Energy from the Sun

Solar radiation, or energy produced by the Sun, is the primary energy source for most processes in the Earth system and drives Earth’s energy budget.

schematic showing incoming radiation and how it is absorbed and scattered by Earth's atmosphere and surface

The Sun is the primary energy source for our planet’s energy budget and contributes to processes throughout Earth.

UCAR/The COMET Program

Energy from the Sun is studied as part of heliophysics, which relates to the Sun’s physics and the Sun’s connection with the solar system.

How Does the Sun Make Energy?

cutaway view of the Sun showing the core and the outer convective zone where thermal energy is transferred to the Sun's surface

The Sun’s energy is generated in its core and moves outward to its surface where it is released as electromagnetic radiation.


The Sun’s energy is generated by nuclear fusion occurring in its core. Here, protons of hydrogen atoms violently collide and fuse to create a helium atom. The nuclear fusion process produces energy in the form of gamma rays, which are transformed into thermal energy, warming up the Sun’s core to around 15 million degrees Celsius. Through a process that takes tens of thousands of years, thermal energy moves from the Sun’s core to its outer layers. Once the thermal energy reaches the Sun’s surface, it is released into space in the form of electromagnetic radiation.

How Does Energy from the Sun Reach Earth?

It takes solar energy an average of 8 ⅓ minutes to reach Earth from the Sun. This energy travels about 93 million miles (149 million km) through space to reach the top of Earth’s atmosphere. Waves of solar energy radiate, or spread out, from the Sun and travel at the speed of light through the vacuum of space as electromagnetic radiation. The majority of the Sun’s radiation reaching Earth is in the form of visible light we can see and invisible infrared energy that we can’t see. A smaller portion of sunlight is made up of ultraviolet radiation, which is also invisible to our eyes.

schematic showing the time it takes solar radiation, including visible light and infrared radiation, to travel to Earth

Most of the Sun’s energy reaching Earth includes visible light and infrared radiation but some is in the form of plasma and solar wind particles. 


Other forms of radiation from the Sun can reach Earth as part of the solar wind, but in smaller quantities and with longer travel times. The solar wind contains plasma and particles and can also include gamma rays and x-rays resulting from solar storms or other bursts of energy from the Sun’s surface.

The Energy We Receive Depends on Distance From the Sun

The Sun’s energy we receive is electromagnetic radiation that travels through space or a medium in the form of waves or particles. The visible light we see from the Sun is similar to the visible light from a light bulb, but the Sun provides much more of it. The energy released from the Sun is equivalent to about 36 octillion (3.6 x 1028) lumens, where a lumen is a measure of the total amount of visible light. In contrast, a light bulb produces about 650-1600 lumens of visible light.

image of the Sun taken from space, with Earth's horizon in the foreground

The Sun is 93 million miles from Earth, yet it still provides us with all of the energy needed to sustain life.


The brightness (or intensity) of light reaching a surface depends on the distance from the source. From the surface of Mercury, the Sun would appear more than three times as large and as much as seven times brighter as it does when viewed from Earth.

The Sun’s Energy is Important to Life on Earth

Energy from the Sun makes it possible for life to exist on Earth. It is responsible for photosynthesis in plants, vision in animals, and many other natural processes, such as the movements of air and water that create weather. Most plants need at least some sunlight to grow, so without light, there would be no plants, and without plants, there would not be oxygen for us to breathe. Infrared radiation from the Sun is responsible for heating the Earth’s atmosphere and surface. Without energy from the Sun, Earth would freeze. There would be no winds, ocean currents, or clouds to transport water.

photo of the sun rising over grain fields

Energy from the Sun enables photosynthesis in plants, which provides the oxygen we breathe and helps grow the food we eat.

Creative Commons Stephen Bowler

How do Humans Benefit from the Sun's Energy?

Throughout history, humans have used technology to harness the Sun’s energy as a source of light and heat and for growing crops. As early as 30 CE, people were constructing greenhouses to grow plants out of season. Did you know that one of the earliest greenhouses was built for the Roman emperor Tiberius using translucent sheets of mica, all so that he could eat cucumbers in any season?

Early civilizations knew that setting up shelters to capture or block sunlight could help with heating and cooling. In cold climates, they would position buildings to face southward, allowing interior spaces to gather heat and light. In warm climates, shelters might be constructed under cliffs or natural overhangs to protect the residents from the Sun’s radiation in the hottest part of the day. Using energy from the Sun effectively also helped with growing crops.

photo of cliff dwelling situated under a rock overhang at Mesa Verde National Park

The cliff dwellings at Mesa Verde National Park in Colorado, USA, were built in the shadows of rock overhangs to help keep the structures cool in the hot desert sunlight.

Creative Commons Steven Zucker

Today, we can intentionally position windows and skylights to help heat or cool our homes through passive solar design. Solar panels can also capture energy from the Sun by gathering sunlight and converting it to electricity. As of 2023, solar power is the third largest source of renewable energy worldwide, behind hydropower and wind.

How is Energy from the Sun Harmful?

photo of a parent applying sunscreen to protect a child's skin from ultraviolet radiation

UV radiation can damage skin and cause sunburn, but simple actions such as wearing a hat and sunscreen provide essential protection from the Sun’s harmful UV rays. 


Some of the Sun’s energy reaches Earth in the form ultraviolet (or UV) radiation. Fortunately, the ozone layer high in Earth’s atmosphere absorbs a lot of this UV radiation and blocks it from reaching Earth’s surface. But some UV still makes it through. UV radiation from the Sun causes sunburn and skin damage but can be blocked with clothes and sunscreen. Wearing hats and sunglasses in bright sunlight and trying to stay in the shade when possible can also help protect you from harmful UV rays. Note that it’s not realistic or advisable to avoid all exposure to sunlight, as sunlight also helps our bodies produce vitamin D, which we need to be healthy.

UV radiation can damage plants and limit photosynthesis. Scientists have found that overexposure to UV radiation reduces size, productivity, and quality in several crop species, including many varieties of rice, soybeans, winter wheat, cotton, and corn. Sometimes, UV can cause bleaching of plants, visible as damage or discoloration. Planting tender young plants in the shadow of larger plants can help protect them from UV radiation.