Circular and Rotational Motion

Understanding the physics of rotation and circular movement

Introduction to Circular and Rotational Motion

Circular motion involves the movement of an object along a circular path, while rotational motion involves the rotation of an object around an axis. These types of motion are crucial in understanding everything from planetary orbits to spinning tops and wheels. Both types of motion involve angular quantities that provide elegant ways to describe rotational phenomena.

Uniform Circular Motion

Uniform circular motion occurs when an object moves along a circular path with constant speed. Despite the constant speed, the object is constantly accelerating because its direction is continuously changing.

Period and Frequency
\[T = \frac{2\pi r}{v} = \frac{2\pi}{\omega}\] \[f = \frac{1}{T} = \frac{v}{2\pi r} = \frac{\omega}{2\pi}\]
Where:
  • \(T\) = period (time for one complete revolution, in s)
  • \(f\) = frequency (number of revolutions per unit time, in Hz)
  • \(r\) = radius of the circular path (in m)
  • \(v\) = linear speed (in m/s)
  • \(\omega\) = angular velocity (in rad/s)
Example 1: Race Track Motion

A car is moving around a circular track of radius 100 m at a constant speed of 20 m/s. Find the period and frequency of motion.

\[T = \frac{2\pi r}{v} = \frac{2\pi \times 100 \text{ m}}{20 \text{ m/s}} = 31.4 \text{ s}\]

\[f = \frac{1}{T} = \frac{1}{31.4 \text{ s}} \approx 0.032 \text{ Hz (revolutions per second)}\]

Centripetal Acceleration and Force

In circular motion, an object experiences an acceleration directed toward the center of the circle. This is called centripetal acceleration. The force that provides this acceleration is called centripetal force.

Centripetal Acceleration and Force
\[a_c = \frac{v^2}{r} = \omega^2 r\] \[F_c = ma_c = m\frac{v^2}{r} = m\omega^2 r\]
Where:
  • \(a_c\) = centripetal acceleration (in m/s²)
  • \(F_c\) = centripetal force (in N)
  • \(m\) = mass of the object (in kg)
  • \(v\) = linear speed (in m/s)
  • \(r\) = radius of the circular path (in m)
  • \(\omega\) = angular velocity (in rad/s)

The centripetal force is not a new type of force; it's the name given to the force that causes circular motion. This force can be provided by tension, friction, gravity, or other forces.

Example 2: Car Rounding a Curve

A 1500 kg car is rounding a curve of radius 50 m at a speed of 15 m/s. What is the centripetal force required?

\[F_c = m\frac{v^2}{r} = 1500 \text{ kg} \times \frac{(15 \text{ m/s})^2}{50 \text{ m}} = 1500 \times \frac{225}{50} = 6750 \text{ N}\]

This force must be provided by friction between the tires and the road.

Angular Quantities in Rotational Motion

In rotational motion, we use angular quantities analogous to those in linear motion. These provide a more natural way to describe rotating systems.

Angular Quantities
\[\text{Angular Position: } \theta \text{ (in radians)}\] \[\text{Angular Velocity: } \omega = \frac{d\theta}{dt}\] \[\text{Angular Acceleration: } \alpha = \frac{d\omega}{dt}\]

Relationships between linear and angular quantities:

Linear-Angular Relationships
\[v = r\omega\] \[a_{\text{tangential}} = r\alpha\] \[a_{\text{centripetal}} = r\omega^2\]
Where:
  • \(v\) = linear velocity
  • \(a_{\text{tangential}}\) = tangential acceleration
  • \(a_{\text{centripetal}}\) = centripetal acceleration
  • \(r\) = radius from axis of rotation

The rotational analogues of the kinematic equations for constant angular acceleration are:

Rotational Kinematic Equations
\[\omega = \omega_0 + \alpha t\] \[\theta = \theta_0 + \omega_0 t + \frac{1}{2}\alpha t^2\] \[\omega^2 = \omega_0^2 + 2\alpha(\theta - \theta_0)\] \[\theta - \theta_0 = \frac{1}{2}(\omega_0 + \omega)t\]

Torque and Rotational Equilibrium

Torque is the rotational analog of force, causing an object to rotate. It is the product of the force and the perpendicular distance from the line of action of the force to the axis of rotation (the lever arm).

