To develop this problem it is necessary to apply the concepts related to the angular resolution of a telescope as well as to the arc length.
The arc length can be defined as

Where
r= Radius
\theta = Angle
At the same time the angular resolution of a body is given under the proportion

Where
= Wavelength
D = Diameter
Our values are given as



Then the angle of separation of the two objects seen from the observer is of


Finally, using the proportion of the arc length, in which we have the radius and angle we can know the separation of the two objects by:

