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The Sun
Life Span of the Sun
• Based on its initial mass; will become a red giant and engulf Earth;
total life span would be about 10 billion years
How does the sun produce energy?
• The nuclear fusion of hydrogen
into helium in the core;
releases energy as
electromagnetic radiation
Main Source of Energy on Earth:
• Electromagnetic radiation travels
through space (a vacuum) to Earth
• Some of that radiation is absorbed
or reflected by Earth’s
atmosphere
• About half is absorbed by Earth’s
surface
• Some is reflected by Earth’s
surface
What are sunspots?
• Cooler areas of high magnetic
activity on the Sun’s surface;
their abundance peaks about
every 11 years
Solar Flares:
• Eruption of energy/radiation
from release of magnetic energy
associated with sunspots
Effects of Solar Flares:
• Can effect our upper atmosphere (create auroras) or potentially
disable our communications satellites
What protects us from solar storms/wind?
• Earth’s magnetic field provides a barrier to most of the sun’s
disturbances

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The Sun Notes

  • 2. Life Span of the Sun • Based on its initial mass; will become a red giant and engulf Earth; total life span would be about 10 billion years
  • 3. How does the sun produce energy? • The nuclear fusion of hydrogen into helium in the core; releases energy as electromagnetic radiation
  • 4. Main Source of Energy on Earth: • Electromagnetic radiation travels through space (a vacuum) to Earth • Some of that radiation is absorbed or reflected by Earth’s atmosphere • About half is absorbed by Earth’s surface • Some is reflected by Earth’s surface
  • 5. What are sunspots? • Cooler areas of high magnetic activity on the Sun’s surface; their abundance peaks about every 11 years
  • 6. Solar Flares: • Eruption of energy/radiation from release of magnetic energy associated with sunspots
  • 7. Effects of Solar Flares: • Can effect our upper atmosphere (create auroras) or potentially disable our communications satellites
  • 8. What protects us from solar storms/wind? • Earth’s magnetic field provides a barrier to most of the sun’s disturbances