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Sun - Wikipedia The Sun is the star at the centre of the Solar System It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light and infrared radiation with 10% at ultraviolet energies
Sun: Facts - NASA Science Our Sun is a 4 5 billion-year-old yellow dwarf star – a hot glowing ball of hydrogen and helium – at the center of our solar system It’s about 93 million miles (150 million kilometers) from Earth and it’s our solar system’s only star Without the Sun’s energy, life as we know it could not exist on our home planet
In Depth | Sun – NASA Solar System Exploration Our Sun is a medium-sized star with a radius of about 435,000 miles (700,000 kilometers) Many stars are much larger – but the Sun is far more massive than our home planet: it would take more than 330,000 Earths to match the mass of the Sun, and it would take 1 3 million Earths to fill the Sun's volume
Meet the Sun - Center for Science Education Like other stars, the Sun is a dense ball of gas that creates energy through nuclear fusion reactions in the core, creating helium atoms from hydrogen atoms The Sun radiates different forms of energy, including ultraviolet, infrared, and light energy, out into space Light and heat energy from the Sun warm our planet and make life possible
The Sun: Facts, size, and fate of Earth’s blazing star Gazing up at the clear blue sky, our eyes are often drawn to the Sun, that magnificent burning orb that illuminates our days, warms our planet, and supports the growth of our food But how much