
(ii) Advantages :
(a) Parabolic mirror is used to remove the spherical aberration.
(b) No chromatic aberration in mirror.
(c) Light mechanical support is required, because mirror weighs much less than a lens of equivalent optical quality.
(iii) In normal adjustment, magnifying power of the telescope M = F0/Fe.
(a) If focal length of the objecctive lens is large in comparison to the eyepiece, magnifying power increases.
(b) Resolving power of the telescope RP = a/1.22λ. To increase the resolving power of the telescope, large aperture of the objective lens is required.