The Earth's atmosphere is dynamic and forever changing
The causes of these changes are sometimes man-made and sometimes part of many natural cycles
Scientists use very complex software to predict weather and climate change as there are many variables that can influence this
The problems caused by increased levels of air pollutants require scientists and engineers to develop solutions that help to reduce the impact of human activity
Composition of Earth's Atmosphere
Nitrogen (about 80%)
Oxygen (about 20%)
Small proportions of various other gases, including carbon dioxide, water vapour and noble gases
Earth's Atmospheric Layers
Troposphere
Stratosphere
Mesosphere
Thermosphere
Ionosphere
Exosphere
Troposphere
Starts at the Earth's surface and extends 8 to 14.5 kilometers high (5 to 9 miles)
Most dense part of the atmosphere
Almost all weather is in this region
Stratosphere
Starts just above the troposphere and extends to 50 kilometers (31 miles) high
Ozone layer, which absorbs and scatters the solar ultraviolet radiation, is in this layer
Mesosphere
Starts just above the stratosphere and extends to 85 kilometers (53 miles) high
Meteors burn up in this layer
Thermosphere
Starts just above the mesosphere and extends to 600 kilometers (372 miles) high
Aurora and satellites occur in this layer
Ionosphere
Abundant layer of electrons and ionized atoms and molecules that stretches from about 48 kilometers (30 miles) above the surface to the edge of space at about 965 km (600 mi)
Overlaps into the mesosphere and thermosphere
Dynamic region that grows and shrinks based on solar conditions
Divides further into the sub-regions: D, E and F; based on what wavelength of solar radiation is absorbed
Critical link in the chain of Sun-Earth interactions
Makes radio communications possible
Exosphere
Upper limit of our atmosphere
Extends from the top of the thermosphere up to 10,000 km (6,200 mi)
Ozone layer
One layer of the stratosphere, the second layer of the Earth's atmosphere
The stratosphere is the mass of protective gases clinging to our planet
Ozone
Only a trace gas in the atmosphere—only about 3 molecules for every 10 million molecules of air
Absorbs bits of radiation hitting Earth from the sun
Acts as a shield for life on Earth
UVB
Causes skin conditions like sunburns, and cancers like basal cell carcinoma and squamous cell carcinoma
UVA
More harmful than UVB, penetrating more deeply and causing a deadly skin cancer, melanoma, and premature aging
The ozone layer absorbs about 98 percent of this devastating UV light
Chlorofluorocarbons (CFCs)
Molecules that contain the elements carbon, chlorine, and fluorine
Inexpensive, don't catch fire easily, and don't usually poison living things
But start eating away at the ozone layer once they get blown into the stratosphere
Ozone molecules are always being destroyed and reformed naturally, but CFCs in the air make it very difficult for ozone to reform once it's broken apart
The ozone layer, which only makes up 0.00006 percent of Earth's atmosphere, is getting thinner and thinner all the time
Ozone holes are inaccurate names for areas of damage to the ozone layer, as the ozone layer damage is more like a really thin patch than a hole
The ozone layer is thinnest near the poles
In the 1970s, people all over the world started realizing that the ozone layer was getting thinner and that this was a bad thing
Many governments and businesses agreed that some chemicals, like aerosol cans, should be outlawed, and there are fewer aerosol cans produced today
The ozone layer has slowly recovered as people, businesses, and governments work to control such pollution
Greenhouse effect
A natural process that warms the Earth's surface
When the Sun's energy reaches the Earth's atmosphere, some of it is reflected back to space and the rest is absorbed and re-radiated by greenhouse gases
Greenhouse gases
Water vapour
Carbon dioxide
Methane
Nitrous oxide
Ozone
Some artificial chemicals such as chlorofluorocarbons (CFCs)
The absorbed energy warms the atmosphere and the surface of the Earth, maintaining the Earth's temperature at around 33 degrees Celsius
Greenhouse Effect
A natural process that warms the Earth's surface when the Sun's energy reaches the Earth's atmosphere, some of it is reflected back to space and the rest is absorbed and re-radiated by greenhouse gases
Greenhouse gases
Water vapour
Carbon dioxide
Methane
Nitrous oxide
Ozone
Chlorofluorocarbons (CFCs)
The absorbed energy warms the atmosphere and the surface of the Earth, maintaining the Earth's temperature at around 33 degrees Celsius warmer than it would otherwise be, allowing life on Earth to exist
Enhanced greenhouse effect
Human activities – particularly burning fossil fuels (coal, oil and natural gas), agriculture and land clearing – are increasing the concentrations of greenhouse gases, contributing to warming of the Earth
Global Warming
The globe is heating up, with both land and oceans warmer now than they were when record keeping began, in 1880, and temperatures still ticking upward
The burning of fossil fuels has released greenhouse gases into the atmosphere, which trap warmth from the sun and drive up surface and air temperatures
Scientists agree that the earth's rising temperatures are fueling longer and hotter heat waves, more frequent droughts, heavier rainfall, and more powerful hurricanes
The earth's ocean temperatures are getting warmer, which means that tropical storms can pick up more energy, turning a category 3 storm into a more dangerous category 4 storm
Antarctica has been losing about 134 billion metric tons of ice per year since 2002, and this rate could speed up if we keep burning fossil fuels at our current pace, causing sea levels to rise several meters over the next 50 to 150 years
Climate Change
The defining issue of our time, with impacts that are global in scope and unprecedented in scale, requiring drastic action today to adapt to in the future
The Intergovernmental Panel on Climate Change (IPCC) is categorical in its conclusion: climate change is real and human activities are the main cause
United Nations Framework Convention on Climate Change (UNFCCC)
A first step in addressing the climate change problem, with near-universal membership of 197 countries, aimed at preventing "dangerous" human interference with the climate system