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Material Type: Assignment; Class: STELLAR STRCTR/EVOL; Subject: Physics; University: University of California - Santa Barbara; Term: Fall 2008;
Typology: Assignments
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Department of Physics
2008 FALL STARS Professor Martin
HOMEWORK PROBLEM #1 Due: September 29th
Assigned Reading: Phillips 1.1-1.4, 1.
Problem 1: Consider a spherically symmetric gas cloud of uniform den- sity ρ 0. We showed that if all pressure support is removed, the cloud will collapse to a point on the free-fall timescale.
(a, 2 pts) Evaluate the integral
∫ (^1) 0
√ (^) x 1 −x dx^ in the derivation and verify that the answer given in class for the free-fall timescale is correct. [See Chapter 1 of Phillips for hints.] (b, 1 pts) Now consider a molecular cloud with the following properties: temperature T = 20 K, mass M = 1000 MØ, and density n = 10^5 hydrogen molecules per cubic centimeter. If the pressure forces supporting this cloud were removed, how long would it take the cloud to collapse to a point? [Hint: Just calculate the free-fall time. You are given more information than you actually need.] (c, 2 pts) Find the gravitational potential energy of a uniform, spherical cloud of total mass M and radius R. [Hint: Use Eqn. 1.6 to show that the coefficient in 1.16 is 3/5.]