equinox
equinox
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.
This is called the "equinox", or "equal nights" - when the night and day are approximately the same duration.
The sun is directly over the southern hemisphere from the September equinox until the March equinox.
On the equator, the sun always seems very high at mid-day. But the sun is precisely over the equator only two moments in the year, the moment of the Vernal Equinox (Spring) and the moment of the Autumnal Equinox (Fall).
This happens twice a year at on of the "equinox" (the spring equinox or the fall equinox) At noon if you are on the equator at thet oment the Sun is at the "Zenith".
The day in March when the sun is directly overhead at noon on the equator is actually called the vernal equinox. It marks the beginning of spring in the Northern Hemisphere and fall in the Southern Hemisphere.
Duration.
It is called an equinox. During an equinox, the sun is directly above the equator, resulting in equal lengths of day and night worldwide.
The Autumnal Equinox occurs in September when the length of day and night is nearly equal. This is when the sun shines directly on the equator. People often have equinox parties to celebrate this date.
This imaginary line is called the equator. On the two equinoxes each year (around March 20th and September 23rd), the sun is directly over the equator, causing nearly equal lengths of day and night worldwide. This phenomenon is known as the equinox.