Acceleration
Let a particle travel a distance
as a function
of time
(here,
can be thought
of as the arc length of the curve traced out by the
particle). The speed (the scalar norm of the vector velocity)
is then given by
|
(1)
|
The acceleration is defined as the time derivative of the velocity, so the scalar acceleration is given by
|
(2)
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|
(3)
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(4)
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|
(5)
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(6)
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The vector acceleration is given by
|
(7)
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|
(8)
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(9)
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where
is the unit tangent vector,
the curvature,
the arc length, and
the unit normal
vector.
Let a particle move along a straight line so that the positions at times
,
, and
are
,
, and
, respectively.
Then the particle is uniformly accelerated with acceleration
iff
|
(10)
|
is a constant (Klamkin 1995, 1996).
Consider the measurement of acceleration in a rotating reference frame. Apply the rotation operator
|
(11)
|
twice to the radius vector
and suppress the
body notation,
|
(12)
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(13)
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(14)
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(15)
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|
(16)
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Grouping terms and using the definitions of the velocity
and angular
velocity
gives the expression
|
(17)
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Now, we can identify the expression as consisting of three terms
|
(18)
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(19)
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(20)
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a "body" acceleration, centrifugal acceleration, and Coriolis acceleration. Using these definitions finally gives
|
(21)
|
where the fourth term will vanish in a uniformly rotating frame of reference (i.e.,
). The centrifugal acceleration is familiar
to riders of merry-go-rounds, and the Coriolis acceleration is responsible for the
motions of hurricanes on Earth and necessitates large trajectory corrections for
intercontinental ballistic missiles.

centripetal acceleration
formula

