Learn in your language
Skip to content
IGCSE · Cambridge (CIE) · 0972

Explain Earth temperature through radiation balance

Distinguish absorbed sunlight, reflected sunlight and infrared exchange at the surface and planetary boundaries.

Thermal radiation pathway · 0972 (9–1) · 2.3.3
Exam scope and assessment notes

Extended only (Supplement) · Physics 0972, 2026–2028, section 2.3.3. These lessons cover steady and unequal rates, Earth radiation balance, emitter/absorber experiments and temperature/area effects. Written calculations and described methods are self-checked; human subject-teacher review, supervised practical competence and cumulative assessment remain pending. Cambridge states that IGCSE 0972 has the same subject content as IGCSE 0625, with 9–1 grading. This StudyForA pathway maps the 2026–2028 syllabus only. This 9–1 graded qualification is available only in a limited number of administrative zones. Confirm that your centre can enter you for this code and exam series with Cambridge International. Cambridge has published a separate syllabus for 2029. StudyForA has not reconciled that version yet; this page supports exams in 2026, 2027 and 2028 only.

Before you begin

  • Distinguish absorption, reflection and emission.
  • Use a complete received-minus-outgoing account.

Work on paper. Try each question before revealing help, and explain why your method works.

Quick readiness check

In the supplied planetary model, 100 units arrive and 30 are reflected. How much is absorbed?

What you will learn

  • Explain factors controlling incoming and outgoing radiation and Earth temperature.
  • Distinguish the surface account from the Earth-plus-atmosphere boundary.
Original conceptual Earth-plus-atmosphere diagram distinguishes solar input, reflected sunlight and thermal infrared leaving to space. A separate surface-atmosphere exchange is internal to the larger boundary and must not be counted as a new external source. The supplied model uses 100 incoming units, 30 reflected and 68 outgoing infrared per interval, giving 2 units gained; these are illustrative rather than present-day global measurements or a forecast.Earth + atmosphere · larger boundarySolar 100Reflected 30IR 68Surface / atmosphereExchange inside boundary is internalAbsorbed: 100 − 30 = 70Net: 70 − 68 = 2 units gainedIllustrative units · not climate data
Original conceptual Earth-plus-atmosphere diagram distinguishes solar input, reflected sunlight and thermal infrared leaving to space. A separate surface-atmosphere exchange is internal to the larger boundary and must not be counted as a new external source. The supplied model uses 100 incoming units, 30 reflected and 68 outgoing infrared per interval, giving 2 units gained; these are illustrative rather than present-day global measurements or a forecast.

Name the boundary before balancing

Sunlight reaching Earth includes several wavelength regions. Some is reflected by clouds, atmosphere and bright surfaces; the rest can be absorbed. The Earth system emits thermal infrared toward space. At the Earth-plus-atmosphere boundary, compare absorbed solar input with outgoing thermal infrared; reflected sunlight was not absorbed and is not counted again as internal-energy gain.

At the surface boundary, absorbed sunlight and infrared from the atmosphere can provide input, while surface emission and other thermal routes provide output. Radiation exchanged between surface and atmosphere is internal to the larger system. Do not add that exchange as a second independent solar source in the planetary account. These distinctions follow the primary NASA radiation-budget explanations; no present-day global measurement is assigned by the schematic.

Explain factors and the initial response

A larger reflected fraction can reduce absorbed sunlight if incoming radiation is otherwise unchanged. Greenhouse gases such as water vapour and carbon dioxide absorb some surface-emitted infrared and emit infrared, including back toward the surface. They do not create energy or block all possible outgoing radiation. Changes can alter the outgoing rate at a given state and therefore the temperature needed for a new balance.

If the whole system initially absorbs more than it emits to space, it gains energy and can warm; the opposite imbalance can cool it. Warmer surfaces generally emit at greater rates, affecting the later balance. Clouds can change both reflection and infrared exchange, so one unspecified cloud change has no universal sign here. Numerical future climate, weather or global-temperature changes are not determined by this qualitative lesson.

Pause and explain

Which greenhouse account preserves energy and the system boundary?

Put the idea to work

Worked example

In an original planetary teaching model, 100 units of solar energy arrive per interval, 30 are reflected and 68 units of thermal infrared leave to space. Find the net system gain.

