A mind map that summarises the 'Conditions for Life on Earth' chapter for the AQA Environmental Science A-Level. Created using the textbook for reference, so should be accurate for the course
The physical features of Earth made it suitable for the
eventual development of life by controlling the abiotic
factors needed by living organisms
Features of Earth that created
suitable conditions for life
Mass
The mass of the earth was great enough to
prevent most gases from escaping into space
This allowed for the creation of an
atmosphere
The atmospheric pressure was high enough to
prevent all liquid oxygen from boiling
Distance from the Sun
The light emitted from the sun and the
distance from the sun created suitable
temperatures on Earth
The time taken for the Earth to rotate
created a day/night cycle
This prevented
extreme heating or
cooling of the planet
Axis or Rotation
Axis of rotation is at an angle to the Earths
orbit, this creates seasons
Speed of Rotation
The 24 hour rotation prevents
temperature extremes
Magnetic Field
The Earths magnetic field deflects the 'solar winds',
which prevents biologically damaging radiation
reaching the Earths surface
Life first developed on Earth
about 3.5 billion years ago
The atmosphere contained
some toxic gases like ammonia
There was no
oxygen
Solar energy reaching the ground contained
high levels of ultra-violet radiation
The chemical composition of
the sea included increasingly
complex organic molecules
Single celled life eventually
formed, likely around geothermal
vents on the seabed
These are archaea, they are similar
to bacteria, some are anaerobic
and are still around today
Conditions on Earth the allowed life to develop
Presence of liquid water
All living things require
water for survival
It performs essential
physiological functions
and controls many
environmental conditions
Solvent Water
The 'general physiological solvent'. Most
chemical reactions in living organisms involve
reactants that are dissolved in water
Transport within organisms
Water is the solvent in blood and sap, where it
transports dissolved gases, sugars, amino acids,
mineral nutrients, waste products, etc.
Temperature Control
The evaporation of water absorbs
heat, reducing temperatures
Anomalous expansion on freezing
Water is most dense at 4°C, so water cooler
than that floats. This stops convection
currents from cooling the whole body of water
High specific heat capacity
Water warm and cools slowly, this helps moderate
the rate and size of temperature change
Aquatic Habitats
Oceans, seas, lakes, marshes and rivers
Absorption of UV
radiation
This protected living organisms
before the ozone layer developed and
absorbed the UV in the stratosphere
Temperature Range
Most areas of Earth have temperatures
between 0°C and 35°C
Most areas are warm enough to
have liquid water, but not hot
enough to denature proteins
Atmospheric Gases
Carbon dioxide for photosynthesis
and the synthesis of
carbohydrates , proteins and lipids
Nitrogen for protein synthesis
Solar Isolation
Sunlight provides the
energy for photosynthesis
The heat produced by the absorption of sunlight
provides the energy that drives the water cycle, and
warms the Earths surface and oceans
How life on Earth caused environmental change
Atmospheric
Oxygen
By 2.7 billion years ago, some Archaea had
developed the ability to photosynthesise
and release oxygen
For millions of years all oxygen produced reacted
with iron in the oceans
Once all the iron had reacted with oxygen, the surplus
dissolved oxygen built up in the oceans, much was
released into the atmosphere where concentrations
started to rise about 2.45 billion years ago
Oxygen in the atmosphere
absorbed UV light
This created a dynamic equilibrium of
reactions involving O3, O2, and O
The time period of oxygen
building up in the atmosphere
lasted about 540m years
The time period was called Proterozoic
Carbon Sequestration
Carbon dioxide is a greenhouse
gas and helps retain heat energy
Photosynthetic organisms absorb carbon dioxide,
some of which is stored in geological sediements
E.g. Carbonate rocks and fossil fuels
The reduction in atmospheric
Co2 helps prevent long-term
temperature rise
The suns brightness increases by
about 10% every billion years
Biogeochemical Cycles
As a greater variety of organisms evolved,
inter-connect biological processes developed,which
produced biogeochemical cycles
This meant that relatively small amounts of some nutrients
could support life for a long time without becoming depleted
Transpiration
Once plants had evolved and colonised land,
transpiration returned water vapour to the atmosphere
This caused rainfall in other areas,allowing for the growth of more plant life