Astronomical observations of our Milky Way galaxy indicate that it has a mass of about 8 x 10- solar masses. A star orbiting near the galaxy's periphery is 5.9 x 104 light years from its center. (For your calculations, assume that the galaxy's mass is concentrated near its center.) What should the orbital period of that star be? yr If its period is 5.8 x 107 years instead, what is the mass of the galaxy? Such calculations are used to imply the existence of "dark matter" in the universe and have indicated, for example, the existence of very massive black holes at the centers of some galaxies. solar masses

College Physics
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Chapter34: Frontiers Of Physics
Section: Chapter Questions
Problem 27PE: If the dark matter in the Milky Way were composed entirely of MACHOs (evidence shows it is not),...
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Astronomical observations of our Milky Way galaxy indicate that it has a mass of about 8 x 10¹¹ solar masses. A star orbiting near
the galaxy's periphery is 5.9 x 104 light years from its center. (For your calculations, assume that the galaxy's mass is concentrated
near its center.)
What should the orbital period of that star be?
yr
If its period is 5.8 x 107 years instead, what is the mass of the galaxy? Such calculations are used to imply the existence of
"dark matter" in the universe and have indicated, for example, the existence of very massive black holes at the centers of
some galaxies.
solar masses
Transcribed Image Text:Astronomical observations of our Milky Way galaxy indicate that it has a mass of about 8 x 10¹¹ solar masses. A star orbiting near the galaxy's periphery is 5.9 x 104 light years from its center. (For your calculations, assume that the galaxy's mass is concentrated near its center.) What should the orbital period of that star be? yr If its period is 5.8 x 107 years instead, what is the mass of the galaxy? Such calculations are used to imply the existence of "dark matter" in the universe and have indicated, for example, the existence of very massive black holes at the centers of some galaxies. solar masses
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