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TAM 212: Introductory Dynamics

Elementary motions #rke

Two of the most common motions are straight-line and circular kinematics. While the general kinematic formulas apply to these situations, we can write simpler formulas just for these special cases.

Rectilinear motion #rke‑sr

Rectilinear motion is motion in a straight line. In the particular case that acceleration is constant, the velocity and position can be found by explicit integration.

Constant linear acceleration. #rke‑er

a=a0=constantv=v0+a0tx=x0+v0t+12a0t2

If the x and y components of a 2D motion are independent, then each direction can be regarded as simple rectilinear motion. For example, if a projectile flies through the air then the horizontal component is linear in t, while the vertical motion with constant gravitational acceleration is a parabola.

Circular motion #rke‑sc

Motion in a circle of constant radius gives velocity in the tangential direction ˆeθ. The acceleration has one component directly inwards in the radial direction (centripetal acceleration) and one tangential component due to angular acceleration α.

Circular motion (constant r). #rke‑ec

r=constantv=rωˆeθa=rω2ˆer+rαˆeθ

Note that for circular motion the velocity v is linear in both the radius r and angular velocity ω. The tangential acceleration is linear in both the radius r and angular acceleration α, while the radial acceleration is linear in r but quadratic in ω.

In the case of constant angular acceleration, the angular components function like rectilinear motion but in a circle, giving the explicit formulas:

Constant angular acceleration. #rke‑ea

r=r0=constantα=α0=constantω=ω0+α0tθ=θ0+ω0t+12α0t2