Exam 14: Our Galaxy
Exam 1: Our Place in the Universe102 Questions
Exam 2: Discovering the Universe for Yourself135 Questions
Exam 3: The Science of Astronomy97 Questions
Exam 4: Making Sense of the Universe: Understanding Motion, Energy, and Gravity103 Questions
Exam 5: Light: the Cosmic Messenger139 Questions
Exam 6: Formation of Planetary Systems: Our Solar System and Beyond174 Questions
Exam 7: Earth and the Terrestrial Worlds180 Questions
Exam 8: Jovian Planet Systems85 Questions
Exam 9: Asteroids, Comets, and Dwarf Planets: Their Nature, Orbits, and Impacts118 Questions
Exam 10: Our Star101 Questions
Exam 11: Surveying the Stars129 Questions
Exam 12: Star Stuff137 Questions
Exam 13: Bizarre Stellar Graveyard110 Questions
Exam 14: Our Galaxy112 Questions
Exam 15: Galaxies and the Foundation of Modern Cosmology152 Questions
Exam 16: Dark Matter, Dark Energy, and the Fate of the Universe97 Questions
Exam 17: The Beginning of Time105 Questions
Exam 18: Life in the Universe82 Questions
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Red and orange stars are found evenly spread throughout the galactic disk, but blue stars are typically found ________.
(Multiple Choice)
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Briefly describe how we can use the orbital characteristics of stars at many distances from the galactic center to determine the distribution of mass in the Milky Way.
(Essay)
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How did star formation likely proceed in the protogalactic cloud that formed the Milky Way?
(Multiple Choice)
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Most of the mass of the galaxy is located at the galactic center in the form of a massive black hole.
(True/False)
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What affects the average orbital speed of a star in our galaxy?
(Multiple Choice)
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Modified Newtonian Dynamics? The case for dark matter in the Milky Way can be viewed as a failure of stars and gas far from the galactic center to obey Newton's law of gravitational attraction-- that is, the stars and gas seem to orbit too quickly for the visible matter their orbits enclose. Why do you think that astronomers choose to "save" Newton's form of gravitational attraction by postulating unseen dark matter, as opposed to regarding the observed orbital motion as a falsification of Newtonian gravitation on the scale of the Milky Way? [Note: At the distance scales involved, the gravitational forces in the galaxy are all fairly weak, much weaker than those encountered in a neutron star or black hole, and hence Einstein's theory of gravity (General Relativity) gives the same predictions as Newton's gravitational law].
(Short Answer)
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Which of the following models best explains why our galaxy has spiral arms?
(Multiple Choice)
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How would you expect a star that formed recently in the disk of the galaxy to differ from one that formed early in the history of the disk?
(Multiple Choice)
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How does the interstellar medium obscure our view of most of the galaxy?
(Multiple Choice)
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How do we learn about the conditions at the center of our own galaxy, the Milky Way?
(Multiple Choice)
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Why do stars in the disk of a spiral galaxy orbit in roughly the same direction, in the same plane in space?
(Multiple Choice)
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