How orbits change when \(\eta = m_g / m_I \neq 1\) — the universality of free fall
What you're seeing: Test particles in a Kepler field
\(\ddot{\boldsymbol{x}} = -\eta\, GM\, \boldsymbol{x}/r^3\),
all launched from the same point with the same tangential velocity.
The parameter \(\eta = m_g/m_I\) is the ratio of gravitational to inertial mass.
If the
universality of free fall (UFF) holds, then \(\eta = 1\) for all matter
and all particles follow the same orbit — regardless of their composition.
Drag the slider to see what would happen if \(\eta \neq 1\): the orbits immediately diverge.
Experimental precision: No deviation has ever been observed.
| Experiment | Year | Precision \(|\Delta\eta|\) |
| Newton (pendulum) | 1687 | < 10−3 |
| Eötvös torsion balance | 1922 | < 10−9 |
| Lunar laser ranging | 1969– | < 10−13 |
| MICROSCOPE satellite | 2022 | < 10−15 |