Friday, February 27, 2009

♥SOLAR/LUNAR ECLIPSE♥

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2008 February 29
See Explanation.  Clicking on the picture will download  an mpeg movie file.

Twelve Lunar Eclipses
Credit & Copyright: Tunç Tezel (TWAN)

Explanation: Welcome to the extra day in the Gregorian Calendar's leap year 2008! To celebrate, consider this grid of lunar eclipse pictures - starting in leap year 1996 and ending with February's eclipse - with the date in numerical year/month/day format beneath each image. Mostly based on visibility from a site in Turkey, the 3x4 matrix includes 11 of the 13 total lunar eclipses during that period, and fills out the grid with the partial lunar eclipse of September 2006. Still, as the pictures are at the same scale, they illustrate a noticeable variation in the apparent size of the eclipsed Moon caused by the real change in Earth-Moon distance around the Moon's elliptical orbit. The total phases are also seen to differ in color and darkness. Those effects are due to changes in cloud cover and dust content in the atmosphere reddening and refracting sunlight into Earth's shadow. Of course, the next chance to add a total lunar eclipse to this grid will come at the very end of the decade.


Total Solar Eclipse 2006

Up one level

Total Solar Eclipse - Observed from Manavgat, Turkey - 29 March 2006

By Odd Høydalsvik, Bergen, Norway

Phases of the Total Solar Eclipse 2006

Montage showing the phases of the total solar eclipse in Turkey, 29th March 2006.
Montasje som viser fasene i den totlae solformørkelsen i Tyrkia 29 Mars 2006.


Sun and Moon

The picture above is a sandwich of two pictures, one of the sun taken just before the eclipse, and one at the start of totality. It shows the difference in size between the sun and the moon at the day of the eclipse. The yellow disk is the sun as it would have been behind the moon, the black ring is the moon. The moon was quite close to the earth, therefore it looks bigger than the sun. Thanks to this, the duration of the eclipse was quite long.

Bildet over er en motasje som viser størrelsesforholdet mellom sola og månen på den dagen formørkelsen fant sted. Den oransje sirkelen er sola slik den ville vært bak månen, den svarte ringen er månen. Månen var ganske nær jorda, derfor har den en del større utstrekning enn sola. Dermed varte formørkelsen ganske lenge.


Corona - total solar eclipse 2006

The picture above shows the corona. It is a composite made of 4 different exposures ranging from 1/125s to 1/4s.
This shape of the corona is typical for periods with low solar activity.

Bildet over viser koronaen til sola. Det er en sammenkopiering av 4 bilder med eksponeringstider fra 1/125s til 1/4s.
Denne langstrakte fasongen på koronaen er typisk for perioder med lav solaktivitet.


Corona - total solar eclipse 2006

The picture above shows the corona further processed in order to show more details. It is a composite made of 4 different exposures ranging from 1/250s to 1/4s.

Bildet over er ytterligere prosessert for å framheve detaljene i koronaen ennå bedre. Det består av 4 eksponeringer fra 1/250s til 1/4s.


Diamond Ring, Eclipse 2006

The picture above shows several images of the diamond ring taken in rapid sequence before (left) and after (right) totality. We can also see Baileys beeds on second image from left and on first, second and third image from right. These are formed by the sun shining through valleys on the moon limb. The picture is a composite consisting of 9 images combined in Photoshop CS2.

Bildet over viser flere bilder av diamantringen tatt i rask rekkefølge like før (venstre) og etter totaliteten. Vi kan også se såkalte "Baileys beeds" (perlekjede) på andre bilde fra venstre og på første, andre og tredje bilde fra høyre. Disse "perlene" dannes ved at sola skinner gjennom daler på måneranda. Bildet er satt sammen av 9 forskjellige bilder vha Photoshop CS2.

Diamond Ring, Eclipse 2006

Diamond ring just before totality. 13:55:04 UT+3
Diamantringen like før totalitet. 13:55:04 lokal tid.
Exposure: 1/1000s, f 11, ISO 400


Corona, Eclipse 2006

Corona near sun. 13:55:27 UT+3
Koronaen nær solskiva. 13:55:27 lokal tid.
Exposure: 1/125s, f 11, ISO 400


Totality, outer corona, Eclipse 2006

Outer parts of Corona. 13:55:42 UT+3
Ytre deler av koronaen. 13:55:42 lokal tid.
Exposure: 1/4s, f 11, ISO 400


Diamond Ring, Eclipse 2006

Diamond ring at end of totality. 13:58:57 UT+3
Diamantringen ved slutten av totaliteten. 13:58:53 lokal tid.
Exposure: 1/1000s, f 11, ISO 400


Inner corona, Eclipse 2006

Composite of two images at beginning and end of totality, showing prominences at both sides of sun.
Montasje av to bilder fra begynnelsen og slutten av formørkelsen. Vi kan da se protuberansene på begge sidene av sola.

Picture of Sun's Chromosphere

The thin pink line along part of the sun's limb is the sun's chromosphere.
Den tynne rosa linja langs deler av solranda er kromosfæren til sola.


Common technical data for all pictures above:
Camera: Canon EOS 20D
Lens: Sigma 100-300mm EX APO HSM f1:4 plus Sigma EX APO 2X Tele Converter (600mm)



Phases of total solar eclipse 2006

Multiple exposure on a single frame of slides film.
I forgot to remove the solar filter during totality, so I had to insert another image of the sun here taken with another camera.
Camera: Canon Rebel G / EOS 500N
Lens: EF 28-105mm at 45mm
Exposure: 1/30s, f 8.0 at ISO 100
Film: Fuji Sensia 100
Image at totality is exposed at 1/15s, f 11 at ISO 400 and scaled to correct size before combining in Photoshop.


The following pictures are taken with a Sony DSC-W1 digital compact camera.

Solar eclipse 2006
Solar eclipse 2006
In the foreground you can see images of the sun produced by pinhole effect through foliage.
Notice that after totality the direction of the images are reverse.


Back to main page

See also report and pictures from the total solar eclipse August 1 2008 in Novosibirsk

♥PHASES OF THE MOON♥

Objectives


Drifting buoys-floats with a floating anchor suspended 15 meters below the surface-are used to track surface currents. They are also useful for meteorologists, since a barometer or wind-measuring device can be fitted to them. Wind data collected by buoys are used to calculate the current due to wind (Ekman current) and, at a larger scale, the current due to the Earth's rotation (geostrophic currents).

