Rotational kinetic energy for a body rotating about multiple axes can be defined by separating the translational and rotational components of motion. When a body, such as a ball, rotates about an axis through its center of inertia while also having its center of mass move along a perpendicular axis, the total kinetic energy is the sum of translational kinetic energy and the rotational kinetic energy calculated using the formula 1/2 I ω². The moment of inertia (I) is dependent on the mass distribution of the body, and for a solid sphere, it is 2/5 MR². The complexity increases when considering systems like the Earth-Sun model, where the axes may not align, necessitating a deeper analysis of the rotational dynamics. Ultimately, understanding the contributions of each motion type is crucial for accurately defining the total kinetic energy in such scenarios.