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ESO Y4B · Biology and Geology
Earth in the Universe · The Universe and the Solar System

The origin of life

4 600 million years ago, the Earth was a sphere of molten rock without a single form of life. Today, any ecosystem shows an immense biological diversity. Between one moment and the other, a decisive transition had to take place: the step from inert matter to living matter, one of the great open problems in science.

Before you start, make sure you know: The characteristics of living things (1st ESO)
Before you start, make sure you know: The cell, the unit of living things (1st ESO)

The early Earth

Landscape of the early Earth: an ocean, an erupting volcano, falling meteorites and an impact crater, beneath a reducing atmosphere with no free oxygen, rich in water vapour, carbon dioxide, methane, ammonia and hydrogen. Ultraviolet radiation from the Sun reaches the surface because there is no ozone layer. ultraviolet radiation no ozone layer reducing atmosphere no free O₂ H₂O · CO₂ · CH₄ · NH₃ · H₂ bombardment by meteorites primitive ocean impact crater volcanic activity intense
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Describe what early Earth was like at the time life emerged: its atmosphere, its oceans and its geological activity.

Describe what early Earth was like at the time life emerged: its atmosphere, its oceans and its geological activity.

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From spontaneous generation to prebiotic synthesis

Apparatus of the Miller–Urey experiment: water boils in a small flask, the steam rises to a large flask containing the gases of the primitive atmosphere (H₂O, CH₄, NH₃, H₂) where electrodes produce electrical discharges, a condenser cools the gases and in the U-tube water containing organic molecules, such as amino acids, accumulates. electrical discharges electrodes H₂O, CH₄, NH₃, H₂ primitive atmosphere water vapour condenser (cooling) cold water boiling water heat water with organic molecules amino acids and other simple molecules
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Look at the diagram of the apparatus with which Miller and Urey carried out their famous experiment in 1953. Identify what the parts labelled ?1 to ?4 represent (the gas…

Look at the diagram of the apparatus with which Miller and Urey carried out their famous experiment in 1953. Identify what the parts labelled ?1 to ?4 represent (the gas mixture, electrical discharges, boiling water and the collection trap), explain what conditions of early Earth they simulated in the laboratory and what type of molecules they obtained.

Heat CH₄ NH₃ H₂ H₂O ?1 ?2 ?3 ?4
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For centuries, it was believed that living organisms could arise from non-living matter: worms from decaying meat or mice from dirty clothes. Describe what the…

For centuries, it was believed that living organisms could arise from non-living matter: worms from decaying meat or mice from dirty clothes. Describe what the hypothesis of spontaneous generation consisted of, and explain how it was experimentally disproved by Redi with his jars of meat, Spallanzani with boiled broths and, above all, Pasteur with his swan-neck flasks.

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Hypotheses on the origin of life

Flow diagram of the hypothetical stages from organic molecules and hereditary material to the first cell. organicmolecules metabolism +membrane firstcell + hereditary material able to copy itself
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Current hypotheses on the origin of life include chemical synthesis in the "primordial soup", panspermia and hydrothermal vents on the ocean floor. Summarise them…

Current hypotheses on the origin of life include chemical synthesis in the "primordial soup", panspermia and hydrothermal vents on the ocean floor. Summarise them briefly and then order and explain the steps necessary to go from individual molecules to the first cell: appearance of hereditary material capable of copying itself, formation of complex organic molecules, appearance of metabolism and formation of membranes.

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Timeline of early life

Timeline with the major milestones in the history of life on Earth, from the origin of the first prokaryotic cells to the diversification of complex life. 3800 Mafirst cells 2400 MaGreat Oxidation 1500 Macells with a nucleus 540 Macomplex life
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An exploration rover on Mars photographs a sedimentary rock with finely layered and domed structures, visually identical to terrestrial stromatolites from $3\,500$…

An exploration rover on Mars photographs a sedimentary rock with finely layered and domed structures, visually identical to terrestrial stromatolites from $3\,500$ million years ago.

