Decoding the 3D Geometry
When you first look at the 2D diagram provided in the question, it can be a bit deceptive. It might seem like all three discs are lying flat in the same plane. However, the way they are drawn—with D1 as an ellipse and D2, D3 as perfect circles—is a classic convention to represent a 3D structure on a 2D page.
Let's visualize this properly. Imagine disc D1 is lying flat in the horizontal plane, much like a plate resting on a table. Meanwhile, discs D2 and D3 are standing upright in the vertical plane, attached to the edges of D1 like the wheels of a car attached to an axle. The axis of rotation, OO′, passes straight up vertically through the center of D1.
The Central Disc
A Straightforward Spin
Let's first tackle the central disc, D1. The axis OO′ is perpendicular to the plane of D1 and passes right through its center.
From our standard formulas, the moment of inertia of a uniform disc about its central perpendicular axis is simply:
This part is straightforward and forms the foundation of our total calculation.
The Outer Discs
Parallel Axis Theorem to the Rescue
Now, what about the outer discs, D2 and D3? Notice how the vertical axis OO′ relates to them. Because D2 and D3 are standing upright in vertical planes, the axis OO′ is actually parallel to their vertical diameters.
To find their moment of inertia about OO′, we must deploy the Parallel Axis Theorem. The theorem states that the moment of inertia about any axis is the sum of the moment of inertia about a parallel axis through the center of mass, plus Md2, where d is the perpendicular distance between the two axes.
For a disc rotating about its own diameter, the moment of inertia is:
Since D2 and D3 are attached at the opposite ends of D1 (which has a radius R), the distance d between their own central vertical axis and OO′ is exactly R.
Let's set up the equation for D2:
Adding them up, we get:
Because the setup is perfectly symmetrical, disc D3 will have the exact same moment of inertia:
Bringing It All Together
Finally, to get the total moment of inertia of the entire system, we simply add the individual moments of inertia together.
Itotal=21MR2+45MR2+45MR2
To make the addition easier, let's write 21 as 42:
This beautifully simplifies to exactly 3MR2. Always pay close attention to the spatial orientation of the objects relative to the axis of rotation—it makes all the difference!