Homework 4 Solutions

21953306 879081014721e05 00557129788009 324699924315

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Unformatted text preview: : 1809.0 4.90181857123e ­05 0.0416026069268 4348.28520045 0.000117824793524 0.064500082889 2804.64755854 7.5997089487e ­05 0.0518012702082 3492.19235886 9.46273817522e ­05 0.057802994924 3129.59562455 8.48021556267e ­05 0.0547199100776 3305.92648532 8.9580164958e ­05 0.0562403296972 3216.55297851 8.71584252372e ­05 0.0554749113002 3260.93356006 8.83609988073e ­05 0.0558563094149 3238.66724986 8.77576521361e ­05 0.0556652837085 3249.78133494 8.80588087344e ­05 0.0557607147595 3244.21953306 8.79081014721e ­05 0.0557129788009 3246.99924315 8.79834228349e ­05 0.0557368416698 3245.60909052 8.79457540899e ­05 0.055724908958 3246.30409242 8.7964586446e ­05 0.0557308749945 3245.95657287 8.79551697639e ­05 0.0557278918964 3246.13032799 8.7959877979e ­05 0.0557293834255 3246.04344927 8.79575238399e ­05 0.055728637656 3246.08688834 8.79587009016e ­05 0.0557290105395 3246.06516873 8.79581123688e ­05 0.0557288240974 3246.07602852 8.79584066347e ­05 0.0557289173184 Final best answers: P = 3250 N/m2, ρ = 8.80x10 ­5 kg/m3, κ = 0.0557m2/kg (2) Internal properties of a solid star [25 pt] Consider a star with mass M, radius R and uniform density, ρ0 = 3M 4π R3 (a) [10 pts] Using the equation of hydrostatic equilibrium, show that the pressure as a function of...
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This document was uploaded on 02/26/2014 for the course PHYS 160 at UCSD.

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