Understanding Earth’s Seasons: Causes, Motions, and Key Terms
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Have you ever wondered why we experience different seasons throughout the year? In this lesson, you'll discover the fascinating science behind Earth's seasonal changes. We'll explore how Earth's movements, rotation on its axis, and revolution around the Sun. You'll learn important terms like solstice and equinox, and clear up common misconceptions about why seasons happen.
What Is Earth's Rotation and Revolution?
Rotation is the Earth spinning on its axis.
It takes 24 hours (one day) for Earth to complete a rotation.
Rotation causes day and night. The Sun appears to rise in the east and set in the west due to Earth's rotation.
Revolution is the movement of Earth around the Sun.
It takes about 365 days (one year) for Earth to complete one revolution around the Sun.
The path Earth takes around the Sun is called an orbit.
Why Does Earth Move Around the Sun?
Earth stays in its orbit because of gravity, the force pulling objects toward each other.
Earth's orbit results from the gravitational pull between Earth and the Sun.
Gravity's strength depends on the mass and distance between objects.