Date: 14/10/2024Instructor: Dr. Niamh Fitzgerald
Uniform Circular Motion
Definition and principles (Sections 6.1-6.3)
Law of Universal Gravitation
Kepler’s Laws and Satellite Motion
Angular Velocity (ω): Rate at which an object rotates about an axis.
Linear Velocity (v): Speed at which an object moves along its circular path.
Radius (r): Distance from the center of rotation to the object.
An object traces an arc when it rotates around an axis.
Units for Rotation Angle:
Radians (rad)
1 complete revolution = 2π radians (360 degrees)
Angular Velocity Formula:
ω = Δθ / Δt
Linear Velocity Formula:
v = Δs / Δt
Relationship: v = rω
Angular velocity influences linear motion—points further from the center rotate through a greater arc length.
Given radius (r) = 0.300 m, speed (v) = 15 m/s.
Calculate angular velocity (ω) and relate it to the speed at the wheel rim.
A change in velocity direction implies acceleration and a corresponding net force.
Centripetal acceleration (ac) is directed towards the center of the circular path.
Centripetal Acceleration Formula:
ac = v² / r
Alternatively: ac = rω²
Determine the acceleration for a car on a curve (radius = 500 m, speed = 25 m/s) and compare it to gravitational acceleration (g).
Centripetal Force: Net force acting towards the center, maintaining circular motion.
Formula: Fc = mac
Can arise from tension, gravity, friction, etc.
Centripetal force can be expressed as:
Fc = mv² / r
Fc = mrω²
Determine the coefficient of friction needed for car tires on a flat curve using Fc = f = μsN, with N = mg.
On banked curves, the incline provides additional centripetal force.
Normal force (N) has components acting towards the center (N sin θ) and balancing gravity (N cos θ).
Equations used to determine the banking angle (θ):
N sin θ = mv² / r
N cos θ = mg
θ = tan⁻¹(v² / rg)