IGCSE Physics Definitions Sheet – Key Terms by Topic (2025)
IGCSE

IGCSE Physics Definitions Sheet – Key Terms by Topic (2025)

Tutopiya Team Educational Expert
• 12 min read

IGCSE Physics Definitions Sheet: All the Key Terms You Need

Physics at IGCSE requires you to define terms with scientific precision. Many exam questions begin with “Define…” or “State what is meant by…” — and full marks depend on using the exact phrasing examiners expect.

This IGCSE Physics definitions sheet covers every essential term from the Cambridge IGCSE Physics (0625/0972) syllabus, organised by topic for quick reference and revision.


1. Measurement and Units

TermDefinition
Scalar quantityA quantity that has magnitude (size) only (e.g. speed, mass, energy).
Vector quantityA quantity that has both magnitude and direction (e.g. velocity, force, acceleration).
SI unitsThe international system of units used in science (e.g. metre, kilogram, second, ampere, kelvin).
AccuracyHow close a measured value is to the true value.
PrecisionHow close repeated measurements are to each other.
Parallax errorAn error in reading a scale caused by viewing it from an angle rather than straight on.

2. Motion

TermDefinition
SpeedThe distance travelled per unit time.
VelocityThe speed of an object in a given direction; the rate of change of displacement.
AccelerationThe rate of change of velocity, measured in m/s².
DecelerationA negative acceleration — a decrease in velocity over time.
DistanceThe total length of the path travelled by an object (scalar).
DisplacementThe straight-line distance from the starting point to the finishing point in a specified direction (vector).
Terminal velocityThe constant maximum velocity reached when the driving force equals the resistive force (e.g. air resistance equals weight).
Free fallMotion under the influence of gravity only, with no air resistance.
Acceleration due to gravity (g)The acceleration of an object falling freely near the Earth’s surface, approximately 9.8 m/s² (often taken as 10 m/s²).

3. Forces

TermDefinition
ForceA push or pull that can change the shape, speed or direction of motion of an object, measured in newtons (N).
MassThe amount of matter in an object, measured in kilograms (kg); a scalar quantity.
WeightThe gravitational force acting on an object; W = mg, measured in newtons (N).
Gravitational field strength (g)The force per unit mass acting on an object in a gravitational field, measured in N/kg.
FrictionA force that opposes the motion of one surface over another.
Air resistance (drag)A frictional force that opposes the motion of an object through air.
Resultant forceThe single force that has the same effect as all the forces acting on an object combined.
Newton’s first lawAn object remains at rest or continues to move at constant velocity unless acted on by a resultant force.
Newton’s second lawThe resultant force on an object is equal to its mass multiplied by its acceleration: F = ma.
Newton’s third lawFor every action there is an equal and opposite reaction — forces always occur in pairs on different objects.
MomentThe turning effect of a force about a pivot: moment = force × perpendicular distance from the pivot.
Centre of gravityThe point at which the entire weight of an object appears to act.
EquilibriumA state where the resultant force and the resultant moment on an object are both zero.
Hooke’s lawThe extension of a spring is directly proportional to the applied force, up to the limit of proportionality.
Limit of proportionalityThe point beyond which the extension of a spring is no longer proportional to the force applied.

4. Momentum

TermDefinition
MomentumThe product of an object’s mass and velocity: p = mv, measured in kg m/s.
ImpulseThe change in momentum of an object, equal to the force multiplied by the time for which it acts: impulse = FΔt.
Conservation of momentumIn a closed system, the total momentum before an event equals the total momentum after the event.

5. Energy, Work and Power

TermDefinition
EnergyThe capacity to do work, measured in joules (J).
Kinetic energyThe energy an object has due to its motion: KE = ½mv².
Gravitational potential energyThe energy an object has due to its position in a gravitational field: GPE = mgh.
Work doneThe energy transferred when a force moves an object through a distance in the direction of the force: W = Fd.
PowerThe rate at which energy is transferred or work is done: P = W/t, measured in watts (W).
EfficiencyThe ratio of useful energy output to total energy input, often expressed as a percentage.
Conservation of energyEnergy cannot be created or destroyed — it can only be transferred from one form to another.
Renewable energyEnergy from sources that are naturally replenished and will not run out (e.g. solar, wind, hydroelectric).
Non-renewable energyEnergy from sources that will eventually run out because they are consumed faster than they are formed (e.g. fossil fuels, nuclear fuel).

