(a) (i) There is no chromatic aberration as the objective is a mirror.
(ii) Spherical aberration is reduced using mirror objective in the form of a paraboloid.
(iii) Image is brighter compared to that in a refractine telescope.
(iv) Mirror requires griding and polishing of only one side.
(v) High resolution is resolution is achieved by using a mirror of large aperture (b) Here, `R = 80 cm`.
`f_(0) = (R )/(2) = (80)/(2) = 40 cm`
and `f_(e) = 1.6 cm`.
As magnifying power, `m = (f_(0))/(f_(e))`
`:. m = (40)/(1.6) = 25`