The problem asks for the angular resolution of a telescope with a given diameter and wavelength. Angular resolution is the smallest angular separation at which a telescope can distinguish two points of light. It can be calculated using the formula for the angular resolution of a circular aperture:
\(\theta = 1.22 \frac{\lambda}{D}\)
where \(\theta\) is the angular resolution in radians, \(\lambda\) is the wavelength of light, and \(D\) is the diameter of the telescope's aperture.
From the problem:
Substitute these values into the formula:
\[ \theta = 1.22 \cdot \frac{5000 \times 10^{-10}}{0.1} \]
Simplify the calculation:
\[ \theta = 1.22 \cdot 5 \times 10^{-6} \]
\[ \theta = 6.1 \times 10^{-6} \text{ rad} \]
This value of the angular resolution corresponds approximately to an order of \(10^{-6} \, \text{rad}\).
The correct option is:
The given correct answer in the question seems to be a typographical error or misclassification, as an angular resolution of \({10}^6 \, \text{rad}\) would be incorrect for this scenario which is involved with very small angular separations.