This eclipse is a part of Saros series 117, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 24, 792 AD. It contains annular eclipses from September 18, 936 AD through May 14, 1333; hybrid eclipses from May 25, 1351 through July 8, 1423; and total eclipses from July 18, 1441 through May 19, 1928. The series ends at member 71 as a partial eclipse on August 3, 2054. 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 9 minutes, 26 seconds on December 3, 1062, and the longest duration of totality was produced by member 62 at 4 minutes, 19 seconds on April 26, 1892. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 57–71 occur between 1801 and 2054: | ||
|---|---|---|
| 57 | 58 | 59 |
 March 4, 1802 |
 March 14, 1820 |
 March 25, 1838 |
| 60 | 61 | 62 |
 April 5, 1856 |
 April 16, 1874 |
 April 26, 1892 |
| 63 | 64 | 65 |
 May 9, 1910 |
 May 19, 1928 |
 May 30, 1946 |
| 66 | 67 | 68 |
 June 10, 1964 |
 June 21, 1982 |
 July 1, 2000 |
| 69 | 70 | 71 |
 July 13, 2018 |
 July 23, 2036 |
 August 3, 2054 |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 117". eclipse.gsfc.nasa.gov.