Step 1: Understanding Normal Adjustment in Refracting Telescope
In normal adjustment, the final image is formed at infinity. In this case, the distance between the objective lens and the eyepiece lens is the sum of their focal lengths:
\[
L = f_o + f_e
\]
Where:
- \( L = 30 \, \text{cm} \) (given)
- \( f_o \) = focal length of objective
- \( f_e \) = focal length of eyepiece
Step 2: Angular Magnification Formula
The angular magnification \( M \) of a telescope in normal adjustment is given by:
\[
M = \frac{f_o}{f_e}
\]
Given: \( M = 2 \)
Step 3: Substituting Values
\[
\frac{f_o}{f_e} = 2 \quad \Rightarrow \quad f_o = 2f_e
\]
Now use this in the total length formula:
\[
f_o + f_e = 30 \Rightarrow 2f_e + f_e = 30 \Rightarrow 3f_e = 30 \Rightarrow f_e = 10 \, \text{cm}
\]
\[
\therefore f_o = 2 \times 10 = 20 \, \text{cm}
\]
Step 4: Final Answer
\[
\boxed{f_o = 20 \, \text{cm}}
\]
So the correct answer is: Option 1: 20 cm
The stopping potential (\(V_0\)) versus frequency (\(\nu\)) of a graph for the photoelectric effect in a metal is given. From the graph, the Planck's constant (\(h\)) is:

In the diagram shown below, both the strings AB and CD are made of the same material and have the same cross-section. The pulleys are light and frictionless. If the speed of the wave in string AB is \( v_1 \) and in CD is \( v_2 \), then the ratio \( \frac{v_1}{v_2} \) is:
