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Draw a ray diagram for a Cassegrain telescope - AQA - A-Level Physics - Question 1 - 2020 - Paper 4

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Draw a ray diagram for a Cassegrain telescope. Your diagram should show the paths of two rays up to the eyepiece lens. The rays should initially be parallel to the ... show full transcript

Worked Solution & Example Answer:Draw a ray diagram for a Cassegrain telescope - AQA - A-Level Physics - Question 1 - 2020 - Paper 4

Step 1

Draw a ray diagram for a Cassegrain telescope.

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Answer

To draw a ray diagram for a Cassegrain telescope:

  1. Start with a concave primary mirror, which is shaped like a U.
  2. Place a convex secondary mirror in front of the primary mirror, positioned to reflect light toward the eyepiece.
  3. Illustrate two rays coming in parallel to the principal axis:
    • One ray strikes the primary mirror and reflects toward the secondary mirror, which then directs it toward the eyepiece.
    • The second ray strikes the secondary mirror directly and follows the same path toward the eyepiece.
  4. Ensure that both mirrors are labeled and the path of the rays is clear.

Step 2

Discuss whether this telescope is suitable for studying a crater with a diameter of approximately 1 km on Pluto.

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Answer

To evaluate if the telescope on the spacecraft is suitable for studying a crater of 1 km diameter on Pluto:

  1. Calculate the resolution capability of the telescope using the formula: Resolution=1.22⋅λDResolution = \frac{1.22 \cdot \lambda}{D} Where (\lambda) is the wavelength (450 nm) and (D) is the aperture diameter (0.21 m).
  2. Substitute the values: Resolution=1.22⋅450×10−90.21≈2.14×10−6mResolution = \frac{1.22 \cdot 450 \times 10^{-9}}{0.21} \approx 2.14 \times 10^{-6} m
  3. Convert the resolution into kilometers, which is approximately 0.00000214 km or 2.14 meters.
  4. The smallest detail the telescope can resolve is about 2.14 meters, which means it can effectively study features larger than this. Since 1 km is significantly larger than 2.14 meters, the telescope is suitable for observing the crater.

Step 3

Compare the collecting power of the Hubble telescope with the telescope on the spacecraft in Question 01.2.

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Answer

To compare the collecting power between the Hubble telescope and the spacecraft telescope:

  1. Use the formula for collecting power, which is proportional to the area of the aperture: A=Ï€(D2)2A = \pi \left( \frac{D}{2} \right)^2
  2. For the Hubble telescope (diameter 2.4 m): AH=π(2.42)2≈4.52m2A_H = \pi \left( \frac{2.4}{2} \right)^2 \approx 4.52 m^2
  3. For the spacecraft telescope (diameter 0.21 m): AS=π(0.212)2≈0.0346m2A_S = \pi \left( \frac{0.21}{2} \right)^2 \approx 0.0346 m^2
  4. Calculate the ratio of their collecting powers: Ratio=AHAS=4.520.0346≈130\text{Ratio} = \frac{A_H}{A_S} = \frac{4.52}{0.0346} \approx 130
  5. This indicates that the Hubble telescope has a collecting power about 130 times greater than the telescope on the spacecraft.

Step 4

Discuss which type of telescope to use.

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Answer

To decide between a reflecting or refracting telescope for the spacecraft:

  1. Reflecting Telescopes are generally preferred for larger apertures, as they avoid chromatic aberration and can be built larger without significantly increasing weight.
  2. Refracting Telescopes can be simpler for smaller apertures but suffer from chromatic aberration, which can distort images.
  3. Given that the telescope must operate in space, where light scattering is less of a problem and higher precision is required, a reflecting telescope is more suitable. Its design will allow for clearer images without distortion, making it the better option for observing features on Pluto.

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