The Sun sends light to us.
This light comes from far away. It gives us warmth. It helps plants grow food. We use it to see the world.
Can you feel the warm sun?
The Sun sends light to our world.
It takes about eight minutes to reach us. This light helps plants make food.
Some light is easy to see. Other light is invisible to our eyes. Some of this light feels like warmth.
This light can also cause a sunburn. The air around Earth filters the light. Sunlight is a very important part of life.
The Sun sends light to our world.
It takes about 8.3 minutes for this light to reach Earth. This light is a mix of different kinds of radiation. Radiation is a type of energy that travels through space.
Some parts of sunlight are easy to see. We call this visible light. Other parts are invisible to our eyes. One type is called infrared. Humans feel infrared as warmth. Another type is called ultraviolet, or UV. UV light can cause a sunburn. It also helps our bodies make vitamin D3.
Sunlight helps plants grow. Plants use a way called photosynthesis. In this way, they turn light into food.
When sunlight hits Earth, the air acts like a filter. This air scatters the light. If clouds block the Sun, the light is diffused. This means the light is spread out. Scientists use tools like a pyranometer to measure how much light hits the ground.
Sunlight is the energy sent from the Sun to our planet.
It is a special kind of radiation called solar radiation. This energy reaches Earth in many different forms. Some parts are visible light that we see with our eyes. Other parts are invisible, like infrared light which we feel as warmth. There is also ultraviolet light, which we call UV. UV light can cause sunburns, but it also helps humans make vitamin D3.
Light travels from the Sun to the Earth in a specific way. It takes about 8.3 minutes for sunlight to reach us. Inside the Sun, light starts at the very center. A tiny particle called a photon must travel to the surface. It can take 10,000 to 170,000 years to get there! This is because the photon hits many charged particles along the way. Once it leaves the Sun, it travels quickly through space. When it hits our atmosphere, the air filters and scatters the light.
Scientists have studied how this energy works for a long time. They use special tools to measure the intensity of the light. One tool is called a pyranometer. Another tool used by researchers is a pyrheliometer. They also use a sunshine recorder to track the light. These tools help us understand how much energy hits a certain area. This measurement is called solar irradiance. Knowing these numbers helps us understand how the Earth stays warm.
There are many interesting facts about the power of sunlight. At the top of our atmosphere, sunlight is very strong. It is about 30% more intense there than at the ground. At the surface, sunlight is made of different parts. About 52 to 55 percent of the energy is infrared light. About 42 to 43 percent is visible light. The last 3 to 5 percent is ultraviolet light.
The amount of light changes depending on the time of year. In January, the energy is about 3.3% higher than average. In July, it is about 3.3% lower.
Sunlight connects to almost everything in our daily lives. It is the main power source for photosynthesis. This is how plants turn light into food to grow.
Sunlight also provides natural lighting for the inside of buildings. This is called daylighting. Using natural light can be better than using artificial lights. For example, sunlight is more efficient than many types of indoor bulbs. It helps light up our world in a beautiful way every day.
Sunlight is the electromagnetic radiation emitted by the Sun. This energy is often called solar radiation. It is a fundamental force that powers life on Earth. When we talk about sunlight, we usually mean the visible light our eyes see. However, it also includes invisible parts of the spectrum. These include infrared light, which we feel as warmth, and ultraviolet light, which can affect our bodies.
The journey of sunlight begins deep inside the Sun. A particle of light, called a photon, starts at the solar core. Because the core is so dense, the photon constantly hits charged particles. These collisions change the photon's direction many times. This process can take between 10,000 and 170,000 years just to reach the Sun's surface. Once it escapes the surface, the photon travels through space. It takes about 8.3 minutes for that light to reach Earth.
When sunlight hits Earth, it interacts with our atmosphere. The atmosphere scatters and filters the radiation. We call the resulting light daylight when the Sun is above the horizon. If clouds do not block the radiation, we experience it as sunshine. This is a mix of bright light and radiant heat. If clouds do block the light, or if it reflects off objects, the light becomes diffused. Scientists measure the rate of solar energy hitting a specific area as solar irradiance.
Sunlight is composed of different regions based on wavelength. Nearly 98.7% of the radiation striking our atmosphere falls between 200 nm and 4,000 nm. This range includes ultraviolet, visible, and infrared light. Ultraviolet radiation is divided into three types. Ultraviolet C (UVC) has the shortest wavelengths and is mostly absorbed by our atmosphere. Ultraviolet B (UVB) also causes significant absorption and can damage DNA or cause sunburn. Ultraviolet A (UVA) reaches the surface and can cause skin aging or cancer.
The visible and infrared ranges make up the rest of the energy. Visible light spans from 380 to 700 nm and is what we see. Infrared radiation spans from 700 nm to 1,000,000 nm. At the Earth's surface, the energy breakdown is quite specific. About 52 to 55 percent is infrared light. About 42 to 43 percent is visible light. Finally, about 3 to 5 percent is ultraviolet light.
Measuring sunlight requires precise tools and complex math. Researchers use instruments like pyranometers and pyrheliometers. They also use sunshine recorders to track light intensity. To calculate the light reaching the ground, scientists must consider the Earth's elliptic orbit. The Earth's distance from the Sun changes throughout the year. In January, the energy is about 3.3% higher than the average. In July, the energy is about 3.3% lower than the average.
Sunlight plays a vital role in biological and human systems. It is the primary driver of photosynthesis. This is how autotrophic organisms, like plants, convert light into chemical energy. This energy is used to create carbohydrates and fuel their activities.
Sunlight also provides natural lighting for buildings, a process called daylighting. Sunlight is very efficient for illumination. It has a luminous efficacy of about 93 lumens per watt. This is higher than most artificial lights, such as fluorescent or incandescent bulbs. Using sunlight helps light a room while heating it less than many lamps.
Where will your curiosity go next?
🖼️ Images & Media (13)
+ 1 more
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.