
Ryan G. answered 10/30/20
Math, physics and astronomy tutor
Density is mass divided by volume. Mathematically, ρ = m/V, where the volume (for a sphere) is given as
V = 4/3 * pi * r3 where r is the radius of the sun
Let's let the new radius R = 200 * r so the new volume is V' = 4/3 * pi * R3 = 4/3 * pi * (200*r)3 = (200)3 * 4/3 * pi * r3. So V' = (200)3 * V and the new density is ρ' = m/V' = m/(2003 * V) = 1/2003 * m/V = 1/2003 * ρ
So ρ' = 1/2003 * ρ
The (average) density of the sun is 1.41 g/cm3. So, the new density is 1.41/2003 = 1.76 x 10-7 g/cm3