CCEA A-Level Physics A2 1 Deformation, Thermal Physics, Circular Motion, SHM and Gravity: a complete overview
A deep-dive CCEA A-Level Physics guide to the A2 1 unit on deformation of solids, thermal physics and ideal gases, circular motion, simple harmonic motion and gravitational fields. Covers Hooke's law and the Young modulus, heat capacity and kinetic theory, centripetal force, the SHM equations and resonance, and Newton's law of gravitation, with the equations CCEA examines.
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What this unit demands
A2 1 brings together the response of materials to forces, the behaviour of gases and heat, and the mathematics of rotation, oscillation and gravity. The examiners test precise definitions and defining conditions, confident calculation across several equations, and the ability to set out short derivations such as the mean kinetic energy of a gas molecule and Kepler's third law.
This guide walks through the five dot points of the unit, then sets out the exam patterns CCEA repeats. Each topic has a matching dot-point page with practice questions; this overview ties them together.
Deformation of solids
Hooke's law gives up to the limit of proportionality. Stress is force per area and strain is extension per original length; their ratio is the Young modulus, a property of the material. The strain energy stored is the area under the force-extension graph, , and stress-strain graphs distinguish brittle from ductile materials.
Thermal physics and ideal gases
Internal energy is the total random energy of the molecules and temperature measures their average kinetic energy. Specific heat capacity and specific latent heat quantify heating and changes of state. The ideal gas equation and kinetic theory combine to show the mean kinetic energy of a molecule is .
Circular motion and SHM
Circular motion has a centripetal acceleration towards the centre, produced by a centripetal force that is whatever real force points inward. Simple harmonic motion is defined by , giving a period independent of amplitude, energy that swaps between kinetic and potential, and resonance when the driving frequency matches the natural frequency.
Gravitational fields
Newton's law of gravitation gives . The field strength follows an inverse-square law, and the potential is always negative. For satellites, gravity provides the centripetal force, giving Kepler's third law , and a geostationary orbit has a 24-hour period over the equator.
How this unit is examined
A typical CCEA profile for A2 1:
- Definitions and conditions. Hooke's law, the SHM condition, field strength and potential.
- Calculation. The Young modulus, heat capacity and gas problems, centripetal force, SHM speeds and gravitation.
- Graphs. Stress-strain curves, displacement-time graphs and resonance curves.
- Derivation. The mean kinetic energy of a gas molecule and Kepler's third law.
Check your knowledge
A mix of recall and calculation questions covering the unit. Attempt them under timed conditions, then check against the solutions.
- Define the Young modulus and give its unit. (2 marks)
- A spring of spring constant is stretched by . Find the energy stored. (2 marks)
- How much energy is needed to melt of ice? Take . (2 marks)
- State what the absolute temperature of a gas measures, according to kinetic theory. (1 mark)
- A car of mass takes a bend of radius at . Find the centripetal force. (2 marks)
- State the defining condition for simple harmonic motion. (2 marks)
- State the condition for resonance and what happens to the amplitude at resonance. (2 marks)
- State Newton's law of gravitation in words. (2 marks)
Sources & how we know this
- CCEA GCE Physics specification — CCEA (2016)