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NotesBiology HLTopic 1.1The search for extraterrestrial life and the presence of water
Back to Biology HL Topics
1.1.86 min read

The search for extraterrestrial life and the presence of water (Biology HL)

IB Biology · Unit 1

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Contents

  1. 1Looking for life means looking for water
  2. 2The Goldilocks zone
  3. 3Exam-style question (step by step)
The big idea: Every search for extraterrestrial life begins with one question: is there liquid water? Life as we know it cannot run without it.

The points to remember

  • Water is the medium for life: the reactions of life happen in water, and the first cells formed in water.
  • So the search for extraterrestrial life is a search for liquid water, present now or in the past.
  • Three places to look: Mars (dry rivers and lakes), icy moons with oceans under the ice, and planets around other stars.
Remember it as: Follow the water: no liquid water, no search.
Three panels: Mars with dark branching river channels and a lake floor; a cross-section of Europa with an ice crust over a blue ocean and a jet of vapour; a star with a planet on a dashed orbit and a telescope dishThree panels: Mars with dark branching river channels and a lake floor; a cross-section of Europa with an ice crust over a blue ocean and a jet of vapour; a star with a planet on a dashed orbit and a telescope dish
Three places we look for life. In every one, the first question is whether there is, or was, liquid water.

Real example: between 2008 and 2015 the Cassini spacecraft flew through jets of water vapour shooting out of Enceladus, a small icy moon of Saturn. It found salt and carbon-based molecules in the jets, which come from an ocean of liquid water under the ice. That ocean is why Enceladus is now a target in the search for life.

On Mars, the Curiosity rover drilled into mudstone in Gale crater in 2013 and showed that a lake of fresh water once filled it. Past water means life could once have lived there.

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The big idea: A planet can only keep liquid water if it is the right distance from its star. That band is the Goldilocks zone.

The points to remember

  • Water is liquid only between 0 °C and 100 °C (at a pressure like Earth's). Hotter, it boils away; colder, it freezes.
  • The Goldilocks zone is the band of distances from a star where a planet's temperature lets water stay liquid.
  • Too close to the star, water boils away (Venus). Too far, it is ice (the outer planets). Earth sits in the zone.
  • In a table of planets, pick the one whose temperature range allows liquid water, with air and gravity a living thing could stand.
Remember it as: Goldilocks: not too hot, not too cold, just right for liquid water.
A star at the left and three planets at increasing distance: a hot cracked planet labelled too hot, an Earth-like planet inside a green band labelled Goldilocks zone, and an icy planet labelled too coldA star at the left and three planets at increasing distance: a hot cracked planet labelled too hot, an Earth-like planet inside a green band labelled Goldilocks zone, and an icy planet labelled too cold
Not too hot, not too cold. Only in the green band can a planet keep liquid water at its surface.

Real example: TRAPPIST-1 is a small, cool star 40 light years away with seven Earth-sized planets found in 2017. The inner ones are too hot and the outer ones too cold, but three sit in the Goldilocks zone. TRAPPIST-1e, an exoplanet that receives about two thirds of the starlight Earth gets, could have liquid water if it has an atmosphere.

Handwritten diagram built in five steps: a star, a hot planet, a shaded Goldilocks band, a cold planet, and Earth inside the band
The Goldilocks zone, drawn one part at a time.

The exam gives you a table and asks which planet falls within the Goldilocks zone. Read the temperature column first:

Table of four planets around other stars with starlight received, estimated temperature and mass: HD 189733 b about 930 °C, TRAPPIST-1e -22 to 11 °C, Kepler-62f -65 to -32 °C, Kepler-186f -85 to -52 °CTable of four planets around other stars with starlight received, estimated temperature and mass: HD 189733 b about 930 °C, TRAPPIST-1e -22 to 11 °C, Kepler-62f -65 to -32 °C, Kepler-186f -85 to -52 °C
An exam-style table. TRAPPIST-1e is the only planet whose temperature range reaches above 0 °C, so it could hold liquid water.
Reading the table: Temperature decides it: the planet must be able to sit between 0 °C and 100 °C. An atmosphere marked unknown does not rule a planet out. A planet at 750 °C or -100 °C is out whatever else the table says; so is one with poisonous gases or a gravity many times Earth's.

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How this is tested: A one-mark multiple-choice item shows a table of planets and asks which one lies in the Goldilocks zone. A short written part can ask you to explain why a particular planet or moon is a target in the search for life.
IB-style questionExplain[3 marks]

TRAPPIST-1e orbits a small, cool star 40 light years from Earth. It receives about two thirds of the starlight that Earth receives, and estimates of its temperature range from -22 °C with no atmosphere to 11 °C with an atmosphere like Earth's. Explain why TRAPPIST-1e is a target in the search for extraterrestrial life.

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Astronomers describe Earth as lying in the Sun's Goldilocks zone.

what is meant by the Goldilocks zone.
[1 mark]

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1.1.1Water as the medium for life1.1.2Hydrogen bonds from the polar covalent bonds in water1.1.3Cohesion of water and its consequences for organisms1.1.4Adhesion of water to polar or charged materials
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