Exam 6: The Tools of the Astronomer

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According to the law of reflection, if a beam of light strikes a flat mirror at an angle of 30° relative to a plane perpendicular to the surface of the mirror, at what angle will it reflect, relative to a plane perpendicular to the surface of the mirror?

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How faint an object we can see with our eyes is limited only by the integration time of our eye (how often it processes input).

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Which of the following phenomena is shown in the figure below? Which of the following phenomena is shown in the figure below?

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Discuss two tools that modern astronomers use to explore the cosmos that are different from traditional optical telescopes and give an example of how and why each is used.

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The major advantage CCDs have over other imaging techniques is that:

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The dispersing element in a spectrograph could be a prism or a diffraction grating.

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Which of the following is the biggest disadvantage of putting a telescope in space?

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Typically, video is shot using 24 to 30 frames per second (one frame each 33 to 42 ms). If a filmmaker shot new experimental video at 100 frames per second (one frame each 1 ms), how would it look during playback to the human eye?

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Astronomers usually study distant galaxies by looking at them directly through the eyepiece of a telescope.

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Samples of which celestial object(s) have been brought back to Earth to be studied in detail?

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Name two reasons why astronomers might use a space telescope over a ground-based telescope.

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Why do reflecting telescopes usually have a secondary mirror in addition to a primary mirror?

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A beam of light passes from air to water at an incident angle of 40°, relative to a plane perpendicular to the boundary between the two. At what angle will it emerge into the water, relative to a plane perpendicular to the boundary?

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The diffraction limit of a 4-meter telescope is _________ than that of a 2-meter telescope.

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Label the eyepiece, primary mirror, secondary mirror, focus, and focal length of the telescope below. Label the eyepiece, primary mirror, secondary mirror, focus, and focal length of the telescope below.

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NASA's Kuiper Airborne Observatory and SOFIA are two examples of telescopes placed in high-flying aircraft. Why would astronomers put telescopes in airplanes?

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In 2008, the Cassini spacecraft made a flyby of Enceladus, one of the icy moons of Saturn. If the spacecraft's high resolution camera had an angular resolution of 3 arcsec, and it flew at an altitude of 23 km above Enceladus's surface, how large an object could be resolved on the surface?

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What is the angular resolution of a 1-m, ground-based, optical telescope that observes at a wavelength of 600 nm compared to that of a 300-ft, single-dish radio telescope that observes at a wavelength of 21 cm?

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Hans Lippershey invented the telescope in the early 1600s.

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The angular resolution of a ground-based telescope (without adaptive optics) is typically:

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