Exam 2: Light and Telescopes
Exam 1: The Night Sky88 Questions
Exam 2: Light and Telescopes111 Questions
Exam 3: The Solar System109 Questions
Exam 4: Earth and Its Moon108 Questions
Exam 5: The Eight Planets112 Questions
Exam 6: Small Bodies in the Solar System108 Questions
Exam 7: Formation of Planetary Systems84 Questions
Exam 8: The Sun95 Questions
Exam 9: Measuring the Stars86 Questions
Exam 10: Star Formation and Evolution85 Questions
Exam 11: Stellar Explosions101 Questions
Exam 12: Black Holes77 Questions
Exam 13: The Milky Way Galaxy82 Questions
Exam 14: Galaxies98 Questions
Exam 15: Cosmology and the Universe98 Questions
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As a star's temperature increases, the frequency of peak emission also increases.
(True/False)
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How do radio interferometers greatly enhance resolution in radio wavelengths?
(Essay)
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In an atom, electrons can have only specific, allowed orbital energies.
(True/False)
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Compared to optical telescopes, radio telescopes are built large because
(Multiple Choice)
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What is the light-gathering power of an 8-inch telescope compared to a 4-inch telescope?
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Why is the angular resolution of radio telescopes much worse than that of smaller optical telescopes?
(Essay)
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Because the changes in energy levels happen in discrete steps, we refer to these as ________ leaps.
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What is white light? Why do we perceive different colors with a prism?
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The light from an object moving tangentially (to your left or right) will exhibit
(Multiple Choice)
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The Sun's blackbody curve peaks in the ________ portion of the spectrum.
(Short Answer)
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Compare how doubling the diameter of a mirror will affect both resolution and light gathering power.
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Due to our ozone layer, ultraviolet astronomy must be done from space.
(True/False)
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Knowing the peak emission wavelength of a blackbody allows you to determine its ________.
(Short Answer)
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What information about a star can be inferred from its Doppler shift?
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The two forms of electromagnetic radiation that penetrate the atmosphere best are
(Multiple Choice)
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What two regions of the electromagnetic spectrum are best utilized by ground-based astronomers, and why?
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