Solar Saros 119
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Saros cycle The saros () is a period of exactly 223 synodic months, 18 years 11 days and 8 hours, that 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 g ...
series 119 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 Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season i ...
s occurs at the Moon's ascending
node In general, a node is a localized swelling (a "knot") or a point of intersection (a vertex). Node may refer to: In mathematics * Vertex (graph theory), a vertex in a mathematical graph *Vertex (geometry), a point where two or more curves, lines ...
, repeating every 18 years, 11 days, containing 71 eclipses, including 54 umbral eclipses (2 total, 1 hybrid, and 51 annular). The first eclipse was on 15 May 850 and the last will be on 24 June 2112. The most recent eclipse was a partial eclipse on 30 April 2022 and the next will be a partial eclipse on 11 May 2040. The longest duration of totality was only 32 seconds on August 20, 1012. The longest duration of annularity was 7 minutes, 37 seconds on September 1, 1625.


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 119 appears in the following table.


All eclipses

Note: Dates are given in the
Julian calendar The Julian calendar is a solar calendar of 365 days in every year with an additional leap day every fourth year (without exception). The Julian calendar is still used as a religious calendar in parts of the Eastern Orthodox Church and in parts ...
prior to 15 October 1582, and in the
Gregorian calendar The Gregorian calendar is the calendar used in most parts of the world. It went into effect in October 1582 following the papal bull issued by Pope Gregory XIII, which introduced it as a modification of, and replacement for, the Julian cale ...
after that.


References

* http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros119.html


External links


Saros cycle 119 - Information and visualization
{{Solar eclipses Solar saros series