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  2. Equilibrant force - Wikipedia

    en.wikipedia.org/wiki/Equilibrant_Force

    Equilibrant force. In mechanics, an equilibrant force is a force which brings a body into mechanical equilibrium. [1] According to Newton's second law, a body has zero acceleration when the vector sum of all the forces acting upon it is zero:

  3. List of types of equilibrium - Wikipedia

    en.wikipedia.org/wiki/List_of_types_of_equilibrium

    Equilibrant force, which keeps any object motionless and acts on virtually every object in the world that is not moving Equilibrium figures of Earth and planets (physical geodesy) Equilibrium mode distribution , the state of fiber optic or waveguide transmission in which the propagation mode does not vary with distance along the fiber or ...

  4. Resultant force - Wikipedia

    en.wikipedia.org/wiki/Resultant_force

    In physics and engineering, a resultant force is the single force and associated torque obtained by combining a system of forces and torques acting on a rigid body via vector addition. The defining feature of a resultant force, or resultant force-torque, is that it has the same effect on the rigid body as the original system of forces. [ 1 ]

  5. Exact solutions of classical central-force problems - Wikipedia

    en.wikipedia.org/wiki/Exact_solutions_of...

    In the classical central-force problem of classical mechanics, some potential energy functions () produce motions or orbits that can be expressed in terms of well-known functions, such as the trigonometric functions and elliptic functions. This article describes these functions and the corresponding solutions for the orbits.

  6. Center of mass - Wikipedia

    en.wikipedia.org/wiki/Center_of_mass

    For a rigid body containing its center of mass, this is the point to which a force may be applied to cause a linear acceleration without an angular acceleration. Calculations in mechanics are often simplified when formulated with respect to the center of mass. It is a hypothetical point where the entire mass of an object may be assumed to be ...

  7. Two-body problem in general relativity - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem_in...

    The two-body problem in general relativity (or relativistic two-body problem) is the determination of the motion and gravitational field of two bodies as described by the field equations of general relativity. Solving the Kepler problem is essential to calculate the bending of light by gravity and the motion of a planet orbiting its sun.

  8. Reaction (physics) - Wikipedia

    en.wikipedia.org/wiki/Reaction_(physics)

    This support force is an 'equal and opposite' force; we know this not because of Newton's third law, but because the object remains at rest, so that the forces must be balanced. To this support force there is also a 'reaction': the object pulls down on the supporting cable, or pushes down on the supporting surface or liquid.

  9. Statically indeterminate - Wikipedia

    en.wikipedia.org/wiki/Statically_indeterminate

    =: the sum of the vertical components of forces equals zero; ∑ M = 0 : {\displaystyle \sum \mathbf {M} =0:} the sum of the moments (about an arbitrary point) of all forces equals zero. Free body diagram of a statically indeterminate beam