This eclipse is a part of Saros series 135, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305; hybrid eclipses on March 8, 2323 and March 18, 2341; and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. 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 16 at 10 minutes, 41 seconds on December 24, 1601, and the longest duration of totality will be produced by member 62 at 2 minutes, 27 seconds on May 12, 2431. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 28–49 occur between 1801 and 2200: | ||
|---|---|---|
| 28 | 29 | 30 |
 May 5, 1818 |
 May 15, 1836 |
 May 26, 1854 |
| 31 | 32 | 33 |
 June 6, 1872 |
 June 17, 1890 |
 June 28, 1908 |
| 34 | 35 | 36 |
 July 9, 1926 |
 July 20, 1944 |
 July 31, 1962 |
| 37 | 38 | 39 |
 August 10, 1980 |
 August 22, 1998 |
 September 1, 2016 |
| 40 | 42 | 42 |
 September 12, 2034 |
 September 22, 2052 |
 October 4, 2070 |
| 43 | 44 | 45 |
 October 14, 2088 |
 October 26, 2106 |
 November 6, 2124 |
| 46 | 47 | 48 |
 November 17, 2142 |
 November 27, 2160 |
 December 9, 2178 |
| 49 | ||
 December 19, 2196 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 135". eclipse.gsfc.nasa.gov.