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 5Q
To determine

(a)

To discuss:

The way, the Milky Way would appear if the Sun were relocated to the edge of the galaxy.

To determine

(b)

The way, the Milky Way would appear if the Sun were relocated to the galactic halo.

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The Milky Way galaxy has about 5 x 10⁹ solar masses of gas in total. If 13 solar masses of that gas is turned into stars each year, how many more years could the Milky Way keep up with such a star formation rate? years (Note for comparison that the age of the universe is about 13.5 billion years, which can be written 1.35e10 years. Also, the value given is in the ballpark of how much gas in the Milky Way is used to make new stars each year.)
Suppose a galaxy is 400 million parsecs from the Milky Way. What is the recessional velocity of this galaxy? (Assume Hubble's constant Ho = 75 km/s/Mpc.) (Hint: 400 x 75 = 30,000) A) 400,000,000 km/s B) 1/10 the speed of light C) 75 km/s D) twice the speed of light
The Milky Way grew through merging with many smaller galaxies. What are the observational signatures of this process? O The motion of old stars in the bulge and halo of our galaxy are randomly orientated, meaning they were formed from collisions of small, accreted, galaxies all on different paths. O The ordered motion of the bulge / halo stars means that they came from many objects. The random motions of stars in the disk means it was formed from collisions of small, accreted, galaxies. O The motion of young stars in the disk are all in the same direction, meaning they came in as seperate objects.
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