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Unit 6: The Atmosphere
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Atmosphere Composition
Different today than long time ago! How? 2 main gases make up 99% of the atmosphere Nitrogen—78% Oxygen 21% Other gases in atmosphere Carbon Dioxide—small amount/important Water Vapor—amount varies also important
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Atmosphere Structure Pressure decreases as you rise in the atmosphere
Air molecules rapidly thin!
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Heat Transfer Radiation Conduction Convection
Heat that travels through empty space Conduction Heat transferred through contact Convection Heat transfer through fluids (air and water Heat is less dense and rises, cold is more dense and sinks
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Heat Transfer 50% is absorbed by earth
20% is absorbed by clouds and atmosphere 30% is reflected back to space
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Atmosphere Structure 4 layers determined by temperature gradients
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Troposphere Closest layer to the Earth Where all weather occurs
Air close to ground is heated by conduction causing temperature to decrease with altitude
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Stratosphere Ozone causes temperature to increase with altitude
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Temperatures decrease with altitude as you move away from ozone
Meteors burn up from friction with our atmosphere Mesosphere
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Thermosphere Outermost layer
Temperatures increase with altitude due to UV radiation from the sun Auroras found here
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Ozone Ozone is a molecule consisting of 3 oxygen atoms
Ozone in the stratosphere is necessary for life on Earth Ozone in the troposphere is a pollutant (smog!) Ozone
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Stratospheric Ozone Ozone can be created or destroyed by the Sun’s UV rays
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Stratospheric Ozone CFCs (chlorofluorocarbons) and other ozone depleting compounds breakdown and prevent new ozone from forming
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Thinning of the ozone layer has caused a “hole” to form
Stratospheric Ozone
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Stratospheric Ozone Good News! The Montreal Protocol (1987)
An international agreement to reduce ozone depleting compounds like CFCs The ozone layer should recover by 2050
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