A physical body with greater mass causes another to orbit around it due to the gravitational influence, but both bodies actually orbit a common center of mass, known as the barycenter. In the solar system, the barycenter is often close to the center of the larger mass, such as the Sun, leading to the common simplification that "Earth orbits the Sun." However, the Sun also orbits this barycenter, which is not located at its center. Mathematically, while the two-body problem can be solved analytically, systems with multiple bodies require numerical solutions. The Earth exhibits a noticeable wobble as it orbits the barycenter with the Moon, but this effect does not significantly impact astronomical observations.