29.
Solution:
Magnifying Power of Astronomical Telescope: It is the ratio of the angle subtended at the eye by the image to the angle subtended by the object at the unaided eye. $M = \frac{\beta}{\alpha}$.
Derivation (Final image at least distance of distinct vision, D):
The objective lens forms a real inverted image $A'B'$ of a distant object at its focus, so $OB' = f_{o}$. Angle $\alpha \approx \tan\alpha = \frac{A'B'}{f_{o}}$.
The eyepiece acts as a simple microscope. The image $A'B'$ acts as an object at distance $u_{e}$. Angle $\beta \approx \tan\beta = \frac{A'B'}{-u_{e}}$.
Magnifying power $M = \frac{\beta}{\alpha} = \frac{A'B' / (-u_{e})}{A'B' / f_{o}} = -\frac{f_{o}}{u_{e}}$.
For the eyepiece, applying the lens formula: $\frac{1}{v_{e}} - \frac{1}{u_{e}} = \frac{1}{f_{e}}$.
By sign convention, $v_{e} = -D$ and object distance is $-u_{e}$.
$\frac{1}{-D} - \frac{1}{-u_{e}} = \frac{1}{f_{e}} \implies \frac{1}{u_{e}} = \frac{1}{f_{e}} + \frac{1}{D} = \frac{1}{f_{e}}\left(1 + \frac{f_{e}}{D}\right)$.
Substitute into M: $M = -f_{o} \left[ \frac{1}{f_{e}}\left(1 + \frac{f_{e}}{D}\right) \right] = -\frac{f_{o}}{f_{e}} \left(1 + \frac{f_{e}}{D}\right)$.
OR
Solution (Alternative):
Refraction at Concave Spherical Surface (Rarer $\mu_1$ to Denser $\mu_2$):
Consider a point object O on the principal axis. A ray OA strikes the concave surface. Since it goes rarer to denser, it bends towards the normal CA, diverging away from the axis. It appears to come from virtual image I.
Let angles with principal axis be $\alpha$ (object), $\beta$ (image), $\gamma$ (normal).
In $\Delta OAC$, exterior angle $\gamma = \alpha + i \implies i = \gamma - \alpha$.
In $\Delta IAC$, exterior angle $\gamma = \beta + r \implies r = \gamma - \beta$.
By Snell's Law for small angles, $\mu_{1}i = \mu_{2}r$.
$\mu_{1}(\gamma - \alpha) = \mu_{2}(\gamma - \beta) \implies \mu_{2}\beta - \mu_{1}\alpha = (\mu_{2} - \mu_{1})\gamma$.
Using $\text{angle} = \text{arc/radius}$ (small aperture): $\alpha = \frac{AP}{PO}$, $\beta = \frac{AP}{PI}$, $\gamma = \frac{AP}{PC}$.
$\mu_{2}(\frac{AP}{PI}) - \mu_{1}(\frac{AP}{PO}) = (\mu_{2} - \mu_{1})(\frac{AP}{PC})$.
By sign convention: $PO = -u$, $PI = -v$, $PC = -R$.
$\mu_{2}(\frac{1}{-v}) - \mu_{1}(\frac{1}{-u}) = (\mu_{2} - \mu_{1})(\frac{1}{-R})$.
Multiplying by -1 yields: $-\frac{\mu_{1}}{u} + \frac{\mu_{2}}{v} = \frac{\mu_{2} - \mu_{1}}{R}$.