Roman C. answered 04/20/17
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Masters of Education Graduate with Mathematics Expertise
Using the convention that the potential has limit 0 infinitely far away, we have the following:
The potential on the outside of the sphere is V(r) = -GM/r, where r is the distance from the center.
Thus if the sphere has radius R, the surface potential is V(R) = -GM/R
Next, the gravity field inside the sphere is a direct variation with the discance from the center, that is:
Φ(r) = Φsurface × r/R = GM/R2 × r/R = GMr/R3
And the potential inside is the integral of this:
V(r) = GMr2/(2R3) + C.
We can solve for C by insisting that V(r) is continuous at r = R.
GMR2/(2R3) + C = -GM/R
GM/(2R) + C = -GM/R
C = -GM/R - GM/(2R) = -3GM/(2R)
So for r < R:
V(r) = GMr2/(2R3) - 3GM/(2R).
This means V(0) = -3GM/(2R).
So the ratio is:
V(R) / V(0) = (-GM/R) / (-3GM/(2R)) = 2/3