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About: Newton–Euler equations     Goto   Sponge   NotDistinct   Permalink

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Type: yago:Abstraction100002137yago:Communication100033020yago:Equation106669864yago:MathematicalStatement106732169yago:Message106598915yago:Statement106722453yago:WikicatEquations New Facet based on Instances of this Class

In classical mechanics, the Newton–Euler equations describe the combined translational and rotational dynamics of a rigid body. Traditionally the Newton–Euler equations is the grouping together of Euler's two laws of motion for a rigid body into a single equation with 6 components, using column vectors and matrices. These laws relate the motion of the center of gravity of a rigid body with the sum of forces and torques (or synonymously moments) acting on the rigid body.