Astronomy Chapter 5 Quiz
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Questions and Answers

What is a primary reason astronomers conduct infrared astronomy from high-flying aircraft?

  • Infrared radiation is more effectively gathered at higher altitudes.
  • High altitude provides a wider range of infrared wavelengths.
  • Infrared observations do not require a clear line of sight.
  • It allows the infrared telescope to operate above dense areas of air. (correct)
  • Why is it beneficial for optical telescopes to be built on mountain tops?

  • To minimize light pollution from the city.
  • To improve accessibility for researchers.
  • To reduce the amount of light that reaches the telescope.
  • To take advantage of thinner air, which improves seeing conditions. (correct)
  • Which factor does NOT contribute to the limitations of observing infrared radiation from the ground?

  • Humidity levels affecting light transmission.
  • Atmospheric absorption of infrared radiation.
  • Scattered light from nearby stars. (correct)
  • The thermal noise from Earth's surface.
  • What technique can astronomers employ to reduce the impact of atmospheric distortion on their observations?

    <p>Active optics to adjust the telescope's optics in real-time.</p> Signup and view all the answers

    What atmospheric condition primarily affects infrared observations?

    <p>The presence of ozone, which absorbs certain wavelengths.</p> Signup and view all the answers

    What is a result of atmospheric distortion during astronomical observations?

    <p>Blurring of images, reducing resolution.</p> Signup and view all the answers

    What can significantly impair infrared observations aside from humidity?

    <p>High levels of pollution in urban areas.</p> Signup and view all the answers

    Which of the following is NOT a significant reason for conducting infrared astronomy from high altitudes?

    <p>Minimization of high-energy cosmic ray effects.</p> Signup and view all the answers

    What is the primary reason why radio observations have poorer resolution than visible light observations?

    <p>The wavelength of radio waves is much longer than that of visible light.</p> Signup and view all the answers

    Which type of electromagnetic radiation can penetrate the Earth's atmosphere and reach the surface unimpeded?

    <p>Infrared radiation</p> Signup and view all the answers

    What characteristic of a telescope primarily determines its resolving power?

    <p>The diameter of the objective.</p> Signup and view all the answers

    Which factor contributes to the correction of atmospheric disturbances in optical observations?

    <p>Adaptive optics adjust for real-time atmospheric effects.</p> Signup and view all the answers

    How does chromatic aberration affect the observations made with a small diameter refracting telescope?

    <p>It causes different wavelengths to focus at different points.</p> Signup and view all the answers

    What is the resolving power of a telescope with a diameter of 2 meters?

    <p>0.1 arc seconds</p> Signup and view all the answers

    What type of device does CCD stand for in astronomy?

    <p>Charge-coupled device</p> Signup and view all the answers

    Which statement is true regarding light-gathering power?

    <p>It is proportional to the square of the diameter of the objective.</p> Signup and view all the answers

    What is the main reason for building large optical telescopes on the Earth's surface?

    <p>To collect as much light as possible from faint objects.</p> Signup and view all the answers

    Why does the Spitzer Space Telescope orbit far from Earth?

    <p>To escape thermal emissions that interfere with its observations.</p> Signup and view all the answers

    What is chromatic aberration primarily associated with?

    <p>Different colors of light not focusing at the same point in refracting telescopes.</p> Signup and view all the answers

    The light-gathering power of a telescope is directly related to which of the following?

    <p>The diameter of the primary mirror or lens.</p> Signup and view all the answers

    What best describes the refraction of light?

    <p>The change in direction of a light ray when it transitions between media of different densities.</p> Signup and view all the answers

    What is the primary purpose of combining signals from multiple radio telescopes spread over a large area?

    <p>To produce higher resolution images.</p> Signup and view all the answers

    Which type of telescope is primarily classified as reflecting?

    <p>A telescope that uses mirrors to gather and focus light.</p> Signup and view all the answers

    What is a characteristic of radio telescopes?

    <p>They utilize large dish antennas for capturing radio waves.</p> Signup and view all the answers

    Study Notes

    Multiple Choice Questions - Astronomy Chapter 5

    • Wavelength of Longest Visible Light: 700 nm
    • Wavelength of Shortest Visible Light: 400 nm
    • Violet Light Wavelength: Approximately 400 nm
    • Electromagnetic Radiation Longer than Visible Light: Infrared radiation
    • Electromagnetic Radiation Shorter than Visible Light: Ultraviolet light and Gamma-rays
    • Nanometers per Meter: 1x109
    • Astronomical Telescope Placement: On mountaintops due to less atmospheric distortion (air) affecting light
    • Ultraviolet Radiation: Does not penetrate Earth's atmosphere; shorter wavelength than visible light
    • Telescope Fine Detail Resolution: Resolving power
    • Infrared Astronomy: Often done from high-flying aircraft because infrared radiation is absorbed by the lower Earth's atmosphere.
    • Adaptive Optics: Technique that uses a computer to adjust telescope optics, compensating for atmospheric distortion
    • Telescope Light Gathering Power Ratio: The ratio of the light-gathering power of a 5-meter telescope to a 0.5-meter telescope is 100.
    • Telescope Magnification: Calculated by dividing the objective focal length by the eyepiece focal length. Example: 200 cm objective / 0.2 cm eyepiece = 1000x
    • Telescope Resolving Power: The smallest angular separation of two objects that can be distinguished by the telescope, expressed in arcseconds (1 arcsecond = 1/3600 of a degree).
    • CCD: Stands for Charge-Coupled Device.
    • Radio Telescope Resolution: Poorer than visible light observations due to radio waves' longer wavelengths
    • Radio wave wavelengths: Long
    • Electromagnetic radiation that reaches the earth surface: Radio waves, visible light
    • Hubble Space Telescope: Not affected by atmospheric distortion (seeing) and chromatic aberration.
    • Spitzer Space Telescope Orbit: Far from Earth to avoid infrared radiation emitted by Earth
    • Large Optical Telescopes: Built to maximize light collection from faint objects and reduce the blurring effect of Earth's atmosphere
    • Refraction Definition: Change of a light ray's direction as it passes into a medium with a different optical density
    • Light Gathering Power of Telescope: Directly proportional to the square of the diameter of the primary mirror or lens.
    • Chromatic Aberration: In refracting telescopes, different colors of light do not focus at the same point.
    • Radio Telescope Signal Combination: Used to enhance resolution and observe more objects simultaneously.

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    Description

    Test your knowledge on Chapter 5 of Astronomy, focusing on the properties of light and its interaction with telescopes. This quiz covers topics like the wavelength of visible light, electromagnetic radiation, and advanced telescope techniques. Dive into the world of astronomy and see how well you understand these concepts!

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