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