This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. 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 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 43–64 occur between 1801 and 2200: | ||
|---|---|---|
| 43 | 44 | 45 |
 June 16, 1806 |
 June 26, 1824 |
 July 8, 1842 |
| 46 | 47 | 48 |
 July 18, 1860 |
 July 29, 1878 |
 August 9, 1896 |
| 49 | 50 | 51 |
 August 21, 1914 |
 August 31, 1932 |
 September 12, 1950 |
| 52 | 53 | 54 |
 September 22, 1968 |
 October 3, 1986 |
 October 14, 2004 |
| 55 | 56 | 57 |
 October 25, 2022 |
 November 4, 2040 |
 November 16, 2058 |
| 58 | 59 | 60 |
 November 26, 2076 |
 December 7, 2094 |
 December 19, 2112 |
| 61 | 62 | 63 |
 December 30, 2130 |
 January 9, 2149 |
 January 21, 2167 |
| 64 | ||
 January 31, 2185 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 124". eclipse.gsfc.nasa.gov.