Parallel-axis theorem
from class:
College Physics II – Mechanics, Sound, Oscillations, and Waves
Definition
The parallel-axis theorem allows the calculation of a body's moment of inertia about any axis, given its moment of inertia about a parallel axis through the object's center of mass and the perpendicular distance between the axes. It is expressed as $I = I_{\text{cm}} + Md^2$, where $I$ is the moment of inertia about the new axis, $I_{\text{cm}}$ is the moment of inertia about the center-of-mass axis, $M$ is the mass of the body, and $d$ is the distance between the two axes.
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5 Must Know Facts For Your Next Test
- The parallel-axis theorem applies to rigid bodies and aids in calculating moments of inertia for different rotational axes.
- The formula for the theorem is $I = I_{\text{cm}} + Md^2$. The terms represent: $I$ (moment of inertia about a new axis), $I_{\text{cm}}$ (moment of inertia about center-of-mass axis), $M$ (mass), and $d$ (distance between axes).
- This theorem simplifies finding moments of inertia without directly integrating over a new rotational axis.
- It is crucial for analyzing systems with shifted rotational points like pendulums or rotating machinery components.
- Understanding this concept requires familiarity with basic moments of inertia for standard shapes such as rods, discs, and spheres.
Review Questions
- What does each term represent in the equation $I = I_{\text{cm}} + Md^2$?
- How would you use the parallel-axis theorem to find the moment of inertia for a rod rotated around one end?
- Why is it important to know both the center-of-mass moment of inertia and the distance between axes in using this theorem?
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