Step 1: The source is isotropic, so the intensity at any point on the hemisphere (all at distance \(r\)) is \(I = \dfrac{W}{4\pi r^2}\). Because every ray leaves the centre radially, it strikes the spherical surface at normal incidence.
Step 2: For a perfectly reflecting surface at normal incidence, the radiation pressure is \(P = \dfrac{2I}{c}\), directed along the outward normal (the radial direction).
Step 3: By symmetry only the component along the axis of the hemisphere survives. Taking a surface element \(dA = r^2\sin\theta\, d\theta\, d\phi\) at polar angle \(\theta\), its axial force is \(dF_z = \dfrac{2I}{c}\cos\theta\, dA\).
Step 4: Integrate over the hemisphere (\(0\le\theta\le\tfrac{\pi}{2}\), \(0\le\phi\le 2\pi\)):
\[F = \frac{2}{c}\cdot\frac{W}{4\pi r^2}\int_0^{2\pi}\!\!d\phi\int_0^{\pi/2}\!\!\cos\theta\sin\theta\, r^2\, d\theta\]
\[F = \frac{2W}{4\pi c}\,(2\pi)\left(\tfrac{1}{2}\right) = \frac{W}{2c}\]
Step 5: Hence the force on the hemisphere is
\[\boxed{F = \dfrac{W}{2c}}\]