FOUNDATIONS OF ASTRON.(LL) >CUSTOM PKG<
FOUNDATIONS OF ASTRON.(LL) >CUSTOM PKG<
13th Edition
ISBN: 9781305780286
Author: Seeds
Publisher: CENGAGE C
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Chapter 15, Problem 22RQ
To determine

Whether the visible halo, the galactic nucleus or the disk formed last.

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How are giant molecular clouds (GMCs), the loci of most star formation, themselves formed out of diffuse interstellar gas? What processes determine the distribution of physical conditions within star-forming regions, and why does star formation occur in only a small fraction of the available gas? How is the rate at which stars form determined by the properties of the natal GMC or, on a larger scale, of the interstellar medium (ISM) in a galaxy? What determines the mass distribution of forming stars, the initial mass function (IMF)? Most stars form in clusters (Lada & Lada 2003); how do stars form in such a dense environment and in the presence of enormous radiative and mechanical feedback from other YSOs?
A two-arm spiral density wave is moving through the Galactic disk. At the 8-kpc radius of the Sun's orbit around the Galactic center, the wave's speed is 120 km/s, and the Galactic rotation speed is 220 km/s. How many times has the Sun passed through a spiral arm since the Sun formed 4.6 billion years ago?
If a standard passenger aircraft can fly at 0.37 km/s (828 mph), how long (in yr) would it take to reach the Sun? yr How long (in yr) would it take to reach the galactic center? (Note: 1 pc = 3.1 x 1013 km. The radius of the Sun's orbit around the galactic center is approximately 8,300 pc.) yr
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