Explanation of parallel axis theorem

In summary, the parallel axis theorem states that the moment of inertia of a rigid body about any axis parallel to an axis through its center of mass can be calculated by adding the moment of inertia about the center of mass axis to the product of the body's mass and the square of the distance between the two axes. This theorem is useful for determining the rotational inertia of objects when the center of mass is not aligned with the axis of rotation.
  • #1
Trollfaz
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For a rotating system with mass m this theorem says that if it rotates about an axis distance x from but parallel to the axis through it's natural mass center (CM), then I moment of inertia is
$$I=I_{CM}+mx^2$$
My thinking is if one move the axis x distance away from the axis through it's CM, and we can treat the object as a point mass at it's CM, then it's as though we are moving that point x distance away from the axis of rotation, contributing another ##mx^2## moment of inertia, is this explanation correct?
 
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  • #2
So for instance I of sphere mass m is ##\frac{2}{5}mr^2## for radius=r. But in Newtonian mechanics, we can treat the sphere as a point mass in its geometrical center. Then if this axis of rotation is x away from it's CM, then the point mass is also x from the axis of rotation add another ##mx^2## to I. Assuming sphere is uniformly distributed in mass
 
  • #3
Trollfaz said:
But in Newtonian mechanics, we can treat the sphere as a point mass in its geometrical center.
We most certainly cannot. Only for certain things such as the gravitational field outside the sphere does this hold.

In particular, the sphere has a moment of inertia around its CM - which the point particle does not.
 
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