Cambridge IGCSE · Physics 0625 · 2026–2028

Complete Physics
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Comprehensive notes, diagrams, formulas, and exam practice for all 6 topics — Core & Extended.

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6
Major Topics
40+
Formulas
30+
SVG Diagrams
60
Exam Questions
A*
Target Grade
01
Motion, Forces & Energy
Mechanics · Kinematics · Momentum · Work · Power · Pressure

1.1 Physical Quantities & Measurement

Length is measured with a ruler (mm precision). Volume of irregular solids is found by displacement in a measuring cylinder.

Time is measured with clocks or digital timers. For short intervals, measure multiple periods then divide.

To find the period of a pendulum accurately: time 20 complete oscillations and divide by 20. This reduces the effect of reaction-time error.
Period T = total time / number of oscillations
Average period calculation

EXTENDED Scalar quantities have magnitude only. Vector quantities have both magnitude and direction.

Scalars

Distance · Speed · Time · Mass · Energy · Temperature

Vectors

Force · Weight · Velocity · Acceleration · Momentum · Electric & Gravitational field strength

Resultant = √(A² + B²)   θ = tan⁻¹(B/A)
Two vectors at right angles (Pythagoras)
A = 130 B = 90 R = √(A²+B²)
Adding two vectors at right angles using Pythagoras' theorem

1.2 Motion

Speed = distance / time. Velocity = speed in a given direction (vector).
v = s / t     average speed = total distance / total time
Speed equations
EXT a = Δv / Δt
Acceleration (Extended)
Free-fall acceleration near Earth's surface: g ≈ 9.8 m/s² (constant, approximately)
Time (s) Distance (m) At rest Constant speed Accelerating Decelerating Distance–Time Graph
Distance–time graph showing different types of motion
Time (s) Speed (m/s) Const. speed Acceleration Deceleration Area = distance Speed–Time Graph
Speed–time graph: gradient = acceleration; area under graph = distance

EXT Terminal velocity: When an object falls, air resistance increases until it equals gravity. Net force = 0 → constant velocity.

Falling Object — Forces object W (weight) F_drag (air resistance) Initially: W > Drag → accelerates Terminal: W = Drag → constant velocity
Forces on a falling object

1.3 Mass & Weight

g = W / m     W = mg
Gravitational field strength (g = 9.8 N/kg on Earth)
Mass is constant everywhere. Weight changes with gravitational field strength.
Locationg (N/kg)Weight of 70 kg person
Earth (surface)9.8686 N
Moon1.6112 N
Jupiter24.81736 N
Deep space≈ 0≈ 0 N

1.4 Density

ρ = m / V
Density (kg/m³ or g/cm³)

Measuring regular solid

Measure dimensions with a ruler → calculate volume geometrically → use ρ = m/V.

Measuring irregular solid

Submerge in water in measuring cylinder. Volume = change in water level reading (displacement method).

Object floats if its density is less than the liquid it's placed in.
V₁ = 50 cm³ V₂ = 70 cm³ ΔV = 20 cm³ Displacement Method
Measuring volume by water displacement

1.5 Forces

Hooke's Law: Extension is proportional to force, up to the limit of proportionality.

EXT k = F / x
Spring constant k (N/m or N/cm). F = kx
Extension (x) Force (F) Proportional region F = kx Limit of proportionality Non-linear Load–Extension Graph (Hooke's Law)
Load–extension graph showing Hooke's Law and limit of proportionality

1.5.2 Turning Effect of Forces (Moments)

Moment = F × perpendicular distance from pivot
Unit: N m
Principle of Moments: For equilibrium, sum of clockwise moments = sum of anticlockwise moments.
Pivot F₁ d₁ F₂ d₂ F₁ × d₁ = F₂ × d₂ (equilibrium)
Principle of moments: balanced beam

1.5.3 Centre of Gravity

The centre of gravity is the point through which the entire weight of an object appears to act.

Low centre of gravity → more stable. High centre of gravity → less stable (easier to topple).

