IB Biology · Theme A · A2.1 · HL only

From soup
to cell.

A planet of chemistry, then a planet of cells. The first cells made themselves — and the rest is biology.

9Sub-topics
16Key terms
HL onlyLevel
CellsLevel of organisation
PROTOCELL
Why this topic

What this topic answers.

Every sub-topic below feeds at least one of these questions.

Guiding question 1

What plausible hypothesis could account for the origin of life?

Guiding question 2

What intermediate stages could there have been between non-living matter and the first living cells?

HL extension

Higher Level only.

An extra 9 sub-topics for HL — same syllabus, deeper mechanism.

HL only

Conditions on early Earth and the pre-biotic formation of carbon compounds

Conditions on early Earth and the pre-biotic formation of carbon compounds

HL only

Cells as the smallest units of self-sustaining life

Cells as the smallest units of self-sustaining life

HL only

Challenge of explaining the spontaneous origin of cells

Challenge of explaining the spontaneous origin of cells

HL only

Evidence for the origin of carbon compounds

Evidence for the origin of carbon compounds

HL only

Spontaneous formation of vesicles by coalescence of fatty acids into spherical bilayers

Spontaneous formation of vesicles by coalescence of fatty acids into spherical bilayers

HL only

RNA as a presumed first genetic material

RNA can be replicated and has some catalytic activity so it may have acted initially as both the genetic material and the enzymes of the earliest cells.

HL only

Evidence for a last universal common ancestor

Evidence for a last universal common ancestor

HL only

Approaches used to estimate dates of the first living cells and the last universal common ancestor

Approaches used to estimate dates of the first living cells and the last universal common ancestor

HL only

Evidence for the evolution of the last universal common ancestor in the vicinity of hydrothermal vents

Evidence for the evolution of the last universal common ancestor in the vicinity of hydrothermal vents

A2.1.1 · Pre-biotic Earth

A planet of chemistry, not biology.

Before life, Earth was a strange place by today's standards: no oxygen, no ozone, scorching ultraviolet, much more CO₂ and methane in the air.

Atmosphere · main gases
N₂ · CO₂ · H₂O

Plus smaller amounts of methane and hydrogen. No free oxygen.

Free O₂
~0 %

Free oxygen only entered the atmosphere later, as a by-product of photosynthesis.

UV radiation
very high

No ozone layer (because no O₂) → intense UV reached the surface.

Surface temperature
hot

High CO₂ → strong greenhouse effect → much warmer than today.

In the 1920s Oparin and Haldane independently proposed that under these conditions, the available energy — UV, lightning, volcanic heat — could drive the spontaneous formation of organic compounds (carbon-containing molecules) from inorganic precursors. Over time, the organic molecules would grow more complex, eventually leading to self-replicating structures and the first cells.

⚗️

Organic vs inorganic

Organic compounds are carbon-containing molecules (excluding simple oxides like CO₂ and carbonates). Everything else is inorganic. Pre-biotic chemistry needed inorganic gases to give rise to organic monomers.

A2.1.2 · Cells as the unit of life

The smallest self-sustaining unit.

The three-part cell theory: cells are the basic unit of life; all organisms are made of one or more cells; all cells come from pre-existing cells.

A cell can carry out, by itself, all seven characteristics of life — metabolism, homeostasis, response, reproduction, growth, development, genetic continuity. Subcellular components (ribosomes, mitochondria) can't. Viruses can't either — they need a host cell — which is the syllabus's exact reason for excluding them from the category "alive".

⚠️

Why viruses aren't alive

Viruses have genetic material (DNA or RNA) inside a protein coat — but no cells, no metabolism, no homeostasis, no response to stimuli, no independent growth, no independent reproduction. They are replicated by host cells. Genetic material alone is not enough.

A2.1.3 · The challenge

Cells are hard to make.

Today, cells only come from other cells. Explaining how the very first one assembled itself is the central puzzle of origin-of-life science.

Four ingredients had to come together before the first cell could exist:

1

Catalysis

Some molecule had to speed up chemical reactions. Modern cells use protein enzymes — but proteins are themselves products of biology. Something simpler had to come first.

2

Self-replication

The molecule of inheritance had to be able to copy itself, so that information could be passed to descendants.

3

Self-assembly

Membranes and compartments had to form from their components spontaneously, without anyone (or anything) building them.

4

Compartmentalisation

The interior chemistry had to differ from the exterior. Without a boundary, no concentration gradients, no metabolism, no cell.

🔬

Nature of Science · testability

Scientific hypotheses must be testable. Origin-of-life hypotheses are unusually hard because the exact conditions on pre-biotic Earth can't be replicated, and protocells didn't fossilise. The best we can do is build plausible chemistry under conditions we believe are close, and see what forms.

A2.1.4 · Miller & Urey (1953)

A jar of amino acids from a jar of gases.

Miller and Urey's classic experiment took the Oparin–Haldane hypothesis seriously and tested it in a flask. The result changed the field.

The setup

  • Methane + ammonia + hydrogen + water vapour, modelling the prebiotic atmosphere.
  • A flask of liquid water modelling the oceans.
  • An electrical spark inside the gas chamber to model lightning.
  • A heat source under the water flask to evaporate it; a condenser to bring vapour back as "rain".

