Exam 4: Light and Telescopes
Exam 1: Here and Now49 Questions
Exam 2: Users Guide to the Sky: Patterns and Cycles165 Questions
Exam 3: The Origin of Modern Astronomy79 Questions
Exam 4: Light and Telescopes95 Questions
Exam 5: Sun Light and Sun Atoms135 Questions
Exam 6: The Terrestrial Planets123 Questions
Exam 7: The Outer Solar System88 Questions
Exam 8: Origins of the Solar System and Extrasolar Planets69 Questions
Exam 9: The Family of Stars105 Questions
Exam 10: Structure and Formation of Stars100 Questions
Exam 11: The Deaths of Stars146 Questions
Exam 12: The Milky Way Galaxy70 Questions
Exam 13: Galaxies: Normal and Active135 Questions
Exam 14: Modern Cosmology69 Questions
Exam 15: Life on Other Worlds55 Questions
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Reflecting telescopes are no longer popular with astronomers because they are expensive and suffer from chromatic aberration.
(True/False)
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What advantages does a large diameter astronomical telescope have over a telescope of a smaller diameter?
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The objective of most radio telescopes is similar to the objective of a reflecting optical telescope in that
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A ____ is a piece of glass with many small parallel lines etched on its surface to produce a spectrum.
(Multiple Choice)
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What is the relationship between color and wavelength for light?
(Multiple Choice)
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Which of the following features of a telescope determines its light gathering power?
(Multiple Choice)
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The ____________________ of a telescope is determined by the size of the objective.
(Short Answer)
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The pupil of the human eye is approximately 0.8 cm in diameter when adapted to the dark. The ratio of the light gathering power of a 1.6 m telescope to that of the human eye is ____.
(Multiple Choice)
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What causes chromatic aberration? Why does it not occur in reflecting telescopes?
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Which of the following sequences of electromagnetic radiation is correct in order of increasing energy?
(Multiple Choice)
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The main lens or mirror of a telescope is called the ____________________.
(Short Answer)
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The ____________________ is a measure of the finest detail that can be seen in an image.
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How does the nature of radio waves allow a radio telescope to use a wire mesh surface? Would you expect millimeter wavelength telescopes to need smoother surfaces than typical radio dishes? Why or Why not?
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