Explanation of parallel axis theorem

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SUMMARY

The parallel axis theorem states that for a rotating system with mass m, the moment of inertia I about an axis parallel to the axis through its center of mass (CM) and at a distance x is given by the formula I = ICM + mx2. This theorem allows for the calculation of the moment of inertia for a sphere with mass m and radius r, where ICM for the sphere is (2/5)mr2. However, it is crucial to note that the approximation of treating the sphere as a point mass at its CM is only valid under specific conditions, particularly when considering the gravitational field outside the sphere.

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  • Understanding of moment of inertia and its significance in rotational dynamics
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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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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
 
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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