⚑ Study Materials

Physics
Study Notes

All notes follow the official WAEC and JAMB approved syllabus. Study a topic first, then take the practice quiz β€” after the test, come back here to see which topics you need to improve.

Ready to test yourself? Jump straight into practice.

100 WAEC & JAMB-style questions Β· 60 minutes Β· Instant score breakdown by topic

⚑ Start practice test β†’
βš™οΈ

Scalars, Vectors & Motion

Distance, displacement, speed, velocity, acceleration, projectiles

πŸ‹οΈ

Newton's Laws & Forces

Three laws of motion, momentum, friction, equilibrium

⚑

Work, Energy & Power

KE, PE, conservation of energy, machines, efficiency

πŸ’§

Pressure & Fluids

Pressure, Archimedes, upthrust, floating and sinking

〰️

Wave Properties

Frequency, wavelength, amplitude, reflection, refraction, diffraction

πŸ”Š

Sound Waves

Speed of sound, echo, resonance, pitch, loudness

πŸ”¦

Reflection & Mirrors

Laws of reflection, plane and curved mirrors, image formation

πŸ”­

Refraction & Lenses

Snell's law, TIR, convex and concave lenses, eye defects

πŸ”‹

Electrostatics & Circuits

Charge, current, voltage, series and parallel circuits

⚑

Ohm's Law & Resistance

V = IR, resistors, power, energy, fuses, safety

🧲

Magnetism & Electromagnetism

Magnetic fields, electromagnetic induction, transformers, motors

🌑️

Heat Transfer & Temperature

Conduction, convection, radiation, specific heat, latent heat

πŸ”₯

Gas Laws & Thermodynamics

Boyle's, Charles', pressure law, absolute zero, ideal gas

☒️

Radioactivity & Nuclear Physics

Alpha, beta, gamma, half-life, fission, fusion

πŸ’‘

Electronics & Photoelectric Effect

Diodes, transistors, logic gates, photoelectric effect

Overview / Scalars, Vectors & Motion

Scalars, Vectors & Motion

βœ“ WAECβœ“ JAMB
πŸ“
Scalars vs Vectors
Quantity TypeDefinitionExamples
ScalarHas magnitude (size) onlyMass, speed, distance, time, temperature, energy
VectorHas both magnitude AND directionVelocity, displacement, force, acceleration, momentum, weight
🎯

Most tested distinction: Speed is scalar, velocity is vector. Distance is scalar, displacement is vector. Mass is scalar, weight is vector (weight = mg, directed downward).

πŸƒ
Equations of Motion (Uniformly Accelerated)

These four equations apply when acceleration is constant. u = initial velocity, v = final velocity, a = acceleration, t = time, s = displacement.

EquationVariables linked
v = u + atv, u, a, t (no s)
s = ut + Β½atΒ²s, u, a, t (no v)
vΒ² = uΒ² + 2asv, u, a, s (no t)
s = Β½(u + v)ts, u, v, t (no a)
Example β€” Free fall under gravity

A stone dropped from rest falls for 3 s. Find distance fallen. (g = 10 m/sΒ²)
u = 0, a = g = 10 m/sΒ², t = 3 s
s = ut + Β½atΒ² = 0 + Β½ Γ— 10 Γ— 9 = 45 m

🎯
Projectile Motion

A projectile moves under gravity alone after being launched. The horizontal and vertical motions are independent.

  • Horizontal: constant velocity (no acceleration) β€” use s = vt
  • Vertical: uniform acceleration due to gravity (g = 10 m/sΒ²)
  • At the maximum height, the vertical velocity = 0
  • Time of flight: t_total = 2u sinΞΈ / g (for projectile at angle ΞΈ)
⚠️

A ball thrown horizontally has zero initial vertical velocity. It falls vertically at the same rate as a ball simply dropped from the same height β€” they both hit the ground at the same time.

