Unit 5: Rotational Motion (Part 1)
Kinematics, Connections to Linear Motion, and Torque
Rotational Kinematics
Rotational kinematics describes motion using angular variables. These variables are analogous to linear kinematics. For variable acceleration, calculus must be used: \( \omega = \displaystyle\frac{d\theta}{dt} \) and \( \alpha = \displaystyle\frac{d\omega}{dt} \).
\( \alpha(t) = \displaystyle\frac{d\omega}{dt} = 12t^2 – 2 \).
Evaluate at \( t = 2 \): \( \alpha(2) = 12(2^2) – 2 = 48 – 2 = 46 \text{ rad/s}^2 \).
Correct Answer: C
Convert to revolutions: \( \text{Rev} = \displaystyle\frac{200}{2\pi} = \displaystyle\frac{100}{\pi} \).
Correct Answer: A
Linear and Rotational Connections
Points on a rigid body share the same angular motion but have different linear properties based on their distance \( r \) from the axis. Use \( v_t = r\omega \) and \( a_t = r\alpha \).
Find speed: \( v_t = r\omega = (0.2)(1.1\pi) = 0.22\pi \text{ m/s} \).
Correct Answer: B
Total speed relative to the ground is the vector sum: \( V + V = 2V \).
Correct Answer: C
Torque
Torque is the cross product of position and force: \( \vec{\tau} = \vec{r} \times \vec{F} \). The magnitude is \( \tau = rF \sin\theta \). It measures the tendency of a force to rotate an object about an axis.
Correct Answer: A
Correct Answer: C
Rotational Formulas Recap
Unit 5: Rotational Motion (Part 2)
Inertia, Rotational Equilibrium, and Newton’s Second Law
Rotational Inertia (Moment of Inertia)
Rotational inertia (\( I \)) represents an object’s resistance to angular acceleration. For point masses, \( I = \sum m_i r_i^2 \). For continuous bodies, use calculus: \( I = \int r^2 dm \). The Parallel Axis Theorem (\( I = I_{cm} + Md^2 \)) allows you to find the inertia about any axis parallel to one through the center of mass.
\( I = \sum m_i r_i^2 = m(L/2)^2 + 2m(L/2)^2 \)
\( I = m(L^2/4) + 2m(L^2/4) = \displaystyle\frac{3}{4}mL^2 \).
Correct Answer: A
The distance from the center to the end is \( d = L/2 \).
\( I = \displaystyle\frac{1}{12}ML^2 + M(L/2)^2 = \displaystyle\frac{1}{12}ML^2 + \displaystyle\frac{1}{4}ML^2 \)
\( I = \displaystyle\frac{1+3}{12}ML^2 = \displaystyle\frac{4}{12}ML^2 = \displaystyle\frac{1}{3}ML^2 \).
Correct Answer: C
– Hoop: \( I = MR^2 \) (constant 1.0)
– Cylinder: \( I = 0.5MR^2 \)
– Sphere: \( I = 0.4MR^2 \)
Since \( 0.4 < 0.5 < 1.0 \), the sphere has the smallest inertia.
Correct Answer: C
\( I = \int_{0}^{L} kx^3 dx = \left[ \displaystyle\frac{1}{4}kx^4 \right]_0^L = \displaystyle\frac{1}{4}kL^4 \).
Correct Answer: B
Correct Answer: D
Rotational Equilibrium and Newton’s First Law
Rotational Equilibrium requires \( \sum \tau = 0 \). For total static equilibrium, both \( \sum \vec{F} = 0 \) and \( \sum \vec{\tau} = 0 \) must be true.
Since the beam only extends 3 m on each side of the center, the girl would need to sit off the beam.
Correct Answer: D
Correct Answer: B
Correct Answer: C
Correct Answer: C
Correct Answer: D
Newton’s Second Law in Rotational Form
The rotational equivalent of \( F = ma \) is \( \sum \tau = I \alpha \). For systems with both translation and rotation, link them using \( a = R \alpha \) for no-slip conditions.
Correct Answer: A
Substitute \( T \): \( mg – 0.5Ma = ma \Rightarrow a = \displaystyle\frac{mg}{m + M/2} \).
Correct Answer: C
\( Mg \sin\theta – f = 2f \Rightarrow f = \displaystyle\frac{1}{3}Mg \sin\theta \).
Correct Answer: B
Correct Answer: B
Correct Answer: B


