Science Essentials: Sun, Matter, Physics
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The Sun: Structure and Activity
Galileo's Solar Observations
Galileo Galilei was among the first scientists to study the Sun in detail (circa 1610).
Sun's Chemical Makeup
The Sun's composition is primarily Helium & Hydrogen.
Inside the Sun
Solar Atmosphere Layers
- Photosphere
- Chromosphere
- Corona
Solar Interior Zones
- Core
- Radiative Zone
- Convective Zone
How the Sun Produces Energy
Solar energy is produced by nuclear fusion in the core region, converting hydrogen into helium. This process is the source of the Sun's energy.
The energy output is approximately 9 × 1010 megatons of TNT per second.
Understanding Solar Wind
Solar Wind is solar material flowing into interplanetary space. The Sun's atmosphere is expanding radially outwards in all directions. Solar... Continue reading "Science Essentials: Sun, Matter, Physics" »