Overview / Newton's Laws & Forces

Newton's Laws & Forces

βœ“ WAECβœ“ JAMB
βš™οΈ
Newton's Three Laws of Motion
LawStatementKey Concept
1st Law (Inertia)A body remains at rest or in uniform motion in a straight line unless acted upon by an external force.Inertia β€” tendency to resist change in motion. Mass measures inertia.
2nd LawThe rate of change of momentum of a body is proportional to the applied force and acts in the direction of the force.F = ma. Larger force β†’ larger acceleration.
3rd Law (Action-Reaction)For every action, there is an equal and opposite reaction.Forces always come in pairs. They act on different bodies.
Newton's 2nd Law β€” F = ma

A 5 kg block accelerates at 3 m/sΒ². Net force = 5 Γ— 3 = 15 N.

πŸ”„
Momentum & Impulse

Momentum = mass Γ— velocity (p = mv). Unit: kgΒ·m/s. It is a vector quantity.
Impulse = Force Γ— time = change in momentum (Ft = mv βˆ’ mu).
Law of conservation of momentum: In the absence of external forces, total momentum before = total momentum after a collision.

🎯

Friction is a resistive force opposing relative motion. Static friction β‰₯ kinetic friction. Reducing friction: lubrication, ball bearings, smooth surfaces. Friction is useful in car brakes, walking, writing.

Overview / Work, Energy & Power

Work, Energy & Power

βœ“ WAECβœ“ JAMB
πŸ“
Definitions & Formulas
QuantityFormulaUnitKey Note
WorkW = F Γ— d Γ— cosΞΈJoule (J)No work done if force βŠ₯ to motion (ΞΈ = 90Β°)
Kinetic EnergyKE = Β½mvΒ²Joule (J)Energy due to motion
Potential EnergyPE = mghJoule (J)Energy due to position above ground
PowerP = W / t = FvWatt (W)Rate of doing work
EfficiencyΞ· = (useful output Γ· total input) Γ— 100%%Always less than 100% due to friction
Conservation of Energy Example

A 2 kg ball is dropped from 5 m height.
PE at top = mgh = 2 Γ— 10 Γ— 5 = 100 J
KE just before hitting ground = 100 J (all PE converts to KE, ignoring air resistance)
Speed: KE = Β½mvΒ² β†’ 100 = Β½ Γ— 2 Γ— vΒ² β†’ v = 10 m/s

βš™οΈ
Simple Machines

Mechanical Advantage (MA) = Load Γ· Effort
Velocity Ratio (VR) = Effort distance Γ· Load distance
Efficiency = (MA Γ· VR) Γ— 100%

MachineExample / VR
LeverCrowbar, scissors. VR = effort arm Γ· load arm
Pulley systemVR = number of pulleys (or segments supporting load)
Inclined planeVR = length Γ· height of plane
Wheel & axleVR = radius of wheel Γ· radius of axle
🎯

A machine cannot have efficiency > 100%. Efficiency is always less than 100% in practice because some energy is always lost to friction, heat, and sound.

Overview / Pressure & Fluids

Pressure & Fluids

βœ“ WAECβœ“ JAMB
πŸ’§
Pressure β€” Key Formulas

Pressure = Force / Area (P = F/A). Unit: Pascal (Pa) = N/mΒ²
Pressure in a liquid: P = ρgh (density Γ— g Γ— depth). Pressure increases with depth and with liquid density.

Atmospheric Pressure

Standard atmospheric pressure = 101,325 Pa β‰ˆ 1 atm β‰ˆ 760 mmHg.
Measured by a barometer. A manometer measures gas pressure.

🚒
Archimedes' Principle & Flotation

Archimedes' Principle: When a body is wholly or partially immersed in a fluid, it experiences an upthrust (buoyant force) equal to the weight of fluid displaced.

Upthrust = Weight of fluid displaced = ρ_fluid Γ— V_submerged Γ— g

Conditions for Floating

A body floats when: Upthrust = Weight of body (density of object ≀ density of fluid).
A body sinks when: Weight > Upthrust (density of object > density of fluid).