1.6 Momentum Extended

p = mv     impulse = FΔt = Δ(mv)
Momentum p (kg m/s), Impulse (N s)
F = Δp / Δt
Resultant force as rate of change of momentum
Law of Conservation of Momentum: In a closed system, total momentum before = total momentum after collision.
WORKED EXAMPLE

Cart A (mass 2 kg, velocity 3 m/s) collides with stationary Cart B (mass 3 kg). They stick together. Find final velocity.

Before: p = 2×3 + 3×0 = 6 kg m/s

After: p = (2+3) × v → v = 6/5 = 1.2 m/s

1.7 Energy, Work & Power

Energy stores: kinetic, gravitational potential, chemical, elastic, nuclear, electrostatic, internal (thermal).

W = Fd = ΔE     P = W/t = ΔE/t
Work done (J), Power (W)
EXT Eₖ = ½mv²     ΔEₚ = mgΔh
Kinetic energy & Change in gravitational PE
EXT efficiency = useful output / total input (× 100%)
Also: efficiency = useful power out / total power in
Sankey Diagram — Electric Motor (40% efficient) Input 100 J Useful: 40 J Wasted heat: 60 J Motor
Sankey diagram: energy input, useful output, and wasted energy

1.7.3 Energy Resources

SourceRenewable?Reliable?Environmental Impact
Fossil fuelsNoYesCO₂ emissions, air pollution
NuclearNoYesRadioactive waste
HydroelectricYesYes (if rain)Habitat flooding
Solar (PV)YesNo (needs sun)Low — land use
WindYesNo (needs wind)Low — noise, visual
GeothermalYesYesVery low
TidalYesYesCoastal habitat impact

1.8 Pressure

p = F / A
Pressure (Pa or N/m²)
EXT Δp = ρgΔh
Pressure at depth in a liquid
Pressure in a liquid increases with depth and with liquid density. It acts in all directions.
02
Thermal Physics
Kinetic Model · States of Matter · Heat Transfer · Thermometry

2.1 Kinetic Particle Model of Matter

SOLID Regular, close, vibrating LIQUID Close, random, flow freely GAS Far apart, fast, random
Particle arrangements in solids, liquids and gases
T (in K) = θ (in °C) + 273
Converting Celsius to Kelvin
Absolute zero = −273°C = 0 K. At absolute zero, particles have minimum kinetic energy.
EXT pV = constant (at constant temperature)
Boyle's Law — fixed mass of gas

2.1.3 Pressure of a Gas

Increasing temperature → particles move faster → more frequent, harder collisions → higher pressure (constant volume).

Decreasing volume → particles collide more often with walls → higher pressure (constant temperature).

Brownian motion (random zigzag of microscopic particles) is evidence for the kinetic particle model.

2.2 Thermal Properties & Temperature

Solids, liquids, and gases all expand when heated. Gases expand most, solids least.

EXT c = ΔE / (mΔθ)
Specific heat capacity c [J/(kg°C)] — energy to raise 1 kg by 1°C
WORKED EXAMPLE

How much energy to heat 2 kg of water (c = 4200 J/kg°C) from 20°C to 100°C?

ΔE = mcΔθ = 2 × 4200 × (100−20) = 2 × 4200 × 80 = 672 000 J = 672 kJ

2.2.3 Changes of State

SOLID LIQUID GAS Melting Solidifying Boiling/Evaporation Condensation ← Energy Input (heating) → ← Energy Output (cooling) →
Changes of state and energy transfers
During melting and boiling, temperature stays constant even though energy is being supplied (latent heat — breaking bonds).
Evaporation causes cooling: the most energetic molecules escape, leaving the liquid cooler.

2.3 Transfer of Thermal Energy

Conduction

Transfer through solids (and poor liquids/gases) via vibrating particles & free electrons in metals.

Best conductors: metals. Best insulators: wood, rubber, air.

Convection

Transfer in fluids (liquids & gases) via density differences creating convection currents.

Hot fluid rises (less dense); cool fluid sinks (more dense).

Radiation

Infrared radiation — does NOT need a medium. Can travel through vacuum.

Dull black surfaces: best emitters & absorbers. Shiny white: best reflectors.

