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How Hot Is the Sun?

SWAP View of Sun
This stunning space wallpaper shows the view of the sun from the SWAP (Sun Watcher using Active Pixel System detector and Image Processing) instrument onboard ESA's Proba-2 satellite. (Image credit: ESA/SWAP PROBA2 science centre)

The sun, a massive nuclear-powered source of energy at the center of the solar system, generates the heat and light that sustain life on Earth. But how hot is the sun?

The answer is different for each part of the sun. Arranged in layers, the sun varies in temperature: It is hottest at its center, and cooler in its outer layers — until it strangely reheats at the fringes of the sun's atmosphere.

At the sun's core, gravity causes intense pressure, and temperatures of up to 27 million degrees Fahrenheit (15 million degrees Celsius). This generates the nuclear fusion responsible for the star's energy.

That energy then radiates outward in the sun's inner radiative zone, which lacks the heat and pressure to cause fusion. In that zone, temperatures drop from 12.6 million to 3.6 million F (7 million to 2 million C). In the next zone, called the convective zone, plasma bubbles carry heat to the surface. This zone hits about 3.6 million F.

Next, energy reaches the surface of the sun, or photosphere, producing the light visible from Earth, and a comparatively chilly 10,000 F (5,500 C ).

For unknown reasons, however, temperatures rise again in the sun's atmosphere, hitting up to 3.6 million F in the star's outermost corona.

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Michael Dhar

Michael Dhar is a manuscript editor at the American Medical Association and a freelance science and medical writer and editor, having written for Live Science,,, The Fix, Scientific American, and others. Michael received a master's degree in Bioinformatics from NYU's Polytechnic School of Engineering, and also has a master's in English and Comparative Literature from Columbia University School of New York, and a bachelor's in English with a biology minor from the University of Iowa.