BGCSE Physics (0571) study materials
BGCSE Physics (0571) study resources

BGCSE Physics (0571) cheat sheet

BGCSE Physics (0571) · Keep the key ideas within reach.

Quick reference

Measurement, Units and Scientific Method

  • SI base units: metre (m), kilogram (kg), second (s), ampere (A), kelvin (K), mole (mol), candela (cd).

  • Prefixes: nano 10^-9, micro 10^-6, milli 10^-3, centi 10^-2, kilo 10^3, mega 10^6, giga 10^9.

  • Derived-unit checks: force = kg·m·s^-2 (N); energy = kg·m^2·s^-2 (J); power = kg·m^2·s^-3 (W); pressure = kg·m^-1·s^-2 (Pa).

  • Precision is set by the smallest scale division; a ruler with 1 mm divisions is read to ±0.5 mm.

  • Percentage error = (measured value − accepted value) ÷ accepted value × 100%; report sign and magnitude.

  • Density ρ = m/V; a body floats in a fluid when its density is less than the fluid's density.

  • Variables: independent variable is deliberately changed; dependent variable is measured; all others are controlled.

  • A hypothesis is a testable prediction; a theory is a well-tested explanation supported by repeated evidence.

Quick reference

Mechanics: Forces, Motion and Energy

  • Newton's second law: resultant force F = ma; weight W = mg with g ≈ 9.8 N/kg near Earth's surface.

  • Uniform acceleration: v = u + at; s = ut + ½at²; v² = u² + 2as.

  • Average speed = total distance ÷ total time; velocity is speed in a stated direction.

  • Momentum p = mv; in a closed system total momentum before a collision equals total momentum after.

  • Work done W = Fs (force along displacement); power P = W/t = Fv for constant speed.

  • Kinetic energy KE = ½mv²; gravitational potential energy ΔGPE = mgΔh.

  • Principle of moments: for equilibrium about a pivot, sum of clockwise moments = sum of anticlockwise moments.

  • Pressure P = F/A; in a liquid P = ρgh, so pressure depends only on depth and density.

  • Hooke's law: extension is proportional to applied force up to the limit of proportionality (F = kx).

Quick reference

Thermal Physics

  • Temperature is a measure of the average kinetic energy of particles; heat is energy transferred due to a temperature difference.

  • Specific heat capacity: E = mcΔθ, where c is energy per kilogram per kelvin.

  • Specific latent heat: E = mL; latent heat of fusion applies at melting point, vaporisation at boiling point.

  • Thermal energy moves by conduction (solids, particle collisions), convection (fluids, density currents) and radiation (infrared, needs no medium).

  • Dark, matt surfaces are good absorbers and emitters of infrared; shiny, light surfaces are poor emitters and good reflectors.

  • Gas laws for a fixed mass: P₁V₁/T₁ = P₂V₂/T₂ with T in kelvin (K = °C + 273).

  • Boyle's law: at constant temperature, pressure is inversely proportional to volume.

  • At a change of state the temperature stays constant because energy changes the potential energy of particles, not their kinetic energy.

Quick reference

Waves, Sound and Light

  • Wave equation: speed v = frequency f × wavelength λ; frequency is set by the source, speed by the medium.

  • Transverse waves oscillate perpendicular to energy transfer (light); longitudinal waves oscillate parallel (sound).

  • Reflection: angle of incidence = angle of reflection, both measured from the normal.

  • Refraction: light bends toward the normal entering a denser medium; Snell's law n = sin i ÷ sin r.

  • Total internal reflection occurs when light travels from denser to less dense medium and the angle of incidence exceeds the critical angle.

  • Sound needs a material medium; it travels fastest in solids, slowest in gases, and cannot cross a vacuum.

  • Frequency determines pitch; amplitude determines loudness; the audible range for humans is about 20 Hz to 20 kHz.

  • Converging lenses focus parallel rays at the principal focus; a real image is inverted and can be projected on a screen.

Quick reference

Electricity and Magnetism

  • Current I = Q/t (ampere = coulomb per second); conventional current flows from positive to negative terminal.

  • Ohm's law: V = IR, valid for a conductor at constant temperature.

  • Series circuit: same current in every component; total resistance R = R₁ + R₂ + …; voltages add.

  • Parallel circuit: same voltage across each branch; total resistance is less than the smallest branch resistance.

  • Electrical power P = VI = I²R = V²/R; energy transferred E = Pt.

  • Charge on one electron ≈ 1.6 × 10^-19 C; charge is conserved and quantised.

  • Magnetic field lines run from north to south outside a magnet; a current-carrying wire in a magnetic field experiences a force.

  • Electromagnetic induction: a changing magnetic field through a conductor induces an emf; faster change gives larger emf.

  • Fuse ratings are chosen just above the normal operating current to protect against overheating.

Quick reference

Matter and Atomic Physics

  • Kinetic particle model: solids vibrate in fixed positions, liquids slide past each other, gases move randomly at high speed.

  • Brownian motion of smoke particles in air gives evidence for randomly moving invisible molecules.

  • Density differences explain floating, sinking, convection and diffusion rates.

  • Atom: protons (+1) and neutrons (0) in the nucleus, electrons (−1) in shells; proton number fixes the element.

  • Isotopes have the same proton number but different neutron numbers; nucleon number = protons + neutrons.

  • Radioactive decay is random: alpha (⁴₂He), beta (electron) and gamma (electromagnetic) emissions differ in charge and penetrating power.

  • Half-life is the time for half the unstable nuclei in a sample to decay; activity halves each half-life.

  • Nuclear fission splits a heavy nucleus; fusion joins light nuclei and powers stars.

Quick reference

Earth and Space Physics

  • Earth orbits the Sun once in about 365.25 days; the Moon orbits Earth in about 27.3 days.

  • Day and night arise from Earth's rotation on its axis (about 24 hours); seasons arise from the tilt of the axis, not distance from the Sun.

  • Gravitational force between masses: F = Gm₁m₂/r²; it provides the centripetal force keeping planets in orbit.

  • Weight differs on other planets because g differs; mass is unchanged.

  • Solar system order: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune.

  • The Moon causes tides; the Sun and Moon align at spring tides and are at right angles at neap tides.

  • The Universe is expanding: distant galaxies show redshift, and Hubble's law links recession speed to distance.

  • Stars form from collapsing gas clouds; the Sun's energy comes from nuclear fusion of hydrogen into helium.

Quick reference

Practical Skills and Experimental Techniques

  • Repeat readings and average them to reduce random error; use the same instrument to keep systematic error consistent.

  • Zero a balance or ammeter before use; check for a zero error and subtract it from readings.

  • Measure time over many oscillations and divide by the count to reduce timing error.

  • Choose an instrument whose smallest division is appropriate: vernier callipers for diameters, metre rule for lengths, stopwatch for periods.

  • Plot the independent variable on the x-axis and the dependent variable on the y-axis; label axes with quantity and unit.

  • A straight-line graph through the origin shows direct proportionality; gradient equals the constant of proportionality.

  • Anomalous points are identified and excluded; a line of best fit balances points above and below it.

  • Safety: use a sand tray under a falling mass, switch off circuits before rewiring, and handle hot objects with tongs.