This eclipse is a part of Saros series 121, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 25, 944 AD. It contains total eclipses from July 10, 1070 through October 9, 1809; hybrid eclipses on October 20, 1827 and October 30, 1845; and annular eclipses from November 11, 1863 through February 28, 2044. The series ends at member 71 as a partial eclipse on June 7, 2206. 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 39 at 6 minutes, 20 seconds on June 21, 1629, and the longest duration of annularity will be produced by member 62 at 2 minutes, 27 seconds on February 28, 2044. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 49–70 occur between 1801 and 2200: | ||
|---|---|---|
| 49 | 50 | 51 |
 October 9, 1809 |
 October 20, 1827 |
 October 30, 1845 |
| 52 | 53 | 54 |
 November 11, 1863 |
 November 21, 1881 |
 December 3, 1899 |
| 55 | 56 | 57 |
 December 14, 1917 |
 December 25, 1935 |
 January 5, 1954 |
| 58 | 59 | 60 |
 January 16, 1972 |
 January 26, 1990 |
 February 7, 2008 |
| 61 | 62 | 63 |
 February 17, 2026 |
 February 28, 2044 |
 March 11, 2062 |
| 64 | 65 | 66 |
 March 21, 2080 |
 April 1, 2098 |
 April 13, 2116 |
| 67 | 68 | 69 |
 April 24, 2134 |
 May 4, 2152 |
 May 16, 2170 |
| 70 | ||
 May 26, 2188 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 121". eclipse.gsfc.nasa.gov.