England · Waves · WA-U4

WA-14 · Black bodies and radiation balance

Planned lecture content and an original worked practice example. Read the scope labels before using Higher or separate-Physics branches.

Status

Lecture detail

WA-14 · WA-U4 · Planned

Black bodies and radiation balance

  • ScopeSeparate Physics + Separate Physics Higher balance
  • Difficulty3 (H 4) / 4 · proposed
  • Time35–40 min · estimated
  • StatusPlanned

Learning objectives

Explain emission at all temperatures and temperature-dependent spectrum; H: relate temperature change to absorbed/emitted power, including Earth.

8463 §§4.6.3.1–4.6.3.2 / No Trilogy counterpart

DfE single-science pp.37–39 / Combined pp.32–33. Evidence checked 30 September–1 October 2026. Skills: WS1.2,1.3,3.5; MS4a.

Needs firstWA-11,EN-03

Explanation

Every object emits radiation, and emission distribution changes with temperature. A perfect black body absorbs all incident radiation and is the best emitter. The Higher energy-balance branch distinguishes absorbed power from incident/reflected power and links net absorption to temperature change.

Concepts, equations and units: Perfect black body absorbs all incident radiation and is best emitter; spectrum intensity/wavelength vs temperature; H power balance W.

Prediction, demonstration and game exercise

Predict, observe, explain

Compare labelled model spectra; H vary absorption/reflection/emission of Earth–atmosphere model.

Planned learner game exercise

Choose surfaces for a satellite; H adjust incoming/absorbed/emitted power and predict warming/cooling/equilibrium.

Independent practice

Interpret two spectra; H annotate an Earth radiation diagram and identify a model limitation.

Original practice example · Separate Physics Higher

A body absorbs 120 W and emits 100 W, with no other transfers in the stated model. Predict its temperature change.

Show working and model answer

Working / reasoning

Net rate into the body = 120 − 100 = 20 W; internal energy rises.

Answer

It warms; net absorbed power is 20 W.

Exit check and success criteria

Correct hotter-spectrum comparison; H temperature change consistent with net absorbed power and equilibrium rates equal.

During practice, compare the prediction with evidence and give an error-specific prompt. The exit item uses a fresh context or fresh values, answered independently.

Misconceptions, practical links and mastery

Check these misconceptions

Cold objects do not radiate; constant temperature means no transfer; greenhouse model proves exact future temperature.

Practical preparation

RP-P10 data revisit; black-body theory and H balance extend beyond shared RP.

Virtual preparation and revision only. Required hands-on activities and school records remain separate.

Proposed mastery

0: not yet evidenced. 1: supported. 2: independent exit criteria met. 3: successful changed-context transfer. Advance at 2; revisit with fresh retrieval. These are not GCSE grades.

Unit assessment

Continue through the unit

Sources and full programme

Sources checked 30 September–1 October 2026. Specifications govern content; textbooks supplement it. England has no single prescribed Physics course book. The full planning document includes sourced comparisons of Collins separate Physics and Trilogy books, Hodder/Hachette Physics and Oxford Physics listings, with access/approval limitations.

Download the complete Markdown programme and coverage matrix

A subsection map is proposed coverage. Clause-level educator review, item moderation, model validation and hands-on provision remain release gates. No all-board alignment or exam-board endorsement is claimed.