Radius of expanded sun is "R_e=200R"
Mass of Sun is "M=1.989 \u00d7 10^{33}" gram.
Volume of expanded Sun will be
"V_e=\\frac{4}{3}\\pi R^3_e"Density will be,
"\\rho_e=\\frac{M}{V_e}=\\frac{3M}{4\\pi R^3_e}\\\\\n\\rho_e=\\frac{1}{200^3}\\rho"where, "\\rho" is the density of Sun before expansion begin. Thus,
"\\rho_e=1.76\\times 10^{-7}\\:g\/cm^3"
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