Sea level anomalies and trajectories of drifting buoys tracked by Argos in the North Atlantic, in a zone where there are no major currents. This diagram shows how the buoys tend to follow eddies. The effect of tides is also clearly visible in the small looping patterns (in particular on the plot farthest north) (see animation, 5.9 Mb).
(Credits Météo France/CLS)


Sea level anomalies and trajectories of drifting buoys tracked by Argos (see animation, 3.7 Mb). The buoys mainly follow the Antarctic Circumpolar Current, despite circling in places due mostly to eddies. According to the data, these buoys must have all lost their floating anchor between May 13 and May 25, 2001. It is odd that they continued to follow the current and eddies.
(Credits Météo France/CLS).


Sea level anomalies and trajectories of drifting buoys tracked by Argos in the North Atlantic, west of Ireland. These buoys have been "trapped" inside eddies, which are clearly visible as peaks and valleys in sea level anomaly maps (see animation, 1 Mb).
(Credits Météo France/CLS).

Sometimes, drifting buoys can be "trapped" in an eddy and circle it in one direction or the other, depending on whether the eddy forms a peak or valley in the ocean surface, and depending on the hemisphere (see A turbulent sea and Current relief). This trapping of drifting buoys collecting meteorological readings proves useful, since the buoys stay in the same place. The advantage of drifting buoys over moored buoys is that they are cheap to produce and deploy. One drawback, however, is that they are sometimes washed up on the shore. Eddies compensate for this natural tendency.


Until now, buoys became trapped in eddies by pure chance. In future, operational oceanography, especially near-real-time altimetry data (from Ssalto/Duacs) and ocean forecasts (Mercator), will make it possible to deploy buoys inside eddies detected by altimetry.

♥IMPORTANCE OF ECLIPSE♥

Observe Eclipses!
Excerpts from book by Dr. Michael D. Reynolds and Richard A. Sweetsir

Eclipse Observing and Vision Safety

Solar observing. The sun emits intense radiation in the infrared, visible and ultraviolet bands of the electromagnetic spectrum. We protect ourselves, at least partially, against the infrared and ultraviolet wavelengths of light with hats, sunscreen lotions, or by seeking shelter out of the sun’s direct rays. We deal with the visible wavelengths of light, reflected from bright surfaces, with sunglasses. Sunglasses, however, do not provide protection to the eyes from looking directly into the sun.


Figure 3-1 The Electromagnetic Spectrum showing the location of visible light with ultraviolet and infrared rays on opposite wavelengths to the visible spectrum. Illustration by David Frantz.

Our eyes are very sensitive to infrared, ultraviolet and intense visual solar radiation, and can easily sustain temporary or permanent damage—even blindness—from staring at the sun. The condition is called solar retinopathy (i.e., burns on the retina) and symptoms may not appear for hours after staring at the sun. In mild cases, symptoms may disappear; in moderate or severe cases, permanent loss of vision or portions thereof result.

This condition is not unique to a solar eclipse, contrary to what many are led to believe by well–meaning astronomers and medical professionals, but is caused by looking at the sun. The emphasis on safety for the impending solar eclipse results in unfortunate wording in media interviews that so convince people not to look at the sun “during the eclipse” that they mistakenly believe it is safe to do so once the eclipse is over.

The sun at totality. During—and only during—totality, it is perfectly safe to look at the totally eclipsed sun, without any filtering devices, even through telescopes. Obviously, during totality it is the new moon which is being observed in silhouette against the sun’s outer atmosphere, and it is safe to view the moon without special filters.

However, great care must be taken to insure that such viewing does not begin until the last bead of direct sunlight winks out, and even greater care must be taken to insure that observations end before the edge of the sun reappears from behind the moon’s limb at the end of totality. This latter task is best left to a reliable volunteer timekeeper, or tape–recorded countdown, to warn of the approach of third contact at the observer’s site, than to the preoccupied observer’s personal judgment.

Lunar observing. The moon, whether in or out of eclipse, presents no danger to the eyes. Thoughtful amateur astronomers should not assume that lay persons or the media know this, and should be prepared to field their concerns and inquiries at times of lunar eclipses with assurances and explanations rather than ridicule. The moon, which is full at times of lunar eclipse, can be uncomfortably bright during the early and late stages of an eclipse, however, and filters can enhance the observing experience.


Photograph 3-2 Nature provides an excellent pinhole camera projector: the overlapping leaves of a tree! 10 May 1994 annular, Baja California, Mexico. Photograph taken by Mike Reynolds.

What’s safe and what isn’t? It is never safe to stare directly at the sun with the unaided eye. At times this seems to be unavoidable. Driving to and from work on east–west highways can expose commuters to the rising and setting sun for extended periods of time. Tinted windshields and sunglasses may handle the casual glances, but are poor substitutes for avoidance. Effective use of sun visors or similar blocking devices is best.

Many believe that viewing the sun’s reflection off a body of water or piece of dark glass or metal automobile hood is safe; it is not, for the sun’s reflected light can also cause eye damage.

The safest way to observe the sun with the unaided eye is to project an image of the sun onto another surface; this projection method guarantees that at no time is the eye exposed directly to solar radiation.

The next–safest way is to obtain approved solar viewing filters from a reputable science supply house or astronomical company. Inspect them carefully for flaws before each use, then discard and replace them after a reasonable period of time.

It is never safe to observe the sun through any kind of optical instrument without suitably approved astronomical filtering devices securely attached. This includes binoculars, small spotter scopes, and camera viewfinders and lenses.

Projection method. The use of projection to view the sun’s image indirectly is by far the safest approach to solar and solar eclipse observing. This method may be applied either with or without optical aid, although the former presents a much larger image and more rewarding appearance. Both approaches will be discussed, along with their advantages and disadvantages.

Pinhole projectors. A simple pinhole projector can be made from a cardboard shoebox. Cut a small opening about 2.5 cm (1 in) square in the center of one end of the shoebox, and tape a piece of aluminum foil over the opening. Make a small opening in the center of the aluminum foil with a pin. The sun’s image will be projected onto the opposite end of the shoebox, where it can be viewed by an observer.

Viewing may be enhanced by leaving the lid on the shoebox and cutting a small viewing slit in the side of the box near the end where the sun’s image is being projected, and placing the eye near this slit. The sun’s image may then be seen against a relatively dark background. The best view is obtained with the observer’s back to the sun and the aluminum pinhole held over the shoulder, guaranteeing that the observer is not tempted to glance at the sun while viewing the eclipse.

A similar device can be made by replacing the cardboard shoebox with a large mailing tube. The pinhole can be made in an aluminum foil cap taped to one end. A paper viewing screen, made translucent by a drop or two of cooking oil, may be taped to the other end in lieu of cutting a viewing slit in the side of the tube.

Mirror projectors. It is possible to view the sun from indoors with a simple mirror device. Select a window facing the sun. Tape a piece of paper, with a 2.5 cm (1 in) hole cut in its center, onto the window, then cover the rest of the window with dark cloth or sheets of newspaper.

