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Speed
Distance ÷ Time
Velocity
Displacement ÷ Time
Acceleration
Change in velocity ÷ Time
Retardation
Negative acceleration
Uniform Motion
Equal distances in equal intervals
Non-uniform Motion
Unequal distances in equal intervals
Equation of Motion 1
v = u + at
Equation of Motion 2
s = ut + ½at²
Equation of Motion 3
v² = u² + 2as
Momentum
p = m × v
Impulse
Force × Time
Impulse-Momentum
The change in momentum
Newton’s Second Law
F = m × a
Weight
W = m × g
Gravitational Force
F = G × (m1m2 / r²)
Work Done
Force × Displacement
Work Against Gravity
m × g × h
Power
Work ÷ Time
Power (alternative)
Force × Velocity
Energy
Capacity to do work
Kinetic Energy
½ m v²
Potential Energy
m g h
Mechanical Energy
K.E + P.E
Pressure
Force ÷ Area
Thrust
Force perpendicular to surface
Density
Mass ÷ Volume
Relative Density
Density of substance ÷ Density of water
Archimedes Principle Loss of weight
Buoyant force = Weight of fluid displaced
Heat
Q = m × c × ΔT
Heat Capacity
m × c
Latent Heat
Q = m × L
Principle of Calorimetry
Heat lost = Heat gained
Current
I = Q ÷ t
Potential Difference
V = W ÷ Q
Ohm’s Law
V = I × R
Resistance formula
R = ρ × (L/A)
Resistivity Constant
Depends on material
Power formula 1
P = V × I
Power formula 2
P = I²R
Power formula 3
P = V² ÷ R
Electrical Energy
P × t
Commercial Unit
kWh (kilowatt-hour)
Series Resistance
R = R1 + R2 + R3
Parallel Resistance
1/R = 1/R1 + 1/R2 + 1/R3
Series Potential
Divides according to resistance
Parallel Potential
Same across all branches
Heat Produced in Wire
H = I² R t (Joule’s Law)
Specific Resistance
Resistance × (Area ÷ Length)
Work Function
hν₀
Photon Energy
E = hν
Einstein’s Photoelectric Equation
hν = hν₀ + ½mv²max
Refractive Index
n = sin i ÷ sin r
Refractive Index (speed)
n = c ÷ v
Critical Angle
sin C = 1/n
Lens Formula
1/v – 1/u = 1/f
Magnification (lenses)
m = v/u
Power of Lens
P = 1/f (in metres)
Total Power
P = P1 + P2
Mirror Formula
1/u + 1/v = 1/f
Magnification (mirror)
Height of image ÷ Height of object
Magnification (mirror 2)
–v/u
Wave Speed
v = f × λ
Frequency
1 ÷ Time period
Numerical Aperture
n sin θ
Echo Formula
Distance = Speed × Time/2
Mechanical Advantage
Load ÷ Effort
Velocity Ratio
Distance moved by effort ÷ distance moved by load
Efficiency
(MA ÷ VR) × 100
Lever Principle
Effort × Effort arm = Load × Load arm
Transformer Equation
Vp ÷ Vs = Np ÷ Ns
Transformer Power
Input power = Output power (ideal)
Step-up Transformer
Secondary > Primary
Step-down Transformer
Primary > Secondary
Force on Charge
F = qE
Electrical Power Loss
P = I²R
Safe Fuse Rating
Power ÷ Voltage
Moment of Force
Force × Perpendicular distance
Principle of Moments
Clockwise moment = Anti-clockwise moment
Center of Gravity
Depends on symmetry and distribution
Universal Gravitational Constant
F = G(m1m2/r²)
Pressure in Fluids
hρg
Upthrust
Weight of displaced liquid
Pendulum Time Period
T = 2π √(L/g)