The Cosmic Perspective (9th Edition)
The Cosmic Perspective (9th Edition)
9th Edition
ISBN: 9780134874364
Author: Jeffrey O. Bennett, Megan O. Donahue, Nicholas Schneider, Mark Voit
Publisher: PEARSON
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Chapter 19, Problem 47EAP
To determine

The future of milk way and the change in its appearance of the over 100 billion years.

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When we observe the most distant galaxies what are we looking at? At galaxies with ages similar to that of the Milky Way, because light travels so quickly that there is no significant time delay. Because of the finite speed of light, we are observing how galaxies looked like in the past. Because of the finite speed of light, we have the opportunity to observe our own galaxy when it started forming in the past. Because of the long light travel time, we are observing old galaxies.
2. A galaxy cluster has a galaxy behind it whose image we see as being smeared out and curved, with an angular radius of curvature on the sky of θE.  The background galaxy is at redshift zgal and the cluster is at zclust.  What is the mass of the cluster in solar masses?  Give your response in scientific notation with one decimal place.  (The Hubble constant is of course 70 km/s/Mpc, and you can assume the Hubble law for these low redshifts).   Values: zgal = 0.11 zclust = 0.07 θE = 117.4 arcseconds
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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