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  1. 1: mass one (kg) m 2 : mass two (kg) d : distance between objects (m) Ƭ: Torque (Nm) F : Perpendicular Force (N) T: Period (s) f: Frequency (Hz) 1 and F 2 represent two different forces created by object 1 or 2 (N) d 1 and d 2 represent two different distances that object one or two are from the fulcrum or

  2. Kinematic equations relate the variables of motion to one another. Each equation contains four variables. The variables include acceleration (a), time (t), displacement (d), final velocity (vf), and initial velocity (vi).

  3. HT = Higher Tier only equations. kinetic energy = 0.5 × mass × (speed)2. k 2. elastic potential energy = 0.5 × spring constant × (extension)2. e k e2. 2. gravitational potential energy = mass × gravitational field strength × height. p = m g h. change in thermal energy = mass × specific heat capacity × temperature change.

  4. d1 and d2 represent two different distances that object one or two are from the fulcrum or rotational point. d : distance between objects (m) m2 : mass two. π : pie (3.14 rounded) G : universal gravitation constant. Fg : Force of Gravity (N)

  5. Frequently used equations in physics. Appropriate for secondary school students and higher. Mostly algebra based, some trig, some calculus, some fancy calculus.

  6. Kinematic equations relate the variables of motion to one another. Each equation contains four variables. The variables include acceleration (a), time (t), displacement (d), final velocity (vf), and initial velocity (vi).

  7. Uniformly accelerated motion is described in terms of relationships between measurable scalar and vector quantities, including displacement, speed, velocity, and acceleration. Solve problems using equations for constant acceleration and a =. Interpret solutions to problems in a variety of contexts.

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