6. Thermal Physics

TermDefinition
TemperatureA measure of the average kinetic energy of the particles in a substance.
Internal energyThe total kinetic and potential energy of all the particles in a substance.
Specific heat capacityThe amount of energy required to raise the temperature of 1 kg of a substance by 1 °C, measured in J/(kg °C).
Specific latent heatThe energy required to change the state of 1 kg of a substance without changing its temperature.
Latent heat of fusionThe energy required to change 1 kg of a solid to a liquid at its melting point.
Latent heat of vaporisationThe energy required to change 1 kg of a liquid to a gas at its boiling point.
ConductionThe transfer of thermal energy through a material by the vibration and collision of particles, without the particles themselves moving from place to place.
ConvectionThe transfer of thermal energy through a fluid by the circulation of currents caused by differences in density.
RadiationThe transfer of thermal energy by electromagnetic waves (infrared), requiring no medium.
Thermal expansionThe increase in size of a substance when its temperature increases, due to increased particle vibration.

7. Waves

TermDefinition
WaveA disturbance that transfers energy from one place to another without transferring matter.
Transverse waveA wave in which the vibrations are perpendicular to the direction of energy transfer (e.g. light, water waves).
Longitudinal waveA wave in which the vibrations are parallel to the direction of energy transfer (e.g. sound).
AmplitudeThe maximum displacement of a point on a wave from its rest (equilibrium) position.
Wavelength (λ)The distance between two consecutive points in phase on a wave (e.g. crest to crest).
Frequency (f)The number of complete waves passing a point per second, measured in hertz (Hz).
Period (T)The time taken for one complete wave to pass a point: T = 1/f.
Wave speedThe speed at which a wave travels: v = fλ.
ReflectionThe bouncing back of a wave when it hits a boundary between two media.
RefractionThe change in direction of a wave as it passes from one medium to another due to a change in speed.
DiffractionThe spreading of a wave as it passes through a gap or around an obstacle.
Total internal reflectionThe complete reflection of a wave inside a denser medium when the angle of incidence exceeds the critical angle.
Critical angleThe angle of incidence above which total internal reflection occurs.

8. Sound

TermDefinition
SoundA longitudinal wave caused by vibrations, requiring a medium to travel through.
PitchThe perceived highness or lowness of a sound, determined by its frequency.
LoudnessThe perceived volume of a sound, determined by its amplitude.
EchoA reflected sound wave heard after a delay.
UltrasoundSound with a frequency above 20 000 Hz — above the range of human hearing.

9. Light and the Electromagnetic Spectrum

TermDefinition
Electromagnetic spectrumThe continuous range of electromagnetic waves ordered by frequency or wavelength, from radio waves to gamma rays.
Electromagnetic waveA transverse wave that can travel through a vacuum at 3 × 10⁸ m/s, consisting of oscillating electric and magnetic fields.
NormalAn imaginary line perpendicular to a surface at the point where a ray meets the surface.
Angle of incidenceThe angle between the incoming ray and the normal.
Angle of reflectionThe angle between the reflected ray and the normal.
Law of reflectionThe angle of incidence equals the angle of reflection.
Refractive indexThe ratio of the speed of light in a vacuum to the speed of light in a medium: n = c/v.
Converging lensA lens that brings parallel rays of light to a focus (convex lens).
Diverging lensA lens that spreads parallel rays of light apart (concave lens).
Focal lengthThe distance from the centre of a lens to its principal focus.
Real imageAn image formed where rays of light actually converge; can be projected onto a screen.
Virtual imageAn image formed where rays of light appear to come from; cannot be projected onto a screen.

