Newton–Euler equations

The Newton–Euler equations are a set of equations that describe the motion of rigid bodies in three-dimensional space, combining concepts from both Newtonian mechanics and Euler's rotation equations. These equations are particularly useful for analyzing the dynamics of a rigid body under the influence of both translational and rotational forces and torques. ### Overview: 1. **Newton's Laws of Motion**: These laws provide the foundational principles for describing the motion of a body.