This eclipse is a part of Saros series 119, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012; a hybrid eclipse on August 31, 1030; and annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. 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 10 at 32 seconds on August 20, 1012, and the longest duration of annularity was produced by member 44 at 7 minutes, 37 seconds on September 1, 1625. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 54–71 occur between 1801 and 2112: | ||
|---|---|---|
| 54 | 55 | 56 |
 December 21, 1805 |
 January 1, 1824 |
 January 11, 1842 |
| 57 | 58 | 59 |
 January 23, 1860 |
 February 2, 1878 |
 February 13, 1896 |
| 60 | 61 | 62 |
 February 25, 1914 |
 March 7, 1932 |
 March 18, 1950 |
| 63 | 64 | 65 |
 March 28, 1968 |
 April 9, 1986 |
 April 19, 2004 |
| 66 | 67 | 68 |
 April 30, 2022 |
 May 11, 2040 |
 May 22, 2058 |
| 69 | 70 | 71 |
 June 1, 2076 |
 June 13, 2094 |
 June 24, 2112 |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 119". eclipse.gsfc.nasa.gov.