Next, place a mirror against an opposite wall so that the sun’s light coming through the opening in the window hits it. Reflect the sun’s light from the mirror onto a piece of paper or white cardboard attached to the wall beneath the window.

Finally, cut a 2.5 cm (1 in) hole in another piece of stiff cardboard, tape a piece of aluminum foil over the hole, and make a pinhole in the center of the aluminum foil. When this pinhole card is moved between the mirror and the cardboard beneath the window, an image of the sun should come into focus on the wall beneath the window.

The mirror will have to be moved to follow the sun’s motion across the sky as the eclipse progresses, but this method assures comfortable indoor viewing of the partial phases as long as the sun is shining through the window opening.

A similar method, recommended by the Royal Astronomical Society of Canada in their Observer’s Handbook 1994, is to cover a small pocket mirror, except for a small opening about 6 mm (1/4 in) square, and position it where the sun’s rays can reflect off the opening and into a darkened room. The reflected spot will be a pinhole image of the sun’s disk. Try varying the size of the opening, and the distance you project the image, to maximize image size, sharpness and brightness.


Photograph 3-3 A number of options can be considered for optical projection. Sun Spotter II, a commercially available product, produced excellent images of the 10 May 1994 annular from Baja California, Mexico. Photograph taken by Mike Reynolds.

Optical projectors. A pair of binoculars or a small telescope can be used without filters to project an image of the sun onto a screen, a hand–held square of cardboard or posterboard. The instrument being used should be securely mounted and carefully monitored at all times to make certain that curious onlookers do not attempt to look directly through the instrument and damage their vision. For public observing sessions, amateur astronomers are urged to rope off the instrument and the screen to keep spectators from placing their eyes between the two.

A round cereal box, such as an oatmeal container, can also be used. Simply slip one end of the box over the eyepiece end of a telescope and view the projected image at the other end through a viewing flap or hatchway cut in the side near the end opposite the telescope.

Viewing filters. Whenever an observer intends to use filters to view the sun or a solar eclipse directly, there are inherent risks in the procedure even when the filters themselves are capable of blocking all of the sun’s harmful rays and dimming the visible light to a comfortable level.

Filters which are used in conjunction with telescopes or other optical devices present the greatest risk to observers, for the sun’s light is being intensified and magnified by the optics of the instrument. Anyone who has ever focused the sun’s light through a magnifying glass and ignited a leaf or a piece of paper has personal knowledge of the sun’s ability to damage the eyes.

The two approaches to filtering the sun’s rays for direct viewing are the rear–mounted and front–mounted methods, so named for their placement with respect to the optical path of an instrument.


Photograph 3-4 The best thing to do with rear-mounted eyepiece solar filters: throw them away!

Rear–mounted filters. The most dangerous type of filter is one that is placed at the eyepiece end of binoculars or telescopes, for these are taking the full force of the magnified image of the sun.

Even though they are capable of safely filtering out the sun’s harmful rays, their rear–mounted placement subjects them to intense heat from the sun. As they heat up, their glass expands within their mounting cells. If they have internal flaws or if their mounting cells are too tight to allow for expansion as they heat up, they will crack; many will crack even if well made and properly mounted. An observer looking through one when it cracks is unlikely to react quickly enough to withdraw the eye before sustaining serious injury. Unfortunately, they tend to be the most common type among beginning amateur astronomers, since such filters frequently come with the popular and inexpensive imported 50–mm to 60–mm (2–in to 2.4–in) refracting or 76 mm (3–in) reflecting telescopes distributed through popular department–store chains. The best advice is to throw them out and obtain a safer, front–mounted filter.

Front–mounted filters. These filters are placed over the front of binoculars, telescopes and camera lenses and filter the sun’s light before it ever enters the optical system. Therefore, the heat stays away from the instrument and the observer’s eyes. For small instruments, they can be full–aperture filters, meaning they have the same surface area as the telescope lens or mirror; for bigger instruments it is usually desirable to mount a smaller filter into a cell which fits over the end of the telescope, effectively reducing the aperture and saving money on the filter as well.

These filters may be made from metal–coated glass, mylar or plastic material, and provide adequate safety and pleasing views. However, they are not without safety concerns which should be constantly addressed.

The coatings on glass filters can deteriorate with time or become scratched; the best of these have the coated surfaces sandwiched between two pieces of glass, protecting them from the elements and from damage due to handling. The mylar and plastic filters can also suffer surface degradation, but are more prone to pin pricks due to handling in use. Some mylar and plastic filters also sandwich their coated surfaces for added protection and longevity, but these types are generally inexpensive enough to warrant replacement after a reasonable amount of use.

Front–mounted filters present an additional risk to the observer intent on direct solar viewing. They are only as safe as the method used to securely mount them to their instrument. Observers who rely on masking tape are risking their vision at every observing session. Even filter mounts which seem to fit snugly over the optical tube have been known to fall or be knocked off.

The best approach, and one that is absolutely essential around the general public or playful school students, is to fashion a mount that attaches snugly and is secured in a way that only you can quickly release at totality. The finder scope should also be equipped with a securely–mounted filter or be removed from the telescope entirely.

Distributors of safe front–mounted filters are listed in Appendix 5, but sources and addresses frequently change; potential purchasers should consult periodicals such as Sky & Telescope and Astronomy magazines for up–to–date listings and prices. They are advised to plan such purchases at least several months prior to an eclipse to guarantee delivery in ample time to practice observations and photography on the uneclipsed sun.


Photograph 3-5a, b Front-mounted filters. Above, a Thousand Oaks coated glass filter. Below, a selection of Tuthill mylar filters.

Other approaches. The classic system of telescopic solar observing employed a combination of an unsilvered glass secondary or diagonal mirror, called a Herschel Wedge, which ejected all but a tiny fraction of the sun’s light from the telescope, and a rear–mounted sun filter of Number 4 density dark glass mounted between the eye and eyepiece. While still a reliable approach, the availability of inexpensive full–aperture front–mounted filters makes changing secondaries and mounting sun filters unnecessarily time–consuming unless you have a telescope dedicated solely to solar observing.

For the naked–eye, the use of a Number 14 welder’s glass provides adequate protection from infrared as well as visible light to allow for safe viewing. They are not recommended for use with telescopes or binoculars.

