Acceleration In physics, acceleration (symbol: a) is defined as the rate of change (or time derivative) of velocity. It is thus a vector quantity with dimension length/time². In SI units, this is meter/second².
To accelerate an object is to change its velocity over a period of time. In this strict scientific sense, acceleration can have positive and negative values—respectively called acceleration and deceleration (or retardation) in common speech—as well as change of direction. Acceleration is defined technically as "the rate of change of velocity of an object with respect to time" and is given by the equation \n:\nwhere a is the acceleration vector, v is the velocity vector expressed in m/s, and t is time expressed in seconds. This equation gives a the units of m/(s·s), or m/s² (read as "meters per second per second", or "meters per second squared").
An alternative equation is:\n:\nwhere is average acceleration (m/s²), u is initial velocity (m/s), v is final velocity (m/s), and t is time (s).
One common unit of acceleration is g, one g being the acceleration caused by the gravity of Earth at sea level at 45° latitude (Paris), or about 9.81 m/s².
In classical mechanics, acceleration a is related to force F and mass m (assumed to be constant) by way of Newton's second law:
External link\n*Conversion: acceleration - English and American units to metric units\nSee also: equation of motion Category:Physical quantity \n\n\n \n\n\n\n\n\n\n\nsimple:Acceleration\n\nzh-cn:加速度 |
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