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Solar Saros 136

Saros cycle series 136 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 56 of which are umbral. The first eclipse in the series was on 14 June 1360 and the last will be on 30 July 2622. The most recent eclipse was a total eclipse on 22 July 2009 and the next will be a total eclipse on 2 August 2027.

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 136 appears in the following table. ==Gallery==
Gallery
File:Solar eclipse 1865Apr25-Cappeletti.png|April 25, 1865. Series member 29 File:Caroline-Island-1883-Eclipse.jpg|An artist's depiction of the total solar eclipse of May 6, 1883, observed from Caroline Atoll, Line Islands. Series member 30 File:1919 eclipse positive.jpg|The total solar eclipse of May 29, 1919, observed from the island of Principe. Positions of star images within the field near the Sun were used to verify Albert Einstein's prediction of the bending of light around the Sun from his general theory of relativity. Series member 32 File:Eclipse CR 1991 a zoom.jpg|Total solar eclipse of July 11, 1991 from Costa Rica. Series member 36 File:Solar eclipse 22 July 2009 taken by Lutfar Rahman Nirjhar from Bangladesh.jpg|Total solar eclipse of July 22, 2009 from Bangladesh. Series member 37 ==All eclipses==
All eclipses
Note: Dates are given in the Julian calendar prior to 15 October 1582, and in the Gregorian calendar after that. ==Notes==
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