The Eastman Kodak Company quotes medical authorities as recommending neutral–density filters of metallic silver and having at least a 6.0 density for naked–eye use. To make these, unroll a newly–opened roll of black–and–white panchromatic photographic film containing silver, such as Kodak Plus–X or Tri–X, to direct sunlight. Then roll it back onto its spool or into its cassette and have it developed for maximum density according to the manufacturer’s recommendations. When it has been processed, cut it into equal lengths long enough to cover one or both eyes, and tape two thicknesses of the film together for viewing. Mounting the film in a cardboard frame makes a convenient holder and protects against fingerprints. The National Society to Prevent Blindness correctly points out that non–professionals frequently misunderstand and misinterpret these critical instructions for making photographic film filters. Color films and newer black–and–white films which do not contain silver are not safe to use, nor are undeveloped film or developed negatives with photographic images on them. Do not use this approach unless you know what you are doing!

Unfortunately, film filters are generally too dark to use as a photographic filter, and less–dense photographic filters do not provide adequate protection to the eyes for even the briefest of glances at the sun through a camera viewfinder. Also, photo processors rarely develop black–and–white film in house anymore, necessitating use of more expensive labs, lengthy shipping delays, or, if you are so equipped, developing the film yourself. Again, the best approach is to use the front–mounted professional sun filters instead, which are safe for visual use and yield pleasing photographs. Planetaria and museums often sell filters especially made for eclipse viewing.


Photograph 3-6 The importance of safe solar viewing as all times, whether during a solar eclipse or solar observing in general, cannot be overemphasized. Mike Martinez (left) and Jeremy Reynolds demonstrate the use of naked-eye mylar and film filters at the 10 May 1994 annular eclipse.

Unsafe methods reemphasized. Never view the sun, either in or out of eclipse, with the unprotected eye. The only exception is totality, when none of the sun’s bright surface is visible. Sunglasses, crossed polarizing filters, color negatives, color transparencies, color films, black–and–white film containing no silver, undeveloped film, bottles of colored or dyed water, reflections of the sun in dark glass or standing water, and smoked glass do not provide adequate protection and are unsafe solar viewing options. Serious eye damage can accompany the use of any of these methods. Shun all rear–mounted filters on optical instruments. Finally, even approved–safe direct–viewing filters should be inspected carefully for flaws, scratches and damage before risking eye injury by their use.

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♥ECLIPSES♥

Eclipse

Near the beginning and end of total solar eclipse, the thin slice of the Sun visible appears broken up into beads of light. These lights are called 'Baily's Beads' after the British astronomer Francis Baily who discovered them. They occur because the edge of the Moon is not smooth but jagged with mountain peaks.


When just one bead is visible, the effect is often likened to a diamond ring.


A solar eclipse occurs when the Moon passes in front of the Sun and obscures it totally or partially. This configuration can only exist at New Moon, when Sun, Moon and Earth are on a single line with the Moon in the middle.

There are four types of solar eclipses:

  • A partial solar eclipse occurs when the Sun is only partially overlapped by the Moon.

  • A total solar eclipse occurs when the Moon completely obscures the Sun. This happens when the Moon is near perigee and its angular diameter as seen from Earth is identical to or slightly larger than that of the Sun. A total solar eclipse is the only opportunity to observe the Sun's corona without specialised equipment.

  • An annular (ring-formed) eclipse occurs when the Moon's center passes in front of Sun's center while the Moon is near apogee. The Moon's angular diameter is then smaller than that of the Sun so that a ring of the Sun can still be seen around the Moon. This is similar to a penumbral eclipse.

  • A hybrid eclipse occurs when the curvature of Earth's surface causes a single solar eclipse to be observed as annular from some locations but total from other locations. A total eclipse is seen from places on the Earth's surface that lie along the path of the eclipse and are physically closer to the Moon, and so intersect the Moon's umbra; other locations, further from the Moon, fall in the Moon's antumbra and the eclipse is annular.

The term "solar eclipse" is a misnomer: the phenomenon is actually an occultation. An "eclipse" occurs when one celestial object passes into the shadow cast by another (as with an eclipse of the Moon). An "occultation' occurs when one body passes in front of another. When at its new phase the Moon passes in front of, or occults, the Sun, as seen from Earth, the Moon also casts a small shadow on Earth. An "occultation" of the Sun is therefore also a partial "eclipse" of Earth.

Observing a solar eclipse

Looking at the Sun is dangerous at any time when any part of the brilliant visible disk of the Sun (its photosphere) is visible; to do so can cause permanent eye damage. This is true at any time, including during solar eclipses; since an eclipse offers an unusually high temptation to look at the Sun, there is a high incidence of eye damage caused during solar eclipses. Viewing the Sun through any kind of optical aid, binoculars, a telescope, or even a camera's viewfinder- is extremely dangerous.

Safe Solar Viewing

The Sun can be viewed using appropriate filtration to block the harmful part of the Sun's radiation. Note that sunglasses are of little use, since they don't block the harmful and invisible infra-red radiation which causes retinal damage; other improvised methods, such as using a reflection in water, or looking through a compact disk, are equally dangerous. Only properly designed and certified solar filters should ever be used for direct viewing of the Sun; and these must be in perfect condition, as even a small defect could cause damage.

The safest way to view the Sun is by indirect projection. This can be done by projecting an image of the sun onto a white piece of paper or card using a pair of binoculars (with one of the lenses covered), a telescope, or another piece of cardboard with a small hole in it (about 1 mm diameter), often called a pinhole camera.

The projected image of the sun can then be safely viewed; this technique can be used to observe sunspots, as well as eclipses. However, care must be taken to ensure that no-one looks through the projector (telescope, pinhole, etc.) directly, as this will cause severe eye damage; particular care should be taken if children are present.It is safe to directly observe the total phase of a total solar eclipse, when the Sun's photosphere is completely covered by the Moon; indeed, this is a very beautiful sight.

The Sun's faint corona will be visible, and even the chromosphere, solar prominences, and possibly even a solar flare may be visible. The danger here is of being caught out by the end of the total phase, and the return of the "exposed" Sun; because all parts of the Sun's disk are of similar intensity, even a tiny sliver of the Sun could cause permanent eye damage. For this reason, viewing the total phase of a solar eclipse through binoculars or a telescope should not be recommended.

Eclipse frequency and cause


Diagram of solar eclipse

Total and annular eclipses both occur when the Moon lines up with the Sun exactly, but since the Moon's orbit is not perfectly circular it is sometimes farther away from Earth and doesn't always cover the entire solar disc from an Earthly vantage point.

It is one of the most remarkable coincidences of nature that the Sun lies approximately 400 times as far away from Earth as does the Moon, and the Sun is also approximately 400 times as large in diameter as the Moon. As a result, as seen from Earth, the Sun and the Moon appear to be nearly the same apparent size. The Moon orbits Earth in an elliptical, or elongated orbit, however, and not in a circular orbit.

Thus during about 55-60% of its orbit the Moon is far enough from Earth ("apogee") that it is too small to cover the Sun's surface completely. During the remaining portion of its orbit, it is closer to Earth ("perigee") and large enough in apparent size to cover the Sun completely.

