Zusammenfassung der Ressource
Conditions for Life on Earth
- Early conditions on Earth
- The Earth was formed about 4.6 billion years
ago
- 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