Doc Al said:
I don't think so. Taking a simplified model of a spherically symmetric earth, as long as the symmetry is maintained it doesn't matter if all the mass were contained in a thin shell: the gravitational field outside the shell will be the same.
But what I'm saying is that model in unphysical. For a hollow earth, its simply wrong.
Here, I'll work through the math:
For a spherical shell of radius [tex]R[/tex], width [tex]\Delta r[/tex], and uniform density [tex]\rho[/tex] the total mass [tex]M[/tex] is:
[tex]
M = \int\int\int \rho r^2 \sin \theta dr d\theta d\phi[/tex]
[tex]
\qquad = \int^{R+\Delta r}_{R} \int^{2\pi}_0 \int^{2 \pi}_0 \rho r^2 \sin \theta dr d\theta d\phi[/tex]
so we can stipulate that the mass of some volume slice in the shell is given by [tex]dm[/tex] as:
[tex]
dm = \rho r^2 \sin \theta dr d\theta d\phi[/tex]
The gravitational field generate by this mass slice is given by:
[tex]
g = G \frac{dm}{s^2} \vec{\epsilon}[/tex]
where [tex]s[/tex] is the distance to the mass slice, and [tex]\vec{\epsilon}[/tex] is the unit vector point towards the mass slice. It can be show geometrically that when calculating the gravtiational field at the point P(R, 0,0) (surface of the sphere)
[tex]
s = 2 r \sin \frac{\theta}{2}[/tex]
The unit vector point from P to the mass slice [tex]\vec{\epsilon}[/tex] is:
[tex]
\vec{\epsilon} = \left [ \begin{array}{l} 1 \\ \theta \\ \phi \end{array} \right ][/tex]
Now, because this is a sphere, and as such is rotationally symmeticraly we can assume that
[tex]
g_\theta = 0[/tex]
[tex]
g_\phi = 0[/tex]
so we get:
[tex]
g_r = \int \int \int G \frac{\rho r^2 \sin \theta dr d\theta d\phi}{4 r^2 \sin^2 \frac{\theta}{2}} dr d\theta d\phi[/tex]
Integrating only over a single hemisphere, and then multiply by two (to eliminate negative r) gives
[tex]
\qquad = \frac{G \rho}{4} \int_{R}^{R+\Delta r} \int_0^{\pi} \int_0^{2\pi} \frac{\sin \theta}{\sin^2 \frac{\theta}{2}} d\phi d\theta dr[/tex]
[tex]
\qquad = \frac{G \rho}{8} \int_{R}^{R+\Delta r} \int_0^{\pi} \int_0^{2\pi} \sin \theta - \frac{\sin 2 \theta}{2} d\phi d\theta dr[/tex]
(check your trig identities if you're not sure how I got that. i used the double angle identity)
[tex]
\qquad = \frac{ G \rho \pi \Delta r}{2}[/tex]
Now, to get a number for that, let's say our Earth has a [tex]\Delta r[/tex] of 0.01 percent the normal radius of the Earth (this derivation requires that [tex]\Delta r \ll R[/tex]). This gives:
[tex]
G = 6.67 \times 10^-11[/tex]
[tex]
\Delta r = 63800 \text{m}[/tex]
[tex]
\rho = 575641 \frac{kg}{m^3}[/tex]
gives [tex]g = 3.847 \frac{m}{s^2}[/tex].
Well that is odd. it came out smaller. Now this is going to bug me even more. I don't suppose someone could check this for me to make sure I didn't screw something up along the way? interesting result though, if its right.