Velocity and Acceleration in Polar Coordinates
📂Classical MechanicsVelocity and Acceleration in Polar Coordinates
Velocity and Acceleration in Polar Coordinates
va=r˙r^+rθ˙θ^=(r¨−rθ˙2)r^+(2r˙θ˙+rθ¨)θ^
Derivation

In the polar coordinate system, unit vectors can be described as follows.
⟹rr^θ^=rr^=xx^+yy^=rxx^+ryy^=cosθx^+sinθy^=r^(θ)=r^(θ+π/2)=−sinθx^+cosθy^
Velocity is obtained by differentiating position with respect to time, and acceleration is obtained by differentiating velocity with respect to time. Note that r˙ is pronounced “dot”. In physics, a dot above a letter means differentiation with respect to time.
r˙=dtdr
Velocity
Differentiating r with respect to t gives the following.
v=dtdr=dtd(rr^)=dtdrr^+rdtdr^=r˙r^+rr^˙
Calculating r^˙, since x^ and y^ do not change over time, dtdx^=0 is true. Hence, it can be given as follows.
r^˙=dtd(r^)=dtd(cosθx^)+dtd(sinθy^)=dtcosθx^+dtsinθy^=dθcosθdtdθx^+dθsinθdtdθy^=−sinθdtdθx^+cosθdtdθy^=dtdθ(−sinθx^+cosθy^)=θ˙θ^
Therefore, the velocity in polar coordinates is as follows.
v=r˙r^+rθ˙θ^
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Acceleration
Differentiating v with respect to t gives the following.
a=dtdv=dtd(r˙r^+rθ˙θ^)=r¨r^+r˙r^˙+r˙θ˙θ^+rθ¨θ^+rθ˙θ^˙
Calculating θ^˙ gives the following result.
θ^˙=dtd(θ^)=dtd(−sinθx^)+dtd(cosθy^)=−dtdsinθx^+dtdcosθy^=−dθdsinθdtdθx^+dθdcosθdtdθy^=dtdθ(−cosθx^−sinθy^)=−θ˙r^
Since r^˙ was calculated when deriving velocity, substituting and organizing gives the following result.
a=r¨r^+r˙r^˙+r˙θ˙θ^+rθ¨θ^+rθ˙θ^˙=r¨r^+r˙θ˙θ^+r˙θ˙θ^+rθ¨θ^−rθ˙θ˙r^=(r¨−rθ˙2)r^+(2r˙θ˙+rθ¨)θ^
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See Also