When a solar eclipse occurs near apogee, there is therefore a small ring or annulus of Sun that remains uncovered even at the moment of maximum eclipse. This produces an "annular" eclipse, during which the brilliant and blinding uncovered ring of the Sun makes the solar corona invisible. When a solar eclipse occurs near perigee, however, the Moon is close enough to Earth and large enough in the sky that it can cover the entire bright surface (the photosphere) of the Sun completely, and the observer sees a total eclipse, at which time the ghostly white solar corona appears.

A solar eclipse can only be seen in a band across Earth as the Moon's shadow moves across its surface, while a total or annular eclipse is actually total or ring-formed in only a small band within this band (the eclipse path), and partial elsewhere (total eclipse takes place where the umbra of the Moon's shadow falls, whereas a partial eclipse is visible where the penumbra falls). The full band is generally around 100 km in width. The eclipse path will be widest if the Moon happens to be at perigee, in which case the eclipse path alone can reach 270 km in width.

Total solar eclipses are rare events. Although they occur somewhere on Earth approximately every 18 months, it has been estimated that they recur at any given spot only every 300 to 400 years. And after waiting so long, the total solar eclipse only lasts for a few minutes, as the Moon's umbra moves eastward at over 1700 km/h.

Totality can never last more than 7 min 40 s, and is usually a good deal shorter. During each millennium there are typically fewer than 10 total solar eclipses exceeding 7 minutes. The last time this happened was June 30, 1973. Those alive today probably won't live to see it happen again, on June 25, 2150. The longest total solar eclipse during the 8,000-year period from 3000 BC to 5000 AD will occur on July 16, 2186, when totality will last 7 min 29 s. (eclipse predictions by Fred Espenak, NASA/GSFC.)

For astronomers, a total solar eclipse forms a rare opportunity to observe the corona (the outer layer of the Sun's atmosphere). Normally this is not visible because the photosphere is much brighter than the corona.

Calculating the date of a solar eclipse

If you know the date and time of a solar eclipse, you can predict other eclipses using eclipse cycles. Two well-known eclipse cycles are the Saros cycle and the Inex cycle. The Saros cycle is probably the most well known, and one of the best, eclipse cycles. The Inex cycle is itself a poor cycle, but it is very convenient in the classification of eclipse cycles. After a Saros cycle finishes, a new Saros cycle begins 1 Inex later (hence its name: in-ex).


Mythology

In the Odyssey, XIV, 151, Homer states that Odysseus will return to his home, and take vengeance on the suitors of Penelope, at the failing of the old moon and the coming of the new. Later in the Odyssey (XX, 356-357 and 390), Homer adds that the Sun vanished out of heaven and an evil gloom covered all things about the hour of the midday meal, during the celebration of the new moon. A total eclipse of the Sun was visible from the Greek island of Ithaca on April 16, 1178 BC. This would be six years after the end of the Trojan War, as traditionally dated (1184 BC), though within the Odyssey narrative it's supposed to be ten years after it.


Historical Solar Eclipses

Ancient civilizations used the movement of the heavens as celestial calendars. They created great stone monuments called astronomical observatories to this end. To the ancients, an eclipse often represented the Eye of God, All Seeing Eye!

A double (solar and lunar) eclipse took place 23 years after the ascension of king Shulgi of Babylon. This has been identified with eclipses that occurred on 9 May (solar eclipse) and 24 May (lunar eclipse), 2138 BC. This identification is however much less commonly accepted than the eclipse of 763 BC.

Ancient observations of solar eclipses from many different cultures and civilizations date back to at least 2500 BC in the writings that have survived from ancient China and Babylon. To establish an accurate luni-solar calendar, people in ancient civilizations observed the moon regularly. Lunar eclipses were the first major celestial events that astrologers learned how to predict based on local historical observation records.

One of the first things civilizations must do to ensure a coherent society is to establish an accurate calendar to organize planting and harvesting of crops. Most early calendars were lunar calendars, because the monthly duration of the lunar cycle is 29.53 days, 12.37 months during a solar seasonal year. Every year, the lunar "synodic" calendar of 29.53 days slips by 0.38 of a month or 11.2 days relative to the seasonal "planting" year.

At the same time that ancient people kept track of how the lunar and solar calendars meshed with each other, they also uncovered some of the factors that lead to lunar and solar eclipses which also require specific timings of the solar and lunar positions across the sky and over the years. In many ways, the ability to predict eclipses was an outgrowth of the pre-existing need to keep track of lunar and solar calendar relationships.


Ancient China

To the ancient Chinese, solar eclipses meant that dragons were devouring the sun.

Astronomy, Planetarium, The Chinese produced the first planetarium, which was actually made by an emperor. The planetarium was a big enclosed place with stars and constellations on the inside. The person using the planetarium would sit in a chair that was hanging from the top of the enclosed dome.

A solar eclipse of 16 June 763 BC mentioned in an Assyrian text is important for the Chronology of the Ancient Orient.

By 2300 BC, ancient Chinese astrologers, already had sophisticated observatory buildings, and as early as 2650 BC, Li Shu was writing about astronomy. Observing total solar eclipses was a major element of forecasting the future health and successes of the Emperor, and astrologers were left with the onerous task of trying to anticipate when these events might occur. Failure to get the prediction right, in at least one recorded case in 2300 BC resulted in the beheading of two astrologers. Because the pattern of total solar eclipses is erratic in any specific geographic location, many astrologers no doubt lost their heads. By about 20 BC, surviving documents show that Chinese astrologers understood what caused eclipses, and by 8 BC some predictions of total solar eclipse were made using the 135-month recurrence period. By AD 206 Chinese astrologers could predict solar eclipses by analyzing the Moon's motion.

Ancient Chinese astronomy was primarily a government activity. It was the astronomer's role to keep track of the solar, lunar, and planetary motions as well as divine what astronomical phenomena may mean for the ruling emperor. Solar eclipses, infrequent and dramatic, were important enough to be recorded in chronicles and on "oracle" bones. Below are a few translated eclipse records found in the documents of ancient China from various dynasties. In general, the translations give the Roman calendar dating of the event, the Chinese dating, and the observation. Following in parentheses is the record in which the observation is noted. More translated records can be found in the references given below. Unless otherwise noted, the translations below can be found in the book Historical Eclipses and Earth's Rotation by F. Richard Stephenson.

"Oracle" bones are pieces of animal bones and tortoise shells inscribed with astronomical observations, that were probably used for divinations. Oracle bones hail from the Shang dynasty (c. 1600, 1050 BC) and make many references to solar eclipses. The eclipse records are often incomplete, however, and the dating of the bones is not reliable.

