= Newton–Euler equations
{wiki=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.
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