Universe: Stars And Galaxies
Universe: Stars And Galaxies
6th Edition
ISBN: 9781319115098
Author: Roger Freedman, Robert Geller, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 22, Problem 28Q
To determine

The reason for the rotation curve to show a rapid increase in the orbital velocity at the distances close to the galactic center.

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The Tully-Fischer method relies on being able to relate the mass of a galaxy to its rotation velocity. Stars in the outer-most regions of the Milky Way galaxy, located at a distance of 50 kpc from the galactic centre, are observed to orbit at a speed vrot determine the mass in the Milky Way that lies interior to 50 kpc. Express your answer in units of the Solar mass. 250 km s-1. Using Kepler's 3rd Law,
GM If the active core of a galaxy contains a black hole of 1o° Me, what will the orbital period be for matter orbiting the black hole at a distance of 0.41 AU? (Hint: Use the formula for circular velocity, V. = \ hr
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