Working Principle:
An astronomical telescope is used to view distant celestial objects. It consists of two convex lenses:
When the final image is formed at infinity, the intermediate image formed by the objective lies at the focus of the eyepiece. The final image is then a virtual, magnified, and inverted image at infinity.
Magnifying Power (M):
For final image at infinity, \[ M = \frac{f_o}{f_e} \] where $f_o$ = focal length of objective, and $f_e$ = focal length of eyepiece.