Show the worked solution
  1. Absorbed solar input is 100 − 30 = 70 units.
  2. Outgoing thermal infrared is 68 units at the larger system boundary.
  3. Net gain is 70 − 68 = 2 units per supplied interval; reflected energy is not counted as absorbed.

Answer A 2-unit system gain per supplied interval, not a measured global climate value.

Try a topic test

Choose Easy, Normal or Difficult. Save your answers and open worked review after finishing.

Test this topic →

From guided practice to a new situation

Write your answer and reasoning first. Use a hint only if you are stuck. The model solution is for self-checking; your written work is not automatically marked.

1 · Guided

Find net gain in the supplied model with solar 100 units, reflection 30 and outgoing thermal infrared 68.

Give me a hint

Use absorbed input at the same boundary as the outgoing value.

Compare my reasoning
  1. Absorbed input is 70 units.
  2. Outgoing thermal infrared is 68 units.
  3. Net gain is 2 units per specified interval.

2 units gained per supplied interval.

Look for these in your work

  • Subtract reflection once.
  • Use the same system boundary.
2 · Independent

With the same 100-unit incoming amount, reflection rises from 30 to 35 while outgoing remains 68 initially. Find the new balance and qualitative initial tendency.

Give me a hint

Keep the stated outgoing value fixed only for the supplied initial comparison.

Compare my reasoning
  1. Absorbed input becomes 65 units.
  2. Net is 65 − 68 = −3 units per interval.
  3. The system initially loses energy; a cooling tendency is supported, not an exact temperature drop.

−3 units per interval; an initial cooling tendency.

Look for these in your work

  • Use changed absorption.
  • Do not extrapolate a complete climate forecast.
3 · Transfer

A diagram includes downward atmospheric infrared as a surface input. A student adds it again to solar input for Earth plus atmosphere. Explain the error.

Give me a hint

The surface and planetary boundaries include different transfers.

Compare my reasoning
  1. Downward infrared enters the surface account.
  2. It leaves another part of the same larger system.
  3. Adding it as independent planetary input double-counts an internal exchange.

The larger-boundary account must not count internal atmospheric exchange as a new external source.

Look for these in your work

  • Name both boundaries.
  • Preserve energy conservation.

Common mistakes

  • Reflected sunlight is not absorbed input.
  • Surface-atmosphere exchange is internal to the larger system.
  • Greenhouse gases do not create energy or block every infrared path.
Recall without your notes

What can you explain now?

Is atmospheric infrared toward the surface a new independent energy source added to solar input for the whole Earth system?

Compare with the explanation

No.

It is an internal exchange at that larger boundary, though it is an input for the surface boundary.

After trying it yourself, choose your next review. This is your self-assessment.

Your review choice appears on Today. Sign in to sync it across devices.

Make it stick

Explain albedo and atmospheric infrared while keeping absorbed solar input, internal exchange and outgoing planetary radiation distinct.

If you needed the solution, close it and solve the problem again from a blank page. A correct answer is stronger when you can explain the reason for each step.

Keep learning Physics (9-1)

Course scope and assessment

491 sequenced Physics lessons provide 1473 guided, independent and application problems. 58 of 58 syllabus sections have full linked teaching sequences; 0 sections remain pending. Three earlier starter overviews remain available but are not counted as full sequences. The map covers all six subject areas for 2026–2028 and keeps review and assessment limits visible. This is available content, not full programme completion, an exam grade or certified mastery. Written practice is self-checked. Supervised practical experience, cumulative assessment and human subject-teacher review remain pending. Paper method exercises do not demonstrate practical competence or complete either practical-assessment route. This is the separate 9–1 qualification 0972; Cambridge states that its 2026–2028 subject content is otherwise the same as 0625. This 9–1 graded qualification is available only in a limited number of administrative zones. Confirm that your centre can enter you for this code and exam series with Cambridge International. The 2029 syllabus is separately published at https://www.cambridgeinternational.org/Images/764368-2029-syllabus.pdf and is not yet mapped here. This course supports exams in 2026, 2027 and 2028 only.

StudyForA · Learn with understanding

Original teaching content and links to official sources. Check your exam year and qualification before using a resource.