(a)
From the figure,
$$ u=\frac{y}{\left|f_{1}\right|} \text { and } u^{\prime}=\frac{y}{\left|f_{2}\right|} $$
The angular magnification is defined as the ratio of image distance to the object. \(M=\frac{u^{\prime}}{u}=-\frac{f_{1}}{f_{2}}\)
The negative sign for a convex lens, because it inverts the image.
(b)
Calculate the focal length as follows:
\(f_{2}=-\frac{f_{1}}{M}=-\frac{95 \mathrm{~cm}}{6.33}=-15 \mathrm{~cm}\)
(c)
For Galilean telescope, \(L_{0}=f_{1}-f_{2}\)
For astronomical telescope, \(L=f_{1}+f_{2}\)
Compare the telescopes as follows:
\(\frac{L}{L_{0}}=\frac{f_{1}+f_{2}}{f_{1}-f_{2}}=\frac{95 \mathrm{~cm}+15 \mathrm{~cm}}{95 \mathrm{~cm}-15 \mathrm{~cm}}=\frac{110 \mathrm{~cm}}{80 \mathrm{~cm}}=1.38\)
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