Define the term 'resolving power' of an astronomical telescope. How does it get
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The resolving power of an astronomical telescope is defined as the
reciprocal of the smallest angular separation between two point objects whose
images can just be resolved by the telescope.
R.P. = 1.22λ / D
reciprocal of the smallest angular separation between two point objects whose
images can just be resolved by the telescope.
R.P. = 1.22λ / D
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Resolving power of a telescope is its ability to see two very closely object just seperate.
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