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The magnification by a simple microscope of focal length $f$ is given by \begin{align} m=\frac{D}{f}, \end{align} where $D=25$ cm is the distant of distinct vision. This condition is called normal adjustment of the simple microscope.
A compound microscope has an objective of focal length $f_o$ and an eyepiece of focal length $f_e$. The image is formed at infinity in normal adjustment. The magnification of a compund microscope is given by \begin{align} m=\frac{v}{u}\frac{D}{f_e} \end{align}
The resolving power of a compund microscope is given by \begin{align} R=\frac{1}{\Delta d}=\frac{2\mu\sin\theta}{\lambda} \end{align}
An astronomical telesocpe has an objective of focal length $f_o$ and an eyepiece of focal length $f_e$. In normal adjustment, the length of the telescope is given by \begin{align} L=f_o+f_e, \end{align} and its magnification is \begin{align} m=-\frac{f_o}{f_e} \end{align}
The resolving power of a telescope for light of wavelength $\lambda$ is given by \begin{align} R=\frac{1}{\Delta \theta}=\frac{1}{1.22\lambda}. \end{align}