The Beauty of Rotational Dynamics
Imagine a large, heavy circular disc spinning smoothly like a playground merry-go-round. It possesses a certain amount of 'rotational momentum'—a stubbornness to keep spinning at its current rate. This problem is a beautiful exploration of what happens when we disturb this system, not by pushing or pulling it, but simply by adding mass to it. It's a classic demonstration of one of the most profound laws in physics: the Conservation of Angular Momentum.
Visualizing the Setup
We start with a uniform circular disc of mass M=50 kg and radius R=0.4 m. It is rotating freely about its vertical central axis with an initial angular velocity ω1=10 rad/s.
Then comes the intervention. Two uniform circular rings, each of mass m=6.25 kg and radius r=0.2 m, are 'gently placed' symmetrically on the disc. The phrase 'gently placed' is the golden key here. It means the rings are dropped onto the disc without any twisting force or external torque. They are placed such that they touch each other exactly at the axis of the disc. This geometric constraint is crucial: it tells us exactly how far the center of each ring is from the main axis of rotation.
The Principle of Conservation
Because the rings are placed gently, the net external torque acting on the entire system (disc + rings) is zero (τext=0). According to Newton's laws applied to rotation, when the net external torque is zero, the total angular momentum of the system must remain constant.
Mathematically, this is expressed as:
Linitial=Lfinal
I1ω1=I2ω2
Where I1 is the initial moment of inertia, ω1 is the initial angular velocity, I2 is the final moment of inertia, and ω2 is the final angular velocity we want to find.
Calculating the Initial State
Before the rings are added, the only object rotating is the uniform disc. The moment of inertia of a uniform disc about its central axis is given by the standard formula:
I1=Idisc=21MR2
Let's plug in the given values to see what we are working with:
I1=21(50 kg)(0.4 m)2=21(50)(0.16)=4 kg⋅m2
The Parallel Axis Theorem Challenge
Now, we need to find the final moment of inertia, I2, which includes the disc and the two rings. The moment of inertia of the disc remains the same, but we must carefully calculate the moment of inertia of the rings.
Here is where many students fall into a trap. The moment of inertia of a ring is mr2, right? Yes, but only about its own central axis! Our rings are not rotating about their own centers; they are revolving around the central axis of the disc.
Because the rings touch each other at the disc's axis, the center of each ring is shifted by a distance d=r from the axis of rotation. To find their moment of inertia about the disc's axis, we must invoke the Parallel Axis Theorem (I=Icm+md2):
Iring=Icm+md2=mr2+m(r)2=2mr2
Since there are two identical rings, their total contribution to the moment of inertia is:
Iadded=2×(2mr2)=4mr2
Let's calculate this numerical value:
Iadded=4(6.25 kg)(0.2 m)2=4(6.25)(0.04)=25(0.04)=1 kg⋅m2
So, the total final moment of inertia is:
I2=Idisc+Iadded=4+1=5 kg⋅m2
The Final Calculation
We now have all the pieces of the puzzle. We return to our conservation equation:
I1ω1=I2ω2
(4)(10)=(5)ω2
40=5ω2
ω2=540=8 rad/s
Conclusion and Physical Intuition
The final angular velocity is 8 rad/s.
Does this make physical sense? Absolutely. We added mass to the system, and more importantly, we added mass at a distance from the axis of rotation. This increased the system's rotational inertia (its resistance to spinning). To conserve the total angular momentum, the system had to slow down its rotation rate. It's the exact same physics that causes an ice skater to spin slower when they extend their arms outward!