🎯

Relative density (specific gravity) = density of substance Γ· density of water. If relative density < 1, the substance floats in water. Ships float because their average density (hull + air inside) is less than water.

Overview / Wave Properties

Wave Properties

βœ“ WAECβœ“ JAMB
〰️
Wave Terms & Formulas
TermDefinitionUnit
Amplitude (A)Maximum displacement from equilibrium positionmetres (m)
Wavelength (Ξ»)Distance between two successive crests (or troughs)metres (m)
Frequency (f)Number of complete oscillations per secondHertz (Hz)
Period (T)Time for one complete oscillation. T = 1/fseconds (s)
Wave speed (v)v = fΞ» (wave equation)m/s
πŸ“Š
Types of Waves & Wave Behaviours
TypeDescriptionExample
TransverseParticles vibrate perpendicular to direction of wave travelLight, water surface waves, electromagnetic waves
LongitudinalParticles vibrate parallel to direction of wave travel (compressions and rarefactions)Sound, seismic P-waves
MechanicalRequire a material medium β€” cannot travel in vacuumSound, water waves
ElectromagneticDo NOT require a medium β€” travel in vacuum at speed of lightLight, radio, X-rays, microwaves
Wave Behaviours β€” Definitions

Reflection: Wave bounces off a surface. Angle of incidence = angle of reflection.
Refraction: Wave changes direction as it enters a new medium (speed changes).
Diffraction: Wave bends around obstacles or through gaps.
Interference: Two waves superpose β€” constructive (crests meet) or destructive (crest meets trough).

🎯

Speed of light in vacuum = 3 Γ— 10⁸ m/s. Speed of sound in air β‰ˆ 340 m/s. Sound cannot travel in a vacuum. Light can. This is tested every year in WAEC and JAMB.

Overview / Sound Waves

Sound Waves

βœ“ WAECβœ“ JAMB
πŸ”Š
Sound β€” Key Facts
  • Sound is a longitudinal mechanical wave β€” it requires a medium to travel.
  • Speed of sound: fastest in solids, slower in liquids, slowest in gases.
  • Sound travels at approximately 340 m/s in air at room temperature.
  • Pitch depends on frequency. High frequency = high pitch.
  • Loudness depends on amplitude. Large amplitude = loud sound.
  • Quality (timbre) depends on the waveform β€” distinguishes different instruments.
πŸ”
Echo, Resonance & Hearing Range

Echo: Reflection of sound from a hard surface. For an echo to be heard separately, the reflecting surface must be at least 17 m away (so the reflected sound reaches the ear at least 0.1 s after the original).

Resonance: When a body is forced to vibrate at its own natural frequency β€” the amplitude becomes very large. Examples: Soldiers break step on bridges to avoid resonance.

Human hearing range: 20 Hz to 20,000 Hz (20 kHz).
Infrasound: Below 20 Hz. Ultrasound: Above 20 kHz (used in medicine, sonar).

🎯

Sonar uses ultrasound to detect underwater objects. Doppler effect: Apparent change in frequency when source or observer is moving. As source approaches, frequency appears to increase; as it moves away, frequency appears to decrease.

Overview / Reflection & Mirrors

Reflection & Mirrors

βœ“ WAECβœ“ JAMB
πŸ”¦
Laws of Reflection & Plane Mirror

Laws of Reflection:
1. The angle of incidence equals the angle of reflection (i = r).
2. The incident ray, reflected ray, and normal all lie in the same plane.

Image in a Plane Mirror

The image is: Virtual, upright, same size as object, laterally inverted, and the same distance behind the mirror as the object is in front of it.

πŸͺž
Curved Mirrors β€” Concave & Convex
Mirror TypeAlso calledUsesKey feature
Concave (hollow)Converging mirrorTorches, makeup mirrors, car headlights, solar cookers, shaving mirrorsParallel rays converge to the focal point
Convex (bulging)Diverging mirrorCar rear-view mirrors, security mirrors in shopsAlways gives virtual, upright, diminished image; wider field of view
Mirror Formula

1/f = 1/u + 1/v
where f = focal length, u = object distance, v = image distance.
Magnification (m) = v/u = image height / object height

⚠️

Sign convention: Real objects and images are positive. Virtual images are negative. Concave mirrors have positive focal length; convex mirrors have negative focal length.

