Presenting the concepts of circular motion and gravitation.
Dr. Val G. Rousseau – Xavier University of Louisiana.
Angular displacement, angular velocity, and angular acceleration are crucial for understanding circular motion.
Arc Length (s):
Distance measured along the circumference of a circle between two points (A and B).
Measurement of angles:
Radians provide an alternative to degrees.
Definition: A radian is the angle θ formed by an arc length (s) equal to the radius (R).
Relationship: Full circle (360°) corresponds to 2π radians.
Formula:
p = 2πR
For a complete rotation:
2π radians = 360°.
Angular displacement (Δθ):
Defined as the change in rotation angle.
Formula:
Δθ = θf - θi
Directionality:
Positive if counterclockwise.
Negative if clockwise.
Angular velocity (ω):
Expresses how fast the angular displacement changes with time.
Average Angular Velocity:
ω_avg = Δθ/Δt
Instantaneous Angular Velocity:
Related to linear speed (v), with v = Rω.
Angular acceleration (α):
Describes the rate at which the angular velocity changes over time.
Angular Acceleration Equation:
α = Δω/Δt
The angular quantities (Δθ, ω, α) follow the same equations and relationships as linear quantities (Δx, v, a) under constant angular acceleration conditions.
Tangent references instantaneous velocity tangential to the trajectory in circular motion.
Tangent Line:
Touches the circle at a single point and is perpendicular to the radius.
Case Reference:
Angular Velocity: Given as 33 ⅓ rpm.
Conversions: Required to find angular velocity in radians per second and the linear speed at a distance from the rotation axis.
Case Reference:
Slow down from 9.20 m/s to rest over 85.0 m.
Calculations include finding angular velocity and angular acceleration, involving direct applications of kinematic equations.
Centripetal force:
A net force causing centripetal acceleration toward the center during circular motion.
Newton's Law:
Every particle attracts every other particle with a force along the line joining them, directly proportional to their masses and inversely proportional to the square of the distance between them.
Gravitational force (F):
F = G (m1*m2/r²)
G: Universal Gravitational Constant.
Understanding these fundamental concepts of angular motion and gravitation is essential for solving problems in physics related to circular contexts.