Parallel Axis Theorem and interia tensors

AI Thread Summary
The discussion clarifies that the parallel axis theorem is applicable to both 2D and 3D objects, including hemispheres. The general formula for the theorem is provided, emphasizing the relationship between the inertia tensor at different points. A correction was made regarding the notation in the formula, ensuring accuracy in tensor types. It was confirmed that one can derive the inertia tensor at the center of mass from the inertia tensor at another point using the theorem. Overall, the parallel axis theorem is valid for various shapes, including complex 3D objects.
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Is the parallel axis theorem always valid for inertia tensors? We have only seen examples with flat (2d) objects and was wondering if it would also be valid for 3d objects, like a h emisphere, for example. Thanks.
 
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Yep, just use the distance projected from the axis that it's being measured around.
 
The general form for the parallel axis theorem is

\mathbf{J} = \mathbf{I} + m(r^2\mathbf{1} - \boldsymbol{r}\boldsymbol{r}^T)

where

\mathbf{J} is the inertia tensor of some object about some point removed from the center of mass,
\mathbf{I} is the inertia tensor of the object about its center of mass
m is the object's mass
\boldsymbol{r} is the displacement of the point in question from the center of mass, expressed as a column vector
\mathbf{1} is the identity matrix.
 
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I think you meant \mathbf{J} = \mathbf{I} + m(r^2\mathbf{1} - \mathbf{r}\mathbf{r}^T), because \mathbf{r}^T \mathbf{r} = r^2, which is not even the right type of tensor.

To show that this gives the correct moment of inertia about a certain axis, let e be a unit vector giving the direction of this axis. Then the moment of inertia about this axis is
\mathbf{e}^T\mathbf{Je}<br /> = \mathbf{e}^T \mathbf{Ie} + m(r^2 \mathbf{e}^T\mathbf{1e} - \mathbf{e}^T\mathbf{rr}^T\mathbf{e})
= \mathbf{e}^T \mathbf{Ie} + mr^2 - m(\mathbf{r} \cdot \mathbf{e})^2
= \mathbf{e}^T \mathbf{Ie} + mr_\perp^2, where r_\perp is the perpendicular distance from the centre of mass to the axis.
 
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adriank said:
I think you meant \mathbf{J} = \mathbf{I} + m(r^2\mathbf{1} - \mathbf{r}\mathbf{r}^T)
:blushing:
Oops. I corrected my post, thanks.
 
so does that mean if we find the inertia tensor at the center of the base of a hemisphere we can use the parallel axis theorem to find the tensor for the center of mass
 
Yes, but in reverse. You know J, and you must find \mathbf{I} = \mathbf{J} - m(r^2 \mathbf{1} - \mathbf{rr}^T).
 
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