📊 Atmospheric Composition
- Nitrogen (N2): 78%
- Oxygen (O2): 21%
- Argon (Ar): 0.9%
- Carbon dioxide (CO2): 0.04%
- Water vapour: Variable (0-4%)
- Trace gases: Methane, ozone, etc.
Database results: examBoard: Cambridge examType: IGCSE lessonTitle: Atmosphere Structure: Layers
The atmosphere is the layer of gases surrounding our planet, held in place by Earth's gravity. It's like a protective blanket that shields us from harmful radiation, regulates temperature and provides the air we breathe. Without it, life as we know it would be impossible!
Key Definitions:
The atmosphere extends about 10,000 km above Earth's surface, but 75% of its mass is contained within the lowest 11 km! That's because gravity pulls the densest air closest to Earth's surface.
Our atmosphere is made up of a mixture of gases, with nitrogen and oxygen being the most abundant:
This specific mixture of gases is vital for life. Oxygen allows us to breathe, nitrogen is essential for plant growth and carbon dioxide helps trap heat to keep Earth warm. Even the trace gases play crucial roles in our climate system.
Scientists divide the atmosphere into four main layers based on temperature changes, composition and properties. Each layer has unique characteristics and plays different roles in protecting our planet.
The troposphere is the lowest layer of the atmosphere and the one we live in. It extends from Earth's surface up to about 8-15 km, depending on location (thicker at the equator, thinner at the poles).
The troposphere is where we live and breathe! It contains most of the water vapour and clouds in the atmosphere. This layer is vital for the water cycle and weather patterns. It's also where most air pollution occurs and where greenhouse gases trap heat, contributing to global warming.
The stratosphere is the second layer of the atmosphere, extending from the tropopause (8-15 km) up to about 50 km above Earth's surface.
The ozone layer is a region in the stratosphere with a high concentration of ozone (O3). This layer absorbs most of the Sun's harmful ultraviolet (UV) radiation, protecting life on Earth from skin cancer, eye damage and harm to plants and ecosystems.
Human-made chemicals called chlorofluorocarbons (CFCs) have damaged the ozone layer, creating the "ozone hole" - particularly over Antarctica.
In 1987, countries around the world signed the Montreal Protocol to phase out ozone-depleting substances like CFCs. This international agreement is one of the most successful environmental treaties ever. Since its implementation, the ozone layer has slowly begun to recover, demonstrating how global cooperation can solve environmental problems. Scientists predict the ozone layer could fully recover by 2050-2070.
The mesosphere extends from the stratopause (about 50 km) to approximately 85 km above Earth's surface.
The mesosphere is where most meteors burn up, creating the "shooting stars" we see. It's also home to strange electrical phenomena like "sprites" and "elves" - brief flashes of light above thunderstorms.
Another fascinating feature is noctilucent clouds - the highest clouds in Earth's atmosphere. These silvery-blue clouds can only be seen at twilight during summer months in polar regions.
The thermosphere is the fourth major layer, extending from the mesopause (about 85 km) to between 500-1,000 km above Earth's surface.
The ionosphere is a region where solar radiation ionizes gas molecules, creating electrically charged particles. This layer reflects radio waves, making long-distance radio communication possible.
The International Space Station (ISS) orbits in the lower thermosphere, at about 400 km above Earth's surface. The aurora borealis (Northern Lights) and aurora australis (Southern Lights) also occur in this layer when charged particles from the Sun interact with Earth's magnetic field.
One of the most interesting aspects of the atmosphere is how temperature changes with altitude. Unlike what you might expect, it doesn't simply get colder as you go higher!
Temperature decreases with height (about 6.5°C per km). This happens because the Sun heats the Earth's surface, which then warms the air above it.
Temperature increases with height due to ozone absorbing UV radiation. This creates a temperature inversion that prevents weather systems from the troposphere extending upward.
Temperature decreases with height again, reaching the coldest temperatures in the entire atmosphere at the mesopause (about -90°C).
Temperature increases dramatically with height as oxygen and nitrogen molecules absorb high-energy solar radiation. Despite temperatures reaching 2,000°C, it wouldn't feel hot to a human because the air is so thin that very few molecules would transfer heat to your skin.
These temperature variations create stability in some layers and instability in others, affecting how pollutants move through the atmosphere. The temperature inversions in the stratosphere trap pollutants in the troposphere, preventing them from escaping higher into the atmosphere.
Human activities affect different layers of the atmosphere in various ways:
While we've studied each atmospheric layer separately, it's important to understand that they function as an interconnected system. Changes in one layer can affect others. For example, increasing greenhouse gases in the troposphere leads to warming at the surface but cooling in the stratosphere. This interconnectedness means we need to consider the atmosphere as a whole when studying environmental issues like climate change and ozone depletion.
The Earth's atmosphere is divided into four main layers - the troposphere, stratosphere, mesosphere and thermosphere - each with distinct characteristics and functions. These layers protect us from harmful radiation, regulate temperature, enable weather patterns and support life on Earth. Understanding the structure and properties of these atmospheric layers helps us comprehend environmental challenges like climate change and ozone depletion and develop effective solutions to protect our planet.
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