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  2. Specific angular momentum - Wikipedia

    en.wikipedia.org/wiki/Specific_angular_momentum

    Using the velocity vector in place of the rate of change of position, and for the specific angular momentum: = is constant. This is different from the normal construction of momentum, r × p {\displaystyle \mathbf {r} \times \mathbf {p} } , because it does not include the mass of the object in question.

  3. Velocity - Wikipedia

    en.wikipedia.org/wiki/Velocity

    Velocity is the speed in combination with the direction of motion of an object. Velocity is a fundamental concept in kinematics, the branch of classical mechanics that describes the motion of bodies. Velocity is a physical vector quantity: both magnitude and direction are needed to define it.

  4. Momentum - Wikipedia

    en.wikipedia.org/wiki/Momentum

    In SI units, if the mass is in kilograms and the velocity is in meters per second then the momentum is in kilogram meters per second (kg⋅m/s). In cgs units, if the mass is in grams and the velocity in centimeters per second, then the momentum is in gram centimeters per second (g⋅cm/s). Being a vector, momentum has magnitude and direction.

  5. Wave vector - Wikipedia

    en.wikipedia.org/wiki/Wave_vector

    The wave vector and angular wave vector are related by a fixed constant of proportionality, 2 π radians per cycle. It is common in several fields of physics to refer to the angular wave vector simply as the wave vector, in contrast to, for example, crystallography. [1] [2] It is also common to use the symbol k for whichever is in use.

  6. Angular velocity - Wikipedia

    en.wikipedia.org/wiki/Angular_velocity

    In physics, angular velocity (symbol ω or , the lowercase Greek letter omega), also known as the angular frequency vector, [1] is a pseudovector representation of how the angular position or orientation of an object changes with time, i.e. how quickly an object rotates (spins or revolves) around an axis of rotation and how fast the axis itself changes direction.

  7. Eccentricity vector - Wikipedia

    en.wikipedia.org/wiki/Eccentricity_vector

    For Kepler orbits the eccentricity vector is a constant of motion. Its main use is in the analysis of almost circular orbits, as perturbing (non-Keplerian) forces on an actual orbit will cause the osculating eccentricity vector to change continuously as opposed to the eccentricity and argument of periapsis parameters for which eccentricity zero ...

  8. Relative velocity - Wikipedia

    en.wikipedia.org/wiki/Relative_velocity

    is the velocity of the Man relative to the Train, v T ∣ E {\displaystyle \mathbf {v} _{T\mid E}} is the velocity of the T rain relative to E arth. Fully legitimate expressions for "the velocity of A relative to B" include "the velocity of A with respect to B" and "the velocity of A in the coordinate system where B is always at rest".

  9. Four-velocity - Wikipedia

    en.wikipedia.org/wiki/Four-velocity

    A four-velocity is thus the normalized future-directed timelike tangent vector to a world line, and is a contravariant vector. Though it is a vector, addition of two four-velocities does not yield a four-velocity: the space of four-velocities is not itself a vector space. [nb 2]