Why Surface Gravity Depends Only on Density and Radius
SERIES X — RECOMPUTING PHYSICS FROM FIRST MECHANICS
What Can Be Derived from Density & Stiffness Alone?

One of the quiet surprises of planetary science is how simple surface gravity really is.
Despite very different compositions, temperatures, and histories, the surface gravity of a rocky body is largely determined by just two quantities:
its average density and its radius
No force laws are required to see this.
No inverse-square attraction needs to be assumed.
The result falls directly out of mechanics.
A Familiar Result, Reached a Different Way
In conventional physics, surface gravity is written as
But mass can be written as
Substituting gives
This is usually treated as a mathematical coincidence.
In a mechanical-medium picture, it is not a coincidence at all.
It is the core insight.
Gravity as a Stress Gradient
If gravity is not a force pulling inward, but a response of a medium under compression, then surface gravity represents something very specific:
the rate at which internal stress changes near the surface
Inside a spherical body:
- each layer supports the weight (stress) of layers above it,
- stress increases smoothly toward the center,
- the surface value reflects the total internal stress gradient.
Mechanically, the surface acceleration scales as
For a roughly uniform body, internal stress itself scales with , giving
This is not a force balance.
It is a material response.
Why Composition Barely Matters
This immediately explains a puzzling observation:
- Earth and Mercury have very different compositions
- Mars and the Moon have very different internal histories
Yet bodies with similar density–radius products have similar surface gravity.
Why?
Because:
- gravity depends on bulk stress, not chemistry,
- chemical structure averages out,
- only density (how much medium is displaced) and size (over what distance) matter.
The medium does not care what the defect is made of—only how much of it exists and how far stress must propagate.
Putting Numbers on It
Let’s compare a few bodies using only density and radius.
| Body | Radius (km) | Density (kg/m³) | (scaled) | Surface g (m/s²) |
|---|---|---|---|---|
| Earth | 6371 | 5514 | high | 9.81 |
| Moon | 1737 | 3344 | low | 1.62 |
| Mars | 3390 | 3933 | medium | 3.71 |
| Mercury | 2440 | 5427 | medium | 3.70 |
Mars and Mercury have nearly identical surface gravity—not because they share mass, composition, or history, but because ρR is nearly the same.
That agreement is not tuned.
It is structural.
Why Radius Enters Linearly
The linear dependence on radius is especially important.
If gravity were a force emanating from the center, we might expect more complicated behavior. Instead:
- each additional layer adds stress,
- stress accumulates linearly with depth,
- the surface gradient reflects total integrated stress.
This is exactly how pressure behaves in ordinary materials.
Planetary gravity behaves like pressure in a very large object.
What This Explains Immediately
This single relation explains:
- why small asteroids have almost no gravity
- why super-dense but tiny objects don’t dominate
- why gravity grows smoothly with planetary size
- why “surface gravity” is a meaningful concept at all
None of this requires spacetime curvature or action-at-a-distance.
It follows from mechanics.
Key Takeaway
Surface gravity is not a force law—it is a stress gradient.
For spherical bodies, that gradient depends only on:
- how dense the body is, and
- how large it is.
Everything else is secondary.
With this result in hand, we can now ask the next natural question:
If gravity is a stored stress, what does it mean to “escape” it—and why does escape speed take the form it does?
That is where we turn next.
