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Our Changing Planet

Francesca Harper Chemistry GCSE English

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Our Changing Planet

  1. Structure of the Earth

    • The Earth is almost spherical with a diameter of about 128000 km
    • At the surface is a thin, solid crust
    • Crust = a very thin layer that varies in thickness between about 5km and 70km
    • The mantle is under the crust and is about 3000km thick - Goes halfway to the centre of the earth
    • The mantle almost entirely solid but parts of it can flow very slowly
    • The core is about half the diameter of the earth
    • The core has a high proportion of magnetic metals, iron and nickel - It has a liquid outer part and a solid inner part
    • The atmosphere surrounds the earth
    • Most of the air within 10km of the surface and most of the atmosphere is within 100km of the surface
    • All of the raw materials and other resources that we depend on come from the crust, the oceans and the atmosphere
    • This means the resources available to us are limited
  2. The Restless Earth

    • Scientists now believe the Earth's crust and upper part of the mantle is cracked into massive pieces called tectonic plates
      • Tectonic Plates
    • Tectonic plates move a few centimetres a year because of convection currents in the mantle beneath them
    • The convection currents are caused by energy released by the decay of radioactive elements heating up the mantle
    • Where the plates meet, huge forces build up
    • Eventually, rocks changing shape or moving suddenly causing earthquakes, volcanoes or mountains to form
    • Scientists still do not know enough about what is happening inside the Earth to predict exactly when and where earthquakes or volcanic eruptions will happen
    • Alfred Wegener put forward the idea of 'Continental Drift' in 1915
      • Alfred Wegener - Continental Drift
    • Other scientists at the time did not accept his ideas, mainly because he could not explain why the continents moved
    • They believed the earth was shrinking as it cooled - In the 1960's scientists found new evidence and the theory of plate tectonics was developed
  3. The Earth's Atmosphere in the past

    • Scientists think that the Earth was formed about 4.5billion years ago
    • In the first billion years, the surface was covered in volcanoes that released Carbon Dioxide, water vapour and Nitrogen
    • As the earth cooled, most of the water vapour condensed to form the oceans
    • Some scientists believe there was also nitrogen, and possibly some methane and ammonia
    • In the next two billion years, bacteria, algae and plants evolved
    • Algae and plants used carbon dioxide for photosynthesis and this released oxygen into the atmosphere
    • As the number of plants increased, the amount of carbon dioxide in the atmosphere decrease and the amount of oxygen increased
  4. Life on Earth

    • The plants that produced the oxygen in the atmosphere probably evolved from simple organisms like plankton and algae in the ancient oceans
    • But we do not know how the molecules of the simplest living things were formed
    • Many scientists have suggested theories of how life began, but no one knows for sure because there is not sufficient evidence
    • In 1952 two scientists, Miller and Urey, did an experiment based on what scientists at that time thought was the early atmosphere
      • Miller & Urey
    • They used a mixture of water, ammonia, methane and hydrogen and a high voltage spark to simulate lightening
    • After a week, they found that amino acids (the building blocks for proteins) had ben produced
    • One other theory suggests that these organic molecules formed a 'primordial soup' and that the amino acids in this mixture combined to make proteins from which life began
  5. Gases in the Atmosphere

    • Plants took up much of the carbon dioxide in the Earth's early atmosphere
    • Animals ate the plants and much of the carbon dioxide ended up in plants and animal remains as sedimentary rocks and fossil fuels (the CO2 formed sedimentary rocks)
    • Limestone was formed from the shells and skeletons of marine organisms
    • Fossil fuels contain carbon and hydrogen from plants and animals
    • Carbon Dioxide dissolves in the oceans and some probably formed insoluble carbonate compounds that were deposited on the seabed and became sedimentary rock
    • By 200 million years ago, the proportions of gases in the atmosphere had stabilised and were much more the same as hey are today
    • The atmosphere is now almost four-fifths nitrogen and just over one-fifth oxygen
    • Other gases including carbon dioxide, water vapour and nobelium's gases make up about 1% of the atmosphere
    • Separating the gases in air
      • The gases in the air have different boiling points and so can be separated from liquid air by fractional distillation
      • Fractional distillation of liquid air is done industrially to produce pure oxygen and liquid nitrogen, which have important uses
      • The air is cooled below -200c and fed into a fractional distillation column
      • Nitrogen is separated from oxygen and argon, and further distillation is used to produce oxygen and argon
  6. Carbon Dioxide in the atmosphere

    • For about 200 million years the amount of Carbon Dioxide in the atmosphere has remained the same
    • This is evades various natural processes that move carbon dioxide into and out of the atmosphere had achieved a balance
    • These processes involve carbon compounds in plants, animals and the oceans an rocks
    • The organic carbon cycle shows some of these processes
    • Carbon dioxide dissolves in water, particularly the oceans, and reactions of inorganic carbonate compounds are also important in maintaining a balance
    • In the recent pasts, the amount of carbon dioxide that human activity has released into the atmosphere has increased dramatically
    • This has been mainly caused by the large increase in the amount of fossil fuels that we burn

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Description
GCSE Chemistry (C1) Mind Map on Our Changing Planet, created by Francesca Harper on 15/05/2017.
Created by
Francesca Harper · May 2017
Updated
Apr 6, 2018
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