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The parallel axis theorem, which provides equations for calculating the moment of inertia and angular momentum of an object rotating around an axis that is not passing through its center of mass. The text uses the example of a dumbbell to illustrate the application of the theorem. This theorem is useful for understanding the motion and rotation of objects with complex trajectories, such as planets or satellites.
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27 October, 2005
Mark Halpern
Our textbook has an equation which it calls the parallel axis theorem in Chapter 10. Let CM (^) Ixx be the moment of inertia of an object for rotations about the centre of mass of the object
and pointing in the x direction. Remember that we will use a direction to describe a rotation; it is the orientation of the axis of rotation and as a matter of convention we choose the end of the axis to look towards, and the end to look from, so that the rotation appears clockwise to us. I have chosen the x axis here completely arbitrarily, but I do not want to write down a moment of inertia without including a direction.
[ Check back to Section 9.5 if you want to review what we mean by centre of mass.]
But let’s imagine that this object is rotating about an axis parallel to the x axis but which does not pass through the centre of mass but at closest approach is a distance D away. For example, imagine your physics book rotating about its corner rather than its centre. In this case, as the text works out, the moment of inertia is
Ixx =CM^ Ixx + M D^2. 10. 18 (1)
This is a very useful theorem, especially if someone nails the corner of your textbook to a table. It provides a recipe for the angular momentum of an object whose motion and rotation have a very particular relation so that one point on the object sits still. But there is another expression which is also called the parallel axis theorem, one which we used in class to calculate an angular momentum of a sliding block. It is a recipe for finding the angular momentum of an object which is moving and rotating but with no restriction on the relation between motion of the centre of mass and rotation about the centre of mass. The earth spins and orbits the sun, but it does not move in a way that some spot sits still. Equation (10.18) is not directly useful.
We will work this out for a very particular case, but the result is general. Imagine a dumbell consisting of two equal point masses, each with mass m, separated by a massless rod of length 2 R. Imagine that the centre of mass of this object is at x = D, that the dumbell is spinning about its centre of mass with angular frequency ωCM and that the velocity of the centre of mass is vy. The angular momentum of the dumbell about the origin can be found from the sum of the angular momenta of the two end masses. The mass nearest the origin is located at x = D − R and has velocity ~v 1 = (vy − ωCM R)ˆy. Its angular momentum is
L^ ~ 1 = ~r × ~p = (D − R)m(vy − ωCM R)ˆz. (2)
The angular momentum of the second mass is
L^ ~ 2 = ~r × ~p = (D + R)m(vy + ωCM R)ˆz. (3)
so the sum is ~L = ~L 1 + ~L 2 = 2Dmvy zˆ + 2mR^2 ωCM ˆz (4)
where we have dropped a number of terms which have opposite signs in ~L 1 abd L~ 2.
The second term is the angular momentum of the dumbell about its own centre of mass. The first term is exactly ~r × ~p for the centre of mass of the dumbell, so
L^ ~ = ~rCM × ~pCM +CM^ Iz ~ωCM. (5)
This is the parallel axis theorem. The angular momentum of a moving spinning object is the sum of the angular momentum from the motion of the centre of mass pluss the angular momentum of the spin of the object about its own centre of mass.