Key term
Edexcel GCSE Physics 1PH0
Key Concepts of Physics
Motion and Forces
Topic overviewScalar and vector quantitiesExamples of vectors and scalars, and velocitySpeed, distance, time and distance-time graphsAcceleration and the equation v squared minus u squaredVelocity-time graphs and free fallMeasuring speed in the laboratory, and typical everyday speedsNewton's first law, and investigating force, mass and accelerationNewton's second and third lawsWeight, mass and gravitational field strengthReaction time, stopping distance and large decelerationsFactors affecting stopping distance and reaction timeBraking distance, speed and work done
Conservation of Energy
Waves
Topic overviewWhat waves transfer, and the evidence for itFrequency, wavelength, amplitude and periodLongitudinal and transverse wavesThe wave equationMeasuring wave speed, and what happens at a boundaryMeasuring waves in ripple tanks, strings and solidsReflection, refraction, transmission and absorption at a boundary
Light and the Electromagnetic Spectrum
Topic overviewReflection, refraction and total internal reflectionWhy objects appear colouredLenses, ray diagrams and imagesProperties of electromagnetic wavesInvestigating refraction in glass blocksThe groups of the electromagnetic spectrumThe continuous spectrum, and what our eyes can detectEmitting and absorbing thermal radiationHow radiation is generated, and why danger rises with frequencyHarmful effects of excessive exposure to radiationUses of electromagnetic radiation
Radioactivity
Topic overviewThe atom and the size of atomsIsotopes, atomic number and mass numberRelative masses and charges of subatomic particlesElectron orbits and energy levelsForming ions, and how the atomic model changedTypes of ionising radiationBackground radiation and detecting radioactivityAlpha, beta and gamma, and their penetrating powerBeta-minus and beta-plus decayEffects of decay on atomic number and mass numberBalancing nuclear equationsActivity and the becquerelHalf-life and the randomness of decayHalf-life calculationsUses of radioactivity, and how danger depends on half-lifeThe dangers of ionising radiationSafety precautions, contamination and irradiationRadiotherapy, medical tracers and PET scannersNuclear power and where nuclear energy comes fromFission of uranium-235 and the chain reactionControlling a reactor and generating electricityNuclear fusion and how it differs from fissionWhy fusion needs extreme conditions
Astronomy
Topic overviewWeight and gravitational field strength on other bodiesThe Solar System and the order of the planetsHow ideas about the Solar System and ways of observing it have changedOrbits of moons, planets, comets and satellitesGravity, orbital speed and stable orbitsThe Steady State and Big Bang theoriesEvidence for an expanding UniverseThe Doppler effect and red-shift in galaxiesThe life cycle of a star like the SunThe life cycle of stars more massive than the Sun
Energy – Forces Doing Work
Topic overviewEnergy stores and energy transfer diagramsChanging a system's energy, and measuring work doneWork done and the energy changes it causesGravitational potential and kinetic energy calculationsDissipation and wasted energyPower as the rate of energy transferThe watt, and calculating efficiency
Forces and Their Effects
Electricity and Circuits
Topic overviewThe atom, and drawing circuit diagramsSeries and parallel circuitsPotential difference and the voltmeterEnergy transferred by moving chargeCurrent, charge and measuring currentResistance and the equation V = IRResistors in series and in parallelDesigning circuits to test componentsInvestigating resistance in circuitsCurrent-potential difference graphs for componentsLight-dependent resistors and thermistorsThe heating effect of an electric currentUses of the heating effect, and the equation E = IVtPower as energy transferred per secondCalculating electrical powerEnergy transfer in domestic devices, and power ratingsDirect and alternating currentAlternating current and the UK mains supplyLive and neutral wires, earthing and fusesFuses in the live wire, mains voltages and electrical dangers
Static Electricity
Magnetism and the Motor Effect
Electromagnetic Induction
Particle Model
Topic overviewKinetic theory and differences in densityCalculating density, and investigating itChanges of state and internal energySpecific heat capacitySpecific latent heat and thermal insulationInvestigating the specific heat capacity of waterGas pressure and the motion of particlesAbsolute zero and the kelvin scaleCompressing gases, and the force a gas exertsPressure and volume of a fixed mass of gas
Astronomy
How ideas about the Solar System and ways of observing it have changed
- 3 things to know
- Paper 1
Overview
The geocentric and heliocentric models, telescope evidence from Jupiter's moons and the phases of Venus, elliptical orbits, why models change, and observing by naked eye, telescope, photography and digital detectors, including radio, X-ray and orbiting telescopes.
What you need to know
Answer each one before you reveal it.
Your recallNot started
Key term
Give one early telescope observation that supported the Sun-centred model of the Solar System.
Key term
State a telescope observation of Venus that supported the Sun-centred model of the Solar System.
Questions from this subtopic
Each one with the model answer underneath.
- 1
Describe the geocentric model of the Solar System.
Model answer
In the geocentric model the Earth sits at the centre and the Sun, Moon, planets and stars all move around the Earth in circles.
- 2
Describe the heliocentric model of the Solar System.
Model answer
In the heliocentric model the Sun sits at the centre and the Earth and the other planets orbit around it.
- 3
Which model of the Solar System is accepted today?
Model answer
The heliocentric model, with the Sun at the centre and the planets orbiting it.
- 4
Give one early telescope observation that supported the Sun-centred model of the Solar System.
Model answer
Four moons were seen orbiting Jupiter, which showed that not everything in the sky moves around the Earth.
- 5
State a telescope observation of Venus that supported the Sun-centred model of the Solar System.
Model answer
Venus was seen to go through a full set of phases, which can only happen if Venus orbits the Sun.
- 6
How were the shapes of the planets' paths corrected after the first Sun-centred model was proposed?
Model answer
Perfectly circular paths were replaced by slightly elliptical orbits, which matched the observed positions of the planets far better.
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