Revolution Of The Earth Causes The Seasons

  • The Earth revolves around the Sun in a fixed path called an orbit.
  • One complete revolution takes 365 1/4 days, which equals one year.
  • The Earth’s axis is tilted at an angle of 23.5 degrees.
  • This tilt is the main reason why different parts of the Earth experience different seasons.
  • As the Earth moves around the Sun, different areas receive varying amounts of sunlight, leading to the seasons.
  • Summer: When a hemisphere is tilted toward the Sun, it experiences summer.
  • Winter: When a hemisphere is tilted away from the Sun, it experiences winter.
  • Spring and Autumn: These are transition periods when neither hemisphere is tilted significantly toward or away from the Sun.
  • During summer, the Sun appears higher in the sky, and days are longer because the Sun’s rays are more direct.
  • During winter, the Sun is lower in the sky, and days are shorter because the rays are less direct.
  • Summer Solstice: The longest day of the year (around June 21).
  • Winter Solstice: The shortest day of the year (around December 21).
  • Equinoxes: Equal day and night (around March 21 and September 23).
  • Rotation: The Earth spins on its axis, causing day and night.
  • Revolution: The Earth moves around the Sun, causing seasons.
  • Seasons affect weather, plant growth, and human activities.
  • They bring variety to the environment and play a key role in the life cycles of living organisms.

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