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Thermal Physics — Key Terms Enrichment

Thermal physics · IGCSE Physics

Thermal Physics — Key Terms Enrichment — IGCSE Physics Notes

Exam years: 2025–2027 Topic: Thermal physics Lesson 20 of 48

Thermal Physics — Key Terms Enrichment

Master these foundation terms to decode questions quickly. Hover/tap the highlighted terms for quick meanings, and use the examples to anchor ideas to real situations. :contentReference[oaicite:0]{index=0}

Quick Meanings & One-line Hooks

Term Student-friendly meaning One-line example (IGCSE-style)
Endothermic Takes in energy (usually heat) from the surroundings. Ice melting absorbs energy → beaker feels colder.
Exothermic Gives out energy to the surroundings. Water freezing releases energy → keeps liquid at 0 °C until solidified.
Temperature Indicator of average kinetic energy of particles (°C or K). At higher T, gas particles collide more → pressure rises at fixed volume.
Intermolecular bonds Attractive forces between particles; must be overcome to melt/boil. At boiling point, energy breaks attractions instead of raising T.
Kinetic energy Energy due to particle motion; increases as T increases. Heating a gas → faster particles → more frequent/forceful wall hits.
Infra-red radiation EM waves (IR) that transfer heat; works even in vacuum. Sun warms Earth via IR; black, matt surfaces absorb/emit best.
Endothermic vs Exothermic — at a glance
  • Endothermic: energy IN to break intermolecular bonds (melting, boiling, sublimation).
  • Exothermic: energy OUT as bonds form/strengthen (freezing, condensation, deposition).

Energy in → (break bonds) → state change to less ordered
Energy out → (form bonds) → state change to more ordered

Temperature, Kinetic Energy & Bonding (Particle View)

  • Raising temperature → increases average kinetic energy → particles move faster.
  • At a flat part of a heating curve (melting/boiling), energy is used to overcome intermolecular bonds, so temperature stays constant.
  • Cooling curves: the reverse — energy released as bonds form (exothermic plateaus).

Infra-red Radiation — Surfaces Matter

  • Black/dull → better absorber & emitter of IR.
  • White/shiny → poorer absorber & emitter; better reflector.
  • No medium needed → IR works through a vacuum (space).
Exam Tips
  • Use K (Kelvin) for gas-law calculations; convert by T(K)=T(°C)+273.
  • On plateaus, write: “Temperature constant because energy changes bonding, not kinetic energy.”
  • Always state the direction of energy flow (into system vs out to surroundings) when saying endo/exo.

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