Convection Current in Water Heat source Hot rises Cool sinks
Convection current created by a heat source

EXT Earth's temperature is maintained by a balance between incoming solar radiation and outgoing radiation. Greenhouse gases affect this balance.

03
Waves
Wave Properties · Light · EM Spectrum · Sound

3.1 General Properties of Waves

v = fλ
Wave speed (m/s) = frequency (Hz) × wavelength (m)

Transverse Waves

Vibration perpendicular to direction of travel. Examples: EM waves, water waves, seismic S-waves.

Longitudinal Waves

Vibration parallel to direction of travel. Examples: sound waves, seismic P-waves.

Wave Anatomy crest trough A λ (wavelength)
Anatomy of a transverse wave

Waves can undergo reflection (bounce off surface), refraction (change speed → change direction), and diffraction (spread through gaps/edges).

EXT Diffraction is greatest when wavelength ≈ gap size.

3.2 Light

Reflection

angle of incidence (i) = angle of reflection (r)
Law of Reflection

Refraction & Snell's Law

EXT n = sin i / sin r     n = 1 / sin c
Refractive index n; c = critical angle
Refraction of Light Air (n=1) Glass (n=1.5) Normal Incident i Refracted r Going into denser medium: bends towards normal (r < i)
Refraction of light at an air–glass boundary

Total Internal Reflection

When light travels from a denser medium and the angle of incidence exceeds the critical angle, all light is reflected back — no refraction.

Optical fibres use total internal reflection to transmit light signals over long distances in telecommunications.

3.2.3 Thin Lenses

Converging Lens — Real Image Converging Lens F F Object Real Image
Ray diagram: real image formed by a converging lens (object beyond 2F)

3.3 Electromagnetic Spectrum

All EM waves travel at c = 3.0 × 10⁸ m/s in a vacuum. They are transverse waves requiring no medium.
Electromagnetic Spectrum (increasing frequency →) Radio Micro IR Visible UV X-rays Gamma rays increasing frequency / decreasing wavelength Long λ / Low f Short λ / High f
The electromagnetic spectrum ordered by increasing frequency
RegionUsesHarmful Effects
Radio wavesTV/radio, astronomy, RFIDMinimal
MicrowavesSatellite TV, mobile phones, ovensInternal heating of cells
InfraredGrills, remote controls, thermal imagingSkin burns
Visible lightVision, photographyNone (normal exposure)
UltravioletSecurity marking, sterilising waterSkin cancer, eye damage
X-raysMedical scanning, securityCell mutation/damage
Gamma raysSterilisation, cancer treatmentCell mutation, cancer

3.4 Sound

Sound is a longitudinal wave requiring a medium. It cannot travel through a vacuum.
Speed of sound in air ≈ 330–350 m/s
Compare: light ≈ 3 × 10⁸ m/s

Human hearing range: 20 Hz to 20 000 Hz. Ultrasound: f > 20 kHz.

Loudness & Pitch

Amplitude ↑ → louder sound.
Frequency ↑ → higher pitch.

Ultrasound Uses

Medical imaging (soft tissue), non-destructive testing of materials, sonar (depth finding).

04
Electricity & Magnetism
Electric Circuits · Electromagnetic Effects · Magnetism

4.1 Magnetism

Like poles repel; unlike poles attract. Magnetic materials: iron, steel, nickel, cobalt.

Temporary magnets (soft iron): easily magnetised/demagnetised — used in electromagnets.

Permanent magnets (steel): hard to demagnetise — used in compasses.

Magnetic field lines run from N to S outside the magnet, and from S to N inside.
N S Field lines N→S (outside)

4.2 Electrical Quantities

R = V/I     P = IV     E = IVt
Resistance (Ω), Power (W), Energy (J)
EXT I = Q/t     V = W/Q     E_emf = W/Q
Current, Potential Difference, EMF
For a metallic conductor: Resistance ∝ length; Resistance ∝ 1/cross-sectional area.
Current–Voltage Characteristics V I Resistor Filament Diode
I–V characteristics: ohmic resistor (linear), filament lamp (non-linear), diode (one-way)

4.3 Electric Circuits

Series Circuit

I_total = I₁ = I₂
V_total = V₁ + V₂
R_total = R₁ + R₂
Series rules

Parallel Circuit

V same across all branches
I_total = I₁ + I₂
EXT 1/R = 1/R₁ + 1/R₂
Parallel rules
The switch must always be in the LIVE wire so that when switched off, the appliance is fully de-energised and safe to touch.

