To determine the minimum separation between objects on the surface of the moon that can be resolved by the telescope, we need to use the Rayleigh criterion. The Rayleigh criterion for a circular aperture states that two point sources are just resolvable when the following condition is met:
\(\theta = 1.22 \frac{\lambda}{D}\)
where:
For this problem:
First, calculate the angular resolution:
\(\theta = 1.22 \frac{5500 \times 10^{-10}}{5}\)
Calculating this gives:
\(\theta \approx 1.22 \times 1.1 \times 10^{-6} \, rad\)
The minimum resolvable separation on the moon's surface, s, is then found using:
s = \theta \times R
where R is the distance to the moon:
Substitute the values into the formula:
s = 1.22 \times 1.1 \times 10^{-6} \times 4 \times 10^8 \, m
Calculating this gives:
s \approx 60 \, m
Thus, the minimum separation between objects on the surface of the moon, so that they are just resolved by this telescope, is 60 m.