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
A particle is moving in a straight line. The variation of position $ x $ as a function of time $ t $ is given as:
$ x = t^3 - 6t^2 + 20t + 15 $.
The velocity of the body when its acceleration becomes zero is:
Evaluate the following limit: $ \lim_{n \to \infty} \prod_{r=3}^n \frac{r^3 - 8}{r^3 + 8} $.
In the given cycle ABCDA, the heat required for an ideal monoatomic gas will be: