Derivation of Moment of Inertia Equation for Solid Discs

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SUMMARY

The derivation of the moment of inertia equation for solid discs, expressed as I = 0.5MR², can be approached using calculus. The process begins with the definition of moment of inertia for an arbitrary mass distribution, represented by the summation I = ΣMᵢRᵢ², where Mᵢ is a mass element at a perpendicular distance Rᵢ from the axis of rotation. Transitioning to a continuous mass distribution involves using density (ρ) and volume (ΔV) to derive the integral form I_{CM} = ∫_M r² dm, where r is the distance from the center of the disk to the infinitesimal mass dm. Utilizing polar coordinates simplifies the integration process significantly.

PREREQUISITES
  • Understanding of calculus, specifically integration techniques
  • Familiarity with the concept of moment of inertia
  • Knowledge of polar coordinates and Jacobian transformations
  • Basic principles of mass distribution and density
NEXT STEPS
  • Study the derivation of moment of inertia for a hoop to build foundational understanding
  • Learn about continuous mass distributions and their integration techniques
  • Explore the application of polar coordinates in calculus
  • Investigate the relationship between density (σ) and mass in two-dimensional objects
USEFUL FOR

Students of physics and calculus, educators teaching mechanics, and anyone interested in the mathematical foundations of rotational dynamics.

kelli105
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This isn't quite a homework question, but my calculus teacher mentioned to those of us also taking physics that it was possible to prove that I = .5MR^2 using calc. I had some extra time on my hands and decided to give it a try. I've tried doing a summation with a geometric series but then ran into trouble defining a and r [using the equation a/(1-r)]. Does anyone out there know how to do this?
 
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go back to the definition of how moment of inertia is defined for an arbitrary mass distribution of an object... you may find that it is given by something like (off top of my head only)
I=\sum_i M_i R_i^2
where M_i is a mass element at perpendicular distance R_i from the axis of rotation.

there should also be a continuous version in your book...if not derive it yourself by introducing \rho (density) such that
\Delta M_i = \rho \Delta V
and when \Delta V goes to zero you sum will become an integral.

hint: before tackling the disc, try a hoop first. then you may use that result to help you solve the disk
 
As mjsd mentioned there is also an expression for the contineous version, which should be

I_{CM} = \int_M r^2\,\textrm{d}m

Where r is the distance from center of the disk to the infinitesimal mass dm. If \sigma is the mass pr. unit area, then assuming that there is a uniform distribution of mass over the disk, \sigma would be constant. Change the above integral so that you integrate with respect to the area instead of mass. You would then have a multiple integral over the area corresponding the to surface area of the disk. Using polar coordinates this would be much easier to solve, so you should change from cartesian to polar coordinates (while remembering the Jacobian). You're integrations limits would change to something much simpler.
Don't worry about the \sigma, you can later replace an expression including \sigma with the mass M.
 
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