10. Electricity

TermDefinition
Electric current (I)The rate of flow of electric charge: I = Q/t, measured in amperes (A).
Charge (Q)A property of matter that causes it to experience a force in an electric field, measured in coulombs (C).
Potential difference (V)The energy transferred per unit charge passing between two points: V = W/Q, measured in volts (V).
Resistance (R)The opposition to the flow of current: R = V/I, measured in ohms (Ω).
Ohm’s lawThe current through a conductor is directly proportional to the potential difference across it, provided the temperature remains constant.
Electromotive force (e.m.f.)The energy transferred per unit charge by a source of electrical energy (e.g. battery), measured in volts.
Series circuitA circuit in which components are connected end-to-end so there is only one path for current.
Parallel circuitA circuit in which components are connected across each other so there are multiple paths for current.
Electrical powerThe rate of energy transfer by an electrical device: P = IV, measured in watts (W).
Kilowatt-hour (kWh)A unit of energy equal to the energy used by a 1 kW device in 1 hour.

11. Magnetism and Electromagnetism

TermDefinition
Magnetic fieldThe region around a magnet or current-carrying conductor where a magnetic force is experienced.
Magnetic field linesLines that show the direction and strength of a magnetic field; they go from north to south outside the magnet.
ElectromagnetA magnet made by passing an electric current through a coil of wire, often with an iron core.
Motor effectThe force experienced by a current-carrying conductor placed in a magnetic field.
Fleming’s left-hand ruleA rule used to predict the direction of the force on a current-carrying conductor in a magnetic field (thumb = force, first finger = field, second finger = current).
Electromagnetic inductionThe generation of an electromotive force (e.m.f.) in a conductor when it moves through a magnetic field or when a magnetic field changes around it.
TransformerA device that changes the voltage of an alternating current using electromagnetic induction between two coils wound on an iron core.
Direct current (d.c.)Current that flows in one direction only.
Alternating current (a.c.)Current that repeatedly reverses direction.

12. Nuclear Physics

TermDefinition
NucleusThe dense, positively charged centre of an atom containing protons and neutrons.
RadioactivityThe spontaneous and random emission of radiation from an unstable nucleus.
Alpha particle (α)A particle consisting of 2 protons and 2 neutrons (a helium nucleus), emitted during radioactive decay; strongly ionising, weakly penetrating.
Beta particle (β)A high-speed electron emitted from the nucleus when a neutron converts to a proton; moderately ionising and penetrating.
Gamma ray (γ)A high-frequency electromagnetic wave emitted from the nucleus; weakly ionising, highly penetrating.
Half-lifeThe time taken for half the radioactive nuclei in a sample to decay, or for the activity of a source to halve.
Background radiationLow-level radiation that is always present in the environment from natural and artificial sources.
Nuclear fissionThe splitting of a large, unstable nucleus into two smaller nuclei, releasing energy and neutrons.
Nuclear fusionThe joining of two small nuclei to form a larger nucleus, releasing a large amount of energy.
Chain reactionA self-sustaining series of fission reactions where neutrons released from one fission event trigger further fission events.

13. Space Physics

TermDefinition
GalaxyA large collection of billions of stars held together by gravity.
Solar systemThe Sun and all the objects that orbit it, including planets, moons, asteroids and comets.
OrbitThe curved path of an object around a larger object due to gravity.
Gravitational forceThe attractive force between any two objects with mass.
Red-shiftThe increase in wavelength (shift towards the red end of the spectrum) of light from galaxies moving away from us — evidence that the universe is expanding.

Exam Tips for IGCSE Physics Definitions

  1. Learn definitions word-for-word — “rate of change of velocity” is accepted for acceleration; “how fast something speeds up” is not.
  2. Include units — when defining a quantity, always state the SI unit (e.g. “measured in newtons”).
  3. Know the difference between mass and weight — mass is measured in kg and does not change; weight is measured in N and depends on gravitational field strength.
  4. Scalar vs vector — examiners love asking you to classify quantities. Speed is scalar; velocity is vector.
  5. Use equations as definitions — stating W = Fd along with “energy transferred when a force moves through a distance” strengthens your answer.

Supercharge Your IGCSE Physics Revision

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👉 Book a free trial lesson with an IGCSE Physics tutor — get 1-on-1 guidance on definitions, problem-solving and exam technique.

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Last updated: March 2026. Based on the Cambridge IGCSE Physics (0625/0972) syllabus.

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