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acceleration, change in the velocity of a body with respect to time. Since velocity is a vector quantity, involving both magnitude and direction, acceleration is also a vector. In order to produce an acceleration, a force must be applied to the body. The magnitude of the force *F* must be directly proportional to both the mass of the body *m* and the desired acceleration *a,* according to Newton's second law of motion, *F*=*ma.* The exact nature of the acceleration produced depends on the relative directions of the original velocity and the force. A force acting in the same direction as the velocity changes only the speed of the body. An appropriate force acting always at right angles to the velocity changes the direction of the velocity but not the speed. An example of such an accelerating force is the gravitational force exerted by a planet on a satellite moving in a circular orbit. A force may also act in the opposite direction from the original velocity. In this case the speed of the body is decreased. Such an acceleration is often referred to as a deceleration. If the acceleration is constant, as for a body falling near the earth, the following formulas may be used to compute the acceleration *a* of a body from knowledge of the elapsed time *t,* the distance *s* through which the body moves in that time, the initial velocity *v*_{i}, and the final velocity *v*_{f}:

a=(v_{f}^{2}-v_{i}^{2})/2sa=2(s-v_{i}t)/t^{2}a=(v_{f}-v_{i})/t

The Columbia Electronic Encyclopedia Copyright © 2004.

Licensed from Columbia University Press

Licensed from Columbia University Press

- For the waltz composed by Johann Strauss, see Accelerationen.

In kinematics, acceleration is defined as the first derivative of velocity with respect to time (that is, the rate of change of velocity), or equivalently as the second derivative of position. It is a vector quantity with dimension L T^{−2}. In SI units, acceleration is measured in metres per second squared (m/s^{2}).

In common speech, the term acceleration is only used for an increase in speed (the magnitude of velocity); a decrease in speed is called deceleration. In physics, any increase or decrease in speed is referred to as acceleration, and also a change in the direction of velocity is an acceleration (the centripetal acceleration; whereas the rate of change of speed is the tangential acceleration).

In classical mechanics, the acceleration of a body is proportional to the resultant (total) force acting on it (Newton's second law):

- $mathbf\{F\}\; =\; mmathbf\{a\}\; quad\; to\; quad\; mathbf\{a\}\; =\; mathbf\{F\}/m$

- $mathbf\{a\}\; =\; frac\{mathrm\{d\}v\}\{mathrm\{d\}t\}\; mathbf\{u\}\_mathrm\{t\}\; +\; frac\{v^2\}\{R\}mathbf\{u\}\_mathrm\{n\}$

- Uniform acceleration
- Angular acceleration
- Coordinate vs. physical acceleration
- Derivatives of position
- Equations of Motion
- Proper Acceleration
- 0 to 60 mph
- Shock (mechanics)

- Acceleration and Free Fall - a chapter from an online textbook
- Trajectories and Radius, Velocity, Acceleration on Project PHYSNET (ERROR - PAGE MOVED)
- Science aid: Movement
- The physics classroom
- Science.dirbix: Acceleration
- Acceleration Calculator
- Motion Characteristics for Circular Motion
- Practical Guide to Accelerometers

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Last updated on Saturday October 11, 2008 at 12:28:44 PDT (GMT -0700)

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This article is licensed under the GNU Free Documentation License.

Last updated on Saturday October 11, 2008 at 12:28:44 PDT (GMT -0700)

View this article at Wikipedia.org - Edit this article at Wikipedia.org - Donate to the Wikimedia Foundation

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