Exam 2: Users Guide to the Sky: Patterns and Cycles
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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Seen from the northern latitudes (mid-northern hemisphere), the star Polaris
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A lunar eclipse that occurs when the moon moves completely into Earth s umbral shadow is called
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The totally eclipsed moon glows coppery red because sunlight reaches the moon s surface after passing through Earth s atmosphere.
(True/False)
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The diagram below shows three approximate locations of the sun along the western horizon. Which number indicates the location of the sun at sunset on December 21st for an observer at latitude 48 N? 

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The __________ moon is visible above the western horizon a couple of hours before sunrise.
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As Earth rotates, circumpolar stars appear to move counterclockwise around the north celestial pole.
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If the Sun passes directly overhead on at least one day per year, then
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Polaris has always been the star nearest the north celestial pole.
(True/False)
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Star A has an apparent visual magnitude of 13.4 and star B has an apparent visual magnitude of 15.4. Star A is ____ than star B.
(Multiple Choice)
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An observer in the Southern Hemisphere takes a time exposure photograph of the night sky. If the illustration below depicts the photograph taken by the observer, which direction was the camera pointing? 

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What causes precession and why does it move the celestial equator?
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The constellation of Orion is currently visible in the evenings in January. Precession will not affect this and Orion will still be visible in January 13,000 years from now.
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The path of totality for a solar eclipse is swept out by the tip of the moon s umbra as the umbra moves over Earth.
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