About How is energy produced in the sun
The core of the sun is the region that extends from the center to about 20–25% of the solar radius. It is here, in the core, where energy is produced by hydrogen atoms (H) being converted into nuclei of heliu.
This is the zone immediately next to the core, which extends out to about 0.7 solar radii.
This is the sun's outer layer, which accounts for everything beyond 70% of the inner solar radius (or from the surface to approx. 200,000 km below). Here, the temperatur.
Lastly, there is the photosphere, the visible surface of the sun. It is here that the sunlight and heat that are radiated and convected to the surface propagate out into space. Te.
The core of the Sun extends from the center to about 20–25% of the solar radius.It has a density of up to 150 g/cm(about 150 times the density of water) and a temperature of close to 15.7 million(K).By contrast, the Sun's surface temperature is about 5800 K. Recent analysis ofmission data favors the idea that the core is rotating faster than the radiative zone outside it.
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