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  2. List of moments of inertia - Wikipedia

    en.wikipedia.org/wiki/List_of_moments_of_inertia

    = [1] Solid sphere of radius r and mass m. = [1] Sphere (shell) of radius r 2 and mass m, with centered spherical cavity of radius r 1. When the cavity radius r 1 = 0, the object is a solid ball (above).

  3. Moment of inertia - Wikipedia

    en.wikipedia.org/wiki/Moment_of_inertia

    Here, the function gives the mass density at each point (,,), is a vector perpendicular to the axis of rotation and extending from a point on the rotation axis to a point (,,) in the solid, and the integration is evaluated over the volume of the body . The moment of inertia of a flat surface is similar with the mass density being replaced by ...

  4. Shell theorem - Wikipedia

    en.wikipedia.org/wiki/Shell_theorem

    A solid, spherically symmetric body can be modeled as an infinite number of concentric, infinitesimally thin spherical shells.If one of these shells can be treated as a point mass, then a system of shells (i.e. the sphere) can also be treated as a point mass.

  5. Ball (mathematics) - Wikipedia

    en.wikipedia.org/wiki/Ball_(mathematics)

    A ball in n dimensions is called a hyperball or n-ball and is bounded by a hypersphere or (n−1)-sphere. Thus, for example, a ball in the Euclidean plane is the same thing as a disk, the area bounded by a circle. In Euclidean 3-space, a ball is taken to be the volume bounded by a 2-dimensional sphere. In a one-dimensional space, a ball is a ...

  6. Equations of motion - Wikipedia

    en.wikipedia.org/wiki/Equations_of_motion

    Galileo deduced the equation s = ⁠ 1 / 2 ⁠ gt 2 in his work geometrically, [4] using the Merton rule, now known as a special case of one of the equations of kinematics. Galileo was the first to show that the path of a projectile is a parabola. Galileo had an understanding of centrifugal force and gave a correct definition of momentum. This ...

  7. Elastic collision - Wikipedia

    en.wikipedia.org/wiki/Elastic_collision

    The final x and y velocities components of the first ball can be calculated as: [5] ′ = ⁡ () + ⁡ + ⁡ + ⁡ ⁡ (+) ′ = ⁡ () + ⁡ + ⁡ + ⁡ ⁡ (+), where v 1 and v 2 are the scalar sizes of the two original speeds of the objects, m 1 and m 2 are their masses, θ 1 and θ 2 are their movement angles, that is, = ⁡, = ⁡ (meaning ...

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  9. Euler's laws of motion - Wikipedia

    en.wikipedia.org/wiki/Euler's_laws_of_motion

    Euler's second law states that the rate of change of angular momentum L about a point that is fixed in an inertial reference frame (often the center of mass of the body), is equal to the sum of the external moments of force acting on that body M about that point: [1] [4] [5]