Eclipse observations from the Chou dynasty and Warring States period (c. 1050-221 BC), and onward, have been reliably dated, and it appears that some astronomers recognized eclipses as naturally occurring phenomena. From the Chou dynasty, 36 solar eclipse observations are recorded in the Ch'un-ch'iu beginning around 720 BC. The Piao and the Shih-chi documents refer to nine solar eclipses from the Warring States period.

Records of solar eclipses from the Han dynasty (206 BC, 220 AD) are found primarily in two official histories: the Han-shu and the Hou-han-shu. There are no records of eclipses from the Ch-in dynasty which came just prior to the Han dynasty (221 BC, 206 BC).

During the Ming dynasty (1368-1644 AD), total solar eclipse observations are found in the histories of Ming provinces after 1500 AD. Prior to 1500 AD, eclipse records can be found in the Imperial Annals. These observations, however, are not of total solar eclipses. Aug 20, 1514 AD: "At the hour of wu suddenly the Sun was eclipsed; it was total. Stars were seen and it was dark. Objects could not be discerned at arm's length. The domestic animals were alarmed and people were terrified. After one (double-)hour it became light." (local history of Tung-hsiang county, Chiang-his province)

Accurate eclipse timings can be used to determine the rate of the Earth's rotation. According to Steele and Stephenson, solar eclipse timings can be found from the periods between 600 and 800 AD, 1000 and 1300 AD, and a brief period during the Ming dynasty. These solar eclipse timings are accurate to about 0.4 hours.


Babylon and Sumer

Babylonian clay tablets that have survived since dawn of civilization in the Mesopotamian region record the earliest total solar eclipse seen in Ugarit on May 3, 1375 BC.

Like the Chinese, Babylonian astrologers kept careful records about celestial happenings including the motions of Mercury, Venus, the Sun, and the Moon on tablets dating from 1700 to 1681 BC. Later records identified a total solar eclipse on July 31, 1063 BC, that "turned day into night," and the famous eclipse of June 15, 763 BC, recorded by Assyrian observers in Nineveh. Babylonian astronomers are credited with having discovered the 223-month period for lunar eclipses.

At this time, the same lunar phase would be recorded at the same time of the solar calendar year. This period also gives a rough guide to when a lunar eclipse will recur at the same geographic location. Ptolemy (ca 150 AD) represents the epitome of knowledge of Grecian astronomy.

Records such as the Almagest show he had a sophisticated scheme for predicting both lunar and solar eclipses. Ptolemy knew, for example, the details of the orbit of the Moon including its nodal points. He also knew that the Sun must be within 20 degrees 41' of the node point, and that up to two solar eclipses could occur within seven months in the same part of the world.

Lunar eclipses were especially easy to calculate because of the vast area covered by Earth's shadow on the Moon. Solar eclipses however required much greater knowledge. The shadow of the Moon on Earth is less than 100 kilometers wide, and its track across the daytime hemisphere is the result of many complex factors that cannot be anticipated without a nearly complete understanding of the lunar orbit and speed.


Ancient India

Indian astronomy is largely wrapped up in the Vedic religious treatises, but one individual, Aryabhata of Kusumapura, born in AD 476 is noteworthy. He is the first known astronomer on that continent to have used a continuous system of counting solar days. His book, The Aryabhatiya, published in 498 AD described numerical and geometric rules for eclipse calculations. Indian astronomy at that time was taking much of its lead from cyclic Hindu cosmology in which nature operated in cycles, setting the stage for searching for numerical patterns in the expected time frames for eclipses, click link above for more.


Ancient Egypt

Nearly all we know about ancient Egyptian civilization's knowledge of astronomy comes to us from tomb paintings, various temple inscriptions, and a handful of papyrus documents such as the Rhind Papyrus. Unfortunately, the Great Library in Alexandria was burned during the time of Cleopatra and Julius Caesar. Later burnings in AD 390 and AD 640 destroyed an estimated 400,000 books on Egyptian secular literature, mathematics, medicine, and astronomy. The burnings were classified as one of the greatest intellectual catastrophies in human history. One can only guess what Egyptian knowledge of astronomy was lost. All that survives is fragments that some scholars see as merely the faded ghosts of Egyptian intellectual legacy.

The oldest example of a sundial is Egyptian from about 1500 BC. The fabulous astrological ceiling of Senmut painted around 1460 BC, includes celestial objects such as Orion, Sirius, and the planets Mercury, Venus, Jupiter, and Saturn. The oldest known copies of an almanac date from 1220 BC at the time of Ramses the Great. In 1100 BC Amenhope wrote "Catalog of the Universe" in which he identified the major known constellations.

Curiously, the catalog does not mention either Sirius or any of the planets previously known to the Egyptians. At least outwardly, there are no surviving inscriptions or documents to indicate that Eqyptian knowledge of astronomy was more than tomb decoration, and not protected over the ages as a body of knowledge.

Numerous temple and pyramid alignments and several papyrus codices suggest a sophisticated knowledge of trigonometry and algebra; no similar astronomy documents survive, or records of astrological observations.

The Vienna papyrus which described lunar and solar eclipses and their portent was probably copied by a scribe in the late second century AD, and presents knowledge of astronomy that is regarded as Babylonian in nature.

Solar Eclipses in the Ancient Nile Valley

A full discussion of the presumed knowledge of solar eclipses by the ancient Egyptians is beyond the scope of these brief comments. However, it is pertinent to note that Greek writers, without exception, gave priority to Egypt in astronomical knowledge. Still, there has not yet come to light an Egyptian document specifically mentioning solar eclipses. However, that the Egyptians possessed accurate knowledge of eclipses is evident from external sources.

Diodorus Siculus (200 A.D.), stated categorically that the ancient Egyptian astronomers possessed the ability to predict solar eclipses. Plutarch related that the ancient Egyptians explained solar eclipses by the passage of the Moon between the Sun and the earth in daylight hours. There is evidence, admittedly disputed by some writers, that an actual solar eclipse was reported in Egypt in the 9th century B.C. and again in 610 B.C.

The report of this latter eclipse has been attributed to Thales, though others, e.g., Herodotus, claim that Thales actually predicted an eclipse in 584 B.C. Thales, Greece's first "philosopher", was actually of Phoenician birth and spent seven years studying in Egypt. Greek commentators attribute Thale's mathematical and astronomical knowledge to this apprenticeship in Egypt.

The golden age of Greek science commences with the Ptolemaic dynasty (330 B.C.) in Egypt, the building of Alexandria, and the founding of the city's Library. The major Greek astronomers studied there. Moreover, several of the Alexandrian astronomers considered Greek were actually Egyptians who had adopted or been given Greek names. One such person was Ptolemy (150 A.D.), author of the Almagest, the most important astronomical text until the Middle Ages, whose knowledge of solar eclipses is well-documented.

