acceleration of a falling body - перевод на греческий
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acceleration of a falling body - перевод на греческий

MATHEMATICAL DESCRIPTION OF A BODY IN FREE FALL
Apples fall from trees; Law of falling bodies; Falling bodies; Law of fall; Falling body
  • ''g''}} is the acceleration of gravity.
  • An initially stationary object which is allowed to fall freely under gravity falls a distance proportional to the square of the elapsed time. This image, spanning half a second, was captured with a stroboscopic flash at 20 flashes per second. During the first 0.05 s the ball drops one unit of distance (about 12 mm), by 0.10 s it has dropped at total of 4 units, by 0.15 s 9 units, and so on.

acceleration of a falling body      
επιτάχυνση σώματος που πέφτει
επιτάχυνση σώματος που πέφτει      
acceleration of a falling body
tangential acceleration         
  • ''s''(''t'')}}.
}}
  • Δ'''v'''/Δ''t''}}
  • '''a'''<sub>c</sub>}} is due to the change in direction of the velocity vector and is normal to the trajectory, pointing toward the center of curvature of the path.
  • '''a'''}}.
  • An oscillating pendulum, with velocity and acceleration marked. It experiences both tangential and centripetal acceleration.
  • Calculation of the speed difference for a uniform acceleration
RATE AT WHICH THE MAGNITUDE AND/OR DIRECTION OF VELOCITY CHANGES WITH TIME
Accelerate; Centripetal acceleration; Deceleration; Accelerative; Accelerating; Accelerations; Centripetal Acceleration; Accelleration; Uniform acceleration; Constant acceleration; Tangental acceleration; Accelerated motion; Accelerated Motion; Radial acceleration; Tangential acceleration; Second temporal derivative of displacement; Uniform Acceleration; Linear acceleration; Exceleration; Decelerating; Constant acceleration formulae; Instantaneous acceleration; Aceleration; Acceleration (physics); Accerlation
επιτάχυνση κατά την εφαπτομένη

Определение

acceleration
n.
Hastening, increase of velocity. See preceding verb.

Википедия

Equations for a falling body

A set of equations describing the trajectories of objects subject to a constant gravitational force under normal Earth-bound conditions. Assuming constant acceleration g due to Earth’s gravity, Newton's law of universal gravitation simplifies to F = mg, where F is the force exerted on a mass m by the Earth’s gravitational field of strength g. Assuming constant g is reasonable for objects falling to Earth over the relatively short vertical distances of our everyday experience, but is not valid for greater distances involved in calculating more distant effects, such as spacecraft trajectories.