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- Slide: 1
- Today I had a very adventurous day! I took a journey to the middle of the sun! Let me tell you all about it.
- Slide: 2
- There is 6 layers! First is the core, secondly the radiative zone, next the convective zone, then the photosphere, the chromosphere, and lastly the transition region
- In the Core it is the Sun's central powerhouse, where the fissions occur. It looks like an extreme hot and dense region. The temperature is 15 million degrees!! Its not physically a layer but it is where all the suns energy originates. Next the Radiative Zone. The energy produced in the core comes in a form of photons travels outwards repeatedly. It looks like a thick dense region where heat transfer happens. The temperature is 2-7 million degrees. It is very thick zone extending from the core.
- Slide: 3
- The Convective zone is energy being carried outward by the movements of hot gas. Gas heated at the bottom rises to the surface, cools, and sinks back down. It looks like a churning motion of gas and creates imprints on the solar system. The temperature decreases significantly. The thickness layer between radiation zone and photosphere. The Photosphere is when the suns visible surface , where light is reduced into space. It is very hot and the temperature is 5,500 to 6,000 degrees
- The chromosphere produces most of the suns ultra violet light. It looks like a pinkish-red and thin. The temperature is from 6,000 to 20,000 degrees. The transition region is a thin boundary where the temperature increases rapidly from much cooler chromosphere to extremely hot. It is very thin.
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