The centroid of the Earth-Moon system, or the center of mass, is calculated by measuring the distances of both the Earth and Moon from a reference point, typically the center of the Earth. This involves multiplying each object's distance by its mass, summing these products, and then dividing by the total mass of the Earth and Moon. The resulting point is where both bodies orbit, which can be either circular or elliptical depending on the total energy of the system. The calculation indicates that the Earth revolves around a point approximately 4,768 km below its surface. The dynamic nature of the system results in an oscillating elliptical spiral over time due to the Earth's rotation and the Moon's orbit.