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Ch 14: Periodic Motion
Chapter 14, Problem 13

A thin, uniform rod has length L and mass M. A small uniform sphere of mass m is placed a distance x from one end of the rod, along the axis of the rod (Fig. E13.34)Diagram showing a rod of mass M and length L with a sphere of mass m at distance x from one end.
. (b) Use Fx = -dU>dx to find the magnitude and direction of the gravitational force exerted on the sphere by the rod (see Section 7.4). Show that your answer reduces to the expected result when x is much larger than L.

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1. Consider a small element of the rod of length dx at a distance x from the end of the rod. The mass of this small element is dM = (M/L)dx.
2. The gravitational force dF between this small element and the sphere of mass m is given by Newton's law of gravitation: dF = G * (dM * m) / (x + d)^2.
3. Substitute dM = (M/L)dx into the expression for dF: dF = G * (M/L) * m * dx / (x + d)^2.
4. Integrate this expression over the length of the rod from x = 0 to x = L to find the total gravitational force F: F = ∫[0 to L] G * (M/L) * m * dx / (x + d)^2.
5. Evaluate the integral to find the total gravitational force F. Then, analyze the result to show that when d is much larger than L, the force reduces to the expected result of F = G * (M * m) / d^2.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Gravitational Force

Gravitational force is the attractive force between two masses, described by Newton's law of universal gravitation. It states that the force is proportional to the product of the two masses and inversely proportional to the square of the distance between their centers. In this scenario, the gravitational force exerted by the rod on the sphere must be calculated by integrating the contributions from each infinitesimal mass element of the rod.
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Potential Energy (U)

Potential energy in the context of gravitational interactions is the energy stored due to the position of an object in a gravitational field. It can be expressed as U = -G(m1*m2)/r, where G is the gravitational constant, m1 and m2 are the masses, and r is the distance between them. The change in potential energy with respect to position is crucial for determining the force acting on the sphere, as the gravitational force can be derived from the negative gradient of the potential energy.
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Differentiation and Force Calculation

The relationship between force and potential energy is given by the equation Fx = -dU/dx, which states that the force is the negative derivative of potential energy with respect to position. This means that to find the gravitational force acting on the sphere, one must differentiate the potential energy function with respect to the distance x. This approach allows for the calculation of the force at any position, including the limit where x is much larger than L, simplifying the analysis.
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Related Practice
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Textbook Question
A uniform, spherical, 1000.0-kg shell has a radius of 5.00 m. (b) Sketch a qualitative graph of the magnitude of the gravitational force this sphere exerts on a point mass m as a function of the distance r of m from the center of the sphere. Include the region from r = 0 to r -> ∞.
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