4.5 Electromagnetic Effects

A conductor moving through a magnetic field, or a changing magnetic field linking a conductor, induces an EMF.

Induced EMF increases with: faster movement, stronger magnet, more turns of wire.
V_p / V_s = N_p / N_s     EXT I_p V_p = I_s V_s
Transformer equations
EXT P = I²R
Power loss in cables — minimised by using high voltage
Step-Up Transformer V_p (low) N_p (few) V_s (high) N_s (many) Alternating current in primary → changing B field → EMF induced in secondary
Step-up transformer: more secondary turns → higher voltage
05
Nuclear Physics
Atomic Model · Radioactivity · Half-life · Safety

5.1 Nuclear Model of the Atom

ᴬ_Z X  : A = mass number, Z = proton number
Neutrons = A − Z
Nuclide notation
ParticleChargeMass
Proton+11
Neutron01
Electron−1≈0
Isotopes: same proton number Z, different neutron number (different A).
Atomic Structure p p n Electrons orbit nucleus

EXT Rutherford α-scattering: most α-particles pass through (mostly empty space); very few bounce back → small, dense, positive nucleus.

EXT Fission: heavy nucleus splits → energy. Fusion: light nuclei join → heavier nucleus + energy (powers the Sun).

5.2 Radioactivity

TypeNatureChargeRange in airBlocked byIonising
Alpha (α)2p + 2n (He nucleus)+2A few cmPaper/skinHighest
Beta (β⁻)Fast electron−1~1 mFew mm AlMedium
Gamma (γ)EM wave (photon)0UnlimitedSeveral cm PbLowest
Half-life: time for activity (or number of nuclei) to halve
After n half-lives: N = N₀ × (½)ⁿ
Radioactive decay
Radioactive Decay Curve Time (half-lives) Count rate N₀ N₀/2 N₀/4 2t½ 3t½
Decay curve — each half-life halves the remaining activity

Safety

• Use tongs — never handle with bare hands.  • Minimise exposure time.  • Keep distance from source.  • Use lead or concrete shielding.  • Store in lead-lined containers.

Effects on living tissue: cell death, gene mutation, cancer.
06
Space Physics
Solar System · Stars · Universe · Big Bang

6.1 The Earth & Solar System

EXT v = 2πr / T
Average orbital speed (r = radius, T = orbital period)
Inner 4 planets: rocky & small. Outer 4 planets: gaseous & large. The Sun holds 99.8% of the Solar System's mass.
Sun Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune
The eight planets in order from the Sun (not to scale)

6.2 Stars & The Universe

1 light-year = 9.5 × 10¹⁵ m. The Milky Way is ~100 000 light-years across.
Life Cycle of a Star (Extended) Nebula / Protostar Main Sequence Star Red Giant White Dwarf Red Supergiant Supernova Neutron Star / Black Hole
Star life cycle — path depends on initial mass (Extended)

The Universe & Big Bang

Redshift: Light from distant galaxies is shifted to longer wavelengths, showing galaxies are moving away. The further the galaxy, the greater the redshift → Universe is expanding → evidence for the Big Bang.
EXT H₀ = v/d     Age ≈ 1/H₀ ≈ 14 billion years
Hubble constant H₀ = 2.2 × 10⁻¹⁸ s⁻¹
EXT CMBR (Cosmic Microwave Background Radiation): microwave radiation present in all directions of space — produced shortly after the Big Bang and stretched as the Universe expanded.
EXAMINATION CENTRE