Overview / Refraction & Lenses

Refraction & Lenses

βœ“ WAECβœ“ JAMB
πŸ”­
Refraction & Snell's Law

Refraction: change in direction of light as it passes from one medium to another due to change in speed.
Light bends towards the normal when going from less dense to more dense medium (e.g. air β†’ glass).
Light bends away from the normal when going from more dense to less dense (e.g. glass β†’ air).

Snell's Law

n₁ sin θ₁ = nβ‚‚ sin ΞΈβ‚‚
Refractive index n = sin i / sin r = speed in vacuum / speed in medium

Total Internal Reflection (TIR): occurs when light travels from a denser to less dense medium and the angle of incidence exceeds the critical angle. Applications: optical fibres, periscopes, diamonds, binoculars.

πŸ‘“
Lenses & Eye Defects
Lens TypeAlso calledUses & Effect
Convex (converging)Positive lensMagnifying glass, camera, projector, eye β€” corrects long-sightedness (hypermetropia)
Concave (diverging)Negative lensCorrects short-sightedness (myopia); peephole lenses
Eye DefectProblemCorrection
Short-sightedness (Myopia)Can see near objects clearly; far objects blurry. Image forms in front of retina.Concave lens
Long-sightedness (Hypermetropia)Can see far objects clearly; near objects blurry. Image forms behind retina.Convex lens
🎯

Dispersion of white light by a prism produces the spectrum: Red, Orange, Yellow, Green, Blue, Indigo, Violet (ROYGBIV). Violet has the highest frequency and is refracted most. Red is refracted least.

Overview / Electrostatics & Circuits

Electrostatics & Circuits

βœ“ WAECβœ“ JAMB
πŸ”‹
Electric Charge & Coulomb's Law

There are two types of charge: positive (+) and negative (βˆ’). Like charges repel; unlike charges attract.
The SI unit of charge is the Coulomb (C).
Coulomb's Law: F = kq₁qβ‚‚/rΒ² β€” force between charges is proportional to the product of charges and inversely proportional to distance squared.

πŸ”Œ
Electric Circuits β€” Series vs Parallel
FeatureSeries CircuitParallel Circuit
CurrentSame throughout: I₁ = Iβ‚‚ = I₃Splits: I_total = I₁ + Iβ‚‚ + I₃
VoltageSplits: V_total = V₁ + Vβ‚‚ + V₃Same across each branch
Total ResistanceR_T = R₁ + Rβ‚‚ + R₃ (adds up)1/R_T = 1/R₁ + 1/Rβ‚‚ + 1/R₃ (decreases)
If one bulb failsAll go outOthers stay on
Series vs Parallel β€” Quick Example

Two 6 Ξ© resistors in series: R_T = 6 + 6 = 12 Ξ©
Two 6 Ξ© resistors in parallel: 1/R_T = 1/6 + 1/6 = 2/6, so R_T = 3 Ξ©

🎯

Household appliances are connected in parallel so each gets full mains voltage and can be switched independently. A fuse is connected in series in the live wire to protect against excess current.

Overview / Ohm's Law & Resistance

Ohm's Law & Electrical Resistance

βœ“ WAECβœ“ JAMB
⚑
Ohm's Law & Key Formulas

Ohm's Law: Voltage is directly proportional to current at constant temperature. V = IR
V = Voltage (Volts, V) Β· I = Current (Amperes, A) Β· R = Resistance (Ohms, Ξ©)

FormulaVariables
V = IROhm's Law β€” voltage, current, resistance
P = IV = IΒ²R = VΒ²/RElectrical power (Watts)
E = Pt = IVtElectrical energy (Joules)
R = ρL/AResistance depends on resistivity (ρ), length (L), cross-sectional area (A)
Power Calculation

A 240 V appliance draws 2 A. Power = V Γ— I = 240 Γ— 2 = 480 W
Energy in 1 hour = P Γ— t = 480 Γ— 3600 = 1,728,000 J = 1.728 kWh

⚠️

Resistance increases with temperature for most conductors (metals). Ohm's Law applies only to ohmic conductors (resistors). Diodes, filament bulbs and thermistors are non-ohmic.

