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saros series
Sign in to saveseries of eclipses separated by a saros period
A saros series is a group of eclipses that repeat in the same pattern after a specific time interval called a saros period. This concept helps astronomers predict and track how eclipses will occur over long stretches of time.
AI-generated from the Wikipedia summary — may contain errors.
In the Vinony graph
Within Vinony's link graph, saros series is referenced by 1,045 other articles, and connects out to list of solar eclipses in the 20th century, lunar month and list of solar eclipses in the 21st century.
It sits within the topics 1st-millennium BC introductions, Chaldea and Eclipses.
Its subject is documented across 52 Wikipedia language editions.
~20 min read
Encyclopedic overview
In astronomy, the saros (/ˈsɛərɒs/ ) is a length of time covering exactly 223 synodic months (18 years 11 days and 8 hours), nearly 242 draconic months, and nearly 239 anomalistic months. Arising naturally due to synchronization between lunar phase, nodal precession, and apsidal precession, it can be used to predict eclipses of the Sun and Moon. One saros period after an eclipse, the Sun, Earth, and Moon return to approximately the same relative geometry, a near straight line, and a nearly identical eclipse will occur, in what is referred to as an eclipse cycle. Every eclipse has an associated saros series and all succeeding or preceding eclipses have a different saros series associated with them - as the eclipse of the same series occurs or occurred with a gap of one saros only. Solar and lunar eclipses have different saros series.
A series of eclipses that are separated by one saros is called a saros series. It corresponds to:
Excerpted from Wikipedia’s “saros series” article, available under the CC BY-SA 4.0 licence.