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By Sciffer S.

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This is where thermonuclear reactions convert about 700 billion tons of hydrogen into helium every second. These reactions release an incredible amount of energy. Through a very complex process, this energy eventually reaches the surface of the Sun and from there radiates throughout the entire solar system. Processes in each of the On Earth we experience this energy three layers, or zones, of the Sun work together to convert as warmth and light, or sunshine. the thermonuclear reactions into heat and light.

Auroras are an even more stunning example of the Sun’s interaction with Earth. These shimmering curtains of light occur in both hemispheres. In the north, they are called the aurora borealis, or the northern lights. In the south, they are called the aurora australis, or the southern lights. Charged particles cause oxygen and nitrogen gases to glow. FFrom space, auroras look like Scientists concluded that some glowing rings of light that surround Earth’s poles. high-speed collisions between 48 The northern lights are colorfully displayed in the sky above this home in Alaska.

Nebula—An immense cloud of dust and gas molecules in outer space. photosphere—The surface of the Sun visible from Earth. radiation—The release of energy in the form of light waves. 59 The Sun red giant—A super-enlarged star that has burned up most of its hydrogen fuel and become many times brighter than it had been. sunspots—Dark areas on the surface of the Sun that are cooler than the surrounding area. satellite—A celestial body that orbits around a planet or star—can be natural or humanmade. For example, the Moon is one of Earth’s natural satellites, while astronomers can launch mechanical satellites that transmit information back to Earth.

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