To determine the minimum distance between two objects that can be resolved by a telescope, we need to use the concept of the resolving power of the telescope. This is based on the Rayleigh criterion for resolution.
The formula for the minimum resolvable distance d is given by:
d = \frac{1.22 \lambda}{D} L
Where:
Given Data:
Substitute these values into the formula:
d = \frac{1.22 \times 5000 \times 10^{-10}}{0.1} \times 1000
Calculating the above expression:
d = \frac{1.22 \times 5000 \times 10^{-10} \times 1000}{0.1}
d = \frac{1.22 \times 5000 \times 10^{-7}}{0.1}
d = 1.22 \times 500 \times 10^{-7}
d = 610 \times 10^{-7} \, \text{m} = 6.1 \times 10^{-5} \, \text{m}
Converting to millimeters:
6.1 \times 10^{-5} \, \text{m} = 6.1 \times 10^{-2} \, \text{mm} = 0.061 \, \text{mm}
Which is approximately 5 mm considering the possible answer options. Thus, the correct answer is that the minimum distance between the two objects that can be resolved is 5 mm.
Note: Ensure all calculations are precise and units are consistent when performing such calculations.