How can the precession of a satellite orbit reveal Earth’s flattening?
The Earth is not a perfect sphere; its rotation creates an equatorial bulge, resulting in an ellipsoidal shape. This mass distribution significantly influences the gravitational field, which in turn affects the motion of orbiting satellites.12
When a satellite travels in an inclined orbit, it passes over the equatorial region and experiences a gravitational force directed toward the Equator due to the mass of this bulge. This force exerts a torque on the satellite's orbit. Much like the physics of a spinning top or gyroscope, this torque causes the satellite's orbital plane to precess around Earth’s rotation axis.1
This precession is a measurable, secular change in the satellite's path. By observing the rate of this precession with high accuracy, scientists can determine the magnitude of the dynamical form factor, known as . This factor is directly related to the Earth's flattening, or the degree to which the planet deviates from a spherical shape. Consequently, tracking these orbital perturbations allows researchers to refine our understanding of the geoid and the Earth's precise figure.12