Torque
\[\vec{\tau} = \vec{r} \times \vec{F}\] \[|\tau| = rF \sin \theta\]
Where:
  • \(\vec{\tau}\) = torque vector (in N⋅m)
  • \(\vec{r}\) = position vector from axis to point of force application
  • \(\vec{F}\) = force vector
  • \(\theta\) = angle between \(\vec{r}\) and \(\vec{F}\)

An object is in rotational equilibrium when the net torque acting on it is zero:

Rotational Equilibrium
\[\sum \tau = 0\]
Example 3: Torque on a Lever

A 2 m long rod has a mass of 5 kg suspended from one end. If the rod is supported at 0.5 m from the end with the mass, what is the torque about the support?

The force due to the mass is \(F = mg = 5 \text{ kg} \times 9.8 \text{ m/s}^2 = 49 \text{ N}\)

The lever arm is 0.5 m

\[\tau = rF = 0.5 \text{ m} \times 49 \text{ N} = 24.5 \text{ N⋅m}\]

Rotational Inertia (Moment of Inertia)

The moment of inertia is a measure of an object's resistance to changes in its rotation. It depends on the distribution of mass relative to the axis of rotation.

Moment of Inertia
\[I = \sum m_i r_i^2\] \[\text{For continuous objects: } I = \int r^2 \, dm\]
Where:
  • \(I\) = moment of inertia (in kg⋅m²)
  • \(m_i\) = mass of particle i
  • \(r_i\) = distance of particle i from the axis of rotation

Common moments of inertia:

  • Solid sphere about a diameter: \(I = \frac{2}{5}MR^2\)
  • Hollow sphere about a diameter: \(I = \frac{2}{3}MR^2\)
  • Solid cylinder about its axis: \(I = \frac{1}{2}MR^2\)
  • Rod about its center: \(I = \frac{1}{12}ML^2\)
  • Rod about one end: \(I = \frac{1}{3}ML^2\)
Newton's Second Law for Rotation
\[\tau = I\alpha\]
Where:
  • \(\tau\) = net torque
  • \(I\) = moment of inertia
  • \(\alpha\) = angular acceleration

Rotational Energy and Angular Momentum

Objects in rotational motion possess rotational kinetic energy and angular momentum, which are the rotational analogs of linear kinetic energy and momentum.

Rotational Kinetic Energy and Angular Momentum
\[K_{\text{rot}} = \frac{1}{2}I\omega^2\] \[L = I\omega\]
Where:
  • \(K_{\text{rot}}\) = rotational kinetic energy (in J)
  • \(L\) = angular momentum (in kg⋅m²/s)
  • \(I\) = moment of inertia (in kg⋅m²)
  • \(\omega\) = angular velocity (in rad/s)

Conservation of Angular Momentum: In the absence of external torques, the total angular momentum of a system remains constant.

Conservation of Angular Momentum
\[L_{\text{initial}} = L_{\text{final}}\] \[I_1\omega_1 = I_2\omega_2\]
Example 4: Rotating Sphere

A solid sphere of mass 2 kg and radius 0.1 m is rotating at 5 rad/s about an axis through its center. Calculate its rotational kinetic energy.

\[I = \frac{2}{5}MR^2 = \frac{2}{5} \times 2 \text{ kg} \times (0.1 \text{ m})^2 = 0.008 \text{ kg⋅m}^2\]

\[K_{\text{rot}} = \frac{1}{2}I\omega^2 = \frac{1}{2} \times 0.008 \text{ kg⋅m}^2 \times (5 \text{ rad/s})^2 = 0.1 \text{ J}\]

Applications of Rotational Motion

Understanding circular and rotational motion is essential for many real-world applications:

Astronomy & Space
  • Planetary motion and satellite orbits
  • Galaxy rotation and stellar mechanics
  • Spacecraft attitude control
Mechanical Engineering
  • Wheels, gears, and transmission systems
  • Motors and turbines
  • Flywheels for energy storage
Navigation & Control
  • Gyroscopes and inertial guidance
  • Stabilization systems
  • Precision instruments
Sports & Recreation
  • Figure skating spins and conservation
  • Discus and shot put throwing
  • Bicycle and motorcycle dynamics

Key Concepts Summary

  • Circular motion: Constant speed but changing direction
  • Centripetal force: \(F_c = \frac{mv^2}{r}\) - always points toward center
  • Angular velocity: \(\omega = \frac{v}{r}\) - rate of angular change
  • Torque: \(\tau = rF \sin \theta\) - rotational force
  • Moment of inertia: \(I = \sum mr^2\) - rotational mass
  • Angular momentum: \(L = I\omega\) - conserved quantity