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Saros cycle The saros () is a period of exactly 223 synodic months, approximately 6585.3211 days, or 18 years, 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. One saros perio ...
series 138 for
solar eclipse A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of the Earth, totally or partially. Such an alignment occurs during an eclipse season, approximately every six mo ...
s occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 events. 16 of these are partial solar eclipses. All eclipses in this series occurs at the Moon's descending node. This solar saros is linked to
Lunar Saros 131 Saros cycle series 131 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 72 member events, with 15 total eclipses, starting in 1950 and ending in 2202. The series contains 57 umbral eclips ...
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Antipode of Lunar Saros 131 is Solar Saros 138


Saros 138

It is a part of Saros cycle 138, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482 with a hybrid eclipse on March 1, 2500. It has total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. The longest duration of totality will be only 56 seconds on April 3, 2554.


Umbral eclipses

Umbral eclipses (annular, total and hybrid) can be further classified as either: 1) Central (two limits), 2) Central (one limit) or 3) Non-Central (one limit). The statistical distribution of these classes in Saros series 138 appears in the following table.


Events


References


NASA - Catalog of Solar Eclipses of Saros 138


External links


Saros cycle 138 - Information and visualization
{{Solar eclipses Solar saros series