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abstraction > mathematical concept > number > quantity > velocity |
velocity comparison table |
Subject | has synonym | has definition |
---|---|---|
equatorial velocity | The velocity at the surface of a rotating body, on its equator | |
escape velocity | The velocity that a body requires to achieve a parabolic orbit around its primary (Ve = sqrt(2GM/R)). Escape velocity at Earth's surface is 11.2 km s-1; of Moon, 2.4 km s-1; of Sun, 617.7 km s-1 (cf. orbital velocity). | |
galactic velocity component | One of three components of a star's motion with respect to the center of a galaxy. | |
galaxy peculiar velocity | A deviation in the velocity of a galaxy from that expected on the basis of a uniform expansion of the universe. (See Hubble law.) | |
orbital velocity | Velocity required by a body to achieve a circular orbit around its primary: Vorb = (GM / r)1/2. | |
peculiar velocity | Velocity with respect to the Local Standard of Rest. | |
radial velocity | The speed at which an object moves toward or away from us. It can be measured from a star's spectrum: a star moving toward us has a blueshifted spectrum, and a star moving away from us has a redshifted spectrum. The larger the blueshift or redshift, the larger the radial velocity. The present radial-velocity champion is a star in the constellation Lacerta named Giclas 233-27, which moves toward us at 583 kilometers per second. | |
space motion | Velocity of a star with respect to the Sun; hypotenuse of the right triangle formed by its radial and tangential velocities (cf. peculiar velocity). Space motion vectors are U (in the direction of the galactic anticenter), V (in the direction of galactic rotation), and W (in the direction of the galactic north pole). | |
tangential velocity | transverse velocity | A star's velocity across an observer's line of sight. To calculate a star's tangential velocity, one must know the star's distance and proper motion. |