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NotesESS HLTopic 6.1
Unit 6 · Atmosphere and Climate Change · Topic 6.1

IB ESS HL — Introduction to the atmosphere

At Higher Level, Topic 6.1 requires deeper understanding of atmospheric physics, radiation budgets, and the quantitative relationships between atmospheric composition and energy balance. Students must demonstrate more precise scientific reasoning in their analysis of atmospheric processes.

Higher Level students should use this topic hub as a map: start with the shared sub-topics, then follow the HL-only extensions and exam-skill links where this topic asks for deeper analysis.

6.1 FlashcardsExam technique guidePractice questions

Key concepts in Introduction to the atmosphere

Key Idea: Topic 6.1 carries few marks, and almost all of them are on the natural greenhouse effect. At HL, also learn the dynamic atmosphere, Milankovitch cycles and how life changed the air.

1. The greenhouse effect (most marks)

  • Sunlight (short-wave) passes through the air and warms the surface.
  • The warm surface gives off infrared (long-wave) radiation.
  • Greenhouse gases absorb and re-emit it, so Earth averages about 15 °C, not about -18 °C.

2. Greenhouse gases and aerosols

  • Main GHGs: water vapour, carbon dioxide, methane, nitrous oxide, ozone, CFCs.
  • Cattle and rice paddies give off methane; burning fuels gives carbon dioxide.
  • Most aerosols, such as sulfate, reflect sunlight and cool; soot absorbs it and warms.

3. The atmosphere and HL ideas

  • Air is about 78% nitrogen, 21% oxygen, under 1% argon and about 0.04% carbon dioxide.
  • Weather happens in the troposphere; the ozone layer is in the stratosphere.
  • At HL: the atmosphere as a dynamic system, gravity and air pressure, Milankovitch cycles and how life changed the air.

How it is examined:

QuestionHow to score
[1] Name a greenhouse gasName it exactly: methane, not 'gas from cows'.
[1] Give evidence a gas is a greenhouse gasIt absorbs infrared, so the temperature rises with it.
[4] Outline the greenhouse effectShort-wave in, surface warms, long-wave out, GHGs absorb and re-emit.
[7] Explain how the atmosphere keeps Earth habitableGreenhouse effect, ozone absorbing UV, heat moved by circulation.

Key terms, one line each:

TermIn one line
Greenhouse gasa gas that absorbs and re-emits infrared radiation
Aerosoltiny solid or liquid particles in the air, such as sulfate or soot
Tropospherethe lowest layer, where weather happens
Stratospherethe layer above, which holds the ozone layer
Tricellular modelthree circulation cells in each hemisphere move heat to the poles
Milankovitch cycleschanges in Earth's orbit and tilt that cause ice ages
Great Oxidation Eventoxygen from early photosynthesis building up in the air

Last-minute check: answer, then tap to see.

Name the three Milankovitch cycles. Eccentricity, obliquity (tilt) and precession (wobble).

Why is most air in the lowest few kilometres? Gravity pulls air down, so pressure and density fall with height.

Where did the oxygen in the air come from? Photosynthesis, first by cyanobacteria.

Is the greenhouse effect natural? Yes; people have enhanced it.

IB-style questionExplain[4 marks]

Ice cores show that Earth has swung between glacials and interglacials about every 100,000 years. Explain how changes in Earth's orbit can start these cycles.

Model answer plan

See the mark-by-mark plan — for / against / judgement, with marking guidance — in study mode.

Claim your free topic →

Exam tips

  • For the greenhouse effect, say short-wave in and long-wave (infrared) out.
  • Say GHGs absorb and re-emit infrared, not that they 'trap' or 'block' sunlight.
  • Do not mix up the greenhouse effect with the ozone hole.
  • Learn the three Milankovitch cycles with their time spans.

What you'll learn in Topic 6.1

  • 6.1.1 The atmosphere and its layers
  • 6.1.2 Uneven heating and global circulation
  • 6.1.3 Greenhouse gases and aerosols
  • 6.1.4 The natural greenhouse effect
  • 6.1.5 The atmosphere as a dynamic system
  • 6.1.6 Gravity and the atmosphere
  • 6.1.7 Milankovitch cycles
  • 6.1.8 Leaving the glacial cycle
  • 6.1.9 Life and the changing atmosphere

Exam relevance

At Higher Level, ESS includes an extended essay component and deeper analytical questioning. Expect longer data-response questions and more complex case study scenarios in both Paper 1 and Paper 2.

Suggested study order: Read the notes for each sub-topic below → test yourself with flashcards → attempt practice questions → review exam technique.

Study resources — 6.1 Introduction to the atmosphere

6.1.1

The atmosphere and its layers

NotesFlashcards
6.1.2

Uneven heating and global circulation

NotesFlashcards
6.1.3

Greenhouse gases and aerosols

Notes
6.1.4

The natural greenhouse effect

NotesFlashcards
6.1.5

The atmosphere as a dynamic system

Notes
6.1.6

Gravity and the atmosphere

Notes
6.1.7

Milankovitch cycles

Notes
6.1.8

Leaving the glacial cycle

Notes
6.1.9

Life and the changing atmosphere

Notes

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Topic 6.1 Introduction to the atmosphere forms a core part of Unit 6: Atmosphere and Climate Change in IB ESS HL. Mastering these concepts will strengthen your understanding of connected topics across the syllabus and prepare you for exam questions that require analysis, evaluation, and real-world application.

Frequently asked questions

What does Topic 6.1 Introduction to the atmosphere cover in IB ESS?
Topic 6.1 covers introduction to the atmosphere as part of the IB ESS syllabus. Students learn key concepts, definitions, and real-world examples that are tested in Paper 1 and Paper 2 exams.
How should I revise Introduction to the atmosphere for IB ESS exams?
Start by reading the micro-topic notes to understand each concept, then use flashcards to memorise key terms. Practise exam-style questions to apply your knowledge under timed conditions and review the marking criteria.
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6.2 Climate change—causes and impacts
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