This eclipse is a part of Saros series 123, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 29, 1074. It contains annular eclipses from July 2, 1182 through April 19, 1651; hybrid eclipses from April 30, 1669 through May 22, 1705; and total eclipses from June 3, 1723 through October 23, 1957. The series ends at member 70 as a partial eclipse on May 31, 2318. 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 19 at 8 minutes, 7 seconds on November 9, 1398, and the longest duration of totality was produced by member 42 at 3 minutes, 27 seconds on July 27, 1813. All eclipses in this series occur at the Moon’s ascending node of orbit.[1]
| Series members 42–63 occur between 1801 and 2200: | ||
|---|---|---|
| 42 | 43 | 44 |
 July 27, 1813 |
 August 7, 1831 |
 August 18, 1849 |
| 45 | 46 | 47 |
 August 29, 1867 |
 September 8, 1885 |
 September 21, 1903 |
| 48 | 49 | 50 |
 October 1, 1921 |
 October 12, 1939 |
 October 23, 1957 |
| 51 | 52 | 53 |
 November 3, 1975 |
 November 13, 1993 |
 November 25, 2011 |
| 54 | 55 | 56 |
 December 5, 2029 |
 December 16, 2047 |
 December 27, 2065 |
| 57 | 58 | 59 |
 January 7, 2084 |
 January 19, 2102 |
 January 30, 2120 |
| 60 | 61 | 62 |
 February 9, 2138 |
 February 21, 2156 |
 March 3, 2174 |
| 63 | ||
 March 13, 2192 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 123". eclipse.gsfc.nasa.gov.