OCRA-LevelPhysics
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Newtonian World and Astrophysics

Thermal physics, gases, circular motion, oscillations, gravitation and cosmology

Practice 116 subtopics in Newtonian World and Astrophysics. All questions match the OCR A-Level specification.

About Newtonian World and Astrophysics

Newtonian World and Astrophysics is a key topic in the OCR A-Level Physicsspecification. This topic covers thermal physics, gases, circular motion, oscillations, gravitation and cosmology.

Master all 116 subtopics below with unlimited AI-generated questions. Each subtopic page includes sample questions and the ability to generate unlimited practice questions with detailed solutions.

All Subtopics (116)

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TemperatureThermal equilibriumAbsolute zeroKelvin scaleCelsius to Kelvin conversionStates of matterInternal energyKinetic energy of moleculesPotential energy of moleculesSpecific heat capacityQ = mcΔθSpecific latent heatLatent heat of fusionLatent heat of vaporisationKinetic theory of gasesAssumptions of kinetic theoryBrownian motionPressure of a gaspV = (1/3)Nm<c²>Boyle's lawCharles's lawPressure lawIdeal gas equation (pV = nRT)Molar gas constantAvogadro constantBoltzmann constantpV = NkTRoot mean square speedKinetic energy of gas moleculesE = (3/2)kTCircular motionAngular displacementAngular velocityRadianPeriod of circular motionLinear speedCentripetal accelerationCentripetal forceF = mv²/rHorizontal circular motionVertical circular motionConical pendulumBanked tracksSimple harmonic motionSHM definitiona = -ω²xDisplacement in SHMVelocity in SHMAcceleration in SHMSHM graphsAngular frequencyPeriod of SHMMass-spring oscillatorSimple pendulumPeriod of pendulumEnergy in SHMEnergy-displacement graphs in SHMDamped oscillationsLight dampingHeavy dampingCritical dampingForced oscillationsResonanceNatural frequencyDriving frequencyEffects of damping on resonanceGravitational fieldGravitational field linesGravitational field strengthUniform gravitational fieldRadial gravitational fieldNewton's law of gravitationF = GMm/r²Gravitational constant Gg = GM/r²Gravitational potentialV = -GM/rGravitational potential energyE = -GMm/rEscape velocitySatellite motionOrbital periodOrbital speedGeostationary orbitLow Earth orbitKepler's third lawEnergy of an orbiting satelliteStarsStellar evolutionLife cycle of starsProtostarMain sequenceRed giantWhite dwarfSupernovaNeutron starBlack holeHertzsprung-Russell diagramLuminosityApparent magnitudeAbsolute magnitudeStefan-Boltzmann lawWien's displacement lawStellar spectraSpectral classesDoppler effect for lightRed shiftBlue shiftHubble's lawHubble constantExpanding universeBig Bang theoryAge of universeCosmic microwave background radiationDark matterDark energy

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