angular displacement
Summary
Angular displacement (Δθ) is the net angle through which an object rotates about an axis, usually measured in radians. Counterclockwise is conventionally positive. The most testable link is s = rΔθ, which holds only when Δθ is in radians.
Detail
Meaning: Angular displacement is the net change in the angular position of a rotating object, the rotational counterpart of linear displacement. Turning back and forth cancels, so only the net turn counts. One full revolution is 2π rad (360°). Every point on a rigid rotating body has the same Δθ in the same time, but points farther from the axis travel a greater arc length.
Equation: s = rΔθ, where s is arc length traveled by a point (m), r is its distance from the axis (m), and Δθ is angular displacement (rad). Δθ itself is θf − θi (rad).
On the MCAT: Passages describe wheels, gears, pulleys, centrifuges or spinning disks. You may convert revolutions to radians (1 rev = 2π rad), find the arc length a point on the rim travels, or use the rotational kinematics equations, which mirror the linear ones: Δθ = ωt for constant angular velocity ω (rad/s) over time t (s), and Δθ = ω₀t + ½αt² for constant angular acceleration α (rad/s²). Expect to compare two points at different radii: same Δθ and ω, but larger s and linear speed farther out.
Common confusion: Students plug degrees into s = rΔθ. The relation holds only for radians, since a radian is defined as arc length divided by radius. Also, one full turn gives Δθ = 2π rad, not zero, unlike linear displacement for a round trip.
Sources
- Physics (Giancoli)
- College Physics (Serway and Vuille)
- Fundamentals of Physics (Halliday, Resnick and Walker)
Written for the MCAT and checked before it was published. For study reference only. Spotted an error? Let us know.