This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836; hybrid eclipses from November 20, 1854 through December 23, 1908; and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. 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 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 18–39 occur between 1801 and 2200: | ||
|---|---|---|
| 18 | 19 | 20 |
 October 29, 1818 |
 November 9, 1836 |
 November 20, 1854 |
| 21 | 22 | 23 |
 November 30, 1872 |
 December 12, 1890 |
 December 23, 1908 |
| 24 | 25 | 26 |
 January 3, 1927 |
 January 14, 1945 |
 January 25, 1963 |
| 27 | 28 | 29 |
 February 4, 1981 |
 February 16, 1999 |
 February 26, 2017 |
| 30 | 31 | 32 |
 March 9, 2035 |
 March 20, 2053 |
 March 31, 2071 |
| 33 | 34 | 35 |
 April 10, 2089 |
 April 23, 2107 |
 May 3, 2125 |
| 36 | 37 | 38 |
 May 14, 2143 |
 May 25, 2161 |
 June 5, 2179 |
| 39 | ||
 June 15, 2197 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 140". eclipse.gsfc.nasa.gov.