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A guide to the energy of the Earth - Joshua M. Sneideman

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    Energy is all around us,
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    a physical quantity that follows
    precise natural laws.
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    Our universe has a finite amount of it;
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    it's neither created nor destroyed
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    but can take different forms,
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    such as kinetic or potential energy,
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    with different properties
    and formulas to remember.
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    For instance,
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    an LED desk lamp's 6 Watt bulb
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    transfers 6 Joules
    of light energy per second.
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    But let's jump back up into space
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    to look at our planet,
    its systems, and their energy flow.
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    Earth's physical systems include
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    the atmosphere, hydrosphere,
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    lithosphere, and biosphere.
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    Energy moves in and out of these systems,
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    and during any energy
    transfer between them,
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    some is lost to the surroundings,
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    as heat, light, sound,
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    vibration, or movement.
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    Our planet's energy comes from
    internal and external sources.
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    Geothermal energy
    from radioactive isotopes
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    and rotational energy
    from the spinning of the Earth
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    are internal sources of energy,
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    while the Sun
    is the major external source,
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    driving certain systems,
    like our weather and climate.
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    Sunlight warms the surface and atmosphere
    in varying amounts,
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    and this causes convection,
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    producing winds
    and influencing ocean currents.
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    Infrared radiation, radiating out
    from the warmed surface of the Earth,
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    gets trapped by greenhouse gases
    and further affects the energy flow.
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    The Sun is also the major source
    of energy for organisms.
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    Plants, algae, and cyanobacteria
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    use sunlight to produce organic matter
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    from carbon dioxide and water,
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    powering the biosphere's food chains.
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    We release this food energy
    using chemical reactions,
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    like combustion and respiration.
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    At each level in a food chain,
    some energy is stored
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    in newly made chemical structures,
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    but most is lost to the surroundings,
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    as heat, like your body heat,
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    released by your digestion of food.
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    Now, as plants are eaten
    by primary consumers,
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    only about 10% of their total energy
    is passed on to the next level.
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    Since energy can only flow
    in one direction in a food chain,
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    from producers on to consumers
    and decomposers,
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    an organism that eats lower
    on the food chain,
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    is more efficient than one higher up.
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    So eating producers
    is the most efficient level
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    at which an animal can get its energy,
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    but without continual input of energy
    to those producers,
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    mostly from sunlight,
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    life on Earth as we know it
    would cease to exist.
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    We humans, of course, spend our energy
    doing a lot of things besides eating.
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    We travel, we build, we power
    all sorts of technology.
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    To do all this,
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    we use sources like fossil fuels:
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    coal, oil, and natural gas,
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    which contain energy
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    that plants captured
    from sunlight long ago
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    and stored in the form of carbon.
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    When we burn fossil fuels in power plants,
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    we release this stored energy
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    to generate electricity.
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    To generate electricity,
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    heat from burning fossil fuels
    is used to power turbines
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    that rotate magnets,
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    which, in turn, create
    magnetic field changes
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    relative to a coil of wire,
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    causing electrons to be
    induced to flow in the wire.
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    Modern civilization depends on our ability
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    to keep powering that flow of electrons.
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    Fortunately, we aren't limited
    to burning non-renewable fossil fuels
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    to generate electricity.
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    Electrons can also be induced to flow
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    by direct interaction
    with light particles,
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    which is how a solar cell operates.
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    Other renewable energy sources,
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    such as wind, water,
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    geothermal, and biofuels
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    can also be used to generate electricity.
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    Global demand for energy is increasing,
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    but the planet
    has limited energy resources
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    to access through a complex
    energy infrastructure.
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    As populations rise,
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    alongside rates of industrialization
    and development,
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    our energy decisions grow
    more and more important.
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    Access to energy
    impacts health, education,
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    political power, and socioeconomic status.
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    If we improve our energy efficiency,
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    we can use our natural resources
    more responsibly
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    and improve quality of life for everyone.
Title:
A guide to the energy of the Earth - Joshua M. Sneideman
Description:

View full lesson: http://ed.ted.com/lessons/a-guide-to-the-energy-of-the-earth-joshua-m-sneideman

Energy is neither created nor destroyed — and yet the global demand for it continues to increase. But where does energy come from, and where does it go? Joshua M. Sneideman examines the many ways in which energy cycles through our planet, from the sun to our food chain to electricity and beyond.

Lesson by Joshua M. Sneideman, animation by Marc Christoforidis.

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Video Language:
English
Team:
closed TED
Project:
TED-Ed
Duration:
04:44

English subtitles

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