Deriving Common Moments of Inertia: Sphere I=\frac{2}{5}mr^{2}

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SUMMARY

The moment of inertia for a uniform sphere is defined as I = \frac{2}{5}mr^{2}. This formula is derived through integration of the mass distribution across the volume of the sphere, specifically integrating r^2 \sin^2 \theta. The process involves calculating the differential volume element dV = r^2 dr d\phi \sin \theta d\theta. Resources such as HyperPhysics provide detailed explanations and examples of these calculations.

PREREQUISITES
  • Understanding of basic calculus, specifically integration techniques
  • Familiarity with the concept of moment of inertia
  • Knowledge of spherical coordinates and their applications
  • Basic physics principles related to mass distribution
NEXT STEPS
  • Study the derivation of moment of inertia for different shapes, such as cylinders and disks
  • Learn about the application of spherical coordinates in physics problems
  • Explore advanced integration techniques relevant to physics
  • Review resources on mass distribution and its impact on rotational dynamics
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Students studying physics, particularly those focusing on mechanics and rotational motion, as well as educators seeking to explain the derivation of moments of inertia.

amcavoy
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Could someone direct me to a site that explains how the common moments of inertia were arrived at? My physics professor put up on the board today that for a uniform sphere:

I=\frac{2}{5}mr^{2}.

He said it was just the anti-derivative of something, but he didn't want to go into it because there is a table in our book with all of the common moments of inertia.

Does anyone know? Maybe someone could show me how the above moment (for the sphere) was derived and I could try it on something else? Thanks, I'd appreciate it.
 
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The general form of the moment of inertia involves an integral of the mass distribution and moments of the mass.

http://hyperphysics.phy-astr.gsu.edu/hbase/mi.html#mi

The fourth and fifth plates provide an example of the integration ('anti-derivative') used to determine the moment of inertia.

Think about how a center of mass is defined.
 
You need to integrate r^2 \sin^2 \theta over the volume of the sphere. Note that this represents the square of the perpendicular distance of a point in the sphere from the axis of rotation. Also, note that dV = r^2 dr d\phi \sin \theta d\theta.
 

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