2nd Equation of Motion for Rotation - Final Angle


In mathematical physics, equations of motion are equations that describe the behaviour of a physical system in terms of its motion as a function of time.This equation applies to a particle moving linearly, in three dimensions in a straight line, with constant acceleration.Since the vectors are collinear (parallel, and lie on the same line) – only the magnitudes of the vectors are necessary and because the motion is along a straight line, the problem effectively reduces from three dimensions to one.

Related formulas


θfinal angle(angular displacement) (rad)
θ0initial angle (rad)
ω0initial angular velocity (rad/s)
ttime taken to rotate from the initial state to the final state (s)
aconstant angular acceleration (rad/s2)