Overview / Magnetism & Electromagnetism

Magnetism & Electromagnetism

βœ“ WAECβœ“ JAMB
🧲
Magnetism β€” Key Facts
  • Like poles repel; unlike poles attract.
  • Magnetic field lines run from North to South outside a magnet.
  • A current-carrying conductor produces a circular magnetic field around it.
  • The right-hand grip rule: grip the wire with thumb pointing in direction of conventional current β†’ fingers curl in direction of field.
⚑
Electromagnetic Induction & Transformers

Faraday's Law: An EMF is induced in a conductor whenever the magnetic flux through it changes.
Lenz's Law: The induced current opposes the change causing it.

Transformer Equations

Vβ‚›/Vβ‚š = Nβ‚›/Nβ‚š (voltage ratio = turns ratio)
For an ideal transformer: Vβ‚š Γ— Iβ‚š = Vβ‚› Γ— Iβ‚› (power in = power out)
Step-up transformer: Nβ‚› > Nβ‚š β†’ voltage increases, current decreases.
Step-down transformer: Nβ‚› < Nβ‚š β†’ voltage decreases, current increases.

🎯

AC generator: converts mechanical energy β†’ electrical energy (uses electromagnetic induction). DC motor: converts electrical energy β†’ mechanical energy. Transformers only work with AC, not DC.

Overview / Heat Transfer & Temperature

Heat Transfer & Temperature

βœ“ WAECβœ“ JAMB
🌑️
Three Methods of Heat Transfer
MethodHow it worksMedium required?Examples
ConductionHeat transferred through a solid by particle vibrations passing energy along. No net movement of particles.Yes (solids best)Metal spoon in hot soup; ironing board; cooking pot
ConvectionHeat transferred by movement of heated fluid (liquid or gas). Hot fluid rises, cool fluid sinks β€” convection currents.Yes (fluids: liquids and gases)Boiling water, sea breezes, room radiators, trade winds
RadiationHeat transferred as electromagnetic waves (infrared). No particles needed.No β€” travels through vacuumSun heating Earth, grill, campfire warmth
🎯

A vacuum flask (Thermos) minimises all three: vacuum between walls (no conduction/convection), silvered walls (reduce radiation). A good absorber of radiation is also a good emitter β€” dull black surfaces. Shiny silver surfaces are poor absorbers and poor emitters.

πŸ”₯
Specific Heat Capacity & Latent Heat

Specific Heat Capacity (c): Heat needed to raise 1 kg of a substance by 1Β°C (or 1 K).
Q = mcΞ”T where m = mass, c = specific heat capacity, Ξ”T = temperature change.
Specific heat capacity of water = 4,200 J/kg/K (highest common value β€” explains why water is a good coolant).

Latent Heat (L): Heat needed to change the state of a substance at constant temperature.
Q = mL. Latent heat of fusion: solid β†’ liquid. Latent heat of vaporisation: liquid β†’ gas.

