system. Unlike simpler two-body problems, the three-body problem does not have a general solution, making it essential to consider the gravitational influences of both the moon and Earth when calculating the minimum speed needed for the boulder to reach its target.
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