For the disc to leave the surface of the hemisphere, the normal force must become zero at the point of leaving. Using the conservation of mechanical energy and Newton's laws, we can set the centripetal force required to keep the disc on the hemisphere equal to the gravitational component acting perpendicular to the surface at the point of leaving, which is at the very top of the hemisphere.
The required velocity \( V \) for this to occur can be calculated by setting the gravitational force \( mg \) equal to the required centripetal force \( \frac{mV^2}{R} \) at the top, where \( m \) is the mass of the disc: \[ mg = \frac{mV^2}{R} \Rightarrow V^2 = gR \Rightarrow V = \sqrt{gR} \]