The result

After one week the water had turned a brownish-black. Chemical analysis showed it contained amino acids and other complex organic molecules — built from the inorganic starting gases by nothing more than the apparatus.

Strengths

What the experiment did well

Modelled the prebiotic atmosphere; demonstrated that organic molecules (including amino acids) can form spontaneously under abiotic conditions; the apparatus was simple, reproducible, and has been replicated many times by other groups.

Limitations

What it didn't settle

The exact composition of the prebiotic atmosphere is still debated — Miller and Urey assumed a strongly reducing mix that may have been less hydrogen-rich in reality. The experiment did not produce all the organic molecules needed for life. It also couldn't simulate every condition (deep-sea vents, mineral surfaces, time-scales).

A2.1.5 · Spontaneous vesicles

Why amphipathic molecules make membranes for free.

Modern cell membranes are phospholipid bilayers. It turns out that simpler amphipathic molecules — fatty acids — form spherical bilayers spontaneously when mixed with water. That's how the first compartments could have formed.

A phospholipid has a hydrophilic phosphate head and two hydrophobic fatty acid tails — it is amphipathic. In water, amphipathic molecules self-assemble: heads face the water, tails huddle together away from the water. Given the right concentration, the result is a closed spherical bilayer — a vesicle.

Fatty acids form spontaneously in Miller–Urey-style experiments. Once enough were around, they would have coalesced into vesicles automatically. If a self-replicating RNA molecule happened to be inside one of these vesicles, you'd have something that looked very much like a primitive cell — a protocell.

A2.1.6 · The RNA world

One molecule. Two jobs.

The biggest reason RNA is favoured over DNA as the original genetic material: RNA can both store information and catalyse chemistry. DNA can only do the first.

  • Stores information. Like DNA, RNA bases can encode sequences.
  • Self-replicates. RNA molecules can pair with complementary nucleotides and act as their own template.
  • Catalyses reactions. Some RNA molecules — called ribozymes — are enzymes in their own right.
🧬

Ribozymes are still with us

Inside every modern ribosome, the peptide bond that joins amino acids during translation is catalysed by RNA, not protein. The catalytic core of the ribosome is a ribozyme. That's a fossil from the RNA world, still doing its original job inside every living cell.

A2.1.7 · Last Universal Common Ancestor

Every living thing descends from one cell.

LUCA — the Last Universal Common Ancestor — is the most recent organism from which every cell now alive ultimately descends. Two strong lines of evidence point to its reality.

Evidence 1

Universal genetic code

The same 64 codons specify the same 20 amino acids in bacteria, archaea, plants, fungi and animals. A code this complicated and arbitrary is wildly unlikely to have evolved independently in different lineages. Far simpler explanation: it was inherited from a common ancestor.

Evidence 2

Conserved core genes

A handful of essential genes — for ribosomal RNA, key metabolic enzymes — are present in all three domains. Their sequences are similar enough across domains to be unmistakably homologous: shared from a common ancestor.

There may well have been other lineages of early life alongside LUCA's ancestors. If so, they were out-competed and went extinct. We see only LUCA's descendants because they were the line that survived.

A2.1.8 · Dating the first cells

How we know when.

Earth is about 4.6 Ga. LUCA appears to be around 4.0 Ga. Two main methods give us these dates.

Method 1

Radiometric dating of rocks

The oldest known fossils — of cyanobacteria-like cells — are about 3.5 billion years old. Rocks around them are dated by measuring the decay of unstable radioactive isotopes (e.g. uranium → lead) which decay at known, constant rates.

Method 2

Molecular clocks

The number of mutations accumulated in a gene since two species diverged is roughly proportional to the time elapsed. Calibrating mutation rates lets us estimate divergence dates — and projecting back to the deepest common ancestor of all life places LUCA ~4 Ga.

Age of Earth
4.6 Ga

From radiometric dating of the oldest mineral grains.

Oldest cell fossils
3.5 Ga

Cyanobacteria-like microfossils.

Estimated age of LUCA
~4 Ga

From molecular clock analyses.

Time since
~4 billion years

Of continuous evolution producing today's biodiversity.

A2.1.9 · Hydrothermal vents

Hot, dark, chemically rich.

The best current candidate location for the origin of LUCA is the vicinity of deep-sea hydrothermal vents. Two lines of evidence make the case.

Geology

Fossil evidence at vents

Fossilised microbial communities (similar to modern cyanobacteria) have been recovered from ancient hydrothermal-vent precipitates. The chemistry around vents is rich in dissolved methane, CO₂, hydrogen and sulfide compounds — exactly the building blocks Miller–Urey-style experiments need.

Genomics

Conserved thermophilic genes

Comparing genes shared across all three domains, biologists find a striking number that look like adaptations to high temperatures — enzymes that work best near 80 °C. This thermophilic signature in LUCA's gene set suggests LUCA itself was hot-adapted, consistent with a vent origin.

HL-only key terms

Pre-bioticOrganic compoundsSpontaneous generationLUCADomainsEubacteriaArchaeaEukaryaEvolutionAmphipathicHydrophilicHydrophobicVesicleRibozymeHydrothermal ventThermophiles
Vocabulary

0 terms to own.

If you can't define one of these in a sentence, that's where to revise next.

IB Linking Questions

“For what reasons is heredity an essential feature of living things?”

“What is needed for structures to be able to evolve by natural selection?”