The Standard Values:
V = Velocity / Speed;
d = Displacement / Distance;
t = Time / Duration;
a = Acceleration / Change in Speed / Change in Velocity;
Formulas for V:
V = a . t ;
V = d / t ;
Formulas for d:
d = V. t ; //linear distance formula: used when "No Change in Speed" or "Acceleration".
d = 1/2 a . t2 ; //quadratic distance formula: used when finding the Displacement of the Projectile on its highest peak before it goes down, when there is "Change in Speed" or "Acceleration".
Formulas for t:
t = V / a ;
t = d / V ;
Formulas for a:
a = V / t ;
a = V2 / 2 d ;
a = 2 d / t2 ;
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Fundamental Formulas:
MASS = (density) x (volume per unit) ;
FORCE = (mass) x (acceleration) ;
WORK = (force) x (displacement);
POWER = (force) x (velocity);
MOMENTUM = (mass) x (velocity);
WEIGHT = (mass) x (gravitational force);
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Law of Conservation of Energy:
"Energy can never be created nor be destroyed... Energy can change."
Ei = Ef ; // initial energy = final energy ;
PEi + KEi = PEf + KEf ; // sum of initial PE & KE = sum of final PE & KE ;
m.g.Yi + 1/2 m.Vi2 = m.g.Yf + 1/2 m.Vf2 ;
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One-Dimensional Motion (Free-Falling Motion
with Constant Acceleration):
Y = height / vertical distance in meters;
(X = range / horizontal distance);
Vi = initial speed in meters/seconds;
Vf = final speed in meters/seconds;
m = mass in kilograms;
g = gravitational force = acceleration inclined with the gravity of Planet Earth (constant value for gravitational force = 9.8 m/s2);
Solving for ΔY:
m.g.Yi + 1/2 m.Vi2 = m.g.Yf + 1/2 m.Vf2 ; // This the Initial Equation.
m.g.Yf - m.g.Yi = 1/2 m.Vi2 - 1/2 m.Vf2 ; // Step 1 : Arrange ;
m.g.Yf - m.g.Yi = 1/2 m.Vi2 - 1/2 m.Vf2 ; // Step 2 : Eliminate common terms ;
[g.Yf - g.Yi = 1/2 Vi2 - 1/2 Vf2 ] 1/2 g ; // Step 3 : Multiply each side by its common terms ;
Yf - Yi = (Vi2 - Vf2 ) / (2 g) ; // This is the Result or Final Equation ;
Note: 'ΔY' is equal to 'final Y' minus 'initial Y'.
"Energy can never be created nor be destroyed... Energy can change."
Ei = Ef ; // initial energy = final energy ;
PEi + KEi = PEf + KEf ; // sum of initial PE & KE = sum of final PE & KE ;
m.g.Yi + 1/2 m.Vi2 = m.g.Yf + 1/2 m.Vf2 ;
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One-Dimensional Motion (Free-Falling Motion
with Constant Acceleration):
Y = height / vertical distance in meters;
(X = range / horizontal distance);
Vi = initial speed in meters/seconds;
Vf = final speed in meters/seconds;
m = mass in kilograms;
g = gravitational force = acceleration inclined with the gravity of Planet Earth (constant value for gravitational force = 9.8 m/s2);
Solving for ΔY:
m.g.Yi + 1/2 m.Vi2 = m.g.Yf + 1/2 m.Vf2 ; // This the Initial Equation.
m.g.Yf - m.g.Yi = 1/2 m.Vi2 - 1/2 m.Vf2 ; // Step 1 : Arrange ;
[
Yf - Yi = (Vi2 - Vf2 ) / (2 g) ; // This is the Result or Final Equation ;
Note: 'ΔY' is equal to 'final Y' minus 'initial Y'.
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