To determine the limit of resolution of a telescope, we use the formula for the angular resolution (or resolving power) of a circular aperture, such as the objective lens of a telescope:
\(\theta_{\text{min}} = 1.22 \frac{\lambda}{D}\)
where:
Substitute the given values into the formula:
\(\theta_{\text{min}} = 1.22 \frac{600 \times 10^{-9} \, \text{m}}{2 \, \text{m}}\)
Calculate:
\(\theta_{\text{min}} = 1.22 \times 300 \times 10^{-9} \, \text{rad}\)
\(\theta_{\text{min}} = 3.66 \times 10^{-7} \, \text{rad}\)
Thus, the limit of resolution of the telescope is \(3.66 \times 10^{-7} \, \text{rad}\).
Therefore, the correct answer is:
\(3.66 \times 10^{-7} \, \text{rad}\)
This option matches with:
\(3.66 \times 10^{-7} \, \text{rad}\)