Moments of inertia by integration

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Homework Help Overview

The problem involves calculating the moments of inertia for a mass distribution shaped like a semicircle in the xy-plane, specifically focusing on the x and y axes using polar coordinates.

Discussion Character

  • Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the integration setup for calculating moments of inertia, with some questioning the limits of integration and the correct interpretation of variables in the formulas. There is also a clarification regarding the definitions of "r" in the context of the x and y axes.

Discussion Status

The discussion is active, with participants providing insights into the correct application of formulas and addressing misunderstandings. Some have offered clarifications on the relationships between coordinates and the moments of inertia.

Contextual Notes

There is a noted confusion regarding the limits of integration and the definitions of variables used in the moment of inertia calculations. Participants are working within the constraints of the problem as stated, without additional information.

Lucy Yeats
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Homework Statement



A mass distribution in the positive x region of the xy-plane and in the shape of a semicircle of radius a, centred on the origin, has mass per unit area k. Find, using plane polar coordinates, its moments of inertia about the x and y axes.

Homework Equations





The Attempt at a Solution



I know that I=∫r^2.dm
dm=k.dA=k.r.dr.dθ in polar coordinates.
So I=k∫dθ∫r^3.dr
But I'm not sure about the limits, or how to differentiate between the moments of inertia about the x and y axes.

Any help would be brilliant.
 
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For the moment of inertia about the x-axis, the "r" in your formula for I is the y-coordinate, and not the polar distance to the origin.

Same thing for the moment of inertia about the y-axis, where "r" is the absolute value of the x-coordinate.
 
For a planar object which lies in the x − y plane, Ix = ∫ x^2dm and Iy = ∫ y^2dm and according to perpendicular axis theorem , Iz = ∫ (x^2 + y^2)dm = ∫ r^2dm is the rotational inertia around the z axis and r is the distance from the z axis.
In that case r changes from 0 to a and since the disk is semicircular , θ will change from 0 to Pi .
 
Last edited:
A.V said:
For a planar object which lies in the x − y plane, Ix = ∫ x^2dm and Iy = ∫ y^2dm

I think you mean Ix = ∫ y^2dm and Iy = ∫ x^2dm.
 
Oh, I see. I wrote rcosθ instead of r for the moment of inertia around the x axis, and rsinθ for the y axis, and got the right answers.

Thanks!
 

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