A car runs on a banked curve with radius
R and slope
θ. What will be the maximum speed to
negotiate the curve without friction?
Problem data:
- Radius of the curve: R;
- Curve slope: θ.
Problem diagram:
Figure 1 -
Banked curve in the old AVUS autodrome in Berlin, Germany.
The forces that act in the car are the gravitational force
\({\vec F}_{g} \)
pointing vertically down, the normal reaction force
\( \vec{N} \)
perpendicularly to the track (Figure 1).
Solution
The bank angle of the track is
θ, the gravitational force
\({\vec F}_{g} \)
is perpendicular to the horizontal plane, makes an angle of 90°, as the sum of the interior angles of a
triangle equals to 180°, the angle between the gravitational force
\({\vec F}_{g} \)
and the banked lane (Figure 2-A)
\[ \alpha +\theta +90°=180° \Rightarrow \alpha =180°-90°-\theta \Rightarrow \alpha =90°-\theta \]
The angle between the banked curve and horizontal plane is
θ, and the angle between the centripetal
force
\({\vec F}_{cp} \)
and the horizontal is also
θ, are alternate angles (Figure 2-B).
The angle between the normal reaction force
\(\vec{N} \)
and the centripetal force
\({\vec F}_{cp} \)
is
α (Figure 2-C), and the angle between the normal force and the vertical axis is
θ,
\( \alpha +\theta =90° \)
(Figure 2-D). This angle will be used to decompose the normal force (Figure 3).
Drawing the forces in a coordinate system
xy, we can apply
Newton's Second Law for
circular motion
\[
\begin{gather}
\bbox[#99CCFF,10px]
{{\vec F}_{cp}=m{\vec a}_{cp}} \tag{I}
\end{gather}
\]
In the
x direction, the centripetal force
\( {\vec F}_{cp} \)
is given by the component of normal force in the
x direction,
\( {\vec N}_{x} \)
(Figure 3)
\[
\begin{gather}
F_{cp}=N_{x} \tag{II}
\end{gather}
\]
The
Nx component is given by
\[
\begin{gather}
N_{x}=N\sin \theta \tag{III}
\end{gather}
\]
The centripetal acceleration is given by
\[
\begin{gather}
\bbox[#99CCFF,10px]
{a_{cp}=\frac{v^{2}}{R}} \tag{IV}
\end{gather}
\]
Substituting expressions (III) and (IV) into expression (I)
\[
\begin{gather}
N\sin \theta =m\frac{v^{2}}{R} \tag{V}
\end{gather}
\]
In the
y direction, there is no motion, the gravitational force and the component of the normal force
in
y direction cancel out
\[
\begin{gather}
F_{g}=N_{y} \tag{VI}
\end{gather}
\]
The gravitational force is given by
\[
\begin{gather}
\bbox[#99CCFF,10px]
{F_{g}=mg} \tag{VII}
\end{gather}
\]
The component
Ny is given by
\[
\begin{gather}
N_{y}=N\cos \theta \tag{VIII}
\end{gather}
\]
Substituting the expressions (VII) and (VIII) into expression (VI)
\[
\begin{gather}
N\cos \theta =mg \tag{IX}
\end{gather}
\]
Equations (V) and (IX) can be written as a system of two equations.
\[
\left\{
\begin{array}{l}
N\sin \theta =m\dfrac{v^{2}}{R}\\
N\cos \theta=mg
\end{array}
\right.
\]
dividing the first equation by the second equation
\[
\begin{gather}
\frac{\cancel{N}\sin \theta }{\cancel{N}\cos \theta }=\frac{\cancel{m}\dfrac{v^{2}}{R}}{\cancel{m}g}
\end{gather}
\]
From the Trigonometry
\( \dfrac{\sin \theta }{\cos \theta} =\tan \theta \)
\[
\begin{gather}
\tan\theta =\frac{v^{2}}{Rg}\\[5pt]
v^{2}=Rg\tan\theta
\end{gather}
\]
\[
\begin{gather}
\bbox[#FFCCCC,10px]
{v=\sqrt{\;Rg\tan\theta \;}}
\end{gather}
\]