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17. Periodic Motion
Simple Harmonic Motion of Pendulums
8:49 minutes
Problem 14.85
Textbook Question
Textbook QuestionA “seconds” pendulum has a period of exactly 2.000 s. That is, each one-way swing takes 1.000 s. What is the length of a seconds pendulum in Austin, Texas, where g = 9.793 m /s² ? If the pendulum is moved to Paris, where g = 9.809 m/s², by how many millimeters must we lengthen the pendulum? What is the length of a seconds pendulum on the Moon, where g = 1.62 m/s² ?
Verified step by step guidance
1
Determine the length of the pendulum in Austin using the formula for the period of a simple pendulum, T = 2\pi \sqrt{\frac{L}{g}}, where T is the period, L is the length of the pendulum, and g is the acceleration due to gravity. Rearrange the formula to solve for L: L = \frac{gT^2}{4\pi^2}.
Calculate the change in length required when the pendulum is moved to Paris. First, find the new length using the same formula, substituting the value of g in Paris. Then, subtract the original length (from Austin) from this new length to find the difference.
Convert the difference in length from step 2 from meters to millimeters by multiplying by 1000, since 1 meter equals 1000 millimeters.
Determine the length of the pendulum on the Moon using the same formula for L, substituting the value of g on the Moon.
Summarize the findings: the length of the pendulum in Austin, the additional length needed in Paris, and the length of the pendulum on the Moon.
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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Pendulum Motion
A pendulum is a weight suspended from a pivot that swings back and forth under the influence of gravity. The period of a pendulum, which is the time it takes to complete one full swing, depends on its length and the acceleration due to gravity. The formula for the period (T) of a simple pendulum is T = 2π√(L/g), where L is the length of the pendulum and g is the acceleration due to gravity.
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Acceleration due to Gravity (g)
The acceleration due to gravity (g) is the rate at which an object accelerates towards the Earth (or another celestial body) due to gravitational force. It varies slightly depending on location due to factors like altitude and the Earth's shape. For example, g is approximately 9.81 m/s² at sea level on Earth, but it can be different in other locations, such as Austin (9.793 m/s²) and Paris (9.809 m/s²).
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Length Adjustment for Pendulum
When a pendulum is moved to a location with a different gravitational acceleration, its length must be adjusted to maintain the same period. This is because the period is directly related to the square root of the length divided by g. By calculating the new length using the period formula for the new g, one can determine how much longer or shorter the pendulum needs to be, often expressed in millimeters for precision.
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