Two refracting telescopes are used to look at craters on the Moon. The objective focal length of both telescopes is \(95.0 \mathrm{~cm}\) and the eyepiece focal length of both telescopes is \(3.80 \mathrm{~cm} .\) The telescopes are identical except for the diameter of the lenses. Telescope A has an objective diameter of \(10.0 \mathrm{~cm}\) while the lenses of telescope \(\mathrm{B}\) are scaled up by a factor of two, so that its objective diameter is \(20.0 \mathrm{~cm}\). a) What are the angular magnifications of telescopes \(A\) and \(B\) ? b) Do the images produced by the telescopes have the same brightness? If not, which is brighter and by how much?

Short Answer

Expert verified
How does the brightness of the images produced by the telescopes compare? Answer: Yes, telescopes A and B have the same angular magnification of 25. However, the images produced by telescope B are 4 times brighter, as telescope B collects 4 times more light than telescope A due to its larger objective lens diameter.

Step by step solution

01

Calculate angular magnification for telescopes A and B

Using the angular magnification formula, we can calculate the angular magnification for each telescope. Since both telescopes have the same focal lengths, we expect them to have the same magnification. \(f_{objective} = 95.0\,\text{cm}\) \(f_{eyepiece} = 3.80\,\text{cm}\) Angular Magnification = \(\frac{f_{objective}}{f_{eyepiece}} = \frac{95}{3.8}\) Calculating the ratio, we get: Angular Magnification = \(25\) So, the angular magnifications of telescopes A and B are \(25\). #b)
02

Calculate the light-gathering power for telescopes A and B

Now, we will calculate the light-gathering power for each telescope, which is proportional to the area of the objective lens. For telescope A: \(d_A = 10.0\,\text{cm}\) Area \(A = \pi(\frac{d_A}{2})^2\) For telescope B: \(d_B = 20.0\,\text{cm}\) Area \(B = \pi(\frac{d_B}{2})^2\)
03

Compare the light-gathering power and brightness

Now, we compare the area of telescopes A and B: \(\frac{\text{Area B}}{\text{Area A}} = \frac{\pi(\frac{d_B}{2})^2}{\pi(\frac{d_A}{2})^2} = \frac{(\frac{d_B}{2})^2}{(\frac{d_A}{2})^2} = (\frac{d_B}{d_A})^2\) Because \(d_B = 2d_A\), substituting into the equation gives: \(\frac{\text{Area B}}{\text{Area A}} = (2)^2 = 4\) Thus, telescope B collects 4 times more light than telescope A, and the images produced by telescope B are 4 times brighter.

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