The sky has a special shield.
It stays high above us. This shield stops bad light from the sun. It helps keep us safe. We need it to live. Can you feel the sun's warmth?
The sky has a special shield.
This shield stays high above us. It catches bad light from the sun. This light can hurt living things.
The shield is made of a gas called ozone. Sunlight hits the air to make it. This gas blocks most of the bad light. It helps keep us safe from sunburn.
Some man-made things once hurt this shield. Now, people have stopped using them. This helps the shield stay strong.
The Earth has a special shield in the sky. This is the ozone layer. It sits in a part of the air called the stratosphere.
This layer is made of ozone. Ozone is a gas. It forms when sunlight hits oxygen. The light splits oxygen into small parts. These parts join together to make ozone.
This shield is very important. It blocks most of the Sun's ultraviolet light. We call this UV light. This light can hurt living things. It can cause skin cancer and sunburns.
In the past, people used certain chemicals. These were called CFCs. They came from big industries. These chemicals went into the sky. They broke down the ozone layer. This created thin spots called ozone holes.
People worked to fix this. Many countries banned those chemicals. Now, the ozone layer is healing. The loss of ozone has slowed or stopped. This helps keep life on Earth safe.
The ozone layer is a special part of Earth's atmosphere. It sits in a region called the stratosphere. This layer acts like a shield for our planet. It absorbs most of the Sun's medium-frequency ultraviolet radiation. Without this shield, life on the surface would face great danger.
This layer is made of a gas called ozone. Ozone is created through a special way it works called the ozone-oxygen cycle. First, ultraviolet light hits ordinary oxygen molecules. These molecules have two oxygen atoms. The light splits them into single atoms. These single atoms then join with other oxygen molecules to create ozone.
This cycle keeps the ozone layer working.
Scientists discovered this layer a long time ago. French physicists Charles Fabry and Henri Buisson found it in 1913. They noticed some radiation was missing from the Sun's light. They realized something in the air was absorbing it. Later, a British meteorologist named G. M. B. Dobson studied it more. He built a tool called a Dobsonmeter to measure ozone from the ground. He even set up a global network of stations. We still use his name today for the "Dobson unit."
This unit helps us measure how much ozone is overhead.
Protecting the ozone layer is a very big job. In 1985, researchers found the layer was being depleted. This means it was getting thinner. This happened because of chemicals from industry called chlorofluorocarbons, or CFCs. These chemicals caused "ozone holes" near the poles. These holes are just thin patches in the layer. These patches let more harmful UV-B radiation reach us. This radiation can cause sunburns and skin cancer.
Scientists found that ozone levels dropped by about 4 percent worldwide since the late 1970s.
People around the world took action to help. Many countries agreed to ban CFCs to protect the sky. Because of these rules, the ozone layer is now healing. Recent evidence shows that ozone depletion has slowed or stopped. This is a great success for the planet. To remember this, the United Nations named September 16 as the International Day for the Preservation of the Ozone Layer.
This day helps everyone learn how to keep our shield safe.
Understanding the ozone layer helps us see how everything is linked. The air moves in patterns called the Brewer-Dobson circulation. This moves ozone from the tropics toward the poles. This is why the layer is thicker in some places. Even the planet Venus has a thin ozone layer. This shows how interesting gas layers can be in space.
It is amazing how a tiny gas protects all living things.
The ozone layer is a vital region within Earth's stratosphere. It acts as a protective shield for our planet. This layer absorbs most of the Sun's medium-frequency ultraviolet radiation. Without this protection, life on the surface would face severe damage. The ozone layer contains a high concentration of ozone (O3) molecules. Even so, ozone is a small part of the stratosphere compared to other gases.
This shield works through a continuous process called the ozone-oxygen cycle. The cycle begins when ultraviolet light strikes ordinary oxygen molecules (O2). These molecules contain two oxygen atoms. The energy from the light splits them into single, individual oxygen atoms. These single atoms then combine with unbroken O2 molecules to create ozone (O3). This process is known as photolysis. When ultraviolet light hits an ozone molecule, it splits it back into O2 and a single atom. This constant cycle maintains the layer's presence in the stratosphere.
Ultraviolet radiation is divided into three distinct categories based on wavelength. These are UV-A, UV-B, and UV-C. UV-C is the most energetic and harmful type of radiation. It is entirely blocked by a combination of dioxygen and ozone. UV-B is the next category and is the main cause of sunburn. The ozone layer is very effective at screening out most UV-B radiation. However, some UV-B still reaches the surface. This small amount is actually important for mammals to produce vitamin D. Finally, UV-A is the longest wavelength and is hardly affected by ozone. Most UV-A reaches the ground, but it is significantly less harmful to DNA than UV-B.
Scientists first discovered the existence of the ozone layer in 1913. French physicists Charles Fabry and Henri Buisson noticed something strange. They found that radiation from the Sun was missing at certain wavelengths. They deduced that something in the atmosphere was absorbing that missing energy. They eventually matched the missing radiation to the chemical ozone. Later, British meteorologist G. M. B. Dobson studied its properties in great detail. He invented a tool called a Dobsonmeter to measure ozone from the ground. He established a global network of monitoring stations between 1928 and 1958. Today, we measure ozone using the "Dobson unit" (DU) in his honor.
The distribution of ozone is not the same everywhere on Earth. Most of the ozone, about 90 percent, is found in the stratosphere. The layer's thickness varies by season and by geography. Most ozone is produced over the tropics by solar radiation. It is then moved toward the poles by atmospheric wind patterns. This movement is called the Brewer-Dobson circulation. Because of this circulation, the ozone layer is often thickest in the spring. In the Northern Hemisphere, ozone levels are highest in April and May. In the Southern Hemisphere, the thinnest patches often appear over the Antarctic during summer.
In 1985, researchers discovered that the ozone layer was being depleted. This depletion was caused by man-made chemicals like chlorofluorocarbons (CFCs). These chemicals release chlorine and bromine radicals into the stratosphere. A single radical can trigger a chain reaction that breaks down 100,000 ozone molecules. This led to the famous "ozone holes" near the poles. These holes are actually areas where the ozone layer is much thinner. Scientists found that worldwide ozone levels dropped by about 4 percent since the late 1970s.
Global action has led to significant environmental recovery. Many countries implemented bans on CFCs to protect the atmosphere. The United Nations even designated September 16 as the International Day for the Preservation of the Ozone Layer. Recent evidence shows that ozone depletion has slowed or even stopped. This is a major success for international environmental regulation.
Understanding the ozone layer shows how human industry and atmospheric science are deeply connected. It reminds us how much we rely on the delicate balance of our atmosphere.
Where will your curiosity go next?
🖼️ Images & Media (8)
More to explore
✨ What else?
Related topics you might enjoy
🔬 Go deeper
More advanced topics to explore
What is Nepedia?
A free, ad-free encyclopedia for children. Every article is written at five reading levels, so the same page works for a five-year-old and a fifteen-year-old — use the level switcher above to see this one change. No account needed to read.