Obtain the speed and acceleration of a body moving in a plane in polar coordinates.
Problem diagram:
In polar coordinates, a point on a trajectory is described by a vector position r making an angle
θ with the x-axis. At the considered point, the direction of the position vector, and the
variation of the angle are given by the unit vectors êr and
êθ.
Figure 1
Solution
The position vector in polar coordinates is given by
When the body moves over the trajectory in a time interval, the unit vectors in polar coordinates also
change position. This means these vectors are not constant in space (their direction changes
point-to-point in the trajectory - Figure 2).
Figure 2
Differentiation of \( r\;{\mathbf{ê}}_{r} \)
Differentiating the product of functions in the form
\[
(uv)' = u' v+u v'
\]
where
\( u=r \)
and
\( v={\mathbf{ê}}_{r} \),
\( u'=\dfrac{dr}{dt} \)
and
\( v'=\dfrac{d{\mathbf{ê}}_{r}}{dt} \)
Interpretation of the terms
\( \dfrac{d{\mathbf{ê}}_{r}}{dt} \)
and
\( \dfrac{d{\mathbf{ê}}_{\theta}}{dt} \)
1stº method
When the body undergoes an infinitesimal displacement dθ, the unit vector in the radial
direction moves from êr1 to êr2, and the
infinitesimal displacement vector will be (Figure 3)
When the body undergoes an infinitesimal displacement dθ the unit vector in the angular direction
moves from êθ1 to êθ2, and the infinitesimal
displacement vector will be (Figure 4)
The position of the unit vectors êr and êθ change with
the value of the angle θ and the angle changes over time, so êr and
êθ are composite functions of the type
If we decompose the unit vectors êr and êθ from the
polar coordinate system in directions i and j of the cartesian coordinate system, we
can write (Figure 5)
for this dot product scalar to be equal to zero the vector
\( \left(\frac{d{\mathbf{ê}}_{r}}{d\theta}\right) \),
it should be perpendicular to the vector êr, remembering that
\( \sin \frac{\pi}{2}=0 \),
therefore it is in the same direction as the vector êθ, and by Figure 3
it is positive
for this dot product scalar to be equal to zero the vector
\( \left(\frac{d{\mathbf{ê}}_{\theta}}{d\theta}\right) \),
it should be perpendicular to the vector êθ, remembering that
\( \sin \frac{\pi}{2}=0 \),
therefore it is in the same direction as the vector êr, and by Figure 3
it is negative
Note: Do not confuse
\( \frac{d}{dt}\left(\frac{d\theta}{dt}\right)=\frac{d^{2}\theta}{dt^{2}} \)
with
\( \frac{d\theta}{dt}\frac{d\theta}{dt}=\left(\frac{d\theta}{dt}\right)^{2} \),
in the first case the second derivative of the angular displacement with respect to time represents the
angular acceleration (γ), in the second case the first derivative of the angular displacement
with respect to time represents the angular velocity (ω) square, it is the angular velocity
squared (ω2).