Clement of Alexandria (2nd century A.D.), author of Stromateis described 49 books of Thoth preserved by the priests of ancient Egypt, at least four of them treating astronomical subjects. One book dealt with the "constitution of the Sun and Moon" and another "the conjunctions and variations of the light of the Sun and Moon." That the ancient astronomer-priests of Egypt could and did predict eclipses was considered axiomatic. Information detailing Egyptian priesthood repeatedly confirm the remarkable ability of that priesthood to predict solar eclipses.


Egyptian Eclipse Disc

Theories about an Eclipse
  • The Sun god Atum is the eclipsed Sun passing the second contact of a total eclipse.

  • Ra/Re is the eclipsed Sun shining past the third contact as the Diamond Ring effect.

  • The Scarab Khepri was a representation of the dark New Moon.

  • The Hawk Horakhty, Horus - is the Sun through totality.

  • The Great Sphinx was the Egyptian 'Lord of Solar Eclipses'.

  • Hathor was the Egyptian goddess of solar eclipses.

  • The God Aten of the Amarna Revolution is the shadow bands phenomenon.

  • Inundation of the Nile Month of Thoth


The Islamic World

Islamic astronomy became the western world's powerhouse of scientific research during the 9th and 10th centuries AD, while the Dark Ages engulfed much of the rest of the western world. The works by Ptolemy, Plato, and Aristotle were translated, amplified upon and spread throughout the Muslim world.

Al-Khwarazmi developed the first tables, trigonometric functions (ca 825 AD) which remained the standard reference well into the modern era. Al-Khwarazmi was known to the west as "Algorizm" and this is, in fact, the origin of the term 'algorithm'. Al-Khwarazmi's calculations were good to five places, allowing for unprecedented precision in astronomy and other sciences.

At Antioch, Muhammad al-Batani (ca 850 AD) began with Ptolemy's works and recalculated the precession of the equinoxes, and produced new, more precise astronomical tables. Following a steady series of advances in Islamic trigonometry, observations by Ibn Yunus of lunar and solar eclipses were recorded in Cairo ca 1000 AD. Ibn Yunus is regarded as one of the greatest observational astronomers of his time.

The pace of Islamic science and scholarship eventually slowed down in the 11th and 12th centuries. Many great books and great ideas of the Islamic Age lay fallow for hundreds of years until they were finally translated into Latin and fueled the European revolution in thinking and the birth of science as we know it today.

Eclipse Ancient Civilizations & Metaphysics

The European appetite for books was no doubt stimulated by the cutting edge technology of that time: the printing press. This period was called the "Renaissance" (ca1500 AD) signifying the rapid growth of fresh perspectives and ideas. Many of these books were scientific, technical, and mathematical works, most of which had been gathered or written by scientists during the Islamic Renaissance that peaked some 600 years before Europe's! Islamic rulers sponsored the systematic collection and translation of scholarly books from every culture they came across.

For nearly two centuries, a diverse group Islamic thinkers (concentrating in Iran and the Middle East, but extending from Spain and North Africa to India and the Far East) amplified, elaborated, and extended the libraries of scientific knowledge that they had collected. They made great advances in math and science, observed nature and human society, amassed discoveries and inventions during the flowering of Islamic culture. The decline of Islamic learning had begun by the 11th century. By the 13th and 14th centuries, European translations of the volumes of Islamic theology, science, and technology had laid a rich foundation for the birth of modern science. Much of the library of Islamic sciences remains in Arabic to this day.


Ancient Greece

Herodotus wrote that Thales of Milete predicted an eclipse which occurred during a war between the Medians and the Lydians. Soldiers on both sides put down their weapons and declared peace as a result of the eclipse. Exactly which eclipse was involved has remained uncertain, although the issue has been studied by hundreds of ancient and modern authorities. One likely candidate took place on May 28, 585 BC, probably near the Halys river in the middle of modern Turkey.

An annular eclipse of the Sun occurred at Sardis on February 17, 478 BC, while Xerxes was departing for his expedition against Greece, as Herodotus, VII, 37 recorded ([Hind and Chambers, 1889: 323] considered this absolute date more than a century ago). Herodotus (book IX, 10, book VIII, 131, and book IX, 1) reports that another solar eclipse was observed in Sparta during the next year, on August 1, 477 BC. The sky suddenly darkened in the middle of the sky, well after the battles of Thermopylae and Salamis, after the departure of Mardonius to Thessaly at the beginning of the spring of (477 BC) and his second attack on Athens, after the return of Cleombrotus to Sparta.

By 450 BC, the Greek civilization was in its ascendancy. The historian Herodotus (ca 460 BC) mentions that Thales was able to predict the year when a total solar eclipse would occur. Details of how this prediction was made do not survive. The eclipse occurred in either 610 BC or 585 BC. Apparently the method used worked only once because what is known of Greek scientific history does not suggest that the method was ever reliably used again. Thales is said to have visited Egypt, and from the empirical rules in use there for land surveying, brought back to Greece the ideas of deductive geometry later codified by Euclid. Before 450 BC, Meton realized that a single period of 235 lunar months (19 years) would cause the popular lunar calendar to return to synchrony with the solar, seasonal calendar.


Ancient Rome

The foundation of Rome took place 437 years after the capture of Troy (1182 BC), according to Velleius Paterculus (VIII, 5). It took place shortly before an eclipse of the Sun that was observed at Rome on June 25, 745 BC and had a magnitude of 50.3%. Its beginning occurred at 16:38, its middle at 17:28, and its end at 18:16. Varro may have used the consular list with its mistakes, calling the year of the first consuls "245 ab urbe condita" (a.u.c.). A new study claims that the Varronian date has been superseded. Its correctness has not been proved scientifically but it is used worldwide.

According to Lucius Tarrutius of Firmum, Romulus was conceived in the womb on the 23rd day of the Egyptian month Choiac, at the time of a total eclipse of the Sun. This eclipse occurred on June 15, 763 BC, with a magnitude of 62.5% at Rome. Its beginning took place at 6:49, its middle at 7:47 and its end at 8:51. He was born on the 21st day of the month of Thoth.

The first day of Thoth fell on 2 March in that year. That implies that Rhea Silvia's pregnancy lasted for 281 days. Rome was founded on the ninth day of the month Pharmuthi, which was April 21, as universally agreed. The Romans add that, about the time Romulus started to build the city, an eclipse of the Sun was observed by Antimachus, the Teian poet, on the 30th day of the lunar month.

