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When a telescope is in normal adjusment,...

When a telescope is in normal adjusment, the distance of the objective from the eyepiece is found to `100 cm`. If the magnifying power of the telescope, at normal adjusment, is `24` focal lengths of the lenses are

A

96 cm, 4 cm

B

48 cm, 2 cm

C

50 cm, 50 cm

D

80 cm, 20 cm

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To find the focal lengths of the objective and eyepiece of a telescope in normal adjustment, we can follow these steps: ### Step 1: Understand the relationship between the focal lengths and the distance between the lenses. In a telescope in normal adjustment, the distance between the objective lens and the eyepiece lens (denoted as \( D \)) is equal to the sum of their focal lengths: \[ D = f_o + f_e \] where \( f_o \) is the focal length of the objective lens and \( f_e \) is the focal length of the eyepiece lens. ### Step 2: Use the given information. From the problem, we know: - \( D = 100 \, \text{cm} \) - The magnifying power \( M \) of the telescope is given by the formula: \[ M = \frac{f_o}{f_e} \] Given that \( M = 24 \), we can set up the equation: \[ 24 = \frac{f_o}{f_e} \] ### Step 3: Express \( f_o \) in terms of \( f_e \). From the magnifying power equation, we can express \( f_o \) as: \[ f_o = 24 f_e \] ### Step 4: Substitute \( f_o \) into the distance equation. Now we substitute \( f_o \) into the distance equation: \[ 100 = 24 f_e + f_e \] This simplifies to: \[ 100 = 25 f_e \] ### Step 5: Solve for \( f_e \). Now, we can solve for \( f_e \): \[ f_e = \frac{100}{25} = 4 \, \text{cm} \] ### Step 6: Find \( f_o \). Now that we have \( f_e \), we can find \( f_o \): \[ f_o = 24 f_e = 24 \times 4 = 96 \, \text{cm} \] ### Final Result: Thus, the focal lengths of the lenses are: - Focal length of the objective lens, \( f_o = 96 \, \text{cm} \) - Focal length of the eyepiece lens, \( f_e = 4 \, \text{cm} \) ---

To find the focal lengths of the objective and eyepiece of a telescope in normal adjustment, we can follow these steps: ### Step 1: Understand the relationship between the focal lengths and the distance between the lenses. In a telescope in normal adjustment, the distance between the objective lens and the eyepiece lens (denoted as \( D \)) is equal to the sum of their focal lengths: \[ D = f_o + f_e \] where \( f_o \) is the focal length of the objective lens and \( f_e \) is the focal length of the eyepiece lens. ...
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