Average speed (ms^-1)
distance (m) / time (s) or v = d/t
Average velocity (ms^-1)
displacement (m) / time (s) or v = s
Period of a pendulum (s)
total time (s) / number of swings or T = t
Acceleration (ms^-2)
(final velocity (ms^-1) - initial velocity (ms^-1)) / time (s) or a = (v - u)/t
Weight (N)
mass (kg) x gravitational field strength (ms^-2) or F = mg
Force (N)
mass (kg) x acceleration (ms^-2) or F = ma
Density (kgm^-3)
mass (kg) / volume (m^3) or rho = M/V
Hooke’s law: Force (N)
constant (Nm^-1) x extension (m) or F = kx
Pressure (Pa)
force (N) / area (m^2) or P = F/A
Fluid Pressure (Pa)
density (kgm^-3) x gravitational field strength (ms^-2 or Nkg^-1) x height (m) or P = rho x g x h
Work (J)
force (N) x distance moved (m) or change in E = Fd
Power (W)
work (J) / time (s) or P = change in E/t
Kinetic Energy (J)
1/2 x mass (kg) x velocity^2 (ms^-2) or KE = 1/2mv^2
Gravitational potential energy (J)
mass (kg) x gravitational field strength (ms^-2 or Nkg^-1) x height (m) or GPE = mgh
Efficiency (%)
useful power output (W) x 100 / total power input (W) or Efficiency = Pout/Pin
Efficiency (%)
useful energy output (J) x 100 / total energy input (J) or Efficiency = Eout/Ein
Moment (Nm)
force (N) x perpendicular distance from pivot (m) or M = Fd
Sum of clockwise moments (Nm)
sum of anticlockwise moments (Nm) or F1d1 = F2d2
Momentum (kgms^-1)
mass (kg) x velocity (ms^-1) or p = mv
Force (N)
change in momentum (kgms^-1) / time (s) or F = change in p/t
Impulse (kgms^-1 or Ns)
change in momentum (kgms^-1) or Ft = change in p
Centripetal Force (N)
mass (kg) x velocity^2 (ms^-2) / radius (m) or F = mv^2/r
Orbital Period (s)
2 x pi x radius (m) / velocity (ms^-1) or T = 2(pi)r/v
Boyle’s Law for changes in gas pressure at constant temperature
P1V1 = P2V2 or PV = constant
Energy (J)
mass (kg) x specific heat capacity (Jkg^-1 x °C^-1) x temperature change (°C) or E = mc(change in)T
Thermal capacity (J°C^-1)
mass (kg) x specific heat capacity (Jkg^-1°C^-1) or C = mc
Energy transferred (J)
mass (kg) x specific latent heat (Jkg^-1) or E = ml
Expansion (m)
linear expansivity (°C^-1) x original length (m) x temperature rise (°C) or Expansion = alpha x l x (change in)T
Current (I)
charge (C) / time (s) or I = Q / t
Voltage (V)
energy transferred (J) / charge (C) or V = E / Q
Voltage (V)
current (I) x resistance (ohms) or V = IR
Power (W)
current (I) x voltage (V) or P = IV
Power (W)
current^2 (I) x resistance (ohms) or P = I^2 x R
Energy transferred (J)
current (I) x voltage (V) x time (s) or (change in)E = IVt
Energy transferred (J)
power (W) x time (s) or (change in)E = Pt
Resistors in series
Total Resistance (ohms) = sum of individual resistors (ohms) or RT = R1 + R2 + R3 + ... + Rn
Resistors in parallel
1 / total resistance (ohms) = sum of individual resistors (ohms) or 1 / Rtotal = 1 / R1 + 1 / R2 + 1 / R3 + ... + 1 / Rn
Resistance (ohms) Note: since wires have a circular cross-section area = pi x radius^2
resistivity (ohms m) x length (m) / area (m^2) or R = rho x l x / A
Transformers
voltage in the secondary coil (V) / voltage in primary coil (V) = turns on secondary coil /turns on primary coil or Vs = Vp / Ns = Np
Transformers
voltage in the primary coil (V) / voltage in the secondary coil (V) = current in the secondary coil (A) / current in the primary coil (A) or Vp = V/s / Is = Ip
Wave speed (ms^-1)
frequency (Hz) × wavelength (m) or c = f(lambda)
Frequency (Hz)
1 / Period (s) or F = 1 / T
Refractive index (n)
sine of the angle of incidence
Refractive index (n)
speed of light in vacuum / speed of light in material or n = cv / cm
Refractive index (n)
1 / sine of the critical angle or n = 1 / sinc
RadioActive alpha decay
Radioactive beta decay
Radioactive gamma decay
Energy (j)
Mass defect (kg) x speed of light² (ms^-1) or E=mc²
The earth speed (v)
2 x (pi) x r / T
Light year (m)
9.5 × 1015m
Hubbles constant (Ho)
v / D or 2.2 × 10–18 per second
Age of the universe
d / v = 1 /Ho