On or about September 23, and again on or about March 20, Earth reaches the equinox position. Its axis does not point toward or away from the sun, so days and nights are of equal length at all latitude lines on Earth.
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On or about September 23, and again on or about March 20, Earth reaches the equinox position. Its axis does not point toward or away from the sun, so days and nights are of equal length at all latitude lines on Earth.