Animated Solution for Physics - Rotational Motion: A flat surface of a thin uniform disk A of radius R is glued to a horizontal table. Another thin uniform disk B of mass M and with the same radius R rolls without slipping on the circumference of A, as shown in the figure. A flat surface of B also lies on the plane of the table. The center of mass of B has fixed angular speed ω about the vertical axis passing through the center of A. The angular momentum of B is nMωR2 with respect to the center of A. Which of the following is the value of n?
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Visualized Solution
Setup and Kinematics
Disk A is fixed.
Disk B revolves around A with angular speed ω.
Velocity of Center of Mass
Distance between centers =R+R=2R
vc=ω(2R)
Condition for Pure Rolling
Velocity of contact point P must be zero.
vP=0
Angular Velocity of Disk B
Let ω0 be the spin angular velocity of B.
vP=vc−ω0R=0
Solving for ω0
ω0R=vc=2ωR
ω0=2ω
Total Angular Momentum
LA=Lcm+rcm×pcm
Calculating Components
Lcm=Icmω0=(21MR2)(2ω)
Lorbital=rcmMvc=(2R)M(2ωR)
Summing Angular Momentum
LA=MR2ω+4MR2ω
LA=5MR2ω
Final Answer
LA=nMωR2
n=5
Food for Thought
What if disk B rolled inside a larger ring?
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The Sigma Insight: Dynamics of Rigid Body Rotation
Solution Diagram
The problem of a disk rolling on another fixed disk is a classic test of your understanding of rigid body kinematics and angular momentum. It beautifully combines the concepts of pure rolling, orbital motion, and spin. Let's break it down step by step.
Analyzing the Setup
Imagine you are looking at the table from above. We have two identical disks, A and B, both of radius R. Disk A is firmly glued to the table, meaning it cannot move or rotate. Disk B, on the other hand, is rolling on the circumference of disk A.
The center of mass of disk B is revolving around the center of disk A with a constant angular speed ω. Because both disks have a radius R, the distance between their centers is simply R+R=2R.
This means the center of disk B is moving in a circular path of radius 2R. Therefore, the linear velocity of the center of mass of disk B, let's call it vc, is given by:
vc=ω(2R)
The Condition for Pure Rolling
Here is where many students make a mistake. The question explicitly states that disk B rolls without slipping on disk A. What does this physically mean? It means that at the exact point where the two disks touch, there is no relative motion between them. Since disk A is stationary, the velocity of the contact point on disk B must be exactly zero.
Let's assume disk B is spinning about its own center of mass with an angular velocity ω0. The net velocity of the contact point is the vector sum of the translational velocity of the center of mass (vc) and the tangential velocity due to its spin (ω0R).
For the contact point to be at rest, these two velocities must perfectly cancel each other out:
vc−ω0R=0
Substituting our earlier expression for vc, we get:
2ωR−ω0R=0
Solving this gives us the spin angular velocity of disk B:
ω0=2ω
This is a crucial insight! Disk B is spinning twice as fast about its own axis as it is revolving around disk A.
The Master Equation of Angular Momentum
Now, we need to find the total angular momentum of disk B with respect to the center of disk A. For a rigid body undergoing both translation and rotation, the total angular momentum about a point is the sum of two parts:
1. The spin angular momentum about its own center of mass (Lcm).
2. The orbital angular momentum of its center of mass about the reference point (rcm×pcm).
Mathematically, this is expressed as:
LA=Lcm+rcm×pcm
Let's calculate each part carefully. The spin angular momentum is the moment of inertia of the disk about its center multiplied by its spin angular velocity:
Lcm=Icmω0=(21MR2)(2ω)=MR2ω
Next, the orbital angular momentum is the cross product of the position vector and the linear momentum. Since the velocity is always perpendicular to the position vector in circular motion, the magnitude is simply rcmMvc:
Lorbital=(2R)M(2ωR)=4MR2ω
Final Calculation
Since both the spin and the orbital motion are in the same direction (counterclockwise), their angular momentum vectors point in the same direction (out of the page). We can simply add their magnitudes:
LA=MR2ω+4MR2ω=5MR2ω
The problem states that the angular momentum is nMωR2. By comparing our result with this expression, we can immediately see that:
n=5
This elegant result shows how the different components of motion contribute to the total angular momentum. The orbital motion actually contributes four times as much angular momentum as the spin!