Inertia Tensor of a cylinder at a distance

AI Thread Summary
The discussion focuses on calculating the inertia tensor of a cylinder when the rotational axis is shifted from the center of mass. The inertia tensor for a cylinder is initially provided, with the bottom right element remaining constant for rotation about the z-axis. The user expresses confusion about maintaining the diagonal form of the tensor and how to apply the parallel axes theorem for an off-center axis. They share a specific example involving a 2 kg mass and a distance vector, initially misapplying the formula but later realizing their mistake. The conversation highlights the importance of understanding the parallel axes theorem and correctly applying it to compute the inertia tensor for different rotational axes.
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I have a cylinder, for which i want to find the inertia tensor.
http://www.mip.sdu.dk/~pino/inertiacyl.JPG
Where the rotational axis are either the x (red) or y (green).

I know that the inertia tensor for a cylinder is of the form
http://www.mip.sdu.dk/~pino/inertiamoment-cylinder.jpg
Then I believe that the bottom right element stays the same, since this describes the rotation around the z-axis.
The tricky part for me is the rest of the matrix. I am no expert, and do not understand inertia tensors fully, so I would like some pointers.

My immediate idea is that the matrix should remain in its diagonal form, the zeros will remain zeros, is this correct?

I know that for complex forms i can split up the moments of inertia, so i have the moment of inertia for the blank space d, which is 0. and then i can add the moment of inertia of the cylinder, but how do i calculate this, when the rotational axis is x-axis for example?
 
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Oops, i should have posted this in the homework section,, don't know how to move it, so will repost there.
 
The wikipedia page

http://en.wikipedia.org/wiki/Moment_of_inertia

contains section 'Parallel axes theorem' at the bottom of the page where they show you how to obtain the tensor for any point of rotation that is offset from the center of mass once you know the tensor for origin at the center of mass.

Keep in mind the axes of the two coordinate systems, one at center of mass and one at your point of choice, must remain parallel, hence the name of the theorem.
 
I have looked at the formula listed, but i don't know quite how to use it...
2b8ad3e76e9f3a4df514e2f2289736eb.png


Suppose i have an inertia tensor in the center of mass like this
\left(\begin{array}{c c c} 1&0&0\\0&1&0\\0&0&1\end{array}\right)
The mass m is 2 kg, and the distance vector R is
\left(\begin{array}{c} 1\\0\\0\end{array}\right)

what i thought of doing was
I+m\cdot R^2=<br /> \left(\begin{array}{c c c} 3&amp;2&amp;2\\0&amp;1&amp;0\\0&amp;0&amp;1\end{array}\right)<br />
But when i look at the formula i read it as
the jk'th of I + M*((R dot R when j equals k) -(the j'th of R times the k'th of R))
for example j=1, k=1, i get
1 + 2* (1-1)=1
for j=2, k=3
0+2* (0-0)=0
and so forth. The M*(R... part always yields 0! what am i misunderstanding?
 
Never mind... i got it now... stupid me :frown:
 
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