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Earth Springs Toward the Vernal Equinox

Published 17-Mar-2008

The vernal equinox will occur on March 20 in 2008, marking the beginning of spring in some cultures and falling around the Easter period in many Christian churches. Sources such as NASA have confirmed the March 20 date for the upcoming vernal equinox in 2008. The vernal equinox will occur at 5.48am at Coordinated Universal Time (UTC) on March 20, 2008. However places that are six hours or more behind UTC will observe the vernal equinox as early as March 19. At Vernal Equniox 2008, the sun is a little east of Indonesia, in the Indian Ocean.

Twice a year, around March 20 or 21 and September 22 or 23, the sun shines directly on the equator and the length of day and night are nearly equal in all parts of the world. These two days are known as the vernal (or spring) equinox and the autumnal equinox.

What does equinox mean?

The word “equinox” derives from the Latin words meaning “equal night” and refers to the time when the sun crosses the equator. The word “vernal” means “spring” in Latin. At such times, day and night are everywhere of nearly equal length everywhere in the world.

It is important to note that while the vernal equinox marks the beginning of spring in the northern hemisphere, it is the start of autumn in many parts of the southern hemisphere.

Vernal Equinox Explained

The vernal equinox is the movement when the sun crosses the true celestial equator – or the line in the sky above the earth’s equator – from south to north, around March 20 (or March 21) of each year. At that time, day and night are balanced to nearly 12 hours each all over the world and the earth’s axis of rotation is perpendicular to the line connecting the centers of the earth and the sun.

The point of intersection of the ecliptic, inclined from south to north, and the celestial equator is called the true vernal equinox. In gyroscopic motion, the earth’s rotational axis migrates in a slow circle based as a consequence of the moon’s pull on a nonspherical earth. This nearly uniform motion causes the position of the equinoxes to move backwards along the ecliptic in a period of about 25,725 years.

Nearly Equal?

During the vernal equinox, the length of night and day across the world is nearly, but not entirely, equal. This is because the day is slightly longer in places that are further away from the equator, and because the sun takes longer to rise and set in these locations. Furthermore, the sun also does not set straight down, but it also moves in a horizontal direction.

During the vernal equinox, the length of daylight is about 12 hours and eight to nine minutes in areas that are about 30 degrees north or south of the equator, while areas that are 60 degrees north or south of the equator observe daylight for about 12 hours and 16 minutes. Many regions around the equator have a daylight length about 12 hours and six-and-a-half minutes during the vernal equinox.

Moreover, one day does not last for the exact same 24 hours across the world and due to time zone differences, there could be a small difference in the daylight length between a far-eastern and far-western location on the same latitude, as the sun moves further north during 24 hours. For more information, click here to find out the length of day in a particular city. Select a location in the drop-down menu below to find out the length of day on March 20, 2008.

Historical Fact

A Greek astronomer and mathematician named Hipparchus (ca. 190-ca.120 BCE) was known for discovering the precession of the equinoxes, the slow movement among the stars of the two opposite places where the sun crosses the celestial equator. Hipparchus made observations of the equinox and solstice.

Astronomers use the spring equinoctial point to define their frame of reference, and the movement of this point implies that the measured position of a star varies with the date of measurement. Hipparchus also compiled a star catalogue, but this has been lost.

Vernal Equinox across Cultures

In the northern hemisphere the vernal equinox marks the start of spring and has long been celebrated as a time of rebirth. Many cultures and religions celebrate or observe holidays and festivals around the time of the vernal equinox, such as the Easter holiday period.

The astronomical Persian calendar begins its New Year on the day when the vernal equinox occurs before apparent noon (the midpoint of the day, sundial time, not clock time) in Tehran. The start of the New Year is postponed to the next day if the equinox is after noon.

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