Template:Solar Saros series 136
This eclipse is a part of Saros series 136, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 14, 1360. It contains annular eclipses from September 8, 1504 through November 12, 1594; hybrid eclipses from November 22, 1612 through January 17, 1703; and total eclipses from January 27, 1721 through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 9 at 32 seconds on September 8, 1504, and the longest duration of totality was produced by member 34 at 7 minutes, 7.74 seconds on June 20, 1955. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 26–47 occur between 1801 and 2200: | ||
|---|---|---|
| 26 | 27 | 28 |
 March 24, 1811 |
 April 3, 1829 |
 April 15, 1847 |
| 29 | 30 | 31 |
 April 25, 1865 |
 May 6, 1883 |
 May 18, 1901 |
| 32 | 33 | 34 |
 May 29, 1919 |
 June 8, 1937 |
 June 20, 1955 |
| 35 | 36 | 37 |
 June 30, 1973 |
 July 11, 1991 |
 July 22, 2009 |
| 38 | 39 | 40 |
 August 2, 2027 |
 August 12, 2045 |
 August 24, 2063 |
| 41 | 42 | 43 |
 September 3, 2081 |
 September 14, 2099 |
 September 26, 2117 |
| 44 | 45 | 46 |
 October 7, 2135 |
 October 17, 2153 |
 October 29, 2171 |
| 47 | ||
 November 8, 2189 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 136". eclipse.gsfc.nasa.gov.