Is this really interesting: Autumnal Equinox

The picture on the left shows the view from the solar system , and from on the surface of the earth.

The Autumnal Equinox signals the end of the summer months and the beginning of winter.

The autumnal equinox is at ecliptic longitude 180° and at right ascension 12h.

In the southern hemisphere, the autumnal equinox corresponds to the center of the Sun crossing the celestial equator moving northward and occurs on the date of the northern vernal equinox.

Burn during Wiccan ceremonies on Mabon , or at that time to attune with the change of the seasons.

When the Sun passes this point, on about 23 September each year, nights begin to grow longer than days, and continue to do so until the Winter Solstice in December.

An equinox is the moment in time when the centre of the Sun can be observed to be directly above the Earth ’s equator, occurring around March 20 and September 22 each year.

In fact, the Sun is at the equator, so both halves of the Earth are getting about the same amount of sunlight.

The dates of maximum tilt of the Earth’s equator correspond to the summer solstice and winter solstice, and the dates of zero tilt to the vernal equinox and autumnal equinox.

The exact date and time of the fall equinox, when the sun moves into the astrological sign of Libra, varies from year to year.

The upper panel shows that on an equinox , neither half of the Earth points directly towards the Sun.

Mabon or the Autumn Equinox is one of the Lesser Wiccan Sabbats and is usually celebrated around September 23rd, though it can occur as early as the 20th, depending on the timing of the actual Astrological event.

At noontime in the Northern Hemisphere the sun appears high in the sky during summertime and low in the sky during winter.

However during Autumn, we begin to see the waning of the Sun more obviously now as the days continue to grow shorter until the Wheel of the Year spins around again to Yule.

The date when night and day are nearly of the same length and Sun crosses the celestial equator moving southward.

On a day which has an equinox, the centre of the Sun will spend a nearly equal amount of time above and below the horizon at every location on Earth and night and day will be of nearly the same length.

The various other names for this Sabbat include the Autumn Equinox, the Fall Equinox, the Second Harvest Festival, Festival of Dionysus, Wine Harvest, Cornucopia, Feast of Avalon, Equinozio di Autunno , and Alban Elfed.

Neither hemisphere gets more sunlight than the other, so both have similar seasons.

The direction of this tilt is effectively constant, relative to the stars, so that the Earth’s north pole always points towards Polaris, the Pole Star, and the south pole always points at the constellation of Octans.

South of the equator, its name is less appropriate, since it corresponds to the beginning of summer, though for historical reasons the name autumnal tends to be used for the September equinox in both hemispheres.

Because the earth is rotating like a top or gyroscope, it points in a fixed direction continuously towards a point in space near the North Star.

When a pole is angled towards the Sun, its hemisphere receives more hours of sunlight, and when a pole is turned away from the Sun, its hemisphere experiences long cold nights.

Some believe that one can only balance an egg within a few hours before or after the exact time of the equinox.

Many people believe that since the equinox is a time of balance where the daylight hours and nighttime hours are equal, that by some mystical force one can balance eggs on their end on these days.

Mabon’s light has been drawn into the Earth, gathering strength and wisdom enough to become a new seed.

It is highest at the summer solstice and lowest at the winter solstice.

Each year, the Earth completes a circuit of the Sun, and for its poles to remain fixed against the stars, their direction must rotate relative to the Sun.

The source of this material is Windows to the Universe, at http://www.windows.ucar.edu/ at the University Corporation for Atmospheric Research.

The bottom panel shows how this looks to someone standing on the ground in Topeka.

Note that the times below were calculated using AutumnalEquinox in the Mathematica application package Scientific Astronomer, which is accurate to within only an hour or so, and in practice gives times that differ by up to 15 minutes from those computed by the U.S. Naval Observatory.