Practice Exam

MCQ · True/False · Calculations · Short Answer across all 6 topics

Section A — Multiple Choice

MCQ[1 mark] Topic 1 — Motion
A car travels 120 m in 8 s. What is its average speed?
  • A10 m/s
  • B12 m/s
  • C15 m/s
  • D960 m/s
MCQ[1 mark] Topic 1 — Vectors
Which of the following is a vector quantity?
  • ATemperature
  • BVelocity
  • CMass
  • DSpeed
MCQ[1 mark] Topic 1 — Hooke's Law
A spring has constant k = 50 N/m. What force produces an extension of 4 cm?
  • A2 N
  • B12.5 N
  • C200 N
  • D0.08 N
MCQ[1 mark] Topic 2 — States
Which process occurs at constant temperature?
  • AHeating water from 20°C to 80°C
  • BCooling a gas at constant volume
  • CMelting of ice at 0°C
  • DHeating a solid above its melting point
MCQ[1 mark] Topic 2 — Temperature
What is −40°C in Kelvin?
  • A313 K
  • B233 K
  • C40 K
  • D−233 K
MCQ[1 mark] Topic 3 — Waves
A wave has frequency 500 Hz and wavelength 0.68 m. What is its speed?
  • A735 m/s
  • B0.00136 m/s
  • C340 m/s
  • D1.36 m/s
MCQ[1 mark] Topic 3 — EM Spectrum
Which EM wave has the longest wavelength?
  • AGamma rays
  • BX-rays
  • CUltraviolet
  • DRadio waves
MCQ[1 mark] Topic 4 — Circuits
A resistor has 12 V across it and 3 A through it. What is its resistance?
  • A36 Ω
  • B4 Ω
  • C0.25 Ω
  • D9 Ω
MCQ[1 mark] Topic 5 — Nuclear
An alpha particle consists of:
  • A2 protons and 2 electrons
  • B1 proton and 1 neutron
  • C2 protons and 2 neutrons
  • D4 protons only
MCQ[1 mark] Topic 6 — Universe
What evidence shows the Universe is expanding?
  • ABlueshift of distant galaxies
  • BRedshift of distant galaxies
  • CThe Sun producing nuclear fusion
  • DThe Moon orbiting Earth

Section B — True / False

T/F[1 mark]
Weight is a scalar quantity.
T/F[1 mark]
Convection can occur in a vacuum.
T/F[1 mark]
Sound waves are transverse waves.
T/F[1 mark]
In a parallel circuit, the current through each branch is the same.
T/F[1 mark]
Gamma radiation has the highest penetrating power of all three types of nuclear emission.

Section C — Calculation Problems

CALC[3 marks] Topic 1 — Energy
A ball (mass 0.5 kg) is thrown upward at 10 m/s. Calculate: (a) its kinetic energy at release, (b) its maximum height. (g = 9.8 m/s², ignore air resistance.)
CALC[2 marks] Topic 1 — Moments
A 4 N force produces a moment of 0.8 N m about a pivot. Find the perpendicular distance from the force to the pivot.
CALC[3 marks] Topic 2 — SHC
How much energy is needed to heat 3 kg of aluminium (c = 900 J/kg°C) from 20°C to 120°C?
CALC[3 marks] Topic 4 — Transformer
A transformer: N_p = 200, N_s = 1000, V_p = 230 V, I_p = 5 A (100% efficient). Find V_s and I_s.
CALC[3 marks] Topic 5 — Half-life
A sample has an initial count rate of 640 counts/min. Half-life = 4 hours. Find count rate after 16 hours.
CALC[2 marks] Topic 4 — Parallel R
Find the combined resistance of 6 Ω and 12 Ω in parallel.

Section D — Short Answer

SHORT[3 marks] Topic 2
Explain why dark, dull clothing makes you warmer in the sun, but light, shiny clothing keeps you cooler.
SHORT[4 marks] Topic 3
Describe how the frequency and amplitude of a sound wave affect what is heard.
SHORT[3 marks] Topic 5
State three safety precautions when handling radioactive sources in a laboratory.
SHORT[4 marks] Topic 1
Describe the motion of an object dropped from rest until it reaches terminal velocity. Refer to the forces at each stage.
SHORT[3 marks] Topic 6
Explain what redshift is and why it supports the Big Bang Theory.
Auto-graded score (MCQ + T/F, out of 15)
Section C & D are self-assessed using the model answers shown above.