This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 57–72 occur between 1801 and 2083: | ||
|---|---|---|
| 57 | 58 | 59 |
 February 1, 1813 |
 February 12, 1831 |
 February 23, 1849 |
| 60 | 61 | 62 |
 March 6, 1867 |
 March 16, 1885 |
 March 29, 1903 |
| 63 | 64 | 65 |
 April 8, 1921 |
 April 19, 1939 |
 April 30, 1957 |
| 66 | 67 | 68 |
 May 11, 1975 |
 May 21, 1993 |
 June 1, 2011 |
| 69 | 70 | 71 |
 June 12, 2029 |
 June 23, 2047 |
 July 3, 2065 |
| 72 | ||
 July 15, 2083 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 118". eclipse.gsfc.nasa.gov.