A trajectory is considered bound when the total energy, which is the sum of kinetic and potential energy, is less than or equal to zero. This negative energy indicates that the object does not have enough energy to escape the gravitational influence, resulting in a closed orbit. However, not all bound orbits are closed; if the ratio of the orbital period to the period of radial oscillations is not an integer, the orbit may not close on itself. In the context of gravity following an inverse square law, the only bounded orbits are elliptical and thus inherently closed. Understanding these energy conditions is crucial for analyzing orbital mechanics.