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Diameter of the objective of a telescope...

Diameter of the objective of a telescope is 200cm. What is the resolving power of a telescope? Take wavelength of light =5000Å.

A

`6.56xx10^(6)`

B

`3.28xx10^(5)`

C

`1xx10^(6)`

D

`3.28xx10^(6)`

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The correct Answer is:
To find the resolving power of a telescope, we can use the formula: \[ R = \frac{D}{1.22 \lambda} \] where: - \( R \) is the resolving power, - \( D \) is the diameter of the telescope's objective, - \( \lambda \) is the wavelength of light. ### Step 1: Convert the diameter from centimeters to meters. Given: - Diameter \( D = 200 \) cm To convert centimeters to meters: \[ D = 200 \, \text{cm} \times \frac{1 \, \text{m}}{100 \, \text{cm}} = 2 \, \text{m} \] ### Step 2: Convert the wavelength from angstroms to meters. Given: - Wavelength \( \lambda = 5000 \) Å To convert angstroms to meters: \[ \lambda = 5000 \, \text{Å} \times \frac{1 \times 10^{-10} \, \text{m}}{1 \, \text{Å}} = 5000 \times 10^{-10} \, \text{m} = 5 \times 10^{-7} \, \text{m} \] ### Step 3: Substitute the values into the resolving power formula. Now substituting \( D \) and \( \lambda \) into the formula: \[ R = \frac{2 \, \text{m}}{1.22 \times 5 \times 10^{-7} \, \text{m}} \] ### Step 4: Calculate the denominator. Calculating the denominator: \[ 1.22 \times 5 = 6.1 \] Thus, the denominator becomes: \[ 6.1 \times 10^{-7} \, \text{m} \] ### Step 5: Calculate the resolving power. Now substituting back into the formula: \[ R = \frac{2}{6.1 \times 10^{-7}} = \frac{2}{6.1} \times 10^{7} \] Calculating \( \frac{2}{6.1} \): \[ \frac{2}{6.1} \approx 0.328 \] Thus: \[ R \approx 0.328 \times 10^{7} \approx 3.28 \times 10^{6} \] ### Final Answer: The resolving power of the telescope is approximately \( 3.28 \times 10^{6} \). ---

To find the resolving power of a telescope, we can use the formula: \[ R = \frac{D}{1.22 \lambda} \] where: - \( R \) is the resolving power, ...
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