• Shuffle
    Toggle On
    Toggle Off
  • Alphabetize
    Toggle On
    Toggle Off
  • Front First
    Toggle On
    Toggle Off
  • Both Sides
    Toggle On
    Toggle Off
  • Read
    Toggle On
    Toggle Off
Reading...
Front

Card Range To Study

through

image

Play button

image

Play button

image

Progress

1/19

Click to flip

Use LEFT and RIGHT arrow keys to navigate between flashcards;

Use UP and DOWN arrow keys to flip the card;

H to show hint;

A reads text to speech;

19 Cards in this Set

  • Front
  • Back

Displacement (s)

Distance traveled in a particular direction (change in position)

Velocity (v; sometimes u)

Rate of change of displacement

Speed (v; sometimes u)

Rate of change of distance

Acceleration (a)

Rate of change of velocity

Newton's First Law of Motion

An object at rest remains at rest and an object in motion remains in motion at a constant speed in a straight line unless acted on by an unbalanced force.

Newton's Second Law of Motion

An unbalanced force will cause an object to accelerate in the direction of the net force. The acceleration of the object is proportional to the net force and inversely proportional to its mass.



F = ma; also F = Δp/Δt (net force = rate of change of momentum)

Newton's Third Law of Motion

When two bodies A and B interact (push or pull), the force that A exerts on B is equal and opposite to the force that B exerts on A.

Translational Equilibrium

The net force acting on a body is zero

Momentum (p)

Product of mass and velocity. Sometimes called "linear momentum".



p = mv

Impulse (J)

Change in momentum.



Impulse = FΔt; Impulse = mΔv

Law of Conservation of Momentum

The total momentum of an isolated system (no external forces) remains constant.

Work (W)

The product of a force on an object and the displacement of the object in the direction of the force.



W = Fs; W = Fs cos θ

Kinetic Energy (EK)

Product of 1⁄2 times the mass of an object times the square of an object’s speed



EK = 1/2 * mv^2

Gravitational Potential Energy (EP)

Product of an object’s mass times the gravitational field strength times the change in height



EP = mgΔh

Principle of Conservation of Energy

The total energy of an isolated system (no external forces) remains constant.



OR



Energy can be neither created nor destroyed but only transformed from one form to another or transferred from one object to another.

Elastic collision

A collision in which kinetic energy is conserved

Inelastic collision

A collision in which kinetic energy is not conserved

Power (P)

The rate at which work is done or the rate at which energy is transferred



Power = Work / time; Power = Energy transfer / time

Efficiency (Eff)

The ratio of the useful energy (or power or work) output to the total energy (or power or work) input



Eff = out / in