Chapter 23: Problem 28
Discuss how the Milky Way would appear to us if the Sun were relocated to (a) the edge of the Galaxy; (b) the galactic halo; (c) the galactic bulge.
Chapter 23: Problem 28
Discuss how the Milky Way would appear to us if the Sun were relocated to (a) the edge of the Galaxy; (b) the galactic halo; (c) the galactic bulge.
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Get started for freeA gas cloud located in the spiral arm of a distant galaxy is observed to have an orbital velocity of \(400 \mathrm{~km} / \mathrm{s}\). If the cloud is \(20,000 \mathrm{pc}\) from the center of the galaxy and is moving in a circular orbit, find (a) the orbital period of the cloud and (b) the mass of the galaxy contained within the cloud's orbit.
Student book bags often contain a wide collection of oddshaped objects. Each person in your group should rummage through their own book bags and find one object that is most similar to the Milky Way Galaxy in shape. List the items from each group member's belongings and describe what about the items is similar to the shape of our Galaxy and what about the items is not similar, then indicate which of the items is the closest match.
How did observations of globular clusters help astronomers determine our location in the Galaxy?
In our Galaxy, why are stars of spectral classes \(\mathrm{O}\) and \(\mathrm{B}\) only found in or near the spiral arms? Is the same true for stars of other spectral classes? Explain why or why not.
Show that the form of Kepler's third law stated in Box 23-2, \(P^{2}=4 \pi^{2} a^{3} / G\left(M+\mathrm{M}_{\odot}\right)\), is equivalent to \(M=r v^{2} / G\), provided the orbit is a circle. (Hint: The mass of the Sun (M \(\mathrm{M}_{\odot}\) ) is much less than the mass of the Galaxy inside the Sun's orbit (M).)
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