A2.1.1—Conditions on early Earth

Early Earth combined an oxygen-poor atmosphere, liquid water, strong natural energy sources, mineral surfaces, and extraterrestrial inputs that could support prebiotic chemistry.

Syllabus
First assessment 2025
Objective
A2.1.1
Level
HL

Exam analysis

Chance of appearing1%of analysed past papers
Latest appearanceMay 2013
Most common paperPaper3
Typical marks2–3

Common command terms

  • State
  • Evaluate
  • Outline

Scoring notes

Common mistake
Treating one proposed environment as the proven location where life began.

Recent exam appearances

May 2013Paper3 ["HL"] · TZ1D1(c)[ 2 ]A2.1.1—Conditions on early Earth
May 2013Paper3 ["HL"] · TZ1D1(b)[ 3 ]A2.1.1—Conditions on early Earth
Practice this objective

Coverage 2013–2013 · Updated 15 Jul 2026

Early Earth Set the Chemical Starting Conditions

HL only

Early Earth had little free oxygen and therefore little ozone, but higher concentrations of carbon dioxide and methane. Warmer conditions and stronger ultraviolet penetration created a chemical setting unlike today's.

Without an ozone shield, more ultraviolet radiation reached the surface and supplied energy for reactions. Under these anoxic conditions, carbon compounds may have formed spontaneously by chemical pathways that are uncommon today.

Build the explanation as conditions -> consequence: little O2 -> little ozone -> more UV; more CO2 and methane -> higher temperatures; energy plus simple chemicals -> possible prebiotic carbon compounds.

An anoxic mixture containing carbon-bearing gases and water can be exposed to an energy source in a controlled experiment to test whether carbon compounds form.

Reconstructing plausible conditions tests chemical feasibility; it does not prove that early life followed the exact laboratory route.

Conditions on early Earth

Assessment in practice

1–3 marks
How it is assessed

This objective is assessed through data analysis, commonly using State / Evaluate / Outline.

Command terms

State / Evaluate / Outline

What earns marks

Build the answer around this relationship: Early Earth had little free oxygen and no protective ozone layer.

Watch for

Treating one proposed environment as the proven location where life began.

Representative question

Question 1

[Maximum number: 3]

This investigation was performed in a chamber at 85C85^{\circ} \mathrm{C} leading to total evaporation of the salt water within one day. The atmosphere inside the chamber consisted of nitrogen, carbon dioxide and water vapour. Evaluate the experiment on the basis of similarity with conditions that existed on the prebiotic Earth.

Pull The Whole Origin Argument Together

A2.1 is usually tested as a connected argument, not as isolated facts. A strong answer builds a chain: early Earth conditions made abiotic organic synthesis plausible; origin models require small molecules, polymers, self-replication, and membranes; experiments and models support parts of the chain; LUCA, dating, and vents provide later evidence and constraints. The highest-scoring habit is to say “supports” when evidence supports, and avoid saying “proves” when it does not.

  • Conditions explain why prebiotic chemistry was possible.
  • Required transitions explain what a first cell-like system needed.
  • Miller-Urey, vesicles, and RNA world support specific steps.
  • LUCA, dating methods, and vents help evaluate when and where early cellular life may have existed.
  • Use careful evidence language: supports, suggests, plausible, not proves.

Concept essentials

  • Early Earth had little free oxygen and no protective ozone layer.
  • Natural energy sources could drive reactions among simple substances.
  • Evaporation cycles could concentrate reactants in shallow water.
  • Mineral surfaces and extraterrestrial material could contribute catalysts or organic compounds.