Step 1: Recall the formula for the rate of precession of a Foucault pendulum.
The angular speed \(\omega_P\) of the precession of the plane of oscillation is given by:
\[ \omega_P = \Omega \sin\phi \]
where \(\Omega\) is the angular speed of the Earth's rotation, and \(\phi\) is the latitude of the pendulum's location.
Step 2: Find the condition for no rotation.
For the plane of vibration to not rotate at all, the rate of precession \(\omega_P\) must be zero.
\[ \Omega \sin\phi = 0 \]
Step 3: Solve for the latitude \(\phi\).
Since the Earth is rotating, \(\Omega \neq 0\). Therefore, we must have:
\[ \sin\phi = 0 \]
This condition is met when the latitude \(\phi = 0^{\circ}\).
Step 4: Identify the geographical location corresponding to this latitude.
A latitude of \(0^{\circ}\) corresponds to the Earth's Equator. At the North or South Pole, \(\phi = \pm 90^{\circ}\), \(\sin\phi = \pm 1\), and the rotation is maximum.