a) Suppose the mass density of a G0 star is given by the following expression: p(r) = Po [4) -]• where R is the radius of the star. i) Determine the central pressure. ii) In our studies, we derived an approximation for the total mechanical energy of a star by assuming its density was constant and given by the total mass divided by the volume of a spherical star. Given the density distribution above, determine a revised equation for the total mechanical energy for the star.
a) Suppose the mass density of a G0 star is given by the following expression: p(r) = Po [4) -]• where R is the radius of the star. i) Determine the central pressure. ii) In our studies, we derived an approximation for the total mechanical energy of a star by assuming its density was constant and given by the total mass divided by the volume of a spherical star. Given the density distribution above, determine a revised equation for the total mechanical energy for the star.
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