In the first example of Figure 6.1.1, consider the ant in motion relative to turntable \(\cF = (O,\bef_1,\bef_2,\bef_3)\text{.}\) Assume that \(\cF\) is in rotation about axis \((O,\bef_3)\) relative to referential \(\cE\text{.}\)
Find the “absolute” velocity and acceleration of point \(A\) from its “relative” velocity and acceleration, given that \(\br_{OA} = \rho(t) \bef_1\) where \(\bef_1\) is a unit vector attached to \(\cF\text{.}\) Assume that \(\bom_{\cF/\cE}=\om (t) \bef_3\text{.}\)
Solution.
The motion of \(\cF\) relative to \(\cE\) is a rotation about axis \((O, \bef_3)\text{.}\) We denote \(\bef_2 = \bef_3 \times \bef_1\text{.}\) The relative velocity and acceleration of point \(A\) are easily found to be
\begin{equation*}
\vel_{A / \cF} = \left( {d \over dt}\br_{OA} \right)_{\cF}= \dro\, \bef_1 ,
\qquad \ba_{A /\cF} =\left( {d \over dt}\vel_{A / \cF} \right)_{\cF}
= \ddro \,\bef_1
\end{equation*}
The transport velocity and acceleration are found by considering the coinciding point \(A(t) \in \cF\) whose motion is instantaneously that of a point in rotation with \(\cF\) about axis \((O, \bef_3)\text{:}\)
\begin{align*}
\vel_{A\in\cF / \cE} \amp = \bom_{\cF/\cE}\times\br_{OA} = \om \bef_3 \times
\rho \bef_1 = \ro \om \bef_2, \\
\ba_{A\in\cF / \cE} \amp = \bal_{\cF/\cE}\times\br_{OA}+ \bom_{\cF/\cE}\times
(\bom_{\cF/\cE}\times\br_{OA})
=\ro \dom \bef_2 - \ro \om^2 \bef_1
\end{align*}
The Coriolis acceleration of \(A\) is given by
\begin{equation*}
2 \bom_{\cF/\cE}\times\vel_{A/\cF} =
2 \om \bef_3 \times \dro\, \bef_1 = 2 \om\dro \bef_2
\end{equation*}
We can now apply formulas (6.2.1)-(6.3.2) to find the absolute velocity and acceleration of \(A\text{:}\)
\begin{equation*}
\vel_{A/\cE} = \vel_{A/\cF} + \vel_{A\in \cF / \cE} = \dro\, \bef_1 +
\ro \om \bef_2
\end{equation*}
\begin{equation*}
\ba_{A/\cE} = \ba_{A/\cF} + \ba_{A\in\cF / \cE} +
2 \bom_{\cF/\cE}\times\vel_{A/\cF}=
\ddro \,\bef_1 +(\ro \dom \bef_2 - \ro \om^2 \bef_1)+2 \om\dro \bef_2
\end{equation*}
or
\begin{equation*}
\ba_{A/\cE} = (\ddro - \ro \om^2 ) \bef_1 + (\ro \dom +2 \om\dro ) \bef_2
\end{equation*}
These results can be obtained much more efficiently by taking two consecutive time-derivatives of vector \(\ro (t) \bef_1\) relative to \(\cE\text{,}\) or by using the polar coordinates \((\ro, \te)\) (with \(\dte=\om\)) of \(A\text{.}\)