This eclipse is a part of Saros series 114, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 23, 651 AD. It contains annular eclipses from February 3, 976 AD through June 11, 1192; hybrid eclipses from June 22, 1210 through December 1, 1480; and total eclipses from December 13, 1498 through June 15, 1787. The series ends at member 72 as a partial eclipse on September 12, 1931. 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 20 at 4 minutes, 33 seconds on February 13, 994 AD, and the longest duration of totality was produced by member 59 at 4 minutes, 18 seconds on April 21, 1697. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 65–72 occur between 1801 and 1931: | ||
|---|---|---|
| 65 | 66 | 67 |
 June 26, 1805 |
 July 8, 1823 |
 July 18, 1841 |
| 68 | 69 | 70 |
 July 29, 1859 |
 August 9, 1877 |
 August 20, 1895 |
| 71 | 72 | |
 August 31, 1913 |
 September 12, 1931 | |
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 114". eclipse.gsfc.nasa.gov.