AP® Physics C: Mechanics · Unit 2 · Topic 2.6
Shell Theorem and Gravity Inside a Planet
The shell theorem says a uniform spherical shell of mass pulls on outside objects as if all its mass sat at the center, but pulls on anything inside it with exactly zero net force.
Picture a point anywhere inside a hollow spherical shell of rock. Draw a thin double cone from that point out to the shell in both directions. The far wall of the shell it hits is bigger in area but farther away, the near wall is smaller but closer. Those two effects trade off exactly: more distant mass but more of it, less nearby mass but less distance to travel. The inverse-square law and the geometry of the cone cancel perfectly, so the pulls from both patches balance. Add up every such pair of patches over the whole shell and the net force at that interior point is zero, no matter where inside the shell the point sits.
This is why, once you tunnel into a uniform solid sphere like a simplified Earth, only the mass strictly closer to the center than you matters. Treat the planet as a stack of nested shells. Every shell farther out than you contributes nothing, by the result above. Every shell inside your radius acts as if it were a point mass at the center. So the gravity you feel only depends on the mass enclosed within radius r, not the mass beyond it.
For a uniform sphere, enclosed mass scales with r3 while the gravitational pull also divides by r2, so the two effects combine to make g scale linearly with r: g(r) = g_surface x (r/R). This is the natural follow-up to treating planets as point masses from a distance: outside a uniform sphere gravity obeys the same inverse-square law as a point mass, but inside, the rules change completely.
Key terms
- Shell theorem
- A uniform spherical shell exerts zero net gravitational force on any point inside it.
- Enclosed mass
- The mass contained within the radius of the point where gravity is being measured.
- Uniform sphere
- A sphere whose density is the same at every point, used to model idealized planets.
- Inverse-square law
- The rule that gravitational force between point masses falls off as 1/r2 with separation r.
Watch it explained
- How it worksHow do the pulls from every scrap of a shell manage to cancel at any interior point?
- How it worksHow does only the mass closer to the center than you are count once you sink into a uniform sphere?
- Worked exampleFind what fraction of the surface gravity you feel 2000 km from the center of a uniform planet of radius 6000 km.
- Going furtherWhat would you feel falling through a tunnel bored straight through the middle of the Earth?
Check yourself
End of topic.