Step 1: Concept (Fresnel Distance):
The distance up to which ray optics is a good approximation is called the Fresnel distance ($Z_F$).
Formula: $Z_F = \frac{a^2}{\lambda}$
where $a$ is the aperture size and $\lambda$ is the wavelength.
Step 2: Calculation:
Given $Z_F = 50\,\mathrm{m}$, $a = 5 \times 10^{-3}\,\mathrm{m}$.
\[ 50 = \frac{(5 \times 10^{-3})^2}{\lambda} \]
\[ \lambda = \frac{25 \times 10^{-6}}{50} \]
\[ \lambda = 0.5 \times 10^{-6}\,\mathrm{m} = 5 \times 10^{-7}\,\mathrm{m} \]
Step 3: Convert to Angstroms:
$1\,\mathring{A} = 10^{-10}\,\mathrm{m}$.
\[ \lambda = 5000 \times 10^{-10}\,\mathrm{m} = 5000\,\mathring{A} \]