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equatorial equinox
The places where the Sun crosses the equator are called the equinoxes. There are two equinoxes each year: the vernal (spring) equinox in March and the autumnal equinox in September. During these times, day and night are approximately equal in length all over the world.
Day and night are of equal length (practically the definition of equinox)
Everyone has a sunset on the equinox because all latitudes have 12 hours of day and night.
For someone at the equator, during an equinox the Sun will get to the zenith.For someone at the equator, during an equinox the Sun will get to the zenith.For someone at the equator, during an equinox the Sun will get to the zenith.For someone at the equator, during an equinox the Sun will get to the zenith.
That is known as the equinox, which occurs twice a year in spring and autumn. During the equinox, day and night are approximately equal in length all over the world.
During an equinox, the sun's rays are most direct at the Earth's equator. This is because during an equinox, the tilt of the Earth's axis is such that the sun is directly over the equator, leading to equal day and night lengths at all latitudes.
During an equinox, the sun is directly over the equator of the Earth. This causes the length of day and night to be nearly equal all over the world.
During an equinox, the sun is directly above the equator, which is located at 0 degrees latitude. This is when day and night are approximately equal in duration all over the world.