This eclipse is a part of Saros series 129, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 3, 1103. It contains annular eclipses from May 6, 1464 through March 18, 1969; hybrid eclipses from March 29, 1987 through April 20, 2023; and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. 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 34 at 5 minutes, 10 seconds on October 4, 1698, and the longest duration of totality will be produced by member 58 at 3 minutes, 43 seconds on June 25, 2131. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 40–61 occur between 1801 and 2200: | ||
|---|---|---|
| 40 | 41 | 42 |
 December 10, 1806 |
 December 20, 1824 |
 December 31, 1842 |
| 43 | 44 | 45 |
 January 11, 1861 |
 January 22, 1879 |
 February 1, 1897 |
| 46 | 47 | 48 |
 February 14, 1915 |
 February 24, 1933 |
 March 7, 1951 |
| 49 | 50 | 51 |
 March 18, 1969 |
 March 29, 1987 |
 April 8, 2005 |
| 52 | 53 | 54 |
 April 20, 2023 |
 April 30, 2041 |
 May 11, 2059 |
| 55 | 56 | 57 |
 May 22, 2077 |
 June 2, 2095 |
 June 13, 2113 |
| 58 | 59 | 60 |
 June 25, 2131 |
 July 5, 2149 |
 July 16, 2167 |
| 61 | ||
 July 26, 2185 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 129". eclipse.gsfc.nasa.gov.