What follows is an at-least-in-principle-slightly more motivated way to prove the key result. (In reality I came here to see the solution after failing to solve the problem on an exam.) I ignore all questions of convergence of the improper integrals that follow, but they shouldn't cause any real problems.
Let $\Omega\subseteq\mathbb{R}^{2}$ be the open unit disk. It suffices to find a continuous, nonnegative "weight distribution" $w\ \colon \Omega\to\mathbb{R}_{\geq 0}$ such that $$\int_{p\ \in\ \ell\ \cap\ \Omega} w\left(p\right)\text{d}\ell\ =\ \frac{1}{2}$$ for any line $\ell\subseteq\mathbb{R}^{2}$ intersecting $\Omega$ and (thus) that $$\int\int_{p\ \in\ \Omega} w\left(p\right)\text{d}\Omega\ =\ 1.$$ Naturally, we should expect $w$ to be invariant of the rotational symmetries of $\Omega$ (at the very least, the symmetrization of any such $w$ shares the relevant properties, so we might as well assume as much), so what we seek is concretely a continuous function $\widetilde{w}\ \colon\left[0,1\right)\to\mathbb{R}_{\geq 0}$ (i.e., $w$ evaluated at a given radius) such that $$\int_{0}^{1} \sqrt{1-h^{2}}\cdot\widetilde{w}\left(\sqrt{h^{2}+\left(1-h^{2}\right)t^{2}}\right)\text{d}t\ =\ \frac{1}{4}.$$ The most obvious way to make this happen is to choose $\widetilde{w}$ so that the integrand is already independent of $h$. It's not hard to see that taking $$\widetilde{w}\left(r\right)\ \propto\ \frac{1}{\sqrt{1-r^{2}}}$$ achieves this ($\sqrt{1-h^{2}}$ factoring out and cancelling), and in particular when $$\widetilde{w}\left(r\right)\ :=\ \frac{1}{2\pi\sqrt{1-r^{2}}}$$ we have that $$\int_{0}^{1} \sqrt{1-h^{2}}\cdot\widetilde{w}\left(\sqrt{h^{2}+\left(1-h^{2}\right)t^{2}}\right)\text{d}t\ =\ \int_{0}^{1}\frac{1}{2\pi\sqrt{1-t^{2}}}\text{d}t\ =\ \frac{1}{4},$$ as desired. (And in fact, this $\widetilde{w}$ is, up to a constant factor, exactly the weight that is implicitly used in the argument that proceeds by projection onto the surface of the sphere bisected by the disk being covered.)
Ps.: Our $w$ ought to be something like the inverse Radon transform of the function on the space of lines in $\mathbb{R}^{2}$ that is $\tfrac{1}{2}$ at the lines intersecting $\Omega$ and $0$ everywhere elese. Someone more proficient in the Radon transform than I might be able to make that concrete...