This eclipse is a part of Saros series 152, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 26, 1805. It contains total eclipses from November 2, 1967 through September 14, 2490; hybrid eclipses from September 26, 2508 through October 17, 2544; and annular eclipses from October 29, 2562 through June 16, 2941. The series ends at member 70 as a partial eclipse on August 20, 3049. 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 will be produced by member 30 at 5 minutes, 16 seconds on June 9, 2328, and the longest duration of annularity will be produced by member 53 at 5 minutes, 20 seconds on February 16, 2743. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 1–22 occur between 1805 and 2200: | ||
|---|---|---|
| 1 | 2 | 3 |
 July 26, 1805 |
 August 6, 1823 |
 August 16, 1841 |
| 4 | 5 | 6 |
 August 28, 1859 |
 September 7, 1877 |
 September 18, 1895 |
| 7 | 8 | 9 |
 September 30, 1913 |
 October 11, 1931 |
 October 21, 1949 |
| 10 | 11 | 12 |
 November 2, 1967 |
 November 12, 1985 |
 November 23, 2003 |
| 13 | 14 | 15 |
 December 4, 2021 |
 December 15, 2039 |
 December 26, 2057 |
| 16 | 17 | 18 |
 January 6, 2076 |
 January 16, 2094 |
 January 29, 2112 |
| 19 | 20 | 21 |
 February 8, 2130 |
 February 19, 2148 |
 March 2, 2166 |
| 22 | ||
 March 12, 2184 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 152". eclipse.gsfc.nasa.gov.