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The saros (/ ˈ s ɛər ɒ s / ⓘ) is a period of exactly 223 synodic months, approximately 6585.321 days (18.04 years), or 18 years plus 10, 11, or 12 days (depending on the number of leap years), and 8 hours, that can be used to predict eclipses of the Sun and Moon.
Macdonald cycle An eclipse cycle equal to 299 years and about ten and a half months, always occurring on the same node. Peter Macdonald found that a series of eclipses of especially long duration visible from Britain occurs with this interval in the period AD 1 to 3000. [3] A Macdonald series has around ten eclipses and lasts about 3000 years.
The exeligmos is an eclipse cycle that is a triple saros, three saroses (or saroi) long, with the advantage that it has nearly an integer number of days so the next eclipse will be visible at locations and times near the eclipse that occurred one exeligmos earlier. In contrast, each saros, an eclipse occurs about eight hours later in the day or ...
2 By time period of history. 3 See also. 4 External links. Toggle the table of contents. ... A solar eclipse occurs when the Moon passes between Earth and the Sun, ...
The last time a significant eclipse event happened in New York was on Aug. 21, 2017. ... and self-proclaimed "eclipse chaser," said the easiest way to calculate when a total eclipse is in your ...
When is the next solar eclipse after 2024? Not for another 20 years. According to NASA, after the total solar eclipse on April 8, 2024, the next total solar eclipse that can be seen from the ...
From the data file we can see that eclipses recur with a period of a combination of 15 inex and 1 saros (5593 synodic months, 165164.58 days, or 452.2 tropical years) throughout the whole panorama (26,000 years), for example from the eclipse of saros series −290, inex series 2 (slightly off the panorama to the left) to the eclipse of saros ...
An eclipse season is a period, roughly every six months, when eclipses occur. Eclipse seasons are the result of the axial parallelism of the Moon's orbital plane ( tilted five degrees to the Earth's orbital plane ), just as Earth's weather seasons are the result of the axial parallelism of Earth's tilted axis as it orbits around the Sun .