This eclipse had a magnitude of 54.6% at Teos, Asia Minor. It started at 17:49 and was still eclipsed at sunset, at 19:20. Romulus vanished in the 54th year of his life, on the Nones of Quintilis (July), on a day when the Sun was darkened. The day turned into night, which sudden darkness was believed to be an eclipse of the Sun. It occurred on July 17, 709 BC, with a magnitude of 93.7%, beginning at 5:04 and ending at 6:57. This eclipse data haa been calculated by Prof. Aurel Ponori-Thewrewk, retired director of the Planetarium of Budapest.

Plutarch placed it in the 37th year from the foundation of Rome, on the fifth of our month July, then called Quintilis, on "Caprotine Nones". Livy (I, 21) also states that Romulus ruled for 37 years. He was slain by the Senate or disappeared in the 38th year of his reign. Most of these have been recorded by Plutarch (Lives of Romulus, Numa Pompilius and Camillus), Florus (Book I, I), Cicero (The Republic VI, 22: Scipio's Dream), Dio (Dion) Cassius and Dionysius of Halicarnassus (L. 2). Dio in his Roman History (Book I) confirms these data by telling that Romulus was in his 18th year of age when he founded Rome. Therefore, three eclipse records prove that Romulus reigned from 746 BC to 709 BC.


Ancient Mayans

While Chinese, Babylonian, and Greek astronomers dominated the knowledge of old world astronomy half way across the globe, Mayan observers were working on calendars and recording celestial observations. The Dresden Codex records several tables thought to be lunar eclipse tables. As in previous civilizations in other parts of the world, the Mayas used records of historical lunar eclipses to calculate how often they occurred over a 405-month period. There is no mention of recorded total solar eclipses, or discussions in the Codex for how to predict these events. After the Spanish Conquistadores, came the missionaries in the 1600s who intentionally destroyed nearly all native written record. Little survives to tell us whether the Mayas, Incas, or Aztecs achieved a deeper understanding of solar eclipses and their forecasting.

Mayan astronomers were well aware that small cycles lead inevitably to bigger ones. Their codex seems to have been a mechanism for predicting not when the first crescent moons of the future could be sighted, but which full moons would be eclipsed and which new moons would eclipse the sun. It must have taken all of a century or more, which means several generations of perceptive astronomical observing, for specialists in skywatching to work through to a conclusion that their Chinese and Babylonian counterparts also had arrived at, i.e. that once a lunar or solar eclipse occurs, it is not possible to have another ( of the same kind) until six, or more rarely, five months pass.

Of the long-range Moon cycle in the Dresden Codex, this much is certain: First, it was used to gain control of astronomical time; and second, it was a time cycle derived from the observation of eclipsed and uneclipsed moons of the past, which could be used as data to generate a model for anticipating the occurrence of future lunar eclipses ­ powerful knowledge in the hands of the rulership.

Is the Dresden Codex a record of eclipses in part intended to warn of possible future eclipses? And, if so, what kind of eclipses? There seems little doubt that the Mayas sought to predict eclipses because of the disaster that they believed threatened them on such occasions. The omens in the table look ominous enough, at least to us. Of course, predictions must be based upon recorded observations of actual eclipses that occurred in Yucatan when the Mayan priests did their work. Though scholars are not in agreement over which particular set of eclipses (lunar or solar) was being observed, there is enough evidence to support the hypothesis that the Dresden Eclipse Table was devised for warning of the possible occurrence of such phenomena.

Both lunar and solar observational eclipse data can be utilized to construct a semblance of the Dresden Table. The hypothesis that lunar data were actually used seems much simpler. In the course of the thirty-three years spanned by the table, the number of such eclipses observable in Yucatan would have been significant enough to enable a single priest to draw up the table. If we assume that solar eclipses alone were used, and this certainly cannot be ruled out, we must extrapolate the base of observations backward many centuries in order to derive the relevant intervals.

The eight pages of the Moon table of the Dresden Codex are a chain of numbers across the bottom line of each page translates into a time packet of lunar synodic intervals. There are clumpings of six lunar synodic months (178 days) followed by one set of five (148 days). Each bunch of five moons is followed by a picture. A close look at all of the pictures together gives very strong clues about what the Mayas would do, parcel out a chain of 405 full moons over more than three decades. The answer is that Mayan astronomers were attempting, apparently quite successfully, to predict eclipses. Some of these illustrations depict half-light, half-dark disks with lunar crescents opposing the kin glyph, symbol of the Sun ( kin means sun and day as well as time in the Mayan language). A serpent devouring the Sun and a dead lunar goddess hanging by her hair from a segmented serpent who represents the sky also appear in the pictorial portion of the table.


Text References, Wikipedia




Eclipses In The News ...



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Metaphysics

Lunar and Solar eclipses have always been markers of change and evolution, dating to ancient times and civilizations. In the days before humanity became en'light'ened, the solar eclipse represented a time of fear and darkness. We have learned to see beyond myth and dark magic that controls through illusion, and moved into scientific truth.

Eclipses not only have gravitational affect on our bodies and planet Earth, but they also affect the collective unconscious, the grids, and in the astrological significance our natal birth charts, as well as the charts of nations. An eclipse seems to stop time, stop energy, and stop movement. Where once there was light filtering through the elemental forces of the zodiac into the Earth's aura, there is suddenly darkness, nothingness, a temporary lack of input from the Sun or Moon that serves to bring our awareness closer to the energy of the Solar or Lunar season, and thus intensify it.

The energies of a solar eclipse create changes on many levels as they represent letting go of the old and embracing the new, destruction, balance, rebirth.


Sacred Geometry

Eclipse of consciousness - enhances dreams,
and other out of bodies experiences.

The diamond shape of an eclipse symbolizes the star tetrahedron,
part of sacred geometry, mathematical patterns
that create the grids, or matrixes, of our reality.

Star Tetrahedron - Star of David, Flower of Life, Qabbalah and Merkabah.

From the Egyptian Pyramid Texts: "The eclipse represents the breaking of the Egg and Splitting the Iron." The iron is the rod, the magnetic poles, north/south, duality of experience creates by electromagnetic energy, the aura, needed to create a physical reality and the illusion of linear time. The Two 'Diamond Ring Effects' crowned the eclipsed shadow on the head of Re.


Emerald Tabets of Thoth

As is above, So is below, Hermes Trismegistus


The Merge of Matter and Antimatter at Zero Point

Polarites, Sun / Moon, Balance

Beads are a metaphor for DNA.


2001: A Space Odyssey
2001 - Thus Spake Zarathustra

Kubrick's masterpiece film, "2001: A Space Odyssey" refers to the heart of the Isis/Osiris mystery. The monolith represents the male, the generative force - the dome (rising sun, egg), the female. The result is a new dawn (beginning). This parallels Egyptian mythology - the synthesis of Isis and Osiris, to create Horus the Star Child.

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