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Earth’s tilted axis causes varying lengths of day and night during revolution.
Earth rotates on its axis and revolves around the Sun.
Rotation causes day and night.
Equatorial regions receive nearly uniform sunlight.
Earth comes between the Sun and Moon during a lunar eclipse.
Revolution changes Earth’s viewing direction in space.
Revolution with axial tilt changes the duration of daylight.
The Moon’s umbra falls on a narrow region of Earth.
One complete rotation defines one day.
Seasons are opposite in opposite hemispheres.
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