Exeligmos - Details

Details

The exeligmos was known by the Greeks as early as 100 BC. A clock they made, called the Antikythera mechanism was able to predict the dates of consecutive exeligmoses.

The exeligmos is 669 synodic months (every eclipse cycle must be an integer number of synodic months), 726 draconic months (which ensures the sun and moon are in alignment during the new moon), and almost exactly 717 anomalistic months (ensuring the moon is at the same point of its elliptic orbit). The first two factors make this a long lasting eclipse series. The latter factor is what makes each eclipse in an exeligmos so similar. The near integer number of anomalistic months ensures that the apparent diameter of the moon will be nearly the same with each successive eclipse. The fact that it is almost exactly 19,756 days ( a whole integer) ensures each successive eclipse in the series occurs very close to the previous eclipse in the series. Because it is over a month longer than a calendar year, the path of each eclipse one exeligmos apart is roughly 600 miles away from the previous one. The sun's apparent diameter also changes significantly in one month, affecting the length and width of a solar eclipse.

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