This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 will be produced by member 51 at 9 minutes, 52 seconds on December 29, 2168. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 5–26 occur between 1801 and 2200: | ||
|---|---|---|
| 5 | 6 | 7 |
 May 25, 1808 |
 June 5, 1826 |
 June 16, 1844 |
| 8 | 9 | 10 |
 June 27, 1862 |
 July 7, 1880 |
 July 18, 1898 |
| 11 | 12 | 13 |
 July 30, 1916 |
 August 10, 1934 |
 August 20, 1952 |
| 14 | 15 | 16 |
 August 31, 1970 |
 September 11, 1988 |
 September 22, 2006 |
| 17 | 18 | 19 |
 October 2, 2024 |
 October 14, 2042 |
 October 24, 2060 |
| 20 | 21 | 22 |
 November 4, 2078 |
 November 15, 2096 |
 November 27, 2114 |
| 23 | 24 | 25 |
 December 7, 2132 |
 December 19, 2150 |
 December 29, 2168 |
| 26 | ||
 January 9, 2187 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 144". eclipse.gsfc.nasa.gov.