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A binary star system is observed using a...

A binary star system is observed using a telescope. The angular separation between both the stars is `5 xx 10^(-6)` radians. Calculate the aperture of objective of the telescope if light of wavelength `5,500 Å` is used.

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To solve the problem of calculating the aperture of the objective of the telescope observing a binary star system, we will use the formula for angular resolution of a telescope. The formula is given by: \[ \theta = \frac{1.22 \lambda}{D} \] Where: - \(\theta\) is the angular separation in radians, - \(\lambda\) is the wavelength of light used (in meters), - \(D\) is the aperture of the telescope (in meters). ### Step 1: Identify the given values - Angular separation, \(\theta = 5 \times 10^{-6}\) radians - Wavelength, \(\lambda = 5500 \, \text{Å} = 5500 \times 10^{-10} \, \text{m}\) ### Step 2: Rearrange the formula to solve for \(D\) We need to rearrange the formula to find \(D\): \[ D = \frac{1.22 \lambda}{\theta} \] ### Step 3: Substitute the values into the formula Now we will substitute the values of \(\lambda\) and \(\theta\) into the rearranged formula: \[ D = \frac{1.22 \times (5500 \times 10^{-10})}{5 \times 10^{-6}} \] ### Step 4: Calculate \(D\) Now we will perform the calculation step-by-step: 1. Calculate \(\lambda\): \[ \lambda = 5500 \times 10^{-10} = 5.5 \times 10^{-7} \, \text{m} \] 2. Substitute \(\lambda\) into the equation: \[ D = \frac{1.22 \times 5.5 \times 10^{-7}}{5 \times 10^{-6}} \] 3. Calculate the numerator: \[ 1.22 \times 5.5 = 6.71 \times 10^{-7} \] 4. Now divide by \(\theta\): \[ D = \frac{6.71 \times 10^{-7}}{5 \times 10^{-6}} = 1.342 \times 10^{-1} = 0.1342 \, \text{m} \] ### Step 5: Convert to centimeters To convert meters to centimeters: \[ D = 0.1342 \, \text{m} \times 100 = 13.42 \, \text{cm} \] ### Final Answer The aperture of the objective of the telescope is \(13.42 \, \text{cm}\). ---
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