Velocity Guide, Meaning , Facts, Information and Description
Velocity (symbol:
v) is a
vector measurement of the rate and direction of motion. The
scalar absolute value (
magnitude) of velocity is
speed. Velocity can also be defined as rate of change of
displacement or just as the rate of
displacement, depending on how the term
displacement is used (see article on
displacement). It is thus a vector quantity with dimension length/time. In
SI units this is
metre per second
In mechanics the average speed v of an object moving a distance d during a time interval t is described by the simple formula:
The instantaneous velocity vector
v of an object whose position at time
t is given by
x(
t) can be computed as the
derivative
Acceleration is the rate of change of an object's velocity over time. The average acceleration of
a of an object whose speed changes from
vi to
vf during a time interval
t is given by:
The instantaneous acceleration vector
a of an object whose position at time
t is given by
x(
t) is
The final velocity
vf of an object which starts with velocity
vi and then accelerates at constant acceleration
a for a period of time
t is:
The average velocity of an object undergoing constant acceleration is (
vi +
vf)/2. To find the displacement
d of such an accelerating object during a time interval
t, substitute this expression into the first formula to get:
When only the object's initial velocity is known, the expression
can be used. These basic equations for final velocity and displacement can be combined to form an equation that is independent of time:
The above equations are valid for both
classical mechanics and
special relativity. Where
classical mechanics and
special relativity differ is in how different observers would describe the
same situation. In particular, in
classical mechanics, all observers
agree on the value of
t and the transformation rules for position
create a situation in which all non-accelerating observers would describe
the acceleration of an object with the same values. Neither is true
for
special relativity.
The kinetic energy (movement energy) of a moving object is linear with both its mass and the square of its velocity:
The kinetic energy is a
scalar quantity.
Polar coordinates
In connection with polar coordinates, 2D velocity can be decomposed into radial velocity, away from or toward the origin, and transverse velocity, in the perpendicular direction, changing the direction of the body from the origin, and equal to the distance to the origin times the angular velocity.
Angular momentum in scalar form is the distance to the origin times the transverse speed, or equivalently, the distance squared times the angular speed, with a plus or minus to distinguish clockwise and anti-clockwise direction.
If forces are in radial direction only, as in the case of a gravitational orbit, angular momentum is constant, hence transverse speed is inversely proportial to the distance, angular speed is inversely proportial to the distance squared, and the rate at which area is swept out is constant (Kepler's second law).
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