  1. a) Justify why the presence of superimposed layers alone is not enough to confirm the existence of past life on Mars and what geochemical or isotopic analysis (for example, the ratio between $^{12}\text{C}$ and $^{13}\text{C}$) should be carried out to provide evidence for a biological origin rather than a purely inorganic process.
  2. b) Explain the biological and environmental significance that stromatolite-forming cyanobacteria had in altering the atmosphere and the precipitation of iron in the oceans of early Earth.
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About $2\,400$ million years ago, the activity of cyanobacteria triggered the "Great Oxidation Event". Although today we consider oxygen an essential gas, for the…

About $2\,400$ million years ago, the activity of cyanobacteria triggered the "Great Oxidation Event". Although today we consider oxygen an essential gas, for the biosphere of that time it was a catastrophic event.

  1. a) Justify why free oxygen ($O_2$) was lethal to the dominant microorganisms of that era and what key adaptive advantage was gained by organisms that developed aerobic cellular respiration.
  2. b) Explain the mechanism by which the increase in $O_2$ reacted with atmospheric methane ($CH_4$) and triggered an almost total global glaciation (Huronian glaciation).
  3. c) Deduce how the subsequent formation of the ozone layer ($O_3$) from this oxygen was a determining factor for the later colonisation of the continental surface by living organisms.
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Astrobiology: the search for life beyond the Earth

Looking at the night sky and wondering whether we are alone has stopped being just a philosophical question: space telescopes are discovering thousands of exoplanets and probes are analysing water geysers on the moons of Jupiter and Saturn; how can science determine whether life exists, or has ever existed, on any of those distant worlds?

A space telescope collects the light from a star that passes through the atmosphere of an exoplanet; in the spectrum, absorption dips of oxygen and methane appear, which together are a biomarker. star filtered light exoplanet atmosphere space telescope spectrum of its atmosphere light received O₂ CH₄ visible light infrared wavelength → Each dip is light absorbed by a gas in the atmosphere. O₂ and CH₄ together: a biomarker, hard to explain without life.
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What is astrobiology? Explain what it studies and why searching for life outside Earth helps us understand the origin of life on our planet.

What is astrobiology? Explain what it studies and why searching for life outside Earth helps us understand the origin of life on our planet.

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Why is the search for life on other worlds so focused on finding liquid water? Explain which properties of water make it so important for living things.

Why is the search for life on other worlds so focused on finding liquid water? Explain which properties of water make it so important for living things.

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A space agency is planning a mission to detect potential metabolically active (non-fossil) microbial life forms in the Solar System and has the following data on three…

A space agency is planning a mission to detect potential metabolically active (non-fossil) microbial life forms in the Solar System and has the following data on three candidates:

  • Mars: Surface exposed to intense ultraviolet radiation and oxidizing perchlorates. Presence of seasonal methane (CH₄) peaks in the atmosphere and possible accumulations of liquid brines kilometers deep.

  • Europa: Global saline ocean beneath an ice sheet 15 to 25 km thick, in direct contact with a rocky seabed subjected to tidal forces from Jupiter's gravity.

  • Enceladus: Global subsurface ocean that expels continuous geysers into space through fractures at the south pole. Water vapor, salts, organic macromolecules, and dihydrogen gas (H₂) have been measured in these plumes.

Answer the following questions with reasoned arguments:

  1. a) Using terrestrial mid-ocean ridge ecosystems as an analogous model, justify why the co-detection of H₂ and water in the geysers of Enceladus is considered a key indirect piece of evidence for habitability by chemosynthetic microorganisms.
  2. b) Compare the biological and engineering difficulties of collecting viable samples on Europa versus Enceladus. Justify which of the two worlds offers a strategic advantage for a probe that can only perform orbital flybys without landing on the surface.
  3. c) If the rover exploring Mars were to detect amino acids in the surface regolith, explain why this finding would not conclusively confirm the existence of past or present life, and what chemical property (chirality) scientists should analyze to obtain strong, though not definitive, evidence of whether their origin is biological or purely abiotic.
Solve

Back to the beginning: The step from molten rock to the biosphere first required the planet to cool enough to hold liquid water, the prebiotic synthesis of organic monomers from inert matter, and their progressive self-assembly into vesicles with metabolism and hereditary material.

Summary

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