Exam 9: The Formation and Structure of Stars
Exam 1: Here and Now97 Questions
Exam 2: A Users Guide to the Sky116 Questions
Exam 3: Cycles of the Sun and Moon154 Questions
Exam 4: The Origin of Modern Astronomy144 Questions
Exam 5: Light and Telescopes156 Questions
Exam 6: Atoms and Spectra125 Questions
Exam 7: The Sun146 Questions
Exam 8: The Family of Stars190 Questions
Exam 9: The Formation and Structure of Stars136 Questions
Exam 10: The Deaths of Stars128 Questions
Exam 11: Neutron Stars and Black Holes99 Questions
Exam 12: The Milky Way Galaxy117 Questions
Exam 13: Galaxies: Normal and Active151 Questions
Exam 14: Modern Cosmology112 Questions
Exam 15: Origin of the Solar System and Extrasolar Planets104 Questions
Exam 16: Earth and Moon: Bases for Comparative Planetology98 Questions
Exam 17: Mercury, Venus, and Mars83 Questions
Exam 18: The Outer Solar System137 Questions
Exam 19: Meteorites, Asteroids, and Comets91 Questions
Exam 20: Astrobiology: Life on Other Worlds97 Questions
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The law of ________________ states that energy must flow from _________ temperature regions to __________ temperature regions.
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The image on the right indicates star formation that we cannot see in the wavelength band on the left. The image on the left is a/an __________ wavelength image of the ___________ wavelength image on the right.


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What characteristic of a star primarily determines its location on the main sequence?
(Multiple Choice)
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While on the main sequence a star's primary energy source comes from
(Multiple Choice)
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Both the CNO cycle and the proton-proton fusion chain convert hydrogen to helium using catalysts.
(True/False)
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What must occur for an object to be considered a main-sequence star?
(Multiple Choice)
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Why do nuclear fusion reactions only take place in the interior of a star?
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In the above cartoon of the Orion constellation, the upper red supergiant star is known as Rigel and the lower right supergiant star is known as Betelgeuse.

(True/False)
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Hydrostatic equilibrium refers to the balance between weight and pressure.
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Absorption lines due to the interstellar medium indicate that some components of the interstellar medium are cold and of a very low density because
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