Centripetal acceleration, angular velocity, and motion in polar coordinates
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=
rv2=
ω2r
Angular velocity:ω=rv
Period:T=v2πr=ω2π
Polar Coordinates
Position in polar coordinates: (r,θ)
Unit vectors: r^ (radial), θ^ (tangential)
Important: These unit vectors are not constant—they change direction as the particle moves.
Time derivatives of unit vectors:dtdr^=θ˙θ^=ωθ^
dtdθ^=−θ˙r^=−ωr^
Velocity in Polar Coordinates
Position vector: r=rr^
Velocity:
v=dtdr=dtdrr^+rdtdr^
v=r˙r^+rθ˙θ^
Radial component:vr=r˙
Tangential component:vθ=rθ˙=rω
Speed:v=vr2+vθ2=r˙2+r2θ˙2
Acceleration in Polar Coordinates
a=dtdv=dtd(r˙r^+rθ˙θ^)
After applying product rule and substituting unit vector derivatives:
a=(r¨−rθ˙2)r^+(rθ¨+2r˙θ˙)θ^
Radial component:ar=r¨−rω2
Tangential component:aθ=rα+2r˙ω
where α=θ¨ is angular acceleration.
Circular Motion (r = constant)
When radius is constant (r˙=0, r¨=0):
Radial acceleration (centripetal):ar=−rω2=−rv2
Tangential acceleration:aθ=rα=rdtdω
The negative sign in ar indicates the acceleration points toward the center (opposite to r^).
Non-Uniform Circular Motion
When speed changes: both centripetal and tangential acceleration exist.
Centripetal: changes direction of velocity
Tangential: changes magnitude of velocity
Total acceleration magnitude:
a=ac2+at2=(rv2)2+(rα)
Example: Spiral Motion
A particle moves in a spiral: r(t)=bt, θ(t)=ωt (both constant b and ω)
Position:r=btr^
Velocity:v=br^+btωθ^
Acceleration:a=−btω2r^+2bωθ^
Notice the 2r˙ω term (Coriolis-like term) appears even though α=0.