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Core (center)

•	What happens: This is where nuclear fusion occurs — hydrogen atoms are fused into helium, releasing a massive amount of energy.

•	Temperature: Around 15 million°C (27 million°F)

•	Density: Extremely dense, like 150 times the density of water.

•	Composition: Mostly hydrogen (about 70%) and helium (about 28%)

  1. Radiative Zone

    • What happens: Energy from the core slowly moves outward by radiation (photons bouncing from atom to atom).

    • Temperature: Drops from about 7 million°C to 2 million°C.

    • Time scale: It can take thousands to millions of years for energy to pass through this zone.

  1. Convective Zone

    • What happens: Energy is transported by convection — hot gases rise, cool gases sink.

    • Temperature: Around 2 million°C down to 5,500°C

    • What it looks like: Like boiling water — rising and falling blobs of plasma.

  1. Photosphere (visible surface)

    • What we see: This is the layer of the Sun we can observe directly with our eyes or telescopes.

    • Temperature: About 5,500°C (9,932°F)

    • Sunspots: Cooler, darker areas caused by magnetic activity.

  1. Chromosphere and Corona (outer atmosphere)

    • Chromosphere: A thin reddish layer seen during solar eclipses.

    • Corona: The outermost layer, extending millions of kilometers into space.

    • Temperature: Corona is incredibly hot — over 1 million°C, much hotter than the surface, and scientists are still studying why.

Summary of Composition:

•	Hydrogen: ~70%

•	Helium: ~28%

•	Other elements (oxygen, carbon, iron, etc.): ~2%
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alex luis

Lvl 2
2mo ago

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