A body orbits the Earth at a mean radius that is twice the distance of the parking orbit of a geostationary satellite. According to Kepler’s third law, the orbital period of a body increases as the radius of its orbit becomes larger. In this case, the greater radius results in a longer orbital period. The body’s period is determined to be approximately 2√2 days, highlighting how the distance from the central body influences the time taken for one complete revolution around the Earth. This demonstrates the proportional relationship between orbital radius and time period.