This eclipse is a part of Saros series 134, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554; hybrid eclipses from January 3, 1573 through June 27, 1843; and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 72 as a partial eclipse on August 6, 2510. 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 totality was produced by member 11 at 1 minutes, 30 seconds on October 9, 1428, and the longest duration of annularity will be produced by member 52 at 10 minutes, 55 seconds on January 10, 2168. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 32–53 occur between 1801 and 2200: | ||
|---|---|---|
| 32 | 33 | 34 |
 June 6, 1807 |
 June 16, 1825 |
 June 27, 1843 |
| 35 | 36 | 37 |
 July 8, 1861 |
 July 19, 1879 |
 July 29, 1897 |
| 38 | 39 | 40 |
 August 10, 1915 |
 August 21, 1933 |
 September 1, 1951 |
| 41 | 42 | 43 |
 September 11, 1969 |
 September 23, 1987 |
 October 3, 2005 |
| 44 | 45 | 46 |
 October 14, 2023 |
 October 25, 2041 |
 November 5, 2059 |
| 47 | 48 | 49 |
 November 15, 2077 |
 November 27, 2095 |
 December 8, 2113 |
| 50 | 51 | 52 |
 December 19, 2131 |
 December 30, 2149 |
 January 10, 2168 |
| 53 | ||
 January 20, 2186 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 134". eclipse.gsfc.nasa.gov.