Temperature Scales

Celsius to Kelvin: K = Β°C + 273
Absolute zero = βˆ’273Β°C = 0 K (no thermal energy β€” molecules at rest)

Overview / Gas Laws & Thermodynamics

Gas Laws & Thermodynamics

βœ“ WAECβœ“ JAMB
πŸ”₯
The Three Gas Laws
LawConstantRelationshipFormula
Boyle's LawTemperature (T)Pressure inversely proportional to VolumePV = constant β†’ P₁V₁ = Pβ‚‚Vβ‚‚
Charles' LawPressure (P)Volume directly proportional to TemperatureV/T = constant β†’ V₁/T₁ = Vβ‚‚/Tβ‚‚
Pressure Law (Gay-Lussac)Volume (V)Pressure directly proportional to TemperatureP/T = constant β†’ P₁/T₁ = Pβ‚‚/Tβ‚‚
General Gas Law (Combining all three)

P₁V₁/T₁ = Pβ‚‚Vβ‚‚/Tβ‚‚
Always use Kelvin (K) for temperature in gas law calculations!
T(K) = T(Β°C) + 273

⚠️

Common mistake: Using Celsius instead of Kelvin in gas law calculations. Always convert Β°C to K first by adding 273. If you use Celsius, your answer will be wrong.

Overview / Radioactivity & Nuclear Physics

Radioactivity & Nuclear Physics

βœ“ WAECβœ“ JAMB
☒️
The Three Types of Radiation
RadiationNatureChargePenetrating PowerStopped by
Alpha (Ξ±)2 protons + 2 neutrons (helium nucleus)+2Least β€” travels ~4 cm in airPaper or skin
Beta (Ξ²)High-speed electronβˆ’1Medium β€” travels ~1 m in airThin aluminium (few mm)
Gamma (Ξ³)Electromagnetic wave (high-energy photon)0 (no charge)Most β€” travels many metresThick lead or concrete
🎯

Remember penetrating power order: Ξ± < Ξ² < Ξ³. Alpha is the most ionising; gamma is the least ionising but most penetrating. All three are deflected by electric fields except gamma (no charge).

⏳
Half-Life & Nuclear Equations

Half-life: Time taken for half the radioactive atoms in a sample to decay. After n half-lives, the amount remaining = Nβ‚€ Γ— (Β½)ⁿ.

Half-Life Example

Initial mass = 80 g. Half-life = 2 hours. After 6 hours = 3 half-lives.
Remaining = 80 Γ— (Β½)Β³ = 80 Γ— 1/8 = 10 g

Nuclear fission: Heavy nucleus splits into smaller fragments + energy (e.g. uranium-235). Used in nuclear reactors and atomic bombs.
Nuclear fusion: Two light nuclei combine to form a heavier nucleus + energy (e.g. hydrogen β†’ helium). Occurs in stars/sun. Fusion releases more energy per unit mass than fission.

Overview / Electronics & Photoelectric Effect

Electronics & Photoelectric Effect

βœ“ WAECβœ“ JAMB
πŸ’‘
Semiconductors & Diodes

Conductors: Allow free flow of electrons (copper, aluminium).
Insulators: Do not allow electron flow (rubber, wood, plastic).
Semiconductors: Conductivity between conductors and insulators β€” conductivity increases with temperature. Examples: Silicon, Germanium.

Diode (p-n junction): Allows current to flow in one direction only. Used in rectification (converting AC to DC).
Half-wave rectification: one diode β€” only one half-cycle passes.
Full-wave rectification: four diodes (bridge rectifier) β€” both half-cycles used.

🌟
Photoelectric Effect

The photoelectric effect: When light of sufficiently high frequency shines on a metal surface, electrons are emitted. Explained by Einstein using the particle (photon) model of light.

  • Threshold frequency: minimum frequency of light needed to emit electrons.
  • Increasing intensity increases the number of electrons but NOT their energy.
  • Increasing frequency increases the kinetic energy of emitted electrons.
  • Photon energy: E = hf (h = Planck's constant = 6.63 Γ— 10⁻³⁴ JΒ·s)
🎯

Logic gates (WAEC): AND, OR, NOT, NAND, NOR are the key gates. Know their truth tables and circuit symbols. A NOT gate (inverter) simply flips 0 to 1 and 1 to 0. NAND = NOT + AND; NOR = NOT + OR.

⚑
Ready to Test Yourself?

You've now covered all major WAEC and JAMB Physics topics. Take the 100-question timed CBT practice to see your score and get a personalised breakdown by section.

Ask us anything