The negative mechanical energy of a body, such as an electron in the first orbit of a hydrogen atom, indicates that the system is bound, with the reference energy level set at an infinite distance from the nucleus. This means the total kinetic energy is less than the total potential energy, preventing the particles from separating indefinitely. For example, a satellite in a circular orbit around a planet exhibits similar behavior, where its total mechanical energy is also negative, reinforcing the concept of being bound by gravitational forces. This principle applies broadly to various systems governed by potential functions. Understanding this concept is crucial for grasping the stability of atomic and orbital systems.