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Unformatted text preview: Ph 441/541 Problem Set 1 Due: Friday, February 3, 2012 1. Hydrostatic Equilibrium: Consider a sphere of mass M and radius R . Calculate the gravitational potential energy of the sphere assuming (a) a density which is independent of the distance from the center and (b) a density which increases towards the cener according to ( r ) = c (1 r/R ) . In both cases (a) and (b), also write down the average internal pressure needed for hydrostatic equilibrium and determine how the pressure within the sphere depends on the distance from the center. 2. Virial Theorem (Ph 441 students only): As the Sun evolved towards the main sequence, it contracted due to gravity while remaining close to hydrostatic equilibrium and its internal temperature changed from about 30,000 K, Phillips Eq. (1.23), to about 6 10 6 K, Eq. (1.31). This stage of evolution is called the KelvinHelmholtz stage. Find the total energy radiated during this contraction. Assume that the luminosity during this contraction is comparable to the present luminosity of the Sun and estimate the time taken to reach the main sequence....
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This note was uploaded on 02/06/2012 for the course PHYSICS 441/541 taught by Professor Pryor during the Spring '12 term at Rutgers.
 Spring '12
 PRYOR
 Energy, Mass, Potential Energy, Static Equilibrium

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