Many people think the seasons are caused by the distance between Earth and the Sun. This is a very common misconception! In reality, the distance only varies by 3% throughout the year, which is not enough to explain the temperature differences between summer and winter.
The Real Story: Earth's Tilt
Our planet is not straight like a pole. It tilts slightly, like a spinning top in balance. It is tilted by about 23.5 degrees relative to the vertical. This tilt, combined with Earth's revolution around the Sun, is the true secret of the seasons.
Why Earth's Tilt Changes the Seasons
Imagine Earth as a slightly tilted ball orbiting a giant lamp, the Sun. Depending on where it is in its orbit, the top or bottom of Earth receives more light and heat.
Summer in the North: The top of Earth (the Northern Hemisphere) is tilted toward the Sun. The rays arrive more directly and warm more strongly.
Winter in the North: The top of Earth is tilted slightly away from the Sun. The rays arrive at an angle, spread out more, and heat less.
Equinoxes and Solstices: Key Moments of the Year
The year is marked by four special moments that signal the start of the astronomical seasons:
Spring Equinox (around March 20): Day and night are of equal length (12 hours of day, 12 hours of night).
Summer Solstice (around June 21): This is the longest day of the year (about 16 hours of day, 8 hours of night).
Autumn Equinox (around September 22): Day and night are of equal length (12 hours of day, 12 hours of night).
Winter Solstice (around December 21): This is the longest night of the year (about 8 hours of day, 16 hours of night).